DATE DUE

OCT 3 1974

1 30 501 JOSTEN'5
UNITED STATES DEPARTMENT OF COMMERCE • John T. Connor, Secretary

NATIONAL BUREAU OF STANDARDS • a. v. Astin, Director

THE SOLAR SPECTRUM 2935A to 8770

A

Second Revision of Rowland's Preliminary Table

of

Solar Spectrum Wavelengths

Charlotte E. Moore

National Bureau of Standards

M. G. J. MiNNAERT J. HOUTGAST

Utrecht Observatory

Printed with financial assistance from UNESCO

under the auspices of

The International Astronomical Union

National Bureau of Standards Monograph 61

Issued December 1966

For sale by the Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402

Price $4
National Bureau of Standards DEC 2 1 1966

/53, 7Z^
Foreword

The present Monograph has been prepared in response to a request by the International

Astronomical Union. At the Seventh General Assembly of this Union, held in 1948 in Zurich,

Switzerland, the following proposal from the Commission on Solar Radiation and Spectroscopy was adopted: "La Commission considere que la publication d'une table revisee du spectre

solaire dans le plus court delai possible est de la plus haute importance pour les astronomes

qui s'occupent de recherches sur le soleil et sur les spectres steUaires . . . .". It was further stipulated that such a revision should "contain wavelengths on the scale

of 1928, measured intensities or equivalent widths from Utrecht, and definitive identifications

from Moore-Sitterly".

The authors have made every effort to carry out the above recommendations. Throughout the span of years since this solar program was started the data collected for the Atomic

Energy Levels project, which has been carried out simultaneously, have aided greatly in the

identification work.

The generous support of the International Astronomical Union is warmly acknowledged.

This compendium could not have been completed without the equally cordial cooperation of the Utrecht Observatory and the Spectroscopy Section at the National Bureau of Standards.

A. V, AsTiN, Director

' Washington, D.C, January 6, 1966.

Library of Congress Catalog Card Number: 66-62199

III
Contents

Page Page

Foreword. _ _ iii

1. Introduction,- __ _____ v

2.7 The Miiltiplet Number or Vibration

Band: Column seven _ _ __ xix

2. Description of the Solar Spectrum Compendium. vi

2.1 The Wavelengths : Column one _ _ _ vi

2.2 The Measured Equivalent Widths:

Colmnn two _ __ _____ ix

2.8 Notes to the Solar-Spectrum Ledger:

Column eight xix, and 344-349

3. General Results _ __ _ _ xx

3.1 Number of Lines _ _ xx

2.3 The Reduced Widths: Column three xii

2.4 Behavior of Atomic Lines in the SunSpot Spectrum : Column four___ _ xvii

3.2 Atoms and Ions in the Sun__ _ _ xxi

3.3 Molecules in the Sun __ __ _ xxi

3.4 Summary of Identifications _ .. xxi

4. References ______ xxix

2.5 The Identifications: Column five _ xviii

2.6 The Low Excitation Potential or Rotation Line: Column six_ _ _ xix

5. The Solar Spectrum Ledger_ _ _ _ _ . _ xxx

5.1 Letters, Symbols, and Special Signs xxx

6. Acknowledgments _ __ __ _ xxx

List of Tables List of Figures

Table Subject Page Figure Caption Page

1 Wavelength Corrections for Reduction to the 1928

Scale of Standards VI

2 Spectrogi-ams from the Utrecht-Mount Wilson Collection, used for Wavelength Measurement VII

3 References to Standard Wavelengths in the Solar Spectrum VII

4 Weighting Factors for Measurements VIII

3 Letters in Column One: Wavelengths VIII

6 References to Data on Equivalent Widths of Fraunhofer Lines XVII

7 Notes on Molecular Lines in the Solar-Spectrum

Ledger . XIX

8 Counts of lines in the Solar Ledger XX

9 The Strongest Unidentified Lines XXII

10 Leading Lines in First and Second Spectra XXIII

11 Molecules in the Sun XXVI

12 Counts of Lines of Individual Spectra in the Solar Ledger XXVI

13 Chemical of Elements in the Sun XXVIII

1 Definition of Equivalent Width IX

2 Comparison of UV Monochromatic Intensity Measure- ments at Gottingen and at Dunsink. (Coordinates

io and ij^ in arbitrary units.) X

3 Disturbed and Undisturbed Fraunhofer Line XII

4 Monochromatic Blend Factor XIII

5 Influence of Background on Equivalent Width. (Ratio

between the equivalent widths of a Fraunhofer line on a background ii and the same line undisturbed. Parameter: equivalent width of the disturbed line in mA. Asterisks represent calculated values for the strong D2 line. The crosses correspond to Thackeray's observations; upright crosses for lines sti'onger

than 100 ml.) XIV

6 Complementing Correction. (Ratio — — of the

equivalent width of a blend W12 to the sum of the equivalent widths of the undisturbed components

Wi and W2 (in m^)-) XV

IV
The Solar Spectrum 2935 A to 8770 A

Second Revision of Rowland's Preliminary Table of Solar Spectrum

Wavelengths

Charlotte E. Moore

National Bureau of Standards

M. G. J. Minnaert J. Houtgast

Utrecht Observatory

The present compendium of solar spectrum wavelengths and intensities is essentially a second revision of Rowland's

Table, corrected and supplemented by material from the Utrecht Photometric Atlas [1].' Approximately 24,000 lines are

listed. In a number of cases new wavelengths were determined. Measured equivalent widths from the Atlas records replace the Rowland estimated line intensities recorded in the 1928 revision. From these directly measured equivalent widths have

been derived reduced widths, which, if necessary, were corrected for disturbing influences. The intensity behavior of atomic

lines in the spot spectrum as compared with the spectrum of the solar disk is indicated by letters denoting strengthening,

weakening, and the like. Atomic lines present only in the spot spectrum are, also, included, 223 in all. Revised identifications of the lines, as to chemical origin, are given for both atomic and molecular lines. For classified atomic lines the lower excitation potential and multiplet number are listed. For molecular lines the rotation branch and

quantum number, and the vibration band are indicated. Note numbers refer to notes in which the complete designation

of the band is given.

An introductory text gives a detailed description of each column of the solar ledger. Figures are included to illustrate the procedure used to derive the observed equivalent widths AX (mA) and the reduced widths AX/X(F).

Tables include counts of lines of each spectrum recorded in the identification column, leading lines in the first and

second spectra, and summaries of molecules and elements present in the sun. About 73 percent of the lines are wholly

or partially identified. Sixty-three elements are recorded as present. A number need further study. The number of molecules identified in the sun totals 11. Key Words: Elements in sun., equivalent widths of solar lines, identification of solar lines, molecules in sun, solar spec- trum, wavelengths of solar hnes.

1. Introduction

In 1895-1897 Kowland published a Preliminary Table of Solar Spectum Wavelengths that is still a challenge to spectroscopists [2].^ The span of observations was from

2975 A to 7330 A. Many featm-es of this rich spectrum

still defy interpretation. Throughout the years this

classical work has provided a threefold incentive: (1) to extend laboratory observations and interpretations of atomic and molecular spectra of various chemical ele- ments, for the purpose of identifying more of the observed

solar lines as to chemical origin; (2) to extend Rowland's

observations in both directions, to shorter and to longer

wavelength-regions by means of modern observing techniques, photographic developments, and the like; (3) fi- nally, to reobserve the solar spectrum in the "accessible"

range. All of these incentives are stUl being carried

out.The first revision of the Rowland Table was made

at the Mount Wilson Observatory in 1928 by C. E. St. John, and others [3]. At this time the Rowland wavelength-scale was converted to the international scale. The correction curve used for this conversion is described

in detail in the text to the 1928 publication. Further

minor corrections to the international scale are discussed

in § 2.1. By comparing the observed solar lines with laboratory

spectra, Rowland reported the presence of 39 chemical

elements in the sun, all but 2 of which have since been

! Figures In brackets Indicate the literature references in § 4.

confirmed. In 1928, 57 elements were reported as present

and 57% of the lines in the solar spectrum were identified. The number of known chemical elements in the sun is now 63, with 2 others dubiously identified. To date some 73% of the lines are whoUy or partiality identified

as to chemical origin. This is described more fully in

§§ 3.2, 3.3. In the 1928 revision no attempt was made to replace

the estimated line intensities from Rowland's Table by

measured equivalent widths. Provisional graphs for

the approximate conversion of the Rowland scale into

equivalent widths were published by Mulders [4]. In

1943, however, the staff at the Utrecht Observatory

started to prepare a catalogue of measured equivalent

widths, based primarily on the Utrecht Photometric

Atlas of the Solar Spectrum [5], in which the profiles of

all Fraunhofer lines between 3612 A and 8771 A are recorded. The spectrograms were obtained by jSIulders at the Mount Wilson Observatory, and the photometric

data were elaborated under the du'ection of Minnaert

and Houtgast. This Utrecht program became part of the cooperative project suggested by the International

Astronomical Union in 1948. The catalogue, just as the Atlas on which it is based, refers to the spectrum of

the center of the solar disk, little different from the

spectrum of integrated stmhght. The Utrecht contribution, consisting of a list of photometric data has

alread}", to a large extent, been published separately [6] V
because the data are so urgently needed for abundance

determinations and for comparisons with other stellar spectra.

The range of the present table has been limited to that long span of the solar spectnmi that overlaps the more recent and current observations from rocket and

orbiting-solar-observatory spectra in the ultraviolet

(short of 3000 A), and from the Jungfraujoch spectra in

the infrared (long of 7500 A). It is essentially a second

revision of Rowland's Table corrected and supplemented

by the Utrecht Atlas material. Even in this range the

work is far from completed. Many more solar lines

will doubtless be added when the spectrum has been

completely reobserved under the best observing conditions and with the best available modern instruments.

The task of remeasuring the complex spectrum and of

extending identifications and intensity measurements

is a heavy one in itself, and one that requires, also, much

additional work on the analysis of individual laboratory

spectra. The present contribution is intended as a convenient handbook for the astrophysicist until the

ideal self-contained compendium of the solar spectrum

from the x-ray to the microwave region becomes a reality.

2. Description of the Solar Spectrum Compendium

The successive columns of the solar ledger are described.

The general procedure by which the data on measured

intensities have been obtained is fuUy explained. The

many users require, also, more detailed information on

the analyses of individual spectra than can be recorded

here, for the many lines classified from laboratory investigations. Sufficient information is given in the ledger to provide convenient cross reference to the separate papers on spectrum analysis. For special details concerning

individual lines the column headed "Notes" should be

consulted.

2.1 The Wavelengths: Column One

A comprehensive revision of Rowland's Preliminary

Table of Solar Spectrum Wavelengths entails a thorough

study of the wavelengths of the lines reported by Rowland.

These remarkably accurate measurements by Jewell, that

date back to 1895-97 [2], were reduced to the International Scale of Wavelengths in the first revision of Rowland's Table in 1928 [3]. The tremendous amount of work that has gone into

interferometric observations for precise wavelength

standards need not be discussed here. Details may be

found in the early Transactions of the International

Astronomical Union [7], in the Allegheny Publications by

Burns, Meggers, and Kiess [8], and in the Mount Wilson

Contributions by St. John, H. D. Babcock and others.

St. John discussed the method used for the reduction to the international system, and has published the correction curve based on the International Standard Wavelength

Scale of 1922 [3]. The wavelengths listed in the 1928

edition are based on this curve. They are in three

categories: (1) Lines marked "m". These lines were

observed by Rowland, but remeasured for use in cor- recting Rowland's wavelength scale. (2) Lines marked

"w", denoting weighted means of remeasured lines and

Rowland's corrected values. (3) Undesignated wavelengths; these formed the great majority. They were

lines listed by Rowland but corrected to the international

scale of 1922 by means of the correction curve adopted

in 1928.

Throughout the years in which the 1928 edition has

been actively used, several problems regarding wavelengths have arisen. Further work on the International

Standards has indicated that a small running correction

is required to reduce the wavelengths based on the 1922

scale to the scale adopted in 1928 by the International

Astronomical Union. These corrections, reported by

H. D. Babcock [9] are as foUows:

Table 1. Wavelength Corrections for Reduction to the

1928 Scale of Standards

Correction to Correction to Region 1922 Scale Region 1922 Scale

(A) (A) (A) (A)

2995-3133 -0. 0012 6125-6290 -0. 006

3133-3370 *(-0. 0010) 6290-6455 -0. 007 3370-3705 -0. 0006 6455-6630 -0. 008

3719-3849 -0. 0015 6630 -0. 009

3850-3969 -0. 0015 6800 -0. 010

4000-5600 -0. 002 6900 -0. 012 5600-5780 *(-0. 003) 7000 -0. 014

5780-5960 *(-0. 004) 7100 -0. 016

5960-6125 -0. 005

Values in parentheses are interpolated.

They must be applied to all wavelengths published in the

1928 edition, in order to comply with the standards

recommended by Commission 14 of the Union.

Although Rowland's observations extend from 2975 A

to 7330 A, his spectrograms did not record the solar

spectrum completely in the ranges short of 3060 A and

long of 6600 A. With the development of new photographic emulsions, Rowland's work has been superseded

in the short- and long-wave regions. Meggers made a thorough study of the spectrum from 6500 A to 9000 A

in 1919 [10] and by means of Doppler displacements,

carefully separated the solar lines from the telluric lines. This work was subsequently extended at Mount Wilson

by H. D. Babcock and others, by comparing line intensities at high and low sun. In the present table the

VI
Table 2. Spectrograms from the Utrecht-Mount Wilson Collection used for Wavelength Measurement

Ttt ^ i. "NT „ Plate JNo. Wavelengta Kange (A) Jrlate JNo. Wavelength Hange (A) T>1 « * « "NT ^ rlate JNo. Wavelengtn Kange (A)

82 3949 to 4035 54 5205 to 5290 60 4690 to 4775

206 3994 to 4081 62 5260 to 5345 56 4875 to 4960

83 4071 to 4158 55 5320 to 5406 66 4933 to 5018

79 4144 to 4228 93 5367 to 5450 89 5018 to 5045

196 4190 to 4275 241 5740 to 5820 90 5070 to 5155

75 4262 to 4347 36 5885 to 5970 46 5395 to 5480

197 4315 to 4400 98 5953 to 6037 49 5462 to 5547

190 4375 to 4460 37 6004 to 6088 A 5520 to 5595

210 4430 to 4516 40 6055 to 6140 B 5580 to 5650

191 4495 to 4580 250 6195 to 6275 c 5635 to 5715

195 4560 to 4640 248 6250 to 6330 41 5663 to 5749

70 4592 to 4678 251 6305 to 6385 42 5800 to 5885

73 4655 to 4738 249 6370 to 6450 18 6125 to 6210

67 4753 to 4840 252 6420 to 6500 120 6582 to 6664

65 4820 to 4907 119 6497 to 6578

59 5044 to 5130 102 6575 to 6655

51 5145 to 5230

wavelengths from 6600 A to 8770 A are mostly taken

from the 1947 Monograph by H. D. Babcock and C. E.

Moore [11]. DetaUs regarding the wavelength scale in this region are given in the Introduction to this Monograph.

In the interval 2935 A to 3060 A, H. D. Babcock has

reobserved the solar spectrum. New measurements for some 665 lines have been reported [12] and used for the

present work. The reference standards for this region

require a correction of —0.002 A according to Babcock

[9]. In this interval Babcock's measurements thus cor- rected have been adopted with Standards indicated by

"S". See Table 3. In the course of the work on intensities by Minnaert

and his staff, many questions have arisen regarding new

lines not listed by Rowland, the reality of faint Rowland

lines, the resolution of close pairs, and the like. A set of

spectrograms taken from the collection made for the

preparation of the Atlas has been measured by C. E.

Moore in an effort to settle some questions about apparent

inconsistencies between the Atlas and the Rowland lines,

and also because it seems desirable to examine further

the lines recorded heretofore only by Rowland. These

measurements extend from 3949 A to 6600 A. The spectrograms from the Utrecht-Mount Wilson

collection that have been measured, are listed in Table 2. In the last column a list of auxiliary spectrograms of

poorer quality than the others is given. These were used

only to supplement the good ones.

Finally, two Mount WUson sun-spot spectrograms

T' 1969 and T' 1971 were used to cover the respective

intervals 4732 A to 4755 A and 4900 A to 4933 A. The

reciprocal dispersion of the Atlas plates is 0.35 A/mm;

that of the T' plates is 0.22 A/mm. The measurements

have been made on comparators at the National Bureau

of Standards, partly by visual and partly by oscilloscope

Table 3. References to Standard Wavelengths in the

Solar Spectrum

Wavelength

Range

(A)

Reference: Trans. Intern. Astron. Union

Commenta

2995 to 3133 7, 150, 1950 Reference Standards to be

corrected by —0.002 A. 3592 to 7122 3, 93, 1928 Recommended X. 7568 to 9889 6, 90, 1938 Recommended X.

settings. An attempt has been made to obtain at least two measurements for every line. The standards have been taken from the second

reference of Table 3. This table contains a complete

list of references to solar standards given by Commission

14 in the Transactions of the International Astronomical

Union.

A supplementary list of "temporary" standards in

the interval 7333 A to 11204 A is given in these Transactions 4, 83, 1932, but these are not designated by "S"

in column one, as are those from Table 3. In drawing the correction curves for the measurements

described above, the lines marked "m" in the 1928 solar

table as corrected from Table 1, have also been utUized

in addition to the "Standards" mentioned above. These

lines were all measured at Mount Wilson prior to 1928.

It is evident that many of the fainter lines that can be detected on the spectrograms under low-power magnification and in the Atlas, are too faint to measure on

the comparators. Some of these faint lines can, however,

be measured to 0.01 A on high-dispersion spectrograms,

with the aid of handscales.

VII
For one region, 5000 A to 6000 A, Zalubas [13] has

made spectrograms at the Georgetown University Observatory, especially for the purpose of observing faint

lines. He used a 21-foot concave Rowland grating having

20,000 lines to the inch, in a Wadsworth mounting;

the reciprocal dispersion (first order) was about 3 A/mm.

The spectrograms were made in the second order and have

a reciprocal dispersion of 1.4 A/mm. He has remeasured some 4,072 previously known lines, and added 234 new

faint lines, many of which may be of atmospheric origin.

All of his wavelengths represent means of measurements

made on thi'ee spectrograms. Of these new lines, 55

that were clear and also measurable in the Atlas records

have been included here. For the remeasured lines, a weighting system was

devised to combine the various kinds of measurements

available. The weighting factors are described in Table 4. The authors have had, also, the benefit of unpublished

notes from H. D. Babcock regarding close pairs, new

lines, improved wavelengths of atmospheric and other

molecular lines, identifications, reality of faint lines, and

other detaUs. The wavelengths published by him and

L. Herzberg [14] in their analysis of the Atm O2 bands

have been adopted with the label "m" (see Table 5). In examining the Atlas, Minnaert and Houtgast have

measured a number of lines to ±0.01 A. Some of these

indicate further corrections to Rowland's list; many

others are new lines (see § 3.1 and Table 8). Long of

6600 A it seemed inefficient to include all of the faintest

lines in the catalogue, which are mostly of atmospheric

origin. Many of them have been dropped, especially if they were not included in the 1928 edition or in the 1947

catalogue of H. D. Babcock and C. E. Moore. All identified solar lines have been kept. The wavelengths determined from the Atlas cannot be compared in precision

with those measured by means of a modern comparator.

If precise wavelengths are needed, the positions of several

neighboring lines should be checked, and the scale, if necessary, slightly adjusted by fractions of a millimeter.

The Atlas is superior, however, when faint lines appear on the

slopes of strong lines, when lines are broad and assymetric,

or when they are revealed only by a tracing, which, being

flat, nevertheless fails to reach the continuum line.

Table 4. Weighting Factors for Measurements

Weight Description of Source Material

10 Wavelengths marked "w" in the 1928 edition as cor- rected from Table 1. 5 Rowland wavelength from the 1928 edition as corrected from Table 1. 5 Measurement by Zalubas [13]. 5 Three or more measurements by C. E. Moore.

3 Two measurements by C. E. Moore.

1 One measurement by C. E. Moore.

J4 One dubious measurement by C. E. Moore.

The behavior of atomic lines in the spot spectrum is discussed in § 2.4. A study of such lines was made by

C. E. Moore in 1932 [15], and a list was published by her

in 1933 [16]. Atomic lines appearing only in the spot

spectrum are entered to two decimals only. They are taken from the 1933 paper. Her measurements of spot

lines have been supplemented by those included in the

1928 revision, and also by unpublished measurements hj

R. S. Richardson in the interval from 4900 A to 5403 A

[17]. The rounded-off wavelengths of spot lines quoted

from Richardson are indicated by a dagger in note 13. His wavelengths have also been utilized for a number of

lines formerly listed as spot lines and later seen on the

Atlas spectrograms.

Table 5 contains the letters used in column one to indicate wavelengths in the different categories discussed

above.

In two special cases, laboratory wavelengths are quoted

with special notes : Note 10. The Baimer series of H, 71- =8 through 17. Note 31. The Paschen series of H, n=12 through 18. All other wavelengths not designated by the letters in

Table 5, are weighted means. All wavelengths are in air. More remains to be done, especially on improving

wavelengths of faint solar lines, and, above all, on extending the list to include many more faint solar lines that appear on spectrograms and photometric records made with

the finest solar instruments available today. The demand for the present compendium is so great that the

further delay that would be necessary to make a more detailed study of new faint solar lines, does not appear justifiable. This is one of the most challenging problems of

the near futm-e.

Table 5. Letters in Column One: Wavelengths

S Standard Wavelength, see Table 3. m This letter is used:

(1) To denote lines measured at Mount Wilson, recorded

as "m" in the 1928 revision, in the interval 3062 A to 6600 A. The 1928 entries corrected from Table 1 are recorded here. For lines longer than 6600 A, many

have been remeasured, but the letter "m" has been

retained only for those solar lines thus noted in the 1928 edition.

(2) For wavelengths of lines in the Atm O2 bands as reported by H. D. Babcock and L. Herzberg [14].

(3) For a few unpublished measurements by H. D.

Babcock.

(4) For measurements of sun-spot lines [16], and for other measurements taken from Richardson.

(5) For selected lines having special notes.

r Lines whose wavelengths are from Rowland's Table. Short of 6600 A the listed wavelengths are from the 1928 edition cor- rected as described in Table 1. To longer waves, the lines in

this category are quoted from the 1947 Solar Table [11], where the correction factors occasionally deviate slightly from

those listed in Table 1. a Two-place measurements furnished by Minnaert and Houtgast,

from their study of the photometric tracings. All of these

lines have been seen as traces on the solar spectrograms as

well as in the Atlas recordings.

VIII
2.2 The Measured Equivalent Widths, AX(mA)

Column Two

According to the general use in astrophysics, the

equivalent width of a Fraunhofer line is the width of a

hypothetical absorption line, which, being perfectly black

and having sharp edges, would absorb from the neighbouring continuum the same amount of energy as the real

line (Fig. 1). Another measure for the line strength

called the reduced width, which will be defined in § 2.3, is listed in column three [18]. The present table has the short-wave limit 2935 A, in order to provide an overlap with subsequent solar tables

that extend to shorter wavelengths. From 2935 A to 3061 A no calibrated plates were available for intensity

measurements. In this range, eye-estimates of the line intensities are entered in brackets between the two col- umns containing measured intensities. The quoted

estimated intensities are from H. D, Babcock [12]. They

are not to be confused with the measured equivalent

widths.

In the present volume, several errors in the provisional

publication [6] have been corrected. The ultraviolet data

have been modified, taking into account the more recently

published Gottingen Atlas [19]. In the red part of the

spectrum a number of dubious faint lines have been

rejected, others have been added, and wavelengths have

been adjusted, so that the catalogue is now a better

description of the Atlas.

The intensity measurements were based on the Utrecht

Photometric Atlas of the Solar Spectrum [5], in which the

profiles of all Fraunhofer Lines between 3612" A and 8771 A

are recorded, from spectrograms made by G. F. W.

Mulders at the Mount Wilson Observatory, Pasadena.

In the introduction of this Atlas, full details about the ini- crophotometric work are found. The region from 3612 A

to 6977 A was photographed in the 2nd order; the one from 6923 A to 8771 A in the 1st order. For the atmospheric lines it may be useful to remember that sec f varied

between 1.26 and 4.92, as listed in the introduction of the

Atlas. Longer than 5560 A it did not exceed 2.22. In the small stretches where two spectrograms overlap, that

with the greatest value of f was selected. The spectral region short of 3612 A was included in the Atlas only as an Appendix based on Utrecht spectra

with much less resolution. It proved surprisingly dif- ficult to find an observatory provided with adequate

instruments for an improved study of this part of the

solar spectrum. Fortunately the Dunsink Observatory was so kind as to obtain a complete set of the ultra- violet region between 3100 A and 3650 A and to record

these spectra with a direct intensity microphotometer,

similar to that originally used for the Utrecht Atlas.

It is clearly an advantage that the same institute that

made the spectrograms also recorded them, making all necessary photometric checks. For some sections, plates

kindly taken by H. D. Babcock at the Mount Wilson

Observatory were also used. On the Dublin records

the lines have a total half-width only slightly (5%)

greater than that of the Mount WUson-Utrecht records;

10 lines in the region of overlap yielded /i=27.8 (Mount

Wilson) and 29.1 (Dublin), expressed in micro-wavelengths (/xX). An analysis of the apparatus curve in this

761-925—66 2
1.00

0.50

0.50 1.00

Figure 2, Comparison of UV monochromatic intensity measurements at Gottingen and at Dunsink.

Coordinates io and ic in arbitrary units.

region, approximated by a Voigt profile, showed that

the Dublin damping coefficient (jSi) was much smaller,

practically absent, while the Doppler coefficient (^2) was

considerably greater. (Mount WUson: /3i=2.19; ^2=

3.48. Dublin: /3i =0.01; /32=11.0). The curve relating

the half-width to the central intensity, was practically

the same for both series. This was a fortunate cir- cimastance, owing to which we felt justified at first in

applying to the whole of the material the same tables

and graphs.

After the Preliminary Photometric Catalogue was

published by the Utrecht Observatory, an Atlas was

published at Gottingen that provided new photometric

tracings for the ultraviolet region [19]. It seemed

important to check against these new records the results which had been obtained on the basis of the Dublin

registrations. Both series of tracings were direct in- tensity records.

On first inspection it became clear that the resolving

power of the Dublin records is slightly better than that

obtained at Gottingen. More important, however, was

the photometric comparison, the more so, since we had

been warned by the Dublin observers that there might be some deviations.

A plot of E.W. (Dublin) against E.W. (Gottingen), for

210 lines near 3330 A, showed a systematic difference, the

ratio D/G varying between 1.2 and 1.4. By plotting for

individual, well selected points the intensities in arbitrary

units ij) against {q, it was also shown that this difference was due to fundamental deviations in the photometric

scale. This method of comparison worked quickly and

efficiently and was independent of the assumed background intensity, the deviations appearing as a curvature

of the plot (Fig. 2). In order to decide which of the two

scales was correct, use was made of ultraviolet spectral

records obtained by J. Houtgast [23] at the Mount Wilson

Observatory in 1960, with the Snow Telescope and the

apparatus of W. E. Mitchell for direct photometric re- cording of the spectrum. Cross-comparisons showed

unambiguously that the Gottingen photometry is the

correct one. X
The effect of a curvature in the photometric scale might

be expected to be different according to the E.W. of the

spectral lines and the intensity of the background on

which they are superposed. This was actually found.

However in practice these differences in the correction

for the individual spectral lines were not important.

Considering the necessity of a simple and practical procedure, in view of the great number of lines involved, it seemed sufficient to divide all values of E.W.d by a mean

factor of (1 +A),

EWn-EWo where A=- EWo

measm"es the relative deviation in the E.W. Near

3330 A the factor (1 +A) amounted to 1.35. It was then necessary to ascertain how the factor +

varied with the spectral region. We assumed that the

photometric scale would be homogeneous within each

DubUn microphotometer record, corresponding to about

10 A. For each of the 52 records, a graph was made of io

against io (Fig. 2) ; the curvature, thus the deviation from

the right scale, was characterised by the ratio r='^^.

^ AM

measiired at the height %=0.50^0 (max). The ratio r was

0.130 near 3330 A and varied between 0 and 0.15 in the

o o wavelength region 3075 A to 3550 A, the difference between

both scales disappearing at longeV wavelengths.

We assumed that A is approximately proportional to

r, so that, in general,

l +A=l+0.35

0.13

The difl&cult and lengthy determination of A was thus

replaced by a very quick measurement of r, easily applied

at a great number of wavelengths.

The correction, finally applied, amounted to dividing

aU equivalent widths and reduced widths of the Preliminary Catalogue (1960) by the factor (1 + Ax), which

is a function of wavelength; this factor varied in general

between 1 and 1.30 and reached higher values, up to 1.43 at only two places.

The equivalent widths, AX, in miUi-Angstroms, as determined by direct measurement from the records, are tabulated in column two. In the first place the

continuous background was located, which sometimes

deviates a little from the Atlas continuum. This was

relatively easy in the infrared and visual regions, but it became increasingly difficult towards the shorter wavelengths. Special difficulties were encountered short of

4000 A, where the determination of the continuous background has been a matter of serious concern. In general we first traced the profiles of the strongest lines, then the

profiles of fainter lines superposed on the first ones, etc. So for each line we obtained a local continuum. The

local continuum for the strongest lines is determined by

the highest points of the stretch of spectrum considered.

Of course some indeterminacy resulted from the extent

of the interval inside of which these highest points were

selected. It is with respect to this local continuum that

equivalent widths of column two have been computed.

In view of further reductions, to be explained in § 2.3, we had, also, to locate the true or maximum continuum,

this being defined as the continuum which would be

found theoretically from the tables of Kc in general use,

e.g. from those of Vitense [26]. These tables yield in the UV a continuum which at the Balmcr limit jumps

discontinuously to a lower value. In the region short

of 4000 A, we have adopted the mean of the continuum

as found by Michard [20], and by Rauer [21], later con- firmed by Mrs. Pecker [22]. This locates the maximum

continuum at an Atlas ordinate, gradually increasing

from 100 at 4000 A to 140 at 3647 A. There it is considered to jump discontinuously to a lower value, the

place of the jump being indicated by parallel horizontal bars

in our catalogue. There is no doubt that actually the

background is depressed gradually and smoothly, be- cause of the accumulating Baimer lines and (nearer to the limit) by the pre-ionization of the hydrogen atoms.

However, these effects are not included in the ordinary

tables of the continuous absorption coefficient. In computing a line profile, the theorist wiU, therefore, refer the

spectral line to this high continuum, and consider the

profile as formed by the blend between the line proper

and the higher Balmer lines. The location of our maximum continuum, as described, conforms to the continuum

of the theorists. Short of 3647 A, we have conservatively assumed that the Atlas ordinate 100 corresponds more or less to the true continuum, as was assumed by

Michard. An investigation by Minnaert concerning the

profiles of strong lines in the region 3500 A to 3600 A

suggests that there the real continuum should also be

higher. Before accepting the consequences of such a

conclusion, more discussion seems to be necessary.

Recent photoelectric measurements of Houtgast on

high-dispersion spectra give the detailed absolute in- tensities of 200 selected points over the range 3000 A

to 4000 A, which should be used in the future as the

basis for the location of the maximum continuiun [23].

For each individual line, where necessary, smoothed

individual profUes of the wings were traced with a sharp

pencU on the Atlas records. In blends, the separation of

a line from the neighbom'ing ones was made there where

it could be done without complications by simple application of the "product rule," meaning that an ordinate

with relative intensity ^> superposed on a background ^>

becomes ^=^X^ (Fig. 3) . This applies to the following

'Z'O '>'0 f'O , cases:

1. two telluric lines, or a teUiu-ic line combined with a

solar line

2. two solar lines, the overlapping parts of which do not

descend below 80% of the continuum.

XI
Figure 3. Disturbed and undisturbed Fraunhofer line.

In all other cases the separation of the blend components was made only in column three (see § 2.3).

The areas of profiles whose dip exceeded 20%, were

determined by a Coradi polar planimeter, of which the

precision had been tested before. Each profile was

measm"ed clockwise and counterclockwise and the mean

was taken. For lines with a maximum dip less than

30%, the planimeter measurments were not considered

to be sufficiently precise, and the areas were found by

counting square millimeters. For a group of medium

strong lines there is an overlap, and the mean was taken

of the planimeter result and of the counts. The same

was done for overlapping parts of the successive Atlas

strips; their differences were treated as accidental, though

in many cases it was obvious that the deviations were

systematic. The areas were reduced to equivalent widths

in mA, taking into account the dispersion and the height

of the (local) continuum. All single lines and all of the

lines which had been directly separated by applying the product rule were treated in this way. For blends not satis- fying the conditions mentioned, the equivalent width of the entire blend as a whole is mentioned in the second

column.

The Balmer lines of the hydrogen spectrum presented

special difficulties near the series hmit at 3647 A. Very

striking is the great depth of Hio, which we considered

as a real anomaly. The lines Hi2, Hn, H14 are masked by

strong superposed lines; H15, H15 and are measurable.

The line His is certainly not seen; we assumed, therefore,

that Hi9 and H20 are also invisible, and that slight depressions there are due to the combination of neighboring

lines. The profiles for H12, H13 and Hu were found by

interpolation. For the further reduction in column three,

where residts of other observers are combined with ours, the results of de Jager (Table 6) have been taken into

account up to Hu.

2.3 The Reduced Widths, AX/XXlO« (F): Column

Three

Next to the equivalent width, another measure for

line-strength has proved useful for many theoretical

investigations: it is the reduced width, defined as 10® times AX/X, and expressed in a unit called the Jraunhojer

(F) [18], This is a dimensionless number, having a convenient order of magnitude and independent of the

unit in which both AX and X are measured. The reduced

width is equal to the equivalent width, expressed in

microwavelengths (/xX=10~®X). The reduced widths are found in column three, improved, however, because the

directly measured equivalent widths of column two had

to be revised, before reduction, taking into account

several considerations, now to be explained.

For a number of Fraunhofer fines, equivalent widths

have already been determined earfier by other workers.

A list of references is found in Table 6, at the end of

§ 2.3. We assumed, that these measurements are direct

determinations of the equivalent width, without the cor- rection for the blend factor to be discussed later. For

this reason all comparisons were made with the numbers

of our second column, where the blend correction has not

yet been applied. We have fisted for each fine aU available measurements, and have taken mean values, assuming

double weight for the Atlas determinations, in order to obtain greater homogeneity in the catalogue between

lines measured at Utrecht only, and lines also measured

elsewhere. For aU fines where other measurements have

been taken into account, the reduced width in the third

column is in itafics. The following remarks should be made : (a) The measurements of Philfips (Table 6) in the ultraviolet have not

been used, because his numbers are so much smaUer than our results, from both Mount Wilson and Dublin plates,

that the homogeneity of the catalogue would have been

lost. The same applies to WooUey's measurements

(Table 6). Short of 3813 A, except for the Balmer lines, no measurements other than the Utrecht values were

used. (^») Of the equivalent widths measured by AUen

(Table 6), these have been used which were derived by

photometry of the profiles, but not those obtained from

depth and halfwidth only, (c) No use has been made of

profiles determined by some authors, but not converted

by them into E.W.; in most of these cases the shape of the

outer wings had not been ascertained.

The next task was to disentangle those blends, which

could not be analyzed by the simple product rule. Practicafiy all blends, even in compficated cases, could be

reduced: (a) to combinations of two lines, or {h) to the

case of a line, formed on a background lower than the

normal continuum. When three fines A, B, C were

found combined, it was in general sufficient to consider

the interaction of A and B and the interaction of B and C,

the mutual influence of A and C being mostly negligible. It is weU known that two Fraunhofer lines combine

according to rules more compficated than those of terrestrial absorption fines, as has been shown by Thackeray,

Houtgast and Minnaert [24] and later by Unsold [25] and

by Rauer [21].^ When these last investigations were published, om* work, started in 1943, had already progressed

so far that it would not have been possible to change the

' In the mean the effects of blending, calculated by Rauer, are less pronounced than

those taken into account by us. This is due mainly to our assumption, that both lines originate in the same layers of the solar atmosphere. XII
method of reduction. Nor would it have been possible,

in a treatment of many blends, to consider the individual

details of each combination. The explanation and graphs

published in paper [24] give more ample information about

the methods appUed. For the reduction it was assumed

that the Hnes behaved as scattering lines, because some of the strongest ones were resonance lines and because we

wished, also, to reduce in the simplest way the very low

central intensities. For moderately deep profiles, the

choice between absorption and scattering is practically

unimportant. Two-dimensional combination tables were

calculated, giving the resultant intensity ii2 at a wavelength where the individual intensities ii and 't2 are superposed; a first table referred to atoms distributed

according to Schwarzschild-Schuster, another to atoms

distributed according to Milne-Eddirigton. Finally, the

geometric mean of both combination tables was taken, = .- for a hypoto I2 square by square. Fig. 4 gives

thetical monochromatic line, indicating in what proportion it is reduced when superposed on a background

ii. If we compare lines superposed on a more or less

.10 .20 .30 .40 .50 .60 .70

Figure 4. Monochromatic blend factor.

80 .90

ii -

.00

XIII
homogeneous background ii, with the Hues which would

have been formed by the same atoms on the background

of the true continuum io, we would expect by the product

(Fig. 5). Conversely, the observed equivalent widths

%2)d\

j^g^^g divided by a factor smaller than

rule that the blend factor would be simply equal to h, ^^^^^ ^^^^ ^^^^ed

the area having decreased in this proportion but the

equivalent width remaining the same. According to the

combination table, however, a further reduction of the area is observed, which affects the equivalent width and

which can be computed easily for normal profiles derived

from the Atlas for lines of different eqmvalent widths

Lines forming a close doublet were analysed by means

of model doublets. Two normal profiles, freed from the

apparatus function, were drawn at a chosen distance from

each other, then combined, ordinate by ordinate, according to the combination table. The resulting doublets,

slightly smoothed by combining them with the apparatus

FiGTJEE 5. Influence of background on equivalent width.

Ratio between the equivalent widths of a Fraunhofer line on a background ii and the same line undisturbed. Parameter: equivalent width of the disturbed line In mA. Asterisks represent calculated values for the strong Dj line. The crosses correspond to Thackeray's observations; upright crosses for lines stronger than 100 ml.

XIV
10

1 1 Q95

Q90 "

-

AX=12jLiX

-

/ A'X.-IRil'X \U.OU,,-

0.95 0.90 0.85^

1 / \

10

Wi(nA,)—

Ratio Wli Figure 6. Complementing correction.of the equivalent width of a blend wn to the sum of the equivalent widths

of the undisturbed components wi and Wi (in ;iX)

as a function of:

function, were considered to apply to the whole spectrum

indiscriminately, provided their abscissae were taken

proportional to the wavelength.^ This was obtained by

assuming as a imit the microwavelength iJ.X=10~^X.

Lines of very different equivalent widths were combiaed two by two, the profile of each pair being computed

for distances of 0, 6, 12, 18, 24 ^X. Atlas doublets could

then be compared with the model doublets. This process

of comparison was made easier by computing once for

aU from the model doublets the ratio: equivalent width

of fainter line/sum of the two equivalent widths

[minimum intensity in fainter line; [minimum intensity in stronger line;

function of - |^^*^^^ blend at height 60% of io; [miQimum intensity in stronger line. The first graph was used for the faint lines, the second

graph for the strong lines. In many cases both graphs

could be used, and the results were, in general, found to agree remarkably well; the mean of the two was taken.

The model doublets give only the ratio between the two

components. When the measured equivalent width of

the blend is divided in that ratio, a correction must stUl be

applied because the equivalent width of the blend is less than the smn of the equivalent widths of the components.

The amount of this complementing correction was also obtained as a byproduct of the construction of the model

or as a

'The apparatus function of a grating appears to have its abscissae proportional to X. A

special test, made later on near 3800A, seems to show that the line widths there, measured

in are somewhat narrower than near 6000 A, by a factor varying between 1.00 and 1.30; this means that we might have overestimated somewhat the blending effects in the UV

doublets. As an example we reproduce the graph for two lines at distances of AX=12;^X or AX=18mX (Fig- 6). For the closest doublets, the methods thus far described

would not suffice. Often the record and the plate showed

only slight indications of asymmetry, which it would

have been very difficult to translate into quantitative

ratios. In these cases we have relied on Rowland's

original visual estimates; we transformed them into

equivalent widths according to Mulders [4], divided the

measured equivalent width in that ratio, and applied

the complementing correction. A special investigation

showed that for lines of a given Rowland number the

equivalent width does not systematically change when

they are found superposed on the wings of other lines. This means that Rowland automaticaUy corrected for

the influence of the background on the equivalent width.

In all cases, where there is a difference between the

local and the maximum background, a reduction was

applied, in the same way as explained for "lines, superposed on a more or less homogeneous background"

(Fig. 3). This applies especially to the whole stretch

between 3647 A and 4000 A.

FinaUy all equivalent widths, already corrected for the

effects thus far mentioned, had to be converted to reduced

widths:

reduced width (F)=equivalent width (mA)X 1000

X(A)

We shall give a few examples of the procedure followed.

3991.121 A Area=136 mm^ (planimeter) Local background =93 mm. Dispersion=19.8 mm/A

136 Equivalent width =- =0.0739 A= 73.9 mA

93X19.8

Measurements by other authors: Thackeray 71, Rauer 80. Weighted mean=74.5

Max. background=102 mm. Thus local background

max. background=0.91

Reduction to max. background (by Fig. 5) 74.5

0.93'

= 80.2

Reduced width= 80.2 3.991 = 20.1 F

4476.021 Al Area=297 mm^ (planimeter) 4476.089 Aj

Background =100. Dispersion = 19.6 mm/A

297

Equivalent width= j^qq"^'^^^ g = 0.152 A=

}

152

Separation not detectable. Rowland estimates: 4

3

Proportional equivalent width

of components:

1151 87

86.5

65.5

202 (Mulders)

152

XV
Complementing correction for mutual influence (by Fig. 6):

Reduced width=

86.5

0.86 101

'4.476'

= 101:

22.6

65.5

0.86'

= 76

76

4.476

17.0

4238.760 297.5 mm^ (planimeter) 4238.816 Aj '

Local background = 99. Dispersion = 19.4 mm/A

Equivalent width

155 mA

Ratio of components from model doublets: 0.15

Equivalent width of components: yt1;=135;

^^^^^"'^^ =20.

Increase for mutual influence (AX= 0.056 A):

0.91^^^' 0.91~^^

Reduced width=

148

' 4.238' 34.9 22

4.238' 5.2

The computation of the equivalent width and of the

reduced width may in some cases increase the importance

of a line in a most surprising way; this occurs especially

for lines superposed on the deepest parts of a spectral

profile. Take e.g. the line 3967.431 A with an area

of only 5 sq. mm in the Atlas, superposed on a local

background of 15%. The equivalent width becomes

^—=0.0192 A=19.2 ml. Now consider, that

15 X 17.3

this local background is only 11% of the maximum

background, and since we consider a faint line, the reduction factor is very important. We have to divide by

0.08. Eventually the reduced width becomes 240 mA

or 60.4 F. Even more striking examples could be given.

The reduced widths (lO'^AX/A), in fraunhofers, obtained by taking into account measurements of other

authors and eliminating, as well as possible, perturbing

influences of neighboring lines, are directly adapted to the theoretical work, but much more uncertain than

the entries in column two. We are well aware of the

uncertainties in this process of reduction. Our calculations give at least an idea of the order of the blending

effect, and a warning that it may become very important,

especially in the ultraviolet spectriun.

In such cases where measurements of different authors

are available, great divergencies are sometimes found.

While the data in italics may be expected to be, in general, more reliable than the others, they may be worse in

individual cases, and they are inevitably less homogeneous.

We have refrained from using question marks for those

many cases in which there were doubts concerning the

reality of a line, the exact profile, the separation of blends,

the correction for the background, etc. Even in the

most dubious cases, we have compelled ourselves to make a decision, considering that others would have to struggle with the same difficulties, without having more

solid ground than we did. It must be clear that our

catalogue is fuU of weak points in all these respects,

and that anyone interested in special lines should study

them in detail himself, on several spectrograms and

repeated records, by using his own critical sense. Nevertheless we hope that the intensity data of the catalogue

will be useful in the present period of solar research.

Symbols and Special Signs Used in Columns

Two and Three

Horizontal separation, indicating the overlap

between successive plates in the spectral region

where telluric lines occur. Equivalent widths of

telluric lines may be compared only on one and

the same plate.

( )

The Hne is so closely blended with adjacent faint

lines, not mentioned in the RRT or in the BM

catalogue, that a separation seems impossible.

The equivalent width given refers to the total

blend.

The line is partly blended with adjacent faint

lines, not mentioned in the RRT or in the BM

catalogue, which have been separated by us. The equivalent width refers to the line alone.

The hnes have not been analyzed in the second

column, either because an analysis of the profile was practically impossible, or because such an

analysis required too uncertain theoretical assumptions. The equivalent width relates to the blend

as a whole.

The reduced width, when entered in italics, is the weighted mean of the Utrecht measurement

and of measurements by other observers.

The equivalent width could not be directly measured, but it was derived by interpolation, or from

multiplets, or from Rowland's estimates.

XVI
Table 6. References to Papers Where Equivalent Widths of Fraunhofer Lines Are Found

Adam, M. G.: Mon. Not. Roy. Astron. Soc. 98, 112 and 544, 1938;

100, 595, 1940.

Allen, C. W.: Mem. Commonwealth Solar Obs., Canberra 1, No.

5, 1934; 2, No. 6, 1938. Astroph. J. 85, 165, 1937; 88, 125, 1938. Mon. Not. Roy. Astron. Soc. 96, 508 and 843, 1936; 100, 10, 1939. Barocas, V. and Righini, G.: Astroph. J. 114, 443, 1951. Bretz, M.: Zeit. Astroph. 38, 259, 1956. Cherrington, E.: Bull. Lick Obs. 17, 161, 1935. Dahme, A.: Zeit. Astroph. 11, 93, 1935. Hindmarsh, W. R.: Mon. Not. Roy. Astron. Soc. 115, 270, 1955. Houtgast, J.: Dissertation, Utrecht, 1942. De Jager, C: Recherch. Astron. Obs. Utrecht, 13 (1), 1952.

KorfiF, S. A.: Astroph. J. 76, 294, 1932. Minnaert, M. and Mulders, G. F. W.: Zeit. Astroph. 1, 192, 1930. Mulders, G. F. W.: Dissertation, Utrecht, 1934. Pecker, J. CI. and Peytureaux, R.: Ann. d' Astroph. 11, 90, 1948. Pecker, J. CL: Ann. d' Astroph. 12, 197, 1949. PhilUps, J. G.: Astroph. J. 96, 61, 1942.

Plaskett, H. H.: Mon. Not. Roy. Astron. Soc. 91, 870, 1931. Rauer, W.: Zeit. Astroph. 37, 1, 1955.

Righini, G.: Mem. Oss. Astrof. Arcetri 48, 29, 1931. Zeit. Astroph.

10, 349, 1935. Roach, F. E. and PhiUips, J. G.: Astroph. J. 96, 71, 1942. Shane, C. D.: Bull. Lick Obs. 16, No. 449, 1932; 19, No. 507, 1941. Thackeray, A. D.: Mon. Not. Roy. Astron. Soc. 94, 99, 1934; 95, 293, 1935. Astroph. J. 84, 433, 1936. Ten Bruggencate, P. and von Kliiber, H.: Veroff. Gottingen No.

78; Nach. Akad. Wiss. Gottingen, Math.-Phys. Kl., pp. 165 to

183, 1944. Ten Bruggencate, P. and Houtgast, J.: Zeit. Astroph. 20, 149, 1940. Ten Bruggencate, P.; Golnow, H.; Giinther, S.; Strohmeier, W.:

Zeit. Astroph. 26, 51, 1949. Unsold, A.: Zeit. Phys. 46, 765, 1928. Weidemann, V.: Zeit. Astroph. 36, 101, 1955. WooUey, R.v.d.R.: Ann. Solar Phys. Obs. Cambridge 3, 88, 1933. Mon. Not. Roy. Astron. Soc. 93, 700, 1933.

2.4 Behavior of Atomic Lines in the Sun-Spot Spectrum:

Column Four

The physical conditions prevailing in sun-spots have

long attracted the attention of the astrophysicist. The

great importance of spot behavior in assigning identifications to the solar lines has been recognized throughout the

present work. The most extensive spot data available are those based on the Mount Wilson observations of spot

spectra. One of the authors (C.E.M.) used this material

for a detailed study of Atomic Lines in the Sun-Spot

Spectrum, in 1932 [15]. At this time an attempt was made

to estimate spot intensities on approximately the same

scale as Rowland used for estimating the disk intensities. Although estimated intensities are far from ideal for work

on determining abundances of chemical elements in the

stars, yet they provide reliable general information as to whether the line is strengthened, unchanged, weakened,

or obliterated in the spot spectrum as compared with the

disk spectrum.

The spectrograms were made with the 150-foot tower

telescope at Mount Wilson with the use of a Nicol prism

and quarter-wave plate to reveal the Zeeman effect in the

spot spectra. The zigzag effect thus produced enables one to select atomic from molecular lines in the spot

spectrum.

For the present it is impossible to include measured

equivalent widths for lines in the spot spectrum, such as are contained in columns two and three for the disk lines. The great amount of stray light in most sun-spot spectra

vitiates the photometric measurements by an amount often

unknown. In place of the equivalent widths the following

letters are introduced in column four to indicate the spot

behavior as compared with the disk intensity, and thus

add weight to the assigned identifications in column five.

S The line is greatly strengthened in the spot spectrum as compared with the disk spectrum. For

atomic lines appearing only in the spot spectrum,

the estimated spot spectrum is 0 or greater, on the

Rowland scale of intensities. For disk lines, the

strengthening is estimated to be 3 or more units on

that scale. This letter is used, also, for selected

unweakened winged lines, which were labeled "W"

in the 1933 publication [16].

s The line is strengthened in the spot spectrum,

probably less than 3 units on the Rowland scale. For atomic lines present only in the spot spectrum

the intensity is estimated as "—1" or less, i.e. 00

or less, on Rowland's scale. u The line is imchanged in intensity in the spot

spectrum.

W The line is greatly decreased in intensity in the spot

spectrum, 3 or more units on the Rowland scale. w The line is weakened in the spot spectrum,* but the

weakening is estimated to be less than 3 units.

0 The line is obliterated in the spot spectrum.

N The line is diffuse. NN The line is very diffuse. d The line is double.

The spot spectrum data are taken mostly from the

publication entitled Atomic Lines in the Sun-Spot Spectrum for the region 3894 A to 6635 A [16]. In general,

for wavelengths longer than 6635 A the estimated spot

intensities from the 1947 publication [11] have been used.

In addition, for a limited number of lines, miscellaneous

unpublished notes furnished by H. D. Babcock and some

unpublished estimates by C. E. Moore have been used.

XVII
It is hoped that the next revision of the solar spectrum

will include homogeneous measured equivalent widths for atomic lines in the spot spectrum, derived from highdispersion spot spectrograms covering the whole range

with the same spot. This is one of the crying needs ia solar spectroscopy today. Difficult as such an observing

program is, it would well repay the effort. The spot

spectrum contains thousands of lines that have not yet

been measured. Many are of molecular origin, but the

atomic lines interspersed with these have not yet been

fully studied.

2.5 The Identifications: Column Five

The entries in this column consist of both atomic

and molecular lines, each of which can be recognized

easily from their chemical symbols. The wealth of

material collected at The National Bureau of Standards

for the program on Atomic Energy Levels has been used

to revise and extend the identifications of atomic lines. Data were collected for as many atomic spectra as possible, from laboratories engaged in spectroscopy throughout the world. The collaboration of many spectroscopists

has made possible the revisions included in this column.

For each atomic spectrum, the individual lines arranged

by multiplets in order of increasing excitation potential

have been examined in making the final identification

assignments. The intensity behavior in the spot spectrum as compared with the disk has also been a valuable

guide throughout.

For molecular spectra the services of various specialists

in molecular spectroscopy have been solicited. These

identifications have been made not by coincidence of wavelength alone, but rather by a study of the behavior

of the various rotation branches of a given molecular

spectrum. The procedure has been similar to that of

studying multiplet structure for atomic lines. If the

intensities of the solar lines vary consistently with the

observed laboratory intensities along the lines of the

branch, and the wavelengths are in reasonable agreement,

the identifications are considered to be plausible. Further

details are discussed in the descriptions of the last three

columns of the table. §§ 2.6, 2.7, 2.8. Several symbols have been used in column five to ex- plain the identifications in some detail. These symbols

have the following meanings

:

II Parallel lines preceding the chemical symbol indicate

the predominant contributor in the case of a blend.

Example: 4844.022 A HFei

Til

Fe I is the predominant contributor, but Ti i is not

completely masked.

I A single vertical line preceding the chemical symbol

denotes one of the principal contributors to a blend.

Example: 5247.923 A |Co i Cri

Here Co i is a stronger contributor than Cr i.

In cases where more than one identification is given and no such symbols are used, no choice has

been possible as to the leading or predominant

contributor. — A dash is used for blends of three types

:

Example: 5041.450 A -C i Here it is felt that C i does not account fully for

the solar intensity. The dash indicates that the line

is probably a blend. It precedes the "C i" because the

laboratory wavelength is longer than the solar wavelength. The other unknown contributor (s) may well

be a line (or lines) having shorter wavelengths.

Example: 5092.309 1 d—

This blend is similar to the one described above,

except that the C2 laboratory wavelength is shorter

than the solar wavelength. Other contributors may

be on the long-wave side or to the red of the solar

line.

Example: 4466.165 A Cr i—

Fei

In the case of this blend, the Cr i is on the short- wave side of the solar line and Fe i is to longer waves.

( ) Parentheses indicate masked lines. Only more

important masked lines are entered throughout the

solar table. Usually the multiplet evidence indi- cates that the masked line should be present. The

most conspicuous examples occur in the wings of

very strong solar lines. Example: 3933.682 A Ca 11 (K)

(Sc i) (V i) (Co i)

? A question mark denotes that the identification is somewhat dubious.

p Chemical symbols followed by "p" indicate identifi- cations based on wavelengths "predicted" from

known atomic energy levels. Such lines have

mostly not yet been observed in the laboratory, but

the multiplet behavior confirms the suggested solar

identification.

Example: 4481.031 A Fe i p

The method of identifying solar lines by prediction

is particularly fruitful for a spectrum like Fe i. The

solar spectrum still provides more Fe i lines than

have as yet been observed in the laboratory. This

situation indicates the need for reobserving this

complex spectrum with a modern laboratory source, such as an electrodeless discharge. StiU more solar

identifications of Fe i could be made if the analysis were extended by means of a new homogeneous line

list. XVIII
2.6 The Low Excitation Potential or Rotation Line:

Column Six

This column contains two types of data. For atomic

lines, the lower excitation potential of the individual line

is tabulated. This excitation potential is that of the lower

level involved in the transition giving rise to the laboratory

line, expressed in eV. The multiphcation factor used to convert cm~' to eV is 0.00012395. This conversion factor

has been used throughout to obtain all the ionization

potentials listed in the volumes on Atomic Energy Levels

[27]. The excitation energies Hsted in this solar table

appear slightly larger than those in the 1928 edition,

because of the revision in the conversion factor. For molecular lines, this column has been used to enter the rotation branch and quantum number. For example,

the solar line at 4084.327 A is identified as CH. This line in the laboratory spectrum of CH occurs in the "P" branch

and has the quantum number 7, denoted as "P 7" in

column six.

2.7 The Multiplet Number or Vibration Band:

Column Seven

This is arranged similarly to column six. It contains

the multiplet numbers taken from the published Multiplet

Tables. These are old multiplet numbers, but since they

are well established in the literature, every effort has been

made to retain them. In cases where lines have been

added to the multiplet, if the multiplet has been assigned a number, that same number is now used for the additional

lines. For lines longer than 3000 A the Multiplet Numbers are from the Princeton University Observatory

Contribution No. 20, 1945 [28]. For lines short of 3000 A,

the Ultraviolet Multiplet Table has been used, as indicated

by "UV" preceding the Ksted multiplet number [29]. For molecular spectra the vibration bands are indicated in this column. For example, the solar line at 4096.941 A is identified as CN. This line of CN belongs

to the vibration band (1, 2); which is entered in column

seven.

2.8 Notes to the Solar-Spectrum Ledger: Column Eight

The numbers in the last column refer to notes that

follow the solar ledger (pp. 344 to 349). Most of these

are self-explanatory.

Molecular Spectra—Solar Lines

A large number of the notes contain information

regarding the molecular lines present in the solar spectrum. Each classified molecular line has a note number.

For each molecule all lines having the same electronic

transition have the same note number. The note gives

the transition, the vibration bands, the spectral range of the

individual bands from laboratory spectra, and references

used for the material on analysis. Only the bands repre- sented in the present solar ledger are included in the

notes.

Molecular Spectra—Atmospheric Lines

For Atm O2 the limiting range of wavelength is quoted

from the paper on analysis by H. D. Babcock and L. Herzberg [14]. A different note number is used for each

isotope of O, the electronic transition being the same. For the classified lines of atmospheric water vapor,

Atm H2O, the limiting spectral range quoted in the notes is taken from the solar table itself. No attempt

has been made to include a detailed picture of this complex molecule. In general, the identifications of atmospheric lines have been taken from the 1928 [3] and 1947

[11] tables. This has been supplemented by unpublished

data from W. S. Benedict, who has made a most exhaustive study of the bands and has kindly furnished his

analysis for use here. Unclassified atmospheric fines are entered as "Atm",

although they are probably due to the water vapor

molecule.

A summary of the notes referriag to molecular hnes

is given in Table 7

Table 7. Notes on Molecular Lines in the

Solar-Spectrum Ledger

Note Molecule Note Molecule Note Molecule

Number Number Number

1 OH 11 CN (blue) 22 AtmOz 0>«0i« 2 CH 12 CN (red) 23 Atm O2 0'60"

3 CH 19 C2 24 AtmOz Qi^'O" 4 CH 20 MgH 26 Atm H2O

6 NH

Selected Lists of Solar Lines

Six notes give solar wavelengths of lines that are in

special categories (notes 5, 7, 8, 15, 18, 27). Three refer

to pairs of lines: (1) formerly Hsted as double, but re- corded here as single (note 7) ; (2) lines that may be double

but are still unresolved (notes 15 and 18).

There are 223 atomic lines appearing only in the sunspot spectrum. These are included in the main ledger

and listed separately in note 13. They can be detected

readily by the absence of equivalent width data in

columns two and three. Numerous spot fines recorded

in the 1932 survey [15, 16] have siQce been detected on

the Atlas spectrograms as present, also, in the disk spectrum, which explains then- absence from the listing in

note 13 as compared with the 1932 listing [16]. In selecting the atomic fines in the sun-spot spectrum

from the appearance of the Zeeman effect, many cases were noted in which it was difficult to separate atomic

from molecular lines with certainty. In cases where the

spot line is possibly a molecular line, note 16 is entered.

Definite blends of atomic and molecular lines in the spot

spectrum are iadicated by note 17. XIX
Laboratory Wavelengths in the Table

Laboratory wavelengths have been used for higher

members of the Balmer and Paschen series of hydrogen,

because of the diffuseness of these lines in the solar spectrum. The Balmer hnes from Hg through H17 are listed

in note 10; and the Paschen lines from n equals 12 through

18, in note 31. Seven notes contain special comments concerning the

data on widths of lines: (notes 9, 14, 21, 28, 29, 30, 32).

The only "forbidden" hnes entered in the table are those of [O 1] reported by Bowen in 1948 (note 25).

3. General Results

In August 1963 an International Symposium on the

Solar Spectrum was held in Utrecht. One paper on

this program dealt with the present revision of the

solar spectrum, and gave a general account of this solar

program [30]. Since that date a new summary of the

data included in the table, has been prepared.

3.1 Number of Lines

It is interesting to compare the approximate counts

of lines in the present revision with similar counts from

the 1928 edition. The 1963 summary [30] has-been

revised and extended in Table 8. Short of 3061 A and

long of 6600 A, new observations replace those of Rowland.

The counts have been made by regions ia order to emphasize the comparison over the long interval from 3061 A

to 6600 A, where the Rowland Table has not yet been

superseded.

Separate counts have not been made for the 223 atomic

spot lines in the various categories: unblended, blended,

and unidentified. They are included in the overall

counts of lines recorded in Table 8. With the aid of

note 13 the spot lines can be easily segregated and counted.

The last three colimans of Table 8 answer a question

that has been persistent over the years, namely, the

reality of the faintest Rowland lines. Rowland's Table

started at 2975 A; consequently the counts of new lines

short of this wavelength are handled separately. A

glance at the last column of this Table indicates an

important trend. It seems extremely evident that many

more faint solar lines remain to be found and that the

rejections of those now recorded wUl be on the decrease.

Table 8. Counts of Lines in the Solar Ledger

Unblended Blended Unidenti- Total Percentage Range

(A)

New Lines Rowland

Lines

Rejected

Difference

fied Identified Added

Range

(A)

1966 Edition

2935 to 3061 389 114 153 656 77 r 2935 to 2975 \

\ 2975 to 3061 / 14280 37 +43

3061 to 4000 4509 1138 1786 7433 76 165 50 + 115 4000 to 5000 3327 697 2143 6157 65 430 76 +354

5000 to 6600 3372 380 1830 5582 67 604 346 + 258

6600 to 7330 1306 163 356 1825 80

7330 to 8770 1699 303 312 2314 87

2935 to 8770 14G02 2795 6580 23977 73

3061 to 6600 11208 2215 5759 19182 70 1199 472 +727

1928 Edition

2975 to 3061 186 49 236 471 50

3061 to 4000 3527 933 2868 7328 61

4000 to 5000 2440 533 2764 5737 52

5000 to 6600 2725 235 2280 5240 56

6600 to 7330 695 48 504 1247 60

2975 to 7330 9573 1798 8652 20023 57

3061 to 6600 8692 1701 7912 18305 57

XX
The strongest unidentified lines are listed in Table 9. The limiting intensities are 2 on the scale of eye estimates

«3061 1). To Ionger waves the selection is quite arbitrary, since both the measured equivalent width in column

two and the reduced width in column three have been

used as guides. The total number listed is 241.

3.2 Atoms and Ions in the Sun

In 1941, W. F. Meggers published tables of leading

lines in first and second spectra [31]. These tables have

been invaluable for astrophysicists. They have been

quoted for the Ultimate Lines of individual spectra in both the Princeton and the Ultraviolet Multiplet Tables

[28], [29]. Since 1941 our knowledge of atomic spectra

has increased steadUy, and some of the material in these

tables has been superseded. Pending the publication of a complete revision containing the designations and a cur- rent bibliography for the "Raies Ultimes", the leading

lines from his tables, with some revisions and extensions,

are given in Table 10 with the low excitation potential

of the transition giving rise to the line. Wavelengths

in vacuo are denoted by "v" in columns three and nine.

All other wavelengths are in air. Laboratory data are

in columns three and four for first spectra, and nine

and ten for second spectra. The laboratory lines are observed in emission. These are followed by solar data.

Some raies ultimes short of 3000 A are strong solar lines,

as, for example, Lyman a of H i at 1215 A. In Table 10,

however, the solar material is limited to the range of

the present volume, 2935 A to 8770 A, all of which is an absorption spectrum. Special notes refer to spectra

whose lines are known in solar, spot, or chromospheric

spectra, particularly in cases where the lines occur beyond the above ranges. Many absences can be explained from a glance at Table 10. For the less abundant elements having their

ultimate lines in the far ultraviolet, the search for the

element should be made in the ultraviolet solar spectrum. The accessible Knes have high excitation potentials, which is unfavorable for their appearance. This was pointed out by H. N. Russell in 1929 [32], as was,

also, the greater abundance of elements having even

atomic numbers.

3.3 Molecules in the Sun

A general survey of this subject was presented by H. P. Broida and C. E. Moore at a symposium in Liege in

1957 [33]. They prepared tables giving counts of the

lines of the various bands of CH, OH, and CN present

in the sun [34]. Two subsequent papers give the detailed

identifications of CH [34] and OH [35] in the solar ledger.

A later summary of the solar lines of molecular origin,

in the range of the present ledger, was given in Utrecht

in 1963 [30]. In 1964 the general question of Molecules

in the Sun, including spot spectra and the infrared solar

spectrum was discussed at the Florence symposium

honoring Galileo [36]. To this should be added the

recent identification by L. Goldberg and his associates

[37] of CO in the solar spectrum near 1600 A. The

molecules identified to date from a detailed study of

the laboratory observations and analysis are listed briefly

in Table 11 [36]. The present identifications of Cz can be extended when

the Berkeley Monograph on this molecule has been completed. Further study is also needed on SiH; this molecule may be present in the disk spectrum.

3.4 Summary of Identifications

It is well known that some spectra, like Fe i, are well

represented in the sun. This laboratory spectrum can be matched line for line in both position and relative

intensity with a solar line. Other less abundant elements

have only their leading lines present in the sun, as, for

example Ag i. In order to summarize the present identifications, counts have been made of the number of lines of each spectrum contained in this compendium. These

are recorded in Table 12. The spectra are in order of in- creasing atomic nmnber. The counts are by regions, and

the blended and unblended lines in the solar spectrum

have been counted separately. Blended lines are solar

lines having more than one contributor to the identifi- cation, as, for example:

4046.341 A Ceil

V II

4043. 768A —Ti i Masked lines, entered in parentheses in the ledger, are not included in the counts. Lines whose identifications are subject to question are counted in with the others.

Counts for spot lines are included.

Finally, a condensed summary of aU elements present

in the sun is contained in Table 13. The results given

here are based on material over the entire spectral range,

i.e. from the far ultraviolet solar spectrum to the infrared.

In preparing Table 13 one of the authors (C.E.M.) has

had the benefit of communication with R. Tousey re- garding identifications in the short-wave region. The

notes to Tables 10 and 13 indicate cases where the evidence

rests upon observations beyond the range of the present

work.

There are 63 elements proven as present without doubt

in the sun. Of these, the spectroscopic evidence is least certain for Os and Ir, but the data from the accessible

region are more favorable for these elements than for

the two elements (Tb and Er) listed as dubiously present.

Both Au and Cd were formerly identified from one Hne

each, in the accessible region. R. Tousey [38] reports

additional confirmation for these elements from the

presence of the raies ultimes in the short-wave region.

The raie ultime of Pt i is also present [38]. One element,

Ne, was fiirst detected from the ultraviolet rocket solar

o spectrum, where the resonance Lines of Ne viii near 780 A, were identified [38]. The element Ar was first found

XXI
Table 9. The Strongest Unidentified Solar Lines

Wavelength

Estimated

Intensity

Wavelength

Equivalent WidthReduced

Width

Wavelength

Equivalent WidthReduced

Width

Wavelength

Equivalent WidthReduced

Width

2942. 85

2975. 038

2984. 574

2987. 052

2990. 876

[5d?]

[2]

[2]

[2]

[2]

3088. 188

3088. 355

3088. 752

3089. 505

3091. 693

64

101 105

66

45

34. 0

32. 7

54. 2

21. 5

32. 0

3618. 523

3618. 999

3619. 114

3621. 105

3631. 265

1231

1284

35

20. 2

43. 2

21. 8

25. 3

45. 4

3935. 216

3937. 974

3947. 693

3965. 930

3967. 636

6 28

4525

7

22. 4

28. 8

21. 6

30. 2

26. 4

2991. 774

2993. 798

2995. 494

2996. 849

2997. 222

[4]

[4] [2]

[2] [2An

3091. 876

3092. 473

3097. 785

3099. 790

3101. 417

96

6366

44

88

31. 2

29. 2

23. 5

47. 2

47. 4

3631. 586

3634. 412

3638. 104

3648. 082

3649. 837

103678**

24

75

31. 2

22. 8

21. 1 34. 5

26. 7

3967. 859

3968. 715

3968. 936

4001. 163

4004. 915

7. 5 3

6 127**

72. 5

29. 5

20. 6

37. 2

27. 2

24. 1

2998. 152

2998. 966

3000. 339

3001. 791

3006. 573

[2]

[2] [2]

[3] [4d]

3101. 694

3101. 974

3113. 838

3119. 198

3130. 631

97

4566

77

63

77. 4

26. 2

21. 1 24. 8

32. 7

3688. 804

3730. 308

3735. 118

3735. 244

3736. 712

7238

6. 5 14

12

24. 6

21. 7

42. 8

56. 0

29. 2

4005. 072

4007. 926

4009. 146

4015. 611

4017. 573

52

6853

88

74

26. 5

17. 0

13. 2

21. 9

18. 4

3007. 96

3008. 470

3016. 872

3017. 418

3017. 854

[3iV"Ar|

[3] [3]

[3] [2]

3148. 900

3152. 000

3179. 166

3183. 05

3186. 86

67

75

7347

98

21. 4

23. 8

45. 4

22. 6

43. 0

3737. 032

3737. 299

3743. 218

3745. 349

3749. 244

10

4. 5 25

(68) # 46

67. 0

31. 6

22. 2

(72. 5)# 103

4020. 272

4025. 823

4033. 588

4045. 715

4045. 968

107**

64

46

7. 5

14

18. 2

15. 2

11. 4

13. 3

23. 0

3023. 068

3024. 242

3024. 802

3027. 016

3027. 699

[3]

[2]

[3]

[2]

[2]

3186. 964

3196. 195

3196. 835

3199. 662

3205. 223

6433

48

5566

28. 7

21. 3

30. 4

21. 4

25. 2

3749. 365

3749. 740

3749. 850

3757. 959

3758. 437

4

15

7. 5 29

15

31. 2

33. 4

22. 7

37. 2

38. 6

4063. 789

4066. 120

4132. 711

4146. 990

4167. 722

1948

40

45

44

18. 7

10. 8

10. 2

10. 8

10. 6

3028. 869

3029. 000

3029. 990

3034. 60

3037. 23

[2] [2N]

[3]

[3] [3]

3211. 634

3215. 844

3222. 944

3225. 712

3227. 631

73

69

24

33

46

40. 6

21. 5

25. 3

57. 7

38. 3

3763. 008

3763. 979

3766. 968

3767. 081

3767. 356

53

1624

7

18

21. 2

33. 8

27. 5

23. 9

34. 5

4181. 974

4219. 199

4226. 970

4227. 321

4231. 954

9342

4544

45

22. 2

10. 0

55. 8

28. 9

10. 6

3040. 761

3041. 038

3044. 228

3051. 04

3053. 744

[2]

[2] [2N]

[3] [2]

3281. 716

3286. 628

3289. 027

3305. 864

3306. 093

70

414844

65

21. 5

31. 0

33. 8

24. 5

27. 3

3780. 706

3792. 686

3794. 887

3795. 155

3796. 803

110 121**

14 547**

33

36. 2

36. 0

24. 0

20. 6

26. 0

4299. 831

4300. 744

4302. 65

4308. 289

4337. 252

93

3343

3146

21. 6

11. 8

19. 5

12. 8

12. 2

3057. 963

3058. 706

3060. 773

[3] [3]

[2]

3315. 420

3335. 923

3336. 831

7450

32

34. 3

21. 6

41. 3

3815. 328

3815. 617

3820. 056

27

3827

21. 7

58. 7

41. 6

4393. 284

4401. 022

4403. 187

46

5862

10. 5

13. 2

14. 5

Wavelength

Equivalent Width

Reduced

Width

3344. 936

3349. 266

70

19

21. 1 27. 7

3820. 196

3824. 573

1384

43. 7

97. 5

4518. 342

4599. 843

40

56

10. 0

12. 2

3062. 83

3064. 015

3064. 515

3064. 829

3068. 476

55

1476580

75

21. 5

48. 0

21. 2

26. 2

24. 6

3360. 351

3369. 665

3380. 313

3391. 107

3392. 894

36

33

7636

17

22. 9

77. 1 43. 4

31. 9

26. 2

3826. 026

3827. 692

3828. 019

3829. 250

3832. 510

7

6. 5 24

10

9. 5

26. 9

21. 9

33. 9

32. 4

27. 6

4672. 334

4678. 172

4699. 340

4748. 141

4771. 472

56

6264

7870

12. 0

13. 2

13. 6

16. 4

14. 7

3069. 334

3074. 07

3075. 035

3075. 455

3075. 595

5782

50

39

78

20. 4

30. 3

24. 7

22. 6

49. 0

3414. 511

3414. 918

3415. 098

3440. 099

3440. 192

53

49

1525

26

34. 2 157

24. 9

22. 1 31. 0

3834. 10

3836. 920

3838. 208

3840. 303

3840. 583

20

34

3

1226

43. 1 20. 8

23. 5

25. 0

40. 4

4971. 351

5053. 577

5271. 054

5298. 497

5341. 151

55

50

3165**

180**

11. 1 9. 9

5. 9

11. 9

10. 2

3078. 915

3079. 105

3080. 877

3081. 725

3082. 38

52

7865

120

64

21. 4

25. 5

27. 8

39. 0

24. 5

3442. 148

3458. 594

3461. 796

3466. 002

3475. 519

34

3232

2422

20. 5

37. 6

30. 9

22. 5

74. 0

3841. 190

3859. 400

3859. 741

3881. 980

3884. 292

143920

5666**

25. 5

32. 6

45. 8

31. 2

23. 4

5390. 527

5418. 775

5421. 178

5654. 501

6020. 016

30

49

44

75

49

5. 6

8. 7

8. 1 13. 3

8. 1

3083. 850

3085. 043

3085. 395

3085. 720

3086. 988

3087. 693

40

64

58

79

16158

24. 0

20. 7

23. 5

25. 6

52. 2

25. 3

3492. 369

3492. 815

3504. 684

3505. 294

3524. 358

3610. 508

60

23

70

92

16 250**

21. 5

20. 2

20. 0

26. 2

24. 6

42. 6

3903. 854

3911. 989

3921. 187

3927. 797

3929. 357

3930. 150

224**

76

59

42

24

26

25. 0

25. 6

24. 0

41. 7

27. 7

40. 8

6299. 588

6449. 127

7032. 319

7375. 251

7435. 584

3634

33

4532

5. 7

5. 3

4. 1

6. 1 4. 3

**Blend. #Parentheses indicate that the equivalent width could not be measured directly. See p. XVI.

XXII
as [Ar x] in the coronal spectrum. The only radioactive

element known to be present is Th; here the raie ultime

of Th II provides the only evidence.

Two elements, Tb and Er, are listed as questionably

present. For both Tb ii and Er ii, the behavior of the

lines in the flash spectrum as having the rare-earth

characteristic described by Menzel [40], has been a guiding

factor in assigning identifications.

No positive statement can be made about the four

elements in the category "Further study needed". The

presence of BH has been reported, but further data are needed [33]. The strongest lines of B i He near 2500 A.

Because of blending they can neither be clearly identified nor ruled out as definitely absent [38]. Sixteen elements are listed as absent on the basis of

spectroscopic study. Two, Tc and Ta, have been added

to this group as a result of additional solar observations.

R. Tousey finds no evidence of the presence of the leading

Tc II multiplet near 2600 A. The strong Ta i line at 2714 A is masked and other strong lines are absent [38]. Further laboratory work on the lanthanon group of rare earths may add to line identifications in spectra of

elements known to be present, and may increase the

number of rare-earth elements present. The third

spectra of these elements extend into the infrared and

may weU be of astrophysical importance. Only one third

spectrum is mentioned in the present table, namely

Ce III. In this spectrum the strongest accessible line is at 3055.589 A, and it may explain the chemical origin of

the faint solar fine observed at 3055.594 A.

Table 10. Leading Lines in First and Second Spectra

Laboratory Sun-Present Volume Laboratory Sun-Present Volume z

Sp X

(A)

Low

E P

X Reduced

Width

Low

E P

Sp X

(A)

Low

E P

X

(A)

Reduced

Width

Low

E P

1 m I 1215. 668v^ 0. 00 6562. 808 649 10. 20

2 He I 584. 334v^ 0. 00 <He II 303. 780v.'^ 0. 00

3 Li I 6707. 761 0. 00 6707. 76A 0. 2 0. 00 Li II 199. 282v 0. 00

4 Be I 2348. 610 0. 00 3321. 352 2. 7 2. 72 Be II 3130. 420 0. 00 3130. 414 27. 3 0. 00

5 B I 2497. 725 0. 00 B II 1362. 460v 0. 00

6 C I 1657. OOSv 0. 01 8335. 150 13. 7 7. 68 C II 1335. 708v 0. 01

7 N I 1134. 979v 0. 00 8683. 384 0. 9 10. 33 N II 1085. 701v 0. 02

8 0 I 1302. 169v 0. 00 7771. 954 9. 14 0 II 834. 467v 0. 00

9 F I 924. 825v 0. 00 F 11 606. 81 v 0. 00

10 Nei 735. 892v 0. 00 Ne II 460. 725v 0. 00

11 Na I 5889. 953 0. 00 5889. 973 120 0. 00 Na II 372. 069v 0. 00

12 Mg I 2852. 127 0. 00 3838. 302 641 f2. 72

\2. 72 Mg II 2795. 528 0. 00 4481. 140 14. S 8. 86

13 Al I 3961. 520 0. 01 3961. 535 220 0. 01 Al II 1670. 786v 0. 00 3900. 660? 7. 1 7. 42

14 Si I 2516. 112 0. 03 3905. 532 219 1. 91 Si II 1533. 445v 0. 04 3856. 026 26. 0 6. 86

15 P I 1774. 942v 0. 00 P II 1542. 321v 0. 06

16 S 1 1807. 341v 0.00 8694. 641 3.9 7. 87 S n 1259.53 V 0. 00

17 CI I 1347. 238v 0. 00 CI II 1071. 036v 0. 00

18 Ar I 1048. 219v 0. 00 Ar II 919. 782v 0. 00

19 K I 7664. 899 0. 00 7698. 977 19. 4 0. 00 K II 600. 765v 0. 00

20 Ca I 4226. 728 0. 00 4226. 740 0. 00 Ca II 3933. 663 0. 00 3933. 682 (4874) 0. 00

21 Sc I 3911. 810 0. 02 3911. 825 18. 2 0. 02 Sc II 3613. 836 0. 02 \ 3613. 809

; 3613. 881

29. 6 "I 29. 6 J

0. 02

22 Ti I 3653. 497 0. 05 3729. 813 39. 4 0. 00 Ti II 3349. 399 0. 05 3349. 447 163 0. 05

23 V I 3185. 396 0. 07 3185. 388 38. 8 0.07 V n 3093. 108 0. 39 3556. 803 55. 7 1. 13

24 Cr I 3578. 682 0. 00 3578. 693 142 0. 00 Cr II 2055. 59 0. 00 3368. 058 56. 3 2. 48

25 Mn I 4030. 755 0. 00 4030. 763 75. 2 0. 00 Mn II 2576. 106 0. 00 3441. 982 107 1. 78

XXIII
Table 10. Leading Lines in First and Second Spectra—Continued

Laboratory Sun-Present Volume Laboratory Sun-Present Volume z

Sd X Low \ Reduced Low Sd X Low X Reduced. Low

(A) E P (A) Width E P (A) E P (A) Width E P

26 Fe I 3719. 934 0. 00 3734. 874 945 0. 86 Fe II 2382. 034 0. 00 3196. 106 76. 7 1. 67

27 Co 1 3453. 516 0. 43 3453. 512 87. 9 0. 43 Co II 2286. 165 0. 42 3387. 718 15. 2 2. 27

28 Ni I 3414. 764 0. 03 3524. 536 363 0. 03 Ni II 1751. 914v 0. 00 3407. 314 26. 0 3. 08

29 Cu I 3247. 538 0. 00 3247. 569 76. 0 0. 00 Cu II 1358. 764v 0. 00

30 Zn I 2138. 56 0. 00 3345. 024 21. 4 4. 08 Zn II 2025. 512 0. 00

31 Ga I 4172. 056 0. 10 4172. 053 13. 9 0. 10 Ga II 1414. 44 V 0. 00 32 Ge I 2094. 258 0. 17 4226. 568 53. 2 2. 03 Ge II 1649. 192v 0. 22

33 As I 1890. 42v 0. 00 As II 1266. 36 V 0. 31 34 Se I I960. 901v 0. 00 Se II 1192. 29 V 0. 00

35 Br I 1488. 452v 0. 00 Br II 1036. 983v 0. 00

36 Kr I 1164. 868v 0. 00 Kr II 917. 434v 0. 00

37 Rb I 7800. 227 0. 00 7800. 29A 0. 6 0. 00 Rb II 697. 04 V 0. 00

38 Sr I 4607. 331 0. 00 4607. 338 7. 8 0. 00 Sr II 4077. 714 0. 00 4077. 724 100 0. 00

39 Y I 4102. 38 0. 07 3620. 971 8. 2 0. 07 Y 11 3710. 30 0. 18 3664. 623 31. 4 0. 18

40 Zr I 3601. 18 0. 15 3575. 765 9. 5 0. 07 Zr II 3391. 96 0. 16 3165. 958 26. 7 0. 16

41 Nb I 4058. 933 0. 13 3802. 959 7. 1? 0. 09 Nb II 3094. 172 0. 51 3619. 536 17. 0 0. 98

42 Mo I 3798. 249 0. 00 5533. 039 1. 3 1. 33 Mo II 2020. 32 0. 00 3320. 915 2. 6 3. 11

43 Tc I 3636. 070 0. 32 Tc II 2543. 227 0. 00

44 Ru I 3498. 944 0. 00 3728. 042 20. 0 0. 00 Ru II 1574. 337v 0. 00 3177. 080 4. 6 2. 40

45 Rh I 3434. 893 0. 00 3434. 896 3. 6 0. 00 Rh II 1607. 86 V 0. 00 3187. 899 4. 2 3. 45

46 Pd I 3404. 580 0. 81 3404. 584 10. 6 0. 81 Pd II 1363. 76 V 0. 00

47 Aff I 3280. 682 0. 00 3280. 681 15. 3 0. 00 Asr II 1112. 46 V 0. 00

48 Cd I 2288. 018 0. 00 3261. 065 7. 0 0. 00 Cd II 2144. 408 0. 00

49 In I 4511. 323 0. 27 4511. 31A 0. 4 0. 27 In II 1586. 37 V 0. 00

50 Sn I 2839. 99 0. 42 3801. 025 2. 5 1. 07 Sn II 1899. 890v 0. 53

51 Sb I 2068. 33 0. 00 3267. 539 3. 5 2. 03 Sb II 1438. 11 V 0. 00

52 Te I 2142. 75 0. 00 Te II 1404. 65 V 0. 00

53 I I 1782 758v 0. 00 I II 1220 887v 0. 00

54 Xe I 1295 5S7v 0. 00 Xe II 1100 432

V

0. 00

55 Cs I 8521 133 0. 00 Cs II 813 85 V 0. 00

56 Ba I 5.'i3,'i 484 0. 00 5535 51 la 0. 00 Ba II 4554 033 0. 00 4554 036 S6. 7 0. 00

57 La I 5249. 929 0. 51 6249. 91 0. 1 0. 51 La II 3949. 10 0. 40 0/94. i i6 d4. O

n OA U. ^4

58 Ce I 5699. 226 Ce II 4186. 599 0. 86 3560. 802 13. 7 0. 68

59 Pr I 495L 355 0. 00 Pr II 4100. 746 0. 55 3994. 810 3. 9 0. 05

60 Nd I 4924. 516 0. 00 Nd II 4303. 573 0. 00 4303. 595 15. 1 0. GO

61 Pm I 4781. 291 0. 00 Pm II 3998. 961

62 Sm I 4296. 743 0. 50 Sm II 3568. 271 0. 48 3735. 964 18. 0 0. 28

XXIV
Table 10. Leading Lines in First and Second Spectra—Continued

Laboratory Sun-Present Volume Laboratory Sun-Present Volume z

Sp X(A)

Low

JCj Jr X

(A)

Reduced

Wiatli Low

XL; r

Sp X

(A) Low

E P

X

(A)

Reduced

Width

Low

E P

63 Eu I 4594. 03 0. 00 4627. 221A 0. 9 0. 00 Eu II 3819. 67 0. 00 3819. 688 28. 2 0. 00

64 Gd I 4225. 850 0. 21 Gd II 3422. 466 0. 24 3100. 524 69. 0 ? 0. 24

65 Tb I Tb II 3568. 55 ? A 1. 8 66 Dy I Dy II 3407. 805 18. 8 0. 00

67 Ho I Ho II

68 Er I 4007. 97 0. 00 Er II 3896. 248 ? 8. 7 0. 05

69 Tm I 4094. 188 0. 00 4094. 20 ? 0. 9 0. 00 Tm II 3848. 02 0. 00 3462. 213 4. 0 0. 00

70 Yb I 3987. 98 0. 00 3987. 966A 5. 0 0. 00 Yb II 3694. 19 0. 00 3694. 199 25. 6 0. 00

71 Lu I 3359. 56 0. 25 Lu II 2615. 42 0. 00 3397. 062 12. 1 1. 46

72 Hf 1 2916. 48 0. 57 3616. 878 0. 1 0. 29 Hf II 3399. 793 0. 00 3505. 232 8. 3 1. 04

73 Ta I 2714. 66 0. 00 Ta n 2400. 62 0. 77

74 W I 4008. 753 0. 37 3207. 248 4- 0 0. 37 W II 2204. 482 0. 76

75 Re I 3460. 465 0. 00 Re II 1973. 13 V 0. 00

76 Os I 2909. 061 0. 00 3232. 076 5. 8 0. 52 Os II

77 Ir I 2543. 971 0. 35 3220. 775 10. 5 0. 35 Ir II

78 Pt I 2659. 454 0. 00 3064. 713 53. 6 ? 0. 00 Pt II 1777. 086v 0. 59

79 Au I 2427. 95 0. 00 3122. 784 ? 1. 6 1. 14 Au II 1224. 57 V 0. 00

80 Hgi 1849. 499v 0. 00 Hg II 1649. 939v 0. 00

81 Tl I 3519. 24 0. 97 Tl 11 1321. 71 V 0. 00

82 Pb I 2833. 067 0. 00 3683. 480 3. 9 0. 97 Pb II 1682. 15 V 0. 00

83 Bi I 3067. 732 0. 00 Bi II 1436. 83 V 0. 00

84 Po I 2450. 11 0. 00 Po II

85

86

At I Rn I

2244. 01

1786. 07 V

0. 00

0. 00

At II Rn II

87

88

Fr I Ra I 4825. 91 0. 00

Fr II Ra II 3814. 42 0. 00

89 Ac I 4179. 98 0. 00 Ac II 4507. 20 0. 00

90 Th I 3719. 435 0. 00 Th II 4019. 129 0. 00 4019. 136 2. 1 0. 00

91 Pa I Pa n •

92 U I 3584. 88 0. 00 U II 3859. 580 0. 04

AProminent in the ultraviolet region of the solar spectrum. Lines of He i and He ii conspicuous in the spectrum of the chromosphere.

AProminent in the sun-spot spectrum.

First identified in the sun from strong lines near X10500. H Present only in the spot spectrum.

AIdentification doubtful; Tb ii lines may account for some lines observed in the spectrum of the chromosphere.

XXV
Table 11. Molecules in the Sun—Summary

Spectrum Molecule Number

Disk OH CH NH C2 CN CO MgH 7 Spot CH C2 CN MgH CaH SiH TiO ZrO 8

Disk and Spot CH C2 CN MgH 4

Total No.

Total No.

represented from detailed reported prior to 1964

study of lines 1128

Table 12. Counts of Lines of Individual Spectra in the Solar Ledger

Range (A) 2935 to 3061 3061 to 4000 4000 to 5000 1 5000 to 6600 6600 to 7330 7330 to 8770 2935 to 8770

Sp. i Unblended

Blended Unblended

Blended UnblendedBlended UnblendedBlended UnblendedBlended UnblendedBlended Unblended

Blended

H 11 3 1 4 19

Li I 2 2 Be I Be II

122 12

2

C I 1 1 1 9 2 16 3 15 5 10 5 52 16 N I 9 4 9 4 0 I 2 5 1 1 1 4 2 12 4 Nai 2 12 3 8 2 24 3 Mg I Mg 11 1 2 17

2

2 12

2

9 1 5 1 24

2 41 67

7

10

1 Al I Al II 2 1 5

1 3 1 1 4 1 5 2 17

1 8

Si I Si II 4 12 1 24 4

1 50

3

13 33 6 64 25 176

5 482 P I 1 1 1 1 2 S I 4 5 4 5 2 13 5 27 11 K I 1 2 6 1 1 1 1 10 3 Ca I Ca II 4 1 39

7 17 34

2

5

1 47

5

3

1 6 1 6

5

5

1 13619 32

3 Sc I Sc II

12 3

1 4

18

2

12

1314

65 33

19

72 1 5154

1820

Ti I Ti II 6

9

910141 14084

72 275

70 98

24 23116

31

4 232 10 61 27

1 737

237

259

111 V I Vii

1830721 71 110 65

78

128

29 5721 9914

14

7

9 1 7 5 332

183 149127 Cr I Cr II 32

37

8

11 211125 11583 346

38

126

16 18027

39

5 25 5 15 9 809227

302

115 Mn I Mn II 1610

77 94

18 42

2 79

3 20

2 31 11 3 1 8 231

31

81

11 Fe I Fe II 11433 50

25 1517

150 39479 1075

76

241

16 869

73

135

23 237

5 543 2147 635 4026

344

937

151 Co I Co II 14 7 277

15 1277 912 32 95 23 12 3 19 10 508

17 202

7 Ni I Ni II 19

1 31 220

10 726 167

3 60 172 25 40 9 42 6 660

14 175

7

XXVI
Table 12. Counts of Lines of Individual Spectra in the Solar Ledger—Continued

Range (A) 2935 to 3061 3061 to 4000 4000 to 5000 5000 to 6600 6600 to 7330 7330 to 8770 2935 to 8770

Sp. i Unblended

Blended Unblended

Blended UnblendedBlended UnblendedBlended Un- Blended

blended

Un- Blended

blended Unblended

Blended

Cu I 2 2 4 1 5 6 2 19 3 Zn I 4 2 5 1 10 2 Ga I 1 1 1 1 Ge I 1 1 1 1 1 3 2 Rb I 2 2

Sr I Sr II 2

1 2

2

93 1 6 2 194

2

3 Yi

Y II 2

1 25

1 1519

12

347

11

6

6

1 2 4 1 1 28

55

1226 Zr I Zt II

1 12 3

9

16 109 20

54 3530

142427

5 43

6 1 1 1 7 5

1 92

157 47

92 Nb I Nb II 3

4

13

18

6 2

1

1 1 1116 4

9 Mo 1 Mo II 1 2

7 42

8

1 21 5 1 15

9 7

3 Hu I Bu II 12

2

5810

1 31

1 1 23

3

99 Rh I Rh II

11 132

2

2

3 1 15

3

5

2 Pd I 1 7 6 1 8 7 Ag I 2 2 Cd I 1 1

In I 1 1 Sn I 1 1 1 2 1 Sb 1 2 2 Ba I Ba II 1 4

2

2 1 2

7 1 La I La II 12 6 16 15

1 10 3 1

1 39 24 €e II Ce III 2

1 36 32 49 32 13 2 100

1 66

Pr II 3 3 4 3 6 13 6 Nd n 18 14 26 14 24 6 68 34 Sm II 39 31 44 16 1 1 1 85 48

Eu I Eu II 1 6 4

2

3 1 1 1

2

11 6 Gd n 4 1 25 11 9 8 1 1 39 21 Tb II 3 1 1 4 1 Dy II 31 13 4 3 3 1 1 39 17 Er II 1 1 Tm I Tm n 6 3

2

1 1 2

7 4 Yb I Yb II

11 1

1 1

1

1

1

XXVII
Table 12. Counts of Lines of Individual Spectra in the Solar Ledger—Continued

Range (A) 2935 to 3061 3061 to 4000 4000 to 5000 5000 to 6600 6600 to 7330 7330 to 8770 2935 to 8770

Sp. i Un- Blended

blended

Unblended

Blended UnblendedBlended Un- Blended

blended

Un- Blended

blended

UnblendedBlended UnblendedBlended

Lu II 1 2 1 2 Hf I Hf II 2

11 4 2 1 2 214 24 W I 2 4 3 2 2 2 8 7 Os I 1 3 1 1 1 4 3 In 4 2 3 1 7 3 Pti 1 1 3 1 3 3 Au I 1 1 Pbi 1 1 1 1 Th II 1 1 CH 100 102 304 214 404 316

CN 428 207 88 62 18 12 105 35 396 221 1035 537

C2 99 18 348 90 447 _ 108 NH 159 106 159 106 MgH 2 81 31 83 31 OH 4 164 127 168 127 Atm 283 53 186 45 106 46 575 144 Atm H2O 407 44 410 84 439 93 1256 221 Atm O2 81 8 158 11 222 3 461 22

Total 391 195 4507 2079 3327 1192 3372 627 1306 287 1699 554 14602 4934

Total 586 6586 4519 3999 1593 2253 19536

Table 13. Chemical Elements in the Sun

Classification Element No.

Present H He Li Be C N 0 Nei Na Mg Al Si P S Ar2 K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge Rb

Sr Y Zr Nb Mo Ru Rh Pd Ag Cd In Sn Sb Ba La

Ce Pr Nd Sm Eu Gd Dy Tm Yb Lu Hf W Os Ir Ft Au Pb Th 63

Present ? Tb Er 2

Further study needed B3 As Ho Hg 4

Absent F 4 CI Se Br Kr Tc Te I Xe Cs Ta Re Tl Bi Ra U 16

Not to be expected Remaining radioactive elements

' Evidence based on discovery of Ne vin and Ne vii in the UV spectrum [38].

2 Evidence based on discovery of [Ar x] in the coronal spectrum [39].

* BH has been reported as present, but further evidence is needed [33].

* No atomic lines present. MgF has been reported as present but further evidence is needed [33].

XXVIII
4. References

1. Trans. Intern. Astron. Union 7, 63, 131 (1950).

2. H. A. Rowland, Astroph. J. 1, 3, 3, 4, 5 (1895 to 1897).

3. C. E. St. John, C. E. Moore, L. M. Ware, E. F. Adams, H. D.

Babcock, Carnegie Inst. Wash. Publ. No. 396; Papers Mt.

Wilson Obs. IH, 238 pp. (1928).

4. G. F. W. Mulders, Zeit. Astroph. 8, 62 (1934) ; Improved dia- gram in Dissertation, Utrecht (Nijmegen, De Gelderlander

1934).

5. M. Minnaert, G. F. W. Mulders, and J. Houtgast, Photometric

Atlas of the Solar Spectrum 33S2 A to 8771 A, Amsterdam,

Schnabel (1940).

6. M. Minnaert and Staff, Preliminary Photometric Catalogue oj

Fraunhofer Lines \3164-\8770, Rech. Astron. Obs. Utrecht 15, 166 pp. (1960).

7. Trans. Intern. Union for Coop, in Solar Research 3, 18 (1907);

3, 134 (1910); Trans. Intern. Astron. Union 1, 35 (1922); 3, 188 (1925).

8. K. Burns and W. F. Meggers, Publ. Allegheny Obs. 6, No. 7, 105 to 124 (1925). (Standards 4073 A to 4754 A) K. Burns and C. C. Kiess, ibid. 6, No. 8, 125 to 139 (1927).

(Standards 5805 A to 7142 A) K. Burns, ibid. 6, No. 9, 141 to 150 (1927). (Standards 3592 1

to 4107 A; 4761 A to 5892 A)

9. Trans. Intern. Astron. Union 7, 150, 151 (1950).

10. W. F. Meggers, Publ. Allegheny Obs. 6, No. 3, 13 to 44 (1919).

(6500 A to 9000 A)

11. H. D. Babcock and C. E. Moore, Carnegie Inst. Wash. Publ.

579; Papers Mt. Wilson Obs. VII, 95 pp. (1947). (6600 A to 13495 A)

12. H. D. Babcock, C. E. Moore, and M. F. Coffeen, Contr. Mt.

Wilson Obs. No. 745; Astroph. J. 107, 287 to 302 (1948). (2935 A

to 3060 A)

13. R. Zalubas, Astroph. J. 133, 544 to 548 (1956) ; and Dissertation,

Georgetown University, unpublished, June 1955.

14. H. D. Babcock and L. Herzberg, Contr. Mt. Wilson Obs. No.

750; Astroph. J. 108, 167 to 190 (1948).

15. C. E. Moore, Contr. Mt. Wilson Obs. No. 446; Astroph. J. 75, 222 to 273 and 298 to 336 (1932).

16. C. E. Moore, Atomic Lines in the Sun-Spot Spectrum, 47 pp, published in Princeton by the Princeton University Observatory and the Mount Wilson Observatory, 1933.

17. R. S. Richardson, Unpublished material, 1932.

18. See Trans. Intern. Astron. Union 7, 70, 398, 403 (1950).

19. G. Bruckner, Photomelrischer Atlas des Nahen Ullraviolelten Sonnenspektruma 2988 A-3629 A (Gottingen, Vaudenhoeck

and Ruprecht 1960).

20. R. Michard, Bull. Astron. Inst. Netherlands 11, 227 (1950^

21. W. Rauer, Zeit. Astroph. 37, 1 (195.5). 22. C. Pecker, Ann. d'Astrophys. 30, 196 (1957).

23. J. Houtgast, Proc. Acad. Amsterdam 68, 306 (196.5). 24. J. Houtgast and M. G. J. Minnaert, Pv-ech. Obs. Utrecht 13

(2), (1951); Introduction. A. D. Thackeray, Astroph. J. 84,

433 (1936).

25. A. Unsold, Physik der Sternatmosphdren § 122, 501 to 508

(Berlin, Springer 1955).

26. E. Vitense, Zeit. Astroph. 38, 81 (1951).

27. C. E. Moore, Atomic Energy Levels, Circ. Nat. Bur. Std 467,

Vol. I (1949); Vol. II (19.52); Vol. Ill (19.58). 28. C. E. Moore, A Multiplet Table of Aslrophysical Interest, Reprinted as Tech. Note 36, PB 151395 (1959), Department of Commerce, Clearing House for Federal and Scientific Information, 5285 Port Royal Road, Springfield, Va.

29. C. E. Moore, An Ultraviolet Multiplet Table, Circ. Nat. Bur.

Std. 488, Sec. 1 (1950); Sec. 2 (1952); Sec. 3, 4, 5 (1962).

30. C. E. Moore-Sitterly, Proc. Utrecht Symposium of Aug. 1963,

ed. by C. de Jager, 89 to 101 (1964). A misprint appears in this paper; in Table 8, the total count of spot lines exceeds 200.

31. W. F. Meggers, J. Opt. Soc. Am. 31, 605 to 611 (1941); ibid. 31, 39 to 46 (1941).

32. H. N. Russell, Astroph. J. 70, 11 to 82 (1929).

33. H. P. Broida and C. E. Moore, Mem. Soc. R. Sc. Lifege [4] 18, 217 to 230 (1957); ibid. pp. 252 to 263 (1957).

34. C. E. Moore and H. P. Broida, J. Res. Nat. Bur. Std. 63A, 19

to 53 (1959).

35. C. E. Moore and H. P. Broida, J. Res. Nat. Bur. Std. 63A, 279

to 295 (1959).

36. C. E. Moore-Sitterly, Proc. Meeting on Sunspots, Florence,

9-12 Sept. 1964, Publ. Natl. Committee commemorating IV

Centen. Birth Galileo 3, 181 to 185 (1966).

37. L. Goldberg, W. H. Parkinson, and E. M. Reeves, Astroph. J. 141, 1293 to 1295 (1965).

38. R. Tousey, Private communication (Dec. 1965) ; See, also, Quarterly J. Roy. Astron. Soc. 5, 132 to 144 (1984) and Space

Science Rev. 3, 45 to 52 (1963).

39. B. Edl6n, Zeit. Astroph. 33, 62 (1942).

40. D. H. Menzel, Publ. Lick Obs. 17, Part I, 8 (1931).

XXJX
5. The Solar Spectrum Ledger

5.1 Letters, Symbols, and Special Signs

For ready reference the letters and symbols used in

this ledger are listed below with brief descriptions. They

are explained fully in the text.

Wavelengths: Column one (see Table 5, p. VIII) S Standard Wavelength

m Measured lines; not taken from Rowland's Table.

r Wavelength from Rowland's Table (corrected to 1928 scale). a Wavelengths from Atlas Recordings and Atlas Spectrograms.

Equivalent and Reduced Widths: Columns two and three (seep. XVI)

Horizontal separation indicating overlap between successive

plates in region where telluric lines occur. 5 Unresolved blend; equivalent width refers to the total blend.

1 51 Partial blend with adjacent faint lines; equivalent width

refers to the line alone.

1 Lines not analyzed in column two. Equivalent width reJ lates to the blend as a whole. 5 The reduced width, when entered in italics, is the weighted mean of Utreclit measurements and of those by other

observers.

( ) Equivalent width not directly measured; derived by inter- polation, from multiplets, or from Rowland's estimated

intensities.

On page 78 the discontinuity in the Balmer continuum

near 3646 A is thus indicated.

Behavior in Sunspots: Column four (see p. XVII)

S The line is greatly strengthened,

s The line is strengthened. u The line is unchanged in intensity.

W The line is greatly weakened. w The line is weakened.

0 The line is obliterated.

A'' The line is diffuse. NN The line is very diffuse. d The hne is double.

The Identifications: Column five (see p. XVIII)

II Predominant contributor to a blend.

1 Principal contributor to a blend. — In case of blends the dash indicates whether the contributor

is on the short- or the long-wave side of the solar line; or whether the solar line has been completely identified.

( ) Masked lines. p Identification based on predicted laboratory wavelength.

6. Acknowledgments

The authors are deeply indebted to many collaborators

who have wiUingly assisted with this large task. In

Utrecht, when the intensity work was started, many

members of the staff and several computers contributed

to the elaboration of the catalogue, especially Messrs.

W. J. Claas, H. Hubenet, H. C. Van de Hulst, C. de Jager,

and later Misses J. Blom and M. Dekkers. At the

Dunsink Observatory in Ireland, H. A. Briick, Mrs. M.

T. Briick, and G. I. Thompson made a most important

contribution in furnishing the photometric tracings

which have been used for the region short of 3650 A.

In Washington, the Spectroscopy Section of the Bureau

has steadily supported the program. The personal

interest of W. F. Meggers and C. C. Kiess has been a source of encouragement over the years since the program

started. Those who have kindly furnished material for

the Atomic Energy Levels program have been no less generous with the solar project. B. Edlen, G. Risberg,

K. L. Andrew and L. J. Radziemski have contributed

material in advance of pubUcation. W. S. Benedict has

provided all of the designations for the II2O lines, from

his wealth of data on the analysis of these bands. The

discussion of elements in the sun could not have been

summarized without the valuable assistance of R. Tousey.

In the Bureau library, Miss S. A. Jones and her staff have been most wUling collaborators. In the PubUcation

Section, J. E. Carpenter and his staff have been most

cooperative. The meticulous details of publication have

been entrusted to Mrs. Betty Oberholtzer, whose skill and competence are revealed throughout the pages of the

book. The authors are equally grateful to Mrs. Isabel D.

Murray whose assistance in preparing the manuscript for

publication, with painstaking care, has been invaluable.

The National Research Council has also been most

cooperative. H. D. Babcock at the Mount Wilson and

Palomar Observatories is one who was keenly interested

in initiating this work. He has furnished many notes

and comments from his records and his wide experience.

It is a privilege and a pleasure to record our thanks

to all who have participated.

National Bureau of Standards

Utrecht Observatory

January 6, 1966.

XXX
The Solar Spectrum

Low RMT Low RMT

vv avc" XLiO Ul Liicl tCU. Solar E P No. ^^£ive~ X-Ji3 111 illd utyl-l Solar E P iri yj. length Snnt Idenlji" or 1 PTl 0"t Vl T n t AM filt V Spot Tflpnti- or

fi f 1 nn Rot. Vib. fi p ft 1 i n n Rot. Vih

(A) Line Band Li n c Band

[ 5? ] Vi- 0.04 UV3 2948.44 [— 1 ] Fe I 2.73 UV166

Fe II 4.15 UV323

2948.66 [— 1 ] -Fe I 2.20 104 2936.20 [ 5? ] Ti n- 3.82 UV26

Fe I? 1.61 UV89 2948.95 [ 3 ] Fo I Zr II 0,97 11

2936.5 r k9 1

I or J JVlg II 4 4*? U V 2949 18 [ 5 ] Fe II 3.77 UV277

r <\i 1

I O' J Fe I 0.00 10 (Mn ii) 1.17 UV5

Ti I 0.02 UVl 2949.62 [ 3 ] V I 0.02 UV3

2937.65

fO.OO UV3 2950.22 [ 5 ] Fe I 2.18 UV120

[ 5 ] Vi \0.02 UV3 (V II) 0.32 UVIO

Fe I 2.20 UV122

2950 62 [_ 1 ] OQ^lR 4.1

[ 5 ] 2.70 UV3

Ti II 3.84 UV26 2950.77 [—1 ] 9Q^Q 9^ [ 20? Pe I 2.22 104 2950 87 [— 1 J Nb u 0.51 UV14

||Mn II 1.17 UV5

2951.09 [ 0 ] Fe II 3.20 UV214

r 9? 1 Fe II 1.04 2 2951.37 [ 0 ] Cr II 4.15 59

904-0 1 ^ r 2 1 Mn I 3.13 UV17

2951.53 [ 0 ] Fe I 9Q4n 'iO r 3 1 Mn I — 2.32 UVIO

Mn I 2.32 UVIO 2952 03 [ 2 ] IV II 0.35 2 Fe I 2^83 UV173 Ti II 3.86 UV26

( Cr II) 4.15 59

9Q4.1 90 r if)^? 1

( XwUL J Fe I 0.09 10 (Vii) o!33 UVIO 2952.24 [ 0 ] Zr II 0.16 UVl

(Vii) 0.39 UVIO

2952 86 [—1 ] Mn I? 2.16 UV4

9Q4.9 ^11 Ti I 0.00 UVl

|iV±g 1 2.72 UV3 2953.36 [—1 ] Cr II 3.71 27

JO. 00 UVl

IV I \0.07 UV3 2953.48 [—1 ] Fe I 2.76 UV166

2942.85 [ 5d? 2953.84 [ 25 ] Fe II — 1.04 2

lire I 0.09 10 2943.10 [ 3 Vi 0.00 UVl

2954.31 [-3 ] V I 0.02 18 2943.59 [ 3 ] Fe I (Ga i) 0.10 UVl 2954.58 [ 2A'" ] — Fe I 2.28 UV132

904*^ R7 r ^1 1

I " J Ni 1 0.03 26 2954.89 [ 0 ] Ti II 4.31 UV34

904.4. no r fi 1 2Q55 1

[ 0 ] Cr II 4.17 59

2944.54 [ 0 ] Fe II— 1.69 8 2955.33 [—3 ] Co I? IIVii 0.37 UVIO

2955.61 [-2 ] V II 3.76 UV196

2944.98 [ 0 ] -Fe 1 2.45 2955.79 [-2 ] Zr 11 1.74 UV61

2945.37 [-1 ] Fe II 1.04 2 IV I 0.07 UV3

904- 49 Tl TT o .oo UV26 2955 92 • [—3 ] F— 1 1 Fe I 2956.08 [ 2 ] Ti I 0.05 30

204^1 70 r 1 1 Fe II 2956.34 [—1 ] Cr I 0.94 UV5

r 1 1 "RpC 1T 11 .U61

2956 64 [ ] Cr II 4.15 58 Fe I 2.18 104 CrV-/1 TT11 4.32 66 2956 82 I 2 ] ITi I 0.02 30 9Q47 04- W I— 0 37 UV5 Fe I 2.69 UV165

Fe I? 3!30 UV182

2956.95 [-3 ] Mn I? 2.19 UV4

2947.70 [ 30 ] Fe II- 1.67 8

||Fei 0.05 10 2957.17 [-1 ] V I? 1.19 UV76

(Vii) 3.76 UV196

2957.24 [-1 ] 2948.22 [-1 Ti I 0.02 UVl

1
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

2957.38 [ 10 ] Fe I 0.11 10 2984.604 [ 6A^ ] -|Fe II 1.72 8

2957.52 [-1 ] V II 0.33 2 2984.84 [ lA^ ] C I 0.00 UVl

2957.64 [-1 ] Co I 2.08 UV134 2985.02 [ 4 ] Fe II 1.69 8

2958.07

2958.26

[-3 ] [-1 ]

Fe I? Ni I Ti II 1.93 3.88 UV74

UV26

2985.28

2965.41

[ 10 ]

[-1 ]

Fe r (Til) Fe II

0.12

1.05

3.42

1094

59

2958.45

2958.73

[ ON ]

[ ON ]

Fe I Vii2.73

3.75

317

UV196

2965.81 [ ins ] |Fe I Til

2.43 /1.05

11.07

UV147

94

94

2958.98 [ ON ] Ti II 4.28 UV34 2988.08 [ 2 ] Cr II 3.87 33

2959.32 [ IN ] Fe I 2988.28 [ 2 ] Fe I 2.22 104

2959.62

2959.95

[ ^N ]

[ 2NI ]

iFe II Fe I Fe II Cr II liFei

3.39

2.81

5.57 4.17

2.69

62 334

18059 316

2988.93

2967.23

2967.662

[ 30 ]

[ OiV ]

[ 3 ]

Fe I

iC I Ti I Cr I

0.00

0.01 0.05

1.00

10 UVl

30

28

2960.28 [ 1 ] Fe I 2.48 148 2988.090 [ 1 ] -Fe II 5.58 180

2980.52 [ 0 ] Fe I 2968.20 [-3 ] Ti I 0.00 29

2960.65 [ INN] -Fe I 2.95 UV178 2968.389 [ 3 ] V II 1.70 28

2981.09

2981.27

[ IN ]

[ 3 ]

V I ICu I Fe II

1.22 L39

1.08

UV76

UV15

2

2968.516

2988.740

[ 2iV ]

[ 1 ]

Fe IFe II Cr II2.42

3.39 4.18

UV135

6158

2961.40 [-IN ] -Ti I? 1.05 2968.97 [-1 ] Zr II 0.47 14

2961.56 [-IN ] 2969.04 [-3 ]

2961.71 [ 3 ] Cr II (Fei)

/3.76

14.18

2.18

2759

105

2969.19

2989.35

[ 1 1

[ 1 ]

Ni I Fe I1.95

0.11

UV74

11

2961.91 [-3 ] 2969.48 [ 8 ] Fe I 0.86 30

2962.12 [ 3 ] Fe I 1.48 57 2989.87 [-IN ] Cr 11 4.32 68

2962.38 [ 0 ] 2989.98 [ 3 ] Fe II 3.81 70

2982.59

2962.67

2962.77

2962.93

2963.05

2983.27

2963.52

[-1 ] [-2 ] [-2 ] [-3 ] [-1 ] [-2 ]

[ 3A^ ]

Fe I

Zr II Vi

Fe II

V II Fe I? |Cr II

0.38

0.04

5.55

2.60

4.17

UV9

18

160

154

58

2970.12

2970.36

2970.519

2970.68

2970.92

2971.118

2971.24

[ 8 ]

[ 3 ]

[ 5 ]

[ lA^ ]

[ lA^ ]

[ 2 ]

[ 0 ]

Fe I

Si I Fe II Fe II

Cr I

f0.09

10.11

0.78

1.08

3.77

0.98

1110

1

2

69

28

[ 3 ] Fe I TTV1 7"^ 9071 fi99 r fl 1 Fe II 3.39 60

2963.80 r_2 1 Vi 1.22 UV75 2971.77 [ 1 ] Fe I

2984.13 [ QN ] Fe II 3.39 60 2971.936 [ 3 1 Cr II 3.77 28

2964.52 I 0 ] W I- Zr II 0.37

0.09 UV5

UVl

2972.03 [-1 ] Fe I Fe II 5.60 180

2
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. iJana

Notes Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. iiana

Notes

2972.274

2972.415

[ 4

[-1

|V 11- Fe I 2 37

2.20 87104 2979.120 [ 6 ] Fe II (Vii)

(Zr 11)

/3.97

2.03 0.36

100

18044

14

2972.65 [-2 Cr 11 3.75 28 2979.370 [ 8 ] Fe II 1.10 2

2973.201

2973.745

2973.93

2974.223

2974.43

2974.640

2974.791

2974.92

2975.038

[ 40

( 2

[ i [-IN

[ 0

[ 3 [-2

[ 2

]

]

]

]

]

Fe I —

Fe I Ni I? V II Mn i7

1' e I

il I

0.05

0.09

1.68

3.79

4.23

2. So

1.07

10

10 UV66

218

UV41

66o

94

2979.59

2979.742

2979.88

2980.02

2980.219

2980.396

2980.558

2980.795

2980.979

[-3 ]

[ 2 ]

[ 1 ]

[ 1 ]

[ 1 ]

[ 0 ]

[ 5 ]

[ 4 ]

[ 4 ]

Cr II Fe I

Fe I Cr I

|Fe 11

ZjT II

3.76

2.76

0.96

3.42

U.OO

28

317

28

61

O A

2975.278 [ 3 — Fe I 2981.20 [ 0 ] V II o o o 8/

2975.480 [ 4 Or I 0.97 28 2981.458 r C AT 1 L 6A' J Fe I 0.05 1

2975.665 [ 3 V II 1.67 28 2981.658 [ 3 ] Ni I 0.11 26

2975.823 [ 0 Fe I? 2981.866 [ 3 ] Fe I 2.18 104

2975.924 [ 5 Fe II 1.10 2 2982.067 [ 3 ] Fe 11 4.48 139

2976.156 [ 7 ] Fe IV II 2.28

1.67 14628

2982.243 [ 3 ] Fe I |Fe II 2.99

3.81 460

70

2976.37 [-2 ] Mn u? 4.93 2982.393 [ 1 ] 2976.540

2976.724

2976.913

[ 7 ]

[ 3 ]

[ 5 ]

V 11 (Je i) Cr II -Fe I

1.69

3.83

2.83

28

27

334

2982.488

2982.768

2982.98

[ 1 ]

[ 2 ]

[-2 ]

Vii

Vii

1.67

/1.68

\1.69

28

2228

2977.236 [-3 ] 2983.20 [-1 ] -Til 0.02 29

2977.533

2977.685

2977.84

[ 2 ] [-1 ] [-3 ]

V I Rh I? Mn II? Fe I?

0.07

0.70

4.93

18 2983.576

2983.84

2984.144

[ 40 ]

[ 1 ]

[ 4 ]

Fe I (Vii)

Ni I

0.00

1.69

0.00

928

12

2978.055

2978.204

2978.294

2978.456

[ 3

[ 0

[ 0

[ 1

Fe I Zr II V II2.45

0.41

2.37

14

87

2984.35

2984.574

2984.71

2984.840

[-2 ]

[ 2 ]

[ 1 ]

[ 7iV ]

Cr II-

|Fe II Fe I

3.76

1.67 0.86

27

829

2978.557 [ 1 ] - Mn I? 2.16 UV3 2985.19 [-3 ] Vii 3.80 218

2978.692

2978.848

[ 1 ]

[ 1 ] Fe II 3.77 69

2985.324

2985.49

[ 0 ]

[ 1 1

Cr n

(Zn)

Til3.75 0.000.02

28

22

29

761-925—60
The Solar Spectrum—Continued

length

(A)

Intensity Spot

Solar

Identifi f 1 nn

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

mo \ji LkiiXyjKZKj. Intensity SpotSolar

IdentiLow

E P

or

x\u u. Line

RMT

NnIN U. or

V ID. Band

Notes

JjiJOO,tJ\J [ 5Nd ]

1X . 72J ^ g 2992 OQS [ 1 ] Ni I?

r 1 1 Fe T OQQO 407 L ^ J — Cr IT % 7fi 98

r 4. 1

L Cr I 0.98 28 2992 fiOO [ 7 ] Ni I \j .yjo 9'?

2986.004 [ 4 ] Cri 1.00 28 2992.958 [-1 ] 2986.145 [ 2 ] Cr I 0.97 28 2993.046 [ 0 ] 9QRR 9QR r 9 1 17p T r 1^? 1

y 1 u . J 2986.478

2986.641

[ 6 ]

[ 6 1

llCri Fe I

|Fe II- Fe I

1.03 0.11

3.42

2.43

28

11

62 200

2993.398 29Q3 7QS

2QQ4 074

[ 2 ]

[ 4 ]

[ 4 ]

Fe n

Cr I

4.49

f) Q4

139

1X 4T:

9QRfi 87*^

2987.052

r nAT 1

I 2 ]

2994 4.'^fi [ 40 ] IIFp t — 1 |r e 1 Ni I

/0.05

10.12 0.03

9

1127

2987.20 [ 2 ] Co I 0.00 11 2994.758 [ 3 ] Cr II 3.75 28

2987.291 [ 10 1 Fei 0.91 30 2994.951 [ 4 ] Ca I 1.88 17

2987.662

2988.033

2988.195

2988.31

2988.481

2988.644

2988.774

2988.926

2989.14

2989.32

2989.630

[ lOAT ]

[ 6 ]

[ 0 ] [-3 ]

[ 1 1

[ 2 ]

[ 0 ]

[ Id? ]

[ 3 ] [-IN ]

I 4 ]

Si I

|Vii Cr II Ni 11

Fe I Cri

Zr II? Fe I |Sc I |Sc 11 Cr II ViiIV II Co I

0.78

1.69 3.77 3.10

1.48

0.94

4.14

2.73 0.02

3.23

3.74

2.38

1.70 0.00

1

27

28

6

56

14

148

316

1134

28

87

28

13

2995.113

2995.260

2995.373

2995.494

2995.588

2995.839S

2996.008

2996.396S

2996.588S

9QQfi 7"^

2996.849 2997 00

2997. 222S

[ 3 ]

I 3 ] [-1 ]

[ 2 ] [-2n ]

[ 2 ]

[ Anl ]

[ 5 ]

[ 5 ]

[ — 2N ]

[ 2 ] [_3^ ]

[ "^N ]

Cr I (Co I) Fe I

Fe I V II Fe I Cr I V II

V I

0.94

2.14

3.02

1.67

2.42

0.98

1.70

2.03

15 UV129

460

27

148

28

28

116

^yoy. /o L KJiy J

r n 1 V II—

X 1 11

2.38

1 4*^ X.10

87 2QQ7 32 [ 3 ] ICa I iFe II- Cu I

1.89 4^49

1.64

17 139

5

9000 *^QC\ [ 6 ] Fe I 2.73 316 2997.54 [-3 ]

2990.618 [-2N ] 2997.72 [-3 ] Fe II 3.90 85

2990.876 I 2 ] 2997.862 [-2 ] Vi 2.04 116

2991.096 [ 5 ] Ni I /0.27

11.93 1480 2997.978S [ 2 ] Pt I 0.10 3

z9yi.Z4ii

2991.411

2991.635

2991.774

r 1 1

[ 1 ]

[ 5 ]

[ 4 ]

"Rp X c TTXI

Zr 11 Fe I

3.42

0.00

60

6

2998.152

2998.336

2998.497S

2998.795

[ 2 ]

[ 1 ]

[ 1 ]

[ 4 ] Cr I (Fe II) 0.94

3.42 1460

2991.882 [ 4 ] Cr I 0.97 28 2998.966 [ 2 ]

4
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

boiar

Identification

Low

ill r

or

itot. Line

RMT

IN 0. or

V ID. Band

Notes Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

V111 rp

or not. Line

RMT

iNO. or

V irj. Band

Notes

2999.04 to 1 l~3 J Kja II U.(j3 r 0 1 1 ^ \ r e 1

2999.205 r o 1

I 3 J r e I onnft 1 70 ouuD.i I " 1 — VI 1 1 A

2999. ODD [ 4 ] r II — 3.0D 33 oUUo.olo L 1 — 1' e I

2999.521 [ 10 ] Fe I 0.86 30 3006.434 [ OiV ]

2999.67 [ 2 ] Ca I 1.89 17 3006.573 [ 4d ] 2999.943 [ 2 ] Cr II 4.01 42 3006.740S [ 3 ] Si I 0.01

3000.Odo

oOOO./l

3000.339

3000.462

r o 1

I 2 J

r o 1 l~3 J

[ 2 ]

[ 3 ]

re II

Fe 1

o.ol

1.48

Dy

56

OUUD.ODOO

3007.152

3007.291

f Q 1 I ^ J

[ 5 ]

[ 6 1

oa I (Vi)

Fe I

|Fe IV II

1 .yu 2.10

1.48

0.09

1.67

1 1 110

55

1127

3000.576 [ 2 ] Co I 0.10 13 3007.497 [ 1 Ti I?

3000.75

o000.94o

3001.230

3001.4iJi5

[ 0 ]

roc 1 I Z5 J

r cr A 7 1

I 5A' J

r 1 AT" 1

Fe IITi I

r e I (Cai)

(Cr i)

V II — r e II

0. 05

n no

1.89

1. UU

1.70

29

y

17OQ

n

3007.65

3007.77

3007.96

3008.152

3008.293

[ 0 [-1 ]

[ 3iViV]

[ 15 ]

[ 2 ]

Mn I Fe ip

Fe I |Mn I Ti TT X 1 II

3.13

2.59

0.11

3.13

1,0

35

262

9

35

00

orvr\ 1 Geo 3001. d5o r o 1

I J r e I oUo r ^ 1

3001.791 [ 3 ] 3008.648 [ 4d ] V II- 1.67 26

3001.932 [-2 ] V I 2.05 116 3008.801S [-2 ] Ce II 0.32 122

3002.041 [-2 ] 3008.922 [-3 ]

3002.193

3002.341

3002.486

3002.660

oUUo.U4o

3003. 463

3003.649

3003.895

[-2 ] [-3 ]

[ 25 ]

[ 10 ]

r o 1

L o J

r o AT" 1

L 3A' J

[ 8 ]

[ 5 ]

Fe n

Ni I Fe II re I

V II Ni I Cr 11

3.94

0.03

1.69 0 OA U.yo

1 fin i.oy

0.11

3.00

98

26

8QnoU

iiO

33

3009.102

3009.214

3009.36

3009.582

3009.921

3010.029

3010.180S

[ 3 ]

[ 2

[ liV ]

[ 12 ] [-3 ] [-3 ] [2 ]

Fe I (Sni)

Ca I

Fe I

Fe I Fe n

2.40

0.21

1.90

0.91

5.82

198

1

17

30

181

3004.120b r o 1 I ^ J J* e I

1 nn lyy r n 1

[ U J

3004.271 [ 2 ] Fe II 3.81 69 oUiU.DZoo r 1 1 r e I

3004.362 [ 0 ] 3010.847 [ 0 ] Cu I 1.39 3

3004.480 [-2 ] Fe ip 2.22 105 3011. 167S [ 0 ] Mn I 3.13 35

3004.630S [ 3 ] Fe I 1,56 57 3011.277S [ 1 1

3005.052S

3005.308S

3005.494

3005.755

[ 4 ]

[ 3 ] [-IN ]

[ 4(i? ]

Cr I Fe I

Zr I Co I1.03

2.40

1.00

1.88

28

199

60

77

3011.369

3011.478

3011.632

3011.736

OiV ]

[ 4 ] [-2 ]

[ 0 ]

Mn I (Cr II) Fe I

Zn3.13

3.83

2.76

0.07

35

27

316

2

5
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3011.88 [ OA^ ] Fe I 2.48 UV135

3012.012 [ 12 ] ||Ni 1-

V 11 0.42

2.05 4143

3012.346 [-3 ] Cr II? 4.01 42

3012.450S [ 3 ] Fe I

3012.60 [-3 ] Fe up 3.81 69

3012.736 [-2 ]

3012.937 [ 3 ] Fe I

3013.048 [ 3 ] Cr I 0.96 26

3013.101 [ 3 ] V II 1.67 26

3013.331 [ lA'' 1 Zr II- 0.56 27

3013.497S [ 1 ] 3013 595S [ 2 ] Co I 0.00 10

3013.730 [ G ] Cr I 0.97 26

3013.831 [ 0 ] Fe II 4.15 124

3013.970S [-1 1 Fe I

3014.105 [ 2 ] Fe I 2.95 458

3014.164 [ 3 ] Fe I 0.96 31

3014.320S [ 1 ] V I 2.12 116

3014.457 [ ON ] Zr I?- 0.00 21

3014.648 [ 0 ] Mn I 3.13 35

3014.781 [ 9 1 |Cr I V II 0.97

1.69 27

27

3014.919 [ 8 ] Cr I 0.98 27

3015.202S [ G ] Cr I 0.96 27

3015.366 [-2 ] Sc I 0.00 10

3015.508 [ 4 ] Cr n 4.41 87

3015.688 [-1 ] Co I 1.88 76

3015.818 [-1 ] 3015.929 [ 5 ] Fe I 2.43 198

3015.989 [ ON ] V II 2.04 42

3016.196 [ 10 ] Fe I (V II) 0.99

1.69 3026

3016.449 [ 2 ] Mn I 3.13 35

3016.522 [ 0 ] 3016.784 [ 6 ] V 11 1.70 27

3016.872 [ 3 ] 3017.08 [-2 ] 3017.187 [ 4 1 Ti 11 1.58 85

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3017.255 [ 4 ] Co 1 1.88 78

3017.418 [ 3 1 3017.631 [ 12 ] |Fe 1 Cn

Co I

0.11

1.00 0.10

927

11

3017.854 \ 2 ] 3017.953 [ 0 ] Ni I 1.93 UV74

3018.031 [ 0 1 -Os I 0.00

3018.141S [ 3 ] Fe I 2.40 199

3018.254 [ 1 ] Fe ip 2.56 263

3018.496 [ 4 ] Cr I 0.97 26

3018.599 [-2 ] Ca I? 1.90

3018.701 [-2 ] 3018.821 [ 4 ] Cr I 0.98 26

3018.992 [ 7 ] Fe I 0.96 30

3019.154 [ V ] Nil 0.00 11

3019.313 [ 4 ] ||Fe ISci2.45

0.02 199

10

3019.56 [-2 ] 3019.911 [ Od ] Zr II?- Mn II 0.04

4.31 6

3020.015 [ 5 ] Si I 0.03

3020.27 [-1 ] 3020.490 [ 20 ] Fe I 0.09 9

3020.656 [ 40 ] Fe I (Cr I) 0.00

0.97 927

3021.077 [ 30 ] Fc I 0.05 9

3021.22 [-1 ] 3021.572 [ 5 1 Cr I 1.03 27

3021.719 [ 0 ] — Mn 11 4.31

3021.883 [ 1 ] 3022.12 [-3 ] V 11? 2.38 86

3022.266 [ 1 ] 3022.359 [ 2 ] Co 1 1.71

3022.472 [-1 ] 3022.602 [ 3/V ] V II 1.67 26

3022.747S [ 3 ] Mn I 3.13 35

3022.91 [-3 ] 3023.068 [ 3 ] 3023.30 [-3 ] Mo II? 4.39

6
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3023.438

3023.695

3023.851

[ 0 ]

[ liV ]

[ 47V ] -Fe 11 |Vii

3.89

2.05 8441

3029.288

3029.345

3029.430

[ 2 ] [-2 ]

r o 1 L — ^ J

Ni I

Mn II?

/1.68

11.95

4.33

56 UV74

3024.060

3024.242

3024.353

3024.577

3024.677

3024.802S

3024.981

3025.286

3025.644

[ 12 ]

[ 2 ]

[ 6 ] [-2 ]

[ 1 ]

[ 3 ]

[ 2N ]

[ 6 ]

[ 8 ]

Fe I

Cri

Cri

V II Fe I Fe I

0.11

0.98

2.97

2.37

0.91

2.40

11

26

117

85

29

198

3029.548

3029.734

3029.990S

3030.147

3030.254

3030.484

3030.607S

3030.760

[-2A^ ]

[ 5nl ]

[ 3 ]

[ 5 ]

[ 5 ] [-3 ]

[ 2 ] [-2 ]

Zr IV II

Ti II

Fe I Cr I OH?

Fe I Fe I Sc I

0.15

1.70

1.57

2.43

1.00

S 9

2.28

2.99

0.02

2226

85

198

27

0,0

1.45

459

10

1

3025.866 [ 18 ] Fe I 0.12 9 3030.85 [-3 ] 3026.221 [-IN ] 3030.941 [ 2d? ] Zr II 0.00 6

3026.377 [ 3 ] Co I 1.88 77 3031.052 [ 2 ] Mnii 4.31

3026.495 [ 8 ] Fe I 0.99 30 3031.211 [ 6 ] Fe I 2.45 198

3026.645 [ 6 ] Cr II 4.43 95 3031.346 [ 6 ] Cr I- 0.98 27

3026.836 [ 2 ] Cr II 4.01 41 3031.474 [ 1 ] Cr I 2.98 117

3026.942 [ 2 ] Fe I? 3031.668 [ 10 ] Fe I 1.01 30

3027.016 [ 2 ] 3031.867 [ 5 ] Ni I 0.00 11

3027.213 [-2N ] 3032.036 [-2 ] Zr II? 2.43 144

3027.35 [-2 ] Fe up 3.94 99 3032.228 [-2Ar ] 3027.607

3027.699

3027.890

3028.020

[ 1 1

[ 2 ] [-IN ]

[ 4 ]

IIVii Gd II

-Pd 1

|V II Zr II

2.38

0.14

0.96

2.38

0.97

85

12

5

85

76

3032.469

3032.645

3032.855

3032.929

3033.105S

[ 1 ] [-ZN ] [-2 ]

[ 3 ]

[ 2 ]

Ni II

Gd II Cr II Fe I

2.86

0.08

2.70

2.42

3

12

15

146

3028.127

3028.287

3028.445

3028.604

3028.686

3028.869

3029.000

3029.069

3029.155

3029.227

[ 4 ]

[ 0 ] [-2iV ]

[ 1 ]

[ 1 ]

[ 2 ]

[ 2A^ ]

[ 2Ar ]

[ 4 ]

[ 3 ]

Cr II

Nb 11 Rh II?

Mn II Cr I Fe I

4.41

0.44

3.40

5.38

0.98

1.56

87

2

1

10

26

56

3033.434

3033.607

3033.817S

3033.949

3034.061

3034.12

ouo^. ± yo

3034.45

3034.50

3034.55

[ 4d? ]

[ lA^ ]

[ 3 ] [-2iV ] [-1 ] [-3 ]

r ^ 1 L ^ J

[ 3 ]

[ 3 ]

[ 3 ]

V II (Fe II)

V II

Gd II Sn I Cr I Co I Fe I Cr II

2.52

5.87

1.82

0.03

0.21

1.00

0.17

1.61

3.86

123

181

34

12

1

26

12

57

33

7
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

isoiar Identification

Low

ill Jr or

rvOl. Line

RMT

IN 0. or

V ID. Band

Notes Wavelength

(A)

Estimated

Intensity Spot

G/>loT» ftoiar Identification

Low

ii/ r

or Kot. Line

RMT "N'T

«

JNO. or

VlD. Band

Notes

QHQ/l fin r q 1 r q 1 Url to 0 u,u11

QHQyl Q1 9 r n 1

I " 1 ivin II l.OU 91 r 1 n 1

[ lU J re I u.y i qr\

oUO'l.yoO r[11 1

J II A (\A AO OU4U.DUO f 9 1 Mn I q 1 q 6.16 34

oUoo.i lo r q 1

I — " i TTrt T*? r e Ii r 9 1

r 1 1 Fe I pq 07 ouo \14A 1

J v^r I

1 00 l.UU 9^7

OUoO.oDU r 9 1

[ Z J Mn II /I qq 4.00 qO/i n Qqc \[4A 1

J P't. tt v^r II A 9r» 4.zy DO

oUi)0.'±OD r 9 1 L'

^ J oU41 .Uoo r 9 1

I J qnqc; oUoO.7A7 ( 41 /

L 4 J r e I — oU-li.iot) r q 1

3035.886 [ 0 ] 3041.220 [ 0 ] Mn I 3.13 34

3035.999 [-3 ] 3041.412 [ 2nl ] Vii 2.03 40 3036.108 [ IN ] Cu I 1.64 5 3041.625 [ 5 ] Fe I 1.56 56 3036.252

3036.397

3036.509 qnq« AO

oUoD. / 0^ qnQR OA

3037.044

[ 0 ]

[ 2 ]

[ 0 ]

r 9 1

r 9 1

r 9 1

I — ^ J

[ 8 ]

Zr II

Zr II V TT 1 II — T*; TT i I II

r e II

Cr I

0.56

0.53

q F^A

1.57

K 09 o.oz

1.03

25

24

00

101

27

3041.754

3041.901

3042.026

3042.263S

3042.486S

3042.664

[ 5 ]

[ 1 ]

[ 7 ]

[ 3 ]

[ 3 ]

[ 10 ]

Fe I Cr II

Fe I Vii

Co I Fe I (Mn i)

0.96

4.41

1.01

2.03

0.10

0.99

3.13

30

95

30

40

10

30

34

qriq7 oq r Q 1

[ o J q04 9 Qt^A r q 1 (^T. TT L/r II A r\i

qnq? qoR r qn i re I U.i i y

QO/i q 01 7 r q 1

qO"?? fid

3037.788

r r> 1

[ U J

[ 3 ] Fe I 0.99 31

Qr\A q 1 9nO

I i i V I (Mn i) (Mn 11)

0 r»9 3.13

4.51 3421 3037.946 [ 15 ] Ni I 0.03 25 3043.263 [-2 ] 3038.091 [ 1 ] Mn II 4.34 3043.355S [ 2 ] Mn I 3.13 34

OVJOO.O

OVOO. O i-O

r q 1

[ z J

r e I

TT

II V II Cr II 4.01 9d

41

oU4o.o4o

3043.759

r q 1

[-2n ]

V I |V II Mn IU.UU

2.04

3.13

1 71 / 40

34

3038.747 [ 3d ] Ti II1 T?^ TT |re II 1.58 85

o4 3043.853 [ 2 ] Ti II- Or II 1.57

4.07 784o

OAQQ Q7Q r 1 1

'"> A 1 1 AAA o044.UU9 [ 5 ] Co I 0.00 11 OUoy .UDO O ^ T Lre I 0.88 2 3044.1^4 r 0 1

[ Z J Zr II — 0.56 z6

3039.202 [-3 ] Mn II? 4.69 3044.228 [ 2A^ ] 3039.325 [ 3nZ ] Fe I 2.43 199 3044.333 [_2 ] OH S 5 0,0 1 ouoy.oo L — •J J 3044.44 ["~3 ] ouoy.oy /

3039.761

[ ins ]

[ 3 ]

L/0 I Mn II —

Cr ICr I

1. /I 5.39

3.00

1.00

52

10

11726

o044.5d»

3014.720

3044.837

[ 3 ] [-3 ]

[ 2 ]

Mn I Nb II? Fe II2.11

1.69

3.97

15

98

3040.020 [-2N ] 3044.94 [-2 ] V I 0.04 17 3040.218 [-3 ] Cr II? 3045.01 [ 4 ] Ni I 0.17 12

8
The Solar Spectrum—Continued

I;OW RMT Low RMT

Wave- Estimated Solar E P No. Wave- Estimated Solar E P No.

length Intensity Spot Identi- or or Notes length Intensity Spot Identi- or or Notes

fication Rot. Vib. fication Rot. Vib.

(A) Line Band (A) Line Band

OU'lO.U i \[4A 1

J r c 1 u.y i 90zy oUOU. 1 0£i [ o J II A '>9 Ac;

oU40.O'±U r 2 1 Tr/Ii TT r e U 0.0 / 1 7o 1 / y

Qnfin 07Q r 9 1

L — ^^^ J Pt* tt? L/r III A 07 ouou.oyo r 9 1 V T V I

11 .OO 7/1

/ 4

Qflyl tC COO r o 1

[ Z J AT T-i T ivin I Q 1

*^ O.IO OU0U.0U4 r o 1 \^0 I i - JO 77

1* e I iy8

OUOU.D QOt^n A7i

r 1 1 A/r r\ TT ivin II 4.0U 91Zl

OU'lO. / Zo r[11 1

J TT Q Ar\ o < OUOU.oiO r 1 fi 1 IN 1 I U.vJo 9ZO1^ OU'lO. / / o

r[11 1

J ivin I O.lO Q/l OUOi .U4 [ O J QA/1 Oft r 2 1 oU0i.Z4 r Q 1 L — " J 011-9:0.0400 r 1 1 r e I OUOI .'fiO r 9 1 AA n TT 4.04

QH/I A 1 7 oU-lo.i / r Q 1

I — <i J OUOI .Dl Pi- TT? v.'r 11

oU'iO.ZOO I UiV J A/Tn TT ivin II O.IU 1 o ouoi . * y4 r 1 1 T?o r I? e 1 i 3046.503S [ 0 ] 3051.987 [-3d? ] Ce II? 0.54 180

OU^tO.O / Z L ^ J T^i TT 1 1 II 1 1 A Al

OUOZ.l^o r 1 1 oU4t0.oU0O r n 1

[ U J jf e I oio

qnco oi q [ U J V T V 1 — n 09 11 o^ oU4t0.yoD r o 1

-T e I

1 OQ lys Pr T o.uo 1 K4. 1 04

Qnyl7 f\AQ. r 0 1

[ z J r e I 9 Of^ y| P17 oUOZ.ZOo [ UCt 1 J

1 A/Trt T

1 iVlu I o.io o4

ouoz.^y 1 o r 1 1 [ i J

[ U J J? e I 9 Q/1 o8za

oUOZ.OoU

r 1 1 Q OO 1 A/I 1D4

OUOZ.D qnco R7/ I — " J Qfi/l 7 Rl A OU4t/ .Oil r Q 1

L J r e I n OO y

qnp;0 7QQ r n 1 r e i p9fi9

0(1/17 70 r o*? 1

[ ol^ J L^r II 9 Tl 1 K 10 ouoz.yzo r 1 1 C!n TT loC II 0.4ii /19 O I oU4o.uU£5 r n 1 oUOo.uOo r Q 1 r e I 9 /19 X4D oU4o.Uy4 r n 1

I " J uo I i.yo 77 OU0O./40 r Q 1

L — "5 J VX TT11 O.04 % ^A UO

oU4o,ziyc) r o 1 [ o J V II 9 Kl 123 OU0O.4ZU qnc^Q /ion r 7/^ 1

1 V 11 — 1 .ou 3048.352 [-lAT ] ffp T fl.Ol 31

X C 1 12.94 398

3048.454 [ 5 ] Fe I3053.55 [-2 Gd II? 0.49 25

r Q 1

I — " J Uxl b 4 U,U 1 ouoo.ooy r 1 1 V I 0.00 17

OU4O.D01 I — ^ J V II? 9 9*7 A7 4.29 64

OU^o. / 0^ Ti TT 1 1 II 1 .08 7ai 8 OUOO. 1 4'x r 9 1

Ofiyl Q QQ'7 [4 J Co I n 1 7

U.17 1

oUoo.ooU \[4A 1

J O-r T1 X .uo 9fi V II 2.04 40 Vii 2.05 40 (Mn i) 3.13 34

3054.315 [ 12 ] II Nil 0.11 25

3049.015 [ 2 ] Fe II- 5.87 181 Mn I 2.14 15 Mn II 4.52 21

i}0o4.D9o r 9 A^f. 1 1 A1 Tj Al I O.OUfin 7

QflylO 1 KA r o 1 Fe II p

A AO Pav>0 t1 n 1

W. 1 / xo

r o 1 [ o J fe I QQO r 1 1 7!r TT Lil 11 11 .Ul 01 7fi

3049.546 [ 2 ] Fe I 3054.940 [ 1 ] Fe I 2.61 263

Eu II 0.21 7 3049.754 [-^N ] 3055.116 [ 1 ] 3049.900 {-ZN ] Cr I 1.03 27

3055.296 [ ed ] |Fei- 1.56 55

3050.074 [ 2 ] Al I 3.60 7 Fe II 5.90 181

9
The Solar Spectrum—Continued

Wavelength

(A)

Estimated

Intensity Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

IdentiLow

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3055.457 [ 1 ] Cr II 3.85 33 3060 989 [ 2 Fe I 1.56 55

3055.594 [ — 3 ] Ceiii? 2.25 1 3061.12 [— 1

3055.720 [ 4(^ ] Fe I — 3061.28 [—3

3055.934 [— 3A'' ] V 11 2.52 123 3061.35 [_ 1 Zr II 0.09 6

3056. IIOS [ 1 ] 3061.40 [— 1

3056.233 [ 2 ] Fe I 2.61 3061.57 [ 1 Cr II 4.04 41 3056.340S [ 2 ] Vi 0.02 17 3061.66 38 12. 4 Cr I 2.54 55

3056.461 [ — 3 ] 3061.825 91 29. 7 Co I 0.10 11

3056.581 [ IN ] 3061 972 67 22. 0 — Co I? 1.74 52

3056.768

3057.004

[ 5d ]

[ ON ]

Ti II- Fe II 1.16 4.07 47

109

3062.12

3062.18

61

127

23. 8

41. 5

Mn I Co I2.16

0.10

15

12

3057.134 [ 2 ] All 3.61 7 3062.29 59 22. 0 Fe II 4.08 108

3057.436

3057.643

3057.788

3057.873

3057.963

3058.075

3058.240

3058.356

3058.488

3058. 706S

[ 25 ]

[ 10 ]

[ 2 ] [-3 ]

[ 3 ]

[ 7 ] [-2N ]

[ 3 ]

[ 4 ] [3 ]

Ti IIIIFei Nil

Fe ip

Cr II

Ti II

Cr II Fe I

(Osi)

0.00 0.86

0.21

0.96

4.32

1.18

4.07

0.00

5 28

26

29

65

47

48

1

3062.52

3062.70

3062.83

3062.873

3063.045r

3063. I75r

3063.241r 3063 405r

3063. 505r

3063. 555r

3063.729r

39

27

55

72

23

44

106

43

60

119

101

12. 7

8. 3

21. 5

23. 7

7. 7

25. 6

34. 6

14. 2

27. 3

38. 9

33. 0

OH?

V II

Fe I Ce II Fe I V II Cu I

Ti n OH

OH

S 1

1.82

2.95

0.90

2.18

2.51

1.64

1.16 R 9 R 8,10

0,0

34

456

185

102

123

4

47

0,0

0,0

1

1

1

3059.094

3059.383

[ 25 ]

[ 0 ]

Fe I (Al i) Cr II0.05 3.60

2.70

9

715

3063.805r

3063.936r

78

86

37. 9

35. 6

Cr II Ni IIllFei3.87

2.95 2.42

32

3 147

3059.516 [ 2d? ] Cr II /2.71

\2.71 15

15 3064.015r

3064.12 a

147

23

48. 0

11. 0 3059.738

3060.039

[ 3 ]

[ Od ]

Ti n

Fe IIII Co I

JO. 01

tl!l6

4.08

1.96

547

109

77

3064.216r

^Ofii. S77f^

135

132

44. 1 OH-

\ji.± Co T

R 7 R 11

0 1

0

0,0 0 0

1 3

1

1

3060.12 [— 1 ] Zr II 0.04 65 21. 2 3060.24 [— 1 ] 4.8 7 Ni T 0 1 1 9fi

3060.345S [-1 ] 3064.713S 83 53. 6 Pt I 0.00 2 3060.455S [ 0 ] V I 0.04 17 3064.829r SO 26. 2 3060.548 [ 0 ] Fe I 2.99 457 3064.955r 83 27. 3 OH R 6 0,0 1 3060.633

3060,773

[ 0 ]

[ 2 ]

3065.094r 133 43. 5 |0H

Cr I (Sc II)

/R 12 IR' 6

3.09

3.45

0,0

0,0 18437

10
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

A\/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notea

3065.316r 103 33. 6 Fe II 3.94 97 3070.380r 58 25. 4 OH R' 2 0,0 1

3065.495r 34 11. 2 3070.492r 86 28. 0 OH R 6 0,0 1

3065.615r 42 13. 8 V II 2.49 112 3070.695r 68 22. 2 Fe II 3.77 68

3065.775r 22 7. 2 3070.795r 49 18. 2

3065.994r

3066. 144r

3066.227r

3066.364r

95

> 565

40. 4

' 18. 9

86. 5

39. 1

OHMn I OHAl I

Ti II

Ti II V I

R 5 2.14

R' 5 3.61

0.01

0.00

0.07

0,015

0,07

5

517

1

1

3071.005r

3071. 145r

3071.253r

3071.429S

3071.555r

38

59

132

41

27

12. 5

22. 0

43. 1

13. 5

8. 8

Cr II OH

Fe II

Ti II

Cr II

4.04 R 14

5.90

1.18

4.07

41

0,0 181

47

47

1

3066.501r

3066.694S

3066.816r

3066.994r

3067.123r

3067.262r

3067.386r

33

31

> 663

. 86. 5

16. 0

15. 0

' 42. 4

93. 3

93. 3

. 42. 4

Fe ITi 11 Fe I? p V II Fe I Fe I V II (Cr II)

Fe I OH2.73

1.16

2.95

2.51

1.61 1.79 /2.71

12.71

0.91

R' 4

313

47

456

123

5634

15

15

28

0,0 1

3071.677r

3071.798r

3071.965r

3072.115r

3072.182r

3072.328r

3072.495r

3072.670r

53

37

69

202

155

109

78

31

17. 4

12. 8

29. 4

65. 6

79. 5

35. 6

25. 5

10. 2

Fe II

Co I

Ti II OH

OHICo I Cr II?- Co I? OH?

4.15

0.22

0.03 R 5 R 16

0.17

3.86

2.28 R' 16

123

12

5

0,0

0,0

11

32

125

0,0

1

1

1

3067.657r 121 46. 6 OH R 10 0,0 1 3072.984r 243 79. 1 Ti II 0.00 5

3067.781S 110 35. 8 OH R 9 0,0 1 3073. 125r 86 39. 0 Mn I 2.18 15

3067.939r

3068. 176r

128

130

41. 8

42. 3

OHFe I Fe I

/R 11 IR 14

2.69

1.61

0,0

0,0 315a

55

3073.235r

3073.370r

3073.525r

62

15

22

28. 8

4. 9

7. 3

Fe I Cr II

Co I

3.05

4.07

1.74

549

47

51 3068.281r 103 33. 7 OH /R 8 \R'14

0,0

0,0 3073. 677r 40 13. 2 Cr I 3.12 184

3068.476r

3068.598r

3068.725r

75

63

148

24. 6

23. 4

48. 3

OH

|0HFe II

R 12 R 3 4.15

0,0

0,0 122

1

1

3073.832r

3073.997r

3074.07 a

50

52

82

16. 4

29. 0

30. 3

V I

Fe I

/0.02

10.04

2.69

15

17

313

3068.796r 102 46. 1 OH R'3 0,0 1 3074. 155r

' 143 46. 5 Fe I 3.02 457

3088.944S 52 18. 7 Fe I 1.48 53 3074.385r 39 18. 4 OH R 4 0,0 1

3069.181r 69 22. 5 OH R 7 0,0 1 3074.435r 105 34. 2 Fe I

3069.334r 57 20. 4 3074.696r 49 15. 9 V II?- 2.49 112

3069.455r 141 46. 3 Fe I 3074.905r 29 9. 4 Cr II? 4.38 73

3069.681r

3069.915r

3070.038r

80

66

55

26. 4

21. 5

17. 9

OH

V I OH

R 13

\j.\j'± R 15

0,0

11 ^

0,0

1

1

3075.035r

3075.135r

3075.239r

50

108

222

24. 7

47. 5

72. 2

OH

Fe II lITi II

R 17

3.81

0.01

0,0

68

5

1

3070.265r 129 42. 0 Mn I 2.16 15 3075.355r 103 102. 1 OH R 16 0,0 1

11

761-925—66- 4
The Solar Spectrmn—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib. (A) (mA) (F) Line Band (A) (mA) (F) Line Band

3075.455r 39 22. 6 3079. 979r 111 36. 2 |0H — Q 2 0,0 1 Fe I 3075.595r 78 49. 0 3080.116r 73 23. 9 Fe I 3075.733r 436 141. 7 Fe I 0.96 28

3080.245r 37 12. 2 OH R 2 0,0 1 3075.895r 51 33. 6 Zn I 0.00 1 (V i) 1.19 57 3080.368r 31 12. 3 V I- 1.18 57

3075.998r 57 35. 4 V 11 1.80 34 3080.422r 46 14. 9 Fe II 4.08 108

3076.265r 40 13. 2 3080.595r 45 14. 6

3076.435r 51 16. 6 Fe II 5.87 181 3080.757r 130 33. 4 Ni I 0.21 26

3076.585r 16 5. 2 Cr If 2.54 55 3080. 877r 65 27. 8

3076.750r 24 8. 5 3081.005r 56 18. 2 —V II 2.50 112

3076.831r 24 8. 0 3081.12 a 19 7. 5

3076.91 a 10 3. 7 Gd 11 0.00 10 3081.247r 58 27. 3 OH R 18 0,0 1 Fe I 3.02 457

3077.027r 44 15. 3 OH R 3 0,0 1 3081.312r 100 32. 5 Mn I 2.18 15

3077.1881' 57 33. 1 Fe II 4.07 108

3081.460r 37 14. 0 3077.225r 92 29. 9 -Cr n 4.50 103 3081.550r 82 26. 6 OH Q 3 0,0 1 3077.395r 12 4. 1 3081. 680r 91 43. 0 OH P 1 0,0 1 3077.5o8r 30 12. 3 Lu II? 1.54 4 Cr II? 3.86 32 3081. 725r 120 39. 0

3077.D40r 91 29. 7 Mo II 4.39 3081. 840r 61 33. 9 Fe I 1.48 53

3077.735r 57 19. 8 3082.035r 82 40. 4 Mn I 2.16 15 OH R 19 0,0 1 3077.835r 46 15. 1 Cr I 3.11 184

Cr II 4.47 103 3082. 168r 257 83. 6 IIAli 0.00 3 V I 0.07 17 3078.044r 141 45. 8 |Fe I- 0.96 29 OH R 17 0,0 1 3082.28 a 56 38. 8

3078.252r 29 13. 0 3082.38 a 64 24. 5

3078.387r 88 47. 2 OH R 18 0,0 1 3082.525r 40 13. 0 V II 2.04 39

3078.445r 173 68. 2 OH Q 1 0,0 1 3082. 626S 107 34. 9 Co I 0.00 10

IIFei 2.48 146 3082.75 a 34 13. 6 Mn I? 4.23 3078.662r 321 104 liTi II- 0.03 5 Fe II 5.82 181 3082. 850r 53 17. 2 Co I — 1.88 73

3078. 82or 18 11. 8 3083. 042r 85 27. 7 Fe II — 3.97 97

3078.915r 52 21. 4 3083. 168r 61 19. 8 |Fe I 2.45 197 V II 2.52 112

3079. 105r 78 25. 5 3083. 282r 110 35. 6 OH Q 4 0,0 1 3079.308r 35 13. 3 Cr II 4.50 102

3083.382r 58 28. 4 OH Q' 4 0,0 1 o079.375r 94 30. 7 Fe II — 4.15 122

|Co I fO.OO 10 3083. 503r 117 52. 9 -V I 1.22 57

11.71 49

3083. 620r 22 25. 2 Cr II 4.07 47

3079.50 a 6 2. 7 onoo 7/iQC! OUoo. / ^yo yo. / Jr e I n QQ

3079.617r 79 25. 8 Mn I 2.19 15 3083.850r 40 24. 0 3079.755r 22 7. 3 3084.055r 67 24. 8 OH R 1 0,0 1 3079.825r 20 6. 7 Fe I p 2.20 102 3084.165r 46 15. 0

12
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

A\

(ml)

Re- duced

Width

AX/\

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(inA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3084.290r 44 14. 4 3089.22 a 24 7. 9

3084.455r

3084.575r

3084. 685r

3084.795r

3084.897r

3085.043r

67

28

3. 5

4

69

64

21. 7

9. 2

1. 0

1. 3

22. 6

20. 7

Cr II —

Cr I

Ti I? OH

4.30

3.12

1.05 R 19

71

184

93

0,0 1

3089.403r

3089. 505S

3089.613r

3089. 745r

3089.868r

70

66

94

134

162

22. 7

21. 5

30. 4

58. 5

52. 6

lITi II Fe II

Co I OH

OH

1.89 4.73

0.10 Q7

/Q 2,3 IQ'2,3,7

90

158

10

0,0

0,0 0,0

1

3085. 206r

3085. 331r

3085. 395r

3085.545r

98

98

58

12

31. 7

31. 9

23. 5

4. 0

OH

Cr II

Q 5

4.07

0,0

47

1 3090.222r

3090.374r

3090.486r

129

98

112

41. 7

32. 0

40. 7

Fe I —

Co I OH

OH

OH

2.76

2.01 Q4

Q 1 Q' 1

313

77

0,0

0,0

0,0

1

1

1

3085.673r 37 16. 7 3090.733r 50 19. 7

3085.720r 79 25. 6 3090.868r 65 32. 4 OH R 21 0,0 1

3085. 885r 38 12. 3 3091.071r 356 115 Mg I 2.71 5

3085.995r

3086.111r

31

41

10. 0

13. 4

3091.213r 77 46. 4 CH

IIOH R 21 /P3

IQ' 5

0,0

0,0

0,0

2

3086.229r 75 24. 3 OH R 20 0,0 1 3091.371r 58 34. 8 OH Q5 0,0 1

3086.400S

3086.530r

3086.636r

3086.787r

3086.988r

3087.076r

3087.345r

3087.453r

3087.533r

3087.693r

3087.843r

64

122

40

177

161

54

107

71

62

58

38

20. 7

39. 5

15. 9

57. 3

52. 2

22. 4

40. 5

25. 3

20. 7

25. 3

28. 8

Co I OH

V IICo I

Ni II OH

Fe IOH

Cr I?

Co ICr II?

1.71 P 2

2.03

0.22

3.10 Q 6

3.24 Q' 6

3.09

2.01 4.47

50

0,0

39

11

7

0,0

0,0

77

102

1

1

1

3091.583r

3091.693r

3091.876S

3092.093r

3092.233r

3092.403r

3092.473r

3092.598r

3092.712r

3092.851r

3092.983r

301

45

96

102

13

48

63

41

^ 927

97. 4

32. 0

31. 2

36. 4

5. 7

34. 6

29. 2

44. 9

183

46. 2

45. 9

Fe I

Mo IIOH

CH

OH

Al I (Fe I) (OH)

Al I Mg I

1.01

1.94

Q 8

R 20 Q' 8

U.Ul 0.96 Q 6

0.01

2.71

28

0,0

0,0

0,0

QO29

0,0

3

5

1

2

1

1

3088.039r

3088. 188r

3088.355r

3088.610r

370

64

101

41

119

34. 0

32. 7

13. 3

Ti II 0.05 5 3093. 123r

3093. 346r

3093.498r

)

56

94

97. 5

V

34. 1

39. 0

V II (V II p) Fe I Cr II (Rh ii)

0.39

2.05

4.78

3.49

39

125

4

3088.752r 105 34. 2 3093.608r 46 19. 2 OH R 21 0,0 1

3088.823r 36 11. 7 3093.723r 35 12. 3 OH P' 1 0,0 1

3089.000r 60 19. 4 OH R 20 0,0 1 3093.823r 106 57. 0 Fe I 1.61 55

3089.096r 39 12. 6 V I 1.19 57 3093.883r 109 35. 4 Fe I 2.56 261

13
The Solar Spectrum—Continued

TTT Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3093.943r 70 35. 7 Cr II 4.07 47

3094.068r 24 7. 9 Fe I p 2.45 165

3094.205r 88 45. 6 V II Nb II 2.04

0.51 39

1

3094. 295r 111 35. 9

/"ITT R 19 0,0 2

3094. 364r 58 24. 9 R 19 0,0 2

3094.469r 28 9. 0 OH Q' 7 0,0 1

3094.626r 67 22. 2 OH Q 7 0,0 1

3094.724r 9 2. 9 V I 1.18 56

3094.897r 75 24. 2 Fe IL-r II 2.73

4.07 315a

47

3095. 078S 27 8. 9 Zr II 0.04 5

3095. 254r 60 21. 2 Fe I 2.69 314

3095.347r 103 33. 4 OH Q 9 0,0 1

3095.554r 14 4. 5 OH Q' 9 0,0 1

3095.724r 29 9. 5 Co I 1.74 49

3095.884r 32 10. 6 llCri Y II 2.71 0.13 11

3096.039r 82 30. 3 Fe I 2.73

3096.138r 86 31. 2 OH

Cr II P 4 4.78

0,0 128

1

3096.324r 43 18. 3 Fe II- CH

3.97 JP 2 IP' 297

0,0

0,0

3096.404r 99 40. 9 Co ITi II 1.78

1.57 52

77

3096. 549r 41 23. 2 Cr I 2.71

3096.624r 55 36. 6 -OH Q' 8 0,0 1

3096. 764r 45 47. 9 Rh II — 3.60 4

3096. 902r 647 209 Mg I 2.72 5

3097. 130r

3097.177r

i 148

J

f 33. 3

[ 29. 6

Ni I

Ti II

0.17

1.23

11

67

3097.355r 21 10. 9

3097.433r 26 12. 1 Fe II 3.94 66

3097.490r 45 18. 6 Fe I 2.42 165

3097. 618r 38 14. 6 Ti II 1.57 77

3097. 785r 68 23. 5

3097.830r 54 19. 0

3097.965r 28 8. 8

3098.072r 68 21. 9 CH R 17 0,0 2

3098.193r 98 31. 9 Fe 1 Co I 2.89 0.17 313

10

Wavelength

(A)

Equivalent Width

AX

(nil)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3098. 325r 14 4. 4

3098. 4d3S 26 8. 6 Mo II? 2.15

3098. 588r 87 28. 2 OH Q 10 0,0 1

3098. 720r 31 10. 1

/-\ TT OH R 22 0,0 1

3098.825r 53 17. 2 OH Q' 10 0,0 1

3098.968r 57 18. 4 Fe I 2.22 102

3099.115r 105 34 Ni I 0.17 13

3099.235r 68 23. 2 Zr II OH0.00 Q' 9

5 0,0 1

3099. 418r 77 29. 3 OH Q 9 0,0 1

3099.575r 65 30. 5 OH — OHP' 3 ro 2 \P3

0,0

0,0

0,0

1

3099.675r 24 16. 6 Co I 1.96 75

3099.790r 44 47. 2

3099.896r

|

3099.987r J 465

rii5

[115

Fe I Fe I

1.01

0.91

28

28

3100.150r 61 64. 5 CH

CH

R 16 R 16

0,0 0,0

22

3100.325r 263 85. 0 Fe I 0.99 28

3100. 524r 98 69. 6 Gd II 0.24 12

3100. 682r 210 69. 6 II Fe I Ti I

0.96

ri.07 \l.07

28

92

93

3100. 839r 100 38. 5 Fe I 2.40 196a

3100. 942r 61 38. 2 V II 2.03 39

3101. 012r 102 32. 9 Fe I 2.73 313

3101. 242r 123 44. 3 OH P 5 0,0 1

3101. 417r 88 47. 4

oiui .o 1 ^r Q1 fi Ni I 0 1

1

^0

3101.694r 97 77. 4

3101.895r 201 64. 6 Ni I 0.42 40

oiui.y / 4r

3102. 148r 94 30. 4 OH /Q 11 \Q' 10

0,0 0,0 } 1

3102. 299r 53 29. 2 CH —

V II R 15

0.37

0,0

1 2

3102. 369r 192 61. 9 OH /Q 10 IQ' 11

0,0

0,0

3102.519r 29 9. 4 Ti I 2.00 181

3102. 643r 68 22. 4 Fe I 0.99 29

3102.764r 48 15. 4
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3102.882r 69 22. 4 Fe I

3102.979r 24 7. 8 Ti II 1.22 58

3103. 109r 23 7. 5

3103.284r 28 12. 5 OH P' 4 0,0 1

3103.349r 80 25. 9 OH P 4 0,0 1

3103.494r 44 14. 3 Cm 4.30 71

3103.614r 16 5. 3

3103.781r

3103.819r

129

J

1

8. 8

1 40. 3

Co I

Ti (1

1.88

1.89

73

90

3103.982r 58 18. 7 Co I 1.71 48

3104.167S 48 15. 6

3104.274r 18 6. 0 Cr II? 4.50 102

3104.349r 39 13. 2 OH R 23 0,0 1

3104.571r 106 34. 1 CHTi II? R 14

1.89

0,0 90

2

3104.71 a

to 3104.79 a

1 44 14. 3

f Mgii

Mo: II

8.86

8.86

6

6

3104.914r 42 13. 7 Vii 2.05 39

3105.094r

3105.174r

1 131

r 22. 2

1 24. 9

Ti II Fe II

1.22 /3.89

6782

3105.324r 20 6. 4

3105.464r 66 21. 3 Ni I 0.27 12

3105.563r 26 11. 5 Fe II 3.89 82

3105.677r 99 31. 9 OH Q 11 0,0 1

3105.894r 21 7. 0 Coi 0.51 26

oiUD.Uo/r 1 \ T I Uxl /Q 12 10 3

0,0

0,0

3106.241r 117 37. 7 Ti II 1.24 67

3106.559r 96 31. 2 Fe II lOHZr II

3.81 P 6 1.00

68

0,0 63

1

3106.809r 26 10. 0 Ti I 1.05 92

3106.907r 76 24. 5 CH R 13 0,0 2

3107.092r 48 15. 7 Co I?- 1.71 49

3107.322r 53 17. 1 Fe I

3107.40 a 7 3. 0 Cai 1.89 16

3107.459r 36 12. 6 OHTi I P 5

1.97

0,0 181

1

3107.565r 82 26. 5 |0H

Cr II P5

4.77

0,0 125

1

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3107.725r 54 17. 4 Ni 1 0.17 12

3107.854r 29 9. 4

3107.983r 58 18. 8 Fe I 2.G9

3108.133r 11 3. 4

3108.263r 20 6. 4

3108.363r 6. 5 2. 1

3108.555r 30 9. 6 Ca I 1.90

3108.681r 63 21. 2 |Cr II- V II 4.15

2.04 5539

3108.885r 26 8. 9

3108.951r 52 16. 8 Ti II 1.58 77

3109.073r 45 14. 6 Fe I 2.47 165

3109.333r 77 24. 8 OH

CH

Q 12 R 12

0,0

0,0

12

3109.503r 25 8. 0 Co I 1.74 50

3109.622S 47 15. 1 Fe I

3109.803r 8. 5 2. 8 OH? S 3 1,1 1

3109.928r 43 14. 0 Ti up 1.22 58

3110.084r 83 26. 7 Ti II 1.58 77

3110.245r 140 45. 2 |0HFe I Q 13 0,0 I

3110.529r 39 12. 5 OH /R 24

lO' 13

0,0 0 0 }

1

3110.704r 148 47. 5 Ti II —

iV II 1.23 0.35 67

1

3110.849r 108 34. 7 |Fe I Co I 0.22 11

3110.894r 97 63. 6 Zr II- 0.09 5

3111.074r 12 4. 0

3111. 179r 38 12. 2 Zr II? 0.56 24

3111.304r 34 11. 1 Ti I 1.98 181

3111.424r 9. 5 3. 1

3111.534r 7.5 2. 4

3111.685r 57 18. 4 Fe I 2.56 260

3111.814r 87 28. 0 Fe I CH R 11 0,0 2

3111.944r 59 18. 9 Cr II 4.14 55

3112.077r 119 38. 4 Ti II-

|Fe I |0H

1.22 2.95 fP 7 IP' 6

67 455

0,0

0,0

3112.214r 96 30. 8 OH P 6 0,0 1

i5
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

ZiA/ A

(F)

Spot

ooiar

Identification

Low

ill ir or

XVOt. Line

RMT

IN O. or

V ID. Band

Notes

"Wavelength

(A)

EquiWidth

A \ (mA)

Re- duced

Width

l\A/ A

(F)

Spot

ooiar

Identification

Low

Hi r

or

xvOt. Line

RMT

IN 0. or

V ID. Band

Notes

ou ID. Z XII X .uo ^1 1 Q1 7r Do 9*^ ZO. 11 xt, y

o

Jl

3112.609r 15 4. 7 3116.982r 100 32. 2 CH R 9 0,0 2

3112.684r 28 9. 2 3117.037r 34 20. 7 OH P' 7 0,0 1

3112.804r 13 4. 2 3117.201r 72 23. 1 OH P 7 0,0 1

3112.954r

3113.097r

3113.214r

3113.384r

3113.454r

39

39

17

112

44

12. 6

12. 5

5. 5

36. 1

20. 8

V ICr 1? OH

OH

Co I

1.19

3.11

fQ' 13

Q13

1.71

56

o,o\

U,UJ

0,0

48

1

1

3117.249r

3117.432r ^117 Rfi9r

3117.768S

3117.890r

59

52

xux

63

74

35. 4

16. 7

20. 4

23. 9

Cr II -ITii

PaTelt Ti II OH

OHTi I

4.07

1.07

u.yy

1.23 Q 14 P 8

1.05

46

92

zy

67

0,0

0,0 92

1

1

3113.591r

3113.666r

3113.838r

3114.078r

3114.125r

3114.316r

89

50

66

74

125

125

28. 2

21. 1

21. 1

33. 5

40. 5

40. 1

V II Fe ip

Ti I Ni 1 Fe n CH

2.90

2.47

2.00

0.11

3.89 R 10

174

165

181

24

82

0,0 2

3118.141S

3118.253S

oi lo.oyur

oi xo.OD i r

3118.656r

3118.827S

66

53

lift

122

59

21. 2

17. 0

^ft OO. 0U 90 7

39. 2

19. 1

ITii Cr II Co I V TT V II

TJi T IN 1 X Cr II

Ti II?

2.02

4.17

0.17 nU.ooq^

q 1

0

o.iy

2.42

1.08

18155

11

i

y**

5

27

3114.353r 94 53. 0 CH R 10 0,0 2 3119.035r 23 7. 4 Fe I 2.76 315a

3114.483r

oil'i.D/or

OlH.OlOT

3114.778r

3115.043r

13

QQoy

101

84

5. 5

1io. Qy

iO. 0

32. 4

26. 8

Y II? Cr I?

r e II OH

Fe I

3.41 3.12

o.oy Q 14

58

oZ

0,0 1

3119.198r

3119.351r

3119.504r

3119.678r

11

88

128

120

24. 8

28. 2

41. 0

38. 6

V n?

Fe I OH

CHCr I (Til)

2.52

2.43 Q 15 R 8

3.09

1.50

110

194

0,0

0,0 183

137

12

3115.283r 43 14. 0 Cr 11 4.17 54 3119.802r 97 31. 2 Ti II 1.24 67

3115.353r

3115.468r

27

30

8. 6

9. 8

Fe 11 Mn I

i? e II 3.37

o.y / 38

Oft yo

3120.012r

QI on hqot*

27

8

8. 7

9 ft

OHFe II

r'l-v T? K^O Ii

Q' 15

3.97

1 QQ i,oo

0,0 96

'7 A

1

oiio.ooor OO 111 ^ 1. o

qi c)(\ 9q7r Uo 90 9 zy. z r e I 9 7A Z. / D

3115.668r 57 18. 2 F« I Cr n

3.07 /4.07

15.32 46

3120.372r

3120.430r

151

100

48. 4

56. 3

Cr II Fe I

2.43

2.45

5

194

3115.883r 31 10. 1 Fe I 3.02 456 3120.602r 41 13. 1 OH 0 5 0,0 1

3116.053r

3116.263r

3116.393r

3116.503r

3116.633r

28

82

46

140

149

9. 1

26. 2

14. S

57. c

47. c

!

)

Fe I Fe I Fe I

|Fe I Fe II

2.45

2.59

2.20?

1.01 3.89

165

261

28

82

3120.732r

QI on QITf

3121.081r

3121. 160r

3121.419r

60

i O

35

140

54

19. 2

OA 0

16. 7

44. 8

17. 3

Vn

Zr I

J e I Cr II? V II Co I

2.56

0.52

4.38

0.39

0.00

13837

72

1

9

3116.727r 69 28. ^ Ni ICr II 3.19

4.77 95

126

3121.604r 119 38. 3 Ti II ||Co I 0.00

0.10 411

16
The Solar Spectrum—Continued.

Wavelength

(A)

Equivalent Wiath

AX

(inA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

ol21.7oor 84 27. 1 *Jil |Fe I K / 2.221,

102

1

3121.859r 50 19. 3 Cr II- OH

4.38 R 9 72

1,1 1

3121.969r 37 11. 8 Cr II 4.15 55

<J122.079fc> 57 18. 0 il II l.z4 08

3122.219r 56 24. 4 OH

CH

R 6 R 7

1,1 0,0

12

3122.317r 145 46. 5 Fe I TT

KjIX K 7 A A

0,0 0

A 0100 C?A— 1 A A 144 46. 2

r\ TT Url

OHCr II Q 15

4.18

A A

0,0

0,0 54

11

olzz.oD4r A 1 41 la. 7 1? e I 0 'TQ iS./O ol4

ol22.784r 5 1. 6 Au 1

1 1 A 1.14

-11

ol22.9(J9r

olzz.y49r

i 62

J

17.7

1. 4. b

V II

r\xx UH

0 AA

li 5

17o

1,

1 0100 Ano« 08 111 A AA u.yu 0/

00 11. 0

ol^o.£54yr 00 1 A 1 /. U r e I 0 /I 0 i04

oizo.44ar OQ A 1 y. 1 Uxl K. 11 1,1

-i1

ol.iO.00lr dU ly. 4 r e I

1 -t 11 0. 0

T> V» t9 rCn li A AA U.OO oUo. / / or A 0 lO. D 11 I 0 A/1 181 0100 nr:n» oizo.yoyr Zi 0 CI / \ 1 r Uxl Jr y A A

0,0 1

ol^4.U9/r 0000 1 A C 10. 0 Fe I 0 AQ 2.48 loo

ol<i4. Joor 1 A 0. 6

3124.488r 11 3. 8

3124.638r 18 5. 9 OH? R 26 0,0 1

oli4.DSor 1

-1 11 0. 4

ol^4.oUor 0 A oO 1 A C 10. 0 UH —

Ge I

T>K 1012

0.88

1,1

1

1

ol.^4.yi»r l.i4 'TA A

<o. y Cxi

OH

Ix 0 Q 16

A A

0,0

0,0

0

1

3124.998r 149 47. 8 Cr II 2.45 5

3125.053r 111 57. 0 Cr u CH

4.30 R 6 70

0,0 2

dliio.^sor loo 49. 8

\r TT V II 0.32 1

3125.467r 47 14. 9 Cr n 4.18 55

3125.667r 152 48. 6 |Fe IFe I p

/0.99

12.40 2.40

28

160 194

3125.920S 48 15. 4 Zr II 0.00 5

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Not<

3126.207r 150 48. 0 Fe IV II 0.37 1

3126. 332r 33 12. 0 OH R 9 1,1 1

3126.472r 37 11. 8 OH R 8 1,1 1

3126. 617r 75 24. 0 CH

OH

OH

R 12 R 10 R 13

1,1

1,1

1,1

2

1

1

3126. 767r 80 25. 8 Fe I

3126. 847r 44 17. 7 Fe I 2.56 260

3127.047r 24 7. 7 OH R 7 1,1 1

3127. 117r 13 4. 1

3127.247r 29 9. 2 Co I 0.43 26

3127.362r 33 10. 6 OH R 11 1,1 1

3127. 491r 29 9. 4 — Nb II 2.16

3127.671r 86 27. 7 lOH

CH

Ti I?

Q 16 R 5 1.97

0,0

0,0 180

12

51 16. 4 OH R 5 0,0 2

00 11 7 WAX OHXL 0 P 9X , X 0,0

X

1

3128.289r 73 23. 2 Sc II |0H

3.46 P 9 39

0,0 1

3128.386r 47 15. 3

3128.521r 60 19. 4 OH JO 6 IR 12

0,0

1,1 }'

3128.706r 98 31. 3 Cr II 2.43 5

3128.776r 32 15. 1 OH

Y II? R 14

3.37

1,1 51

1

3128.897r 47 15. 1 Fe I 1.56 54

3129. 007r 25 8. 1 Co I —

Fe II 0.51 3.97 96

3129. 107r 60 19. 4 Fe I

3129. 177r 32 12. 2 Zr II Fe I 0.53 2.45 23

161

3129.320r 85 27. 2 Ni I-

|Fe I 0.271.48 1252

3129.532r 34 10. 9 OH R 5 1,1 1

3129.767r 50 16. 0 Zr II 0.04 5

3129.947r 23 7. 3 Y II? 3.41 51

3130. 137r 48 15. 4 |0HTi I R 13

1.98

1,1 180

1

3130.267r 104 33. 2 |V II- OH

0.35 P 101 0,0 1 3130.414m 85 27. 3 Be II 0.00 1 5
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3130.567r

3130.631r

3130.795r

77

63

106

24. 7

32. 7

33. 9

|0H

Fe II

II Ti 11 Ti 1 (Nb n)

Q 17

3.77

0.01

0.44

0,066

4

1

1 3134.937r

3135.046r

3135.181r

3135.356r

87

24

24

92

27. 8

8. 3

7. 8

29. 4

V 11

Ti I Y II Fe II Cr n

2.52

2.00

0.18

3.89 4.77

122

180

11

82

124 3131.058m 80 25. 6 Be 11 0.00 1 5 3135.453r 62 19. 7 Fe I

3131.236r

3131.361r

3131.446r

3131.526r

3131. 708r

3131. 806r

3131.951r

3132.055r

3132.189r

38

29

44

42

51

18

37

137

89

12. 2

9. 3

14. 1

13. 5

16. 5

6. 8

13. 9

44. 0

36. 2

|Cr ITm II

OH

OHCr II

Fe II Ni I Co I

Cr II OH

3.11 0.00

R 15 R 4

/4.17

\4.18

4.08

3.31

1.74

2.48 R 14

183

1,1

1,1 55

53

107

9448

5

1,1

1

1

1

3135. 589r

3135.706r

3135.870r

3136.015r

3136.085r

3136.195r

3136.345r

3136.506r

3136.590r

3136.707r

53

87

69

43

28

53

46

82

145

141

17. 1

28. 0

22. 1

13. 9

8. 8

17. 1

14. 8

26. 4

46. 2

45. 1

Fe I Cr II Fe I Ca I Fe I p OH

|Fe I CH

V II OH

II Cr II- Co I

2.73

4.43

2.45

1.88

2.40 Q 2

R 2

2.51 Q 18

2.45

0.00

94

194

15

160

1,1

0,0

122

0,0

5

8

1

2

1

3132.288r 73 30. 4 Mn I?- 4.33 3136.890r 84 26. 7 OH P 11 0,0 1

3132.521r

3132.635r

3132.821r

3133.066r

96

84

49

69

30. 8

34. 5

15. 7

22. 1

Fe I -Fe I Cr I

||Fe IISc II

3.21

3.12

3.89

3.47

578

183

8239

3137.025r

3137.100r

3137.330r

3137.445r

47

29

88

32

15. 0

9. 3

28. 2

12. 3

Co I?-

OH

Cr II? Co I Co I

1.74 R 2

5.33

0.22

2.04

48

1,1

10

108

1

3133.216r 87 28. 0 OH Q 17 0,0 1 3137.560r 31 9. 8 Cr II 4.15 54

3133.335r 95 30. 4 V II 0.33 1 3137.710r 26 10. 2 OH R 16 1,1 1

3133.491S

3133.59 a

3133.676r

3133.966r

3134.116r

62

7

7. 5

108

414

19. 9

2. 7

2. S

62. 7

132

Zr II Nd II

Fe I p — OH

Fe I |Ni I

0.96

2.42 R 3

0.96

0.21

63

161

1,1 28

25

1

3137.765r

3137.896r

3138.014r

3138.076r

3138.206r

66

53

34

19

8

21. 0

17. 1

10. 9

6. 5

2. 6

Co I OH

OH

V II- OH

Cr I

1.78 P 1 Q 3

3.76 R 17

3.12

49

1,1

1,1

205

1,1

183

1

1

1

3134.337r

3134.396r

3134.541r

106

63

28

55. 9

41. 2

11. 9

|0H

Cr II Fe I? OHOH

P 10

4.41

2.69 R 16 Q 1

0,0

94

1,1

1,1

1

1

1

3138.306r

3138.406r

3138.518r

3138.674r

6

25

78

57

1. 9

8. 1

24. 8

18. 3

Cr I? Fe I Fe I

Zr II

3.85

1.56

0.09

53

5

3134.626r 60 22. 3 OH Q' 1 1,1 1 3138.786r 37 11. 9

3134.716r 48 24. 4 OHHf II R 15 0.38

1,15

1 3138.916r

3139. 106r

27

11

8. 8

3. 6 Fe ip 2.45 161

18
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX (ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3139.164r

3139.306r

57

23

18. 3

7. 3

OH

CH

Q 18 R 1

0,0

0,0

1

2

3143.486r 73. 1 V II CH

2.51 /Q 14 to IQ 17

122

0,0

0,0 }^

3139.486r

3139.666r

13

61

4. 3

19. 6

Fe 1 Fe I 2.40 155 3143.575r 33. 4 CH /Q 13 IQ 18

0,0

0,0 }^

3139. 761r 107 34. 2 II Vn

Sc nOH

2.51 3.49 Q4122

39

1,1 1

3143.764r 133. 3 II Ti II CHOH

0.03 Q 11 P 12

4

0,0

0,0 2

1

3139.937r 106 25. 1 jFei

Co I (Cr II) 0.10 4.14954

3143. 896r 15. 9 CH

Cr II Q 9, 10

4.43

0,094

2

3140.016r

3140.209r

3140.388r

3140.511r

3140. 757r

3140.938r

36

50

81

62

101

13

16. 6

16. 1

25. 9

19. 8

32. 1

4. 1

Cr II Fe I OH

|0HCa I

4.78

3.24

P' 11 P 11

1.89

124

578

0,0

0,015

1

1

3143.996r

3144. 116r

3144.236r

3144.326r

1237

73. 1

15. 9

15. 9

15. 9

CH

Fe I CH

CH

CH

lOH

Q8, 9 3.21 Q6, 8 fQSto

Q 5 Q 7 IQ 21 Q 6 Q 6

0,0 578

0,0

0,0

0,0 0,0

0,0

0,0

1,1

2

2

1

2

1

3141. 106r

3141. 181r

39

54

15. 8

17. 2

CH?-

Dy II Cai

R 5

1.89

1,1

15

2 3144.453r

3144.501r

33. 4

33. 4 CHFe I CH

Q5

2.47 Q4

0,0

161

0,0

2

2

3141.296r

3141.513r

3141. 666r

3141. SOlr

3141.908r

29

56

23

5. 5

68

9. 5

18. 1

7. 3

1. 7

21. 8

Ti I (Vii)

Ti I Cr II? -OH

0.90

2.60

2.13

5.32 Q 5

66

152

192

175

1,1 1

3144.629r

3144.737r

3144.816r

3144.925r

37

67

15. 9

33. 4

17, 7

21. 3

CH

V IIIFe II

CH

Fe I

/Q 3 IQ 22

2.52

3.90

Q 1 2.43

0,0

0,0

122

82

0.0 195

2

3142.021r

3142.156r

3142.224r

3142.470r

3142.511r

3142.676r

3142.731r

3142.897r

3143.016r

3143.156r

3143.242r

3143.336r

20

21

58

1 123

13

32

88

75

27

76

23

6. 5

8. 1

18. 4

f 38. 7

[ 0. 5

4. 7

10. 1

28. 1

23. 7

9. 3

25. 6

7. 8

OH

OHV n?

Fe II |FeiVii

OH

Mn I Cr II Fe I OH

Ti i?p Fe I Til

Q' 5 R 18

2.90

1.67

2.45

2.22 P2

2.89

4.41

2.28 Q 19

0.00

0.00

2.04

1,1

1,1 172

7

16452

1,1

85

144

0,0

28

7

180

1

1

1

1

3145.091r

3145.136r

3145.369r

3145.526r

3145.725r

3145.791r

3145.976r 3146 106r

3146.256r

3146.301r

3146.466r

123

80

128

71

115

80

74

18

69

18

47

39. 3

40. 4

40. 8

22. 6

36. 6

34. 5

23. 7

5. 9 2L 9

7. 8

14. 9

|Fe I Cr 11 (CH)

Ni IV II OH

Ni I Cr II CHCH

V II

V II Fe I Fe I

2.99

2.45 Q 23

0.00

/0.35

10.39 Q 19

0.17

4.41 Q 24 Q 24

0.37

2.56

2.42

455

5

0,0

7

1

1

0,0

11

85

0,0

0,0

1

138

160

2

1

2

2

19
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or

itot. Line

RMT

No.

or

V ID. Band

Notes Wavelength

(A)

Equivalent Width

AA

(mi)

Re- duced

Width

A \ /\ AA/

A

(F)

Spot

Solar

Identification

Low

E P

or

rtot. Line

RMT

No.

or

V ID. Band

Notes

3146.598r 106 33. 9 CHCH

nwyjti

Q 25 Q 25

0,0

0. 0

1 1 1, i

22

1

3151. 005r

olo i.uy ix

66

90ZU

20. 9

D.

OH

1 1 I i

P 13

n 00

0,0

OQ

1

3146.756r

3146.934r

3147.068r

48

73

89

15. 3

23. 2

28. 2

Fe II OH

Co I

3.77 Q7

0.17

67

1,1

10

1

3151.237r

3151. 352r

69

114

21. 9

36. 2

Ni I Ca I Fe I (Vii)

1.90

2.73 2.54

15

311 138

3147.235r

3147.267r

> 152

) yu

( 34. 3

1 25. 1

V

A OU.

Cr II

Fe Iyj 1

1

KJ Ll —

|0H

/2.48

14.17

n A

r o P 12

5 54

0,0

11

111

3151. 517r

olOi.D'izr

3151. 863r

3152.000r

3152.117r

11

114A

82

75

66

3. 5

4. 4

26. 5

23. 8

21. 1

K^ci I Fe I

OH

1i.yu on

0.05

Q7

110

7

1,1 1

3147.599r 102 32. 4 Fe ICH Q 26 0,0 2 3152.262r 142 45. 1 lITi II- OH

0.12 Q 2010

0,0 1

3147.784r 100 31. 9 Fe I 3.02 455 3152.457r 38 12. 2 OH P 4 1,1 1

3148.042r 114 36. 2 Ti II 0.00 4 3152.597r 10 3. 3

oi'lo.lOor

3148.307r

3148.440r

DO

43

103

on fi Zu. D

13. 8

32. 8

Mn I -OH?

OH

|Fe I ^r I

Q' 5 Q 5 2.43

9 07

1,1

1,1 194

111^ 1 10

1

1

OlO^. i o iT

3152.857r

3152.957r

DO

14

58

90 Q

4. 4

18. 4

V^O 1 — CH

Cr I? OH-

\jn

9 01 P 3

3.00

P' 2 P 9

7*^ 0,0

116

1,1

1 1 1,1

2

1

1

3148.797r

3148.900r

1 A

61

67

A A

19. 4

21. 4

TTq T? r e I

!

o on

3153.058r

3153.191r

50

118

16. 0

37. 4

Fe I

|Fe I OH

J Z.ZU \2.95

2.45 Q 9

yy 452

161

1,1 1

3149.122r 8 2. 5 Cr II? 4.41 84 3153.319r 95 30 Fe I 2.45 160

3149.317r

3149.397r

3149.497r

3149.642r

3149.724r

3149.852r

3149.898r

3150.077r

3150.229r

3150.307r

OlOV.il IT

3150. 512r

3150.652r

3150.747r

63

20

27

11

55

1 133

93

49

94

oy

20

18

73

20. 0

7. 6

8. 7

3. 6

17. 4

f 31. 2

[ 20.6

29. 5

17. 2

29. 8

6. 5

5. 7

23. 3

Co I

Fe I

OH

(Cr II) OH

OHCr II Fe i?p Fe IOH

Co I? Ca I

0.17

2.95

Q 20

4.14 Q 8 Q 6

4.15

2.48

3.28

P' 1

Jr Z

1.90

9

453

0,0 54

1,1

1,1 54

161

578a

1,1

0,0

15

1

1

1

1

2

3153.568r

3153.751r

3153.870r

3154.005r

3154.120r

3154.200r

3154.420r

3154.493r

3154.595r

3154.643r

3154.788r

3154.940r

3155.130r

27

70

10

31

57

144

137

93

82

75

76

18

101

8. 6

22. 3

3. 2

10. 0 2L 4

45. 7

43. 6

29. 5

26. 0

45. 3

24. 1

5. 7

32. 0

|Cr ITi I? Fe I

Fe I

|Fe II Ti II Fe I OH

Fe I Ni I-

|0H

OH

Co 1

|Cr I Fe I

3.37

1.61

3.77

0.11

2.18 P 13

2.47

1.95 Q 8 0 9

1.88

2.98

2.48

200

53

66

10

100

0,0 161

78

1,1

0,0

73

115

161

1

1

1

3150.832r 16 5. 5 Co I?

20
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(uiA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3155.290r

3155.405r

3155.622r|

3155.658rj

3155.795r

85

35

160

66

27. 1

11. 2

f36. 2

136. 2

20. 9

Fe I V II CH

|Ti II Zr II Fe I p

2.43

2.22 P 4

0.13

0.93

2.40

193

51

0,0

10

63

192a

2

3159.261r

3159.349r

3159.436r

3159.531r

94

95

39

122

39. 0

30. 2

15. 4

38. 7

Rh II |Fei

Fe II?- V 11? Fei

INi I OH

3.15

2.G1

4.15

2.37

2.76

0.17 Q 21

2 259

120

83

11 0,0 1

3155.905r1

3155.940rl

3156.090r

3156.190r

84

6

18

[23. 8

1 6. 4

1. 9

7. 0

CH

Fe II

OH

P 4

3.77

P' 3

0,0

67

1,1

2

1

3159.D71r

3159.831r

3159.935r

85

38

127

38. 6

14. 4

40. 4

Co I -Cr II ||CH- Mn I

(0.22 10.58

4.17 Q 13

2.92

926

54

1,1 2

3156.272r

3156.450r

3156.565r

137

65

48

43. 6

20. 7

15. 4

Fe I Fe I CH

Pt I

3.24

2.99 Q2

1.26

578

454

1,12 2

3160.082r

3160.213r

3160.347r

46

121

72

16. 0

38. 5

22. 8

OHCr II Fe I Fe I

P 4

4.15

3.26

2.40

1,1 54

578

192a

1

3156.727r 38 12. 2 CH Q 4 1,1 2 160.472r 35 12. 3

3156.845r

3156.916r

3157.031r

3157.143r

69

89 234

148

33. 9

40. 9

74. 1

88. 6

OH

-CH

Fe I (Zr II) |0HFe I p

Q 10 Q 5

2.42 o!53 Q21

2.28

1,1

1,1

160

23

0,0 144

1

2

1

3160.612r

3160.647r

3160.801r

188

)

109

(27. 2

[48. 1

34. 7

Cri

CH

Fe I

Vii-

|0H

2.98 Q 14

2.42

(2.26 \2.56

fQlO

IQ 11

115

1,1

155

65

138

1,1 1,1

2

3157.294r 49 24. 6 Fe I 3160.923r 84 37. 0 Fe I p 2.47 160

3157.411r 189 59. 9 Ti II 0.01 4 3161.033r 68 21. 7 Mn I 2.30 19

3157.501r 123 64. 0 -OH Q9 1,1 1 3161.204r 147 46. 6 Ti n 0.11 10

3157.634r

3157.751r

46

95

18. 2

30. 1

CH

CH

OH?

Q8

Q9

P 5

1,1

1,1

1,1

2

2

1

3161.382r

3161.423r

1 145

f 39.8

i 14. 8

Fe I CH1.56 P 6 52

0,0 2

3157.882r

3157.996r

3158.049r

3158.191r

3158.351r

153

95

90

46

48

48. 6

30. 1

63. 0

14. 7

26. 9

llFeiVii

Fe I Cr II- Mo I Fe II p —

2.47 2.22

2.42

4.38

0.00

3.94

164

50

159

70

2

95

3161.553r

3161.653r

3161.774r

3161.901r

3161.952r'

46

44

147

44

123

14. 6

14. 2

46. 6

21. 1

39. 1

Fe I Co I

Ti II OH

|Fe I Fe II

2.45

1.96

0.12 P 14

2.40

1.69

195

73

10

0,0

160

7

1

3158.403r 137 43. 5 CH P 5 0,0 2 3162.123r 10 3. 3

3158.521r 96 30. 4 OH P 14 0,0 1 3162.178r 13 4. 2

3158.633r 80 32. 3 CH P 5 0,0 2 3162.353r 107 33. 8 Fe I (2.45 12.69 159 310

3158.783r

3158.886r

3159.011r

3159.111r

78

288

70

83

60. 2

91. 2

43. 4

33. 3

Co I CH

Ca 11 Fe I Cr II

0.10 Q 11

3.12

2.95

2.48

10

1,1

4

452

5

2

31 62 433r

3162.570r

3162.703r

3162.803r

33

172

26

68

15. 3

54. 4

11. 2

21. 6

CH

Cr II

Ti II V II Fe II

Q 16

4.07

0.13

2.38

4.15

1,1

46

10

83

120

2

21
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(inA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3162.923r 8 2. 5

3163.028r

3163.095r 1 101 1 4.71 27.4

V II Fe II

2.37

1.67

84

7

3163.223r 45 14. 3 OH P 6 1,1 1

3163.423r 89 28. 2 Nb II- 0.38 Q 17

1 1,1 2

3163. 558r 4 1. 2

3163.683r 13 4. 2

3163.768r 51 16. 2 Cr I 3.00 115

3163.888r 96 30. 8 Fe I

3163.930r 78 50. 7 Cr II- CH

4.30 P 7 69

0,0 2

3164.068r 63 20. 0 CH P 7 0,0 2

3164.173r 36 11. 5 Ni I 1.95 79

3164.295r 84 26. 5 Fe I Zr II 2.45

0.71 16350

3164.418r 61 19. 1 OH P 5 1,1 1

3164.548r 72 22. 9 OH Q 11 1,1 1

3164.685r 70 22. 3 CH Q 18 1,1 2

3164.833r 80 25. 5 |V II OH

1.10 Q 22

8

0,0 1

3164.898r 32 17. 0 Ti II

3165.005r 90 28. 6 Fe I 2.42 155

3165.084r 18 5. 7 Feip 2.45 194

3165.157r 72 22. 8 OH

Fe I p Q 122.18

1,1 100

1

3155.266r 62 20. 7 Fe I

3165.35 a 7. 6 2. 8

3165. 420r 23 7. 7 Zr II 1.00 63

3165. 512r 64 20. 4 Ni I 0.03 21

3165.675r 16 5. 1

3165.875r 95 29. 9 Fe I 2.45 160

3165. 958r 84 26. 7 Zr II 0.16 5

3166.130r 71 22. 6 CH Q19 1,1 2

3166.255r 83 26. 4 Fe IZr II 2.45

0.80 15548

3166.335r 46 14. 7 OH P 15 0,0 1

3166.438r 108 33. 2 Fe I 2.56 259

3166.595r 46 18. 2 Fe I p 2.20 100

3166.674r 120 37. 9 CH

Fe II P 81.67

0,06

2

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3166.767r 69 35. 7 CH P 8 0,0 2

3166.865r 16 6. 2

3166.985r 50 15. 7 Fe I 3.02 455

3167.177r 53 16. 7 OH Q 22 0,0 1

3167.295r 3. 5 1. 0

3167.415r 19 5. 9 V 11 3.79 217

3167.595r 38 12. 2

3167.790r 1 14. 3 Fe 1 CH

2.18 Q 20

99

1,1 2

3167.859r

y 199

] 37. 0 Fe II 3.81 66

3167.910r j I 17. 5 |Fe I Fe II p3.24

3.89 57882

3168.045r 20 8. 5 Co I 2.08 108

3168.151r 1077 340 V II 1.07 8

3168.280r 24 8. 2

3168.435r

3168.528r

I 217

J [ 61. 9 Ti II 0.15 10

3168.672r 100 58. 0 OH Q 12 1,1 1

3168.856r 89 28. 1 Fe I 2.47 160

3168.955r 79 25. 0 -OH P 7 1,1 1

3169.075r 24 7. 9 OHFe I pP' 6

3.57

1,1 813

1

3169.192r 48 15. 2 |0HCr II P 6

4.78

1,1 123

1

3169.366r 87 27. 4 CH P 9 0,0 2

3169.427r 71 28. 6 CH P 9 0,0 2

3169.616r 74 23. 5 OH P 15 0,0 1

3169.753r 81 25. 7 Co I 2.08 109

3169.861r 56 18. 5 OH Q 13 1,1 1

3170.006r 18 5. 7 Dy II

3170.128r 39 12. 5

3170.256r 19 7. 7

3170.344r 107 33. 9 Fe II 1.69 6

3170.481r 47 15. 8

3170.54 a 9 3. 1 3170 711r 65 20. 7 Ni I 1.93 78

3170.806r 13 4. 2

3170.985r 43 13. 9 Fe I?

3171. 141r 22 7. 0

22
The Solar Spectrum—Continued

VV ftVc"" length

(A)

EquiV MiC 11 Li Width

AX

(ml)

ReLI UL-cU Width

(F)

Spot Identification

Low

ill jr or Rot. Line

RMT

Nr. IN U. or Vib. Band

Notes

VV dVL,** length

(1)

Equixr c\ 1 An f V tXlCll \j Width

AX

(ml)

Re-

(_1 U C(JCJ Width

AX/X

(F)

Spot Identification

Low

F. P

or Rot. Line

RMT

i>i M<->o. or Vib. Band

Notes

3171.216r 13 4. 3 3175.39 a 16 9. 1

3171.355r

3171.466r

3171.665r

3171.771r

3171.936r

3172.051r

3172.087r

3172.297r

3172.377r

3172.507r 3172 fi47r

3172 722r

3172 852r

3172.997r

73

12

75

33

19

1

144

46

7

43

19

12

16

58

23. 1

3. 7

23. 8

11. 1

7. 2

( 26. 2

1 31.5

14. 9

2. 4

13. 3

6. 2

4Tt. n

1

18. 3

Fe I

Fe I

IIFei Cr n

Fe I p (CH)

Fe I

— Ru II?

Ti I Tm II? OH

/1.48

\3.05

2.48

/2.20

12.45 4.38

2.20 P 10

2.76

4.18

0.90

0.03 Q23

52 548

160

99

193

71 100

0,0 312

65

8

0,0

2

1

3175.451r

3175.555r

3175.710r

3175.820r

3175.988r

3176.100r

3176.299r

3176.351r

3176.445r

3176.600r

3176.675r

3176. 835r

3176.930r

3177.080r

3177.302r

119

29

12

12

57

7.5

83

94

37

5

6

7

3

14

91

37. 5

11. 5

3. 8

3. 9

18. 0

2. 4

41. G

29. 8

14. 5

1. 5

2. 1

2. 4

1. 1

4. 6

28. 8

Fe I Mn I Mn I?

Fe I

Ni I Fe I

W I?

Hf II?

Ru II Co ICH

2.40

4.34

4.33

2.88

1.95

2.61

0.21

0.61

2.40

P 12

155

333

77

258

5

8

2

0,0 2

3173.210r 67 21. 2 OH Q 13 1,1 1 3177.542r 74 23. 3 Fe II 3.90 82

3173.408r 87 27. 4 Fe I 2.88 333 3177.6S0r 61 19. 3 OH P 16 0,0 1

3173.550r

3173.605r 3173 fi83r

3173.840r

3173.950r

3174.055r

1 121

12

5

26

f 15.4

[ 28. 1 0^— Q lO. t7

4. 0

1. 5

8. 2

Co I Cr II? Fei

Fe I OH

Vii

1.88 4.41

2.86

2.20 0 11

2.38

7283

333

101

0,0

84

1

3177.822r

3178.021r

3178.161r

3178.326r

3178.43 Ir

3178. 509r

56

129

58

5

26

68

17. 7

40. 6

18. 3

1. 9

8. 5

22. 4

Fe I OH

Mn I —

Fe I

2.40 Q 14

2.32

3.02

156

1,1

19 454

1

3174.155r

3174.221r

3174.380r

3174.490r

23

39

35

69

7. 5

12. 3

11. 0

21. 7

Co I Fe I p

OH

OH

(Vn)

2.70

3.28 P7

P 16

3.80

138

578

1,1

0,0 217

1

1

3178.641r

'^1 7R 7R(\r

^1 78 Qfifir

3179.061r

'

18

16

21

6. 1

5. 8

1 7 4

11. 3

Ti II Fe I Cr II? Fe I3.84

5.33

2.43

120

173

192a

3174.697r 98 31. 0 CH P 11 0,0 2 3179.166r 73 45. 4

31 74 7S'ir ^1 10. 2 Ti II ^1 7Q S49r fJOKJ 1 S9 Ca II 3.15 4

3175.045r

Q4.

69

*i J. o

25. 8

OH

ISni

OH

(Fe ii)

O 1 4

0.42 P8

4.73

1 1 X , 1

1 1,1 157

1

J.

1

o^1 7Q "^r i. 1 a. OX or

3179. 671r

Q9

17

\JO. o

9. 2

Fe II Fe IFe I4.73

l!61 157

52

3175.165r 26 8. 2 3179.901r 71 26. 3 CH P 13 0,0 2

3175.314r 83 26. 4 OH

Fe I Q 232.76

0,0 1 3179.966r

3180.121r

34

59

17. 4

22. 3

OH

-Fe II

P 8

4.74

1,1

157

1

23
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. rJanu

Notes Wavelength

(A)

Equivalent Wiuth

AX

(mA)

Re- duced

W idth

AX/X

(F)

bpOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3180.236r 53 17. 8 Fe I 2.45 155 3184. 114r 67 21. 1 Ti II 0.01 3

3180.491r 82 26. 2 OH- Q 15 1,1 1 3184.210r 49 15. 4 Fe I

3180.710r

3180.746r 1 476

fllO [no

Cr II Fe I

2.54

0.09

9

7

3184.379r

3184.442r

93

32

29. 1

17. 4

Ni I Fe II p

0.27

3.81

11

67

3180.881r 27 8. 7 3184.547r 20 6. 8

3180.991r

3181. 131r

olol.2Ulr

ol»l.z7br

c5181.42Ur

16

9.5

1 oo

7o

5. 0

3. 6

1 o o

C '7 A 01. 4

Fe I

II UH

Cr II

OIK

r y 2.54

A4

t

-1 1,19

1

3184.615r

3184.762r

3184.895r

3185.022r

3185.092r

49

19

130

96

25

15. 4

5. 9 4L 0

34. 1

13. 3

Fe I

Fe I CH

Feji

/2.45

12.45

0.05 P 15

3.81

155

162

7

0,0

67

2

3181.531r 91 35. 4 Fe I 2.59 258 3185.222r 17 6. 3

3181. 641r 50 15. 7 OH Q 24 0,0 1 3185.327r 114 35. 8 Fe II 1.72 7

3181.7451- 27 8. 5 Ni I 1.93 78 3185.388r 82 38. 8 V I 0.07 14

3181. 864r 71 22. 4 Fe I 2.87 333 3185..564r 39 12. 3

3181.911r 49 15. 4 |Fe I Zr II

/2.47

\ O AO [o.UZ 0.71

155 oUo

48

3185.674r

3185.804r

55

12

17. 4

4. 0 OH P' 9 1,1 1

3182.061r 78 24. 5 Fe ICH

/2.42

12.85 P 9

159 333

1,1 2

3185.979r

3186.104r

46

86

14. 6

27. 5

OH

OH

P 9 P 17

1,1

0,0

1

1

3182.121r 44 17. 1 Co I 2.01 73 3186.272r 25 9. 1 Fe I

3182.246r

3182.316r

3182.471r

3182.651r

01 CO Qn'7».

o 1 oo o cr\« oloz.ooUr

oloz.yyur

43

37

81

35

o4

41

85

13. 5

11. 6

25. 6

11. 0

14. /

12. 9

2b. 7

CH

-V II

Zr II

II Fe I Ni I

P 14

2.60

0.56

2.20

1.99

0,0

150

23

10078

2

3186.383r

3186.453r

3186.634r

3186.752r

3186.794r

3186.86 a

3186.964r

63

124

18

> loo

98

64

26. 2

39. 0

6. 8

r 43. 9

1 19. 2

43. 0

28. 7

Co I OH

Ti I

Fe II -Fe I

0.17 Q 16

0.00

1.69

2.22

8

1,1

27

6

100

1

3183.05 a 47 22. 6 3187.064r 15 6. 3 Mn II 4.69

3183. 124r 87 27. 4 Fe II 1.69 7 3187. 168r 63 20. 1 Fe I 2.88 333

3183.261r 62 19. 4 Ni I 1.95 78 3187.308r 69 21. 8 Fe II 4.15 120

61o6.6i.tT

3183.422r

3183.520r

ocDO

73

36

11. 8

23. 0

11. 3

Cr II V I OH

(Ce II)

4.41

0.02 Q 15

0.56

82

14

1,1 216

1

3187. 556r

3187.713r

3187 .899r

87

111

13

27. 3

34. 9

4. 2

CH —

CH

V II Rh II

P 16 P 16

1.07

3.45

A A

0,0 0,0

84

o

Z

2

3183.581r

3183.762r

3183.964r

3183.998r

66

2

1 119

20. g

0. g

1 24. 7

1 22. t

Fe I p

V I V I

2.43

0.04

1 0.00

192a

14

14

3188.034r

3188.059r

3188.199r

1 119

9

( 29. 8

[ 19. 8

2. 8

OH

Cr I V II

P 10

2.99

2.22

1,1 92

49

1

24
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(niA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3188.335r

3188.376r

3188.544r

3188.822r

3188.934r

3189.084r

3189.169r

3189.317r

3189.494r

3189.634r

3189.764r

3189.824r

168

111

24

2. 5

0. 5

35

18

1.5

29

10

r 21.3

1 21. 3

55. 5

34. 7

9. 3

0. 8

0. 6

10. 9

5. 7

0. 5

9. 1

3. 7

CH

Co I V II- Fe I Fe I

OH

Ti II Fe I Co I Cr II?

P 11

1.96

1.10 2.40

2.48

Q 16

3.82

0.22

4.78

1,1

74

8

159

159

1,1

120

9

123

2

1

3192.396r

3192.534r

3192.617r

3192.724r

3192.824r

3192.917r

3193.054r

3193.234r

3193.301r

3193.549r

3193.734r

115

89

39

71

172

15238

264

J 24

1 217

36. 3

30. 1

20. 1

35. 7

54. 0

67. 0

18. 3

f 64. 4

1 55. 2

8. 1

r 25. 5

Fc I

||Fe ICH?

CH

OH

Fe I Fe II OH

Fe I Fe I Hf lire I Fe II p

/2.22

13.40

P 18 P 18 Q 17

2.48

1.G7 Q 25

0.00

2.47

0.38

3.27

3.89

100

711

0,0

0,0

1,1

155

0

0,0

7

159

2

682

79

2

2

1

1

3189.964r

3190.042r

3190.104r

3190.164r

15

95

105

33

5. 0

29. 8

52. 2

11. 5

Mn I

Fe ICH

CH

/4.35

14.36

2.59 P 17 P 17259

0,0

0,0

2

2

3193.816r

3193.979r

3194.094r

3194.234r

32

67

55

[ 51. 1 n. 3

20. 9

17. 4

Fe II Mo I V II -Cu I Hf II—

|Ti II

1.72

0.00

2.22

1.64

0.45

3.86

6

349

3

10 120

3190.294r 23 7. 4 OH R7, 12 2,2 1 3194.339r 26 9. 4

3190.404r 11 3. 4 OH? R 9 2,2 1 3194.431r 98 30. 7 Fe I 2.47 155

3190.539r 24 7. 7 3194.524r 74 23. 1 CH P 13 1,1 2

3190.683r

3190.849r

3190.899r

3191. 124r

3191. 194r

3191.314r

97

1 202

62

23

20

30. 6

f 44. 5

1 34. 7

19. 6

9. 3

6. 2

V II Fe I Fe I

Ti II Fe I Fe I Co I

1.13 3.05

3.05

1.08

2.56

2.99

0.17

8 548

548

26

258

452

7

3194.586r

3194.764r

3194.849r

3194.973r

3195.085r

94

20

68

41

76

29. 5

6. 4

2L 3

12. 9

23. 7

Ti II

Ti II? Ni I p OH

Ce II Nb II CH

OH

3.88

3.42 P 18

0.61

0.33 P 19 P 11

120

108

0,0 217

1

0,0

1,1

1

2

1

3191.414r 81 25. 4 Fe I p CH

3.25 P 12 682

1,1 2 3195.140r 45 18. 5 Ru II CH

4.22 P 19 0,0 2

3191.564r 11 3. 9 W I? 0.00 5 3195.230r 80 25. 3 Fei

3191.664r 89 28. 1 Fe I 0.00 8 3195.37 a 19 7. 2

3191.799r 57 17. 9 OH P 18 0,0 1 3195.405r 24 7. 5

3191. 889r 46 14. 5 Ni IZr II 3.54

0.80 12550

3195.593r 126 39. 4 NiiY II 0.27 0.10 1210

3192.008r

3192.039r

t 145

f 37.3

1 17.8

Ti I Fe II

0.02

3.81

27

66

3195.725r

3195.875r

70

20

22. 7

7. 2

Tin 1.08 25

3192.194r 65 20. 6 Co I 1.96 72 3195.990r 51 32. 2 Fe I 2.45 192a

3192.274r 71 22. 3 Ti II 1.08 25 3196.106r 245 76. 7 Fe II 1.67 7

25
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3196.195r 33 21. 3 3200.791r 81 25. 5 Fe I 0.09 8

3196.340r 39 13. 6 Cr II? 2.54 9 3200. 962r 71 22. 2 OH P 19 0,0 1

3196.465r 30 9. 4 3201.014r 50 16. 5

3196.570r 49 15. 5 Vii 2.27 62 3201. 127r 12 3. 8 Fe I

3196.625r 47 14. 9 Fe II p 3.97 95 3201. 262r 40 12. 5 Cr II 4.74 114

3196.75 a 31 11. 6 3201. 382r 26 8. 3

3196.835r 48 30. 4 3201. 512r 42 13. 3 OH Q4 2,2 1

3196.925r

[ 218

J

274

r 43. 9 Fe I 2.42 155 3201. 612r 34 10. 8 Ti I 1.05 90

3196.973r

3197.110r

I 43. 9

96. 3

Cr II-

|Fe I Cr IINi I

2.54

0.05

2.54

0.21

98

9 24

3201. 722r

3201. 892r

3201. 957r

10

14

17

3. 1

4. 5

5. 3

Ce II Fe I0.86

2.45

76

159

3197.206r 25 13. 0 3202.141r 68 21. 4 Ni I 3.19 94

3197.361r 8. 5 2. 7 3202.257r 40 13. 4 OH Q 18 1,1 1

3197.541r 105 32. 8 Ti II Fe I 0.03 3.42

3 711 3202.382r 76 26. 7 IV I OH0.04 P 12 14

1,1 1

3197.596r 64 25. 8 Vii?-

CH

2.60 P 20150

0,0 2 3202.539r 156 48. 9 Ti II- Fe I 1.08

3.05 26 547

3197.710r 75 23. 6 CH P 20 0,0 2 3202.667r 86 26. 9 Fe I p 1.61 52

3197.871r

3198.021r

3198.101r

3198.20 a

3198.276r

3198.487r

3198.687r

3198.902r

3199. 137r

1

57

25

1748

58

23

10

52

0. 3

17. 8

8. 8

5. 5

15. 0

18. 2

7. 2

3. 3

16. 2

Vi

Cr I

Fe I Fe I Co I Fe I?-

OH0.02

2.99

2.61

0.63

P 11

14

91

258

26

1,1 1

3202.695r

3202.822r

3202.942r

3203.032r

3203. 162r

3203.323r

3203. 440r

3203.512r

29

50

15

16

4

71

78

24

9. 1

15. 6

4. 7

5. 2

1. 3

22. 4

24. 4

7. 5

CH

OH

CH

Fe I Co I

Y II

Ti II Fe IIII Cr n

P 22 Q 26 P 22

0.10

0.10

0.00

3.90

4.07

0,0

0,0

0,0

9

10

3

7946

2

1

2

3199.237r 11 3. 6 3203.612r 3 1. 3 Ti I? 0.02 26

3199.342r 60 19. 7 Co I- 0.17 9 3203.712r 3 1. 1 Fe II 5.95 196

3199.527r

3199.662r

3199.822r

3199.922r

3200.137r

3200.295r

3200.469r

3200.622r

196

55

23

114

59

147

207

13

61. 2

21. 4

9. 4

35. 8

20. 6

46. 2

64. 8

5. 3

Fe I (Fe ip)

V I?

Ti I CH

Y II- Ni IIIFei

2.42

0.11

1.86

0.05 P 21

0.13

0.03 /2.47

12.47

156

7

27

0,0

10

23 155

162

2

3203. 832r

3203.980r

3204.113r

3204.284r

3204.453r

3204. 573r

3204.693r

3204.863r

3204.953r

57

37

2

52

14

2

2.5

28

20

17. 9

11. 5

0. 6

16. 2

4. 5

0. 6

0. 8

8. 7

6. 3

Ti I OH

-Fe I Fe I

Ti I Nb n

0.02 P 19

3.27

1.05

2.16

27

0,0

90

1

26
The Solar Spectrum—Continued

Wavelength

Equivalent Width

AX KmA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib.

JDallU

Notes Wavelength

(.A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Notes

3205. 113r 41 12. 9 Cr II 4.75 114 3209. 185r 117 36. Ti Cr II 2.54 9

3205.223r 66 25. 2 3209.299r 130 40. 5 Fe X /2.81

13.42 333711 3205.333r 18 17. 7 CH P 23 0,0 2 3209.434r 35 10. 9 OH Q 19 1,1 1

3205.408r

3205.573r

3205.653r

3205.783r

3205.838r

168

36

28

35

20

52. 5

11. 3

8. 7

11. 0

6. 2

Fe I CH

V I

Ti up

Fe I

Ti I

2.48 P 23

1.35

1.16

2.56?

0.00

155

0,0

73

46

252

26

2 3209.489r

3209.624r

3209. 674r

3209. 764r

3209.934r

16

12

5. 5

10

72

5. 2

3. 8

1. 7

3. 1

22. 6

OH

Fe II

Ca I |Ni I

Q 7

4.48

1.88

3.31

2,2

137

1394

1

3206.007r 45 14. 0 Ti II 1.08 26 3210.046r 35 11. 1 OH P 13 1,1 1

3206.113r 12 4. 0 3210.225r 158 49. 5 Fe I 2.42 159

3206.238r

3206.348r

30

19

9. 5

5. 9

OH

Ti I

P 12

2.02

1,1

179

1 3210.452r

3210.480r 1 164

r39. 3 Us. 2

Fe II OH

1.72 P 20

6

0,0 1

3206.493r 9 3. 6 Fe 1? 3210.639r 52 16. 5 Fe I?

3206.533r

320D.7D3r

3206.943r

16

45

65

5. 0

14. 1

20. 2

OH

— OH

Mn I —

Ni I

Q 6 Q 19

2.11 3.40

2,2

1,1

1494

1

1

3210.724r

3210.836r

3210.944r

42

113

26

20. 5

35. 3

8. 3

CH

OH

Fe I

Zr II

P 25 Q 27

2.47

1.00

0,0 0,0

156

63

2

1

3207.081r 59 18. 6 Fe I 2.40 159 3211.064r 25 7. 9 Fe II 3.94 95

3207. 178r 203 63. 3 Sm II 0.00 2 3211. 169r 32 10. 1

3207.248r 12 4. 0 W I 0.37 9 3211.209r 28 8. 8 CH? P 18 1,1 2

3207.34 a 5.5 1. 7 Ti I 1.05 90 3211.309r 18 5. 7 Cr I 3.42 220

3207.413r 30 9. 6 V I 0.07 14 3211.490r 91 28. 4 Fe I 2.48 162

3207.563r 15 4. 8 3211.634r 73 40. 6

3207.676r

3207.711r 58

f 13. 3

1 7.5

Fe IFe I2.83 382 3211.684r

3211.884r

121

88

37. 7

46. 0

Fe 1

Fe I

3.33

/2.22

13.40

711

98

711

3207.893r

3207.989r

3208.094r

3208.214r

3208.352r

10

36

45

10

66

3. 2

11. 3

14. 0

3. 1

20. 5

Ti I CHCH

Cu I V 11

1.98 P 24 P 24

1.64

1.10

179

0,0

0,0

3

8

2

2

3212.005r

3212. 165r

3212.323r

3212.440r

200

76

59

• 24

62. 4

29. 1

18. 4

O. 0

Fe I

XT' _ _ r e I

r e I f V I

2.40

1.38

158

73

3208.474r 90 28. 0 Fe I 3.43 711 3212.545r 57 17. 9 Cr II 4.41 81

3208.595r 88 27. 8 Cr II 2.54 9 3212.690r 33 10. 2 Ti II p 0.11 9

3208.689r

3208.794r

45

21

17. 5

8. 4 OH P 3 2,2 1

3212.892r 94 29. 2 Mn I 2.11 4.76 14 114

3208.894r 27 8. 8 Ni II 2.86 2 91 31. 8 Ti I Ti II 1.07

0.01 90

3 3209.004r 22 8. 8 Ti I 1.97 179

3213.311r 185 57. 5 Fe n 1.69 6 3209.1 17r 51 30. 3 Fe I 2.18 97 32l3.404r 28 18. 4 Ni I 3.40 91

27
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3213.474r

3213.564r

57

32

22. 8

10. 6

OH

Ti II Fe I

P 20

3.88

0,0

120

1 3217.392r

3217.545r

133

65

41. 6

32. 3

IIFei Cr II Fe I p

2.40

2.54

2.59

157

9

254

3213.694r 44 13. 9 3217. 725r 11 3. 6

3213.744r

3213.929r

55

26

17. 4

15. 4

OHFe I P 13

3.02

1,1 452

1 3217.841r

3217.935r

3218.075r

72

35

37

22. 3

11. 1

11. 6

Ni I Til

OH

3.19

1.97 P 14

91

179

1,1 1

3214.030r

3214. 072r

3214.222r

i 229

1

68

f 46. 0

[ 56. 1

27. 7

Fe I

|Ni I Fe I

Zr IITi I

/2.45

13.37 3.19

2.45

0.09 0.05

156 71193

158

327

3218.205r

3218.276r

3218.450r

3218.614r

12

84

13

28

3. 7

26. 1

4. 2

8. 8

Ti II

Ti II p

Sm II

1.57

1.16

84

46

3214.402r 105 32. 7 Fe I 0.09 7 3218.684r 33 10. 2 Cr I 2.99 92

3214.494r 44 18. 4 OH Q 20 1,1 1 3218.864r 16 5. 8 V I 1.35 72

3214.6141- 38 12. 0 Fe I 2.28 143 3218.984r 29 9. 0 Ce II? 0.86 75

3214.776r

3214.864r

3215.029r

3215.179r

3215.204r

3215.354r

3215.404r

3215.594r

3215.644r

3215.714r

3215.844r

3215.948r

3216.049r

3216. 214r

3216. 359r

3216.546r

106

30

29

1 105

28

71

8.5

19

14

69

123

23

50

4. 5

62

33. 2

11. 3

9. 0

f 20. 4

1 20. 4

10. 8

22. 2

2. 7

6. 1

4. 3

21. 5

38. 6

9. 3

15. 7

1. 4

19. 6

Ti II V II CH?

OH

Cai

Fe I Cai

Fe I Nb II Fe I

Fe I Fe I p

Ti I Fe I?

Cr II

0.05

1.13 P 19 Q7

1.89

1.89

0.44

2.81

2.47

3.30

1.07

4.41

3

8

1,1

2,2

13

13

1

332

156

682

90

82

2

1

3219. 146r

3219. 199r

3219.369r

3219.429r

3219.597r

3219.805r

3219.965r

3220. 145r

3220.312r

3220.433r

3220.550r

3220.607r

3220.775r

3220.835r

3220.970r

3221. 135r

76

34

35

8. 5

192

167

43

31

51

60

39

30

32

30

22

46

23. 6

12. 0

14. 7

4. 6

59. 6

52. 0

15. 2

9. 5

16. 1

18. 7

12. 2

10. 1

10. 5

9. 2

7. 1

14. 3

Co I

Ti I Fe I p OH?

Fe I Fe I

OH

Ti II Co I

Ir I Fe II

OHTi I

0.10

1.98

2.69 P 5

2.45

2.42

P 21

0.12

2.96

0.35

4.08

Q 9 0.02

8

179

308

2,2

156

158

0,0

9

152

5

106

2,2 26

1

1

1

3216.694r 69 21. 6 Yn 0.13 10 3221.274r 80 24. 8 Ni I 3.83 185

3216.815r 49 15. 3 Ni I 3.31 93 3221. 385r 39 13. 1 Ti I 2.00 179

3216.927r

3217.070r

3217.097r

3217.300r

119

j 168

10

37. 0

1 39. 6

1 27. 6

4. 8

Mn I Fe I

Ti II Vi

IV II

0.00

0.03

0.04

2.05

3

2

1438

3221. 545r

3221.659r

3221. 760r

3221. 888r

3221.920r

38

104

29

1 98

12. 1

32. 4

12. 2

f 18. 8

1 34. 2

OH

Ni I

Ti up

Fe I

Q 28

0.00

1.16

2.48

0,0

8

46

156

1

28
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (mA)

Re- ducod

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3222.087r 258 80. 0 Fe I 2.40 156 3226.446r 48 16. 9 OH P 15 1,1 1

3222.260r 33 18. 2 3226. 541r 42 14. 1 Cr I 0.98 25

3222.444r

3222.584r

36

44

12. 2

13. 7

Zr II 1.76 104 3226.738r

3226.764r 1 130

1 24.8

1 27. 0

Fe I

Ti II

0.09

0.03

8

3

3222.729r 51 28. 7 Ti I 0.02 26 3226.891r 40 14. 4 V II 3.12 185

3222.855r

3222.944r

3223.099r

3223.263r

3223.364r

3223.449r

3223.616r

3223.639r

3223.744r

205

24

44

85

44

32

66

34

25

63. 6

25. 3

13. 8

26. 5

13. 7

13. 8

20. 5

10. 6

7. 4

Ti II

Fe I Fe I OH

Fe I

|Tii

Ni I

Gd II? OH?

0.01

3.30

1.48 P 21

3.30

2.02 /3.19

13.50

0.24 Q 28

2

682

51

0,0

17992

94

10

0.0

1

1

3227.007r

3227.059r

3227.176r

3227.276r

3227.426r

3227.496r

3227.631r

3227.761r

3227.809r

3227.996r

92

61

70

19

24

19

46

1 424

57

28. 5

19. 1

27. 0

7. 0

10. 5

10. 2

38. 3

f 99. 6

1 99. 6

45. 9

Co I |Ni I Fe I Fe I p

Vi?

Fe II Fe I Fe I

2.33

0.00

2.48

2.56

2.37

1.67

2.42

2.83

124

7

156

247

134

6

157

379

3223.847r 51 15. 8 Fe I 0.99 27 3228.103r 75 33. 9 Mn I 2.11 14

3224.039r 9. 5 3. 0 Fe I p 3.64 920 3228.254r 107 38. 2 Fe I 2.47 157

3224.253r 104 32. 5 Tilii 1.58 84 3228.387r 31 15. 2 Ti II p 1.16 46

3224.425r 9. 5 3. 0 3228.502r 52 16. 9 Ru II — 4.04

3224.485r

3224.635r

11

45

3. 3

14. 1 Co I 1.88 71

3228.619r 106 33. 1 |Ti II Fe I Fe II

1.08 24

3224.767r 31 9. 5 Mn I 0.00 3 3228.837r 54 21. 6 Zr II 0.80 49

3224.925r

3225.031r

3225.122r

3225.372r

76

125

22

Zo

18

23. 5

41. 4

14. 7

Q 1 O. 1

7. 8

Fe I Ni I OH

Cr n

0.42 Q 11

4.92

39

2,2

1,1

140

1

11

3228.900r

3229.147r

3229.208r

3229.352r

95

1 191

26

29. 6

1 37. 2

1 49. 6

10. 9

|Fe I OH

Fe I

Ti II Co I Cr II

2.48 P15

0.12

0.00

3.02 4.07

157

1,1

8

2

152

46

1

3225.462r 27 13. 5 Cr II—

II Nb II 4 07

0.29 451 3229.426r

3229. 588r

104

99

32. 3

30. 9

Ti II Fe I

1.13

2.83

36

333

3225.617r 36 29. 5 Fe I /2.43

\3.64 192 920 3229. 795r 66 25. 8 Fe I 2.59 247

3225.712r 33 57. 7 3229. 883r 104 32. 3 -Cr II 4.76 114

3225.804r 506 157. 1 Fe I 2.40 155 3229.990r 104 34. 6 Fe I 3.05 546

3225.909r 26 27. 6 Ca I 1.90 13 3230.097r 45 18. 8 Fe I 0.96 27

3226.028r 40 26. 4 Mn I 2.14 14 3230.207r 131 40. 6 Fe I 2.47 158

3226.151r

3226.227r

3226.347r

59

14

18

29. 4

6. 5

7. 0

Ca I Ti I

Ti I Cai

1.90 2.04

0.05

1.90

13 179

27

13

3230.472r

3230.592r

3230.727r

56

34

70

17. 4

10. 5

22. 5

-Fe II Sm II OH

|Mn I

3.97

0.18 P22

2.14

95

21

0,014

1

29
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3230.846r 44 13. 5 3234.932r 50 2L 2 Fe II 0.99 1

3231.007r 97 32 Fe I 2.45 157 3235.027r 30 11. 7 Mn I 3.07

3231.077r

3231.11 a

3231.222r

24

10

42

9. 0

3. 7

13. 1

Ni ip

OH?-

Ce II

3.42

P 7 0.50

106

2,2 149

1

3235.187r 35

oo

12. 4

1 Q 1

Fe IOH

Fe I Mn I

P 16

2.73

3!07

1,1 309

1

3231.326r 106 36. 5 Ti II 0.13 9 3235.557r 1"

[ 10. 2 Co I /1.96

\2.79

71 138

3231.472r 36 11. 3 OH /Q 22 IP 6

1,1 2,2 3235. 584r J [ 15. 7 Fe I 2.69 308

3231. 587r

3231.707r

49

27

16. 4

8. 4

Fe I Fe II Zr II1.48

3.89 0.04

50

80

3

3235. 771r

3235. 796r

3235. 933r

\ 84

J

10

f 19. 6

[ 11. 6

3. 0

Ni I Co I

Ti I? p

0.27

2.01

0.83

11

72

47

3231. 842r 6. 5 2. 0 3236. 134r 96 31. 6 Ti II 1.08 24

3231.947r 39 12. 2 V II 2.26 61 3236.232r 47 18. 8 Fe I 0.05 7

3232. 076r 18 5. 8 Os I 0.52 3 3236.423r 41 23. 7 Nb II- 0.38 1

3232.156r 30 9. 5 Fe I 2.61 258 3236.586r 385 118 Ti II 0.03 2

3232.290r

3232.392r

3232. 547r

3232. 687r

3232. 797r

3232.938r

3233. 054r

87

13

3

36

45

214

93

27. 1

4. 2

0. 9

12. 9

20. 4

66. 1

46. 6

Ti II

Sb I Fe I —

Ni I Fe I

1.12

2.29

rt . 1 O

0.00

3.24

36

2

II 1I Qy

7

620

3236.788r

3236.923r

3237.037r

3237.143r

3237.233r

3237.431r

89

10

49

13

52

83

49. 4

4. 0

16. 6

4. 5

16. 7

25. 7

Mn 1 OH

Co I

Fe I Mn I Fe II

/2.14

13.07 P7

0.10

2.59

3.07

3.89

14

2,2

7

256

81

1

3233.167r 52 23. 6 Ni I /3.31

13.83 91 184

3237.583r 21 6. 5 OH P8 2,2 1

3233.277r

3233.437r

3233. 537r

3233.669r

3233. 762r

3233. 976r

3234.072r

45

4. 5

33

51

65

127

88

14. 8

1. 5

10. 9

16. 8

25. 6

45. 0

53. 0

Cr I-

|Fe I

Vii

OH

V II

||Fe I Mn I

|Cr II- Mn I

0.97 2.28

2.27 P 22

2.27

2.42

3.07

4.29

3.07

25

142

61

0,0

61

158

63

1

3237.723r

3237.850r

3238.038r

3238.088r

3238.213r

3238.318r

3238.518r

3238.553r

23

87

22

71

12

14 1"

7. 1

26. 3

9. 8

22. 0

3. 9

4. 5

r 5. 5

i 8. 8

Cr I

|Fe II- Vii

Cn

Til

Fe I Cr IIFe I OH

2.97

3.89 2.04

2.98

2.02

3.05

4.07 3.04 P 16

114

8138

114

179

545

45 397

1,1 1

3234.277r 11 6. 2 Ce II 0.27 80 3238.767r 52 18. 8 Cr II 4.32 63

3234.352r

3234.518r

3234.647r

32

49

109

22. 3

15. 2

69. 0

Ru II?-

Ti II Ni I Fe I

4.08

0.05

0.11 0.05

2

21

8

3238.897r

3239.052r

3239. 317r

73

267

94

37. 2

82. 5

41. 0

OHCo I

Ti II — Fe I p

Q13

3.07

0.01

2.84

2,2

2

379

1

3234.777r 13 9. 6 Fe I? 3239.456r 161 49. 7 Fe I 2.42 157

30
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identi- Ocation

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3239.668r

3239.848r

102

16

31. 6

4. 9

Ti n V II

1.08

2.27

24

61

3244. 139r 1

3244. 199r J 177

1

9. 3

1 58. 9

Cr I Fe I

1.00

2.42

25

156

3240.019r

3240.121r

3240.263r

3240.404r

3240.498r

3240.608r

3240.708r

3240.873r

3240.963r

3241.050r

3241. 138r

35

25

9

53

7

49

62

8

20

49

9.5

10. 9

7. 9

2. 8

16. 6

2. 1

15. 1

19. 2

2. 5

6. 4

15. 1

2. 8

Fe I Fe I

Mn I

Mn I

Ti II

Ti I? p

Cr I

Zr II OH?-

Sm II

3.05

2.45

2.11

2.16

0.11

0.85

0.96

0.04 Q14

0.04

545

158

13

14

9

47

25

4

2,26

1

3244.354r

3244.498r

3244.548r

3244.703r

3244.868r

3245.018r

3245.138r

oz45.z75r

oz4o.39or

O O y1 C Af\ ^ OZ45.49 a

3245.543r

53

24

18

24

30

39

34

35

76

25

48

21. C

7. 4

5. 5

7. 4

9. 4

12. 1

10. 5

10. 9

23. 6

10. 6

14. 8

on

OHTi i?p

-Cr I?

La II

y^r II!

"NT; T JNl I Or I Cr I

/P 23 \P 17 Q 14

0.84

2.98

0.17

4.32

Q A Q o.4o

r\ AO

2.97

0,01 1,1/

2,2

47

114

32

62

108

25

113

1

1

3241. 248r 5. 5 1. O

o o /* cr TOO— 3245. 728r 9. 5 2. 9 L/O I 2.79 138

3241. 391r A 'T 47 1 A C 14. 5 i^e I OO /I C TOO— 3245. 788r 18 5. 5 Fe I p 3.84 920

oci At cno—

DO

on

1 ri K ly. 0

0. 0

re I om 111i.Ui

U.iy

Z

oo

i}J45.y»5r OO A G A01.- Oii4o.U31r J 1112d. 3

1 IOC

Fe I Fe Iu.y 1

U.l 1

27

o8

o241.Door A O4z lo. 2 re II o.yu QCl OU 3246. 171r 6. 5 2. 0

3241.818r 27 11. 8 3246.310r 8. 5 2. 6

3242.007r 270 83. 0 Ti II 0.00 2 3246.494r 68 21. 0 Fe I 2.59 252

3242.108r 14 8. 8 3246.684r 12 3. 7 Ce 11? 0.42 130

3242.277r

3242.413r

3242.489r

65

5. 5

4

23. 6

1. 8

1. 3

Fe IlY II 2.59 0.18 255

10 3246.770r

3248.977r

3247.192r

16

108

110

5. 1

33. 4

31. 0

Fe I

|Fe II Co I

2.20

3.89

1.88

95

8170

3242.629r

3242.709r

3242.834r

3243.014r

3243.071r

3243.214r

3243.414r

27

26

20

> 157

40

83

8. 5

8. 0

6. 2

f 16.7

1 39. 2

14. 8

25. 6

Pd I OH

Ni I OH

Fe I

0.81 P 8

0.03 Q 23

/2.83

13.33

3

2,2

22

1,1

381 710

1

1

3247. 301r

3247.406r

3247.569r

o o .1 T Ton 3247. 789r

0 0,1T rvT/? — 3247.976r

3248.129r

3248.220r

76

46

246

40

21

80

117

23. 6

29. 7

76. 0

14. 4

6. 5

38. 0

36. 1

||Fe I Cr I Fe II Cu I

Fe IFe I

2.47

0.97

4.15

0.00

2.45

15725

119

1

157

3243.564r 20 6. 4 Co I 1.74 47 3248.323r 20 7. 6

3243.765r

3243.860r

3244.029r

98

67

6. 5

30. 5

32. 0

2. 0

Fe II- Mn I Co I4.15

2.16

1.88

119

14

69

3248.470r

3248.518r

3248.612r

43

62

148

1

14. 0

22. 6

46. 0

Ni I Mn I

iTi II Ti I

0.03

2.16

1.24

1 1.05

21

14

66

1 89

31
The Solar Spectrum—Continued

VV tl V c— length

(1)

Equivfl Ipn t, Width

AX (ml)

Re- Width

AX/X

(F)

Spot

Solar

Identifi p n t i nn

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes length

(A)

EquiWidth

AX (ml)

Ref\ 1

1

0(^r\ Width

AX/X

(F)

Spot

Snlnr

IdentiLow

or

xvu u. Line

RMT

IN U. or

V 1 u. Band

Notes

3248.722r 54 16. 7 Ti II p 0.12 9 3253.154r 25 9. 0

OjiiTtO.OUOi 21 6. 7 3253 271 r 23 7. 1 Cr I — 3.00 114

56 17. 4 Fe I 2.73 308 3253 411 r 15 4. 8 Sm II

3249.194r

3249.378r

95

55

29. 6

20. 4

Fe I

Ti II

2.56

1.08

253

23

3253.564r

3253.611r 1 73

r 4. 5

1 20. 8 Fe I 3.25 681

3249.458r 81 25. 1 Ni I 0.27 10 3253.721r 11 3. 5 Hf II 0.38 1

3249.535r

^94.0 fi84.r

^594.0 0^^«/>OVJ SfilrXL

3249.927r

42

18

ov

34

26

19. 7

7. 9

18. 4

10. 5

8. 2

Fe IV I V II Fe II Fe I Fe II1.56 0.07

2.05

3.89

3.89

51

13

38

O J78

3253.844r

3253.958r

3254.060r

3254.194r

3254.261r

61

58

37

48

161

19. 0

19. 4

13. 1

47. 7

49. 5

Fe I Fe I Mn I Co I

Ti II (Fei)

2.56

2.61

2.11

1.88

0.05

2.56

250

257

12

69

2 249

53 16. 5 Co I 0.58 26 3254 ^^tj^ttj377r 111. 80 33. 0 Fe I 3.27 620

31 9. 6 3254 470r 53 16. 4 Fe I p 2.45 158

3250.395r 130 40. 2 Fe I (Zr II)

/2.28

12.86

1.77

142 379

125

3254.761r 93 28. 6 IFe IV I |V II2.69

0.07

2.03

308

1338

3250.637r 116 35. 8 Fe I 2.18 95 3255.030r 17 5. 2

3250.767r

3250.941r

3251. 154r

3251.256r

3251.353r

114

25

76

109

58

40. 5

7. 8

29. 1

33. 5

25. 1

|Ni IV II Mm

Fe I Fe II p

Sc II?

0.42 2.90

2.18

2.20

4.49

0.01

39

171

14

93

137

5

3255.163r

3255.293r 3255 4Q7r

3255 68flr

3255 81 7r

3255.901r

10

18

31

23

\ 124

3. 0

5. 4

9. 7

7. 2

f 0 1 1< 37.9

Cr II? OH —

Sc I V I?

Fe II

4.92 P 24

0.00

1.08

0.99

138

0,0

9

1

1

3251.539r 18 5. 6 3255.982r I 0.1

3251.612r 22 6. 7 Cr I? 3256.144r 56 17. 4 Mn I 2.18 14

3251.685r

3251.857r

3251.937r

3252. 125r

3252.239r

25

162

24

17

7. 7

r 16.

7

i 38.4

7. 3

5. 2

Pd I? Co I Cr I-

|V II

Ti 11 Fe I p -Fe I

1.25 2.93

2.98

2.52

0.01

2.56

6 152

113 108

2

247

3256.262r

3256.496r

3256.710r

3256.961r

3257.103r

10

45

52

12

47

3. 1

13. 9

16. 2

3. 9

14. 5

Fe ip

Fe 1

OH-

|Fe I

/2.47

13.00

P 18

158 397

1,1 1

3252.440r

3252.609r

3252.745r

3252.892r

88

39

40

27. 2

12. 0

12. 5

( 44. 4

Fe I OH

-Fe I

|Ti II Fe I

P 24

0.03

2.56

0,0

2 252

1

3257.235r

3257.360r

3257.428r

3257.600r

69

26

56

77

21. 4

8. 3

17. 4

24. 7

Fe I

Fe II

Fe I

/0.99

\2.99

3.97

2.18

27 451

94

90

3252.970r

3253.038r

• 175 i 33.9

i 0.7

Mn I (Ti II p)

OH

2.18

1.08 Q 24

1423

1 1 1

3257.823r

3257.907r

42

30

12. 9

9. 2

Cr I V 11 (Fe II)

3.00

2.49

5.57

113

108

178

32
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Wirith AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot.

Li ne

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3258.020r 26 8. 0 Co I 1.71 47 3263. 133r 30 9. 4 OH P 11 2,2 1

3258.100r

3258.287r

3258.421r

27

6. 5

50

8. 3

2. 0

15. 4

Fe I

Mn I 2.19 14

3263. 234r

3263.370r

19

02

5. 9

19. 2

Co I —

|Vi

-Fe I (V II)

2.28

0.00

2.42 2.04

124

12

14438

3258.631r 33 10. 2 Fe I 2.48 157 3263.466r 19 6. 0 Fc I 3.25 680

3258.783r 62 19. 3 Fe II 3.89 81 3263.691r 64 19. 7 Ti 11 1.16 45

3258.913r 7 2. 2 3263. 838r 25 7. 8 OH- P 19 1,1 1

3259.062r 58 18. 0 Fe II 3.90 81 3263.975r 24 8. 9 Fe I?

3259.236r 5 1. 5 Co I? 3.07 153 3264.065r 34 10. 4

3259.373r 2 0. 6 3264.185r 29 10. 4 OH P 25 0,0 1

3259.446r 5. 5 1. 7 Fe II? p 5.57 178 3264.283r 50 15. 5 Cr II 4.29 61

3259.599r 25 7. 9 -Cr I? 0.98 25 3264.406r 38 11. 6 Nil

3259.713r 20 6. 1 Fe I 3264.524r 73 22. 4 Fe I 2.20 90

3259.856r

3259.989r

3260.145r

3260.265r

13

70

17

96

3. 9

21. 7

5. 3

31. 6

Co I?

llFei Cri

Zr I

Ti I |Ti II |Mn IIIFe I

2.45 3.00

0.52

1.07

1.16 2.19

2.56

157 114

35

8945

14 250

3264.711r

3264.784r

3264.861r

3265.054r

3265.188r

1

100

29

87

11

/ 16. 6

[ 16. 6

8. 9

26. 8

3. 5

Mn I —

Fe I (Co I) Fe II p Co I Fe I

2.14

2.47

1.74

1.04

2.04

0.09

13 157

47

1

105

8

3260.472r 10 3. 3 Fe I? 3265.332r 54 16. 7 -Co I 2.08 106

3260.552r 20 6. 1 Nb II 2.17 3265.556r 59 27. 3 Fe I p 2.73 308

3260.692r 10 3. 2 Fe I? 3265.640r 102 24. 2 Fe I 2.18 91

3260.829r 38 11. 9 Co I 2.04 107 3265.700r 18 8. 1 La II 0.32 45

3260.958r 7 2. 3 Ce II? 1.01 258 3265.894r 37 11. 3 V II 2.37 74

3261.065r 23 7. 0 Cdi 0.00 1 3265.980r 10 3. 1

3261. 198r 9. 5 2. 9 3266.153r 9. 5 2. 9

3261.339r 59 18. 1 Fe I 3.42 712 3266.240r 12 3. 9 Cr II /4.32

14.78 62

121 3261.584r

j 142

f 26. 6 Ti II /1.23

11.89 66

89 3266.439r 35 10. 9 Ti II- 1.24 57

3261. 639r [ 26. 6 Fe I?- 3266.676r 5. 5 1. 6 Cr I- 1.03 25

3261. 817r 39 12. 1 Fe I 1.56 50 3266.950r 49 15. 0 Fe II 3.77 65

3262.021r

3262.288r

3262.717r

3262.902r

3263.073r

62

69

0

10

50

30

19. 0

21. 3

3. 3

15. 5

9. 2

Fe I Fe I (Sn I) (Osi)

Fe I Fe I

3.37

1.07 0.52

710

33

3267.062r

3267.206r

3267.269r

3267.439r

3267. 539r

3267.712r

56

26

16

23

11

82

17. 3

8. 1

4. 9

7. 2

3. 5

25. 2

Fe II —

OH

Fe I

Sb I V II

3.90 P 25

2.03

1.07

80

0,0

2

7

1

33
The Solar Spectrum—Continued

Ecjui- -tve- Low xviVl i Ec[ui- iie- Low w vEilent duced TP P IN 0. w a,vG- Vtilcll b duccd Solar ill r IN 0.

I an fri'rt IcLlJ^ LLl VV luLIl VV i Ll 1 11 opu I Idcnti" or or Icilg Lll WVV 1ILILII H t h VV I U 1 11 opot Identi- or or

NTNotes

ii A/ A fics-tioD. PXvOl, nt V lU. A "X Li A

A \ /\ Zi A/ A fication not. V ID.

f 'a \ (A) (mA) (F) Line JJtilltJ. (A) (mA) (F) Line jjanu

ozo Q0P,7/ • 7R8r * oor 7 s J? L. 1 9fl 8 1 0. 1 Co I ^ n7 1 IVTn T iVl.il 1

4- 9'? ^979 fiOfir 01 Fe I 01

i 0. y 0970 7qo« 19 0 Fe I ^ 4^ 719

P.7 D / 9n R T?P T 2 22 ^979 RARr 1 y 7

Q0 9 4 3273.052r 78 23. 9 Zr II 0.16 3 3268.435r 16 5. 0 Cr II? 4.29 62 3273.188r 7 2. 1 3268.521r 39 12. 0 Fe n 4.15 118

3273.354r 8 2. 4 3268.724r 17 5. 2 Mn I 4.19

'^97'? 489r fin io. 0 Sm II TTo T? |Fe II A ^K lis

3268.975r 29 9.

7

Ni I- 3.46 91 3273.634r 37 11. 4 Sc I 0.02 9 Ca I 1.88 12 327.S 72flr 6 2.

1

R1Dl io. 0 o.*±u 71 n 1f n 9

I 221 OOCQ qoQr 98 0. 0

^97*^ Q79r J fi7 4 Cu I n nn 11

3269.432r 28 8. 7 Fe i 2.20 95 3274.226r 39 13. 3 OH P 20 1,1 1 IIFei P 2.22 95

OiiDy.ou'ir 10. 0 n\j. 8s00 i. tJ^ ^2744 ^.rxtj 4'ilr1.1 28 8 7 Fe I 3.37 71 n 3269.624r 12 3. 9 -Zr I 0.52 34

3274.553r 5 1. 5

OiiDy. / D / r Oi 10. 0 iTTp TT lis

Ti TT 1 22 0 i ^974 fi7Rr ^4 1 n Ca I1x.oy8Q 1 9 QOAQ Q1 At t OL- 1 n fin Qy ^974 7S'?r 0 . 0 11. nu

K sn > oU

3269.966r 1 19.8 Fe I 2.18 90 3274.909r 39 12. 0 Ni II 2.86 1

3270.142r 68 20. 8 II Cr II 4.32 61 3275.025r 4 1. 4 V II 2.47 94

3275.152r 6 2. 0 Zr II 0.36 12 3270.350r 30 9. 2 Mn I 4.25 3275.229r

]

r 3.4 Nd II —

3270.533r 29 9. 0 Ti I? 1.44 123

\ 66 Fe I P 1.01 27

0/ / U.D / ir DO r e I p o.oy yo4 qo7K 9QQ,.

J 17 7

L it. t Ti II 11 .Uo OS 9^

3270.749r 14 5. 0 OH P 12 2,2 1 3275.405r 4 1. 2

3271.006r 172 52. 7 Fe I 2.20 91 3275.479r 5 1. 5

3271.143r 107 40. 4 |V II 1.10 7 3275.592r 16 5. 0 Ni I 3.48 107 Ni I 0.11 23 (Zr II) 0.53 22 3275.685r 54 16. 5 Fe I 2.76 308

0^ / i.oior 0.S 0 097c QAKr oy I i. y Fe I

3271. 413r 24 8. 5 3275.979r 20 6. 2

3271.498r 62 19. 2 Fe I 3.25 680 3276.135r 104 3L 9 V II 1.13 7

3271.668r 130 39. 9 |Ti II- 1.24 66 3276.262r 31 9. 5 OH P 26 0,0 1 Fe I 1.48 49 (Vi) 0.02 12 3276.470r 94 26. 1 Fe I 2.29 90

0071 Q c: 00 \yO I

1i.yo Qfi 7n 0^ 4 o.Di /r '±)J 10. u Fe II o.y'i 09

327l.962r 23 7. 1 3276.781r 84 25. 8 Ti II 1.18 45

3272.094r 104 31. 9 Ti II 1.22 66 3277.000r 63 19. 2 -Ti II 0.12 8

3272.244r 78 23. 8 |Zr II- 0.00 3 3277.101r 19 5. 9 V II 2.56 137 Ce II 0.70 73

3277.191r 47 14 5 Ni I 3.46 90

34
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3277.358r

3277.671r

3277.724r

3277.873r

3278.096r

155

41

46

34

27

47. 5

13. 5

14. 7

10. 5

8. 4

Fe II Co I V nFe uCo I0.99

2.96

2.56

3.77

2.96

1

152

137

65

153

3282.334r

3282.447r

3282.540r

3282.705r

94

29

51

82

28. 9

9. 0

15. 6

25. 0

Zn I lITi n

Fe I V II Ni IFe I

4.00

1.22

2.37

0.17

2.95

466

72

7 449

3278.295r

3278.449r

3278.562r

3278.742r

3278.849r

98

16

45

91

24

30. 0

5. 0

13. 8

27. 9

10. 0

Ti II

Mn I

Fe I

Co I

1.23

2.14

/2.42

12.59

2.01

66

12

144 250

72

3282.837r

3282.904r

3283.054r

3283.161r

3283.207r

1 109

21

36

f 18. 8

[ 18. 8

6. 4

1 6. 0

1 6. 0

II Nil

Zr II Fe I Cr II

Ti 11 p

3.48

1.83

3.27

4.99

1.24

106

125

680

159

57

3278.935r 110 33. 7 Ti II Ti I 1.08 0.90 23

63

3283.333r 26 8. 2 Co I V I 2.28 0.04 12

3279. 154r

3279.275r

54

76

16. 5

23. 2

OH

||Zr II Co I

P 26

0.09

1.96

0,0

370

1 3283. 450r

3283.554r

100

33

30. 6

13. 4

Fe ICoi

Fe I

0.96

2.08 27107

3279.449r 28 8. 8 3283. 686r 5. 5 1. 7

3279.519r 15 4. 8 Cr II 4.77 121 3283. 803r 13 4. 1 Co I 1.74 47

3279.659r 44 13. 3 Fe II 1.15 118 3283.933r 11 3. 8 NH? R 25 0,0 6

3279.747r 61 18. 8 Fe I 2.99 449 3283.990r 28 8. 5 NH? R 25 0,0 6

3279.848r 73 22. 5 V II 2.37 73 3284. 130r 5. 5 1. 6

3279.995r 76 23. 1 Ti II 1.12 35 3284.240r 4. 5 1. 4

3280.131r

3280.267r

3280.368r

3280.498r

3280.681r

3280.775r

29

90

23

16

44

64

8. 8

27. 3

7. 2

5. 0

15. 3

19. 7

Fe 1 -Ti I?

Ag I Fe I Mn I

3.30

1.07

0.00

3.02

2.14

620

88

1

451

10

3284.363r

3284.433r

3284.522r

3284.597r

3284.721r

3284.842r

8. 5

47

28

75

43

5

2. 9

14. 3

11. 5

22. 8

13. 1

1. 5

Vi

Ni I Nil

Fe I

Zr II

1.38

3.31

2.20

0.00

71

96

91

4

3280.975r

3281. 125r

23

44

7. 1

13. 4

NH?

Vii

fR29

R 30 [R31

2.56

0,0] 0,0

o,oJ

136

6 3285.022r

3285.198r

28

. 43

8. 8

13. 2

jViiOH

Fe I (Ce II)

2.52 P 21

3.00 0.50

108

1,1 396

148

1

3281.304r 117 36. 0 Fe II 1.04 1 3285.295r 33 10. 3 NH R 24 0,0 6

3281.527r 18 5. 5 3285.421r 72 23. 1 Fe II 1.08 1

3281.600r 19 5. 9 Co I 0.17 8 3285.552r 34 IL 2 Fe I p 2.56 248

3281.7l6r 70 21. 5 3285.702r 16 5. 7

3281.868r 66 20. 2 Ni I 3.54 106 3285.782r 23 8. 1 Zr II 1.49 91

3281.997r 19 5. 7 NH? R27 0,0 6 3285.908r 45 16. 0 Zr n 1.00 62

3282.247r 27 9. 3 Co I 1.78 47 3286.038r 71 25. 6 Fe I 2.22 90

35
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

HAA \ (mA)

Rediiced Width

iiA/ A (F)

Spot

ooiar

Identification

Low

or

Line

RMT

"Mr* IN 0. or

V I D. Band

Notes length

(A)

Equivalent Width

(ml)

Re- duced

Width

A \ /\ £i A/ A (F)

Spot

ooiar

Identification

Low

T? T>

11/ tr or

rtOt. Line

RMT

rs 0. or

V ID. Band

Notes

o^oo.u/ ir ly. o L^a I

1 on 1 9 Q9QQ Qfi9T> O-iOy.ouZr ID A O 4. y

o/oo. io4r QO o. 6 oZoy.yuyr A K 4. 0

91 S 7 o. / om II OOOn 1 1 9r y. 0 9z. Qy iVl g I i p D.oy

3286.368r 4.5 2. 2 Cr I? 3290.249r 22 6. 8 V II 2.49 108

3286.454r 46 21. 5 Fe I 3.40 710 3290.349r 7. 5 2. 2

3286.541r 25 14 9 Co I? 1.74 46 3290.476r 22 7. 7 NH R 21 0,0 6

3286.854r

3286.960r

4 1

ODU

20

58

ol. U

43. 5

44. 3

r 6 I NH

Ni I

9 1 S R 23

0.03

Q

1

0,0

19

6

oZyu.OiDr

3290.639r

3290.716r

44

15

70

1 Q A lo. 4

4. 7

21. 2

IN xl —

Ni II?

Fe I (Ni II)

"P 91 ±1 Zl 3.10

2.18

2.95

5

90

1

aO

3287.098r 44 26. 4 Fe I 2.94 396 3290.993r 92 28. 1 Fe I 2.22 95

3287.221r

3287. 334r

3287.434r

3287.471r

3287.583r

OOQ7 7Q7i<

3287.860r

3288.049r

65

21

11

32

9

OA

8. 5

31

32. 8

10. 3

5. 1

13. 3

4. 1

OO. /

ID. 0

2. 9

10. 2

Ni I |Co I

Zr II

Fe II Co I T^ TT 1 1 II

Co I? Cr II?-

1.68

1.96

0.32

4.15

3.10

i.oy

1.71

4.32

55

71

12

118

154

oy

43

62

3291. 134r

3291.284r

3291.430r

3291. 544r

3291.697r

3291.770r

3292.024r

3292.079r

3292.210r

43

14

26

8. 5

26

49

! Ill

11

14 9

4. 2

8. 1

2. 8

7. 9

15. 1

f 23. 6

1 15. 6

3. 3

Mg i?p

Fe I

Fe I Cr II Fe I

Ti I Gd II?- Co I?

6.59

3.69

4.30

3.25

0.90

1.10 3.10

954

68

680

62

74

153

3288. 155r 89 28. 7 Ti II- 0.13 8 3292.324r 39 11. 9 Mo II— 3.14 6

3288.327r

3288.435r

3288.579r

3288.813r

3288.977r

36

74

79

45

72

11. 5

23. 2

24. 2 Q7 7 O/. /

13. 8

22. 8

V II Fe I

Ti II

Ti II

77,1 r r e I

Zr 11

IFe IV TT V II

2.38

1.24

1.23 9 AO

1 u.uy

10.96

2.20 9 p;9

89

66

66

A462

90

3292.509r

3292.601r

3292.743r

3292.869r

3292.926r

3293.149r

990*3 99'3»* ozyo.zzor

31

95

13

10

6. 5

54

ID

10. 2

28. 8 4 1

3. 2

2. 0

16. 5

0. o

NH

Fe I

Fe II? p

Fe I

( V ii;

R 20

2.22

4.49

1.61 A 9 A

^ 09

0,0

91

136

51

1 ^A

6

3289.027r 48 33. 8 3293.478r 23 7. 0 Ti up 1.24 67

3289. 146r 11 3. 5 Rh I? 0.43 3293. 673r 42 12. 7 Fe I

3289. 246r 12 3. 6 3293. 773r 24 7. 5

3289.372r1

3289.442rJ

3289. 579r

3289.749r

111

25

10

1

' 21. 1

. 17. 3

7. 6

3. 2

Fe II Yb II-

|V II Fe I

3.81 0.00

1.10

2.83

65

17

380

3293.862r

3293.998r

3294. 108r

3294. 198r

3294.335r

11

5

8

7. 5 4 5

3. 5

1. 5

2. 5

2. 2

1. 4

Co I Cr I

Co I — Ru II Nb II?

2.08

3.45

3.10

2.54

1.98

107 219

154

2

3'^6
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3294.442r 6. 5 2. 0 3298.742r 66 20. 1 V II 1.13 7

3294.555r 7. 5 2. 5 Co I 3.13 152 3298.868r 8 2. 3

3294.622r 29 8. 8 Fe I 3299.084r 32 9. 9 Fe I 3.40 710

3294.722r 23 7. 2 NH R19 0,0 6 3299. 178r 12 3. 6

3294.822r

3294.942r

3295.022r

37

44

20

11. 5

13. 5

6. 1

NHIn rl

a e ii

AT III

R19

R19

0.76

0,0

0,0

36

6

6 3299.350r

3299.437r

3299.525r

8.5

67

52

2. 8

20. 5 2L 0

Ti I Fe I—

NH

0.90

1.56 R17

61

49

0,0 6

3295. 116r 39 11. 8 3299.677r 24 7. 2 NH R 17 0,0 6

3295.248r

3295.435r

3295.605r

3295.635r

3295.824r

47

53

16

9

76

14. 5

16. 1

5. 0

3. 3

23. 1

Fe 11 Cr n

Fe II

3.89

4.18

1.08

79

51

1

3299.778r

3299. 890r

3300.077r

3300. 170r

22

6

1

47

6. 6

1. 8

0. 4

14. 3

NH

Fe II?

Ce II?- Nd II?

R 17 6.70

0.72

0,0

166

6

3296.041r 16 4. 8 Mn I 2.16 11 3300.317r 0. 5 0. 2

3296.261r 40 12. 4 Ni I- 3.40 93 3300.490r 3. 5 1. 1 Rh I? 1.28

3296.377r 14 4 9 Zr II 0.96 62 3300.675r 6 1. 8

3296.475r 47 14. 2 Fe I 2.59 250 3300. 817r 3. 5 1. 1

3296.594r 8 2. 5 3300.912r 6 1. 8 V II 2.27 60

3296.821r

3296.887r

3297.067r

3297. 174r

3297.254r

3297.384r

3297.517r

3297.593r

47

30

22

22

22

2

2. 5

3. 5

14. 2

11. 1

6. 6

6. 6

6. 6

0. 6

0. 8

1. 1

Fe IFe II Mn I NH

NH

NH

Fe I? Vii

3.30

3.97

2.16 R18

R18

R18

2.50

619

92

12

0,0

0,0

0,0

108

6

6

6

3301.016r

3301. 136r

3301. 225r

3301.425r

3301. 579r

3301.681r

3301.782r

3301.869r

6

4

43

25

6

41

16

11

1. 8

1. 3

13. 0

7. 7

1. 8

12. 4

5. 0

3. 8

Fe I Fe I Os I -Ti II

Sr I? OH?

Pti

2.84

0.00

1.16

1.77 P 28

0.81

380

1

44

7

0,07

1

3297.666r 9 2. 8 3301.928r 37 n. 3 Fe I 3.24 617

3297.836r

3297.882r

3298.013r

3298. 141r

1

8

77

f 3. 8

1 15. 1

2. 5

23. 5

Fe II Ni I p

Fe I (Vi)

3.94

3.50

2.22

0.07

91

91

90

12

3302.105r

3302. 162r

3302.316r

3302.383r

\ 86

18

112

f 26. 1

{ a.

7. 3

34

Ti II- NH

Pd I NH

Na I

0.15 R 16

1.25 R 16

0.00

8

0,03

0,0

2

6

6

3298.234r 39 14. 7 Mn I 3.37 3302.593r 55 16. 8 Zn I 4.03 4

3298.324r 25 8. 8 Cr I 3.09 161 3302.768r 15 4. 8

3298.418r 17 5. 4 3302.863r 72 2L 9 Fe II 1.04 1

3298.558r

3298.69 Ir

37

16

11. 4

6. 5

Fe I Co I3.43

2.01

710

70

3302.982r 83 25. 1 Na I (Zni)0.00

4.03

24

37
The Solar Spectrum-—Continued

Wave1 PTl 0"f',}l

(A)

Equivalent Width

AX

(.mAJ

Re- duced

Width

AX/X

Spot

Solar

fication

E°P

Rot.

RMT

No.

Vib. Band

3303.121r 21 6. 5 La II 0.23 45

3303.271r 30 9. 3 Mn I 3.38

3303.474r 69 20. 9 Fe II 1.10 1

3303.571r 76 23. 0 Fe I 3.02 449

3303.781r 16 4. 9

3303.895r 14 4 3 Co I 1.78 47

3304. 136r 18 5. 4 Co I 3.07 154

3304.248r 20 6. 1

S304.365r 52 15. 7 Fe I 3.42 710

3304. 450r 37 11. 3 Fe II 3.94 93

3304.484r 13 6. 0 V II 2..54 136

3304.592r 25 7. 5

3304.754r 34 10. 3 OH?- P28 0,0 1

99 6. 7 NH R 15 0,0 6

S3fl4 Qfi2r 55 16. 6 Ni I 3.42 108

3305 067r 26 8. 1 NH R 15 0,0 6

t>t>v/U» J- v'Jl 72 21. 8 Fe I Zr II 0.04 2

3305.227r 20 7. 4 NH R 15 0,0 6

3305.307r 9 2. 9

7 2. 2

ao 2. 4

17. 4 Fe II 3.90 79

46 16. 0 Co I Fe I p

3.10

3.27 152 618

3305.864r 44 24. 5

3305.977r 153 47. 1 Fe I 2.20 91

3306.093r 65 27. 3

3306. 168r 23 11. 6

3306.284r 49 15. 0 Zr II 0.04 3

3306.378r 145 43. 9 Fe I 2.22 91

3306.495r 61 25. 6 Fe I 3.30 680

3306.598r 60 18. 5 Fe I

3306.702r 17 5. 2 Fe I 3.00 396

3306.775r 14 4. 3

3306.882r 28 8. 6 Ti I 2.13 190

3306.986r 16 8. 1 Cr II- Mn I 4.94

3.38 150

WaveIpriorf.Vl

(%\

Equivalent Width

AX

Re- duced

Width

AX/X

(r

)

Spot

Solar

TdpTiti- fication

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

3307.037r 99 30. 2 IFe I Ni I

II Cr n

2.95 3 42

4!l7

460

107

51 3307 152r 50 15. 1 Co I 1.96 69

3307.246r 65 19. 8 Fe I 3.24 617

3307 345r 10 3. 0 Rh II? 3.49 5 3307 508r 20 6. 1 NH'

Sr I R 251.80

1 17

g

3307.717r 97 29. 3 Fe I? Ti II? —

|Cr I 0.122!71 878

3307.907r 48 14. 6 NH R 14 0,0 6 3308 11 Ir 59 17. 9 NH R 14 0,0 6

3308.277r 14 4. 4 NH? R 23 1 1 6

3308.399r 32 9. 7 Ti I 1.05 87

3308.491r 17 5. 3 ICo I V II 3.07

2.54 155

137

3308.621r 14 4. 4

3308.760r 29 10. 6 Fe ip —

Mn I 2.40

2.18 190

11

3308 819r 84 25. 6 Co I [Ti II 3.07 0.13 153

7

3308.937r 24 14. 5 Ni I p 3.60 107

3309. 031r 6 1. 8 Co I? 2.54

3309.084r 15 4. 7 NH R22 1,1 6

3309.197r 7. 5 2. 3 Vi 1.19 55

3309.324r 13 3. 9 Ni I p 3.42 105

37 11. 3 Ni I

3309.530r 73 22. 1 Ti I 1.05 87

3309.723r 30 9. 1 Ti I 2.12 190

3309.846r 12 3. 6 Cr I f3.00 13 09 161

7 2. 5 Zr II 0.97 72

3310.030r 28 8. 5 NH /R 21 \R 28

1 11 1.1/ 6

3310.120r 20 6. 5 NH R21 1,1 6

3310.210r 56 16. 9 Nil 0.42 38

3310.344r 76 23. 0 Fe I 2.95 449

3310.498r 59 17. 2 Fe I 3.25 679

3310.649r 67 20. 1 Cr 11 NH

/4.78

14.98 R 13

120

158

0,0 6

3310.868r 46 13. 8 NH R 13 0,0 6

38
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3310.918 14 6. 3 Fe I 7

3311. llOr 45 13. 6 NH R 13 0,0 6

3311.215r 39 11. 8 Fe I

3311.349r 20 6. 0 Zr II 0.71 34

3311.459r 32 9. 8 Fe I 0.99 27

3311.599r 9 2. 7 NH R 29 1,1 6

3311.715r 19 5. 9 Sc II- NH

3.69 R2941

1,1 6

3311.895r 23 11. 8 Mn I 2.18 10

3311.935r 68 20. 6 Cr II 4.15 51

3312.059r 19 5. 3 Cr I 2.71 78

3312.197r 63 19. 2 II Cr II Coi-

|Fe I

4.14

1.96 2.99

5169 450a

3312.325r 54 16. 5 Ni I 3.42 106

3312.435r 35 10. 7 Sm II 0.18 21

3312.601r 53 15. 9

3312.699r 76 23. 0 Ti III Fe 11 (Sc n)

2.10

1.08 3.70

190

1 41

3312.842r 25 7. 6 NH R 19 1,1 6

3312.925r 23 7. 5 NH R 19 1,1 6

3313.009r 66 19. 9 Ni I 3.60 106

3313. 078r 36 12. 1 Cr II 4.78 119

3313. 173r 33 12. 4 — Mn I 3.07 30

3313.304r 9 2. 6 Eu II 3.00 24

3313.434r 28 8. 7 Mn I 3.07 30

3313.548r 30 9. 2 Mn I 3.07 30

3313.646r 59 17. 8 NH R 12 0,0 6

3313.725r 35 12. 5 Fe I 1.61 50

3313. 801r 12 4. 1

3313.914r 30 9. 1 NH R 12 0,0 6

3313.996r 59 17. 8 Fe II 1.10 1

3314.086r 44 17. 6 Co I Fe I

/1.74

\2.88

3.41

43

149 736

3314.206r 14 4. 4 NH R 12 0,0 6

3314.348r 34 11. 3 Co INH

3.07 R 18 152

1,1 6

3314.446r 72 21. 7 Ti I-

|Fe I (Zr II)

1.07

2.61 0.71

87 250

47

Wavelength

(I)

Equivalent Width

AX

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3314.535r 58 17. 6 Ti ICr II 1.05 4.93 87

150 ——

3314.614r 55 20. 5 NH R 18 1,1 0

3314.748r 90 27. 2 Fe I 3.30 680

3314.867r 52 15. 8 |V II Mn I 2.56

3.07 13630

3315.050r 26 8. 0 Co I Pt I?

(2.28 13.13 0.00 154

1

3315.175r 32 9. 8 Fe I Vii

3.30

2.37 61871

3315.257r 11 4 8 Ti I-

|Cr II 2.09 4.18 190

51

3315.329r 96 29 Ti II 1.22 65

3315.420r 74 34. 3

3315.557r 25 9. 9 V II 2.56 136

3315.679r 153 46. 2 NI I 0.11 22

3315.953r 17 5. 1

3316.000r 10 3. 7

3316.197r 24 7. 2 Fe II p — NH

1.67 R 175

1,1 6

3316.339r 23 7. 0 IMn I Dy II? 2.19 11

3316.432r 43 13. 1 Mn I 3.07 30

3316.486r 14 4. 4 NHCr I R 17 3.85

1,1 255

6

3316.569r 31 8. 5 Fe ISm II 2.18? 86

3316.649r 33 10. 2

3316.742r 35 10. 7 NH R 11 0,0 6

3316.851r 34 10. 2 Fe IV II 2.54 137

3316. 905r 16 6. 0 NH R' 11 0,0 6

3317.045r 20 6. 0 NH R 11 0,0 6

3317. 133r ' 74 22. 4 Fe I 2.28 139

3317. 264r 53 16. 0 Mn I 3.07 30

3317.385r 44 13. 2 NH R 11 0,0 6

3317. 591r 36 11. 0 Ni I 1.68

3317. 701r 6 1. 9

3317. 831r 14 4. 4

3318.031r 103 3L 0 Ti II 0.12 7

3318.210r 29 8. 7 NH R 16 1,1 6

3318. 367r 60 IS. 1 Ti ICo I 2.08

1.71 19045

39
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3318.516r

3318.612r

3318.766r

3318.906r

3319.043r

24

19

27

18

23

7. 3

5. 8

8. 0

5. 6

7. 3

NH

Zr II Fe II? p

V II

Zr 11

R 16

0.76

4.49

2.56

0.04

1,1 35

136

137

4

6 3322.481r

3322.655r

3322. 704r

3322.874r 1

3322.949 J

68

40

15

495

23. 4

17. 5

11. 2

[ 23. 1

ll57. 3

Fe I NH

Cr II NH —

Ti II (Zr II)

2.94 R 14

4.17 R 14

0.15

0.76

396

1,1

51

1,1

734

6

6

7

3319.078r 59 18. 0 Ti 11 0.13 8 3323.084r 41 39. 4 Fe II 3.97 92

3319.169r 18 5. 5 Co I 3.02 155 3323.127r 19 18. 2 NH R 9 0,0 6

3319. 258r 54 16. 3 Fe I 2.99 449 3323.297r 5. 5 2. 3 Cr I? 3.10

3319.362r 30 9. 0 3323.395r 47 17. 8

3319.490r

3319.544r

3319.686r

3319.824r

3319.903r

3320.032r

3320.129r

3320.262r

48

34

5. 5

32

41

12

15

122

14. 5

13. 1

1. 6

9. 8

12. 4

3. 7

5. 0

36. 8

Co I Co I

Co I NH

Dy II

Sm II Ni I

2.93

1.71

2.93 R 10

0.00

0.18

0.17

154

45

153

0,0

20

9

6

3323. 540r

3323.752r

3323.919r

3323.999r

3324.071r

3324.150r

3324.364r

42

84

18

11

87

31

64

14. 5

28. 5

6. 3

5. 9

27. 8

13. 6

19. 7

|NH

Cr II Fe I

Ti I? NH

Cr II- Cr II Fe I? Cr II —

Fe I

R 9 4.15

2.83

2.32 R 9

2.43

4.77

4.41 3.27

0,051

379

255

0,0

4

120

80 617

6

6

3320.379r 19 7. 7 NH R 15 1,1 6 3324.544r 60 18. 0 Fe I 2.40 191

3320.492r 39 11. 9 3324.678r 40 12. 1

3320.654r

3320.778r

77

79

23. 2

23. 8

IIFei NH

INi IFe I

2.43 R 10

3.60

3.04

190

0,0

108 396

6 3324.791r

3325.012r

3325.038r

42

33

10

12. 6

10. 0

4. 0

Fe I Fe 11 NH

3.97 R 1393

1,1 6

3320.915r 8. 5 2. 6 Mo II 3.11 6 3325.158r 6. 5 2. 0 Ti I 2.13 190

3321.043m

3321.19.5r

7. 5

11

2. 2

3. 4

Be I Be I Cr I? |Sm II

2.72

2.72

3.11 0.38

1

1

18240

5 3325.251r

3325.332r

3325.479r

46

15

61

14. 0

6. 3

18. 4

Co I NH

Fe I

2.01 R 13

2.45

70

1,1

191

6

3321.237r 31 9. 5 Ni I 3.31 92 3325. 582r 15 4. 6 NH R 13 1,1 6

3321.352m 9 2. 7 Be I 2.72 1 5 3325. 690r 3 1. 0

3321.430m 16 5. 1 5 3325.756r 4 1. 2

3321. 538r 33 12. 8 V II 2.37 71 3325.898r 4. 5 1. 3

3321. 586r 40 12. 6 Ti I 1.07 87 3325.975r 3. 5 1. C

3321. 707r 92 28. 7 Ti II 1.23 65 3326.082r 3 0. S

3321.918r 23 7. £ Co I 2.08 106 3326. 205r 11 3. 6

3322.061r

3322.202r

12

43

4. 1

14. ^ Co I /2.04

\2.87 104

149

3326.302r

3326. 423r

10

24

3. S

8. 1

Co I? NH

/1.78

13.05 R 8

46

157

0,0 6

3322. 325r 108 35. ii Ni I 0.42 39 3326.597r 31 14. S Cr I 3.09 182

40
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3326.695r 25 29. 9 Ni I 3.54 108 3330.435r 8. 5 2. 7

3326.777r

3326.868r

3326.997r

3327.167r

3327.294r

3327. 403r

214

42

38

14

7. 5

53

64. 0

22. 8

14. 9

4. 5

2. 3

16. 1

||Ti IIZr II -NH

Co I

INi INH

0.11

1.53 R 8

2.93

3.31 R 8

7 91

0,0

152

90

0,0

6

6

3330.515r

3330.615r

3330.672r

3330.784r

3330.926r

3331.064r

3331. 254r

17

20

47

24

38

8. 5

19

5. 2

7. 8

14. 1

7. 2 IL 3

2. 5

5. 7

NH

Mn I Mn n NHNi I p—

R 11

2.16

4.69 R7

3.54

1,1

9

0,0

107

6

6

3327.503r 59 20. 1 Fe I 2.40 190 3331. 397r 10 3. 1 Gd II 0.00 8

3327.627r

3327.731r

3327. 886r

3327.971r

3328.211r

20

7. 0

64

37

34

6. 1

2. 1

19. 4

16. 8

10. 4

NHZr II

Y 11 Fe I NH

Co I

R12

0.32

0.41

2.18 R12

3.10

1,111

18

86

1,1

6

6

3331. 617r

3331.785r

3331.930r

3332.053r

3332. 109r

3332.195r

43

48

31

22

1 ...

> 194

12. 9

14. 5 IL 2

12. 2

1 35.7

1 35.7

Fe I Fe I

Zr nTi II Mgi

2.43

2.48

0.36

1.24

2.71

191

144

11

65

4

3328.357r 66 19. 9 Cr II 2.42 4 3332.290r 15 9. 8

3328.475r 28 8. 5 Fe I 3332.350r 24 10. 9

3328.583r 6. 5 2. 0 Fe I? 3332.41 a 11 4. 0

3328.719r 42 12. 6 Ni I 0.11 20 3332.576r 11 3. 5

3328.803r 7 3. 4 Cr I 3.09 160 3332.719r 8. 5 2. 6

3328.870r 67 20. 3 Fe I 3.27 617 3332.834r 33 10. 1 Fei?

3328.96 a 5. 5 2. 1 3332.895r 12 4 9 Cri 3.11 182

3329.056r 55 16. 7 Cr I |Fe I- Fe II

3.12 182 3333.029r

3333.119r

10

29

3. 0

8. 9 NH

NH

R 10 R6

1.1

0,0

6

6

3329. 103r 33 16. 5 3333.222r 10 3. 0

3329.208r 6. 5 2. 1 Mo II 3.06 6 3333.395r 49 14 7 Co I 0.51 25

3329.305r 12 5. 8 3333.597r 42 12. 5 Cn 2.90

3329.438r

3329.518r

3329.632r

3329.772r

3329.852r

3329.914r

3329.972r

183

42

9

33

15

118

J

54. 9

26. 1

4. 6

11. 0

7. 4

1 24. 0

1 17. 8

llTi 11 Co I Fe I Fe I NH

Vi

Mg I Fe I

0.13 3.02

3.05

R 7

1.22

2.71

3.02

7 153

542a

0,0

55

4

6

3333.723r

3333.822r

3333.915r

3333.985r

3334.135r

3334.225r

3334.275r

32

21

9. 5

21

51

92

44

9. 6

6. 4

2. 8

6. 4

32. 2

27. 7

13. 2

NH

NH

Til

Co I Fe I

|Fei Zr II

R6

R 10

0.00

0.43

2.43

3.27

1.00

0,0

1,1

25

23

190

617

58

6

6

3330.082r

3330.234r

23

30

8. 7

9. 2 Fe I-

|NH

2.83 R 7 378

0,0 6

3334.482r

3334.622r

33

27

10. 1

8. 2

||NH

Nd II

Zr II

R 6

0.18

0.56

0,0 42

21

6

3330.308r 49 14. 7 Fe I 3.02 3334.715r 30 9. 1 Cn 2.89

41
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3334.802r 10 3. 3 Cri? 3.37 3338.920r 12 3. 8 Cr II? 6.79

3334.934r 21 6. 4 Cn 3.08 160 3339.049r 41 12. 3 Ni I 3.54 104

3335.061r

3335.185

3335.308r

3335.422r

15

144

69

40

6. 7

43. 0

21. 7

12. 1

Ti ri Cr n

Fe I Cr 11

0.12

4.41

2.56

4.43

7

80

246

92

7

3339.202r

3339. 307r

3339.446r

3339.582r

62

16

11

52

18. 8

5. 0

3. 4

15. 6

Fe I NH

Fe I

f2.45 12.95 R 8

3.02

190 446

1,1

502

6

3335.535r 121 53. 6 Fe I — 1.56 49 3339. 687r 39 11. 6 Fe I

3335.728r

3335.784r

3335.848r

25

89

33

7. 6

27. 1

18. 0

Fe I p

Fe I NH

2.73

2.84 R 9

307

379

1,1 6

3339. 80 Ir

3339.879r

97

45

29. 2

21. 1

Co I —

|Cr II NHCr II

2.96

2.43 R 4

4.41

155

4

0,0 92

6

3335.923r 50 21. 6 3340.041r 19 5. 6

3336. 128r 34 12. 1 3340.178r 9. 5 2. 7 Fe I

3336.260r 58 30. 5 Fe I 3.30 618 3340.356 157 47. 2 Ti II 0.11 7 7

3336.346r

3336.504r

3336.548r

3336.689r

3336.831r

3336.967r

3337.007r

3337. 188r

84

25

12

416

32

11

54

55

32. 5

16. 3

16. 2

124. 8

41. 3

5. 9

23. 3

19. 6

Cr II NH

Fe I p

Mg I

Ti II Ni I |Coi- NH

2.42 R 5

3.02

2.72

1.18

0.03

0.43 R 5

4

0,0

450a

4

43

17

25

0,0

6

6

3340.570r

3340.691r

3340.825r

3340.89Sr

3341.005r

3341. 168r

3341. 285r

3341. 348r

79

29

6

43

11

14

5. 5

33

26. 0

9. 6

1. 8

12. 8

3. 3

4. 2

1. 9

10. 1

|Fe I Zr II NH

Fe I Dy II

Co I

2.28 0.16 R 4

2.87

139

3

0,0

148

6

3337.340r 11 3. 8 Ni I p 3.61 122 3341.451r 9. 5 2. 9 Mn 11? 4.69

3337.393r

3337.499r

3337.672r

3337.853r

3337.923r

3338.010r

3338. 116r

3338.237r

3338. 347r

3338. 430r

3338.520r

3338.628r

18

49

65

81

51

5

31

26

1824

37

93

5. 8

15. 2

19. 4

24. 5

31. 3

1. 4

9. 4

8. 0

5. 6

7. 2

11. 1

28. 0

Mn II La II Fe I

|V II Ti II Fe I

NH

Zr II Fe n

Fe I

4.69

0.40

2.69

3.12

1.24

3.02

R 5

0.96

3.89

3.00

45

304

184

55

0,0

61

76

396

6

3341. 558r

3341.688r

3341.835r

3341. 930r

3342. 148r

3342.226r

3342.310r

3342.374r

3342.474r

3342. 585r

3342.697r

13

25

152

194

27

110

58

5

8. 5

89

45

6. 0

14. 0

126

58. 1

10. 7

33. 0

27. 6

2. 0

2. 9

26. 8

14. 6

Ti I?

Ti 1 Ti II Fe I

Ti I Fe I Fe I NH

Cr I? Cr II

Ti I lICoi

/0.90

11.98

0.00 0.57

2.69

0.00

2.28

2.84 R 7

3.37

2.45

0.00 2.08

60

178

24

16

303

23

137

378

1,1

4

25

105

6

3338.774r 41 12. 3 Ni I 1.68 54 3342.760r 30 17. 0 Fe ip 3.04 396

33.38.813r 22 11. 3 NH R 8 1,1 6 3342.900r 16 5. 0
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Wiatn

AX (ml)

Re- duced

W icltn AX/X

(F)

opot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width AX

(mA)

Re- duced

W Idtll AX/X

(F)

bpOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3343.024r 18 5. 5 NH R 7 1,1 6 3347. 135r 7. 5 2. 3 Cr II? 6.77

3343.234r

3343.347r

3343.524r

3343.672r

3343.776r

3343.904r

3344.083r

3344.183r

3344.389r

3344. 523r

3344.589r

57

21

23

42

90

8. 5

17

29

13

59

19

17. 2

6. 3

7. 0

12. 6

27. 0

2. 5

5. 2

8. 6

4. 0

17. 7

6. 7

NH-

|Fe I Cr I Sm 11 —

Fe I

Ti II

Fe I NH

Ca I La II

R 3

2.18

3.09

3.02

0.15

2.99 R 3

1.88

0.23

0,0

88

159

449

7

450

0,0

11

45

6

6

3347.318r

3347.375r

3347.506r

3347.628r

3347.838r

3347.939r

3348.121r

3348.237r

3d48.o87r

od4!5.o4Ur

3348.687r

4

30

30

14

68

64

42

11

32

1. 2

9. 1

8. 9

4. 2

20. 5

19. 2

12. 5

4. 0

o o o. J

y. 0

11. 0

Sm 11

Fe I NH

Cr II Fe I Co I

V TT V II —

X 1 1 Sm II — NH

0.48

2.99 R2

2.43

2.28

2.04

0 no

R 5

48

449

0,0

4

138

103

1 QA

ZO

1,1

6

6

3344.699r 10 3. 1 3348.910r 122 43. 9 Ti II- 0.12 7

3344.792r

3344.883r

3344.936r

3345.024r

3345. 166r

38

21

70

62

17

11. 5

9. 6

21. 1

21. 4

5. 1

O A o. 4

Zr II (Ceil)

NH

Zn I Co I?

Mn I Cri?

1.01 0.53 R6

4.08

1.74

z. io

3.43

72 165

1,1

4

45

218

6

3349.002r

3349.079r

3349.266r

3349.447

oo4y.oozr

o£)4y.D5Zr

3349.741r

j 135

19

546

14

f 29. 6

1 23. 3

27. 7

163

Oo. i

8. 2

Ti II Cri

Ti 11

IN jn

TSTTT IN XI Cr II? Fe I

0.61

3.01

0.05

XL O 2.71

2.83

16

1

1 1 1 J J. 14

377

7

ft

«

3345.486r 13 4. 2 NH R6 1,1 6 3349.832r 1. 5 6. 9

3345.583r 50 14. 9 Zn I 4.08 4 3349.947r 11 4. 2

3345.629r 27 10. 1 NH R 3 0,0 6 3350.081r 16 5. 5

O£J40. /Uor ID 5. 2 re I O AO 1 y1 1 OOCA 01 A-^ oy

1 1 i 1

3345.915r

1 O

20

3. 7

6. 0 ViiZn I 4.51 4.08 244

4

3350.296r

3350.379r

29

55

9. 6

17. 2

Fe I

Ca I

12.45

1.89

191

11

3346.022r 34 10. 3 Cri 3.00 112 3350.412r 12 4 0 Ni II 2.95 1

3346. 152r

3346.282r

3346.426r

3346.602r

oo4D.74Dr

19

28

39

22

119

5. 8

8. 5

11. 7

7. 0

35. 6

NHCo I NH

Ti II (Cri)

(Cn)

R 6 1.74 R 2

2.98 2.97

1,1 45

0,0

112 112

6

6

7

3350.515r

3350.64 a

66o\}.ib a

3350.852r

3350.956r

58

4. 5

0

11

16

17. 3

1. 4

1. 0

3. 5

4. 6

Ti I Ti II (Gd II)

NHomQm TT? 11

NH

1.98

1.16 0.14

R' 1

R 1

178

43

7

0,0

0,0

6

6

3346.934r 65 19. 6 CoiIFe I 2.96 2.18 15387

3351.068r 18 5. 6 Ni I p — NH

0.00 R 4

3

1,1 6

3347.025r 22 7. 8 3351.156r 9. 5 2. 8

761-925—66-^6 43
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

Hi r

or

ixOt. Line

RMT

IN 0. or

V ID. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

DOlar

Identification

Low

hi c

or Rot. Line

RMT

JN 0. or

Vib. Band

Notes

/. 0 Z. O br I I.OO QQcA noQ*' o4 in Q iU. o aV II u.uy Q<3

oooi.ooyr 1. o

0 Q Ji. o ooOD.zo / r A A X e II 1 O c:

OQ CI /II Qy* oooi.4ior 1 -I 1 i o. o Mn I y"37 1 A Q -T e I u.y i

oool.ozor oy 1 /. 0 jf e I QQoy 0000.414" 7'3 zi. y i: e I O OQ 1 *37 16/

3351.612r 24 9. 4 Cr I 3.10 160 3356.542r 26 7. 9 NH Q 2 0,0 6

3351.751r 58 17. 5 Fe I 2.73 304 3356. 687r 50 14. 9 Fe I 3.05

3351.968r 45 14. 5 Cr I 0.00 5 3356.842r 14 4. 2 Co I? 3.07 151

3352.065r 71 21. 4

4. /

lITi II oC II 1.22 U.UU 54 3356.958r

3357.122r

3357.278r

7. 5

12

50

2. 3

3. 8

15. 1 ||Zr IIIN Xl 0.00

\i o

3

aD

3352.638r 14 4. 2 3357.403r 36 10. 5 Cr II 4.41 79

3352.775r 6 1. 8 3357.569r 30 8. 9 Fe I

3352.825r 18 5. 5 Co II 2.24 2 3357.682r 4 1. 2

3352.932r

oooo.i/yr

3353.269r

47

0 /

43

14. 1

12. 8

IIFei Ti I

v^r II Fe I

2.45 0.02

O AO.

2.43

19025

A

190

3357.740r

3357.825r

3357.942r

33

35

8

9. 6

10. 6

2. 4

NH

Fe I Fe II

Q 1,4

2.99

4.15

0,0 448

117

6

3353.405r

3353.528r

14

8

4. 2

2. 4

3358.048r

3358. 142r

44

13

13. 5

4. 1

|NH

Fe I?

/Q 5 IR 0

o,o\

0,0/ 6

3353.635r

3353.742r

3353.924r

3354.066r

3354.217r

3354.390r

3354.537r

3354.645r

3354.890r

3355.064r

3355.230r

3355.364r

3355.528r

3355.664r

3355.824r

3355.947r

24

80

18

51

32

68

19

65

18

17

71

8

21

6

12

11

7. 8

23. 8

5. 5

15. 4

9. 6

19. 6

5. 6

19. 5

5. 5

5. 2

21. 2

2. 4

6. 4

1. 7

3. 7

3, 2

|NHZr I?

Sc II NH

Fe I Co I

lICoi

Zr II Fe I? Ti II? p

Ti I

Fe I V II Fe I

Co I

R 1 0.15

0.31 R' 0

2.86

2.96

0.51 0.76

1.22

0.02

3.30

2.60

0.96

2.04

0,018

12

0,0

378

152

2334

64

24

617

149

25

103

6

6

3358.282r

3358.408r

3358.515r

3358.637r

3358.698r

3358.795r

3358.901r

3359.010r

3359.114r

3359.286r

3359.408r

3359.502r

3359.635r

3359.689r

75

35

100

23

59

32

70

21

106

89

38

90

27

102

23. 6

10. 3

30. 0

9. 0

17. 7

9. 5

20. 9

6. 9

32. 1

27. 5

12. 1

28. 3

9. 1

32. 2

|Ti I Fe 11-

NH

NH

Cr II Gd II NH

NH

Fe II p

NH-

|Fe I NH

Ni I Co I NH

NH

iFe INH

NH

Sc II

0.00

3.89 Q 6 Q 2

2.45

0.03 Q 8 Q 3

1.67 Q 9

2.99 Q4

3.48

1.71 fQ6

IQ 11 Q7

0.86 IQ 12 Q 9 001

23

77

0,0

0,0

4

8

0,0

0,05

0,0

0,0

10844

0,0\

0,0/

0,0

25

o,o\

0,0/

0,04

6

6

6

6

6

6

6

6

6

6

44
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3359.802r 69 28. 4 NHFe I

fo in IQ 13

3.30

0,0/

617

6 3362.802r 89

lO. o

27. 9

Ti II Ni I

1.22

0.21

64

23

3359.932r 39 18. 1 NH

Zr II Q 11

1.49

0,0 91 6 3362.973r

3363.164r

30

15

8. 8

4. 7 NH Q 21 0,0 6

3360.047r 89 29. 7 NHNH

/Q 7,8

IQ 14 Q 6, 9

0,01 0,0/

0,0

6

6 3363.308r 33 10. 0 Co INH

3.05 Q 21 0,0 6

3360.124r 79 28. 0 NH fQ 10 IQ 12

0,01 0,0/

6 3363.408r 50 14 8 Fe I Fe II- NH

4.08 Q 5 105

0,0 6 3363.616r 50 15. 0 iNi I NH

3.48 Q 22105

0,0 6

3360.211r 40 19. 9 NH Q 11 0,0 6 3363.720r 55 16. 4 Cr II 2.43 3

3360.310r 89 31. 9 Cr II NHNH3.10 Q 15 fQ 4,12

IQ 13

21

0,0

0,01 0,0/

6

6

3363.821r

3363.921r

31

33

9. 2

9. 7

Fe I (Zr II) NH

2.76 0.36 Q 22307

11

0,0 6

3360.351r 36 22. 9 3364.014r 25 8. 3 NH Q 22 0,0 6

3360.497r 51 21. 7 NH Q 13 0,0 6 3364.098r 5. 5 1. 6

3360.607r

3360.694r 3360.808m

32

23

14

15. 1

12. 9

8. 1

NHNH

NH

NH

Q3,14

Q 16 Q 14 Q 15

0,0

0,0

0,0

0,0

6

6

6

6, 8

3364.228r

3364.274r

3364.400r

14

47

29

6. 1

14. 1

8. 7

Fe II p

Fe I Fe I NH

1.72

3.05 Q 23

5

0,0 6

3360.921r 22 16. 1 NHFe I Q 15

2.42

0,0 142

6 3364.614r 55 16. 4 Ni IFe I 3.38

2.59 107 245

3361.007r 26 22. 1 NH

Ti I

/Q 2 \Q 17 0.02

0,01 0,0/ 24

6 3364.651m

3364.735m

23

20

10. 3

6. 4 NH

NH

Q 23 Q 23

0,0

0,0

6,8

6,8

3361.107r

3361.193r|

3361.287rJ

8

939

19. 7

r265

169. 3

NH

Ti II

|Tii Sc II

Q 16

0.03

0.02 0.00

0,0

1

23

4

6 3364.946r

3365.032r

3365.112r

5

8

3. 5

1. 6

2. 3

1. 0

NH

Ndii?

Co I

P' 2

2.01

0,0

69

6

3361.434r

3361.570r

3361.772r

20

90

47

25. 7

46. 4

22. 3

NH

Ni I (Vii)

Cr II

/Q 17

0.11 2.37

3.10

0,01 0 Of

1970

21

6 3365.206r

3365.316r

3365.446r

3365.549r

16

7

31

27

4 9

2. 1

9. 2

8. 2

NH

Fe II— NH

V I

Q 24

3.89 Q 24

1.18

0,0

78

0,0

54

6

3861.854r

3361.953r

3362.141r

3362.268r

60

81

61

76

27. 5

30. 9

22. 1

26. 6

NHTi I

ICa I |Sc II- Fe I Cai

Cr Ir e I NH

(Gd II) NH

Tm 11

/Q 18 IQ 19 0.02

1.90 0.00 2.84

1.90

2.54

0,01 0,0/ 25

114 377

11

54

6

3365.773r

3365.992r

3366.176r

3366.359r

107

24

116

19

3L 9

7. 3 34 6

5. 7

Ni I

Ti I ITi n

IINii NH

Sr I

0.42

2.04

1.24 0.17 Q 25

1.85

38

17854

8

0,07

6

3362.394r

3362.593r

26

8

9. 0

2. 7

Q 19 0.08 Q 20

0.03

0,08

0,0

6

6

3366.459r

3366.552r

3366.656r

14

8

5

4 4

2. 4

1. 5

NH

Ce II

Q 25

0.55

0,0

99

6

45
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3366.796r

3366. 874r

3366.982r

3367.098r

3367. 162r

3367.299r

3367.392r

1 180

23

1 146

30

12

r 31.

5

I 31. 5

7. 1

^ 22. 1

1 29. 2

9. 0

3. 9

Fe INi I Fe I Fe II Co I Fe I Fe I NH

2.69

3.38

2.20

5.57

0.43

2.42

Q 26

302

108

87

177

22

142

0,0 6

3370.195r

3370.333r

3370. 449r

3370. 635r

3370.798r

3370.884r

3370.974r

30

54

69

61

118

18

83

9. 6

16. 6

20. 7

18. 6

35. 2

9. 2

24. 9

NHCoi

Ti I NHFe I

NH

Co II

Q9

0.58

0.00 Q 8,10

2.69

Q 7,9 2.27

1,1

24

23

1,1 304

1,12

6

6

6

3367.440r 45 13. 2 Cr II 4.41 79 3371. llOr 39 13. 9 NH Q 3 1,1 6

3367.552r

3367.677r

80

48

23. 9

14. 5

Cri

NH

Fe I

/2.54

\2.54

Q 3

54

54

1,1 6

3371. 160r

3371. 295r

3371. 399r

28

51

17

11. 2

15. 2

11. 7

NH

Fe I NH

Q 8,11

Q 9,10

1,1

1,1

6

6

3367.818r 29 11. 6 Zr II 0.32 11 3371. 457r 107 31. 5 Ti I 0.05 24

3367.894r 29 11. 6 Ni I 0.03 20 3371.609r 24 7. 2 NH Q 12 1,1 6

3368.058r

3368.184r

189

26

56. 3

12. 9

Cr II Fe I2.48 4 3371. 716r

3371.763r j 65

f 10.9

1 10.9 NH

NH

Q 10 Q 11

1,1

1,1

6

6

3368. 247r 8. 5 3. 4 Fe I p 3.25 678 3371.988r 104 47. 7 Ni I 0.17 7

3388. 361r

3368.445r

3368. 545r

3368.e)58r

5. 5

6. 5

19

22

1. 8

2. 0

5. 7

6. 6

NH

Fe II? NH

NH

Q 27

4.49 0 27

IQ 27

0,0

134

0,0

1,1 0,0

6

6

3372.089r

3372.178r

3372.226r

118

1 216

59. 9

r 16. 3

1 73. 1

IIFei NH

Sc II

|Ti II NH

2.18 P 3

0.02

0.61 P 4

83

0,0

4

16

0,0

6

6

3368.725r

3368.821r

36

45

10. 9

13. 9

Cr II Fe I4.43 91 3372.352r

3372. 473r

24

29

11. 9

14. 0

Fe I NH

Fe I

2.99 Q 12447

1,1 6

3368.948r

3369. 055r

101

18

32. 4

9. 1

|Sc II —

Fe I NH

Cr II

0.01 2.83 Q 6 4.38

4 376

1,1 686

3372.623r

3372.812

3372.969r

9

459

22

8. 8

135. 9

20. 3

Ti II NH0.01 Q 131

1,1

7

6

3369. 151r

3369.2 17r

39

75

30. 6

28. 2

|Fe I NH

Ti 11 NH

2 45 P 2

1.23 Q 3

191

0,0

64

1,1

6

6

3373. 093r

3373. 233r

3373.316r

6

34

44

3. 1

12. 4

14. 4

Co I Fe I

2.28 122

3369. 37 Ir 27 15. 0 Fe II- NH

3.89 Q 7 76

1.1 6 3373.419r 39 12. 5 NH

Zr II P 41.01 0,074

6

3369. 498r

3369.578r

13

407

17. 5

120. 5 NH

|Ni I Fe I

Q4

0.00

2.73

1,1

6 304

6 3373.506r

3373. 606r

36

9

11. 4

2. 8

NH- /Q 14 10 15 i.n

1 11 6

odoy .DDOr

3369.797r

66

30

77. 1

15. 2 NH

Fe II p Q 5,8 3.89

1,1 766

oo7o.7oDr

3373.880r 35

6. 0

10. 7

t^e II W I Fe I

U.OD

0.41

2.73 303

3369.9 17/r

3370.038r

26

20

10. 9

6. 9 NH Q 6 1,1 6

3373.983r 72 2L 4 Co I Ni II 1.71 2.86 44

1

46
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Widtt

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Widtl

AX/X

(F)

1 Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3374. 135r 7. S 3. 6 NH Q 15 1,1 6 3377. 587r 68 20. a Ti I 0.02 23

3374.222r

3374.351r

3374.452r

3374.642r

3374.736r

150

32

53

98

58

44. 8

9. 5

16. 6

28. 9

24. 5

IINii Fe I

Ti II Fe I Ni I

Zr nNH

0.03

2.22

1.24

3.38

1.00 Q 16

1789

54

106

61

1,1 6

3377. 701r

3377.807r

3377.977r

3378.066r

3378.183r

3378.339r

5. 5

5. S

68

7

19

39

1. 7

1. t

20. 3

2. 1

5. 7

11. G

-Fe I? Fe I

NH

Cr II

Q 20

3.10

1,1

21

6

3374.845r 12 4. 0 NH Q 16 1,1 6 3378.586r 19 6. 5 NH Q 20 1,1 6

3374.932r

3375. 095r

3375.215r

3375.3421-

35

24

9

19

10. 7

7. 2

2. 8

5. 7

Cr I? Cr II NH

Co I? NH

|Fe I

3.12

2.48 Q 17

3.07 P 4

1814

1,1

153

0,0

6

6

3378.687r

3378.744r

3378.868r

3379.024r

1

143

50

92

1 30. 7

1 17. 9

18. 1

27. 6

Fe I Co I NH

Fe I p

Fe I

2.69

2.28 P 5

2.28

2.18

30]

121

0,0 137

85

6

3375.465r

3375.562r

3375.632r

8. 5

43

15

2. 5

12. 8

5. 3

Ni I — NH

NH

3.60 Q 17 Q 17

108

1,1

1,1

6

6

3379. 200r

3379.377r

3379.440r

71

) "

21. 9

r 23. 2

1 0. 9

Cr I |Tii

Cr 11 NH

0.00

0.05

3.10 Q 21

524

21

1,1 6

3375.730r 20 5. 9 Fe I 2.99 3379.550r 7. 5 2. 5 Cr I? 2.54 54

3375.855r 8 2. 3 3379. 646r 1. 5 0. 4

3375.945r 7 2. 1 3379. 706r 2 0. 8 Fe I

3376.028r 20 5. 9 NH —

V I Q 18

1.19

1,1 54

6 3379.824r 71 25. 3 |Cr II Cr I 3.10

2.54 2154

3376.102r 11 3. 4 3379.923r 44 21. 1 Ti II 1.24 64

3376.205r 8 2. 3 Co I? 3.02 3380.020r 2. 5 1. 3 Fe I 3.33 709

3376.278r 24 7. 2 Cr II? Zr II- NH

4.41 0.96 P 5

78

60

0,0 6

3380.118r

3380.260r

62

30

27. 5

31. 2

Fe I

Ti n

2.76

0.05

304

1

3376.335r 56 16. 7 Ni I 3.48 104 3380.313r 76 43. 4

3376.494r

3376.595r

3376.678r

54

8

7

15. 9

2. 4

2. 1

NH —

IIFei Cr n?

Cr II?

Q 18

4.41

4.74

1,1

90

112

6 3380.468r

3380.585r

3380.752r

6

809

17

9. 7

239

27. 1

Ni I

|Sr II- Fe I

0.42

2.94

37

4

3376.758r 12 3. 8 Fe I 3380.889r 87 51. 0 Ni I 0.27 7

3376.842r

3376.948r

3377.066r

3377.272r

3377.361r

3377.486r

7

5. 5

35

17

5. 5

54

2. 1

1. 6

10. 5

4. 9

1. 6

16. 1

Co I? Co I NH

NH

Fe I—

V I

lITii Zr II

2.54

1.71 Q 19 P 5

1.19

0.05

0.41

42

1,1

0,0

54

25

11

6

6

3381.033m

3381. 132r

3381.353r

3381.495r

3381.532r

3381.649r

3

30

58

2

4. 5

2. 5l

1. 9

14. 1

21. 6

0. 8

1. 4

0. 9

Fe II- NH

Fe IFe I

Co I Fe I

5.57 P 6

/2.84

13.25

2.04

1.61

177

0,0

376

677

8849

86

47
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3381.759r

3381.866r

3381.993r

3382.088r

6

11

33

16

1. 8

3. 5

9. 8

4. 9

NH?

Fe I Co I? Cr I?

P 3

3.04

2.33 3.12

1,1

123

181

6

33S5.673r

3385.725r

3385.869r

Q'iS'i q4qr

i 70

I

7. 5 70

f 17. 8

1 4.

2

2. 5 90 7

Ti I NH

Fe I? NH

TiXIXT

0.05 P 7

Q 25

u.uo

24

0,0

1,1

9*? ^o

6

6

21

123

6. 3

11. 9

36. 5

NH

Ti I Fe I

P 6

1 07

2.18

0,0

86

84

5 3386.174r

3386.272r

30

16

9. 0

5. 7

NH

NH

NhXN U TT? XX

1

IQ 25 Q 25

1 99

1,1

1,1 6

^^89 4fi8r oo 19. 2 1

0

xv^ O. X

q 3. 4 1X 7I O.'i 0o XTTpC TTXX 88

^^89 fi8Qr oo 9^1 2 Cr II 2.45 3 «-> OU . VtJ KJl. 94 7 1 J . X

OOOZ/i ^^89 VQflr / <J\JL 14 O. OOOU . ^ O t/i ao. o 2. 4 Ti^P X? TTXX ^^89 QOOr 99 A O* T 0.00 \

9ii ^o 7 4 ^^89 QQ'^r 10. 6 Fe I OtJ O . O 1 Ol 1xo8 o. o

^^fi"^ flQfir q o^ 2. 9 xo 4. 4

oooo ^^8'^ .-i90fir VUL i . o 2. 4 Cn T? 3.07 OOO < • X 1 -Li X o. v., IN XX 1 1 AO

OOoO.O -LOl P 4 ft OOO / .Ov/Ol Oo Qy. 7/ fTo TT O.U *\ 07t

3383.376r 28 10. 1 Fe I 2.61 245 3387.418r 87 25. 8 Fe I 2.76 306

3383.493r 7 3. 0 3387.464r 38 20. 0 Ni I 0.11 17

3383.573r 13 7. 9 3387.626r 86 25. 5 Fei

3383.697r

1 430

f 56.2 Fe I r2.20 \2.95

85

444 3387.718r 31 15. 2 Co II 2.27 2

3383.765r 1127 Ti II 0.00 1 3387.852r 187 55. 2 |Ti IIZr II 0.030.97

1 74

3383.997r 64 32. 2 Fe I 2.18 83 3388.054r 22 6. 8 NH Q26 1,1 6

3384.089r

3384.239r

3384.325r

3384.425r

3384.592r

19

6

11

14

8. 5

8. 7

1. 8

3. 6

4. 4

2. 8

NH

Cr I NH

Fe I? Vi?

Mo I?

P 7

2.54 Q 24

1.06

1.47

0,0

54

1,1

46

9

6

6

3388.175r

^^88 oooo.ox^^t ^1 9fl

'^'^88 OOOO.T:wOi 4fiar

3388.625r

3388.760r

103

Oii 'i9

44

52

89

30. 4

xo. o

13. 1

15. 5

26. 6

IICoi Co II

/il 7,r TTXX NH

Fe I

Ti II

0.58

2.24

0 on VX ao

1.24

23

2

2

0 n

53

A

3384.646r 32 9. 4 Cr I 2.54 54 3388.858r 13 4.3 Dy II 0.59

3384.772r

oooO.uoir

56

1

1

X 1 9Q^y

16. 7

^o. 9^ a 7

Fe IMTT IN XX

X^ C 1

Tt\J uy TT11

0.99 P-IT 7t 25

RU 3388.971r

3389.121r

3389.251r

42

19

37

12. 4

5. 8

11. 2

Fe I

NHFe I

3.07

P8

502

0,0 6

OOQC n7Qr xo A Q OOOi? .O^^l Xo o.^ 0o Sni II 0 ^4

3385.225r 77 22. 7 Co I 0.51 22 ooo9.404r o o 00 11. 4

3385.332r 13 4. 1 Cr I 3.55 236 3389.611r 6 1. 8

3385.441r 47 14. 2 Fe I 3389.748r 48 14. 1 Fe I 2.22 87

3385.552r 57 16. 8 Fe I

48
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E 1' or Rot. Line

RMT

No.

or

Vib. Hand

Notes

3389.824r 8 3. 0 Hf II 0.45 8 3393.845r 90 27. 9 Cr 11 3.10 21

3389.924r 4 1. 2 3393.927r 43 16. 5 Fe I 2.28 13G

3390.018r 17 5. 2 NH /Q 27 IP 6

1,1

1,1 3394.085r 63 18. 5 Fe 1 2.45 ]S8

3390.108r

3390.264r

3390.408r

3390.518r

3390.600r

3390.683r

3390.783r

17

21

24

12

21

40

20

5. 2

6. 3

7. 4

3. 8

6. 9

11. 9

6. 5

Fe II? Fe I p Co I

Til

Cr I?-

Co I?

6.80

2.43

2.04

1.05

3.55

3.19

207

188

102

86

236

3394.17 a

3394.297r

3394.383r

3394.550r

3394.611r

3394.740r

3394.823r

3394.950r

10

93

41

1 204

24

13

12

3. 0

27. 6

20. 3

f 36. 8

I 36.8

9. 3

4. 4

3. 5

Cr II Fe I

Ti II Fe I

Co I

3.10

0.01

2.20

1.71

21

1

81

42

3390.897r 14 6. 2 3395.077r 29 8. 7 Fe I 3.02

3391.039r 238 70. 2 Nil 0.00 5 3395.16 a 7 2. 2

3391. 107r 36 31. 9 3395.273r 19 6. 5 NH P 10 0,0 6

3391.273r

3391.373r

3391.442r

3391.590r

3391.670r

21

15

99

40

11

7. 5

5. 8

29. 2

11. 8

3. 8

Fe II Cri

Cr II NH

4.15

3.85

2.42 P9

117

254

3

0,0 6

3395.386

3395.615r

3395.747r

3395.877r

111

44

40

16

32.8

12. 9

11. 8

5. 2

Co I (Fe II) Cr II NH

Fe I? p

0.58

4.15

4.47 P 10

/2.45

13.05

25

117

100

0,0

189 543

7

6

3391.841r 30 9. 0 Fe I p 3.30 678 3395.990r 35 15. 1 Fe I

3391.973r

3392.017r 1 113 [ ^

1 20.0

Zr II Fe I

0.16

3.02

1

499

3396.043r

3396.185r

79

63

23. 6

18. 5

Fe I Ni I 3.61 122

3392.123r

3392.305r

3392.498r

3392.624r

3392.678r

48

102

31

i 144

J

19. 2

32. 9

11. 5

1 41. 0

1 25.4

NH

Fe I -Gd II Fe I Vii-

|Ti I

P9

2.20

0.08

2.18

2.37

1.50

0,0

83

7

85

70

136

6 3396.302r

3396.388r

3396.507r

3396.607r

3396.657r

31

47

15

6. 5

25

9. 3

14. 0

4. 4

2. 2

7. 4

|NHZr II Fe I Ni I p Eu II?

Zr II

P 10

0.96

0.96

3.61

3.33

1.66

0,058

25

118

30

103

6

3392.791r 18 17. 1 NH P 9 0,0 6 3396.830r 8. 5 2. 6 Rh I 0.00 3

3392.894r 17 26. 2 3396.927r 19 7. 7

3392.978r

3393.025r

1 570

fl60

1

1 70.7

Ni I Cr II0.03

3.10

20

21

3396.981r

3397.062r

7928

23. 3

12. 1

Fe I Lu II

0.96

1.46

26

4

3393.150r 54 41. 3 Zr u 0.04 3 3397.221r 40 12. 1 Fe I 3.02 503

3393.292r 31 14. 1 3397.316r 8. 5 2. 7 3393 391r 47 18. 5 Fe I 2.86 376 3397 436r 29 8. 8

3393.61 a 56 18. 7 Fe I Dy II

/2.76

12.83 305

376

3397.556r

3397.644r

43

68

13. 8

20. 3

Fe I Fe I

3.02

0.99

447

26

3393.710r 7 2. 0 3397.796r 13 4. 6

49
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3397.839r

3398.017r

37

5. 5

10. 9

1. 5

Ni n 3.60 8 3402.2 18r

3402.266r 1 114

1 0.

6

1 33.5 Fe I 3.24 614

3398.1 lOr

3398.223r

3398.307r

3398.377r

3398.417r

3398.612r

3398.705r

3398.815r

3398.925r

3398.992r

3399.05 a

3399.160r

3399.242r

3399.355r

6

45

1 68

10

41

15

14

j 48

4

28

83

159

1. 8

13. 2

1 8.

8

1 9. 2

2. 9

11. 8

4. 9

4. 1

r 13. 5

1 0. 6

1. 2

13. 1

31. 0

46. 6

Fe I p Fe I

Fe n

Fe I |Ti I

Co I NH

Fe I -NH

Fe I

IIFei Zr 11

3.24

2.76

4.07

1.05

3.13 P 11

P 8

2.73

2.20

0.32

615

304

105

86

157

0,0

1,1 302

85

11

6

6

3402.420r

3402.552r

3402.709r

3402.792r

3402.900r

3403.012r

3403.155r

3403.271r

3403.345r

3403.439r

3403.592r

3403.693r

o 4 AO Tr\ o

3403. 792r

95

28

9. 5

14

35

12

21

1 155

59

27

22

7

27.9

8. 4

2. 6

4. 1

10. 3

3. 7

6. 2

r 23. 8

I 28. 8

18. 5

7. 9

6. 6

1. 9

|Ti II Cr II NHMo II? |NH

Zr II

Fe I

Cr II

tvt: * JNl I Or I

Zr II

1.22 3.10 P 12

4.16 P 12

1.53

/2.73

12.83

/2.43

13.10

3.42

3.85

1.00

53

21

0,0

0,0 91

304

377

321

108

254

59

6

6

3399. 520r 26 8. 2 Or II 4.50 100 3403 .872r 6. 5 1. 9

3399.612r 12 3. 7 Fe 1 3403.995r 8. 5 2. 6 Cr I? 3.37

3399.808r 38 11. 3 NH P 11 0,0 6 3404.069r 13 3. 8

3400.019r 8. 5 2. 5 Gd 11 0.35 22 3404.159r 17 5. 3

3400.145r 16 4. 7 Ti I Mn II 2.40

4.93 3404.280r i 26. 2

1

Fe I fl.Ol 12.73 25 301

3400. 232r 8 2. 3 3404.31 a [ 1<6 1 51. 3 Mo I? 1.47 9

3400.395r 8. 5 2. 6 V I 1.08 46 3404.378r ) I, 35. 3 Fe I 2.20 83

3400.495r 9 2. 6 Co I 1.74 42 3404.448r 10 3. 4 V II? 4.51 243

3400.645r 35 10. 3 Fe I 3.02 3404.584r 36 10. 6 Pd I 0.81 2

3400.845r 19 5. 6

n A r\ A f> A 3404.764r 70 21. 2 Fe I 2.73 300

3400.987r 42 12. 2 Fe I 3.02 3404.839r 43 15. 8 Zr II 0.36 11

340].173r 25 7. 4 Ni I 3.42 107 3404.911r 30 11. 6 Fe I 2.69 300

3401.344r 28 8. 2 3404.964r 10 4. 8 Ti II? 1.22 63

3401. 530r 104 30. 6 Fe I 0.91 26 3405.126 206 60. 5 Co I 0.43 23 7

3401. 644r 17 5. 1 Co I? 1.74 44 3405.26 a 7 2. 5

3401.766r 37 10. 9 Ni II 3. 07 4 3405.371r 10 3. 2 NH? P 10 1,1 6

3401.858r 10 3. 1 3405.504r 10 3. 2 Ni I p 3.70 122

3401.924r 20 6. 0 Co I 3. 23 157 3405.583r 35 10. 4 Fe I

3402.074r 20 5. 9 Co I 2.33 123 3405.704r 10 3. 1

3402. 128r 13 4. 1 NH P 9 1,1 6 3405.838r 56 16. 6 Fe I 2.69 299

50
The Solar Spectnim—Continued

WaveicXlg I'll

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(c\ \r)

Spot

Solar

THpnt.i- fication

Low

E P

or Rot. Lin6

RMT

No.

Vib. Band

i. 'I \J UUD Wave1 pn (rt, Yi

(A)

Equivalent Width

AX

^mA)

Re- duced

Width

AX/X

(t)

Spot

Solar

XTrlpnt.i- KA v-> L* VL fication

Low

E P

or Rot.

Li116

RMT

No.

or Vib. Band

Not-cs

3405.978r 17 5. 1 Ce 11- 0.55 96 3410.651r 7 2. 2

3406.121r 35 10.3 NH P 13 0,0 6 3410.791r 20 5. 9

3406.171r 14 4. 0 Fe I p 2.84 376 3410.903r 84 24. 8 Fe I 0.91 25

3406.258r 6 1. 8 3411.028r 26 7. 6 Cr i?-

3406.358r 9. 5 3. 1 3411. 142r 54 16. 0 Fe I 2.69 299

3406.439r 76 22. 2 Fe I 3.27 676 3411.234r 9. 5 2. 8

3406.564r 34 9. 8 3411.366r 70 20. 5 Fei 2.73 301

3406.810r 136 39. 9 Fe I 2.22 85 3411.568r 6 1. 8

3407.054r 28 8. 2 Fe 1? p 2.83 377 3411.67 a 17 5. 0 Ti I 2.41

3407.205r 101 30. 5 Ti 11 0.05 1 3411. 751r 6 1. 8

3407.314r 56 26. 0 Ni 11 3.08 4 3411.877r 14 4. 1 Fe 1 p 2.69 298

3407.404r 16 12. 5 3411.977r 20 5. 9

3407.464r

3407.561r 1 248

r 50. 9

1 28. 4

Fe I Fe 1 p

2.18

2.18

83

81

3412.030r

3412.170r

4

23

1. 2

6. 6

3407.712r 10 3. 7 3412.349r 123 36. 0 Co I 0.51 25

3407.805r 60 18. 8 Dy 11 0.00 3412.463r 9. 5 3. 2 Ni I p 3.40 90

3407.959r 37 10. 8 Mn I 2.92 26 3412.643r 108 32. 0 Co I 0.00 6

3408.085r 58 17. 0 Zr 11 0.97 72 3412.777r 8. 5 2. 6

3408.185r 20 6. 9 3412.887r 30 9. 1 NH P 12 1,1 6

3408.352r 13 3. 8 3413.00 a 11 3. 7

3408.505r 22 6. 5 Fe 1 3413. 143r 156 48. 4 Fei 2.20 85

3408.679r 8. 5 2. 9 Sm 11 3413.270r 29 10. 7 NH P 12 1.1 6

3408.779r

3408.938r

3409.078r

3409.170r

3409.2 14r

3409 398r

340Q ."iyQr

S40<) fi71r

131

56

9

j 134

40

100

25

38. 4

17. 9

2. 9

f 23.5

1 23. 5

11. 7

29. 2

9. 1

Cr 11 -V II

Co I Fe I Fe I p

Ni I INH

Co I

2.48

2.51

0.51

3.24

3.02

0.00 P 14

0.51

3

120

23

614

445

5

0 024g

3413.410r

3413.492

3413.650r

3413.723r

3413.803r

3413.947r

3414.137r

3414.267r

1 160

53

19

8

112

28

6. 5

r[ 54. 4

17. 5

8. 6

2. 9

36. 1

10. 0

2. 6

Zr nNH

Ni 1 NH

Dy 11 Nil

Fe 11

1.00 P 15

0.17 P 15

0.10

0.11

3.94

60

0,0

5

0,0

17

91

6

7

6

3409.818r 80 23. 6 Till 0.03 1 3414.403r 9 4. 7 Fei?

3409.948r 21 6. 3 NH P 14 0,0 6 3414.511r 53 34 2

3410.038r

3410.181r

3410.254r

3410.394r

3410.564r

60

80

48

5. 5

23

17. 6

23. 5

21. 1

1. 6

6. 7

Fei

Fe I

Zr 11

Fei

3.05

3.41

0.41

2.59

542

735

11

244

3414.637r

3414.779r

3414.9 18r

3415.098r

3415.147r

54

816

49

15

8

156

237

157

24. 9

4. 4

II Zr 11 Zn

Ni I

1.01 0.07

0.03

73

17

19

61
The Solar Spectrum—Continued

length

(A)

Equivalent Width

A\

(ml)

ReducG(l

Width

AX/X

(F)

Spot

Solar

Identifi p Q ti r^n

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

^Wavelength

(A)

EquiWidth

AX

(mi)

ReH 1

1

Width

AX/X

(F)

Spot

Solar

IdentiM p Q f inn

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3415.330r 3. 5 1. 3 Cr I? 3.45 3419.704r 60 17. 7 Fei 2.84 377

3415.443r 6 2. 2 Cr n? 4.50 100 3419.80 a 4. 5 1. 5

3415.540r

3415.683r

3415.790r

3415.897r

3416.032r

3416.142r

3416.289r

3416.409r

3416.512r

3416.639r

82

44

28

4

63

6. 5

42

6

10

5. 5

28. 1

14. 4

9. 4

1. 3

19. 6

2. 1

12. 9

1. 9

2. 9

1. 9

Fei

(Co I) Ni I p Co II

Fe II

Fe I

"Ih'p t n NH

2.22 0.00

3.54

2.20

2.28

3.37 P 16

83

5

123

2

16

7ns

0,0 6

3419.881r

3420.001r

3420. 108r

3420.228r

3420.285r

3420.443r

3420.488r

3420. 598r

3420.748r

3420. 808r

4

3. 5

18

9

23

30

23

6. 5

i 84

J

1. 2

1. 0

5. 3

2. 9

6. 9

8. 8

6. 7

1. 9

f 22. 8

1 2. 6

Mn II? NH

Fe I? NH

NH

Co I

Nil

Mn I Co I

4.93 P 17

P 17 P 17

1.74

0.27

4.23 2.08

0,0

0,0

0,0 42

9

102

6

6

6

3416.676r 44 13. 2 Fei 2.48 142 3421.015r 14 4. 1 NH P 14 1,1 6

3416.782r 16 4. 7 3421. 121r 9 3. 1 Ni i?p 3.42 105

3416.869r

3416.963r

3417.066r

5417.169r

3417.269r

3417.359r

21

68

12

121

51

25

6. 1

19. 9

4. 4

35. 3

20. 3

9. 4

NH

Fe I

Ti II NH

Co I Fei

NH

P 16

1.24 P 16

0.58

1.01 P 13

0.26

0,0

53

0,0

23

26

1,14

6

6

6

3421.221r

3421.350r

3421.487r

3421. 625r

3421.727r

3421 900r

103

50

10

23

20

2

30. 2

16. 7

2. 8

6. 7

fi 0

0\J. fi\J

Cr II Nil

Cr II? Co I?

Fe I

2.42

3.54

/4 29

14!32 2.04

3

122

60

60

101

3417.486r 6 1. 8 Ce II? 0.70 100 3421.954r 4 1. 0 3417.549r 5 1. 5 3422.127r 45 13. 1 Fei

3417.687r 28 8. 0 Co I 2.33 122 3422.214r 8. 5 2. 5 3417.816r

3417.870r

3418.029r

3418.171r

3418.316r

i 139

J 26

70

13

f 22. 5

1 22. 5

7. 6

20. 5

3. 9

Co I

Fe II p Fe I

0.43

2.22

4.08

3.28

19

81O J104

577

3422.335r 3422 496r

3422.661r

3422.769r

48

113

65

165

14. 0

33. 0

48. 1

Nil

Fe I (Gd n)

Fe I Cr II (Ce II)

3.54

2.99 o!24

2.22

2.45 0.45

105 444

2

85

3 144

3418.39 a

3418.522r

3418.732r

3418.88 Ir

3418. 976r

3419. 150r

3419.292r

3419.422r

8. 5

111

29

55

4

48

3. 5

6

2. 7

32. 4

8. 5

16. 1

1. 2

14. 0

1. 0

1. 8

Fei

Gd II Fei

Fei

Fe I? Mn II

2.22

0.00

3.04

3.24

4.93

81

7

576

3422.883r

3423. 020r

3423.08 a

3423.174r

3423.247r

3423.320r

3423.534r

43

12

7.5

14

19

9

6. 5

14. 9

3. 6

2. 3

4. 5

6. 0

3. 1

3. 2

|Nii

Co I Cn?

Cr I?

NHFei?

3.70

1.74

3.85

P 18

12242

0,0 6

52
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3423. 627r 17 16. 9

3423.7 15r 366 104 Ni I 0.21 20

3423. 839r 18 16. 2 NH—

Co II P 18

2.27

0,0

2 6

3423.994r 22 8. 9 Fe I n A C\ A I o 3424.13 a 12 3. 9

3424. 178r 6 2. 6 NH

Fe II? p

P 15

4.15

1,1 116

6

3424.299r 128 38. 8 Fe I 2.18 81

3424. 446r 17 5. 8 NH P 15 1,1 6

3424.5 13r 51 14. 9 Co I 2.08 103

3424. 599r 21 7. 0 Gd II 0.35 22

3424. 7 13r 20 6. 0 NH P 15 1,1 6

3424. 833r 30 9. 0 Zr II 0.04 2

3425.019r

3425.063r

1

> 96

j 27.7

1 0. 6

Fe I Tm II

3.05

0.03

541

7

7 2. 0

3425.37 a 8 2. 3

3425. 446r 16 4. 7 Fe I Nb II 1.35 7

3425. 583r 52 15. 2 Fe II 1.67 5

3425. 746r 6. 5 1. 9

3425. 843r 19 5. 5

3425. 968r 11 3. 2 Cri 3.09 158

3426.092r 22 6. 6 Fe I p

3.11 502

3426.215r 15 6. 5 Ce n 0.12 44

3426, 332r

3426.401r

i 143

J

r 21.3

1 26.0

Fe I

Fe I

2.28

/0.99

12.18

135

25

82

3426.635r

3426. 673r

1

> 121

r 23.6

1 17.8

Fe I Fe I p

2.20

3.27

82

615

3426. 795r 10 3. 2 Fe II p 4.08 103

3426.912r 5 1. 9 NH P 19 0,0 6

3426. 992r 101 48. 4 Fe I 0.99 26 3427.086m 9 14. 0 NH- P 19 0,0 6,8

3427. 129r 218 63. 8 Fe I 2.18 81

3427.206r 18 15. 2

3427. 358r 5 1. 6

3427.462r 3. 5 1. 2

Wavelength

(A)

Equivalent Width AX

(ml)

Re- duced

Width

AX/X

(F)

bpOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3427.522r 19 5. 7

3427.612r 11 3. 1 Cr I?

3427.765r 14 4. 5 Co I? 3.19

3427. 838r 24 7. 1

3427.948r 11 3. 5 NH P 16 1,1 0

3428.020r 41 11. 9 Feip 3.30 616 OAOQ 0r\7r- o^iio. / r 1 1

t OX

1

1o. 0 IXU I u. uu

110

r 1 7 a Ni I p Feip

•J . / U

2.76 302

3428.492r 1 [ 17. 8

3428.642r 24 6. 8 Fe II p 3.97 90

3428.758r 69 20. 1 Fe I 3.60 836

3428.932r 19 5. 5 Ti I 1.89 168

3429.038r 6. 5 1. 9

3429. 148r 4. 5 1. 3 Fe I?

3429.334r 10 2. 9

3429.471r 8 2. 3

o4<iy.554r o 1 K

o4Z9.717r K A O. ^

3429.817r 22 6. 4 Fe I

j i&.Oi \3.05

OA A 540

3429.937r 5 1. 5

3430. 083r 2 0. 6 Fe I?

3430. 160r 6. 5 1. 9 Fe II p 3.94 89

3430.293r 19 5. 4 NH P 20 0,0 6

3430.410r 22 6. 4 NH P 20 0,0 6

3430.536r 49 14. 3 Zr II 0.47 11

3430.642r 5. 5 1. 6

3430. 735r 5 1. 5 Ru I 0.34 3

3430.885r 1. 5 0. 4 Fe I p 3.27 614

3430.955r 8 2. 3

3431.072r 3 0. 9 343L185r 8 2. 3

3431.288r 20 5. 8 Cri 2.54 53

3431. 455r 21 6. 3

3431.586r 106 30. 9 Co I 0.10 6

3431.695r 13 3. 9 Cri 2.54 53

53
The Solar Spectrum—Continued

Wave-

(A)

Equivalent Width

A\

(mA)

Re- duced

Width

AX/X

\F)

Spot

Solar

fication

Low

E P

or Rot. Line

RMT

No.

Vib. Band

Notes Wave-

\A)

Equivalent Width

AX

\mA)

Re- duced

Width

AX/X

vF;

Solar

fication

Low

E P

or Rot. Line

RMT

No.

or Vib.

S-JCillil

iNotes

3431.830r 90 26. 2 Fe I /2.83

13.30 376

676 3435.826r 39 11. 3 Cr I /2.54

12.54 53

53

3431. 942r 8 2. 5 NH P 17 1,1 6 3436.038r 40 11. 8 Fe I 3.27 614

3432.022r 47 13. 7 Fe I 2.86 377 3436.1 14r 15 5. 9 Fe II 3.97 91

3432. 135r

3432.215r

3432.312r

18

7. 5

38

5. 1

2. 2

11. 1

NH

ICr I Co I

P 17

2.54

2.08

1,1

53

102

6 3436.196r

3436 336r

3436. 416r

80

9

16

23. 3

2. 6

4. 6

Cri /2.54

\2.54 5252

19 5. 5 Zr II 0.93 58 3436. 530r 7. 5 2. 3

3432.572r 13 3. 8 3436.650r 6 1. 7

3432. 728r 42 12. 5 Nb II 2.01 3436.746r 13 3. 8 Ru I 0.15 4

3432. 888r 15 4. 7 3436.840r 15 4. 4

3433.048

3433. 155r

3433. 3 18r

3433. 455r

3433.579r

111

4

80

12

492

40. 9

1. 6

33. 8

12. 2

143

Co I

Cr II PdiIINiiCr I

0.63

2.43

1.45

0.03 2.54

23

3

11

19 52

7 3436.980r

3437 0.'>4r

3437. 146r

3437.291r

3437.480r

6. 5

126

22

184

34

2. 3

36. 4

12. 8

53. 6

10. 5

Co I?-

NH

Fe I

Zr II Ni I

3.13 P22

3.05

0.71

0.00

0,0

539

33

3

6

3433.769r

3433.917r

3433.981r

3434.047r

3434.123r

3434.247r

3434.376r

3434.490r

3434.610r

3434.693r

3434.826r

3434.896r

0*100. iour

0^00.^^or

26

6. 5

4. 5

64

25

13

11

3. 5

2. 5

1. 5

8. 5

13

It:

9

0. 0

15. 1

2. 6

1. 7

21. 4

10. 5

4. 1

3. 3

1. 0

0. 7

0. 6

2. 5

3. 6

4 1

u. 0

n Q

1. u

NH

NH

Zr II

Fe I Cr I

Dy II

Rh I Fe I

Fp t?

P21

P21

1.00

2.76

2.54

0.00

0.00

3.55

0,0

0,0 58

300

52

2

776

66 3437.636r

3437.693r

3437. 790r

3437.876r

3437.958r

3438. lOOr

3438.240r

3438.319r

3438.420r

3438.503r

3438.715r

3438.956r

3439.035r

3439. 132r

3439.229r

3439.342r

49

20

7. 5

9

61

22

1 132

13

23

27

1 140

7. 5

10

12

14. 2

7. 8

2. 2

2. 6

17. 9

6. 4

f 23. 0

1 22. 7

4. 2

6. 7

8. 1

1 27. 0

1 18.9

2. 3

3. 5

3. 8

Fe I Co I

Fe I Fe I p

Zr II Fe I

Co 1 Mn n

Fe I

Gd n

Ti IAl I

2.43

3.25

3.27

2.73

0.09

2.04

1.17

2.73

0.38

1.46 0.00

187

162

614

300

1

87

1

299

23

120

2

3435.373r 4. 5 1. 3 V II 2.56 133 3439. 499r 5 1. 7 NH P 19 1,1 6

3435.492r 29 8. 4 Ni I 1.68 53 3439.599r 8 2. 9 NH P 19 1,1 6

3435.593r 14 4. 4 3439.705r 9 3. 6

3435.683r 29 8. 4 Cr I 2.54 52 3439.805r 66 26. 4 Gd II 0.42 22

54
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3439.872r 13 6. 7 Fe I 3444.081r 5. 5 3. 2

3440.002r

3440.099r

7. 5

25

5. 4

22. 1

Gd II 0.24 7 3444. 266r

3444.331r

1

[ 148

1 22. 9

1 37. 2

Nil

Ti II

3.74

0.15

122

6

3440. 192r 26 31. 0 3444.454r 5. 5 3. 0

3440.369r 10 32. 2 NH P 23 0,0 6 3444.518r 38 1.3. 2 Fe 1

3440.499r 8 33. 2 -Sm ri? 0.66 54 3444. 638r 4. 5 1. 5

3440.626r 1243 361 Fe I 0.00 6 3444.71 Ir 16 5. 4

3440.739r 11 40. 1 Fe I p 2.76 301 3444.894r 11 3. 5 All? 0.00 2

3441.019r 634 322 Fe I 0.05 6 3445.125r 137 41. 9 -Fe I 2.20 81

3441. 112r 16 53. 5 Cn 2.54 52 3445.342r 11 3. 5 Fe I

3441.255r 14 15. 1 3445.462r 17 5. 4

3441.452r

3441.552r

3441.672r

3441.739r

3441.899r

3441.982r

3442.052r

3442. 148r

3442.232r

40

6. 5

4

9

14

329

9

34

13

20. 6

3. 5

2. 0

4. 8

11. 9

107

10. 8

20. 5

6. 2

Cri

Mn II Nil

Fe II

/2.54

\2.54

1.78

3.42

3.97

52

52

3

104

89

3445. 606r

3445.770r

3445.812r

3445.992r

3446. 105r

3446. 179r

3446. 271r

3446. 401r

66

66

8

2. 5

29

6. 5 470

19

20. 2

21. 0

2. 9

1. 2

15. 8

4. 9

136

13. 3

Cri

(Dy II) Fe I

Co I

Ni I

|Co II Ki

/2.54

12.54 0.00

3.21

0.11

2.24 0.00

51

51

162

20

2

4

3442.367r 70 27. 0 Fei 2.28 134 3446.485r 6 2. 9

3442.560r 36 12. 9 Ni I 3.70 124 3446.612r 3 1. 0 Til 1.88 168

3442.677r 85 27. 8 Fe I 0.96 26 3446.722r 12 4. 9

3442.785r 5. 5 1. 9 Fe II p 3.89 76 3446.796r 65 20. 8 Fe 1 2.61 244

3442.923r

3442.965r j 131

f 35. 4

1 19. 5

Co I Fe I

0.17

/3.07

13.55

6 499

776

3446.954r

3447.019r

77

34

23. 8

24. 3

Fe I Cri1.01

2.54

26

52

3443.045r

3443.194r

3443.299r

20

42

8. 5

8. 4

14. 4

3. 8

Co I -NH P 20 1,1 6

3447. 155r

3447.285r

3447. 434r

9. 5

100

48

2. 9

29. 8

14. 0

NH

Fe I Cr I (Ki)

P 21

2.20

2.54

0.00

1,1

82

52

4

6

3443.381r 60 21. 2 Ti II 2.05 99 3447.539r 8. 5 2. 5

3443.439r 9 4. 6 Co I? 3.05 3447.639r 16 4. 6

3443. 555r 15 11. 4 Zr II 0.97 73 3447.766r 45 13. 0 Cn 2.54 52

3443. 655r

3443.772r

3443.884r

3443.991r

141

28

655

8. 5

59. 0

31. 1

190

13. 1

Co I (Al i) Cri

Fe r

0.51

0.01

2.97

0.09

22

2

110

6

3447.905r

3448.009r

3448.092r

3448.205r

11

66

9. 5

44

3. 2

19. 1

5. 8

12. 8

Fei

Fei 2.40 186

55
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3448.359r 29 8. 4 Co I 3.25 163

3448.462r 27 7. 8 Fe II- Fei3.97

3.02 90

444

3448.592r 23 6. 7 Fe I

3448.692r 14 4. 1

3448.791r 1

[ 88

f 13. 6 IIFeiYii

2.83

0.41 37217

3448.868r J I 13. 6 Fe I 2.56 242

3448.964r 20 6. 6 In 0.50 1

3449. 051r 21 6. 8 Fe I p 2.95 442

3449. 175r 115 33. 3 Co I 0.58 22

3449.311r 12 3. 9

3449.448r 138 40. 0 Co I 0.43 22

3449.63 Ir 11 3. 3 Gd 11? 0.03 7

3449.698r 14 4. 2 Co I? 3.30 160

3449.861r 23 6. 7 Til 0.82 46

3449.988r 26 7. 4

3450. 140r 25 7. 3 Fe I p 2.59 242

3450.238r 5 1. 7

3450.334r 97 28. 4 Fe I 2.22 82

3450.454r 12 3. 8

3450.607r 5 1. 4 Mn I 4.27

3450.747r 7 2. 0 Fe I Ti r 0.81 46

3450.860r 9. 5 2. 8 Cr II? 4.29 60

3450.994r 8. 5 2. 5 NH P 22 1,1 6

345].120r 18 5. 2 NH- P22 1,1 6

3451. 234r 13 3. 8 Gd ir Fe II? 0.38

6.81 22 208

3451. 342r 37 10. 7 Fe II? 6.81

3451.474r 38 10. 9

3451. 626r 72 20. 7 |Fei

Fe I p

2.42

2.56 139 241

3451.780r 8 2. 6 Fei

3451.922r 110 31. 8 Fei 2.22 81

3452.284r 151 43. 7 Fe I 0.96 25

3452.475r 68 20. 5 Ti II 2.05 99

3452.628r 19 6. 2

3452.785r 15 6. 5

3452.905r 247 73. 1 Nix 0.11 17

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3453. 035r 50 26. 8 Fe I 2.76 301

3453. 121r 17 6. 7 V II 2.56 132

3453. 221r 3. 5 1. 3 Cr I 3.85

3453. 335r 24 10. 3 Cr I 2.54 52

3453.512a 310 87. 9 Co I 0.43 22

3453. 751r 20 7. 5 Cr I 2.54 52

3453. 848r 9 2. 9

3454. 169r 59 17. 5 Ni 11 2.95 1

3454. 321r 24 7. 0 Dy II

3454. 468r 5 1. 4

3454. 591r 9. 5 2. 9 Zr II 0.93 59

3454. 695r 6 1. 7

3454.800r 3 0. 9

3454.924r 8. 5 2. 6 Gd II 0.03 7

3454.987r 39 11. 3 Cr II 4.94 136

3455.070r 14 4. 3 NH P 23 1,1 6

3455. 245r 114 33. 0 II Co I Cn

0.22

2.54

651

3455.360r 30 9. 3 Fei?

3455.467r 16 4. 6

3455.602r 44 12. 9 Cn /2.54

12.54 5151

3455. 694r 11 3. 5 Fe I?

3455. 794r 12 3. 4 Ti I- 0.82 46

3455. 947r 14 4. 3

3456. 014r 40 11. 7 Fe II p 1.67 4

3456. 094r 20 6. 1

3456. 249r 62 18. 7 Fe I

3456. 394r 115 33. 3 Ti II 2.06 99

3456. 500r 15 5. 6

3456.580r 13 3. 9 Dy II

3456.667r 44 12. 7 Til 1.50 134

3456.810r 19 5. 5

3456.934r 64 18. 5 Fe II Co I 3.90

0.10 76

5

3457.096r

3457.147r 1 92

f 25. 5

1 2. 0

Fe I Vii

13.60 2.60

o / 4 835

147

3457.280r 9 2. 9 Til 0.83 46

3457. 404r 10 3. 2
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Hot. Line

RMT

No.

or

Vib. Band

Notes

3457.514r 15 2. 0 Fei 2.45 187 3462.213r 11 4. 0 Tm ir 0.00

3457.574r 56 17. 5 Zrii 0.56 20 3462.358r 66 21. 8 Fei 2.20 79

3457.624r 12 4. 6 Cr II 4.94 135 3462.533r 6. 5 2. 2

3457.774r 3 0. 9 3462.733r 32 17. 5 Cr n 2.42 2

3457.894r

3458.010r

3458. 120r

3458.308r

3458.467r

3458.594r

3458.700r

3458.940r

3459.060r

3459.154r

3459.280r

22

8. 5

30

52

656

32

18

14

5. 5

12

35

7. 5

4. 0

13. 0

37. 0

189

37. 6

9. 8

5. 1

2. 0

4. 0

11. 3

Fei—

Til

|Cr T Fe II? p

Fei

Nil

Zrn

NH

Cr II Fe I p

0.84

3.85

1.96

2.42

0.21

0.96 P 24

4.92

3.28

46

253

10

139

19

58

1,1

136 576

6

3462.816r

3463.019r

3463.189r

3463.310r

3463.386r

3463,526r

3463.643r

3463.803r

3463.979r

3464.033r

3464.141r

126

33

23

70

14

13

16

25

59

19

65

38. 4

10. 1

7. 1

20. 8

4. 9

3. 9

4. 8

7. 2

17. 3

7. 4

18. 8

Fe I |Coi

Zr II NHTi I Fe I

Co I Mn I

Fe II Cr II Fei

2.83 0.63

1.49 P 25

1.05

1.48

1.78

4.68

1.67

2.43

373

23

90

1,1 85

48

42

4

2

6

3459.434r 81 24. 2 Fei 2.69 297 3464.31 a 10 2. 9

3459.580r

3459.627r

3459.747r

3459.918r

11

13

70

159

3. 3

3. 8

21. 2

53. 8

Fe I p

Fei

Fe IFe I p

3.28

3.02

2.28

577

501

133

3464.474r

3464.709r

3464.836r

3464.918r

63

10

6. 5

44

18. 2

3. 0

2. 0

13. 0

Sr II (Fe 11)

Cr I Fei

3.04

4.15

2.54

2.59

4 114

51

241

3460.040r 100 36. 7 Mn II— 1.17 1 3465.033r 7. 5 2. 3

3460. 160r 24 9. 0 3465.166r 5 1. 4 Mn I?

3460.326r 181 53. 3 Mn II 1.81 3 3465.256r 21 6. 9 Cr I 2.54 51

3460.434r 44 18. 3 Cri- 3.01 141 3465.333r 2 0. 9

3460. 557r

3460.607r

3460.740r

I 32

J 34

f 5. 5

1 5. 5

10. 8

NH?

Coi-

|Pdi

P 29

0.92

0.81

0,0

35

2

6

3465.439r

3465.553r

3465.645r

3. 5

56

. 23

1. 2

22. 2

16. 9

Ti 11 Cr I Ni II

2.06

2.54

3.07

99

51

4

3460.887r 20 7. 1 3465.766r 69 84. 2 Co I 0.00 5

3460.977r 35 12. 4 Dy 11 0.00 3465.880r 544 158 Fe I 0.11 6

3461. 187r 91 32. 9 Co I 3.17 162 3466.002r 24 22. 5

3461.279r 12 7. 1 Cni? 4.94 148 3466.052r 7 4. 9

3461.499r 120 74. 8 Tin 0.13 6 3466. 185r 18 8. 2

3461 fifiTr 1 00 91^ J. Qi7 u.uo 17 36 13. 7 Fe I 2.40 185

3461.796r 32 30. 9 3466.372r 5. 5 2. 0

3461.939r 22 12. 4 3466.504r 74 23. 4 Fei 0.86 24

3462.083r 4 1. 6 Rh I?- 0.32 3 3466.638r 52 15. 9

57
The Solar Spectrum—Continued

WaVG- length

(A)

EquiV d/iKZLl \j Width

AX

(mi)

Re- duccd

Width

AX/X

(F)

Spot Identification

Low

V P

or Rot. Line

RMT

or Vib. BandNotes

VV HVtJ- length

(A)

Equi-

^rsi V cLlK^LL 1 ATrfu Width

AX

(mi)

Re- Width

AX/X

(F)

Spot

ouiax Identification

Low

Hi t or Rot. Line

RMT

IN O. or

Vib. Band

Notes

3466.718r 15 4. 6 347l.000r 2 0. 6

3466.898r

3467.018r

70

21

20. 3

6. 0

Fe I Cn /3.01

\3.85 141 253

3471. 120r

3471.268r

7. 5 2. 3

f 26. 8

Zr II Zr I Fe I1.74 0.00

2.22

114

15

82

3467. 135r

3467.272r

22

29

6. 3

8. 4

Nil

Ti I

3.77

1.05

123

84

3471. 363r 169

J [ 33. 2 re I (Co I) (Ni II)

2.28

3.17

3.08

130

161

4

3467. 382r 10 2. 9 -NH P26 1,1 8 3471.462r 29 12. 1 Cr I 2.71 77

3467.509r 96 27. 7 Nil 0.17 3 3471.614r 14 4. 5 Ni I p 3.70 124

3467.7 lOr 70 20. 2 Cr I Ni I 2.98

3.74 110

123 3471.720r 7. 5 2. 3

3467.872r 18 5. 2 Y II 0.41 17 3471.774r 12 3. 7 NH P27 1,1 6

3468.02 a 5 1. 4 3471.899r 36 IL 4 Fe I

3468.075r 22 6. 3 3472.054r 37 11. 5 Cr II 4.92 135

3468. 212r 13 3. 7 3472. 180r 43 14. 8

3468.351r 7. 5 2. 3 3472.307r 32 14. 0 -Fe I

3468.477r 40 11. 5 Ca I 1.88 10

3472. 457r 16 16. 8 — Lu II 1.54 4

3468.686r 66 19. 0 Fe n 4.15 114 3472.558 374 136 Ni I 0.11 20 7

3468.851r 75 21. 8 Fe I 2.56 242 3472.714r 7. 5 4. 9 Coi- 3.17 160

3468.979r 1 r 4. 9 Co I 3.28 159 3472.780r 11 4. 5 Cn 2.71 77

3469.020r 1 20. 6 Fe I 3.30 614 3472.904r 9. 5 3. 3 |Cr I Fe II? 2.97 4.74 111 156 3469.16 a 11 3. 2 3473.010r 9. 5 3. 2 Fei 3.26 576

3469.26 a 18 5. 6 Fe I 2.56 3473.054r 3. 5 1. 2 3469.397r

3469.493r

19

180

8. 8

52. 2

Fe I Ni I (Vii)

2.84

0.27

2.27

375

858

3473.227r

3473.299r

3

61

1. 1

18. 5

Gd II Fe I p

Fe I

0.03

3.21

3.05

7 576

3469.601r 26 9. 9 Cri- /2.71

13.01 77

141 3473.501r 62 18. 5 Fe I 0.99 26

3469.691r

o^ucf .oo 1 r

3469. 941r

10

ou

7. 5

3. 0

1 7 Q

2. 1

|Fei

Co I?

J; 1

Zr II

2.70

1.00

137

9J.9

59

3473.620r

3473.686r

3473.81 3r

10

54

6

3. 7

16. 1

2.0

Cr I Fe I2.71 77

3470.02lr 3 0. 8 Mn I 4.68 3473.969r 27 11. 2

}

f Co I ro.oo \0.58

423

3470.141r 1. 5 0. 5 3474.060r 203 59. 2 1 Mn II 1.81 3

3470.244r

3470.400r

3470.542r

3470.640r

3470.740r

3470.864r

5. 5

17

25

11

15

1

1. 5

5. 0

7. 2

3. 0

4. 3

0. 3

Fe II-

|V II Cr I Cr I Rh I? Cr I

3.97 2.27

2.71

2.71

0.43

2.71

89

58

77

77

3

77

3474.150r

3474.273r

3474.386r

3474.439r

3474.532r

3474.663r

3474.767r

78

5. 5

4. 5

79

19

3. 5

30

46. 7

2. 0

2. 4

23. 8

7. 4

1. 1

10. 7

Mn 11

Cr I? Fe I Co I

Ca I

1.83

0.58

1.89

3

24

10

58
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(D

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelen gth

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3474.886r

3475.006r

3475.133r

3475.269r

3475.319r

3475.457r

13

1

49

23

8. 5

622

4. 8

0. 3

22. 9

16. 0

13. 6

179

Cr I Sr n

Cr II Fe II p

Fe I

3.01 3.04

2.43

1.69

0.09

141

4

2

4

6

3478.915r

3479.025r

3479.135r

3479.263r

3479.393r

3479.565r

10

28

7

45

50

14

3. 1

8. 2

2. 1

12. 9

14. 2

4. 0

Til

Zr II Cri

Nil

Zr II Co I? Nb II

1.05

0.53

3.01

3.48

0.71

1.78

1.31

84

20

14]

105

46

6

3475.519r

3475.665r

3475.757r

3475.873r

22

112

34

30

74. 0

56. 0

28. 2

12. 3

Fe I Fe II p

Fe I

2.18

1.67

/2.43

12.84

78

4

186 373

3479.691r

3479.831r

3479.923r

3480.033r

48

31

78

25

13. 8

10. 9

22. 3

7. 2

Fe I

Vii

Fe 11 Co I

/2.95

13.57

1.07

1.69

1.88

443

812

6

4

67

3476.026r

3476. 193r

3476.342r

6

8. 5

59

2. 2

3. 2

22. 6

Co I? NH

Fe I

1.74 P 28

/2.28

\3.60

1,1

133 835

6

3480.177r

3480.304r

3480.338r

62

1 82

17. 8

f 0.

I 23. 6

Ni I Cn

Fe I

/3.61

13.77

3.01

123 124

141

3476.453r 4 2. 3 Til 1.07 85 3480.411r 12 4. 0 Zr II 0.93 58

3476.619r 17 17. 9 Nil 3.70 123 3480.531r 58 16. 7 Til 1.07 84

3476.7 12r 465 136 Fe I 0.12 6 3480. 647r 19 5. 2

3476.865r

3476.988r

46

74

38. 4

35. 4

Fe I (Ce II)

Ti II- Fei

2.59

1.32

0.15

2.42

242

132

6 139

3480.737r

3480.886r

3481.057r

9

75

25

2. 9 2L 5

7. 8

Ti II 1.08 22

3477.186r 102 26. 8 Ti II 0.12 6 3481. 164r 74 21. 5 Zr II 0.80 46

3477.363r 9. 5 3. 2 3481.301r 53 15. 2 Cri 2.71 77

3477.499r 16 4. 9 Vii 2.27 58 3481.451r 15 4. 3 Zr II? 0.96 59

3477.633r

3477.719r

3477.865r

3477.985r

40

7. 5

88

17

12. 1

2. 2

26. 8

5. 0

IFei

Ni I Fe I p

2.22

3.61

3.65

82

124

836

3481. 557r

3481.664r

3481.751r

3481.814r

70

13

1 78

20. 2

4. 6

f 7. 2

1 17.8

Fe 1 Cri

Ti I?

Gd II

2.28 3.00

2.49

0.49

132 110

271

22

3478. 118r 5 1. 5 3481.937r . 31 8. 9 Fe II p 4.07 102

3478. 178r 10 2. 9 3482.057r 23 6. 6 Fe II? p 2.03 10

3478.300r

3478.366r

3478.551r

1 88

45

r 13.

8

i 15. 3

18. 1

Zr II-

|Nii

Fe I Co I Fe I

0.09 3.70

2.43

2.28

2 173

185

120

3482.187r

3482.22 a

3482.30 a

3482.451r

63

1 37

18. 1

1

2.

0

I 1.7

10. 6

Fe I

Fe I Fe II

3478.738r 10 3. 6 Co I 1.88 67 3482.574r 50 14. 7 Cr II 5.67 184

3478.785r 55 15. 7 Cri

IIFei 3.01 2.42 141 137

3482.7l7r

3482.909r

52

153

14. 9

43. 9

Nil

Mn II

3.61

1.83

120

3

59
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

valent duccd Solar E P No. ^Vave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/\ fipfitinn Rot. Vib. AX AX/X fication Rot. Vib.

(A) (luA) (F) Line Band (A) (mA) (F) Line Band

3483. 017r 109 44. 4 Fe I 0.91 24 3487.276r 8. 5 2. 4

3483. 157r 26 7. 5 Co 1? 2.28 3487.403r 13 3. 7

3483. 414r 114 35. 1 Co I 0.51 23 3487. 604r 64 18. 2 Ca I 1.90 10

3483. 528r 43 13. 2 Fe I? — 3487.718r 31 9. 0 Co I 1.88 65

II Zr II 0.76 33

3487. 820r 20 5. 7 3483. 630r 14 5. 3 Ni I p 3.70 120

3487.992r 65 18. 6 Fe II 1.69 4 3483.784r 198 56. 8 Ni I 0.27 6 3488.150r 19 5. 6 3483.884r 35 13. 4 Fe I 3488.298r 46 13. 2 Ni I 3.61 121 3484.033r 13 4. 0 3488.450r 36 10. 5 Cr I 2.97 109

3484. 156r 87 25. 0 Cr II 2.45 2 3488.563r 17 5. 2 Ce II? 0.87 187

3484.213r 22 6. 3 3488.678r 126 36. 0 Mn II 1.85 3 3484. 343r 32 9. 5 Fe II 4.15 115

3488.826r 66 19. 5 Fe I 3484. 553r 27 7. 8 Fe I? 3489.003r 52 16. 5 3484. 670r 27 8. 9 V II? 1.10 6 3489.163r 98 28. 9 Fe II p 4.07 102

3484. 783r 35 10. 0 3489 43 14. 3 3484.856r 63 18. 1 Fe I 2.45 185 548Q 407r 135 40. 2 Co I 0.92 36

3484.982r 110 31. 5 Fe I — 2.42 138

(Ce II) 0.00 44 3489. 674r 1 f 24. 6 Fe I 2.95 442

[ 130

3485. llOr 100 29. 2 Ni I 3.70 118 3489.750r J [ 18. 3 Ti 11 0.13 6

3485.230r 21 6. 0 3489.909r 8 2. 9

3485.354r 150 45. 8 |Fe I- 2.20 78 3489.965r 3. 5 1. 3 V II 2.56 131 Co I 3.12 162 34Q0 052r 4 1. 6 Fe I? p 2.87 331

3485.506r 22 6. 3 3490. 162r 20 9. 2 3485. 580r 22 6. 3 3490.202r 5. 5 3. 2 3485.706r 60 17. 2 Co I 1.96 68

Ti I 1.05 84 3490.302r 5 3. 6

3485.902r 122 35. 8 IINii 0.21 17 3490.395r 11 10. 8 V II 1.10 6 3490.489r 10 17. 3 Fe I p 3.60 835

3486.040r 18 5. 2 3490.594r 830 238 Fe I 0.05 6

3486. 143r 35 10. 3 Fe I 3490.757r 34 26. 4 Co I 0.51 20

3486.223r 16 4. 9 CFe I dI 2.28 133

3486. 336r 1 f 4 0 12 7. 2 66

3486. 383r J [ 16. 1 104 39. 5 Ti II 0.11 6

3486. 552r 64 18. 3 Fe I 2.22 79 22 8. 4

3486.643r 13 4. 0 3491.323r 76 26. 6 Coi— 0.22 6

3486. 750r 11 3. 2 9 3. 0

d486.823r 8 2. 3 3491. 755r 20 6. 6 Fe I?

3486.956r f 7. 2 3491.882r 10 3. 3

3487.006r 1 5. 4 3491.973r 34 IL 5 Co I 3.25 159

3487. 150r 13 3. 7 Fe I? 4.14 3492.035r 8. 5 3. 0

60
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3492. 145r 11 3. 9

3492.229r 35 12. 5

3492.369r 60 21. 5

3492.539r 28 12. 9

3492.719r 10 7. 0

3492.815r 23 20. 2

3492.975r 826 239 Nil 0.11 18

3493.089r 11 15. 6

3493.174r 21 14. 9 Vii 1.07 6

3493.291r 47 23. 8 Fe I 1.48 48

3493.479r 38 15. 2 Fe n 4.15 114

3493.582r 28 10. 6 Fe I p 2.83 327

3493.695r 53 18. 6 Fe I 2.73 297

3493.865r 21 7. 2 Fe I?

3494.015r 8. 5 2. 7

3494. 169r 53 16. 3 Fei 2.42 137

3494.262r 7 2. 1 Fe I p 2.43 185

3494.359r 10 3. 0

3494.412r 13 3. 7 Gd II 0.08 7

3494.515r 46 13. 2 |Cr II Dy II 2.48

0.10

2

3494.676r

3494.732r

[ 94

f 26. 6

1 0. 9

Fe II Nil2.28

3.80

16

154

3494.855r 14 4. 0

3494.969r 33 9. 5 Cn 2.98 109

3495.039r 6. 5 2. 0

3495.12 a 11 3. 0

3495.245r

3495.284r

\ 116

f 5.7

I 30. 8 Fe I 2.56 238

3495.383r 61 20. 0 Cr II 2.45 2

3495.519r 30 8. 6 Cr II 4.94

3495.663r

3495.714r

] 138

1 26. 9

1 20. 0

Co I (Fe II) -Til0.63

4.15

1.05

22

11584

3495.835r

3495.885r

i 141

1

f 24. 3

1 24. 3

Mn II Fei1.85 3

3495.962r 10 3. 7

3496.085r 48 13. 7 Yii 0.00 3

Wavelength

(1)

Equivalent Width

AX

(in A)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Lino

RMT

No.

or Vib. Band

Notes

3496. 209r 96 28. 0 Fe I Zr II 2.45 0.04 186

1

3496.352r 64 19. 0 Nil 3.61 118

3496.475r 14 4. 1

3496. 582r 49 17. 1 Fe I p 3.21 .572

3496.681r 101 30. 3 Co I 0.51 19

3496.813r 77 24. 1 Mn n

(Co I) 1.83 3.12

3 161

3497.009r 62 32. 3 -Vii 2.60 146

3497. 102r

3497. 162r

\ 166

f 34. 0

)

I 30.6

Fe I Fe I

2.18

2.20

78

78

3497.282r 8. 5 3. 3 Co II

3497.395r 31 12. 4

3497.529r 59 25. 9 Mn II 1.85 3

3497.735r 12 12. 3 Fe II p — 4.15 114

3497.843r 726 205 Fe I (Feip)

0.11 3.02 6 499

3497.977r 12 9. 4

3498. 183r 49 22. 3 Fe I p—

Ni I p

2.81 0.00 326

2

3498.312r 15 6. 1

3498.395r 11 4. 1

3498.529r 20 7. 0

3498.749r 42 13. 4 Fei 2.85 330

3498.945r 31 9. 7 Ru I 0.00 4

3499. 109r 31 9. 4 Til 1.07 84

3499.269r 21 6. 6 Fe I

3499.353r 23 6. 7

3499. 469r 2 0. 6

3499.572r 26 7. 3 Zr II 0.41 9

3499.709r 5 1. 4

3499.835r

3499.874r

\ 44

r 0.

3

1 12. 5

Vii

Fe II

1.07

4.15

5

115

3499.992r 21 6. 0

3500. 157r 39 n. 1 Fe I 2.87 327

3500. 335r 90 25. 6 Ti II 0.12 6

3500.438r 7 2. 1

3500.567r 86 24. 6 Fei 2.59 238

3500.691r 16 5. 1

61
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib. (A) (ml) (F) Line Band (1) (ml) (F) Line Band

o5UU.oo7r 4d. D IM I U.l / 0 3505. 232r 24 8. 3 Hf II

1 Ay* 1.U4 7

i

ooUU.yoor A4

1i. o 3505. 294r 92 26. 2

ooUl.U/ ir 1I 21

( OA 3505. 386r A C 9. 5 3. 0

21 ooUl.io/r J O A

[ z. y 3505. 489r 51 14. 5 Zr II

1 CO 1.53 AA90

(Gd ii) 0.49 OO ooUl.^oor n

I O A z. u 3505.67 Ir o3 15. 1 Zr II A 1 A -Ii ooUl.ooor 10 O A ZiF 1

1

0.0/ 14 3505.789r 9. 5 2. 7

i>oU1.4DDr 1 o o. 4 v^e 11 o o*3 U.-iO R7D« 3505. 899r OO6o 11. 0 ii II

1 CA CQOO

ooUl.oYlr 1 Q13 o. / 3506. 050r OO

8. 0 Zr II 1.Z4 84

ooUl. /Uzr 1 lo. 1 84 3506. 241r A C 45 24. 0 Fei O Q7 Q07 oZi ooU1.729r J t lo. 1 L 0 II o 3506. 328r 1 >1 A 14U 40. 0 L-o I A 1 0

1

ooUl.oolr 1 c 4. O 3506. 506r 1 OO

37. 6 J^e I O OQ 1 QA

ooOLybor 1 o C 1 o. 1 MrMo II o. /4 3506. 594r

I 71

1 31. 4 Fe I p

O CQ Q07

O C AO AOCi* oO

O A

Z. 4 71

3506. 654r J t 1. 0 ll I U.Oo zz

o cAo 1 r\ ^ lb 4. D 3506. 752r 14 4. 4

O CAO OA "t 111 111 Ol. D LyO I U.4o Ol 3506. 841r 4o 13. 8 Dy II — A 1 A 0. lU 3502. 469r 61 1 A ^7 10. 7 r e I p 3.24 07d

3506.938r lo 4. 4 lie I o mo cf\o_ 3502. 59Sr

1 111

JNl I 0.00 3 jiii 3507. 145r 1 18. 8 J^e I O.DO

3502. 636r [ 21. 2 Co I 0.17 6 94

3507.211r J 1 11.1 3502.760r 12 3. 6 35O7.308r 10 3. 0 Rhi 0.32 2 3502.862r 28 8. 0 Fe I 3.26 577

3507.404r 50 14. 3 |Fe II 2.34 16 3502.973r 9 2.5 Coi? 2.63 135 Fe I 3.07 500

3503. 117r 16 4. 6 3507.548r 13 3. 7 Vii 2.76 159

3503.303r 7. 5 2. 1 3507.698r 80 23. 1 Nil 0.17 3

3503. 473r 50 14. 3 Fe II 1.72 4 3507.818r 17 4. 8 Co II

3503. 560r 6 1. 7 3507.951r 19 5. 6 Ce II- 0.17 51

3503. 727r 22 6. 3 Lo I 2.14 88 3508. 095r 11 3. 2 Or I.'

3503.909r 13 3. 7 3508.211r 48 13. 4 Fe II 1.72 4

3504. 053r 3 0. 9 3508. 348r 11 3. 3

3504. 193r 3. 5 1. 0 3508. 487r [ 22. 0 I'e I O AA 2.99 /i /I o

\ 105

j 3504. 260r 6 1. 7 3508.531r J [ 13. 4 Fe I 2.56 OO A

3504.442r 65 18. 5 1 \ II 1.10 6 3508.708r 23 6. 7 Fe I 2.83 371

3508.898r 21 6. 0 3504.594r 15 4. 3 3509.018r 14 4. 2 Vii 2.52 117 3504.684r 70 20. 0

oy 1 Q R PelT 326

3504.892 132 37. 6 Fe I 2.28 131 7

|Ti II 1.89 88 3509. 331r 18 5. 4 Zr I 0.07 15

3505.063r 94 26. 8 Fe I 3.02 498 3509.43 Ir 14 3. 9

3505. 149r 7 2. 4 Coi 3.12 160 3509.551r 16 4. 9

62
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3509.731r 41 13. 4 Fe I 2.88 327 3514.33 a 12 4. 1

3509.853r 105 33. 9 IICoiFe I (Ti II)

0.58

2.22

1.89

22

78

88

3514.468r

3514. 635r

47

56

15. 9

21. 9

Fe ip

Fe I

1.48

2.40

47

183

3510.070r 7. 5 3. 2 3515.066r 718 202 Ni I 0.11 19

3510.192r 22 13. 1 Fe I p 3.69 836 3515.409r 18 8. 3 Fe I 2.61 243

3510.327r 489 140 Nil 0.21 18 3515.535r 17 6. 8 Fe I

3510.457r 25 22. 5 Fe I Co I (Zr II)

2.48 0.10

0.56

139

620

3515.647r

3515.807r

4. 5

3

1. 5

1. 1 Fe II? 6.80 208

3510.554r 10 5.7 Cn 3.00 109 3515.881r 2 0. 6

3510.685r 33 13. 5 Fe I 3516.016r 7 2.3 Vii 1.13 6

3510.846r 87 29. 1 Ti II 1.89 88 3516.121r 4. 5 1. 3

3511.070r 10 3. 1 3516.219r 55 16. 8 Ni I 3.54 123

3511.217r U 3. 2 Sm II 0.10 12 3516.301r 6. 5 2. 3

3511.314r 9 2. 6 3516.414r 60 18. 2 Fe I 3.02 442

3511.444r 13 3. 6 3516.56 Ir 67 19. 9 Fe I 2.86 326

3511.537r 16 4. 6 Zr II? 1.83 124 3516.714r 9. 5 2. 9

3511.624r 31 8. 7 Nil 3.63 152 3516.819r 35 10. 5

3511.744r 41 13. 6 Fe I 2.56 238 3516.953r 22 6. 6 Pdi 0.96 1

3511.839r 90 26. 1 Cr II 2.48 2 3517.033r 16 4. 5 Ni I p 3.74 123

3511.927r 27 9. 4 Nil 3.74 124 3517. 170r 15 4. 2

3512.089r 71 20. 0 Fe I 2.85 327 3517.306r 79 22. 9 Vii 1.13 6

3512.230r 70 19. 8 Fe I 2.85 326 3517.383r 10 3. 5 Ce II 0.90 230

3512.381r 42 12. 1 3517.513r 16 4. 5 Co II- 2.24 1

3512.500r 9 2. 8 Gd II? 1.25 89 3517.720r 3 0. 9

3512.646r 132 37. 2 Co I 0.58 21 3517.820r 5. 5 1. 4

3512.730r 27 12. 7 Fe I p 3.27 613 3517.963r 8 2. 3

3512.811r 24 8. 2 Fe I p 2.86 330 3518.060r 7 2. 0

3512.960r 50 17. 7 Fe I 3.07 501 3518.220r 15 4. 2 Fe I p 3.24 575

3513.060r

3513.282r

3513.483r

3513.604r

3513.728r

3513. 825r

3513.942r

97

24

98

20

2. 5

307

}..

27. 7

7. 2

31. 8

9. 7

1. 8

87. 5

f 7. 7

|Cr II- Fe I

Co I Fe X p

Fe I

INii

Ni II

4.74

1.56

0.10

2.81

0.86

0.21 2.86

10748

5

327

24

17

1

3518.348r

3518.496r

3518.650r

3518.685r

3518.793r

3518.874r

3519.099r

3519.270a

93

12

1 96

6

67

18

3. 5

26. 3

3. 5

f 18.6

1 14. 2

2. 1

19. 1

5. 2

1. 0

Co I

Nil

Fei

Fe I Ce II?

1.05

3.54

2.87

2.20

0.33

36

124

327

78

92

3513.998r [ 5.

9

3519. 505r 3. 5 1. 0 Fe I

3514.242r 10 3. 3 Co II 2.27 1 3519.618r 7. 5 2. 6 Zri 0.00 13

63
The Solar Spectrum—Continued

WEve- length

a)

EquiWidth

Zi A (mA)

Re- Width

A A/ A (F)

Spot

oOlal Clnlar IdentiLow

F P

or nut. Line

RMT

or Vih V lU. Band

Notes

VV aVc- length

(A)

EquiWidth

A \ LA A (mA)

ReducGcl Width

A \ /\ (F)

Spot

ooiar

Identification

Low

or

XVOb. Line

RMT

iNNr.0. or

V lU. Band

Notes

171 IM 1 oo^t:.Uo ir uo 97 9 i; e 1 9 t^Q

OKI Q Qftlr V. 0 1 no Fo T 9 98 1XOXJ "in

3520.088r

I 114

1 19. 2

V TT V 11 Co I1 (17

0.10

r. 0

4 3524.536r 1271

9/t

363 Nil 0.03 18

3520.257r 75 22. 3 Till 2.05 98 3524. 742r 39 33. 3 Vii LIO 5

3520.391r 5. 5 1. 7 3524.922r 12 7. 6

3520.535r

3520.611r

3520.731r

3520.851r

13

4

4. 5

47

4. 1

1. 2

1. 4

16. 2

Ce 11-

Vii

|Fei

Zr II

0.17

2.27

2.61 0.56

55

57

238

19

3525. 130r

oD^D.^ 4 01

3525.388r

3525.515r

3525.618r

14A

2. 5

3. 5

30

6. 1

1. 0

1. 0

1. 3 n. 3 -Fe I

3520.978r

3521.065r

3521. 178r

3521.270r

3521.546r

3521. 608r

3521.748r

3

25

12

381

1 109

18

1. 2

10. 2

9. 3

110

1 17. 6

1 27. 1

6. 9

}

Fe I

Co I

Co I

0.91

0.43

/0.63

12.04

24

20

24

100

3525. 845r

3525.962r

3526.042r

00^ qcofi0. X

1 7nr / ur

3526.257r

3526.385r

3526.484r

75

13

84

4.99

23

108

67

32. 3

n. 6

62. 5

1 '^9

29. 2

49. 2

38. 2

Zr II-

|Fe I

Fe I

X c 1 Fe I Fe I Fe I

0.36

2.85

0.09 n Qfi

2.86

2.86

2.28

9 829

6 24

327

326

131

3521.844r

3522.044r

3522. 144r

3522.272r

3522.449r

3522.537r

3522.617r

3522.737r

3522. 834r

3522.908r

3523.072r

3523. 184r

3523.312r

3523. 444r

72

6. 5

7

61

21

5. 5

16

12

20

58

43

35

55

96

23. 4

2. 0

2. 2

19. 0

6. 4

2. 0

5. 2

3. 9

7. 3

18. 3

14. 2

11. 5

18. 4

30. 9

Vn

|Fei Fe II? p

Cr II? Fe I

Fe I p Co I Fe I Ni I Fe I p

Fe I

Ni I |O0 I

2.27

2.22

2.03

5.67

2.83

3.05

3.21

2.87

0.42

3.25

2.87

0.03

U. Do

57

78

10

184

326

538

159

330

34

673

326

16

3526.545r

3526.680r

3526.847r

3526.974r

3527. lllr

3527.227r

3527.317r

3527.447r

3527.531r

3527.609r

3527.795r QC97 00^ ( .yuui onnr

23

82

209

24

18

2. 5

17

8. 5

18

48

107

4.7

S7

1 9

18. 9

35. 8

63. 0

12. 6

5. 6

0. 6

5. 1

2. 5

6. 1

14. 1

31. 4

1X 7 1

i , 1

9'^ 1

1 4. 1

^ 4- 0. t;

Ni I Fe I Co I Fe I p Cr I

Zr II Nd II?

Fe I Fg I p

X>Nl1 XT

"Pp T Fp t?

3.65

2.87

0.00

3.65

3.98

1.76

2.85

2.76

0.17

2.45

1.56

155

326

4

835

274

103

326

296

6

182

3523.560r 21 8. 2 3528.41 Ir 11 3. 1

3523.710r 21 7. 5 Co I 1.88 66 3528.574r 7 1. 9 Osi 0.00 1

3523.784r 4 1. 5 3528.787r 3. 6 1. 0

3523.990r 4 6. 5 Dy II 0.54 3528. 894r 49 13. 5 Nil 3.65 154

64
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E F

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3529.040r 76 21. 7 Co I 0.17 5 3534.530r 44 12. 5 Fei 3.57 811

3529. 187r 8. 5 2. 3 3534.591r 8. 5 2. 8

3529.354r 12 3. 3 3534.688r 6. 5 1. 8

3529.521r 68 19. 2 Fe I 3.05 537 3534.778r 21 5. 9 Co I 2.28 118

3529.627r

3529.731r

3529.823r

25

46

148

8. 8

17. 8

42. 0

Ni I Vi

Fe I Co I

1.93

1.19

2.88

0.51

76

53

326

22

3534.918r

3534.948r

3535.038r

1 66

3. 5

1 18. 0

1 1.2

1. 0

Fe I Dy n

/1. 48

11.50 0.10

4848

3529.994r

3530. 122r

3530.232r

3530.391r

3530.592r

3530. 777r

3530.965r

3531. 105r

3531.282r

3531.440r

20

9

14

92

34

75

23

4. 5

7

60

5. 9

2. 5

3. 9

25. 9

9. 7

21. 3

6. 4

1. 3

1. 9

17. 1

Zr II

Zri

Fe I Nil

Vii

Fe I Cr I?

Fe I (Vii)

1.21

0.63

2.81

3.54

1.07

2.48

2.43 LIO

84

52

326

121

5

138

182

4

3535.158r

3535.304r

3535.412r

3535. 518r

3535.624r

3535.726r

3535.847r

3535.92 a

3536.023r

3536.117r

3

25

79

14

25

73

1. 5

4. 5

23

7. 5

1. 0

7. 7

22. 5

4. 2

8. 2

20. 7

0. 4

1. 3

6. 7

2. 2

Zn

Vii?p

Nb I?

Ti II Hf II Fe II

Sc 11

Co II Dy II

1.00

1.07

0.09

2.06

0.61

3.89

0.31

59

4

4

98

9

75

11

3531.619r 20 5. 6 3536.263r 4 1. 3

3531.709r 45 12. 5 Dy II 3536.567r 189 53. 6 Fei 2.87 326

3531.840r 68 19. 2 Mn I 2.28 18 3536.C90r 11 4. 3

3532.001r 81 24. 5 Mn I 2.28 18 3536.792r 39 11. 6

3532. 120r 101 28. 7 Mn I 2.28 18 3536.963r 36 10. 2 Zr II 0.36 10

3532.327r 45 12. 8 3537.123r 2. 5 0. 7

3532.459r 31 8. 7 3537.243r 40 11. 2 Cri /2.54

12.54 5050

3532.579r

3532.635r

3532.82 a

3532.899r

3533.014r

3533. 203r

3533.364r

3533.538r

3533.694r

76

50

7

12

97

223

72

6

21

21. 6

16. 8

2. 9

4. 5

31. 4

63. 2

26. 1

2. 1

6. 0

Fe IFe II

Cr I? Fe I Fe I Co I

|ViV I

4.48

3.37

2.88

2.88

0.22

1.22

1.18

132

326

326

5

53

53

3537.297r

3537.496r

3537.630r

3537.737r

3537.903r

3538.077r

3538.257r

3538.310r

3538.413r

1070

31

83

107

1640

60

8. 5

3. 1

19. 7

12. 3

23. 8

31. 3

4. 6

16. 5

16. 9

2. 5

Fe I Nil

Fe I Fei

Vii

Fe I

2.59

3.54

2.61

2.83

1.13

3.55

239

120

239

327

4

775

3533.858r 43 12. 3 Ti II 2.06 98 3538.501r 20 5. 6 Dy II 0.00

3534.064r 14 4. 1 Ce II 0.52 44 3538.559r 63 17. 8 Fe I 2.48 137

3534.258r 20 5. 6

65
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3538.690r 7. 5 2. 1 Fe I

3538.795r 29 8. 1 Fe I 3.57 811

3538.939r 13 3. 6

3539.076r 12 3. 4 Ce 11 0.32 118

3539.249r 2 0. 5

3539.371r 3 1. 0 Fe I

3539.446r 5. 5 1. 5

3539.542r 2. 5 0. 5 Fe II?

3539.629r 6 1. 8

3539.750r 7. 5 2. 3

3539.896r 23 6. 5

3539.956r 5 1. 5

3540.126r 93 26. 4 Fei 2.86 329

3540.322r 10 2. 8

3540.396r 9 2. 7

3540.502r 8 2. 3 -Vi? 1.06 45

3540.715r 95 26. 6 Fe I 0.91 23

3540.808r 43 15. 4 Fei

3540.966r 21 9. 1 Nb II 1.03 4

3541. 095r 214 60. 9 Fe I 2.85 326

3541. 242r 14 5. 8 Fe I p 1.48 47

3541.332r 16 5. 4 Vn 2.60 145

3541.545r 16 4. 6

3541.648r 14 4. 0

3541.875r 39 13. 2

3541.987r 21 13. 4

3542.090r 224 63. 7 Fez 2.86 326

3542.255r 47 17. 1 Fei 2.28 128

3542.331r 10 3. 6 Dy II

3542.441r 4 1. 5

3542.491r 6. 5 2. 0

3542.571r 60 17. 2 Fe I p 2.86 321

3542.633r 18 7. 2 Zr II 1.76 113

3542.768r 7. 5 2. 2

3542.948r 3 2. 3

3543.001r 16 4. 5 Co I 0.43 19

3543.101r 11 3. 4 Fe I p 2.40 182

3543. 168r 12 3. 3

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3543. 265r 44 12. 6 Co I 1.88 64

3543.389r 59 16. 5 Fe I 2.43 183

3543.495r 13 3. 6 Vi 1.18 53

3543. 682r 61 17. 3 Fe I 3.41 734

3543.795r 6. 5 1. 8

3543.933r 5 1. 3 Rhi? 0.70

3544.013r 13 3. 8

3544.087r 15 4. 1

3544.229r 38 10. 6

3544.347r 2 0. 5

3544.520r 11 3. 1

3544.634r 57 16. 1 Fe r 2.61 239

3544.746r 3 0. 7

3544.859r 4. 5 1. 3 Fe I p 2.48 154

3544.912r 13 3. 6

3544.986r 20 5. 6

3545.052r 4 1. 0 Co II 2.20 1

3545.194r 73 20. 5 Vii 1.10 5

3545.339r 3 1. 0 Vi 1.19 53

3545. 512r 43 13. 3 Ni I 3.65

3545.644r 108 30. 5 Fe I 2.85 321

3545.829r 72 20. 3 Fe I (Gd II) 3.05 0.14 536

2

3545.906r 16 6. 6

3546.019r 2. 5 0. 7

3546.206r 42 12. 0 Fe I 2.43 183

3546.346r 6. 5 1. 8

3546.426r 3. 5 1. 0

3546.542r 9. 5 2. 7

3546.64 a 4 1. 0

3546.709r 13 3. 8 Co I 1.71 41

3546.779r 7 2. 0

3546.832r 6. 5 1. 7 Dy II 0.10

3546.979r

3547.026r 30

J {[ 118. 5 Ti I 1.50 133

3547.199 100 28. 2 Fe I /2.81

13.30 321

613

7

3547.369r 18 5. 1 Ca I 2.52

3547.498r 6 1. 7

66
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- ducod

Width

AX/X

(F)

Spot

Solar

Identification

Low

K P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3547. 638r 1

[ 28

[ 4. 2 3551. 871r 6 1. 7

3547.67 a 1 4. 2 Zr I 0.07 13 3551.957r 56 15. 4 Zr II 0.09 1

o547.7yyr Q /I Q o4. O ivin I

1 clo Q c CO 1 1 O*- ooOii. 1 izr / U r e I lyy

3547.945r 35 12. 7 3552.308r 2. 5 0. 7

3548.033r 107 34. 0 |Mn IFe I 2.30

3.02 18 496

3552.433r

3552.558r

32

4. 5

9. 0

1. 3

Fe I 2.45 182

3548.190r

3548.305r

139

3. 5

38. 4

1. 0

Ni I — Mn I

/0.27

10.21 2.30

320

18 3552.62 a

3552.725r

7. 5

55

2. 1

16. 6 Co I (Yi)

0.22 0.00 6

8

3548.38 a 2. 5 0. 8 3552.845r 120 33. 1 Fe I 2.87 321

3548.451r 38 10. 5 Co I 1.71 41 3552.945r 14 5. 1

3548. 545r 28 7. 6 Fe II p 4.49 132 3552.991r 37 10. 4 Co I 1.96 67

3548.651r

3548.738r

9

6

2. 5

1. 7 Cri? 3.43

3553. 095r

3553. 163r

1

\ 48

r 3. 4

1 10. 1

Pdi

Co I

1.45

2.79

9

137

3548.84 a 7 1. 9 3553. 275r 12 3. 4 Vi 1.22 53

3548. 905r 10 3. 1 3553.350r 8. 5 2. 5

3549 009r 54 15. 1 Y 11 0.13 9 3553. 483r 96 26. 6 Ni I 0.11 16

3549 118r 4 1. 1 3553. 594r 27 8. 5

3549.242r 38 10. 4 3553.746r 116 32. 3 Fei 3.57 810

3549.371r 26 7. 0 Gd 11 0.24 7 3553.870r 17 5. 4

3549.525r 12 3. 4 Zr 11 1.24 84 3553.974r 3 0. 8 Cri? 3.08 157

3549.631r

3549.72 a

3549.765r

3549.872r

3550.106r

3550.222r

3550.369r

3550.486r

3550.599r

3550.798r

3550.951r

3551. 112r

3551. 235r

3551.401r

3551. 533r

3551.659r

3551.771r

1

5

7. 5

84

9. 5

43

22

19

87

24

13

53

14

26

94

44

10

0. 2

1. 4

2. 3

23. 1

2. 7

12. 0

6. 1

5. 6

24. 0

6. 3

3. 5

14. 5

3. 8

7. 3

26. 1

12. 4

3. 0

Zr I

Fei

Cai

-Dy II

Zri?

Co I

Fe I

Nil

Co I

1.00

1.61

2.52

0.00

0.17

2.85

0.17

1.96

48

12

4

321

5

67

3554. 122r

3554.277r

3554.297r

3554.36 a

3554.452r

3554.510r

3554.648r

3554.797r

3554.937

3555.044r

3555.177r

3555.284r

3555.357r

3555.455

3555.617r

3555.724r

3555.804r

127

18

46

86

41

16

404

15

6

2

5. 5

49

4

12

4. 5

35. 3

r 3. 8

1 1.

0

6. 2

18. 1

27. 2

17. 7

9. 0

111

13. 5

3. 1

0. 7

1. 8

14. D

1. 1

3. 2

1. 3

Fei

(Zr ii)

Fe I p Fei

Fe I p

Fe I

Vi?

Cr I? Fei

Cr I?

0.96

1.18

2.94

2.88

2.47

2.83

1.19

1.00

2.54

23

83

395

325

154

326

53

f 67

761-925—66—7
The Solar Spectrmn-—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3555.947r 16 4. 5 Co II 2.27 1 3560. 163r 26 7. 3

3556. 150r 8. 5 2. 2 Til 3560.296r 23 6. 5 Co I 1.88 64

3556.264r 8. 5 2. 5 3560.416r 22 6. 2

3556.374r 4 1. 3 3560.509r 10 3. 9

3556.490r 13 3. 9 3560.589r 62 18. 8 Vii 1.10 4

3556.597r 23 7. 0 Zr II 0.47 9 3560.704 75 21. 0 Fe I 3.25 675

3556.689r 95 34. 3 Fe I 2.86 325 3560.802r 32 13. 7 Ce II 0.68 51

3556.803r 143 55. 7 Vii 1.13 5 3560.897r 82 22. 4 Co I 0.63 21

3556.896r 243 67. 2 Fe I 2.85 327 3561.063r 17 4. 8

3557.064r 5 1. 7 Gd II 0.60 22 3561. 136r 16 4. 5 Co II

3557. 164r 9. 5 3. 1 3561.279r 12 3. 5

3557.230r 11 3. 4 3561. 376r 14 3. 9

3557. 355r 15 4. 4 3561.469r 6 1. 7

3557.464r 4 1. 1 3561.582 58 16. 3 Ti II 0.57 15

3557.677r 5. 5 1. 5 3561. 656r 8. 5 2. 7 Hf II 0.00 1

3557.767r 8 2. 4 3561.757 77 21. 6 Ni I 0.00 2

3557.880r

3558.000r

3558.072

3558.210r

3558.337r

3558.430r

4

3. 5

30

6

7. 5

13

1. 3

1. 1

10. 7

2. 4

4. 6

15. 9

Fe I p

Fe I p

3.24

2.61

572

239

3561.903r

3562.021r

3562.096r

3562.191r

3562.270r

57

11

32

7

40

15. 6

3. 4

8. 8

2, 1

10. 9

|FeiTi II

Co I

Fei?-

Cr I?

1.16

2.28

3.25 4.45

42

115

308

3558.532r

3558.634r

3558.783r

3658.877r

3558.984r

3559. 079r

3559.207r

3559.274r

3559.464r

3559.516r

3559.610r

oooy Qc;t;Q 7nf)r

.

t uur

3559.814r

485

10

38

5

2. 5

41

25

9. 5

1 94

6. 5

oQ

24

137

10. 5

16. 4

1. 8

1. 0

12. 8

7. 2

2. 8

1

7. 9

[ 22. 2

2. 0

9 9

6. 7

|Fe ISc II

Co I

Fe I Fe I?

Fe I p Fe I

Cr I?

0.99

0.01

0.58

2.88

3.07

2.87

24

3

20

321

498

89

3562.410r

3562. 550r

3562.607r

3562.709r

3562.926r

3563.013r

3563. 159r

3563.403r

3563. 611r

3563.716r

3563.789r

3563.926r

3564.126

7. 5

6. 5

11

7. 5

37

6

20

8. 5

23

4

18

4

71

1. 9

1. 9

2. 9

1. 9

10. 1

1. 6

5. 6

2. 3

6. 3

1. 1

5. 2

1. 2

21. 0

Fe I p

Co I

Dy II

Fe I Vii

Cr II? Fe I (Co I)

2.56

1.88

0.10

2.81

1.13

4.94

1.61 3.17

237

64

325

4

134

48

159

3559.923r 48 13. 5 Ni I 3.54 118 3564.279r 2. 5 0. 8 Cr I? 4.10 281

3560.076r 42 11. 6 Fe I 2.86 321 3564. 398r 12 3. 9 Ca I 2.52

68
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

ik)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3564. 524r r 16.

Fe I 2.45 183 3568.55 a 5 1. 8 Tb 11?

3564.565r 1 11. 5 Fe I p 2.45 183 3568.628r 16 5. 2

3564.683r 11 4. 3 Fe I 3568.829r 72 23. 4 Fei 3.25 673

3564.796r 15 6. 4 3568.983r 82 27. 2 Fei 2.69 294

3564.959 70 32. 7 Co I 0.58 19 7 3569.142r 6. 5 2. 5 Cr I? 4.10 281

3565. 129r 7. 5 7. 2 -Cr I 2.54 50 3569.232r 9. 5 3. 8

3565.306r

3565.396r

3565.596r

13

990

49

26. 6

274

42. 8

-|Ti n

Cr n

Fe I

Fe I

1.58 4.75

0.96

/2.86

12.86

76

107

24

321 328

3569.384r

3569.510r

3569.622r

3569.734r

116

86

8

12

44. 0

41. 7

4. 1

13. 6

Co I Mn I

0.92

2.32

35

18

3565.716r 4 3. 1 3569.819r 37 33. 4 Mn I 2.32 18

3565.838r 16 7. 8 Fe I p 3.26 571 3569.921r 5 6. 2

3565.972r

3566.088r

3566.175r

41

13

53

20. 6

7. 6

30. 2

Ti II

Zr I Cr I

|Vii

Fe 11

1.16

0.15

f3.14 t4.19

1.07 4.49

42

15 284

4 132

3570.044r

3570.134r

3570.276r

3570.427r

10

1380

42

7. 5

30. 5

387

61. 3

9. 9

|Mn I Fe I Fe I Fe I

2.32

2.42

0.91

2.81

18 135

24

326

3566.315r 9. 5 16. 0 Fe 1 p 2.28 127 3570.521r 10 8. 8

3566.383r

3566.485r

3566.589r

3566.668r

3566.758r

3566.845r

3566.922r

3567.042r

3567.195r

3567.377

3567.455r

3567.572r

3567.696r

3567.742r

3567.944r

3568.008r

3568.142r

3568.248r

458

10

28

4

3

5. 5

38

82

11

58

11

22

1 110

22

3. 5

6. 5 28

141

18. 2

17. 2

2. 1

1. 3

2. 4

14. 0

25. 9

3. 4

16. 5

3. 1

6. 2

j 25. 8

1 9. 5

6. 4

1. 1

2. 1

8. 5

Nil

Fe I

Sm II

Fe I

Fe I

So II Fe I Nil

Zr II Sm II

0.42

2.40

2.87

2.45

0.00

3.24

3.61

0.80

0.48

36

181

325

183

3

571

46

47

3570.597r

3570.687r

3570.861r

3570. 987r

3571.111r 3571.233m

3571.30 a

3571.407r

3571. 551r

3571.689r

3571.774r

3571. 875r

3572.016r

3572. 141r

3572.321r

3572.478r

3572.573r

6

7

4

16

9. 5

60

5

11

5. 5

49

9. 5

237

64

52

39

1 106

J 112

4. 2

3. 9

1. 7

6. 3

3. 5

20. 7

1. 8

3. 6

1. 8

19. 7

6. 0

69. 8

29. 7

17. 2

11. 6

30. 6

32. 0

Fe I p —

Ru I

Fe I

Ni I Fe I

Fe I p

Zr II

Sc II (Fei)

2.45

1.93

1.48

0.17

2.83

2.43

0.00

0.02

2.85

154

46

5

321

182

1

3 325

3568.312r 12 3. 6 3572.751r 30 8. 6 Cr I 2.71 75

3508.448 70 21. 4 Fei 2.87 321 3572.878r 1 0. 3

69
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3572.948r 7. 5 2. 1 3577. 063r 10 3. 1

3573.067

3573.181r

40

4

11. 5

1. 1

|Fei

Zr 11 0.32 9 3577. 159r

3577.245

4. 5

39

1. 1

10. 9 NilCo I 0.27

1.74

3

41

3573.278r 6 1. 7 Ni I p 3.70 123 3577.392r 11 3. 4

3573.402

3573.5 Ur

66

21

18. 5

5. 9

Fe I ViVii?

3.30

2.13 2.37

673

12278

3577.465r

3577.565r

47

4

13. 1

1. 1

Ce II Fe I 0.47 51

3373.653r 39 13. 5 Cr I 2.71 75 3577.745r 22 6. 8

3573.735r 84 25. 5 Ti II 0.57 15 3577.875 105 30. 6 Mn I 2.11 8

3573.836r

3573.911r

1 156

r 27. 5

1 22. 4

Fe I Fei

2.40

3.30

181

611

3577.998r

3578.100r

12

48

4. 5

15. 2

Co II Co I2.24

2.28

1

117

3573.996r

3574. 035r 1 69

f 11.9

1 11. 9 Cr I r2.7i 14.45 74 308

3578.218r

3578.392

14

52

4. 8

21. 9

Zr II Fe I1.21

2.88

83

321

3574. 158r

3574.253

7. 5

45

2. 0

12. 6

Dy II

Ti IFe I 2.27 3.28 247 574

3578.562r

3578.693

3578.838r

4. 5

488

8. 5

3. 1

142

8. 1 Cn 0.00 4

3574.360r

3574.416

3574. 584r

3574.805

3574.967

3575.121

3575.252r

3575.374

24

60

5. 5

50

90

75

83

115

7. 3

16. 8

1. 5

14. 3

25. 1

22. 5

26. 5

32. 2

Vii

Fe I

Fe I Cri

Co I Fe I Fe I |Coi Fe I

2.37

2.43

2.71

0.58

2.88

2.83

0.10

3.02

78

181

75

21

321

322

4 496

7

3578.907r

3578.982r

3579.045r

3579.128r

3579.368r

3579. 508r

3579. 562r

3579. 672r

3579.835

13

11

14

4

7. 5

5

27

6. 5

34

8. 9

6. 4

6. 3

1. 5

2. 7

1. 8

9. 9

2. 5

13. 4

Co I

Cox

Fe I

Fe I

1.74

1.74

3.24

41

41

573

3575.560r 15 4. 2 3579.90 a 9 5. 0

3575.765r 34 9. 5 Zri 0.07 12 3579.958r 6 2. 8

3575.94 a

3575.994a j 90

1

8. 9

1 21.3

Ni I Fei3.70

/2.87

12.87

120

321 328

3580.087r

3580.216r

924

4. 6

12. 1

Mn I 3.07

3576.156r

3576.253r

3576.329r

3576.387r

3576. 599r

3576.766r

9. 5

12

1 116

3

87

2. 8

3. 8

1 30.8

[ 2. 8

0. S

24. 3

Dy II

Sc II

Fe I Ni II

0.59

0.01

3.27 3.07

3

613a

4

3580. 412r

3580.542r

3580.758r

3580.927r

3581. 044r

35»l.z(jyr

3581.391r

20

14

13

54

6. 5

7

12. 5

12. 0

15. 8

53. 5

19. 7

oyy

15. 6

Fei

Sc II

±6 1

0.00

U.oD

3

3576.863r 44 13. S Zr II 0.41 9 3581. 477r 8. 5 16. 0

3576.959r 1. S 0. 4 3581. 665r 36 34. 2 Fe I 2.69 295

70
The Solar Spectrum—Continued

Wavelength

(I)

Equivalent Width

AX

Re- duced

Width

AX/X

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

3581.817r 29 22. 7 Fe I 3.07 497

3581.941r 24 16. 4 Fe I

3582.09 Ir 12 8. 6 Zr II 1.G6 101

3582.205 64 30. 2 Fe I 3.24 612

3582.331r 33 15. 2 Fe I 3.28 568

3582.437r 17 7. 8 Fe I

3582.571r 40 17. 7 Fei 2.45 181

3582.698r 72 26. 5 Fei 2.88 328

3582.744r 19 7. 7 3582.877r 18 6. 6 Fe I?

3582.964r 16 5. 9 Fe I

3583. 104r 16 5. 4 3583.217r 18 6. 8 3583.339 122 38. 6 Fe I- 3.29 574

3583.441r 9. 5 3. 6 3583.497r 17 5 7 3583.597r 11 O. £7 Fe I

3583.697r 112 33. 2 |Fe I —

V I 1.08 45

3583.911r 96 27. 9 Fe I

3584.007r 8 3. 1 3584.097r 34 10. 3 Fe I

3584.257r 5 1. 5 Fe I

3584.317r 10 3. 2 Cri 3.19

3584.383r 25 7. 9 Fe I

3584.476r 4 1. 4 Fe I?

3584. 520r 44 20. 0 Yii 0.10 9 3584.661 182 59. 7 Fe I 2.69 294

3584.800r 72 39. 3 Co I Fei

0.17

2.86 6 322

3584.965 78 33. 8 Fe 1 /3.00

13.27 395

611

3585.074r 8. 5 7. 5 Dy II 0.00

3585. 170r 45 37. 0 IICoiFe I 0.51

2.95 21 438

oooO.ooyr 231 |Fe I Cr II 0.96

2.70 2313

3585.5 18r 35 28. 8 Cr II 2.71 13

3585. 637r 7 9. 2

3585.714in 168 63. 0 Fe I 0.91 23

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3585.844r 25 22. 6 Co i7-

Ti I 2.08 100

3585.907r 50 26. 6 Ni I p 3.70 172

3586.017r 24 12. 7 3586.118m 122 38. 4 Fe I (Fe ip)

3.24

3.02 611 497

3586. 250r 16 6. 0 Cr i?-

Zri

3.10

0.00 157

12

3586.354r 21 7. 2 Fe I?

3586. 484r 10 4. 5

3586. 544r 74 27. 3 Mn I 2.14 8

3586.750r 42 22. 2 Fe I 2.81 325

3586. 884r 12 15. 3 3586.990m 532 147 Fe I 0.99 23

3587. 146r 3. 5 11. 4 li II 0.61 15

3587.230r 250 145 |CoiFe I 1.05 2.86 35 325

3587.357r 7 4. 6 Fe I? 3587.429m 54 23. 4 Fe I 2.42 134

3587.617r 110 34. 9 Fe I? 3587.760m 112 32. 3 Fe I 3.27

3587.943r 129 35. 6 Nil

(Zr II) 0.03 0.32 16

10

3588. 122r 35 9. 8 -Vii 2.38 78

3588.246r 80 22. 3 Fe I p 1.56 47

3588.325r 36 11. 0 Zr II 0.41 10

3588.422r 9. 5 2. 8

3588.534r

3588.622r

i 161

1

[ 22. 6

1 27. 3

Fe I Fe I2.94

2.83

394

325

3588.775r 33 8. 9 Zr II 1.00 57

3588.925 94 25. 6 Fe I 2.87 322

3589.112m 104 28. 4 Fe I 0.86 23

3589.222r 18 5. 7 Ru I 0.38 4

3589.305r 24 6. 7 3589.461m 97 26. 5 Fe I 2.73 295

3589.632r 108 29. 6 Sc II 0.01 3

3589.767r 102 28. 0 Vii 1.07 4

3589.882r 16 4. 7 Fei?

3589.968r 45 12. 8 Mn I 2.93 25

3590.094r 76 20. 9 Fe I 2.95 440

71
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Wiatn \ AX

(mA)

Keiuced

A* lath t AX/X

(F)

?pot SolarIdentification

Low

E P

or Rot. Line

r> ATT' No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width ' AX

(mA)

Re- duced

idth t

(F)

5p0t Solar

Identification

JLow E P

or Rot.

L/ine

RM i No.

or Vib. Band

?^otes

3590.242r 16 5. 0 3595.413r 5.5 1. 5 Fei?

3590.302r 33 11. 9 Fe I p 3.02? 497 3595.540r 1 0. 3 Fei

3590.368r 44 16. 2 3595. 683r 14 4. 0 Fe I 2.88 322

3590.489 136 37. 9 Sc II 0.02 3 7 3595.879m 50 13. 9 Fei 2.45 181

3590.662r 20 5. 6 Fei 3.69 953 3596.054r 95 26. 7 Ti II 0.61 15

3590.835r

3591.008r

3591. 142r

3591.225r

3591.355r

3591. 488r

3591.591r

3591.744r

3591.904r

3592.027S

3592.207r

3592.271r

3592.367r

ooyz.o / or ocno QQQr

2

44

4

13

59

60

11

10

10

75

4

15

3. 5 AO

1 Pi

/y

±0

0. 6

12. 3

1. 1

3. 6

16. 5

16. 8

3. 1

2. 8

2. 9

21. 0

1. 1

4. 2

1. 1

19IZ. o

A n 0. u

OQ A

Idl*!. 0

Fe I Fei?

Cai

Fe I Fe I

Co I

Vii

Fe I

r e I Sm II re I

|re I Yi

3.21

2.52

2.85

3.29

2.54

1.10

j.oy

U.OO

0.00

573

321

568

134

4

/

ooy

77

8

3596.205r

3596.313r

3596.392r

3596.509r

3596.645r

3596.752r

3596.859r 3597.047m

3597.152r

3597.252r

3597.399r

3597.512r

3597.712r

3597.852r

3597.979r

3598. 025r

3598.182r

57

2. 5

0. 5

22

3. 5

1. 5

3

86

11

6

6

13

181

26

3

15

8

15. 9

0. 7

0. 2

6. 4

1. 1

0. 4

0. 8

23. 9

3. 3

1. 7

1. 7

3. 6

50. 2

8. 3

0. 9

4. 3

2. 2

Fe I (Rui)

Fei?

Co I Fe I? Fei?

Fe I Fe I Rhi

Fe I p

Fei?

Ni I

Ce II?

2.43 0.26

2.28

3.26

0.41

3.63

0.21

0.33

181

3

118

569

5

856

18

116

ooyo.Ui / r QO 1. J Ru I O.o4 4 3598.271 67 18. 6 ooyo.Uozr in ^3 lU. 0 i 1 II

1i.OO 3598. 469r 4 1. 1 3593.261r 2. I. 1. C 3598.612r 11 3. C ooyo.o4ur QQOO oy. t l|V II Fe I 1.13 3.26 4 571

3598. 720r 60 16. 7 llTi I Fe I 0.90

3.25 59 674

3593.495r 436 127 Cn 0.00 4 3598.811r 6 1. 7 3593.694r

3593.794r

5

10

2. ]

3. 55 Fe I 2.45 182

3598.939r

3598.986r

1

[ 87

f 13. f

1 13. £

Fe I Fe I

3.28

2.88

568

322

3593.997r 40 14. () Cai 2.52 3599.145r 87 24.

:

Fe I 3594.104r 11 3. c

) Fe I p 2.42 154 3599.381r 28 7. S Cr I? 2.91 89

3594.317r 7 2. ][ Fe I? 3599.544r 18 5. C) Ni I 3.61 121

3594.387r 6 1. iI 3599.631m 78 22. C) Fe I 3.57 809

3594.638m 146 40. !: Fe I 2.85 322 3599.764r 6. I 1. £ Ru I 1.09

3594.876r 92 25.

'1 Co I 0.17 4 3599.831r 6. I 1. S Fe I 3595.115r 74 20. ( Mn I 2.16 8 3599.970r 58 16. 2 Fe I 3595.308r 74 20. ( Fe I 2.87 322 3600.171r 12 3. e

72
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3600.371r

3600.454r

3600.591r 3600.739m

3600.824r

3600.918r

3601.078r

3601. 198r

3601.284r

3601.358r

3601.428r

3601.544r

2. 5

3. 6

2. 5

69

6. 5

3. 5

2. 5

13

6

8

16

5

0. 7

1. 1

0. 8

19. 2

1. 7

1. 0

0. 7

3. 6

1. 7

2. 2

4. 4

1. 4

Tb n?

Ceil

Yii

Co I

Zn

Fe I

Fe I

0.79

0.18

1.96

0.15

2.28

236

9

63

13

127

3004.277

3604.378

3604.464r

3604.558r 3604.702m

3604. 805r

3604.933r

3605.019r

3605.082r

3605.201r

3605.339r

42

75

9. 5

5

60

2. 5

17

18

16

26

495

12. 8

20. 8

2. 8

1. 4

17. 3

0. 8

5. 5

6. 9

7. 8

24. 1

136

Ti I (Smii)

Fe I Co I

Fei

Cn

Co I

-Fe I

llCri Co I

0.02

0.48

2.88

2.79

3.30

2.71

2.04

3.30

0.00

0.51

2147

323

136

74

97

420

3601.664

3601. 788r

51

8

14. 2

2. 2

Cri

Mn I

2.71

2.92

74

25

3605.475r

3605.529r 1 83

r 43. 8

1 43. 8

Fe I Fe I p

2.73

2.81

294

322

3601.922m 57 15. 8 Yii 0.10 9 3605.692r 4. 5 1. 7 Mn I 2.94 25

3602.085

3602.287m

103

94

28. 5

26. 2

|Co I —

Fei

Nil

0.22

2.88

0.17

4 322

3

7 3605.916m

3606.039r

75

26

21. 8

7. 5

Fe I Fei?

Co II?

3602.469r

1

f 25. 3 Fe I 2.86 322 3606.132r 9 2. 8 Dy II

3602.544r > 172 I 29. 2 Fe I /2.86

12.94 324

391 3606.251r 4. 5 1. 4 Fe I

3602. 598r J i 0.1 Cri 2.71 74 3606.378r 31 9. 6 Fe I 2.56 233

3602.708r 13 4. 7 Fe I p 2.94 390 3606.538r 44 21. 4 Fei 2.42 133

3602.771r 47 13. 2 Fei 2.83 370 3606.611r 9 10. 5

3602.878r 1. 5 0. 5 Fe I 3606.694 271 75. 1 Fe I 2.69 294

3602.971r 3 0. 9 3606.854r 18 6. 9 Nil /3.61

13.83 120

173 3603.097r 3603.210m

3603.438r

3603 578r

3603.621r

3603.691r

45

119

3. 5

1 106

18

14. 8

33. 6

0. 9

f 11. 8

1 23.9

9. 0

Fe I Fez

Fe I Cr II Fe I

2.69

2.43

2.70 /2.56

\2.69

295

181

13

3607.004r

3607.124r

3607.251r

3607.379r

3607.533m'

3607.625r

1. 5

6

3

13

66

2

0. 4

1. 7

0. 8

3. 9

19. 0

0. 7

Fe I Fe I

Zr II Mn I Ce II

1.24

2.14

0.67

83

8

178

3603.781r

3603.831r

3603.950r

3604.07 a

3604. 118r

1 155

43

2

2

r 28. 6

1 23. 6

12. 6

0. 5

0. 5

Cr 11 Fe ICr II Fei

Fei?

2.71

3.07

2.71

13

496

13

3607.772r

3607.865r

3607.972r

36Uo.UlUr

3608.07 a

3608.155m

6

12

55

J

1. 5

82

1. 8

3. 7

f 0. 2

1 Q A

[ iO. D

1. 0

32. 8

Fe I -Cai?

Fe I

1.89

/2.85

l\2.99

325

438

73
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

E.MT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3608.319r

3608.412r

3608.491r

11

15

38

5. 7

8. 6

22. 4

Co I Cn

Mn I

0.63

3.85

2.16

20

252

8

3612.941

3613.109r

90

1

139

25. 2

r 25. 7

Fe I

|Zr II Fe I p

/1.56

12.18

0.04

2.87

46

77

1 322

3608.589r

3608.639r

OOUO. / O^l

3608.869

3608.995r

ouuy. luor

2

5. 5

R

1046

3

V

2. 5

7. 2

X o. o

287

8. 2

7 ^

^1 TT Ti

Fe I 1.01

A

23

3613. 176r

3613. 332r 3613.449m

3613.605m

3613.719r

14

86

86

21

[ 18. 5

3. 9

23. 8

24. 4

9. 7

Fe ICr II Cr II Fe I Fe I Fe I Ce II2.87

2.71

2.71

3.25

3.30

2.45

0.32

324

13

13

672

110

ouuy .'x #

yju 49

^9 n

17 9

I

t Cr I Sm II

n 1

1

U. X X

9 Sfi 2.54

0 9S

1 y)

49

oo

ooio.isuyr

QC 1 Q CO 1 ^ oDlo.ooir

oDio.yozr

1 194

J 0

f 90 fi

1 9fl ft

O. D

\ Sen

J Fe I

0.02

3.27

2

612

OUU»7. «J<JOX X o Vc\ X U 1 9 oDli.uZ ir 1xyQ 0. <)

]^ n 4 Ce II 1X 70(

y

QC 1 /111 Qt-« oo 14:. i iom oU 99 c: Fe I 3.30

3609.768r 9 3. 0 Co I 2.88 147 3614.23 a 4. 5 1. 4 Ti I?

3609.978r 3 1. 2 Fe I? 3614.308r 10 2. 9

3610.056r 10 5. 4 Cri 2.54 49 3614. 411r 7. 5 2. 0 Fe I?

3610.166r

3610.296r

3610.460r

3610.508r 3610.702m

3610.83 Ir

3610.944r

3611. 050r

OU^filX 1i . 1i S/1t orrl

231

35

1 250

76

17

4. 5

80

X o

65. 4

25. 5

J

52. 0

[ 42. 6

24. 8

5. 1

1. 4

22. 2

1 n

o. o

Qy. ^0

IIFei Ti I Mn I Ni I

Fe I

Fe I? Yii

T?0 T

Ni I p

2.81 0.90

2.18

0.11

2.87

0.13

ftU. 171 <

32158

8

18

323

9

9

3614.561m

3614.651r

3614.718r

3614.784r

3614. 891r

3615.004r

3615.084r 3615.197m

3615.324r

3615.393r

3615.531r 3615.665m

98

3

j 141

28

7. 5

3. 5

62

3

26

2

71

27. 0

1. 1

f 25. 1

1 18. 0

8. 0

2. 0

0. 9

17. 1

0. 8

7. 0

0. 5

19. 6

Fe I

Fe I

Zr II Fe II Fe I

Fe I Fe I Co I Fe I? Cri

IIyrFee TX

3.25

0.36

4.15

2.40

3.28

1.96

0.00

1X .TtO 48

9

112

154

569

66

346

3611. 723r 61 16. 9 Co I 2.33 115 3615.811r 9 2. 5 Fe I

9"^ 7 7.-r TT ZjL 11 1 1 Q cSblo.yDZr 61 lU. ^ Fe I o .ow lis X 1 o 0 1. D TTo T J? e 1 aolD.U/ a

Qo U. O

TpQ r T? e I f

3612. 382r

Q£7

5

9 R

1. 5

±1 1 Q A 1 A 1 Kfiw oDiO.iotJr

3616.219r

1 116

)

r o 1 A 21.

i 14. 6

Var T e I 91 out/

3612.519r 20 5. 8 Fei 3.30 613a 3616. 327r 56 16. 6 Fe I 2.42 132

3612.605r 13 3. 9 Cri 3.85 252 3616.431r 2. 5 0. 8 3612.744m 160 45. 2 Nil 0.27 6 3616.570m 92 25. 9 Fe I

74
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Widtli

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

1 Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3616.728r 3. 5 1. 0 Fei 3621. 105r 84 2.5. 3

3616.878r

3617. Ollr

3617.105r

0. 5

36

35

0. 1

10. 6

11. 2

Hf I Fe I Fe I0.29

3.05 535

3621.20 Ir

3621.26 Ir

72

36

2L 8

19. 7

Vii

Co II Sm n-

|Fe II

2.37 2.20

0.10

4.61

76

1

12 144

3617.321 82 25. 4 Fe I 3621. 381r 10 4. 1

3617.437r 42 16. 0 3621.467m 140 40. 6 Fei 2.73 294

3617.539r 8. 5 2. 9 Wi 0.37 8 3621. 601r 29 9. 1

3617.717r 29 10. 8 3621.725m 76 22. 4 Fei 3.57 808

3617.796r 124 41. 4 Fe I 3.02 496 3621.868r 14 4. 1

3617.960r 46 18. 5 Fe I 2.45 181 3622.009m 127 36. 5 Fe I 2.76 295

3618.090r 1 0 4 3622. 158r 31 9. 1 Ce II- 0.86 71

3618.187r 11 5. ;} Fe I 3.02 3622.268r 17 5. 2 Vii? 2.60 144

3618.304 110 48. 9 Fe I 2.83 324 3622.438r 3 0. 8 Fe I

3618.394

3618.523r

3618.61or 3618.777m

3618.923r

74

12

44

1410

2

89. 0

20. 2

63. 8

385

7. 5

Fe I

Fe I p Fe I Vii

Fe I p

/2.73

\3.24

3.26

0.99

2.76 2.42

295

571

569

23

158 130

3622.555r

3622.655r

3622.795r

3622.901r

3623.041r

3623.095r

3. 5

0. 5

14

0. 5

2. 5

15

1. 0

0. 1

4. 1

0. 1

0. 8

4. 4

Eu II?-

Ti I?

1.38 18

3618.999r 31 43. 2 3623.192m 105 29. 9 Fez 2.40 180

3619.114r 12 21. 8 3623.321r 12 4. 0 Sm II 0.10 12

3619.273r

3619.400r

17

568

34. 2

204

Mn I Nil2.19

0.42

8

35

3623.450

3623.510r

\ 97

r 24. 2

1 5. 2

Fei

Fe I p

/2.56

3.00

233

4c5o 393

3619.536r 15 17. 0 Nb n 0.98 4 3623.610r 14 4. 1 3619. 670r 19 11. 5 Fe I 2.42 130 3623.67 a 1. 5 0. 5 3619. 776r

3619. 937r

3620.032r

48

34

28

23. 2

13. 8

10. 6

Fe I Fe I Nil

Fe I p

2.40

0.27

2.88

180

3 324

3623.785r

3623.917r

3624.064r

118

46

1 139

33. 8

14. 2

f 18. 5

|Fei- Mn I

Zr IFe I

2.86 2.18

0.07

3.26

323

8

12

570

3620. 156r 6. 5 2. 5 3624. 118r 1 24. 6 Cai 1.88 9 3620.247

3620.36 a

3620.439r 3620.468m

3620.619r

3620.772r

51

3. 5

I Id.

1

2. 5

7

17. 4

1. 1

j 0.1

1 24. 4

0. 8

2. 2

Fe I

Co I Fe I2.85

2.28

324

116

3624.304m

3624.460r

3624.567r

3624.733r

OD.i4.Ooyr

95

2. 5

4

132

27. 0

0. 7

1. 1

37. 1

'XA A

04:. 4

|FeiCoi

Nil

ll II (Fe II)

2.42

1.78

0.00

4.61

133

41

2

144

3620.879r

3620.971r

51

24

16. 0

8. 2

Fe I Yi

/2.88

13.30

0.07

323

611

8

3624.963r 3625.147m

39

106

11. 0

29. 8

Co I Fe I

0.63

2.83

21

323

761-925—66 8
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT "NT JNo. or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

JNo. or

Vib. Band

Notes

3625.249r 7. 5 2. 4 3629.905m 47 13. 9 Nil 3.84 182

3625.366r 1. 5 0. 4 3630.027m 31 9. 4 Zr II 0.36 10

3625.501r 49 13. 5 Fe I 3630.112r 8 2. 5

3625.626r

3625.753r

3625.853r

3625.9<4or

3626. 016r

3626. 109r

3626. 187r

10

23

2A K

0. 0

2

39

50

2. 8

6. 5

0. 6

U. 1

0. 6

11. 8

13. 9

Vii

Cai

JNl I.r

L'O I

ll I

ll e I

2.38

2.52

3.31

1.78

0.02

76

41

3630.234r

3630.355m

3630.478r

3630.578r

3630.658r

3630.754

26

84

1. 5

41

9. 5

133

8. 3

27. 2

0. 6

14. 5

6. 6

50. 1

Dy II Ni I p

Fe I

Nil

Cai

Sc II

3.84

2.85

3.83

1.89 0.01

180

323

172

9 7

3626. 386r 6 1. 6 3630. 985r 56 36. 6 Ca I 1.89 y

3626.493r 1 0. 2 3631. 105r 98 54. 5 Fe I 2.83 322

3626.606r 4 1. 1 Rh I 1.14 3631. 265r 35 45. 4 3626.739m 59 16. 3 3631. 356r 4. 5 17. 4 Co I 0.10 4

3626.906r

3627.061r

3627. 169r

6. 5

56

18

1. 8

15. 5

5. 0

Fe I Fe II?- CH

3.57

5.95 R 3

808

193

1,0 3

3631.475m

3631. 58Dr

3631.711r

1364

10

35

369

31. 2

38. 6

Or II

Cr II

0.96

2.70

2.71

23

1 O

12

3627. 359r 14 4. 0 Fe I p 3.04 395 3631. 789r 5 5. 2

3627. 456r 12 3. 2 OH R 1,2 1,0 3 3631. 959r 27 18. 1 Co I — 2.54 ioo

3627. 623r

3627. 715r

40

19

11. 3

7. 2

Mg I CH

Vii

Ti II

6.59 R4

2.37

45

1,0

7662

3 3632.049m

3632. 173r

3632. 299r

117

24

16

55. 6

10. 6

6. 1 Fe II

3.07

4.15 1 1 o

3627.813m 98 27. 4 Co I 0.51 19 3632.446r 5 1. 7

3627. 959r 9 2. 5 bm 11.'^ 0.10 12 3632. 560m 72 22. 6 re I O A C

3628.098r 78 21. 8 Fei 2.20 77 3632.693r 0. 5 0. 2

3628.279r

3628.439r

24

8

6. 8

2. 2

CH

Fei

R2 1,0 3 3632.840r 64 19. 1 Co I Cr I

2.87 /2.54

12.54

14749

49

3628.599r

3628.707r 3628.828m

3628.879r

3629.006r

3629. 146r

3629.25 a

3629.352r

3629.512r

45

57

64

11

15

2

1

16

0. 5

12. 7

16. 4

18. 3

3. 4

4. 4

0. 6

0. 3

4. 4

0. 1

CaiFei

Yii

Fe I Fe I CH

CH

2.52

0.13

2.99

R 5

R 5

9

438

1,0

1,0

3

3

3632.984r

3633. 076r

3633. 138r

3633.308r

3633.512r

3633.652r

3633.835r

3633. 892r

3634.005r

60

1 134

23

47

23

92

9

9

17. 9

1

28. 2

I 19. 0

6. 6

13. 8

6. 3

25. 4

3. 7

2. 8

Fe I Fe I Yii

CH

Zr II Fe I p

Fe I

Tiii?pCr II

2.48

2.94

0.00 Ql

1.76

3.04

2.99

3.09 4.94

135

390

2

1,0

102

395

440

116

147

3

3629.737m 48 14. 0 Mn I 2.16 8 3634.08 a 3. 5 0. 9

76
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Wlutu AX

(mA)

Re- duced

TXT" W

1* ^ + v. lutn

AX/X

(F)

fepot Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

W idth

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Joanursotes

3634. 198r 58 15. 7 3 63 7. 73 7r 48 12. 9 Fei 2.56 229

3634.278r 7. 5 4. 5 Sm II 0.18 19 3637.873m 93 25. 2 Fei 2.94 385

3634.332r 136 36. 9 Fe I 2.94 389 3637.975r 23 6. 9 Til 0.00 18

3634.412r

3634.472r

36

38

22. 8

14. 9

3638.058r

3638.104r 1 78

1 0. 3

[ 21. 1

3634.535r 60 16. 2 Fe I p 2.87 323 3638.168r 28 10. 2 Feip 2.85 324

3634.618r

3634.710r

13

134

5. 0

36. 0

CH

|Coi

ll-fe I Pd I

R7

2.88

0.81

1,0

146

1

3 3638.245r

3638.304r

3638.472r

> loo

5. 5

r 19. 0

I 28. 3

1. 5

Fe I 2.76 294

3634. 865r 14 5. 1 CH R7 1,0 3 3638.605r 7. 5 2. 0 CH P 1 1,0 3

3634.952r 129 34. 7 Ni I 0.42 33 3638.772r 1 0. 3 Sm II

3635.025r 34 9. 1 Cr I?- 4.10 3638.905r 16 4. 4 CH Q3 1,0 3

3635.085r 9. 5 2. 6 Fe i?p 3.64 919 3639.030r 34 9. 1 Vi- 1.80 83

3635. 197r 115 31. 7 Fe T —

Til

(Mo II)

3.02 0.05

3.14

490

20

5

3639.132r

3639.285r

3

52

0. 8

14. 3

3635.280r 12 3. 9 Cn 0.00 3 3639.332r 11 3. 3 Fe I

3635.352r

oDoo.Do/r

28

y /

1 7

7. 7

OA 1

A 7

Yiiil II P

T'l" T 11 I

i 1 II .'^ P CH

3.41

1 9Q

U.UU

o.uy Qi

46

ly

lift lit) 1,0 3

3639.450r

3639.525r

3639.695r

3639.804

69

36

3. 5

76

18. 7

12. 3

1. 0

20. 6

Co I Fe ICr I

1.96

2.54

64

47

3635.828r 16 4. 4 Fe I p 2.83 321 3639.985r 10 2. 6 Fe I

3635.895r 1 0. 3 3640.1 18r 8. 5 2. 3 Fez

3636.045r 2 0. 6 3640.265r 12 3. 4 Dy II 0.59

3636. 166r

3636.238r

I 1 QO 1 22.7

I 16. 5

Fei

Fe I

/2.20

13.21 3.55

77 568 774

3640.394m 132 35. 8 Fe I (Cn)2.73

J Z.o-i 12.54

295

A 147

3636.485r 92 24. 9 Zr II-

|Fei

0.47 /1.56

13.26

947

568

3640.645r

3640.765r

18

1. 5

4. 9

0. 5

3636.589r 36 10. 3 Cn /2.54

12.54 4747

3640.905r 3 0. 8

3636.663r

3636.751r

3636.865r

3637.000r

3637.058r

66

92

4

> 11^

23. 1

25. 1

1. 4

r 21. 5

1 10. 7

Fe I Co I Fe II p Fe I Fe I3.02

1.96

4.15

2.59

3.02

493

64

112

233

438

3641. 032r

3641.228r'

.3041. ooom

3641.45Qr

3641. 646r

48

11

luy

52

51

13. 2

3. 0

29. 6

14. 0

14. 0

Fe II? p

T'l TT ll II Fe I Cn

Nil

4.15

1.^4

2.88

2.54

0.27

111

323

47

6 3637.255m

3637.317r

68

10

18. 5

3. 4

Fe I Co I

2.43

2.33

180

117

3641. 792r

3641. 832r 1 72

r 6. 3

1 15. 5

Co I Cn2.04

2.54

99

47

3637.444r 1 0. 2 3641. 964r 32 8. 8 Fe I

3637.554r 24 6. 6 3642.147r 8. 5 2. 3 -CH P2 1,0 3

77
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3642.281r 22 5. 9 CH Q4 1,0 3 3646.352r 1. 5 0. 4

3642.398r 19 5. 2 Ni I 1.99 75 3646.40 a 1 0. 2

3642.537r 12 3. 3 Fe II? 3646.504r 23 6. 6 CH Q 5 1,0 3

3642. 682r 93 31. 8 Ti I 0.02 19 3646. 618r 54 15. 9

3642.806

3642.971r

150

20

40. 9

5. 4

Sc II CH

0.00 P 2

2

1,0

7

3

3646.809r

3646.837r 1 40

f 3. 3

1 9. 9 -CH Q 5 1,0 3

3643. ]24r 94 25. 8 Fe I See

3643. 204r

3643.354r

3643. 477r 3643.627m

66

2. 5

5

113

30. 2

0. 7

1. 3

30. 8

CoiCr II

Fe I

2.04 2.48

2.94

99

1

385

3646.988

3647. 095r

3647.255r 3647.428m

58

14

4

94

24. 6

7. 5

2. 1

50. 7

(Ce II) Co I

IIFei Cr 11

0.30

2.33

1.56 2.43

66

118

46

1

§2.2

3643. 729r 112 41. 2 Fe I 2.61 233 3647. 562r 24 25. 6 Fe I p 3.26 574

3643. 811r

3643. 951r

81

27

43. 4

7. 4

Fe I

Ni I

/1.61

13.25

3.68

46 670

174

3647.669r 3647.851m

39

970

59. 6

313

Co I Fe X (Fei)

0.22

0.91 3.24

4

23 569

3644.074r 3. 5 1. 0 3648.082r 24 34. 5

3644.151r

3644.21 a

3644.317r

3644.417

3644.591r

3644.695r

3644.794r

1

3

1 141

46

58

119

0. 3

0. 8

{ °'

[ 38.0

12. 4

15. 8

32. 4

Fe II p Hf II Cai

Fe I p Cr II |CaiFe I

4.48

0.79

1.90

2.59

2.45

1.90 3.24

131

6

9

235

1

9 570

3648.228r

3648.322r

3648.530r

3648.639r

3648.759r

3648. 815r

3648.998

18

5. 5

23

0. 5

5

36

52

14. 0

3. 8

11. 2

0. 3

2. 3

15. 3

21. 4

Fe I p —

CH

Cri

Cn

3.88 P 3

2.54

2.54

978

1,0

47

47

3

3644.978r 38 12. 0 Cai 1.90 9 3649.094r 4 1. 5

3645.082r

3645.186r

3645.313

3645.413r

1. ) :.

97

7

132

32

26. 4

2. 1

35. 8

11. 7

Fe I

Co I

Sc II |Dy II La II

r2.85 13.02

1.96

0.02

0.10 0.00

323

495

61

2

14

7

3649. 184r

3649. 298r

3649. 336r 3649.511m

3649. 698r

13

] 124

134

44

5. 2

f 29. 9

1 24. 4

45. 7

16. 2

Fei

Co I Fe I Fe I p

0.00

2.87

2.69

2.94

5

146

291

391

3645.497r 90 24. 4 Fe I f2.86 3.00

[3.02

323

391

441

3649.837r

3650.037

75

115

26. 7

39. 2 Fe I 3.00 394

3645.626r 3645.827m

3645.935r

3645.989r

3646.097r

3646.196r

8

103

20

2. 5

23

52

2. 2

28. 0

6. 6

0. 7

6. 4

14. 0

Fe I Vii

Fe I p

Ti I

1 (Gdii)

3.11

2.38

2.87

0.00 0.24

496

76

324

18

2

3650.17 a

3650.285m

36^0 tjyjtjyj .o\j 3fi7r1

1

3650.538S

3650.720r

3650.887r

13

115

16

72

9

10

5. 5

39. 3

5. 9

25. 5

3. 3

3. 7

La II Smii

Fe I Cr II -Fe I

Zr II

0.00

0.25

2.43

4.98

3.25

3.12

1225

180

156

146

78
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3651.039r 20 11. 0 Fe I 3.21 571 3655.472m 88 31. 2 Fe I 2.83 369

Sfi.'il 107r

3651. 197r

3651.260r

98

31

16

33. 8

15. 3

8. 0

Fe I —

Nb II Co I

/2.85

13.30

0.93

2.04

322

674

4

85

3655.580r

3655.661

3655.851r

12

100

15

6. 6

36. 4

5. 9

Zr II (Fei)

|Ce II- Cri

0.97

0.32 2.54

71

5146

3651.353r 6. 5 2. 7 3655.941r 3. 5 1. 4 3651.474m 136 46. 6 Fe I 2.76 295 3656.078r 3 1. 2

3651. 654r

3651. 800r

80

114

28. 0

39. 1

Nil

Cr II

So II

3.65

2.42

0.01

153

1

2

3656.219r

3656. 265r j 116

f 31. 2

1 17. 8

Fc I Cri3.27 /2.54

12.54 46

46

3651. 921r

3652. 107r

3652. 260r

3652.397r 3652.551m

3652. 680r

3652.883r

3653.020r

3653. 120r

3653.200r

64

10

27

7

70

2. 5

1

9. 5

7. 5

3. 5

25. 6

3. 8

10. 4

2. 7

25. 6

1. 0

0. 4

3. 7

3. 0

1. 4

Fe ICH

Fe II? Fe I

Co I

Ce II

Q 6

3.02

0.17

0.36

1,0

494

4

38

3 3656.357r

3656.548r

3656.705r

3656. 858r

3656.965r

3657.137

3657.298r

3657.423r

3657. 571r

3657.711r

36

13

2. 5

1

33

72

4. 5

48

5. 5

57

13. 7

4. 9

1. 0

0. 3

12. 6

26. 0

1. 6

17. 9

2. 2

21. 2

Fe I p

Ni I? Vi

Co I Fe I Mn II? Fei

Ru II Nil

|Fei

2.87

3.65

2.05

0.58

2.42

2.40

3.94

323

115

21

130

1

183

3653.352r

3653.501m

3653.659r

3653.761

44

98

8

66

16. 6

33. 6

3. 0

23. 6

Fe I

Ti I Ce II Fe I

/2.59

12.86

0.05

0.47

2.43

229

324

19 50

180

3657.818r

3657.905r

3658.024r

3658.099r

5

102

40

71

2. 2

35. 4

21. 0

25. 8

Fe I Fei

Til

3.04

3.02

0.02

395

438

19

3653.912r

3653.979r 102

1

1 20. 2

1[ 20.2

Cr I Fe I

2.54 47

3658. 167r

3658.274r

8

4. 5

3. 6

1. 8

Cr II

Vii

14.93

2.51

146

116

3654. 126r 5 1. 9 3658.390r 3 1. 1

3654.252r 3. 5 1. 4 3658.550r 50 18. 3 Fe I 2.56 231

3654.386r 13 5. 7 CH P 4 1,0 3 3658.644r 1. 5 0. 7

3654. 446r 25 9. 6 Co I 1.96 63 3658.864r 3 1. 2 Tb II?

3654.598r

3654. 673r

3654. 859r

64

35

4

23. 5

17. 8

1. 5

Ti I (Gd ii) Fe I0.00

0.08

2.22

184

77

3658.970r

3659. 124r

3659.234r

0. 5

1. 5

10

0. 3

0. 7

3. 8

Fe II? Fe I Ce II Fe I 0.17 54

3655.003r 50 18. 6 Fe I 3659.310r 7 2. 7

3655.059r 12 4. 6 3659.524m 98 34. 2 Fe I 2.45 ISO

3655.219r 33 12. 3 3659.762 103 35. 8 Ti 11 1.58 75

3655.355r 40 14. 91 Fe I 2.42 131 3659.877r 5 2. 3

79
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3659.971r 9. 5 3. 7 3663.831r 16 5. 9

3660.08 a 5 1. 8 3663.967r 65 25. 6 Fe I 2.95 435

3660.21 Ir 40 15. 2 3664.097 130 43. 8 Nil 0.27 4

3660.329r

3660.41 Ir

60

32

22. 0

13. 1

Fe I Fei2.86

2.61

323

229

3664.211r

3664.238r

1

1 48

1 20. 7

I 4. 9

Sc II? 0.31 10

3660.525r 9. 5 3. 6 3664.411r 16 5. 9

3660.636r 51 18. 9 Ti I 0.02 18 3664.540r 103 35. 0 Fe I 3.00 391

3660.778r 50 18. 4 3664.623r 68 3L 4 Y II 0.18 9

3660.921r 9 3. 3 Zrii 0.76 32 3664.701r 63 33. 8 Fe I 3.00 390

3661.038r 28 10. 4 CH P5 1,0 3 3664.828r 35 13. 0 CH Q 8 1,0 3

3661.151r 5. 5 2. 0 Fe II p 4.15 111 3664. 945r 29 11. 3 Cr II 4.99 156

3661. 258r 14 5. 3 Fe I p 3.69 952 3665.028r 37 13. 9 -CH Q 8 1,0 3

3661.372m 64 22. 6 Sm II Fe IVii

0.04

2.45

3.33

6 179

191

3665. 188r

3665.304r

12

7. 5

4. 6

2. 9

Nd II

3661. 537r 5. 5 2. 0 3665.437r 9. 5 3. 5 Cri 2.54 48

3661.637r 6 2. 3 3665.594r 4 1. 5

3661.737r 11 4. 4 3665. 724r 29 10. 4

3661.837r 5 1. 9 3665.850r 17 6. 3 Fe I

3661.957

3662.10 a

3662. 170r

70

5. 5

59

25. 4

2. 2

28. 2

Ni I La II Co I (Zr II)

0.21

0.13

2.28

1.66

16

12

115

101

3665.997r

3666. 064r

3666. 164r

34

105

11

6. 9

35. 8

5. 2

Cn

Fe I Cri

/2.54

12.54

2.54

48

48

46

3662.240r

3662.364r

94

17

32. 8

6. 8

Ti II Cri

1.57

2.54

75

46

3666.250r

3666.284r 1 105

1 24. 8

1 19. 4

Fe I Fe I p

/2.43

\2.94 3.30

179 389

672

3662.470r

3662.624r

3662.737r

3662.841

8

17

30

1 96

3. 2

6. 6

11. 8

r 33. 2

Fe I p Cri

Fe I

3.02

2.54

490

46

3666.367r

3666.539r

3666.644r

3666.770r

14

83

26

75

5. 8

29. 3

11. 3

26. 4

Sc II Cn

Fe I

0.02

2.54

2

46

3662.897r

3663.0l7r

3663.070r

3663.208r

3663.264r

ODOO.'4:U-±l

3663.459r

3663.598r

3663.698r

9. 5

4. 5

1 100

1I 116

10

40

I 0. 3

3. 6

1. 9

1 18. e

1 22. £

r iQ

1 21. i

4. ^

15. ^

i

t

Fe I p —

Sm II

Cr I Fe I

Fe I Vi

Zr I2.95

0.38

2.54

2.99

/2.56

12.59 2.03

0.15

436

39

46

439

229

231

114

12

3666.849r

3666.931r

3667.097r

3667.14 a 3667.261m

3667.424r

3667.604r

3667.750r

3667.877r

16

92

8. 5

4

103

8. 5

7. 5

15

5. 5

8. 0

31. 6

3. 2

1. 9

35. 2

3. 3

2. 9

5. 5

2. 2

Fe I -Fe I

Zr IIFe I

Zr II

V I

3.04

1.61

0.41

3.21

0.71

2.04

393

46

8

570

32

114

80
The Solar Spectrum—Continued

Wavelength

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot.

Li 116

RMT

No.

or Vib. Notes

3667.996 89 31. 0 Fe I (Ce II)

/2.99

\3.21 0.36

438

569

40

3668.217r 82 29. 4 |Fei

Nil

3.24

3.94 568182

3668.354r 5 1. 9

3668.460r

3668.497r

> 53

1 11. 2

1 11. 2

Zr II Yii0.41

3.52

9

46

3668.659r 35 13. 2

3668.770r 6 2. 2

3668.891r 47 20. 6 Fe I 2.59 229

3668.969r 65 23. 0 Ti I 0.02 18

3669.155r 78 35. 7 Fe I 2.99 437

3669.244r 103 35. 0 Ni I 0.17 2

3669.406r 40 18. 0 Vii 2.52 116 3669.526m 120 40. 5 Fe I 2.73 291

J. O. 1 Fg I p

3669.839r 24 9. 1 Mn I 2.14 7

3670.03 2r

[ 143

f 29. 4 Fe I (Co I) 2.84

2.01 369

64

3670.104r 1 [ 24.5 Fe I 2.95 435

3670.220r 4. 5 1. 6 Fe I p 1.61 47

3670.310r 18 7. 2

3670.431 120 40. 6 Ni I 0.17 4

3670.542r 37 17. 0 Mn I 2.11 7

3670.650r

3670.724r

i 52

J

r 1-1

L 17. 7

Sm II?

3670.817r 86 30. 0 ||Fe ISm II 2.48

0.10 13311

3670.910r 13 4. 9

3671. 090r 4. 5 1. 6

3671. 222r 8 3. 1 V I Gd II 1.35 0.08 70

2

3671.276r 37 13. 9 Zr II 0.71 45

3671.370r 3 1. 1

3671.524r 43 15. 8 Fe I 3.26 570

3671.682m 67 23. 8 Til 0.05 19

3671. 857r 2 0. 8

3671.947r 10 3. 8

3672.124r 16 6. 0 Fe I

3672. 316r 10 3. 8 Dy II 0.59

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3672. 465r 22 8. 3

3672.606r 6 2. 2 Zr II? 0.09 1

3672.712S 68 24. 0 Fe I 2.45 180

3672.803r 5 1. 9 Ce II 0.90 233

3672.913r 1. 5 0. 5

3673.046r

3673.087

97

J

0. 3

32. 7 Fe I —

3673. 226r 44 17. 2 — CH Q 9 1,0 3

3673.426r 40 14. 9 V I —

Cai

2.05

2.52 11428

3673. 543r 9 3. 4 Nd II

3673. 683r 31 10. 4 Fe I 3.88 978

tjyj i o . 1 t Oi 53 19. 8 Fe II ?p 1 "^1 ±o ± O ^ o o o o 3673.888 63 22. 4 Fe I

3674.062

1 178

f 33. 0 Fe I |Nii 0.03 15

3674.150 [ 33. 0 Nil 0.42 32

3674.316r 8 3. 0

3674.413 58 20. 6 Fe I

3674.563r 8. 5 3. 1

3674.729r

3674.773r

1

1 106

f 16. 6

1 26. 8

Zr II Fe I0.32

2.83

9

369

3674.923r 2. 5 1. 1 Cr II 2.48 1

3674.999r 11 4. 1 In? 1.62

3675.119r 2 0. 8 Mgi?p 6.98

3675.18 a 3 1. 1

3675.294r 42 15. 6 Cai 2.52 28

3675.449r 25 9. 5 Fe I 2.61 229

3675.556r 2. 5 0. 9

3675.689r 38 14. 0 Vi 0.28 29

3675.766r , 24 9. 0 Fe I 3.88 996

3675. 882r 1. 5 0. 7

3675.976r 18 6. 8 Fe I?

3676.155r 6. 5 2. 4 3676.322m 102 34. 7 Fe I 2.56 228

3676.562r 66 23. 2 Co I 2.87 145

3676.700r 6 2. 2 Vi 2.12 115

3676.814r 16 8. 2

3676.878 73 25. 6 Fe I 3.00 389

81
The Solar Spectrum—Continued

WaveICii^ til

kA)

Equivalent Width

AX

(.mA;

Re- duced

Width

AX/X

\i)

Spot

Solar

Identification

Low

E P

or Rot. LinG

RMT

No.

or Vib. Band

^r\f pet Wave1 pn crt.Vi

KA)

Equivalent Width

AX

(.mA;

Re- duced

Width

AX/X

Spot

Solar

fication

Low

E P

or Rot. Line

RMT

No.

or Vib.

1>I O bcH

3676.962r 13 4. 8 Mn I 4.66 3681.653m 72 25. 6 Fe I 3.00 390

3677.095r 4. 5 1. 6 3681.884r 30 11. 1 Fe I 3.69 951

3677.172r 2 0. 7 3682.024r 15 6. 8 Mn I? 4.68 3677.318m

3677.462r

3677.514r

3677.628r

3677. 695r

3677.855r

3677.909r

3678. lOOr

3678.234r

3678.355r

3678.455r

93

85

32

147

48

98

88

35

67

7. 5

3. 5

29. 2

29. 4

26. 4

48. 9

34. 4

38. 5

51. 8

12. 9

23. 6

2. 8

1. 2

Fe I Fe I Fe I Fe I Cr II Cr II Fe I |Cr II CH

Cai

3.55

2.28

3.30

2.76

2.70

2.71

2.71 P 7

2.52

773

125

666

291

12

12

12

1,0

28

3

3682.173r

3682.245r

3682.524r

3682.670r

3682.884r

3683.045r

3683.092

3683. 377r

3683. 480r

3683.623

1 202

47

44

5

1 166

4. 5

10

52

j 31. 2

[ 45. 6

16. 8

15. 8

1. 8

f 29.2

1 37. 0

1. 9

3. 9

18. 5

Fe I p Fe I

Fe ii?pCoi

IIFeiVi

Pb I

Fe I

/2.94

\3.00

3.55

4.48

2.08

0.05

0.27

0.97

12.48 13.30

386

385

772

131

99

5 29

1

130

671

3678.582r 0. 5 0. 1 3683.756r 2 0. 8 Fe I p 3.93 996

3678.728r 3 1. 1 Mn 11 3683.882r 6. 5 2. 7 3678.869m

3679.002

tj\J t ij . X X Ail

3679.539

89

64

26

35

29

30. 7

22. 6

11. 0

13. 9

13. 2

Fe I (Zr II) Fe I

Fe I

Fe I

2.42

1.76

2.28

2.56

/3 00

13!07

131

101

124

228

393 490

3683.968r 3684.123m

3684.222r

3684.322r

3684.462r

3684. 542r

6. 5

129

8. 5

10

11

38

2. 4

43. 2

4. 1

3. 8

4. 9

14. 1

Fe I Cr II Vi?

Co I Fe I

2.73

4.94

2.05

2.08

3.25

292

145

114

99

3679.685r 43 24. 7 Ti II 1..58 75 3684.720r 8. 5 3. 0

3679.811r 22 21. 2 Cr I 2.54 48 3684.862r 25 9. 5 3679.923m

3680. 211r

448

)

4. 5

6. 5

jl40

I 8. 8

3. 9

3. 8

Fe I

VV TX

Cr I

0.00

2.07

12.54 \2!54

5

114

48

48

3685.002r

3685.196m

3685.527r

3685.662r

30

275

56

11

15. 0

84. 7

20. 4

4. 1

Ti II

Cr I Fe I p

/0.57

io.61

2.54

2.61

14

14

44

231

3680.389r 52 21. 2 Fe I 3685.775r 15 5. 7 -Ndii

3680. 505r 4 1. 8 3685.888r 7. 5 3. 7

3680.665r 70 30. 3 Fe I 3.21 568 3686.004 151 50. 0 Fe I 2.94 385

3680.802m 128 44. 6 Fe I 3686. 108r 18 9. 2

3680.944r

3681. 117r 3681.230m

66

7

59

23. 8

2. 7

21. 0

Fe I Ni I Fe I

1.93

3.30

3686. 188r

3686.263m

7

85

3. 7

32. 0

Cr I

Fe I (Vi)

/2.54

\2.54

2.42

1.38

44

44

1 O 1 loi70

3681. 364r 4. 5 1. 9 Co II 3686.381r 7 2. 8

3681. 467r 3. 5 1. 3 3686.472r 7. 5 2. 8 Co I 2.63 134

82
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

A\

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3686.674r 22 8. 7 Cr II 4.78 118 3690.459 63 21. 8 Fei r3.ii 13.28 497

570

3686.787r 44 18. 2 Cr I /2.54

12.54 44

44 3690.593r 3. 5 1. 2

3686.871r

3686.944r 3687.102m

3687.241r

3687.334r

13

0. 5

73

14

13

6. 6

0. 3

33. 0

14. 0

33. 1

be I Cri

CriITii

2.18

2.54

2.54 0.05

75

44

44

19

3690.731m

3690.8G0r

3690.973r

3691. 176r

3691.314

86

2. 5

10

8. 5

50

29. 5

0. 8

3. 8

3. 0

18. 4

Fe I (Coi)

Fe I Fe I

3.57

2.04

2. 01

807

86

229

3687.466m

3687.551r 3687.660m

3687.760r

3687.866r

3687.986r

3688.071r

3688. 173r

3688.286r

3688.419r

3688.478r

3688.63 a

3688.680r

3688.804r

3688.874r

3689.002r

3689.080r

3689.206r

3689.320r

3689.374r

3689.469m

3689.630r

3689.7001-

3689.880r

3689.914r

3690.066r

564

3. 5

59

2. 5

16

1. 5

32

47

2

1

134

2. 5

3. 5

72

27

52

40

1

1 68

158

9. 5

7. 5

79

J

15

182

9. 8

41. 7

1. 6

7. 6

0. 7

13. 3

19. 0

0. 9

r 29. 5

I 23. 8

0. 8

1. 4

24. 6

14. 9

18. 2

19. 5

0. 4 r[ 26. 6

51. 0

4. 1

2. 8

f 10. 0

1 21. 6

5. 6

Fe I (Vi)

Cri

Fe I Gd II CH

Nb II? Vi

Fe I Mo II

llNi I Eu II Fei

Fe I Fei

Fe I

Ni I? Cri

Fe I p

Fei

Cri?

Fe I Til

Ru II —

Fei

0.86

2.10

2.54

2.73

0.35 P8

2.16

0.29

3.30

3.11

0.27 0.00

3.25

2.45

2.43

3.68

2.54

3.04

/2.84

\2.94

3.43

3.05

0.05

2.40

2.59

21 114

44

291

20

1,0

29

5

52

669

179

178

17348

391

3G9

386

216

533

18

1 231

3

3691.395r

3691. 535r

3691. 686r

3691.816r

3691.963r

3692.113r

3692.226r

3692.360r

3692.440r

3692.570r 3692.650m

3692.816r

3692.886r

3693.032r

3693. 120r

3693.246r

3693.366r

3693.478r

3693.666r

3693.783r

3693.940r

3694.027r 3694.199m

3694.436m

3694.654r

3694.817r

3694.904r

4

4. 5

2

0. 5

3

4. 5

40

6

2

4. 5

47

11

0. 5

86

35

8. 5

26

61

36

24

24

272

67

38T

24

2

1. 6

1. 8

0. 8

0. 3

1. 1

1. 6

14. 9

2. 2

0. 8

2. 1

16. 8

4. 1

0. 3

29. 2

17. 9

3. 1

9. 7

21. 9

15. 0

11. 0

21. 4

90. 0

25. 6

14. 9

0. 5

9. 2

0. 8

Fe I p

Fe II?

Vi

Rh I 0 I?

Zr II? Fe I (Mo II) Mn I

Fe I Co I

Coi

Coi

Mn I

Fe I p

Nil

(Sm 11

)

Fe I Yb II -Til

Dy II Ce II

3.43

0.28

0.00

9.52

0.96

3.06

2.16

3.02

2.08

2.01

2.04

4.23

/1.56

\3.07

0.11 0.00

3.04

0.00

1.44

0.10

0.30

707

29

1

6

56

5

7

439

97

64

95

46 490

15

2

394

1

117

63

3690.281r 39 14. 3 Vi 0.26 29 3695.056S 98 33. 5 Fei 3.05 534a

83
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

xte- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

TP A/TT' No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

rte- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

xtiVl i No.

or Vib. Band

Notes

3695.207r

3695.342r

2. 5

27

1. 1

10. 1

10, o

Vi 2.12

/2.56

13.42

114

225

707

3699.740r

3699.825r

3699.925r

3

32

1. 5

1. 1

12. 0

0. 5

Gdii

Hf II Fe I Fe II p

0.35

1.67

4.49

20

18

131

3695.652r 55 19. 8 Fe I 3700.045r 7. 5 3. 0 Ti I

3695.869r 42 16. 2 Vi 0.27 29 3700.132r 8 3. 0 Vii 2.49 102

3696.038r

3696.153r

37

9. 5

14. 0

3. 8

Fe I 2.42 128 3700.269r

3700.342r 1 -

J

J" 2. 3

[ 10. 5

Tmii

Vii

0.03

2.51

6

116

3696.296r 24 9. 3 Nil 1.93 74 3700.459r 4 1. 5

3696.383r 46 18. 7 Ti 11 1.57 73 3700.600r 28 10. 5 Fei 3.24 569

3696.523r

3696.570r 1 53

1 17. 6

I 15. 4

Fei

Mn I

3.05

2.89

530

24

3700. 739r

3700.805r

5

4. 5

1. 9

1. 6 Fei?

3696.663r

3696.753r

3696.812r

12

6. 5

18

6. 1

4. 6

7. 0

Ni I

Fe I p Cr II?

1.93

3.02

74

434

3700.915r

3700.995r 3701.095m

/ loO

( 0. 8

0. 8

, 59. 8

CN?

Rhi?

Vii

Fei

R 111

0.19

2.49

3.00

1,12

102

385

11

3696.911r 34 13. 9 Nil 3.68 172 3701.272r 11 4. 9

3697.07 a 3. 5 1. 6 3701.375r 9 3. 5 Tm II 0.00 2

3697.15 217 69. 0 ^17 10.20 3 10 3701. 535r 5. 5 2. 2

3697.16 a 2 0. 9 3701. 612r 3 1. 1 Nil? 3.54 138

3697.261r 5 2. 3 3701. 729r 20 7. 8 Mn I 2.14 7

3697.433

3697.537

3697.747r

3697.871r

101

82

8. 5

1

40. 0

30. 8

3. 5

0. 4

Fe I (Zr II) Fe I Gd II Nbi?3.00 0.47

3.30

0.03

0.05

389

7

670

4

3

3701. 869r 3702.037m

3702.245r

3702.272r

1

68

1 69

0. 4

26. 2

[ 16. 0

[ 16. 0

Cr II? Fe I Co I -Til

5.32

2.84

2.88

1.05

168

369

145

83

3698.017r

3698.167r

3698.327r

3698.477r 3698.609m

3698.694r

3698.804r

3699.017r

3699.144

37

52

1

19

75

13

1. 5

26

69

14. 4

20. 3

0. 4

7. 3

26. 7

6. 8

0. 6

9. 7

24. 8

Cr II- Fei

Zr II (Til)

CN?

-CH

Fei

CH

Co I Fei

4.77

2.20

1.01 2.25 R 113 P 9

3.02 P 9

2.87

3.02

118

75

71 222

0,0

1,0

491

1,0

145

490

11

3

3

3702.493

3702.645r

3702.825r

3702.961r

3703.00 a

3703. 104r

3703. 231r

3703.448r

3703. 545r

77

1. 5

3. 5

10

1. 5

1

5

14

1 114

27. 6

0. 5

1. 5

4. 3

0. 7

0. 5

2. 0

5. 9

1 28. 6

Fei

CNTb II? CN?

Fe I p

Fe I

/1.61

12.18

R 111

R 110

3.37

/2.76

12.76

46

75

0,0

1,1

704

291 292

11

11

3699 277r 1. 5 0. 7 3703. 591r [ 22. 7 Vi 0.30 29

3699.396r 5. 5 2. 2 Fe I p 3.93 996 3703. 696r 62 28. 1 Fe I 2.94 389

-3699. 573r 2 0. 7 Fe I p 3.02 436 3703.829m 78 30. 2 Fei

(Vn)

2.86

1.56 36915

84
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(raA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3703.86 235 76. 5 Hl6 10.20 3 10 3707.826m 88 30. 2 Fe I 0.09 5

3703.94 a 1. 5 0. 7 3707.929m 114 50. 5 Fei 2.18 76

3704.038r

3704.083r 1 103

1 20. 5

I 26. 8

Fe I Co I3.07

1.05

495

35

3708.085r

3708.188r

40

16

16. 5

6. 3 Fe I p 2..59 228

3704.203r 4 1. 6 Fe I 3708.315r 3 1. 1

3704.297r

3704.347r 3704.469m

1

[ 50

98

f 5. 9

J

1 15. 7

35. 4

Til Fe I Fe I1.46

3.24

2.69

117

609

290

3708.435r

3708.611m

3

53

1. 1

21. 8

Sm II Fe I p

Fe I

0.04

2.99

/2.45

12.59

5 436

178 225

3704.58 a 8 3. 5 3708.695r 3 1. 4 -Vi? 1.89 104

3704.704 46 18. 0 Vi 0.29 29 3708.825r 45 21. 8 Co I 2.04 98

3704.797r 5. 5 2. 4 Fe I p 3.69 950 3709.031r 60 40. 0 Fe I p 3.04 390

3704.913r

3705.033r

3705. 113r

3705.263r

3705.423r 3705.577m

3705.709

3705.830r

3705.937r

3706.037r

3

33

7

9

6

562

44

14

6. 5

290

1. 4

15. 3

3. 6

5. 8

10. 5

180

48. 3

13. 6

10. 5

105

CN?

Vi

Nil

Fe I p

Fe I

Fe I p

Ca II (Mm)

/R 109 IR 109

0.28

0.42

3.40

0.05

/2.76

13.27

3.12

4.25

1,11 2,2/

29

30

704

5

293 610

3

11 3709. 151r 3709.256m

3709.401r 3709.537m

3709.670m

3709.828r 3709.953m

3710.075r

3710.165r

3710.292S

7. 5

573

8

55

56

3. 5

39

7. 5

6

74

15. 4

186

13. 0

33. 2

26. 0

1. 6

16. 1

3. 2

2. 7

27. 2

Fe I (Zr II) (Ce II) -CN

Fe I Fei

Ce 11-

|Tii

Cr I?

Yii

0.91 0.80

0.52 R 108

2.99

2.56

0.12

1.05

4.45

0.18

2145

40

0,0 435

225

40

83

7

11

3706.220m 70 37. 2 Ti II 1.57 73 3710.448r 23 9. 3

3706.337r 9. 5 4. 9 3710.638r 27 10. 8

3706.483r 1. 5 0. 7 3710.741r 1. 5 0. 7

3706.563r

3706.697r

3706.77 a

3706.882r

1. 5

10

1. 5

12

0. 7

4. 2

0. 5

5. 1

Sm II CN?

0.48 R 10847

1,1 11

3710.881r

3711. 115r 3711.229m

3711.301r

6

7. 5

83

12

2. 6

3. 2

32. 0

7. 0

Sm II? CN?

Vii

Fe I Fe I p

0.18 R 106

2.49

2.59

2.20

19

1 1

102

228

75

11

3707.052m 121 41. 5 Fe I /3.00

13.00 385

392 3711.412m 66 29. 6 Fe I 3.07 494

3707.176r

3707.329r

3707.465

3707.562

3707.676r

10

78

66

83

12

4. 7

27. 6

25. 4

29. 2

5. 5

Sm II?- CN

-Fe I Co I Fe I

Ti IFe I

0.33 R 109

3.02

2.04

2.56

2.02 3.88

35

0,0

437

96 229

177 978

11 3711.535r

3711.665r

3711.784r

3711.940r

3711.97

6. 5

10

3. 5

24

333

3. 0

4. 3

1. 6

10. 6

108

Sm II CoiCN

CN

Vii

Fe I p —

Fe II? ^15

0.25

2.01 /R 107 IR 106 R 106

2.52

2.45

5.91 10.20

25

63

0,0\

2,2/

2,2 116

178

192

3

11

11

10

85
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3712.090r

3712. 180r

19

11

8. 5

4. 9 Co I 2.04 84

3716.84 a 1. 5 0. 7 CN

CN

R 103

/"r> T AO IK 103 IR 103

1,1

2,1}

11

11

3712.304r 1. 5 0. 8 3716.945r 2 0. 8 CN? R 103 2,2 11

3712.400r 8. 5 3. 8 Fe II p 2.28 15 3717. 072r 3 1. 2 Nb II 1.69

3712.527r 2 0. 9 Vii? 2.76 157 3717. 187r 9. 5 4. 3 Fe I p 3.33 704

3712.717r 9 4. 2 Gdii 0.38 20 3717.271r 2. 5 1. 1 Ti I 1.46 116

3712.767r 6 2. 6 Sm 11 0.25 25 3717.397m 48 19. 9 Til 0.00 17

3712.898

3712.943 |iii

f 20.8

I 30.2

Cr II Cr n2.71

2.71

12

12

3717. 557r

3717. 673r

0. 5

1

0. 3

0. 4

3713. lOOr 4 1. 6 3717.733r 7 3. 2 Fe I p 3.88 997

3713.207r 0. 5 0. 1 3717. S36r 28 11. 6 Fe I p 3.42 706

3713.340r 14 5. 7 Nil 1.95 74 3717. 954r 8 3. 4

3713.554r 7. 5 3. 0 La II 0.17 26 3718.152r 38 16. 5 V II 1.68 21

3713.714r

3713.834r

3713.970r

3714.157r

3714.220r

3714.30 a

3714.407r

3714.567r

22

2. 5

2

0. 5

1. 5

2

3

2. 5

8. 8

1. 0

0. 8

0. 3

0. 5

0. 8

1. 2

1. 1

Ni ITi I CN

Vi

Zr I

Yii

Cr I?

1.95

1.43 R 106

0.07

0.15

3.62

3.89

74

116

0,0

11

12

61

269

11

3718.228r

3718.321r 3718.412m

3718.526r

3718. 615r

o7io.7Ubr

3718. 9olr

12

15

77

4

10

1

7

32

6. 5

7. 0

32. 0

2. 3

5. 4

0. 5

4. 0

t '~f A 17. 4

CN

Fe I

CN

Zr II

TVMnT« »I Pd I

R 104

2.76

R 102 R 102

0.36

4.26

1.25

0,0

292

2,2

2,2

9

3

11

11

11

3714.674r 6 2. 4 3719.028r 8. 5 5. 6

3714.787r 28 11. 0 Zr II 0.53 18 3719. 192r 8 6. 7

3714.930r 1 0. 5 3719. 265r 3. 5 3. 9 Hf II 0.61 7

3715.040r 3 1. 2 3719.458r 7 15. 3 Nil 3.70

3715. 180r 58 22. 2 Cr II 3.10 20 3719.543r 6. 5 2. 3

3715.397r

3715.476r

1

I 105

f 5. 4

1 34. 0

Ti I? Vii 1.57 15

3710. 656r

3719.765r

11

1

3. 6

0. 8

3715.714r 7. 5 3. 2 3719.947m 1664 538 Fe I 0.00 5

3715.799r 3. 5 1. 5 Ti I 1.44 116 3720.165r 1. 5 1. 1 Fe II p 2.54 23

3715.916m 80 29. 4 Fe I 2.28 124 3720.260r 11 3. 6 Zr II? p 0.76 32

3716.05 a

3716.154r

3716.378r 3716.451m

3716.538r

6. 5

28

\ 166

2. 8

11. 5

r 2.

2

{ 56. 0

[ 1.6

CN

CN

Ce II (Gd II) Fe I Cr I

R 105 R 105

0.00

0.03 /2.94

13.37 3.89

0,0

0,0

40

2 388

705

269

11

11 3720.404r

3720.48 a

3720.564r

3720.692r

10

10

11

4

21. 2

10. 5

12. 5

4. 2

CN

Til

CN

/R 103 IR 101

2.04 (K 103 IR 101

0,0

2,2 177

0,0

2,2

}"

1"

3716.699r 3. 5 1. 6 Fe I p 2.99 434 3720.790r 1. 5 1. 3 CN R 101 1,1 11

86
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3720. 907r 3 2. 4 3725.837r 6 2. 4

3721.030r

1 0. 3

I Ni I p 3.83 181 3725.95 a 5 2. 0 Cr I?

3721.071r \ 0.1 3726.023r 14 5. 4 Nil 3.84

3721. 185r 58 40. 0 Fe I 3.02 491 3726.065r 3. 5 1. 3 Fe I p 2.95 433

3721.277r

3721.399r

3721.506r 3721.635m

3721. 930r

3721.94

45

41

53

110

66

(536)

27. 6

25. 1

32. 5

55. 8

39. 2

(176)

Fe I

Fe I Fe I

|Ti II Fe I Fe I

/2.18

\3.33

2.48

3.04

0.57 3.02

10.20

75 705

131

389

13 437

3 10

3726.23 a

3726.36 a

3726.48 a

3726.665r

3726.842r

3726.920r

0. 5

2

2

37

9. 5

202

0. 2

0. 7

0. 8

14. 5

5. 6

70. 3

Nbi?

CN?

Go I -CN

lire I Ru I

0.02

1.71 R 98

3.04

0.15

3

40

385

2

11

3722.028m 42 28. 8 Fe I 2.76 291 3727.026r 36 30. 8 Fe I p 3.27 668

3722. 139r 4 4. 2 Vii 1.55 15 3727.098m 118 55. 1 Fe I 2.94 387

3722.236r 36 28. 1 Fe I p

/2.42

\3.07 127 490

3727.347r 59 37. 0 Vii

(Cr II) 1.69 4.78 21 117

3722. 377r 4 6. 4 3727.449r 1 1. 9

3722.498r 22 54. 8 Nil 0.21 18 3727.531r 8. 5 26. 8 Fe I p 3.42 705

3722. 588r

3722.758r

3723. 284r

3723.392r

3723.510r

3723.609r

3723. oSor

3723. 844r

3723.912r

3724. 092r

694

8

7

9. 5

10

47

5

41

16

43

249

14. 8

3. 9

5. 0

5. 4

20. 8

2. 7

17. 6

8. 1

17. 6

Til

IIFei Fe I p

(Sbi)

Cr n

Ndii

Ti II?

Fe II p — Ti II

0.02 0.09

3.42

2.03

4.94

1.57

2.28

1.58

17

5

707

1

144

72

14

73

3727.634m

3727.685r

3727.818m

3728.042r

3728.137r

3728.332r

3728.402r

3728.48 a

3728.671r

3728.862r

632

14

85

40

12

30

5. 5

5

73

5. 5

205

112

73. 8

20. 0

5. 9

12. 6

2. 4

2. 3

26. 0

2. 6

Fe I |FeipZr II Fe I Ru I Nd II Vii

-Ce II Sm II Fe I |Coi- Mn I

0.96

2.59

1.74

3.00

0.00

2.51

0.68

0.66

2.56

2.63 2.92

21

225

112

386

2

116

47

54

227

13324

3724. 258r 6 3. 0 Ni I p 3.94 183 3728.954r 80 28. 1 Ni I —

Fe I CN

3.84 181 3724.385m

3724.574m

124

60

44. 6

23. 1

Fei

Til

2.28

1.50

124

131 3729.072r 7. 5 2. 7 /R 99 IR 96

0,0

2,2 }"

3724. 743r

3724. 829r

3724. 949r 3725.158m

3725.306r

3725.496S

3725.665r

8

52

19

42

12

67

7

3. 5

20. 2

7. 7

16. 5

4. 6

24. 6

2. 7

CN

Nil

Eu II Til Fe II Fe I Fe I p

/R 101 IR 99

3.83

0.00

1.07

4.48

3.05

2.22

0,0

1,1

182

2

83

130

534

75

3729.18 a

3729.339r

3729.524r

3729.723r 3729.813m

3730.012r

3730.141r

3

10

6

7

83

22

1. 5

2. 4

4. 0

2. 4

2. 7

39. 4

8. 4

0. 7

CN?

Fe I p

Zr II

Ti I CN?

R 99

3.05

0.47

0.00

0,0 530

8

17

11

87
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3730.308r 38 21. 7 3734.664r 1 8. 8

3730.392r 118 41. 8 Fe I 3.05 533 3734.874m 3027 945 Fe I 0.86 21

3730.483r

3730.590r

3730.756r

3730.808r 3730.950m

3731. 159r

102

15

1 106

87

14

37. 0

7. 0

1 23. 6

I 22. 6

33. 2

6. 4

Co I (Feip)

CN

Nil

Cr I Fe I Fe I p

1.88 3.00 R 96

0.27

0.00

2.61

3.69

62 389

1,1

2

2

228

950

11

3735. 118r

3735.244r 3735.334m

3735.444r

3735.551r

3735.700r

6. 5

14

69

8

5

15

42. 8

56. 0

81. 3

11. 4

6. 0

10. 6

Fe I CN

Ndii?

Ti I?-

Fe I p

2.94 R 96

2.42

388

0,0

127

11

3731.261r 31 13. 7 Sm II

II Zr II (Co I)

0.10

1.74 2.04

11 112963735.898r

3735.964r

27

22

21. 4

18. 0

Coi

Sm II

2.08

0.28

95

29 3731.381m

3731.621r

3731.727r

3731.814r

3731.930r

3732.035r

3732.142r

3732.214r 3732.406m

80

12

8

1. 5

22

54

3

7

142

32. 0

5. 8

4. 0

0. 8

10. 2

24. 0

1. 7

3. 7

58. 9

Fe I

CN?

CN?

Mn I Cr I

|Fe I Co I

2.61

4.27

0.00

2.20

1.88

225

2

76

62

3736.044r

3736.291r

3736.476r

3736.592r

3736.712r

3736.816r

3736.917r

3737.032r 3737.141m

3. 5

1

6. 5

11

12

39

290

10

1071

3. 9

1. 2

7. 6

17. 7

29. 2

95. 9

261

67. 0 428

CN

Vii

CN

Nil

Ca II

Fe I

R92

2.52

R 93

0.42

3.15

0.05

2,2 102

1,1

30

3

5

11

11

6 i oZ. Do4r

3732.752r

i 1

64

D. 4

32. 4

V_/JN —

Vii

/R 95 \R 94

1.56

1,1 2,2

15

111 3737.299r

3737.576r

4. 5

78

31. 6

87. 0 Cr u?-

CN

4.77 R 95

117

0,0 11

3732.885r 3. 5 2. 4 CN? 3737.758r 6 6. 1 CN? R 91 2,2 11

3732.985r 4 3. 2 CN? 3737.884r 0. 5 0. 5

3733.079r 23 14. 9 3737.986r 1 1. 1 Vi? 1.85 91

3733. 195r 75 56. 2 Fe I p 2.56 225 3738.069r 5. 5 3. 9 Nd II 3733.330m 228 107 Fe I 0.11 5 3738.139r 5 3. 3 Zr II 0.56 17

3733.492r

3733.655r

77

10

62. 7

11. 0

Co J 2.08 98 3738.312r

3738.363r

136

J

f 41. 4

1 27. 8

Fe I Cr II

3.27

3.10

609

20

3733.767r 5. 5 6. 2 3738.510r 47 22. 4 Fe I p? 3.64 918

3733.841r 2 2. 3 Cr I? 3.89 3738.631r 4 2. 0

3734.017r 1. 5 2. 5 3738.758r 6 2. 8 Vi 1.89 97

3734.135r 17 18. 8 Co I 2.04 96 3738.998r 14 6. 4

3734. 285r 9 21. 7 CN R 93 2 2 3739 118r 53 20. 8 Fe I 2.22 75

3734.37 (1014) (323) ^13 10.20 3 10 3739.228r 104 40. 1 Ni I 0.17 2

3734.465r

3734.536r

r 15.3

[ 36. 2

Ru II — CN

-CN

2.54 R 94

R 94

1 1,1

1,1

11

11

3739.325r 3739.529m50

112

20. 6

39. 4

Fe I Fe I

2.18

3.30

74

88
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

3739.783 55 20. 8 Ni I 3.94 180

3739.944r 3 1. 3

3740.064 65 24. 1 Fe I /3.05

13.40 532a707

3740.245r

3740.336.r

[ 142

1 31. 8

1 12. 3

Fe I -CN3.25 R 91

667

1,1

3740.464r 4 1. 6 CN?-

CN?

3740.531r 1. 5 0. 7

3740.72 a 2 0. 8 Nb n? 1.62

3740.811r 0. 1 0.03

3740.884r 0. 5 0. 1

3741.065S 93 32. 0 Til 0.02 17

3741. 198r 3. 5 1. 5 -CN R 89 2,2

3741. 312r 13 5. 0 Sm II —

Eu II 1.38 11

3741.479r 56 20. 7 Fe I 3.43 701

3741.561 15 8. 8 Fe II p 2.28 15 3741.645m 133 44. 6 Ti II 1.58 72

3741.833r 5 2. 1 CN R 93 0,0

3741.903r 8. 5 3. 2 CN R 93 0,0

3742.079r 20 10. 2 Fe I 2.59 225

3742. 146r 66 24. 6 Fe I 3.94 978

3742.278r 6 2. 4 Ru I 0.34 2

3742.567r

3742. 623r

] 137

r 25. 9

1 36. 1

Fe I p Fe I

3.04

2.94

389

387

3742.80 a 0. 5 0. 3

3742.950 75 36. 4 IFe ICri

3.43 2.54 704

43

3743.129r 20 13. 6

3743.218r 25 22. 2 3743.368m 592 193 Fe I 0.99 21

3743.485r 92 101 Fe I (Gd II) 3.57

0.14 806

2

3743.585r 70 43. 6 llCriVii

/2.54

12.54

1.67

43

43

21

3743.779 47 24. 0 Fe I 2.73 290

3743.888 74 32. 4 Cri

(Sm n)

2.54 /0.18

10.33

43

1834

3743.997r 3. 5 1. 9 CN R 92 0,0

Notes

11

11

11

11

11

Waver X^ \A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

\b)

Spot

Solar

Tflrinf i- fication

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

3744.110m

3744.162r 1 176

1 67. 0

1 1.7

Fe I 3.04 385

3744.372r 1 0. 5

3744.493r

3744.556r

\ 84

]

f 1.3. 9

1 26. 2

Cri

Ni I

2.54

3.84

43

180

3744.756r 3. 5 1. 9 CN?

3744.817r 2. 5 1. 3

3745.048r (2. 5) (1. 3) CN?

3745.137r (2. 5) (1. 6)

3745.229r (8) (8. 6)

3745.349r (68) (72. 5)

3745.475r 9. 3 49. 6 Co I 0.92 34 3745.574m

3745.609r

1 1202 J459

i 66. 6

Fe I Sm II?-0.09

0.00

5

2

3745.83 a 12 64. 0 Vii 1.55 15 3745.910m 540 301 Fe I fZr ii) 0.12

1.76

5 112

3746.048r 14 26. 7 — CN /R 91 IR 88

0,0

1,1

3746.144r 4 7. 2

3746.244r 20 14. 4

3746.368r 0. 5 0. 5

3746.475r 72 36. 8 Fe I 2.20 73

3746.574r 46 32. 5 Fe II p 2.28 14

3746.721r 2. 5 1. 6 Cai 2.71

3746.922r

3747.004r

1 141

I

1 40. 3

1 29. 5

Fe I Fe I p3.00

3.00

386

388

3747.225 26 13. 9 -Cri 4.18 289

3747.348r 6 3. 5

3747.552 44 22. 2 Yn 0.10 8

3747.720r 2 1. 5

3747.821r 4. 5 3. 5 Dy II

3748.000r 50 44. 3 Vi-

||Ti II

/1.87

11.93 2^60

9798

107

3748.088r 10 29. 0 CNTi I?

/R 90 IR 85

1.87

0,0

2,2 166

3748.271m 497 228 Fe I 0.11 5

3748.405r 2. 5 12. 8 Ca I 2.52 27

89
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3748.506r

3748.605r

3748.677r

3748.799r

3748.905r

3748.966r

3749.051r

3749.244r

3749.365r 3749.495m

3749.620r

3749. 740r

3749.850r

3749.938r

3750.139r

3760.15

3750.205r

3750.304r

3750.505r 3750.678m

19

8

17

0. 5

15

103

48

46

4

1907

1. 5

15

7. 5

13

1. 5

(1388)

3. 5

25

1. 5

27

29. 8

14. 5

19. 2

1. 2

24. 0

82. 9

99. 1

103

31. 2

578

18. 1

33. 4

22. 7

26. 9

3. 2

(430)

5. 3

22. 4

1. 6

18. 7

Fe I Fe II Cr I Cr II

Fe I p

|Fei

Cr I

Nil

Fe I

Co I CN

^12

CN

Ca I

Fe I

3.57

4.73

2.54

2.70

2.69

2.94 /2.54

12.54

0.00

0.91

2.04 R 89

10.20 R 89

2.52

2.61

805

154

43

11

289

386

4343

1

21

95

0,0

2

0,0 27

225

11

10

11

3752.688r 3752.860m

3752.992r 3753.142m

3753.340r

3753. 525r

3753.620m

3753. 751r

3753. 867r

3754.04 a

3754.123r

3754.225r

3754.339r

3754.505r

3754.578r

3754.725r

3754.874r

3755.006r

3755.134r

3755.280r

5

95

40

60

56

8. 5

132

12

4

1. 5

0. 5

6. 5

18

1 120

22

5

3

13

3. 5

2. 1

34. 6

17. 0

23. 2

20. 8

3. 6

45. 0

5. 2

1. 6

0. 5

0. 3

2. 4

6. 9

1 26. 6

1 16. 5

7. 7

1. 9

1. 1

4. 8

1. 3

Nd II?

Ti I

Fe I Cai

Dy II- CN

|FeiTi I Dy II

Fei?

CN

Co I Fe I Cr II Co II Fe I p Fe II? -CN

Sm II —

CN

0.00

0.05

2.40

2.52

0.00 R 84

2.18 0.02

R87

2.54

3.00

3.10

3.69

R 81

0.33 R 81

33

17

177

27

1,1

73

17

0,0

132

386

20

949

2,2

34

2,2

11

11

11

11

3750.773r 8. 5 6. 4 Mn I 2.94 24 3755.452r 44 16. 1 Co I 2.08 96

3750.872 26 15. 7 Vii 1.68 21 3755.573r 15 5. 3 Fe II 4.74 154

3750.993r 3751.090m

1

32

0. 7

17. 9

CN?

Fei

Fei

2.20 3.30 74 667

6700.7 ^^T

3755. 823r

1. 6

2. 5

U. 6

0. 7

VI.'

Cr I

/2.27

12.29

2.71

124

124

72

3751.224r 15 8. 0 Vii 2.49 100 3755.939r 0. 2 0. 1

3751.449r 2. 5 1. 3 3756.072m 65 24. 8 Fe I 2.18 74

3751.592 42 20. 0 Zr II 0.97 71 3756.264r 6. 5 2. 4 CN R 86 0,0 11

3751. 659r

3751.824

3751.912r

3752.191r

3752. 265r

3752.418S

10

50

4. 5

6

5. 5

78

5. 3

22. 7

2. 3

2. 7

2. 7

30. 6

CoiCN

Fe I

CN

CN

Fe I

2.08 R 85

2.69

R 88 R 88

/3.04

13.04

98

1,1

287

0,0

0,0 385

392

11

11

XI

3756.339r

3756.45 a

3756.564r

3756. 650r 3756.941m

3757.072r

3757.165

6

1

4. 5

7. 5

96

2

32

2. 1

0. 4

1. 6

2. 7

34. 8

0. 9

13. 5

CN

Sm II? CN

CN

Fe I CN

Cr I

R 86

0.43 R 80 R80

3.57

2.54

0,0

44

2,2

2,2

805

43

11

11

11

3752.506r 12 6. 0 Nd II- Osi 0.34 2 3757.304r

3757.368r

14

16

8. 8

8. 2 Dy II 0.10

90
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Reducecl Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

3757.458m 68 30. 6 Fei 3.30 608 3762.210r 58 19. 8 Fe I 3.37 705

3757.684r

3757.810r

3757.959r

3758.033r

3758.129r 3758.245m

92

14

29

13

2

1647

46. 8

17. 3

37. 2

34. 8

9. 6

497

Ti II Cri

Zr II

Cri

Fe I p

Fe I

1.57 2.54

1.83

2.54

3.42

0.96

7243

120

43

704

21

3762. 309r

3762.350r

3762.477r

3762.618

3762.757r

3762.870r

}.

4

34

8

16

1 15. 2

I 10. 4

1. 5

12. 5

3. 2

6. 4

CN

CN

Ni I CN

CNFe II

R 83 R 83

2.74 R 79 R 79

5.95

0,0

0,0

1,1

1,1 192

11

11

11

11

3758.316r 3 24. 5 CN /R 85 IR 79

0.94

0,0

2,2 }» 3763.008m 53 21. 2

3758.437r

3758.596r

3758.723r

3758.827r

3758.956r

15

10

8. 5

1

4. 5

38. 6

14. 9

3. 5

0. 7

3. 1

Cri

Nd II?- Sm IX

12

3763. 175r

3763.288r

3763. 376r

3763. 476r

3763. 571r 3763.803m

9

4. 5

6. 5

14

24

829

4. 8

2. 9

4. 9

14. 9

33. 1

255

CN

CN

Mn I Nd II Fe 1 p Fe I

R 76 R 76

2.95

2.48

0.99

2,2

2,2

24

128

21

11

11

3759.075r 29 19. 9 La II 0.24 13 3763. 979r 16 33. 8

3759.157r 22 21. 0 Fe I 3.63 865 3764.113r 27 30. 2 -Ce II 0.36 41 3759.299m 334 115 Ti II 0.61 13 3764.221r 39 24. 2 Fe I 2.20 74

3759.473r 19 12. 8 Fe II 4.74 154 3764.284r 7. 5 5. 4 CN R 82 0,0 11

3759.585r

3759. 689r

29

4. 5

13. 8

2. 1

Fe I Co I

3.43

2.54

701

131

3764.384r 28 14. 4 Sm II Zr I CN

0.33

0.00 R 82

34

10

0,0 11

3759.800r 3. 5 1. 5 3764. 590r 10 4. 7 CN R 78 1,1 11

3759.892r 8. 5 3. 2 CN R 78 2,2 11 3764. 650r 5 2. 1 CN R 78 1,1 11

3760.055m 105 35. 0 Fe I 2.40 177 3764.849r 5 1. 9 CN R 75 2,2 11

3760.224r 24 8. 6 Vii 1.69 21 3764.922r 3 1. 1 CN R 75 2,2 11

olO'J.oZ a

QO 1. o u,u 1

O / OO.Uu (

A

t: RVi T? 0.71

3760.392r

3760.537S

23

100

8. 2

32. 8

CN —

Co I Fe I

R 84

1.74

2.22

0 040

76

11 3765.16 a

3765. 304r 3765.551m

0. 5

32

174

0. 1

12. 0

56. 2 Fe I 3.24 608

3760.705r 12 4. 4 Sm II f0.18 \0.54

18

51 3765. 710r. 68 27. 6 Fe I 3.27 608

3760.80 a 3 1. 1 CN? 3765.88 a 1. 5 0. 6

3760.931r 14 5. 0 CN R 80 1,1 11 3766.094m 56 21. 5 Fe I 2.59 226

3761.067r 46 18. 5 Fe I 3.37 706 3766.240r 25 10. 6 CN R 81 0,0 11

3761.320m

3761. 429r 277

J

r 61.0

[ 37. 2

Ti 11 Fe I

0.57

2.59

13

227

3766. 323r

3766.457r

16

9. 5

6. 9

4. 6

CN

CN

R 81 TP 77 IR 74

0,0

1 1 1 ,

2,2

11

3761. 556r

3761.690 3761.874m

12

60

78

5. 2

20. 2

26. 2

CN

Cr II

Ti II

R 77

2.70

2.59

2,2

11

107

11 3766.666m

3766.820m

78

39

36. 1

25. 8

Fe I Fe IZr II

3.04

0.41

386

7

91
The Solar Spectrum—Continued

Wavelength

(I)

Equivalent Width

AX

A')

Re- duced

Width

AX/X

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(X)

Equivalent Width

AX

I'm a')

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3766.968r 24 27. 5 3771.18 a 1. 5 1. 1 CN?

3767.081r 7 23. 9 3771.278r

1 ^

r 0.

4

Fe I? 3767.204m 820 262 Fe I 1.01 21 3771.331r 1 1 1.1 CN R 71 2,2 11

3767.356r 18 34. 5 3771.38 a 3. 5 2. 1 CN R71 2,2 11

3767.437r 20 19. 7 Cr I 2.54 42 3771.497 44 23. 2 Fe I 3.24 607

3767.545r 11 10. 1 CN 3771.658r 62 29. 8 Ti I 0.05 17

3767.650r

3767.705r

15

13

9. 3

7. 7

CaiV II

2.71

2..50 100

3771.75 a 7 4. 8 CN /R74

1R70

1,1 3,3 }"

3767.897r 3 1. 6 Zr 11 0.71 31 3771.814 14 7. 7 CN /R 74 IR 70

1,1 3,3 111

3768.034m 78 32. 4 Fe I 2.22 73 3771.971r 1 0. 6 Zr II? 0.71 44

3768.095r 12 6. 6 Cri

CN

/2.54

12.54 R 73

4242

2,2 11

3772.104 3772.188m

19

13

8. 8

6. 4 CN

CN

R 78 R 78

0,0

0,0

11

11

3768.16 a

3768.248

4. 5

60

2. 5

24. 3

CN

Cri

Fe I

/R 76 \R73

2.54 2.84

1,1 2,2 43

368

3772.384r

3772.533r

3772. 591r

3. 5

1 86

1. 6

1 27. 6

[ 8.1

CN?

Nix 0.21 15

3768.406r 22 9. 4 Gd II 0.08 2 3772. 779r 2. 5 1. 2

3768.50 a 1 0. 5 3772.931r 24 10. 0 -Vii 2.49 100

3768.661r 32 14. 1 -Ir I? 1.47 3773. 206r 30 12. 0

3768.733r 44 18. 3 Cr I 2.54 43 3773.364m 43 17. 0 Fe I 3.05 531

3768.89 a

3769. 019r

3769.22 a

3769. 316r

3769.463

3769.653r

3769.722r

3769.813r

3769.994S

3770.169r

3770.307r

3770. 413r

6. 5

21

0. 5

5. 5

58

4

5

7. 5

77

25

65

49

3. 1

9. 2

0. 4

2. 8

26. 4

2. 3

3. 1

3. 4

39. 8

15. 3

37. 7

34. 2

CNCN

Cr I

Fe INi II Nd II CN

CN

Fe-i CN

Fe I

II Fe I Ti II

R72

R72

2.54

3.10

0.20 R 72 R 72

3.00 /R 79 \R 71

2.69

2.43

2.60

3,3

3,3

42

4

67

2,2

2,2

387

o,o\

3,3/ 287

177

107

11

11

11

11

11

3773.472m

3773.561m

3773.699m

3773.890r 3774.033m

3774.111m

3774.218r 3774.336m

3774.515m

3774.652r

3774.832m

3774.998r 3775.204m

11

10

88

12

13

11

0. 2

74

8. 5

74

100

6

10

4. 2

4. 4

31. 7

5. 0

5. 3

4. 2

0. 1

26. 0

3. 2

26. 2

34. 0

2. 4

3. 7

CN

CN

Fe I

CN

CN

Y II CN

Ti II Co I? Fe I CN

CN

R 73 R 73

3.04

R 77 R 77

0.13 R 69

0.57

2.08

2.22

R 72

1,1

1,1

386

0,0

0,0

7

2,2

1296

73

1,1

11

11

11

11

11

11

3770.531r 4 3. 7 Fe I? 3775.290m 14 5. 4 CN R 72 1,1 11

3770.599r 23 18. 6 3775.423r 6. 5 2. 4 CN?

3770.63 1860 621 Hii 10.20 2 10 3775.578r 144 47. 2 Nil 0.42 33

3770.719r 3 3. 3 3775.710r 9 3. 2 3770.972m 44 29. 2 Vii 1.67 21 3775.860 48 17. 5 Fe I 2.73 287

3771.113 1 4 3. 2 CN- 3775.949m 12 4. 6 CN R 76 0,0 11

92
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivaksnt Width

AX (ml)

Re- duced

Width

A\/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3776.059m 84 28. 8 Ti II 1.58 72 3780.228 10 3. 7 CN R64 3,3 11

3776.198ni 21 7. 7 CN- R 68 2,2 11 3780.32 a 9 3. 2 CN R64 3,3 11

3776.334r 7. 5 2. 6 CN 3780.420m 24 8. 6 CN R69 1,1 11

3776.461r

3776.559r

90

46

30. 0

18. 0

Fe I Y II (Mn i)

2.18

0.13

2.11

74

8

6

3780.516m

3780.706

26

110

9. 5

36. 2

ICNZr I R69

0.00

1,18 11

3776.692r 1. 5 0. 5 3780.856m 15 5. 7 CN R65 2,2 11

3776.839r

3777. 074r

3777. 232r

3777.332r 3777.456m

1. 5

68

4. 5

50

94

0. 5

23. 0

1. 6

17. 5

31. 0

Fe I? Fe I

Cr I Fe I

2.99

2.54

2.56

432

41

223

3780.989r

3781. 190S

3781.321r

3781.41 a

7. 5

76

3. 5

4

2. 6

25. 6

1. 3

1. 3

Fe I?-

CN?

Fe I Fe I?

Vi?

2.20

fO.OO 11.93

74

1097 3777.569m 8. 5 3. 2 Co I 2.08 96 3781. 516r 18 6. 3 Fe II 4.49 130 3777.664m

3777.752m

3777.846m

8

6

14

2. 9

2. 1

5. 0

CN

CN

CN

R 67 R 67 R752,2

2,2

0,0

11

11

11

3781.615m

3781.687m

1> S58

[ 25. 1

1 5. 8

CN

Fe I CN

JR 73 \R63

JR 73 IR63

0,0

3,3

0,0

3,3

}"

}"

3777.928m 23 7. 9 CN R75 0,0 11 3781. 796r 2. 5 0. 9

3778.066 66 22. 0 Ni I 0.03 15 3781.938m 70 24. 6 Fe I 3.64 917

3778.163r 3778.327m

3778.515m

20

82

88

7. 1

27. 8

29. 4

Sm II Fe I —

Vii

Fe I

2.83

1.68

3.25

367

21

664

3782. 119r

3782.218m

70

19

24. 6

7. 4

Fe I CN

CN

(Osi)

(Zrii)

R 68 R 68

0.52 0.80

1,1

1,1344

11

11

3778.703r 88 29. 1 |Fe I V I 2.20

0.29 7328

3782.318m 18 6. 3 CN

1 Y II R 64

3.62

2,261

11

3778.798m 58 23. 9 CN

Fe I?

JR 70 IR65

Ijl 3,3 3782.453m

3782.613m

74

64

24. 9

21. 2

re I re I3.00

3.07

o o o

491

3778. 911r 7 2. 6 CN R 65 3,3 11 3782. 729r 4 1. 6 Zr II 1.77 IZU

3779.027r 13 4. 6 3782. 848r 3. 5 1. 2 re I

3779.098r 1. 5 0. 5 CN 3782.995r 4 1. 6 CN R 62 3,3 11

3779.207m 48 16. 3 Fe I 2.76 290 3783. 085r 11 4. 0 CN R 62 3,3 11

3779.316m 8. 5 3. 1 CN R66 2,2 11 3783. 189r

19 6. 9

3779.431r

3779. 519r

3779. 575r 3779.731m

> 178

24

f 35. 7

1

1 23. 8

I 6. 1

8. 7

Fe I Fe I Fe I Fe II p CN2.56

3.27

2.22

2.54 R74

222

665

74

23

0,0 11

3783.349m

3783.462r

3783. 535r

3783.73 a

68

\ 164

4. 5

23. 5

r 2.1

1 52. 7

1. 9

Fe II CN

Ni I Co I Fe I

2.28 R 72

0.42

2.08

14

0,0 30

11

3779.808m 16 6. 1 CN R74 0,0 11 3783.818m 29 10. 4 CN JR 67 IR 63

1 1 2^2

1}"

3780.00 a

3780.087

1

3. 5

0. 4

1. 2

Cr I? Fe I? 2.71 3783.900m

3784.02 a

248~58. 7

3. 2

CN /R 67 IR 63

1,1 2 2

93
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

3784.252r

3784.365m

3784.504m

16

6

30

5. 8

2. 1

10. 8

Nd II- Fe I p CN

3.27 R 61607

3,3 11

3788.145r

3788.215r 3788.439m

0. 6

2

38

0. 4

1. 2

14. 8

Sm II

Dy II CN

0.25

0.10 R 60

25

2,2 11

3784.675r

3784.826r

3785.013r

3785.084r

3785.234r

6

4. 5

6

6

20

2. 1

2. 3

2. 1

2. 1

6. 9

CN

Fei?

Fe I CN

CN

CN

/R 71 IR 62

0,0 2 2

3788.528 3788.701m

3788.815r

3788.861r

3788.970

3789.046

18

84

] 69

30

25

6. S

28. 2

f 8. 3

1 17.4

12. 4

8. 4

CN

Yn

CN

|Cr ICN

CN

CN

R 60

0.10 R 64

3.01 R 64 R 69 R 69

2,2

7

1,1

139

1,1

0,0

0,0

11

11

11

11

11 3785.317m 31 11. 1 CN }" 3789.184m 110 35. 4 Fei 2.73 289

3785.397m

3785.496m

3785.578m

3785.707m

3785.790r 3785.952m

3786.042r 3786.175m

3786.329r

3786.448r

3786.522r

28

20

16

96

46

122

42

144

80

80

26

10. 0

6. 9

5. 8

31. 4

22. 2

39. 0

20. 8

45. 4

26. 4

26. 6

15. 8

CN

CN

CN

Fe I Fe I p Fe I Til Fe I (Dy II)

Ti up

Fei?

/R 71 IR 62 R 66 R 66

3.24

3.33

2.43

0.90

2.83

0.61

0,0

2,2

1,1

1,1 608

704

177

57

307

12

11

11

3789.300

3789.419

3789.499 3789.577m

3789.728 3789.822m

3789.921r 3790.098m

3790.223m

3790.332

3790.447r

22

146

24

56

22

98

25

179

138

32

1 96

9. 2

45. 3

18. 2

19. 8

7. 9

33. 8

10. 5

54. 9

61. 8

13. 4

f 12. 6

Ti I -Fe I Cn?-

Fei

Cn

Fei

CN

Fe I Cri

11 Mn I Vi

II Cr I CN

1.46

2.54

2.61

0.97

3.37 R 59

0.99

3.01

2.11

0.28

3.01 R 63

115

41

226

24

702

2,2

22

139

6

28

139

1,1

11

11 3786.682m

3786.842

3786.965r

132

22

6

42. 0

7. 9

2. 3

Fe I

Fei?

1.01 22 3790.491r

3790.657m 157

[ 25. 3

59. 4

ViRu I Fe I1.38 0.26

3.04

69

387

3787.101r ' 2. 6 3790.759m 119 38. 6 |FeiCN

/2.18

12.48 R 68

73 127

0,0 11 3787.166m

3787.236m

139 33. 4

. 17. 2

Fe I CN

Vii

CN

3.64 fR70

IR 65

2.52 /R 70 IR 65

916

o,o\

1,1/ 100

0,0\

1,1/

11

11

3790.833

3790.994r 3791.110m

38

6

45

21. 6

2. 2

16. 3

ILa II CN

CN

CN0.13 R 68

12

0,0 11

3787.420r

3787.482r

6. 5

6. 5

2. 6

3. 2 CNFei

3791. 194r

3791.26 a

8. 5

4

3. 2

1. 6

CN

Nb I Sm II?

0.13 2

3787.575r 5 2. 9 3791.380m 43 15. 5 Cr I 3.01 139

3787.714r 0. 5 0. 8 3791.509m 75 25. 8 Fe I 2.56 223 3787.891m 512 157 Fe I 1.01 21 3791.749m 69 24. 0 Fe I 3.42 703

3788.051r 2. 5 4. 2 3791. 904r 12 4. 5 CN

94
The Solar Spectrum—Continued

Wavelength

\A)

Equivalent Width

AX

unA;

Re- duced

Width

AX/X

IFj

Spot

Solar

Identification

Low

E P

or Rot.

RMT

No.

or Vib.

XJcXjLLU.

Notes

3792.079r

i 110

J

2. 8

35. 6

CN

Fe I Cri

R 62

2.73

3.01

1,1 287

139

11

3792.347m 86 29. 8 Ni I 0.27 2

3792.565 33 15. 0 |CN

Y 11 R 67

3.54

0,0 61

11

3792 65 Ir 1 121

J

J 11. 6

•'.6 n CN R 67 0 0 11

3792.832m 72 26. 0 Fe I 2.22 74

3792.932r 18 7. 4 CN R 57 ^, 11

3792.991r 7 3. 0

3793. 125r 29 11. 3 Fei?

CN?

37Q3 291 27 17. 6 Cr I 3.01 139 3793 358 66 24. 8 Fe I 3.04 388

3793 485m 64 25. 0 Fe I 3.00 387

3793.605m 123 43. 2 Ni I 0.27 4

3793.707 10 5. 7 CN R 61 1,1 11

3793.782 9 3. 4 CN R 61 1,1 11 3793.876S 80 30. 8 Cri

Fe I 3.01 2.84 139

OU 1

3793.970r 7. 5 3. 0 Sm II 0.10 11

3794.088r 2 1. 1

3794.176r 3 1. 6 Fei?

3794.347m

3794.418r

> 122

44. 0

. 10. 0

Fe I (CN)

(Vn)

CN

2.45 /R 66

1 "R 5fi 2.52 IR 56

177

0,0 9 9 100

2,2

I

O < Ot: J- 1 n 6. 6

3794.615 22 12. 7 Cri 3.01 139 3794 773m 48 34. 3 II n '^4. 1 9

37Q4 887 14 24. 0 3795 m 2m

1

174

(Vi) /0.02

9199R

O # i/ij. J- J . 20. 6

3795.302 25 14. 8 CN R 60 1,1 11

3795.375 10 6. 6 CN R 60 1,1 11

3795.444ni 30 18. 5 3795.538m 65 31. 9 Fe I

Wave-

(A)

Equivalent

vv lULn AX (mA)

Reduced

VV 1 CILXl AX/X

(I)

Solar

icienLifi cation

Low

E P

or Rot. Line

RMT

No.

or Vib. Notes

3795.743r 10 5. 4 Tm II CN

0.03

IV o»j 6 9 9 1

1 i

21 1 1 1 CN iV oo5 5 9 9 1

1

16 8 4 Ti I 1 44 II 1I .J5

O ( iJ\J.\J 1. OlLl 95 1 4 n FpX C 1t 9 40 11 7fi / D

o 1 ijyjt i ill 16 8. 7 CN 1\. f;5 VJO 0 0 1

1 X

*^7Qfi O / t/U. 11 Sfim OlJlll 1 7 7 CN T?XV fl5 uo 0 0 1 1 1 X

O t UK} ,KJ\J<J 2. 4 CN

0( JU.Ot/J-lil 14 8. 7 Gd II 0 0'^ 2

3796.496 15 9. 2 Zr II 1.01 71

3796.66 a 3 2. 6 CN?

^7Qfi RO'^m oo 9fi 0

'?7Qfi S87m 76 44 fi |Ti II Fe I 0 57

3.30 12 667

3796.974 20 16. 1 CN

Cr I R 59

2.54

1,1 41

11

3797.065 9. 5 12. 2 CN

'^7Q7 1 "^Qm "^7 28. 7 Cr I 3.01 139 3797.245m 20 16. 6 CN R 54 2,2 11

3797.459r 3797.522m

I 1 (T?

1 6. 3

[ 67. 4 Fe I 3.24 607

3797.720m 34 37. 4 Cri

(Sm ii) 3.01 139

3797.851m 17 21. 6 CN R 64 0,0 11

3797.90 3463 1085 ^10 10.20 2 10 3797.954m 54 54. 6 IFei

CN

2.59 R 64 222

0,0 11

3798.086r

3798.168r

1 11

1

r 15. 0

1 6. 6

CN

CN

3798.257m 12 20. 6 |Moi

Ti I 0.00

1 4'^

1 115

o 1 1 Q Fe II p 2.34 14

O 1 ijO.O^ 1 111 out: 1 5Q Fe I 0.91 21

1 8 oo.5 fiu CN R 53 2,2

•^708 77 ir nJ J. 1. V CN

0Q7QQ / yo.yUfjni OnQm 9n 14 0 Ru I 0.15 X

3799.021r 1 1. 1 Fe I?

3799.135 7 7. 4 CN

3799.251m 30 25. 3 Mm 2.14 6

3799.348 16 17. 1 Ru I 0.00 1

95
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3799.448r 5 14. 4 3799.558m 622 309 Fe I 0.96 21

3799.677 16 25. 8 CN R 63 0,0 11

3799.792ni 41 37. 4 Ti n 0.61 13

3799.908 44 26. 3 Vi 0.27 28

3800.034 58 29. 2 CN /R 57 IR 52

1,1 2,2 In

3800.113 18 13. 7 CN R 57 1,1 11

3800.19 a 3 1. 8 Fe I? CN?

3800.319 38 18. 4

3800.546 34 15. 8 Mn I 3.84 45

3800.627 16 8. 2

3800.739r 9 4. 4 Zr II 0.53 17 3800.850m 28 13. 2 -Yii

(Sm II) 3.56 0.28

6129

3801. 025r 5. 5 2. 5 Sn I 1.07 2

3801.113 33 15. 0 Ti I? 1.88 165

3801.192 18 8. 5

3801.303 17 10. 8 CN R 62 0,0 11 3801.371m 75 30. 2 Fe ICN

3.69 R 62 948

0,0 11

3801.47 a 6. 5 3. 4 Fei?

3801.542 50 21. 0 Ce II CN

0.90 /R 56 IR 46

172

1,1 3,3 3801.683m 108 40. 0 Fe I 2.83 367 3801.815m 112 40. 5 Fe I 2.84 367

3801.909 2. 5 2. 4 Mn I CN

3.13

3801.990m 105 38. 9 Fe I 3.33 704

3802.132 30 12. 9 3802.285m 80 30. 5 Fe I 3.30 666

3802.482 19 7. 9 CN

3802. 587r 9 3. 8 CN

3802.731 28 11. 1 CN /R 50 IR 45

2,2

3,3

3802.813 23 9. 3 CN /R 50 IR 45

2,2

3,3 }"

3802.959r 3803.009m 1 50 \

[ 18. 7

Nb I? CN0.09 R 613

0,0 11

3803.090m 61 22. 9 CN /R 61 IR 55

0,0

1,1

^Wavelength

(A)

EquiV (Aji-KyLl \j Width

AX

(ml)

ReLi. UL-CU Width

AX/X

(F)

Spot

Solar

Identifi p ft i" 1 TI

Low

F P

or

XVL, b. Line

RMT

No

or Vih V ID. BandNotes

3803 1 77 1 fi ft 7 XV UtJ 1 \

1

1

X X 3803 2'S8m o\i 90 S 2.28 1 99

3803 482Tn 42 16. 0 V I 0 9Q 28

3803.576m 14 5. 8 CN

3803.678m 11 4. 2 CN

3803. 772r 6. 5 2. 5 V I? 1.35 68

3803. 906r 11 4. 6 ViCN0.04 R 4410

3,3

1 on ou. u X t: X o .oo 709

3804 099 Ro ^ 0 CN PXV 4QTt .7 2 2 w

3804.178 31 11. 6 CN R 49 2,2 11

3804.286 25 9. 5

3804.346r 7 2. 9 CN

.'^804 486 1X Qu 7/ . 1X CN —

Fe I

23. 9 CN PXV "14 Ct: 1 1 w

3804.696m 29 14. 1 CN fP 60 J X\. UL, IR 54

0 0

1^1

1

3804.793m 95 31. 8 CN

\Cr T

1 \jl X R 60

O . 01U X 0,0 139

11

1X 0J fi 7 PN

^sfif) no n o X . o XFpC t?X !

'^RO'i 1 1 7r ^o 11XX. 1J PN XV o, o3

O <J\J \J. J-iJ Ol 1X o% tj. o CN R 43 3 3 3805.349m 171 55. 0 Fe I 3.30 608

3805.450 12 9. 2 CN R 48 2,2 11

3805.530 60 23. 2 CN R 48 2,2 11

3805.745r 32 11. 3 CNTTp T

3805.850r 10 4. 2 CN

3805.964r 7 2. 6 CN

3806.119m 27 11. 2 CN R 53 1,1 11 3806.219m 105 84. 9 |Fe I CN

3.41 R 53

731

1,1 11

3806.375m 67 22. 0 CN /R 59

1l_XV R 49Tt.i 0,0

o, o ) Fe I

3806.445 48 23. 4 CN /R 59 IR 42

0,0

3,3

3806.572r 20 8. 1 Cri 0.98 24 3806.718m 209 64. 6 Mn I |Fei

2.11 3.276 607

96
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3806.860m 54 28. 4 CnCN3.45 R 47 214

2,2 11

3807.009r 7. 5 3. 1 3807.151m 193 59. 8 Nil 0.42 33

3807.285 43 18. 6 CN

3807.397 27 11. 6 CNZr n 0.71 31 3807.544m 178 55. 1 Fe I (Vi)

2.22 0.26 7328

3807.689 32 13. 4 CN R 52 1,1 11

3807.775r 14 5. 5 CN

3807.937m 111 35. 2 ICnCN3.01 R 58

139

0,0 11

3808.083r

3808.134r

1 110

r 14.

J

I 28.4

Co I Ce II- CN

0.43

0.30 /R 58 IR 46

17

59

0,0

2,2 3808.286m 90 29. 2 Fei 3.02 489

3808.522m 37 12. 7 Vi 0.00 9

3808.630r 4. 5 1. 8 CN

3808.734m 114 36. 5 Fe I 2.56 222 3809.049m 85 28. 1 Fe I 2.86 367

3809.162 24 9. 5 Fei

3809.25 a 5 1. 8

3809.31 a 4 1. 4 Fe I?

3809.412r 20 8. 3 CN R 45 2,2 11

3809.490 26 11. 0 CN R 45 2,2 11 3809.586m 132 41. 8 Vi

11 Mm 0.28

2.14 28

6

3809.692 3809.755m

1

J

f 21. 0

1 16. 3

CN

CN

R57

R 57

0,0

0,0

11

11

3809.85 a 6 2. 2 CN? R39 3,3 11

3809.921r 20 7. 0 CN R39 3,3 11

3810.034r 15 5. 5

3810.22 a 1. 5 0. 4 CN?

3810.294r 21 7. 3

3810.540 41 13. 8 CN R 50 1,1 11

3810.618 23 9. 7 CN R 50 1,1 11

3810.713r 3810.760m 1 120

i 37. 8

CN

Fei

R 44

3.30

2,2

665

11

3810.900m 28 10. 0 Fe I p 2.61 224

Wavelength

(A)

3811.041m

3811. 176r 3811.298m

3811.380m

3811.526r

3811.646r 3811.807m

3811.894m

3811.982m

3812.062m

3812.199r

3812 248r

3812 448r

3812 592r

3812 672r

38i2 859r

3812 962

3813 075

3813.262

3813.394m

3813.491m

3813.640m

3813.892r

3813. 928r

3814.012r

3814.122m

3814.244r

3814.358r 3814.521m

3814.596m

3814.784m

3814.892m

Equivalent Width

AX

(ml)

72

2. 5

67

35

0. 5

3. 5

147

48

37

44

18

3. 5

17

322

104

40

138

54

86

182

38

8. 5

22

170

47

26

Rcuced

l^idth AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

23. 9 Co I Fe I

0.92

/2.59

12.73

31 223

287

0. 9 CN

22. 0 Ni I-

|CN

0.21 R 5615

0,0

16. 0 CN

Ti 1? R 561.87

0,0 165

0. 3

1. 1 CN

21. 0 Fe I- 3.37 701

31. 2 Fe I 2.76 287

19. 9 CN /R49

IR 43

1,1 2,2

16. 5 CN /R 49 \R 43

1,1 2,2

4. 5 CN

Yii

R 37

3.55

3,3 61

10. 7 Cri 3.43 214

6. 3 Co I 1.78 40

1. 3 CN

6. 7 CN

13. 4

95. 7 Fei 0.96 22

97. 6 Fei 2.59 222

19. 1 CN /R 42 \R 36

2,2

3,3

38. 0 Ti II 0.61 12

28. 4 Vi 0.02 9

27. 8 Fe I 2.69 283

36. 2 Fe I 3.63 854

25. 6 Co I —

Fe I p

3.57

2.43 176

12. 9 GdiiCN

0.00 2

16. 0 Fe II 4.74 153

3. 1 CN

8. 1 CN R 35 3,3

34. 9 Fei 1.01 22

66. D X 1 II (Cri)

U.O 1 3.42

1 9 214

18. 9 Fe I 3.41

15. 7 CN

Til

R 47

2.09

1.1 189

97
The Solar Spectrum—Continued

W^Evelength

(A)

EquiWidth

AX

(ml)

ReducGd,

Width

AX/X

(F)

Spot

ooidr

Identification

Low

V1 , V1 or Rot. Line

RMT

XN O. or

Vib.

xjana.

Notes

3815.080r 4 1. 8 CN

3815.210r 13 8. 9 Fe IO O 1 c o oo«^ ooLo.o^oxn. 07/ 0 1 7

I V ii; o on 1 AA

ooloAo ITO.

Pi 1 Oi 4U. y Hy T 9 71 71

3815.617r 38 58. 7 3815.851m 1272 330 Fei 1.48 45

oolo.llUr

3816.191 39 50. 9 Cn

CNCN

f2.54 R 53

J Ix Oo IR 46

40

0,0

1,1/

11

11

3816.345m 100 53. 3 |Fei

I 2.20 73

£)olo.4Dom Oo Q 1 Q Hn T V^O I i .yo f!9 DZ

dolD.ooo 1 7 S 7 o. ( "R '^Q XV oo

1 1 11

oolD.74om 4 < ly. D ivin I O 1 A Z. i 0 0

oolD.ooor 1 U. 0 <^0 I O 1 A Z. 1 -1 OD

oolD.yzzm > oU / OQ Q S ^O. O J? e I O.U'l QQ7

3ol6.y72r J

1 Q 1

I, rf. 1 It oy 1 1

<jol7.U5or 1 / 7 Q /. o xt oy 0 9 1 1 OOIT 1 /IC ool7.14sr y. o

Q 7

d817.25 a

11

f\ /I U. 4 r e Ii 3817.382m 34 12. 8 -CN

3817.459 18 8. 0 -Wi 0.37

3817.583r ' 12. 0 Zr II 0.53 18 3817.647m

. 165

29. 3 Ti I |FeiCN

2.10

3.33 /R 52 IR 32

189

701

0,0

3,3 }"

3817.734 . 19. 6 CN /R 52 IR 32

0,0

3,3 }"

o817.o4om 40 Id. 0 V I CN

Cr I

0.0/ R 45

2.54

1,1 40

11

3817. 947r 1 o A 7

4. 7 Co I

1 O 1 loi

OOJ-O.UOOi 12 4. 4 CN

3818.195r 3818.243m

1 „

1

[ 5. 2

1 23. 3

CN

Vi

R 38

0.00

2,2

9

11

3818.345m 55 22. 3 Y 11 0.13 7

3818.475m 38 13. 9 Cn /2.54

\2.54 40

40 3818.620m 60 21. 7 Fe I

W^avelength

(A)

Equivalent Width

A \ A A (mA)

Re- duced

Width

A A/

A

(F)

Spot

ooiar

Identification

Low

T? "D or Kot. Line

RMT

iN 0. or

Vib. Band

Notes

3818.749r 16 6. 3 CN R 31 3,3 11

oolO.oyOr o no. 0

1 K

1. 0 iM D II i 1.59 QQ1 ooiy.UDom n nftQw 4y iy. D it 44 1,1 11

OQ1 n onQ

QQ1 n 07Q

1 68

j

10. 4

1 7 PL [ 1 /. 0

It Ol

T> Kl IX ol

U,U 11

11

o o 1 n o o 1 cjsiy.ooi 1 A 14 T>K O 7 o7 2,2 11

ooiy.'iy4m OQOO OO. ^ r e I Q /I A 0.4U 7nO /Oo

ooiy.o/o f;Q OO /f /I 7 44. / (^r I 9 71 Z. / I 7n/U

3819.688 43 28. 2 Eu 11 0.00 1

3819. 797r 9 9. 4 CN R 30 3,3 11

3819.901r 7. 5 11. 2 Co I 2.54 130

3819.961r 21 27. 8 IV I y^T I 0.30

Z.04 28

A f\ 40

rfozJ.Uoor 97Z / 41. 0

Q C9n 1 ."^i^w 1 QJ.O /I Q 7 4o. / 3820 303r 2. 5 19. 6 V I — 1.06 44 3820.436m 1712 512 Fe I 0.86 20

3820.561r 5. 5 41. 1 -CN R 36 2,2 11

3820. 656r 23 60. 7 CN — R 36 2 2 11

3820.748r 13 34. 6 CN 1 XV OU IR 29

0,U

3,3 }"

3820.809r

41

f 32. 4 CN /R 50 IR29

0,0

3,3 }"

OQOn Q77« oo^O.o t IT J QO /I

!_ oZ. 4 or I O Pi A /.04 A r\ 40

oo/o.yyor 1 n 9 y. z OiN

3821. 187S 93 49. 1 Fe I 3.27 608

O oo 1 A{^ A 00.ril.494 1 A 14 7 Q

/. O V I a 07 OQ-SO

O OO 1 c oc OO^i.OOO 1

1

1

1

1 0. 1 I /.04 A f\

3821.728m 52 32. 9 CNri 4Z R 35

T> O O [K zo

1,1 2,2

o o 6,6 J 0001 o /I r\*« 00.^1. o40m 1 or\ liiO /I c o

46. z r e I O A 1 z.Dl 909

3821.937r 64 28. 2 Fe II p 2.34 14 OOOO A17« oozz.olTr by OA A OD. b V I 0.u4 9 OOOO 11 oozz.llOr 1 C lo A O

D. 0 or I O C /J z.o4 /I n40 OOOO OCA

3822.328

\ 86

J

C 1 7 O 1 /. O

1[ 17.0

OAT CN

K 4y

R 49

0,0

0,0

1

1

11

11

3822.418r 17 6. 8 Zr I 0.00 10

3822.52 a 4 1. 4

3822.648 18 6. 5 CN

98
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3822.785r

3822.856

4. 5

75

1. 7

25. 6 CNCN

Vi

R 27 /R 34 IR 27

0.29

3,3 2 2

3,3 28

11

3826.207r

3826 313r 3826.418m

18

12

25

37. 9

16. 2

16. 2

Sm II CN

CN

Cri

0.54 R 31 R 31

2.71

51

2,2

2 2

70

11

11

3822.954 14 7. 3 CN R 34 2 2 11 3826.500r 1 0. 8 CN

3823.023 46 16. 0 CN R 41 1,1 11 3826.625 44 23. 8 Fe I- 2.45 176

3823.088

3823.216ni

3823.356 3823.514m

29

25

18

116

13. 5

8. 6

6. 3

37. 4

CN

V I CN

Mn I CCr i)

R 41

0.28

2.14

0.96

1,1 28

6 24

11 3826.709

3826.770

3826.852m

58

15

88

39. 2

11. 2

39. 5

CN

CNV I Ni I Fe I

/R 46 IR 23 /R 46 IR23

1.04 3.84

2.73

0,0

3,3

0,0

3,344

283

}"

}"

3823.757 51 25. 0 CN /R 48 \R 26

0 0

3^3 }" 3826.957 32 21. 7 CN-

|Vii

R 38

2.56

1,1 128

11

3823.818 23 15. 4 CN /R 48 IR 26

0,0

3,3 }" 3827.084 7. 5 4. 7 Fe II 4.73 153 3823.895m 93 34. 2 Mn I 2.16 6 3827.213 8 5. 2 CN?

3824.001r

3824.082m

3824.235r

3824.olzm

3824.452m

3824.573

3824.643r

1 106

10

85

519

84

6

r 9. 9

[ 40. 7

9. 9

79. 5 225

97. 5

7. 8

ViCN

Fe I

Fe I Fe I

1.05 R 33

2.59

3.30

0.00

44

2,2 224

607

4

11 3827.301m

3827.383

3827.486r 3827.580m

3827.692r

3827. oo2m

3828 OlQr

34

17

8

73

6. 5

897

24

19. 3

13. 3

7. 8

58. 6

21. 9

276

33. 9

CN

Zr II? Fe I

If e I

R 30

1.83

2.69

1.56

2,2

121

284

45

11

3824.750r 11 10. 5 CN

Fe I p R 25

2.61

3,3 221

11 3828.160r 60 39. 2 CN /R 45 IR 37

0 0

lil

3824.799r 3. 5 3. 1 CN R25 3,3 11 3828.224r 34 33. 0 CN /R 45 IR 37

0,0

1,1 }»

3824.926m 52 27. 7 Fe n 2.58 29 3828.404 15 10. 0 CN R21 3,3 11

3825.046r

382.5 126m

8

11

5. 2

7. 1 CN

CN R 32 2 2 11

3828.510r

3828.566r

94

I

f 36. 4

[ 18. 5

|Fei CN

Vi

2.76 R29

0.02

287

2,2

9

11

3825.236r

3825. 311r

34

25

22. 5

21. 7

CNCN

CN

/R 47 \R 32 R47

R 47

0,0

2,2 0,0

0.0

11

11

3828.659r

3828.835r

10

26

4. 8

13. 6

CN

Vi?

CN

1.38 67

3825 408m

3825.599r

40

28

32. 4

41. 8

Fe I Cr I -CN

2 28

2.71 R 39

12370

1,1 11

3828 Q72r

3S2Q O t7 . O'iQr VO i7 J. 3829.154m

13

9

77

9. 4

9. 7

61. 4

CN

Fe I 3.69 948

3825.683r 11 35. 3 CN- /R39

[K 24

1,1 6,6 111

J oo2y.250r 1 nlU QO A o2. 4 3825.891m 1519 421 Fe I 0.91 20 3829.365m 874 308 Mg I 2.71 3

3826.026r

3826.093r

7

5

26.9

16. 7 1 CN3829.480 23 54. 9 iFeiCN

/2.84

13.27 R28

366

663

2,2 11

99

761-925—66 9
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width ^ AX

(mA)

Reduced

Widths

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width ^ AX

(ml)

Reduced

SVidth i AX/X

(F)

3pot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3829.592

3829.685 3829.769m

22

69

40

29. 0

54. 4

38. 7

CN

Mn I Fe I

R44

2.18

2.56

0,0

6

221

11 3833.783m

3833.866m

34

63

38. 4

46. 7

CN

|Mn I CN

/R 41 \R 15

2.18 R 41

0,0

3,3

6

0,0

}"

11

3829.901r

3830.00 a 3830.076m

3830.311r

12

4. 5

50

7. 5

5. 5

2. 1

23. 5

3. 8

CN

Cr I CN

CN?

3.45

n 1 n U. lU

3833.959r

OQOA A9 Q

QQQ yl 1 A Q

OOO'l.ZoOlIi

6

y. o

12. 2

1 R n

1 4:0, 1

Cai

TTo T r c 1

2.71

A OA 90

OOOU.O i O ZD p 1 0 xt ly Q ^ o,o

1 1 1 ± QQQJ. Q71 m 91 Do. / A/Tn T iVlD 1 9 1 0

oooU.4yu i i. o QQQA A7A 12 9^ 9 Fe I p

Q 9f^ RR'i DDo

oooU.Duyr 1 Q n T? Q Pi 1 1 1 , ±

1 1 ooot^.oo QQOJ. Qa.

1 7 9*? 1^ R 9^ 9 9 1 1 1 i

3830.665r 10 7. 8 CN R 35 1,1 11 3834.629 3 4. 7 CN

QQQA IPiArr^ Oo6\j. i D^lli / 0 Q1 n J? e I 9 A1 99J. QQQA 79Qm

i 9. 5

f ft ^ O. O 9z. 71/

1

7A

3830.867m 65 28. 4 Fe I 2.69 284 3834.841r 1 3. 9 CN?-

QQQ1 HQ^TY^ 77 CNCN

I .UU R 43 R 43

9A

0,0

0,0 11

11

QQQJ QQf^T

3835.037

A ^

4

0. z

5. 2 -Wi? 0.41 2

3831. 198r

3831.380r

17

8. 5

9. 4

5. 5

CN

CNR 18 3,3 11 3835.161r

3835.205r 1 68 J 33. 4

[ 33. 4

CN

CN

R 40 R 40

0,0

0,0

11

11 QQQ1 con**

oooi. /uum

3831. 888r

3832.034r

7

26

14

7

7n /I

32. 4

24. 8

om II IM I CN

CN

A /i 9 R 34 R 17

AQ

Q1

1,1

3,3

11

11

QQQ Q7A

3835.39 3835.552m

±o

2362

33

QA A

33. 1

CN

CNVi

RXV 0^1

1

R 31

10.20 R 22

1.04

1 1 1,1

2

2,2 44

1

1

i X 11

10

11

3832. 166r 12 33. 2 CN? 3835.725r 12 12. 0 Sm II? 0.18 18

3832.310m

3832.510r

3832.649

3832.753r 3832.888m

oooo.Uiyr

3833.084r

1685

9. 5

16

5

51

33

600

27. 6

36. 5

8. 9

42. 7

10. V

26. 4

Mgi

CN

Nil

1 X II

Fe II p CN

be II

/2.71

\2.71

R 25

0.17 U.io

K. 66

2.64 R 33

u.UU

3

3

2,2

1

1

1,1 23

1,1

i

11

11

11

3835.978r

3836.090S

3836.199r 3836.337m

3836.501r

3836.551r

4

58

2. 5

72

1

i 80

J

3. 7

35. 4

2. 2

38. 0

r 27. 1

[ 27. 1

Zr I

|Ti II Cr I Vi?

Fe I

CN

CN

0.00

0.61

2.71 1.05

3 30

XL oy R 30

T? 91 [ XV

XV 0(7 R 30 R 91 l^xv ^1

8

127044

664

1,1 9 9

1,1 9 9

JY

zo io. / T*; t9 ooob.b/ Ur Q 9 1

3833.317m 53 34. 7 Fe I 2.56 221 3836.769m 39 23. 2 Zr II 0.56 16

3833.491r 2.

;

) 2. ] Cn 0.94 11 3836.920m 34 20. S 3833.608m 23 17. -

) CN R 24 2,2 11 3837.141m 54 3L 8 Fe I 2.61 222

3833.702m 25 19. ii TilCr I 2.71 70

3837.266r 3837.423m5. 5 24

5. C

19. ^

) CN R 20 2,2 11

100
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Not

3837.635m 46 38. 6 CNCNR 29 R 29

1,1

1,1 11

11

ooo / .oZ6t

3837.898r

[ 55

6i. a

1 37. 8 CN R 38

0,0

0,0

11

11

3838. 051r 15 44. 3 Fe I?

3838.208r 3 23. 5

3838.302m 1920 641 Mgi /2.72

12.72 3

3

3838. 538r 24 50. 5 — Ce 11 0.33 114

3838.751 63 30. 8 CNCNR 28 R 28

1,1

1,1 1111 3838.996m 17 15. 9 Nd n—

IVi

0.00

1.06 28

44

3839.139 36 32. 3 CN

CN?

R37

R 18

0,0

2,2 1111 3839.263m 104 52. 6 Fe I 3.05 529

3839.439m 44 26. 1 CN

3839.625m 68 36. 2 Fe I 3.96 995

3839.785m 82 43. 0 Mn I 2.19 6

3839.850r 8 10. 4 CN R 27 1,1 11

3839.929 11 8. 1 3840.105m 20 18. 2 CN R 17 3,3 11

3840.201 13 18. 7 Fe I p 2.28 120

3840.303r 12 25. 0 3840.447m 567 267 Fe I 0.99 20

3840.583r 26 40. 4 3840.756m 38 39. 4 IIVi- 0.04 9

3840.897r 20 33. 3 CN R 26 1,1 11 3841.058m 517 165 ||Fe I Mn I 1.61 2.18 45

6

3841. 190r 14 25. 5 3841.280m 44 38. 0 Cr I 2.71 69

3841 .349r 9 10. 2 Fe II? 4.48 128

3841.460m 22 13. 3 Co I 0.92 32

3841.583r 8. 5 4. 0

3841.730 124 42. 4 CNCN

R 35 R 35

0,0

0,0 11

11

3841.822r 11 7. 9 3841.950m 43 23. 6 CN R 25 1,1 11 3842.054m 126 39. 5 Co I 0.92 33

3842.217r 49 16. 1 CNCN

Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

TP T> or

Jiot. Line

RMT

IN 0. or

V ID. Band

004:Z.ODor 14 0. O

oo'±Z.4oUr OD OIN 3842.644m 46 15. 0 CN R 14 2,2

3842.767r 12 3. 9 Fe I? 3842.903m 26 8. 7 Fe I 2.59 222

3842.990r \

\ 141

f 28. 4 CN

Fe I-

/R 34

yix z4

2.59

tx o4

0,0

J ,1 221

A A U,U

QO/I Q OKQ« OO o JuV II A 0

(

3843. 264S 138 42. 1 Fe I 3.05 528

3843.463 73 23. 3 CN R 13 2,2

3843.626r 5 2. 3 Cr I? 3.09 3843.715m 145 44. 2 |Fei Pa t \yO I 3.42 OTA

703o4

3843. 826r 15 6. 5 CN

3843.998m

3844.031r 1 109

r 30. 9

1 0. 4

Mn I CN

2.19 R 23

6

1,1

3844.131r 3844.237m

I 1 OCX

f Izo 1 LO

1 39. 0 CNCN

Ni I

R 33 /P 6

1 "D OO {It 66

3.54

0,0

4,4 A A

U,0 137 3844.448m 53 17. 4 Vi 0.00 7 3844.574m 38 12. 8 CN

Ml' T iNl I Q CiA o.y4

3844.725r 23 7. 9 CN P 7 4,4

oo44.oy/m 46 15. o V I i.Uo A i 44 oo40.U/Um il OO o T? OO 1,1

3845.174r

3845.222r

> 14U

1 33. 8

1 19. 2

Fe I Fe I p2.42

3.40

124

701

3845.325r 16 7. 4 CN

3845.470m 135 41. 6 11 Co I CN0.92 R 32 34

0,0

3845.593r 13 5. 7

o54o. /UUm o c 00 OA O oU. 6 r e I o c c O.OO 111

c$o4o.ol£)r 1 O A (""IVT UiN —

CN P 2 3,3 3o45.9y3m 104 OO c 32. 5 |r e I CN

O O T R 21

/ Uo

1,1

3846.15 a 18 6. 5 3846.288m 55 20. 8 Fe I p CN

3.69 947

3846.417m 105 33. 3 Fe I 3.57 804

101
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot,

Line

RMT

No,

or

Vib,

Band

Notes

3846.531r 30 12. 9 CN 3849.977m 608 181 Fei 1.01 20

3846.642r

3846.679r

1 104

[ 26. 0

[ 26. 0

CN

CN

/R 31 IR 9 R 31

0,0

2,2

0,0

}"

11

3850.165m

3850.303m

59

10

27. 3

6. 5

CN

CN

R28

P 12

0,0

3,3

11

11

3846.809m

3846.950m

3846.986r

160

1 110

49. 4

[ 39. 5

1 9. 6

Fe I Fe I CNZri3.25

2.43 R 20

0.07

664

176

1,110

11

3850.402

3850.492r

3850.566r

20

65

15

9. 9

26. 0

11. 2

CN

Vii

Fe I

fP 26

\P 48

1.40

4,4

4,411 }"

3847.126r 16 7. 0 fP 13 3,3 3847.259r

3847.339

52

53

19. 4

17. 6

CN

Vi

V II 0.022.76 7 156

3850.653m

3850.826m

54

222

28. 1

67. 7

CN

Fe I

P 27 1p 46 iR 16

0.99

4,4

4,4

1,1 22

J

3847.432

3847.519r

32

13

11. 9

4. 7 Sm II? 0.33 34

3850.960m 42 23. 9 CoiFe I? Gd II

0.51

0.00

17

2

3847.63 a 4 1. 3 3851.086r 11 4. 0 CN P 32 4,4 11

3847.692r

3847.848

7

146

2. 6

47. 0 CN- R 30 0,0 7, 11

3851. 172r

3851.291m

24

102

9. 6

31. 7

Vi

CN

CN

1.06 P 32 R2744

4,4

0,0

11

11 3847.965r 18 12. 2 CN /R 30

IR 19

0,0

1,1 }" 3851.446r 6. 5 2. 3

3848.051r

3848.1 14r

18

16

7. 9

6. 2

CN

Tm II CN

P 16

0.00 R 7

4,4

2

2,2

11

11

3851.536m

3851. 599r

68

13

24. 9

6. 1

CN

CN

Fe I

R 15 1,1 11

3848.194r 19 8. 0 CN 3851.679 33 11. 3 CN

3848.297m 92 29. 4 Fe I 2.61 224 3851.756 14 5. 4 Nd II 0.18 35

3848.446r

3848.533r

12

25

4. 4

10. 9 Nd II- CN

3851.858m

3851.998r

24

1. 5

8. 0

0. 5

CN

Co I 2.54 128

3848.611r 41 13. 5 CN

Ce II P 18

0.52

4,4 36

11 3852.111r 3852.217m

15

63

5. 4

20. 5

CN

Cri 0.97 24

3848.706r

3848.847m

17

70

6. 5

24. 6

CN

CJN

/P 8 IP 18 R 18

3,3 4,4

1,1 11 3852.407m 52 19. 5 CN

fR26

R 14

[P Head

0,0

1,1 4,4 Jh

3849.006m

3849.114r

121

12

37. 7

4. 7

|Cr I CN

(La II)

2.71 R 29

0.00

69

0,012

11 3852.579m

3852.709

3852.765r

148

1

45. 2

f 14.3

{ 5.,

Fe I CN

CN

2.18 P 52 /P 20

IP 52

73

3,3

3,3

3,3

11 }"

3849.266r 14 5. 6 CN

Zr I 0.00 6 3852.912 25 8. 3 CN P 51? 3,3 11 3849.367m 88 31. 7 Cr I 3.01 138 3853.047m 46 15. 0 Til 1.97 176

3849.543m

3849.69 a

. 3849.757m

53

3. 5

36

23. 6

3. 7

25. 1

Cri

Fe I CN

0.98

R 17

24

1,1 11

3853.203m 82 26. 2 Cr ICN2.71 fR 13 ]P 22 IP 5069

1,1 3,3

3,3 }"

3849.879r

1 24. 1 CN /P 11 IP 23

3,3

4,4

3853.341m 54 24. 6 CN? /P 23 IP 49

3,3

3,3

102
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent w iQtn

AX

(ml)

Reduced

Wi'rf+Vi w luxn AX/X

(F)

ispoi SolarIdentification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Wave-

(A)

Equivalent

vv luin AX

(mA)

Reduced

vv luon AX/X

(F)

opoi

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

rNoi^js

3853.483m 148 44. 6 Fe ICN

2.95 /R 25 IP 49429

0,0

3,3 }"

3857.000r 8 3. 5 CN fP 68 IP 52?

1,1 2,2

3853.670r 23 12. 2 Si II- CN

6.86 /P 48? \P 24

1 3,3

3,3 }"

OOO 1 .UOUl

3857.154m 54

'i. I.

18. 9 CN

JP 68 \P 8 R 8

1,1 2,2

1,1

111

11 3853.732m 58 18. 7 Til 1.98 176 3857.336 28 9. 6 CN

3853.832r 31 12. 2 CN fP 47 IP 25

3,3 3,3 }" 3867.445r 23 8. 0 CN P 51? 2,2 11

3853.905r 38 13. 0 CN P 46 3,3 11 3857.667m 149 46. 4 Cr ICN

2.71 R21

G9

0,0 11

3854.059m

3854.211

67

81

21. 8

29. 3

CN

CNICr I

/R 12 IP 45 P 44

2.71

1,1 3,3

3,3 69

}>'

11

3857.819 3857.892m

3858.011r

1 73

18

1 10.9

1 16.6

10. 0

CN

CN

CN?

P 67 R 7

1,1

1,1

11

11

3854.266r

3854.370m

3854.571m

3854.673r

3854.734r

7. 5

130

189

1 64

7. 8

40. 2

57. 1

J 17.6

I 17.6

CN

Fe I

fcN

]CN

ICN

/P 28

\P 44

3.21 /PJHead

IR 24 PHead

PHead

3,3

3,3 567

3,3 0,0

3,3

3,3

}"

}"

11

11

3858.132m

3858.303m

3858.472

3858.507r

3858.589m

71

202

1 55

38

33. 2

66. 1

r 24. 8

I 4.1

21. 5

Ti I Ni I CNFe I p CN

CN

2.00

0.42 P 66

3.24 P 66 /P 49 \R 6

176

32

1,1 565

1,1

2,2

1,1

11

11 }"

3854.854m

3854.953r

3855. 124r

3855.316

3855.412r

1 84

20

1 151

1 27. 0

1 15. 0

6. 7

f 29. 4

1 22. 8

CN

CN

CN

Fe I

IV I Zr II

R 11

2.73

0.00

0.56

1.1

283

718

11 3858.689m

3858.865r

3858.917r

3858.993r

95

131

J

36. 8

' 50. 0

, 25.0

, 6. 0

CN

Mg I CN

Cr I CN

/P 49 IR 20

4.34

3.01 /P 13 \P 48

2,2

0,0

21

138

2,2

2,2

}"

}"

3855.586r

3855.631r 1 122

f 14.3

I 33. 7

Cri

CN

2.71 /R 23 IR 10

69

0,0

1,1

3859.111r

3859.223m

17 13. 7

f 53. 4

CN

Fe I

JP 65 \P 48

2.40

1,1 2,2

175

}"

ooOO.oOiin

3855.972r 3856.026m

3856.147r

ORyo

56

J

13

<!7 1 04. i

f 6. 2

1 26.0

12. 4

T e I IV I CN

Si n

0.07 P 53?

6.86

00 /9

2,2

1

11

3859.280r

3859.400r

3859.435

108

J

39

13

1 3.1

32. 6

16. 4

CN

CN

P 47 [R 5

2 2

2^2

1,1 }"

3856.232r 19 26. 8 CN

Cr I?

JP 69 IP 6

2.71

1,1 2,2 69

111 3859.668

3859.741r

51

20

62. 5

45. 8

CN JP 46 IR 19

2,2 0,0 }"

3856.381m 648 197 Fe I 0.05 4 3859.922m 1554 400 Fe I 0.00 4

3856.539r 18 26. 0 Mn I 3.37 3860.092r 17 39. 5 -Cr I? /2.54 39

OJ

3856.664m

3856.820r

66

7

39. 1

3. 6

CN

Co I

fP 7 \R 22

1.88

2,2 0,0

60

}- 3860.219r

3860.292r

32

18

41. 6

28. 4

CN

CN

P 44? 2 2 11

3856.923m 27 11. 9 CN 1 P 52? 2,2 11 3860.431r 21 18. 5 CN fP 63 IP 43

1,1 2 2

103
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3860.495r

3860.626m

3860.728r

20

61

5. 5

17. 9

34. 4

3. 8

CN

CN

Fe I p

P 63

fP 19 P 42 [R 18

3.37

1,1

2,2 2,2

0,0

701

11 h

3863. 600r

3863.701r

3863.754r

16

1 157

7. 9

1 18.9

1 40. 6

CN

Co I Fe I p

Fe I (Vn)

JP 72 IP 1 2.63

3.26

2.69

1.80

0,0

1,1 131

565

280

33

}"

3860.828m

3860.930m

3861.023m

3861.167m

35

34

51

104

18. 3

21. 8

23. 0

39. 4

CN

CN

Fe II CNCN

11 Co I

CN

fP 20? IP 41

/P 21 \P 40

P 40

1.05 fP 62

[P 39 P 62 P 22

[P 39

2,2

2,2

2,2

2,2

2,2

33

1,1 9 9

2,2

1,1 2,2

2,2

}"

11

111

11"

3863.868m

3863.976m

3864.111m

3864.305m

3864.492r

3864. 586r

23

50

46

61

1 68

9. 1

17. 1

15. 5

20. 2

1 13. 2

1 10. 4

Zr I

Fe II- CN

11 Mo I CN

CN

Feip

CNCN

1.35 0.07

/4.49

14.74 P 57

0.00 P 2 R 14

1 z.oy

13.21 P 71 P 71

66

8

127

152

1,1

1 1,1

0,0 991 565

0,0

0,0

11

3861.344m 103 42. 2 Fe I /2.69

13.27 283 663 3864.668r 16 5. 6 CN P 3 1,1

3861. 458r

3861. 547r

3861. 600r

12

]

> 250

1

10. 4

( 40. 3

[ 65. 6

CN

CN

CN

JP 24 IP 37

/P 25 IP 36 /R 17 IP 36

2,2 2,2

2,2

2,2

0,0

2,2

}"

In

}"

3864.874 3865.003m

3865.079r 3865.151m

78

28

1 76

25. 6

9. 8

J

X,0

[ 26. 9

V I — CN

CN

CN

0.02 P 55 P 55 /R 13 IP 4

7

1,1

1,1 0,0

1,1

3861.712m 35 25. 8 CN PHead 2,2 11 3865.320r

1 40

j 9. 0 CN P 70 0,0

3861.837m 51 22. 4 CN PHead 2 2 11 3865.420r 1 22. 0 CN P 70 0,0 11

3861.980m 32 10. 4 CN- 3865.533m

377

1

Fei 1.01 20

3862.114r 1 0. 4 CN 3865. 659r [ 10. 9 CN P 5 1,1

3862.227r

3862.324r

6. 5

20

2. 2

7. 0

Vi

CN

0.02 P 60

8

1,1 11

3865.913r 3865.990m 1 112f 9. 1

1 31. 0 CN /R 12 IP 53

0,0

1,1 3862.407r 18 8. 3 CN P 60 1,1 11 3866.104 39 16. 6 CN P 6 1,1

3862.494m 84 27. 4 CN 1 K Id IR 0

U,U

1,1

1}" 17 7. 1 AT

ir 69 A A U,U

3862.593m

3862.693r

3862. 763r

38

22

12

14. 8

9. 6

4. 4

Si ri CN

CN

6.86 P 73 P 731

0,0

0,0

11

11

3866. 393r 3866.445m

67

7. 2

5.7

[ 18. 1 ITiiCN

c oy

2.02 P 52

A A

1,1

176

1,1 3862.829 31 10. 9 Ti I 1.97 175 3866.553m 28 9. 8 CN P 7 1,1 3862.907r 13 5. 2 CN P 59 1,1 11 3866.722m 31 10. 6 Vn 1.43 11

3862.979r 3863.068m

3863.207r

14

41

2. 5

4. 7

13. 7

0. 9

CN

Ni I

P 59

3.83

1,1

181

11 3866.826m

3866.981m

80

61

24 7

19. 9

CN

CN

/R 11 IP 51

fP 68 IP 8

0,0

1,1

0,0

1,1

3863.401m 89 29. 2 CN /R 15 IP 58

0,0

1,1 }" 3867.064m 26 11. 1 CN P 68 0,0

3863.521r 26 9. 6 CN P 58 1,1 11 3867.224m 110 45. 0 Fei 3.02 488

104
The Solar Spectrum—Continued

Equivalent Width

AX

(mA)

24

45

9

87

54

100

35

50

58

7

78

23

45

22

80

46

88

y 120

154

94

95

50

Re- duced

Width Spot

AX/X

(F)

Solar

Identification

Low

E P

or Rot. Line

11. 9 CN P 50

15. 0 CN P 9

4. 0 Fe I p 2.61

22. 8 CN

V I

/R 10 IP 49

0.04

11. 6 -CN P 49

20. 1 Ti I —

|CN

1 98

fP 67 IP 10

1. 6 CN

Ru I P 670.81

31. 3 Fe I 2.59

15. 0 CN P 48

16. 8 CN P 11

19. 1 Fe I 2.95

3. 0 Nil 3.83

25. 3 CN

Til

R 9 1.98

10. 1 CN P 47

15. 2

8. 8

CN

CN

JP 66

IP 12 P 66

15. 5 CN- P 46

13. 4 CN P 13

20. 1 CNCN

P 45 P 45

29. 2 CN R 8

ll I — CN

l.y / fP 65 IP 44

22. 2 CN JP 65 \P 15

31. 0 Fei 2.73

18. 0 Fe I 2.73

15. 0 CN P 16

12. 1 CN P 42

25. 0 CN /R 7 \P 17

15. 8 CN /P 64 \P 41

23. 8 CN JP 64 \P 18

10. 1 |Cri- CN

0.94 P 40

14. 2 CN P 19

RMT

No.

or

Vib. Band

1,1 11

1,1 11

221

0,0

1,17 }"

1 1 11

176

0,0

1,1 1,1

0,09

11

221

1,1 11

1.1 11

430

0,0 175

11

1,1 11

0,0

1,1

0,0 11

1,1 11

1,1 11

1,1

1 1 1111

0,0 11

170

0,0

1,1 }'•

0,0

1,1 }"

284

284

1 1 11

1 1 1 1 1

0,0

1,1

0,0

1,1 }"

0,0

1,1 }"

11

1,1 11

1,1 11

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Reduc(;d Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3870.483

1 -

r 20.

CN

Cai

P 39

2.52

1,1 26 »

3870.552 1 I 19. 4 CN

Co I P 20

2..54 129

3870.664

i 53

1

23. 0 CN /R 6 \P 38

0,0

1,1

3870.714r J i 10. 6 CN P 21 1,1 3870.800m [ 27. 9 CN P 63 0,0

3870.887m

85

J 28. 4 OAT fP 63 \P 22

0,0

1,1 3871.016m 19 17. 0 CN P 23 1,1 3871.136m 13 18. 8 CN

Vi?

P 24

1.38

1,1 66 n

3871.234m 12 22. 7 CN P 25 1,1

3871.392 764 226

(CH)

fPHead

IR 5 R 7

1,1 0,0

0,0

In

3

3871.563m 77 24. 5 CHCN

Ki I

R 6 P 62

3.84

0,0

0,0 181

3

11

3871. 651r 25 15. 7 La 11 CH

0.13 R 7

13

0,0 3

3871.758m 132 41. 8 Fe I (CH)

2.95 R 8 429

0,0 3

3871.903m 37 14. 4 CH R 6 0,0 3

3872.062 59 25. 8 CN

CH

(L>y II)

R 4 R 8

0.00

0,0 0,0

113

3872.179m 19 12. 4 CN

Fei?

P 61 0,0 11

3872.273m 28 20. 9 |CN- CH

P 61 R 5

0,0 0,0

113

3872.510m 612 181 Fe I (Cai)

0.99

2.52 20

26

3872.732m 44 31. 8 |CN

Vi?

CH?

R 3

1.08 R 5

0,0 43

0,0

11

3

3872.834 30 21. 9 CH R 9 0,0 3

3872. 932m 70 31. 0 IFei

CN

2.73 P 60 284

0,0 11

3873.090r

3873. 133r

1 135

r 30. 0

1 B2. 1 CHCoi

R 9

0.43

0,0

18

a

3873.199r 15 7. 5 Ti I 2.00 176

3873.294 3S 15. 5

3873.371 26 10. 6 CN R 2 0,0 11

3873.502r

3873.575 j 97

1 13.7

1 20.9

CN

CN

CH?

P 59 P 59 R 4

0,0

0,0 0,0

11

11

3

105
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3873.767m 105 33. 4 Fe I 2.43 175

3873.959 106 S9. 6 Co I 0.51 18 3874.060m 116 47. 6 Fe I (CH)

2.28 R 4 120

0,0 3

3874.123r 12 9. 5 CN P 58 0,0 11

3874.193 35 16. 0 CN P 58 0,0 11

3874.356r 2 0. 8 Zr II? 1.49 89 3874.524m

3874.573r

85

J

f 23. 4

I 8. 0 -CH

Cr I—

CN

R 10

3.01 R 0

0,0

138

0,0

3

11

3874.726r

3874.776 j 87

f 10. 1

1 22. 4 CN

CHCN

P 57 R 10 P 57

0,0

0,0

0,0

11

3

11 3875.085m 74 25. 3 V I 0.04 7

3875.290

]

> 109

{ 24. 5 Til

CN

fO.OO \2.00

P 66

15 175

0,0 11

3875.378r I 14.7 CN P 56 0,0 11

3875.546r 45 15. 0 Sm II— 0.18 17

3875.658r 50 16. 5 3875.780m 72 23. 7 CN

|Ca I P 1 2.52

0,0 26

11

3875.884r

1 74

f 16. 5 CNV I P 55

0.02

0,07

11

o rt n A Ci 3875.948r J [ 19. 3 CN —

CH

P 55 R 30,0

0,0

113 3876.051m 141 43. 3 Fei

(Vi)

1.01 0.07 22

8

3876.310 30 10. 2 CN P 2 0,0 11

3876. 420r

3876.486r 1 64

f 12. 1

1 10.8 CN

CN

P 54 P 54

0,0

0,0

11

11

3876.566r 7 2. 4 3876.678m 40 13. 3 Fe I 2.28 121

3876.845 91 29. 2 CN

llCo I P 3

fO.43 12.01

0,01762

11

3876.978m 84 26. 9 CN—

CN

(CH)

P 53 P 53 R 11

0,0

0,0

0,0

11

11

3

3877.096r 6. 5 2. 6 3877.198m 58 19. 1 CH R 11 0,0 3 3877.344m 54 20. 6 CN P 4 0,0 11

3877.451r

1 76

f 19. 1 CNCH

P 52 R 2

0,0

0,0

113

3877.510r i 16.0 CN P 52 0,0 11

Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3877.609r 12 5. 4 Til

Zr I 1.981.00 17558

3877.709r 8. 5 4. 0

3877.835 37 29. 6 CN P 5 0,0 11

3877.935r 12 28. 3 CN P 51 0,0 11 3878.027m 555 202 Fe I 0.96 20

3878.194 30 35. 6 Fe I p 3.28 565

3878.302 78 63. 4 Mg I CN

Y II

4.34 P 6

0.18

20

0,07

11

3878.412r 13 33. 2 CH

CNCN

R 2 P 50 P 50

0,0

0,0

0,0

311

11 3878.580m 724 248 Fe I 0.09 4

3878.679r

3878.747r

\ 50

J

1 61.9

i 61. 9

Fe I Fe I |Vii- CN2.45

3.27

1.82 P 7

175

664

33

0,0 11

3878.838r

3878.900r

]

> 26

r 14. 4

1 14. 4 CN

CN

P 49 P 49

0,0

0,0

11

11

3879.041r 6 3. 0 Ru II? Zri?

3.41 0.07 6

3879.194r ' 28. 0 CN P 8 0,0 11

3879.257r 122 ^ 14. 0 CN

Cn

P 48

3.01

0,0 138

11

3879. 321r j ^ 12. 0 CN P 48 0,0 11 3879.576m 49 21. 1 CN P 9 0,0 11

3879. 659r

3879.7 14r 1 84

f 19. 6

I 13. 2 CN

CN

P 47 P 47

0,0

0,0

11

11

3879.849 21 7. 6 3879.964m 45 22. 4 CN P 10 0,0 11

3880.038r

3880.098r 100

J

[ 21. 4

L 16. 2

CN

CN

P 46 P 46

0,0

0,0

11

11

3880.190

3880.255r 1 63

r 25. 7

1 1.0

CH R 12 0,0

3880.327r ' 17. 0 CN P 11 0,0 11

3880.394r 139 ^ 22. 0 CN

(CH)

P 45 R 12

0,0

0,0 11

3880.458r . 14. 0 CN P 45 0,0 11

3880.546r 2 0. 6

3880.677r ( 16. 7 CN P 12 0,0 11

3880.74 a \ 130 \ 17. 8 CN P 44 0,0 11

3880.793r J I 14. 7 CN P 44 0,0 11

106
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3880.900r 3 1. 0 3883.639m 26 9. 3 Cri 3.01 138

3881.002r ( 24. 0 CN P 13 0,0 11 3883.76 a 2. 5 0. 9 Hf II? 1.67 18

3881.04 a i 121 \ 16.0 CN P 43 0,0 11 3884.097r 5. 5 1. 9 Ti I 1.98 175

3881.116r

3881.206 21

i 12. 0

7. 5

CN

-Cri

P 43

3.01

0,0

138

11 3884.222r

3884.292r 1 66

1 10. 8

1 23. 4

CH R 13 0,0 3

3881.307r

3881.405r

3881.490r

3881.591r

1 147

7. 5

1 127

1 30. 6

I 24. 2

3. 2

r 27. 6

CN

CN

Til

CH

CN — CN

P 14 P 42

0.02 R 1 P 15 P41

0,0

0,015

0,0

0,0

0,0

11

11

11

11

3884.369m

3884.440r

3884.609r

3884.673r 3884.844m

j 136

1 69

22

1 39. 6

1 9. 5

r 16. 2

1 11. 3

8. 7

Fe I CH

Co I Fe I Vii

2. 09 R 13

1.05

3.28

1.79

282

0,0

32

565

33

3

3881.687r [ 19. 8 CN P 41 0,0 11 3884.962r 4. 5 1. 8

3881.875 117 37. 4 CN /P 16 IP 40 }

0,0 11 3885.066 15 7. 2 Cn 3.01 138

3881. 980r 56 31. 2

Co I (Nil)0.58

0.00 18

1 3885.151

3885.225

28

1 115

22. 9

f 38. 1

Fe I Cr ICr I

2.99

0.97

430

23

3882.085r

1 136

f 24. 5 CN JP 17 IP 39 } 0,0 11 3885.286r I 7.5 Sm II Co I 0.48

0.92 4631

3882.170r

3882.300r

3882.391r

1

> 141

J

1 24. 5

( 30. 9

l 19. 1

CN

Til

Til

CN

P 39

2.02

2.02 fP 18 \P 38 P 38

0,0 175

176

r

0,0

11

1 -1 1 i

11

3885.519m

3885 657r 3885.756m

3885.865r

3885.933r

87

6. 5

35

6. 5

30

3S. 7

3. 9

19. 0

6. 4

20. 6

Fe I

Fe I p

Nil

Fe I p

2.42

3.26

0.27

3.69

124

567

1

946

3882.511r

1 127 I 28. 3 CN /P 19 IP 37 } 0,0 11 3886.065r 10 15. 9

3882 594r [ 17. 8 CN P 37 0,0 \\ 3886 155r 6. 5 16. 7

3882.754r

i 112

J [ 13. 9 CN

/P 20 IP 36

P 36

f IJ)'-'

0,0

1

1

11

3886.294m

3886.428r

3886.564r

920

11

8. 5

306

31. 6

11. 8

Fe I CHVi?0.05 Q 1

1.38

4

0,0

64

3

3882.847r

> 140 1

28. 3 CN fP 21 \P 35 }

0,0 11 3886.804m 50 26. 2 Cri 1.00 23

3882 894r J \ 28. 3 Ti I 2.04 176 3886 940r 4. 5 5. 4

3882.996 118 38. 9 CN P 35 0,0 11 3887.059m 219 96. 9 Fe I 0.91 20

o»8d.ll4r n 1 91 30. 4 CN fP 22 \P 34 \ 0,0 11 3887.372r' 8 4. 9 Ti I? 2.00 176

3887.526r 1 0. 5 3883.200r 27. 0 CN

(Vii)

fP 23 IP 34

1.43

} 0,011

11 3887.730r

3887.890r

3

10

1. 7

5. 4

3883.287r

3883.394r

3883.429r

3883. 551r

228

band

3

27. 0

? edge

- 1. 0

|Cr I r e I CN

Head

CN

0.98

P 24

to P 33

23 DDo

0,0

0,0

11

11

3888.041

3888.21 a

3888.29 a

3888.422

9

3. 5

4. 5

23

15. 5

2. 6

4. 6

35. 2

Til

Fe I

2.00

3.26

175

565

107

761-925—66—10
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

bolar

Identification

Low

ill r

or KOl. Line

RMT

IN 0. or

V ID. Band

Notes Wavelength

(1)

Equivalent Width

A \ AA

(ml)

Reduced

Width

AX/X

(F)

Spot

bolar

Identification

Low

ii; r

or Kot. Line

RMT

iNO. or

Vib. Band

Notes

O O O O C O /I *^ oo!3».o24m /DO 1 1 A ilo r e I A n: 40 ooyo.cSi / / ZD. U r e 1 Z.OO od4

oooo. / /or 1 f\ TO 1 ooyo. 4U^II1 V 1 QO > ioZ < oZ. 0 r e I 0 0 K

oooo.o/ym A n4y do. D Fe I Q no o.VZ AQQ 4oo ooyo.4Dor ) \ 4. »

3888.938r 6 8. 2 CH Q 2 0,0 3 3893. 606r 5. 5 1. 8

3889.05 2346 722 Hs 10.20 2 10 3893. 795r 1 0. 4

3889.105 12. 5 23. 9 CH Q 1 0,0 3 3893.920m 70 26. 2 Fe I 2.43 175

3889.231 25 22. 5 CHr e I

.'^ R 14

z.oy

0,0 3 3894.029

1

} 154

f 26. 1 Fe II 3.30

0 OA u.yo 663OQ

oooy.ooo 4U. 0 zo. y Fe I

It 14

/3.21 \3.27

U,U 562

660

Q Q CO/1 1 no

3894.21 8r

J

9 3. 1

Oo I Pd I

1 .uo

1.45

QAo4

8 3889.676m 42 22. 6 Nil 0.21 15 3894.493 33 11. 3 u Fe I 3.21 566

3889.848m 28 22. 1 CH Q2 0,0 3 3894.63 Ir 9 5. 4 u Nd II 0.06 29 3889.929m

ooyU.Uoor

3890.196

3890.311r

55

Z. b

35

6. 5

26. 7

1 A

1. 4

16. 4

3. 1

Fe I1 li 1

torn II ViZri

3.26

U.UU

0.04

0.15

564

1 K 10

1 /

8

8

3894.713r

3894.85 a 3894.986m

3895.088m

11

1. 5

78

58

6. 6

0. 9

25. 6

21. 2

u

s?u

Gd II

Co I CHCe n

0.00

0.63 Q 5 0.61

1

18

0,0 210

3

3890.399m 44 19. 5 Fe I 3.24 567 3895.167r 21 12. 6 CH R15 0,0 3

3890.568

3890.722r 3890.849m

38

3

64

16. 7

1. 4

27. 0

II CHIN a II Nil

Fe I

Q 3

3.54

2.73

0,0

280

3 3895.242m

3895.334 3895.448m

58

46

87

19. 8

19. 3

42. 3

su

u

Til

CHFe I-

|CH

2.04 R 15

3.29 Q 5

176

0,0

565

0,0

3

3

3890.945r 20 8. 3 Nd II 3895.582r 10 15. 7 Mgi 7.17 QQ01 1 OQ

QQQ1 QQO ooyi.ooo

3891.511

3891. 682r

ID

35

3

A A

D. 4

14. 6

1. 2

iiV I U.io

U,U

1 1 1 i

6 3895.667m

3895.794r

3896.139

\ 361

J 58

{115

[ 10. 0

19. 9 u

l*e I (Mgi)

Vi

IIV II

n 1 1 7.17

1.08

1.40

447

43

10

3891.781 30 11. 6 Ba II 2.51 4 3896.248r 24 8. 7 u Er II? 0.05 3891.934m

3892.015r

3892.11 a

88

9

11

32. 4

3. 9

4. 1

Fe I (Mg i;

Co I

3.41

7 1 7 /.I /

2.54

733

47

130

3896.363r

3896.472

3896.534r

20

62

14

6. 5

19. 2

5. 9

u

s

Zr I? CH?

0.07 P 29

0,0 3

3892.314 28 10. 3 Fe I 3.55 3896.622r 27 8. 7 u Fe I p 3.65 834

3892.452r 3892.591m

3892.898

3892.988

3893.074

3893.214r

3

49

78

72

63

6. 5

1. 2

16. 4

26. 2

29. 8

30. 3

2. 2

Fei?

CH

|Fei

Vi

(CH)

Fe I CH

Q4

2.76 0.04 P 1

3.26 Q4

0,0

283

7

0,0 567

0,0

3

3

3

3896.781m

3896.982r

3897.073r

3897. 199r

3897. 345r

3897. 458S

21

2. 5

2

6

10

83

5. 9

0. 8

0. 6

1. 9

3. 1

28. 4

u

u

u

u

u

u

Ni I (Ce 11) Sm II Vi?

TiiFe I (CH)

3.80

0.56

0.04

2.26

2.00

2.95 P 2

188

5

126

175

429

0,0 3

108
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3897.648r 27 8. 5 u -Cr I

3897.778r 26 8. 8 u 3897.900m 98 28. 7 s Fei 2.69 280

3898.014

3898.094r 158

1

f 55. 1

\ 18. 7 J

Fe I CH1.01 Q 620

0,0 3

3898.277r 22 7. 2 u Vi?

Ce n 0.47 52 3898.394m 74 22. 4 u CH Q 6 0,0 3 3898.512m 42 14. 9 s llTii CoiDy n

0.00

1.88 0.59

1358

3898.65 a 2. 5 0. 8 Fe I?

3898.774r 1 0. 3

3898.878r 4 1. 3 3899.036m 85 25. 4 s? Fe I 2.45 175 3899.142m 62 22. 6 u Vii 1.80 33

3899.326r 8 3. 1 Mm?

3899.393m 22 9. 0 u

3899.719m 436 132 s Fe I 0.09 4

3900.224 16 5. 6 u Nd II

3900.333r 4. 5 1. 5

3900.412r [ 5. 6

3900.44 m \ 157 - S 13 3900.541m J u Fe I-

||Ti 11 3.241.13 56534

3900.660r 20 7. 1 Al II? 7.42 1

3900.770r 12 4. 6

3900.836 52 15. 9 u 3900.963m 37 11. 3 s Til 0.02 15

3901.060r 7 2. 2 Fe I? p 3.60 834

3901. 160r 4 1. 3 u Vi? 2.29 126

3901.337r 0. 5 0. 1

3901. 484r 4. 5 1. 4 u

3901.598 62 20. 0 u CH Q 7 0,0 3

3901. 741r 3 1. 0

3901.866 71 21. 4 u CH Q 7 0,0 3

3901.977 36 13. 3 11 CH —

Cr I P 3 0,0 3

3902. 104r 17 5. 2 u

3902.262 61 21. 5 Vi

1 (CH)

0.07 R 167

0,0 3

Wavelength

(1)

Ec(ui- valent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3902.430 44 14. 9 u Gd II —

CH

0.42 R 1619

0,0 3

3902.632 35 15. 9 CH P 3 0,0 3

3902.779r ( 6. 1 3902.956m

> 530 IU2 u Pel

Cr I (Mo I)

1.5G 0.98

0.00

45

23

1

3903.079r . 6. 0 3903.161m 18 15. 4 s Cr I 0.97 23 3903.257m 40 19. 5 u Vii 1.48 11

3903.416r 4 1. 5 Sm II

3903.546r 11 3. 8

3903.731r 8. 5 3. 4 3903.854m

3903.915m

[ 224

f 25. 0

1 52. 2 u,n Mgi

Fe I

4.34

2.99

19

429

3904.076 28 10. 2 u

3904. 173r 1. 5 0. 6

3904.330r 4 1. 3 Mn I? 4.68

3904.476r 1 0. 3

3904.630 20 7. 3 u Ni I p 0.42 29 3904.790m 60 2L 3 s Til 0.90 56

3904.879 28 13. 1 u

3905.009 29 12. 7 u Fe I p 3.42 703

3905.189 28 14. 9 u Fe I p 3.24 564

3905.360r 8 15. 1 3905.532m 816 219 S Si I 1.91 3

3905.679 48 46. 1 |CH

Fe I p

Q 8

2.47

0,0 153

3

3905.769r 24 14. 9 3905.905m 61 25. 9 u CH Q 8 0,0 3

3906.032r 19 7. 9 u,N — Fe n 5.57 173

3906. 181r, 1. 5 0. 5

3906.300 52 19. 1 s Co I (Er II) 0.51 0.00

17

3906.402r 7. 5 4. 3 3906.490m 164 66. 9 s Fe I 0.11 4

3906.626r 8 3. 1

3906.752S 77 24. 3 s Fe I 3.30 664

3906.963m 34 10. 7 u Fe I p 3.28 56"

3907.114 28 8. 7 u Eu II 0.21 5

109
The Solar Spectrum—Continued

VV ilVc- length

(A)

EquiTTO 1 An "f V cllcii L Width

A (mA)

Re- Width

A \ /\ iSA/ A

(F)

Spot IdentiLow

or

T?nt Line

RMT

Nn1> u. or Vih V lU. Band

Notes

3907.231r 17 5. 4 u,N

3907. 296r 6. 5 2. 0 Ce n 1.11 253

QQn7 j.7ft oyu* .4t / o 1 o s

IC!/> T |oC I Fe I u.UU

2.76 g 284

3907.672m 36 11. 0 u Fe I 3907.774m 41 12. 8 XI Cri 3.84 PX 4^1 262

qo S9 9J. ft H r e I 9 7fi Z. 1 D 980

3908.067r 6 1. 9 Pr ri? 0.55 11

3908.174r 5. 5 1. 8 sons 974- lO. o 11 P 4 Qo

3908.411 26 7. 9 It Ce IIPr II 0.86

0.00 65

11

3908.548 36 11. 1 U Ce II Fe II p0.46

9 7n

1279Qzy

oyuo-Ooor oonc oyuo. 7A9m 1 D^iii1 98

J

f 4. 1

S

r e I

v^r I

Z.40

i.UU

loo

9^ZO

oyuo.y Do iy. o 11 INI I o.Dl 117 11^

oyuy .u / or K0 i. o

3909.285 25 7. S s,N

QQflQ AnOr oyuy .T:U.ir X. O U, 0

QoriQ c;n9T- csyuy .ouzr 0. O It 3909.668m

OQAQ oyuy.797r i LiT 89

J

1 39. 2

I. U. o

u Fei 3.28 565

oyuy.oo * in i 10 u r e I oD*

oyuy.y^:!!!! Q7y / A^11. 7/ s liCo I Vi

A nn U.UU /0.07

11. oO

qo

7DO

3910.075r 9 2. 8

OQ1 n 91 9r cD

QQ1 n ^^j. / y 94 1 n n U,U qO

OQ1 n ^707* oyiu.'i / yr

oy lu.oo"*

1 114

J

7.8

4

u

U,U qO

oyOQ1lU.DD n fifi7/ A ID. u u

QQl n Q/1 Qr>i oy iu.o'iyin. CAOD OR 1 ZD. 1 u l<e I 2.7d Z»4

oyi i.uuoni 1

A

ZZ. 0 u l*e I O.Zl ceo 5dZ

oy i Luy-ir O. O 0. 1

3911.180 40 12. 3 s Til 2.04 175

3911.308r 8 2. 6

3911.417r 11 3. 6 u,N -Mn 1? 4.19

3911. 571r 0. 5 0. 3

VV diVc- length

(A)

Equivalent Width

A \ (mA)

Red.uc6d Width

AA/ A

(F)

Spot

ooiar

Identification

Low

T? P

or

itot. Line

RMT

1% 0. or

V ID. Band

Notes

QQ1 1 701 oy 1 i, * ui QA in c lU. 0 u i? e I q qn o.cSU DD4

3911.825m 60 18. 2 s Sc I 0.02 8

3911.989 76 25. 6 u

3912.087r 17 6. 3 u,N

3912.203r 15 5. 1 s Vi ri.04 11.05 4243

QQ1 9 9QJ.m DO u Ml* iM TI Qo.oUftn 101

3912.422 14 4. 6 u Ce II 0.30 60

3912.594r 3. 5 1. 0 s Til 2.02 175

3912.797r 11 3. 3 u Fe I

3912. 892r 6 2. 0 ViJrr II I 1.06 n 9n 42

11 7

1

QQ1 oy i^.yoiiii 9 QQ1 m 01 ID. O s iM I U.Uo 10

QQ1 Q 1 A^.?* Qo

oy lo.^oo A O 1/1 ft 11 QQ1 O A^lfi 1 qo loo QQ A oy. 'I u Tl TT 1 1 II 119 04

QQ1 Q A'?7m oy io.Do / III lUl OQ 9 /y. z s X e I 9 9ft 1IZUon

QQ1 O CO Q K C

0. 0

1 A 1. D

3913.89 a 2. 5 0. 9 3914.013m 53 16. 6 CH P 5 0,0 3

3914.181r 35 15. 8 u

3914 287r

OQ1 A QQQtI 133

]

f25. 0

- OO O |,ZZ. z \J

r Fei

11

1

l(Vii)

3.28

U.DO

1.79

567

lO33

OQ1 A /t9fi 7n OA 1 ZD. 1 u PTT1

L

p n n Qo

OQ1 /t K1 9- tiA D4 A q 14. o u

T?C» TT r e II Fe I p

11 .DR7/ 3.27 660

3914.740r 7 2. 3 s Fe i11

1

3.25

u.UU 662

14

QOI /I OA o oyi4.yu a. 1 A Q

U. O n

1

^9 / 2. 4

Pr- T v^r I o.Ulni 1lo^7/

3915.05 m 5. 5 1. 7 3915.218m 46 H. 0 u Fe I

3915.34 a 4. 5 1. 4 Ir I? 1.22 6

QQ1 K 79 oyio.'i/o 49 14. 5 u

[1 T?^ - \\be I—

Co I 2.28 113

3915.612 78 23. 0 CH QIO 0,0 3

3915.811 110 32. 0 s? CHCr I Q 10

3.01

0,0 136

3

3915.939 47 14. 4 u Zr II 0.53 17

3916.067r 22 6. 5 u La II 0.23 42

110
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/\

(F)

Spot

Solar

Identification

Low

E P

or Rot.

Line

RMT

No.

or

Vib. Band

Notes

3916.244 67 19. 1 s Cr I 0.97 23 3921.187 59 24. 0 u

3916.405 85 25. 8 u — V 11 1.43 10 3921.276 40 18. 6 u Fe I 2.56 220

3916.521r 11 3. 8 Gd II 0.60 20 3921.428m 50 19. 3 s Ti I 0.00 14

3916.605r 8 2. 6 Zr I? 0.15 6 3921.556 79 27. 8 w CH Q 11 0,0 3

3916.737S 90 SO. 2 u Fe 1 3.24 606 3921.716 75 26. 8 u CH Q 11 0,0 3

3916.852r 8 2. 7 3921.904r 3. 5 1. 3 s Vi 1.05 42

3916.985r 17 6. 1 u Cr I — 3.01 137 3922.020r 4. 5 1. 8

3917.124r

3917.184r

3917.36 m

1 151

29

1 16. 6

9. 5

s

u

Co I Fe I

2.28

0.99

113

20

3922.084

3922.421r

24

34

9. 5

14. 3

u,d

s

Fe I Sm 11 —

ilVi

/2.48

13.29

0.38

1.06

153 564

38

42

3917.591r

3917.653r

3917.867r 3918.017m

3918.113m

3918.256r 3918.324m

3918.424m

3918.573r 3918.651m

3918.789r

3918.895r

3919.069

3919.168

3919.359r

3919.568r

J 23

11

1

4. 5

1

190

1 121

11

19

156

J

2. 5

9

f 6.

6

1 1.0

3. 7

0. 3

1. 5

1" 6. 6

< 33.4

I 28. 8

f 6. 1

1 34. 4

3. 6

6. 5

[ 26. 5

1 30. 1

0. 9

3. 3

s

u

u

u

u

u

u

u

u

s

u

Cn

Hf II? Ce II Fe I Fe I Fe I p

Fe I

Fe I Cr I

3.01

0.45

0.70

2.48

2.84

2.83

3.02

2.99

1.03

137

7

12

124

364

362

430

430

23

3922.674

3922.768r 3922.923m

3923.041r

3923.107r

3923.236r

3923.333r

3923.502r

3923.692r

3923.926r

3924.067r

3924.174r

3924.353r 3924.533m

3924.652r

42

18

414

23

5. 5

1. 5

7

11

2

1

20

19

2. 5

68

13

28. 3

24. 5

124

35. 0

5. 9

1. 0

3. 6

4. 8

0. 8

0. 4

8. 5

8. 5

1. 0

29. 4

5. 6

u

u,N

S

u

w

u

u

u

su

Fe I p (Mn i) Co I Fei

Fe I p

Ce II

Mn I?

Sc II

Hf n?

Mn I Nil

Til

Ce IIIV I

2.99

3.85

1.05

0.05

3.25

0.56

4.25

0.31

1.60

3.86

4.10

0.02

0.56

1.87

429

44

32

4

661

191

9

18

44

240

13

19090

3919.730r 5. 5 2. 0 u 3924.790r 1 1. 0

3919.817r

3919. 975r

8

4

3. 1

1. 8

s Ce II-

|Ti I 0.701.50 60 130

3925.014r 3925.209m7. 5

70

3. 1

32. 0 s Fe I (Vi)

3.29 0.07 567

8

3920.125r 7. 5 9. 7 3925. 352r 8. 5 4. 0 3920.269m 341 101 s Fe I 0.12 4 3925.45 a 5. 5 2. 6 Pr II 0.00 11

3920.452r 28 16. 1 3925.538 33 16. 6 u Fe I p 3.25 660

3920.629 76 31. 6 u Fe I 2.42 153 3925.651m 74 32. 8 u Fe I 2.83 364

3920.729

3920.844m

3921.049r

69

77

125

27. 8

27. 6

42. 1

u

u

s

CHFe I Cr I (CH)

JP 6 IR 18

3.26

0.98 P 6

0,0

0,0

567

23

0,0 3

3925.800r

3925.949

3926.027

3926.181r

9. 5

86

76

8. 6

4. 8

38. 9

51. 2

5. 1

uu

Fei

Fei

2.86

3.24

364

562

111
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent

vv lutn AX

(mi)

jxeduced

rt7; W ^ + V. latn 1 AX/X

(F)

spot

Solar

Identification

Low

E P

or Rot. Line

iXiVL 1 No.

or Vib. liana

IN otes Wavelength

(A)

Equivalent W icitn AX

(mi)

Ke- duced

Wicttn AX/X

(F)

bpot

Solar

Identification

TLow

E P

or Rot. Line

RMT

No.

or Vib. BandI^otes

3926.326 13 7. 9 s Til 2.58 292 3932.018m 10 34. 7 U Ti II 1.13 34

3926.458 34 19. 0 u Mn I 3.84 44 3932 254 1. 5 5. 6 U Fe I

3926.639 6. 5 4. 2 u Cri 4.53 3932.484r 1 6. 9 U

3926.777r

3926.939r

3927.129r

3927.252r

3927.344r

0. 5

2

4

1

4

0. 5

1. 4

3. 1

0. 6

3. 1

u

u Nd II? -

3932.637m

oyo^. yior

oyoo.DoiSlIl

10

1. 0

52. 9

11 0 i i. y

u Fe I

r e I

»^a II ) (Sci)

( V I) (Coi)

/2. 73

U. UU

0. 02

X. Uo

0. 58

280

8

17

3927.443 25 16. 3 u 3934.366r 6 35. 3 Fe I

ovZl.bUoV zo 1 Q A io. D Fe I p Z.io ono c oi At. aD

0,?

0927.// m 1 9lc5 lo. o /. 0

oci 0 ZD. u X e I

3927.797 r 42 41. 7 3935.446r 2 8. 4

3927 933m 187 s Fe 1 (CH)

0.11 P 7 4

0,0 3 3935.645r 11 3L 0 u,N CH /P8

IQ 13

0,0

0,0 }^

3928.091 63 50. 6 u Fe I 3.21 565 3935.73 a 5. 5 18. 0 CH Q 13 0,0 3

3928.217

3928.345

3928.496 r 3928.644m

3928.764 r

3928.93 a

3929.122

3929.223

68

46

6

45

1

Z. 0

37

37

49. 4

32. 8

6. 6

82. 8

1. o

Q 7 O. (

33. 8

33. 8

u

s

u

u

CH

CH

Cn

± 1 I P

Fe 1 Fe 1 La 11

/P 7 IQ 12 Q 12

1.00

2.76

3.25

0.17

0,0

0,0

0,0

23

I/O

280

659

27

}^

3

3935.826m

3935.979

3936.557r

3936.770r

3936.963r

3937.06 a

3937.141r

3937.336S

35

30

7

8

2

2

2

38

66. 4

59. 4

16. 2

16. 8

4. 1

3. 8 4 3

u

s

u

u

s

Fe I Co I (CH)

(Fe 11) Fei

Fe I p

Fei

2. 83

0. 92 P8

5. 57

3. 21

2. 69

362

32

0,0 173

564

278

3

3929.357 24 27. 7 u 3937.438r 4 7. 1

3929.523 r

3929.724 r 3929.885m

3930.040 r

o

Z

20

37

20

O. D

25. 6

39. 1

32. S

s

u, N

su

llZr I Zr II Vii

Til

ViU.U/ 2.43

1.43

0.00

1.38

'J 142

10

13

63

oy^ / .ooor QQ07 QOOt' oyo / .oour

QflQ7 07/1t»

oyoo.uior

0. 0 9

0. 0

0. U

9 8

OQ Q Zo. 0

u |i* e I Til 2. 27 246

3930.150 r 26 40. S 3938.184r 7 8. 8

3930.308m 108 181 u Fe I 0.09 4 3938.298 31 37. 4 w Fe II 1. 67 3

3930.513r 32 49. C) u Eu II — 0.21 5 3938.409 71 47. 7 u Mgi 4. 34 18

3930.663 r 7. t) 20. i) u Yii 0.41 16 3938.630r 11 11. 4 u Fei

3930.889

r

3. f) 10. [ u Fe i- 2.45 3938.734r 2. S 2. 4 Ni I 4. 17 240

3931.129m 22 50. i u Fe I 3.26 565 3938.865r 6. 5 6. 0 u Co I 3. 57 171

3931.342

r

3931.898r

3

1. .

11.

'

j 6. ][

Vi?

Ce II Fe I

1.85 0.30 90

61 3938.970r

3939.146r

3939. 391r

4

8. 5

2. 5

3. 5

7. 4

2. 3

uu,N

Fe 11 5. 91 190

112
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Banc

Notes Wavelength

(1)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notc-s

3939.518r 3. 5 2. 8 u So n? p 0.31 9 3944.541r 2 1. C

3939.66 a

3939.885r 3940.041m

3940. 183r

3940.358r

3940.671r 3940.890m

1

1

28

1. 5

9. 5

13

84

0. 9

0. 9

16. 2

0. 9

6. 3

7. 6

S8. 6

u

u

u

s

Fe I

Ce IICoi

|Fe I

3.41

0.32

0.63 0.96

731

50

1820

3944.684r

3944.744r 3944.898m

3944.988 3945.127m

3945.218 3945.332m

1 73

72

32

79

28

68

f W. 4

I 22. 6

37. 4

15. 6

38. 1

13. 8

24. 8

Iu

V

sw

u

f Fei?

Dyii

i Fei

Fei

Fe I Fe II p Co I

0.00

2.84

2.99

2.76

1.69

0.92

361

430

280

3

29

3941. 049r 7 4. 1 3945. 493r 10 3. 8 u Cn 3.01 135

3941.182 30 15. 0 u 3945.687r 0. 5 0. 3

3941.284r 60 37. 6 u Fei 3.26 562 3945.854 36 13. 7 u

3941.369r 5. 5 2. 6 3945.961r 10 3. 8 u Cr I 3.01 134 3941.496m

3941.612r

3941.737

3941.856

52

3. 5

47

25

26. 8

1. 6

20. 8

11. 9

s

s?u

Cn

Co I |NiiSm II

1.03

0.43

3.83 0.00

23

17

171

1

3946.048r

3946. 200r

3946.38 a

3946. 459r

7. 5

2. 5

1

2. 5

3. 0

1. 0

0. 5

1. 1

u

u

Cai

Fe I Ni I

2.71

0.17 1

3942.016r 5. 5 2. 5 s Vi 1.38 63 3946.553r 9. 5 3. 3 u

3942.155 10 4. 7 u Ce II 0.00 37 3946.660r 22 6. 6 u

3942.239r 1. 5 0. 8 Ci? 7.68 3946. 813r 5. 5 2. 0

3942.370 41 21. 6 u Fe I 3947.002m 83 38. 8 u Fe I 3.21 561

3942.448

3942.607r

72

7

29. 4

3. 2

u Fe I 2.84 364 3947.133r

3947.161r

] 24

\ 6. 6

1 2. 8

u Co I 1.96 58

3942.746r 15 6. 6 u Ce II 0.86 57 3947.27 a 3 1. 0 Oi 9.14 3

3942.844r 15 6. 6 u -Mm? 3.84 3947.385 49 17. 0 u Fei 2.40 153

3943.098r

3943. 182r 3943.348m

3943.482r

3943.581r

3943.679r

3943.820r

3943.918r

0944.Ulom

3944.11 a

3944.179r

3944.352r

33

22

52

20

33

5. 5

36

3

1 37

16

15. 3

11. 5

23. 9

11. 1

18. 8

4. 6

39. 6

8. 9

-too

1 29. 4

1 33. 1

7. 8

uu

u

uu

s? u,N

co

u

Fei

Fei

Vi

CH

Ce 11-

|CH

A 1 -r Al I

J Nil

1 CH

2.20

1.08 Q 14

0.79 JP 9 IQ 14

o.uo

3.63 P9

72

42

0,0 234

0,0

0,0

1

151

0,0

3

3

3947.538m

3947.693

3947.778

3947.978r 3948.109m

3948.281

3948.476

3948.680 3948.785m

3948.900

3949.061

3949.141

86

45

74

9. 5

99

354 5 94

80

50

1

89

38. 1

21. 6

24. 3

3. 5

31. 1

12. 7

1. 8

32. 7

25. 6

16. 7

i 19. 7

u

u

s

uu

su

s u,N

u

Fei

Til

Fe I p

Fe I Fe I p Fe I Til

Fei

Cai

La II Fe I

(2.83 12.95

0.02

3.30

3.24

3.24

3.21

0.00

3.27

1.88

0.40

3.41

361 426

14

652

562

561

560

13

604

6

41

730

113
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3949.230 21 6. 8 u Fe I p 2. 48 153 3953.661 7 2. 1

3949.402 3 1. 0 u — Pr 11? 0. 20 16 3953. 706r 3 1. 0

3949.605 6. 5 2. 3 u Cr I 3. 01 136 3953. 861S 51 16. 2 u Fe I 2. 83 362

3949.70 a 2 0. 8 Cr I? 3. 01 136 3953. 966r 2. 5 0. 9

3949.814 9. 5 3. 0 u 3954.046 9. 5 3. 0 u

3949.959S 103 33. 4- u Fe I 2. 18 72 3954.276r 0. 5 0. 3

3950.139 14 4. 6 u 3954.396 4 1. 3

3950.253 4 1. 3 V 1? 3954.540 37 12. 1 u Ni I 3. 65

3950.358 55 17. 7 V Y n 0. 10 6 3954.718 29 9. 6 u Fe I 3. 27 606

3950.469 15 5. 1 u 3954.95 a 4 1. 3

3950.58 a 1. 5 0. 5 3955.09 a 5 1. 6

3950.795 3. 5 1. 1 Fe I p 2. 45 153 3955.219 38 15. 4 u Fe I 3. 05 527

3951.081

3951.171

1 126

j

[

9. 8

1 30. 6

uu

Cr I Fe I

3. 01

3. 27

136

661

3955.343

3955.484

107

16

33. 8

5. 4

u Fe I 3. 28 562

3951.310r 9 2. 8 3955.606 11 4. 0 u

3951.435 10 3. 2 3955.762 13 3. 8 u Fe 1 p 2. 56 219

3951.626 22 7. 1 u Fe I 2. 86 362 3955.831r 1 0. 3 Zr II? p 0. 56 17

3951.776 20 6. 6 u Cr I- 3. 01 136 3955.963m 64 20. 7 u Fe I 3. 07 488

3951.839r 1 0. 4 Hf I? 0. 29 3956.059 9 3. 2

3951.964 63 19. 2 u Vii 1. 48 10 3956.179r 5 1. 6

3952.096 5. 5 1. 8 3956.339 110 35. 0 s Ti I 0. 02 13

3952.201 14 4. 6 u Nd II 0. 00 23 3956.463m 94 29. 3 u Fe I 3. 24 604

3952.338 s Co I 0. 43 16 3956.686m 133 41.8 u Fei 2. 69 278

3952.408 \ 46 s? Cri 3. 01 136 3956.891 11 3. 9

3952.468r J

1 133

I 0. 9

[ 0. 9 Ce II JO. 33

10. 82

113

177

3957.041m

3957.287r

123

2

4 0. 3

0. 8

u FeiCai

3. 26

1. 89 562

6

3952.616 [ 37. 9 u Fe I 2. 69 278 3957.485r 1. 5 0. 5

3952.756r

->

\ 100

r 07 A Zi. D

1 6. 3

u J: e I CH

Z. 04

P 10 0,0 3 3957.797

OO4 5

1 O 1 iZ. J.

1. 6

u X e I O. iSO

3952.905r

3952.982 1 159

1 28. 0

1 28.

0

[ Coi

I CH

0. 92

fP 10 IQ 15

28

0,0

0,0

3957.936

3958.093

54

9. 5

17. 7

3. 4

s Co I Cri?

0. 58

4. 45

18

307

3953.082 27 12. 5 0? CH Q 15 0,0 3 3958.216 86 27. 0 s IITiiZr 11

0. 05

0. 53

1316 3953.158m

3953.256

3953.408

3953.502

97

37

7

40

38. 8

14. 0

2. 3 n. 7

u

u

u

Fe I Cri

Fei

Fei

3. 02

3. 01

3. 55

430

136

770

3958.338r

3958.416

3958.508

3958.636

2. 5

27

3. 6

3

0. 9

9. 6

1. 3

1. 1

u Fei

Pdi 1. 45 8

11 4
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Idcntificatioii

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3958.740 31 10. 8 u Fe I 3964.190 15 13. 2 0? Ni I 3. 65

3958.870r 3. 5 1. 3 Rh I? 0. 97 7 3964.280 48 SO. 6 Ti I 0. 02 12

3959.03 a 1. 5 0. 5 3964.406 1 0. 9

3959.195 8 2. 9 u 3964.526m 53 32. 8 u Fe I 2. 84 361

3959.293 5 1. 8 u 3964.759r eTs 6. 0

3959.453 4. 5 1. 7 s Fe I p 3. 21 556 3965.016 1 0. 9 Co I 1. 05 31

3959. 542r 2. 5 1. 0 Gd II? — 0. 73 44 3965.230 3. 5 4. 3 u Co I 0. 92 30

3959.726r 1 0. 4 3965.349r 2. 5 3. 0

3959.833

3960.153

15

2

5. 9

0. 8

u 3965.470

3965.516

] 39

2. 8

[ 33. 2 u

Fe I Fe I

3. 25

3. 24

658

565

3960.284S 50 18. 7 u Fe I 3. 64 913 3965.618 2 3. 5

3960.410 2 0. 8 3965.726 12 15. 9 u

3960.647 3. 5 1. 4 u Fe I 3965.845 9 12. 8 11 Fe 1 p 2. 42 122

3960.765 6. 5 3. 6 u Cri 2. 71 68 3965.930 25 30. 2 u

3960.916 7. 5 4. 2 u Ce n 0. 32 84 3966.073m 66 60. 0 s Fe I 1. 61 45

3961.010 11 6. 3 u Cox 2. 63 128 3966.356r 4 9. 1 3961.149m

3961.286r

44

2

28. 0

3. 0

u Fei 2. 86 361

3966.511 35 46. 1 u Fe I

r3. 29

^3. 30

l3. 55

562

652

766

3961.535m 621 220 s All 0. 01 1 3966.639 44 70. S u Fe I /2. 76

13. 21 282

562

3961.916

3962.090

3962.179

3962.360

3962.398r

3962.649

3962.722 3962.861m

3962.972r 3963.115m

14

33

41

1 60

10

22

46

5. 5

81

11. 9

20. 8

21. 4

24. 2

8. 8

6. 3

12. 0

2A. 0

3. 3

S8. 6

uuu

u

u

u

s

u

-Nil

CHFei

CH

Fei

Fei

Til

Sm 11 Fei

(CH.)

3. 85 P 11

3. 26 P 11

3. 64

0. 00

3. 28 Q 16

199

0,0

566

0,0

913

12

562

0,0

3

3

3

3966.824

3967.055r 3967.431m

3967.636

3967.859

3967.975r 3968.492m

3968.715r

3968.936

11

5

19

7

7. 5

7

15467

3

6

28. 2

15. 1

54. 0

26. 4

29. 5

34. 8

(3435)

20. 6

37. 2

u

u

ul

Fe I CeiiFei

Fe I Ca II (H)

(V II) (Dy ii)

3. 30

0. 33

3. 30

3. 24

0. 00

1. 40

0. 00

659

84

604

561

19

14

3963.222 47 28. 5 u CH Q 16 0,0 3 3969.06 a 5 18 Cr I 2. 54 38

3963.347 4 2. 5 Ti I? 1. 05 81 3969. 148r 5 18 Co I 2. 54 128

3963.437 20 12. 1 u Fei 3. 27 654 3969.268m 52 103 u Fe I 1. 48 43

3963.564r 2 1. 5 3969.407 10 35. 8 Fe II pfl. 67 \L 693

3 39DO.D91b

3963.806

3963.919

3964.030

56

3

1. 5

3. 5

SO. 4

2. 3

1. 0

2. 5

s

u

Lr I 2. 54 38

3969.507 3969.641m

3969.758

2

7. 5

14

8. 1

25. 2

SO. 7

u

s?

Fei

Cn

3. 25

2. 54

657

38

115
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

3969. 927

3970.076m

3970.166r 3970.272m

3970.399m

3

76

3. 5

18

29

11. 3

(776)

8. 8

32. 2

42. 9

w

u

u

Fei?

He

Fe I

l*e I

10. 20

3. 07

1

488

14

3974.398

3974.486

3974.634

3974.763

61

50

48

89

27. 3

25. 9

23. 6

33. 9

u

u

u

u

Fei

(CH)

CHNi I Fei

Co I

3. 24 Q 17 Q 17

3. 85

2. 22

0. 51

564

0,0

0,0

198

72

18

3

3

3970.495 10 19. 7 u

"NT" - JNi I 3. 65 151 3975.051 4. 5 2. 0 Fe II?— 5. 95 191 15

3970.569 3 6. 6 3975.210m 36 15. 6 u Fe I 2. 47 153

3970.660 6. 5 12. 4 w 3975.362 20 8. 6

3970.843 2 3. 3 — Fe I? 3975.519 2. 5 1. 0

3971.007 16 21. 6 u,N ie I— 4. 10 1074 3975. 691r 1. 5 0. 5 Ti I? 2. 10 186

3971. 126r 4. 5 7. 8 3975.845 43 17. 1 u Fe I 3. 88 977

3971.261 9 16. 7 Or I 2. 71 67 3975.960 2 0. 9 3971.332m 56 4-5. 0 u he I 2. 69 277 3976.089 44 17. 1 u

3971.468 6. 5 10. 4 3976. 185r 6. 5 2. 5

3971.720 5. 5 7. 8 u 3976. 276r 5. 5 2. 1 Sm II 0. 10 9

3971.826 15 16. 2 u bei 2. 76 281 3976.390 44 16. 7 u Fe I 3. 02 487

3971.994 17 16. 7 u,N Eu II 0. 21 5 3976.553 r 16. 3 s? Fei 3. 25 655

3972.173

3972.263

51

21

37. 0

15. 8

uw1

Nil

CH

0. 42 P 1229

0,0 3

3976.632

3976.694

> 162

J

< 23. 9

I 16. 7

Fei

Cri

3. 41

/2. 54

12. 54

729

38

38

3972.440 44 31. 2 u,N CH

(Co i) P 123. 51

0,0 1713,18

3976.868m 64 22. 6 u Fe I — /3. 02

13. 30

431 662

3972.575 27 19. 0 s Ca I 2. 71 41 3976.986 21 7. 8 u

3972.687 6 5. 0 Cr I 2. 71 67 3977.081 7. 5 2. 7 Mn I 4. 27

3972.916 17 12. 1 u Fe I 3. 57 803 3977.191 12 4. 3 u Co X 2. 33 113

3973.012r 0. 5 0. 4 3977.336r 1. 5 0. 5

3973.126

3973.168

19

9

14. 2

8. 3 Co I 1. 88 58

3977.45 a

3977.575r

4

8. 5

1. 5

3. 2

Fei?

Fei

3973.276

3973.418r 3973.564

.3973.657

3973.715

11

1. 5

74

1

101

8. 0

1. 3

43. 1

f 29. 2

1 29. 2

u

u

s

Nd II

Ni I Fei

V II Cai

0. 63

0. 42

3. 55

1. 43

1. 90

19

31

769

9

6

3977.747S

3977.895r

3978.014

3978.164

3978.346

104

7

1

19

32

33. 2

2. 6

0. 5

6. 4 IL 0

u

u

u

Fe I (Vii)

2. 20

1. 48

72

10

3973.871 17 10. 9 11. 3978.462m 50 16. 8 u Fe I 2. 83 361

3973.916 30 16. 2 u Fei 3978.572 8. 5 3. 2 Dy II

3974.023

3974.170

2. 5

28

1. 6

14. 0 w? Fe II 2. 70 29

3978.667m 68 22. 8 u |CoiCri

(Ceil)

0. 51

2. 71

0. 54

1767

175

:3974.274 2. 5 1. 4 3978. 775r 3. 5 1. 3

116
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

liMT

No.

or

Vib. Band

Notes

3978.855 10 3. 5 w Co I 3. 69 173 3983.540 35 10. 3 u Fei

3979.011r 1 0. 3 3983.666 10 3. 2 u Dy II 0. 54

3979.115r 4 1. 4 Fe I p 2. 99 426 3983.813 u,N Fe I p 3. 02 426

3979.196

3979.323

3979.522

3979.642

7

5. 5

67

42

2. 3

1. 8

23. 4

13. 6

u

u

Sm II Cr I? Cri?

Co I Fe I

0. 54

4. 45

4. 10

0. 10

3. 26

51 307

280

3

561

3983.921

3983.970

3984.150

3984.336

\ 155

J

70

54

24.0

[ 27. 0

19. 7

15. 7

] u

u

s

Cn

Fei

Nil

Cn

2. 54

2. 73

3. 68

(2. 54

12. 54

38

277

171

38

38

3979.791

3979.902r 3980 012

19

1. 5

21

6. 2

0. 5

6. 8

s

u

ICri

Fe I?

Fe I

2. 71

3. 02

67 3984.451

3984.564r

3984.665

9

3. 5

55

2. 6

1. 0

15. 7 u

Fei

Vi?

(Ce ii)

2. 59

1. 85

0. 96

219

89

252

3980.147r 3 1. 0 3984.839r 2. 5 0. 7 Ru I 1. 00 9

3980.292 4 1. 2 3984.941 37 10. 7 11 Fe I 3. 28 561

3980.522 3. 5 1. 1 Vi? 3985.070 5. 5 1. 7

3980.634 25 8. 2 11 Fe 1 2. 42 153 3985.16 a 4 1. 1

3980.821r 3. 5 1. 1 s Ti 1 2. 09 186 3985.242 35 11. 8 11 Mn I 3. 13 33

3980.883 6 1. 9 Ce 11 0. 71 194 3985.321 27 15. 8 11 Fe I p 2. 56 219

3980.982 23 7. 2 u 3985.392 99 27. 3 u Fe I 3. 30 661 3981.105m 32 10. 0 u Fei 2. 42 122 3985.600 11 3. 2 s Ti I 2. 09 188

3981.233 25 7. 5 u Cr I 2. 71 67 3985.628 5. 5 1. 8

3981.325r 1. 5 0. 5 3985.789 5. 5 1. 5 u Vii 3. 75 202 15

3981.448

3981.516

3

16

0. 9

5. 2

Ti 1 2. 12 188 3985.999 3986.180m

5

82

1. 5

23. 2 11 Fe I 3. 25 655

3981.616

3981.775m

21

101

6. 5

31. 0

u

s

Fe II p Fe i?p

Fe 1 Til

1. 72

2. 99

2. 73

0. 00

3 428

278

12

3986.295

3986.370r

3986.574r

25

9

4. 5

8. 2

3. 0

1. 5

u Fe I p

Ni I?

3. 24

3. 19

560

3981.997

3982.166

3982.332

3982.486

3982.598

71

12

4

60

62

20. 7

3. 6

1. 1

17. 3

18. 3

u

su

Ti II- Zni?

Mm?

Til

Mn I IIY II

0. 57

2. 49

4. 27

0. 00

3. 13

0. 13

11 142

11

33

g

3986.760

3986.837

3987 000

3987.096

3987 183

j 267

^

163

/

r 70.

I 15. 8

I 13.

34. 3

I 12. 3

u,N

u1 u,N

u,N

u,N

Mgi

Mn I CH — Mn I Nii-

|Co I

4. 34

3. 13 Q 18

3. 13

3. 66

0. 51

17

33

0,0

33

137

16

3

3982.757 3 0. 9 3987.374 20 5. 8 u

3982.911 12 3. 8 u Ce II- 0. 82 172 3987.473 12 3. 3 u Mm 3. 13 33

3983.004 52 15. 3 CH- P 13 0,0 3 3987.612m 52 14. 8 u -Ti up 0. 61 11

3983.198

3983.360

57

24

16. 5

7. 0

u

s

IICHCa I Fei

P 13

2. 93

3. 02

0,0

485

3 3987.80 a

3987.966

4

18

1. 0

5. 0 s Ybi 0. 00 2

117
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

115r 0. 5 0. 1 3988 332 7 2. 0 u

( 4 2

J

1 « 3QS8 51 fi > 44

1

< 6. 2 La II 0. 40 40 3Q88 562 I 2. 8 11 3QS8 66Sr 5. 5 1. 5 — Zr I 0. 62 46 3Q88 834 7. 5 2. 1 Vi 1. 86 89

3Q88 QQ2 69 18. 8 u — Fe I 3. 57

3989.084 56 19. 5 u

3989.251 13 3. 6 u Fe I p 3. 28 561

3989.452 5 1. 5 Ce II? 0. 90 240

3989.607 17 4. 8 s Fe I p

Ti I?

3. 27

1. 07 60581

3989.768 105 SO. 0 s Til 0. 02 12

3989.864 69 23. 8 u Fei 3. 55 768

3989.983 44 13. 1 u Cn

(Mn i)

3. 89

3. 13 26833

3990.104 27 7. 5 u Nd II 0. 47 19

3990. ISSr 5 1. 5 Til? 2. 08 188

3990 301 21 7. 0 11 Co I 1. 96 58

3QQ0 379m 74 20. 0 u Fe I 3. 05 527

3990.565 28 7. 8 s |Vi

Fe I p

fl 85 IL 85

3. 24

89

89 556

3990.760r 3. 5 0. 9

3990.949 4 1. 0

3991. 121S 74 20. 1 u |CriZr II

2. 54

0. 76

3830

3991.314r 9 2. 3

3991.434 40 11. 0 u

39Q1 "144 20 5. 6 u Co I 3. 63 173

39Q1 68^1

3991.745

1 72

1

f 14.

2

I 5.

8

SyTi

Co I Cri

Nd II Fe I

0. 58

2. 54

0. 00

1738

19

3991.834 8 2. 0 Co I? 2. 63 129

3991.898 6. 5 1. 9 u

3992.019r 3. 5 0. 9 Co I 0. 17 3

3992.115 8 2. 0 Ir I? Cri

1. 22

2. 54

538

3992.250 56 15. 0 u

3992.392 30 8. 0 u Fei 3. 30 604

W^avelength

(A)

Equivalent Width

AX

(ml)

Rerill OpH

Width

AX/X

(F)

Spot

Solar

Identi-

"fi Oft f.iriTi

Low

V.Hi PX or Rot. Line

RMT

I't (J. or

Vib. Band

3992.486 10 2. 8 u

3992.643 13 3. 6 u Fei 2. 59 219

3992.828 65 17. 2 s VillCr T

1. 86

9 71 89

67

3992. 975r 4. 5 1. 1 3993.101m 43 11. 5 Ff> T

3993 304 6. 5 1. 6 u,N ftrn TT n 04. U. U'x 4

3993.470r 2 0. 5

3993.612 19 5. 0 u -Fei

3993.733 16 4. 3 u

3993.827 11 2. 9 u Ce II 0. 91 12

3993.950 62 16. 5 If Nii1 Cri

3. 68

2. 71 170

67 3994 012 15 5. 8 ) Fp t r> o. 3994.119m 80 20. 8 u Fei 3. 05 526

3994.270r

3994.328r 1

4.

5

1

0. 6

1 0. 6

Fe I p 2. 87 320

3994.469

3994.512

i 72

1

r 2.

3

I 17. 6

s?u CH-

|Co I P 14 0,017 3994 684 62 16. 5 u Ti I Nd II CH

9 HQ

PX 1J. 4T:

188

0 0

3994.810 15 3. 9 Pr II 0. 05 11

3994. 950r 5 1. 3

3995 071r 2. 5 0. 6 399 208

3995 315

1

[ 146

J

f 11 7

I 28,

4

u

11

Fp t Co I

S 97

0. 92

604

31 3995 439r 12 3. 3 Fe I?

399^1 622r 3 0. 8 3995.751m 38 10. 0 u,N La II— 0. 17 27

3995.862r 3. 5 0. 9 Ni I p 4. 17 238

3995.990m 82 21. 4 s? Fe I 2. 73 279

3996.117 15 4. 0 u Fei?

3996.264 47 12. 4 u Fei /2. 99

1 ^ 9Q 427

13 4. 0 u Gd II

3996.546 10 2. 6 Fe I

3996.600 18 4. 6 s,N Sci 0.00 7

3996.697 7 1. 8 Dy II 0. 59

3996.788 32 8. 5 u Fei 4. 15 1074

Notes

15

118
The Solar Spectrum—Continued

vv d/Vt;-* length

(A)

EquiV ditrju u Width

AX (ml)

Re- Width

LiA\/\ A/ A

(F)

Spot

Solar

IdentiiiCdjUiOXX

Low

HiTT, J-P

or

XvO b. Line

RMT

XN O. or

V lu. Band

Notes

O 3996.971m 70 18. 2 u Fe I 3. 69 945

3997.112 50 12. 9 u Vii 1. 48 9

3997.215 9 2. 4 Mn I?

3997.401

I

r S^. 6 u Fei 2. 73 278

3997.482

170

I 18. 0 u Fe I p

/3. 24 556

ouo

"^QQ? fil Or Qo 9 1 ^QQ7 74Sr D. 0 1 ft

Oi7.7 1 .t/UO 114 J. Itc 9Q^i7. SO u Co T X. \JO ^9o^

oyyo.uooiii lit; OU. 0 11 PelT ^. oy 97fi

^QQS oy i7o.^97f1r / ur Q 9 9

^QQS 4.7 T OU 7 7 11 Fe I p O. OU DUO 3998.643m 110 SO. 6 s Ti I 0. 05 12 ^QQS oyyo.7/lRr / xor 1 4 4 VV TX

1X. S7O 1 oy

« 1. u Cr\JL T?X i OU t ^QQS oyyo.yiQ71i

oyyy.uoo

1

\ 62

J

f lift X X. u 4 8

uu

u. 1xoft

oyyy.io a

AO X. t> V TT V 11 ^ 7fi O. 4 O 909

^QQQ oyyy 94. .4(5^0 1 fi 4 1 TC. X XL rio v^e TT11 U. OU (^7

oyyy.ort^ 1 9 O. \J s TiXXIT 9^. inxu xoo

oy yy.ov/Ui o 1X. 9^ ^QQQ R7n 7 1 ft X. u ^QQQ oyyy.7Q7r i u t l

1 n 4

4nnn 09*? Qo 9 n XL 1; e 1 9 8*^ ^. oo ODU

4000. 150r 2. 5 0. 6

4000.257 66 16. 5 u Fe I 3. 26 556

4000.371 14 4. 2 u

4000.465 78 19. 5 u lire I Dy II

2. 99

U. lU 426

^UUU.Ooo QO

D

1 1 1. 1

4000.812 16 4. 0 u

^uuu.y / or 0. 0 11. A4t s

Pi- T? \JL I .' J."i. "±0 ^07

d.nni '±\J\J L .111 111 \ / fin D. U

4001.163

4001.241

• 127

27. 2

1. 0

u,N

Fe I 3. 64

40G1.343r , 1.0 4001.449m 68 17. 0 u Cr I 3. 89 268

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4001. 558r 3 0. 9 4001.670m

4001.753

\ 103

J

1 24. 2

[ 2. 2

11 Fe I 2. 18 72

4001.940 16 4. 0 Mn I? 15

4002.077 38 9. 5 u Fe II 2. 78 29

4002.162r 4 1. 0 Mm? 3. 77

4002.26 a 2 0. 5

4002.395 15 3. 7 Q

4002.503 34 8. 5 ITi I I J. 1 J. Nil2 12

4. 17 188

4002.665m 32 8. 0 s Fe /2. 88

13. 25 320

655

4002.803r 3. 5 0. 9

4002.929 61 15. 2 u Vii 1. 43 9

4003.085r 1. 5 0. 4

4003.17 a 2 0. 5

4003.275 10 2. 5 u Mm—

Fe I

4. 64

4003.512 7 1. 7

4003.620 6 1. 5 Co I — 2. 63 130

4003.769S 70 17. 5 u |Fe I Til

(Ce ii)

3. 41

2. 13

0. 93

728

188

188

4003.915 9. 5 2. 4 11 Cr I 3. 89 268 16

4004.016 9. 5 2. 4 XI Nd II 16

4004.164 9 2. 2 %t Fe II p 4. 48 127 16

4004 267r 2. 5 0. 6

4004.386 6. 5 1. 6 11 16

4004 601 14 3. 7 16

4004.710r 7. 5 2. 0 Cr I? 4. 20 295

4004.838 83 40. 2 u Fe I 3. 24 601

4004.915 72 24. 1 u

4004.983 82 36. 8 Fe I /3. 02

\3. 21 486

557

4005 072m 52 26. 5 zt 4005.254m 416 110 s? Fe I I. 56 43

4005.388m 42 21. 5 u Fe I p 2. 42 123

4005.482m 42 15. 2 u Fe I p Z. o9 LVd

4005.657r

4005.708 1 85

f 0. 9

1 23.

u Vii 1. 82 32

119
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4005.849r 2. 5 0. 6 4010.054r 3 0. 7

4005.965 18 4. 7 s Til 2. 10 187 4010.179 36 9. 0 u Fei 3. 64 915

4006.023r 2. 5 0. 6 4010.287r 5. 5 1. 4

4006.156

4006.317m

4006.473 4008.633m

4006.758

4006.825

4006.997

4007.039r

4007. 164r

4007.20 a 4007.279m

4007.443

4007.596

4007.72 a

4007.802r

4007.926

4008.060

54

89

13

93

1 102

1 65

3. 5

4

86

14

11

5

11

68

28

13. 5

22. 2

3. 2

23. 6

r 17.

0

1 10. 5

f 14. 5

1 3. 0

0. 9

1. 0

S3. 0

3. 5

2. 7

1. 2

2. 7

17. 0

7. 7

u

u

u

uu,N

u

su

u

u

u,N

s

Nil

Fe I p

Fe I

Fe I Fe I -CH

CH

Til

Fe I Nd II Fe I

Ti I

3. 26

3. 27

3. 11

2. 88 P 15 P 15

2. 09

2. 76

2. 12

564

603

488

320

0,0

0,0

187

277

187

3

3

4010.374

4010.492

4010.588

4010.650r 4010.780m

4010.933m

4011.080

4011.20 a

4011.3 04r 4011.414m

4011.546 4011.718m

4011.893

4012.016

4012.158

4012.253

4012.390

12

11

j 68

56

51

7. 5

3. 5

4. 5

55

16

50

10

10

33

39

93

3. 0

2. 7

r 16.

7

1 0. 6

14. 0

12. 2

1. 9

0. 9

1. 1

13. 7

4. 0

12. 5

2. 5

2. 5

8. 2

9. 7

23. 2

u

u

u

u

s

u

suu

uu

u

u

Fei?

-Fei

Fei

Fei

Co I

Vi?

Fei

Ti I Fei

Fe 1 p

Fei

Nd 11 Ce II lITi II

(2. 61

12. 86

0. 10

1. 22

2. 56

0. 00

2. 45

2. 95

3. 24

0. 63

0. 56

0. 57

219 320

2

218

10

153

424

601

10

206

11

4008.172

4008. 361r

4008.418

24

3. 5

5. 5

6. 0

0. 9

1. 4

u

1}"

V II

Sc II p

1. 79

0. 61

32

16

4012 478

4012.602

31

25

10. 5

6. 2

u

u

Cr I Cr II NiiFei3. 89

5. 66

4. 17

268

183

4008.602 14 3. 5 u So II p — 0. 60 16 4012 705 14 3. 5 u Nd 11

4008.736r 13 3. 2 u W I 0. 37 6 4012 796 5 1. 2 11 Ti 1 2. 12 186 4008 878

4008.930

1

\ 106

f 13. 2

I 17. 2

1}"f Fe I

1 Til 0. 02 12

4012 959r

4013.075

1

3. 5

0. 2

0. 9 u,N

4009 055r 7 1. 7 4013 232 7 1. 7 Ti I p 2. 10 186

4009.146 53 13. 2 u 4013.466r 2 0. 5

4009. 255r

4009.420r

4. 5

3. 5

1. 1

0. 9

Fe 1 Fei

4013.582 4013.639m 1

83

r 4.

2

1 18. 2 I Fei

2. 13

3. 21

187

557

4009.547

4009.660r

4009.714

4009.9 lOr

43

]

} 122

9. 5

10. 7

f 11. 0

1 24.

4

2. 4

u Fe I p

j Til

1 Fei

Ru 11 Ci?

3. 21

0. 02

2. 22

3. 75

7. 68

556

11

72

4013.816m

4013.960

4014.126r

4014.272m

102

34

3

50

25. 4

a. 5

0. 7

12. 0

u

u,N

s

Fe I Fei

Co 1

Fei

3. 02

3. 02

2. 01

/3. 02

13. 02

485

486

58

426

427

4009.984 18 4. 5 u Nil 3. 63 150

120
The Solar Spectrum—Continued

Equivalent Width

AX

(mA)

4. 5

117

18

7

34

14

3

23

20

88

14

4. 5

8. 5

5

13

68

12

12

30

24

149

24

86

74

34

2

139

92

16

7

1. 5

1

9

7

49

Re- duced

Width

AX/X

(F)

1. 1

29. 1

4. 5

1. 7

8. 5

3. 5

0. 7

5. 7

5. 2

21. 9

3. 5

1. 1

2. 1

1. 2

3. 2

16. 9

3. 0

3. 0

7. 5

6. 0

19. 7

23. 9

6. 2

21. 4

18. 4

8. 5

0. 5

34. 6

22. 9

4. 2,

1. 7

0. 4

0. 2

2. 2

1. 7

12. 2

Spot

w,iV

sw

u

u,N

su

u

Solar

Identification

8U

s?

So IX- IIFei Cri

Ce IITii

Ni II

Cai

Til

Fei

Fei

Cn

Vii

Til

Fei

Fei

Vii

Nil

Til

Cr u?

Mn I Fei

Zr II Fe II p

Nd n

Nil

Fei

Low

E P

or Rot. Line

0. 31

3. 57

3. 89

0. 53

2. 08

4. 03

2. 93

2. 13

3. 28

2. 73

3. 43

3. 76

2. 16

2. 76

3. 05

3. 79

3. 70

2. 09

5. 33

2. 11

3. 26

0. 96

2. 28

0. 06

1. 93

2. 61

RMT

No.

or

Vib. Band

802

268

157

185

12

186

560

277

202

208

279

527

216

171

185

166

5

560

54

13

19

72

219

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RM"]

No.

or

Vib. Ban(

4019.136 8. 5 2. 1 Th 11 0. 00 3

4019.297 18 4- 4 s Co I 0. 58 16

4019.431r 1 0. 2

4019.598 2 0. 5

4019. 838r 4. 5 1. 1

4019.885r 2 0. 5 Fei

4020.029

4020.074

1

1 93

f 8. 5

1 17. 4

ulu -CH

Fe I p

P 16

3. 26

0,0

5.56

4020.193

4020.272

1 1071 10. 7

I 18. 2

uu,N-CH P 16 0,0

4020.397 56 13. 9 s Sc I 0. 00 7

4020.488 44 10. 9 u Fei 3. 64 913

4020.650r 3 0. 7

4020.778r 5. 5 1. 4 4020.905m 80 19. 9 s Co I 0. 43 16

4021. 089r 3 0. 7

4021. 197r 5. 5 1. 4 u

4021.338 16 4. 0 u Ndii 0. 32 36

4021.496r 2. 5 0. 6

4021. D2om c o DO Id. y u Fe I /2. 42

\3. 24

120 557

4021.740 10 3. 0 11 4021.870m 121 SO. 1 u Fe I (Til)

2. 76

2. 10 278185

4022.049 23 5. 7 u Nil /4. 09

14. 10 241 238

4022.226

4022. 252r

]

[ 55

f 10. 4

1 5. 5

1 Fei

1 Cn

2. 83

3. 89

360

268

4022.446 25 6. 2 u Fe I 2. 40 173

4022.536r 4. 5 1. 1 Fei?

4022.625 10 2. 5 u Cu I 3. 78

4022.745m 52 12. 9 u Fei /3. 25

13. 28

654

556

4022.86 a 5 1. 2 C I? 7. 48

4023.011 18 4. 6 u Nd II

4023.14 a 5. 5 1. 4 Vi? /I. 89

1 9

4023.230r 3 0. 7 s Sm 11 0. 04 4

4023.384 67 16. 6 u Vii

(Co I)

1. 80

1. 96 32

59

121
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

(F)

Spot

ooiar

Identification

Low

TP P

or

jnot. Line

RMT

iN 0. or

V ID. Band

Notes

^^Vave- length

(A)

Equivalent Width

^A (mA)

ReducGci Width

ilA/ A

(F)

Spot

ooiar

Identification

Low

TP P

or

Line

RMT

iM 0. or

V ID. Band

Notes

4023.556r 1 0. 2 4028.346m 90 22. 3 u Ti II 1. 89 87

4023.687 57 14. 2 s Sci 0. 02 7 4028.492 9. 5 2. 4

4023.831 3. 5 0. 9 Fei 4028.605 6. 5 1. 6

4024.003

4024.100

4024.224r

4024.330r

4024.441

33

66

3

3

18

9. 2

16. 4

0. 7

0. 7

4. 7

u

u

u

II Nil

Zri

Fe I Fe II

Zr II

3. 70

0. 69

2. 76

1. 00

170

46

277

54

4028.763

4028.93 a

4029.09 a

4:U^y .*±rtO

43

0. 5

2. 5

0. 0

lU

10. 7

0. 1

0. 6 n Q u. y

u

s

u

Fei

Zri

Ni I p

0. 52

Q 7n 0. < U p 1

i /U

1 1 1,1 0

4024.576 80 19. 9 s Til

(Si e II;

0. 05

A /I Q 12 4029.642S 108 26. 8 u IIFei Ar II

J 0. \3. 26

U. / 1

000

563

A 1

4024.732m 104 25. 8 u Fe I 3. 24 560 4029.869 12 2. 7 s

4024.894r 8. 5 2. 1 s Zri 0. 65 46 4030.049r 3 0. 7 s Zr I- 0. 60 46

4025.009 29 7. 0 u Cri 2. 54 37 4030.190S 64 16. 1 u |Fei 2. 20 72

4025.134m 84

14

20. 9

0. 5

u ITi II

AT,* T JNl I

\jS±

0. 61

A f\(\

"D A

11

O.I n ^4U

i>i 0

4030.348

4030.497

36

92

9. 7

27. 3

u

u- |Fei

T'l' T 3. 21

0 1 Qlo 5601lot)

/I AOr /I OA 40^5. 429 48 11. y u I Cri

0. /U

/2. 54

yz. 54

I 1 ^7 II / 37

6i

4U0U.D40

4UoU. i DO

\ 326

J

17.1

[ /o. / Mn I n on U. UU <

4025. 584r 7

11. 7 4UoU.oyi4 4s 17 ft 1 / . D u r e I p — 0. oy y4o

4025.823 64 15. 2 Zl 4031.116 15 4. 2 u Cr I 3. 89 268

4025.930r 6 1. 5 4031.245 42 10. 9 u Fei 3. 02 486

4026.071r 8. 5 2. 2 4031.340 12 3. 0 u Ce II 0. 32 108

4026.168 43 10. 7 s,d Cri /2. 54

l,A 54

37

0/ 4031.447r 5 1. 2 Fe II 4. 73 151

Af\^R Old 40/0. oil)

40z6.4dD

4026.542

7. 5

00

42

1. y 10 0 lo. ^

10. 4

u

s

OM

Mn 1 Til

0 1 0

6. lo

2. 12

1,1

185

3 4031.563r

4031.716r

4031.793r

1. 5

I C\A

f y4

0. 4

f 12. 6

1 12. 6

M?

M?

Fe I p

^ija 11 ) Mn I (Nd 11)

3. 02

U. OiS

3. 13

427"] 4U > 7

y

0 A Z. 4 s 4Uoi.yDym by 17 1 1 / . 1 u r e I Q 07 DOO

4026.918r 4 1. 0 4032. 116r 3. 5 0. 9

4027.043

4027.104 1 67

f 11. 7

1 6. 0

s

s?

Co I Cri0. 17

2. 54

3

37

4032.268 4032.463m

7

75

1. 7

18. 6 u Fe I 2. 88 320

4027.251

Af\c\>j ATA 4Ui47.474

9. 5

25

2. 4

0. i

d. 0

s

u

s

Zri-

/ ' 1

J

CM

0. 62

it 2 46

1.1 3 4032.641m

4032.837r

4032.964r

106

12

• 229

26. 3

3. 1

1 1.9

u Fe I

Fe IIO^a I

1. 48

4. 49

0 no

44

126

11

4027.672 49 12. 2 u Ni I 3. 90 4033.072 i 54. 8 S Mn I 0. 00 2

4027.790r 2 0. 5 4033.186 60 28. 5 Fei 2. 56 218

4027.943 28 7. 0 u CH R 6 1,1 3 4033.277r 21 6. 2 Cri 2. 54 36

4028.123r 3 0. 7 Cri? 4. 20 4033.430r 8 2,0

122
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4033.588 46 11. 4 u

4033.660 24 7. 7 u Fe I

4033.790 9. 5 2. 4 u CH Q 1 1,1 3

4033.904 14 3. 5 s Til 2. 16 208

4033.972r 4. 5 1. 1 Cri

Cri

2. 54

2. 54

36

36

4034.091 16 4. 0 u Zr 11 0. 80 42 4034.232 50 12. 9 u -CH P 17 0,0 3 4034.386 4034.492m

]

[ 213

f 9. 9

1 46. 1 s

CH

Mn I

P 17

0. 00

0,0

2

3

4034.733 16 4. 2 u

4034.870 28 6. 9 s Ti I 2. 15 208

4035.118 24 5. 9 u Sm II 0. 33 33

4035.250 23 5. 7 u Fe I p 3. 60 831

4035.427r 9 2. 2

4035.547r 5. 7 Co I 3. 58 173 4035.606

4035.732

• 216

18. 8

31. 2

u,N

s

Vii

Mn 1

1. 79

2. 14

32

5 4035.833 / . 2.0 Til 2. 17 208

4035.984 16 4. 0 u Fe I p

Ni I p

3. 02

3. 65 426

150

4036.12 a 4. 5 1. 1 4036.244a 6. 5 1. 6 u

4036.377 24 5. 9 u Fe I 2. 76 279

4036.567 8. 5 2. 1 u Fp t 4036.670 6 1. 5 CH 0 1 1 1 3 4036.773 31 7. 7 u V'li 1. 48 9 4036.929r

4037.121S 44 10. 9 u Fe I 4037.301 18 4. 5 s Cn

(Gd II)

/2. 54

0. 66

36

36

49

4037.438r 5 1. 2 CH P 1 1,1 3 4037.548

ml

4. 5 1. 0 4037.688 22 5. 1 u Fe I 2. 28 118 4037.913a 4. 5 1. 1 Gd n 0. 56 49 4Uo / .y /D 4. 5 1. 1 4038.124 13 3. 2 s 4038.276 3 0. 7 u,N Nil 3. 65 150

4038.479r 3. 5 0. 9

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

4038.627 26 6. 4 u Fe I /3. 30

13. 41 600

728

4038.795 64 15. 8 u Fei

4038.946r 2. 5 0. 6

4039.096 42 10. 4 s Cn 3. 85 251

4039.296 7 1. 7 u Cn- 3. 85 251

4039.432r 0. 5 0. 1

4039.574 9 2. 2 u Vii 1. 82 32

4039.743 8 2. 0

4039.864

4039.946 1 44

1

2. 2

[ 8. 9

suYi

Fe I

0. 00

2. 73

5

276

4040.097m 61 15. 1 u Fei

4040.270

4040.310 J

1

4. 0

[ 4. 0 s

Zr II- Tii

CH

0. 93

2. 12 P 1

54

185

1,1 3

4040.514 27 6. 9 u -CH Q3 1,1 3

4040.647m 78 19. 9 u Fei 3. 30 655

4040.790 39 9. 6 s Ce II— Nd n

0. 45

0. 18 138

30

4040.951 r 4 1. 0

4041.066 8 2. 0 u

4041.283r

4041.374

1 168

f 16. 3

I 28. 4

w?

s

Fei

Mn I

/3. 30

to. ou

2. 11

603

5

4041.656m 58 14. 3 u Fei

4041. 809r 3 0. 7 u? Cn 2. 54 36

4041.914 13 3. 2 u Fei 3. 30 602

4042.05 a 3. 5 0. 9

4042.149r 3. 5 0. 9

4042.245 10 2. 5 s Cn 2. 54 36

4042.363 6 1. 5 u?

4042.443r 3. 5 0. 9

4042.592 13 3. 2 u Ce II 0. 50 140

4042.758 10 2. 5 u Feip 3. 28 556

4042.907 18 4. 4 u Sm II La II

0. 10

0. 93

966

4042.997r 1. 5 0. 4

4043.346 24 5. 9 u,N CH Q4 1,1 3

4043.47 a 2. 5 0. 6

4043.608 6. 5 1. 6 s Zn 0. 52 32

123
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4043.695

4043.768

4043.906

4043.988

4044.145

4044.274r

4044.380

4044.497

17

27

146

16

0. 5

6. 5

40

4. 7

7. 4

[ 22. 0

[ 14. 1

4. 2

0. 1

1. 7

14. 3

u

u

u

u

s

u

Cri

Fe I p

-Til

Fei

Fe I p Ki

CH

Fe I p

4. 45

2. 48

2. 16

/2. 73

13. 24

3. 24

0. 00

P 2

4. 10

306

122

208

276

557

559

3

1,1

1073

3

4048.400r

4048.555r

4048.671

4048.753

4048.996

4049.152 4049.336m

4049.438

7

4

1 138

29

23

62

9

1. 7

1. 0

[ 8. 6

'. 28. 2

7. 2

5. 7

15. 3

2. 5

M?

s

u

u

u

Fei

Zr II ||Mni

Cr I Mm

Cr II? Fei

Gd K

Til?

0. 80

2. 16

3. 85

4. 34

6. 48

2. 59

0. 66

2. 13

43

5 251

48

193

218

50

185

4044.615 105 28. 0 u Fe I 2. 83 359 4049.565 41 10. 1 u CH P 18 0,0 3

4044.843r

4044.959r

4045.115

4045.217

4045.390

4045.508

4045.600

2. 5

1

50

19

48

9

29

0. 7

0. 4

17. 3

17. 4

25. 0

8. 2

26. 4

u

u,m

u

u

llFei Mn I Mn I Co I

Fe I p —

IZr II

3. 02

4. 33

4. 23

1. 05

3. 21

0. 71

425

48

31

559

30

4049.731

4049.862

4050.029

4050.104r

4050.329

4050.492

4050.566r

47

11

4

1

20

13

3. 5

11. 6

2. 7

1. 0

0. 2

4. 9

3. 2

0. 9

u

s

u

s

CH

(Cr I) Gd 11 |Fei

Cri

La II

Zr II

Dy II

P 18

3. 85

2. 54

1. 96

0. 71

0. 59

0,0 251

36

85

43

3, 18

4045.715r 7. 5 13. 3 4050.580m 57 14. 1 u Fei

4045.825m 1174 316 s Fe I 1. 48 43 4050.813r 3 0. 7

4045.968 14 23. 0 4050.948 6 1. 5 s Vi 2. 13 121

4046.074 44 36. 1 u Fe I p — 3. 26 557 4051.052 10 2. 5 0? Vii 1. 80 32

4046.341

4046.459

9

19

4. 4

7. 1 u

Ce II Vii

Fe I p

0. 55

3. 12

4. 15

81 177

1075

4051.187

4051.337

21

33

5. 0

8. 1

u

s

Ni I |Vi

Vii

4. 10

2. 14

3. 80

239

121 215

4046.615r 1 0. 4 Fe I 3. 07 487 4051.49 a 1. 5 0. 4 Rui 1. 09

4046.760

4047.016

7. 5

10

2. 3

2. 7

u

u

ICri

Nil

2. 54

4. 09

36 4051.734

4051.918

12

79

3. 0

19. 5

uu

Mn I Fei

|Cr 11

3. 40

3. 10 70019

4047.189r 5 1. 4 4052.020 16 4. 7 u

4047.23 a 5 1. 4 s Ki 0. 00 3 4052.166r 4. 5 1. 1

4047.310 41 10. 9 u Fez /2. 28

13. 63 117

853 4052.303m 60 14. 8 u Fei f3. 37

13. 63 700 852

4047.407r

4047.673

4047.802

4047.91 a

4048.072

4048.235r

3. 5

21

-[ I

2

24

1

1. 0

5. 4

2. 7

0. 5

5. £

0. 2

s

s

u

YiCH

OC 1

-CH

0. 00 Q5

Q 5

6

1,1

7

1,1

3

3

4052.456

4052.499

4052.660

4052.720

4052.842r

4052.940

1 96

1 88

1

32

f 11. 6

1 15. 5

[ 12. 1

1 12. 1

0. 2

7. 9

ut

w?

su

u

Fei

Mn I Fe I Fei

TiiCH

3. 28

4. 35

3. 05

3. 24

2. 17 Q 6

563

48

524

557

208

1,1 3

124
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4053.113r 0. 5 0. 1 4057.733r 11 3. 2 CH P4 1,1 3 4053.271m

4053.430

4053.491

4053.59 a

4053.824S

61

22

7

2

65

15. 0

5. 4

1. 9

0. 5

16. 0

uw,N

u?

u

Fei

Ce 11 Vii

Ti n

Fe I

0. 00

3. 80

1. 89

3. 07

36

215

87 485

4057.813r

4057.893r

4057.957

4058.221

16

1 72

101

4 7

f 9. 4

J

I 9. 4

24. 9

|s,iV

u,N

s

Mn I Co I IIFei (Til)

1. 32

3. 85

3. 07

0. 51

3. 21

2. 32

1 251

29

16 558

254

15

4053.936r 5. 5 1. 4 4058.391r 4 1. 0

4054.077 28 6. 9 w,N Cr II 3. 10 19 4058.467r 15 3. 7 Fe I p 3. 64 914

4054.185 50 12. 3 s Fe I 3. 26 557 4058.598 29 7. 1 u Co I 2. 01 58

4054.308r

4054.442

4054.560

4054.711

4054.815

4054.873

4055.039

0. 5

28

14

22

135

J

80

0. 1

6. 9

3. 4

6. 4

[ 24. 7

[ 18. 5

19. 7

u

s

u

uu

u

Fe I

Sci

Mgi

Fei

Fe I Tii-

|Fei

/O. 00

10. 00

4. 34

3. 40

3. 42

1. 05

2. 56

6

6

698

698

80 218

4058.765

4058.931

4059.091r

4059.222

4059.386

4059.502 4059.722m

74

89

6

23

58

20

70

18. 2

21. 9

1. 5

5. 7

14. 3

5. 7

17. 2

u

s

uu,N

uu

Fe 1 Cr I Mn I (Nbi)

CH

Mn I CH

Fe I

2. 42

3. 85

2. 18

0. 13

Q7

3. 07 Q7

3. 55

120

251

5

1

1,1

29

1,1

767

3

3

4055.215 22 5. 4 u Mn I 4. 36 48 4059.966 6 1. 5 u Nd II 0. 20 63

4055.384r 9 2. 2 4060.094 4 1. 0 s Tiip 2. 30 254

4055.551m 114 28. 1 u Mn I 2. 14 5 4060.269m 34 8. 4 R Til 1. 05 80

4055.706r 8. 5 2. 1 u 4060.491 17 4. 2 u

4055.858r 2. 5 0. 6 4060.634 6 1. 5 Cn 4 45

4055.990 20 4. 4 u Fe I 3. 64 914 4060.768 25 6. 2 u Fe I

4056.070 18 4. 4 u Cn 4. 45 4060.936 1 0. 2

4056.195

4056.347

4056.452

4056.559r

4056.65 a

4056.806r

4056.907r

4057.075

4057.218

30

38

29

7

2

6. 5

12

13

57

7. 4

9. 4

7. 1

1. 7

0. 5

1. 6

3. 0

3. 2

14. 3

u

u

u

s

s

s

Ti II Fez

Fe I

Cn

Vi

ICoiNi I?

0. 61

2. 86

4. 45

2. 12

0. 22

3. 31

11

320

306

121

3

4061.097

4061.443

4061.733

4061.956

4062.045

•

4062.232

4062.321

4062.447S

4062.642

57

19

64

54

14

6

2

98

22

14. 0

4 7

15. 8

13. 3

3. 4

1. 5

0. 5

25. 2

5. 9

u

u,N

u,N

u

uw?

Nd IIFe I

Mn I Fe I

Ce II

Fe I Cui

0. 47

3. 07

1. 37

2. 84

3. 82

10

29

34

359

15

^fcuo i .oooni 11 r e I 9 7fi Z. / 0 977 12 3. 4 u

4057.515 197 48. 5 u Mgi 4. 34 16 4062.952 4 1. 4

4057.670 38 13. 0 s,N Fe I |Ti I

3. 41

2. 30 729

254

4063.288m

4063.424r

68

12

32. 2

8. 9

u Fe I Gd II

3. 37 698

125
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4063.605m

4063.789r

4063.926r

4064.050

4064.214

4064.371

787

19

5. 5

28

28

15

219

18. 7

3. 4

11. 6

8. 6

5. 2

S

w?

su

Fei

(Mn I)

Vi

Fe I p Til

Ti II-

|Ni I

1. 56

2. 16

2. 11

2. 95

1. 05

2. 60

3. 84

43

5

121

423

80

106

179

4068.404r

4068.544

4068.650r

4068.843

4068.90 a

4068.968

4069.070

0. 5 27

5

3. 5

1

5

48

0. 1

6. 8

1. 2

0. 9

0. 2

1. 2

11. 8

su

su

su

Cr I? Co I Til

Ce 11 Fe I Til

Fei

1. 96

2. 29

0. 70

2. 74

3. 28

58

254

82

299

557

4064.456 64 17. 2 s Fei L 56 44 4069.155 5 1. 2

4064.577

4064.70 a

4064.761

4065.087

9. 5

2. 6

2

52

2. 5

0. 6

0. 5

12. 5 s

Sm II

Fe n p ViiIITii

rO. 25

10. 33

2. 85

3. 79 L 05

24

33

39

215

80

4069.272

4069. 437r

4069.610

4069.84 m

4070.036

8.5

1. 5 34

11

2. 1

0. 4

8. 4

2. 7

s,d?

u

s

u

Nd 11

Fe I

Fe I

0. 06

2. 87

20

320

13

4065.236 4065.388m

4065.587

5. 5

64

15

1. 4

15. 7

3. 7

Vu

Ci?

Fe I Til

CH

7. 49

3. 43

2. 15 P 5

698

207

1,1 3

4070.281

4070.443

4070.626r 4070.777m

66

5

3

94

16. 0

1. 2

0. 7

23. 6

uu

u

Mn I Fe I

Fe I

2. 19

3. 05

3. 24

5

525

558

4065.708 14 3. 4 u Cn 4. 10 279 4070.985 3 0. 9 Cri 4. 45 306

4065.810r 0. 5 0. 1 4071.093 17 5. 2 u Zr II- 1. 00 54

4066.004

4066.120

4066.220

12

48

25

3. 0

10. 8

6. 8

u

u

u

Fe I p —

CH

— CH

3. 33 P 5

P 19

695

1,1

0,0

3

3

4071.21 a

4071.350r 4071.536m

2. 5

8. 5

50

0. 9

3. 2

22. 9

s

u

Tii

lIFeiVi

2. 30

2. 59

1. 93

254

218

96

4066.373 76 18. 7 s Co I 0. 92 30 4071.638r 7. 5 12. 3 4066.590m 80 19. 7 u Fei 2. 99 424 4071.749m 723 191 s Fei 1. 61 43

4066.721 20 4. 9 u Sm 11 0. 28 28 4071.901 19 17. 9 u,N

4066.820 30 7. 6 u CH Q8 1,1 3 4071.970r 3 2. 5 4066.984m

4067.280m

4067.407r

4067.492

4067.600

4067.766

4067.856 4067.988m

4068.117r

4068.20 a

4068.337r

130

96

5. 5

18

23

21

27

133

10

5

4. 5

32. 0

23. 6

1. 5

4. 4

5. 6

5. 6

7. 9

32. 7

2. 7

1. 2

1. 1

s

u

u

u

u

u

u

s

Fei

(Cr I) Fe I La II Fe I p

Fe I p

Fe I p Fe I Til

Sm II?

2. 83

2. 71

2. 56

0. 17

2. 95

3. 30

4. 18

3. 21

2. 15

0. 43

358

66

217

26

422

655

1103

559

207

42

4072. 144r

4072.351 4072.512m

4072.696

4072.888

4073.125

4073.342r

4073.486

4073.629r

4073.767S

4073.95 a

8

12

63

7

6

5

0. 5

18

4. 6

90

4

2. 9

3. 7

17. 4

2. 0

1. 5

1. 2

0. 1

4. 4

1. 1

22. 1

1. 0

u

u

su

u

u

su

Fe I Fe I Zri

Nil

Dy II

Ce 11

Fei

3. 43

0. 69

3. 85

0. 54

0. 48

3. 26

698

46

197

4

558

15

126
The Solar Spectrum—Continued

V V d V C" length

(A)

EquiWidth

A\

(ml)

Re- Width

AX/X

(F)

Spot

Solar

IdentiiiofA f.in'n

Low

E P

or Rot. Line

RjMT

or Vib. BandNotes

4074.04S 12 2. 9

4074.17 a 6 1. 5

4074.332 18 4 4 Til

W I

2. 32

0. 37 254

fi\j 4074 "i^Or \

4074.684 42 14. 0 u Fe I p 3. 64 912

4074.794 110 27. 0 u Fe I 3. 05 524

4074 QOO 30 8. 1 Ni I 0. 42 28

62 15. 2 (Nd II) 0. 20 62

4075.316 31 7. 6 u,N Nd II?- 0. 06 19

X) 1 Qo

4075.510r 0. 5 0. 1

4075.65 a 2. 5 0. 6 Cr II? p 3. 10 19

4075.706 12 2. 9 u Ce II 0. 70 57

4075.851 14 3. 9 u Sm II —

Cf TT

0. 54

n fii 51

407'i Q4Q 83 20 4 Fp t

16 4- 4- 4T:. 1XVJ0 27Q

4076 1 32 1

rin T 0 =i8 1xuR

4076 226 14 9 u Pa t 3. 07 4076 364 8 1=; o. o 9 1 s J. I 1 0 09 Q

4076.495 62 16. 2 u Fe I 2. 61 218

4076.637m 127 31. 4 u Fe I 3. 21 558

4076 80S 94 9'^ S 3 26 oo i 4076 877 19 7 V Pr TT Fe I

o. 1xun

3. 26

1xy0 559

4077.072 20 5. 2 u Zr II-

!Cri

0. 96

2. 71 54

66

4077.16 m s Til 2. 16 207 13 4077 1Q8 7 9 1

4077.347 41 111 i. Ro s II |Yi

n 9'^

0. 00

41t:X7

4077.486 11 4. 4 Ce II- Pr TT

0. 30

o.^ inxu 60

1 Q

4077 ^iSOr /" 9 Q

4077 724Tn \ 1 no o Sror TTix fi fin 1

4077.834r J \ 2. 9

4077.969 26 8. 8 w Dy II 0. 10

4078.164 3. 5 1. 0

4078.365 1 124 31.9 w Fei 2. 61 217

length

(A)

Equi-

"uft V dit/l-l 1 r^n t\j Width

AX

(ml)

RedllCGcl Width

AX/X

(F)

Spot Identifi f'ii f 1 An

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

t:VJ I O.^ 4 O OVJ 21. 6 Ti I 1X. 07W 1 80

4-07 R fi'^Or 2. 5 0. 6

4078.823 19 4. 6 w Fe I 3. 64

1xo

4079.012 8 2. 0 w

407Q 184 4070 9^7

1[ 144

J

1 18. 1

94 0

1 f FpX e T1 Dp

1 1 1 IVTn T

L 1 ivx u X

3 42

9 14

700

4079.357r

4079.416 1 104

[ 25. 0 s Mn I 2. 19 5

4079.556r 4. 5 1. 1

4079.711 12 2. 9 s Ti I CNh t") V

i"» u X ;

2. 16

0 OQ 207

407Q 84^S Q4 23. 0 Fe I 9ilf. 8fi ou 359

8 ^ 9 1X Fe I p 3 fiO 944

4080 21

6

rt.\JO\J . X\J 21. 8 zc Fe I 3. 28 558 4080 36 f) 2 0

1. 2 Hf II? 0. 61 40R0 fiOOr 1 9 Ru I 0V. 81O X 9

X. o 0u. 4r±

4080.770r 1 0. 2

4080.880 61 14. 9 u Fe I 3. 29 557

4081.039r 6. 5 1. 6

4081.234r

1

> 63

r 6.

\

f Ceil

J IZri l^jx X

0. 48

0. 73

446

4nS1 9fi9 J i 12. 2 r Fp t

4081 49Qr o 1. 2 s 1xofi

4081 "iRfir 0 0. 1

4081 7^fir K). o 1. 6 It Pr T 9 71 fifi

4081.909r 7. 5 1. 8 Cr I? 4089 ^uo^.xxoixi 1 1 'im 7fi 1X 8 fi o. u u RpX" C TX 49 fiQ8

4089 978 QO 2 0 Pr\yl TT? Xi i "^9 1X fi'i \JO 4089 4*^0 89 20. 1 s !Fp t 1 X C 1 SciITi T [ X i X

% fi*? 0. 02

1X. 07U i

QOfi6so 4089 tiQfi 1

Xrr 3 4 s Po T 0 fi'^ u. uo 1xufi

4082.778r 0. 5

4082.943S 94 23. 0 s Mn I 2. 18 5

4083.093r 3 0. 7 CN? R67 1,2 11

4083.226 26 6. 4 u Ce n 0. 70 60

127
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

Irmt

No.

or Vib. Band

Notes

4083.365r 3. 5 0. 9 4088.564m 56 13. 7 u Fei 3. 64 906

4083.565

4083.630

1 181

J

J 17. 9

I 32. 4 }'

J

J Fe I

1, Mn I

2. 28

2. 16

117

5

4088.727r

4088.850r

13

8

3. 2

2. 0

Fe II p

Cr II?

2. 84

3. 10

39

19 4083.763m 71 21. 1 u Fe I 3. 42 697 4089. 049r 16 3. 9 u,N

4083.999 20 4. 9 u CH? P 7 1,1 3 4089.224m 62 15. 2 u Fei 2. 95 422

4084. 150r 5. 5 1. 3 Fe I p 3. 21 557 4089. 418r 4 1. 0

4084.327 23 6. 4 u CH P 7 1,1 3 4089. 598r 3 0. 7 Cr I 3. 85 260

4084.501m 156 38. 2 u Fe 1 3. 33 698 4089.785r 6 1. 5

4084.611r 2 0. 7 Fe II p 4. 74 151 4089.961 21 5. 4 u Mn I 4. 27

4084.71 a 4. 5 1. 2 4090.081 70 17. 1 u Fe I 3. 40 700

4084.794r 12 2. 9 4090. 188r 1. 5 0. 4 4085.013m

4085. 153r

4085.258

107

5. 5

152

26. 2

1. 4

f 10. 5

u

]

\ u,d

Fe I

f Ceil

1 Feip

2. 84

0. 67

2. 76

358

172 276

4090.324

4090.521

4090.573

24

56

J

5. 9

\

[ 9. 8 J

Cn

Fei

[ Vi

2. 71 L 61

0. 76

1. 08

6644

29

41

4085.309 I 31. 3 J [ Fei 3. 24 559 4090.772 10 2. 4 u Fe I p 3. 69 943

4085.445r 7 1. 8 CN? R 66 1,2 11 4090.959 57 13. 9 u Fe I 3. 37 695

4085.574 10 2. 4 Gd n 0. 73 50 4091. 085r 4 1. 0

4085.731r 7 1. 7 Zr II 0. 93 54 4091.22 a 3. 5 0. 9

4085.858r 7. 5 1. 8 4091.438r 1 0. 2

4085.984 55 13. 5 u Fe I 4. 15 1073 4091. 557S 60 15. 0 u Fe I 2. 83 357

4086.134 32 7. 8 u Cr II 3. 71 26 4091.678r 2. 5 0. 6

4086.316 104 25. 4 u,d? Co I 1. 88 58 4091.85 a 1. 5 0. 4 4086.713m 42 10. 3 u La II 0. 00 10 4091.999r 8. 5 2. 1 s,N Ca I 2. 93

4086. 838r 5 1. 2 4092.098r 9 2. 2 ul

4086.965r 6 1. 5 s Cri? 3. 85 4092.281 57 16. 9 u Fei 3. 63 4087.101m

4087.277

4087.37 a

4087.49 Ir

81

15

3. 5

2

19. 8

3. 7

0. 9

0. 5

u

u

Fei

Fe II p

3. 33

2. 58

694

28

4092.396

4092.516m

4092.669

108

36

115

26. 9

9. 3

28. 6

s

u

Co I (V I) Fe I CaiVi0. 92

1. 19

0. 91

2. 52

0. 29

29

52

18

25

27

4087.601 8 2. 0 u,N Cr II 3. 10 19 4092.825r 12 3. 2 u Co I 2. 01 59

4087.705r 6. 5 1. 6 CN? R 65 1,2 11 4092.892 6. 5 1. 7

4087.798 19 4. 6 u,N Fe I p —

CN?

3. 65 R 65 832

1,2 11 4093.034 12 2. 9 u Ni ICr I

4. 23

3. 85 260

4087.94 a 6. 5 1. 6 4093.15 a 4 1. 0 Hf II 0. 45 6

4088.050r 5. 5 1. 3 4093. 284r 6 1. 5 u

4088.183r 5 1. 2 4093.48 a 4 1. 3 S Vi L 18 52

4088.298r 3. 5 0. 9 s,N Co I 0. 10 2 4093.650r 2 0. 5 Nil 0. 17 1

4088.446r 0. 5 0. 1 4093.990r 3 0. 7

128
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4094.069r 3 0. 7 4098.795r 3. 5 1. 1

4094.20 a 3. 5 0. 9 Tm I? 0. 00 4098.901r 4. 5 1. 3 Gd II? 0. 60 49

4094.304r

4094.422

4094.610r

3

47

7. 5

0. 7

12. 0

2. 1

u

Fei

Fe I CN R 62 1,2 11

4099.048

4099.175

19

11

5. 6

3. 4

s,d

s,d

Fe I

|Tii

CN

/3. 30

13. 25

2. 17 R 60

eoo

651

207

1,2

}"

17

11

4094.698 23 5. 9 u CH P 8 1,1 3 4099.401r 4 1. 2

4094.938S 100 25. 4 s Cai 2. 52 25 4099.574r 4. 5 1. 5 s

4095. lOOr 11 2. 9 4099.788 57 17. 8 S Vi 0. 28 27

4095.268

4095.356

4095.481

40

18

29

10. 2

4. 9

7. 6

u

u

s

Mn I Fe I Fe I Vi

4. 19

1. 06

1075

41

4099.989 4100.165m

4100.345

13

58

26

4. 6

19. 0

9. 3

uw

s

Fe I p

Fe I

Fe I p

3. 43

f2. 85 U- 26

698

320

1103

4095.644r 4. 5 1. 2 Fe 1 3. 63 851 4100.508r 4 1. 6

4095.749r 8. 5 2. 2 4100.578r 2 0. 9

4095.816r 4095.981m

4096.108

5. 5

99

67

1. 5

25. 6

17. 6

siu

Fe 1 Fe I

2. 59

3. 64

217

911

4100.747m

4100.914

82

9. 5

29. 8

4. 6

u

u,N

Fe I (Pr 11)

IFe ipNb I

0. 86

0. 55

2. 45

0. 05

184

173

1

4096.213 39 10. 7 s Fe I p 0. 96 IS 4101.096 13 7. 1 w? 17

4096.329r 11 2. 9 4101.272m 47 25. 6 u Fe I 3. 40 698

4096.523r 15 4. 2 4101.378r 1. 5 1. 1 CN R 59 1,2 11

4096.643r

4096.696r

1 . 45

f 3. 7

1 9. 0 s

Zr n

Fe I

0. 56 15

16

4101.484r

4101.682

14

18

14. 9

43. 9 u Fe I 2. 48 120

4096.824r

4096.941

5. 5

39

1. 5

13. 2

CN

Fe I p CN

R 61

2. 43 R 61

1,2

173

1,2

11

11

4101.748m

4102.167

3133

15

746

10. 5

S

S

H5

(In i) V I

10. 20

0. 00

1. 05

1

1

41

4097.016r

4097.086 95

J

1 2. 4

1 23. 7 u

Fe I p Fe I3. 43

3.28

700

558

4102.380

4102.621r

5

3

2. 7

1. 5

s Y I 0. 07 7

4097.237r 15 4. 2 4102.761r 2. 5 1. 1 u Ni I p 4. 23 255

4097.32 a 2. 5 0. 7 4102.943m 106 35. 3 u,N Si I 1. 91 2

4097.460r 3. 5 1. 0 4103.19 a 1. 5 0. 6

4097.581r 7. 5 2. 1 4103.315 12 4. 1 u Dy II 0. 10 17

4097.650 19 5. 1 s Cr I 2. 89 97 4103.463 8. S 2. 9 s CN R 58 1,2 11,16

4097.796r

4097.962

5

30

1. 3

8. 2 s

Ru I Cri

Cr I

1. 14

2. 89

2. 89

9

9797

4103.611

4103.814r

28

3. £

9. 3

1. 1

s

s

Fe I

Cr I

/3. 25

I.O. DO

3. 12

650

oo J.

180

}17

4098.183m 113 30. E\ u Fei 3. 24 558 4103.988r 2 0. 6

4098.435r 6 1. EI s 4104.133m 100 28. 3 u Fei /2. 83

\3. 26 356

558

4098.539

4098. 594r

1

f 23. C

j 13. ^

) s,n

1

Cai

Cai

(Gd ii)

2. 52

2. 52

0. 82

25

2549

4104.306r 13 3. £

129
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4104.465

4104.54 a

4104.654r

4104.748

4104.862

29

5

9. 5 24

11

8. 5

1. 5

2. 9

6. 8

3. 4

s,d

s

s

IFe I Vi?

V I Cr I

2. 99

2. 14

1. 95

2. 97

422

112

108

4109.751r

4109.800

4109.960r

4110.042

4110.299

1 134

7

11

8. 5

[ 17. 8

I 23. 2

2. 0

2. 9

2. 2 s

|V.

[ Fei

CN

Zr II Ca II- Fe I

0. 26

2. 84

R 55

0. 76

7. 51

27

357

1,2

30

17

11

17

4104.944 54 14. 9 u Fe I 3. 33 694 4110.393r 3. 5 0. 9 Ce II 1. 09 29

4105.063r 8 2. 4 Fe I p 3. 43 700 4110.537m 97 24. 4 s Co I 1. 05 29

4105.164 61 16. S s V I 0. 27 27 4110.700r 4. 5 1. 1 s,N

4105.356

4105.654r

15

2. 5

4. 1

0. 7

u Mn I CN

4. 33 R 57

47

1,2 11

4110.867 65 16. 3 s Mn 1 Cr 1?

4. 33

2. 90

47

97

4105.726r 3. 5 1. 0 CN R 57 1,2 11 4111.000 44 10. 9 0 Cr II f3. 10

13. 76

1826

4105.828r 2 0. 6 S Tm I? 0. 00 16 4111.202r 1 0. 2

4106.05 a 1. 5 0. 4 Cr I 3. 11 180 4111.358m 42 10. 2 s Cr I 2. 90 97

4106.141r 0. 5 0. 1 4111.47 a 4. 5 1. 1 Gd II?

4106.266m 64 17. 0 s,n Fe I 2. 59 217 16 4111. 589r 6 1. 5

4106.432m 74 19. 5 u Fe I 3. 40 697 4111.680 14 3. 6 s? Cr I 2. 90 97 17

4106.585 14 3. 7 4111.787 106 26. 3 s V I 0. 30 27

4106.730 15 3. 8 u CH P 9 1,1 3 4111. 986r 11 2. 7 s,N

4106.944 12 3. 2 ul,N 17 4112.081r 14 3. 4 Fe I 3. 55 766

4107.10 a 1. 5 0. 4 4112.174r 6. 5 1. 6 Fe I p 2. 69 275

4107.297 8. 5 2. 2 s 17 4112.323m 69 17. 0 u Fei 3. 40 695

4107.492S

4107.662r

4107.781r

4107.886

125

1. 5

4

6

31. 9

0. 4

1. 1

1. 6

u Fei

(Vi)

CN

Fe I p CN

2. 83 L 19

R56

3. 60 R 56

354

52

1,2 831

1,2

11

11

4112. 450r

4112.569

4112.716

4112.914r

4112.958

7

9. 5

43

114

J

1. 7

2. 3

9. 7

\ 10. 0

[ 22.

2

s

}"J

Nil

Cr II

Ti I

Fe I

4. 15

3. 10

0. 05

4. 18

18

9

1103

4108.027 14 3. 6 u 4113.094r 8. 5 2. 1

4108.134 39 10. 0 s Fei 3. 24 559 4113.221 29 7. 3 Cr II 3. 10 18 17

4108.301r 6 1. 6 Fe 1 p 3. 69 833 4113.528 8 2. 1 S Vi 1. 22 52 17

4108.394r

4108.532

4108.75 a

4108.907

9

80

2. 5

25

2. 3

20. 2

0. 6

6. 6

s

s

w

Cri

Zri

Cai

2. 71

0. 54

2. 71

6532

39

4113.681

4113.866

4113.98 a

4114.118r

12

11

5

16

2. 9

2. 7

1. 2

3. 9

su

u

Mn I

CN

CN

4. 35

R53

R 53

47

1,2

1,2 11

11 4109.062m 75 19. 0 u Fei 3. 29 558 4114.308r 2. 5 0. 6

4109.220r 2 0. 5 4114.451m 100 25. 6 u Fe I 2. 83 357

4109.450 39 9. 6 s Nd 11 0. 32 10 4114.618r 9 2. 2

4109.582 18 4. 6 s Cn 2. 71 65 4114.780 9 2. 2

130
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AA (mA)

Recluced Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMl

No.

or

Vib. Banc

Notes

I

Wavelength

(A)

Equivalent Width

AX (mA)

Re- Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMl

No.

or

Vib. Banc

Notes

4114.942 65 15. 8 u Fe I 3. 37 695 4119.797 24 5. 8! u Ce II? 1. 09 22 4115.177m 98 23. g s V I 0. 29 27 4119.918 30 7. li u

4115.376 11 2. 7 s Ce II 0. 92 22 16 4120.048 8. ^> 2. ] s Ti'i 2. 30 253

4115. 562r 2 0. 5 4120.212S 97 23. I Fe il 2. 99 423

4115. 681r 1 0. 2 4120. 472r 10 2. AI S

4115.808r 5 1. 2 s Ir I? 1. 73 4120.622 21 ) s Cr I 2. 71 65

4115.890 15 3. 9 s Fe I p 3. 64 910 4120.773r 4. L) 1. 1 s?

4115.980 35 8. 0 u Ni I 4. 15 255 4120.838 13 2. L) u Ce n 0. 32 112

4116. 123r 4. 5 1. 1 u 4121.06 a 7. £ 1. ? u

4116.208r 6. 5 1. 6 CN R, 52 1,2 11 4121. 155r 4. 5 1. 1

4116.321r 5 1. 2 4121.325m 125 30. 3 u Co I 0. 92 28

4116.481 58 14. 1 s Vi'x 0. 28 27 4121.495 8 1. 9 Zr I — 0. 54 32

4116.553

4116.60 m

4116.704

14

35

4. 0

7. 3

S

u

V ip 0. 26

0. 27

27

27

13

4121.650

4121.810m

8. 5

94

2. 1

22. 8

S

u

Ti IRh.i?

|FeiCr I

0. 97

2. 83

2. 98

9

356

108

4116. 821r

4116.957

4117.164r

8

34

0. 5

2. 1

8. 2

0. 1

u Fe I 3. 24 558

4121.990

4122.150

16

30

3. 9

7. 3 s

Ni I —

Fe I p Til—

|Cr I

3. 66

3. 55

2. 66

2. 71

765

296

65

4117. 261r 2 0. 5 4122. 243r 7 1. 8 CN R 49 1 2 11

4117.434r 2. 5 0. 6 4122.358 10 2. 4 Mn I 4. 36 47 4117.56m s 13 4122.523m 86 20. 8 u Fei 2. 84 356

4117.588r 9 2. 2 4122.665 63 U. 8 w,n Fe II 2. 58 28

4117.741r 8 1. 9 Fe I 3. 65 833 4122.783r 10 2. 4 Mn I 4. 34 47

4117.856 76 18. 4 u Fe I /3. 42

14. 28

700\

1103/ 17 4122.874r 4 1. 0

4117.995r

4118.153

4118.194r

4118.428r 4118.555m

7

27

13

8

154

1. 7

6. 6

3. 4

2. 1

37. 4

s,N

s?

s

u

Ce II- Vi

Fe I (Sm II)

0. 70

1. 95

3. 57

0. 66

11

112

80154

4123.031r 4123.234m

4123. 277r

4123.388

4123.514

4123.561r

7. 5

54

24

I 73

1. 8

[ 11. 2

1 2 4

5. 8

[ 17. 2

[ L2

s,N

V

f La II

Tl I Cri

1 VI

I Til

0. 32

2. 78

3. 00

0. 27

2. 68

41

302

108

27

296

16

4118.782 148 35. 9 u Co I 1. 05 28 4123.753m 109 26. 4 u Fei /2. 61

12. 99 217422

4118.895

4119.054r

4119.259 4119.400m

4119.526

4119.671

75

16

12

72

26

23

26. 0

3. 9

2. 9

17. 5

7. 1

5. 6

u

s,d? u

u

s

s,d?

Fe I

Fei

Fe II p

Fe I p —

CH

3. 26

2. 54

2. 86 P 10

559

21

320

1,1

16

17

3

4123.878r

4123.939

41/4. lObr

4124.207r

4124.358r

4124.489

23

16

9

6. 5

2

31

5. 8

4. 9 o o

z. z

1. 6

0. 5

7. 5

u?u

su

s

Ce II - Sm II? V I

Fei?

Fe I

0. 86

0. 48

1. 22

3. 64

60

46

52

131

761-925—66 11
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4124.630r 5. 5 1. 3 4129.505r 3. 5 1. 0

4124.786 33 7. 3 u Fe 11 2. 54 22 4129.608r 9. 5 2. 4

4124.915 18 4. 1 u Yii 0. 41 14 4129.724 54 12. 1

! s d \ XNNj Eu II 0. 00 1

4125. 133r

4125.228

1. 5

6. 5

0. 4

1. 6 Feip 2. 45 173 4129.958 18 4. 8 u

(1. 56

13. 11 444125.377r 4 1. 0 486 4130.038 64 15. 6 s Fe I

4125.460 10 2. 4 Cri? 4. 21 4130.139r 4 1. 0 CN R 45 1,2 11

4125.626

4125.694 4125.886m

4126.048r 4126.191m

4126.380

4126.519

4126.646r

4126.857

1 100

75

5. 5

113

6

47

7

36

1 19. 9

1 6. 3

18. 2

1. 5

27. 4

1. 5

10. 9

1. 7

7. 3

uu

s?

su

s

s

Fe I

Fei

-Cri

Fei

Cn

XT' ^ ie I

4. 22

2. 84

2. 71

3. 33

2. 54

2. 84

1103

354

65

695

35

354

4130.249r

4130.368r

4130.455 4130.657m

4130.695r

4130.856

4130.999r

4131.117

3

11

19

45

5

26

7

49

0. 7

2. 7

4. 6

10. 9

1. 3

6. 3

1. 7

11. 9

s?

u,d

u,N

s

Gd II Cn

Ba II Ce II -Si II

Mn I (Ce II)

fO. 60

10. 73

2. 91

2. 72

0. 56

9. 84

4. 23

0. 33

1949

97

4

209

3

112

4126.918 7 1. 7 s Cri 2. 71 66 4131.267r 6. 5 1. 6 s Til 2. 30 253

4127.073r 6. 5 1. 6 s Ti i?p 1. 46 114 4131.348 21 5. 1 s Cn 3. 84 261

4127.275 32 7. 8 M? Cri /2. 54

14. 10 35 17 4131.454r 5 1. 2 Mn I 3. 38 37

4127.376

4127.537r 4127.613m

16

1 121

4. 1

1

2. 7

1 27. 6

M?

su

Ce II Til

Fe I (Cri)

0. 68

2. 69

2. 86

2. 71

4

296

357

65

17 4131.596r

4131.760

4131.798 4131.957m

1. 5

23

4

60

0. 4

7. 0

1. 7 44 0

u

s

Fei

Fe I p

CN

Fe 1 p

Fe I p

4. 22 R44

3. 26

3. 42

1075

1,2

558

695

11

4127.803m

4127.941r

4128.098

97

9

107

23. 5

2. 3

25. 9

u

s

Fei

Fei

Vi

(Si II)

/3. 28

\3. 41

0. 28

9. 83

558

727

27

3

4132.067m

4132.283r

4132.409

404

5

19

m

1. 8

5. 6

S

u

Fez

(Vi)

Gd II Cr II

1. 61

0. 29

0. 60

3. 76

43

27

49

26

4128.309 12 2. 9 s Yi 0. 07 5 4132.538 77 20. 1 u Fei 4. 26 1103

4128.391r 8 1. 9 w? Cri 4. 10 4132.711 40 10. 2 s

4128.506r

4128.595r

4128.742

4128.88 a

3. 5

2. 5

50

10

0. 8

0. 6

12. 1

2. 4

w Fe II Rh I Vi2. 58

0. 97

1. 94

27

8 112

4132.908m

4133.133r

4133.290r

4133.357

123

3

2

11

29. 8

0. 7

0. 5

2. 7

V,

u

Fei

(Sci)

Nd II

2. 84

1. 94

0. 32

357

20

19

4128.975r 9 2. 2 4133. 474r 7 1. 7

4129.184

4129.324r

84

13

20. 3

3. 1

s llCri Fe I2. 91

3. 42

97 698

4133.610m

4133.722r

48

6

11. 6

1. 7

w Fe I CN?-

CH?

R 43 R35

1,2 0,0 114

4129.463 57 13. 8 u Fei 3. 40 695

132
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4133.815

108

J

f 5. 6

94. 0

Ce 11

X' C J.

10. 52

10. 86

4

4

yJVO

4138.618r

4138.756r

4

8. 5

1. 0

2. 1 CN R31 2,3 11

4134.009

4134.196

30

22

7. 5

5. 3

u

Fe I 2. 61 217

4138.853

4138.987r

4139.089

17

10

27

4. 1

2. 4

6. 5

u

u

Fei

-CN

CN2. 28 R 40 R40

117

1,2

1,2

11

11

4134.347 ( 20. 3 s Fe I 0. 00 3 4139. 225r 14 3. 4 u

4134.438 > 186 < 28. 0 1 Fei /3. 02

13. 42 482\697/ 15 4139.371r 14 3. 4 CH R31 0,0 4

4134.524r i 6. 5 I Vi 0. 30 27 4139.458r 8 1. 9 Co I 2. 04 94 4134.685m 129 31. 2 u Fe I 2. 83 357 4139.610 14 3. 4 CH R31 0,0 4

4134.897

4135.037

4135. 173r

4135.297

26

38

6

26

6. 3

9. 2

1. 5

6. 3

su

s,N

Mn I CH?

Rhi?-

Nd II

4. 25 R33

0. 71

0,0

17

4

4139.732r

4139.936S

4140.062r

4140.162r

3. 5

86

1

4

0. 8

20. 8

0. 2

1. 0

u

u

Fei

Nbi

Fei

CN?

0. 13

0. 99

R 30

1

18

2,3 11

4135.458

4135.686r

4135.760

19

7

22

4. 6

1. 8

5. 3

u,N

J

CN?

CH?

(Ce II)

f ZnIFei

I Osi

R 42 R 33

0. 56

0. 63

4. 19

0. 52

1,2 0,0 188

50|

1073]

3

114

17

4140.247

4140.407

4140.457r

4140.54 a

18

68

10

5. 5

~ 4. 3

16. 4

2. 9

1. 3

u

u

FeiSci

Fe I p

Fei

2. 95 L 95

3. 42

3. 40

418

20

695

694

4135.938r 9 2. 2 4140.755 18 4. 3 CN R 39 1,2 11

4136.093r 1 0. 2 s Vi? 1. 87 4140.831r 6. 5 1. 6 u CN R 39 1,2 11

4136.293r 2. 5 0. 6 4141.056 18 4. 3 u Mn I 4. 26

4136.375r 4. 5 1. 1 s Vi? 0. 29 26 4141.311r 1. 2 Fei? 3. 02 480

4136.527S 73 17. 6 s Fe I 3. 37 694 4141.529 18 4. 3

4136.738r 6 1. 5 4141.652 19 4. 6 CN?- R 29 2,3 11

4136.881r 4. 5 1. 1 s Ti I? 2. 25 221 4141.755r 3 0. 7 La II 0. 40 40

4137.005m 104 25. 1 u Fe I 3. 41 726 4141.871m 68 16. 4 u Fei 3. 02 422

4137.120r 7. 5 1. 9 Nbi? 0. 00 1 4142.026 6. 5 1. 6 s

4137.274 48 11. 6 s Til

(Mn I)

2. 32

3. 38 25337

4142.177 51 12. 3 w Ni I Cri

3. 90

4. 45 212

4137.415 59 14. 3 u Fe I 4. 28 1103 4142.308 43 10. 4 u Ni I

4137.655

4137.773r

4137.886r

4137.979

4138.136

4138.20 a

33

11

12

26

18

6

8. 0

2. 8

2. 9

6. 3

4. 3

1. 4

s

suw

Ce II Fe I

Fe I

0. 52

2. 83

2

320

4142.407r

4142.474

4142. 588

4142.768r

4142.842

4142.944

10

45

70

8

22

28

2. 9

11. 6

16. 9

1. 9

5. 3

6. 8

suu

s

s

Ce 11 Cn

Fei

Yi

VnNii

0. 70

3. 12

4. 30

0. 00

3. 97

4. 09

10

179

1103

5

226

16

4138.360 34 8. 2 4143.041 23 6. 0 s Til 2. 30 253

4138.494 13 3. 1 Nix 4. 17 237 4143. 160r 12 3. 1 Pr II 0. 37 4

133
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4143.274r 5. 5 1. 6 Til 2. 29 253 4147.675m 110 26. 5 s Fei L 48 42

4143.416r 134 36. 2 u Fei 3. 05 523 4147.863r 4. 5 1. 1

4143.508r 35 16. 9 w1 Fe I p 3. 37 697 4147.975r 2. 5 0. 6

4143.626r 6. 5 2. 7 4148.169 2. 5 0. 6

4143.747r 12 8. 0 4148.252 6 1. 4 Fe I p 3. 65 832

4143.878m

4143.974r

4144.075

4144.l97r

466

1

1 "

15

121

{ 1. 7

1

1 8. 2

5. 1

S

u,N

Fe I (Fe i)p

IRuiCN

1. 56

2. 86

1. 00 R37

43 354

9

1,2 11

4148.395

4148.493

4148.618r

4148.720r

4148.783

8. 5

13

3. 5

6. 5

20

2. 0

3. 1

0. 8

1. 7

4. 8

u

u1

u,N

CN?

Nil

Mn I

R 24

3. 46

4. 27

2,3

89

11

4144.242 6 1. 8 CN R37 1,2 11 4148.917 5 1. 2 Ce II? 1. 09 28

4144.33"a 1 0. 2 S 4149.128 21 6. 0 w,m

4144.387 6. 5 1. 8 4149.202 62 14. 9 u Zr II 0. 80 41

4144.519 13 3. 4 s,d 17 4149.370m 111 26. 8 u Fe I 3. 33 694

4144.668r

4144.768

6. 5

14

1. 6

3. 4 CN? R 27 2,3 11

4149.495

4149.538 38

J

f 7. 0

1 2.

9

u,N Fe I p

CH

3. 69 R 28942

0,0 4

4144.855 11 2. 7 4149.699r 3. 5 1. 0 CH R 27 0,0 4

4145.005m 19 3. 6 s,d Ce II- 0. 70 9 17 4149.765 67 16. 1 s Fei 0. 05 3

4145.086r 2. 5 0. 6 4149.897 14 3. 6

4145.201 38 8. 2 u Fei 2. 69 274 4149.979 7. 5 1. 9

4145.308r 6 1. 4 4150.06 a 4. 5 1. 1 -Viip 2. 03 37

4145.442 14 3. 6 w 4150.254 75 18. 1 s Fei 3. 43 695

4145.559 32 7. 7 w -CH R 29 0,0 4 4150.375 10 3. 1 0? Ni I 3. 94 178

4145.760 57 13. 0 w -Cr II 5. 32 162 4150.445 43 10. 4 w Coi- 0. 58 16

4145. 863r

4145.975

4146.068

4146.234a

6

23

72

18

1. 7

5. 5

17. 4

4. 3

u

u

s,d

Fei

Cri

/R 36 \R 26

2. 99

3. 84

1,2 2,3

422

260

111

17

4150.548r

4150.706r

4150.801

4150.970

9. 5

9

11

43

2. 3

2. 2

2. 7

10. 4

s

u

s

Tii

-CN?

-Ti I?

||Ti I Zrii

2. 30 R 33

2. 24

2. 17

0. 80

253

1,2

221

206

42

11

4146.384 5 1. 2 4151.066r 5 1. 2 s

4146.500 10 2. 4 w 4151. 201r 2 0. 5

4146.689 19 4. 6 -Cri 2. 97 107 4151. 270r 2 0. 5

4146.835

4146.990

6

45

1. 4

10. 8 w

4151.30 a

to 4151.50 a } = 1. 2 Fei4147.213 15 3. 6 CN? R 25 2,3 11 4151. 567r 4 1. 0 Cr ir 2. 97

4147.347 52 12. 5 w Fei 3. 33 693 4151.666 6. 5 1. 6

4147.492

4147.520r 1 38

f 8. 2

I 1.7

w Fe I p Mn I

3. 60

3. 37

832

37

4151.768

4151.950

36

62

8. 7

14. 9

w

u,d

Fe 11 p

|Fei

La II

2. 28

3. 55

0. 23

12

764

40

134
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

A\

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4152 092 68 27. 2 Fe I p 4. 07 1049 4156.455 51 12. 3 w Fe I 3. 37 693

4152.176

4152.317

107

16

25. 8

3. 8

Fe I CN?

0. 96

R 32

18

1,2 11

4156.604

4156.672 1 80

f 3 1

I 17. 3 u Fei 2. 95 419

4152.36 m s Sc 1 1. 97 20 13 4156.806m 126 30. 3 u Fe 1 2. 83 354

4152. 388r 8. 5 2. 0 CN R 32 1,2 11 4157.004 26 6. 5 Mn I 4. 64

4152 5'>7

41 52 fim

8

8

1. 9

1. 9 Nb I 0. 09

4157.195

4157.234

[ 26

J

1

5. 3

I 1 1

s,N

4152.766 22 5. 3 u Cri 3. 85 261 4157.427 6 1. 4

4152 913 7. 5 1. 8 4157.577r 8 1. 9

4152 97 a 2. 5 0. 6 Fe II p 2. 89 45 4157.788m 127 30. 5 u Fe I 3. 42 695

4153.066

4153.124r

9

1. 5

2. 2

0. 4

s,N Cn 2. 54 35 4158.007

4158.081r 1 56

1

7.

0

1 7.

CH

CNR 26 R 16

0,0

2,3

14

11

4153.242 1 0. 2 4158.267r 3. 5 0. 8 s Ti I?

4153.389m

4153.494

36

3

8. 7

0. 7

u,d2 CH

Fe I R 27 0,0 4 4158.376

4158.425

1

6. 0

1 2.

s,d Fe I Co IFe II p

2. 87

2. 28

144

12

17

4153.620 24 5. 8 s CH- R 27 0,0 4 4158.539r 6 1. 4 Nil 4. 26

4153.820

4153.906

4154.105 4154 204r

4154.287 4154 379

4154.505m

21

138

69

6. 5

18

23

126

8. 7

33. 2

16. 6

1. 7

4. 8

7. 0

30. 3

u

u

u

%L

U

Cn

Fell

Fe^i

CH

CH

Fe I

/2. 54

12. 54

3. 40

3. 40

R 26 R 26

2. 83

3535

695

694

0,0

0,0

355

4

4

4158.798m

4159.044 4159.186m

4159.240r

4159.401r

4159.479r

4159.645

103

12

1 114

5. 5

1. 5

13

24. 8

3. 1

1 26. 7

I 0. 6

1. 3

0. 4

3. 1

u

w

s

s

Fei

Ce II? (CH)

CH

llTiiVi

3. 43

1. 03 R 25 R 25

2. 16

0. 29

695

246

0,0

0,0

206

25

4

4

4154.665 17 4. 6 W 4159.865 18 4. 3 u,N CN- R 27 1,2 11, 17

4154.814S 120 28. 9 U Fe I 3. 37 694 4160.092 24 5. 8 w

4154.966r

4155.052

4155.199r

4155.316r

4155.428r

4155.523r

4155.641

4155.715r

4155.915

4156.083

4156.235

4156.307

8

4. 5

3. 5

2. 5

6. 5

6

7

2. 5

AO

30

j 103

1. 9

1. 1

0. 8

0. 6

1. 6

1. 4

1. 7

0. 6

8. 4

7. 2

r 7.

1 20. 4

W

su

u

Sm II?

-CN?

Mn I

l^e I Ndii

Zr II Fe I

0. 54

R 30

3. 38

0. 18

0. 71

50

1,2

37

10

29

11

4160.246

4160.368

4160.559.

4160.778

4160.928r 4161.085m

4161.208

4161.310r

4161.408 4161.517m

4161.670

19

64

30

20

2

52

58

7

26

96

7. 5

4. 8

15. 4

7. 2 4 8

0. 5

12. 5

13. 9

1. 9

6. 7

23. 1

1. 8

w

su

uw

u

u

CNFe II? p

Fe IFe I Fe I p

Fe I

Zr II Nil

Cn

Fe I Ti II

R 14 4 74

2. 95

4. 21

3. 37

0. 71

3. 19 4 45

3. 02

L 08

2,3 149

419

1116

689

42

86

305

422

21

11

135
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Widtn

AX

(mA)

Re- duced

Vv latn AX/X

(F)

bpot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. xsana

Notes Wavelength

(A)

Equivalent w lutn AX

(mA)

Re- duced w icitn AX/X

(F)

opOt

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. xSanu

Notes

4161.799m

4161.949r

30

4. 5

7. 2

1. 1

w Sr n 2. 94 3 4166.298

4166.352r 1 20

I 0. 7

S -|Tii

Zn

1. 88

0. 69

163

45

4162.120r 4 1. 0 4166.532r 4 1. 0 CN? P 36 3,4 11

4162.292 6 1. 4 CN R 12 2,3 11 4166. 664r 21 5. 0 s,d

4162.460

A 1 CO C AH

29

Q A

7. 0

o. /

0?

u

ICHCN?

R 25 r 0

xl Zd R 25

0,0

1,2

4, 17

li

4

11

4166.854

4166.965

4167.038r

26

37

8

6. 5

8. 9

2. 4

ul Ni I CN4. 10 P 34 3,4

17

11

4162.90Sr 4. 5 1.

1

u,N Fe I p 3. 02 476a 4167.173 24 8. 2 CN P 33 3,4 11

4162.984r 3 0. 7 CN P6 3,4 11 4167.277m 200 48. 0 w Mgi 4. 34 15

4163.121r 1 0. 2 -Cr I 2. 54 35 4167.400 14 5. 8 CH R 24 0,0 4

4163.289r 3. 5 0. 8 CN R 11 2,3 11 4167.52 m 11 3. 4 S Yi 0. 07 7

4163.356r 7 1. 7 Fe I p 4. 19 1073 4167.571 54 13. 2 u CH R 24 0,0 4

4163.480

4163.654S

4163.799r

A 1 onot. 4iDo.yuyr

4104. loor

4164.263

42

107

6

0. 0

1

0

1 66

10. 1

25. 7

1. 4

1. o

O. D

1 O

( 8. 9

u,d

u

« .*> wc

su

CNllTi n

iCri Fe I

V II

111 Fe I p—

CH

P 7

2. 59

/2. 54

12. 54

/2. 69

13. 42

0 r\A Z. U4

1 <J'7 1. o7

3. 42 R 24

3,4

105

35

35 274

699

O 1

694

0,0

11, 15 17

164

4167.722

4167.864

4167.968

4168.120r

4168.177r

4168.287r

4168.475r

4168.620S

4168.794

4168.950

44

50

67

5. 5

3. 5

1

13

51

5. 5

55

10. 6

12. 7

16. 1

1. 3

0. 8

0. 2

3. 1

12. 2

1. 3

13. 2

u

u

u

w

s

s?

Fei

Fei

Nbi

Cr I?

Fe I

Fe I

3. 30

3. 64

0. 00

3. 84

3. 37

3. 42

599

1

261

689

694

16

j I 7. y u

T r Oil R 24 A A

(J,U

A t ^ 4,16 4169.093 8 1. 9 s Fe I p 1. 01 18

4164.513r 3 0. 7 4169.252 7. 5 1. 8 w1 CN? R 20 1,2 11

4164.642

At ft A '7Q 1 41d4. /^ol

19

O A z4

4. 6

0. 6

s

s

Ni I (Nb i)

r e I

0. 42

0. 05

z. yy

28

1

A t O 41o

4169.336

4169.469

10

9

2. 4

2. 2

s

s

Ti I CN?-

Sm II

1. 89 R4

0. 25

163

2,3 24

11, 17

4lD4.yDlr

4lD0.1iy

41o5.lD»r

y. 0

1

o o

Z. 6

r "7/1

[ 3. 1

•V\s,NN

J

Mg I CN —

Sci

4. 34

R 9

1. 99

2,3 20

17

11

4169.615

4169.765

4169.853

54

52

17

12. 9

12. 5

4. 3

u,al

u

/ < r T (jti —

CH

Fe I Cri

R 23 R 23

3. 40

4. 10

0,0

0,0

693

278

4

4

4165.391m 84 20. 2 u,d? -Fei 3. 64 4169.986 4. 5 1. 1 Fe II p 2. 28 12

4165.516 5. 5 1. 8 Cri 4. 45 305 4170.142 16 3. 8 u

4165.595 48 11. 5 u Ceii- 0. 91 10 4170.210 15 3. 8 Cri 4. 10 278

4165.791r 5. 5 1. 3 4170.347r 1. 5 0. 4

4165.999

4166.100

4166.193

9

8

2. 5

2. 2

1. 9

0. 6

s |Ba 11 CNCN

CN

2. 72 P38

R 8 P 37

4

3,4

2,3

3,4

17

11

11

11

4170.485

4170.635

4170.740r 4170.912m

7. 5

8

4. 5

97

1. 8

1. 9

1. 1

23. 2

1 s,d

u

CN

Cr II

Fei

R 19

3. 10

3. 02

1,2

18

482

11

136
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Not

4171.050 92 22. 0 u Tii- 2. 15 206 4175.464r 7. 5 1. 8

4171.273r 12 2. 9 4175.643m 110 26. 3 u Fei 2. 84 354

4171.432 11 2. 6 4175.780r 5 1. 2

4171.558

4171.695

8

73

1. 9

17. 5

u,N

u IIFei Cri3. 69

3. 85

941

261

4175.910

4176.061r

45

6

9. 4

1. 4

u IIFeip

Cr I

3. 40

3. 00 694

106

4171.908 90 21. 6 u Fe I Ti n

3. 30

2. 60 650

105 4176.267 8. 5 2. 0 CNCN

R 14 R 14

1,2

1,2 1111

4172.053 42 13. 9 s Gai 0. 10 1 4176.411 19 4. 8 Fe II? p 4. 74 149

4172.131 99 23. 7 u Fei 3. 25 649 4176.577 124 29. 7 u Fe I 3. 37 689

4l72.287r 4 1. 0 4176.872 25 6. 0

4172.349r 6 1. 4 4176.990 10 2. 4 CN P7 2,3 11

4172.482 48 12. 0 u CH R 23 0,0 4 4177.080 27 6. 5 s Fe I 3. 33 690

4172.588r

4172.644

1 108

f 5. 8

[ 25. 4

1 w

|Tii

Cr 11? Fei

1. 88

3. 10

3. 33

163

18

689

4177.195r

4177.332

2

29

0. 5

6. 9 s

Cr I? Nd nTii3. 01

0. 06

1. 89

133

10 163

4172.759 110 26. 4 s Fei 0. 96 19 4177.421r 3 0. 8 CN P8 2,3 11

4172.885r

4172.975

4173.149r 4173.323m

4. 5

49

11

76

1. 2

11. 7

2. 6

18. 2

w

s

CN

Fe I p

Fe I p Fei

R 17

/3. 64

14- 22

3. 40

2. 84

1,2

909

1073

698

355

11 4177.537r

4177. 611r

4177.698

4177.849

1 151

41

48

f 20. 8

1 20. 8

13. 6

11. 5

} »

1

0 w,N

Yii

Fei

Fe II p |CH- CN

0. 41

0. 91

2. 54

R 22 P 9

14

18

21

0,0

2,3 4

11

4173.470

4173.542

90

59

21. 6

21. 8

1 w

Fe n

Ti II

2. 58

1. 08

27

21

4177. 999r

4178.059 1 83

1

2. 4

1 18. 2 w

CH

Fei

R22 0,0 4

4173.681r 7 1. 7 4178.235 15 3. 6 CN P 10 2,3 11

4173.790r 4173.933m

4174.077

2

85

40

0. 5

20. 4

9. 8

su

Fei

|Ti II Ti I

0. 99

2. 60

0. 90

19

10555

4178.382

4178.479

4178.625

25

16

16

6. 0

4. 1

3. 8

s

u

CNVii

CN

R 12

1. 69

P 11

1,2 25

2,3

11,

11

4174.15 m 3 0. 7 s Yi 0. 07 6 4178.859S 79 18. 9 w Fe 11 2. 58 28

4174 2 0. 5 Fe I 4178.944 7 1. 9 CN P 1 9 9 '\ z,o 1

X X

4174.317 17 4. 3 u,N Mn II — 1. 81 2 4179.057 . 6. 5 1. 6 Cri 3. 85 250

4174.405

4174.486r

33

6. 5

7. 9

1. 6

w Fei

Til

3. 57

2. 23

799

220

4179. 198r

4179.249 1 49

r 3.

1 8. 8 u,N

-Co I?

|Cri

2. 88

/3. 11

13. 85

144

179 250

4174.646r 2. 5 0. 6 CN? P 13 2,3 11

4174.812 4174.917m

4175.130

33

103

66

9. 8

24. 7

15. 8

s

s w,N

Cr I Fe I CHCN

0. 91 R 22 R 1519

0,0

1,2 4

11

4179.383

1 y.o / o

4179.674

126

110K

2. 5

30. 2

O. 0

0. 6

s

u

-IIVi

Cr n

Fei

0. 30

3. 83

Jt O'i

25

26

11, J

4175.222r

4175.332

11

16

2. 9

3. 8

Cr I 3. 85 261 4179.811 14 3. 3 u Zr II CN

1. 66 P 33 99

2,3 16

11

137
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

A\

(mi)

Re- duced

Width

A\/\

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(niA)

Re- duced

Width

AA/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

R MT

No.

or

\'ib. Band

Notes

4179.86 m Ti I 2. 17 206 13 4184.996r 14 3. 6 s,N CN- R 22 0,1 11, 16

4179.998r

4180.045

4180.154

4180.242

4180.403

4180.571r

10

3

6

46

6. 5

i::

0. 7

1. 4

11. 0

1. 6

U

CN

Cri?

CN

CN

CN

Fei

CN

P 32

4. 62 /P 16 IP 32 P 31 P 31

2. 73

fP 19 IP 29

2,3

2,3 2,3

2,3

2,3

274

2,3

2,3

11 )"

11

11

}"

4185.151r

4185.364

4185.546

4185.651

4185.779

4185. 971r 4186.126m

2. 5

14

14

12

19

1

42

0. 6

3. 3

3. 3

2. 9

4. 5

0. 2

10. 0

s,d u,N

s

s

Cr I

Fe I p Fe I

Ti I p Til

2. 98

4. 26

2. 24

1. 50

106

1104

220

129

17

4180.678r

1 4180.811

6. 5

80

1. 6

19. 1

CN

CH

P 28 R 21

2,3

0,0

11

4

4186.336 39 9. 3 u,N CNCri

R 21

/3. 85

13. 86

0,1 249

11

li

4180 904r 12 3. 3 CN—

CN

fP 22 \P 26 fP23

IP 25

2,3 2,3

2,3 2,3

111 In

4186.464r

4186.622

12

95

3. 1

22. 7 u,N Ce II- ICH0. 86 R 201 0,0 4

4180.99 a 4 1. 0 CN P 24 2,3 11 4186.797r 12 2 9

4181.083 5 1. 2 4186,84m s 13

4181.189 13 3. 1 Fe I 3. 63 908 4187.047m 204 48. 7 u Fe I 2. 45 152

4181.353

4181.551 4181.764m

4181.974

4182.216r 4182.387m

4182.589

4182.763

4182.851

10

62

148

93

26

88

7

63

12

2. 4

14. 8

35. 4

22. 2

6. 2

21. 0

1. 7

15. 1

3. 1

U

u

u

u

su

CN

Fe I Fei

-CN

Fe I Vi

Fei

R 9

3. 55

2. S3

R 24

3. 02

0. 28

3. 42

1,2

763

354

0,1

476a

24

694

11

11

4187.255

4187.335

4187.457r

4187.594

4187.720r

4187.812

4188.097

4188.315

31

22

15

76

j- 224

39

16

7. 9

5. 5

3. 6

18. 6

[ 7. 2

1 53. 5

9. 3

3. 8

u,N

su

u

ICo I CN

Ce II?-

Fei

Fe I

Fe I CN

2. 04 P 49

0. 55

3. 43

2. 42

P 48

93

1,2

86

694

152

1,2

11

7

15

11

4183.008 36 8. 6 u Fei 3. 40 697 4188.450r 8. 5 2. 0 CN? R 0? 1,2 11

4183.186 9. 5 2. 3 Fe II? p 2. 64 21 4188. 583r 10 2. 4

4183.326 32 8. 6 u Ti ICH2. 24 R 21 220

0,0 4 4188.737 120 28. 6 u,d1 Fe I-

(Ti I)

4. 21

2. 24

1116 220

4183.457 78 18. 6 u |V II- CH

2. 05 R 21 37

0,0 174 4188.978 72 17. 2 Ni I CH

3. 70 R 20 0,0 4

4183.628 17 4. 1 Fe I 4189.102 44 11. 0 CH R 20 0,0 4

4183.805 28 6. 7 u,N 4189.332r 2. 5 0. 6 4183.998m 131 31. 3 w -Fe I 4189.565 70 16. 7 u Fe I 3. 69 940

4184.312 76 18. 2 si Ti II 1. 08 21 4189.816 16 3. 4 s Vi 0. 29 24

4184.478 21 5. C w1 Ni IFe I

3. 40 89 4189.989 21 5. 0 u Mn I Cri

4 25

2. 97 106

4184.635r 4 1. f Cri? 4. 53 4190.130 25 6. 0 u Cr I 2. 87 84

4184.900S 97 23. 2 u Fe I (Cri)2. 83

3. 09 355

155 4190.239

4190.396

20

10

4. 8

2. 4

s Vii 1. 67 25

138
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Pow

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4190.530r 7. 5 1. 8 4194.848 05 1.5. 5 u CH R 19 0,0 4

4190.717

4190.893

58

11

13. 8

2. 6

s u,NCot

Vii

0. 00

2. 03

1

37

4194.996 47 11. 2 s,dl CH

Cr I CN

R23

3. 85 P 35

1,1 248

1,2

4

11

4191.079 9. 5 2. 3 Gdii- 0. 43 34 4195. 161r 9. 5 2. 4

4191. 164r 9 2. 1 4195.340m 127 30. 3 M Fe I 3. 33 693

4191.277 4191.437m

47

181

14. 1

43. 2

s

s CnFei

(Vi)

2. 54

2. 47

0. 27

35

15224

4195.415r

4195.528

11

38

3. 6

10. 7 W

Cr 11—

CH

Ni I

4. 98 R22

4. 09

155

1,1 239

4

4191.683S

4191.863

98

14

23. 4

3. 3

u Fe I (Cri)

CN

2. 86

2. 54 P 4

355

35

1,2 11

4195.627

4195. 830r

86

3

20. 5

0. 7

S Fex .3. 02 478

4192.016 52 12. 4 u CN?-

CH

P 62 /R 23 IR24

0,1

1,1

i!i

11, 17 4195.945

4196.214m

20

98

4. 8

23. 4 u

CN

Fei

/P 14 IP 32

3. 40

1,2

1,2

693

}"

4192.101r

4192.204

22

14

6. 9

3. 6

s,N Cri

CH

3. 98 R 24

273

1,1 4

4196.359r

4196.419r

\ 25 J 3.1

1 3.1

u Ce 11-

CN

0. 42

fP 16 IP 30

123

1,21 1,2/ 11

4192.400 10 2. 4 CN

Fei

fP 5 IP 41

1,2 1,2 4196.542 67 16. 0 u Fe 1 (La ii)

2. 95

0. 32 418

41

4192.572 66 15. 7 u CH R 19 0,0 4 4196.675 42 10. 0 u,N Fei

4192.752 2 0. 5

fP 6 \P 40

0. 74

1,2 1,2

79

4196.767 11 2. 6 CN /P 18 IP 28

1,2

1,2

A-i no Qns

4193.107

0V

7. 5 1. 8 Ce II111 4196.878 15 3. 6 CNCN

P 27 /P 19 IP 27

1,2

1,2 1,2

11

4193.278 5. 5 1. 3 CN P 61 0,1 11 4196.996r 9. 5 2. 4 CN fP 20 IP 26

1,2

1,2 4193.383

4193.447

4193.621r

4193.679r

5. 5

7. 5

1 46

1. 3

1. 8

1

3. 3

I 8. 3

CN

CN

Fe I Cri

(Nil)

/P7

IP 39 P 39

3. 85

3. 83

1,2

1,2

1,2

248

)"

11

4197.100m

4197.234

4197.360

66

21

16

15. 7

5. 0

3. 8

s

sw

Fei

CNCN

Cn

Fe I p

0. 99 P 25 /P 22 IP 24

3. 85

3. 88

18

1,2 1,2

1,2

249

976

11 }"

4193.811

4193.874

23

8. 5

5. 5

2. 1

CN

Ce II?- CN

Cn

JP 8 IP 38

0. 55 P 38

3. 85

1,2

1,2

85

1,2 248

}"

11

4197.508r

4197. 648r

4197.741

2. 5

1 23

0. 6

j

2. 9

I 2. 9

s,N

s,N

Fe 1 CN? —

Gd II? P 57 0,1 11

4194.089r 2 0. 5 Fei 4197.895r 12 2. 9

4194.241 10 2. 4 CN fP 9 IP 37

1,2

1,2 111 4198.068

4198.138

93

11

23. 1

5. 7

u,N Fei4194.316

4194.488

6

17

1. 4

4. 0 u

CN

Fei

JP 60 IP 37

2. 73

0,1

1,2 274

}" 4198.242

4198.330

1

1 234 1 27.5

1 36. 3 }«

Fe 1

liFei

3. 37

2. 40

693

152

4194.627r

4194.736

6. 5

42

1. 7

10. 5 u,N

CN

CN?-

CH

JP 10 IP 36 P 36 R 19

1,2

1,2

1,2 0,0

}"

11, 16

4

4198.426r

4198.522

12

24

4. 5

8. 1 u

Co I Cn0. 10

/3. 85

13. 98

2

249 272

761-925—68 12 19
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EF

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4198.638S

4198.732r

4198.861r 4199.105m

4199.278

128

11

15

183

12

30. 5

2. 9

3. 6

43. 6

3. 3

u

u

CHFei

Ce II?- CN

Fe I Yii

R 18

3. 42

0. 52 P 56

3. 05

0. 10

0,0 693

3

0,1

522

5

4

11

4203.692r

4203.773

4203.942r

4204.004r

4204.200

1

2. 5

1 123

1

26

0. 2

0. 6

J 14. 7

1 19. 5

6. 2

u

J u

Fe I p CNJFei

IFei

Vii

Cr I

4. 58 R 5

16. Z/

13. 63

2. 84

1. 70

2. 54

1245

0,1

850

355

25

35

11

4199.372 22 5. 2 Fe I p 2. 95 416 4204.344 5 1. 2 CN P 50 0,1 11

4199. 524r 3. 5 0. 8 Fei 4204.461 13 3. 1 u Cri 3. 98 272

4l99.673r 5 1. 2 CN P 55 0,1 11 4204.602r 1 0. 2 CN R4 0,1 11

4199.743r

4199.888

4. 5

45

1. 1

11. 7 u

CN

-Ru I

P 55

0. 81

0,1

8

11 4204.725r

4204.753 1 82

1

10. 5

1 16. 4

ut Yii

CH

0. 00 R 171

0,0 4

4199.990 79 18. 8 s,N Fei 0. 09 3 4204.895r 4 1. 0

4200.101

4200.292r

4200.454

4200.601

4200.700

17

0. 5

38

56

23

4. 0

0. 1

9. 0

13. 3

7. 1

w

w

Fe I p

Ni I CH

CH

3. 88

3. 31 R 18 R 18

993

89

0,0

0,0

4

4

4205. 027r

4205.072

4205.262r 4205.390m

J

2. 5

41

r 9. 5

[ 12. 8

0. 6

9. 8

u,N

u,N

w,N

Eu II (Viip)

Vii

Mn II CH

0. 00

1. 69

2. 04

1. 81 R 20

1 25

37

2

1,1 4

4200.780 51 12. 1 u Ti I Fe I p

2. 25 L 61 220

44

4205.544m 89 21. 2 s Fei

(CH)

3. 42 R 20 689

1,1 4 4200.932m 96 22. 8 u Fe I 3. 40 689 4205.735r 4 1. 0 4201.068 16 3. 8 u Ca I 2. 93 4205.886 5 1. 2 CN P 48 0,1 11

4201.240 9. 5 2.3 4205.963 3. 5 0. 8 CN P 48 0,1 11

4201.327r 6 1. 4 4206.130r 4. 5 1. 1 Sm II? 0. 38 38

4201. 426r 5. 5 1. 3 Zr I? 0. 62 45 4206.297 18 4. 3 s 4201.577 30 7. 4 w -CH R 21 1,1 4 4206.423 6. 5 1. 5 4201.715

4202.040m

65

326

17. 1

77. 6

w

3

|Nii Fe I Fe I4. 09

3. 57

1. 48

238

799

42

4206.578 4206.702m44

122

10. 5

30. 0

u

s

CH

|Fei

CH

R 17

0. 05 R 17

0,0

3

0,0

4,16

4 4202.348 63 16. 4 u Vii 1. 70 25 4206.897 13 3. 1 u Cn 4. 62

4202.502 20 5. 0 CN P 52 0,1 11 4206.950r 2. 5 0. 6

4202.591 11 2. 9 CN P 52 0,1 11 4207.13.3m 84 20. 0 u Fei 2. 83 352

4202.759

4202.940

58

17

13. 8

4. 0

u

u,N

Fei

CN?

Ce II

/3. 02

13. 05 R 6

0. 56

476a

521

0,1 186

11

4207.251

4207.408

4207.628

2. 5

59

2. 5

0. 6

14. 0

0. 6

w,N

Mn II CH

Co I?

1. 83 R 19

2. 70

2

1,1 4

4203.129

4203.305r

4203.461

4203.574

40

0. 5

13

53

9. 5

0. 1

3. 1

12. 6

s,d

s

s

CaiCH

Fei

Til Fe ICri

2. 93 R 20

3. 02

2. 25 L 01

2. 54

1,1

418

220

1935

4,17 4207.820 4207 qiSl r

4208.104

4208. 174r

4208.256r

21

J., ij

4. 5

4

6. 5

5. 0

0. 4

1. 1

1. 0

1. 5

w

CN

CN

P 45 P45

0,1

0,1

11

11

140
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4208.351

4208.452

16

8. 5

3. 8

2. 0

11 Cr I 3. 85 249 4213.160

4213.272

15

4. 5

3. 6

1. 1

s,d? CN —

|Cri

CN

P 36

3. 08 P9

0,1 155

0,1

11, 17

11 4208.608S 98 23. 3 s Fei /3 40

13; 40 689

696 4213.422 6. 5 1. 5 Feip 2. 73 274

4208.784 9. 5 2. 3 CN P 44 0,1 11 4213.518 10 2. 4 CN P 35 0,1 11

4208.856r 4 1. 0 CN P 44 0,1 11 4213.653m 90 21. 4 u Fei 2. 84 355

4208.985 46 10. 9 u Zr II 0 71 41 4213.839 17 4. 7 u CH R 18 1,1 4

4209.184 4. 5 1. 1 u,N 4213.909 45 10. 7 CH R 18 1,1 4

4209.363 29 6. 9 s Cri 3. 85 248 4214.039 7 1. 7 0 Ce II? 0. 61 203

4209.500 27 6. 4 CH R 19 1 1 4 4214.136r 1. 5 Cr I? 2. 54

4209.602

4209.754

30

15

7. 1

4. 3

u

u

CH

Cn

Vii

R 19

3. 10

1. 67

1 1

155

25

4 4214.246

4214.363

6. 5

11 2. 6

CN

CN

CN

P 33 P 33 P 12

0,1

0^1

0,1

11

11

11

4209.826 64 15. 2 s Vi 0. 30 24 4214.475 9 2. 1 u Fe I p

2.47 152

4210.065r

4210.335r

4210.402r

4210.503r

4210.618

23

1 183

8

13

5. 5

r 28. 7

1 21. 8

2. 0

3. 1

w

s

CNCN7

Fe I Fe I p

CN

P42

P 42

2. 48

3. 07

P 41

0,1

0,1

152

482

0,1

11

11

11

4214.628r

4214.834 4214 91 5r

4215 057

4ZiO.I /I o 1 r 1 7n< u

17

21

8. 5

27

1 Q

4. 0

5. 0

2 1

6. 4

4. O

-CN

CN

CN

AT

P 13 P31

P 14

/P 15 IP 30

0,1

0,1

0 1

0,1

0,1

11

11

11

Ui

4210.701r 5. 6 1. 3 CN P 41 0,1 11 4215.297 16 4. 0 CN P 29 0,1 11

4210.967 100 23. 7 CH R 16 0,0 4 4215.423 91 45. 1 u Fe I /2. 76

12. 99 274

419

4211. 191r

4211.349

4211.512

4211 634

4211.740

4211.895

7

20

3. 5

3

19

65

1. 7

4.1

0. 8

0. 7

4. 5

15. 4

s,d

su

CNCri

Cr I

Til

IZr II- CH

P 40

/3. 01

13. 09

2. 98

2. 49

0. 53 R 18

0,1

133

106

279

15

1,1

11

4

4215.539

4215.764r

4215. 811r 4215.976m

4216.191m

4216.354

233

1 56

91

130

27

55. 3

f 11. 4

[ 2. 8

21. 6

30. 8

7. 4

s

u

s

s?

Sr II Cr II- CN

CN

Fei

Fei

Cr I

0. 00

3. 10 P 26 P 26

2. 69

0. 00

3. 01

1

18

0,1

0,1 273

3

132

11

11

4212.044

4212.13 a

4212.225

8. 5

2. 5

10

2. 0

0. 6

2. 4

u Ru I Fg I p

CNCN

0. 81

3. 42

P 38 P38

6 697

0,1

0,1 11

11

4216.599

4216.806r

4216.901r

4217.061

49

0. 5

0. 5

10

11. 6

0. 1

0. 1

2. 4

u,N

u

CH

Cr II

R 17

3. 10

1,1

18

4, 16

4212.398 4212 642

4212.850

5. 5

93

7

1. 3

22. 1

1. 7

u,N

CN

CH —

CH

(Cr I) NiiCN

P 7 R 16 R 16

O. Ui

3. 85 P 8

0,1

0,0

oio

0,1

11

4 16 4

11

4217.214 4217 268

4217.757r

1 102

J

4. 5

[ 14. 0

I 14.

0

oU. o

1.

SI

CH

CH

-T e I (Cri)

Ni

R 15 R 15

o. 4o

3. 01

3. 54

0,0

0,0

oy o 132

136

4

4

4212.971 4 0. 9 Pdi 1. 45 7 4217.878r 2.5 0. 6

141
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

bolar

Identi- ncation

Low

XT' TD hit: or Kot. Line

RMT "NT ^ JNo. or

V lb. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

oolar

Identification

Low

or Rot. Line

RMT

JN 0. or

Vib. Band

Notes

4218.047 8. 5 2. 0 u 4223.345 15 3. 6 u

4218.224 44 10. 4 u Fe I p 2. 43 172 4223.486 57 13. 5 CH r:i4 0,0 4

4218.392

4218.565r

4218.725

4218.920r

4219.016r

4219.199

53

1

78

3

1. 6

42

12. 6

0. 2

18. 5

0. 7

0. 4

10. 0

u,N

u

CHCH

/"ITT

Feii

R 17 R 17

K 15

1>1

1,1

0,0

44

4

4223.574

4223.731

4223.900r

4223.978r 4224.178m

4224.300

67

34

11

7. 5

135

32

15. 9

8. 3

2. 6

1. 8

32. 9

9. 5

s

uu

CH

Fei

Fe I

Zr II Fe I p

R;14

2. 95

3. 37

0. 76

4. 28

0,0

417

689

29 1104

4

4219.355r

4219. 4iyr

4219. 595r

4219.727

4219.903r

[ 146

J

10

7

5. 5

1 23. 5

-1 T O

[ 17. 3

2. 4

1. 7

1. 3

}»J

Fei

Fe I p Fe I p Fe I p

3. 57

2. 99

3. 55

3. 65

800

419

763

832

4224.459r

4224.632r

4224.860

114

1

11

91

1 5.7

[ 23.

9

2. 8

22. 7

s l|Fe I Cr 1 Fe I p

CH

Cr II

o. 43

3. 09

2. 76 R 19

5. 33

689

155

274

0,0 162

4

4220.051

4220. 169r 4220 347S

48

4. 5

87

11. 4

1. 1

20. 6

u Vii

|r e I

Fe I

1. 67

3. 93

3. 07

25 994

482

4225.046r

4225.215

4225.330r

3

32

8

0. 8

8. 8

2. 4

u

Ni I p

Vii

Sm II Pr II

3. 83

2. 03

0. 19

0. 00

169

37

22

co

,4 00 A /*0 0_ 4220. 482r 2 0. 5 Cr i."^ 2. 97 106 4^Z0.40im 120 32. 9 s Fe I 3. 42 693

4220. 57d 5. 5 1. 3 J

\ w,d

J

Mn I 4. 19 iZZO. 1 ID 52 15. 8 s Fe I p — 4. 22 1102

4220.644 11 2. 6 [bm II

fO. 18

10. 54

1550 4zzo.oiir 0. 5 0. 1 Fe I p 2. 42 118

4220. oOor 4 0. 9 izzo.yozm 74 25. 1 s 1 e I O. 05 521

4221. Olyr 0. 5 0. 1 3 1. 4

4221.170 4. 5 1. 1 4226.222r 2 1. 2 4221.304 9 2. 1 u 16 4226.349 6. 5 7. 1

4221.469 54 12. 8 CH R 16 1,1 4 4226.431m 71 52. 5 u Fei 2. 84 352

4221.572

4221.692

4221. 815r

4221.95 a 4222.221m

,4000 — 4222.451r

yl OOO CO ^ 4222.52 a

A ooo o r\o 4222.602

14

9. 5

3

7. 5

180

10

4

22

3. 6

2. 3

0. 7

1. 8

42. 6

2. 4

0. 9

5. 2

u

u

s

u

Cri

Ni I

Fe I

Le II

/3. 08

13. 85

3. 31

2. 45

0. 12

155 248

86

152

36

4226.568 4226.740m

4226.970r

4227.157r

4227.321 4227.440m

4227.660

4227.756

18

1476

45

9

44

185

12

35

53. 2

342

55. 8

9. 2

28. P

60. 8

4. 5

11. 1

s

u,N

u

u

Gei

Cai

Fe II p

Fei

Til

Ce II

1 rj |Zr I

2. 03

0. 00

2. 89

3. 33

2. 49

0. 70

0. 73

4

2

45

693

278

8 45

4222.728 21 5. 0 u Cn 3. 01 132 4227.944m 54 15. 6 s CH R 15 1,1 4, 16

4222.898 12 2. 8 u 4228.106r 3. 5 1. 1

4223.091 66 15. 6 CH R 16 1,1 4 4228.19 a 2 0. 6 4223.236 22 5. 2 s Fei 4228.312 11 2. 8 C I 7. 68 17

142
The Solar Spectrum—Continued

length

(A)

Equi-

\TfA 1 ATI t Width

A\

(mi)

Rer1 1 1 pprl Width

AX/\

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes length

(A)

EquiVillon, fc Width

AX

(mi)

Recluccd Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Banc

Notes

n A 4233 fi12S 298 70. 4 Fp t 2. 48 152 790 94. v). 1 u Fp 1 O. O i 4234.010 13 3. 3 s IIVi JO 04

11.' 94

g

111 4228.874r 1. 5 0. 4 Co I 0. 00 1

4229. 048r 5. 5 1. 3 4234.224 7 1. 8 u Vn 1. 69 24 422Q 2fi1r KO 1 9 4234 407 2 0. 6 n

4229.408m

4229.520m

28

81

7. 1

19. 4

Fei

Fei (2. 95

13. 27 416649

4234.547 18 4. 2 8 IV I Vii

(Cri)

0. 00

3. 76

3. 12

6 200

178 Nil 3. 85 4234.737r 1. 5 0. 4 4229.774m

4229.914

4230. 109r

4230.254

4230. 402r

4230.481

4230.575

115

67

7

19

2. 5

16

29

27. 2

16. 3

1. 7

4

0. 6

4. 0

6. 8

s

u

uu

u

Fei

(CH)

CH

— Cr I? Ni I p

Cr I Fei

1. 48

R 13 R 13

2. 98

3. 80

3. 01

3. 02

41

0,0

0,0

106

150

132

478

4

4

16

4234.896r

4234.997r 4235.144m

4235.291m

4235.521r

4235.641

4235.736

1

1

64

91

3

9, 5

20

0. 2

0. 2

15. 3

23. 4

0. 7

2. 6

7. 6

S

S

uw?

Mn I Mn I Ni I? Fe I p Yii

(Vi)

2. 92

2. 89

4. 15

2. 56

0. 13

1. 94

23

23

256

215

5

111

4230.703r 1 0. 2 4235.836r 16 15. 1 Fe I p 2. 40 172

4230.827r 4231.026m

4231.202r

4231.415r 4231 fiOQr

0. 5

95

3

1

76

0. 1

22. 4

0. 7

0. 2

r 9 7

u

u,N

Ni I (CH)

Vn

CH —

Zr II

3. 54 R 13

1. 70

R 14

1. 76

136

0,0 25

1 I 99

4

4, 16

4235.949m

4236.122m

4236.263m

4236.380

4236.556r

385

37

86

24

5

90. 9

12. 0

23. 8

6. 4

1. 2

S

uu,N

Fe I (Cri)

(Yi)

CH

CH

Ni I

Zr II2. 42

3. 01

0. 07

R 12 R 12

4. 10 L 76

152

132

5

0,0

0,0 237

110

4

4

4231.688r

4231.839r 2

I 9. 7

0. 5

u,N CHFeiR 14 1,1 4, 16 4236.643r

4236.78 m

1

1 68

0. 2

f 7. 6 u,N

Fe I p

lIFei Sm II

3. 64

.3. 63

0. 66

907

906

53 4231.954m|

4232 043r 4232 2f)4

4232 384

4232.462

45

6

12

16

8. 5

10. 6

1. 4

2. 8

3. 8

2. 1

u

u

s

s

V II — Cr I Nd II —

Vi

3. 97

4. 21

0. 06

1. 95

225

294

8

111

4236.806

4236.958

4237.083

4237.182 ,

32

40

[ 161

[ 12. 0

7. 8

17. 9

[ 28. 8

u

u

u

u

CH

Vii

CH

Fe I Fe I CH

R 13 L 69 R 13

0. 96

R 12

1,118

1,1

19

0,0

4, 16

4, 16

4

4232.602 3. 5 0. 8 4237.254r 1 [ 14. 2 si CH R 12 0,0 4 4232.734m 58 13. 9 s Fe I 0. 11 3 4237.55 a 3. 5 0. 8 s 16

4232.855r 5. 5 1. 4 Cri /3. 01

13. 09

132

155 4237.677 25 5. 9 w,N Fei

(Cri)

3. 02

3. 01 418

132

4232.927

4233.169m

4233.250

62

1 139

15. 1

r 31. 4

1 2. 1

tl

w?

CHV I Fe II Cr II

R 14

1. 95

2. 58

3. 86

1,1 111

27

31

4 4237.790

4237.891

4238.029m

4

16

111

0. 9

4. 0

26. 2

s

s

s

Til

Til

Fe I

2. 30

2. 50

/3. 42

\3. 42

252

284

689

696

4233.406r 3. 5 1. 1 4238.240 17 4. 0 u

143
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

42oo.oy5ni

4238.621

4238.757 4238.816m

A 1 41

18

1 155

y. /

4. 2

f 5. 2

I 34. 9

u,ai

s

u

La II Fe I p—

Fei

T? on It zu

0. 40

3. 63

3. 40

2,2 41

849

693

A4

aoao onn»* '3:iS4z.yuur

4243.203

4243.365

0

1i

55

151

1 0 1. 2 A 0 U. 2

14. 8

35. 6 u

V II

CHCHFei

6. to

R 12 R 11

3. 64

200

1,1

0,0 906

4

4

4238.944 29 9. 7 s,N Cn 3. 01 131 4243.454 39 16. 3 u? CH R 11 0,0 4

4239.044r

4239.145r

4239.23 a

4239.367

4239.485

4239.599

4239.733

14

10

1. 5

66

8. 5

11

78

3. 8

2. 4

0. 4

15. 6

2. 1

2. 6

19. 8

u

u

uu

Fe I p CH

Fei

CH

CH

Mn I —

Fe I

2. 76 R22

3. 64 R 21 R 21

2. 94

2. yo

274

2,2

907

2,2

2,2

23 4IO

4

4, 16

4, 16

4243.547m

4243.819m

4243.993r

4244.085r

4244.244

AO A A Q Ad 4Z44.04U

AOA A ACi'i 4Z4:4.4UO

4244.558r

56

63

9. 5

6. 5

9

1 *3 16

1 A 14

1

13. 7

14. 8

2. 2

1. 5

2. 1

0 1 0. 1

0. 2

w?w

w?

u

11

Fei

Fei

V^xl —

Fei

Fe II p

3. 69

3. 88

T> 1 0 R la

"D 1 Q

2. 34

994

2,2

2,2

12

4, Id

A If; 4, lb

4239.848m 132 31. 1 s Fei

/"A OA ju. yo

12. 69

1 010 273 4244.741 3 0. 7 Sm II 0. 28 27

4239.953 39 16. 5 u Fei 3. 07 476a 4244.812r 8. 6 2. 0 u,N? Ni II 4. 03 9

4240.087r 1. 5 0. 4 Vi? 1. 94 111 4244.945r 1 0. 2

4240.199 20 4. 7 w? CH R 19 2 2 4 4245.082 28 6. 6 w,N CH- R 17 2,2 4

4240.380 101 23. 8 u Fei 3. 55 764 4245.264m 118 28. 5 u Fei 2. 86 352

4240.455 58 23. 1 s Cai 2. 71 38 4245.359 77 18. 1 u Fei 3. 33 691

4240.610 9 2. 2 CH R20 2,2 4 4245.512r

j

9. 5

f

s Til

4240.702m 60 14. 1 u Cri (2. 98

13. 09

105 178

4245.613r i 0. 5

4240. oUUr

4240. y.i a

4241.12.3b

A(^ A t OOO 4241.328

8. 5 o

2

50

5

2. i

U. 0

11 o

11. o

1 o 1. 2

w?

u

r e I

\ Uxi

Vi?

2. 06 R 25

1. 95

OKI o51

0 0 Z,Z 111

17

A4

4245.810r

4245.912r

4246.021

4246.089

4246.256r

3. 5

10

23

95

3. 5

0. 8

2. 4

8. 9

22. 4

0. 8

u

u

Fe I p

Fei

3. 27

3. 64

649

906

4241.521 12 2. 8 s,d CH- R 25 2,2 4, 16 4246.418r 3. 5 0. 8 Cr II- 3. 85 31

Ad A t ^AZ? 4241.706 6 s,a U. DO 45 1 T17 Af^ A C C ^A», 4240. o/Ur 6. 0 A Q

(J. 0 J e I 6. 4o AQA boy

4241. 843r 2. 5 0. 6 4246.837S 171 40. 3 w? So II 0. 31 7

A Ct A AAO 4242. 008r A C 0. 5A<~t A'7 1 1 A 4247.1 14 1 c 16 0. 0 W,iV

4242.162 45 1 A C10. o Tm 11 —

|CH

A AO

U. 06 R 12

r0

1,1 4

A<^ A'^ 01 C*« 424/.c515m DO 0,1 0 24. 2 u r e I p Fe I p

0 A K 40

3. 63

1 *70 1/2

905

4242.283r

4242.379

)

\ 160

r 5.

2

1 21. 2 \w,N

J -CH

Cr 11

R 12

3. 87

1,1

31

4 4247.432m

4247.560

162

61

38. 1

18. 1

uw,N

Fe I CH3. 37 R 11

693

1,1 4

4242.455r i 20. 0 CH R 11 0,0 4 4247.726 49 11. 5 CH R 11 1,1 4

4242.604m

4242.734m

87

61

20. 5

15. 1

u

u

FeiCH

Fei

2. 73 R 11

3. 30

273

0,0 649

4

4247.899r

4248.055

2. 5

31

0. 6

7. 3 w?,N CH R 16 2,2 4, 17

144
The Solar Spectrum—Continued

Wavelength

Equivalent Width

A\

Cm X)

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

E P

or Rot. Line

RUT.

No.

or

Vib. Banc

Note

1

4248.231m 97 22. 8 u Fe I 3. 07 482

4248.320 22 7. 3 0 (Cri) 3. 01 131 4248.414m 65 15. 3 s IFe I p CH

1. 01 R 11 19

1,1 4

4248.534 38 9. 4 w CH R 11 1,1 4 4248.726m 81 19. 1 CH

(Cri)

R 10

2. 98

0,0 105

4

4248.944m 70 16. 5 CH R 10 0,0 4

4249.114 10 2. 4 s Til 2. 30 252

4249.258r 2. 5 0. 6

4249.347 7 1. 6 Fe I p 2. 42 117 4249.494m 60 14. 6 CH R 10 0,0 4 4249.637m 91 23. 0 u,d -CH R 10 0,0 4, 17

4249.802r 4 1. 2

4250.048r 4250.130m 1 342

f 4. 9

I 79. 5 u Fei 2. 47 152

4250.466 15 4. 9 u

4250. 706r 4250.797m

] 400

[ 14. 1

1 90. 6

u,N?

s

Mo II Fe I

3. 14

1. 56

3

42

4250.913 63 46. 1 u Fe I p 3. 07 478

4251.331 32 8. 2 s -CH R 15 2,2 4

4251.506 1. 5 0. 4 Fe II p 2. 34 12

4251.628 7. 5 1. 9 s Til 1. 88 162

4251.748 11 2. 8 u Gd ITii

0. 38

2. 30

15 251

4251.887 0. 5 0. 1 s Fe I p 2. 61 216

4252.055 18 4. 5 u,d? Nii- 3. 74 136

4252.232 6. 5 1. 5 w? Cn 3. 01 131

4252.306 32 7. 5 s Co I 0. 10 1

4252.461 8. 5 2. 0 u Nd II

4252.630 30 7. 3 u Cr II 3. 86 31 4252.756m 50 11. 8 u CH R 15 2,2 4 4253.004m 38 8. 9 CH R 10 1,1 4 4253.210m 40 9. 4 s CH R 10 1,1 4, 17

4253.366 6. 5 1. 6 u Gd II Ce II

0. 56

0. 46

46

77

4253.532 9. 5 2. 4 u,d1 Fe I p

Fe I p

3. 33

4. 59 690

1245

4253.735 36 9. 2 CH R 10 1,1 4

Wavelength

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

E P

or

liot. Line

RMl

No.

or Vib. Banc

Notes

1

4253.912m 63 16. A s,d CHFei

R 10

3. 64

1,1 9054, 17

4254.G81r 2. t 0. 7 4254.346m 393 92. 4 S Cn

(V 11)

0. 00

1. 68

1 18

4254.666r 5. 5 1. 5

4254.846 12 3. 3 u CH R 14 2,2 4

4254.979 108 27. 0 u,d Fe ICH

/3. 02

13. 02 R9

419

477

0,0 4 4255.251m 69 16. 9 CH R9 0,0 4 4255.507m 51 12. 0 s Cri

Fei

3. 00

3. 02

105 416

4255.637m 68 16. 0 CH R9 0,0 4 4255.839m 83 19. 5 s CHFe I R9 0,0 4

4256.026 20 4. 7 s Ti I 2. 32 252

4256.136 19 5. 2 0 CH — R 14 2,2 4

4256.208 54 12. 7 u Fei 3. 42 690

4256.316 23 5. 4 u Fe I 2. 43 172

4256.420 9. 5 2. 3 u Sm II 0. 38 37

4256.605 16 3. 8 u -Cri /3. 01

13. 01

131 131

4256.812 33 7. 8 u Fe I 4. 26 1102

4257.140r 4. 5 1. 1

4257.360 7 1. 6 u Cr 1 3. 01 131

4257.507r 0. 5 0. 1

4257.661S 56 13. 2 s Mn 1 2. 95 23

4257.823r 3 0. 7

4257.925r 1. 5 0. 4

4258.049 22 5. 2 u Zr II 0. 56 15 4258.166m 61 14. 3 w,N Fe II 2. 70 28 4258.324m 82 19. 2 s Fe I 0. 09 3 4258.488 37 9. 4 u CHTi I R 9

2. 29

1,1 252

4

4258 619m 82 19. 2 u Fe I 2. 83 351 4258.731m 50 12. 9 w CH — R 9 1,1 4

4258.959m 50 IL 7 u Fei 3. 02 419

4.9 KQ HQ 8

4259.152r 23

Q 4

6. 3 u,N Cn-

"Rit, Qy

3. 01 131 4

4259.305 59 14. 3 s,d? Vi

Fe I (CH)

0. 02

2. 99 R9

6 416

1,1 4

145
The Solar Spectrum—^Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes

4259. 511r 1. 5 0. 4 s 16 4264.925 24 5. 6 w Zr II 1. 66 98

4259.57 a 1 0. 2 4265.084r 11 2. 6 Sm"ii? 0. 18 15

4259.764 32 8. 2 w? CH- R 13 2,2 4, 17 4265.266m 76 17. 8 s IIFe^i /3. 93

13. 96 993994

4260.004m 86 24. 4 s Fe I 3. 33 689 Ti'i 2. 29 252

4260.128 84 26. 3 u Fei 3. 07 476a 4265.431 16 3. 8 w

4260. 341r 12 8. 2 4265.542 20 4. 7 w CH- q:3i 0,0 4 4260.486m 595 139 S Fe I 2. 40 152 4265.679 25 5. 9 s Tii 1. 87 162

4260.622 14 13. 6 4265.925m 61 14. 3 s Mn I 2. 94 23 4260.733m

4260.828

4261.010 4261,223m

4261.343

4261.531

4261. 595r 4261.738m

4261.935

4261.978

4262.128

50

19

7. 5

64

28

68

12

66

1 107

23

20. 6

6. 6

2. 1

16. 0

7. 0

16. 4

3. 3

15. 7

1 14. 5

I 14. 5

5. 4

s,N

sw

s?

w,d1 w

s,d

Fe I p

Ti I Vii

CH

Cr I CH

Til

CH

Cr II CH

Cr I (Gd II)

2. 84

2. 30

Jl. 67 U. 70

R 8

2. 91 R 8

2. 30

R 8

3. 86 R 8

f2. 91

13. 11

0. 73

351

251

1824

0,0

96

0,0

252

0,0

31

0,0

84

17844

4

4, 16

4

4

4266.078r

4266.216

4266. 431r

4266.623

4266.742

4266.968S

4267. 135r

4287. 283r

4267.389

4267.588

4267.749

4267.827

4267.984

4

10

2

18

44

81

2

5

60

20

1 156

25

0. 9

2. 3

0. 5

4. 7

10. 3

19. 0

0. 5

1. 2

14. 1

4. 9

1 13. 1

1 26. 7

6. 1

s,N

s u,N

wl

u

s u,N

u

u

Til

CH

CH

Fei

CH

CH

CH

|Fei

CH

2. 30

Q 30 Q 30

2. 73

R 7 R 11 R 7

3. 11 R 7

252

0,0

0,0

273

0,0

2,2

0,0 482

0,0

4

4

4

4, 16

4

4

4262.346

4262.585

4262.710

4262.87 a 4263.142m

4263.429

4263.608

27

20

31

1

47

18

6. 5

37

6. 3

4. 7

7. 3

0. 2

11. 0

4. 2

1. 5

8. 7

w?w

s

u

-Cr I CH

CH

Ti I Cr I

CHCH

3. OS R 12 R 12

1. 89

3. 85

R 12 R 12

154

2,2

2,2

162 247

2,2 2,2

4

4

4

4

4268.112m

4268.294

4268.448

4268.628 4268.756m

4268.921

4269.034

4269.185

76

8. 5

5

23

69

15

15

4. 5

17. 8

2. 0

1. 2

5. 6

16. 2

3. 5

3. 5

1. 1

u

s

s

s

uu

CH

Co I Vi

Fe I (Cri)

-Til

Ci

fR 7 IQ 29

2. 54

1. 87

3. 30

3. 98

2. 29

7. 68

0,0

0,0

127

88

649

271

252

16

16

16

4263. 843r 9 2. 1 Vii 1. 69 24 4269.290 38 8. 9 w Cr II 3. 85 31

4263.980m

4264.217m

4264.281 4264.468m

4264.580

41

102

J

57

25

9. 6

1 22. 3 o o

t 2. 0

13. 4

6. 1

w

uu

su

CH

Fei

CH

R 8

3. 37

iX o R 8

1,1 692

1,1

4

A4

4, 16

4269.478m

4269.585

4269.740

4269.849

39

30

76

76

9. 1

7. 2

17. 8

17. 8

w

uuu

CHLa II CH

Fei

CHFe 1 p

R 7

1. 78 Q 28

R 7

3. 40

1,1 76

0,0

1,1 690

4

4

4

4264.741m 86 20. 2 u Fe I (CH)

3. 96 R 8 993

1,1 4 4269.966 16 3. 7

1

^ Cr I 3. 09 154

146
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4270.170m

4270.332

4270.489

63

13

19

15. 0

3. 3

4. 7

s,d

u

0?

|Tii

CH

Fe I p

2. 32 R 7

2. 59

251

1,1

215

4

17

4275.513r

4275.557

4275.661

10

63

1 79

2. 6

14. 7

r 10. 5

CH

Cr II CH

La II

R 9

3. 86 R6

0. 32

2,2

31

1,1 40

4

17

4

4270.724r 22 5. 6 Ce II- 0. 96 21 4275.713r [ 10. 5 Fei 2. 56 215

4270.957r ' 0.

4275.897r 2 0. 5

4271. 057r

4271.164m

- 240 < 6.1

. 52. 2 u

CHCri

Fe I

R 10

3. 10

2. 45

2,2 154

152

4 4275.997

4276.103

11

20

2. 6

4. 7

u Cr I CH

Fei

3. 88 R9240

2,2 4

4271.374 42 16. 2 u CH Q27 0,0 4 4276.274 19 4. 4 -CH R9 2,2 4

4271.460 21 10. 3 CH Q27 0,0 4 4276.434 19 s Til 1. 73 148

4271.560r

4271.638 1 20

{ 3. 3

s Vi

Fe I p

1. 86

2. 20

88

70

4276.532r

4276.680S

0. 5

57

0. 1

13. 3 u IIFei

f3. 27

13. 88 597976

4271.774m 756 177 S Fe I 1. 49 42 Til 2. 30 252

4271.949

4272.144r

28

5

18. 2

2. 1

u,N Fe I p CH2. 43 R^IO171

2,2 4 4276.826 4276.995m

7

42

1. 6

9. S s,d

Na I? ViCH

2. 10

1. 85 Q 26 88

0,0 4

4272.301 17 5. 4 w 4277.233m 37 8. 6 CH- Q 26 0,0 4

4272.436 4272.544m

4272.714r

10

39

1

2. 8

10. 5

0. 2

s

s,d

Til Fe I0. 83 44 4277.391

4277.535m

24

72

5. 6

16. 8

u

u,d

|Fei Zr u?

CHCH

2. 61

0. 80 Q 24 Q 24

214

40

0,0

0,0

4, 16 4

4272.888 32 8. 0 u,d? -Cri 2. 90 96 4277.680 14 3. 3 s Fei 2. 43 172

4273.118 2. 5 0. 6 4277.815r 2 0. 5 4273.332m 90 21. 5 u |Fe II Ti I (CH)

2. 70

2. 30 Q26

27

251

0,0 4

4277.907r

4278.000r

1

2

0. 2

0. 5 Fe I p 4. 26 1102

4273.485m

4273.682

58

32

14 3

7. 7 w

CH /R6

IQ 26

0,0 0,0 4278.155

4278.235

14

73

4. 9

17. 1

u

s

Fe n

Fei

Til

2. 69

3. 37

2. 58

32

691 291

4273.797 43 14. 0 CH R6 0,0 4 4278.442r 8. 5 2. 0 u,N

4273.891r

4273.942r

i 114

1

J 17. 3

1 14. 0

[ V d Fei

CH

3. 07 R6

478

0,0 4

4278.551r

4278.689

1. 5

11

0. 4

2. 6 u

Tb II? Mm 4. 72 4274.193m 65 15. 2 CH R6 0,0 4 4278.79 m S Til 2. 30 252 13

4274.391 19 4. 4 u -Til 2. 29 252 4278.853m 46 10. 8 u CH

(Vii)

Q25

4. 00

0,0

225

4, 16

4274.596m

4274.806m

69

196

16. 4

45. 8

s

S

Til

Cn

fO. 82

\1. 88

0. 00

44

162

1

4.97Q nfi7m

4279.227r 1. 5

9. 1

0. 4

CH

Mo II 3. 06

0 0

'3 4•±, 17±/

4274.959

4275. 108r

63

14

20. 1

3. 5

u,N CH

Cui?

R 6

4. 84

1 1 4 16 427Q 4Q0m 63 14. 7 Hi Fe I CH

3. 88

R 5 993

0,0 174

4275.258 49 15. 0 CH R 6 1,1 4 4279.720 93 21. 7 CH /R5

IQ 23

0,0 0,0 4275.386 104 24. 3 CH R 6 1,1 4 4279.874m 60 14. 7 W Fei 2. 86 351

147
The Solar Spectrum—Continued

yy civ c" length

(A)

Equi1 pn f. Width

A\

(.mA;

Re- Width

AX/X

\i)

Spot

Solar

Identification

Low

E P

or Rot.

LiiiG

RMT

No.

or Vib. Band

Notes

4280.037m 64 15. 0 w,d? CH

(Til)

R5

2. 32

0,0 252

4

4280.220m 70 16. 4 w CH

Fe I R 5 0,0 4, 16

2. 6

4280.403 61 14. 2 w Cri

CH

3. 85 R 5 247

1 1

J- 4

4280.494r 7. 5 2. 8

\ ' Gd n 0. 35 15

4280.542 57 13. 8 1 Fei 3. 24 598

24 7. 2 Fg I p CH

3. 02 R 5 416

1,1 4

rt^OKJ, i OOlli 13. 7 Sm II CH

0 48 Q 2446

0,0 4

4280.964m 49 11. 4 CH fQ 24 \R 5

0,0

X X }^J

T^^O i. t J-\J\J 111. 77 18. 0 |Mn I —

CH

2. 92 R 5 23

1,1 4

4281.257r 1. 5 0. 4

4281.376 20 S,N Til 0. 81 44

4281.598 4 0. 9 s Fe I p 2. 45 171

7aOX. f 1 111 s 1 o

4-95^1 rr^O 1.17^0r Oul 0. 6 Q79m 76 17. 7 CH 0 29 0 0 4

A9ft9 91 7r 1 9 9 s s |Zr I Zr II 2. 42 132

4282.412S 146 34. 1 s Fei 2. 18 71

4282.579r 14 3. 7

4282.708 32 8. 4 s Til 1. 87 162

4282.796 56 13. 1 w CH Q 23 0,0 4 4283.014m 133 31. 0 s Cai 1. 89 5

4283.258 6. 5 1. 5 AOQQ 41 1 7 J. c t1 2. 61 215

4283.752r 1 0. 2 Fei?

4283.904r 8. 5 2. 0 s Fe I p 0. 99 19

4284.071 32 7. 5 s ViIVTn T XVJ. 11 1

1. 85

9^. JO 88

9'^

4284.228 86 20. 1 w |CH

Ct tt Q 21

o. oo

0,0

0 1

1

4

4284.411 27 6. 3 u Fe I 2. 99 417

4284.533 8. 5 2. 0 u Nd II 0. 63 10 4284.686m 50 11. 7 u Nix

(Cri)

3. 19

2. 89

86

96 4284.837m 48 11. 2 CH Q 22 0,0 4

^Wavelength

(A)

Equivn 1 pn f

,

V tXlCll u Width

AX

(ml)

Rer\ T T p prl Width

AX/X

(F)

Spot

Solar

Identifi p C1 1" i rt

Low

E V

or

Ttni Line

RMT

IN O. or Vih V ID. Banc

Notes

^^Otj • V/ VOi. 1-1 7'i 17^ CH

Ti I O 991. 74

f)u,un 148

A.

4285.201 8. 5 2. 0 u,N Ni I p 3. 40 86

4285.371r 20 7. 9 CH R4 0,0 4

4285.450 120 28. 0 u Fei 3. 24 597

4285.538r 40 15. 4 CH R4 0,0 4

4285.680r 2 0. 5 4285.815m 59 13. 8 s Co IT?P 1 c T1 (CH)

0. 17

fi4 R4

1

1,1 4

4285.938r 5. 5 1. 8 CH R4 1,1 4

4286.015 119 27. 8 s Til 0. 83 44 4286 OQOr 16 o CH R 4 4

4286OW• 1Q6m A i7\Jlll O i 1 4 CH R 4 0,0 4

9 ^

4286.477m 114 26. 6 u,d Fe I CH2. 95 Q 20 414

0,0 4

4286.587r 31 11. 2 u,N CH R4 1,1 4, 16

4286.733 2. 5 0. 6

4286.884m 54 13. 8 u Fei

\ j

(2 4*^ 13. 42 O 91

172

691 4

4287 004

[ 101

f 19. 8 Fe I (La ii)

3. 94 L 95 976

75

4287.051r J [ 6. 5 u1 CH Q 21 0,0 4, 17

4287.240r 1. 5 0. 3 4287.412m 57 IS. 6 S Til 0. 84 44

4287. 582r 15 3. 5 s Fei 17

4287.718 4 0. 9 s Ti I p 0. 82 45

4287.884 90 21. 0 w Ti II 1. 08 20

4287.992 76 19. 4 u Nil 3. 83 178 4288.155m 64 14. 9 s Fe ITi I

2. 76

f n 89

11. 05

273

4^

79

4288.268r 5 1. 2 Fei?

1^1 9 9 8

4288.566r 3. 5 0. 8 4288.736m 75 17. 5 CH Q 19 0,0 4

4288.962m 74 17. 2 u |Fei

CH

2. 59 Q 20 214

0,0 4 4289.080m 73 17. 0 s Til

(CH)

0. 82 Q 2044

0,0 4

4289.210r 6 1. 5 Zr II? 1. 83 117 1

148
The Solar Spectrum—Continued

VV cl V Kj^ length

(1)

EquiA7n 1 pttI" V CbLKjlL \j Width

AX

(ml)

Re- Width

AX/X

(F)

Spot

Solar

Identifi pfi t.inn

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes length

(A)

Equivalent Width

AX

(mA)

Re- Width

AX/X

(F)

Spot

Solar

Identifi1-1 pfi K/CAi f.inn \jt\J Lk

Low

E P

or Rot. Line

RxMT

X^NoU. or

Vib. Band

Notes

4289.372m 131 30. 5 s Cai 1. 88 5 4293.802 37 8. 6 u

4289.540r 5 1. 5 4293.921r 3 0. 8 4289.729m 230 53. 6 S Cri 0. 00 1 4294.048r 36 24. 7 ul Fe I p — 2. 56 214 4289.922m 65 19. 1 u Fei

(Ce II)

3. 40

0. 33

691

111 4294.142 217 50. 5 s FeiTi II

1. 48

1. 08

4120

4290.057 20 4. 9 u CH R 6 2,2 4 4294.370 25 6. 3 u CH R 5 2,2 4, 16 4290.226m 117 27. 3 u Ti n L 16 41 4294.48 m 6. 5 1. 5 s 16 4290.384m

4290.573r

4290.709r

4290.880r

4290.956

4291.019r

62

6

2. 5

35

137

19

14. 4

1. 4

0. 6

18. 2

31. 9

10. 2

s

u

s

Fei

Fe I

Ti I (CH)

CH

2. 99

2. 83

0. 81 Q 18 Q 19

416

351

44

0,0

0,0

4

4

4294.623

4294.781m

49Q4 S.'iQr

4295.040

4295.226

31

62

6. 5

99

107

7. 2

14. 4

1. 6

23. 0

24. 9

u,d

u

Wi

CH

Sc II

CHCH

CHCH

0. 37 R 5

0. 61 R 5 Q 17 Q 17 Q 16 Q 16

6

2,2

15

9 9

0,0

0,0

0,0

0,0

4

4

4

4

44

4291.121

4291.220r

110

32

26. 1

14. 2

u

u

CH

CH

Til

/R3

IQ 19 R 3

fO. 84

\1. 74

0,0

0,0

0,0 45

147

4

4295.422r

4295.591r 4295.757m

5

0. 5

55

1. 2

0. 1

12. 8 s |TiiCri

0. 81

2. 71 44

64

4291.472S

4291.621r

4291.735

4291.839

4291.979r

49Q9 O'^'i

84

5. 5

8. 5

11

1

[ 77

J

19. 6

1. 3

2. 0

2. 6

f 6. 5

19 ^

s

s,dw

Fei

(Feip)

ViCriCH

CH

fO. 05 U. 56

2. 73

2. 14

3. 42 R ^ R 3

341 273

120

1 1 I) i 4

4

4295.887m

4296.075

4296.217

4296.392

4296.584

4296.683r

42

17

35

3. 5

105

84

9. 8

4. 0

8. 1

0. 8

24. 4

f 13.

3

u

s

w

\ .r s,N

Ni I Vi

(La ii) CH

Fe II (CH)

CH-

(Ca TT^

3. 84

2. 13

0. 77 R 2

2. 70

R 2 R 2

n 'i9

178

120

53

1,1

28

0,0

0,09

4

4

4

1 7

4.9Q9 1 9Q 95 99 1 ul CH —

Fe I R 3

(2. 18

1 9 70

91

4

49Qfi Q^ifi

J 110

7 n

9^ fi

J 7v TT Zjr 11

V_yXX

1 7fi n 1 fi

yo

4 4909 9Q4m 50 11. 6 u Fp t 9 90 701 yJ 49Q7 OA'^r 41 IS fi \jT I 9 71

4292.460r 4. 5 1. 0 4297.219 62 22. 3 CH Q 15 0,0 4

4292.583r 1. 5 0. 3 4297.291r 90 20. 9 CH Q 15 0,0 4

4292. 67 Ir 3. 5 0. 8 s Til 1. 05 79 4297.530m 75 17. 4 CH- R 2 1.1 4

4292.784r

4292.879r

4293.036r

4293.114

1

1

1

[ 136

J

0. 2

0. 2

f 15. 1

1 20. 5

Zn I CH

CH

4. 03 Q 18 /Q 17 IQ 18

3

0,0

0,0 0,0

4

\ 4

4297.751

4907 Q7Qr

49QS n^fi

4298.197m

55

1xO^

111 1 1 X

52

12. 8

7 4

9^^ 8

12. 1

s,N

su

u

llCri

V X f

r"TT1

i? e I Fe I p

3. 85

9 19xz P 9

o. uo

3. 11

247

1XZU90

0 0

^^90

476a 16

4293.330r 8 1. 9 s 16 4298.374r 4 0. 9

4293.556 14 S. 0 s,d7 Cri 2. 91 96 4298.516 15 3. 5 u Nil 3. 84 178

4293.661r 4. 5 1. 0 4298.676m 76 17. 7 s Til 0. 82 44

149
The Solar Spectrum—Continued

Wavelength

Equivalent Width

AX

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(m\mri./ A)

Re- duced

Width

AX/\

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4298.813m 96 22. 3 u CH Q 15 0,0 4 4303.595m 65 15. 1 s Ndn 0. 00 10 4298.994m 112 27. 2 s Cai 1. 89 5 4303.723 41 13. 2 w CH- Q 14 1,1 4

4299.138 48 24. 2 w? CH Q 14 0,0 4 4303.835 81 28. 6 u CH Q 12 0,0 4, 16

4299.249

4299.367r

4299.483

212

37

71

49. 3

19. 1

18. 1

u

u

iFei

Ti I (CH)

(Ce u)

CH

Fe I p

2. 42

1. 75 Q 14

0. 17 R 1

3. 25

152 148

0,0

47

1,1 648

4

4

4303.937

4304.141r 4304.256m

4304.395m

119

7. 5

63

68

27. 6

1. 7

14. 6

16. 0

w,N

w

— CH

Fei

CH

CH

JQ 12 IR 1

3. 30 Q 15 Q 11

0,0 0,0

647

1,1

0,0

1 A

4, 17

4 4299.645m 82 19. 1 s ||Ti I Fei

0. 83

3. 02 43 416

4304.571m 108 25. 1 w Fe I—

CH

2. 95 Q 11 414

0,0 4

4299.689r 22 7. 4 Cr I 2. 90 96 4304.721 35 9. 0 CH Q 13 1.1 4 4299.831m

4299. 977r

93

9

21. 6

3. 7

4304.852 56 13. 0 u,N CHFei

Q 13

/3. 30

13. 55

1,1 598

756

4

4300.053

4300.219

4300.318

166

37

87

38. 6

11. 9

20. 2

w

uw

Tin

Fei

CH

(Ce n)

1. 18

3. 88 R 1

0. 45

41

975

0,0 1344, 16

4305.110m

4305.217 4305.322m

82

34

52

19. 0

9. 3

13. 5

u

CH

Fei

Fei

CH

Q 14

2. 73

3. 55 Q 11

1,1 272

760

0,0

4

4 4300.573m

4300.744

126

33

29. 3

11. 8

s

u,N

||Ti 1-

CH

0. 83 Q 14 44

0,0 4 4305.456m 124 28. 8 u |Fei

Sr n

(Cri)

(CH)

3. 02

3. 04

2. 89 Q 11

476

3 96

0,0 4

4300.827 99 23. 0 u Fei 3. 98 976 4305.613r 20 5. 6

4301.000r 48 23. 7 u,N CH Q 13 0,0 4 4305.713m 67 15. 6 u Sc n 0. 60 15

4301.103

4301. 174r

4301.280

4301.501

4301.749

179

25

28

9

59

41. 6

18. 1

8. 6

2. 1

15. 1

s

u,m

w

Ti I (Vn)

CH-

|Cri

CHCH

0. 84

4. 02 Q 13

3. 45

Q 16 Q 16

44 225

0,0

1,1

1,1

4

44

4305.847r

4305.918

4306.145

4306.18 m

4306.360

4308.599

15

156

90

12

33

5. 8

36. 2

21. 1

2. 8

12. 5

S

Sw

u,N

CH

Til

(CH)

CH

Vi

Fei

Q 12

0. 85 Q 10 Q 10

0. 02

3. 43

1,1 44

0,0

0,0

5

691

4

4

4

13

4301.927m 128 29. 8 u Ti n 1. 16 41 4306.701 95 25, 1 CH Q 10 0,0 4

4302.080r 12 3. 0 u Nil 3. 48 102 4306.855 120 29. 2 CH Q 10 0,0 4

4302.199 48 21. 8 u Fei 3. 05 520 4306.91 m s Ti I 0. 81 43 13

4302.297

4302.539m

4302.65 a

4302.754

135

165

43

101

31. 4

38. 4

19. 5

24. 2

S

CH —

CH

Cai

CH

Q 13 Q 13

1. 90

Q 12

0,0

0,0

5

0,0

4

4

4

4307.058

4307.181 4307.311m

4307.564

3

4. 5

64

82

0. 8

1. 2

17. 2

28. 8

s

Fe I p Vi

CH

CH?-

CH

3. 37

0. 00

Q9

Q 10 Q9

690

5

0,0

1,1 0,0

4

4

4 4302.913m 79 19. 0 CH Q 12 0,0 4 4307.748 59 40. 2 s Cai 1. 89 5

4303.089r

4303.177

32

103

9. 3

23. 9

w?,N wCH

Fe II

R 1

2. 70

1,1

27

4 4307.912m 723 165 S |Fei

Ti n

(CH)

1. 56

1. 16 Q 9

42

41

0,0 4 4303.426m 72 16. 7 CH Q 16 1,1 4 4308.046r 6 7. 7

150
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib.

Jj cL 11

Q

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. P 0 n iJtXXXO.

Notes

4308.176m

4308.289r

29

31

16. 7

12. 8

CH Q9 0,0 4 4312.302m 70 18. 6 w?,d CHCa I

/Q5

IQ4

2. 93

0,0

0,0 }4, 17

4308.381r

4308.441r

'lOUo.0'1 III

46

35

1. 0

14. 2

11. 1

"i 7 0. ( c0

CH

CH

11 I

Q9

Q 10

I. u

/

1,1

1,1 7Q/ y

4

4

4312.504r

4312.564 1 99

1 4. 6

i 20. 9

u CH

Mn I —

CH

Q 3

2. 94 Q3

1,1

23

0,0

4

4

4308.595

4308.777r

98

3. 5

25. 1

0. 9

CHCH

Cr II?

Q8

Q 9

0,0

1,1 4

4

4312.709

4312.875m

34

153

8. 8

35. 5 w?

CH

|Ti II- CH

IQ2

1. 18 Q4

0,0

0,0

41

0,0

}^

4 4308.905m

4309.040

4309.131

43G9.205r

4309.383

4309.458

71

131

1 79

126

40

20. 4

31. 6

f 13. 2

1 13. 2

29. 9

21. 6

u

u

w

CH

Fei

CH

CH

|Fei

CH

CH

Fe I p

Q 8

3. 63 QS

Q9

2. 95 Q8

Q8

0. 11

0,0

849

0,0

1,1

4. 14

0,0

1,1

'±(0

4

4

4

4

4

4313.035m

4313.237

4313.418

TtOlO.DO ilu

4313.890

rtOlTc.Uc/ J.1II

72

6. 6

8. 5

o±

11

19. 5

1. 6

2. 0

J.O. 0

2. 6

9^; A

w,N

s

tc

|CH

Fe I p

CH

-Vi?

Sf> TI11

Q4

2. 76

r> ^.5 Q3

1. 85

yj. vzi

0,0 273

0,0

1 K

4

4rr4

4309.634

4309.711

93

45

21. 8

17. 2

u

w?

llYii CH

CH

0. 18 Q8

Q7

5

1,1

0,0

4

4

4314.221

4314.314

24

66

7. 9

15. 3

w

u

CH

iFe 11 Fe I?

Q2

2. 68

0,0

32

4

4309.834

4309.900 4310.106m

4310.225

4310.379r

4310.467

29

71

108

53

15

126

94.

9. 5

16. 5

25. 0

18. 3

5. 8

29. 2 Qy. 0 99 7

s,N

u,N

u

s

CH

Vi

CH

CH

CH

Fei

CH

1.^x1

Q7

0. 04

Q 8 Q7

Q7

3. 93 Q7

n 7

r> p.

1,15

1,1

0,0

1,1 994

0,0

1 1 1,1

u,u

4

4

4

4

4

A1, 171 /

4314.36 m

4314.512

4314.73.3r

4314.77 m

4314.807

4314.981 4315.098m

4315.285r

4315.458

19

1

82

82

153

5. 6

10

4. 4

f 3. 7

I 16. 2

28. 0

35. 4

1. 3

2. 3

S,Nw

S

su

u

Til

Nd IITi I p Til

Ti 11 Fei

0. 84

0. 00

0. 82

0. 84

1. 16

2. 20

45

9

43

43

41

71

13

13

15

4310.897 28 10. 0 CH IQ5

1,

1,1 4315.602 6. 5 1. 5 u

4310.984 104 24. 1 CH Q 6 0,0 4 4315.740r 3 0. 7 4311.167m 77 17. 9 CH Q 6 0,0 4 4315.877 4. 5 1. 0 La II? 0. 40 41

4311.322 17 5. 6 CH Q4 1,1 4 4315.951' 8 1. 9 u,N Fe I p 2. 43 171

4311.446 14 8. 8 CH Q 6 0,0 4 4316.083 11 2. 5 u,N Gd II?- 0. 66 43

4311.509 171 39. 6 CH Q 5 0,0 4 4316.559r 1. 5 0. 3 Fe I?

4311.63 m 18 6. 5 S Ti I 2. 15 205 4316.671r 3. 5 0. 8

4311.718 82 19. 0 CH Q5 0,0 4 4316.802m 38 10. 2 u Ti II 2. 05 94

4311.888 18 4. 4 u 4316.962 16 3. 7 w

4312.086r

4312.150r 1 141

j 23. 0

[ 14. 8

CH

CH

Q 5 Q4

0,0

0,0

4

4

4317.055

4317.15 a

11

2

2. 5

0. 5

w Fei 3. 55 762

15]
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4317.321

rtO ± 1 ,rtO 1 1

4317.719

4317.903r

4318.070

13

Qo

8. 6

1. 5

13

2. 8

n 7

2. 0

0. 3

3. 0

w,N

u

w

Zr IICr I

0. 71

4 21

40 4323.063

4323.226m

21

101

6. 5

23. 6

CH

CHCH

/Q 2,7

IQ 12

[Q 5, 6 <Q10to

iQ 13 JQ 4, 9 IQ 13

2,2

2,2

2,2

2,2

2,2

2,2

2,2 V

4318.207

4318.362

4318.470r

4318.659S

8. 5

13

4

116

2. 0

3. 0

0. 9

26. 8

u

u,d7

s |Cai

Til

1. 90

2. 25

5 235

4323.367

4323.512

4323. 611r

43

105

56

11. 1

24. 7

18. 7

u

u

u,N

|CH

Fe I p CHCH

/Q 3,8

IQ 14

2. 45

fQ 3to

Q9

IQ14

/Q6

IQ 10

2,2

2,2 171

2,2 2,2

2,2

2,2

2,2

}^

V

\ 4

J 4318.796

4318.936

4319.091r

18

10

2. 5

4. 9

2. 3

0. 6

u

u

Fe I p Sm II2. 59

0. 28

215

27

4323.711r 12

113

3. 7

2d. D

Nil

Cxi

3. 40

fQ 5 to Q9

Q 11

2,2

2,2

2,2 4319.294r 2. 5 0. 6 LQ 15 2,2 1 4319.452

4319.636

13

15

3. 0

3. 6

s?

.s?

Fei

Cn

2. 61

2. 89

214

96

4323.973 42 13. 2 CH

fQ4, 5 Q 10 IQ 15

2,2 2,2

2,2

4319.808r

4319.986

2. 5

6

0. 6

1, 4 u

4324.087 41 9. 9 CH [Q4 Qii

[Q 12

2,2

2,2

2,2 V

4320.143

4320.373

4320.500

6

17

24

1. 4

3. 9

5. 6

ww

s,d

Fe I p Fe I Fe I4. 39

3. 40

3. 42

1170

691

691 17

4324.176

4324.412m

38

73

9. 2

17. 8

CH

CH

CH

/Q3

IQ 12 Q 2 /Q 13 IQ 16

2,2

2,2

2,2

2,2 2,2

4

4320.593 7. 5 1. 7 u Cri r2. 90

12. 91 9696 4324.616 6 1. 5 s Nai 2. 10 4320.749m 94 21. 8 u Sc II 0, 61 15 4324.725r 7 2. 0 u

4320.958m 63 16. 4 w Ti II 1. 16 41 4324.819 39 9. 9 w -CH Q 14 2,2 4

4321. 133r

4321.232

5

8

1. 2

1. 9

u

s Cn 2. 87 S3

4324.998m 117 29. 4 u Fei11 Sc II (Cn)2. 20

0. 60

2. 97

70

15 104

4321.412 9. 5 2. 2 s Nai- 2. 10 4325.141 55 16. 6 s Til 2. 25 235

4321.517r 1. 5 0. 3 4325.356m 49 15. 5 u CH Q 15 2,2 4 4321.658m 26 6. 0 s Tii 2. 24 235 4325.487r 20 8. 6 u

oyj 1 ^. u u "Po T u Ni T O. O J. OU

4322.043

4322.212r

4322.358

9. 5

2. 5

4. 5

2. 2

0. 6

1. 0

u,N

u

Vii- 1. 68 17 4325.775m

4325.953

793

56

174

32. 4

s

u

Fe I (Feip)

Fe I p

1. 61

0. 00

3. 27

42

2

598

4322.505 12 2. 8 u La II 0. 17 25 4326.052r 23 13. 2 u,N CH /Q16

IQ18

2,2 2,2

4322 701 r 3 0. 7 TTo T T\ X' C 1 jj 2. 61 215 4326 222r 6. 5 2. 1

4322.828 6 1. 4 s 16 4326.357m 22 6. 2 s Til 0. 83 43

4323.013 66 15. 5 CH fQSto

IQ 11

2,2 2,2 4326.479r 0. 5 0. 1

4326.616 4 1. 0 Mn n? 5. 40 6

152
The Solar Spectrum—Continued

ll.qui- Re- Low PlMT Equi- Re- Low RMT

Wave- valent duced Solar EP No. Wave- valent duced Solar EP No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(A) (ml) (F) Line Band (A) (mA) (F) Line Band

4326.762m 56 14. 1 u lei 2. 95 413 4331. 782r 4. 5 1. 0

4326.917 34 8. 6 w Cll — Q 17 2,2 4

/< 0 0 A AAf 4332.006 5 1. 2 0/"ITT CH — T> A r 4 1,1 4

Oil Q 17 2,2 4 4332.169 4. 5 1. 0 CH P4 1,1 4 4326.97 m 7 2. 0 s Ti r 0. 81 43 4332.453 8 1. 8 w I'e I Id 4327.110m j' 18. 2 w Fe I 3. 55 761

\ 83 4332.583 29 6. / AT M,iV Cr I— 3. 12 176

4327. 157r J [ 2. 0 M? /~1TT CH /P3

IQ 19

1,1 2,2

I A

/-"-ITT CH Q 22 2,2 A4

4332.831 20 4. 8 S Vi 0. 02 5 4327.317r 5. 5 1. 4

/I 0 0 A A "1 0 4332.918 36 8. 3 w

T T CH — T> A P 4 1,1

A4

vl OOT A tin 4327.453 9 2. 2 u,N

4333.051 12 2. 8 w CH Q 21 2,2 4

4327.61 a £5 1. 3 Fe I p 4. 29 1135

4327.791 18 4. 2 u 4333.206 14 3. 2 w Ni I? CH? Q 21 2,2 4 4327.917m 69 16. 2 u Fe I 3. 30 597 (Zr II) 2. 41 132

4328.035 23 6. 2 CH Q 18 2,2 4 4333.365 6. 5 1. 5 u,N

4328.203r 8 2. 0 CH? P 3 1,1 4 4333.421 3 0. 7 u,N

i. 0

1 1

I. 1 4ooo. / ooixi 0 c 00 Q 00. 0 u La II U. i / OA

4328.439 5 . 1. 2 4333.898 19 4. 4 s

432o.ol0 0 A 34 8. 1 u CH Q 20 2,2 4, 16 4334.018 1 CH r 4

f\ A

0,0 A4 20 j 4328.845r 9 2. 1 u CH P 3 0,0 4 4334.067r I [ 2.

s,N

4328.927r 5. 5 1. 3 CH P3 0,0 4 4334.166 1 19

[ 2.

Sm II 0. 28 27 15

19

12 2. 8 u Sm II 0. 18 15 4334. 246r J [ 2.

/I oon 1/1/1 0 1. 2 CH P 3 0,0 4/I 0 0 /( £? '70 4334.672 1 G Id 6. 9 0 T T CH "D A A4

4o>i9.^oy 30 D. 9 u CH Q 19 2,2 4, 16 /J 0 0 /f 0 AA 4334.800 Id 0 A

3. 9 s CH — "D A C\ (\ U,U

A4

|Ti I A CO0. 62 4.5

y| O OA O A 1 4329.391 26 6. 0 u CH Q 19 2,2 4, 16 4334.938 13 3. 2

X? tO

Jb e I!^

/I oon COT 4329.537 7. 6 1. 7 u Fe I p 70 16

4335.087r 1. 5 A 0

0. 3 4329. D91r 03 A T

0. 7 4335.274 0

31 7. D u

/ 1 T T CH y 23 2,2 A 17 4, 17

4329. 9U2 9 2. 1 u

/4 0 0 1" /I r 0 4335.452 -1 013 0 0

3. 2 r e I p

0 A7 3. 0/ A

yl oor^ rvo 4 4330.024 0 c 35 5. 1 s V I 0. 00 5 4335. 602r 5

1 0

1. 3 4330. 24om 38 9. 7 w Ti II 2. 05 94

/< 0 0 r >'7 00 4335.783 51 0

1. 3 u re I

1 K

4<j30.4Uo f 5.CO3

\ M

CH Q 21 2,2 4

1 u,N 4335.913 6. 5 1. 6 u,jy T^re I 0 CQ 3. 00 A A 1 991

4330.451 I 5. 3 4335.987r 2 0. 5 4330.581r 2 0. 5 Gdii? 0. 52 46

4336.135r 0. 5 0. 1 Fei

4330.708m 64 14. 8 w |Ti II 1. 18 41 Nil 3. 80 149 4336.273r 2. 5 0. 6 Ce II 0. 70 89

4330.820 10 2. 5 u Fe I 3. 02 475 4336.442r 0. 5 0. 1 4330.956m 42 9. 7 u Fe I 3. 27 597 4336.614r 2. 5 0. 7 Fe I p 3. 88 990

4331.053 14 3. 5 w CH- Q 20 2,2 4 4336.791 8. 5 2. 3 u CH P 5 1,1 4, 16

4331.243 7 1. 6 Coi 3. 41 168 4336.873 18 4. 8 Fe I p 3. 42 692

4331.442 19 4. 4 w,N Fe I- 4337.055m 120 30. 4 u Fei 1. 56 41

4331.651S 56 is. 6 u Ni I 1. 68 52 4337.252 46 12. 2 u

153
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4337.411 18 4. 8 u CH P 5 1,1 4 4342.990r 6 1. 7 w? CH? P4 2,2 4 4337.566m

4337.792

4337.925S

4338.0S5r

4338. 132r 4338.271m

88

14

89

4

10

54

23. 3

3. 9

24. 0

1. 3

3. 0

15. 4

suw

u

Cri

Ce II

Ti II

Fei

0. 97

0. 33

1. OS

2. 18

22

82

20

70

4343.216

4343.268

4343.416r A^AQ Add

4343.705m

1 112

9. 5

71

r 15.

0

I 16. 0

3. 0

18. 6

u,d

u

u

|CriFe I p Fei

Fe I (CH)

2. 71

3. 25

3. 25.

r 0

3. 05 P 6

64 644

645

517

0,0 4

4338.445 26 7. 8 u,d -Ti I 2. 16 204 4343. 854r 3 0. 8 CHFe I p P 4

3. 55

2,2

7. 56

4

4338.627 10 3. 2 CH fP5

IQ 24

0,0 2,2 4343.968m 44 11. 5 u CH P 6 0,0 4

4338.694

4338.829

30

20

9. 2

6. 4

u

u,d

Nd II Fe II p

Cri

Fe I p

0. 74

2. 69

3. 37

2. 48

68

32

198

117

4344.145r 4344.290m

4344.511m

3. 5

75

98

0. 9

IS. 2

2It. 3

u

s

Ti II Cri

1. 08

1. 00

20

22

4339.010r 7 2. 3 u CH P 3 2,2 4 4344.669r 8 2. 1

4339.129 19 6. 4 w 4344.746 3. 5 0. 9 u Nai 2. 10

4339.259

4339.456m

4339.722m

4339.910r

4340.032r

4340.142 4340.475m

4340.848

4341.003

4341. 126r

4341.250 4341.371m

4341.551

4341.710

4341.826

4341.924

4342.059r

4342.180

23

82

69

3

1. 5

14

2855

2. 5

16

1. 6

6. 5

53

12

16

7. 5

14

3. 5

20

8. 1

25. 0

23. 8

1. 5

0. 9

10. 8

659

1. 8

7. 6

0. 7

3. 0

19. 6

4. 8

5. 8

2. 8

4. 8

1. 2

6. 4

u

s

s

s

s W,N

S

sw

w?

u,Nw

u

ul

u

u

Fei

(CH)

Cn

Cri

Ti I? Cn

H7

Vi

Zri Fe I

Ti II Fe I p CH

Fe I CH

Ru I? Gd n CH

P 5

0. 98

0. 96

2. 02

2. 71

10. 20

0. 04

1. 40

3. 40

1. 12

3. 27 P 6

3. 55 P 6

1. 14

0. 60 P 6

0,0

22

22

174

64

1

5

61

691

32

644

1,1

1,1

9

15

1,1

4

15

4, 16

4

4

4344.891

4345.084

4345. 2 l?m

4345.238r

4345.345r

4345.432r

4345.594

4345.772

4345.895

4346.116 4346.295m

4346.418r 4346.561m

4346.673 4346.831m

4346.904r

4347. 037r

4347. 104r 4347.242m

32

10

1

1. 5

1. 5

1

9. 5

8

23

10

49

3. 5

68

14

39

7

2. 5

1. 5

41

8. 0

2. 5

0. 2

0. 3

0. 3

0. 2

2. 3

2. 1

5. 8

2. 5

12. 0

0. 8

16. 6

3. 7

9. 4

1. 8

0. 6

0. 3

9. 6

u

u

s,N

u

uu

su

u

u

u

s

-Fei?

Cr I

CH

Til

CH

Fei

CH

Cn

V II

Fe I

3. 37

P7

2. 24 P7

3. 30

P 7

2. 98

1. 67

0. 00

198

1,1

234

1,1

598

1,1

104

17

2

4

4

4

4342.305 14 4. 8 u,N 4347.370r 3. 5 0. 8 -CH Q 26 2,2 4

4342.47 a 1. 5 0. 5 4347.545m 37 9. 0 CH P 7 0,0 4

4342.590r 1. 5 0. 5 4347. 683r 3 0. 7

4342.840 1. 5 0. 5 s Vi 1. 87 103 4347.841m 65 15. 4 w1 Fe I (Sm II)

3. 60

0. 38 82837

154
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent W Id til AX

(mA)

Re- duced w icitn AX/X

(F)

opot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib.

Jiancl

Notes Wavelength

(A)

E(|iii- valent W icltn AX (mA)Reekie ed Wi(Un

AX/X

(F)

Spot

Solar

Idcii ti- fication

Low

EP

or Rot. Line

RMT

No.

or

Vib.

rJaiiu

Notes

4347.973m 55 13. 1 CH P 7 0,0 4 4353.843 10 2. 3 Co I? .3. 97

4348. 104r 11 2. 5 CH P 5 2,2 4 4353.948 24 5. 5 u Cr I 3. 37 198

4348.187r 2. 5 0. 6 4354.067r 8 1. 8 s Ti I 2. 16 204 4348.338m 50 12. 0 CH P 7 0,0 4 4354.266 32 7. 3 u,N Fe I p 3. 88 975

4348.492

4348.636

9. 5

7. 5

2. 3

1. 7

U

U

CH

CH

P 5 P 5

2,2

2,2

4

4

4354.436r

4354.514

13

34

3. 4

8. 3

La 11 Mgi

0. 92 4 34

58

13

4348.77 Ir 1. 5 0. 3 Yi? 2. 01 16 43.54.615m 70 16. 1 u So II 0. 61 14

4348.947S

4349. 168r

4349.376r

4349.799

58

3. 5

3

7. 5

13. S

0. 8

0. 7

1.4

U

U

Fei

'

Ce 11

2. 99

0. 70

414

59

4354.762

AO r A r\ei_ 4354. 951r 435o.0yom

25

zl

5. 7

5. 6

ZD. U

s,a!

s

CH

r e II — V I

*^a I (CH)

P 9

1 on

O 71/ 1 P 9

1,1

1 f\0

•i 1 1,1

4

ID

4

4349.958 4. 5 1. 0 4355.351

\ A O

f 8. 0 u CH P 9 1,1 4

4350.156 14 3. 4 u 4355.417r 1 48

1 3. 2 u,N

4o6U.z4y OOza C A 0. 4 u

"D O r 8 1,1 A4 4355.589 10 2. 3 u Jo

AO Cf\ O OO 4o5U.ooo Iz 2. 8

A. .9 Wl 4355.704 A O 48 11. 0 D O 1 V) r\ f\ U,U A

4o5U.5oo OO o o u Fe I —

CH P8 1,1 4 4355.902 O / 11. 5 s JNl I V I

O P.O

0. 02 5

4350.760r 15 3. 9 CH P 8 1,1 4 4356.000 73 16. 8 CH P 9 0,0 4 4350.840m 61 14. 0 u,d Ti II 2. 06 94 4356.136 14 3. 4 u 4351.056m 90 SO. 0 s Cr I 0. 97 22 4356.253r 8 2. 0

4351. 177r 6 1. 4 4356.367 55 12. 6 CH P 9 0,0 4

4351.303 14 3. 4 Ndii 0. 18 10 4356.604 54 12. 4 CH P 9 0,0 4

4351.392 16 3. 7 Fe I p 3. 42 691 4356.743 20 4. 6 s Cri 3. 01 130 4351.554m 72 18. 6 u Fe I 2. 99 413 4356.910 19 4. 4 u 16

4351.710r 4351.767m

4351.921m

4352.072

4352.261

4352.391

4352.557 4352.743m

4352.880

4353. 053r

4353.172

4353.435

4353. 517r

4353.644

1 133

283

38

49

26

52

142

67

11

30

9. 5

27

16

1

0. 5

1 43. 2

65. 0

16. 8

12. 2

6. 2

12. 2

32. 6

21. 1

2. 5

6. 9

2. 3

6. 2

3. 7

s

w

sS

0? u,N

CH

|Cri Fe 11 Mgi

CH

CH

CH

Fei

V I CH

-CH

CH

P 8

1. 03

2. 70

4. 34 P 8 P 8

P 8

2. 22

0. 07 P 6 P 6 P 6

0,0

22

27

14

0,0

0,0

0,0

71

5

2,2

2,2

2,2

4

4

4

4

4

4

4, 16

4357.063r

4357.152r

4357.297

4357.514

4357.705r

4357.869

4358.014

4358.170

4358.361r 4358.512m

4358.718

4358.820

4358.916

2. 5

4

16

38

4

24

18

38

4

95

75

53

25

0. 6

0. 9

3. 7

8. 7

0. 9

5. 5

4. 4

8. 7

0. 9

21. 8

17. 2

15. 6

8. 0

u

u,d

u

u

s

u

u,d?

u,N

Co I?

Cri

Fe I p

CH

Nd n

Fei

Y II -CH

Fe I p

4. 05

3. 37

/3. 96

14. 43

P 7

0. 32

2. 95

0. 10 P 10

3. 88

198 994 1170

2,2

10

412

5

1,1

987

16

4, 16

16

4

155
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4359.076r 5 1. 1 4364.041m 48 11. 0 CH P 11 0,0 4

4359.194 15 3. 4 w? 4364.189m 53 12. 1 CH P 11 0,0 4

4359.341 29 6. 6 CH P 10 1,1 4 4364.322 14 3. 2 w

4359.493

4359.623m

49

139

13. 8

31. 9 s

CH

Nil

llCri

fP 10 IP 10

3. 40

0. 98

0,0

1,1

86

22

4364.502r

4364.663

4364.871r

3

12

1

0. 7

2. 7

0. 2

u Ce II Cri

0. 50

3. 10

135

153

4359.744

4359.907r

4359.983

53

5

9. 5

15. 6

1. 1

2. 2

w

s,d

Zr n CH

Cri

1. 24 P 10

/2. 98

13. 37

79

0,0

103 198

174 4365.008r

4365.286

4365.532

4365.725r

1. 5

3

28

1

0. 3

0. 7

6. 4

0. 2 s Vi 1. 71 79

4360.120r 4 0. 9 4365.904S 48 10. 8 u Fei 2. 99 415

4360.289m 58 13. 3 CH P 10 0,0 4 4366.086r 2. 5 0. 6 4360.480m

4360.636r 4360.797m

4360.931r

4361.059?r

/loci OKO

4361.314r

59

3

51

5

3. 5

29

13. 5

0. 7

11. 7

1. 1

0. 8

I

I 3.4

s

u

1 w,N

Til

CH

Fe I

Co I? Fe II—

2. 17 P 10

3. 64

0. 22

204

0,0

903

1

4 4366.202r

4366.413

4366.500 4366.675m

4366.908

4367.060

4367.195

4

20

63

72

14

4. 5

11

0. 9

5. 5

14. 4

16. 5

3. 2

1. 0

2. 5

u,N

u

-CH

CH

CH

Fe I p Nil

CH

P 12 P 12 P 12

4. 39

4. 09 P9

1.1

0,0

0,0

1170

2,2

4

4

4

4

4361. 668r 2 0. 5 Ce II 0. 53 157 4367.333 12 2. 7 Nil 3. 46 88

4361.795r 4 0. 9 4367.475 21 5. 7 u CH fP 12 IP 9

1,1 2,2 }4, 16

4361. 861r

4362.038r

1. 5

5

0. 3

1. 1 u? Sm II 0. 48 45

4367.594 143 32. 7 u |Fei

CH

2. 99 P 12 414

0,0 4

4362.099

4362.216

29

24

6. 6

5. 5

0?u

Ni II CH

4. 03 P8

9

2,2

17

4

4367.679

4367.723r

[ 59

J

f 22. 4

1 3. 2

w,'N Ti 11 CH

2. 59 P 12

104

0,0 4

4362.382r 4 0. 9 s 16 4367.912m 90 20. 6 s Fei I. 61 41 4362.533m 53 12. 1 w? -CH P 11 1,1 4 4368.065r 6 1. 6 s,N Vi 0. 04 5

4362.746 45 10. 3 u CH P 11 1,1 4, 16 4368.131 38 8. 7 w?

4362.953 16 3. 9 u ICri

Cr II

2. 87

5. 66

82

179 4368.303 26 6. 0 u ICr I Ni I

3. 01

3. 42

130 102 4363.108m

4363.293

72

60

16. 5

13. 8

u,d

w,d

CHCn

CH

P 11

2. 97 P 11

0,0 103

0,0

4, 17

4, 17

4368.470r

4368.639

1

21

0. 2

4. 8

u

u Nd II- Fe I p

0. 06

3. 25

11 644

4363.467 4363.54?m

4363.602

4363.819r

4363.976r

24

3

27

2. 5

3

5. 5

0. 8

6. 2

0. 6

0. 7

uSw

CH

Vi

-CH

P 11

0. 28 P 11

1,1

23

1,1

4

4

4368.897m

4368.92 m

4369. 095r

4369. 269r

9. 5

1. 5

6. 5

2. 2

0. 3

1. 5

ul

S

Mn I —

Cri

Til

Fe i?p

4. 71

3. 37

2. 27

4. 59

198

245

1244

13

156
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4369.406m

4369.546

4369.714r

4369 779m

4369 866r

4370.034

42

29

\ 162

/

16

9. 6

6. 6

[ 6. 2

30. 9

I 2. 3

3. 7

ly

u

u,N

Fe II

TiiFe I p

Fe I CH

Ni I

2. 78

2. 58

3. 94

P 13

3. 05 P 13

3. 63

28

290

976

0,0 518

0,0

149

4

4

4373.791

4373.888

4374.048r

4374.182

4374.226r 4374.472m

1 64

7. 5

1 108

110

1

7. 8

I 7. 8

1. 7

1

14. 4

1 14. 4

25. 1

u

u

u

CH

CH

Fe I p

Cn

CH

|Sc II- Fe I

P 14 P 14

3. 64

3. 00 P 14

0. 62

3. 30

1,1

1,1 904

104

0,0

14 648

4, 16

4

4

4370.154 27 6. 2 CH P 13 1,1 4 4374.617r 19 4. 6 u

4370.292 26 5. 9 CH P 13 1J.J 1J. 4 4374.825 41 9. 6 w1 Ti n 2. 06 93

4370.413 7 1. 6 4374.944m 88 20. 1 u Y II 0. 41 13

4370.584r 1. 5 0. 3 4375.058r 10 2. 3 Nd II? 0. 00 8

4370.656r 5. 5 1. 3 4375.202 55 12. 6 CH P 14 1,1 4 4370 857r 11 2. 5 Mn I 2. 30 17 4375.335 30 7. 3 Cr I 2. 98 103 4370 9S5r

4371.062r

20

78

5. 7

17. 8

\ w,d

Fe I |Zr II CHCH

2. 18

l! 21 P 13 P 13

69

79

0,0

0,0

174

4

4375 485r

4375.578

4375.658

9. 5

49

69

2. 3

15. 3

15. 8

Fe I p CH

CH

3. 57 P 15 P 15

797

0,0

0,0

4

4

4371. 161r 30 9. 2 u,N Co I 2. 08 93 4375.944m 152 34. 7 s Fe I 0. 00 2 4371.286m 110 25. 2 s Cri 1. 00 22 4376.216 23 5. 2 CH P 11 2,2 4

4371.426

4371.582

46

12

11. 9

2. 7

w,d? CHCH

CH

P 13 P 13 P 10

1,1

1,1

2,2

4

4

4

4376.405

4376.563

25

21

5. 7

4. 8

CH P 11 2,2 4

4371.794

4371.956r 4372 025r 4372 201r

4372.335

4372.41 m

18

4. 5

5. 5

6

27

9. 5

4. 1

1. 0

1. 3

1. 4

6. 2

2. 3

u

J

s,d

Ru I CHTii

0. 93 P 10

2. 49

13

2,2

277

16

4

4376.782m

4376.955r

4377.087 4377.234m

4377.374

52

7

12

87

32

11. 9

1. 6

2. 7

19. 9

8. 4

s

u

IFei

Cri

CH

CH

Fe I CH

/3. 02

13. 64

4. 45

P 11 P 15

3. 88 P 15

471 904

304

2,2

0,0 990

1,1

4

4

164

4372.493 13 3. 0 CH P 10 2 2 4 4377.543 14 3. 2 s Cri 2. 91 83 4372 588r

4372 743

4372 TtV 1 ^ • 844 *J -I- -1,

4372 991m

6

32

69

34

1. 4

9. 1

15. 8

7. 8 u

Fe I CH

CH

Fe I

P 14 P 14

3. 02

0,0

0,0

473

4

4

4377 793m

4377.991r

'

4378.255m

39

0. 5

83

8. 9

0. 1

19. 0

u Fe I (Moil)

CHCH?

3. 27

3. 02

P 16 P 16

645

3

0,0

0,0 4

4

4373. 119r 5 1. 1 4378.512 25 5. 7 Fei

4373.264m 45 10. 3 s Cri 0. 98 22 4378.744r 0. 5 0. 1 Fe I p 3. 55 759

4373.396 7. 5 1. 7 4378.913m 44 10. 0 CH r 15 l.-l 4

4373.568m 65 u Fei /2. 56

13. 02 214

413

4378.97 m 1 0. 3 S,N

4373.655r 8 1. 9 Cri

Co I?

4. 45

3. 51 304

4379.074r 4379.238m

7

110

1. 6

26. S Vi 0. 30 22

157
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4379.407r 2. 5 0. 6 4384.819 30 10. 9 u7 Sc II 0. 60 14

4379.531 6 1. 4 4384.983m 80 18. 9 s Cn 1. 03 22

4379.640r 2. 5 0. 6 4385.124m 59 14. 1 CH P 19 0,0 4

4379.771 25 5. 7 s llCri Zr n

3. 01

1. 53

130

88 4385.254m 62 12. 1 u |Fei -

CH

3. 02 P 18 415

0,0 4

4379.908r 2 0. 5 4385.387m 81 18. 7 w Fe II 2. 78 27

4380.067

4380.237r

4380.367

68

4

15

15. 5

0. 9

3. 4

u,N

u

Ce II? Co I?-

Mg"i

(CH)

0. 62

3. 51

4. 34 PJ6

155

12

0,0 4

4385.611

4385.670

4385.857 4386.063m

10

15

16

43

2. 5

3. 4

3.6

9.8

s

CH

Nd II

-CH

P 13

0. 20

P 17

2,2

50

1,1

4

4 4380.496 38 8. 7 u 16 4386.275r 2. 5 0. 6 4380.724 92 21. 0 CH- P 17 0,0 4 4386.460 14 3. 2 u Nil 3. 83 168 4380.852

4380.990

4381.112

4381.297

4381.709

4381.885

4381.989

36

12

27

4. 5

7. 5

13

11

9. 6

2. 7

6. 2

1. 0

1. 7

3. 0

2. 5

w,N

u?

suu,N

u

u

CHCH

Cri

Mn I CH

CHFe I p

P 16 P 12

2. 71

4. 79 P 12 P 12

3. 69

1,1

2,2

64

2,2

2,2 938

4

4

4

4

4386.592r

4386.694 4386.853m

4387.063m

4387.20 m

4387.262r

4387.398

8. 5

23

59

59

7. 5

38

1. 9

5. 2

13. 4

13. 4

1. 7

10. 5

u,N

u

s

u

Fei

Fe II p

ch:

Ti II CH

Vi

-CH

3. 63

2. 58 P 13

2. 60 P 20

1. 04

P 18

899

26

2,2

104

0,0

40

1,1

4, 16

4

13

4 4382.167

4382.317r

8

1

1. 9

0. 2

uu,N

Ce II 0. 68 2 4387.497 61 13. 9 s Cn

(CH)

/2. 99

13. 00 P 19

84

103

0,0 4

4382.521 32 8. 2 CH P 16 1,1 4 4387.595 38 9. 6 CH P 19 0,0 4

4382. 689r 13 5. 7 CH P 17 0,0 4 4387.748r 2. 5 0. 6 4382.764

4382.998

4383. 174r

4383.310r

4383.377r 4383.557m

4383.721r

4383.832r

4383.964r

4384.120

79

47

12

16

10

1008

9. 5

18

6. 5

22

22. 4

16. 4

6. 8

13. 0

11. 4

S35

12. 1

13. 7

3. 4

8. 4

u

S

CH-

|Fei

-CH

Fei

CHCH

P 17

3. 57

P_18

1. 48

P 17 P 17

0,0

799a

0,0

41

1,1

1,1

4

4

4

4

4387.899m

4388.101r

4388.252r 43S8.414m

4388.586

4388.729

4388.870

4389.031r

4389.088r

4389.253S

4389.396r

73

26

19

103

22

35

47

3

3. 5

67

7

16. 6

5. 9

4. 3

23. 5

5. 0

8. 0

10. 7

0. 7

0. 8

15. 5

1. 6

s

s,d

uu,N

u

s

Fei

TiiFei

CH

Fe I Fei?

3. 07

2. 24

3. 60

P 21

0. 05

476

219

830

0,0

2

4

4384.317m 31 9. 4 w Fe II p 2. 66 32 4389.504 19 4 6 CH P 18 1,1 4

4384.540 2S 7. 3 u Nil 3. 46 86 4389.638 45 10. 2 CH P 20 0,0 4

4384.712m 110 26. 7 S Vi JO, 07

10. 29

522

4389.776

4389.877

30

25

6. 8

5. 7

CH

Nil

P 20

3. 46

0,0

87

4

158
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Eciui- valent Width

A\

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or

Itot. Line

RMT

No.

or

Vib. Band

Notes

4389.988m 84 19. 1 S Vi 0. 28 22 4394.51 m s,N 13

4390. 114r 11 2. 7 CH P 14 2,2 4 4394.623r 7 1. 6

4390.222 16 3. 6 w CH P 14 2,2 4 4394.791 8. 5 2. 5 Vi? 1. 35

4390.328 18 4. 1 u Nil 3. 66 136 4394.852 51 IL 6 s Til 1. 05 78

4390.461 53 12. 1 u Fei 2. 99 413 4395.040m 135 30. 7 w Ti n 1. 08 19

4390.545

4390.630

4390.773r

4390.843r

4390.966

4391.033

4391. 147r

4391.299

4391.488

4391.668

33

30

7

6

92

34

10

7. 5

38

44

8. 9

7. 5

1.6

1. 4

21. 0

13. 0

2. 3

1. 7

8. 6

11. 8

u

uw

u

u?

CH

CH

Sm II Fei

Ti 11

CH

Ce II- CH

P22

P 19

0. 18

3. 02

1. 23

P 14

0. 32 P 21

0,0

1,1

15

414

61

2,2

81

0,0

4

4, 16

4

4

4395.251m

4395.289r

4395.504

4395.684r 4395.848m

4396.079

4396.153r

4396.309

4396.430

1 100

66

5. 5

61

22

18

36

17

f 21. 6

1 3. 4

15. 0

1. 3

IB. 0

5. 0

4. 1

8. 2

4. 1

s

u,d

w?

u

Vi

Fe ICH

CHFe I

Ti II CH

-CH

CH

CH

0. 27

3. 65 P 23 P 23

/3. 88

13. 88

1. 24 P 26 P 26 P 20

P 20

22

828

0,0

0,0 991 992

61

0,0

0,0

1,1

1,1

4

4

4

4

4

4, 16 4391.768m

4391.863 4392.071m

67

36

54

15. 2

9. 1

10. 9

s

w,N

s

Cri

(CH)

Fei

Vi

CH

1. 00 P21

3. 93

0. 27 P23

22

0,0

992

23

0,0

4

4

4396.631r

4396.772r 4396.961m

4397.143

3. 5

1. 5

45

22

0. 8

0. 3

10. 2

5. 0 u

Mo I?

CH

CH

2. 08

P 24 P 24

0,0

0,0

4

4

4392.300 12 2. 7 u,N Fe I p 3. 55 757 4397.22 m S Cn 3. 01 129 13

4392.432r 3. 5 0. 8 u 4397.264 25 5. 7 u

4392.587m 37 8. 4 u Fei 3. 88 973 4397.381 14 3. 4 u

4392.788r 6. 5 1. 5 4397.583r 1 0. 2

4392.924 21 4. 8 u CH P 19 1,1 4, 16 4397.778 9. 5 2. 2

4393.025 27 6. 1 s? CH

Fei

P 19

/3. 02

13. 55

1,1 473

4, 16 4398.020S

4398.174

46

11

10. 7

2. 5

u

u

Yii 0. 13 5

4393.284 46 10. 5 s? 4398.299 28 6. 4 w Ti II 1. 22 61

4393.33 m S Nai 2. 10 17 13 4398.491 34 7. 7 CH /P 25 IP 28

0,0

0,0 4393.524

4393.700

71

28

16. 2

6. 4

u,d?

w

-CH

(Cri)

Fe I p CH

/P 22 \P 24

2. 97

3. 64 P 22

0,0

0,0 102

899

0,0

}4, 17

4

4398.621

4398.712

24

17

5. 4

4. 3

w

w

Vii

Nil

CH

CH

3. 33

3. 54 P 28

P 25

187

102

0,0

0,0

164

4, 16

4393.808

4393.931m

4394.068m

4394. 183r

4394.304r

28

22

72

11

2

6. 4

5. 0

18. 0

2. 5

0. 5

u

sw

u

CH

Vi

Ti I Ti 11

Fe I p

P 20

1. 05

2. 27

1. 22

3. 94

1,1 40

244

51

975

4 4398.844

4399.067

4399.224

4399.290

4399.482

18

6. 5

5. 5

7. 5

15

4. 1

1. 5

1. 3

1. 7

3. 6

w

s,N u

u

8

Ce 11 Fei?

CH?

In?

0. 33

P 16

2. 05 1

81

2,2

17

4

159
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4399.602m

4399.778m

32

115

7. 3

26. 4

w

w?

Nil

Ti II (Cri)

3. 85

1. 24

3. 01

196

51 129

4405.033m

4405.314r

28

0. 5

15. 9

0. 1

s Vi

Fe I p

0. 28

0. 05

23

2

4399.989 21 4. 8 CH P 26 0,0 4 4405.411 4. 5 1. 4 u Fe I p 3. 93 991

4400.185

4400.398

41

85

9. 3

19. 6 u

Nil

CH?

So II

3. 63 P 26

0. 61

146

0,0

14

4 4405.569

4405.732

2

25

0. 6

6. 4 s,d Ti ICH?

1. 05 P 30 78

0,0 174

4400.580 61 11. 6 s Vi 0. 26 22 4406.036 12 3. 0 u CH? P30 0,0 4

4400.688 4400.858m8

42

1. 8

9. 5 u Nd IIJNl I

0. 06

3. 65

10 149

4406.157

44Uo./y5r

23

oO

5. 7

0. 7

u CH

V I Cr I

P 17

1. 06

6. 09

2,2

1 CO

4, 16

4401.022 58 13. 2 u

A A r\£i er\ A 19 4. 5 u r 16 1,1 4

4401.16 a 15 3. 6

A A f\t2 a tret 4406.652 TO 18. 2 o V I 0. 30 11

4401.298m 101 22. 9 u Fe I 3. 60 828 A A r\c ooc 4406. 8o6 1 nlU 2. 3 4401.451m 48 15. 0 u Fe I 2. 83 350 A A no r\n A 4406.994 D. 5 1. 5 4401.552m 115 26. 1 u

"NT; - Ni I 3. 19 86 A A 1 on.- 44U7.1d9r 7. 5 1. 7

4401.668 10 2. 5 CH? P 27 0,0 4 4407.272 25 5. 7 u,N -Ce II? 0. 70 64

4401.80 a 5. 5 1. 2 4407.375r 12 2. 7

4401.87 a 2 0. 5 4407.522r 5 1. 1

4402.343

4402.475

4402.685r

4402.841a

6

7

4

18

1. 4

1. 6

0. 9

4. 1

u

u

Co I? CH3. 51 P28 0,0 4, 16

4407.652r

4407.706

4407. 864r

4407.934

> i4d

2. 5

16

f 14. 1

1 24. 5

0. 6

3. 6 u

Vi

Fei

(Cr I)

0. 29

2. 18

6. Ul

22

68

1 on

4403.077 18 4. 5 u,N CH P 28 0,0 4, 16 4408.078r 7 1. 6 4403.187m 62 14. 5 u 4408.208m 74 n. 2 S Vi 0. 28 22

4403.374

4403.496

46

21

10. 7

5. 4

s

u

llCri Zr 11 Cr I

3. 01

1. 18

3. 98

12879 4408.425m

4408.523

130

65

29. 5

24. 5

s?

s?

Fei

Vi

2. 20

fO. 26

\0. 27

68

22

22

4403.649 10 2. 3 — V I? 1. 87 4408.660 18 4. 1

4403.829 3 0. 8 4408.798r 10 2. 3 -Pr II? 0. 00 4

4403.972 16 4. 3 w? 4408.941 19 4. 3 V II 6. 97 oo /I iZ'i

4404.101 12 3. 4 u Fe I p 3. 93 987 4409.128m 51 11. 6 u Fe I 3. 30 645

4404.277m 35 12. 0 u ITiiCH

/2. 25

12. 25 P 29

218

219

0,0 4

4409.248m

4409.359

2S

12

6. 8

2. 9

w

„ . AT"

Ti II — Dy II

1. 24 ol

4404.400 9 4. 3 s Til 1. 05 78 4409.526m 33 7. 9 w Ti II 1. 23 61

4404.548r 8 5. 2 CH? P 29 0,0 4 4409.695r 1. 5 0. 3

4404.599r 8 7. 0 4409.857r 2 0. 5 Mg I? 7. 19 48

4404.761m

4404.924r

898

6

181

7. 3

s

u

Fei

TilCo I

1. 56

1. 88

2. 63

41

161 127

4410.014 25 5. 7 -CH? fP 24

IP 25

1,1

1,1

160
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4410.167 25 5. 7 -CH? P 24 1,1 4 4415.563m 86 21. 7 u So II 0. 60 14

4410.306 14 3. 2 s Cr I 3. 01 129 4415.785 11 2. 5

4410.525 51 11. 6 u Nil 3. 31 88 4415.915r 6 1. 4

4410.659r 3 0. 7 Ce 11? 1. 35 33 4416.065r 12 2. 7

4410.765r 2 0. 5 4416.160r 6. 5 1. 5 Fe I?

4410.861r 4. 5 1. 0 4416.360 13 2. 9 -CH? P 19 2,2 4

4410.953r 4411.082m9. 5

56

2. 2

12. 7

suCri

Ti II- Cn

2. 98

3. 09

3. 01

102

115

129

4416.475m

4416.651r

36

10

8. 1

2. 3

S,d1

s

IIViTii?

0. 27

1. 87

22

161

4411.227

4411.35 a

4411.590r

4411.724r

4411.884r 4411.935m

24

6

4. 5

2. 5

j 55

5. 4

1. 4

1. 0

0. 6

[ 12. 0

u,N CHCH?

Mo I? Mo I Mn I

|Ti II Fe 1?

P 18 P 18

2. 08

2. 08

4. 71

1. 22

2,2

2,2

61

4

4 4416.828S

4417.003r

4417.115r 4417.287m

4417.412

4417.574 4417.723m

77

7

2

45

15

11

96

17. 4

1. 6

0. 5

10. 2

3. 4

2. 5

22. 4

w

s

suwt

Fe 11

Til

Co I CH

Ti II

2. 78

1. 89

3. 07 P 26

1. 16

27

161

150

1,1

40

4

4412.138r

4412.257

4412.424

8

29

7

1. 8

6. 2

1. 6

s

s,d

s

Vi

Fe I CriITii Fe I p

0. 26

1. 03

0. 90

2. 18

23

22

54

69

4417.884r

4418.035

4418.206r 4418.342m

4

8

6. 5

70

0. 9

1. 8

1. 5

15. 8

w

u Ti II 1. 24 51

16

4412.698 8. 5 1. 9 4418.430 21 5. 4 s Fei 2. 99 412

4412.877 6 1. 4 u 4418.574r 7 1. 6 — Fe I p 3. 63 899

4413.121 11 2. 5 4418.63 a 4 0. 9 s

4413.399 7. 5 1. 7 u Fe I p 4. 07 1046 16 4418.785 17 3. 8 u Ce II 0. 86 2 4413.599m

4413.785r

39

3. 5

8. 8

0. 8

w !Fe II CH?

2. 68 P 2532

1,1 16

4 4418.940

4419.104

22

12

5. 0

2. 7

u

u Cn

Fei

3. 01

4. 39 128 1170

4413.853 29 6. 6 u Cri 3. 55 234 4419.273 16 3. 6 Fe I p 3. 63 893

4414.048r

4414.124

1

> 26

r 1.6

I 4.3 u

Fe I p

-CH?

3. 60 P 19825

2,2 4

4419.513

4419. 607r

3

2

0. 7

0. 5

Fe I

4414.234 17 3. 8 u Fe I p 3. 07 475 4419.778

' 18 4. 1 u Fe I 3. 30 644

4414.458 9 2. 3 u Fe I 3. 27 643 4419.942m 6. 5 1. 5 s Vi 0. 28 21

4414.554 23 5. 4 u Zr II 1. 24 79 4420.105r 3. 5 0. 8

4414.737r 3. 5 0. 9 Fei 4420.287 34 7. 7 u Fei

4414.890 59 20. 2 s? Mn I 2. 89 22 4420.46 m s Osi 0. 00 1 13

4415. 040r

C

4. 5 4420.526 14 3. 2 u Sm II 0. 33 32 4415.135m > 417 < 92. 9 s Fe I 1. 61 41 4420.671 15 3. 4 w Son 0. 62 14

4415.255r [ 3.4 4420.929r 2 0. 5

4415.427r 3. 5 1. 1 4421.125 10 2. 3 u,N — Sm II 0. 38 37

161
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

4421.334 21 4. 8 u Co I —

CH

2. 93 P27150

1,1 4

4421.455r 13 2. 9 u

4421.573ni 35 7. 9 S Vi 0. 28 22 4421.763m 34 7. 7 s Til 2. 24 218

4421.944m 51 11. 5 w Ti II 2. 06 93

7 9 XL

4422.304 23 5. 2 u,N

4422.40 a 15 3. 8

4422.505r

j 117

f 2. 7 u Vi fl. 71

11. 86

79

4422.576m L 24. 6 s |Fe I Yii2. 84

0. 10 350

5

4422. 711r 6 1. 5 Cri 3. 56 234

4422.829m 29 6. 6 s Ti I 1. 07 78

4422.973 34 7. 7 V Ni I 3. 68 168 4423.140m 59 13. 3 s Fe I 2. 99 412

4423.265 37 9. 0 s,d? Na I —

Cri

2. 10

3. 01

16 128

4423.468r 2 0. 5

4423. 585r 1 0. 2

4423. 681r 3 0. 7 Ce II 1. 06 21 4423.847m 53 11. 8 w? Fe I 3. 65 830

4424.072 24 5. 4 u Fe ICr I 2. 91 82

4424.204 14 3. 4 u Fe I 3. 55 757

4424.294 41 9. 3 u Cri 3. 01 129

4424.369 7. 5 1. 9 s,N Sm 11 —

Ti I

0. 48

2. 27

45 243

4424.586 26 5. 9 u,d V I? —

IFei

1. 38

4424.811 9. 5 2. 1 u Nil? 4. 16 262

4425.148 8. 5 1. 9 s Cr I 3. 10 152

4425. 444S 145 SI. 6 s Ca I 1. 88 4

4425.664 40 9. 0 u Fe I 3. 57 798

4425.769 20 5. 0 u,N Fe I p

Fe I p

3. 26

3. 64 555

899

4425.85 m 6. 5 1. 6 s Til 1. 07 78

4425.959r 9. 5 2. 3 S

4426.040m 38 8. 6 s ViTii0. 29

1. 88

22

161

4426.377 5 1. 2

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Banc

Notes

4426.458 14 3. 2

4426.677r 9 2. 0 Cr I? — 5. 24

4426.892r 6 1. 4 4427.105m 64 14. 4 ; s Ti I 1. 50 128 4427.317m 147 S4. 6 S Fe I (Feip)

0. 05

3. 65

2 828

4427.461r 12 2. 9

4427.598r 9. S 2. 1

4427.713r 2. 5 0. 6 u Cri 3. 01 129

4427.75 a 2. 5 0. 6

4427.80 a 4 0. 9

4427.916 12 2. 7 u Ti II p 1. 24 61

4428.094 6 1. 4

4428.276 6. 5 1. 5

4428.52 m 13 3. 4 s |Vi

Cri

0. 27

3. 01

21 129 4428.549m 35 7. 9 u? Fei 3. 94 973

4428.707 10 2. 3 u — Fe I p 3. 64 899

4428.916r 2 0. 5

4429.203 15 3. 4 u Fe I p —

Pr 11?

3. 93

fO. 00

10. 37

987

24

4429.288 11 2. 7 u Ce II- Fei1. 09

3. 94

19 972

4429.503r 2. 5 0. 6

4429.643r 1. 5 0. 3

4429.794

4429.906

7. 5

30

1. 8

7. 2 \s,N

)

V I

11 La II Cri

0. 30

0. 23

3. 55

22

38 234

4430.057m 52 IL 7 u Tii- 2. 41 267

4430.197m 68 15. 3 u Fe 1 3. 02 472

4430.368 27 6. 1 s Til 1. 44 113

4430.483 20 5. 0 u Cri 3. 56 234

4430.622S 115 26. 0 s Fe I 2. 22 68

4430.765 40 9. 7 w,N

4431.036 24 5. 4 u Nil 4. 17

4431.292r 5 1. 1 s Til 2. 23 218

4431.360 30 6. 8 u Sc II 0. 61 14

4431.499r 7. 5 1. 7

4431.621 6. 5 1. 5 Co 1? 2. 88 L 43

4431.846 41 9. 2 u

162
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Banc

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Banc

Note

4432.089 15 3. C w Ti II 1. 24 51 4437.507 22 5. 0 w? Ni I 3. 68 168

4432.169 37 8. 3 u Cri 2. 87 81 4437.699 12 2. 7 u Fei 2. 69

4432.316r 2. 5 0. 6 4437.842 27 6. 4 S Vi 0. 29 21

4432.426r 1. 5 0. 3 4438.030r 6 1. 4 s Sr I I. 85 6 4432.575m 47 10. 6 u Fe I 3. 57 797 4438.197r 6 1. 4

4432.743r 5. 5 1. 2 -Cr I? 5. 25 4438.25 m 6. 5 1. 5 .s Til 2. 25 218

4432.927r 2. 5 0. 6 Fe I? p 2. 73 271 4438.349m 45 10. 4 w Fei 3. 69 828

4433.046r 11 2. 5 u 4438.520 8. 5 1. 9 Fe I p 3. 88 969

4433.230m 97 3 u Fe I 3. 65 830 4438.627 12 2. 7 u

4433.396 19 4. 3 u Fe I p 3. 02 412 4438.790r 3. 5 0. 8 4433.588 11 2. 5 s Til 2. 40 267 4438.964r 4 0. 9 4433.788m 73 16. 5 s Fei 3. 60 825 4439.01 m 5. 5 1. 2 s

4433.896 6. 5 1. 7 Sm II 0. 43 41 4439.163 20 4. 5 u,N Feii?p- 2. 69 32

4433.97 m S Cn 3. 01 128 13 4439.358r 19 4 3

4434.196

4434.344

49

5

15

y. 0

1. 1

3. 4

s

s

111

Sm II —

Til?

/I. 43

11. 87

0. 38

113

161

36

4439.486r

4439.642

4439.748r

4439.888S

6. 5

22

3. 5

47

1. 5

5. 0

0. 8

10. 6

u

s

Fei

Fe I

3. 05

2. 28

515

116

4434.439 33 7. 4 u 4440.068r 9. 5 2. 1 4434.655 19 4. 3 u Si I 4. 92 4440. 179r 10 2. 3 Fei

4434.756r 9. 5 2. 3 Cri 3. 01 128 4440.348m 25 5. 6 s Til 1. 87 159 4434.967m

4435.156m

4435.328

4435.441 4435.688m

171

83

26

11

127

40. 6

20. 3

5. 9

2. 7

28. 8

s

su

s

Cai

Fe I Nil?

Cai

(Eu II)

1. 89

0. 09

3. 66

1. 89

0. 21

4

2

44

4440.482m

4440.630 4440.827m

4440.993

4441.092

46

19

47

22

36

10. 4

4. 3

10. 4

5. 2

8. 1

w

uu

u

Fei

Zr II

Fe I Fe I

3. 60

1. 21

3. 96

3. 30

829

79

992

645

4435.838r 12 2. 7 4441.273m 15 2. 9 s Til 1. 87 160

4436.000r 8. 5 1. 9 Mn I? 3. 77 40 4441.436 13 3. 1 u Ni I? 3. 31 4436.145 34 8. 0 s Vi 0. 26 21 4441.555 20 4. 5 u Fe I p 3. 88 987

4436.356m

4436.589

4436.687

4436.787r 4436.951m

70

8. 5 6

4. 5 75

16. 1

1. 9

1. 4

1. 0

16. 9

s

s

s

u,d

Mn I Til

Til

|Fei

Ni I

2. 92

1. 88

2. 43

3. 05

3. 50

22

160

267

516

86

4441.719m

4441.964r

4442.078r

4442.15 a

4442. 258r

79

13

9

5

7. 5

16. 7

2. 9

2. 0

1. 2

2. 1

s,N

u

llViTiiip

Fe I

Mo I? Cr I

0. 28

1. 18

2. 08

3. 00

2140

102

4437. 135r

4437.267r

2

0. 5

0. 5

0. 1

4442.349m

4442.416r 1 171

[ 39. 2

\ 0. 9

s Fe I Nil2. 20

3. 50

68

87

4437.427r 1 0. 2 4442.588r 5. 5 1. 2

163
The Solar Spectrum—Continued

Wavelength

(k)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(m A)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4442.679r 4. 5 1. 0 4449.466 8 1. 8 4442.838m 57 12. 8 s Fe I 2. 18 69 4449.60 m 6 1. 3 s Vi 1. 35 62

4443.001 26 5. 8 Zr 11 1. 49 88 4449.719 4 0. 9 s Dy II- 0. 00 4443.201m 95 £S. 5 u Fe I 2. 86 350 4449.930r 3. 5 0. 8 Si I 4. 95

4443 .296r 9 2. 0 4449.97m 2. 5 0. 6 s Til 1. 88 159

4443. 560r 5 1. 1 4450.101 5 1. 1 M Nil 3. 94 178 4443.812m 124 30. 8 w Ti 11 1. 08 19 4450.235r 5. 5 1. 2 Nil 4. 10 236

4443.970r 7. 5 1. 7 4450.323m 53 11. 9 U Fe I 3. 11 476

4444.080r 6. 5 1. 5 4450.491m 79 17. 8 wl Ti II 1. 08 19 4444.218m 31 7. 4 S Vi 0. 27 21 4450.631r 5 1. 1

4444.401 5. 5 1. 2 Ce II 0. 92 19 4450.764 25 5. 6 u Fe I 3. 88 972

4444.562m 50 12. 4 w Ti II 1. 12 31 4450.901m 45 10. 6 s Til 1. 88 160

4444.697 6 1. 3 Ce II 1. 06 19 4451. 116r 3. 5 0. 8

4444.80 a 1. 5 0. 3 4451. 357r 2 0. 4

4445.065r

4445.319 4445.479m

4445.683

4445.849

4446.075r

4446.242

4446.399

4446.541r

4446.630 4446.843m

4446.896

4447.027r 4447.137m

4447.359

4447.555r 4447.728m

4447.789r

4448.021r

4448.279

4448.444r

4448.945

2

2. 5

30

7. 5

5

0. 5

4. 5

8. 5

1. 5

3

2

60

11

2 }-

1. 5

4. 5

1. 5

12

0. 4

0. 6

7. 2

1. 7

1. 1

0. 1

1. 0

1. 9

0. 3

0. 7

f 15. 7

1 0. 2

0. 4

13. 5

2. S

0. A

1" S7. &

\ 2. 0

0. 3

1. 0

0. 3

2. 7

u

u

s

u

u

u

s

u,d

s

u,d?

s,d

s?

Fei?

Fe I -Co I

Zr II?

Fe II? Nd II

Fe I Fe I p

Fe I

Fe I

Fe I p

0. 09

3. 10

1. 66

5. 95

0. 20

3. 69

3. 30

2. 20

2. 22

3. 64

2

150

96

187

49

828

596

69

68

891

16

16

16

4451. 588S

4451.833r 4452.007m

4452. 147r

4452.323

4452.617

4452.741

4452.809 4453.006m

4453. 163r 4453.321m

4453.524 4453.710m

4453.841

4454.005

4454.109r

4454.222r

4454.388S

4454.535r

4454.793m

90

1. 5

22

2. 5

0. 5

26

6. 5

13

46

1. 5

59

7. 5

36

7

2

2

4

84

14AA

176

20. 2

0. 3

4. 9

0. 6

0. 1

5. 8

1. 5

2. 9

11. 0

0. 3

13. 7

1. 7

9. 0

1. 6

0. 4

0. 4

0. 9

18. 8

3. 4

11 A

46. 2

s

s

u

u,N

s

s

u

s

u

s

1/?

s

Mn I (Nd II)

Vi

Fe I p

Fe I Sm II

Mn I

Til

Ti I

Fe I

Pel

Ca I (Zr II)

2. 89

0. 38

1. 87

3. 64

3. 94

0. 28

2. 94

1. 43

1. 87

2. 83

0. uo

1. 90

0. 80

22

50

87

898

969

26

22

113

160

350

440

4449.150m

4449.341

53

15

13. C

3. 4

5

u

Ti I Ce II1. 89

0. 61

160

202

4455.030m 90 20. 2 s,N Mn I —

|Fe I

3. 07

3. 88 28

974

164
The Solar Spectrum—Continued

Equi- Re- Low RMT

Wave- valent duced Solar EP No. Wavelength w lutn "ITT": J f u W latn Identi- or or Notes length AX AX/X fication itot. V ID. (A) (mA) (F) Line r>an u (A)

4400.1 / /r 1 1 /. 0

A A Cir\ AAA4400. o^um 70/y 17 7 S iVln 1 — Q ri7 44DU.1 izr

IT'; T 1 A 4

1. 44 1 1 Q 4400. z/or

4400. 40/ D. 0

1 K

1. 0 or I o. Ul 1 07

/i /f AO Q01 4400. o4or 6. 0 U. o

^ /I AO Q A 1 *- 44DU.£)Dlr 4400. Dour 7/ i. D

/1/lAO KQA». AAKK Q1 Q 4400. oiy 45 ^ A Q 14. o

1 ivin I Q /17 4460.778

4455.893 106 23. 8 1 [Cai 1. 90 4 4460.930r 4456.060r 15 3. 4 4461.084m

4456.176 6. 5 1. 5 4461.205m

4456.333in 48 11.4 u Fe I 3. 05 516

4456.460r 12 2. 7 4461.386

AA^Pi 440D.DZR97rr> / in DO 10. 0 s ua I 1. yu 4 44Dl.4Zyr

4456. 780r 5. 3 1. 2 4461.660m

4400.0/ or

OO n 7 r e I 44Dl.oZUr 440 / .U4o oo o. 0 u iVin I Q f\7 90Zo 44DZ.UU0m

4^0 / . ioor 4. 0 J., u 440 / .z / ur QO n 7 U. / 44DZ.ZU4 AA^7 TilO 1 .rtO il^7m 4 111 oi io. Z s

II t; t 1. 40 1 lo

Zir II 1. lo 70 yl /I AO O CO

|V I 91Zl

440/5. 4oim

440 / .04 / in OD s Mn I Q n7 90Zo

A A no KOT^ AAK7 A71 440 / .0 / ir 9 Pi Z. 0 U. 0 4462.700

4457.773 13 2. 9 s Vi 1. 87 101 4462.769

4457.946r 6 1. 3 4462.897r 4458.088m 61 13. 7 u Fe I 3. 88 992

4462.993 4458.255m 66 14. 8 s Mm 3. 07 28

440o.OODr 1. D 4463.137

4458.529 43 9. 6 s Cn 1 o. Ul

[6. DO

1 07 A /* AQ OA1

(^bm II ) U. lU n

I 4463.40/

440o.DoDr 9 9

A A GO con

AA^Q. QQQ»« Q 1 C 1. o

4463. D80r

440y.U4Z 1 ly. / u JNl I O 0

O. 6l 86

I 1 on A A do OO A ^ 4463. »o4r

44oy. 1 oom J 9fi K

y ZD. 0 u r e I 9 TO /. lo DO

A A GO A'TCTM 4463. y /or 4459.361m 70 15. 7 s Cn 2. 71 63 4464.226r

4459. 506r 9. 5 2. 1 4464.340r 4459.616 7 1. 6 4464.457m

4459. 755S 48 10. 8 s Cn- 3. 01 127

IV I 0. 29 21 4464.685

4459.896 4 0. 9

Equivalent Width

AX

(mA)

2. 5

5. 5

100

5. 5

13

6

63

48

55

116

11

118

31

17

62

4

14

8. 5

6

13

19

9

41

12

1

0. 5

1

1. 5

5

68

94

Spot

I

9. 4

3. 8

28. 0

2. 5

26. 4

6. 9

3. 8

13. 9

0. 9

3. 1

1. 9

1. 3

2. 9

4. 2

2. 0

9. 2

2. 7

0. 2

0. 1

0. 2

0. 3

1. 1

15. 2

21. 0

u

s

u

u

w

sw?

w

su

u

s

u

s

Sohir

Identification

Rui?

Fe I p Ce II Vi

Mn I Fe I p Cr I

Mn I

|Fei Zr II Fe I Fe II p Fe I Fe I p

Fe I Mn I Fe I p Vi

Nil

Cr I

Nd II

Fe I

IITii- Nii

Til

Low

EP

or Rot. Line

Vii

Ti II- Mn I (Cn)

1. 09

2. 76

0. 48

0. 30

3. 07

4. 22

2. 71

3. 07

3. 02

1. 01

3. 41

2. 58

0. 09

3. 02

f3. 07

3. 60

'3. 64

3. 07

3. 60

1. 86

3. 46

3. 01

0. 56

'3. 07

,3. 64

1. 88

3. 48

1. 89

3. 76

1. 16

2. 92

3. 01

RMT

No.

or

Vib. Band

Notes

271

2

21

28

1100

63

165
The Solar Spectrum—Continued

Wave1 on o^" Vi

(A)

valent

Wirlth VV 1 Ll Kjll AX

(mA)

Re- duced

Wirlth AX/X

(F)

Solar

Identification eT

or Rot. Line

RMT

No.

or

Vib. Band

Waveivjii^ I'll

(A)

Equivalent Width

AX

(mA)

Re- duced

Wirlth VV in UXl AX/X

(F)

opot

Solar

Identification

liOW

EP

or Rot. LinG

HXXXVX MTX No.

or

Vib. R«JjdllCl TI H

4464.774 41 13. 7 U Fe I 3. 02 472 4469.937r 5. 5 1. 2

4464.911 14 3. 1 S Cri 3. 01 127 4470.138m 49 11. 6 u Mn I 2. 94 22

4464.980r 6. 5 1. 5 Euii? 3. 38 27 4470.314r 7. 5 1. 7

4465.132 19 4. 2 u,d -Cri 3. 89 267 4470.485S 69 16. 6 u Ni I 3. 40 86

4465.222r 7. 5 1. 7 4470.636r 6 1. 3

4465.358 20 4. 5 s Cr I 3. 01 127 4470.712r 2. 5 0. 6

4465.504r 2 0. 4 4470.858m 54 12. 5 u -Ti II 1. 16 40

4465.611 2. 5 0. 6 u 4471.003r 3. 5 0. 8

4^0O.i 0 a. 9 U. u 4471 087r

4466.165

"in

u. 0

7

/ . 0 n 1 U. X

1. 6

s

s

Ti T

CriFei

1 7A

3. 01

3. 64

1 dfi

127

901

44.71 94-4m

4471.408r

4471.560

6

12

0. 0

1. 3

2. 7

s

u

Ti I (Ce 11)

Co I

1 7"^ X. 10

0. 70

3. 07

X 8

150

4466.252r 2. 5 0. 6 4471.682 19 4. 2 s Fei 0. 11 2

4466.387 24 5. 4 u Ni I 3. 70 168 4471.810 6. 5 1. 5 u,N Fe I 3. 94 972

4466.562m

4466.723r

4466.854r 4466.940m

4467.085r

125

8

11

48

3

28. 0

1. 8

2. 5

11. 6

0. 7

s Fe I (Feip)

Co I Fe I

2. 83

0. 11

3. 02

3. 93

350

2

150

992

4471.913r 4472 078r

4472.208r

4472.415r

4472.541

3. 5

2. 5

4. 5

3. 5

4

0. 8

0. 6

1. 0

0. 8

0. 9 s

Ca II

Fe I p —

Fe I p

6. 47

1. 48

2. 95

6

39

411

4467.210r

4467.339

4467.440r

4467.555

4467.830

4467.999

4468.154r

4468.30Gr 4468.500m

4468.637r

4468.751r

4468.987r 4469.154m

4469.278r 4469.383m

4469.564

3

8

1. 5

11

10

8

5

6. 5

120

7. 5

9. £

6. £

49

1 ... 110

38

0. 7

1. 8

0. 3

2. 5

2. 2

1. 6

1. 1

1. 5

1. 8

2. 1

1. 5

11. C

f 0. 2

1

I 24. 6

8. 5

u

su

s

uw

s

swl

uu,N

Sm II Fe I Cri

Vi

Mo I —

Ti II

Vi

Ti II

Fei

Co I

0. 66

4. 14

3. 01

1. 85

2. 08

1. 13

1. 87

1. 08

3. 65

2. 96

53

1048

127

87

31

102

18

830

150

4472.723

4472.802

4472.930

4473.137r

4473.222r

4473.470r

4473.635r

4473.764r

4473.834

4474.049

4474.169r

4.474 4n9r

44.74 f^ftQ

4474.755

4474.859m

63

33

39

4. 5

3

0. 5

2

5. 5

4

4. 5

5

7 ^

1 9

15

18

14. 1

9. 8

8. 7

1. 0

0. 7

0. 1

0. 4

1. 2

0. 9

1. 0

1. 1

1X . 7/

9 7

3. 4

4. 0

w

sw

M?

.s

s

s

s

Fei

Mn I Fe II

Mo I?

Cri

Vi

Fe II?

IV'Tn iviU Ti V I

Til

/3. 27

13. 64

2. 95

2. 84

2. 29

2. 71

1. 95

5. 57

9 OR

1. 89

fl. 44

12. 10

595 900

22

37

63

110

171

101

113 184

4469.711m 18 4. C s Vi 1. 85 87 4475.01 Ir 4 0. 9

4469.808r 6 1. 3 4475.096r 2. 5 0. 6

166
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes

Wav(!-

length

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

KMT

No.

or

Vib. Band

Notes

4475.171r

4475.306

4475.469r

4475.50 m

4475.722r

1. 5

14

2

1. 5

9

0. 3

S. 3

0. 4

0. 3

2. 0

s

s

s

Tiip

Crip

Cr I

Til

Yi

Vii

2. 09

2. 71

2. 89

2. 12

1. 40

3. 75

18463

95

184

14 199

4480.704r

4480.825

4481 031

4481.140m

4481.273m

4481.338m

4. 5

30

10

63

1 97

1. 0

6. 9

2. 5

3

J 16. 3

[ 8. 5

u

w

s

0

Fe I p Mg IX Til

Mg II

3. 63

8. 86

1. 75

8. 86

893

4

146

4

4476.033

4476.089r

4476.235r

4476.432r

4476.62 m

4476.640r

4476.864r 4477 O'lR

4477.236

4477.469 4477 646r

1 152

11

6

3

2. 5

7

5

8

[ 22. 6

I 17. 0

2. 5

1. 3

0. 7

0. 6

1. 1

1. o

0. 6

u

s

u

u

Fei

Fe I

Ti I p

Cr I

Y I

2. 84

3. 69

2. 08

2. 71

350

830

184

63

14

13

4481. 483r

4481. 616S

4481.776r

4481.914r

4482.006r

4482.174

4482.268

4482.439r

4482.540r 4482.740m

5. 5

46

6

7. 5

2

1 165

12

6. 5

67

1. 2

10. 3

1. 3

1. 7

0. 4

1 25. 0

I 14. 7

2. 7

1. 5

14. 9

s

u

si

u

s,d

Cri

Fe I

Zni?

Fe I Fe I

Ti II p

Ti IFe I

/3. 98

14. 59

3. 69

2. 41

0. 11

2. 22

1. 12

1. 46

3. 65

270

827

131

2

68

30

113 828 4477 85 Ir 0. 5 0. 1 4482 87^ 16 0. u Cr I 3. 37 197 4478 024 15 3. 6 g Fe I 2. 20 69 44-?^^ n9Qr 2^. 0 0. 6 447R(_7«J.I42r JLiUX 1. 5 0. 3 I 0 2 4478 323 10 2. 2 Co I 3 IQ 44^^^ rJ:T:00 .00 ^^1J- 1 1^ 1. u 0

4478.44 a 4 0. 9 In? 1. 62 4483.538 2 0. 4

4478.626 12 2. 7 u -Fe I 4483.661r 1 0. 2

4478.818r 4 0. 9 u 4483.782 11 2. 5 u Fe I 3. 64 898

4478.998

4479.240r

4479.386

4479.611m

4479.713m

4479.851r

4479.968 4480.145m

4480.273

4

0. 5

18

61

16

2. 5

42

54

24

0. 9

0. 1

4. 0

13. 6

4. 2

0. 6

9. 4

12. 0

5. 4

u

s

s

u

s u,N

Fe I p Fe I p Ca II Ce IIFe I

Til

Fe I p Fe I

llCri Fei? p

3. 64

3. 96

6. 47

0. 56

/3. 69

13. 63

1. 73

3. 98

3. 05

3. 37

3. 60

899 987

6

203

828

848

146

974

515

197 823

4483.911

4484.086r 4484.227m

4484.391r

4484.503r

4484.695r

4.4-84 S9Qr

44QC rt^OO.UOOl flSflr

4485.422r

15

5

77

5. 3

6

1. 5

I0

\

5

3. 3

1. 1

19. 2

1. 2

1. 3

0. 3

0. 2

n 4

1. 1

u

u

s

Co I

Fe I

Ni I-

|Co I Cri

Tl" T?

Zr II

3. 13

3. 60

3. 60

0. 92

3. 08

9 fIS

1. 24

150

828

\ 102

27

151

J, OT^

79

4480.384r 6 1. 3 Cu I 3. 78 8 4485. 537r 6. 5 1. 4

4480.469r 2. 5 0. 6 4485.683m 65 15. 4 n Fei 3. 69 830

4480.588 33 7.4 s Nil

ITii

3. 90

1. 74

211 146 4485.839r 3 0. 7

167
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RM i No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

T ^ Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes

4485.976 18 4. 0 w Fe I p 3. 65 825 4490.614r 6 1. 3 u Fe 1 p 3. 64 891

4486. 122r

4486.223r

4486.324r

4486.598r

4486.750r

4486.914

4487.004r

4487.12 a

4487.258

4487.370

4487.513

4487.747

4487.870r

4487.944r

4488.061 4488.138m

4488.329m

0. 5

1

2. 5

3

1

11

5. 5

1. 5

10

6

5. 5

15

4. 5

3

11

46

45

0. 1

0. 2

0. 6

0. 7

0. 2

2. 5

1. 2

0. 3

2. 2

1. 3

1. 2

3. 3

1. 0

0. 7

2. 9

10. 2

10. 7

uu

?t

u

u

u

s

uu

uw

w

Ce II Fe I p

Yi

Fe I p Yi

Fei

Cri

Fe I

Ti II

0. 30

3. 93

1. 37

3. 60

1. 36

3. 24

2. 99

3. 60

3. 12

57

988

14

824

14

594

283

819

115

16

4490.781

4490.811r

4490.949r

4491. 108r

4491.18 m

4491. 213r 4491.408m

4491.660

4491.852

4491.975r

4492.114r

4492.312

4492.541 4492.688m

4492. 852r

4492. 968r

1 76

3. 5

2. 5

1. 5

66

20

10

1. 5

1. 5

21

8

29

1. 5

0. 5

[ 14. 2

L 4. 0

0. 8

0. 6

0. 3

16. 0

4. 4

2. 2

0. 3

0. 3

6. 0

1. 8

6. 2

0. 3

0. 1

w?

s

w

s

s

s

s

\i

Fe I Vi

Vi

Fe 11 Cri

Cr I

Cri

Ti I re I

Nb II? Fe I p

/3. 94

13. 94

1. 85

1. 38

2. 85

2. 90

2. 99

3. 37

2. 10

3. 98

2. 61

3. 25

973

974

86

62

37

95

83

197

184

969

639

13

4488.523r 2. 5 0. 6 4493.227r 0. 5 0. 1

4488.59 a 1 0. 2 4493.380 5 1. 1 s Fe I 3. 57 796

4488.688r 0. 5 0. 1 4493.530m 26 6. 4 w Ti II 1. 08 18

4488.764r 1 0. 2 4493.753r 9 2. 0

4488.912m 45 10. 0 s Vi fl. 85

11. 94

86

110 4493.952 19 4. 2 w

4489.101

A AOn 1 O A 44oy.lo4

A A on 0/ll_ 4489. o41r

4489.467

25

bl

6

17

6. 9

13. 6

1. 3

3. 8

s

AT w,N

u

Fe I

Ti I Fe II

Cr I

/2. 56

13. 65

1. 74

2. 83

/2. 71

13. 56

213

827

146

37

63

4494.062m

4494.196

4494.384r

4494.492r 4494.573m

4494. 739r

32

18

16

16

139

10

7. 1

S. S

3. 6

5. 1

37. 2

2. 4

u

s

Fe I p Na 1

Zr II Fe I p Fe I Co I

3. 98

2. 10

2. 41

2. 95

2. 20

3. 53

973

15

130

411

68

168

4489.602r 3. 5 0. 8 4494.867r 10 2. 2 4489.748m 81 18. 9 s Fe I 0. 12 2 4495.008m 12 2. 7 * Ti 1 4489.928 3. 5 0. 8 4495.15 a 4 0. 9 4490.089m 67 15. 4 s Fe I Mn I

3. 02

2. 95 46922

4495.267 8 1. 8 u Cri 4. 10 275

4490.234r

4490.397r

4490.543

7

1. 5

20

1. 6

0. 3

4. 4

Fe I p

|NiiCr I

2. 88

/3. 54

14. 17

3. 89

319

134 235

267

4495.575

4495. 757r

4495.961

24

5. 5

41

0. i

5. 3

1. 2

9. 1

u

u

u

ll-re I Zr II Fei

Fe I

/2. 88

13. 88

1. 21

3. 60

3. 65

319 970

79

827

825

168
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4496.157m 39 10. 2 s Til 1. 75 146 4502.052r 3. 5 0. 8

4496. 245r 9. 5 2. 2 s Til 0. 02 8 4502.221S 49 11. 8 s Mn I 2. 92 22

4496.377r 2. 5 0. 6 4502.441 7. 5 1. 7 u

4496.515 7. 5 1. 7 4502.600m 21 4- '9 u Fe I .3. 57 796

4496.661r 7 1. 6 4502.760 1 0. 2 4496.860m 79 21. 1 Cr I 0. 94 10 4503.063r 2 0. 4 Cn? 4. 70 310

4496.974 24 5. 8 u Zr II 0. 71 40 4503.320a 2. 5 0. 6

4497.103r 2. 5 0. 6 4503.354r 2 0. 4

4497.264r 1. 5 0. 3 4503.489r 0. 5 0. 1

4497.406r 4 0. 9

- 4503. 761r 8 1. 8 Til 2. 13 184 4497.680m 27 5. 2 s,N Na I 2. 10 15 4503.874 7 1. 6 u

4497.73 m s Ti I 2. 12 184 13 4504.059r 0. 5 0. 1

4497.865r 6. 5 1. 4 Ce II? 0. 96 19 4504. 206r 1 0. 2 Fe I p 3. 96 988

4498.000a 2. 5 0. 6 4504.542r 2 0. 4

4498.13 a

4498.296

2. 5

7

0. 6

1. 6 u

4504.737 4504.838m

]

\ 46

r 1. 8

I 8.

u

u Fe I 3. 26 555

4498.560r 8 1. 8 Fe I p 3. 88 988 4505.031r 4. 5 1. 0 Cai 2. 52 24

4498.732 21 4. 7 s Cri 2. 91 81 4505. 239r 4 0. 9 4498.900m 48 10. 7 s Mn I 2. 94 22 4505.482r |1| 0. 2

4499.036r 4 0. 8 4505.73 m 1 0. 2 s Til 2. 10 184 4499.143m 43 9. 6 u 4505.791 4. 5 1. 0 u

4499.360r 3 0. 7 4505.926r 2 0. 4 s Yi 1. 37 14

4499.501r 2 0. 4 Sm II? 0. 25 23 4506.093r |4| 0. 9 u,N

4499.68 a

4499.957r

4500.288

4500.369

4500.504r

4500.639

4500. 767r

4500.949r

1. 5

2. 5

1 39

1. 5

14

2

3

0. 3

0. 6

[ 6. 2

I 2. 4

0. 3

2. 9

0. 4

0. 7

sw

u

Cri

Fei

3. 08 150

4506.326

4506.452r

4506.608

4506.747

4506. 973r

4507. lOOr

4507.227

9

1. 5

7

7. 5

1

3

6. 5

2. 0

0. 3

1. 6

1. 7

0. 2

0. 7

1. 4

s

s

0

s

S

wl

Nil

|Tii

Ca I

Ti up

Cr T

Zr I Fe I

3. 54

2. 52

1. 13

4. 1 R

0. 54

3. 11

133

24

30

31

474

4501.102 27 6. 0 s Cri f2. 91

13. 55

81 4507.395 7. 5 1. 7 s Cai 2. 52 24

4501.278m 111 29. 1 w Ti II 1. 12 31 4507.754 3. 5 0. 8 s

4501.457 10 2. 2 u,N 4507.858 3. 5 0. 8 s Cai 2. 52 24

4501.651

4501.780

4501.990

8. 5

22

5. 5

1. 9

4. 9

1. 2

u

s

s

Cri?-

Nii

Cri

Vi

3. 56

3. 70

2. 91

1. 38

115

81

62

4508.011r

4508.084r

4508.289S

6

3. 5

74

1. 3

0. 8

17. 6

s

w

Ti I

Fe II

2. 78

2. 85 38

169
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent

VV IQUIl AX

(mA)

Re- duced

VV Itilll AX/X

(F)

Solar

Identification

Low

EP

or Rot.

Li 116

RMT

No.

or Vib.

"Rn n fl J_) ci li Ll

Wave1 oil o'l" n

(A)

Equivalent Width Win LIL AX

(mA)

Re- duced

VV ILl Hi AX/X

/T-^^ (F)

Snnt

Solar

It-lt li \jl fication

Low

EP

or Rot. Line

RMT

No.

or Vib.IN oijes

4508.472r

4508.550r

1 3

J

f 0. 3

1 0. 3

4514.432

4514.496

/ Do

[ 9. 3

I 6. 9 s? Cri 2. 91 95

4508.689 13 3. 1 w 4514.651r 2 0. 4

4508.97 a 1 0. 2 4514.791r 3. 5 0. 8 16

4509.128r 2 0. 4 Fe I p 2. 61 213 4514.968r 2. 5 0. 6

4509.290

4509.449 4509.742m

4509.995r

4510.178r

14

14

34

3. 5

1. 5

3. 1

3. 1

8. 0

0. 8

0. 3

U

SU

U

Fe I

Ca I

Cr I Pr II

/3. 05

13. 69

2. 52

4. 53

0. 42

514

937

24

20

4515.107r

t:0 10.1/0

TrtJlO.OrTOill

^010.T:TUr

trOi D.Dv 1 1

4

1 ^

1

)

U. 0

0. 9

^ 1 0. X

f 11.0 17 Q

\ 1 8

1. ri

1iw

s

0

Q , iNV

Sm 11

X e 1

1^ e TTn

^1 1

V 1 Til

9 ft J

0. Ul

11. oyQQ

2. 12

Q 1 0

0 i

1 9A

lUU 184

4510.830 8 1. 8 w?,N Fe I p 3. 60 823 4515.863 3. 5 0. 8 u,N

4510.96 m 0. 5 0. 1 4516.089r 1 0. 2 Fe I p 3. 25 639

4511.072 5 1. 1 w Fe I p 3. 94 970 4516.272 9. 5 2. 6 M Fe I 3. 60 819

4511.171 8 1. 8 s Til 4516.461 3. 5 0. 8 S Fe I p 3. 65 825

4511.31 m 2 0. 4 s In I 0. 27 1 4516.661 12 S. B u,N

4511. 350r 0. 5 0. 1 4516.928r 2 0. 4 u

4511.567

4511.82 m

8 1. 8 w,N

s 13

4517.089r

4517.154 1 28

[ 0. 7

\ 6. 6

M?U

Co I Fei?3. 13 150

4511.900m 31 8.4 s Cr I 3. 09 150 4517.305r 2. 5 0. 6

4512.062 4. 5 1. 0 u 4517.373r 1 0. 2

4512.273

4512.436r

18

0. 5

I 0

0. 1

s Cai

-' ,i

2. 52 24 4517.534S

4517. 598r

1 61

1 12. 4

1 1.1

u Fe I Fe I p

3. 07

3. 96

472

992

4512.497r 1 0. 2 4517.757r 2 0. 4

4512. 566r 1 0. 2 4517. 838r 3. 5 0. 8 Ni I? 3. 54 103

4512.741S 55 13. 6 s Til 0. 84 42 4518.032m 62 H. 8 S Til 0. 83 42

4512.997 16 3. 5 w Nix 3. 70 163 4518.183r 2 0. 4

4513.219r 2. 5 0. 6 Cr I? 3. 09 150 4518.342m 40 10. 0 u

4513.325r 3. 5 0. 8 4518.447 6 1. 3 M Fe I 3. 24 593

4513.437

4513.582

13

5

2. 9

1. 1

w

s Yi 1. 90 15

4518.587 14 3. 1 u,d Fe I Cri

2. 22

f 9

12. 97

69o4

100

4513.720

4513.872r

9

3

2. 0

0. 7

s |Tii

Fei

Ni I p Cri?

1. 43

2. 59

3. 54

3. 09

112 213

131 175

4518.700m

4518.861r

4518.982r

12

1. 5

1

2. 6

0. 3

0. 2

s Ti I

Mn II?

1. 43 112

4513.912r 3 0. 7 4519.08 a 1 0. 2 4514.193m

4514.320r

48

1

10. 6

0. 2

s

s

Vi

IIFei Cri?

1. 94

3. 05

4. 18

110 514

287

4519.299r

4519.458r

4519.637

1

0. 5

5

0. 2

0. 1

1. 1 s

Co I?

Sm II —

3. 71

0. 54 49

170
Ihe Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

lie- duced

Width

AX/X

(F)

Spot

Solar

IdcutificiUion

Low

EP

or Rot. Line

KMI) iXyf

No.

or

Vib. Banc

Notes

1

Wavelength

(A)

Equivalent Width

AX (mA)

Ki'y- ducod

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

4519.843r 3. .5 0. i5 M Cr I 3. 01 126 4524.944 32 7. w Ba II 2. 51 •J•J 4519.992

4520. 11 6r

30

1

6. (

0.

5 s Ni 1 1. 68 51 4525.146S

4525.245r 1 120

1 25. (

[ 0.C

) s

)

Fei 3. GO 820

4520.229m

4520.399r

4520.536

4520.62 a

69

3

6. 5

1. 5

16. i

0. 7

1. 4

0. 3

' w

u,N

|Fe n

Fei

Ti II p

2. 81

3. 07

1. 12

37

471

30

17

4525.616r

4525.72 a

4525.866

4526.103

2

1. 5

17

16

0. 4

0. 3

3. 6

3. 5

I

u,d

s

Fei

Cri

(La ii)

2. 88

3. 37

0. 77

319

196

50

4520.804r 1

f 0. 7

.1 4526.264r 2 0. 4 s

4520.966r

• 5

1 t 1 1

\ 0. 4

s I /4. 10

14. 18 277 287

4526.442

4526.568m

107

38

23. 6

8. 4

s

u

Fe I p —

ICn

Fe I

3. 88

2. 54

3. 11

969

33

471

4521.33 a 3 0. 7 4526.720r 3. 5 0. 8

4521. 432r 0. 5 0. 1 4526.788r 3. 5 0. 8 Co I 3. 71 177

4521.668r 0. 5 0. 1 Feip 3. 27 641 4526.933m 75 17. 4 s Cai 2. 71 36 4521.78 a 1. 5 0. 3 4527.165r 4 0. 9

4521.887r 4522 02qr

2

1- 5

0. 4

0. 3

NiiCr I

3. 74

3. 09

116

173

4527.325m 67 14. 8 S IITii |Cri

0. 81

2. 54

42

33

1 Oft

4522.120r

4522.252r

2

0. 5

0. 4

0. 1

fO. 00

11. 25

4527.468m

4527.640r

25

1. 5

5. 5

0. 3

s Til

Cri

0. 00

2. 99

782

4522.372 8. 5 1. 9 u La II 874 4527.788 21 4- 6 u Fei 3. 25 641 4522.528 4522.638m

101

\ 4. 6

J

[ 18. 8

uw

Fei

Fe II (Eu n)

2. 84

0. 21 384

4527.930r

4527.98 m

4. 5

1

1. 0

0. 2 s

Co I Fe I Vi

3. 05

3. 64

156 897

4522,807m 65 15. 5 S Til 0. 82 42 4528.05 a 2 0. 4 Si I

4522.950r 1 0. 2 4528.143r 4. 5 1. 0 4523.080 12 2. 6 u Ce II 0. 52 2 4528.306r 4. 5 1. 0

4523.246r 4523.407m

4523.585r

1. 5

36

3. 5

0

0. 3

8. 2

0. 8

1. O

s s,N

Fei

JNl I.f

3. 65

/3. 54

14. 23

829

99

4528.484

4528.627m

4528.768

4528.824'

, 275

' 7. 3

43. 0

8. 4

. 8. 4

w?,N

S

u

u

Ce II- Vii

Fei

Fe I p Fe I p

0. 86

2. 27

2. 18

3. 30

3. 02

1 56

68

595

468

4523.924 11 2. 4 u Sm II 0. 43 41 4529.018r 3 0. 7

4524.096r 5. 5 1. 2 V Fe I 16 4529.227r 2. 5 0. 6 4524.223 8 1. 6 s Vi 1. 89 99 4529. 315r 2. 5 0. 6 s Vi 1. 89 95

4524.418r 2 0. 4 4529.492 13. 0 u Ti 11 1. 57 82 4524 SlQr

4524.691

4524. 843r

1. 5

18

8

0. 3

4. 0

1. 5

u

u

Ti II Cri

1. 23

4. 10

60

276

4529.686m

4529.852

99

55

15

i i. u

8. 8

3. 3

11

u

s

r e I (Vi)

Fe I Cri

0. CO

1. 87

2. 54

007 yo / 99

33

Notes

761-925—66 -14 171
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar EP No. Wave- valent duced Solar EP No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes

i-i A AX/X fi fr» f i on Rot. Vib. AX AX/X iIKjcI null (A) (ml) (F) Line Band (A) (ml) (F) Line Band

^DO\j .yjyjoi 0 1 yj. X 1

1' 16. 3 T' T fl 89 49 147

1 4530.16 a 1 0. 2 4536.054m 1 [ 16. 3 s Til 0. 81 42

4530.338r 1 0. 2 4536.209r 1. 5 0. 3

4530.500r 3 0. 7 s 4536.364r 4 0. 9 s?

4530.698r 1

f 7.1 s? Cn 2. 54 33 4536.504 10 2. 2 u Fe I 3. 64 896

76 1 (Cri) 3. 32 190

4530.738 J i 12. 8 s Cr I 2. 54 33

4536.75 a 1 0. 2 4530.955m 69 15. 2 Co I 2. 93 150 4536.907r 1 0. 2 4531.158m 106 23. 4 S Fe I 1. 48 39 4537.05 m 2 0. 4 s 4531.350r 2 0. 4 4537.221r 5 1. 1 s Til

4531. 457r 2 0. 4 Fe I 4537.424r 3 0. 7 u

[3. 21 555

4531. 631S 55 13. 2 Fe I 3. 63 847 4537.676 13 2. 9 s Fe I 3. 27 594

[3. 93 992

4537.818r 1. 5 0. 3 s,N Ti I? 4531. 806r 1. 5 0. 3 4537.970r 4. 5 1. 0 u Sm 11 0. 48 45

4531.907r 2 0. 4 u

4538.12 a 0. 5 0. 1 4532. 138r 2 0. 4 s (Vii) 3. 80 212

4538.371r 1. 5 0. 3 4523.317r 2 0. 4 4538.466r 2 0. 4 4532.50 a 1 0. 2 4538.597 9. 5 2. 1 u,d? Fe I p 3. 98 972

4532.776r 4 0. 9 M Cr I 3. 42 212

4538.758

]

^ 5. 3 u Fe I 2. 28 115 4532.968 ]

f 8. 8 U 51 72 1

J 4538.843 J 6. 4 u Fe I 3. 94 969

4533.046 ] [ 7.5 U Fe I? 4538.956r 2. 5 0. 6 u Fe I p 4. 19 1048

4533.249m 90 20. 9 S Til 0. 85 42 4539.094 4 0. 9 s Til

4533.542r 2 0. 4 4539.250 5. 5 1. 2 u

71 Qr Qu 4539. 397r 2. 5 0. 6 109 24. C Ti1 J 11Ti 1 94. 1. 4539.593 12 2. 6 w,N

4^1 rxOO^. 11 711 Xiii m 1 1 7 to JTTpfc; TTli o / 4539.777 37 8. 1 s Ce II- 0. 33 108

4'i^4 '^7 n \ 0 9 II Cr I 2. 54 OO

4534.478r 3 0. 7 4539.999r 2 0. 6 s Vi 1. 89 100

11. 9 T e I p4 4'? I 1 i\Q I I oy 4^140 91 7r 2 0. 4 s

SI s Ti T n R4 49 rtOTiU.^ AKACi 97ar / OI 11 0. 2

4534.984r 4 0. 9 4540.406 2. 4 s 17

Oft ft0. fu oo 'iO'lU.OUDIil J 10. 1 s 9 fi4 oo

4535.322 12 2. 6 W 4540.710m 52 s Cri 3. 10 150

4535.447r 1 0. 2 4540.873 9. 5 2. 1 s,N Til 1. 44 112 4535.576m 79 19. 8 s Til 0. 83 42 Cr T [2. 99

13. 10 82

150

(2. 54 33 4541.068 22 5. 3 s Cr I 2. 54 33

4535.712 84 18. 5 u |Cr I- 2. 54 33 7

14. 10 276 4541. 185r 2. 5 0. 6 s 16 Zri 0. 52 30

4541.318 17 3. 7 w Fe I 3. 25 640

4535.86 m s Ti I p 1. 44 112 13 4541.35 m s 13

172
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4541.523S

4541.61 m

4541.656r

4541. 809r

4541.943

4542.067r

4542.234 4542.433m

4542.617

4542.704

4542.845r

4542.90 m

4543.035r

4543.13 m

4543.229

4543.740

4543.818 4544.022m

4544.198r

4544.281

4544.488r

4544.621

4544.694

58

3. 5

3

8

2

4. 5

40

1. 5

0. 5

1

1. 5

3

3. 5

14

35

0. 5

1

8

11 97

12. 8

0. 8

0. 7

1. 8

0. 4

1. 0

8, 8

1

^'

[ 3. 7

0. 3

0. 1

0. 2

0. 3

0. 7

0. 8

3. 1

7. 7

0. 1

0. 2

1. 8

r 11.

1 13. 9

w

s

w

s

s u,N

s

u

s

s u,N

s

u,dw

u

u

s

Fe II (Cr I) Nai

Fei

Zr I Fe I Cn

Fe I

Fe I p Cn

Co I

Ti IIFe I p Cn

Ti I

2. 85

3. 08

2. 10

3. 27

0. 63

3. 64

/3. 09

14. 10

3. 69

3. 64

2. 98

2. 72

1. 24

3. 98

2. 54

0. 82

38

149

14

593

49

894

149 275

827

893

100

142

60

970

33

42

13

17

4546.679

4546.807r

4546.934

4547.022

4547.232

4547.30 m

4547.418r

4547.646r

4547.853S

4547.996r

4548.132r

4548.20 a

4548.445r

4548.583

4548.770S

4548.900r

4549.018r

4549. 104r

4549.189

4549.283 4549.474m

4549.638m

4549.820

7. 5

1

1 92

1

1

73

3

3

0. 5

2

6

63

2

1. 5

2. 5

1 33

231

1

53

1. 6

0. 2

1

8. 8

[ 13. 0

1 7. 0

[ 0. 4

0. 2

0. 2

17. 6

0. 7

0. 7

0. 1

0. 4

1. 3

U. 5

0. 4

0. 3

0. 6

[ 5. 0

f 18. 2

1 32. 5

11. 6

u

sw

s

u

s

s

s

w,N

S

0uw

w

u

Fe I p Nb I? Ni I Fei

Ni I

Ti I?

Fei

(Til)

Ti I

Ti I

Fe II

Fe II

Ti II (Co I)

Ti II p

3. 96

0. 20

4. 16

1. 56

3. 63

.3. 55

2. 48

2. 49

0. 83

5. 91

2. 83

1. 58

3. 07

1. 18

989

261

39

146

755

270

270

42

186

38

82

150

39

4544.841r 3 0. 7 4549.992r 2 0. 4

4544.971 9 2. 0 u 4550.121 15 3. 3 u 4545.143m 42 10. 6 u Ti n 1. 13 30 4550.274 6 1. 3

4545.338

4545.397

1

} "

[ 4. 6

1 2. 0

1 [ 1 B,d

1 Cn

Vi

2. 54

1. 95

33

109

4550.431r

4550.573r

1. 5

1. 5

0. 3

0. 3

4545.545r 2 0. 4 Fe I p 3. 64 894 4550.773S 72 16. 0 w Fe I

4545.602r 1. 5 0. 3 4550.969r 3. 5 0. 8

4545.693r 2. 5 0. 6 Ir I? 1. 62 4551.091r 1. 5 0. 3

4545.815r 3 0. 7 4551.228 23 Jf. 9 11,

d

Ni I 4. 17 236

4545.962m 73 17. 4 Cr I 0. 94 10 4551. 521r 0. 5 0. 1

4546.108r 2. 5 0. 6 4551.654 23 5. S u Fe I 3. 94 972

4546.260r 1. 5 0. 3 4551. 848r 1 0. 2 s Vi? 1. 80 82

4546.476 5. 5 1. 2 u Fei 4. 19 1047 4552.144 20 4. 4 w'!,N

173
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

oolar

Identification

Low

hi r

or Rot. Line

RMT

JN 0. or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

bolar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

4552.293 27 5. 9 u Ti II? p 1. 12 30 4558.113m 19 4. 2 s |Fei (3. 64

13. 98

894

974

4552.463

4552.549

4552.653r

4552.894r

1 109

3

1

[ 15. 4

I 10. 3

0. 7

0. 2

s

u

Ti I Fe I Sm n0. 84

0. 25

42

23 4558.226

4558.470

7

5

1. 5

1. 1

w

XL

Til

Vii

La II

/2. 34

12. 34

3. 80

0. 32

262

263

212

39

4553.048r

4553.174

4553.375r

4553.625r

4553.838r 4554.036m

4554.252r

4554.313r

2

12

3. 5

3

1. 5

159

1. 5

1. 5

0. 4

2. 6

0. 8

0. 7

0. 3

36. 7

0. 3

0. 3

s

w

s

Zr IVi

Ni I

Ba II

0. 52

2. 36

3. 66

0. 00

31 133

135

1

4558.650m

4558.774

4558.930

4559.353

4559.556r

4559.72 a

4559. 808r

4559.930

66

8

1

1. 5

0. 5

2

1

18

15. 4

1. 8

0. 2

0. 3

0. 1

0. 4

0. 2

3. 9

w

s

Cr II

Til

(Nil)

4. 07

1. 46

3. 54

44

112

115 4554.460m 26 5. 7 s Fei 2. 86 319 4560.097m 42 9. 2 u Fe I 3. 60 823

4554.536r 4 0. 9 s Ru I 0. 81 5 4560.278 13 2. 8 u Ce II 0. 91 8

4554.698r 1. 5 0. 3 4560.417r 1. 5 0. 3 s

4554.834 7. 5 1. 6 s Cri 3. 11 173 4560.568r 2 0. 4 4554.992m 39 8. 6 w Crii 4. 07 44 4560.720 7. 5 1. 7 s Vi 1. 95 109

4555.092

4555.295 4555.492m

4555. 658r

4555.738r 4555.892m

4556.137m

8

3. 5

54

2. 5

3

77

100

1. 8

0. 8

13. 2

0. 5

0. 7

16. 9

21. 9

s

s

s

sw

u

Ti I Cri

Cri

Til

Fe I p

Fe II

Fe I

(Cr 1)

2. 41

3. 10

3. 43

0. 85

3. 27

2. 83

\2. 95

3. 60

[3. 94

3. ]1

266

149

212

42

640

37

410

820

974

173

4560.869

4560.966

4561.192 4561.417m

4561.731

4561.985

4562.234r

4562.367

4562.477r

14

4. 5

6

28

4

1

0. 5

17

1. 5

3. 1

1. 0

1. 7

6. 1

0. 9

0. 2

0. 1

3. 7

0. 3

w

uu,N

u

s

u

s

Fe I? Ce II

Fe I

Ce 11

0. 68

2. 76

0. 48

2

1

4556.377r 2 0. 4 4562.637m 8 2.4 S Til 0. 02 7

4556.547r 2 0. 4 4562.885 1.5 0. 3

4556.760 1 0. 2 4563.08 a 1. 5 0. 3 4556.932m 21 4. 6 s Fei 3. 25 638 4.563.237 6 1. 3 s Cri 3. 85 246

4557.088 1. 5 0. 3 4563.427m 11 2. 4 s Ti I 2. 43 266

4557.284 26 5. 7 w,N Fei 4563.66 m S Cri 3. 09 172 13

4557.520 1. 5 0. 3 4563.766S 120 28. 0 w Ti II 1. 22 50

4557.62 a 1 0. 2 4563.886 6 1. 3 u,N

4557.754 3. 5 0. 8 4564.031r 2. 5 0. 5 4557.867m 5. 5 1. 2 s Ti I 2. 47 270 4564.173 13 2. 8 u Cri 4. 78 312

174
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

til r

or

ItOt. Line

RMT

JN 0. or

VlD. Banc

Notes

4oDy.5zo 1 AlU 2. 2 s Cr I O 1 o

o. 12 173

4oDy.olo O A z4 5. 1 8 Or I o. 12 1 TO 173

A cert ocir\^ 4oDy.»zUr 1 0. 2

45 /U.UZO 0 1. 1 U,I\ <../0 I — o. d3 1 TO 17o

/I c 'rn on ^ 0. 5 A 1 U. 1

4o/U.oo/r lol A A U. 4

n AT S,l\ — VI 1. JO 1 AO iuy

4o/u.DUyr Z A A U. 4

4o/u.yia D. 0 i. 4 s III Z. 4U ZDD

A d1 1AOO s Mg I A OA U. UU 1

45/ l.zysr A4

A n u. y

4571.444 18 3. 9 u Fei 2. 87 319

45/ 1.548r U. 0 A 1

4571. D75m onoy

o c

5. 0 s O C^A 2. 54 OO32

4571.803 14 3. 1 5 iVi

Cri

1. 94

f f} in

i o. lU

13. 85

109

1 /I A i4y

246

4571.982S 126 29. 7 W Ti II L 57 82

4572. 194r 5 1. 1 s Cn f3. 32

I.O. SO

190

OA A Z40

C 'TO OO /I 457z.zo4 1 Q *3 o. O u Ha TT \jQ II AU. Do 1

A C TO /I 00_ 457/.4z»r O K

Z. 0 u. 0

A CTrt c AO 4572.590 4. 0 i. U 3,0,1 1 T"

A CTO m « 4572.70 a

QO U. /

C TO O /I 4572. sd4 1 1 i i O A

Z. 4 w? T?Q T

-T e I — O. DO 1 7

/I c TO n /I . 457/. 94 m U. o

co

4573.Uoyr U. 0 u, i

4573.09 m Nb I? 0. 27 13

4573.656r 0. 5 0. 1 Si I

4573.790 2 0. 4

4573.996r 3 0. 7 s Sci?

Si I? 4574.225m 33 7. 2 Fei 3. 21 554

4574.365r 1. 5 0. 3

4574.483 5 1. 1 Zr II C^r I

2. 43

O AO

3. (Jo 139148

4574. 5D7r A K

U. 5 A 1

4574.728m 52 11. 4 s Fei 2. 28 115

4574.902 9. 5 2. 1 La II — 0. 17 23

4575.113 9 2. 0 Cn 3. 37 196

4575.230r 1. 5 0. 3

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RM^

No.

or

Vib. Banc

4564.23 m s Til 1. 46 112

4564.329 5. 5 1. 2 w

4564.457r 4. 5 1. 0

4564.578 14 3. 1 w Vii 2. 27 56

4564.702 30 6. 6 w,N Fe I 3. 65 823

4564.828 24 5. 2 u Fei 3. 07 472

4565.043r 3 0. 7 Ci?p 7. 48

4565.15 a 2. 5 0. 5 Ni I p 3. 40 88

4565.316 26 5. 7 u Fe I 3. 27 641

4565.418 26 5. 7 u Zr 11? Ni i?p1. 77

3. 38

116

99 4565.518m 67 14. 7 s Cr I (Coi)

0. 98

3. 02

21 150

4565.668

4565.729 J

[ 14. 9

1[ 3. 1

u

u?

Fei

Cr II?

3. 24

4. 04

554

39

4565.856 5 1. 1 Ce II 1. 09 21

4566.026r 1. 5 0. 3 Fe I p 4. 47 1169

4566.233 7. 5 1. 6 u,N Sm II — 0. 33 32

4566.383r 0. 5 0. 1 4566.524m 36 7. 9 u Fei 3. 30 641

4566.662r 5 1. 1 Fe I p 2. 56 212 4566.873m 40 8. 8 w Fe I

4566.993 17 3. 7 s Fe I 3. 41 723

4567.173r 0. 5 0. 1

4567.28 a 1. 5 0. 3

4567.409 2 0. 4 u Ni I 3. 54 102

4567.583r 2 0. 4

4567.745r 0. 5 0. 1

4567.89 a 1 0. 2

4568.043 1. 5 0. 3

4568.20 a 3 0. 7 4568.328m 25 6. 1 w Ti II 1. 22 60

4568.50 a 3 0. 7

4568.608 14 3. 1 u Fe I p 3. 93 989

4568.771

4568.855

60

r 9. 6

I 5.

w?uFei

Fei

3. 26

3. 63

554

894

4569.071r 3 0. 7 u Fe I p 3. 27 593

4569.253r 2 0. 4 Co 11

4569.360 5. 5 1. 2 u

Notes

13

175
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Vv^idth AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4575.42or

4575.48 m

4575.546

4575.790

5

10

15

1. 1

2. 2

3. 3

(S

s

u

Zr I

Fei

0. 00

/3. 30

13. 88

5

593

970

13

4581.046

4581.196

4581.30 m

4581.406

3. 5

22

]

0. 8

4. 8

f 21. 8

s

w

s

s

Cn

Fe I Yi

Cai

/3. 01

13. 09

1. 90

2. 52

125

148

15

23

13

4575.924r 2 0. 4 4581.519 i 201 1 21. 8 u Fe I 3. 24 555

4576.096r 0. 5 0. 1 4581.630 j [ 4. 4 u,N Co I 2. 96 150

4576.339S 56 12. 4 w Fe II 2. 84 38 4581. 835r 5 1. 1

4576.517 6. 5 1. 4 s Ti I 2. 33 262 4582.075 5 1. 1

4576.597r 2. 5 0. 5 4582.309 16 3. 5 w Fe I

4576.785r 1 0. 2 s Cn 3. 08 148 4582.43?m 3 0. 7 s 16

4577.009r 2 0. 4 4582.510 4 0. 9

4577.184 25 5. 9 S Vi 0. 00 4 4582.679r 1. 5 0. 3

4577.331 3 0. 7 4582.833m 49 10. 7 w Fe II 2. 84 37

4577.484r 1. 5 0. 3 u 4582.952 6 1. 3 u Fei 2. 84 348

4577.694 4 0. 9 u Sm 11 0. 25 23 4583.123 10 2. 2 u

4577.816 1. 5 0. 3 4583. 251r 0. 5 0. 1

4578.047 3 0. 7 u,N 4583.415 25 5.4 u Ti II 1. 16 39

4578.326 4. 5 1. 0 s Cri 3. 85 246 4583.576r 2 0. 4

4578.47m

4578.559S 73 15. 9

S

s Cai 2. 52 23

13 4583.724 4583.839m 1 124

1 2. 8

[ 24. 2

swFe I Fe II3. 11

2. 81

472

38

4578.732 11 2. 4 s Vi 1. 94 109 4583.90 m s Cn 3. 01 125 13

4578.890 3 0. 7 u 4583.992 16 3. 5 0? Fe 11 p 2. 70 26

4579.054

4579. 187r

4579.338m

4579.514

4579.687

4579.820

4579.908r 4580.062m

4580. 154r

4580.291r 4580.414m

4580.589m

4580.739r

4580.881

12

1. 5

22

3. 5

7. 5

20

3. 5

80

7

1. £

42

40

4

3

2. 6

0. 3

4. 8

0. 8

1. 6

4. 4

0. 8

17. 6

1. S

0. 3

9. 8

8. 7

0. c

0. 7

u,d

s

u

sw

w,N

S

s

S

u

Fe I p

Fe I p Vi

Fe I

Fe I p Fei

Cn

Co I

Vi

|Fei

Ni I

3. 27

3. 88

1. 95

/2. 83

13. 69

3. 64

3. 07

0. 94

0. 92

0. 02

3. 65

3. 65

640

988

109

319

936

894

469

10

27

4

827

146

16

4584.090

4584.274

4584.443

4584.726

4584.824m

4584.945r

4585.079

4585. 195r

4585.343

4585.597

4585.698

4585.874

4585.973

4586.144

11

2. 5

1. 5

32

49

5. 5

5. 5

1. 5

14

2

3. 5

1 134

15

2. 4

0. 5

0. 3

7. 0

10. 7

1. 2

1. 2

0. 3

3. 0

0. 4

0. 8

1 23. 5

1 6. 8

3. 3

s,d?

su

u

s

u

w,N

s

s

s

Cn

Ru I

IIFei Cn

Fe I Cn

Cn

Fe I Fe I p

Si I Cai

Vi

Cai?

Cn

3. 12

1. 00

3. 60

3. 01

3. 60

3. 37

3. 45

3. 02

2. 52

1-35

2. 52

3. 11

172

5

820

125

822

196

212

468

23

61

23

172

176
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4586.234 38 8. 3 w 4592. 219r 3. 5 0. 8 4586.378m 38 8. 7

ry V I 0. 04 4 4592.355 12 2. 6 w,N

4586. 543r 0. 5 0. 1 4592.531m 67 14. 6 u Ni I 3. 54 98

4586.721 0. 5 0. 1 4592.659m 95 20. 7 s Fe I 1. 56 39

4586.93 m s 11 I P 2. 43 266 13 4592. 816r 3 0. 7

4586.994 9. 5 2. 1 Cr I.' 3. 01 126 4592. 928r 2 0. 4

4587. 134S 46 10. 0 M Fe I 3. 57 795 4593.170 6. 5 1. 4 u

4587.396 3. 5 0. 8

A p r\f^ coo 4593.533m 22 4. 8 u Fe I 3. 94 971

4587.602 7 1. 5 4593.709r 1 0. 2

4587.723 14 3. 0 M Fe I p 3. 98 971 4593.832 10 2. 2 u Cr I 3. 32 190

4587.878r 2. 5 0. 5 Cn 3. 01 125 4593.935 12 2. 6 u Ce II 0. 70 6

4588.006r 4588.204m

4588.400

A COO COO— 4588.o23r

>4 ET o o z? o ri 4588.682

3

66

2

1. 5

12

0. 7 n. 4

0. 4

0. 3

2. 6

W

M

Cr 11 4. 07 44

4594.126m

4594.285r

4594.416r 4594.50?m

46

1. 5

1. 5

10. 0

0. 3

0. 3

S

s

Vi

(Eu i)

Cr I?

Ti I p

0. 07

0. 00

2. 34

4

1

262 13

4588.76 m 1. 5 0. 3 S Co I 0. 43 15 4594.639 10 2. 2

1I u

1 CoiJ 3. 63 176

4589.017 2 0. 4 u,iy 4594. 790r 1 0. 2

i4 ET Ork C\C\ A 4589.294 3. 5 0. 8 u 16 A d f\ A OCX A 4594.894 26 5. 6 u Ni I

4589.36 m 0. 5 0. 1 8 4595. 052r 4. 5 1. 0 s Cr I 3. 32 190

^ c or* CI 4589. 512r 0. 5 0. 1 4595.216 10 2. 2 u Fe 1 p 3. 63 846

A c or» o_ 4589.738r 2 0. 4 4595.365m 61 13. 3 s Fe I 3. 30 594

/(Cor\ recoct 4589.953S 70 15. 9 W — Ti II 1. 24 50 4595.476 8. 5 1. 8 u

4590.072r 5. 5 1. 2 4595.593 21 4. 6 s Cr I 4. 18 286

4590.216 2 0. 4 4595. 690r 8. 5 1. 8 Fe II p 2. 85 38

A ^ C\C\ ^ A C\ 4590.340 1 0. 2 Mo I? 4595.88 m 3. 5 0. 8 s

A ^c\r\ A r\ A 4590.494 1 0. 2 V II? 3. 79 210 4595.956 34 7. 4 u Ni I 3. 42 101

4590.55 m s Zr I 0. 54 31 13 4596.069m 61 13. 3 u Fe I 3. 60 820

4590.677r 2 0. 4 s Cr I 3. 01 125 4596.242 3 0. 7

4590.793 25 5. 4 w Fei 4596.416m 29 6. 3 u Fei 3. 65 823

4590.945 3. 5 0. 8 4596.578 6 1. 3 u

4591.113 4. 5 1. 0 u 4596.682r 2. 5 0. 5

4591.247r 4591.400m

4591.520m

4591.737r

4591.850 4592.057m

2. 5

59

34

1. 5

1. 5

44

0. 5

12. 8

7. 4

0. 3

0. 3

9. 8

s

s

u

w

Vi

Cn

Fei

Sm n?-

Cr II

2. 37

0. 97

2. 76

0. 18

4. 07

133

21

14

44

4596.905

4597.036r

4597.255

4597.383

4597.601

14

5. 5

18

23

6

3. 0

1. 2

3. 9

5. 0

1. 3

u

s

u

us,N

|Coi

Cr I? Fe I p

Fei

3. 63

3. 09

0. 99

177

171

17

177
The Solar Spectrum—Continvied

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

4597.754 36 7. 8 w 4603.490r 1 0. 2 4597.876m 44 9. 6 u 4603.620 1. 5 0. 3

4598.125S 76 16. 5 s Fei 3. 28 554 4603.729 2. 5 0. 5

4598.364

4598.437r

4598.617r

4598.745

4599.008r

4599.227

4599.577

4599.74 a

4599.79 m

4599.843m

4599.970 4600.107m

4600.204 4600.364m

4600.562r 4600.757m

4600.938

4601.025

4601.144

4601.270

16

6

2

12

2

6

1

3

56

1. 5

28

12

53

4. 5

80

26

27

7

7. 5

3. 5

1. 3

0. 4

2. 6

0. 4

1. 3

0. 2

0. 7

12. 2

0. 3

6. 1

2. 6

11. 5

1. 0

18. 2

5. 6

5. 9

1. 5

1. 6

s

s

u,du

s

s

u

suw

s

u

s

s

Fe I p

Fe I p Cn

Fei

Cr I Ti I p

Ti I

Cn

Vii

Ni I

Cn

Fe I Cn

Cr I

Si I

0. 96

3. 94

3. 11

3. 69

3. 09

2. 33

2. 54

2. 26

3. 60

1. 00

3. 24

2. 54

3. 12

5. 08

17 970

172

819

171 262

32

56

98

21

591

32

172

13

4603.852

4603.953

4604.13 a

4604.239

4604.405r 4604.560m

4604.688r

4604.852 4604.996m

4605.104

4605.255r

4605.357

4605.466 4605.594m

4605.75 a

4605.844

4606.014

4606.12 m

4606.226m

4606.396

10

15

1. 5

5

1

37

6

10

62

8

3. 5

19

15

40

2

10

2. 5

3

39

9. 5

2. 2

3. 2

0. 3

1. 1

0. 2

8. 0

1. 3

2. 2

13. 5

1. 7

0. 7

4. 1

3. 2

8. 6

0. 4

2. 3

0. 5

0. 7

8. 5

2. 1

uu

sSw

s?u

s

uuw

s,dl

S

u

u

Fei

Fe I p Zn

-Fe I (Cn)

Fe I Nil

Fe I Fei?

-Mn 1

Fei

La 11

Fe 1 p

Vi

Nil

CriCe II

2. 99

2. 83

0. 52

3. 32

3. 63

3. 48

2. 86

4. 72

0. 71

3. 64

0. 02

3. 60

4. 45

0. 91

410

348

29

190

846

98

348

52

893

4

100

303

6

4601.376 7. 5 1. 6 0 Fe II p 2. 89 43 4606.511r 3 0. 7 Sm II 0. 00 1

4601.556 1 0. 2 4606.797 5. 5 1. 2 s,dl Nb I 0. 35

4601. 742r 0. 5 0. 1 4607.087 3. 5 0. 8 w Fe I p 3. 41 724

4601.838r 0. 5 0. 1

- 4607.217 1 0. 2

4602.008S 60 13. 0 s Fe I 1. 61 39 4607.338m 36 7. 8 s Sri 0. 00 2

4602.181r 2 0. 4 4607.511 4. 5 1. 0

4602.389 1 0. 2 4607.654S 75 16. 3 u Fe I /3. 26

13. 98 554

969

4602.542r 3 0. 7 s Cn?-

Zr I?

3. 45

1. 87 2104607.856 8. 5 1. 8

4602.756 5. 5 1. 2 Fe II? p 2. 54 19 4608.126 3 0. 7

4602.949S 97 22. 2 s Fe I 1. 48 39 4608.230r 1. 5 0. 3

4603. 107r 10 2. 2 4608.709 4 0. 9 0

4603.20 a 3 0. 7 4608.842 4. 5 1. 0

4603.348 14 3. 0 s,d Si I Fe I p 2. 84 348

4608.98 a 2 0. 4

1"!8
The Solar Spectrum—Continued

length

(A)

EquiV tllcll li Width

A \ ISA (mA)

Retlucecl Width

ii A/ A

(F)

Spot IdentiLow

Jjj X or

XVOL. Line

RMT

IN 0. or

Vi'h Band

Notes length

(A)

liquiVlll(?Il t Width

(mA)

Width

A \ f\ iiA/ A

(F)

Spot IdentillCrt LlUll

Low

Jli X or

Pr.t iwOL. Line

RMT

N 0. or

V ID. Band

1 1 i i 9 4 0 Ti TT rt 1X. ISxo 0 J u. 0 Sni II fl tiJ. 4Q

0

1 1 1 . X s Ti I T vj i tj . 'J u m 9 u T

^Duy.0 4 ur 9 fl 4 A(\^ 'iU 1 u. 79nr # >^ VJl 0. 0 1.1 s0 s fem II flU. 11 0J 99

^Duy.00 /

9 flu. 0 s VV XT 1. 00 \) X

c: 000,.

99 4 8 to Ni I? 4 flQ r±U-lU. 10^ III 71# X 17 1 0 Prv>i T1fl0. OSyo 91

AfinO rk\J\JiJ .cfQ71 m111 X 0

A.A1 9Qfir 1 1 X. X

rtOiu.Uy il Q fl 7 Au. y

1 1 ± 1 2. 4 1X 71 rrU XU . U.iiOlll •^7 0.R n\j w Cr TT 4 fl7 AA

q n 7 'ioxo. < '± / r 0. 0 n ft U. 0

4fii n f^Qf^r f) ttUX 7I .UUol OASir X. 0 u. 0

4610.941 3 0. 7 s Vi 1. 04 39 4617. 276S 49 If. 1 s Til 1. 75 145

4611.070 r 3. 2 u Fe I p 3. 30 641 4617. 460r 4 0.

4611.194 1131 i 4. 3 u Fe I p 2. 85 319 4617.870 6 1.

u

4611.290

4611. 488r

*±\J X X ,\J^\JX

12

0. k)

\J, 0

u. 0

0. U

I 22. 8

2. 6

X.1 s0

1X. 4a:

1X. 4T:

fl S

s Fe I (Feip)

PrXL 11TT?I

3. 65

3. 65

'?7 0. 0 i

fl fin

826

819

xyo

4617.967

4618.127r

4618.360r

4618.512r

4618.60 a 4618.792m

7. 5

2

3

4

1. 5

78

1. 6

0. 4

0. 7

0. 9

0. 3

16. 9

u

w,d

Ni I

Fe I p Fe ICrv^x TT11

3. 77

4. 31

2. 95

4 fl7

115

1151

409

Ad.

fl Q 0<J fl jtt 1

X 1 4fi1 ^uxo.yoox S QliSr 7 1. 0

4612.470r 2. 5 0. 5 s,d? 17 4619.110r 3 0. 7

4612.611 8 1. 7 u Fe I p 2. 83 349 4619.297m 70 15. 2 s Fe I 3. 60 821

4612.749r 3. 5 0. 8 4619.432 3 0. 7

4612.952 4613.213m

4613.367m

4613.562r

4613.713 4613.921m

4614.208m

12

66

62

7

11

29

27

2. 6

14. 3

13. 4

1. 5

2. 4

6. 3

5. 8

u,N

u

s

u

su

s,d

Fe I Cri

Zr II CnX L. i

3. 29

0. 96

0. 97

3. 10

"i '^fi

554

21

67

148

4619.539m

4619.677r

4619.780

4fi1 Q eQ7r ARon 1 QO ^O^iU.XOZI

4fl9fl 947

4R9fl t;9flm

33

3. 5

6. 6

9 f\

0

0

4.7

7. 1

0. 8

1. 6

fl 1^

1. 1

1 1 1. 1

If) /

s

sS

U

XI w

Ti I |Cr I Vi

Vi

\j2L II F6 I p — J-M I

T?0 r TT e II

2. 33

2. 99

0. 04

X. i 0

fl7

0. Do

9Z. 00

261

81

4

7fi / u

4fiQ

1IDoR'i

00

rrOl^. OOor 1. 0 u. 0 ^o.iU.oi ir I. 0

fl Q U. 0 Pr» T \yO I 9 79

4.fi14- '^'^4. rt\j X^.OO^ J 1 1 s Cr T 0. oO 94 4f\91 fl99 9 fl 4 0 I Pr T ^9

4614. 585r 5 1. 1 u Ni I 3. 60 99 4621.124 3 0. 6

4614.726 5 1.

s Cn 3. 37 196 4621.35 a 1. 5 0. 3 Mgi? 2. 71

4614.938r 1.

0. 3 4621.479r 2. 5 0. 5 Si I

4615.20 a 1 0. - 4621.618 2. 5 0. 5 Fe I p 3. 96 981

1719
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

4621.770 0. 5 0. 1 4627.549 12 2. 6 N,s'! Fe I 3. 30 593

4621.888 f 3. 2 s Cri 2. 54 32 4627.654r 2. 5 0. 5

4621.942

4622.132r

4622.258r 4622.453m

4622.558r

4622.751

4622.896r

4623.02 a 4623.101m

4623.303

4623.578

4623.878r

4624.083

4624.269

4624.419r

4624.558

1 45

3. 5

2. 5

33

8. 5

20

4. 5

3

46

4

17

0. 5

8

1. 5

6

6. 5

1

0. 8

0. 5

7. 1

1. 8

4. 5

1. 0

0. 6

11. 0

0. 9

3. 7

0. 1

1. 7

0. 3

1. 3

1. 4

s

s

s

S

u

w

s

u

Cr I

Cn

Cri

Co I Til

Vi

CoiCr I?

f2. 54

13. 85

3. 55

2. 99

3. 19

1. 74

1. 05

2. 72

32 244

233

81

156

145

39

141

4628.160

4628.276

4628.457

4628.685r

4628.917r

4629.064 4629.342m

4629.533

4629.669r

4629.804r

4629.950r

4630.128S

4630.407r

4630.563

4630.783

4631.036

14

2

6

3. 5

7

5

80

11

2. 5

4

5. 5

61

4

14

3. 5

7

3. 0

0. 4

1. 3

0. 8

1. 5

1. 1

18. 1

2. 4

0. 5

0. 9

1. 2

13. 6

0. 9

3. 0

0. 8

1. 5

u

s

s,N

s

s,d

u

w

0

0

Ce II

Cri

Fei

Co I

Zr II

ITii

|Fe II- Co I

Zn I Ni I p Fe I

Fe I Fe I p

0. 52

3. 14

3. 69

0. 51

2. 49

1. 73

2. 81

3. 05

5. 79

4. 09

2. 28

3. 94

4. 10

1

186

819

15

139

14537

156

8

223

115

969

1 AT 1 1071

17

4624.748r 4 0. 9 4631.212 2. 5 0. 5

4624.901 6 1. 3 Ce II- 1. 12 27 4631. 337r 0. 5 0. 1

4625.052S 76 17. S s? Fei 3. 24 554 4631.484 10 2. 2 w Fe I /4. 37

14. 55

1152

4625.203r

4625.314r

4625.441

4625.771

3. 5

5

4

7

0. 8

1. 1

0. 9

1. 5 u,N

Cn?-

Fe I p Coi3. 113. 98

3. 71

171

974

176

4631. 725r

4631. 954r

4632.139

1

3

12

0. 2

0. 6

2. 7 s Fe I p —

Cri

3. 55

3. 56 754233

4625.920 12 2. 6 s Cr I 3. 85 244 4632.331 2 0. 4

4626.023r 1 0. 2 4632.479r 1. 5 0. 3

4626.182m 67 16. 6 S,d Cri 0. 97 21 4632.650r 4 0. 9

4626.357r 4626.49?m

5 1. 1

s

Fe I p Vi3. 25

1. 04

636

39 13

4632.819

4632.918

1 97

1

J

6. 9

1 14. 0

u

s

Fe I p

Fe I

3. 65

1. 61

820

39

4626.538 21 4. 5 s Mn I- 4. 71 4633.097r 5. 5 1. 2 Fei?p- 1. 01 17

4626.650r 2 0. 4 4633.25G 10 2. 2 s Cr I 3. 12 186

4626.792 6. 5 1. 4 u Fe I 2. 99 410 4633. 380r 0. 5 0. 1

4627.015r 1 0. 2 Fe I p 3. 25 637 4633. 547r 1. 5 0. 3

4627.221 4 0. 9 s Eu I 0. 00 1 4633.767 21 4. 5 u Fe I 3. 02 410

4627.368

4627.49 a

14

5

3. 0

1. 1

0 Si I Mo I?

5. 08

2. 28

4634.012r

4634.079 1 53

r 0. 2

I n. 2

swZr I Cr II0. 07

4. 07

5

44

180
The Solar Spectrum—Continued

W3iV6~

length

(A)

Equivalent Width

AX

(mA)

ReH n ppH

Width

AX/X

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

4634.266r 4. 5 1. 0

4634.372r 1. 5 0. 3

4634.605r 1 0. 2 Cri

Fe n p

3. 11

2. 58

17125 4634 71Qm 28 6. 0 11 Fe I? 4634 871 4 0. 9 Ti I?

4635.035r 0. 5 0. 1 4635 177 2. 5 0. 5 s V I 0. 07 4

4635.311 14 3. 0 Q Fe II 5. 95 186 4635 423r 2 0. 4

4635. 561r 4 0. 9 Ti I 2. 33 261

4635.620 10 2. 2 U Fe I p 2. 86 319

4635. 709r 2 0. 4 4635 853S 44 10. 1 11 Fe I 2. 84 349

4636. 017r 2 0. 4

4636. 164r 2 0. 4 4636 324 14 S. 2 W Ti 11 1. 16 38 4636 565r 1 0. 2

4636.675 4. 5 1. 0 u Fe I 3. 05 513

4636.934r 2. 5 0. 5

4637.044 3. 5 0. 8

4637.178 18 3. 9 s llCn

Ti I

2. 54

2. 33

32

261

4637.300r 6. 5 1. 4

4637.510S 77 17. 2 u Fe I 3. 28 554

4637.671r 4. 5 1. 0

4637.764 20 4. 3 s Cri /2. 54

12 54 32

32 4637 875 10 2. 2 Ti I 2. 34 261 4638 017S 82 IS. S u Fe I 3. 60 822

4638.531 8 1. 7 u?

4638.705r 2 0. 4 4638 Q56 13 2. 8 u

4639 176 3. 5 0. 8 4639.368m 36 8 A Ti I 1. 74 145

4639.506 15 3. 2 u Cr I 3. 11 186 4639.671m 37 s Til 1. 75 145 4639.946m 31 7. S s Til 1. 73 145

4640.106r 4. 5 1. 0 s Vi- 1. 05 39

Notes

17

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

oolai

Id(;nti- fication

Low

111 i or

IvOl. Line

OO DO

A fKAf\ A A Tv-i 4D*±u.'i4 in Qo U. D

Tl* 111T

At\An t\CiA O. 0 I. o 0

A(^Ar\ 7nOn 4D'*u. / uyr 1 U. A V T V 1

1 Oft

1. 0 U. 6

Pr> T yj. Qo

'±o4U.y / or lo Q O O. Z

Pf» T?

4041 AP.A'i 91 A .ZID OAZ4 0. z If Fg I p

9 8"^

4D41.0/ a I. 0

4D4JL.0iyr 4, 0 I. U

4041.0/ iT 1. 0 U. o

A(\A 4041.03 1 QQ Qaf\ CC U. 1 4AA9 404i6.UUU nnn Qo U. o s Cr T O. OO

A A/1 9 1 Q9»» 404Z. lozr 9 K

U. 5 0

404^. Af{Ao 9/1 Z40 7 K I. D M Sm, II

404Z.4U a 1. 0 U. 6

404.i.Oo4 7 K 1 A 1. 0

-)/? "Fp t

J; t; 1 4(1

/I A/1 9 QQ 1 »» 4D4ii.OOir 4 U. 9

/I aA Q HAI 404o,U0ir U. 0 U. 1

404o.ZU^ Af^A^ 909 A K

o. o 1. 4 s Fc I p

11. 48

4D4o.oUl r 9 U. 4

4040.4 / yjo AQOO 1.3. O J? C 1

AAJ^Q 404o 79 rr>

. / Z III eo Y I n no

404o. / ooT 15 O. w2

4D40.oy.*ir QO I. /

404o.y4 m S

AfKAA nt^ o 4044,UO a

cO I. 1

4644.19 a 0. 8

4644.398r 8. 5 1. 8

4644.526 8. 5 1. 8 0?

4644.80 a 2. 5 0. 5

4644.86 m s Zri fl. 44

1 1 89

4040.U4 a Z U. 4

A dA ^ TOO lb O A 6. 4 s,a J. 1

4645.308r 2 0. 4 La II 0. 13

4645.492 9 1. 9 0?

4645.644r 1. 5 0. 3

4645.790r 2 0. 4

xNo. or

Vib. Band

181
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solai- Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BancNotes

4645.883r 1 0. 2 4652.31 a 3 0. 6

4645.94 a 1 0. 2 4652.55 a 5 1. 1

4645.993r 1. 5 0. 3 Vi? 0. 04 4 4652.78 a 1. 5 0. 3 4646.169m 77 20. 0 S Cr I 1. 03 21 4652.895r 1 0. 2

4646.376 14 3. 0 s Vi 1. 06 39 4653.042r 1 0. 2

4646.498 9. 5 2. 0 s Cri 3. 08 147 4653. 149r 0. 5 0. 1 4646.640m 27 5. 8 s 4653.314 3. 5 0. 8

4646.780 16 3. 4 s Cn 3. 10 186 4653.370 9 1. 9

4646.970r 3. 5 0. 8 Nii?p 3. 63 145 4653.490 8 1. 7 s Fe I p 0. 99 17

4647.185 5. 5 1. 2 s 4653. 645r 1. 5 0. 3

4647.283 19 4. 1 u 4653.786r 1 0. 2

4647.442S 78 16. 8 u Fe I 2. 95 409 4653. 903r 0. 5 0. 1

4647.701r 9. 5 2. 0 Fe I p 3. 41 722 4654.044r 1 0. 2 C2 4647.958m 42 9. 0 u 4654.153 14 3. 0 s 4648 1 20 19 4. 1 Cr I 2. 54 32 4654.303 4 0. 9

4648.322r 5. 6 1. 2 s u*) .1

- 4654.504m ' 16. 8 s Fei 1. 56 38

4648.416r 1. 5 0. 3

> i / i

/ 0 1 A u i e I /3. 21

13. 60 554821 4648.657m 67 15. 7 u Nil 3. 42 98

4654.730 . 2. 6 s Cn 3. 10 186

A a AO O CO In 9 A Or I /2. 54

13. 55

32 233 4654.93 a 3 0. 6

4648.948 18 3. 9 0 Fe II 2. 58 25 4655.10 a 1 0. 2

4649. 163r 3. 5 0. 8 4655.245r 5 1. 1 u 1 6

4649.302r 0. 5 0. 1 4655. 460r 1 0. 2 La II L 95 75

A C A C\ AOO 4. O s KjV I /2. 54

\3. 56 32 233 4655.656 16 3. 4 s Ni I Til

3. 70

2. 34

115

261

2 1

4649.643 20 4. 3 u,N 4655.787 12 2. 6 u

4649.817 16 3. 4 s Fe I 3. 24 592 4655.953r 3 0. 6

4650.019 14 3. 0 s Til 1. 74 145 4656.051 9 1. 9 s,d Ti I L 75 145

4650.122r 3. 5 0. 8 4656.188 18 3. 9 s Cr I 3. 09 147

4650.308 10 2. 1 u 4656.307r 1. 5 0. 3

4650.550 5 1. 1 u 17 4656. 474S 55 13. 8 s Til 0. 00 6

4650.815 3. 5 0. 8 u 17 4656.641r 4 0. 9

4650.947r 2 0. 4 4656.818r 1. 5 0. 3 Cr I 4. 78 311

4651.119 6 1. 3 Cui? 5. 07 4656.981m 27 6. 6 w Fe II 2. 89 43 4651.290m 66 15. 6 s Cr I 0. 98 21 4657.204m 38 9. 2 w Ti II 1. 24 59

4651.511r

4651.871r

4652.024r 4652.167m

5

1

2

82

1. 1

0. 2

0. 4

19. 5 S

Pr II

C2Cri

0. 20

1. 00

6

21

4657.380r

4657.451r

4657.590rn

3. 5

1

24

0. 8

0. 2

5. 6 u

1

Co I Ni I

Fei

3. 23

4. 26

2. 84

156 254

346

1S2
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Ickniti- or or Notes

1.1 \jC\j Ulull Rot. Vib. AX ak/k fW"i 1 iViri Rot. Vib. Line Band ImA; —

\r

)

Lino Band

1. 5 —

0 4663 822iTi 28 6. 0 Cr I 3. 11 18G

4658.044r 2. 5 0. 5 Fe ii?p- 5. 57 170 4663.954 12 2. 6

4664. 185r 3. 5 0. 8

dfi^iS 'iUiJO.ii 1 1 d« 1X 0 9 4664 324r 4 0. 9 Ni I p 3. 63 147

4fi5S 170r 0. 5 0. 1 li 'M 2,1 1 9

14 3. 0 Fe I 3. 27 591 4664 547r 1. 5 0. 3

*!Vl (JO • OV/ i. 4. 5 1. 0 4664 7948 52 11 A s,N |Cr I 3. 12 186 Na I 2. 10 12

5. 5 1. 2 4665 172 5. 5 1. 2 s XI 2. 4

4665. 257r 3 0. 6 Fe I p 4. 21 1115

4 0. 9 4665.42 a 1 0. 2

3 0. 6 4665 547 5 1. 1 u,N Fe I 4. 07 1044

^UU t/ . »JO ^1 2. 5 0. 5 4665 679r 3. 5 0. 8 C,

4fi^Q 7fi7r 0. 5 0. 1 4665 76 m 4. 5 1. 0 Q 3 0. 6 4665 825r 6. 5 1. 4 Fe II p 2. 70 26

4fififl 071 4 0. 9 4665 906 28 6. 0 Cr I 3. 55 233

4fifi0 241 2. 5 0. 5 Co 4666 111 23 4. 9 u — V I 1. 89 94

4fifi0 42fi 17 3. 6 to 4666 203 18 3. 8 g Cr I 2. 97 99

4fifi0 Tt VJ U . fi28r OJ. 0. 2 Co II 4666 353r 0. 5 0. 1 4660 72Qr 1. 5 0. 3 4666 484m 34 7. 3 Cr I 3. 14 186 4660 Qn7 19 4. 1 u Fe I? 4666 615 16 3. 4 u

4661 151 3 0. 6 Q Fe II? p 5. 57 170 4666 754m 45 9. 6 to Fe II 2. 83 37

4661 328 3 0. 6 11 Fe I p 2. 83 347 4666 893r 3. 5 0. 8 4661 53Qm 28 6. 9 w?,d? Fe I 4. 56 1207 4666 QS6 35 7. 5 Ni I 3. 80 146

4661 788 2 0. 4 0? Zr II 2. 41 129 4667 162 16 3. 4 Cr 1 2. 97 99

4661 Q2?m Eu I 0. 00 1 1 3 4667 255 34 7. 3 w?,N

4fifil Q7Qm 35 8. 6 Fe I 2. 99 409

4667 460m 75 16. 1 u Fe I 3. 60 822

4662 105r 4. 5 1. 0 4667 5q4m 60 12. 8 Ti I 0. 02 6 4662 21 7r 2. 5 0. 5 4667.770m 36 7. 7 w,N Ni I 3. 70 163

4662.323r 1 0. 2 4667.924 4 0. 9 C2? P64 2,1 19 4662.512 4. 5 1. 0 s La II — 0. 00 8 4668.073 1 8. 6 u Fe I p 3. 69 826

4662.755 11 2. 4 U:N Ti II p- L 18 38 \ 112 Moi? L 47 6 4668.149 J I 17. 6 u Fei 3. 26 554

4662.98 a 2. 5 0. 5 2 1 4668.375 11 2. 4 s Ti I 1. 05 77

4663.182 18 3. 9 u Fei 3. 55 754 4668.572m 39 10. 0 s Nai 2. 10 12

4663.28?m S 1 3 4668.78 a 5 1. 1 C2?

4663.317 27 5. 8 s Cr I 3. 10 186 4668. 844r 1. 5 0. 3

4663.406 25 5. 4 s,m Co I 3. 13 156 4668.991r 2 0. 4

4663. 561r 4 0. 9 4669.176m 60 12. 8 w? Fei 3. 65 821

4663.709 21 4. 5 0 Fe II 2. 89 44 4669.323 31 7. 5 s Cr I 3. 17 186

183
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes

4669. 395r 6. 5 1. 4 Sm II 0. 10 7 4675.112m 30 6. 4 S Til 1. 07 77

4669.527r 2. 5 0. 5 4675.280r 2. 5 0. 5

4669.651

4669.828r

4669.982r 4670.173m

4670.413m

4670.559r

4670.742r

4670.905

4671.049r

4671.215r

6. 5

0. 5

2

27

55

6. 5

0. 5

2. 5

2. 5

1

1. 4

0. 1

0. 4

5. 8

12. 2

1. 4

0. 1

0. 5

0. 5

0. 2

s

w

us,N

Sm II Cr I

Si I

Fe II

50 II

51 I?

0. 28

3. 09

2. 58 L 36

26

170

25

24

4675.392

4675.604

4675.846r

4676.015r

4676.165r

4676.234

4676.358

4676.540r

4676.656r

4676.926

4

14

1

2

2. 5

3

5. 5

1. 5

2

3. 5

0. 9

3. 0

0. 2

0. 4

0. 5

0. 6

1. 2

0. 3

0. 4

0. 7

w?w

s s,N

s,N

Nil

Sm II Til?

3. 61

0. 04

2. 50

115

3 17

4671.422m 27 5. 8 w 4677.086r 1. 5 0. 3

4671.569r

4671.687

4671.914r

4672.036r

4672. 197r 4672.334m

4672.46 a 4672 537r

4672.632r 4672.837m

4672.971r 4673.169m

4673.278m

4673.444r

4673.645r

4673.790

4673.958r 4674.099m

4674.303

4674.475r

4674.656

4674.762

4674.880r

3. 5

11

2

4. 5

5

56

2

4. 5

1

31

3

72

39

2

2

7. 5

2

34

13

1, 5

18

14

1

0. 7

2. 4

0. 4

1. 0

1. 1

12. 0

0. 4

1. 0

0. 2

6. 6

0. 6

15. 4

8. 3

0. 4

0. 4

1. 6

0. 4

7. 3

2. 8

0. 3

3. 8

3. 0

0. 2

e,N

w

su

wl

u

uu,N

s

w

S

C2Mn I

c,Fe I p

Fe I p

Fe I Fe I p

c,

Fei

c,Fez

(Sm 11) Nil

Yi

/P63

IP 64

2. 89

4. 14

L 61

3. 65

3. 65

1. 56

0. 18

3. 63

0. 07

2,11 2,1/

21

10^5

40

820

822

40

14

4

19 4677.30 a

4677.43 Ir 4677.53?m

4677.596

4677.724r

4677.873r

4677.997r

4678.172S

4678.420r

4678.521

4678.625r

4678.854S

4679.076r 4679.230m

4679.421r

4679.578r

4679.73 m

4679.822r

4679.983r 4680.142m

4680 'i06m

4680.482

4680.560

4680.749

1

3. 5

1

12

4

3

5. 5

62

9

10

6

97

7

47

4

1

1

6. 5

42

43

1 58

4

0. 2

0. 7

0. 2

2. 6

0. 9

0. 6

1. 2

13. 2

1. 9

2. 1

1. 3

21. 2

1. 5

10. 0

0. 9

0. 2

0. 2

1. 4

9. 0

9. 2

f 7. 3

[ 5. 1

0. 9

8W

0?

w

u

u

u

w

s

w

s

s

u

s

C2

C2Coi

Fei

Fe I p

Fe I

FeiTi I p

c,Fe I p Zui

Fe I Fe ICri

Nd II?

R25

R24

0. 58

4. 15

3. 42

3. 60

3. 37

L 05

4. 22

4. 00

1. 61

2. 86

3. 11

0. 06

2,1

2,1

15

1072

688

821

688

77

1071

2

39

346

186

4 .

19

19

17

13

184
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4680.863 26 5. 6 s Cri 3. 09 170

4681.049r 5. 5 1. 2 Ni I p 3. 63 143

4681.208r 1. 5 0. 3

4681.308r 0. 5 0. 1 4681.474m 26 5. 8 u,d Fe I

4681.607r 2. 5 0. 5

4681.744r 1 0. 2 4681.919m 64 15. 0 S Til 0. 05 6 4682.121m 49 10. 5 u Fei

4682.351m 39 8. 3 u YiiCoi

0. 41

3. 19 12 156

4682.570 22 4. B u Fe I 2. 94 384

4682.766r 6. 5 1. 4

4682.960r 0. 5 0. 1 Cs

4683.15 a 1 0. 2

4683.253r 3 0. 6 C2 fP56

IP57

2,11 2,1/ 19

4683.401r 6 1. 3

4683.44 m s Zn 1. 53 63 13 4683.567S 46 10. 0 u Fei 2. 83 346

4683.708r 2. 5 0. 5

4683.827r 1. 5 0. 3

4683.981r 6 1. 3

4684.12 a 3. 5 0. 7

4684.218r 7 1. 5

4684.28 m s 13

4684.351 9 1. 9 c, fR32

IR19

1,01 2,1/ 19

4684.50 m S Ti I 2. 16 203 13

4684.528r 4 0. 9 C2 R30 1,0 19

4684.601 22 4. 7 u Cri

Ce II?

3. 08

0. 90

146 228

4684.750r 6 1. 3 fP 65 IP 66

1,01 1,0/ 19

4684.884r 5 1. 1 s,N C2 P 64 1,0 16,19

4685.034 16 3. 4 s Fe I 2. 84 347

4685.17 m 2 0. 4 s 4685.275m 53 11. 6 s Cai 2. 93 51

4685.499r 4. 5 1. 0 C2

4685.696r 1 0. 2

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4685.854r 5 1. 1 Gei

Co I

2. 03

0. 92

3

4686.006r 3. 5 0. 7 C2 R18 2,1 19

4686.122r 2. 5 0. 5

4686.222 56 12. 4 u Ni I 3. 60 98

4686.370r 5 1. 1 Fe I?

4686.630r 1. 5 0. 3 Fez?

4686.750r 2. 5 0. 5

4686.87 m 2 0. 4 s Til 2. 15 203

4686.96 m 2 0. 4 s Vi 1. 87 93

4687.186 5 1. 1 s?,N Srn II —

Cj?

0. 04 R 19 3

2,1 19

4687.312

4687.393

1 44

I 2. 3

,)

i 7. 0

s

u

Fe I p Fe I0. 96

2. 83

17

347

4687.538r 3 0. 6

4687.676 6. 5 1. 4 u Fe 1 p 2. 86 347

4687.805 7. 5 1. 6 S Zr I 0. 73 43

4687.943r 1. 5 0. 3 C2 4688.184m 40 9. 0 w -Fe I

4688.372 17 3. 6 u Fe I p —

Til

4. 19

3. 09

1071 306

4688.477r 11 2. 3 S Zr I 0. 15 5

4688.56 a 7 1. 5

4688.688r 30 6. 4 C2C2 R 28 Head

1,0 2,1 19

19,30

4689.062r 4 0. 9 C2

4689.214r 3 0. 6 C2 4689.361m 31 6. 6 s Cn 3. 12 186 4689.499m 25 5.3 u Fe I

4689.760r 0. 5 0. 1

4689.974r 0. 5 0. 1

4690.144S 51 10. 9 w Fe I 3. 69 820

4690.379 13 2. 8 s Fe I 1. 01 17

4690.559r 5 1. 1 C2

4690.798 3 0. 6 S Til 1. 07 76

4690.974r 4. 5 1. 0

toy i . 1 y / r 0. 0 fl 7

4691.347

4691.420 1 104

1 6. 0

1 18. 1

S

u

Til Fe I

1. 07

2. 99

75

409

4691.599m 37 7. 9 w,N

185
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Banc

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMI

No.

or Vib. Banc

Notes

I

4691.7791- 6 1. 3 C2?- R 17? 2,1 19 4697.808r 0. f) 0. ]

4691.969r 5. 5 1. 2 C2?- R 17? 2,1 19 4698.081r 4. £ 1. c» C2? R 12'' 2,1 19

4692.219r '40. 9 4698.280 10 2. 1 Sc 11 0. 60 13

4692.45 m

4692.524r

4692.653

3. 5

8. 5

21

0. 7

1. 8

4. 5

S

w,N

Ti I p La II —1. 07

1. 75 R29

77

75

1,0 17, 19

4698.402

4698.462

1 65

f 5. 5

I 9. 4

u

s

Co I Nil

Cn

3. 25

4. 09

3. 14

156 235

186

4692.847r 8. 5 1. 8 4698.623m 45 9. 6 Cr I /2. 71

13. 09

62 146

4692.974r 5. 5 1. 2 Cri 2. 98 99 4698.771m 40 8. 5 S Til 1. 05 75

4693.195 17 3. 6 u,dl Co I 3. 23 156 17 4698.83 m s Ti I 2. 16 203 13

4693.338r 4 0. 9 C2?- R 16? 2,1 19 4698.942 9. 5 2. 0 s Cr I 3. 08 146

4693.674 12 2. 7 S Ti I 0. 02 6 4699. 134r 5 1. 1

4693.789r 3 0. 6 4699.340m 64 13. 6 w

4693.947m 22 4.9 s Cr I 2. 98 99 4699.583 8 1. 7 s Cr I 4. 21 292

4694.117 12 2. 6 0? S I 6. 52 2 17 4699.724r 3 0. 6

4694.303r 1 0. 2 4699.854r 2 0. 4

4694.457r 3. 5 0. 7 -C2 R 28 1,0 19 4699.990r 1. 5 0. 3

4694.655r 10 2. 1 4700. 162S 52 11. 1 u Fei 3. 69 935

4694.870

4694.903r

32

J

1

5. 5

I 1. 9

w,N Fe I 4700.298r

4700.431

3

2

0. 6

0. 4 u

C2Fe I p 2. 20 67

4695.152 17 3. 6 s Cri 2. 98 99 4700.619 12 2. 8 s Cn 2. 71 62

4695.446 8 1. 7 S I 6. 52 2 4700.814r 0. 5 0. 1

4695. 607r 1 0. 2 C2? R 13 2,1 19 4700.915r 4. 5 1. 0

4695.751r 1 0. 2 C2 R 14? 2,1 19 4701.054m 38 8. 1 s Fei 3. 69 820

4695.857r 1 0. 2 C2 4701.172 10 2. 1 s Mn I 2. 92 21

4696.030 3 0. 6 C2 R 11 2,1 19 4701.361m 34 7. 2 u Nil 3. 48 101

4696.262 8 1. 7 S I 6. 52 2 4701.542m 46 9. 8 u Nil 4. 09 235

4696.38 a 4 0. 9 -C2 R27 1,0 19 4701.719r 4 0. 9 C2? R 24 1,0 19

4696.512r 1 0. 2 C2 R27 1,0 19 4701.898 15 3. 2 u Fe I pCri

3. 43

3. 11 688170

17

4696.622 4 0. 9 c,, fP.59 IP 60

1,01 1,0/ 19 4702.135r 4 0. 9

4696.755r 1. 5 0. 3 4702.295 12 2. 6 u

4696.932 6 1. 3 s Ti I 2. 15 203 4702.603 11 2. 3 w

4697.058m 26 5. 5 s Cri 2. 71 62 4703.003m 326 71. 9 s Mg I 4. 34 11

4697.294r 4 0. 9 u C2 fRlO

^P 46 [P47

2,11 2,1}

2;ij 19 4703.491r

4703.584

3

10

0. 6

2. 1 s

C2 R 23 1,0 19

4697.398 14 3. 0 s Cn 3. 37 195 4703.818m 58 12. 3 w Nil 3. 66 133

46:)7.f>3S 4 0. 9 Co 4704.021r

4704.190r

5

7

1. 1

1. 5

186
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4704.412

4704.482

4

17

0. 9

3. 6

[ w,d

Sm II 0. 00 1 17 4710.561r

4711. 021r

4

2

0. 8

0. 4

s Vi 2. 13 119

4704.675r 2 0. 4 4711.491m 28 5. 9 w? Fe I

4704.787r 1. 5 0. 3 4711.628 3. 5 0. 7 C2 R 18 1,0 19

4704.954S 58 12. 6 u Fe I 3. 69 821 4711.68 m 1 0. 2 s Ti I p 1. 44 111

4705. 150r 6 1. 3 C? R 22 1,0 19 4711.81 a 2 0. 4

4705.246 5. 5 1. 2 C2 R 22 1,0 19 4711.91 m 2. 5 0. 5 s Zri 1. 53 64 4705.473m

4705.65 a

4705.79 a

4705.925

4706.094

4706.17 m

4706.302

4706.554

36

2

2. 5

9

7. 5

1

6. 5

26

7. 6

0. 4

0. 5

1. 9

1. 6

0. 2

1. 4

5. 5

s

u,d?

s

su

s

Fe I

Nil?

Cri

Vi

Fe I p

Nd II —

IV I

3. 55

3. 66

3. 11

1. 93

3. 64

0. 00

2. 14

752

128

170

94

890

3 119

4712.083

4712.257

4712.497

4712.701

4712.97.5r

4713.185

4713.34 a

4713. 520r

34

18

13

16

18

14

3. 5

3

7. 2

3. 8

2. 8

3. 4

3. 8

3. 0

0. 7

0. 6

u,d

u

uu,N

Ni I-

|Fei

Fe I

C2? Fe II p

C2

3. 66

3. 02

R 17

2. 78 R 17

131 467

1,0

26

1,0

16

16

17

19

19

4706.72 a 4 0. 9 Si I 5. 08 4713.65 a 2 0. 4

4706.83 a 5 1. 1 Co? R 21 1,0 19 4713.803 9 1. 9 u,N Ni I? p 3. 54 128

4706.94 a 4 0. 9 C2? R 21 1,0 19 4714.071 36 7. 6 u,N Fei 4. 56 1206

4707.074r 8. 5 1. 8 4714.12 m s Vi 2. 12 119 13

4707.285m 107 22. 7 s Fe I 3. 24 554 4714.206 22 4. 7 u Fe I 3. 30 591

4707.496m

4707.69?m

65 13. 8 s

s

Fe I 2. 84 346

13, 16

4714.371r

4714.420

1 132

f 5. 7

1 25. 0

u

u

Fe I Ni 1 3. 38 98

4707.752 8 1. 7 s Cri 3. 37 195 4714.553r 16 3. 4 C2 R 16 1,0 19

4708.019m 52 11. 3 s Cri 3. 17 186 4714.732r 17 3. 6 C2 R 16 1,0 19

4708.288r

4708.4611- 4708.672m

4708.976

4

6

46

|,.,

0. 9

1. 3

10. 0

f 7. 8

w

u

C2

Ti II

|Fei

Til

JP 35

IP 36

1. 24

3. 64

2. 16

2,1 2,1

49

889

203

|l9 4714.911r

4715. 102r

4715.299

4715. 453r

4715.607

17

12

11

1

6. 5

3. 6

2. 5

2. 8

0. 2

1. 4

S

s

u

Ti I

Nd II?

0. 05

0. 20

G

49

4709.096m [ 15. 7 u Fe I 3. 65 821 4715.767m 68 15. 0 u Nil 3. 54 98

4709.332r 4. 5 1. 0 s Sc I? 2. 30 22 4715.893 14 3. 0 s,N Vi? 2. 36 136

4709.505r 4709.718m

4709.868r

4710.077

4710.192

3. 5

62

4

9. 5

1 98

0. 7

14. 0

0. 9

2. 0

j 3. 0

s

s

&

Ru I Mn I

Zri

Til

1. 13

2. 89

0. 69

fl. 05

12. 17

14

21

43

75 203

4716. 141r

4716.508r

^ i 10.000

4717. 127r

4717.314

2. 5

2

6

9

0. 5

0. 4

1 1 1. 1

1. 3

1. 9

s

w

Sc II p —

C2Fei?

i; e 1

0. 61 R 15

3. 25

13

1,0

634

19

4710.290m [ 17. 8 u Fe I 3. 02 409 4717.579 28 5. 9 u

187
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

4717.710

4717.877

4718.05 a

4718.23 a 4718.423m

4718. 587r

9

8

2

2. 5

60

6

1. 9

1. 7

0. 4

0. 5

IS. 9

1. 3

s

8

Vi

Cri

Cr I

2. 11

3. 12

3. 19

119 170

186

4724.538r

4724.68 m

4724.847

4725.098r

4725.455

4725.584r

7. 5

2. 5

4. 5

1. 5

3

1. 5

1. 6

0. 5

1. 0

0. 3

0. 6

0. 3

u

8 u,N

u

Ti I

C2

/ c.

2. 17 R 8 R7

P 40 P40

R7

203

1,0

1,0

1,0

1,0

1,0

19

19

19

19

19

4718.833r 2 0. 4 R 13 1,0 19 4725.81 a |2| 0. 4

4719.12 m

4719.225

4719.510

4719.686

4719. 856r

4720.133

4720.391r

4720.577r

4720.816r

2. 5

4

11

7. 5

5. 5

3. 5

1

4. 5

1. 5

0. 5

0. 8

2. 3

1. 6

1. 2

0. 7

0. 2

1. 0

0. 3

8

W

0?

Zr I Fe I?

Ti II

Sm II Fe II p

Fe I? p

c,

1. 86

1. 24

0. 04

3. 20

4. 21 R 11

66

59

3

54

1114

1,0 19

4725.948

4726.145

4726.334

4726.80 a

4727.003

4727.156

4727.272

4727.406

4727.488

7

16

4

2. 5

7. 5

25

17

1 122

1. 5

S. 8

0. 8

0. 5

1. 6

5. 3

3. 6

I 16. 5

[ 11. 0

s

u

s,N

s

uu

s

|Cr I Fei

Fei

C2

Si I? Fe I p Cr I

Fe I Mn I

3. 00

4. 29

3. 00 P39

5.08

3. 27

3. 00

3. 69

2. 92

99

1134

384

1,0

635

99

821

21

19

4720.999S 47 10. 0 8 Fe I /2. 99

\4. 15 409

1071 4727.850 8. 5 1. 8 wl Nil 3. 63 146

4721. 130r

4721.312

4721.525r

4721. 975r 4722.163m

4722. 284r

5. 5

5

3

3

63

4. 5

1. 2

1. 1

0. 6

0. 6

14- 2

1. 0

s

w

s

Cr I?

Vi

C2Zn I

Sr I

R 11

3. 55

1. 95 R 10

4. 03

1. 80

1,0 232

108

1,0

2

5

19

19

4727.947

4728.167

4728.416r

4728.552S

4728.787r 4729.023m

8. 5

18

7. 5

73

6

35

1. 8

3. 8

1. 6

16. 3

1. 3

7. 4

8

uu

uS

u

Co I Fe I Nil

Fei

Sci

Fei

0. 43

3. 74

3. 65

1. 44

4. 07

15

115

822

14

1043a

4722. 466r 1 0. 2 s 16 4729.202r 8. 5 1. 8 S,N Sci ri. 43

11. 43

14

14

4722.615 14 S. 0 S Ti I 1. 05 75 4729.277 16 3. 4 u Ni I 4. 10 235

4722.754 3 0. 6 s Cn 3. 37 195 4729.45 a 7 1. 5 Anna ct e~> -* 4722. 881r 1 0. 2 s V I 1. 95 108 4729.54 m 1 0. 2 8,N V I 1. 89 93

4722.999r 4. 5 1. 0 Ni I 4. 15 4729.682m 45 9. 5 u Fe I 3. 40 688

4723.114

4723.175 \- 1

[ 3.4

S

S

Cri

Ti I

3. 08

1. 07

145

75

4729.859 4730.038m11

65

2. 3

13. 3

s,N

u

Cri

Mg I

3. 09

4. 34

169

10

4723.347r

4723.448r

4723.752r

4723.898r

4724.10 a

4724.415

6

3. 5

3. 5

2. 5

2

27

1. 3

0. 7

0. 7

0. 5

0. 4

6. 5 s

Ni I p

c,

Ni I

Cr 1

3. 68 P42

R9

R9

3. 68 R 8

3. 09

162

1,0

1.0

1,0

167

1,0

145

19

19

19

19

4730.403

4730.60 m

4730.720m

4730.997

4731.173

4731.287r

11

1

43

31

11

0. 5

2. 3

0. 2

9. 6

6. 6

2. 3

0. 1

s

8

8US

ViCri

Til

1. 94

3. 08

2. 17

108

145

202

188
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(A) ^mA; (r

)

Line Band \A) unAj \v

)

Line Rand

47Q1 47am 79 16. 7 uo IFe II Fe I

2. 89 43 4738 30 a 4 0. 8

ATi9, 44 a 0 0. 6 47S1 fifi2r 0. 5 0. 1 4738 65 a 1. 5 0 3 4731 804m 39 8. 2 XL Ni I 3. 83 163 4738 83 a 1 0. 2 Si i?p 4. 93 4732 04Qr 1. 5 0. 3 Co I 0. 51 15 4738 958r ,5 1. 1 4732 174r 2 0. 4 P 32 1 0 19 4739 113m 56 11.// Mn I 2. 94 21 4732 323r 1. 5 0. 3 Zri 0. 63 48

4739 290r 1. 5 0. 3 4732 46fim 39 8. 7 UO Ni I 4. 10 235 4739 454 6 1. 3 s Zr I 0. 65 43 4732 81 7r 2 0. 4 P 31 1 0 19 473Q fi5fir 1 0. 2 4732. 948r 3 0. 6 Ti II p 1. 13 29 473Q 81 a 0. 5 0. 1 4733 222r 1 0. 2 4739 91fir 0. 5 0. 1 4733 426 11 2. 3 Ti I 2. 16 202

473Q 96 fl 0. 5 0. 1 4733 598S 76 16. 0 s Fe I 1. 48 38 4740.168 14 3. 0 s,d Nil 3. 48 99

4733.758r 4 0. 8 4740.344m 37 7. 8 s Fei 3. 02 409

4733.984 13 2. 7 s 4740 48'^ 31 6. 5 4734.105m 30 6. 3 |Fe I 4. 29 1133

So I 1. 43 14 4740 70 a 3 0. 6

4734 1 83r Q0 0. 6 4740 948 32 7. 0 w

4734.28 a 3 0. 6 4741.075 33 7. 0 g Sc 1 — 1. 44 14

|Fe I 3. 33 688

47*^4 TCI 4'?4r 4. 5 1. 0 ^2 P ''R 1 0 19 4741 355r 3. 5 0. 7 Ni I p 3. 68 166

4734.577 8 1. 7 J. j^O 1,0 19 4741 71 7J-.00(-'O 535S 69 14. 6 11 Fe I 2. 83 346

4734 669r 3 0. 6 s Til 2. 24 233

4741 796r 3 0. 6 4734.832 5 1. 1 Co I 3. 25 156

4741. 942r 1. 5 0. 3 Sr I 1. 77 5 4735.003r 3 0. 6 C2 P 27 1 0 19 4742 71 7^. 1±^71 24r 5 1. 1 s Ti I 2. 15 202 4735 314r 4. 5 1. 0 Co? P 26 1 0 19 4742.294 11 2. 3 s,d Ti I p 1. 46 111 4735 446r 2. 5 0. 5 Co P 26 1 0 19 4749 8 1. 7 11)^ 4735 664 5 1. 1 Co? P 25 1,0 19 4749 64 m 1 0. 2 s V I 2. 33 128 4735.848S 59 12. 4 u Fei 4. 07 1042 4742.798m 27 5. 7 s Ti I 2. 24 233

4736.030 13 2. 7 c. P 24 1,0 19 4742.936 10 2. 1 u Fe I 4. 19 1072

4736. 232r 6 1. 3 C2 P 23 1,0 19 4743. 105r 8 1. 7 u,N La II — 1. 78 75

4736.508 12 2. 5 Nil 3. 48 99 Cr I 4. 20 290

4736.783S 144 30. 8 s Fe I 3. 21 554 4743. 297r 1. 5 0. 3

4736.965r 18 3. 8 C2 P 19 1,0 19 4743.490r 0. 5 0. 1

4737. 117r 10 2. 1 C2 P 20 1,0 19 4743.817 7. 5 1. 6 S,N Sci 1. 45 14

4737.355m 55 Cn 3. 09 145 4744. 117r 3. 5 0. 7 Fei?p 4. 39 1168

4737.635m 38 8. 0 u Fei 3. 27 590 4744.387m 60 12. 6 w Fei

4737.66 111 S Sex 1. 43 14 13 4744.642r 8. 5 1. 8 s Fei 0. 99 17

4737.764r 6 1. 3 Co I 1. 96 57 4744.836r 9 1. 9

4738.13 a 1. 5 0. 3 4744.946 7. 5 1. 6 u

189
The Solar Spectrum—Continued

Wavelength

CKJX) Al

Equivalent Width

AX

Cm X)

Re- duced

Width

AX/X

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(m a")

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. B;ind

Notes

4745.138

4745.312

12

12

2. S

2. 3

s,d

s

Fei

Cri

2. 22

2. 71

67

61

4752.55 a

to 4752.80 a 1 «

J

1. 7

4745.48 a 1. 5 0. 3 4752.902r |3| 0. 6 s Cr I 3. 37 194

4745.706r 3 0. 6 Sm II 0. 10 7 4753.18 m |2.5| 0. 5 S Sci 0. 00 5

4745. 807S 69 15. 0 u Fe I /3. 65

14. 10 821 1068

4753.375r 1 1 0. 2

4745.960r

4746. 120r

4746.266

3. 5

3

6

0. 7

0. 6

1. 3 u

Co I 3. 93 182

4753.55 a

to 4753.80 a 4754.039m

1

f

130

1. 1

27. 8 s Mn I (Vi)

2. 28

2. 07

16 113

4746.39 a 1. 5 0. 3 4754.360 11 2. 3 u Co I 3. 23 156

4746.64 m 0. 5 0. 1 s,N Vi 2. 03 113 4754.62 a 12. 51 0. 5

4747.07 a

4747.27 m

4747.284r

4747.683r

4747.830r

4747.96 m

4747.980 4748.141m

4748.367r

4748.50 m

4748.549r

4748. 737r

4749.258r

4749.662

2

1. 5

4. 5

3

15

78

8

3

1

4

6

35

0. 4

0. 3

0. 9

0. 6

2. 5

16. 4

1. 7

0. 6

0. 2

0. 8

1. 3

7. 4

S

s

S

w

s

u,d

Til

Ti I

Na I

Si I

Vi

La II Fe I p Co I

1. 07

2. 25

2. 10

4. 93

2. 04

0. 93

4. 26

3. 05

75

233

11

113

65

1098

156

13

13

4754.765m

4755.149

4755.264

4755.529r

4755.704

4755.837 4756.117m

4756.366 4756.521m

4756. 728r

4756.98 a

4757.027r

4757.313

49

7. 5

5. 5

1. 5

26

14

60

11

75

7

1

0. 5

6

10. 3

1. 6

1. 2

0. 3

5. 5

2. 9

12. 6

2. 3

15. 8

1. 5

0. 2

0. 1

1. 3

s

s

o1

w

ul

s

0u

s

Ni I Cri

Cr I

Si I

Fei

Cri

Fei

Nil

Co I

|Cr I Vi

3. 63

3. 09

3. 01

4. 92

3. 10

3. 48

3. 93

4. 24

2. 10

141 168

124

145

98

290

113

17

4749.952m 33 6. 7 u Fei 4. 56 1206 4757.48 m s Vi 2. 03 113 13

4751.00 m 2 0. 4 s Vi 2. 05 113 4757.585m 54 11. 1 s? Fei /3. 27

14. 26 634

1115

4751.093 26 5. 3 w Fei (Cri) 3. 55 231

4751.29 m 1. 5 0. 3 s,N 4757.856r 3 0. 6 Ru I 0. 93 12

4751. 363r 2. 5 0. 5 4758.124m 40 8. 2 s Til 2. 25 233

4751. 553r 6 1. 3 4758.425 5 1. 1 Nil 3. 85 193

4751.58 m s Vi 1. 93 94 13 4758.726 11 2. 3 s,N -Vi? 1. 22 51

4751.825 15 5. 7 S,d Nai 2. 10 11 4758.917 4 0. 8 s Ti I 0. 84 41

4751.940r 2 0. 4 4758.99 a 2 0. 4 Si I 4. 95 4752.104m

4752.286r 4752.430m

47

3

60

9. 9

0. 6

12. 6 w

Cr I (Nil)

Ni I

4. 18

3. 68

3. 66

165

132

4759.276m

4759.44 a

4759.529r

4759. 671r

41

1

1

3

8. 6

0. 2

0. 2

0. 6

s Ti I

Til

2. 25

2. 17

233

202

190
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4759.772r

4759.926r

4760.074

4760.218r

4760.45 a

4760.80 a

4760.97 m

4761.101

4761.246

4761. o28m

4761.711r

4762.08 a 4762.375m

4762.631m

4762.782

4763.29 a

4763.62 a

2

5

8

2

2

1. 5

2. 5

16

11

74

3

2. 5

105

53

30

1. 5

1. 5

0. 4

1. 1

1. 7

0. 4

0. 4

0. 3

0. 5

3. 4

2. 3

15. 5

0. 6

0. 5

22. 0

11. 1

6. 3

0. 3

0. 3

s

s

S

u

s

s

s

s

su

Cr I Cn

Fe I Ni I p

Yi

Cn

Mn I Cn

Mn I (C I)

Nil

Ti n

3. 01

3. 11

3. 04

3. 70

0. 07

3. 12

2. 95

3. 37

2. 89

/7. 48

\7. 48

1. 93

1. 08

124

169

384

114

4

169

21

194

21

6

6

71

17

4767. 150r

4767.270

4767.40 a

to 4767.75 a

4767.857

4768.082

4768.326

4768.400

4768.700

4768.832

4769.033r

4769.50 a

4769.799

4769.997

4770.39 a

4770.683

4771.089

7. 5

14 }"

20

14

1 110

25

6

1. 5

'2

16

16

3

5. 5

20

1. 6

2. 9

2. 3

4. 2

2. 9

j 14. 3

I 10. 7

5. 2

1. 3

0. 3

0. 4

3. 4

3. 4

0. 6

1. 2

4. 2

s,d

s

s,d u

u

u

s

0?

sS

Co I Fe 1 Cr I

Cn

Co I Fe I Fei

Fe I

Ti I Ci

Cn

ITii Coi

4. 06

3. 56

3. 56

3. 19

3. 69

2. 94

2. 25

7. 48

3. 01

0. 83

3. 13

182

231

231

156

821

384

233

6

124

41

156

17

17

4763.89 m

4763.93 m 1 90

1 11. 8

1 11.

8

uu Nil 3. 65 146

4771.288 4771.472m

13

70

2. 7

14. 7

uw

4764.094r

4764.293

4764.531

4764.650r

4764.757

4764.87 m

4764.994r

3. 5

26

31

5. 5

11

2

2. 5

0. 7

5. 4

6. 5

1. 2

2. 3

0. 4

0. 5

s

u

s

s,iV

Cn

Ti II? Cn

3. 55

1. 24

3. 01

231

48

124

4771.712m

4771.897r

4772. 170r

4772.310

4772.625r

4772.823S

61

6. 5

2. 5

7

1

88

12. 8

1. 4

0. 5

1. 5

0. 2

19. 1

s

S

s

Fei

(Ci)

Zn

Fez

2. 20

7. 49

0. 62

/I. 56

13. 02

67

6

43

38 467

4765. 125r 2. 5 0. 5 4773. 021r 3 0. 6 4765.472m 95 19. 9 s,N Fei 1. 61 40 4773.143 11 2. 3 u

4765.662r 3 0. 6 4773.283r' 1. 5 0. 3 4765.864m 71 15. 5 s Mn I 2. 94 21 4773.413 17 3. 6 u Nil 3. 70 167

4766.08 a 4 0. 8 4773.527r 4. 5 0. 9 Fe I 3. 02 408

4766.33 m 5 1. 0 SI Til 2. 25 233 17 4773.704 5 1. 0 4766.423m 89 18. 7 s Mm 2. 92 21 4773.959 8. 5 1. 8 w? Ce II 0. 92 17

4766.636 21 4. 4 S V I Cn

(C I)

2. 04

3. 55

7. 48

113 231

6

4774. 540r

4775.127

1

5. 5

0. 2

1. 2

s

u CnCn

3. 01

3. 55

124

230

4766.780 33 6. 9 u 4775.502r 5. 5 1. 2 Cn? 4. 16 283

4766.869 20 4. 2 u Fe I p 3. 42 688 4775.67 a 1. 5 0. 3

191
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4775.877 20 4. 2 0? C I 7. 49 6 17 4784.711r 3. 5 0. 7

4776.070 29 6. 1 s Fe I 3. 30 635 4784.94 m 1 0. 2 S Zri 0. 69 44

4776.32 m

4776.360

4776.487

4776.81 a

4777. 183r

4777. 593r

4777.725

4777.85 a

1 52

24

2

2

1. 5

2. 5

1. 5

[ 4. 0

1 8. 2

5. 0

0. 4

0. 4

0. 3

0. 5

0. 3

s

8

S

-Co I Fe I -

Vi

-Vi

Cr I

Sm II

3. 30

4. 56

2. 05

2. 38

3. 01

0. 04

158

1206

113

128

124

3

4785.057

4785.19 a

4785.34 a

4785.688 4785.960m

4786.120 4786.289m

4786.542m

1. 5

2

2

16

30

3. 5

41

110

0. 3

0. 4

0. 4

3. 3

6. 0

0. 7

8. 6

23. 0

sw?

8

S

Co I?

Fe I

Nil

IINii Vi

3. 95

4. 14

1. 68

3. 42

2. 07

186

1044

50

98

113

17

4778.258m 16 3. 3 8 Ti I 2. 24 232 4786.814m 95 19. 0 u Fei 3. 02 467

4778. 580r 3 0. 6 4787. 102r 4. 5 0. 9

4779.05 a ? 1. 0 4787.503 11.51 0. 3 Fe I p 3. 02 408

4779.34 m S,N Sc I 0. 02 5 13 4787.64 m 8 Ti I p 0. 82 40 13 4779.445m 51 9. 8 u Fe I 3. 41 720 4787.833m 43 8. 8 U Fe I 3. 00 384

4779.69 a 4 0. 8 4787.97 a 3 0. 6 4779.984m

4780.453r

4780.54 a

4780.810

4781.014r

4781.32 a

4781. 452r

4781.720

4782.068

4782.280r

4782.56 a

76

3

2

10

1. 5

1. 5

8

15

10

2?

15. 9

0. 6

0. 4

2. 1

0. 3

0. 3

1. 7

3. 1

2. 1

0. 4

0. 6

w

w

Sw

Co I ITiii

Fe I

Co I Til

3. 28

2. 05

3. 25

1. 88

0. 85

158

92

633

57

41

17

4788.218

4788.51 a

4788.785S

4788. 935r

4789.137r 4789.342m

4789. 451r

4789.658S

4789.79 m

4789.92 a

4790.334

2. 5

1. 5

72

2

2. 5

71

5

96

3. 5

1. 5

16

0. 5

0. 3

1/,. 4

0. 4

0. 5

14. 7

1. 0

19. 4

0. 7

0. 3

S. 1

u

8

S

uS

s

Fei

Cri

Fe I

Ti I

Cr I

3. 24

2. 54

3. 55

0. 84

/2. 54

12. 54

588

31

753

41

3131

4782.801 5. 5 1. 1 Fe I 3. 24 588 4790.560 10 2. 1 u Fe I 4. 15 1068

4782.983 29 6. 1 0 Si I 4. 95 4790.748 10 2. 1 u Fe I 3. 25 632

4783.14 a 5 1. 0 4790.968 14 2. 9 8 Nil 1. 95 71 4783.424m 157 31. 8 s Mn I 2. 30 16 4791.143 30 6. 3 u,d 16

4783.69 a 7 1. 5 4791.256m 40 8. 3 u Fei 3. 27 633

4783.862 10 2. 1 s 16 4791.53 m 1 0. 2 S Sci 0. 02 5

4784.000 31 6. 5 w 4791.597 2. 5 0. 5 Sm 11 0. 10 7

4784.10 a

to 4784.55 a

4784.45 m

1 ' 1. 3

S

(Sri)

Vi

1. 80

0. 02

5

3 13

4791.83 a

4792.214

1

12

0. 2

2. 5 s,N? Si I Ti I p

4. 93

0. 81 40

192
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

ReH n f*pH Width

AX/X

(F)

Spot

Solar

Identification

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivakint Width

AX (mA)

(luceci Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

4792.315 28 5. 8 s,d Six 4. 95 17 4800.319r 1 0. 2 4792.514m

4792.862m

4793.10 a

4793 30 a

4793 433

4793. 741r

4793.967

77

40

1

2

4. 5

3. 5

9

16. 1

7. 5

0. 2

0. 4

0. 9

0. 7

1. 9

s

u

w

|Cri

Ti I Co I

Ni I

Fe I

3. 11

2. 33

3. 25

3. 70

3. 05

168 260

158

158

512

4800.545 4800.653m

4800.841r 4801.031m

4801. 235r

4801.612

4801.914r

8. 5

72

2. 5

56

4

6

1

1. 8

15. 0

0. 5

11. 7

0. 8

1. 2

0. 2

w

s

S,N

Fe I p Fe I

Cri

Fe I p

/ Tiip

1 Ti I D

3. 30

4. 14

.3. 12

4. 28

0. 83

0. 82

590

1042

168

1115

4040

4794.359 13 2. 3 u Fe I 2. 42 115 4802.30 a 1. 5 0. 3

4794.644r HI 0. 2 4802.522 19 4. 0 u Fe I 4. 61 1206

4794.838r 2. 5 0. 5 Ti II p 1. 13 29 4802.693r 1. 5 0. 3

4795.835 7 1. 5 s,d Co I 3. 95 185 17 4802.887S 70 13. 7 u Fax /3. 64

\3. 69 888

934

4796.042r

4796.189

6. 5

24

1. 4

5. 0 s CriII Ti I

4. 19

2. 33 283

260

4803. 047r

4803.31 a

3. 5

1 1 51

0. 7

0. 3

4796. 365r 3. 5 0. 7 s Co I 0. 43 14 4803. 685r 3. 5 0. 7

4796.54 a 2 0. 4 4804. 047r 4 0. 8

4796.657 6 1. 3 4804.13 a 3 0. 6

4796.905 12 5 s V I 2. 10 113 4804.23 a 1. 5 0. 3

4797.046 9 1. 9 4804.38 a 2 0. 4 Zr II 1. 21

4797.168 2. 5 0. 5 s,d 17 4804.521 26 5. 4 u Fe I 3. 57 794

4797.358r 0. 5 0. 1 4804. 648r 8. 5 1. 8 Cr I 2. 71 61

4797.622

4797.722r

4797.975

6

3

7. 5

1. 3

0. 6

1. 6

1

) s

Cr I

Ti I

3. 56

2. 33

230

260

4804. 850r

4805.007

4805.099

3

1 128

J

0. 6

j 6. 0

[ 20. 6

11 w Ti II 2. 06 92

4798. 107r 2. 5 0. 5 4805.292 3. 5 0. 7 Cr I? 4. 17 283

4798.270m 47 9. 2 u Fe I 4. 19 1042 4805.420m 37 7. 7 Ti I 2. 34 260

4798.537m 50 9. 6 wl Ti II L 08 17 4805.55 a 4 0. 8 Fe I? 4. 64 1207

4798.736 35 6. 9 Fe I 1. 61 38 4805.89 m 2 0. 4 s Zr I 0. 69 43

4799.070 2. 5 0. 5 Fe I p 4. 28 1098 4806.252

' 7 1. 5 Cr I 2. 71 61

4799.251r 0. 5 0. 1 4806.333 6 1. 2 U Ti II p 1. 08 17 4799.413m 36 7. 5 u Fe I 3. 64 888 4806.616r 5. 5 1. 1

4799. 585r 3 0. 6 4806.799r 4. 5 0. 9 S Ti I p 0. 81 40 4799.794m

4799.890

1

1

''^

f 10. 2

[ 6. 0

s

u

ViIjTii Fe I0. 00

2. 27

3 242 4806.994m

4807.225

70

16

IS. 7

3. 3

w

s,N

Ni I

Fe I

3. 68

/3. 30

14. 26

163

634

1098

4800.022 1. 5 0. 5 4807.40 a 4 0. 8

4800.134 19 4. 0 s Fe I 3. 04 384 17 4807.533 15 3. 1 S Vi 2. 12 113

193
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4807.716m 60 11. 4 s Fe I 3. 37 688 4815.491r 2 0. 4

4807.91 a 3 0. 6 4815.637r 2 0. 4 -S Zr I 0. 60 43

4808.00 a 2 0. 4 4815.816 2. 5 0. 5 u Sm II 0. 18 14 4808.158m 30 6. 2 s Fei 3. 25 633 4815.932 16 3. 3 s,d Ni I 3. 54 131 17 4808.545m 34 7. 1 s Ti I 3. 06 305 4816.129 4 0. 8 s?,N Cr I 4. 53

4808.685 47 9. 8 u Fe I 4816.423r 3 0. 6 Cn? 4. 19 283

4808.879 28 5. 8 u Ni I 3. 70 160 4816.46 m 3 0. 6 S,N Tiip 0. 82 40

4809.02 a 2. 5 0. 5 La II? 0. 23 37 4816.682r 3 0. 6 Fe I p 3. 27 588

4809.145 17 3. 5 u Fei 3. 69 933 4816.965r 3 0. 6

4809.267

4809.477r

4809.619r

4809.941

12

3

2

20

2. 5

0. 6

0. 4

4. 2

ul

s

s

Fe I Cr I?

Zr I?

Fe I

4. 07

3. 55

1. 58

3. 57

1039 230

793

4817.20 a

4817.376r

4817.637r 4817.808m

1. 5

9. 5

2. 5

62

0. 3

2. 0

0. 4

12. 9 s,d

C I

|FeiNi I

7. 48

2. 22

4. 15

5

67 254

4810.26 a 3. 5 0. 7 Cr I? 4. 53 4818.032 19 3. 9 u Fei

4810.537m 84 16. 2 w Zn r 4. 08 2 4818.245r 1 0. 8 Fe II p 2. 28 11

4810.733 13 2. 7 s Cr I 3. 08 144 4818.29 m

1

8. 5

1 0. 8 s 4811.046m

4811.352

4811.89 m

4811.993

4812.241

4812.352

4812.894

4813.005

4813.117

4813.264r 4813.479m

4813.719

4813.973

16

9. 5

3. 5

25

6

41

8. 5

7. 5

24

2. 5

51

6. 5

9. 5

3. 3

2. 0

0. 7

5. 2

1. 2

8. 5

1. 8

1. 6

5. 0

0. 5

10. 0

1. 3

2. 0

s

s

sw

sw

s

s

s,d

Fe I ITii Nd II Sn

Nil

Ti I Cr II Til

Fe I

Co I Fe I p Co I Vii

3. 07

1. 89

0. 06

1. 85

3. 66

2. 34

3. 86

0. 85

3. 27

3. 21

4. 58

3. 30

3. 76

467

158

3

5

130

260

30

41

630

158

1243

158

197

17

4818.386r

4818.660r

4819.022r

4819. 186r

4819.342r

4819.644

4820.13 a 4820.414m

4820.58 a

4820.78 a

4821.000

4821.126

4821.29 m

4821.479

4

2. 5

3

10

4

3

1

44

1. 5

1. 5

6. 5

33

3

8

0. 8

0. 5

0.6

2. 1

0. 8

0. 6

0. 2

8. 7

0. 3

0. 3

1. 3

6. 8

0. 6

1. 7

s

s

w

s

0

Fe I p

Ti I

Yi?

Til

Ti II p

Ni I Til

3. 41

1. 36

1. 50

1. 12

4. 15

2. 16

719

13

126

29

254

201

4814.268 12 2. 5 s Cn 3. 09 144 4821.601 4 0. 8 Fei

4814.369 13 2. 7 s,d Fei 17 4821.85 a 2 0. 4

4814.594 20 3. 7 w Nil 3. 60 98 17 4822.324 7 1. 4

4814.874r 4. 5 0. 9 4822.564 11 2. 3

4815.056r 2 0. 4 s Zr I 0. 65 44 4822.667 9 1. 9 u Fei 3. 27 633

4815.223 14 2. 9 u Fei 3. 41 720 4822.820r 3 0. 6

4815.309r 5 1. 0 4822.962r 5 1. 0

194
The Solar Spectrum—Continued

length

(1)

Equivalent Width

(ml)

Re- duced

Width

i\K\K (F)

Spot

ooiar

IdentiLow

IT T> 11/ i or

ivOTj. Line

RMT

IN 0. or

V ID. Band

Qy. o 9 n o AT

4823.309 29 6. 0 W Yii 0. 99 22

4823.514in 165 S2. 5 S Mm 2. 32 16

4823.896 16 3. 3 Cr I 4. 53

4824. 143S 94 19. 5 W II Cm

T i? C 1

3. 87 30 ooo

AQ.OA 90 TYi Ko 1. u co U. DO

9 O A

O. 0 ±. o

9 c; U. 0 IN 1 1 Ai. nouy

i. 0 u. o

9 nu. A^

4824.956 8. 5 1. 8

Qo

K 9 w J: c 1

1ios 7 s"NTH TT TilIPt- t

u. io

2. 32

Q no 2501/1/1

4,00 c Afl4.r D. 0

1 ivin I Q QA

4825.720 7. 5 1. 6 Fe II p 2. 63 30

4826.12 a 1. 5 0. 3

4826.364 6 1. 0

4826.841 19 3. 9 s,N Ci?-

Mn T?

7. 49

O. oO

5

/I Q

111 n 9

9 7 oo \T T V I U. U4 Qo

91 ^. o -111? AI ii I — 9 Qn ^OU

^o^o.UU III U. o

n 1 s ZjV I

fi fi9 A A 44

rto-uo.OOUl 9 p; u. o

Q 9 n s li Q 1 oi

4828.859r 3 0. 6 4829.027m 91 18. 0 u Nil 3. 54 131

4829.168r 3. 5 0. 7

4829.309r 1. 5 0. 3 SI

4829.369in 84 17. 4 s Cri /2. 54

Lz. 54

31

31

4829.695r 5. 5 1. 1 Fe i?p 4. 24 1038

4830.303r 1. 5 0. 3

4830.519 3 0. 6

4830.93 a 1. 5 0. 3

Notes

17

21

VV dVvi- length

(A)

Equivalent Width

A \ LA A (ml)

Re- duccd

Width

(F)

Spot

oolctr Identification

Low

111 1 or

J tot. Line

RMT

XNO. or

V ID. Band

4831.182m 81 75. .9 w Nil 3. 61 111

rioo i .oyo 9A 0. u s

4831.651 16 S Vi

(Cri)

0. 02

3. 42

3 208

4831.916r 2 0. 4 /R 92 0,01

U,UJ

4832.041 7 1. 4 s Sri

1, 11 1;

11.// n 77 U- 80

9 ?n

5 9^n

4832.277r 3 0. 6 s

1 9 'P 7 o V I V 1 n on o.

^lOOiii.ooo 1. O u. O 4K^9 71 QC? ^oo.^. / lyo Do It:. 1 IN 1 1 —

|Fei

O. OU

;3. 64

1 4 "^n

11t:U 4K 888

ivjyo

AQOO QQ9« 'ioo^.oy^r 9 u. ^

^oOo.UO 111 1. O U. O ojiV VV T1 1±. 71/

7R

AQ'\'X 1 Q9 Qy 11. Qy

TTo TT ir\ IT tJ 11 \J 9 ftp. ou

^ooo.o / or 9 p; u. o

"1:000.0 * Ol 9 Pi u. o

4ooo.oiy QO 11. 74 s JC c 1

4ooo.yoir 7/. 0

1 Pi 1. o

4oo4. 1 / or 0 ±. u

^oort.ooor 1 0 9 Cn T? 9 m o^7/

'IOOt:. 01 / III 98 o.

P^ So TTp T JC C 1 2. 42 J. J. o

'ioO'l:. DUy co 11. 7/ SmOiJLl TT? 11 1 0 48 4^TtO

4oo4.oior 9 P. u. o 1\ 1 1 ^

^ fi8 1

1 O 9 ^cqc 979 O. 0

1 1 1. 1

4oo0.040r 9zl. O^ n Pi u. o

/I PI '7C\A 4ooO. / U4 9 U. 4 s v-^r 1

'if; O. OO 99Q

4835.875m 44 9. 1 s Fei 4. 10 1068

4835.999

' 5 1. 0

4836.122 5. 5 1. 1 s Til 2. 27 241

4836.238 33 6. 8 w f|Cr 11

"Ml' IN T 1 1

3. 86

74 30114

4ooD.oO a 9 flyj. 4t: Cr r ^ 80

4836.460 7 1. 4

4836.674r 3 0. 6

4836.857 16 3. 3 s Cri 3. 10 144

4837.046r 2 0. 4

761-925—6€ -15 195
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

cr Rot. Line

RMT

No.

or Vib. Band

Notes

AQO'7 A no

4oo / .oOor

U. O

i. o

O. 0

U. 1

U. o n 1 U. /

s 11 I P

r e I

0 00

4. 00 1 OA ^

AOA A nOOvr^

4844.222r

4844.311

4

12

0. z

0. 8

2. 5

s

s,TSI

lli'e I Ti I Sm II Mn X

0. 55

2. 24

0. 28

3. 84

/ oil 217

26

43

4837.825r 2. 5 0. 5

fT? Ql IR 92n n

0,0 }19 4844.503 12 2. 5 s

4837.946r 1. 5 0. 3 Co I 0. 63 15 4844.701r 0. 5 0. 1

4838.092 9 1. 9 w Fe I 3. 25 630 17 4844.875r 1 0. 2

4838.219r 4 0. 8 Mn I 3. 86 43 4845.165 3. 5 0. 7 s Ni I 3. 70 115

4838.3411- 2 0. 4 4845.338 3 0. 6 4838.521m 51 10. 5 s? Fe I 3. 42 687 4845.506r 0. 5 0. 1 4838.650m 45 9. 3 Ni I 4. 16 260 4845.656m 36 7. 6 s Fe I /3. 27

yo. DO 588

000

4838.827r 3. 5 0. 7 Fe i?p 4. 43 1167 (Yi) 1. 40 13

4839. 120r 4. 5 0. 9 4845.805r 4. 5 0. 9

4839.25 m 1. 5 0. 3 s Ti I 2. 23 217 4846.001r 0. 5 0. 1

4839.363r 2 0. 4 4846. 156r 2 0. 4

4839.551S 55 11. S s? Fe I 3. 27 588 4846.33 m 5 1. 0 s,lS! Or I 3. 45 208

4839.782 7. 5 1. 5 Fe I p 4. 61 1206 4846.385r 10 2. 1

4839.884 12 2. 5 s Yi 1. 43 13 4846.64 a 1 0. 2

4840.004 9 1. 9 Fe II p 2. 68 30 4846.712r 3 0. 6

4840.263

I CQ 1

8. 7 Co I 3. 17 158 4846.87 a 1 0. 2

4840.316

! oo

1 12. 6 u Fe I 4. 15 1068 4847.191 3. 5 0. 7 Or I 3. 10 144

4840.66 a 3. 5 0. 7 4847.311 20 4.5 s Ca I 2. 93 50 4840.884m 60 IS. 6 s Ti I 0. 90 53 4847.44Sr 6 1. 2

4841. 497r 3. 5 0. 7 4847. 623r 3 0. 6 Fe II p 2. 69 30

4841.674 8 1. 7 s? Fe I p 3. 30 633 4847.734 4. 5 0. 9 Sm II 0. 66 53

4841.791 24 5. 0 Fe I 4. 19 1070 4847.924r 0. 5 0. 1

4841.969 6 1. 2 s,iV Nil 4. 16 260 4848.087r 1. 5 0. 3

4842. 209r 2 0. 4 Fe i?p 3. 05 511 4848.252m 52 11. 1 w Cr II 3. 86 30

4842. 588r 2. 5 0. 5 4848.418 5 1. 0 S Ti I p 2. 25 217

4842.727

4842.793 1 44 j X.7

[ 7. 8 u

Fe I p Fe I

4. 22

4. 10

1098

1069

4848.471

4848.650r

11

2. 5

2. 3

0. 5

S Ti I 2. 17 201

4842.937r

4843.152m

4843.368r

4843.507

4. 5

67

12

20

0. 9

13. 8

2. 5

4. 1

u

u

C2 ?

|Fe I

"Ml* iM rI Fe I p

|Co I Ni I

/R 90 \R 91

3. 40

1. DO

3. 57

3. 28

4. 17

0,0

0,0 687

OU

794

158 235

4848.887m

AQACi A*7C — 4o4y.u/Dr

A QA n 1 '70

4849.341r

4849.42 a

33

A

OZ

6. 5

4

6. 8

U. 0

D. 0

1. 3

0. 8

a

w

Fe I

Ni I p —

Ti II p

2. 28

0. 0^

1. 13

114

29

4843 .694r 3 0. 6 4849.553r 9 1. 9

4843 .846r 1 0. 2 W I 0. 41 1 4849.663 16 3. 3 u Fe I 3. 57 793

196
The Solar Spectrum—Continued

VV tl V c— length

(A)

EquiWidth

AX (mA)

Recluccd Width

(F)

Spot

Solar

IdentiTlXlK^cHjiK/ Cfl t i OTlLI

Low

Hi it or Rnt IXU t. Line

RMl

Ol'

V I u, B;uic

Notes

1

Icngth

(A)

EquivnV CiilV^ lori1 1 fu Width

AX

(ml)

Ref 1 UCCfl Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMl

No.

or Vib. Banc

Notes

I

Qo 4857 OOQr 4 0 ^> 2r II 1. 24

QO yj. L 4857 39 'im 42 0 ^ Ni I 3. 74 111

4.Rp;n 901r 1 c 1. c Cr I? 3. 37 4857 'ifi'^r

4850.749r 2 0. 4 4857.786r 2 0. 4

4850.941r 1 0. 2 Cr I? 3. 37 4857.97 a 1 0. 2 Co I 0. 58 15

4851. 136r 1 0. 2 4858.142 8 1. 9 w7

4851.323r

4851.35 m

4851.496m

2. 5

31

0. 5

6. 8

S

s

Zr I V I0. 62

0. 00

3. 43

43

3 208

13

4858.254

4858 330

4858 494r

8. 5

o. o

I

2. 0

1 2

0. 2

Fe I /4. 19

14. 28

1069

1098

48*11 fiSflr 5 14.. nu 4859 039 1 ^ 3 jj 0. 32 3

8o. o"i 1 7 4859 134 1 S 4 7 U Fe I 4. 19 1068

^(JxJJL .\J J. V 11 2. 3 4859 3n4r nO. 9<J 11 AT Fe I p 3. 30 632 4852 'ifi2m 36 7. 4 tv Ni I 3. 54 130 4859 4Sfir 0 7 4852 fi8 m 0. 2 Y I 1. 37 13 4859 747m 108 27. 4 S Fe I 2. 87 318

0. 5 0. 1 4860 022r 9 0o. 7/ 4853 03 7r 3. 5 0 7 4860 21 7 Q 2 7 0 CrV.-'X TTXI 3 87 30

4853.277 7 1. 4 w Ni I p 3. 90 207 4860.986 3. 5 2. 3 s Fe I 3. 40 688

4853.543r 2 0. 4 Cr I? p 2. 71 61 4861.19 m s? Cri 2. 54 31 13

4853.777 16 3. 3 w Ni I 3. 54 99 4861.342m 3680 750 w 10. 20 1

4853.877

4854WTC t 161 I.\J X

5

3

1. 0

0. 6 ^ Fe I p

/R88

\R 89

4. 59

0,0 0 0

1243

}19

4861.849

4861.952

15

11

5. 6

4. 1

s

s

Cr I Fe I (Mn i)

2. 54

3. 85

31

TO

4854.352r 2. 5 0. 5 s Sm II 0. 38 36 17 4862.187r 2. 5 0. 8 4854.616 4 0. 8 Mn I 3. 86 43 4862.26 m S,d? 13,16 4854.76 m 2. 5 0. 5 s Ti I 2. 24 217 4862.551r 1. 5 0. 4 Fe I p 4. 15 1070

4854.873m

4855.154

4855.234r 4855.418m

4855.556 4855.681m

4855.905 4856.019m

4856.195

4856.398r

4856.62 a

4856.901r

41

7. 5

3. 5

73

13

60

14

39

19

3

1. 5

2

8. 8

1. 5

0. 7

15. 4

2. 7

13. 0

2. 9

8.4

3. 9

0. 6

0. 3

0. 4

w

s

s?w

0

sw

s w,N

|Y II Fe I Cr I Co I Ni I Fe II p

Fe I

Ti I Cr 11

0. 99

4. 14

2. 71

0. 51

3. 54

2. 70

3. 37

2. 25

3. 85

22

1043

61

14

130

25

687

231

30

4862.598

4862.90 m

4863.096r

4863.250r

4863.468r 4863.650m

4863.75 m

4863.784 4863.936m

A oc A 1 on 4864. 180 4864.323m

4864.738

4864.85 mi

16

1. 5

1. 5

0. 5

48

8. 5

22

3

50

24

2

4. 5

0. 4

0. 4

0. 1

11. 7

2. 2

5. 3

0. 7

11. 7

5. S

0. 4

s

s

u

s

u

Ct o

w,d

S

s

Fe i?pCoi?

Fe I Tiip

Fe I p Nil

il I Cm

Vi

Vip

4. 15

1. 96

3. 43

2. 25

3. 04

3. 74

2. 16

3. 86

0. 02

1. 18

1069

687 217

384

113

201

30

3

50

13

13

197
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

' Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

4865.08 a 1 0. 2 4873.092r 2 —

0. 4

4865.21 a 1 0. 2 4873.255 24 4. 9 w Ni I p 3. 74 112

4865.42 a 1. 5 0. 3 4873.446m 58 11. 9 w Ni I 3. 70 111 4865.618m 34 7. 6 w Ti II 1. 12 29 4873.608r 2. 5 0. 5

4866.07 m 3 0. 6 s Zr I 0. 73 44 17 4873.750 12 2. 5 s Fe I 3. 30 633

4866.277m 66 14. 6 u Ni I 3. 54 111 4873. 872r 1 0. 2

4866.50 a

to 4866.65 a } '

1

0. 6 4874.014

4874. 196r

34

3

7. 0

0. 6

w — Ti II 3. 09? 114

4866.743 2 0. 4 Fe I p 4. 18 1093 4874.360 18 3. 7 s Fe I 3. 07 467

4866.883 2 0. 4 Si I? 4. 95 4874. 510r 2 0. 4

4867.26 a 1 0. 2 4874.651r 2. 5 0. 6 s Cr I 3. 11 167

4867.537 7. 5 1. 5 s,N Fe I 1. 61 38 4874.793 21 4. 3 w? Ni I 3. 54 98

4867.639r 2. 5 0. 5 Fe I p 3. 27 587 4874.85 m 3. 5 0. 7 s,N

4867.874m

4868.122

54

5. 5

11. 5

1. 1

u

u

Co I 3. 12 158 4874.994r

4875.033

i 27

J

1 0. 3

[ 5. 2 u

4868.263m 26 5. 5 s Ti I 2. 24 231 4875.198r 3 0. 6 CH? Q 8 0,1 4

4868.38?m

4868.45?m

26

J

[ 2. 9

1 2. 9

w?

M?

Fe I 1. 56 38

J

4875.26 m

4875.339r

2

2. 5

0. 4

0. 5

s,N Fe I? p 4. 19 1038

4868.808r 2 0. 4 Fe II p 2. 68 30 4875.492m 41 8. 4 S V I 0. 04 3

4868.931 2. 5 0. 5 0 4875.739r 3. 5 0. 7 Fe I p 4. 59 1243

4869. 147r 2. 5 0. 5 Ru 1 0. 93 11 4875.881m 55 11. 3 s Fe I 3. 33 687

4869.469 20 4. 1 u Fe I 3. 55 751 4876.093r 3. 5 0. 7 Sr I? 1. 80 4

4869.65 a 1. 5 0. 3 4876.195 8 1. 6 Fe I 3. 25 631

4870.043 12 2. 5 u Fe I? 3. 93 985 4876.401 41 8. 4 w Cr II 3. 85 30

4870.136m 36 8. 8 s Ti I 2. 25 231 4876.485 25 5. 1 0 Cr II 3. 86 30

4870.419r

4870. 645r 4870.816m

5. 5

3

74

1. 1

0. 6

15. 2 u

C2

llCri Ni I

/R 85 IR 86

3. 08

3. 74

0, 0

0, 0

143

131

4876.673r

4876.80 a

4877.08 a

to 4877.33 a

4. 5

2

} ^

0. 9

0. 4

0. 4

4870.94 a 4 0. 8 4877.596 21 4. 3 u Fe I 3. 00 384

4871.049 9 1. 8 4877.851r 13 2. 7

4871.325m

4871.680

228

15

46. 6

3. 1

u Fe I 2. 86 318 4878.128

4878.220

187

i

f 19. 5

[ 24. 2

sw

Ca I Fe I2. 71

2. 88

35

318

4871.935m 45 9. 2 u Fe I p 3. 25 630 4878.509r 5 1. 0

4872.144m 195 39. 2 s Fe I 2. 88 318 4878.721r 3 0. 6 CH Q 7 0,1 4

4872.508r 7 1. 4 s Sr I 1. 80 4 4879. 150r 2 0. 4 CH? Q 7 0,1 4

4872.688 9 1. 8 Fe I p 4. 26 1115 4879.520r 1 0. 2

4872.908 1 10 2. 1 u Fe I p 4. 22 1097 4879.702r 0. 5 0. 1

198
/Vr

The Solar Spectrum—Continued

"Wavelength

(A)

Equivalent Width

AX

(ml)

ReducGcI Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width AX

(ml)

Re- Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or

Rot.- Line

RMT

or

Vib. Band

Notes

4880 045 5 1. 0 Cr I 3. 12 167 4886.709 8 1. 6 Ni I 3. 70 158

4880.27 m

4880. 320r

4880.527

1 1.5

1

8

f 0. 1

[ 0. 2

1. 8

s

s,N

Co I

V I

0. 51

1. 19

15

50

4886.846

4887.009m

3

63

0. 6

12. 9 S

V I —

CH?

llCri Ni I

1 10 Q4

3. 09

3. 63

0,1

143

141

16

4

4880.59 m 1 0. 2 S 4887.195m 62 12. 7 w,N Fe I- 4. 19 1065

4880.935 9 1. 8 S Ti I 2. 15 201 4887.363 18 3. 7 u Fe I p 4. 07 1037

4881.08 a 3 0. 6 4887.533r 5 1. 0

4881.24 m

4881.267r

4881.31 a 4881.561m

2

2

49

0. 4

0. 4

10. 0

s

S

Zr I CH?

V I

0. 65 Q 6

0. 07

44

0,1

3

13

4

4887.690

4888.158

4888.525 4888.639m

7

3 5

1. 4

0. 7

1

3. 7

I 15. 7

s

su

Zr I? Or I

Cr I Fe I

0. 73

2. 54

4. 10

43

.A

31

1066

16

4881.724m 61 12. 5 u Fe I /3. 30 U. 14 588

1041 4888.829r 7. 5 1. 5 -CH? Q 3 0,1 4

*iooi.y4or

4882.148m

4882.337r

4882.489r

c0

70

9

4

1 n 1. U

IS. 9

1. 8

0. 8

11

s

Fe I

Ti I Ce II

3. 42

2. 25

1. 35

687

231

4889.004

4889.111

4889.648r

121

J

1

f 14. 3

I 12. 7

0. 2

s

u

Fe I

Fe I

C2

ro on

J Z. zU

13. 55

3. 88

0/ 749

985

4882.60 a 1. 5 0. 3 4890.215r 5 1. 0 s Cr I /5. 49

15. 50

4882.705 6 1. 2 Co I 3. 25 158 4890.438r 9 1. 8 Q Ni I 3. 77 114

4882. 91 Or 3 0. 6 4890.763m 220 47. 6 XL Fe I 2. 87 318

4883.132r 2. 5 0. 5 4891.041 12 2. 4

4883.35 a 2 0. 4 4891 150 15 3. 1 0?

4883.44 a 6. 5 1. 3 11 V II — 3. 79 209 4891.502m 312 64. 8 u Fe I 2. 85 318

4883.690m 51 10. 6 w Y II 1. 08 22 4891. 866r 2. 5 0. 5 s? Ti I 2. 17 201

4883.900 6. 5 1. 3 0 4891. 957r 2 0. 4 Cr I? 2. 71 61

4884.051 7. 5 1. 5 V II 3. 76 197 4892.865m 44 9. 0 w Fe I 4. 22 1070

4884.598 21 4. 3 0 Cr n 3. 86 30 4893.047r 3 0. 6 s Til 2. 25 231

4884.803r

4884.941 4885.088m

4885.236r 4885.434m

4885.620r

4885.774

4885.949

4886.086r

4886. 177r 4886.337m

7. 5

11

53

3

60

1

22

12

1

0. 5

68

1. 5

2. 2

12. B

0. 6

12. 7

0. 2

6. 1

2. 4

0. 2

0. 1

13. 9

S,N

s

u

s?

s

s

s

s

CH?-

Cr I

Ti I

Fe I

Cr I Cr I CH?

Fe I p Fe IQ 5

2. 54

1. 89

3. 88

2. 54

3. 09 Q 4

3. 11

4. 15

0,1

30

157

966

30

143

0,1 467

1066

4

17

4

4893.13 m

4893.253r

4893.425r

4893.570r

4893.704

4893.817

4893.92 m

48yd. your

4894.370r

4894.562

4894.797r

0. 5

0. 5

2

1

4

11

1. 0

3

8. 5

1

0. 1

0. 1

0. 4

0. 2

0. 8

2. 2

U. 0

0. 6

1. 7

0. 2

s

s

u

0

s

w

Zr I

Til

Fe I p Fe I Fe II Til ue tt9 III Cr I

rO. 69 U. 58

4. 18

4. 21

2. 83

2. 16

5. 52

43

1096

1113

36

201 13

199
The Solar Spectrum—Continued

Wave1 PTl crt.Tl

Equivalent Width

AX \mA)

Re- duced

Width

AX/X

\r )

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

Equivalent Width

AX

Re- duced

Width

AX/X

\r >

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib.

Baiiid

Notes

4894.85 a 1. 5 0. 3 4902.236 11 2. 2 w

4895.034r 0. 5 0. 1 4902.384 8. 5 1. 7 u Fe I

4895.661r 2 0. 4 Fe I? 4902.62 a 3 0. 6

4895.85 a 1 0. 2 4902.75 a 2 0. 4

4895.99 m s 13 4902.97 a 2 0. 4

4896.05 a 1 0. 2 4903.099r 4. 5 0. 9 Fe I? p 3. 30 589

4896.442m

4896.580

26

8

5. 3

1. 6

u Fe I 3. 88 984 4903.259

4903.316 1 157

[ 9.

0

1 27. 5

s

ul

Cr I Fe I2. 54

2. 88

31

318

4896.94 m 0. 5 0. 1 s 4903.61 a 3 0. 6

4897.200r 4 0. 8 Co I 3. 93 4903.717r 1. 5 0, 3 s Ti I?

4897.36 a 1. 5 0. 3 4904.171r 4 0. 8 Co I 2. 87 141

4897.473r 6. 5 1. 3 0? 17 4904.30 m s V I 1. 19 50 13

4897.65 m 1. 5 0. 3 s 4904.418m 91 18. 6 u Ni I 3. 54 129

4897.85 a 3 0. 6 4904.830r 2 0. 4

4898.27 m 1 0. 2 s 17 4905.138m 30 6. 1 u Fe I 3. 93 986

4898 473r 2 0. 4 Cri 5. 50 4905.22 a 2. 5 0. 5

4898 619r 2. 5 0. 5 4905.32 a 2. 5 0. 5 4898 81 a 1. 5 0. 3 4905.802r 1 0. 2

4898.94 a 3. 5 0. 7 Fe I? 4905.90 a 2. 5 0. 5

4899.513 5 1. 0 u,N Co I 2. 04 92 4906.133 5 1. 0 Fe I?

4899.56 a 2. 5 0. 5 4906.44 a 1. 5 0. 3 S,N 17

4899.738r 0. 5 0. 1 4906.706r 3 0. 6 4899.917m 57 12. 2 s IITii La II (Ba II)

1. 88

0. 00

2. 72

157

7

3

4906.775

4907.053r

7

1 5

1. 4

f 0. 4

0 Fe I p 4. 22 1096

4900.02?m s? Ti I p 2. 66 295 13 4907.12 a 1 1 0. 6 Co I 0. 43 14 4900.124m 54 10. 8 u Y II 1. 03 22 4907.315r 1 0. 2

4900.276r 3 0. 6 4907.43 a 1. 5 0. 3

4900.469r 2 0. 4 4907.502r 1 0. 2

4900.629r

4900.821

4900.970

3

12

17

0. 6

2. 4

3. 5

s,d Ti I V I Fe I Ni I Ti I

2. 68

2. 12

3. 48

295

118

98

4907.735m

4908.032

4908.272r

4908.45 m

61

37

1. 5

12. 0

7. 5

0. 3

s

s

s

Fe I -Fe I

Ti I

3. 43

4. 22

2. 69

687

1065

295 13

4901. 319r 1 0. 2 4908.495r 1. 5 0. 3 Co I 3. 53

4901.614r 2 0. 4 4908.611 4. 5 0. 9 u Fe I 2. 48 115

4901.75 a 1 0. 2 4908.834r 0. 5 0. 1

4901.91 a 3 0. 6 4908.95 a 1 0. 2

4902.078r 3. 5 0. 7 Cr I? /4. 21

14. 21

4909. lOor 5. 5 1. 1 S Til 0. 83 39

4909.199r 3 0. 6

200
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

ixe- duccd

Width

AX/X

(F)

Spot

Solar

Identification

Tjow

EP

or Rot. Line

iA-iVi R MTL No.

or Vib. Band

Notes Wavelength

(1)

valent Width

AX (ml)

itC- ducod

Width

AX/X

(F)

Spot

Solar

Identification

IjOW

EP

or Rot. Line

No.

or

Vib. Band

Notes

4909.387m 66 IS. 6 u Fe I 3. 93 985 4916.674 4. 5 0. 9 0 Fe I p 3. 93 986

4909.51 a

4909.710r

4909.87 a 4910.020m

4910.330m

4910.44 m

4910.570m

4910.774r

4911.027r 4911.199m

4911. 390r

4911.536 4911.782m

4912.025m

4912.185r 4912.39?m

4912.491

4912.62 a

4912.787r

4912.980r

4913.135

3

5

2

91

79

2. 5

80

4

1. 5

50

6. 5

24

44

47

4. 5

1

9. 5

1. 5

0. 5

1

12

0. 6

1. 0

0. 4

18. 1

16. 1

0. 5

16. 3

0. 8

0. 3

10. 6

1. 3

4. 9

8. 8

9. 6

0. 9

0. 2

1. 9

0. 3

0. 1

0. 2

2. 4

su

su

u

uu

u

s?u

w

Nil

Fe I Fei

Fe I

-Ti II

Fe I p

Fe I Nil

Co I Fe I

3. 77

3. 40

4. 19

4. 22

3. 12

4. 26

3. 93

3. 77

0. 58

4. 14

687

1068

1068

114

1098

984

111

14

1040

16

4916.852r

4916.958r 4917.235m

4917.353r

4917.828r 4918.015m

4918.173r 4918.371m

4918.50 m

4918.709m

4918.998m

4919.306r

4919.448r

4919.749

4919.872

4920.065r

4920.298r 4920.514m

4920.686r 4920.963m

3. 5

2. 5

60

5. 5

2

53

4. 5

75

3

39 278

3

9

11

24

4

I 471

1 29

0. 7

0. 5

12. 2

1. 1

0. 4

10. 8

0. 9

15. 2

0. 6

7. 9

53. 7

0. 6

1. 8

2. 2

4. 9

0. 8

/I 85. 6

I 6.9

5. 9

u

u

uS

u

s

s

s

S

s,N? u

Fe I

Fe I

Nil

Nil

Fe I

C2Cr I Fe I p

Til

Co I Fei

-Nd II |CriLa 11

/R 76 IR 77

4. 19

4. 23

3. 84

3. 77

2. 86 R 69

5. 52

3. 27

2. 16

1. 96

2. 83

0. 06

3. 10

0. 13

0,0

0. 0

1066

1070

177

113

318

1, 1

631

200

57

318

2

143

7

}'»

16

19

4913.273r 2 0. 4 Sm II 0. 66 53 4921. 168r 2. 5 0. 5 Nii?p 3. 60 100 4913.622m 49 10. 0 s Til 1. 87 157 4921.30 a 1 0. 2

4913.803r 3 0. 6 4921.42 a 1 0. 2 4913.978m 57 11.4 w Nil 3. 74 132 4921.50 a 0. 5 0. 1

4914.13 a 4 0. 8 4921.598r 0. 5 0. 1

4914.224r

4914.406r

4914.522

4914.68 a

4914.92 a

4915.234

4915.775r

3. 5

6. 5

5. 5

2. 5

|2. 51

6

2

0. 7

1. 3

1. 1

0. 5

0. 5

1. 2

0. 4

s

ul

s

s

Til

Ti I? Fe I?

1. 89 157

4921.785m

4921.988r

4922.162- 4922.267m

4922.489r

4922.62 a

4922.821

40

1. 5

J 97

2. 5

0. 5

6. 5

8. 1

0. 3

{

"

[ 15. 8

0. 5

0. 1

1. 3

s

u

8

S?

ITiiLa II

Fe I p

Cn

2. 17

0. 24

4. 21

3. 10

200

7

1110

143

4915.849r 3. 5 0. 7 4922.979r 1 0. 2

4916.238 6. 5 1. 3 w 4923.154 16 3. 2 Fe I 17

4916.487 14 2. 8 u 4923.28 a 4 0. 8 Cr I?

201
The Solar Spectrum—Continued

^Wavelength

(A)

EquiV <XlCi-i U Width

AX

(ml)

Re- Width

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- Width

AX/X

(F)

Spot

Solar

Identi-

"fi pft firm

Low

TTS2j PIT or

T?XY(n+) t. Line

RMT

iN 0. or

V ID. Band

Notes

3. 5 0. 7 4930. 479r 3. 5 0. 7

4923.57 a 4. 5 0. 9 4930.66 m 2. 5 0. 5 s

4923.68 a 5. 5 1. 1 4930.800 19 3. 8 s Ni I? 3. 85 193 4923.930m 167 S3. 3 w Fe II 2. 89 42 4930.94 a 2 0. 4

4924.123r

4924.302

4924.56 m

4924.588r 4924.777m

4924.964r

4925.085r

4925.279

4925.418 4925.574m

4925.70 a

4925.89 a

4926.154

4926.401r

4926.694

4926.845

4926.947r

4927.271r 4927.428m

4927.474r 4927 59 m

4Q27 fififir

4927 872m

4928 03 a

4. 5

18

5

101

5. 5

2

20

7. 5

58

3

1. 5

5. 5

1. 5

4. 5

6. 5

OO

5. 5

j 55

3

2

68

4. 5

0. 9

3. 6

1. 0

20. 3

1. 1

0. 4

4. 1

1. 5

11. 8

0. 6

0. 3

1. 1

0. 3

0. 9

1. 3

0. 6

1. 1

f 10, 4

1 1. 0

0. 6

0. 4

IJf. 0

0. 9

s S,N

s

sS

uS,N

S

u

s

s

s

C2

Fe I

Fe I

Ti I Ni I V ITi I

Fe I p

Fe I

Fe I

/R69

IR70

2. 28

4. 10

1. 88

3. 65

1. 22

0. 82

3. 63

3. 57

1,1

1,1

114

1065

157

141

50

39

844

792

13

16

16

1 3

4931. 120r

4931.50 m

4931. 735r

4932.016

4932.068

4932.29 m

4932.98 a

4933.190 4933.338m

4933.671r 4933.873m

4934.030

4934.095

4934.41 a

4934.66 a

4934.872r

4935.00 a

4935.16 a

4935 419r

4935.651r 4935.834m

4936.15 a 4936.341m

4936.699

5

1

4. 5

1 45

1. 5

4. 5

39

97

5. 5

41

j 207

1. 5

2

4

2. 5

1. 5

2. 5

3

65

1. 5

43

3

1. 0

0. 2

0. 9

{

"

l 7. 5

0. 3

0. 9

7. 9

19. 7

1. 1

8. 3

[ 21. 5

1 27. 8

0. 3

0. 4

0. 8

0. 5

0. 3

0. 5

0. 6

13. 2

0. 3

8. 9

0. 6

u

s

s

s

w

u

s?

s?

w?

u

s

Cr I

V I C I

Fe I p Fe I

Fe I Fe I Ba II

Cr I

Fe I p

Ni I

Cr I

C2

5. 54

1. 22

7. 68

4. 19

4. 23

3. 94

4. 15

0. 00

3. 85

3. 64

3. 94

3. 11 /R72

1r 73

50

13

1070

1065

968

1068

1

259

886

177

166

0,0 0 0 }19

) 4928 124 3. 5 0. 7 4937 Ofil 18 3. 6 Q 4928 341

m

30 6. 1 Ti T 2. 15 r±t/0 1 . J. U Hi s 13 4928 47 a 2 0. 4 ^kjO* .OriOiii 86 17. 4 Ni I 3. 61 114 4928 89 m 1 0. 2 Q Ti I 0. 84 0 0 2 0. 4 4929 44 a 11 51 0. 3 ^tJO 1 . \J\J iii 2. 5 0. 5

4929.80 a |2.5| 0. 5 4937.733m 10 2. 0 s Ti I 0. 81 39

4930.065r 5. 5 1. 0 Fe I p 3. 30 631 4937.88 m 4 0. 8 s

4930.21 m s Cr I 3. 84 259 13 4937.973 3. 5 0. 7 4930.310m 82 16. 6 u Fe I 3. 96 985 4937.99 m s Ti I 2. 00 173 13

202
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

WlCltll AX/X

(F)

bpot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. rSand

IN otes Wavelength

(A)

Equivalent w iGtn AX

(mA)

Re- duced

Widtn

AX/X

(F)

Spot

Solar

inenLification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

4938.177m

I no

1 92 J 16. 0 u Fe I 3. 94 966 4945.289 3 0. 6 Feip 3. 02 460

4938.293 I 2. 6 S Ti I 2. 58 289 4945.447m 44 8. 9 w Ni I 3. 80 145

4938.46 a 2 0. 4 4945.642m 42 8. 5 u Fe I 4. 21 1113

4938.62 a 1 0. 2 Si I? 4945.82 a 2. 5 0. 5 4938.820m 119 23. 6 s Fe I 2. 87 318 4946.034 24 4. 8 u Ni I 3. 80 148

4939.05 a 4 0. 8 4946.168r 3 0. 6

4939.242m

4939.479r

4939. 694S

4939.823r

4939.972

4940.069

88

2

96

3

8. 5

14

17. 8

0. 4

19. 6

0. 6

1. 7

2. 8

u

s

M?

M?

Fe I

Fe I p Fei

/4. 22

14. 15

4. 19

0. 86

1065 1070

1043

16

4946.395m

4947.04 a

4947.19 a

vd'ii .06 m

4y4/ DUU

113

1

1. 5

0

L

22. 4

0. 2

0. 3

0. 4

3. 4

u

Si

u

Fei

r e I r

V II —

Si I

.3. 37

6, iO

5. 08

687

4940.30 m S 13 4947.944r 2 0. 4 4940.492 6 1. 2 4947.98 m s Ti I 0. 82 39 13

4940.710r 3. 5 0. 7 4948.191 7. 5 1. 5 s Ti I 2. 17 200

4940.958r 0. 5 0. 1 4948.345 7. 5 1. 5 w1

4941.02 m s Til 1. 98 173 13 4948.597r 3 0. 6 Sm II 0. 54 49

4941.219 3. 5 0. 7 4948.78 m 1 0. 2 s Zr I 0. 52 28

4941. 322r 2 0. 4 S Til 0. 83 39 4948.87 m 1 0. 2 s

4941.38 m s 13 4949.10 a 5 1. 0 4941.569 3 0. 6 S Til 2. 16 200 4949.34 a 2 0. 4 4941.833 3. 5 0. 7 C2? R 73 0,0 19 4949. 576r 3 0. 6 Cr I 3. 85 259

4941.907 6 1. 0 Nil 3. 61 114 4949.78 a 2 0. 4

4942.25 a 4 0. 8 4950.111m 76 16. 0 u Fe I 3. 42 687

4942.484m

4942.598

4942.78 a

4942.94 a

I 1 fin

2

2

1 17. 2

1 3. 0

0. 4

0. 4

s

It?

Cri

Fe I p

0. 94

4. 26

9

1097

4950.378r

4950.624r

4951.411

8

6

4. 5

1. 6

1. 2

0. 9

C2

Cj

/R63

(T> AO

J tx Da IR70

1,1

1 1 i,i

u,u

0,0

}19

}19

4943.06 m 1 0. 2 s Til 0. 90 52 4951.52 a 2. 5 0. 5 4943 305r 1. 5 0. 3 4951.75 a 1 0. 2

4943.448r

4943.82 a

4943.912r

4944.10 a

1. 5

1. 5

2

1

0. 3

0. 3

0. 4

0. 2

Ce II? 1. 21 4952.284m

4y5^.4oor

4952.647m

28

C

54

5. 6

1. 0

10. 5

u

sw

Ni I-

|r e I

Fe I

3. 61

(A in

U 21

113

lUDo

1111

4944.287 10 2. 0 s,d Fei 17 4952.839r 3 0. 6 Cr II 6. 28

4944 564 5 1. 0 s Cn 3. 85 259 4953.021r 2 0. 4

4944.82 m s 13 4953.212m 53 10. 7 u Ni I 3. 74 111

761-925—66 16 203
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4953.36 m

1 ^

f 0. 5 s Ti I p 0. 85 39 4963. 550r 2 0. 4 C2

4953.436r J 1 0. 2 4963.75 a 1. 5 0. 3

4953.49 m

[ 2. 5

J

f 0. 2 s 4964.131 14 2. 8 w

4953.57 m 1 0. 3 s 4964.726m 7 1. 4 S Ti I 1. 97 173

4953.728 5 1. 0 s Cr I 3. 12 166 4964.933m 35 7. 3 s Cr I 0. 94 9

4954.016 4 0. 8 Fe II? 5. 57 168 4965.173 27 5. 4 w Ni I 3. 80 147

4954.296r 4 0. 8 Fe I p 4. 18 1093 4965.30 a 2 0. 4 4954.605m 37 7. 5 u Fe I 4965.405r 5. 5 1. 1 Vii 3. 80 209

4954.809m 54 10. S s Cr I 3. 12 166 4965.58 a 2 0. 4

4955.974

4956.09 a

6

2

1. 2

0. 4

C2? R 70 0,0 19 4965. 811r

4965.857 {

"

[ 4. 6 s,N Mn I 2. 89 20

4956.746r 2. 5 0. 5 MgH R 38 0,0 20 4966.095m 114 23. 0 s Fe I 3. 33 687

4957.307m

4957.475r 4957.613m

\

• 696

t 66. 7

6. 6

128

s Fe I (Dy 11)

Fe I

2. 85

2. 81

318

318

4966.281

4966.576

4966.803r

16

3

2. 5

3. 2

0. 6

0. 5

s,N

Fe I p

Co I Cn

3. 96

0. 43

3. 85

986

14

259

4957.697 1 \ 8. 7 Fe I p

4. 19 1066 4967.273r 2 0. 4

4958.032r 5 1. 0 4967.32 m s Ti I 0. 00 5 13

4958.257

4959.12 m

4959. 145r

4959.202

4959.36 a

4959.70 a

14

7

14

1. 5

1

2. 8

1. 4

2. 8

0. 3

0. 2

s

s

0?

Til

Nd II

Co I

0. 90

0. 06

0. 63

52

1

14

13

17

4967.395r

4967.523

4967.683r 4967.80?m

4967.903m

2

12

1. 5

2. 5

74

0. 4

2. 4

0. 3

0. 5

14. 9

0?

S

u

C2

Ni I

Fe I (Sr I)

/R59

\R 60

3. 80

4. 19

1. 85

1,1

1,1

141

1067

4

}-

4960.351r 4 0. 8 4968.391 21 4. 2 s

4960.856

4961.054

4961.389r

4961.48 a

4961.70 a

4961.920

7

17

5

1. 5

2. 5

26

1. 4

3. 4

1. 0

0. 3

0. 5

5. 2

wl

u

C2

Fe I

Fe I

/R 67 IR 68

3. 63

0,01 0,0/

845

19

17

4968.593

4968.705

4968.852r

4968.93 a 4969.922m

'±1) / u. i lor

29

46

2

1

69

iU

5. 8

9. 2

0. 4

0. 2

13. 9

z. u

su

u

Ti IFe I

Fe I

i~i

1. 98

3. 64

4. 22 /R65

IR66

173

887

1066

0,0 0,0

119

4962. 123r 1 0. 2 4970.206r 6. 5 1. 3 C2 R64 0,0 19 4962.267 2 0. 4 s Sri 1. 85 4 4970.501m 51 10. 3 s Fe I 3. 63 883 4962.292r 5. 5 1. 1 Zr II 0. 97 66 4970.651m 31 6. 2 s,d — Fe I p 3. 96 985

4962.576m 52 10. 5 s? Fe I 4. 18 1097 4971.06 a 1. 5 0. 3 4962.730r 2. 5 0. 5 4971.351m 55 11. 1 s 4962.912r 2. 5 0. 5 c, 4971.50 a 3. 5 0. 7 4963.070r 3 0. 6 C2 4971.62 m s 13,16

204
The Solar Spectrum—Continued

Wavelength

(I)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(V)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(I)

Equivalent Width

AX

Cm X")

Re- duced

Width

AX/X

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

4971.920r 2. 5 0. 5 Co I 3. 17 158 4978.937r 4. 5 0. 9

4972.03 a 1 0. 2 4979.057r 3. 5 0. 7

4972.181r 2 0. 4 4979.206 7 1. 4 MgH? R35 0,0 20

4972.396r 0. 5 0. 1 Fe I 4. 18 1096 4979.310r 5 1. 0

4972.656r

4972.916

4973.06 m

4973.104m

4973.352

4973.51 a

4973.652r

4974.05 a

4974.247

4974.363

4974.460

3

4. 5

88

10

1

1

2

8

8. 5

7. 5

0. 6

0. 9

n. 3

2. 0

0. 2

0. 2

0. 4

1. 6

1. 7

1. 5

,Su

C2?

Fe I p

Ti I Fe I

Fe I Ni I

C2

/R51

iR52

3. 30

2. 00

3. 96

3. 80 /R64

IR65

2,2

2,2

631

173

984

144

0,0

0,0

}-

13

4979.40 a

4979.590

4979.705

4979.835

4979.967 4980.177m

4980.296

4980.539

4981.10 a

4981.279r

4981.358 4981.740m

2

19

5. 5

4. 5

6

1 112

10

1. 5

5

8. 5

112

0. 4

3. 8

1. 1

0. 9

1. 2

1 20. 1

1 2. 8

2. 0

0. 3

1. 0

1. 7

22. 9

s

uu,N

S

Fe I

Fe I p Co I Ni I Fe I

Ti II p

Ti I

3. 64

3. 02

4. 06

3. 61

4. 18

1. 57

0. 85

883

465

112

1092

71

38

4974.552 4 0. 8 C2? R 66 0,0 19 4982.136 14 2. 8 u Y II 1. 03 20

4975.351

4975.412 1 35

1 3. 6

1 3. 6

sw1Ti I Fe I2. 50

3. 30

283

586

4982.507m

4982.825m

138

83

27. 7

16. 2

u

s

Fe I Na I

4. 10

2. 10

1067

9

4975.554r

4975.85 a

4976.00 a 4976.138m

4976.333m

4976.496r

4976.693

4976.881r

4. 5

1. 5

2. 5

27

36

2

6

2. 5

0. 9

0. 3

0. 5

5. 4

7. 2

0. 4

1. 2

0. 5

w

s

C2

Ni I Ni I

Ni I p

C2

/R57

IR58

.3. 61

1. 68

4. 23

fP 92 IP 93

1,1

1,1

112

49

254

0,0 0,0

}- 4983. 03 Ir

4983.260S

4983.470r

4983. 603r 4983.859m

4984.122m

4984.302r

4984.458r

4984.625

7

114

14

10

123

91

5. 5

5. 5

18

1. 4

22. 9

2. 8

2. 0

24. 7

18. 2

1. 1

1. 1

3. 6

u

uu

u

Fe I

C2

Fe I Ni I

4. 15 R64

4. 10

3. 80

1067

0,0

1066

143

19

4977.24 a 1. 5 0. 3 4984.76 a 3 0. 6

4977.655

4977.719

f 5. 2

1 1.8

w

S

Fe I

Ti I

3. 93

2. 02

985

173

4984.83 a

4984.96 a

2

3

0. 4

0. 6

4977.929r 1. 5 0. 3 4985.259m 101 20. 1 u Fe I 3. 93 984

4978.112

4978.194 J

j 1.8

[ 5. 0

w7

S

Fe I

Ti I

3. 96

1. 97

986

173

4985.554m

4985.758

103

11

21. 6

2. 2

s Fei 2. 86 318

4978.369r 5 1. 0 4985.986 25 5. 0 u Fe I p 4. 26 1094

4978.555 ( 9. 0 s Na I 2. 10 9 4986.228m 45 9. 0 w Fe I 4. 22 1070

4978.606 < 17. 5 u Fe I 3. 98 966 4986.45 a 2. 5 0. 5 Co I? 2. 72

4978.691 [ 1. 2 Fe I p 4. 07 1035 4986.908 18 3. 6 w Fe I 4. 26 1092

20,15
The S olar Spectrum—Continued

Wavelength

(I)

Equivalent Width

AX

Re- duced

Width

AX/X

Kr J

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

4987. 085r 1. 5 0. 3

4987. 277r 2 0. 4 /R 54

IR 55

1,1

1,1

4987.435r 3 0. 6

4987. 652r 2. 5 0. 5 Fe I p 4. 18 1094

4987.852 4. 5 0. 9 Co I Fe i?p

0. 58

3. 88

14 966

4988.01 a 2. 5 0. 5 Co I 4. 06

4988. 138r 6 1. 2 C2 /R61

IR 62

0,0

0,0 4988.24 a 3. 5 0. 7

4988.360r 3 0. 6

4988.64 a 1. 5 0. 3 4988.955m 80 16. 0 s Fe I 4. 15 1066 4989.141m 29 5. 8 s Ti I 1. 98 173

4989.41 a 2 0. 4

4989.553 3. 5 0. 7

4989.954 6. 5 1. 3 Nd II? 4990.453m 26 5. 2 u Fe I 4991.072m 102 21. 2 s Ti I 0. 84 38 4991.275m 87 17. 4 u Fe I 4. 19 1065

4991.861 16 3. 2 .$ — Fe I 4. 22 1094

4992.076r 0. 5 0. 1

4992.287 6 1. 2 C2 R 62 0,0 19

4992. 480r 4. 5 0. 9 Fe I?

4992.778 8 1. 6 u Fe I 4. 26 1110

4992.996r 1 0. 2 Co I? 4. 07

4993.352 34 6. 8 wl Fe II 2. 81 36 17

4993.522r 1 0. 2 S I?

4993.683

4993.747

1

} "

f 8. 4

1

1 2. 2

u Fe I 4. 21 1111

16

4993. 937r 2. 5 0. 5

4994. 138S 95 19. 6 Fe I 0. 91 16

4994.60 a 2. 5 0. 5

4994.99 m 13

4995. U^s 6. 0 U. 7

4995.08 m 3 0. 6 S Ti I 2. 25 216

4995.267 1. 5 0. 3

4995.409 13 2. 6 W Fe I 4. 26 !lll3

length

(A)

Equi- Vfliclit Width

AX

(mA)

ReMil r*Ari Width

AX/X

(F)

Spot

Solar

IdentifipQf ion

Low

or Rot. Line

RMT

XN 0. or Vih

Band

Notes

4QQ5 ^16 m s? 13 4QQ5 6*19 16 3. 2 Ni I 3. 63 145 4995 877 1. 5 0. 3 Ti II p 1. 58 71 49Q6 00 a 1 0. 2 AQOR IQ5 7 1. 4 Fe I?

4Q96 378 12 2. 4 If?

4QQ6 'lO a 2 0. 4

1 0. 2

49 9. 8 Ni I 3. 63 144

49Q6 979 3. 5 0. 7

4QQ7 inOm 27 5. 6 ;S Ti I 0. 00 5

4QQ7 353 0. 5 0. 1

4QQ7 'ifi fl 1 0. 2

4.QQ7 74 -m 2. 5 0. 5 4QQ7 qc;q 9. 5 1. 9 4998.230m 56 11. 0 Zf Ni I 3. 61 111

4998.44 a 2 0. 4

4998.567 3. 5 0. 7 Cr I? 3. 01 123

4998.959 2. 5 0. 5 C2 /R51

iR 52

1,1

1 1 }19

4000 1 1 Q 29 5. 8 w Fe I 4. 19 1040

499Q 264 6 1. 2 4QQQ f^lOm 104 s Ti I 0. 83 38

3. 5 0. 7

2. 5 0. 5

2 0. 4

24 4 8 ^000 '^4Qm 70 14. 0 NI I 3. 63 145

p^OOO f>4fi 2. 5 0. 5 MeH R 32 0,0 20

^000 7*^^ 12 2. 4 Fe II p 2. 78 25

r:nOO QQOm 44 8. 8 Ti I 2. 00 173

'^OOI 91 0 7. 5 1. 5 R 32 0,0 20

^001 479 2n 4 fl Ca II 7. 50 15

' p^OOl 5^70m 168 S^. u Fe I 3. 88 965

5002.328 6. 5 1. 3 s V I 2. 36 132

5002.592 18 3. 6 s 17

5002. 798S 85 16. 4 s Fe I 3. 40 687

5003.098 10 2. 0

206
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/\

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

\ib.

Band

.Votes

5003.25 a

to 5003.60 a

5003.747 34

1. 6

6. 8 s Ni I 1. 68 50

5011.204

5011.37 a

to 5011.70 a

2

J

0. 4

1. 0

Fe I 4. 22 106G

5003.879 1 0. 2 Fe I p 2. 01 211 5011.761 3.0. 7 Ce II? 1. 05 5004.049m

6004.212

50

8

10. 0

1. 6

s

6

Fe ICo I?

4. 21

2. 87

1112

141

5012.075

5012.156

1 154

1

1 24. 0

[ 11. 5

s

w?

Fe I Fe I p0. 86

4. 19

16

1070

5004.365 17 3. 4 s,d Cr I 3. 01 122 5012.307 8 1. 6

5004.50 a

to 5004.75 a 1

1. 0 5012.448m

5012.594

58

4

11. 6

0. 8

u Ni I 3. 70 111

5004.894 14 2. 8 s Mn I 2. 92 20 5012.700 40 8. 0 u Fe I 4. 28 1093

5005.171

5005.401

26

14

5. 2

2. 8

s,d? Ti II p

C2

1. 57 R5971

0,0 19

5012.87 a

to 5013.13 a } « 1. 2

5005.509 6005.719m

5006.120m

5006.379

5006.533

5006.694

5006.897

5007.217

5007.280

5007.734

5007.922

5008.044

5008.225

5008.453

5008.646

5009.196

6009.427

5009.534

5009.655

5009.832

5010.024

5010.218

5010.327

6

136

190

11

13

9. 5

6

1 174

33

2

4

3

1

14

3

12

1

24

5

35

25

9. 5

1. 2

27. 2

38. 0

2. 2

2. 6

1. 9

1. 2

r 24.

I 19. 2

6. 6

0.4

0. 8

0. 6

0. 2

2. 8

0. 6

2. 4

0. 2

4.6

1. 0

7. 0

5. 0

1. 9

s?

s

s

u

s

w

w

s

uw

0

C2? Fe I Fe I

Fe I p

Ti I

Fe I

Fe I?

MgH

Fe I?

Ca?

Ti I

Ni I

Ti II Fe I p

R59

3. 88

2. 83

2. 59

0. 82

/3. 94

14. 10

4. 29

R31

R58

R58

0. 02

3. 77

3. 09

2. 56

0,0 984

318

211

38

966

1065

0,0

0,0

0,0

5

111

113

211

19

20

19

19

5013.305m

5013.472

5013.690

5013.779

5013.920

5014.197

5014.285

5014.47 a

5014.60 a

5014.74 a

5014.951S

5015.126

5015.303

5015.41 a

5015.66 a

to 5015.93 a

5016.039

5016.168m

5016.326

5016.480

5016.686 5016.886m

59

6

1 55

22

1 148

3. 5

7

4

125

2. 5

16

4

}

^

6

60

2. 5

33

2. 5

45

11. 8

1. 2

1 8. 5

I 3. 0

4. 4

J 13. 5

1 19. 2

0. 7

1. 4

0. 8

24. 9

0. 5

3. 2

0. 8

1. 0

1. 2

12. 1

0. 5

6. 6

0. 5

9. 0

s

w

w

s

s

u

s

u

s

TiiCr I

Ti II

C2Fe I Til

Ti I

Vi

Fe I

Fe I MgH

C2-

Ti I

Fe I

Fe I

2. 02

2. 71

1. 58 R 57

0. 00

0. 81

r2. 37

\2. 68

3. 94

3. 98 R30

fP 83 \P 84

0. 85

4. 26

17360

71

0,0

5

38

132

965

968

0,0

0,0

0,0

38

1089

19

20

}l9

5010.943m 46 9.2 u Ni I 3. 63 144

207
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

duced

Width

AX/X

(F)

Spot

Solar

Identification EPor Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification EP

or Rot. Line

RMT XLiVi X No.

or Vib. BandNotes

5017.047 7. 5 1. 5 C2 JR 46 IR47

1,1

1,1 }- 5024.218 15 3. 0 w

5017.193

5017.381 5017.584m

5017.814

5018.036

6

5

90

18

17

1. 2

1. 0

17. 9

3. 6

3. 4

w

C2

Ni I

C2Fe I p

R 45

3. 54 R 56

3. 63

1,1

111

0,0 884

19

19

5024.595 5024.850m

5025.082

5025.305 5025.566m

3

62

20

18

52

0. 6

13. 0

4. 0

3. 6

10. 3

S

u

uS

Ti I Fe I p Fe I

Ti I (Cri)

0. 82

4. 26

4. 28

2. 04

0. 98

38

1110

17320 5018.286m

5018.450m

5018.878

5019.176

5019.22 m

5019.478

5019.732 5020.031m

58

210

3

10

4

7. 5

24

86

11. 6

41. 8

0. 6

2. 0

0. 8

1. 5

4. 8

16. 5

uw

s u,N

u,N

S

Ni I Fe II

Fe I Cr I Fe II? —

Fe I Ti I (Ca 11)

3. 83

2. 89

4. 58

0. 97

5. 57

3. 98

0. 84

7. 51

162

42

1242

20

168

966

38

15

5025.764

5025.908

5026.189

5026.488

5026.740

5026.877

5027.130

5027.230

11

5

1. 5

3

2. 5

5

105

46

2. 2

1. 0

0. 3

0. 6

0. 5

1. 0

20. 9

9. 2

u

u

Fe I C2

C2?

Ni I

Fe I Fe I

3. 07 R54

R54

3. 70

4. 15

3. 64

466

0,0

0,0

158

1065

883

19

19

5020.347 2 0. 4 s 16 5027.354 32 6. 4 w1 Fe I p 3. 98 968

5020.496 8. 5 1. 7 5027.525 12 1. 8 Fe I p 3. 88 960

5020.688 13 2. 6 u Fe I p 3. 25 629 5027.617 7 1. 3

5020.819 17 3. 4 u Fe I 3. 55 748 5027.762m 61 12. 1 w Fe 1 4. 21 1110

5020.997 6 1. 2 5027.924 4. 5 0. 9

5021.151 4 0. 8 Ca 11 7. 51 15 5028. 133S 83 16. 5 s Fe I 3. 57 791

5021.35 a 2 0. 4 5028.351 13 2. 6

5021.602

5021.686

]

> 69

1

9. 5

1 5. 0

su

FeiFe I p

4. 26

4. 22

1093

1067

5028.545

5028.78 a

7

5

1. 4

1. 0

5021.923 22 4. 4 s,d Cri

Fe I C2

0. 94

3. 27 R55

8 629

0,0

17

19

5029.03 a

5029.220

5

1

1. 0

0. 2

MgH R 28 0,0 20

5022.059 4. 5 0. 9 0? C2? R55 0,0 17,19 5029.484 4. 5 0. 9 MgH R28 0,0 20

5022.241m 114 22. 7 w? Fe I 3. 98 965 5029.623m 41 8. 2 u Fei 3. 41 718

5022.629 4 0. 8 5029.815 12 2. 4 u Mn I 2. 94 20 5022.874m 72 11 5 S Ti I 0. 83 38 5029.917 9. 5 1. 9 C2 R 53 0,0 19

5023.043 3 0. 6 s 5030.035 5 1. 0 C2? R 53 0,0 19

5023.189 35 7. 0 u Fe I 4. 28 1095 5030.633 4 0. 8 s,N

5023.348 3. 5 0. 7 s Ti I 2. 16 199 5030.782 20 4. 0 u Fe I 3. 24 585

5023.496 26 5. 2 u Fe I 4. 31 1150 5030.880 1 0. 2 C2 R41 1,1 19

5023.644

5023.832

6

6. 5

1. 2

1. 3 Ci 7. 94

5031.024m 65 12. 9 w ||Sc II- Fei

1. 36

/3. 55

13. 64

23 746

883

.5024.010 4 0. 8 O2 /R44

IR45

1,1

1.1 5031.182

5031.753

11

6. 5

2. 2

1. 3

u Fe I? 3. 64 885

208
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

bpOt

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Wiutn

AX/\

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Bund

Notes

C AO 1 f\1 £1 ouoi.yiD Ol 4. Z V, r e I 4. 0/ oUoy .oDO f, 0 D. Z

"M; T INI I 0. D.5 ^ AO I 4Z

5032.076

5032.379

5. 5

8

1. 1

1. 6

CP 7Q IP 80

A A U,U 0,0 }19

oUoy .oU /

5039.774

4. 0

7

1. 0

1. 4 C2 If(X> 77// IP 78

A A u,u 0,0

1}19

5032.733 23 4. 6 U Nil 3. 90 207 5039.964m 66 14.

•s Ti I 0. 02 5

6033.129 131 0. 6 5040.122 7 1. 4 C I 7. 94

5033.538 4 5 0. 9 5040.249 10 2. 0 s Fe I p 4. 22 1093 16

5033.61 m S 13,16 5040.465 3 0. 6 C2

5033.652 4. 5 0. 9 C2 R 52 0,0 19 5040.614 16 3. 2 Ti I 0. 83 38

Ov66.il 1 4. 0 u. y

A A U,U [r A/1 A IQK 0U4U. / 00 A K

4. 0

A A

u. y

5034.057 2 0. 4 Co I 2. 04 91 5040.890m 116 23. 0 Fe I /4. 28

14. 26

1094

1092 },a

5034.178 5 1. 0 C2 1 K 41 IR 42

1,1

1,1 5041.076m 112 22. 2 s Fe I 0. 96 16

5034.356

5034.520

7

6

1. 4

1. 2

C2 R 40 1,1 19 5041.324 28 5. 6 u,N C2Fe I p

R50

(A 0 Q

J 4. Zo

15. 02

0,0

1328

19

5034.678 4 0. 8 5041.450 37 7. 3 u,N -C I 7. 94

5034.991 |4| 0. 8 Fe I 3. 64 885 5041.619m 86 17. 0 s Ca I 2. 71 34

5035.12 a 5035.370m

3

109

0. 6

21. 1 U Nil 3. 63 143

5041.763

5041.854 1 158

1 27. 7

I 5. 9

s Fe I Fe I?

1. 48 36

5035.733 1131 2. 6 5042.027 3. 5 0. 7

5035.910

5035.974

1> 115

f 16. 8

1 11. 2

s

u1

Ti I Ni I

1. 46

3. 65

110

145

5042.192m

5042.58 m

61

sTs

12. 1

1. 7

u

s

Ni I Mn I?3. 66

2. 95

131

20

5036.277 42 8. 3 w Fei 5042.921 8 1. 6 MgH R26 0,0 20

£0*^ A A71 rY-» OUoD.^/ ini DO 20. i s il I

1 A A 1. 44 1 1 A IIU 5U4o.Uy4 Q0

1 R 1. D

OUoO. / ol

5036.924

4. 0

23

A Ci

4. 6 s,d Fe I Fe II

3. 02

2. 83 465

36

17

5043.295

5043.461

10

3. 5

2. 0

0. 7

C2 J x / 0 \P 77

A n

0,0

1}I9

5037.200 3. 5 0. 7 Atm 5043.588m 14 2. 8 S Ti I 0. 84 38

5037.314

OUo t .iov

ouo/./uy

oUo/.oUo

13

o. 0 on

/

2. 6 A 1 U. /A 4. L)

1. 4

C2

/I^2

O2

Ti II p

T>R OA39 R 51 R 51

1. 58

1,1

0,0

0,0 71

1 A19

1 A19

19

5043.709

5043.833

5043.988

5044.033

3. 5

2. 5

7

1

0. 7

0. 5

1. 4

0. 2

C2

C2

Ce II?

/R 38 \R39

R37

1. 21

1,1

1,1

1,1

16

19

5038.403ni 60 i^. £> s Ti I 1. 43 110 5044.218m 70 13. 9 s Fe I 2. 85 318

5038.596m 50 9. 9 w Ni I 3. 83 166 5044.635 1 0. 2

5038.799

5038.891

5039.060 5039.258m

2

8

16

73

0. 4

1. 6

3. 2

14. 5 wt

Fe I? p

C I Fe I

3. 05

7. 94

3.37

510

4

687

5044.772

5045.082

5045.270

5045.407

1. 5

2. 5

12

10

0. 3

0. 5

2. 4

2. 0

0

s

C2

Fe I? QTii

JP 67 IP 68

R49

0. 85

1,1

1,1

0,0

38

},9

19

209
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5045.636 5 1. 0 5052.627 11 2. 2 u -C2 R 47 0,0 19

5045.77 al

to 5046.07 a J

5 1. 0 5052.738 5052.880m

6

14

1. 2

2. 8

u

s

C2?

Ti I

R47

2. 17

0,0

199

19

5046.202 4 0. 8 5052.990 12 2. 4 u Fe I 3. 27 585

5046.55 m s Zr I? 1. 53 62 13 5053.125 5 1. 0

5046.929m

5047.120

5047.302

4. 5

7

7. 5

0. 9

1. 4

1. 5

5 Fe I p

Vi-

|V II

/R 37 IR 38

4. 58

1. 93

2. 56

1,1

1,1

1242

127

16

5053.295

5053.577

5053.818 5054.083m

3. 5

50

2. 5

7. 5

0. 7

9. 9

0. 5

1. 5

s

s

W I

Ti I

0. 21

2. 68

1

294

5047.404 4 0. 8 5054.647m 35 6. 9 s Fe I 3. 64 884

5047.558

5047.719

5047.942

5048.062

5048.225 5048.439m

5048.64 m

5048.76 m

2

5

22

30

26

70

3

9. 5

0. 4

1. 0

4. 4

5. 9

5. 2

13. 9

0. 6

1. 9

W

u

su

s?s

C2

C2

Nil

Til

Fe I Til?

Cr I

/P 66 IP 67 P 65

3. 83

2. 15

3. 96

0. 98

1,1 1,1

1,1

161

199

984

20

}"

19

5055.426a

5055.583

5055.794

5055.988

5056.126

5056.252

5056.434 5056.846m

1. 5

6

6. 5

24

12

11

12

|24|

0. 3

1. 2

1. 3

4. 7

2. 4

2. 2

2. 4

4. 7

s,d

s

wl

MgH

MgH

Fe I

C2

C2 -MgH

Fe I MgH

Q38

Q 38

4. 31 R46

R46

R24

4. 26 R24

0,0

0,0

1149

0,0

0,0

0,0 nil

0,0

20

17

20

17

19

19

20

1720

5048.853m

5049.016

5049.204

5049.425

5049.592

5049.682 5049.827m

5050.138

52

3. 5

3

5

8

4

135

6. 5

10. 3

0. 7

0. 6

1. 0

1. 6

0. 8

27. 3

1. 3

u

u

Ni I

C2MgH

C2Fe I Fe I p MgH

3. 85

R 25 R 26

2. 28

3. 88 R 25

195

0,0

2,2

114

963

0,0

20

19

20

5057.487

5057.594

5057.696

5057.839 5057.985m

5058.242

5058.28 m

5058.495

17

10

1

7. 5

29

7

1

10

3. 4

2. 0

0. 2

1. 5

5. 7

1. 4

0. 2

2. 0

w

w

s,d

Fe I

Fe I p Fe I

Ti I? Fe I

/4. 19 U 41

4. 55

3. 94

3. 64

1067 1150

1185

967

884

17

16

5050.291

5050.443

5050.571

5050.737

5050.965

5051.305 5051.504m

2. 5

5

2

6

10

3. 5

47

0. 5

1. 0

0. 4

1. 2

2. 0

0. 7

9. 3 u

C2

Fe I p

Ni I

4. 22

3. 65

1089

144

5058.812

5058.930

5059.229

5059.393

5059.788

5059.929

5. 5

5

3. 5

1. 5

12

5. 5

1. 1

1. 0

0. 7

0. 3

2. 4

1. 1

0

C2

C2

C2

C2 -C2

C2

/R 33 IR34

P 73

R45

R48

1,1

1,1

0,0

0,0

0,0

}«

19

19

19

5G51.642m 111 22. 0 s Fe I 0. 91 16 5060.074m 60 11. S s Fe I JO. 00

14. 30

1 1095

5051.905 20 4.S s Cr I 0. 94 8 5060.313 3 0. 6

5052.151 40 7. 9 0 C I 7. 68 12 5060.436 2. 5 0. 5

5052.388 6 1.2 5061.108 3 0. 6

210
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Refhiccd Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5061.396 2 0. 4 C2 5069.088 15 3. 0 s,d Ti II 3. 12 113 17

5061.525 3. 5 0. 7 MgH Q37 0,0 20 5069.36 ni s Ti I 2. 15 109 13

5061.697 8. 5 1. 7 -C2 P 72 0,0 19 5069.415 6 1. 2

5061.892 3 0. 6 MgH Q37 0,0 20 5069.46 m 9. 5 1. 9 s 5062.104m

5062.384

15

475

3. 0

0. 9

s Ti I

C2

2. 16

fP 61 \P 62

199

1,1

1,1 }n

5069.625

5069.795

2

2

0. 4

0. 4

MgH

Fe I p

C2

R22

2. 59 R31

0,0 211

1,1

20

19

5062.910 3 0. 6 5069.991 9 1. 8 C2- R31 1,1 19

5063.07 a

5063.174

5063.306

5063.522

5063.753

5063.884 5064.066m

5064.336

5064.386 5064.658m

5064.815

5064.974

3

11

5. 5

2. 5

1

1

6. 5

79

3

1 118

0. 6

2. 2

1. 1

0. 5

0. 2

0. 2

1. 3

1

0. 8

1 1.2

16. 4

0. 6

f 7. 9

su

S

u

MgH

C2-

C2MgH

Ti I

Sc I —

Ti I

Fe I p

(Zri)

R23

R44

R44

R23

2. 69

1. 44

0. 05

4. 26

1. 48

0,0

0,0

0,0

0,0

294

13

5

1095

62

20

19

19

20

5070.140

5070.23 m

5070.295

5070.438

5070.922

5071.133

5071.260 5071.491m

5071.774

5071.909 5072.080m

5072.298

9

3

2

2. 5

2

1. 5

25

7. 5

3

80

31

1. 8

0. 6

0. 4

0. 5

0. 4

0. 3

4. 9

1. 5

0. 6

15. 8

6. 1

s

s

ww

C2MgH

Sc I

C2?

Ti I

c,

Fe I

Ti 11

R42

R22

L 43 R42

1. 46 P 69

4. 28

3. 12

0,0

0,0

13

0,0

110

0,0

1089

113

1920

13,16

19

19

5065.030 [ 19.

8

u Fe I 4. 26 1094 5072.473 5 1. 0 5065.194m 68 13. 4 s Fe I 3. 64 883 5072.677m 60 11. 8 w1 Fe I 4. 22 1095

5065.375 4. 5 0. 9 5072.922m 31 6. 6 s Cr I 0. 94 8

5065.714 2 0. 4 5073.170 4. 5 0. 9

5065.904 12 2. 4 s Cr I 2. 71 60 5073.453 9. 5 1. 9 0? C2- R 41 0,0 17,19

5065.989 19 3. 8 S Ti I 1. 44 110 5073.592 4. 5 0. 9 C2 R 41 0,0 19

5066.268 4 0. 8 Fe I p 3. 63 882 5073.748 5. 5 1. 1 MgH Q35 0,0 20

5066.368 6 1. 2 5074.072 1. 5 0. 3

5066.727 10 2. 0 c. R43 0,0 19 5074.342 1. 5 0.3

5066.859 7. 5 1. 5 R43 0,0 19 5074.753m 115 £2. 7 u Fe I 4. 22 1094 5067.155m 73 14. 4 w Fe I 4. 22 1092 5074.976 10 2. 0 R 29 1,1 19

5067.504 6 1. 2 MgH

c,Cr I Ni I Cr I Ti I

Q36 0,0 20 5075.164 7 1. 4 Fe I p 4. 18 1089

5067.746

5067.829

5068.302

24

12

10

4. 7

2. 4

2. 0

s

0?

S,d

2. 71

3. 80

1. 00

2. 66

60

141

20 294

5075.300

5075.541

5075.818

5076.093

28

5V5

4. 5

5. 5

1. 0

0. 9

0. 9

s

s?

C2-

Sci

MgH

P 68

1. 43 R 21

0,0

13

0,0

17,19

20

6068.454 5068.771m2. 5

129

0. 5

25. 4 s Fe I 2. 94 383

5076.275m

5076.326 J 78

r 13.

1 3. 6

u Fe I Ni I4. 30

3. 65

1089

143

211
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. rSanaNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5076.478

5076.617

6. 5

15

1. 3

3. 0 s,d MgH

R 40 R 21

0,0

0,0 17,19 20

5083.032

5083.186

14

7

2. 8

1. 4

C2-

p^2

C2

R38

it 00 R38

0,0

0,0

19

1lyQ

19

5076.766 6. 5 1. 3 C2 R40 0,0 19 5083.345m 95 19. 8 s Fe I 0. 96 16

5076.879 4 0. 8 5083.535 2. 5 0. 5

5077.380

5077.55 m

5077.603

5077.834

5078.074

5078.180

5078.28 m

8. 5

2

1

4

1

1. 7

0. 4

0. 2

0. 8

0. 2

s

u

s

CaCo I?

C2?

C2

Zr I

R 28

3. 95

R 28

/P 55

1. 44

1,1 184

1,1

1,1\ 111

62

19

13

19

16,19

13

5083.703

5083.858 5084.105m

5084.414

OUot:.OOZ

5084.696

5084.838

7. 5

12

93

2

0. 0

7

5

1. 5

2. 4

18. 3

0. 4

1 . 0

1.4

1. 0

s

w

Sc I

Nil

e 1 —

C2?

C2C2?-

MgH

1. 44

3. 68

0. oy R25

P 65 R25

Q33

13

162

1,1

0,0

1,1 0,0

19

19

1920

5078.352 5. 5 1. 1 P 67 0,0 19 5085.010 2. 5 0. 5 C2

5078.455

5078.539

5078.711 5078.981m

O. 0

/. 0 no9o

n 7

1 A

I. 4

1. 0

is. O s

J: 6 ll p

\JL I — r e I

0. 00

i. 0\J

5085.167

5085.340

5085.489

3. 5

5. 5

18

0.

7

1.

1

3. 5

s

s

C2

Ti I Ni IIQn |oC TI

TP J i 00 IP 36

1. 43

3. 66

1 J.Q i. ^0

9 9

2,2

109

130

}19

5079.230m lUO in 7 s r e I OD ouoO-o / y D I. 1 u Fe I p iuyo

5079.544 6 1. 2 MgH Q34 0,0 20 5085.911 2. 5 0. 5 Fe I p 3. 94 963

5079.745S 87 15. 7 S Fe I 0. 99 16 5086.248 12 2. 6 w C2 R37 0,0 16,19

5079.965m 47 9. 2 s Ni I 1. 83 60 5086.398 6. 5 1. 3 u C2 R37 0,0 16,19

5080.111

5080.347 5080.539m

5080.789

5080.938 5081.119m

5081.358

5081.581

5081.767

5081.852

5082.053

5082.190 5082.349m

10

25

93

9

12

91

2

8

4

D

1

2. 5

58

2. 0

4. 9

18. 3

1. 8

2. 4

17. 5

0. 4

1. 6

0. 8

1. Z

0. 2

0. 5

11. 6

uw

su

S,N

w

C2

Fe I Ni I

Fe I Nil - Ti I p

Sc I

C2

i*e I p

C2Ni I

/R 39 IR27

3. 65

3. 27

3. 85

1. 43

1. 45 P 66

Q Q Q 0. 00

R26

3. 66

0,0

1,1

143

585

194

109

13

0,0

1,1

130

|l9

19

19

5086.623

5086.772

5086.931 5087.062m

5087.254 5087.426m

5087.847

5088.006

5088.158

5088.543

5088.757

5088.960

5089.212

5

7. 5

3

22

1. 5

40

1

4. 5

32

26

3

25

14

1. 0

1. 5

0. 6

4. 3

0. 3

8.4

0. 2

0. 9

6. 3

5. 1

0. 6

4. 9

2. 8

s s,N

s

w

u s,NN

w,d?

Fe I p Sci

Ti I

C2Yii

Co I?

C2Fei

NiiMgH

Nil

C2-

Ca

4. 15

1. 43

1. 43

1. 08

4. 02 P 64

4. 15

3. 85 R 19

3. 68 R 36 R 36

1067

13

109

20

0,0

1066

190

0,0

162

0,0

0,0

19

20

15,19 19

5082.55 a

5082.654

5082.895

2. 5

111

3

0. 5

0. 2

0.6

MgH

Fe I p

MgH

R20

3. 11 R20

0,0 466

0,0

20

20

5089.367

5089.831

7

1. 5

1. 4

0. 3

CaNd II?

/R 36 IR23

0. 20

0,0

1,1

46

212
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Rorluced Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5090.068 0. 5 0. 1 5097.492m 38 7. 4 u Fe I

5090.221

5090.393

7

|2. 5|

1. 5

0. 5 MgH Q 32 0,0 20

5097.711 5. 5 1. 1 C2 fP 46 P 47 [R 16

1,1 1,1

1,1

1r

5090.782S 85 16. 7 u Fei 4. 26 1090 5097.876 1 0. 2 C2 P 45 1,1 19

5090.976 6 1. 2 C2? P 61 0,0 19 5098.132 10 2. 9 s -C2 R 33 0,0 19

5091.179 2 0. 4 C2 R 22 1,1 19 5098.318 7. 5 1. 5 u

5091.302 6 1. 3 C2 R 22 1,1 19 5098.578m 70 13. 7 u Fe I 3. 93 984

5091.491 2 0. 4 C2 R 22 1,1 19 5098.707m 102 20. 0 s Fe I 2. 18 6G

5091.725

5091.888

5092.114

7. 5

9. 5

2. 5

1. 6

2. 1

0. 5

s,d

Fe I

Cr I

/3. 41

13. 55

1. 00

717 745

20

5098.930

5099.081 5099.329m

9

52

70

1. 8

10. 2

13. 7

s,N

u,N

Fe I Ni I (Sc I)

3. 98

3. 65

1. 44

965

141

13

5092.309 14 2. 9 C2- R 35 0,0 19 5099.575 10 2. 0 C2 R 18 1,1 19

5092.485 |8l 1. 6 0? C2 R 32 0,0 17,19 5099.788 7 1. 4 C2 P GO 0,0 19

5092.803 6. 5 1. 3 s Nd II- 0. 38 48 5099.936m 79 15. 5 w1 Ni I 3. GS 161

5093.284 1. 5 0. 3 C2? R 21 1,1 19 5100.239 4. 5 0. 8

5093.450 2. 5 0. 5 s Cri 1. 03 20 5100.466 1. 5 0. 3

5093.684 5T51. 2 C2? /P 48

\P 49

1,1

1,1 5100.656 17 3. 1 Fe II 2. 81 35

5094.026 5094.418m

|8.5|

25

1. 9

5. 5

M?WC2-

Ni I

P 62

3. 83

0,0 164

17,19 5100.854

5100.945

12

10

2.4

2. 0

Fe II

C2Fe II

5. 91 R32185

0,0 19

5094. G 12

5094.85 a

1

3

0. 2

0. 6 MgH R 18 0,0 20

f -i f\-i /\ 00 5101.083 9 1. 8 C2 —

Sc I

/R32

\R17

1. 45

0,0

1,113 |19

5094.945 10 2. 0 s,d Co I 2. 04 92 17 5101.275 5 1. 0 C2 R 17 1,1 19

5095.03 m 1 0. 2 s 5101.486 475 0. 9 C2 R 17 1,1 19

5095.176 |5.5| 1. 1 R 34 0,0 15,19 5101.60 a 3. 5 0. 7 C2 P 43 1,1 19

5095.341 7. 5 1. 7 MgH R 18 0,0 20 5101.823r 3 0. 7

5095.503 1 0. 2 C2 R 18 1,1 19 5102.013r 0. 5 0. 1 C2

5095.665 2. 5 0. 5 C2 R 17 1,1 19 5102.243 3 0. 6 Fe I p 2. 22 65

5095.892

5096.046

5096.183

5096.487

5096.586

4. 5

1. 5

3

1

1

0. 9

0. 3

0. 6

0. 2

0. 2 s?

C2

C2MgH

JP 47 IP 48

Q 31

1,1 1,1

0,0

>

20

5102.431

5102.673 5102.973m

5103.125

5103.391

12

3

42

3. 5

6

2. 2

0. 6

8.4

0. 7

1. 2

u

C2?

Nil

Sm II?

C2

P 59

\. 68 L 17

fP 43 \P 44

0,0

49

1,1

1,1

19

5096.740 5. 5 1. 1 s So I 1. 43 13 5103.551 1. 5 0. 3 C2 P 42 1,1 19

5096.865

5097.005

5097.321

35

90

12

6. 9

17. 9

2. 4

u

u

u

Ni I Fe I Cr II3. 74

4. 28

3. 71

111

1092

24

5103.743

5103.912

11

4

2. 2

0. 8

C2-

C2

C2

R 31 R 31 R 31

0,0

0,0

0,0

19

19

19

213
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Rediiced Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

5104.033

5104.195

5104.440

5104.645

5104.896

25

25

29

3. 5

2. 5

4. 9

4. 9

6. 7

0. 7

0. 5

sw

w

Fe I Fe I Fe I

C2?

3. 02

4. 18

4. 28 R 15

465

1092

1090

1,1 19

5111.253

5111.367

5111.634

4

7

9

0. 8

1. S

1. 8

MgH

Co

CoMgH

C2

0 28 R 11

fP 37 P 38 iP 39 Q 28 R28

0,0

1,1

1,1

1.1 lil

0,0

0,0

20

19

1r

20

19

5105.091 2 0. 4 C2 R 15 1,1 19 5111.740 6. 5 1. 3 C2? R28 0,0 19

5105.182 2. 5 0. 5 C2 P 41 1,1 19 5111.871 8 1. 6 C2 R25 0,0 19

5105.364 7. 5 1. 5 C2 P 58 0,0 19 5112.279 8 1. 6 u Zr II 1. 66 95 5105.545m 82 16. 0 u Cui 1. 39 2 5112.490 3. 5 0. 8 s Cr I 1. 00 19

5105.752 3 0. 6 5112.648 3 0. 6 MgH R 15 0,0 20

5105.957 1 0. 2 5112.779 1 0. 2 C2 RIO 1,1 19

5106.009

5106.238

5106.379

0. 5

2. 5

4. 5

0. 1

0. 5

0. 8

Vii

C2

2. 56 R 30

127

0,0 19

5112.983

5113.127

4

23

0. 8

4. 5 s,d

C2

|Cr I MgH

fP 37 IP 38

2. 71 R 15

1,11 1,1/

60

0,0

19

17

20'

5106.451

5106.601

5106.877 5107.457m

5107.651m

5107.884

5107.977

5108.187

5108.394

5108.629

5108.85 m

5108.912

10

9. 5

4. 5

91

97

11

3

4

18

3. 5

1. 5

4. 5

2. 0

1. 9

0. 9

17. 8

19. 0

1. 8

0. 6

0. 8

3. 5

0. 7

0. 3

0. 9

s

s

u,N

s

Fe I? C2MgH

MgH

Fe I Fe I C2-

C2

C2

C2

Co I?-

Cr I

R30

Q29

R 16

0. 99

1. 56 P 57 R 13 P 55 R 13

3. 93

2. 71

0,0

0,0

0,0

16

36

0,0

1,1

0,0

1,1

18160

19

20

20

19

19

19

19

16

5113.246 5113.447m

5113.753

5114.028

5114.263

5114.505

5115.001

5115.199 5115.398m

5115.672

5115.790

5115.878

5116.049

8. 5

23

1

1. 5

16

16

2

4

72

6

23

5

3. 5

1. 7

4. 5

0. 2

0. 3

5. 1

3. 1

0. 6

0. 8

14. 1

1. 2

4. 5

1. 0

0. 7

s

0

u

Co I

Ti I

-C2

Fe I p La II

C2

Ni I

Fe I

C2Cr II

2. 08

1. 44

R27

4. 59

0. 23 R 8

3. 83

3. 57 R 8

3. 71

91

109

0,0

1242

36

1,1

177

789

1,1

24

19

19>

19

5109.122 10 2. 0 C2-

C2 R 29 R 29

0,0

0,0 1919 5116.188 4. 5 0. 9 MgHC2 Q 27 R 7

0,0

1,1 20

19

5109.306 4. 5 0. 9 C2 R 29 0,0 19 5116.473 7 1. 4 MgH Q 27 0,0 20

5109.435m 5 1. 0 S Til 1. 44 109 5116.662 7. 5 1. 5 C2? R26 0,0 19

5109.657S 69 IS. 7 s Fe I 4. 30 1089 5116.772 12 2. 3 -C2 R26 0,0 19

5110.017 4 0. 8 C2? R 12 1,1 19 5116.902 6. 5 1. 3 C2 R26 0,0 19

5110.372

5110.435 1 126

f 10. 9

1 18.

7

s

Fe I p

liFei

3. 57

0. 00

790

1

5117.166

5117.348

3

3. 5

0. 6

0. 7

Ce II?

C2?

1. 40 R 6

23

1,1 19

5110.763 27 5. S s Cr I 2. 71 60 5117.764 2 0. 4

5110.972 2. 5 0. 5 C2 R 11 1,1 19 5117.942 21 4. 1 s Mn I 3. 13 32

214
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

5118.073 7. 5 1. 5 C2 P 53 0,0 19

5118.184 9 1. 8 C2? P 51 0,0 19

5118.360 3 0. 6 MgH R 14 0,0 20

5118.557 1 0. 2

5118.822 5 0. 9 MgH R 14 0,0 20

5119.120 14 2. 7 0 Yii 0. 99 20

5119.212 4 0. 8 0 C2?- R 25 0,0 19

5119.25 m 2 0. 4 s

5119.379 7 1. S C2 R 25 0,0 19

5119.652 2. 5 0. 6

5119.773 1. 5 0. 3 C2

5119.903 3. 5 0. 8 Fe ip 3. 88 960

5120.111 2 0. 4

6120.346 14 2. 7 Fe II p

C2

2. 83 R 2 35

1,1 19

5120.420 31 6. 0 s Ti I 2. 58 288

5120.633 8. 5 1. 6 -C2 P 52 0,0 19

5120.729 3. 5 0. 7 C2 P 52 0,0 19

5120.886 7. 5 1. 5 MgH

Fe I p

Q 26

4. 44

0,0 1150 20

5121.030 3 0. 6

5121.226 3. 5 0. 7 MgH Q 26 0,0 20

5121.438 11 2. 1 C2 R24 0,0 19

5121.563 34 6. 6 w1 Ni I 3. 94 177

5121.649 71 13. 9 u Fe I 4. 28 1095

5121.982 5 1. 0 Fe I? p 3. 55 745

5122.121 11 2. 1 s Cr I 1. 03 19

5122.309 5 1. 0 C2? P 30 1,1 19

5122.447 2 0. 4 C2? P 30 1,1 19

5122.798 19 3.6 C2Co I P 51

3. 66

0,0 170

19

5123.006 11 2. 1 u La II 0. 32 36

5123.222 29 5. 7 u Yii 0. 99 21

5123.291 13 2. 5 0 Fe I /3. 30

14. 41 629

1150

5123.470 17 3. 3 s Cr I 1. 03 20 5123.730m 101 20. 1 s Fe I 1. 01 16

5123.901 5 1. 0 MgH R 13 0,0 20

5124.051 19 3. 1 C2 R 23 0,0 19

Wavelength

(I)

Equivalent Width AX

(ml)

Re- duced

Width

AX/X

(v) vl' )

Spot

Solar Idcmili cation

Low

E P

or Rot. Line

RMT

No.

or

Vib,

Band

Notes

5124.197 2. 5 0. 5 C2Fe I P 26

4. 19

1,1 1035

19

5124.389 3. 5 0. 7 MgH R 13 0,0 20

5124.617 20 3. 7 s,N Fe I p 3. 30 585

5124.810

5124.92 a

1

} ^»

f 1. 6

J

[ 0.

s

C2?

C2?

P 27 P 27

1,1

1,1

19

16,19

5125.128 100 19. 5 u Fe I 4. 22 1090

5125.250 52 10. 1 u Ni I 3. 68 160

5125.475 11 2. 1 C2MgH

P 26 Q25

1,1 0,0 1920

5125.637 10 2. 0 Si I? 5. 08

5125.839 11 2. 1 MgH Q 25 0,0 20

5125.990 8 1. 6 C2-

C2 R22

P 25

0,0

1,1 19

19

5126.199m 75 14. 6 u Fe I (Co i)

4. 26

3. 62 1089

170

5126.513 3 0. 6 Cr I 3. 37

5126.686 5 1. 0 C2? P 24 1,1 19

5126.864 6. 5 1. 3 C2 P 22 1,1 19

5127.018 4 0. 8 C2

5127.189 4. 5 0. 9 C2 P 23 1,1 19

5127.368m 85 17. 6 s Fe I 0. 91 16

5127.688 20 3. 9 s Fe I p 0. 05 1

5127.874 9 1. 7 Fe II C2

5. 57 P 20

167

1,1 19

5128.081 18 3. 3 C2?-

Ni I P 213. 70

1,1 113

19

5128.201 7 1. 4 C2? /R21

IP 21

0,0

1,1 }.9

5128.316 5. 5 1. 1 C2 R21 0,0 19

5128.494 8. 5 1. 7 s C2-

V I

/R 21 IP 20

2. 29

0,0

1,1 123

} 17,19

5128.642 3 0. 6 C2? P 18 1,1 19

5128.913 6. 5 1. 3 C2 P 17 1,1 19 5129.162m 70 13. 6 w Ti II 1. 89 86

5129.377m 62 12. 1 w Ni I 3. 68 159 5129.634m 48 9. 4 w Fe I 3. 94 965

c 1 on 000 51.!!y.o^o 4

A C

U. 0 JN'igil U,U

5129.945 2. 5 0. 5 MgH Q 24 0,0 20

5130.135 2. 5 0. 5

5130.260 8 1. 6 C2 R20 0,0 19

215
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

bolar

Identification

Low

E r

or Rot. Line

RMT "NT ^ JNo. or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

boiar

Identification

Lo"w E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

5130.372 23 4. 5 Ni I 3. 84 177 5137.867 2 0. 4

5130.588

K1 01 ono Olol.oUo olol.4/Dm

olol.bUz

15

1 K

i. 0

1 1 11TO

-t -1 1

1

2. 9

U. 0

0 -1 /. 1

if: 0

10. 0 0 1 Z. 1

s!

C2-

Nd II Fe I p

Ti II p Fe I

R20

1. 30

4. ol

1 00

0 00

Jr 4/

0,0 75

1 1 0

OD

DO

A A U,U

19

1 Aly

5137.961

5138.110

5138.347

5138.516

5138.717

3. 5

7. 5

Ti

11

13

0. 8

1.4

2. 1

1. 9

2. 4 s

Cn

C2MgH

C2Cn- T\T„'rT Mgxl

3. 42 R 16 Q 22 R 16

0. 98

207

0,0

0,0

0,0

19

0.0

19

20

19

17OA20

oicSi. / / oin A 0 0. z u i\I I cS. /U 11/1 PI QQ QCa Oloo.SDy D. 5

1 0

1. 0 KjI 11 0 07 6. 61

OioZ. IDO z v. 4

r 1 OA A01 oloy.021 1 013 I. 5

OL0Z.60I 7 f; /. 0 1. 0 u ^2 "Din A A U,U 1 1

0

Id, ly C 1 OA OC 1 oloy.zDlm 1 01 137 ZD. D s r e I 0 AA

6. UU 000 383

5132.501 5 1.

0

s C2- R 19 0,0 19 5139.473m 152 29. 6 s Fe I 2. 94 383

5132.674 24 4.

7

w Fe II p 2. 81 35 5139.648 46 8. 9 s Cr I 3. 42 207

5132.950 3. 5 0.

7

s Ti I 2. 25 230 5139.924 13 2. 5 0? C2? R 15 0,0 19

5133.038

5133.198

5133.478

5133.699m|

5133.820 J 5134.072

5134.205

5134.333

1

161

18

165

6

4. 5

8. 5

0. 2

1.

2

3.

5

J 30. 4

I 3. 5

1. 4

0. 9

1. 7

u

Fe I p Co I Fei

C2

MgH

C2

3. 60

3. 93

4. 18 P 44

Q 23 R 18

818

180

1092

0,0

0,0

0,0

19

20

19

5140.160

5140.380

5140.823

5141.025

5141.211

5141.323

5141.540

5141.74Dm

9

5. 5

17

2. 5

13

7. 5

5

90

1. 7

1. 1

S. 1

0. 5

2.4

1. 6

1. 0

16. 9

w?

s

s

C2?-

MgH?

C2Fe I

C2

^2Fe I p re I

R 15 R 10 R 15

P 42

"D /I 0

1 4z

3. 69

0 /1

0

Z. 4/

0,0 0,0

0,0

0,0 A A U,U

930

11/1 114

1920

19

17

19

1 A19

5134.528 18 3. 5 MgH fQ 23

1 T> 1 1 [ix 11

0,0 A A U,U I20 J 5141.902 7. 5 1. 5 C2 "DK 114 A A U,U 19 5134.683 17 3. 3 C, R 18 0,0 19 7 1. 4 C, R 14 0,0 19 5134.855 3 0. 6 5142.276 6. 5 1. 3 s Cr I 2. 71 60 5135.104 2 0. 4 MgH R 11 0,0 20 5142.32 a 7 1. 4 MgH Q 21 0,0 20

5135.184 6. 5 1. 2 Yi? 2. 29 5142.530m 117 22. 8 Fe I /4. 26

\4. 30

1092 1090

5135.582

5135.707

5135.931

5136.099

5136.273

5136.455

5136.664

5136.800 5137.080m

5137.393m

5137.579

5137.696

10

6. 5

1. 5

20

11

8

5. 5

14

92

102

20

8

1. 9

1. S

0. 3

3. 9

2. 0

1. 5

1. 1

2. 7

17. 9

19. 8

3. 9

1. 6

0

s

0

su

C2-

C2Cn

Fei

C2

C2

c,Fe II Nil

Fe I

C2C2-

P 45 P 43

3. 37

4. 19 R 17 R 17 R 17

2. 84

1. 68

4. 18 P 44 P 44

0,0

0,0

1036

0,0

0,0

0,0

35

48

1090

0,0

0,0

19

19

19

19

19

19

19

5142.786m

5142.936m

5143.121

5143.342

5143.593

5143.728

5143.864

5144.039

5144.374

5144.585

5144.64 m

89

111

14

8. 5

8. 5

23

6

4

4. 5

12

17. 3 2L 6

2. 7

1. 6

1. 7

4. s

1. 2

0. 8

0. 9

2. 5

w

s

s

ol s,N

Ni I Fe I

C2

C2Fe I

C2

C2?-

Cr I

3. 70

0. 96

R 13 R 13

2. 20 R 13

P 40

2. 71

161

16

0,0

0,0

65

0,0

0,0

60

19

19

16

19

19

13

216
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5144.674 21 4. 1 MgH

C2-

R9

P 40

0,0 0,0 20

19

5144.927 6. 5 1. 3 C2 R 12 0,0 19 5145.102m 44 9. 2 u Fe I 2. 20 66

5145.237 7 1. 4 c. R 12 0,0 19 5145.468m 37 6. 4 s Ti I 1. 46 109

5145.740 9. 5 _ 1. 8 Fe I p 3. 69 931

5146.119 37 6. 6 0? Fe II p 2. 83 /P 38 IP 39

35

0,0

0,0

17

5146.314 27 5. 2 ul Fe I 4 37 1150 17 5146.491m 76 14. 8 u Ni I 3. 70 162

5146.776 28 5. 4 0? Co IC23. 57 Rll

170

0,0 15,17 19

5147.103 24 6. 0 0 Fe I Fe II

5147.290 4 0. 8 5147.482m 36 6. 7 Ti I 0. 00 4

5147.697 18 S. 0 C2 P 38 0,0 19

5147.823 10 1. 9 C2 P 36 0,0 19 5148.051m 74 14. 4 u Fe I 4. 28 1090 5148.237m 89 17. 3 s Fe I 4. 26 1095

5148.458 3. 5 0. 7

5148.549a 3 0. 8 C2? R 10 0,0 19

5148.676 13 2. 5 s Ni I 3. 68 158

5148.846 14 2. 4 s,N Na I 2. 10 8

5149.095 18 3. 5 w? C2? P 37 0,0 19

5149.214 9 1. 7 u C2? P 37 0,0 19

5149.343 4 0. 8 C2 R8 0,0 19

5149.520 6 1. 1 MgH

Fe IFe II

R8

3. 94

0,0 962

20

5149.796 11 2. 1 Co I MgHL 74 Q 19 39

0,0 20

5150.042 2. 5 0. 5 MgH R 8 0,0 20

5150.197 22 3. 9 MgH

Fe I p Q 193. 57

0,0 789

20

5150.359 4 1. 0

5150.563 13 2. h C2 P 36 0,0 19

5150.674 9. 5 1. 8 C2 P 36 0,0 19

5150.852S

5150.938 j 114

f 20. 3

1 3. 7

S Fe I Fe II p

0. 99

2. 85

16

35

Wavelength

(A)

Equivalent Width

AX

(mA)

lie- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5151.174 7 1. 4 C2 R8 0,0 19

5151.463 161 1. 1 5151.917m 100 19. 8 S Fe I 1. 01 16 5152.190m 38 6. 8 S Til 0. 02 4

5152.529 |4| 0. 8 C2 R 5 0,0 19

5152.959 4 0. 8 C2? R7 0,0 19

5153.168 5153.241m

1 56

f 3. 2

I 8. 5 u,N

C2Cu I

P 34

3. 78

0,0

7

19

5153.410 24 4. 6 s,N Nai 2. 10 8

5153.505 21 4. 1 Cr II 3. 76 24

5153.679 7. 5 1. 5 MgH Q 18 0,0 20

5153.756 2. 5 0. 5 C2? R 6 0,0 19

5153.818 3. 5 0. 7 C2 R4 0,0 19

5154.075m 73 11 2 u Ti II 1. 57 70

5154.337

5154.412

13

28

2. 5

5. 4

1

1

fC2

J[Pe 11 p

P 33

2. 84

0,0

35

17,19

17

5154.747 4. 5 0. 9 MgH R7 0,0 20

5154.881 3. 5 0. 7 Co I? 4. 15

5155.132m 52 9. 3 u Nil 3. 90 206 17

5155.524 14 2. 5 u C2? P 32 0,0 19

5155.771m 78 14. 9 s? Ni I 3. 90 210

5156.072 17 3. 3 Fe II

5156.356 10 1. 9 Co I 4. 06 180

5156.557 16 3. 1 C2 P 31 0,0 19

5156.652 26 4. 8 MgH- Q 17 0,0 20

5156.997 6. 5 1. 3 MgH Q 17 0,0 20

5157.204 18 3. 5

5157.424 2 0. 4 La II 2. 21 97

5157.619 12 2. 3 s,d C2 P 30 0,0 17,19

5157.742 12 2. 3 u C2? P 30 0,0 19

5157.984 19 3. 5 u Ni I 3. 61 111

5158.30 m S,N 13

5158.37 a 1 0. 2

5158.525 11 2. 1 0 C2- P 29 0,0 19

6 1. 3 C, P 29 0 0 19

5158.860 4. 5 0. 9 Co I 4. 05 188

5158.93 m 0. 5 0. 1 s

5159.0658 65 13. 4 w Fe I 4. 28 1091

217
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

CI CO 909

5159.464

A

t:

12

\J, 0

2. 3 w? C2-

R 6 P 280 0

0,0

20

16,19

5164.913 22 4. 2 s? C2Fe I

fP 1

7

IP 18

4. 14

0,0 1033

1} 17,19

5159.605 6 1.4 s 5165.035 29 5. 6 Co? P 17 0,0 19

5159.779 4 0. 8 MgH Q 16 0,0 20 5165.128 15 2. 9 C2- JP 16 IP 17

0,0

0,0 }-

5159.966 4 0. 8 Fe I p 4. 30 1095 Co I 1. 71 39

5160.124

5160.244

5160.387

5160.568

5160.835

5161.028

4

16

6

2. 5

12

16

0. 8

3. 1

1. 2

0. 5

2. 3

3. 1

Fe I?

C2

Fe 11

P 27 P 27

5. 57 P 26

0,0

0,0

167

0,0

19

19

19

5165.248

5165.415m

5165.581

5165.963 5166.284m

17

87

9

5

115

3. 3

18. 0

1. 7

1. 1

22. 2

w

S

C2

Fei

MgH

MgH

Fe I (Cri)

fP 15 IP 16

4. 22 Q 14 Q 14

0. 00

3. 43

0,0

0,0

1089

0,0

0,0

1 207

20

20

5161.179

5161.28 a

5161.683

16

4. 5

6

3. 1

0. 9

1. 2

w1 Fe II p —

C2?

C2?

2. 85 P 24

P 25

35

0,0

0,0

16

19

19

5167.327 5167.508m

5167.718

5167.954

1 935

18

4. 5

f 173

1 76.

0

6. 4

1. 2

S

su

Mgi

Fe I Fe I p

Cr I

2. 71

1. 48

3. 41

3. 43

2

37

717

207

5161.764

5161.78 ra

14 2. 7 u?

s

C2

Cr I

P 25

2. 71

o,o|

60

15,16, 19

13

5168.194 |8| 1. 8 MgH

Fe I p Q 13

r3. 94

13. 94

0,0 964

960

20

5161.856 9 1. 7 C2? P 25 0,0 19 5168.663m 67 13. 7 u Ni I 3. 70 112

5161.987 12 2. 3 5168.908m 114 23. 0 s Fe I 0. 05 1 5162.281m 154 SI. 4 w Fe I 4. 18 1089 5169.050m 154 31. 0 w Fe II 2. 89 42

5162.525 25 4. 8 C2 P 24 0,0 19 5169.300 30 6. 0 w Fe I p 4. 07 1032

5162.733 16 3. 1 MgH Q 15 0,0 20 5169.43 m 10 2. 0 s

5162.907 21 4. 1 C2 P 23 0,0 19 5169.495 3. 5 0. 7

5163.040 14 2. 7 C2 P 23 0,0 19 5169.707 4 0. 8 Dy 11

5163.160

5163.415

5163.591

5163.834

5164.001

5164.13 a

9

14

14

13

11

6

1. 7

2. 7

2. 7

2. 5

2. 1

1. 2

C2-

MgH

C2

C2

QjC2

P 7 Q 15 P 22 P 22 P 21 P 21

0,0

0,0

0,0

0,0

0,0

0,0

1920

19

19

19

19

5170.106

5170.46 m

5170.479

5170.598

5170.767

5171.028

3

2. 5

3

6

32

5

0. 6

0. 5

0. 6

1. 2

6. 6

1. 0

s

w

Fe I p

MgH

Fe I Ru I MgH

4. 59

Q 12

0. 93 Q 12

1241

0,0

11

0,0

20

20

5164.236 18 3. 5 C2 P 20 0,0 19 5171.610m 160 32. 9 s? Fei 1. 48 36

5164.391 10 1. 9 C2 P 20 0,0 19 5172.221 13 5. 4 Fe I p 2. 56 210 5164.552m 48 9. 3 u Fe I 4. 43 1166 5172.698m 1259 234 s Mgi 2. 71 2

5164.680

5164.781

15

17

2. 9

3. 3

u

u

Fe I p

C2

C2

2. 59 P 10

fP 11 IP 18

210

0,0

0,0

0,0

19 5173.326

5173.487 5173.749m

5173.911

2. 5

3

67

3. 5

0. 8

0. 9

13. 5

0. 8

s

s

MgH

Fei

Til

Pr II

Qll

0. 00

0. 97

0,0

4

35

20

218

J
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5174.035 3 0. 7 5184.829 1. 5 0. 4 MgH P 31 0,0 20

5174.427 5. 5 1. 2 5185.035 2. 5 0. G S,d -IMgH Q 3 0,0 17,20

5174.943 4 0. 8 MgH Q 10 0,0 20 5185.75 m 1. 5 0. 3 S,d MgH- Q 2 0,0 20

5175.252 5 1. 0 5185.908m 58 12. 7 w Ti II 1. 89 8G

5175.411 4. 5 0. 9 MgH Q 10 0,0 20 5186.109 3 0. G

5175.749

5176.026

5176.138 5176.565m

5176.792

sTs

6

9. 5

56

10

1. 1

1. 2

1. 8

10. 8

1. 9

w

Fe I p —

Ni i?p

Co I Ni I |Vi- MgH

0. 09

3. 85

2. 08

3. 90

Q 9

1 188

92

209

0,0 20

5186.331

5186.557

5187.11 m

5187.263

5187.457

5187.838r

7

16

2

3

15. 5|

8

1. 3

3. 1

0. 4

0. 6

1. 1

1. 5

s,d

u

s

Ti INi I

Ce II Ni I

2. 12

3. 90

L 21

3. 70

183

205

15

159

5177.011 4 0. 8 5187.917m 50 10. 4 w1 Fe I 4 14 1032

5177.241 24 4. 6 u Fe I 3. 69 930 5188.062 7 1. 3 MgH P 30 0,0 20

5177.411 20 3. 9 u Cr I 3. 43 201 5188.238 5 1. 0 La II 2. 45 95

5177.610 4 0. 8 MgH P 33 0,0 20 5188.407 5. 5 1. 1

5177.811

5177.994

2

2. 5

0. 4

0. 5

Cri 3. 42 206 5188.698m

5188.852m

1 .202

1 20. 5

1 21. 6

w

s

Ti II Ca I1. 58

2. 93

70

49

5178.480 5. 5 1. 1 MgH Q8 0,0 20 5189.136 7. 5 1. 4

5178.801 24 4. 6 w Fe I 4. 39 1166 5189.338 1. 5 0. 3

5179.125

5179.530

5179.800 5180.069m

5180.405

5180.583

5180.875

5181.165

U XOX . tjOXJ

18

|2.5|

7. 5

50

6

4. 5

2. 5

4. 5

18

3. 5

0. 5

1. 5

9. A

1. 2

0. 9

0. 5

0. 9

3. 7

0

u

u

Ni I

Nd II Fe I

MgH

MgH

Fe I?

3. 90

4. 47

Q7

P 32

fP32

IQ6

202

1166

0,0

0,0

0,01 0,0/

20

20

17,20

5189.581

5189.785

5190.19 m

5190.26 a

5190.50 a

to 5190.90 a

5191.078 5191.465m

5191.602

2

1. 5

1. 5

1 '

|9|

160

18

0. 4

0. 3

0. 3

1. 3

1. 7

S2. 4

3. 5

s

s

s

Sii?-

Ti I p

MgH

MgH

Fe I

||Zr II Fe II p

2. 24

P 29

P 29

3. 04

1. 76

3. 20

215

0,0

0,0 383

95

52

13,17

20

20

5181.545 6 1. 3 5191.747 • 18 3. 5

5181.844 8. 5 1. 8 5191.868 4. 5 a 9

5181.957 3. 5 0. 8 MgH Q 6 0,0 20 5191.998 42 8. 1 s Cr I 3. 39 201

5182.241 2. 5 0. 6 5192.353m 176 36. 6 s Fe I 3. 00 383

5182.740r 0. 5 0. 2 Ni I? 4. 09 5192.497 25 4. 8 Ni I 3. 70 111

5183.619m 1584 SOS s Mg I 2. 72 2 5192.621 14 2. 7 s Nd II L 14 75

5184.196 9 4. 4 Fe I p 4. 31 1147 5192.755 5 1. 0

5184.273m 42 14. 5 w Fe I 4. 28 1089 5192.978m 80 15. 8 s Ti I 0. 02 4

5184.562m 43 11. 6 u |Ni I Cr I

3. 70

3. 41 159 201

5193.177 5 1. 0

219
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Z3

Notes

5193.336 3 0. 6 MgH P 28 0,0 20 5204.246 |8| 1. 5 MgH P 23 0,0 20

5193.502

5193.863

10

2

1. 9

0. 4

s Cr I MgH

3. 42 P 28206

0,0 20

5204.513r

5204.601r 1 212

1 28. 8

1 21. 8

j Cri

1 Fei

0. 94

0. 09

7

1

5194.056 10 1. 9 s Ti I 2. 10 183 5204.945 6. 5 1. 2 Fei 2. 99 407

5194.77 m

5194.949m

5195.480m

5196.065m

5196.268

5196.452

5196.578

5197.170

5197.376 5197.576m

5197.789

5197.942

5198.342

5198.718S

5198,866r

126

114

78

1

34

32

25

4

80

4. 5

37

2

87

5. 5

25. 0

21. 9

15. 0

0. 2

6. 5

6. 2

4. 8

0. 8

15. 4

0. 9

7. 1

0. 4

17. 9

1. 1

s

suw

s?

s

u

sw

u

s

V I?

Fe I Fe I Fe I Fe I p Cr I

Cr I Mn I Ni I

Fe II

Fe I MgH

Fe I MgH

Fe I

/2. 29

12. 26 L 56

4. 22

4. 26

2. 95

3. 45

/2. 71

13. 45

3. 13

3. 90

3. 23

4. 30 P 26

2. 22 P 26

3. 55

125 125

36

1092

1091

406

207

58

20732

204

49

1091

0,0

66

0,0 743

}13

20

20

5205.15 a

5205.302 5205.730m

5206.044m

5206.202

5206.545

5206.811

5207.097

5207.286

5207.623

5207.864 5207.935m

5208.105 5208.432m

5208.601m

5209.09 a

5209.24 a

2

|6| 52

1 216

17

5. 5

1. 5

2

4. 5

8

19

12

247

117

141

|4|

0. 4

1. 2

10. 0

[ 36. 6

1 8.4

3. 3

1. 1

0. 3

0. 4

0. 9

1. 5

3. 6

2. 5

47. 4

22. 5

0.8

0. 8

uS

u

swl

s,Nu

uS

wl

MgH

Fe I p

Yii

Cri

(Til)

Crip

Fe I p

MgH

MgH

MgH

Til

Fei

Cri

Fei

MgH

MgH

P 8

4. 26

1. 03

0. 94

2. 49

3. 43

4. 28 P 21 P 10 P 21

2. 09

3. 63

0. 94

3. 24 P 19 P 12

0,0

1112

20

7 276

206

1095

0,0

0,0

0,0

183

880

7

553

0,0

0,0

20

20

20

20

20

20

5199.600 3. 5 0. 7 s,d -MgH P 5 0,0 17,20 5209.609 1 0. 2 MgH P 19 0,0 20

5199.718

5200.185

3

22

0. 6 14 s,N

V II Cr I

2. 27

3. 38

55

201

5209.777 3 0. 6 MgH

fP 12 P 13 Ip 18

0,0

0,0 0,0 20

5200.415m 37 7. 1 w? Y II 0. 99 20 5209.892 9. 5 1. 8 u Fe I 3. 24 584

5200.824 3 0. 6 MgH P 6 0,0 20 5210.043 3. 5 0. 7 Co I 3. 41 167

5201.095

5201.294

11

3

2. 1

0. 6

s Ti I 2. 09 183 17 5210.257 4. 5 0. 9 S,N MgHfP 14 P 17 [P 18

0,0 0,0

0,0

] 16,20

5201.606 3. 5 0. 7 S,d MgH P 6 0,0 17,20 5210.392m 86 17. S S Ti I 0. 05 4

5201.82 m s 13 5210.851 12 2. 3 Cr II 3. 76 24

5201.931

5202.00 a

5202.082

5202.273 5202 348

3. 5

6

11

] 155

)

0. 7

1. 2

2. 1

r 14. 9

21 8

M?

-I/?

Fe I

X e i

4. 26

9 1 S

1090

UO

5210.939

5211.206

5211.535

o^l i.oiD

3. 5

8

29

o

0. 7

1. 5

5. 8

U. \J

sw

MgH

Ti I Fe ITi II

C.n T?

/P 15 IP 16

0. 84

2. 59

o. vo

0,0

0,0

37

103

}20

5202.781 2 0. 4 S MgH P 7 0,0 16,20 5212.231 10 1. 9 s,N Cri 3. 32 189

5202.990 2. 5 0. 5 MgH P 24 0,0 20 5212.27 m 6 1. 2 s Ti I 2. 25 215

5203.513 3. 5 0. 7 s,d -MgH P 7 0,0 17,20 5212.346 4. 5 0. 9 Nd II 0. 20 44

220
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5212.691 21 4. 0 w,dt Co I 3. 51 170 5223.190 26 5. 0 s Fei 3. 63 880

5212.996 5 1. 0 s Ti I? 2. 23 215 5223.368 1 0. 2 Fei?

5213.352 9 1. 5 w? Fe I p 4. 39 1165 5223.543 4 0. 8

6213.57 a 2 0. 4 5223.628 11 2. 1 S Ti I 2. 09 183

5213.812 7. 5 1. 4 u Fe I 3. 94 %2 5223.896 2. 5 0. 5 s

5214.130 16 S. 5 s Cri 3. 37 193 5224.074 10 1. 9 s Cri 3. 41 201

5214.616 17 2. 9 s,N Cri 3. 32 189 5224.16 m 1 0. 2 s Ti I 0. 83 37

5214.732 3 0. 6 5224.310m 36 6. 9 S Til 2. 13 183 5215.188m

5215.571

116

26

24- 7

5. 0

sw

Fe I 3. 26 553

16

5224.551 26 5. 0 S Cr iTii

/2. 71

13. 37

2. 10

59 193

183

5215.885 1. 5 0. 3 V II? 2. 27 55 5224.725 1. 5 0. 3 5216.283m

5216.484

5216.853 5217.396m

5217.675

5217.870

5217.922

6218.09 m

5218.209m

6218.516

5219.028 5219.706m

108

29

1

102

2. 5

48

3

2. 5

25

22. 2

5. 6

0. 2

20. 7

0. 5

j

2. 6

1 6. 1

9. 8

0. 6

0. 5 4.6

su

s

u

su

s

Fe I Ni I

Fe I Fe I p

Fe I

Ti I Cu I Fe I p

Pr II

Ti I

L 61

3. 74

3. 21

3. 98

3. 64

3. 82

4. 58

0. 79

0. 02

36

113

553

965

880

7

1240

37

4

13

5224.937 1

5225.032 J 5225.348

5225. 634S

5225.713

5225.813

5226.061

5226.209

5226.384 5226.545m

5226.870m

80

2

68

3. 5

16

17

12

10

94

160

[10. 0

[ 6. 2

0. 4

12. 4

0. 7

3. 1

3. 2

2. 3

1. 9

18. 4

32. 5

S,N

s

S

su

w?

s

TiiCr I Cri

Fe I

Cn

Fe I

Fe I p

Ti II Fe I (Cri)

2. 12

3. 45

3. 43

0. 11

2. 71

3. 41

2. 95

1. 57

3. 04

3. 37

183

201

201

1

58

716

406

70

383

193

5219.883

5220.086

6220.296

5220.585

5220.912

5221.039

5221.763

2. 5

14

26

3. 5

9. 5

19

27

0. 5

2. 7

5. 0

0. 7

1. 8

3. 6

6. 0

u

u

s

s,d?

s

Cu I Nil

Cr I -Fe I

|Cr I Fe I

3. 82

3. 74

3. 38

4. 29

3. 37

3. 27

7

114

201

193 628

5227.192m

5227.473

6227.737

5227.881

5228.103 5228.383m

5228.562

277

2. 5

5

2. 5

22

60

7. 5

53. 4

0. 5

1.0

0. 5

4. 2

11. 5

1. 4

u

s

su

Fei

{

Cn

Ti up

Cr I Fe I

1. 56

(2. 42)

2. 71

2. 60

3. 37

4. 22

37

114

58

103

193

1091

6222.190 2 0. 4 Sr I? 2. 25 5228.60 m s 13

5222.397

5222.509

5222.67 m

18

5

3. 4

1. 0

s,N

s,N

Cr I Fe I p

Co I Cri

3. 43

2. 28

3. 97

2. 71

206

112

59 13

5229.25 a

to 5229.80 a

5229.860m

5. 5

J

124

1. 1

23. 5 u Fe I /3. 28

14. 22

553 1090

5222.684 23 4. 4 s Til 2. 08 183 5230.056 3. 5 0. 7

5222.876

6222.98 m

5. 5 1. 1

s 13,16

5230.216 25 4. 8 s IICoi Cr I

1. 74

2. 71 3958

221
The Solar Spectrum—-Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notea

5230.392 5 1. 0 Fe I? 5240.359 5 1. 0 u Fe I p 3. 27 584

5230.696 6. 5 1. 2 u 5240.475 8. 5 1. 6 s Cr I 3. 67 237

5230.984 3. 5 0. 7 s Ti I 2. 24 215 5240.878 4 5 1. 1 s V I 2. 37 131

5231.25 m 3 0. 6 s 16 5241.182 0. 5 0. 1 V II 4. 52 241

5231.396 9 1. 7 u Fe I 3. 57 787 5241.461 3. 5 0. 7 s Cr I 2. 71 59

5231.46 a 4 0. 8 5241.923 5. 5 1. 0 u Fe I 4. 41 1150

5231.52 m s 13 5242.070 15 2. 9 w

5231.63 a 4 0. 8 5242.284 2 0. 4

5231.83 a 3 0. 6 5242.500S 80 16. 0 s Fe I 3. 03 843

5232.503 12 1. 4 w,N Cr ir 4. 07 43 5243.178 14 2. 7 w

5232.82?m s,N 13 5243.360 19 3. 6 s Cr I 3. 39 201 5232.952m 346 64- 9 S Fe 1 2. 94 383 5243.471 6. 5 1. 2

5233.72 m 1. 5 0. 3 s 5243.783m 60 11. 4 s Fe I 4. 26 1089

5233.854 2 0. 4 s Ti I 0. 82 37 5244.170 1. 5 0. 3

5234.090 5. 5 1. 1 s V I 2. 36 131 5244.535 4 0. 8

5234.213 8 1. 5 u Nd 11 0. 55 74 16 5244.951 1 0. 2

5234.436 5234.630m

5234.82 m

5234.879

5235.032

5235.188

5235 3Q0m

2

81

3

8. 5

23

] 96

0. 4

16. 2

0. 6

1. 6

4. 4

1 14. 2

w

s

s

s

u

Fe II

Co I

Fp t

3. 22

2. 14

/2. 59

14. 07

49

83

210

1031

13

5245.629

5245.737

5246.004

5246.147

5246.556

5246.65 m

5246.777

6

6

3

2. 5

4

1. 5

17

1. 1

1. 1

0. 6

0. 5

0. 9

0. 3

3. 2

s

s

s

ss

sw

Ni I? Fe I p

Fe I Fe I p

Ti I

Ti I

Ti I Cr II

4. 09

4. 31

3. 41

3. 25

2. 50

0. 84

3. 71

1149

715

628

282

37

23

5235.508 [ 5. 6 u Ni I 3. 90 208 5247.058m 59 11. 4 s Fe I 0. 09 1

5236.207 27 5. 2 u Fe I 4. 19 1034 5247.297m 10 1. 9 S Ti I 2. 10 183

5236.378 9 1. 7 u Fe I p 4. 31 1146 5247.574m 76 H. 8 s Cr I 0. 96 18

5237.087 5237.325m

5237.843

4

49

3. 5

0. 8

9. A

0. 7

w,N

Co I?

, Cr II

4. 17

4. 07 43

5247.923

5248.375

16

5. 5

3. 0

1. 0

s,N

s

|Co I Cr I

Ti I

1. 78

2. 71

/O. 81 \L 88

39

58

37 156

5238.249 3 0. 6 u?,N Fe I 3. 98 962 5248.991 6. 5 1. 2 s

5238.52 m S Sr I 2. 26 13 5249.111 30 5. 7 u Fe I 4. 47 1166

5238.568m

5238.969

5239.460 5239.823m

5239.95 m

5240.144

15

16

5

55

3

2. 5

2. 9

3. 0

1. 0

10. 5

0. 6

0. 5

S

s

w

s

Ti I

Cr I

Sc II

Ti I

fO. 85

12. 09

2. 71

1. 45

0. 81

37

183

59

26

37

5249.425

5249.579

5249.717

5249.829

5250.023 5250.216m

11

11

7

3

4. 5

62

2. 1

2. 1

1. 3

0. 6

0. 9

11. 6

u

u

u

s

Cr II Nd II

Co I Fe I

3. 76

0. 98

4. 17

0. 12

23

75

190

1

222
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notea

5250.433 3 0. 6 5261.35 a 2 0. 4 5250.654m 104 19. 6 s Fe I 2. 20 06 5201.501 3 0. 6 Fe I p 2. 95 406

5250.913 15 2. 8 S Ti I 0. 83 37 5261.708m 99 20. 0 s Cai 2. 52 22

5251.487 2. 5 0. 5 S Ti I 0. 82 37 5261.959 3. 5 0. 7

5251.607 5251.974m

1

40

0. 2

7. 6 u Fe I

5262.150

5262.248

1

1 128

f 5. 7

J

i 2€. 0

u

s

Ti II Cai1. 58

2. 52

70

22 5252.106m 16 3. 0 S Ti I 0. 05 4 5262.457 4. 5 0. 9 Fe II p 3. 20 52

5252.36 m s,N 13 5262.623 12 2. 3 u Fe I p 4. 32 1149

5253.033 16 3. 0 s Fe I p 2. 28 113 5262.887 19 3. 6 s Fe I p 3. 25 628

5253.259 3. 5 0 7 Fe I p 3. 63 875 5263.077 6 1. 1 Fe I?

5253.468S 75 14. 9 s Fe I 3. 28 553 5263.314m 121 24. 5 s Fe I 3. 26 553

5253.685 4. 5 0. 9 5263.494 13 2. 5 s Ti I 2. 13 183

5253.951 8. 5 1. 6 5263.718 11 2. 1 s,N Cr I 4. 49 309

5254.651 7 1. 3 Co I 3. 97 187 5263.865m 47 8. 9 u Fe I 3. 57 788

5254.953m

5255.123

5255.325

5255.517

5255.663

5255.743

5255.812

5256.933

92

38

36

7

1

J

18

17. 5

7. 2

6. 8

1. 3

( 3. 2

\ 4. 9

I 0. 3

3. 4

s

s s,N

su

uSw

Cri-

|Fei

Cr I Mn I Nd II Fe I p Fe I p

Ti I Fe II (Sr I)

3. 41

0. 11

3. 46

3. 13

0. 20

4. 22

4. 28

2. 12

2. 89

2. 27

201

1

225

32

43

1089

1091

183

41

5263.992

5264.160

5264.246

5264.405

5264.591 5264.808m

5264.977

5265.153

5265.254

3. 5

1 153

9

2

45

3

27

9

0. 7

1 19. 1

[ 15. 5

1. 7

0. 4

8. 5

0. 6

5. 1

1. 7

u

uw

s

s

f Cri

1 Cai

Fe II

Cr I Fe I p

0. 97

2. 52

3. 33

3. 43

3. 02

18

22

48

201

407

16

5257.080 2 0. 4 Cr I? 3. 43 205 5265.418 13 2. 5 s Fe I p 4. 31 1145

5257.362 3 0. 6 5265.560m 112 21. 3 s Ca I 2. 52 22

5257.645

5257.832

5258.323

5258.828

5259.089

5259.488

5259.735

5259.974 5260 265

5260.390

5260.670

5260.778

20

3. 5

1. 5

12

4

|7. 51

3

6

2

28

7

3. 5

3. 8

0. 7

0. 3

2. 3

0. 8

1. 4

0. 6

1. 1

0. 4

5. 3

1. 3

0. 7

u,d

s

0

u

s

s,N

s

Co I Fe I p

Sc I

Fe I p

Ni I

Pr II Til

Cai

Mn I

3. 97

3. 57

2. 51

4. 37

3. 74

0. 63

2. 74

2. 52

3. 13

188 788

23

1149

35

298

22

32

5265.723m

52G5.964m

5266.078

5266.309

5266.472

5266.563m

5267.034

5267.104

5267.275

5267.492

5267.655

93

55

9. 5

12

1

252

5

4

25

2. 5

8

17. 7

10. 4

1. 8

2. 3

( 2. 0

[ 46.3

0. 9

0. 8

4. 7

0. 5

1. 5

s

s

u

s

uu

Cr I

Ti I Cr I? Co I

Ti I? p

|Co I

Fe I

Fe I p

0. 97

1. 89

3. 43

3. 69

0. 83

2. 04

3. 00

4. 37

18

156

205

172

36

83

383

1146

223
The Solar Spectrum—Continued

Wavelength.

\A)

Equivalent Width

AX

( -r^ \ \

Re- duced

Width

AX/X

\r

)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BancNotes

5267.80 a

to 5268.10 a

! e

1

1. 1

5268 186r 13 51 0. 7

5268.342 37 7. 3 11 Ni I 4. 54 273

5268.495 9 1. 8 11 Co I 3. 73 172

5268.614 28 5. 6 u Fe r Ti n 2. 60 103

5268.803 3 0. 6

5268.961 10 2. 1 u

5269.418

1

( 7.4 5269.550m \ 478 I 87. 0 S Fe I 0. 86 15

5269.701 [ 7.4

5269.905 6. 5 1. 6 s? Til 1. 87 156

5270.064 7. 5 1. 7 u? Fe I p 3. 63 877

5270.269

5270.383 1 255

1 30. 0

I 35. 0

s

u

Cai

Fe I

2. 52

1. 61

22

37

5271.054 31 5. 9 u

5271.291 21 4. 0 u

5271.618 5. 6 1. 0 s Ti 1?

5271.844 1 0. 2 Fe I

5272.003 21 4. 0 s Cri 3. 45 225

5272.265 14 2. 6 u

5272.400 9. 5 1. 8 0 Fe II 5. 95 185 5273.170m 103 19. 5 s Fe I 3. 29 553

5273.389S 104 19. 8 u Fe I 2. 48 114

5273.43 m s Cri 3. 45 201 13

5273.602 2 0. 4 Fe I p 4. 31 1147

5273.755 1. 5 0. 3 5274236 6. 5 1. 2 w Cen 1. 04 15

5274.403 2 0. 4

5274.534 9 1. 7 u

5274.787 4. 5 0. 9 s

5274.979 48 9. 1 w,N |Cr II Fe I

4. 07

4. 07

43

1029

5275.107 8 1. 6

5275.170 39 7. 4 s Cr I (Cri)

2. 89

3. 37 94192

5275.284m 62 11. 8 s Fe I p 3. 55 742

6275.473 3 0. 6

Wavelength

\A)

Equivalent Width

AX

Re- duced

Width

AX/X

Spot

Solar

Identification

Low

E P

or Rot. Lino

RMl

No.

or Vib. BancNotes

5275.594 2. 5 0. f Vii 3. 76 195 5275.759m 73 13. S s Cri 2. 89 94

5276.002

1

f 21. 4 w Fe II 3. 20 49

5276.071 > 152 < 8. 4 ul Cri 2. 89 94

^97Pt/ U. 11 74/ 1 1 CnK^U T1

1 on

5276.441 3 0. 6

6276.878 1. 5 0. 3 Nd II 0. 86 81

6277.308 7. 5 1. 4 u Fe 1 p

/3. 27

14! 41 584 1149

5277.42 m 2 0. 4 s Zn 0. 64 27

5277.572 2 0. 4 Fe I 3. 96 983

5277.812 4 0. 8

5278.10 a 4 0. 8

5278.254 |8| 1. 5 s Cri 4. 47 309

6278.577 2 0. 4

6278.787 9 1. 7 u

5278.961 6. 5 1. 2 0 S I 6. 86 4

5279.179 3 0. 6 6279 31

5

4 0. 8

5279.671 6. 5 1. 0 s Fe I p 3. 30 584

5279 877 18 3. 4 w Cr II 4. 07 43 6280 072 16 3. 0 w2 Fe I —

Cr II 4. 07 43

5280.284

5280.369 1 60 1

[ 8. 8

su

Cri

Fe I

3. 37

3. 64

192

880

5280.633 20 3. 8 u Co I 3. 63 172

6280.928 1. 5 0. 3 Fe I p 2. 61 210

6281.163 4 0. 8 ul Fe I p 4. 58 1240 17

5281.321 11 2. 1 u

5281.511 3. 5 0. 7

5281.666 5281.798m 1 164 1

[ 30. 1 s

Ni I Fe I

4. 10

3. 04

231

383

5282.170 4 0. 8 5282.402m 22 IS s Ti I 1. 06 74

5283.163 14. 61 0. 9

5283.443 6283.629m 1 212

3. 0

39. 6

S

s

Ti I Fe I1. 88

3. 24

156

553

6283.917 7 1. 3 6284.112m 67 12. 7 w Fe II 2. 89 41

224
The vSolar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Widtii Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(I) (V) Line Band (A) Line Band

5284.280 3 0. 6 Fe I p 3. 63 875 5294.122 5 0. 9

5284.428 23 4. 4 S Fe I 3. 63 842 5294.31 m s 13,16

||Ti I 1. 05 74

5294.399 1 0. 2 5284.615 21 4 0 s Fe I p 4 19 1032

5294.553 13 2. 4 s Fe I 3. 64 875

5284.772 1 0. 2 5295.070 1 0. 2 5285.130 25 4. 7 u,d Fe I p 4 43 1166

5295.321 27 5. 1 u Fe I 4 41 1146

5285.262 3 0. 6 Ca II 7. 50 14 5295.608 2 0. 4 s? 5285.386 2 0. 4 Cr I? 4 18 285

5295.784 10 1. 9 s Ti I 1. 07 74

5285.649 4 0. 8 s Cr I 3. 37 192 5296.075 4 0. 8 5286.07 m 1 0. 2 s,N 16 5296.483 2. 5 0. 5 5286.241 2. 5 0. 5 5296.702m 95 17. 7 S Cr I 0. 98 18 5287.183 9. 5 1. 8 s Cri 3. 44 225

5297.02 a 6 1. 1 5287.569 3. 5 0. 7 Co I 3. 63 175 5297.233 18 3. 4 s Ti I 1. 87 156

5287.788 6 1. 1 Co I 4 05 187 5297.385m 87 16. 4 s Cr I 2. 90 94

5288.218 2 0. 4 Fe I p 3. 60 818

5298.023m 83 15. 7 s Cr I 2. 90 94

5288.375 2 0. 4 Fe I p 2. 99 406 5298.283m 110 20. 8 s Cr I 0. 98 18 5288.40 m s 13 5298.415 ] \ 0. 6 s |Ti I 2. 50 281 5288.533S 56 10. 3 s? Fe I 3. 69 929 65 Cr ip 2. 90 5298.497m J [ 11. 9 s

5288.804 3 0. 6 s Ti I? 5298.784m [ 8. 3 s Fe I 3. 64 875

5288.99 m 1. 5 0. 3 s,N 46

5298. 832r J I 0. 4 5289.282 2 0. 4 s Ti I 0. 84 36 Cn 3. 37 192 5299.643 0. 5 0. 1

5289.510 3 0. 6 5299.984 21 4. 0 s Ti I 1. 05 74

5289.820 2. 5 0. 5 Yii 1. 03 20 5300.408 5 0. 9 Fe I 4. 59 1240

5290.817 |5| 0. 9 u1 Fe I p — 4 32 1147 17 5300.562 2 0. 4 C I 8. 64 La II? 0. 00 6 5300. 751S 56 11. 3 s Cr I 0. 98 18 5291.60 m s 13,16 5300.919 2 0. 4 5291.650 1 0. 2 5301.047 21 4. 0 s Co I 1. 71 39 5292.216 4 0. 8 5301.312 3 0. 6 u,N? Fe I p 4 39 1162

5292.399 2. 5 0. 5 5301.490 0 0. 4 5292.590 36 6. 6 u Fe I 5301.874 9. 5 1. 8 s 5292.81 m 2. 5 0. 5 s 5302.054 3. 5 0. 7 5292.873 4 0. 8 s Cn 3. 45 205

Mn I 3. 38 36 5302.307m 157 SO. 0 s Fe I 3. 28 553 5293.042 12 2. 3 u Fe I p 4. 39 1165 5302.563 9 1. 7

5293.169 10 1. 9 u Nd II 0. 82 75 5302.657 6 1. 1

5293.375 4. 5 0. 8 s,d Cn 3. 37 192 5302.953 3 0. 6 Mn I 5. 40

5293.64 m 1. 5 0. 3 s 5303.223 4 0. 8 V 11 2. 27 54

5293.773 1 0. 2 8 5303.415 1. 5 0. 3

5293.963 29 5. 5 U Fei 4 14 1031 5303.567 2. 5 0. 6

225
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar EP No. Wave- valent duced Solar EP No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib AX AX/X fication Rot. Vib.

(A) (mA) (F) Line Band (A) (ml) (F) Line Band

6303.845 7 1. 3 0? Fe I? 5314.272 1 0. 2 5304.00?m 1. 5 0. 3 s 5314.57 m 1 0. 2 s,N

5304.185 14 2. 6 s Cr I 3. 46 225 5314.741 2. 5 0. 5 u

5304.566 2 0. 4 5314.927 8 1. 5 u

6304.992 2 0. 4 5315.077m 34 6. 4 u Fei 4. 37 1147

5305.430 2 0. 4 Fe I 3. 63 877 5315.784 151 0. 9 u Fe I p 3. 64 877

OoUO.oOU 9'^ 4. 7 %0 Cr TT 0. 00 24 00 X U.^ X u 0|

9~^ 00 X U. 0 c7 i A <^ *±. 0 w. 0

cqric AQA 11 n 9 s 00CQ1X AVJ. A9nm U^WXLL 1X

1X'^9 91^X. 1X w P tJ 11 ^ 1 Pi 0. X 0 40T:y

ooUD.oy a

1± n 9 •i^l R 79Qr 0. 0 U I

I

[ Q7y < Oouo.yuu u. 0 n 1 i^^l fi 7S0 ] [. 1xo.^ nu H) Fe II 3. 22 4S (On yy^o 1)A A 09 1 09 OoU < .^oX 7( i. 0 Pav^a TTix 1

4

Xt: 00 X / .u / 0 0. 0 0 7 s Ivin I 0. 00 ou^fi cqr»7 9C1 a 2 fl 4 Prv>X TX 0. / u 007

Cqi 7 9A ryi 00 X i .^U XIX 1X. 0 u. 0 s 1 ft

J. u OOU / .ooyo ou lU . u 0 J; t; X X. ux ou

OOX ^i^l 7 f;2fi

J -O^w 5

1X. X1 1 "Rp X C XT n|J Ar±, \AXrt 1 0*^9

u. 0 u. ± TTc X; c T?1 i u

ciqiy ci7n tJO J. 1 .tJ 1 W 5 0. 9 } cqnQ 4.90 9St 0. 0 w Pr IT V>1 XX 4 07 4*^ ^0

KOI 7 m u. 0 nU. 1X xu DoUo.Dyi 7 K 1 4 u x e X 4 9fi 1xuynoiX KOI 7 QQ rn 0 AT 1 ^ 1 fi OoUo.oyo 0. 0 1. u

X. 0 \j. 0 Fe 1 0. 406

oouy.iou -11 n 9

coi 0 qci 1x^9 9 9 w RnOL- TTXX 1 ^fi X. 00 99

cQfiQ A.r,7 OoUy.^0 < 11 n 9 PrwX TX

4-^. 1XoS ^00

n 1 s — V ii?p 2. 27

coin 949 0q n A Pn T? 4 91 xyo

(JO J. 0. 1 < u x^ 2. 6 s Cr I 225

0£)lU.'±Oi c0 u. y ooiy.Ut:0 7 f^

< . 0 1X. 4 u

txsiu.oy /

1 A 9 A 0 Pr TT i.>r XI 4 07 A'i 40 oo±y KOI Q 91 J. .iii'i A u. 0

TTo T in J. t; 1 ^

4 07 1 09Q

CO -1-1 TOO Soil. loo n c n 1 u. 1 KOI Q 01

Q

0. 0 X.1 nu

K0 1 1 on T-^ s

1io, 1IDA

KOI Q 70 Q 9 n 4

CO 1 -1 /I Q rv^ s 7r T /jr I 0 1^9 97 Xo1 KOI Q OOA 1

1

X X 9^. 1X s NH TT 0 fi^ 7fi

< 0 CO 1 1 /i "TA Oc5i 1.4/0 9 c n c

u. 0 i> u Ix u. yy oU

p;'^90 040 1

8

xo 0. 4T s FaX' 0 1i ^ fi4 S77 oil

CO 11 AO

1

t)Oil.Dol Q0 n A u xll II 1 7Q X. /O Q7

00-"U.t:O KOOn 40 ^111 X. 0 \j. 0 s X1 fi\j CQ 1 1 '7Q0 OOll./oZ 00 n A ZiX II; — 1 7A QCyo coon QQl c0 u. y YX 11TT — 1X. 08uo 90

CQ 1 o 1 n n ooiz.iy a

9 C n c u. 0 KO91 1 1 Am 4^^0 7 0 s "Rp J c T1 4rt. A'i 'XO 1 165

CQ no /^C\A n c

u. 0 n 1 u. 1 Oo^i.^y 111 i. 0 u. 0

CO 1 O A C A 7 c 1. 4 w K^O I A 91 4. Zl 1 07 ly < KOO-I 7Kn q n fi CO 1 O Q AO OOI2.SDO ly 0. 0 s t^r I Q /I C

0. 40 99K

00^1. Ot: 111 9 C 0. 5 s CO 1 0 HTO oolo.u/y A c 4. 0 U. 0 s 5322.049S 60 11. 1 s Fe I 2. 28 112 5313.244m 3 0. 6 s Ti I 1. 07 74

5322.819 2 0. 4 Pr II 0. 48 35

5313.411 1. 5 0. 3 Fe I p 4. 58 1239

5323.507 1 0. 2 Fe I 2. 28 113 5313.585m 35 6. 6 u Cr n- 4. 07 43

5323.789 0. 5 0. 1 5313.755 2 0. 4 Ti II? p 1. 57 81

226
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

A\

(mA)

Re- duced

Width

AX/\

(F)

Spot

Doiar

Identification

Low

ill tr or Rot. Line

RMT

IN 0. or Vib. Band

Notes w avclength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

A\/X

(F)

Spot

Solar

Identification

Low

111 Jr or Rot. Line

RMT

i\ 0. or

Vib. Band

Notea

53io.9o m oo 11 I A OO O £• 1 olo c o o o 'Tiin 0000.709 o c

^. 5 A C0. 5 s re I p — O AO o. UZ A C A 4o4

COO ,H r»r\T 5324.097 5324.191m

334

1[ 59. 5 s

Ur I ! Fe I3. 37

3. 21 553

ooo4.1o m

5334.222

1

3. 5

A O

0. z

0. 7

8, IN

Sc II 1. .50 30

5324.705 1. 5 0. 3 Dy II? 5334.330 2 0. 4 Fe I p 4. 10 1064

6325.280 8 1. 5 w? Co I 4. 02 192 16 5334.44 m 0. 5 0. 1 8

5325.388 5325.560m

5325.959

5326.149m

0. 5

45

3

32

0. 1

8. 4

0. 6

6. 0

w

u

s

Fe II Co I

Fe I

3. 22

4. 21

/3. 02

Lo. 5/

49

194

407

too

5334.870m

0Oo4.yDD

coo C All oooo.uy m

coo t O/l »^

32

o c o. 5

1

6. 0

A *?

(). 7 A O

U. 2

W

S

3

Cr n

(Co IJ

4. 07

/I no 4. U-i 43

1 A

191

1 o lo

5o/o.,i.54 U. 4

CO O C Ofl oooo.oo m « AT S,l\ T; T? 11 II 1 o lo

0Oii0.4i m s

1 0 1 coo C /I 0 OOO0.4O m S,iV 1 olo

C OO C '"AC

1. 5 U. cJ c o o c c1. 5 A O

0. 0

roo/? QOo

1 1 2. 1 U,l\ r e I A /II 1 1 ^ 114/ COOA A7 1 A O o<J

C 00'7 O/?

O

00^7. 2uo 6. 5 A '7 0. 7 u r e I p

Q A/I OT C OlO COO 1 A OOOD.loy 4A ^7 U. 7 K^O I 4. U-i 1 A 1 191 cooo ri ^ 1 oo^JS.uolm O T C TA /I /U. 4

ao rex u, yi 15 CO O A O A C A ,1 u. 4

oo^s.do/sm 74 1 A C 19. 5 S KjV I A/f 94 0OOO.4/0 o c A CU. 0 5 5328.542m 210 39. 4 s Fe 1 1. 56 37 5336.591 2. 5 0. 5

5328.925 2 0. 4 5336.794m 71 12. 9 Ti II 1. 58 69

oo-sy.l47in lo. 4 s v^r I o m 94 CO 07 1 11 A O

s

coorv /I r\ ^ 00.^9.40 a

to oozy.Do a

coon /I 5£)Z9.794

1

1

31

0. 9

c o

5. a s I o m 0/1

C O O '7 O OO ooo/.osZ

C007 '70'7». boot .1 / /r

C O O"? 'TG

ooo/.7dU

oJ,

1 35

J

A /I U. 4

f C /I 0. 4

1 o

I 1. b

1

\ w,d

J

r reT?/i TTII

L Or II

O OO o. Z6

A A'7

4. 07

4a

A O 4o

0O/9.99D m DU 1 1. z u 1' e I 4. U/ COO"? A7A ooo/.y/y 1 c1. 0

n o U. o

5330.44 a 1 0. 2 5338.333 13 2. 4 s Ti I 0. 83 35 15

5ooU.5d4 OO U. b s 11

U. O/ 1 o

liS 1 T COOQ C/i/i 0ooa.o44 oO A s

1 'T 17

coo 1 1 r\r» 1 A O (J. r e 1 p O OO Q 1 '7 81 / coo Q '7yf O oooa.74o oo U. D coo 1 /IOC

5oi}1.4a0 15

J

U. o

1 O 1 I ^.1 \s,N

J

L/O I

L re I p

1 TC 1. /o OQ

O 1 A

KOOO 0*7/1 Oooo.y /4

CO OA O 1 T oooy.zl7

o

oO

A A

U. 4

AU. D Ua n 8. 44 OAZD

C001 fTca 1 A O CO OA O C oooy.oo m oJi A /I U. 4

C AT

5331.98 m s 13 5339.426 9 1. 7 0? Fe I p 4. 43 1162

5332.14 m s 13 5339.535 3. 5 0. 7 Co I 4. 23 199

5332.363 6 1. 1 5339.65 m 2 0. 4 s,iV 5332.665m

6332.908S

5333.148

5333.253

5333.656

45

96

4. 5

8. 5

7

8. 4

0. 8

1. 6

1. 3

s

0

V II Fe I Fe I Fe I p

Co 1

2. 27

4. 19

1. 56

4. 07

4. 02

54

1031

36

1023

190

5339.696 5339.82?m

5339.937m

5340.193

5340.454

1

161

12

16

0. 2

29. 1

2. 4

3. 0

s

3UU

S

K I

Fe I

Cr I

1. 62

3. 26

3. 44

553

225

13

227

761-0;125—66 17
The Solar Spectrum—Continued

Equi- Re- Low RMT 1 Equi- Re- Low RMT

V fXlCii u U. Ut^tiU. Solar E P No. vs-lent r\ 1

1

0(^r\ Solar IN U. length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes

A \ ZA A A^ /\ lAA/ a fi pn ti np Rot. Vib. AX AX/X rvo L

.

V lU. (A) (ml) (F) Line Ban (A) (ml) (F) Line Band

1. 0 Ti I 0. 82 36 'i'?48 '^26S 92 17. 8 Cr I 1 on 1

8

uo -t V. 1 ox Q 0. 6 'i34S 760 5. 5 1. 0 16 5341.033m f 25. 5 IIFei Mn I

1. 61

2. 11 374 5349.098 5 0. 9 u Co I 4. 15

> 180 (Sc I) 1. 94 19 5349.292 2 0. 4 s Sci 1. 85 17

5341.151 1 I 10. 2 s? 5349.469m 91 17. 0 s Ca I 2. 71 33

5341.328 12 2. 2 u Co I 4. 14 199 5349.745m 49 9. 2 s IIFei; Sci

4. 39

0. 02 1163

4

4 0. 7 Ti I 4. 33 316

5349.872 16 3. 0 Mm 5. 37

X 0. 2 5350.093 6 1. 1 0 Zr II 1. 83 115

'i342 228 1 0. 2 Fe I?

18 5350.363 6 1. 1 Zr II 1. 77 115 5342.504 0. 5 0. 1 Vii 2. 26 54 5342.708m 29 5. 4 w? Co I 4. 02 190 5350.454 1 0. 2 Fe I?

5342. 88?m 1 0. 2 s 5350.55 a 0. 5 0. 1 5342.962 1 0. 2 S |Sc 1 0. 00 4 5350.789 3. 5 0. 7 Fe I K 1 1. 61 5350.919 2 0. 4 5343.125 1. 5 0. 3

0. 3 5351.071 9. 5 1. 8 s Ti I 2. 78 300

5343.225 1. 5

I

1 Co I 4. 02 190

5351.662 1 0. 2 Cr I? 5343.392

1 a. 5343.438

\ 65 > w

1 Fe I 5351.838 2 0. 4 Ni I p 3. 94 177

J i 8. 7 J

5343.66 m 0. 4 s,N

5352.049m 21 3. 9 u Co I 3. 58 172

2

5343.874 0. 6 5352.232 1. 5 0. 3 3 5344.16?m 0. 4 s,N Nb I? 0. 35

5352.405 1 0. 2 Vt II? 0. 48

2

5344.25 a 0. 5 0. 1 5352.800 2 0. 4

5344.458 11 2. 0 w Mn I 5. 38 5352.995 2 0. 4

5344.583 2. 5 0. 5 Co I 4. 02 191 5353.167 2. 5 0. 5

5344.763 8. 5 1. 6 s Cr I 3. 45 225 5353.383m 75 14. 0 s |Fei

"NT." 1 INl I

4. 10

i. y5j. 1062

5345.037 1. 5 0. 3 5353.515 30 5. 6 u Co I 4. 14 lyo 5345.543 8. 5 1. 6 Cr I p 3. 46 225

5353.670 2 0. "3 5345.807m 107 £1. 0 S Cr 1 1. 00 18 5353.920 3 0. 6 5346.082 15 2. 8 0 Cr II p 3. 83 24

5354.68 m s 13 5346.336 3 0. 6 Fe I p 3. 60 817

5354.727 1 0. 2 5346.545 20 3. 7 u,d Cr II- 3. 76 23 16 5354.900 0. 5 0. ] 1 TTo TT |r e II o.

5o4o.8l5 D 1. I s 5355.625 1 0. 2

5346.970 2. 6 0. 5 5355.731 4 0. 7 s,N Sci 1. 95 19

5347.09.^ 1. 5 U. o s 5356.084 2 0. 4 S Sci 1. 86 17

5347.514 3. 5 0. 7 Co I — 4. 15 196 OOOD.^O K*i C^fi A'i m111 13

5347.717 4. 6 0. 8 w Ni I 3. 80 145 5356.60 m s 13

5347.89 m 0. 5 0. 1 s 5356.991 2 0. 4 Nd II? 1. 26 80

6348.070 4. 5 0. 8 s Mn I 3. 38 36 5357.190 4 0. 7 Sen I. 51 30

228
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Refhjc(!d Width

AX/X

(F)

1

Spot

Solar

Identification

1 Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5358.120 8 1. 5 s Fe I p 3. 30 628 5368.546 5 0. 9 8 Cr I 3. 85 258

5358.287 HI 0. 2 5368.850 1 0. 2

5358.478 0. 5 0. 1 5368.920 1. 5 0. 3 Co I 3. 53 1G7

5358.665 1 0. 2 5369.220 1. 5 0. 3

5358.940 4. 5 0. 8 Co 1? 4. 14 5369.360 6 1. 1 Cr n 3. 87 29

5359.05 m s 13 5369.596m 40 7. 8 s Co I 1. 74 39

5359.203 9. 5 1. 8 wl Co I 4. 15 194 5369.974m 182 33. 9 u Fe I 4. 37 1146

5359.528 2 0. 4 K I 1. 62 5370.330 14 2. 6 u -Cr I

5359.718

5360.144

5360.467

5360.710

5360.928

5361.372

5361.507 5361.629m

5361.71 m

5361.818

5362. 176r

5362.57 m

5362.760

3. 6

1. 5

2

0. 6

2

3

9

36

3

|1.51

|1.5|

1 110

0. 7

0. 3

0. 4

0. 1

0. 4

0. 6

1. 7

6. 7

0. 6

0. 3

0. 3

J

.a

s,N

u

s

s

s

Cr I?

Nd II- Fe I

Ti I

Zr I

|Fe I —

Co I

0. 68

4. 41

0. 84

0. 54

4. 23

74

1143

35

27

198

13

5371.339m

5371.501m

5371.927

5373.58 a 5373.714m

5373.950

5374.158

5374.413

5374.767

5374.887

5375.180

5375.323

5375.875

1 294

9

1. 5

59

3

2. 5

|2|

1

1

2

2. 5

2. 5

[ 11. 6

1 44. 1

1. 8

0. 3

10. 6

0. 6

0. 5

0. 4

0. 2

0. 2

0. 4

0. 5

0. 5

us

s

s

Ni I Fe I (Fe I p)

Nd n

Fe I

Fe I p

So I Cr I

4. 42

0. 96

4. 43

1. 41

4 47

3. 57

1. 97

15 1163

79

1166

785

19

5362.867 [ 14. 1 w Fe II 3. 20 48 5375.978 3 0. 6

5364.166 3 0. 6 5376.132 3 0. 6 Cn

5364.426 4. 5 0. 8 5376.30 a 2 0. 4 5364.880m 133 24- 6 u Fe I 4. 44 1146 5376.464 2. 5 0. 5

5365.224 8 1. 5 5376.60 m 0. 5 0. 1 s Ti I 0. 00 3

5365.407S 78 H. 7 u Fe I 3. 67 786 5376.673 0. 5 0. 1 s? 16

5366.417 6 1. 1 s,d? 5376.836 13 2. 4 s Fe I 4 29 1132

5366.645 2. 5 0. 7 S Ti I 0. 82 35 5377.064 4 0. 7 u La II 2. 30 95

5366.759 4. 5 0. 8 5377.193 2. 5 0. 5 u

5366.85 a

to 5367.13 a I ' 1. 5 5377.310

5377.35 m

1 0. 2 s,N 13 5367.476m 157 29. 1 u Fe I 4. 41 1146 5377.408 0. 5 0. 1

5367.772 2 0. 4 5377.614m 45 8. 4 s Mn I 3. 84 42

5367.94 a 1. 5 0. 3 5377.793 8. 5 1. 6 s,N 16

5368.296 5. 5 1. 0 5377.928 3 0. 6

5368.438 5 0. 9 5378.223 6 1. 1 u

229
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

valent SoIep E P No. valent Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(1) (mA) (F) Line Band (1) (ml) (F) Line Band

5379.144 1 0. 2 5387.70 a

to

1 * 0. 7 5379.325 0. 5 0. 1 5388.00 a J

5379.581S 56 10. 4 s Fe 1 3. 69 928 5388.351 12 2. 2 s Ni I 1. 93 70

537Q 950 0. 5 0. 1 5388.504 5 0. 9 u,N Mn I 3. 37 36

5380.322 26 4. 8 ?,A/' C I 7. 68 11 5388.675 1 0. 2

53S0 737 12 2. 2 5388.796 0. 5 0. 1 5381.028m 56 10. 4 w II|j TiJ. 1 IIX* 1. 57 69 5389.169 5 1. 1 s Ti I 0. 81 35 Fe I? 5389.486S 90 16. 7 s Fe I 4. 41 1145

5381 172 3 0. 6 5389.678 3 0. 6 5381.318 1. 5 0. 3 5389.847 12 2. 2 w

5381.772 5. 5 1. 0 s,N Co I — 4. 24 196 5390.007m 7. 5 1. 4 s Ti I 1. 87 155 5382.033 1. 5 0. 3 5390.377 12 2. 2 Cr I 3. 37 191 5382.277 23 4. 3 s? 5390.527 30 5. 6 u

5382.484 2 0. 4 5390.777 5 0. 9 5382.649 2 0. 4 5391.070 1 0. 2 Ti I p 1. 88 155 5382.755 1 0. 2 Fe I 3. 55 741 5391.35 m 3 0. 6 Cr I 3. 37 191 5382.92 m s Ti I p 1. 87 155 13 5391.465m 76 14. 1 S Fe I 4. 15 1062

5383.015 1. 5 0. 3 5391.623 37 6. 9 Fe I 5383 07 a 1 0. 2 5391 796 3 0. 6 Fe I p 2. 69 270

5383 3S0m 204 36. 0 Fe 1 4. 31 1146

5392.014 7 1. 3

"1 5383 7fifi 2 0. 4 5392.06 m J Sc I 1. 99 19 13 4 0. 7 5392.330 14 2. 6 u,N Ni I 4. 15 250

(JO O • ^V/ <J 1X. o 0. 3 Fe I p 3. 65 817

5392.50 a 1 2 0. 4 Ti I 0. 83 35 to 12 2. 2 5392.95 a J 5384.873 2. 5 0. 5 V II 2. 27 53 5393.176m 153 27. 2 s Fe I 3. 24 553 5385.128 1. 5 0. 3 S Zr I 0. 52 26

5393.381 12 2. 2 Ce II 1. 10 24

5385.305 1 0. 2 Cr I? 3. 84

5393.67 m 2. 5 0. 5 Atm?

5385.587 5. 5 1. 0 u Fe I p 3. 69 927 O

1. 0 U. t_ 2 0. 4

5386.102 1. 5 0. 3 5394.200 0. 5 0. 1 Atm?

OOoO.OTiUlIl 1=; fi o. u s X t; 1 4. 15 1064 5394 351 2 0. 4

5386.556 1

i. 0. 2 5394.641 f 7 3

"1 74 Mn I 0. 00 1 tJOoU. / U 1 2 0. 4 5394.706 1 7. 3 1

5386.971 91 o. y 3. 64 875 5395 Oil 1. 5 0. 3 Cr I 3. 37 191 5395.222 20 3. 7 s Fe I 4. 44 1143 5387.126 2 0. 4 Fe II 5395.470 3. 5 0. 6 6387.283 1 0. 2 5396.001 4. 5 0. 8 5387.484 f 2. 9 s -Fe 1 4. 14 1031

1 25 5396.247 12 2. 2 5387.565 I 1.8 s Cr I 3. 37 191

230
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5396.578

5396.734

5396.904 5397.141m

7. 6

3

2. 5

239

1. 4

0. 6

0. 5

^jf. 7

S,N

S

Ti I

Fe I p

Fe I (Til)

fO. GO

10. 02

3. 02

0. 91

1. 88

3

3

4C4

15 155

5405.785m

5406.183

5406.337

6406.480

5406.603

266

1

9

2

0. 5

46. 8

0. 2

1. 7

0. 4

0. 1

S

u

Fe 1

Fe I p

0. 99

4. 07

15

1020

5397.623m 24 4. 4 s Fe I 3. 63 841 5406.779m 37 6. 8 s Fe I 4. 37 1148

5397.930 4 0. 7 5406.93 a 2. 5 0. 6

5398.287S 76 14. 1 s Fe I 4. 44 1145 5407.112 3 0. 6

5398.519

5398.859

4. 5

3. 5

0. 8

0. 6 s

Atm?

16

5407.384

6407.482 1 67

\ 6. 3

I 6. 3

1 s,d Mn I 2. 14 4

5399.479 39 7. 2 s,d? Mn I 3. 85 42 15 5407.617 21 3. 9 w Cr 11 3. 83 23

5399.777 5 0. 9 Co I? 4. 21 5407.825 2. 5 0. 5 5400.263 2 0. 4 5408.088 3 0. 6 Co I? 2. 28 112

54C0.423r

]

f 0. 4 5408.205 3. 5 0. 6 5400.511m i 143 < 21.

Fe I 4. 37 1145 5408.367 1 0. 2 5400.629 J [ 7. 6 s Cr I 3. 37 191 5408.823 5. 5 1. 0 Fe II 5. 95 184

5400.855 2 0. 4 5408.932 3. 5 0. 6 s Ti I 0. 00 3 16 5401.271 24 4. 4 u Fe I 4. 32 1146 5409.139m 57 10. 5 s Fe I 4. 37 1147

5401.39 m 3. 5 0. 6 s Ti I 0. 82 35 5409.428 3 0. 6 5401.701 6. 5 1. 2 s,N 16 5409.501 3. 5 0. 6

5401.92 m

5401.949

5402.072

5402.320

5402.600

5402.783

5403.07 a

5403.468 5403.829m

5403.98 m

5404.145m

4. 5

16

1. 5

1

12

1

2

60

239

0. 8

3. 0

0. 3

0. 2

2. 2

0. 2

0. 4

11. 8

44. 2

s

u

w

s

s?

s

Vi

Y II

Fe I

Ti I Fe IFe I

(2. 36

12. 68

1. 84

4. 07

2. 33

4. 31

4. 43

130

139

35

1029

259

1145

1165

}>3

13

5409.609m

6409.799S

5410.054

5410.428 5410.918m

5411.223m

5411.395

5411.558

6411.725

5412.007

5412.184

5412.574

8. 5

154

1. 5

8. 5

169

30

4

1. 5

1

3

3. 6

2

1. 7

27. 0

0. 3

1. 6

29. 0

5. 9

0. 7

0. 3

0. 2

0. 6

0. 6

0. 4

sS

s

s

u

Ti I Cr I

Si 1?

Fe I Ni I Fe I p

Fe I p

1. 89

1. 03

5. 61

4. 47

4. 09

3. 64

4. 58

155

18

1166

222

870

1237

5404.550 9 1. 7 u 5412.791 19 3. 5 s Fe I p 4. 43 1162

5404.677

5404.842

5404.993

5405.136 5405.358m

12

2

10

5

43

2. 2

0. 4

1. 9

0. 9

8. 0

u

s

s

Cri

Fe I p

3. 37

4. 39

191

1162

5413.101

5413.17 a

to 5413.50 a

5413.684

18

} ^

24

3. 3

0. 9

4. 4

w

s,N

lo

Atm

Mn I 3. 86 42

231
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar EP No. Wave- valent duced Solar EP No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(A) (mA) (F) Line Baud (A) (mA) (F) Line Band

o4io.yio 0 ^U. 0 04:^0 .i7D± s

5414. U/ 0 iSl 5. / w Fe II 0. zz 48A Q 04Z4.UoUni i 9^0 \ 4Z. S s rex 4.A Q9oZ 1 1 /I ft 1 14D

o414.^4-^

11 \ U. 4

l^G. re T? r^ I : pfl A7 4. U/ 1lUZD n9ft

5414. 00/ 0 0 S,l\ 1 A +TV1 TT n XV 0

/1 1 1 41 .1 ZD KAOA KAA O4Z4.044: 1lUn 1 8 1. 0 u "Ml* T 44. 171 / OQ1 Zol

r\ 9 KAOA P,KArr\ 4.9 ^z 7 7 s IN 1 1

1 Of; 1. yo 7n

eA "i A QQ1 5414, ool c0 _

r e I p 0. 04 874. 8/4

KAOA Q7Q 04/4.0/ 0 0 7 54l0.^iUo 0/. 0 s r e I 4. oy 1 IDO 04zo.zoyiu AS48 8 8 8. 8

AT WjISi T?13 TT r e II 0. zu 40

0410.1)00 00 u. 0 04ZO.OZ / 191 U. Q AT Pn T V_yO 1 4 07 1lyoOR

SAt a OQ A 54lD.oo4 11 u. ^

TVTrl TT XN u II U. 00 8U

KAoa OKQjy^ 0'±ZD .ZOoili i. 1 1 n ri9 u. uz Q0 541 /.U4Z 0 / 0. 0 s r e I 4. 41 11

1148AC

04ZO. 00 a 1 541/. oU a Z. 0 U. 0 5

PiJ.97 OA Q Ot:Z / .UD ti J 5417.929 2. 5 0. 5 5427.224 1 0. 2 5418.156 |8| 1. 5 5427.803 5. 5 1. 0 0 Fe n

5418.288 3. 5 0. 6 5427.997 1 0. 2 Cr I? 3. 85 5418.775m 49 5. 7 s (Ti II) 1. 58 69 5428.327 4 0. 7

5419.109 2. 5 0. 5 5428.616 3 0. 6

5419.217r 3. 5 0. 6 s,NN Ti I? 2. 34 258 5428.707 6 1. 1 Fe I p 4. 19 1032

5419. dao 0

A A u. y Atm A XT f\ £12'-' T>K 0z/111 411 Ofi ZD r /I 00 Q KA 0. 0 1. u i>i 1 1

1101fii

5419.703 1. 5 0. 3 5428.981 2 0. 4

o4iy.yuo 9 U. 4 o4zy.ioum lu 1. 0 t; t Z. Orr 9fi0 zoy

5420.318 5429.432r f 0. 8 Fe I p 4. 14 1029

78

{

Mn I 2. 14 4 5420.412 1 i 7. 6 1 5429.511m 1 10. 2 u,N Fe I p 4. 19 1062

5420.622 7 1. 3 Atm H2O R 1 411 26 5429.706m f 48. 0 S Fe 1 0. 96 15

/• Z80

ZU 0. / S.' Or II 0. /D Z6 1 / c A OQ Q KA oizy .o04 J A P,

[_ 4. 0 U r e I p

4 47 1 1 fi9 1 IDZ

F /|0-i -1 fyo 44 Q 1 ^, AT Si I- 0. DZ 04oU.oD4 Q8 1. 0 U) Ni I 0. 00

54zl .4Uo 1 1 0

1. 0 Fe I p d. D4 0/4 54ol.UDZ 11 n 9 u. z

54iil.o77 0 K

Z. 0 A K

U. 0 IN Cl II

.' A ^ A U. /4 *7A

/ y 04ol .ool 9 ^

z. 0 n f; u. 0 re i; 54ol.541r /i 4. 0 A Q U. 8 IN Q 11 11. 19IZ 6421.843 14 0 c

2. b s,a Fe I p 4. 00 1100 1180

Kyi Q 1 on 54ol.oU a 1 A 0 u. z

C /! 00 ICO A C

y. 5

1 0

1. 0 u re I p

/I QO 4. oz 1 1 /I K 1140

KAQO AAQ V. 0 U. 1 VV TT? 11

1

9 9fi

K/1 00 Kin A A U. 4 o4oZ.oo rm 1I

1

^

r n 9 u. z s Ti I 9Z. 41rxl zuo

54ZZ.0D1 1 A 0

0. 2 L5

54oZ.o54 J 1. 0U. 11 Orwl I1 ^0. 49^Z 904

C /I 00 ACT 5422. yol 6. 5 1. 2

A TT Atm ri2U li 1 All 41

1

ZD

KAQO KAQr.-^ 54oZ.54oni 40 8 F: 0. 0 0 Mn I u. uu 1X 5423.327 1. 5 0. 3 5432.746 1. 5 0. 3 s

4:. 0 u. 0 5432.955S 72 13. 2 5 Fe I- 4. 44 1143

5423.598 1 0. 2 5433.200 6 1. 1 U

5423.752 6. 5 1. 2 s Fe r p 3. 69 927

5433.403 6. 5 1. 2 U -Mn I? 5. 37

5433.644 6. 5 1. 2 U

232
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(D

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5433.938 1. 5 0. 3 5441.947 1. 5 0. 3

5434.045

5434.179 5434.534m

5434.861

5435.039

5435.183

5435.587

5435.704 5435.866m

5436 058

5436.161 5436.302m

5436.447 5436.596m

5436.731

5436.845

5436.990

5437.091

5437.203

5438.051

5438.307

5438.468

5438.716

1

4

184

3

3. 5

8. 5

4

1

46

1

0. 5

36

1

37

3. 5

1

1. 5

8. 5

16

2. 5

4

1

0. 5

0. 2

0. 7

S4. 0

0. 6

0. 6

1. 6

0. 7

0. 2

8. 5

0. 2

0. 1

6. 6

0. 2

6. 8

0. 6

0. 2

0. 3

1. 6

2. 9

0. 5

0. 7

0. 2

0. 1

S

u

s

s

u

s

s

suu

s

Fe I

Fe I p

Ni I

Fe I

Fe I

Ti I 0 I? Co I?

Fe I p Fe I

Ti I

1. 01

4. 43

1. 99

4. 39

2. 28

0. 90

10. 74

4. 11

4. 31

4. 59

1. 43

15

1161

70

1161

113

51

11

1145

1237

108

5442.293

5442.420

5442.768

5442.977

5443.426

5443.619

5443.80 a

5444.089

5444.588

5444.727

5444.85 m

5444.875

5445.053S

5445.341

5445.504

5445.606

5445.776

5445.854

5445.959

5446.061

5446.230

5446.372

5

8. 5

1. 5

2. 5

3. 5

4

0. 5

0. 5

14

3.5

1

3. 5

121

2

2

2

3

2. 5

2

2

3. 5

2

0. 9

1. 6

0. 3

0. 5

0. 6

0. 7

0. 1

0. 1

2. 6

0. 6

0. 6

23. 0

0. 4

0. 4

0. 4

0. 6

0. 5

0. 4

0. 4

0. 6

0. 4

s,N

s

u

u

s

s

s

AtmHjO

Nd II Cr I

Fe I p

Co IFe I

Cr I?

Fe II p

P 1

0. 68

3. 42

4. 10

4. 07

4. 39

3. 34

411

76 204

1059

196

1163

53

16,26

13, 16

5438.925

5439.054

1. 5

2. 5

0. 3

0. 5

5446.591m 74 14. 5 s Ti I Fe I p

JO. 02

\2. 33

4. 41

3 259

1144

5439.303 2 0. 4 V II 2. 27 53 5446.924m 238 ^2. 8 ,s Fe I JO. 99

1(1.61) 1537

5439.475 1 0. 2 5447.248 3 0. 6 Nii?p 3. 84

5439.708r 2 0. 4 Atm 5447.533 2. 5 0. 5 u

5439.920 2 0. 4 Fe I 5447.687. 2 0. 4

5440.503 2 0. 4 s Ti I p 1. 43 107 16 5447.938 1. 5 0. 3 s,N Ti I?

5440.652 3. 5 0. 6 s 16 5448.098 3 0. 6 s

5440.824 1 0. 2 5448.378 16 2. 9 s Fe I

5440.978 1. 5 0. 3 5448.674 1 0. 2

5441.146 2 0. 4 5448.933 2 0. 4 s Til 2. 33 259

5441.347m 28 5. 1 s Fe I 4. 31 1144 5449.159 2 0.4 s Ti I 1. 44 107

5441.528 1. 5 0. 3 Fe I 5449.403 1. 5 0. 3

5441.678 1 0. 2 5449.707 1. 5 0. 3

23;;3
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5450.798 8. 5 1. 6 M 6460.701 2 0. 4

5450.924 4 0. 7 5460.888 7 1. 3 u Fe I 3. 07 464

5451.127 6 1. 1 Nd II 5461.144 1 0. 2

6451.40 a 4 0. 7 5461.393 1 0. 2

5451.957 3. 5 0. 6 s,N Ti I 2. 40 265 5461.659 22 4. 0 s,d Fe I 4. 44 1145 17

5452.101 12 2. 2 u Fe I 3. 64 870 5461.823 2. 5 0. 5 Fe I p 3. 69 817

5452.298 3. 5 0. 6 Co I 3. 81 175 5462 .06 5r 1. 5 0. 3

5452.850 14 2. 6 u Ni I 3. 84 5462.269 1. 5 0. 3

5453.085 3 0. 6 5462.501m 40 7. 3 s Ni I 3. 86 192

5453.236 11 2. 0 u Ni I 4. 09 231 5462.662 3 0. 5

5453.40 m 1 0. 2 s 5462.784 2. 6 0. 6

5453.650 4 0. 7 s Ti I 1. 44 108 5462.970S 93 17. 4 u Fe I 4. 47 1163

5453.857 2. 5 0. 5 5463.114 1. 5 0. 3

5453.996 6. 5 1. 2 u Fe I p 4. 15 1064 5463.289m 118 21. 6 s Fe I 4. 43 1163

5454.128 4. 5 0. 8 5463.481 1. 5 0. 3

6454.364 1 0. 2 s,N 5463.641 2 0. 4

5454.580 13 2. 4 s Co I- 4. 07 195 5463.829 2. 5 0. 5

5455.095 2 0. 4 Fe I p 3. 25 627 5463.89 m 2. 5 0. 5 s 5465.465m 112 24. 6 s Fe I 4. 32 1145 5463.972 9. 5 1. 7 s Cr I 3. 43 204 5455.624m 219 40. 1 s Fe 1 1. 01 15 5464.116 1. 5 0. 3 5455.914 2. 5 0. 5 5464.288m 33 6. 0 s Fe I 4. 14 1030

5456.113 1 0. 2 6465.154 2. 5 0. 5 AtmH20 P 4 411 26

5456.366r 8. 5 1. 6 Atm H2O P 3 411 26 6465.380 1. 5 0. 3 5456.528 8 1. 5 s Fe I 3. 60 817 6465.75 m S 13,17 5456.800 2 0. 4 5466.031 2. 6 0. 5 Fe n

6456.885 1. 5 0. 3 s,N1 5466.201 1. 5 0. 3 54^7 104

5457.244

5467.474

5457.832

q

1

11

HI

U. 0

0. 2

2. 0

0. 2

s,N Mn I Cr I2. 16 4 7

O'iDO.IUOIll

5466.592

5466.766

7A

2

2. 5

1 Q Q

0. 4

0. 5

s r e I (Yi) 1. 43 12

6468.58 a 6 1. 1 Fe I 5466.993m 29 6. 3 s Fe I /3. 57

13. 66

784 817

5459.20 Ir 1. 5 0. 3 Atm H2O P 3 411 26 6467.152 1 0. 2

5459.389 6. 5 1. 0 6467.277 1 0. 2

5459.745 1 0. 2 5467.402 2 0. 4

54fin ofifi 9 u. ^ O'^tD/ .0/1 1. 0 u. 0 5460.190 2 0. 4 5467.785 3.

5

0. 6 s,N Fe I p— 3. 56 741

5460.365 7. 5 1. 4 0 5467.862 0. 6 0. 1

5460.513 8. 6 1. 6 S Ti I 0. 05 3 5468.114 10 1. 8 8 Ni I 3. 86 192

234
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5468.392 3. 5 0. 6 s,d Ce n? 1. 40 24 17

5468.637 1. 5 0. 3 s,N 16

5468.846 0. 5 0. 1

5469.068 1 0. 2 Fe I p 4. 29 1131

5469.280 7. 5 1. 4 s,N Co I |Fe I p

1. 88

4. 31 561143

16

5469.44 a

to 5469.80 a1. 0

5470.093 22 4. 0 s Fe I 4. 44 1144

5470.228 5 0. 9 Atm HjO P 5 411 26

5470.446 3. 5 0. 6 Co 1 3. 77 175

5470.48 m 0. 2 s Ti I 1. 44 108 13

5470.636 46 8. 4 s,N Mn I 2. 16 4 15

5470.965 0. 5 0. 1 s 5471.205m 6. 5 1. 2 S Ti I 1. 44 106

5471.32 a 1 0. 2

5471.96 a 2 0. 4

5472.304 3 0. 5 Ce II 1. 25 24

5472.487 2. 5 0. 5 5472.713m 39 7. 1 8 Tii-

|Fei

1. 44

4. 21 107 1108

5472.928 2 0. 4

5473.010 0. 5 0. 1

5473.168 18 3. 3 S Fe I 4. 19 1064

5473.394 7. 5 1. 4 U Yii 1. 74 27

5473.553 4 0. 7 s Ti I 2. 33 259

5473.742 3. 5 0. 6

5473.910S 80 U. 4 s Fe I 4. 15 1062

5474.094 2 0. 4 Fe I p 4. 99 1314 5474.232m 9. 5 2. 0 S Ti I 1. 46 108

5474 467 3 0. 5 s Til 2. 34 259

5474.764 1. 5 0. 3

5475.440 4 0. 7 w Nil 3. 83 159

5475.729 3 0. 5

5476.016 2. 5 0. 5

5476.183 5476.295m 1 86

f 4. 0

1 12.

u

s Fe I 4. 14 1029 5476.576m 104 19. 0 s Fe I 4. 10 1062

VG- Icngth

(1)

Equivalen t Width

AX

(ml)

ReWifitli AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMl

No.

or Vib. Band

*J % 1 \J , ij ^ J. ill 164 29. 9 Ni I 1. 83 59

5477.090 6 1. 3 Co I 3. 71 175

5477 285 4. 5 0. 8 5477 502 6. 5 1. 2 Cr II? 4. 14 50 5477 705

5477.791

j 26

f 2. 9

1 2. 0

gu

Ti I

Zr II?

2. 43

1. 83

265

115

5477 968 1. 5 0. 3 5478 157r 2 0. 4 Atm

5478 378

5478.464

] 46

J

f 2. 9

1 5 7

vfl

Q

Cr II Fe I

4. 18

4. 19

50

1062

5478 697 1 0. 2 s?

5478 793 2 0. 4

5479.028 1 0. 2 Ni I? p 3. 83 159

5479.248 1 0. 2

5479.427 3 0. 5

5479 785 0. 5 0. 1

5479.980 1. 5 0. 3 Fe I p 4. 95 1282

5480.205 0. 5 0. 1

5480.362 1 0. 2

5480.518 9. 5 1. 7 s Cri /3. 45

\3. 89 204

5480 761 1

[ 68 Y II Nil

1 72

3! 85 27

191 5480.865m 1 [ 10. 5 s -Fe I (Sri)

4. 22

2. 27

1062

9

5481 072 1. 5 0. 3

5481 252m 56 10. 2 Fe I 4. 10 1058

ftAP.'i 443m 64 11. 7 Ti I Mn I—

|Fe I

2. 41

2. 16

4. 19

265

4 1061

^481 610 1 0. 2

5481 71 m g

5481 742 3 0. 5

."1481 873m 10 1. 8 g Ti I 1. 43 106

5481 999 3 0. 5 s Sc I 1. 86 16

5482 264 3 0. 5 Fe I p 3. 63 873

5482.606 3 0. 5

5482.931 0. 5 0. 1 5483.108m 42 7. 7 s Fe I 4. 15 1061 5483.364m 42 7. 7 s Co I 1. 71 39

761-925—«e -18 235
The Solar Spectrum—^Continued

^Wavelength

(A)

Equi-

\75i V tillcllu 1 cm Width

(ml)

Reduccd. Width

iiA/ A

(F)

Spot Identii_l \. \jX\Ji-L

Low

Xli X or

XI U ly. Line

RMT

Nn

or Band

Notes length

(A)

EquiVf\ 1 p n t, Width

AX

(ml)

Re- Width

AX/X

(F)

Spot

Solar

IdentiJ-LL Ct UJ.'J JUL

Low

TT, P

or Pnt

Line

RMT

or

V IJJ. Band

Notes

O^oo .000 1X 0 9 5492 894 12 2. 2 V)

DrtOO .VOO 0 0 4 5493 068 3 0. 5

0'±00. ^Ak'^ 0)1 C? IZr9 0 8 — Co I 3. 63 175 5493 244 16 2. 9 XL Si I 5. 08

5484.042 3. 5 0. 6 5493.354 1. 5 0. 3 Fe I p 3. 64 873

5484.314 1 0. 2 5493.506m 35 6. 4 s Fe I 4. 10 1061

5484.646 3 0. 5 S Sc I 1. 85 16 5493.661 1 0. 2

5485.068

5485.378

5485.548

5485.706

5485.813

5486.120

5486.524

5486.767

5486.965 5487.153m

5487.327

5487.524

1. 5

1

3. 5

2. 5

3

1. 5

1

1

4. 5 32

1. 5

22

0. 3

0. 2

0. 6

0. 5

0. 5

0. 3

0. 2

0. 2

0. 8

5. 8

0. 3

4. 0

0?

s?

5

Nd II

Cr I?

-V n

Fe I

Fe I p

1. 26

4. 53

2. 26

4. 41

/3. 64

\4. 19

79

53

1143

870

1064

5493.857

5493.990

5494.155

5494.328

5494.474

5494.706

5494.888

5495.706

i^AQK Qlfi

tkAOR 9c;S! UrtV\J m^OCj

t;4Qfi 411 a

5496.573

27

4

2. 5

1. 5

25

5

18

2

0. S

2

9

4. 9

0. 7

0. 5

0. 3

4. 6

0. 9

3. 3

0. 4

0. 2

0. 1

0. 4

1. 6

s1,d

s

su

s

Fe I

Fe I Til

Ni I Co I?

Fe I p

/3. 02

\4. 22

4. 07

1. 46

4. 10

3. 41

4. 91

464

1062

1024

108

231

166

1281

16

5487.755S 88 16. 0 S Fe I 4. 14 1025 5496.807 5 0. 9

5487.934 8. 5 1. 5 S V I 2. 37 129 5496.991 1. S 0.3

5488.170

5488.344

5488.614

5488.989

tjrtiju ,\J<J\J

tiTlOi? CJACQ •OVJO SRQ

tj *! J w . X »j y111

5490.327

18

2

1

18

fi\j

1 4.

1XOS

1

3. 3

0. 4

0. 2

3.3

1 1 X . X

0. 2

s,d

v,N

i,N

sS

Fe I p—

|Tii

Co I Fe I p

Ti T

C2?

4. 61

2. 40

4 44

1X, 4f> T:U R 24

1183 265

1X 1X 48TiO

1XO07/

2,3 19

5497.115

5497.241

5497.356 5497.526m

5497.707

5497.901

5497.98 m

5498.189

4

3

1 128

2

3

2

2. 5

0. 7

0. 5

r

[ 22. 2

0. 4

0. 5

0. 4

0. 5

S

s

Yii

Fe I

Co?

Ti i?p

S I Fe up

1. 75

1. 01

0. 90

7. 86

2. 58

27

15

51

1224

5490.475 0. 5 0. 1 5498.365 1. 5 0. 3

X i 0. X f^JQS 74Q \j. 0 \J. X R 21 2 3 19

14Q

5491 6SS

1X

1X

u. 0

0 9

0 9

S

s

Ti T 00 5499.030

5499.169

2. 5

|L5|

0. 5

0. 3

C2

C2

/P 59 IP 46

fP 57

1 P 44

1,2 2,3

1,2 2 3

}I9

}") 5491.845 11 2. 0 u,N ^e I 4. 19 1031 5499.434 2. 5 0. 5 JNl I 3. 84 17o

5492.037 1 0. 2 5499.598 3 0. 5 Fe I p 4. 47 1159

5492.218 3. 5 0. 6 5500.355 0. 6 0. 1 C2

6492.362 | 3. 5 0. 6 5500.603 1 2. 5 0. 4 C2

236
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

5500.749 3 0. 6 C2 R19 2,3 19 5508.633 17 3. 1 w Cr II 4. 15 50

5500.983 3. 5 0. 5 C2 R 20 2,3 19 5508.851 2 0. 4

5501.259 4. 5 0. 8 C2? R20 2,3 19 5509.114 0. 5 0. 1 Prii? 0. 48

5501.477S 115 22. 2 S Fe I 0. 96 15 5509.544 7. 5 1. 4 u,N Mgi? 5. 11 16

5501.712 7. 5 1. 4 C2 R42 0,1 19 5509.727 5. 5 1. 0 u

5501.876 8. 5 1. 5 C2 5509.909 19 3. 4 u Yii 0. 99 19

5502.092 23 4. 2 u Cr II 4. 17 50 5510.020 41 7. 4 u Ni I 3. 85 190

5502.270 1. 5 0. 3 5510.237 2. 5 0. 4 s,N Fe I p 4. 07 1023 16

5502.577 0. 5 0. 1 5510.376 1 0. 2

5502.747 1 0. 2 5510.619 15 2. 7 u,N C2- R 16 2,3 19

5502.943 14 2. 5 w 5510.730 16 2. 9 u,N Cr II- 3. 83 23

5503.080m 42 7. 6 s Fe I 5510.958 0. 5 0. 1

5503.240 15 2. 7 w Cr II 4. 14 50 5511.167 1 0. 2

5503.500

5503.720 5503.904m

5504.106

10

3

13

10

1. 8

0. 5

2. 4

1. 8

u,N

su

Ti I Ni I2. 58

3. 83

287

175

5511.436

5511.659

5511.802

4. 5

2

6. 5

0. 8

0. 4

1. 2 s

C2-

C2Fe I

Til

R 30 R 29

/I. 46

12. 49

1,2

1,2

108 275

19

19

6504.227 2 0. 4 Mn I 3. 13 31 5512.062 9 1. 6 u Ce II 1. 01 24

5504.395 11 2. 0 s 5512.265m 38 6. 9 u Fe I 4. 37 1143

5504.665 1. 5 0. 3 C2 R30 1,2 19 5512.408 15 2. 7 u Fe I p 4. 41 1148

5504.894 1 0. 2 s 5512.535m 47 8. 5 s Til 1. 46 106

5505.284 0. 5 0. 1 5512.715 2. 5 0. 4 Cr I 3. 01 121

5505.543 1. 5 0. 3 C2? R 18 2,3 19 5512.818 3. 5 0. 6 C2? R 15 2,3 19

5505.728 2. 5 0. 4 Fe I p 4. 47 1162 5512.989S 94 16. 8 s Ca I 2. 93 48 5505.889m

5506.043

5506.189

5506.368

5506.510

5506.618 5506.791m

5506.992

5507.771

5507.951

5508.083

5508.245

52

3

6. 5

4

5. 5

1. 5

120

7

|2.5|

1

0. 5

0. 5

9. 4

0. 5

1. 2

0. 8

1. 0

0. 3

23. 0

1. 2

0. 4

0. 2

0. 1

0. 1

s,N

s

S

s

||Mn IFe I

C,?

C2

C2Mo I

Fe I

S I V I

C2? Cr I?

2. 18

4. 41 R18

R41

1. 33

0. 99

7. 87

2. 36

R 15

4 1145

2,3

0,1

4

15

12

129

2,3

19

19

19

5513.231

5513.384

5513.558

5513.714

5513.850

5514.221 5514.353m

5514.544m

5514.689

5514.802

5514.935

5515.110

2

2. 5

2

1

0. 5

1. 5

3543

1

7. 5

5

3

0. 4

0. 4

0. 4

0. 2

0. 1

0. 3

6. 2

7. 6

0. 2

1. 4

0. 9

0. 5

s

s

s

u

C2

C2

Fe I p

Sci

Ti I

Ti I W I Ni I

C,

Co

P 55 P 53

3. 69

1. 85

1. 43

1. 44

0. 41

3. 85 R 40 /R 39 \R 27

1,2

1,2

925

15

106

106

1

189

0,1

0,1 1,2

19

19

19 }n

5508.419 18 3. 3 u 5515.354 2 0.4 Cj

237
The Solar Spectrum—Continued

length

(A)

EquiVa 1 p 11 1, Width

AX

(mA)

Re- Width

(F)

Spot

Solar

IdentiLow

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

TVavelength

(A)

Equivalent Width

AX

(ml)

Re- Width

iAA/ A\/\A

(F)

Spot

Solar

IdentiLLK- Cli \j1.\J1±

Low

Hi .u or

Vint Line

RMT

IN 0. or Vih V 1 u. Band

Notes

5515.491 2 0. 4 5522.454m 43 7. 8 w Fe I 4. 21 1108

5515.649 7 1. 3 u 5522.673 2. 5 0. 4

5515.93 a 1 0. 2 5522.971 0. 5 0. 1

5516.045

5516.300

2

4. 5

.1

0. 4

0. 8

0. 9

3.

3

4 4

u

Oj IV

1 s,N

J

TTa t X c 1 ^

Mn I

4. 10 R 11

2. 18

1057

2 3

4

1 Q

5523.261

5523.338

5523.573

5523.753

5523.870

5

2

3

1 0. 9

[ 1.1

0. 9

0. 4

0. 5

1 u,N

u,N

Co I

C2

2. 33

fP 33 \P 34

112

2,3

2,3 }19

JO 1 1 .\J 1 o -L O 3. 3 Fe I 4. 21 1109 5594 noo 9. 5 1. 7 u

O'J L i .AO 111 VV T?11 0. 00 2 13 5594 108 1 0. 2

5517.254 0. 5 0. 1 5524.268 5 0. 9 Fe r 4. 15 1059

5517.380 0. 5 0. 1 5524.471 1. 5 0. 3 C2 R26 1,2 19

5517.552 14 2. 5 u,N Si I 5.08 5524.578 2 0. 4 C2 R25 1,2 19

5517.774

5518.095

5518.170

5518.371

5518.545

5518.796

5518.980

5519.077

5519.426

5519.585

5519.858

OOZi\J.\JOO

5520.226

5520.511

5520.715

1. 5

2

1. 5

2

4. 5

2

1. 5

2

4

25

5. 5

2

3

7. 5

1. 5

0.3

0. 4

0. 3

0. 4

0. 8

0. 4

0. 3

0. 4

0. 8

4. 5

1. 0

0. 4

0. 5

1. 4

0. 3

s

d,w?

s,N

s,d

Ti I p

CsFe I p

C2

C2

Fe I Fe II p —

C2

Fe I? p

Sc I

2. 41 R27

R 12

5. 03 R 12

/R39

IR 40

3. 34 /? 53 \R 10

4. 44

1. 86

265

1,2

2,3

1314

2,3

0,1

0,1

52

1,2 2,3

1144

15

19

19

19

}-

17

5524.800

5524.999

5525.135

5525.354

5525.552S

5525.716

5525.853

5526.194

5526.313

5526.572 5526.821m

5526.993

5527.112

5527.410

2

3. 5

13

2

102

3. 5

4. 5

3. 5

1

1

76

1. 5

2

1. 5

5

0. 4

0. 6

2. 4

0. 4

18. 4

0. 6

0. 8

0. 6

0. 2

0. 2

13. 8

0. 3

0. 4

0. 3

1. 1

s,Nw

u

u

s d?

C2

Co I Fe II? p

Fe I

C2

Sc 11

C2

C2

Y I—

Til

/R 24 IR 7

4. 11

3. 27

4. 23

fP 51 IR 6

1. 77 P 31 P 30

1. 40

2. 43

1,2 2,3

192

56

1062

1,2 2,3

31

2,3

2,3

12 265

}n

16

19

19

5520.946

.5521.139

10

7

1. 9

1. 3

u

u Ca I Fe I

1. 89

3. 63 839

5527.873

5528.086

6. 5

3

1. 2

0. 5

C2 /R 37

\R 38

0,1 0 1 }19

5521.302 6. ^> 1.

2

u Fe I p 4. 43 1162 5528.418m 293 5S. 8 S Mgi 4. 34 9

5521.437 3 0. £ Ni I 3. 84 175 5528.905 22 4. 0 u Fe I p 4. 47 1161

5521.590

5521.791

5522 197

5. t

1. ^

5. i

) 1. C

) 0. S

) 1. (

) w

)

Y I IIYii

Sr I?

C2

1. 90

1. 74

2. 25 P 34

27

9

2,3 19

5529.171

5529.347

5529.46 a

17

4

2

3. 1

0. 7

0. 4

s Fe I 3. 64 872

238
The Solar Spectrum^—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Banc

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

R.MI

No.

or

Vib. Band

Notes

5529.791 1. 5 0. 3 Fe I p 2. 86 344 5537.119 3 0. 5 o7 Ni I 3. 85 188

5529.966 5 0. 9 5537.297 1 0. 2

5530.281

/—

1 0. 2 5537.517 2 0. 4

5530.491

5530.786

11

|14|

2. 0

2. 5

s

8,d Co I 1. 71 38

5537.718

5537.811 1J

j

2. 7

[ 3. 6

s Mn I 2. 19 4

5531.113 1. 5 0. 3 c. F 27 2,3 19 5538.045 2 0. 4

5531.444 1. 5 0. 3 5538.189 2 0. 4

6531.697 1. 5 0. 3 5538.316 1. 5 0. 3

5531.985

5532.137

18

6. 5

3. 2

1. 2

w Fe I

C2

4. 91 /R 35 IP 281281

0,1 2,3 }19

5538.522m

5538.718

38

3

6. 9

0. 5

u Fe I

C2

/3. 63

14. 22 P 20

839

1064

2,3 19

5532.355

5532.751m

5532.879

5

39

21

0. 9

7. 0

3. 8

uw

C2

Fe I Fe I?

fP 47

IP 26

3. 57

1,2 2,3

783

}l9 5539.063

5539.291

5539.534

2. 5

22

3. 5

0. 4

4. 0

0. 6

u

C2Fe I Cr IC2R22

3. 64

P 19

1,2

871

2,3

19

19

5533.039 7 1. 3 s Mo I 1. 33 4 5539.832 9. 5 1. 7 u Fe I 4. 29 1130

5533.156

5533.438

13.51

2

0. 6

0. 4 C2 fR 23 IP 25

1,2 2,3 }l9

5539.978

5540.181

5

4. 5

0. 9

0. 8

C2?

C2

fP 17 IP 18 P 17

2,3

2,3

2,3 19

5533.584

5533.798

5534.295

2

3

3

0. 4

0. 5

0. 5

C2

C2

C2

R 24 R 24 P 25

1,2

1,2

2,3

19

19

19

5540.452

5540.724

8

6. 5

1. 4

1. 0

C2

C2

fP 15 \P 16

fP 14 IP 16

2,3

2,3

2,3

2,3 5534.406 |2.5| 0. 4 5540.898 6. 5 1. 2 u C2 P 44 1,2 16,19

5534.676

5534.848S

5535.062

10

63

2

1. 8

11. 4

0. 4

sw

Fe I

Fe II

/3. 64

14. 15

3. 24

871 1063

55

5541.290

5541.592

5541.909

5542.149

1

1. 5

1. 5

1. 5

0. 2

0. 3

0. 3

0. 3

Fe I p

C2?

C2

3. 30 R21

R21

627

1,2

1,2

19

19 5535.190 5 0. 9 u1 C3 fP 48 IP 25

1,2 2,3 5542.326 1. 5 0. 3

5535.425m

5535 51 m

5535.561

5535.767

. 113

1

13. 6

<

V 7.

0. 2

u

s

u

Fe I

Ba I

f3. 25

14. 19

0. 00

626

1029

2 13

5542.541

5542.749

5542.897

5543.046

1

0. 5

2

10

0. 2

0. 1

0. 4

1. 8 u Fe I p

r3. 69

\4. 19 926

1064

c CO c o crr\ 5535.859 1. 5 0. 3 5543.199m 61 11. 0 u Fe I 3. 69 926

5536.086 3. 5 0. 6 C2 P 24 2,3 19 5543.411 3. 5 0. 6

c c o r»o r» 5536.280 4. 5 0. 8 C2 R 34 0,1 19 5543.57 a 2 0. 4

5536.465 2 0. 4 C2? R23 1,2 19 5543.758 2 0. 4

5536.598 7 1. 3 s Fe I p 2. 83 345 5543.944m 63 11.4 u Fe I 4. 22 1062

5536.814 1 0. 2 C2 P 23 2,3 19 5544.174 6 1. 1

5536.929 1 0. 2 C2? P 23 2,3 19 6544.348 4 0. 7 R20 1,2 19

239
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F;

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Notes Wavelength

\A)

Equivalent Width

AX

Re- duced

Width

AX/X

Spot

Solar

Identification

Lov? EP

or Rot. LinG

RMT

No.

or Vib. D d-IlU,

Notes

5544.616

5544.770

8

2

1. 4

0. 4

M? Y I llYii

C2

1. 90

1. 74 R20 1,2

1727

19

5552.855

5553.130

5553.235

1. 5

5. 5

3. 5

0. 3

1. 0

0. 6

w?

Fe I p

Fe I p

2. 83

4. 22

344

1064

5545.052 4 0. 7 C I /8. 64

18. 64 5553.400 1. 5 0. 3

5545.275 2. 5 0. 4 Fe II p 2. 58 24 5553.589m 40 7. 2 s? Fe I 4. 43 1161

5545.433 2 0. 4 5553.707 22 4. 0 s Ni I 1. 93 69

5545.704 0. 5 0. 1 5554.00 a 2 0. 4 C2 R 16 1,2 19

5545.936

5546.032

5546.344

5546.514S

5546.745 5547.000m

5547.06 m

5547.306

5547.694

5547.945

5548.200

5

6. 5

1

53

6

1 29

4

3. 5

2. 5

2. 5

0. 9

1. 2

0. 2

9. 6

1. 1

j\ 0. 7

0. 7

0. 6

0. 4

0. 4

s,d

u

u

uS

IV I Co I Y II

Fe I

Fe I V I

1. 06

4. 11

1. 75

4. 37

4. 22

1. 08

R31

38

191

27

1145

106]

38

0,1 19

5554.245

5554.528

5554.660

5554.820 5554.900m

5555.178

5555.358

5555.469

5555.646

5555.734

5556.202

2

1. 5

2

1 102

7

2

2. 5

3. 5

5. 5

1

0. 4

0.3

0. 4

1 2. 2

[ 16. 9

1. 3

0. 4

0. 4

0. 6

1. 0

0. 2

s

s,d

C2

C2

Fe I Fe I p

Cr I C2

R 16 R 16

4. 55

3. 55

P 38

3. 01 R 15

1,2

1,2

1183

740

1,2

121

1,2

19

19

17,19

19

5548.318

6548.481

5548.617

5548.76 m

5548.93 a

3

2. 5

2

1. 5

0. 5

0. 4

0. 4

0. 3

s

Cr I? 3. 42

13

5556.478

5556.714

5556.974

5557.070

1

1. 5

4

5

0. 2

0. 2

0. 7

1. 1

s?

M?

S

Yb I02

All

0. 00 R 15

3. 14 JP 37 IP 39

0. 02

/3. 11

1.4. 4/

3. 14

1 1,2

6

1719

5549.325

5549.532

5549.656

5549.958

1. 5

1

9. 5

10

0. 3

0. 2

1. 7

1. 8

u

s

C2Fe I p Fe I p

Fe I

R18

4. 39

4. 99

3. 69

1,2

1159

1314

926

19

5557.728

5557.916

c

2

i i 1 . 1

0. 4

f 4. 1

s

u

Vi?

Fe I p All

1,2

1,2

1

464

i 1d4

6

llfi 1Q

5550.29 a 1. 5 0.3 5557.995 [ 6. 8 u Fe I 4. 47 1163

5550.659 1 0. 2 5558.177 2 0. 4

5550.891 1 0. 2 5558.260 2. 5 0. 4

5551.025 2. 5 0. 4 5558.600 1 0. 2 C2 R 14 1,2 19

5551.311 1 0. 2 Fe I p 3. 41 714 5558.77 a 3 1. 1 s,N Vi 1. 71 77

5551.548 5. 5 1. 0 C I? 8. 64 5558.850 3 0.5 Co I? 3. 53 166

5551.778 6 1. 1 Fe I p 4. 10 1059 5559.061 5. 5 1. 0

5551.978 8. 5 1. 5 u Mn I 5. 49 5559.648 7. 5 1. 3 0 Fe X p 4. 99 1282

5552.237 5. 5 1. 0 w So II 1. 45 25 5559.896 4. 5 0. 8 u

5552.459 1 0. 2 s 16 5560.025 0. 5 0. 1

5552.700 7 1. 3 u Fe I p 4. 95 1281

240
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or

P^ot. Line

RMT

No.

or Vib. Band

Notes

6560.220m

5560.431

5560.552

5560.694

5561.015

5561.246

5561.479

5561.608

5561.825

5562,125

5562.283

5562.497

44

2

1

1

1. 5

8. 5

2

4

3. 5

8

5. 5

5

8. 3

0. 4

0. 2

0. 2

0. 3

1. 5

0. 4

0. 9

0. 6

1. 4

1. 0

0. 9

u

s

w?

0

Fei

Vi

C2

C2

Fe I p

C2

4. 43

0. 04 R 13 R 13

4. 39 R 12

1164

1

1,2

1,2

1162

1,2

19

19

19

5567.776

5568.075

5568.280

5568.470

5568.705

5568.871

5569.034

5569.157

5569.329 5569.631m

5570.069

5570.397

7. 5

3

3. 5

1

2. 5

8. 5

1. 5

2

1. 5

162

2. 5

6. 5

1. 3

0. 5

0. 6

0. 2

0. 4

2. 0

0. 3

0. 4

0. 3

30. 3

0. 4

1. 2

s

s,d

8

s

s u,N

s

Y I? Mn I Fe I p

Cr I Fe I p Fe I p

Fe I

Fe I Fe I p Mo I

1. 92

5. 52

4. 15

3. 00

4. 15

4. 14

3. 63

3. 42

2. 84

1. 33

10.59

1058

1026

869

686

345

4

17

16

5562.716m 52 9. 3 u Fe I /3. 27

14. 43 626

1163 5570.613 2. 5 0. 4

5562.929 3. 5 0. 6 5570.763 1. 5 0. 3 C2 R7 1,2 19

5563.286

5563.405

5563.608

5563.702

5

1

I Q9

0. 9

0. 2

r 14.

1 3. 4

u

s

Fe I

Fe I p

4. 19

/2. 42 U- 14

1062

112 1023

5571.488

5572.155

5572.352

| 5572.454 J

4. 5

4. 5

4. 5

0. 8

0. 8

[ 0. 4

1 0.4

C2Cr I C2-

R7

R6

1,2

1,2

19

19

5564.134 1. 5 0. 3 -C2? R 11 1,2 19 5572.652 4. 5 0. 8 C2? R 27 0,1 19

5564.58 a 1 0. 2 C2 R 11 1,2 19 5572.851m 205 36. 8 s Fe I 3. 40 686

5564.972 4 0. 7 C2 R 11 1,2 19 5573.107m 44 7. 9 u Fe I 4. 19 1061

5565.32 a 2. 5 0. 4 5573.308 1. 5 0. 3 5565.485m

5565.713m

5565.953

1161

79

4. 5

2. 9

14. 2

0. 8

s

s

Ti I Fe I

C2

2. 24

4. 61 /R28

IRIO

229

1183

0,1

1,2

5573.544

5573.655

5573.757

2

4

2

0. 4

0. 7

0. 4

0 -C2

Mm?

Co

/R6

IR 5

5. 54 P 28

1,2 1,2

1,2

}-

19

5566.085 16 2. 9 u 5574.04m 1 0. 2 s Vi? 0. 04

5566.241 2 0. 4 5574.399 3 0.5 s Cr I 4. 45

5566.415 0. 5 0. 1 C2 R 10 1,2 19 5574.912 2 0. 4 C2 P 29 1,2 19

5566.563 0. 5 0. 1 Cr I? 3. 43 5575.093 1. 5 0. 3 C2 R 5 1,2 19

5566.729 5 0. 9 5575.396 0. 5 0. 1

5566.814

5586.994

5567.152

5567.285 5567.400m

5567.586

3

1

0. 5

10

57

2

0. 5

0. 2

0. 1

1. 8

10. 2

0. 4

s

s

C2

|Fe I p

Fe I

R 10

3. 25

2. 61

1,2 625

209

19 5575.544

5575.683

5575.862 5576.099m

5576.371

5577.028

1. 5

2. 5

4

113

6

13

0. 3

0. 4

0. 7

21. 9

1. 1

2. 7

u

w

C2

C2

C2Fe I

Fe I

R 26 R 26 R 26

3. 43

5. 03

0,1

0,1

0,1

686

1314

19

19

19

241
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent w lutn AX

(ml)

Re- duced

Wiutn

(F)

bpOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib.

5577.341 6 1. 1 w1 C2

11^ li P 27

1 Q7

1,2 or

19zo

00/ /.ODZ Q (1. 0

ool 1 .1X3 a i n 0

00/S.O.iO 0 u. y

00/ o. { /ym A A y. 0 s In 1 I i. Do 4 /

00 /y. (Joy A4

n 7 li ZD U,i 1lyQ

oo/y.ioo Z. 0 U. 4 s 111!

00/y.ooz iU 1 Q s Fe I p '±. Zo lUDi 1

7

oo/y.4yo 0. 0 U. D IT ^0 iy

oo/y./u a 0. 0 u. 0

oo/y.yu/ Q0 u. 0 S,l\ 1

7

OOOU.U4 a 0. 0 n A

OOoU.oUy 0 U. 4 s

OO0U.4OO 0. 0 n A rt<^2 1 0 ly

OOoU.DD'l 4. 0 u. 0

r r Q -1 ri r Q OOOl .UOo 0. 0 n A

00ol.^io4 0 u. y P 1 0 ly

5581 524 3 0. 5 P 21 1 2 19

5581.706 5 0. 9 C2 R24 0,1 19 5581.979m 91 16. 7 S Ca I 2. 52 21

r coo 1 /1

0

^. 0 V. 4

5582.287 5. 5 1.

0

C2

fi 6 IP 20

lyZ

1,2

5582.414 3. 5 0. 6 C2 fP 4

[ir 10

1,2

I,"' J

oooz. / O/ 1). 0 J.. U t^2 "Dot 1 0

1,/ ly

5582.970 3. 5 0. 6 s Ti I

5583.145 1 0. 2

5583.391 2 0. 4 C2 P 20 1,2 19

5583.627 1. 5 0. 3 C2 /P5,6

1 T> 1 0

1.1 lo

1,2

1,2 |l9

J 5583.991 8 1. 4 u,N Fe I p 4. 19 1059

5584.313 1. 5 0. 3 C2 P 18 1,2 19

00o4.0l4 4. 0 1. 1 8 V I 1. Ud 0 7 67 5584.773m 32 6. S 8 Fe I (Vi)

3. 57

1. 87 782

85

5585.045 4. 5 0. 8 C2 /R23

\P 17

0,1

1,2 5585.180 12 2. 1 C2

1 P 16 1,2 19

Wavelength

(1)

Equivalent Width

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

5585.325 3 0. 5 C2 111

^P 12

"D 1 0

1,2

1,2

1,2

c c 0 C CIO 00O5.51C5 A4

A '7 P 16 1,2

c c 0 c ceo 5. 0 1. u s ll I

OOov.vUZ 0 U. 4

ft AT" V I

1 OA

1. 80 85

0000. zoU 8. 0 1. 0 s

C COG C CO« 0600. oo2r

C C OC 771 0080. / / im > z4o < 4-'. ^ s Fe I 0 07 6. 67 686

0080.yi m J \ 0. y s

c c 07 100 4 U. i

C r 07 OAn 008/.ooy 1 r; 1. 0 U. 0 Fe I p

0 07

0. Zl 583

c c 07 c 0

1

008/.0olm Q 1 01 6. 4 u Fe I 4. 14 1026

C C07 70Q 008/ . / /a 1 A 9 U. Z 021 TDK 00ZZ A 1 0,1 CCO7 OAOv.n 0087. 8Dom A fi 49 9. 8 s Nl I 1. 93 7n70

0088. 14.i A C

4. 0 U. 8

c c 0 0 0 c 1 0088.ZOi 00

n c

U. 0

0088. /D4m 141 ZO. 1 s Oa I 0 cro 5z 21

OOoy.UlU 11 9 n ft AT S,iV Fe I p

^ A'7 4. 4/ 1 1 A A lloO

oooy .ZU / n c

U. 0

n 1 U. 1

C C on OA A 0089.ODD 9 K /O 0. 2 u

tvt: -w Vil 1 0 A A 0. 90 205

c c on c7

0

oosy.o/a 1

C\ 9 U. Z

c c on OA 1 oooy.ool 1 Alo 9 n

9 If re I ccnn 10AC? 5590. 1 ^ob OA60 10. 0

c0Oft T Ca I 0 CO

Z. oZ 0

1

zl

c c nn 071 Oo90.o71 Z. 0 U. 4

/-I Ca T)K 0 1 zl 0,1

c cnn c no 1 A 9

U. Z C2 K zl A 1 0,1

5590.706 6 1. 1 s Co I 2. 04 90

5590.818 5. 5 1. 0 s

5591.003 1. 5 0. 3

5591.369 7 1. 3 s,N Sc IFe II? p1. 99

0 07

6. zl

1855

5591.978 lo 1 f\ A U. 4

e c no ICO 55y.^.l6ii 00 K 7 5. 7 u JNl I A 00

4. zo OCA z50

5592. 2bom 50 0 n8. 9 s Nl I 1. 95 69

5592.4/7 5 0. 9 8 V I

1 AC

1. 05 0737

5592.663 5 0. 9 8

5592.958 1 0. 2 s,N V I 0. 04 1

5593.240 0. 5 0. 1 c, R20 0,1

5593.458 3 0. 5 u?

242
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5593.746m 42 8. 0 u Ni I 3. 90 206 5602.773

C

6. 6 }• J Fei 4. 15 1062

5593.979 1. 5 0. 3 5602.864 1

215 1 15. 9 I Cai 2. 52 21

5594.169 2. 5 0. 4 5602.969 [ 18. 6 s Fe I 3. 43 686

5594.471m

5594.666m

5594.897

5595.067

117

60

1. 5

6. 5

20. 9

10. 7

0. 3

1. 2

s

s

8

Ca I (Nd II) Fe I

Fe I p

2. 52

1. 12

4. 55

5. 06

2179

1182

1314

5603.303

5603.519

5603.771

5604.198

6. 5

2. 5

20

1

1. 2

0. 4

S. 7

0. 2

u

s

C2

C2

V I

R 16 R 16

(1. 85

11. 95

0,1

0,1

85

19

19

5595.486 1 0. 2 5604.956 3. 5 0. 9 S Vi 1. 04 37

5595.691 0. 5 0. 1 Cj R 19 0,1 19 5605.348 1. 5 0. 3 C2 R 15 0,1 19

5595.912 1. 5 0. 3 C2? R 19 0,1 19 5605.649 1. 5 0. 3 C2? R 15 0.1 19

5596.185 6 1. 1 C2 5605.903 5 0. 9 C2 R 15 0,1 19

6596.341 1 0. 2 C2 P 41 0,1 19 5606.049 2 0. 4 C2 P 37 0,1 19

5[>96.591 1 0. 2 5607.003 2 0. 4 0? Nil 3. 90 205

559.' 372 3. 5 0. 6 U 5607.154 0. 5 0. 1 Fe II? p 2. 58 24

5597.-43 0. 5 0. 1 5607.399 1 0. 2

6597 471 2 0. 4 5607.542 1. 5 0. 3 C2 R 14 0,1 19

5597. m s,N Ti I? 13,16 5607.669 13 2. 3 u Fe I p 4. 15 1058

5597.r<6 3 0. 5 s,N Cr I 3. 84 239 16 5607.842 1. 5 0. 3 C2 R 14 0,1 19

5''^8..05m b598.491m

5598.820 5598.86?m

5598.956

5599.147

5600.028

5600.103

5600.234

5600.463

5600.695

5600.821

5601 .286S

5601.435

5601.820

5602.076

5602.562

83

118

} ^

2

3

23

5

35

2

3. 5

|12|

100

4. 5

16

|7|

|9|

1 :. 8

.1 1

1 c,

I 0. 2

0. 4

0. 5

4. 1

0. 9

6. 2

0. 4

0. 6

2. ]

17. 8

0. 8

2. 8

1. 2

1. 6

u

s

u

u,N

sS

u,N

s,Nu

Fe I Ca I

In.' )

Fe I

Co

Ti I Ca I

Cn?

Fe I p

4. 65

2. 52 P 42

P 40

4. 09

/3. 63

14. 26

R 17

2. 52

3. 45

4. 95

1183

21

0,1

0,1

219

866

1108

0,1

21

1281

19

19

19

17

5608.174

5608.314

5608.981

5609.180

5609.682

5609.806

5609.987

5610.246

5610.391

5610.601

5610.90 a

5611.056

5611.368

5611.644

5612.498

5613.715

5614.041

1. 5

1

8. 5

0. 5

1. 5

3

6

5

4

2. 5

2

2

8

3

"i

1

3

1. 5

0. 3

0. 2

1. 7

0. 1

0. 3

0. 5

1. 1

0. 9

0. 7

0. 5

0. 4

0. 4

1. 4

0. 5 n 7

0. 2

0. 5

0. 3

u s,m

u

s

8

U

0

u,N

C2

C2Fe I p Cn

C2

Fe I p

Ce II C2

C2

Fe I p

1^2

C2Fe I p

C2

fP 37 IP 38 P 36

4. 21

3. 45 R 13

3. 64

1. 05

P 37 P35

3. 63

"RIO p 34

5. 01 R 11

o.n

0,1/

0,1

1108

223

0,1

866

26

0,1

0,1

869

0,1

1282

0.1

19

19

19

17

19

19

1 Q

19

19

243
The Solar Spectrum^—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

N0I

5614.282 14 2. 5 u,N Fe I p 5. 08 1314

5614.423 2 0. 4 fP 35 \R 11

0,1

0,1 |l9

5614.602 2 0. 4 Fe I? p 3. 55 739 6614.781m 40 7. 1 wt Ni I 4. 15 250

5614.983 8. 5 1. 5

5615.163 f 0. 4 Fe I p 4. 37 1143 5615.308m

68

J 1 12. 6 s Fe I 2. 59 209

5615.529 5615.658m 1 288

f 8. 7

1 45.2

u,m

s Fe I 3. 33 686

5616.188 3 0. 5

5616.331 2. 5 0. 4 C2

fP 34 IR 10

0,1

0,1 ll9

5616.952 1 0. 2

5617.148

5617.236

30

j

1 2. 8

[ 2. 5

u

w1

Fe I p Fe I4. 22

3. 25

1088

626

5617.421 1 0. 2

5617.755 0. 5 0. 1 C2 R 9 0,1 19

5617.918 1. 5 0. 3 C2 P 33 0,1 19

5618.080 1 0. 2 C3 P 33 0,1 19

5618.38 m

}

1

r a: S 16

5618.431 J 1 0. 1 5618.642m 42 8. 0 s Fe I 4. 21 1107

5618.847 1. 5 0. 3 C2 R 8 0,1 19

5618.979 0. 5 0. 1

5619.239 3. 5 0. 6 w Fe I? p 3. 69 923

5619.423 1 0. 2

5619.609 29 6. 0 u Fe I 4. 39 1161

5619.819 3 0. 5 C2 P 32 0,1 19

5620.030 7 1. 2 w?,N Fe I /4. 14

\4. 56 1026 1205

5620. 17?m 0. 5 0. 1 s Zr I 0. 52 25

5620.236 0. 5 0. 1

5620.411 7 1. 2 s?

5620.496 30 5. 3 u Fe I 4. 15 1061

5620.647 2 0. 4 Nd II 1. 54 86

5621.221 5 0. 9 C2 P 30 0,1 19

5621.385 5 0. 9 C2 P 29 0,1 19

5621.621 11 2. 0 Si I 5. 08 16

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5621.77 a

to 5622.12 a

5. 5

J

1. 0

5622.231 5. 5 1. 0 Si I 4. 93 11

5622.782 2. 5 0. 4 u C2

5622.959 7 1. 2 u,N C2 P 28 0,1 19

5623.639 0 0. 4 Fe I p 3. 27 625

5624.030m 49 9. 2 u Fe I 4. 39 1160

5624.192 4. 5 0. 8 C2 P 29 0,1 19

5624.356 2. 5 0. 4 -C2? P 29 0,1 19

6624.558S 140 25. 6 s ||Fe IV I3. 42

1. 06 68637

5624.880 6 1. 1 S V I 1. 05 37

5625.092 2 0. 4 5625.328m 37 7. 1 w Ni I 4. 09 221

5625.541 1 0. 2 C2? P 28 0,1 19

5625.687 28 5. 2 w'!,N -Fe I

5626.027 3. 5 0. 7 S,d? V I 1. 04 37 17

5626.250 1 0. 2

5626.599 1. 5 0. 3

5626.819 3. 5 0. 6 C2 P 27 0,1 19

5627.097 2. 5 0. 4 Fe I p 4. 18 1084

5627.262 1 0. 2

5627.373 0. 5 0. 1

5627.502 7. 5 1. 3 0 Fe II p 3. 39 57

5627.642 20 3. 6 S V I 1. 08 37

5627.874 0. 5 0. 1

5628.022 2. 5 0. 4 0 -C2 P 26 0,1 19

5628.193 1. 5 0. 3 C2 P 26 0,1 19

5628.354 14 2. 8 u Ni I 4. 09 215

5628.650 15 2. 7 s Cr I 3. 42 203

5628.883 0. 5 0. 1

5629.048 2 0. 4 C2? P 25 0,1 19

5629.237 4 0. 7 C2? P 25 0,1 19

5629.709 1 0. 2

5629.876 0. 5 0. 1

5630.101 3 0. 5 s C2Y I? P 24 L 360,112

19

5630.303 2 0. 4 C2 P 24 0,1 19

5630.980 1. 5 0.3 C2 P 23 0,1 19
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

-Votes

5631.157 1. 5 0. 3 5640.687 1 0. 2

5631.693 3 0. 5 Fe X 4. 47 1159 5640.989m 39 6. 9 w Sc II 1. 50 29

5631.826 8. 5 1. 5 P 22 0,1 19 5641.131 4 0. 7 Ni I 4. 10 230

5632.011 2. 5 0. 4 C2 P 20 0,1 19 5641.291 1 0. 2

5632.455 3. 5 0. 7 s,N V I 0. 07 1 5641.448S 64 12. 0 u Fe I 4. 26 1087

5632.756 3 0. 5 C2 P 21 0,1 19 5641.737 3. 5 0. 6 Cr I 3. 82

5633.220 4 0. 7 C2 P 20 0,1 19 5641.893 24 4. 2 wt Ni I 4. 10 234

5633.443 1. 5 0. 3 c. P 20 0,1 19 5642.178 3 0. 5

5633.646 2. 5 0. 4 C2 5642.381 5 0. 9 s Cr I 3. 86 239

5633.753 2. 5 0. 4 C2 P 19 0,1 19 5642.623 4. 5 0. 8 u Ni I 3. 90 203

5633 953m 68 12. 4- Fe I 4. 99 1314 5642 761 9. 5 1. 7 s? Fe I p 4. 61 1184

5634.231 3. 5 0. 6 C2 P 18 0,1 19 5643.087 14 2. 8 w? Ni I 4. 16 259

5634.523 4. 5 0. 8 C2Fe I p P 18

4. 99

0,1 1281

19 5643.290

5643.934

0. 5

10

0. 1

1. 8 u Fe I p 4. 07 1021 5634.874 7. 5 1. 3 C2 fP 16 IP ]7

0,1

0,1 }- 5644.037 14 2. 5 u Fe I

5635.198 |6.5| 1. 2 C2? P 16 0,1 19 5644.146m 29 5. 1 s Ti I 2. 27 240

5635.346 3 0. 5 C2 P 15 0,1 19 5644.350 4 0. 7 Fe I p 4. 15 1057

5635.514

5635.831m

5636.003

5636.124

5636.234

5636.475

5636.705

5636.901 5637.123m

5637.414m

5637.707 5638.271m

5638.485

5638.758

5639.353

5639.555

5639.996

5640.176

5640.319

3

30

0. 5

1. 5

3. 5

1

17

0. 5

31

44

3. 5

74

2. 5

10

4

1

1

4

18

0. 5

5. 7

0. 1

0. 3

0. 6

0. 2

S. 5

0. 1

5. 8

8. 2

0. 6

IS. 6

0. 4

1. 8

0. 7

0. 2

0. 2

0. 7

3. 2

s?

u,N

s?

uw

s

u

u

s?

w

C2

Fe I Fe I p

Co I Ru I

Fe I

Ni I Fe I -Co I? Fe I

Ni I

Co I

JP 13 IP 14

4. 26

4. 19

4. 15

1. 06

3. 64

4. 09

4. 15

4. 22

3. 90

2. 04

0,1

0,1

1088

1058

10

868

218

195

1087

203

16

5645.039

5645.292 5645.618m

5645.837

5646.111

5646.319

5646.689

5647.241

5647.447

5647.550

5647.779

5647.896

5648.279' 5648.578m

5648.756

5648.914

5649.087

5649.390

5649.682

15.51

2

35

12

5

0. 5

6

11

1

0. 5

1. 5

2

5

10

2

1

10

8

32

1. 0

0. 4

6. 2

2. 1

0. 9

0. 1

1. 6

2. 3

0. 2

0. 1

0. 3

0. 4

1. 2

1. 9

0. 4

0. 2

1. 9

1. 4

6. 2

0

w,N

uS

w?

s

u

s

si

s

s {"-

Si I

V I

Fe I p Co I

Cr I Cri

Ti I

Fe I p

Cr I Fe INi I

4. 93

1. 05

4. 26

2. 28

3. 82

3. 82

2. 49

3. 25

3. 84

3. 63

4. 17

10

37

1109

112

239

269

625

239

838

231

17

5640.502 2. 5 0. 4 Fe I 4. 56 1202 5649.996m 33 6. 4 u Fe I 5. 10 1314

245
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

5650.204 1. 5 0. 3 5659.916 1 0. 2

5650.285 1 0. 2 Fe I p 4. 55 1180 5660.144 1. 5 0. 3

6650.460 5. 5 1. 0 5660.310 1. 5 0. 3 5650.694m 34 6. 7 w? Fe I 6. 08 1314 5660.520 11 1. 9 0 Si I 5. 61

6650.883 1. 5 0. 3 5660.680 13 2. 3 w Si I 5. 61

5651.040 0. 5 0. 1 5660.809 16 2. 8 s Fe I 3. 64 869

5651.275 1. 5 0. 3 5661.025 4. 5 0. 8 s,N Fe I p 4. 58 1234

5651.477 16 S. 5 Fe I p 4. 47 1161 5661.204 1 0. 2

5651.742

5652.029 5652.327m

6653.171

6653.685 5653.874m

5654.018

6654.501

5654.774

5654.937 6655.183m

5655.343

6655.500S

2

2. 5

24

1. 5

2

36

1

75

0. 5

16

49

1

68

0. 4

0. 4

4. 6

0. 3

0. 4

6. 7

0. 2

13. 3

0. 1

2. 8

8. 7

0. 2

12. 0

M

U

s u,N

u

u

s?

Co I?

Fe I p Fe I

Fe I

Si I Fe I

Fe I

fl. 96

14. 26

4. 22

4. 26

4. 39

5. 61

5. 06

/4. 26

15. 03

56

1059

1108

1159

1314

1107 1314

5661.354

5661.497

6661.617

5661.86 a

5661.986 5662.159m

5662 319

5662.624m

5662.754 5662.939m

5663.132

5663.25 a

5663.523

19

} -

1

4. 5

21

2. 5

92

3

49

1

2. 5

|4|

3. 9

f 0. 2

1 0. 1

0. 2

0. 8

3. 7

d. 4

17. 1

0. 5

9. 4

0. 2

0. 4

0. 7

u

u1

s

s

s

Fe I

Fe I p

Ti I

Fe I

IFe I iTi IY II

4. 28

4. 26

2. 32

4. 18

3. 69

2. 48

1. 94

1108

1109

249

1087

924

26938

5655.694 3. 5 0. 6 5663.824 5 0. 9

5656.900

6657.260

6657.450

5657.677 5657.880m

5658.165

5658.346 5658.542m

5658.668 5658.830m

5659.112

5659.16 m

6659.335

5659.593

1

0. 5

5. 5

1. 6

64

3. 5

31

1

222

9

3

19

0. 2

0. 1

1. 2

0. 3

12. 2

0. 6

5. 5

( 9.

5

I 21.

4

1. 6

0.5

S. 9

S

w

w

u,N

u

s

s

w,N

Vi

So II

So II Fe I Fe I p

Fe I

Ti I? Co I

1. 06

1. 51

1. 50

3. 43

4. 28

3. 40

0. 90

2. 04

16

37

29

29

686

1087

686

50

82 13

5664.009m

5664.198

6664.26 m

5664.365

5664.52 m

5664.581

6664.77 a

5665.00 a

5665.343 6665.563m

5665.920

5666.686

5666.794

35

1. 5

1. 5

0. 5

4. 5

1. 5

1

2

40

1. 5

22

6

6. 2

0. 3

0. 3

0. 1

0.8

0.3

0. 2

0. 4

7. 2

0. 3

3. 9

1. 1

s

s

8

S

w, N

w

u1

Ni I |Cr I

Zr I

Cr I

Si I AtmHjO

Si I

Fe I

4. 54

3. 43

0. 63

3. 82

4. 92 R 3

5. 61

/4. 15

272

203

47

10

203

1053 1060

13

16

26

6659.784 1. 5 0.3

246
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- It.;- Low RMT

Wave- valent duced Solar E P No. Wave- vakjnt (Inccd Sohtr E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot IdfTiti- or or Notes AX AX/X fication Rot. Vib, AX AX/X fication liot. Vib. (A) (mA) (F) Line B;ind (A) (ml) (F) Line Band

5667.153 25 4. 4 w? Sc II 1. 50 29 5678.003 1 0. 2 Fe I p 4. 98 1200

5667.328 2. 5 0. 4 5678.390 5 1. 2 0? Fe I p 3. 88 082 17

5667.524S 48 8. 5 u Fe I 5678.609 3. 5 0. 6 M Fe I p 2. 42 113

5667.786 3 0. 5 5678.808r 1. 5 0. 3 Atm

5668.091 2 0. 4 5679.032S 58 10. 9 U Fe I 4. 65 1183

5668.369 5 1.S, d1 V I 1. 08 37 5679.284 3. 5 0. 6

5668.916 3 0. 5 Ce II- 1. 01 23 5679.604r 1 0. 2 Atm

C I? 8. 53

5679.70 a 1. 5 0. 3 5669.040m 34 6. 4 w Sc II 1. 50 29 5679.933 6. 5 1. 1 s Ti I 2. 47 269

5669.251 2 0. 4 5680.248 10 1. 8 u,N Fe I 4. 19 1026 5669.746 19 3. 4 w, N Si I 5. 62

5680.551r 0. 5 0. 1 Atm?

5669.950 16 2. 8 u Ni I 4. 26 250

5680.760r 1 0. 2 Atm

5670.153 1 0. 2 5680.91 m 1 0. 2 s Zr I 0. 54 25 5670.358 1 0. 2 Atm

5681 068 4 0. 7 Cr I? 5670.858 16 3. 0 S V I 1. 08 36

5681.237 5 0. 9 u Cr I? 5671.073 2 0. 4 5681.529 3 0. 5 5671.491 9. 5 1. 7 w

5681.747 1

f 0. 4 Atm

5671.826 14 2. 5 S Sc I 1. 45 12 J 5681.813r J 1 0. 4 Atm?

5672.266 3 0. 5 Fe I 4. 58 1234 5682.208m 52 9. 7 w? Ni I 4. 10 232

5672.807 1 0. 2 5682.493 7 1. 2 u Cr I 3. 84 239

5673.059 1. 5 0. 3 s Ti I? 5682.647m 104 18. 5 s Na I 2. 10 6 5673.422 3. 5 0. 6 s Ti I 3. 11 5683.006 |8| 1. 4 u

5673.75 a 1. 5 0. 3 5683.25 a 3 0. 5 5673.982r 1. 5 0.3 Atm?

5674.170 2. 5 0. 4 Cr I? 3. 55

5683.4V 9r 8 1. 4 u

s 5683.782 3 0. 5 Atm

5674.280r 2 0. 4 Atm

5683.878 8 1. 4 Atm H2O R 7 203 26

5674.45 a 2 0. 4 5684.198m 37 6. 9 w Sc II L 51 29 5674.623 4. 5 0. 8 5684.493m 63 11. 2 w Si I 4. 95 11 5674.88 a 3. 5 0. 6 5684.733 3. 5 0. 6 5675.092 |7. 5i 1. 3 s Fe I p 3. 30 583

5685.033r |2| 0. 4 Atm

56/5.434m 71 12. 5 s Si 1 5. 62

Ti I 2. 30 249 5685.438 3. 5 0. 6 Atm H2O R 6 203 26

5675.732 12 2. 1 u,N Si I?- 5. 62 16 5685.779r 1 0. 2 Atm?

6676.105 3. 5 0. 6 5685.881 2 0. 4 Fe I p 4. 99 1281

5676.351 3 0. 5 5686.155r 1 1

0. 7

5676.790 2 0. 4 AtmHaO R 5 203 26 5686.207 } 1 4.w Fe I?

5676.957 1. 5 0. 3 5686.360 10 1. 8 u Rh I? 1. 68

5677.462 1. 5 0. 3 5686.540m 72 12. 7 u Fe I 4. 55 1182

5677.695 6. 5 1. S u Fe I p 4. 10 1057 5686.839 12 2. 1 s Sc I 1. 44 12

247
The Solar Spectrum—Continued

length

(A)

Equi-

\7 0 1 PTl "f. Width

AX

(ml)

Rer\ 1 1 pprl Width

A\/X

(F)

Spot

Solfir Identifi p 0 t.i nn

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes length

(1)

Equiv3;lGnti Width

AX

(ml)

Re- Width

AX/X

(F)

Spot

SoIrp

Identi-

"fi f*fi t i on

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

2 0. 4 0. 2 Xi. Atmu Ail H.,0 XA 2 R 3 203 26

5687.32 a 2. 5 0. 4 5697.579r 1. 5 0. 3 Atm

5687.486 |12| 2. 1 Atm H2O R 3 203 26 5697.832r 1. 5 0. 3 Atm?

5687.617 3 0. 5 Atm? 5698.027 14 2. 4 u Fe I 3. 64 867

5688.217m

5688.535

5688.598

121

1

24

•J

19

22. S

4. 2

0. 5

n 4

1. 9

M?

Nai

(Nai)

fNdii

[Atm

Co I

Atm?

Ti I

2. 10

2. 10

0. 99

2. 08

2. 30

6

6

79

90

249

5698.194

5698 340m

5698.530m

5698.695

5698.887

5699.321

8. 5

30

34

4. 5

2

7

1. 5

5. 3

5. 8

0. 8

0. 4

1. 2

s

S

AtmHaO

llCri Fe I V I AtmHsO

Atm H2O

CFpx: e t") x;

R 2

3. 88

4. 29

1. 06 R 2

R 1

203

239

1130

35

203

203

26

26

26

u 1. 1 Atm H,0 R 4 203 26 'ifiQQ 494 4 n 7 U

tlUO t/ • t3 U J. 2 n 4 A.tin I 0 9

5690.070 1 0. 2 Fe ip 5. 01 1281 5699.76 a 1 0. 2

6690.228 4 0. 7 Atm H2O R3 203 26 5700.186

1 29

1

2. 6 s Sc I 1. 43 12

5690.433S 53 5. 7 W Si I 4. 93 10 5700.284 I 2. 6 s Cu I 1. 64 2

5690.957 3. 5 0. 6 Cr I? 3. 10 5700.524 6 1. 1 s,N Cr I /3. 45

1.0. 00 203

228

5691.08 a

to 5691.38 a 5691.505m

1

5. 5

38

1. 0

7. 0 u NiiII Fe I4. 10

4. 30 228

1087

'\7(\(\ 797

^7(\C\ Q9n

5701 108m 40

1X . 71 n 4

7. ;S

zo

TV Si I

R 1

4. 93 10

2fi

5. 5 1. 0 Fe I p 4. 22 1084 4 n 7 S X \J

KfiQO 424 9. 5 1. 7 R 3 203 26 Sfi ou i-O fl . V S

TTp X c TX 9 ^fi 209

2. 5 0. 4 (J ( (JX , 1 to 2 0 4

RVI1 1 1 . X 0 t \jx *OJO K0 Atm H„0 JX X 0\j\J 9R

9 =1 0. 4 C I 0. 00 9 fl 4

00 U. 6 5702. o^8m 27 4- 7 s Or I 3. 45 203

48 8. 6 Fe I ^1709 fn^^ 1i.. 0^ u. 0

569.^ 0. 2 f V/^ .UU X 7 1X. ^9 0SI Tl T 2. 29 249

2 0. 4 Atm TT,0 R 3 ^^709 7Q7r 0id n 4 £\. Li.il 5694 744 19 3. 3 Cr I Sfi ^7CiO Q1 7 R 1 1 X. X w7

5694.991m 41 7. 6 w Ni I 4. 09 220 5703.090 2 0. 4 Fe I p 4. 19 1053

5695.241r 3. 5 0. 6 Atm? 5703.223 3 0. 5 Atm H2O R 1 203 26

5695.959 2. 5 0. 4 Atm H,0 R 2 203 26 5703.382 1. 5 0. 3

5696.099

5696.367r

5696.652

5696.824

13

3

3. 5

5

2. 3

0. 5

0. 6

0. 9

w,N

u,N

Fe ip

Fe II p

S I? AtmHjO

4. 55

2. 64

7. 86 R 3

1179

18

11

203 26

5703.587m

5703.697

5703.882

5704.212r

26

5. 5

1. 5

1

4. 6

1. 0

0. 3

0. 2

s V I Ni I

Atm H2O

1. 05

3. 94

Q4

35

203 26

248
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

bpot

Solar

T ^1 - J Identification

how

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(mA)

lie- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5704.390 0. 5 0. 1 .5713.11a 2 0. 3

5704.57 a 1 0. 2 5713.458 2 0.3

5704.740 21 3. 7 W Fe I 5713.896 5 0. 8 S Ti I 2. 29 249 17

5705.066r 0. 5 0. 1 Atm? 5714.060r 1. 5 0. 3 Atm H2O Q 1 203 26

5705. 309r

5705.473m

5706.008m

5706.108

5706.34 a

5706.715

5706.982

5707.048

1

37

74

25

5. 5

14

0. 2

6. 8

13. 0

4. 4

1. 0

2. 4

{[ 5.

UW

w,N

w,N

S

u

Atm?

Fe I p

Fc I Fe I Fe I p

V I Fe I

4. 22

4. 30

4. 61

4. 28

1. 04

3. 64

1058

1087

1183

1088

35

868

5714.159

5714.397

5714.554

5714.744

5714.901 5715.094m

5715.318

21

2

7. 5

1

1. 5

73

2. 5

3. 7

0. 3

1. 3

0. 2

0. 3

13. 1

0. 4

u

0

s!

Fe I

Fe I p

JN 1 I Fe I Ti I

3. 24

4. (jy

r4. 19

14.

2. 25

552

1061 lOOD 228

5707.245 4 0. 7 Fe I p 3. 64 866 5715 471 4 0. 7 u Fe I p 4. 15 1054

5707.398

5707.713

5707.921 5708.102m

5708.214 5708.405m

5708.663

5708.892?

5709.110 5709.386m

5709.555m

5709.779

5709.929

5710.297

57l0.800r 5711.095m

5711.398r

Oi il.o4or

0/11.7o m

6711.884m

1. 5

1. 5

1

37

4

77

6

6

4

103

90

3

12

1

6

107

8. 5

6

3. 5

77

0. 3

0. 3

0.2

6. 5

0. 7

13. 7

1. 1

1. 1

0. 7

18. 0

15. 8

0. 5

2. 1

0. 2

1. 0

18. 9

1. 5

0. 5

0. 6

13. 5

w

Sw

S

s

s

s?

u

u

o,iV

s

Fe I p

Fe I

Ti I

Si I

Sc I

Fe I Ni I

Fe I p

Atm H2O

Mg 1 Atm H2O

Atm II2U !

be I

|li 8 I Ni I

4. 10

4. 43

2. 32

4. 95

1. 45

3. 37

1. 68

4. 26

R 1

4. 34

Q 2

1. 43

4. 28

1. 93

1056

1161

249

10

12

686

46

1088

500

8

203

500

12

1087

69

26

26

zo

5715.821

5716.226 5716.455m

5716.970r

5717.311

5717.508

5717.695 5717.841m

5718.122

5718.294r

5718.60 a

5718.938

5718.992r

5719.320r

5719.584

5719.718

5719.828

5720.450

5720.54 a

5720.722

3. 5

2

6. 5

1. 5

2. 5

7. 5

3. 5

63

4

4. 5

} ^

3. 5

5. 5

1

5

3. 5

3

0. 5

0. 6

0. 3

1. 1

0. 3

0. 4

1. 3

0. 6

11. 2

0. 7

0. 8

0. 2

J

0. 8

I 0. 1

0. 6

1. 0

0. 2

0. 8

0. 6

0. 5

0. 1

s

S,d

S

u

0

s s,N

Ca I Fe I p

Ti I Atm

Sc I AtmHaO

Fe I Nd II? — Atm?

AtmTEjO

AtmHzOAtm?

IIAtmHaOAtmHjO

Cr I

Ti I AtmHaO

2. 71

4. 56

2. 30

1. 44 Qi

4. 28

1. 41

Q4

Q 3

Q 2 Q 3

3. 01

2. 29 Q 2

1198

249

12

203

1107

86

203

500

203

203

119

249

203

26

26

26

26

26

26

5712.138m 54 9. 8 w? Fe I 3. 42 686 5720.898 14 2. 4 u Fe I p 4. 55 1178

5712.400 3 0. 5 5721.053 2 0. 3

5712.627

5712.778

5

17

0. 8

3. 0

s

s

Cr I Cr I

4. 53

3. 01 119

5721.706 4. 5 0. 8 Fe I p

/4. 15

14. 28

1057

1088

249
The Solar Spectrum—Continued

length

(A)

EquiWidth

AX

(ml)

Rediiocd Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

^Vavelength

(A)

Equivalent. Width

AX

(ml)

ReH n ppH

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

tj I ^ 1. .00 -L X 2 0. 3 Atm H2O 0 ] 500 26 5731 552 I 0. 2

3 0. 5 Atm H2O P 1 203 26 5731 772S 59 10. 1 iv Fe I 4. 26 1087

K722 1 Sir 1. 5 0. 3 Atm 5731 996 2. 5 0. 4 ^722 510 2. 5 0. 4 5732.121 0. 2

5722.781 1 0. 2 5732.304 15 2. 6 w? Fe I p 4. 99 1313

J 0. 2 Atm? 5739 57fir 1. 5 0. 3 Atm H2O 0 1 500 26

572S 54R 1. 5 0. 3 5732 730 3. 5 0. 6 Fe II p 3. 39 57

572.^ fi71

572 77.^

4

3. 5

0. 7

0. 6

] s,N

J

Fe I 4. 47 1160 5732 881

5733 092r

3. 5

3. 5

0. 6

0. 6

Fe I p Atm H2O4. 10 P 2

1055

203 26

5723 895 4 0. 7 AtmH20 Q 3 203 26 5733 332 1. 5 0. 3

5724 095 1. 5 0. 3 s Sc I 1. 43 12 5733 694r 1 0. 2 Atm H2O Q 5 203 26

5724 4fifi 5 0. 8 Q Fe I 4. 28 1109 5733 KJ 1 0(J .OCX 891 0. 5 0. 1 Gd II 1. 37 94

5725 008 0. 5 0 1 V/. J- 5734 048 4 0. 7 g V I 2. 36 135

5725.298 0. 5 0. 1 5734.355 1. 5 0. 3

5725.36 m 0. 5 0. 1 S 16 5734.569 6 1. 0 w

5725.658 2 0. 5 s Vi 2. 36 135 5735.574 4. 5 0. 8 Atm H2O Q4 203 26

5725.953r

5726.489

5726.705 5726 885

5727 057in

5727 286

5727 467

2. 5

1

1. 5

4

37

]^

0 5

0. 4

0. 2

0. 3

0. 7

6. 5

0. 2

0. 1

s

Fe II p —

Atm

Atm H2O

Atm HoO

V I

3. 42

Q 3

1. 08

57

203

203

35

26

26

5735.713

5736.028

5736.644

5737.073

5737.316r

5737.476

5737.691

7. 5

1. 5

4

11

1. 5

1

8. 5

1. 3

0. 3

0. 7

1.9

0. 3

0. 2

1. 5

s

S

0?

Zr ICr I V I Atm H2O

Atm H2O

Fe II p

0. 00

3. 56

1. 06 Q 5

P 3

3. 42

4

228

35

203

20358

26

26

5727 661 7 5 S s V I 1. 05 35 5737 90 a 0. 2 Kin 882 0W. *J^ 0. 1 5738 240 13 2. 3 It Fe I 4. 22 1084

5728.106 1 0. 2 5738.479r r 0. 4 Atm?

5728.26 a 1 0. 2 5738.552 } *

1 0. 4 s Cr I 3. 55 227

5728.527r 3 0. 5 Atm H2O Q4 203 26 5739.061r 1 0. 2 s,N Ti I p 2. 30 249

5728.877

57 2Q 202

4. 5

3

5 5

0. 8

0. 5

1 0

0 Atm —

II Y TT

II iCr T Atm HoO

1 84

3 34 P 2

34

257

9fi

5739.244 5739.483m

5739.807r

0. 5

6. 5

0. 5

0. 1

0. 1

s Ti I Atm?

Fe I p

2. 25

4. 19

228

1057

572Q 822 9 0 Atm TTnO P 2 203 26 s7Qq 007 7 1. ^ Ti I 2. 24 228

5729.901r 0. 5 0. 1 Atm H2O Q4 203 26 5740.158 0. 5 0. 1

5730.862 7 1. 2 w,d1 5740.369r 0. 5 0. 1 Atm

5731.037 I 0. 2 5740.606 0. 5 0. 1

5731.220

6731.323

7. 5

3. 5

1. 3

0. 6

S

S

Vi 1. 06 36 5740.875r 2 0. 3 Atm

Nd II? 1. 16 86

250
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

Wa\'Cleiigth

(A)

E(|ui- valcnt

Wi.lth AX

(ml)

!;(;- duced

Width

AX/X

(F)

S])ot Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or Vib. Band

Notes

5741.219r

5741.400

5741.502r

5741.712

5741.856S

5742.079

5742.212

5742.572r

5742.812

5742.968

5743.195

5743.432

5743.561r

5743.748r

5743.940

5744.202

1. 5

2

10.51

0. 5

31

2. 5

4. 5

2. 5

1

12

7

8

1

1. 5

4

0. 5

0. 3

0. 3

0. 1

0. ]

6. 6

0. 4

0. 8

0. 4

0. 2

2. 4

1. 2

1.4

0. 2

0. 3

0. 8

0. 1

S

u

w?

uS

Ti I Atm?

Fe I

Atm H2O

Atm —

Fe I

V I Atm H2O

Atm H2O

2. 50

4. 2G

P 3

4. 18

1. 08 P 3 Q 3

280

1086

203

1084

35

203

500

26

26

26

.5749.641

5750.057r

5750.216

5750.5]0r

5750.643

5751.145

5751.42 m

5751. 8C5r

5752.042S

5752.246r

5752.86 m

5752.892r 5753.132m

0/ Oo.oUO

0 / oo.D4oni C7CQ non

2

2. 5

1

1

1

4

1

3

56

3

1 "

78

D. 0

0. 3

0. 4

0. 2

0. 2

0. 2

0. 7

0. 2

0. 5

10. 1

0. 5

1. 3

14. 6

2. 1

5. 0

1. 1

s,N

sw1

8

U

w,N

s

Fe I p Atm

Atm

Mo 1? Atm HiO

Fe I -Atm?

1 AtmHjO

Fe I Fe I p

01 I

r e I p Atm?

4. 43

1. 42 P 4

4. 55

2. 24 P 4

4. 26

A OP. 4. ZD

K *^ 1 0. Di

0 A K

1160

5

203

1180

214

203

1107

1 (\Q.A lUo4

1 7n 1 / U

26

13

26

1 A10

5744.470 1 0. 2 Ti 1? 3. 21 5754.093 7. 5 1.3

5744.782r 3 0. 5 Atm H2O? P 3 500 26 5754.235 12 2. 1 w Si I 4. 95 10

5744.952r 3. 5 0. 6 Atm H2O P 3 203 26 5754.411 18 3. 1 u Fe I 3. 64 866

5745.077r 1. 5 0. 3 Atm 5754.666m 73 13. 4 s Nil 1. 93 68

5745.278r 1 0. 2 Atm 5754.922 4. 5 0. 8 Fe I p 2. 48 113

5745.493r 1 0. 2 Atm 5755. 157r 6 1. 0 Atm

5745.7l9r 2 0. 3 Atm H2O P 4 203 26 5755.372r 2 0. 3 Atm

5745.793 6. 5 1. 1 Atm H2O P 4 203 26 5755.488r 2 0. 3 Atm

5746.422 3. 5 0. 6 s Cr I 3. 85 243 5755.757r 1 0. 2 Atm

5746.812r 3 0. 5 — Atm 5755.969 1 0. 2 Atm

5747.289r |3| 0. 5 Atm H2O Q2 500 26 5756.40?m s Ti I 2. 25 228 13

5747.41 a 2. 5 0. 4 5756.60 a 1 0. 2 5747.669m 35 6. 1 w,N Si I 5. 61 5756.828m 28 5. 0 w1

5747.858 7 1. 2 Cr I Fe I p Fe I Fe I p

Ni I

Vi

Ni I

3. 89

2. 83

4. 61

5. 01

1. 68

1. 89

3. 94

343

1182

1290

45

92

176

5757.080r 1. 5 0. 3 Atm

5747.955m

5748.170 5748.361m

5748.524

5748.725

5748.899

5749.298

35

2

26

2. 5

1. 5

2. 5

6

6. 1

0. 3

4.5

0. 4

0.3

0. 4

1. 0

u

s

sw? 17

5757.948r

5758.280r

5758.441r

5758.764

5758.907r 5759.02?m

5759.125r

1. 5

1. 5

1. 5

2. 5

1. 5

0. 5

1

0.3

0. 3

0.3

0. 4

0. 3

0. 1

0. 2

s

Atm H2O

Atm

Atm H2O

Atm H2O

Cr I Atm

Q4

P 2

P 4

500

500

203

26

26

26

251
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

bolar

Identification

Low

T? "D Hj Jr or Rot. Line

RMT

JNo. or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

hi ir or Rot. Line

RMT

JNo. or Vib. Band

Notes

5759.273 6. 5 1. 1 w Fe I 4. 65 1184 5771.828 1 0. 2

5759.545

5760.359m

5760.532

5760.701r

10

18

3. 5

1. 5

1. 7

3. 6

0. 6

0. 3

w,N

u

u

Fe I

Fe I Fe I p

Atm?

Fe I p

/4. 30

14. 56

3. 64

4. 15

4. 15

1087

1204

867

1054

1056

5772.149m

K'T'TO /I 1 K

0 / /z.oobr

0/ /z.o/4

5772.941r

47

Z. 0

1. 5

2

1

8. 5

0. 7

0. 6

0. 3

0. 2

w

s

Si I Vi

Atm H2O

Cr I Atm

5. 08

1. 93 P D

3. 56

17

92

203

227

26

5760 841

S

28 5. 6 Ni I 4. 10 231 5773. 149r 1 0. 2 Atm H2O P 7 203 26

5761 091 2. 5 0. 4 Fe I p 4. 22 1057 5773 504r 2 0. 3 Atm —

5761 270

5761.424

2. 5

0. 5

0. 4

0. 1

Fe I Atm?

V I?

3. 63

1. 06

867

35

5773 769

5774.038

0. 5

9

0. 1

1. 6 s

r n I 3. 30 309

5761 5SS 7 1. 2 Atm H9O — P 5 203 26 5774.240 5 0. 8 0

5761 854 1 0. 2 5774.38 a 2 0.3

5762 266 7 1. 2 s Ti I 3. 28 309 5774.547 2. 5 0.3 Atm

Ti I? 2. 25 228

5762.423m 22 3. 8 Fe I 3. 64 866 5774.803 0.5 0. 1 5762. 626r 3 0. 5 UyN Atm —

5775.088m 48 9.4 u Fe I 4. 22 1087 5762 845 10 1. 9 Q Fe I p 4. 30 1086 5775.305 2. 5 0. 4 5763.002m 101 17. 5 u Fe I 4. 21 1107 5775.617 1 0. 2 5763. 246r 1 0. 2 Atm H2O P 6 203 26 5775.755r 0. 5 0. 1 Atm

5763 410 8. 5 1. 5 Atm H,0 P 6 203 26

5776. 079r 1. 5 0.3 Atm H2O P 5 203 26 5765 866r 1 0. 2 Atm

5776.254r 2. 5 0. 4 Atm

5766. 271r 1

> 8. 5

f 0.

2

— Atm H2O P 5 500 26 5776.744r 1. 5 0. 3 S,d Vi?- 1. 08 36

5766.333 J1 13 Ti I 3. 29 309 5776.978 2 0. 3 Atm

5766 592 0. 5 0. 1 5777.07 a 1. 5 0. 3 Cr I? 5767. 144r 121 0. 4 Atm H2O P 5 203 26

5777.521 1 0. 2 5768. OUr 1. 5 0. 3 Atm

5777.762 1. 5 0. 3 Cr I 3. 85 257

5768.361r 1 0 2 Atm

5778.296 1 0. 2 5768.902 1 0. 2 Ce II? 1. 32 32 5778.463m 16 3. 1 s Fe I 2. 59 209

6769.081r 2. 5 0. 4 5778.676r 1. 5 0. 3 — Atm

5769.28 m

5769.335 }

' 1. 2 U

Atm H2O

Fe I

P 5

4. 61

203

1179

26 5778.811r 1 0. 2 Atm?

Fe I p 4. 56 1203

5769.482 1 0. 2 5779.098 1 0. 2

5769.686r 1. 5 0.3 Atm 5779.369r 1. 5 0. 2 I^tm

5770.191r

5770.305

5770.500r

5771.381r

1

1. 5

1. 5

1. 5

0. 2

0. 3

0.3

0.3

U

Atm H2O

Fe I p

Atm

Atm

P 5

4. 58 2031236a

26

16

5779.564

5779.696

5779.963r

5780.167

1

3. 5

2

3. 5

0.2

0. 6

0. 3

0. 6

I

I

1

Itm

^tm H2O

VIn I P 6

4. 25

203 26

5771.608 6. 5 1. 1 s 5780.306 4 0. 7

252
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RAIT

vjilent ducGci Solar E P No. vfT ion t, f 1 u cod Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fiCtition Rot. Vib AX AX/X fication Rot. Vib.

(A) (ml) (F) Line Band (A) (mA) (F) Line Band

5780.388 22 3. 8 w Si I 4. 92 9 5787.730 0. 5 0. 1

5780.608ni 29 5. 0 u Fe I 3. 24 552 5787.926m 36 7. 1 s Cr I 3. 32 188

5780.812 21 3. 6 s Ti I- 2. 25 214 5788.102m 2. 5 0. 4 Atm O2 R 13 3,0 22

f3. 26 552

|li e I 3. 69 922 5788.187m 1 0. 2 Atm O2 T> 1 1 K 11 0 A

3,U 22

[4. 43 1159 5788 289m 0. 5 0. 1 Atm O2 R 15 3 0 22

5780.919 6. 5 1. 1 s Cr I 3. 32 188 5788 394 5 0. 8 Cr I 3. 01 119 5781.067 0. 5 0. 1

/3. 01

l3. 32

119 188

5788.549m 1. 5 0. 3 Atm O2 R 9 3,0 22 5781.187 12 2. 1 s Cn 5788 61 m V I 1. 87 92 13

5781.359 2. 5 0. 4 5788.650r 0. 5 0. 1 Atm

X 0. 2

- 5788.763m r 0.11 Atm O2 R 17 3,0 22

tj 4 OX t * xjO 16 2. 8 s,d? Cr I 3. 32 188 5788.801m J 0 1 Atm O2 R 13 3,0 22

5781.923 3. 5 0. 6 5788.877m 1 0. 2 Atm O2 R 11 3,0 22

ir-il 5782.136 62 10.7 s Cu I 1. 64 2 7 5788.995m 1 0. 2 Atm O2 R 15 3,0 22

5782.371 3 0. 5 K I 1. 61 5789.189m f 0. 2 Atm O2 R 7 3,0 22

5782.601 1 0. 2 s,N Vi fl. 08

12. 38

35

127 5789.234m

5789.350r

\ I. 0

0. 5

1 0. 2

0. 1

Atm O2 Atm

R 9 3,0 22

5782.863 0. 5 0. 1 JR 17 1r19

3,0

3,0 5789.489m 1 0. 2 Atm O2 |22 5783.073m 24 4- 7 s,d Cr I 3. 32 188

5783.248 1. 5 0. 3 5789.635r 0. 5 0. 1 Fe I Aim I 5783.485 0. 5 0. 1 0 /oy. /Dor U. 5

n "I U. 1 s ill.' 5783.676 0. 5 0. 1 o/oy.5Dom 1 U. R 7 ^o,un 99 5783.866m 34 6. 6 s Cr I 3. 32 188 o/oy.y / ir (J. 0

Ci 1 A fm

5784.051 2 0. 4 o/yu.iUim 1 n o U. J> ±x 0 99

5784.385 1 0. 2 s Vi 2. 77 141 o/yu.io m aO 1. Ueo

5784.ODom 20 4- 1 u Fe I 6. W OoO 5790.227m 1. 5 0. 3 Atm O2 R 19 3,0 22

5784.822 1 0. 2 5790.366r 1 0. 2 5784.976m 26 6. 4 s Cr I 3. 32 188 5790.534m 1 0. 2 Atm O2 R 21 3,0 22 5785.285m 40 7. 8 w Mgi 5. 11 24 5790.663r 2 0. 3 s Cr I 1. 00 17 Fe I

5785.561 u1 Mgi 5. 11 24 5790.769m 2 0. 3 Atm O2 R 5 3,0 2212 2. 1 5785.735m Cr I 3. 32 188 5790.990 • 74 12. 8 s Cr I 3. 32 188 7 24 4. 1 s X: Ki L

"i 91

o t oo.yrt in <1 Cr I /O. 97

10. 98

17

17 ll3 5791.191 4. 5 0. 8

5785.980 11 1. 9 s Ti I 3. 32 309 0/y i.-^ycsm QO U. 0 Aim A +rr> CiKJ2 /R3

\R21

3,0

3,0 I99

5786.159 0. 3 Vi

("9 79 1 41 5791 405r

0 / yi.ooo

1 0. 2

1 0

Atm

2 s \2. 74 141

71 Ujd Fe I p

5786.536 0. 5 0. 1 5791.760 4 0. 7 s Cr I 3. 85 243

5787.021 6 1-4 s,d llCri 3. 01 119 Fe I 0. 2 p 4. 26 1084 5791.92 m 1 s

5787.275 0. 5 0. 1 Fe I p 3. 25 625 5791.946m 1 0. 2 Atm O2 R 3 3,0 22

253
The Solar Spectrum^—Contin ued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E r

or Rot. Line

EMT

JNo. or Vib. Band

Notes

5792. 096r 0. 5 0. 1 Atm

5792. 190r 0. 5 0. 1 s Cr I 0. 96 17

5792.7D9ni 0. 5 0. 1 Atm U2 K 1 o,U 22

5792. 790r 1 0. 2

5792.87c) 0. 5 0. 1 5793.079m 38 7. ;g w,N Si I 4. 93 9 5793.411m 4. 5 0. 8 Atm O2 R 1 3,0 22

5793. 705r 2. 5 0. 4 Fe I p 4. 59 1236a 5793.922m 28 5. ;g u Fe I 4. 22 1086

5794.168 1. 5 0. 3

5794.348 0. 5 0. 1

5794.455 1 0. 2 C 1? 7. 94

5794.624 1. 5 0. 3 Cr I? 4. 53

6794.999 0. 5 0. 1

6795.292 0. 5 0. 1

. . .:.

6795.884 2 0. 3 • n 6796.092m 6. 5 1. 1 u Atm O2 Ni I p 1

1. 95

3,0 68

22

6796.422 1 0. 2

5/96.671 2 0. 3 Fe I p 4. 19 1054

5796.770 2. 5 0. 4 s Cr I 4. 53

6797. 282r 0. 5 0. 1 Atm

5797.436 2 0. 3 s Ti I 3. 30 309

5797.530m l 2. 5 0. 4 Atm O2 P 3 3,0 22

5797.55 m J s Cr i?p 3. 10 185 13

5797.601 1. 5 0. 2 La II 0. 24 4

5797.751 2 0. 3 S Zr I 0. 07 4 6797.865m 32 5. 5 W,N Si I 4. 95 9

5798.010 3. 5 0. 6 Atm

5798.182m 37 6. 4 s Atm O2

IIFei P 3

3. 93

3,0

982

22

5798.513r 2. 5 0. 4 s Cr I 1. 03 17

5799.150 0. 5 0. 1 Atm

5799.840r 1. 5 0. 3 Atm

5799.90 m s 13 5799.963m 1. 5 0. 3 Atm O2 P 5 3,0 22

5800.228r 4. 5 0. 8 Atm —

5800.640m 7 1. 2 Atm O2 P5 3,0 22

5800.842r 2 0. 3 Atm

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5801.271 5. 5 1. 0 u,d

5801. 749r 1. 5 0. 3 K I 1. 62

5802. 330r 0. 5 0. 1 5802.663m 1 0. 2 Atm O2 P 7 3,0 22 5803.327m 1 0. 2 Atm O2 P 7 3,0 22

5803.590 1 0. 2 5804.038m 20 3. 4 u Fe I 3. 88 969

5804.266m 12 2. 1 s Til 3. 34 309

5804.462 18 3. 1 w,N Fei 4. 28 1087

5805.030 0. 5 0. 1

5805.226S 38 6.6 w Nil 4. 17 234

5805.419 2 0. 3 6805.631m 1 0. 2 Atm O2 P 9 3,0 22

5805.769 11 1. 9 u Fei

(La 11)

5. 03

0. 13 1313

4

5805.98 m 0. 5 0. 1 Atm

5806.289m 2 0. 3 Atm O2 P 9 3,0 22

5806.534 0. 5 0. 1

5806.732m 51 9. 1 u Fe I 4. 61 1180

5807.097 2 0. 3

5807.14 m s V I 3. 09 142 13

5807.249 0. 5 0. 1 Fe I p 3. 24 581

5807.30 m s 13

5807.792 7. 5 1. 3 u? Fe I 3. 29 552

5807.992 3. 5 0. 6 Fe I p 4. 61 1178

5808.190r 1 0. 2 s Cr I?

5808.314 0. 5 0. 1 La II? 0. 00 4

5808. 565r 0. 5 0. 1 Atm?

5808.878m 1 0. 2 Atm O2 P,ll 3,0 22

5809.040 0. 5 0. 1

5809.224S 60 8. 6 u Fei 3. 88 982

5809.451 1. 5 0. 3 5809.523m

5809.614 } =

f 0. 8

1 0. 2

Atm O2 P 11 3,0 22

5809.873 |2.5| 0. 4 Fe 1 p 4. 28 1084

5810.08 a 1.5 0. 3

5810.38 a 1 0. 2

254
The Solar Spectrum—Continued

length

(A)

Equivalent Width

AX

(mA)

Reduced. Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

Wtivelength

(A)

Equivalent Width

AX

(mA)

Red uced Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5810.792 6.5 1. 1 w 16 5820.912m 1 0. 2 Atm O2 P 17 3,0 22

5811.00 a 2.5 0. 4 5821.30 a 1 0. 2

5811.117 |1| 0. 2 5821.890 7 1. 2 u

5811.606 5.5 1. 0 s,N 16 5822.465 5. 5 1. 0 s

5811.919 10.5 1. 9 u Fe I 4. 14 1022 5822.863 0. 5 0. 1

5812.131 1 0. 2 Ki 1. 61 5823.176 2 0. 3 Fe II 5. 57 164 5812.400m ]

[ 2.5

f 0. 4 Atm O2 P 13 3,0 22 5823.366 1 0. 2

5812.502 ( a: 5823.695 3 0. 5 S Ti I 2. 27 239

5812.839 2.5 0. 4 s Til 3. 32 309 5824.173 1. 5 0. 3 5813.041m 4 0. 7 Atm O2 P 13 3,0 22 5824.414 2. 5 0. 4 Fe II p 3. 42 58

5813.339 2 0. 3 Fe I p 4. 19 1054 5824.636m 1. 5 0. 3 Atm O2 P 19 3,0 22

5813.670 |5| 0. 8 0 Fe H 5. 57 163 5825.755 4 0. 7

s,d 5813.81 a 1 0. 2 5825.81?m 1 0. 2 Cri 0. 96 17

5813.97 m S Til 1. 07 73 13 5826.110 0. 5 0. 1 Fe 11? p 5. 91 182

5814.006 6.5 1. 1 u,N 5826.330 1 0. 2 Co I 3. 62 169

5814.570 0.5 0. 1 5826.646 3. 5 0. 6 s Fei p 4. 28 1084 16 5814.815m 21 3. 6 s Fei 4. 28 1086 5827.086 1 0. 2

5815.029 0.5 0. 1 5827.377 2. 5 0. 4

5815.224

5815.448

5815.546

5815.650

5815.868

5816.068 5816.263m

5816.380S

5816.631 5816.833m

10

0.5

0.5

3.5

1

12

1 85

0.5

3

1. 7

0. 1

0. 1

0. 6

0. 2

2. 1

1

3. 6

1 11. 3

0. 1

0. 5

u

0?

w

u

si

u,N

Fei

Fe I p

Cri?

rei?p

Atm O2 —

Fei

Atm O2 — Mm

/4. 15

14. 59

4. 22

3. 85

4. 29 P 15

4. 55

P 15

4. 26

1055

1234

1053

1127

3,0

1179

3,0

22

22

5827.475

5827.682r

5827.884

5828.245r

5828.765

5829.147

5829.44 a

5829.983

5830.090r

5830.684

5831 253r

5

2

9. 5

0. 5

2. 5

0. 5

1. 5

2

3. 5

3

0. 5

0. 8

0. 3

1. 7

0. 1

0. 4

0. 1

0. 3

0. 3

0. 6

0. 5

0. 1

u

u

s

— Atm

Fe I p Atm H2O

Atm H2O

V I Atm

3. 28

R' 6

R' 4

3. 11

552

321

401

142

16

26

26

s VV T1 — OoO i .UuDin 99 0. 0 IN 1

14. 17

14. 23 233 250

5817.381 1.5 0. 3 5831.753 4 0. 7

5817.493 2 0. 3 8 Vi 3. 10 142 5831.938 0. 5 0. 1 s,N Ki 1. 62

5818.173 0.5 0. 1 Atm 5832.01 ?m 1 0. 2 s,N

5818.279

5819.302

5819.564

5819.931 5820.278m

0.5

1.5

2

13.51

0. 1

0. 3

0. 3

0. 6

0. 4

Atm

Vn

Atm O2

2. 52 P 17

99

3,0 22

5832.275

5832.480

5832.978

5833.52 a

0. 5

2

2

1. 5

0. 1

0. 3

0. 3

0. 3

s Til 3. 34 309

25.5
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

1 Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5833.670 0. 5 0. 1 Fe II 5845.750r 1 0. 2 Atm?

5833.937 3 0. 5 s,N Fe I p 2. 61 209 5845.970 5 0. 8 w

5834.036 14 2. 4 s Fei 5846.272 5 0. 8 s,d -Vi 3. 13 142 17

5834.225r 1 0. 2 5846.569 2 0. 3 Co I 3. 57 169

5834.537 1. 5 0. 3 5846.799 0. 5 0. 1

5834.855r 1. 5 0. 3 5847.006m 19 3.4 s Nil 1. 68 44

5835.109 12 S. 2 w? Fei p 4. 26 1084 5847.719 1 0. 2 Atm H2O R' 4 321 26

5835.262 1. 5 0. 3 Fei 5847.893 1 0. 2

5835.434

5835.588

8

7

1. 4

1. 2

uw

Fei p Feip

5. 06

2. 83

1313

343

5848.03 m

5848.122m 1 38

f 0. 4

1 6.3

su Fei /3. 26

14. 61 552

1175

5836.149

5836.777

5837.28 m

5837.709

1

1. 5

2

9

0. 2

0. 4

0. 3

1. 6 s,d

Atm

Fe I 4. 29 1129 16

5848.449

5848.673r

5848.975

1

0. 5

13.51

0. 2

0. 1

0. 6

s

s,NN

Atm

Mn I?-

Atm H2O

4. 27 R' 3 321

16

26

5838.015 3 0. 5 s 5849.204 2 0. 3 s,NN

5838.167 5 0. 8 u,N 5849.691 7 1. 2 s?,d? Fe I p 3. 69 922

5838.381m 16 2. 9 u -Fe I 3. 94 959 5849.933 0. 5 0. 1

5838.555r 1 0. 2 Atm 5850.105 3 0. 5

5838.678 5 0. 8 s Cr I 3. 01 119 5850.338r 1 0. 3 Atm

5838. 939r 2 0. 3 -Atm H2O R' 5 401 26 5S50.810r 1. 5 0. 3 Atm H2O R' 4 321 26

5839.42 m 1 0. 2 Atm 5851. 005r 0. 5 0. 1 Atm H2O R' 3 321 26

5839.53 m 0. 5 0. 1 s Cri 5851.210 5. 5 1. 0 w

5839.607 3. 5 0. 6 5851.791 1 0. 2

5839.768 1 0. 2 s Til 1. 46 105 5852.011 2. 5 0. 4

5839.92 a 1 0. 2 5852.228m 36 6. 5 s? Fei 4. 55 1178

5840.835r 1 0. 2 Atm 5852.34 m 2 0. 2 S Til

5841.188 1. 5 0. 3 s,N Til? 5852.569 4 0. 7

5842.385 1. 5 0. 3 Nd II? 1. 28 86 5853.161 7 1. 2 s Fei 1. 48 35

5842. 541r 2 0. 3 Atm 5853.326 1 0. 2

5842.897 3 0. 5 5853.479 2 0. 2 Fei? p 5. 07 1340

5843 227 3 0. 5 s Cr I 3. 01 119 5853. 688S 55 10. 1 s Ba 11 0. 60 2

oo4o.D04r 11 u. ^ oooo.yooi JL. 0 yj, 0 Atm

5843. 842r 0. £> 0. ] Atm? c: 0 c /I 11 o« ooo4.lizr U. 0 n 1 U. 1 Atm .'

6844. 190r 1 0. 2

> Atm? 5854.319 3. 5 0. 6 Sc II? p 1. 36 21

5844.608 4. I) 0. iI s Cri 3. 01 119 5854.596r 1 0. 2 Atm H2O- R' 5 321 26 5844.933 3 0. ^) w Fei 4. 15 1056 5854.845r 2 0. 2 Atm

6845.294

5845.481r

6. 1

2. I

5 1. ]

)| 0. 4

u

1

Fe I p Atm H2C5. 03 R' 5

1313

321 26 5855.086m 18 3. t u Fei 4. 61 1179

256
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5855.262

> 2. 5

1 0. 2 5864.81 2r 1 0. 2 Atm

5855.352r 1 0. 2 Atm? 5865.026 0. 5 0. 1

5855.540 0. 5 0. 1 5865.418r 0. 5 0. 1 Atm

5855.888 2 0. 3 s 5865.637r 2 0. 3 Atm

5856.096m 29 5. 1 u Fei 4. 29 1128 5865.853r 1. 5 0. 3 Atm

5856.28 a 2 0. 3 AtmHzO R' 2 401 26 5865.957r 0. 5 0. 1 Atm

5856.433 1. 5 0. 3 5866.148r f 0. 2 Atm

5856.623 2 0. 3 5866.264 } ^

1 0. 2

5857.048 11 1. 9 5866.461S 40 7. 3 S Til 1. 07 72

5857.459S

6857.608 1 132 J 24.6

1 0. 4

S Cai 2. 93 47 5866.642

5867.004

1

0. 5

0. 2

0. 1 Fei p 4. 64 1203

5857.758m 56 9. 6 u Nil 4. 17 228 5867.084 3.5 0. 6 Cri 3. 55

5857.992 5 0. 8 5867.248 2 0. 3

5858.280

5858.533

5858.785

5859.000r

4. 5

3

12

1

0. 8

0. 6

2. 0

0. 2

s

u

u

Mo I Fe I p

Fe I p — Atm

1. 47

2. 43

4. 22

5 170

1084

5867.572S

5867.797

5867.920

5868.151

5868.296

22

1. 5

1

1

1. 5

4.3

0. 3

0. 2

0. 2

0. 3

s Cai 2. 93 46

5859.245

5859.411

5859.596S

5859.959

5860.091r

5861.111

5861.630r

5861.806r

5862.03 a

5862.368S

4. 5

1. 5

74

2. 5

1

8. 5

141

2. 5

3. 5

87

0. 8

0. 3

13. 1

0. 4

0. 2

1. 4

0. 7

0. 4

0. 6

15. 2

Fe I

Fei

Fe I p Atm?

Fei p AtmHzO

Atm

Fei

4. 30

4. 55

4. 19

4. 28 R' 3

4. 55

1084

1181

1054

1084

401

1180

586S.773r

5869.106

3. 5

4

0. 6

0. 7

Atm

s

u

s

26

5869.351r

5869.673r

5869.793r

5870.644

5870.887

5871. 149r

5871.308

1. 5

2. 5

3

7

0. 5

3

7. 5

0. 3

0. 4

0. 5

1. 2

0. 1

0. 5

1. 3 u,dl

Atm H2O

Atm

Atm

Fe I p

Atm

Atm H2O

Fei

R' 4

4. 58

R' 3

4. 15

321

1235

321 1055

26

16,26

5862.599 5 0. 8 5871. 784r 1 0. 2 Atm

5862.859 5 0. 8 5872.031r 1 0. 2 Atm

5863. 165r 1. 5 0. 3 Atm 5872.211r 1. 5 0. 3 Atm

5863.470r 3 0. 5 u AtmHjO ? R 3 302 26

5872.274r 1. 5 0. 3 Atm H2O R' 2 401 26

5863.722 1. 5 0. 3 La n? 0. 93 62

5872.939 2. 5 0. 4 Fei

5863.952 5 0. 8 Cri

Nil?

3. 12

4. 26 185 253 5873.123 2. 5 0. 4

5864.053 2 0. 3 u 5873.218m 18 3. 1 u Fe I 4. 26 1087

5864.246 6. 5 1. 1 w Fei 4. 30 1086 5873.579 3. 5 0. 6 Atm H2O R 6 401 26

5864.360r 4 0. 7 Atm 5873.769 6 1. 0 w,N Si I 4. 93

5864.531 2. 5 0. 4 Fe II p 2. 70 24 5873.959r 2 0. 3 Atm

257
The Solar Spectriim—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5S74.649r 2 0. 3 Atm 5881.279 16 2. 7 u Fe I p 4. 61 1178

5874.778 0. 5 0. 1 5881.420r 3. 5 0. 6 Atm

5875.143 6. 5 1. 1 u,N Atm — 16 5881.545 2. 5 0. 4

5875.444r I4| 0. 7 Atm H2O R' 2 302 26 5881.722 5. 5 1. 0 Fe r 2. 18 63

5875.596 8 1. 4 Atm H2O R 5 401 26 5881.871 12 2. 0 Atm H2O R 7 401 26

5875.769r 3 0. 5 s,N Atm — 5881. 987r 7 1. 2 Atm H2O R 4, 7 401 26 5876.124 11 1. 9 Atm H2O R 5 302 26 5882.196r 3. 5 0. 6 Atm

5876.296 7 1. 2 u Fe I p 4. 30 1084 5882.373r 3 0. 5 Atm H2O R 5 401 26

5876.449 9. 5 1. 6 Atm H2O R 5 401 26 5882.493 4 0. 7 Atm H2O R 4 401 26

5876.556 3 0. 5 s Cr I 3. 01 119 5882.808 12 2. 0 Atm H2O R4 401 26

5877.057r 2 0. 3 Atm 5883.001 8. 5 1. 4 Atm

5877.328 4 0. 7 Atm H2O R 4 302 26 5883.070 2 0. 3 Fe I? p 4. 29 1124

5877.426 1. 5 0. 3 Co I? 4. 39 5883.313r 0. 5 0. 1

5877.564r 2 0. 3 Atm 5883. 373r 1 0. 2 Atm

5877.685 1. 5 0. 3 5883.442 1 0. 2 Co I 2. 04 90

5877.797

5878.029

16

3. 5

2. 7

0. 6

s

u

Fei

Til

FeiCn

Atm

Atm —

Atm

4. 18

/3. 56

13. 58

5. 66

1083 5883.574

5883.814

5883.905

0. 5

) 95

J

0. 1

1 13. 3

I 3. 3

s Fei

Atm H2O

3. 96 R 6

982

401 26

5878. 288r

5878.572

5879. 009r

5879.201r

5879.294

1

2

151

5

3

0. 2

0. 3

0. 8

0. 8

0. 5

3,1-1 s,NN

1201

16

5884.033

5884.194

5884.439

5884. 744r

5884.94 a

5885.050

1. 5

8

3

2. 5

1

6

0. 3

1. 4

0. 5

0. 4

0. 2

1. 0

s

u,d?

Atm H2O

Cr I Atm

-Cr I?

R 4

3. 01

3. 85

401

119

26

17 5879.493 12 2. 0 s,d? Fe I p 4. 61 5885.377 3 0. 5 5879.606 12 2. 0 Atm H2O /R3

IR6

302

401 |26 5885.517r 2 0. 3 Atm H2O R 1 302 26

5879.729 12 2. 0 Atm H2O R 5 401 26 5885.629 2. 5 0. 4 u Zri- 0. 07 2

5879.79 m

5879.819r

5879.88a

5880.026

5880.270

5880.429

5880. 509r 5880.616

5880.734

2

2

15

7. 5

1

2. 5

1. 5 7

0. 3

0. 3

2. 6

1. 3

0. 2

0. 4

0. 3

1. 2

S

w?

S

Zri

Fei

Til

Atm

Atm H2O

0. 15

4. 56

1. 05

R 4

4

1201

71

401

13

16

26

5885.757r

5885.977m

5886.170

5886.337

5886.405

5886.687

5886.829r 5887.222m

0. 5

19

3

8

4

4

2. 5

17

0. 1

3. 2

0. 5

1. 4

0. 7

0. 7

0. 4

2. 9

Atm?

Fe II? Atm H2O

Atm H2O

Atm

Atm

Atm

Atm H2O

R 5

R4, 5

R 3

401

401

401

26

26

26

5880.933 14 2. 4 Atm H2O R 8 401 26 5887.476 6 1. 0 u Fe I p 4. 56 1203

5881.101 10 1. 7 Atm 5887.660m 14 2. 4 Atm H2O R3 401 26

258
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

5887.840 5. 5 1. 0 Atm H2O R 1 302 26 5895.140 5. 5 1. 0 Atm HjO R 2 401 26

5888.193 |1| 0. 2 5895.366 2 0. 3

5888.440 111 0. 2 5895.685 ( 0. 2

5888.703 10 1. 7 Atm H2O R 4 302 26 5895.940m \ 564 J

< 91. 0 s Na i(D,) 0. 00 1

5888.898 3 0. 5 5896.145 [ 1. 0

5889.085 3 0. 5 Atm H2O R 4 401 26 5896.294 5 1. 0 Atm H2O Q 6 401 26

5889.370 0. 5 0. 1 5896.418 1 1.3 Atm H2O R 5 321 26

5889.637 14 2. 4 Atm H2O R4 401 26 5896.492 [ 2. 4 Atm H2O R 2 401 26

5889.756

5889.973m

5890.203

5890.314

• 752

C 3. 7

1 u. u

< 120

2. 5

. 0. 4

S

S I? Atm H2O

Nai(D2)

Atm H2O

7. 87 R3

0.00

R4

401

1

302

26

26

5896.643

5896.832

5897. 084r

5897.186

5897.250

1

10

2. 5

4

4

0. 2

1. 7

0. 4

0. 7

0. 7

Atm H2O

Atm H2O

Atm

Q' 4 R 2401

401

26

26

5890.495

5890.734r

5890.909r

5891.178

4. 5

1

1

17

0. 8

0. 2

0. 2

2. 9

s?

s

|Coi

Fe I p Atm

Atm?

Atm H2O

Fe I p

2. 04

0. 06

R3

4. 65

82

1313

401 1179

17,26

5897.461

5897.542

5897.755

5897.939

5898. 166S

7. 5

2. 5

3. 5

3

1 30

1. 3

0. 4

0. 6

0. 5

f 4. 7

J

Atm H2O

Vii

Atm

Atm

Atm H2O

IR5

2. 49

R 2

401

321

98

401

}26

26

5891.361 1. 5 0. 3 Fe II 7. 27 211 5898.218 I 0. 4 u Fei 4. 73 1259

5891.500 6 1. 0 Atm 5898.399r 3. 5 0. 6 Atm

5891.660 18 3. 0 Atm H2O R 3 302 26 5898.533 0. 5 0. 1

5891.887 4. 5 0. 8 u Fei 4. 59 1236 5898.764r 1 0. 2 Atm

5892. 055r 1 0. 2 Atm? 5898.998 12 2. 0 Atm H2O R 1 302 26

5892.277r 1. 5 0. 3 Atm? 5899.106 0. 5 0. 1 Fei 3. 55 738

5892 397m 17 2. 9 Atm HoO R 3 401 26 58QQ .Sn4m 26 to Ti I 1. 05 72

5892.478 3 0. 5 Fe I p 4. 64 1201 5899.532 14 2. 4 w,N

5892.700 18 3. 0 u Fei 4. 26 1086 5899.673 4 0. 7 5892.883S 66 11. 2 s Nil 1. 99 68 5899.919 14 2. 4 Atm H2O R 2 302 26

5893.045 11 1. 9 Atm H2O R 2 401 26 5900.045 32 5. 4 Atm H2O R 1 401 26

7 11. 9Z Fg I p iUOO conn AO Q 1 0 0 Aim

5893.508 9. 5 1. 6 Atm H2O R 3 401 26 5900.48 a 0. 5 0. 1

5893.68 a 2. 5 0. 4 5900.760 1 0. 2 Atm H2O Q 2 302 26

5893.834r 0. 5 0. 1 Atm? 5900.920 5 0. 8 Atm H2O R 6 321 26 58Q4 22 fl I n 2 Atm? 1L xA. till 1

5894.385 5 0. 8 Atm H2O R 3 302 26 5901.243 6 1. 0 Atm H2O R 5 321 26

5894.604r 2. 5 0.4 Atm 5901.468m

1 42

r 6.Atm H2O R 1 401 26

5894.944 8. 5 1. 4 Atm H2O R 2 302 26 5901. 529r 1 0.

u Fe I p 4. 22 1083

761-925—66 19 259
The Solar Spectrum—Continued

VV »i Vc- length

(A)

EquiV cLlKiLl. Li Width

AX

(mA)

Re- Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

TVavelength

(A)

EquiV CiiXdX \J Width

AX

(mA)

ReH n oc^f] Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

or

Vib. Band

Notes

5901.712 1. 5 0.3 5907.852 15 2. 5 u AtmHaO?- fQ3

IR4

302

321 } 16,26 5901.815

5902.025

5902.143

5902.248

0. 5

2. 5

10

2. 5

0. 1

0. 4

1. 7

0. 4 s

Atm

Atm

(Cr i) 3. 01 119

5908. 042r

5908.208

5908.424r

1. 5

9. 5

2

0. 3

1. 6

0. 3

Atm H2O

Atm H2O

(Fei)

Fei

Atm?

Q 3 R 0

2. 48

302

401 150

26

26

5902.476 |12| 2. 0 s? Fe I 4. 59 1234 5908. 579r 0. 5 0. 1 Atm?

5902.654r 1. 5 0. 3 Atm H2O R' 1 321 26 5908.726 0. 5 0. 1

5902.819r 1. 5 0. 3 Atm ^ c\r\C\ 0 r\c\ 5908.802 0. 5 0. 1

5903.118r 0. 5 0. 1 5908.997m 18 3. 0 Atm^H20 R[3 321 26

5903.332 5. 5 1. 0 S Ti I 1. 07 71 T' c\r\c\ 1 5909.179 2. 5 0. 4

5903.534 9. 5 1. 6 Atm H2O R 1 401 26 f c\ r\r\ A A ^ 5909.447 2. 5 0. 4 Atm H2O Q 3 401 26

5903.702r 4 0. 7 Atm H2O R 4 321 26 5909.662r 0. 5 0. 1 Atm?

5903.854r 4. 5 0. 8 Atm 5909.844r 1. 5 0. 3 Atm H2O Q 2 302 26

5903.944r 3 0. 5 Atm H2O R 5 321 26 5909.983 30 5. 1 s Fei 3. 21 552

5904.204r

5904.376r

69U4.yoo

5Q0,5 05 a

2

1. 5

1. o

2. 5

2

0. 3

0. 3

0. 3

0. 4

n 7 u. <

0. 3

J

Cri

Atm?

Atm H2O

Atin

Atm

Fe I?

5. 67

R 0

5. 41

302 26

16

5910.181

5910.312r

5910.489

5910.639r

5910.769

5910.924r 5911.148

10

4

4. 5

6

12

3. 5

1. 7

0. 7

0. 8

1. 0

2. 0

0. 6

f 0. 2

Atm H2O

Atm

Atm

Atm H2O

Atm H2O

Atm H2O

r:3

r:3

R!3

q:i

321

321

321

302

26

26

26

26

oyuo.iiy /I n 7 ALIIl Xl2w 401 9fi 5911. 219r

i 2. 5

J 1 0. 2 Atm H2O Q' 5 321 26

7 1. z XIA ftill m TTII0V7n "^91 9fi 5911.494r 1 0. 2 Atm

prance QVO 1 3. 5

u. O i\Atmtill TToO i.J.2W ^91 9fi 5911.877 2 0. 3 Atm

5yUo.4oD J n 1

L u. 1 5912.020 2. 5 0. 4 Atm H2O R[5 321 26

oyuo.o.6yr 11

fl 9 U. 5912.129 2 0. 3 OyUO.DOUb OO lU. Z u J: e 1 ^. DO 1 1 <51 5912.541r 4 0. 7 Atm H2O Q6 401 26

oyuo.yi'ir 9 A+m?

5912.698 6. 5 1. 1 u AtmH20? R[3 321 26

KCi{\R 1 '7/1 *.

J. n 9 u. ^ A +m

5912.996m 16 2. 7 Atm H2O Q^2 401 26

oyuD./syr o U. o iitin A f m TTXI2Wn T? 1 ^09 ^0 5913.142r 2. 5 0.4 Atm?

5906.512 4. 5 0. 8 s i 1 I 1. 46 105 5913.353 0. 5 0. 1 Fe I p 3. 57 781 5906.843 14 2. 5 u

5913.719 1 0. 2 S Til 0. 02 2 5907.001 4 0. 7 u

5913.905 2. 5 0. 4 5907.260 6. 5 1. 1 Atm H2O R 2 302 26 5914.120

\ 139

1" 10. 1 u Fe I 4. 61 1180

5907.359 3 0. 5 Atm H2O R 4 321 26 5914.213 1 15. 2 s Fei 4. 61 1181

5907.476 3 0. 5 Atm 5914.484r 4 0. 7 Atm?

5907.661 1 0. 2 5914.636 1. 5 0. 3

260
The Solar Spectrum—^Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduccfl Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5914.928 9 1. 5 Atm 5922.123m 17 2. 9 /S Til 1. 05 72

5915.166 1. 5 0. 3 Dy II? 5922.365 7. 5 1. 3 Atm H2O Q3 401 20

5915.432 10 1. 7 Atm H2O Qi 401 26 5922.519 15 2. 5 Atm H2O Q.,3 401 26

5915.565 5 0. 8 s Co I 2. 14 82 5922.711 6 1. 0 Atm H2O 0 4 401 26

1. / Aim /R 4 \Q5

321 4015922.92 a 0. 5 0. 1 Atm H2O Q 5 321 26

5915.834r 2. 5 0. 4 Atm

5923. 188r

5923.284

3

1. 5

0. 5

0. 3

Atm H2O R 2 321 26

5916.024 5. 5 1. 0 s Cri- fl. 03

\3. 14 17 185 5923.484 1. 5 0. 3

5916.257S 50 8. 8 S Fei- 2. 45 170 5923.646 14 2. 4 Atm H2O R 2 321 26

5916.456 2 0. 3 5923.751 5. 5 0. 9

5916.585 6 1. 0 Atm H2O R 2 321 26 5923.827 19 3. 2 Atm H2O Q2, 3 401 26

5916.772 4 0. 7 s Cri 3. 14 185 5923.963 8 1. 4 u,N Nil 4. 16 259

5916.877r 1 0. 2 Atm 5924.272m 26 4. 4 Atm H2O P 1 401 26

5917.149r 0. 2 Atm 5924.570 2. 5 0. 4 Atm H2O Q 5 401 26

5917.385 6. 5 1. 1 Atm H2O R 2 321 26 5924.752 2. 5 0. 4 Atm

5917.609 0. 2 5924.865 0. 5 0. 1

5917.806 1 0. 2 Fe I 5925.003 16 2. 7 Atm H2O Q 4 401 26

5918.009r 0. 8 Atm 5925.246 2. 5 0. 4

5918.204r 1. 5 0. 3 Atm H2O Q'4 401 26 5925.582r 0. 5 0. 1 Atm?

5918.422 27 4. 6 Atm H2O /R 2, 3 IQ4

321

401 |26 5925.830 0. 5 0. 1 Ni I p 1. 68 42

5918.554 14 2. 4 S Til 1. 07 71 5926.199 1 0. 2 Fe I

5918.764 3 0. 5 s,?N 5926.618r 2 0. 3 Atm H2O Q 2 302 26

5918.959 8. 5 1. 4 Atm H2O

Fe I R3

4. 26

321 1083

26 5926.823r 3. 5 0. 6 Fe I p Atm?

4. 58 1231

5919.054S 34 5. 7 Atm H2O 0 1 401 26 5927.210 1 0. 2

5919.291 3 0. 5 Cr I? 5927.532 0. 5 0. 1

5919.369r 1. 5 0. 3 Atm? 5927.797S 39 6. 7 u Fei 4. 65 1175

5919.644S 41 6. 9 Atm H2O 0 2 401 26 5928.059 2 0. 3

5919.844r 2. 5 0. 4 Atm? 5928.291 18 3. 0 Atm H2O Q5 401 26

5920.163 1. 5 0. 3 Atm 5928.523 3 0. 5 Fe I p 4. 22 1055

5920.330r 0. 5 0. 1 Atm H2O P'3 401 26 5928.673r 1 0. 2 Atm?

5920.560

5920.765r

5921.154

5921. 341r

12

1. 5

3. 5

0. 5

2. 0

0. 3

0. 6

0. 1

Atm H2O

(Fe I) Atm?

Atm

Cri

Atm?

Q 2

3. 24

401

581

26 5928.843

5928.888

5929.129

5929. 413r 5929.682m

4. 5

3. 5

4. 5

2

38

0. 8

0. 6

0. 8

0. 3

6. 7 s

Atm H2O

Vii

Atm H2O

Atm H2O

Fei

Q4

2. 52 R 1 0 4

4. 55

321

98

321

401

1176

26

26

26

5921.655 3. 5 0. 6 Atm 5929.928r 2 0. 4 Atm?

5921.884 2 0. 3 Atm? 5930.013 2 0. 4

261
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5930.191S 86 14. 6 s Fe I 4. 65 1180 5939.235 1 0. 2 Fe I

5930.423 2 0. 3 5939.423 1. 5 0. 3

5930.607 5 0. 8 Atm 5939.757 0. 5 0. 1

5930.766 2. 5 0. 4 5939.966 6. 5 1. 1 Atm H2O Q 4 321 26

5931.014 3. 5 0. 6 Atm H2O Q 3 401 26 5940. 183r 3. 5 0. 6 Atm II2O Q 4 401 26

5931.903 3 0. 5 Fe I p 4. 07 1017 5940.423 16 2. 7 Atm II2O P 3 401 26

5932.092S 26 4. 4 Atm H2O P 2 401 26 5940.658 4. 5 0. 8 S Ti I 0. 05 2

5932.239r 3. 5 0. 6 Atm? 5940.872 7 1. 2 Atm H2O Q 1 321 26

5932.482r 1. 5 0. 3 Atm? 5940.997 14 2. 4 u Fe I 4. 18 1083

5932.784m 17 2. 9 Atm H2O P 2 401 26 5941.076m 37 6. 2 Atm II2O P 3 401 26

5933.016r 3 0. 5 Atm H2O Q 2 302 26 5941.252 7 1. 2 Atm H2O Q 3 321 26

5933.208 1 0. 2 5941. 413r 5 0. 8 Atm?

5933.453r 1. 5 0. 3 Atm? 5941.627 28 4. 7 Atm H2O Q 2 321 26

5933. 655r 1. 5 0. 3 Atm H2O Q 6 321 26 5941.764 17 2. 9 S Ti I 1. 05 72

5933.803 7. 5 1. 3 Fe I p 4. 64 1198 5942. 003r 2. 5 0. 4 Atm?

5933.923r 2 0. 3 Atm H2O Q 3 321 26 5942.179 2 0. 3

5934.088 5 0. 8 Atm 5942.285 6. 5 1. 1 Atm

5934.275 2. 5 0. 4 Atm H2O Q3 302 26 5942.419 19 3. 2 Atm H2O Q2,3 321 26

5934.441 2 0. 3 5942.573 33 5. 6 Atm H2O Q3 321 26

5934.665S

5934.948r

5935.186

78

3. 5

6. 5

12. 8

0. 6

1. 1

s

s

Fei

Zri

Atm H2O

3. 93

0. 00 R 0

982

2 321 26

5942.721

5942.905

5943.110

9

2. 5

3

1. 5

0. 4

0. 5

Fe I p Atm H2O

Fe I p

4. 58 Q 5

4. 19

12.33 302

1021

26

5935.402 3. 5 0. 6 u Co I 1. 88 55 5943.394 5 0. 8 u,N

5935.646r 1 0. 2 Atm? 5943.592 10 1. 7 s,N Fe I p

/2 20

14. 26

63 1085

5935.818 9. 5 1. 6 Atm H2O P 2 401 26 5943.849 0. 5 0. 1

5936.068 0. 5 0. 1 5944.015 0. 5 0. 1

5936.211r 0. 5 0. 1 Atm? 5944.312 16 2. 7 Atm H2O Q 4 321 26

5936.966 1. 5 0. 3 Atm H2O Q 5 321 26 5944.500 0. 5 0. 1

5937. 128r 2 0. 3 Atm 5944.68 m 1 0. 2 S Ti I 0. 00 2

5937.306r 1. 5 0. 3 Atm 5944.732 12 2. 0 Atm H2O Q 1 321 26

5937.453r 2. 5 0. 4 Atm H2O Q 5 401 26 5945.015 3. 5 0. 6

5937.814 7 1. 2 S Ti I 1. 07 72 5945.250

} "

J

[ 0. 9 Atm H2O P 3 401 26

5937.944 3. 5 0. 6 Atm H2O Q 2 302 26 5945.313 [ 0. 9 Atm H2O Q4 321 26

5938.052 8 1. 3 Atm H2O Q 2 321 26 5945.648 10 1. 7 Atm H2O Q3 321 26

5938.283r 2 0. 3 Atm 5945.887r 4. 5 0. 8 Atm H2O Q5 321 26

5938.593r 2. 5 0. 4 Atm H2O P 3 302 26 5946.006S 28 4. 7 Atm H2O P 3 401 26

5938.753 1. 5 0. 3 Fei 5946.268r 1 0. 2 Atm?

262
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent

Vvicitn AX

(ml)

Re- duced

Widtn

AX/\

(F)

opOt

Solar

Identification

Low

E P

or Rot. Line

RMI

No.

or

Vib. Hanc

JNo

5946.466 1. 5 0. 3 Co I 3. 66 169

5946.646 2 0. 3 Atm H2O Q 6 321 26

5946.846 14 2. 4 Atm H2O P 3 401 26

5947.067 23 3. 9 Atm H2O Q 4 321 26

5947.284 1 0. 2 Feip 4. 19 1056

5947.427r

5947.506

1

f 95y. 0

1

0. 2

I 1.4 u,d?

Atm H2O

Fei

Q3

4. 61

302

1199

26

16

5947.738r 0. 5 0. 1 Atm?

5947.978r 0. 5 0. 1 Atm H2O Q6 401 26

5948.224 7. 5 1. 3 Atm H2O P4 302 26 5948.548m 88 14. 8 w Sir 5. 08 16

5948.767 11 1. 8 Atm

i

1 0 1. z Atm A 4-TM XT r\ XI 2U \i 4 Zb

oy4y.l75 6Z 5. 4 Aim A +TM XT r\ tl2U "D A r 4

A A1 401 2d

5949.346 40 6. 7 s,d Fe I

J u. yj. 14. 61

1 A 14 1176

5949.576r 4. 5 0. 8 Atm H2O Q2 321 26

5949.673 8 1. 3 Atm H2O Q5 321 26

1 ft 0 c Atm ±12^ "D A r 4 4(Ji ZK) cocn fit f\ Z U. 0

oyou.i4o 0 1. U 0! Aim XI2U Fe I p y 5

4. 56

001 1200

Zb

5950.344 12 2. 0 Atm H2O Q 5 321 26

5950.474 1 0. 2

5950. 852r 2. 5 0. 4 Atm H2O Q 5 401 26

5950.966 6. 5 1. 1 Atm H2O P 4 302 26

5951.095 4 0. 6

5951. 222r 4 0. 6 Atm H2O Q4 321 26

5951. 312r 3 0. 5 Atm

5951.500 16 2. 7 Atm H2O P 1 321 26

5951.802 3 0. 5

5952.190 0. 5 0. 1 Fei p 5. 08 1313

5952. 360r 1 0. 2 Atm

5952.522 5 0. 8 Fe II? p 5. 95 182

oyoz, / zoo Do 11.4 X e T1 OR yoy

oyo^.997 7. 5

1 0

1. 0 5953.170m 34 5. 5 Til 1. 89 154

5953.365r 2. 5 0. 4 Atm?

5953.467 6 1. 0 Atm H2O Q6 1 321 26

Wavelength

(1)

5953.717

5953.982r

5954.377r

5954.688

5954.953

5955.113

5955.16 m

5955.352r

5955.671

5955.821r

5956. 034r

5956. 146r

5956.352

5956.505

5956.706S

5956.957

5957.037

5957.147r

5957.569

5957.881

5958.080

5958.244

5958.344

5958.623

5958.807r

5959.160

5959.320

5959.610

5959.720

5959.90 a

5959.990

5960.343

5960.587 5961.228

5961.445

5961.738

Equivalent Width

AX

(ml)

0. 5

2

3

3

22

2. 5

Re- duced

Width

AX/X

(F)

0. 1

0. 3

0. 5

0. 5

3. 7

0. 4

Spot

Solar

Identification

1 0. 2

1. 5 0. 3

4 0. 6

1 0. 2

1 0. 2

12 2. 0

3. 5 0. 6

60 9. 6

2. 5 0. 4

1. 5 0. 3

1. 5 0. 3

5. 5 0. 9

35 5. 9

5. 5 0. 9

36 6. 0

12 2. 0

24 4. 0

5. 5 0. 9

5. 5 0. 9

4 0. 6

|5| 0. 8

4. 5 0. 8

3 0. 5

10 1. 7

3 0. 5

2. 5 0. 4

2 0. 4

8. 5 1. 4

5. 5 0. 9

u,N

Atm

Atm H2O

Atm H2O

Fe I p

Zri

Fei

Atm H2O

Atm

Atm H2O

Atm H2O

Fei

Atm?

Atm H2O

|Atm H2O

Fei

Fe I p

Atm H2O

Atm?

Cn?

Atm H2O

Atm H2O

Atm H2O

Fei

AtmHjOLow RMT

E P No.

or or Rot. Vib. Line Band

Q 6

P 4

4. 58

0. 00

4. 26 Q5

P' 2 P 4

0. 86

Atm H2O

fP 5 IP 2

P 5

fO. 96

14. 56

2. 18 P 5

4. 45

P 5 Q 5

Q7

4. 14 P 2

.321

401

1233

3

1106

321

401

401

14

Notes

26

P 2

302

321

401

14 1199

63

401

302

321

321

1020

321

321

•263
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

5961.894 3 0. 5 Fe I p 4. 22 1080 5970.260r 1 0. 2 Atm

5962. 170r 7 1. 2 Atm 5970.687r 1 0. 2 Atm

5962.299 2 0. 3 Atm? 5971. 145r 0. 5 0. 1 s

5962.469

5962.53 m }J

1 1.8

[ 0. 4 s

Atm 5971.335

5971.771

10

1

1. 7

0. 2

Atm H2O P 3 321 26

5962.621 3 0. 5 5972.755 3. 5 0. 6 Atm H2O P 3 302 26

5962.914 2 0. 3 Fe I 5972.986 1. 5 0. 3

5963.104 1. 5 0. 3 5973.356 2 0. 3 Fe I p 4. 65 1175

5963.268

5963.570

5963.983

5964.612

4

5

2

1. 5

0. 6

0. 8

0. 3

0. 3

s,N Atm

Fei

Atm H2O

C I Cr I?

2. 22 Q6

8. 64

3. 01

63

302

16

26

5973.475

5973.67 a

5973.870

5974.277

2

2

1. 5

3

0.3

0. 3

0. 3

0. 5

Nil 4. 17 226

5964.943r 2. 5 0. 4 Atm

(Co i) 3. 51 169

5974.596

5975.101

1

10

0. 2

1. 7

Fe I p Atm H2O

4. 19 P 41055

321 26

5965. 150r 0. 5 0. 1 Atm? 5975.200 3 0. 5 Atm H2O P 6 401 26

5965.323r 0. 5 0. 1 Atm? 5975.353S 44 7. 9 u Fe I /4. 07

14- 83 1017

1260

5965.516 1. 5 0. 3 5975.602 1. 5 0. 3

5965.835 23 4. 2 s Ti I 1. 88 154 5975.824 1 0. 2 Ce II? 1. 33 30

5966.005 4. 5 0. 8 5975.929r 1 0. 2 Atm

5966.214 2. 5 0. 4 Atm 5976.168 2 0. 4 Fe I p 4. 29 1125

5966.333 3. 5 0. 6 Atm H2O P' 3 302 26 5976.281 1 0. 2 Atm H2O Q4 321 26

5966.486r

5966.665

1. 5

10

0. 3

1. 7 Atm H2O P 5 401 26

5976.479

5976. 509r } -

J

[ 0. 9

1 1.8

s,d Atm H2O —

Atm

P 6 401 26

5966. 998r 4. 5 0. 8 Atm 5976.787S 64 11. 4 s Fe I 3. 94 959

5967.319 5 0. 8 Atm H2O P 3 321 26 5977.028 18 3. 0 Atm H2O P4 321 26

5967.501 2 0. 3 5977.291 1. 5 0. 3

5967.672 6 1. 0 s,N Atm H2O /Q'2

IP 6 321 302 |26 5977.434r 3. 5 0. 6 Atm H2O Q5 321 26

5967.840

5968.063

5968.278

5968.409

14

4. 5

14

3. 5

2. 3

0. 8

2. 3

0. 6

u

Atm H2O

Atm H2O?

Atm H2O

Atm H2O

P 6 P 6 P 3 P 6401

401

321 302

26

26

26

26

5Q77 804

CQ77 070

5978.072

5978. 144r

7. 5

9

3. 5

J

1. 3

U. 0

r 0.1

[ 0. 5 u

Atm HoO

Fe I p

P 7

4. 64

401

1199

26

5968.662r |1.5| 0. 3 Atm? 5978.343 1 0. 2

5968.90 a 2 0.3 5978.549m 20 3. 5 s Til 1. 87 154

5969.035 6 1. 0 Atm H2O P3 321 26 5978.789 2. 5 0. 4 5969.290r 3. 5 0. 6 Atm? 5978.910 5. 5 0. 9 Si II? 10. 07 4 5969.578 5 0. 8 s,d Fe I 4. 28 1086 17 5979.311 0. 5 0. 1 5970.058 1. 2 Atm H2O P 5 321 26 5979.692 1 0. 2

264
The Solar Spectr um—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

5980.171 3. 5 0. 6 Atm

5980.51 9r 1. 5 0. 3 Atm H2O P 6 302 26

5980. 744r 0. 5 0. 1 s V I 1. 19 49

5980.822r 1 0. 2 s Ti I 1. 07 72

5980.93 m 0. 5 0. 1 S,N

5981. 229r 3 0. 5 Atm H2O P 4 321 26

5981.392 1. 5 0. 3 Fe I p 3. 63 837

5981. 709r 2 0. 4 Atm H2O P 6 401 26

5981.868 2 0. 4 s?,NN

5981.983 |2| 0. 4 Cri

Atm H2O

3. 17 P 4185 302 26

5982.312 3. 5 0. 6

5982.537 1 0. 2 s Ti I? 2. 41 264

5982. 61 7r 1 0. 2

5982.877r 4 0. 6 s Cr I 3. 17 185

5983.186 1 0. 2 Atm H2O P'4 401 26

5983.304r 3 0. 5 Atm H2O P 7 302 26

5983.428 1. 5 0. 3

5983.6S8S 68 11. 9 u Fe I 4. 55 1175

5983.974r 5 0. 8

5984.066 4. 5 0. 8 Co I 1. 74 37

5984.274 4. 5 0. 8 s Co I Atm H2O4. 39 P 5 201

321

1626

5984.440 1 0. 2

5984.594 2 0. 4 S ITii V I0. 02

1. 18

249

5984.826S 84 14. 9 s Fe I 4. 73 1260

5985.215 12 2. 0 Atm H2O P 5 321 26

5985. 394r 1. 5 0. 3 Atm?

5985.510r 0. 5 0. 1 Atm?

598o.703r 1. 5 0. 3 Atm H2O P 7 401 26

3 0. 5 u 16

5986.454 1

5986.755 1. 5 0. 3 5987.070m 68 12. 0 u Fe I 4. 79 1260

5987 310 1. 0

5988. 105r 1. 5 0. 3 Atm H2O P 5 321 26

5988.361 1 0. 2 5988.562 9. 5 1. 6 s tITii Atm H2O

1. 89 P 8 154

401 26

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

5988.768 6 1. 0 V}

5988.966 1. 5 0. 3

5989. 093r 1. 5 0. 3 Atm?

5989.287 6 1. 0 u,d? Atm H2O - P 5 321 17,26

5989.568 1 0. 2

5989.812 1 0. 2

5990.072 0. 5 0. 1

5990.377 1 0. 2

5990.610r 3. 5 0. 6 Atm H2O P 5 321 26

5990.845 6. 5 1. 1 w Atm H2O- P 5 321 17,26

5991.015 0. 5 0. 1 5991.378m 29 5. 2 w Fe II 3. 15 46

5991.569 0. 5 0. 1 Fe I p 4. 58 1232

5991.791

5991. 90?m

]1

6. 5

f 0.

1 0.

s,N

Co I 2. 08 90

5991. 998r 12 2. 0 Atm H2O P 5 321 26

5992.183 1 0. 2

5992.332 0. 5 0. 1

5992.677 1. 5 0. 3 Fe I p 4. 18 1080

5993.055r 2. 5 0. 4 Atm

5993.453 1 0. 2

5993.655 1. 5 0. 3

5993.915r 2. 5 0. 4 Atm H2O P 7 401 26

5994.41 a 1 0. 2

5994.529 5 0. 8 Atm H2O P 6 321 26

5995.18 a 2 0. 4

5995. 271r 0. 5 0. 1 Atm H2O P 6 321 26

5995.698 1. 5 0. 3 S Ti I 3. 46 311

5995.944 2 0. 4 Fe I p 4. 61 1198

5996.033 2 0. 4 S Ti I 1. 88 154 5996 505 1 0. 2 Fe I p 4. 28 1083 o99D.740m 1 r\ 19 c? 0

0. 0

.,..9 ID! JNl I 4. Zo Z49

5996.978 1. 5 0. 3

5997.214 2 0. 4 5997.352 10 1. 7 Atm H2O P6 321 26

5997.604 11 1. 8 w,N Ni I 4. 23 252

5997.782m 67 IL 2 u Fe I 4. 61 1175

5998.225 3 0. 5

265
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

5998.544 2. 5 0. 4 6010.65 a 5 0. 8 Ci 8. 64

5998.897 3. 5 0. 6 Ni I?- 4. 10 226 6011.45 a 1 0. 2

5998.984 2. 5 0. 4 s 6011.67 m 2 0. 3

5999.047 0. 5 0. 1 S Ti I 2. 17 198 6011.95 a 1 0. 2

5999.209 7. 5 1. 3 w 6012.229 22 3. 6 ^l Nil

5999.698

6000.150r

6000.678

6001. 126r

11

2

4

3

1. 8

0. 3

0. 7

0. 5

S,d

s,d?

Atm H2O

ITi I Atm H2O

Co I Atm

P9

2. 24 P 6

3. 62

401 227

321

169

26

26

60l2.443r

6012.770

6012.98 m

6013. 199r

3

4

1

7

0. 5

0. 7

0. 2

1. 2

s s,N

Fe I p —

Ci

4. 56

(8. 64

IS. 64

1198

6001. 546r 2 0. 3 Atm 6013.497S 86 14.1 S Mn I 3. 07 27

6002. 156r 1 0. 2 Atm 60l3.914r 4 0. 7

6002.30 m 1. 5 0. 5 S Vi 1. 22 49 6014.425r 1. 5 0. 2

6002.648

6002.751r

6003.022S

6003.319r

6003.52 a

6003.876r

6004.384r

6004.670

6004.879r

6005.009r

6005.367r

6005.551m

I6|

1. 5

86

2

3

3

1

3

1

HI

Ul

21

1. 0

0. 2 U- 5

0. 3

0. 5

0. 5

0. 2

0. 5

0. 2

0. 2

0. 2

3. 7

S

s

s

IIVi AtmHaO?

Fe I

Atm

Atm H2O

Atm?

Co I

Fe I

1. 05 P 6

3. 88

P7

1. 71

/2. 59

\4. 18

34

321

959

321

37

207

1079

26

26

60l4.842r

6015.042r

6015.253

6015.611

6015.850

6016.017r

6016.408r

6016.647S

6016.925r

6017.00 m

6017.56 m

6017.92 m

6018.300

4. 5

2. 5

4

0. 5

2

1

2

1 92

1. 5

1. 5

0. 5

8

0. 7

0. 4

0. 7

0. 1

0. 3

0. 2

0. 3

1 15.4

1 0. 5

0. 2

0. 2

0. 3

1. 3

S

s

s

s

0

Ci

Fe I p

Atm H2O

Atm H2O

Atm H2O

Ci?

Mn I Fe I p

Tii?p

Vi? — Fe I p

8. 64

2. 22 P 7 P 7 P7

8. 64

3. 07

4. 59

2. 33

1. 19

4. 65

63

321

321

321

27

1232

257

49

1176

26

26

26

6005.784r 1. 5 0. 2 6018.40 m 1 0. 2 S Til 2. 15 198

6006.061r

6006.387r 6007.317m

6007.68 m

6007.717 6007.968m

6008.566S

6008.813r

6009,359

6009.848r

3. 5

4. 5 20

} ^

59

88

2

2

1

0.6

0. 7

S. 7

j 0.

2

1 0. 5

10. 0

15. 1

0.3

0.3

0. 2

s

s

s

s

Atm

Ci?

Atm

Nil

Fe I p Fei

Fei

Atm HjO

Fei p

Atm?

8. 64

1. 68

3. 27

4. 65

3. 88

P7

3. 25

42

581

1178

982

321

624

16

26

60l8.545r

6018.66 m

6018.824r

6019. 157r

6019.364

6019.785r

6020.016 anon 1 or

6021.803m

6022.04 a

6022.226r

2

0. 5

121

5

1. 5

49

Q4.

96

2.5

4. 5

0. 3

0. 1

0. 3

0. 8

0. 2

8. 1

10. 0

16. 0

0.4

0. 7

S

s,d1

u

uS

Til

Atm?

Atm H2O

Fe I p

pel

Mn I

1.05

P8

3. 57

3. 07

70

321

780

1 1 78

27

26

266
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6022.476r 3. 5 0. 6 Si I? 6036.221r 2 0. 3

6023.025r 0. 5 0. 1 6036.459 7 1. 2 u Atrii —

O

Nil

Vi

Si

Fe I

Ceil

Fe II

-IIS I

6023.42 m

6023.957r

6024.068S

6025.211r

6025.44 m

6025.767

6026. 166r

6026 .401r

6026.826r

6027.059S

6027.436r

6027.726

1. 5

1 117

|2.5|

1

4

2

1. 5

1. 5

1611

1. 5

4

0. 2

1

0. 2

1 19. 8

0. 4

0. 2

0. 7

0.3

0. 2

0. 2

10. 8

0. 2

0. 7

S

u

su

u

Yi

Fei

Zr I? Nil

Atm?

Fe I

Fe I p Atm

0. 00

4. 55

0. 15

4. 23

4. 07

4. 99

3

1178

3

251

1018

1312

16

6036.796r

6037.10 m

6039.327r

6039.736

6039.977r

6041.93 a

6042.104S

6042.267r

6043.40 a

6045.492r

6045.772r

6046.015?

11.51

1. 5

2

11

1. 5

|3. 5|

51

3. 5

2

3. 5

3

16

0. 2

0. 2

0.3

2. S

0. 2

0. 6

8. 4

0. 6

0. 3

0. 6

0. 5

2. 6

S

w

u,N

0

4. 23

1. 06

7. 86

1. 21

6. 21

7. 87

248

34

10

30

200

10

6028.006r 2 0.3 Atm 6047.067r 1. 5 0. 2 Atm?

6028.276r

6028. 506r

3

0. 5

0. 5

0. 1

Vii?-

AtlH A f TY\?

i

2. 49 97 6047.667r

6048.798r

1. 5

|2|

0. 2

0. 3

s?

S,d

Cri?

OAtm

3. 85 242

17

6029.00 a 3 0. 5 V II 2. 56 125 6049. 124r |41 0. 7 Co I 4. 50 201

6029.286r 2 0.3 Cn 3. 85 242 6051.032r 1. 5 0. 2 Feip- 2. 56 207

6029.876 15 2. 5 u,NN Atm — 16 6051.848r 2 0. 3

6030.336r 2. 5 0.4 6052.615r |3| 0. 5

6030.68 m 1. 5 0. 2 S,N Mo I 1. 53 5 6052.682 11 1. 8 Si 7. 87 10

6031.016 6 1. 0 w,N -Vii 2. 52 97 6052.93 a 1. 5 0. 2

6031.306r 2 0. 3 Nd II? 1. 28 6053.08 a 1. 5 0. 2

6031.718r 1 0. 2 S Til 0. 05 2 6053.263r 1 0. 2

6032.00?ni 1 0.2 6053.475 5 0. 8 Cr II 4. 74 105

6032. 161r 2 0.3 6053.693 18 3. 0 u Nil 4. 23 247

6032.60 m s Zri? 1. 48 13 6053.912r 2 0. 3

6032.672r 1 0. 2 s Fei 4. 22 1082 16 6054.075 8 1. 3 u Fei 4. 37 1142

6033.317r 1. 5 0. 2 6055.097r 3 0. 5 Cn?

DUoo.oy (

o

u. O DUOO.rrU 1 P fi d. U. rt

6034.038 7 1. 2 s Fei p 4. 31 1142 6055.767r 1. 5 0. 2

6034.227r 1 0.2 Nd II? 1. 54 6056.013m 73 12. 2 u Fei 4. 73 1259

6034.502r 1 0. 2 6056.343 5 0. 8 6034.924r 2 0.3 6056.897r |1.5| 0. 2 6035.350 6 1. 0 u Fei?p 4. 29 1125 6057.08 m 1. 5 0. 2 s 6035.97 a 2 0.3 6057.251 5 0. 8 ot

761-925—66 20 267
The Solar Spectrum—Continued

WtlVGlength

(A)

Equiva IpTi ti Width

AX

(mA)

RecluC6Cl Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Reduccd. Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6057.867r 1. 5 0. 2 6078.499S 91 15. 0 u Fe I 4. 79 1259

6058. 172r 3 0. 7 S Vi 1. 04 34 6078.766r 2. 5 0. 4

6058.76 m S Tiip L 07 70 13 6079.016S 55 9. 0 w Fe I 4. 65 1176

6059.271r 13| 0. 5 Sc II? p 1. 36 20 6080.018r 4. 5 0. 7

6059.757r 1. 5 0. 2 6080.238r 3 0. 5

6060.17 a 1. 5 0. 2 6081.210r 2 0. 3

6060.45 a 2 0. 3 6081.448 15 £ 6 S Vi 1. 05 34

6060.640r 1. 5 0. 2 6081.718r 3 0. 5 Fe I p 4. 41 1142

6060.824r 1. 5 0. 2 Fe I p 4. 22 1081 6081.838r 2 0. 3 Fe I p 4. 14 1018

6061.05 a 2 0. 3 6082.35 a 5 0. 8 u Co I 3. 51 169

6061.657r 2. 5 0. 4 M? 6082.54 m 5. 5 0. 9 s

6062.676 4 0. 7 Cn 3. 19 185 6082.718S 34 5. 6 s Fez 2. 22 64

6062.856

6063.15 a

6063.309r

18

1

2

3. 0

0. 2

0. 3

Zri

IIFei

0. 07

2. 18

3636083.703r

6084.105

|3| 22

0. 5

3. 6

s?,N w

Fe I p—

Fe n

3. 88

3. 20

981

46

s 6085.257S 40 6. 6 S

s Til

Fez

1. 05

2. 76

69 269

6064 .046r 3. 5 0. 6 6086.288S 43 7. 1 w Niz 4. 26 249

6064.626 7 1. 2 s Til 1. 05 69 6086.673r 4. 5 0. 7 s Co I 3. 41 165

6065.18 a 3. 5 0. 6 6087.50 m 1. 6 0. 2 s V z 1. 05 33

6065.494S 115 s Fe I 2. 61 207 6087.790 1171 2. 8 0? Si I 5. 87 17

6065.808r 2. 5 0. 4 Fe I p 3. 30 581 6088.278r 1. 5 0. 2

6067.638r 4 0. 7 Si I 5. 08 15 6088.65 a 1 0. 2

•

6067.960r 3 0. 5 6089.063r 2. 5 0. 4

6068.39 a 1. 5 0. 2 6089.574S 32 5. 2 u Fez 5. 02 1327

6070.09 Ir 1 0. 2 6089.798r 1. 5 0. 2

6070.55 a 4 0. 7 6089.974r 1 0. 2

6071.363r 2 0. 3 6090.075r 1 0. 2

6071.758r 2 0. 3 6090.216S 29 4. 6 s Vi 1. 08 34

6073.198r 2. 5 0. 4 6090.510r 1. 5 0. 2 s Vi p 1. 06 33

6073.560r 1. 5 0. 2 6091.177 14 2. 3 s Til 2. 27 238

6074.018r 2 0. 3 6091. 368r 3 0. 5

DU / D.i'ior QO U. 0 DUyi.oU/r Z. 0 U. 4

6076.608r 2 0. 3 6091.730 6 1. 0 u Fe I p 4. 61 1200

6076.896 12 2. 0 u,N 17 6091.920 30 4. 9 w Sii- 5. 87 15, 17 Rn77 9fiST 1 i. 0 Duyz.io a 0. 0 n Q

6077.37 m s Vi? 0. 00 13 6092.525r 3 0. 5

6077.490r 1 0. 2 6092.818r 6 1. 0 S Tiz 1. 89 153

6077.848r 4. 5 0. 7 6093.151 11 1. 8 s Coz 1. 74 37

268
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes', Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6093 .368r 2 0. 3 Atm? 6107.350r 2. 5 0. 4 Fe I p 4. 07 1015

6093.649S 31 5. 1 u Fei 4. 61 1177 6107.898r |3.5| 0. 6

6093.863r |21 0. 3 Vi? 0. 04 6108.125m 60 10. 3 s Nil 1. 68 45

6094.20 a 3 0. 5 6108.293r 4 0. 7

6094.377 20 3. 3 u Fei 4. 65 1177 6108.465r 2. 5 0. 4

6094.70 a 2. 5 0.4 6108.895r 5 0. 8

6095.364r 3 0. 5 Nil 4. 42 6110.345r 3 0. 5

6096.149r 1 0. 2 6110.795r 2 0. 3 s 6096.671S 36 5. 9 si Fei 3. 98 959 6111.078S 36 5. 9 w Ni I 4. 09 230

6096.884r 2. 5 0.4 6111.336r 1. 5 0. 2

6097.101r 4. 5 0. 7 s Fe I p 2. 18 64 6111.652 12 1. 8 S Vi 1. 04 34

6097.294r 4 0. 7 S Cai 2. 52 6112. 026r 3 0. 5

6097.46 m 2 0. 3 s Vi 1. 08 33 6112.291r 3. 5 0. 6

6097.67 a 3 0. 5 6112.412r 1 0. 2

6098.250 16 2. 6 u Fe I p 4. 56 1200 6112.932 11 1. 8 w1,N -Sii 5. 61

6098.664 7 1. 1 S Til 3. 06 304 6113. 131r 6 1. 0 Si I 5. 61 30

6100.271

6100.95 a

6102. 183S

6102.425r

6102.727S

6103.079r

10

2

84

8

135

1. 6

0. 3

1. 3

22. 1

( 0.2

ut

w?

S

/Fei p IFeip

Fei

Cai p

Cai

4. 56

4. 61

4. 83

2. 52

1. 88

1199 1199

1259

3

17 6113.329

6114.391r

6114.801r

6115.751r

6116.059r

6116. 198S

17

1. 5

1. 5

|2|

5

If 65DO

2. 8

0. 2

0. 2

0. 3

0. 8

f 8.

u

Fe II Fe I p

Zr II

Fe II p

Ni I

3. 22

3. 93

1. 66

3. 23

/4. 09 U- 26

46

981

93

46

218

251

6103.190 • 89 I 10. 0 u Fei 4. 83 1260 6116.246r 1 2.

u Fei

6103.298 J 1 ... u 16 6116.456r 3 0. 5

6103.480r 3. 5 0. 6 6116.76 a 1. 5 0. 2

6103.586r 2 0.3 6117.001 8 1. 3 s Co I 1. 78

6104.620r 2 0.3 6117.206r 5 0.8 u Ca I p 2. 71

6105.132 12 2. 0 u Fe I p 4. 55 1175

6117.414r 1 0. 2

6105.520r 1. 5 0. 2 Co I 2. 04 6117.637r 1. 5 0. 2

6105.785r 3 0. 5 Nil 4. 23 6117.819r

1 .

1 0.1

6106.441r 3. 5 0. 6 Zr II 1. 76 106 6117.930r 1

'

I 0. 2

6106.616 10 1. 6 0 Si I 5. 61 30 6118.111r 5 0. 8 Nil 4. 09 230

6106.78 m s 13 6119. 175r 1. 5 0. 2

6106.860r 3. 5 0. 6 Fe I p 2. 61 208 6119.532 20 S. 3 S Vi 1. 06 34

6106.98 m S Vi 1. 38 60 13 6119.760 12 2. 0 wt Nil 4. 26 244

6107.099r

6107.26 m

3

2

0. 5

0.3 s

Fe I Cai4. 26

2. 71

1081 6120.249

6120.50 a

6

2. 5

1. 0

0. 4

s Fe I 0. 91 14

269
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6120.802r 4 0. 7 6135.370 12 1. 8 S Vi 1. 05 34

6121.006 5 0. 8 S Til 1. 88 153 6135.775 17 2. 8 w Cri?- 4. 82 314

6121.333r 4 0. 7 6136.293r |4| 0. 7

6121.778r 2 0. 3 6136.624S 137 23. 8 s Fe I 2. 45 169

6122.226S 222 S3. 8 s Cai 1. 89 3 6137.002S 64 10. 4 s Fei 2. 20 62

6122.622r 3 0. 5 Co I 3. 57 169 6137.221r 2.5 0. 4

6123.260r |4.5| 0. 7 6137.294 7 1. 1 s

6123.45 m 14| 0. 7 0? Sii?p 5. 62 6137.506 12 2. 0 s Fe I p 3. 33 685

6124.495r 1 0. 2 6137.702S 129 21. 8 s Fei 2. 59 207

6124.82 m 1.5 0. 2 s Zri 0. 52 24 6138.059r |3| 0. 5 6125.026m

6125.313r 6126.224m

6126.456r

6126.792r

6127.475r

6127.643r

6127.912S

6128.112r

6128.33 m

6128.984S

6129.222r

6129.532r

6129.732r 6130.141m

6130.352r

6131.282r

6131.577

6131.858

6132.282r

6132.496r

6132.812r

6133.232r 6133 977

6134.57 m

36

4

20

1

2

3.5

1.5

48

5

2

21

3

7

5

23

2.5

6

26

27

4

4

1.5

|5|

5

3.5

5. 9

0. 7

S. 3

0. 2

0. 3

0. 6

0. 2

7. 8

0. 8

0. 3

3. 5

0. 5

1. 1

0. 8

3. 6

0. 4

1. 0

4. 2

4. 4

0. 7

0. 7

0. 2

0. 8

0. 8

0. 6

w

S

S

u

s

s

w

0

0

S

Si I

Til

Zn

Fe I

Vi

Ni I Cr II

Fe II p Nil

Fei p

Si I

Si I

Ni r Zn

5. 61

1. 07

0. 15

/4. 14

14. 28

1. 05

1. 68

4. 75

3. 20

4. 26

3. 25

5. 61

5. 61

4. 09

0. 00

30

69

2

1017 1082

33

42

105

46

248

624

30

30

229

2

6138.43 m

6138.522

6139.651

6140.46 m

6141.058r

6141.388r

6141.727S

6142.018r

6142.213r

6142.494

6142.837r

6143. 183r

6144.343r

6144.781r

6145.020S

6145.411

6146.235

6146.85 m

6147.173r

6147.742

6147.834

6148.092r

6148.272r

6148.662r

6149.001r

8

17

3

2

2

3.5

113

5

4

34

13.51

2.5

2.5

1

38

4

3

13.51

111

1 76

2

0.5

13.51 2

1. 3

2. 8

0. 5

0. 3

0. 3

0. 6

19. 4

0. 8

0. 7

5. 5

0. 6

0. 4

0. 4

0. 2

6. 2

0. 7

0. 5

0. 6

0. 2

1

5. 4

i 7. 6

0. 3

0. 1

0. 6

0. 3

S

0

S

s

w

S

W

uS

0u

Tii?-

Yi

Fe I p Zn

IBaiiFe I Nil

Si I p

Six

Zn

Si I Fe I p Til

Cr II? Fe n

Fe I

Fe I p

2. 15

0. 07

2. 59

0. 52

0. 70

3. 60

4. 15

5. 62

5. 62

0. 07

5. 61

3. 37

1. 87

4. 76

3. 89

4. 07

4. 32

197

3

208

24

2 816

244

30

30

2

29

685

153

105

74

1016

1141

6134.71 m s 13 6149.249S 35 5. 8 W Fe II 3. 89 74

6135.072r 12.51 0. 5 S Vi L 35 60 6149.558r 2 0. 3

270
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(raA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Banc

Notes

6149.742r 2. 5 0. 4 S Til 2. 16 197 6164.567r 2 0. 3

6150.154 12 1. 8 s Vi 0. 30 20 6165.168r 1 0. 2

6151.623S 41 7. 0 s Fe I 2. 18 62 6165.363S 33 6. 0 s Fe I 4. 14 1018

6151.846r 1 0. 2 6165.550r 1 0. 2

6152.018r 2 0. 3 6165.895r m 0. 3

6152.312r 3 0. 5 6166.056r 1 0. 2

6152.646r 1. 5 0. 2 6166.440S 54 10. 2 s Ca I 2. 52 20

6152.847r 2 0. 3 Fe I? p 5. 03 1312 6167.872r 1. 5 0. 2

6153.921r 1 0. 2 6168.75 a 2. 5 0. 4

6154.230S 27 4. 6 s Nai 2. 10 5 6169.044m 85 13. 8 S Cai 2. 52 20

6154.442r 2. 5 0. 4 Cr I? 4. 80 314 6169.564S 98 16. 5 S Cai 2. 52 20

6154.689r 2 0. 3 6169.967r 6 1. 0

6154.892r 2. 5 0. 4 6170.209r 2 0. 3 6155.142m

6155.241r

6155.706

j 72

5

1 11. 0

[ 0. 6

0. 8

W,N

u

Si I Fe II? p

Si I

5. 62

5. 57

5. 62

29

161

29

6170.33 m

6170.516S

3

66

0. 5

10. 7

swVi

Fei

(Nil)

0. 29

4. 79

/4. 09

14- 10

20

1260

228

230

6156.030

6156.281r

6 156.80 Ir

6157.241r

6157.421r

6157.733S

6157.921r

6158.171r

6158.679r

6159.09 Ir

6159.382

6160.228r

6160.40 a

6160.753in

6161.089r

6161.295S

6161.634r 6162 180S

7

4

5

11.51

3

48

1. 5

3. 5

1. 5

0. 5

8

2. 5

2

44

2. 5

52

3 222

1. 1

0. 6

0. 8

0. 2

0. 5

8.4

0. 2

0. 6

0. 2

0. 1

1. S

0. 4

0. 3

7. 5

0. 4

8. 4

0. 5

S8. 5

S

0?

u

s?

u,d1

S

S

s

Cai

(Oi)

Oi

Fe I p

Fe I

Oi

Fe I

Nai

Cai

Ca I

2. 52

10. 74

10. 74

3. 30

4. 07

10. 74

4. 61

2. 10

2. 52

1. 90

20

10

10

624

1015

10

1175

5

20

3

16

6170.817r

6171.004r

6171.232r

6171.59 a

6171.950r

6172.734r

6173.065r

6173.341S

6173.57lr

6174.737r

6175.11 m

6175.162

6175.370S

6175.595r

'

6176.816S

oil / .U43r

6177.253

6177.535r

6178.518r

3. 5

2. 5

1

2

1. 5

1. 5

1. 5

50

2. 5

2

} ^

36

131

50

Z. 0

10

23

0. 6

0. 4

0. 2

0. 3

0. 2

0. 2

0. 2

9. 7

0. 4

0. 3

0. 5

5. 8

0. 5

8. 7

0. 4

1. 6

0. 3

0. 5

u

r

w

u

s

Fe I p

Eu II Fei

Til?

Fe II Nil

Nil

Ni I Nil p

4. 73

1. 32

2. 22

2. 66

6. 22

4. 09

4. 09

1. 83

4. 23

1256

9 62

293

200

217

228

58 244

17

6163.421 29 4. 7 w? Nil 4. 10 230

6179.395 2. 5 0. 4 Fe II 5. 57 163 6163.554 24 3. 9 u Fe I 2. 20 64 6180.061 3 0. 5 6163.754m 49 8. 0 S Cai 2. 52 20 6180.209S 40 7. 1 s Fei 2. 73 269

271
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

bolar

Identification

Low

TP "D

ill Jr or Kot. Line

RMT

IN 0. or

VlD. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

tooiar Identification

Low

"I T5 hi r

or Rot. Line

RMT

JN 0. or

Vib. Band

Notes

6180.375r 5 0. 8

C O AO O /I 1. 5 A O

0. Z

6182.637r 1. 5 U. J, CO A/1 CI A»Tn 1 cId o c

z. b

"NT I , JN 1

1

4. 09 226

6183. 122r 1. 5 U. Z JNl I Q /I ^;

<i. 40 COAK OQ TV* 1 K1. 0 A O U. z

CT o

6183.574 12 1. 9 o! 1 17 io , 1 / Dzuo.4/ m 11 A O U. z

6183.872 5

A O

0. 8 JNl I 4. 1/ /ZD COA7 OQO DZU/.ZOZ o c z. 5 C. 6 r e I

6185.38 a 1. 5 0. 2 Fe I CO AO 0 1 O DZUo.ZlZ o c o. 5 A C

(J. b

6185.704 12 1. 9 w!,a c COAO CCA 5 A O

U. a

6186.14 m [0. 3

cr il I 17 1 A"? COAO OAO« DzUo.oyzr A C

0. 5

A 1 U. 1

6186.217

|91 [l. 1 CO AA "7 C /I « Dz0y.754r 1 A O

0. Z Fe I p

O AC 981

6186. 717S 22 3. 9 W JNl I

A 1 A 4. lU C01 A C71 bzlu.D/

1

1 o 1 |2| A O

U. O

CT o be I A AA 0. W o

z

6187.410 2. 5 0. 4 Fe I p 2. 83 342 coil 1 A Dzll.iy m 1 A O

U. z

6187.995S 36 6. 3 U li e I O A /! o. 94 AC A C0 1 O AC?.. DzlZ.UD/r o c Z. 0 A /I U. 4 r e I

A 07 4. £>/

1 1 y1 O 114z

6188.55 a 1 0. 2 CO 1 O 0*7 1 T. Dzlz.z/ Ir 1 A O U. z s

6188.998 6 1. 0

« A7 OO I1 '71

1. /I o/ C0bzlo.lz 1 O 1 O mm A K

U. 0 A 1 U. 1 s Zir I A KAU. 54 OAZ4

6189.383r 0. s

ct O V I A OO on AO 10 y1 CIbl 1 i Q 11. OCT o r e I O OO Z. zZ CObZ

6190.400r 2 0. 3 C0 1 O CO o« bzlcS.bozr A K

I). 0 A 1

6190.837r 2 0. 3 C0 1 o occ bzlo.obb oO A O CT O V I A OA OAZU

6191.186m 56 9. 8 s Ni I 1. 68 45 C0 1 /I C A .i-. bzl4.5U m 1 A O

U. z s

6191. 571S 110 19. 7 u Fe I 2. 43 169 C0 1 ;4 ceo 4. 0 A 7 0. / s,a

1 7

6191.74 m 3 0. 5 o

"\7" _ Y I A AA 0. UU o

z CO 1 C AOO-». DZlo.Uzor A CU. 0

6192.95 m s,N Zr I 0. 54 z4 13 C0 1 C 1 /I AG DZl0.14yt5 A A 4U C /I b. 4 u r e I

/I 1 Q 4. ly 1 ni Q iUlo

6193.69 m S Sci 0. 00 3 13 6215.22 m 11 1. 8 S Til 2.69 293

6193.77 a 1. 5 0. 2 CO 1 C /I OA bzl5.4zU ^77

1 1 1. 1 0

6194.230r 2 0. 3 6215.723r 1 0. 2

6194.424 11 1. 8 0

/I c

4. 0

A 7

6194.873 3 0. 5 OA 0. 1

CT O V I A OC U. ZO 1 Qly

6195.18 m 1. 5 0. 2 Cr II 4. 76 105 DZlD.OU*ir oo

A C

U. O

6195.448 13 2. 1 w 6217.45 ni A C

0. 5 A 1 0. 1

6196.163r 1 0. 2 6217.690 3 A C

0. 5

6196.68 m 2 0. 3 Fe II? p 3. 22 46 1 c

1. 0 A OU. Z

6198.655r 1 0. 2 Ni I 4. 26 1 A O U. Z

6199.186 8 1. ^ S V I 0. 29 19 0219.2870 OO8z IS. s

CT r e I O OA Z. zU CObz

6199.508 3. ^) 0. e) s Fe I 2. 56 208 6219. 522r 2. 5 A A 0. 4 Fe I p

O /I o

3. 4z boo

6200.321S 55 9.6 s Fei 2. 61 207 6219.943 5 0. s

6200.481r 1. 1) 0.2) 6220.235 11 1. s 0

6200.64 a 2 0. c\ 6220.488 9 1. 4 S Til 2. 68 293

6200.967r 2 0. cJ 6220.791 17 2. 7 u,d Fei 3. 88 1 958

272
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes A\ AX/X fication Rot. Vib. AX AX/X ficatiori PtOt. Vib. (I) \r) Line Band (I) (A.J Line Band

6221 OlSr 1. 5 0. 2 6243,114m 24 3. 8 s V I 0. 30 19

6221 342 13 2. 1 S Til 2. 66 293 6243.331r 2 0. 3

|Fe I 3. 93 981

6243.57 a 1. 5 0. 2 6221. 643r 2. 5 0.4 Fe I 0. 86 13 6243.823m 43 6. 9 w Si I 5. 61 28 6221 72 m 1 0. 2 6244.118 7 1. 1 Si I p 5. 61 28

6222.61 m 1. 5 0. 2 Yi 0. 00 2 6244.476S 45 w Si I 5. 61 27 6223.990m 24 U Nil 4. 10 228

6245. 204r 1 0. 2 s V I 0. 26 20

6224.196 2 0. 3 Fe I? p 4. 73 1257 6245.620S 30 5. 0 Sc II 1. 51 28

6224.506 5 0. 8 s Vi 0. 29 20

6245. 891r 2. 5 0. 4 Fe I? 5. 01 1289

6225. 173r 2. 5 0.4 6246.327S 112 19. 4 Fe I 3. 60 816

6225.493r 2. 5 0. 4 6247.350 5 0. 8 6226.320r 3. 5 0. 6 Vii? 2. 56 124 6247.562S 49 8. 3 W Fe II 3. 89 74 6226.740S 24 s? Fe I 3. 88 981

6248.26 m 1. 5 0. 2 6227.556 8 1. 3 s,N,d 17 6248.910 141 0. 6 Fe II 5. 51 6229.232S 33 5 A Fe I 12. 84 342

6249.05 a 3 0. 5 6229.645r 1 0. 2 6249.501r 4 0. 6 Cox 2. 04

6229. 843r 1. 5 0. 2 6249.643 6 1. 0 Fei 3. 37 685

6230.098 18 2. 7 w Nil 4. 10 227

6249.91 m 0. 5 0. 1 s,N La I 0. 51 7 6230.736S 151 26. 4 s IIFei 2. 56 207

Vi 0. 27 19 6251.286r 2 0. 3 Fe I p 4. 61 1176

6230.85 m 13 6251.825 11 2. 1 S Vi 0. 29 19

6231.003r 2. 5 0. 4 Co I 1. 78 37 6252.201r 1. 5 0. 2

6231.34 m 2 0. 3 6252.565S 109 18. 7 s Fe I 2. 40 169

6232.648S |76| s Fei 3. 65 816 6253.55 a 2. 5 0. 4 Si 1? 5.08

6233.201 4 0. 8 Vi 0. 28 20 6253.834 17 2. 7 s,d Fe I p 4. 73 1256 17

6233.498 4 0. 6 — Fe II '5. 48 17 6254.173r? 1

r 4 7 1 rsi I 5. 62 28

> 115

6235.92 a 2 0. 3 6254.253S J [ 15.

J [Fe I 2. 28 111 6237.328m 60 9. 8 Si I 5. 61 28

6254.845 4. 5 0. 7 Si I 5. 62 28

6237.84 m 2. 5 0. 4 6255.952 18 2. 7 Fe I 6238.390m 41 6. 9 Fe II 3. 89 74

5. 08 6256.367S 81 12. 9 s Fe I 2. 45 169 Ni I 1. 68 43

6239.361 6 1. 0 So I 0. 00 2 6256 887 3 0. 5 S V

0. 28 19

6239. 771r 2 0. 3 s Sc I 0. 00 3 6257 594r 2 0. 3 Co I O, 71t L 6239.948 10 1. 6 Q Fe II 3. 89 74 6257 63 m s? 1 'i 6240. 16 Ir 2 0. 3 S Vi 0. 27 20

6257.81 m 3 0. 5 S Til 0. 00 1 6240.318 13 2. 1 s Fei- 4. 14 1015

6258. UOS 42 7. 2 s Til 1. 44 104 6240.653S 40 6. 9 s Fe I 2. 22 64

6258.362r 2 0. 3 6241.31 m s 13

6242.838 7 1. 1 S Vi 0. 26 19

273
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6258.573 14 2. 2 S Vi 0. 26 19

6258.713S 43 6. 9 S Til 1. 46 104

6258.936r 3 0. 5 S Sci 0. 02 3

6259.594 |14| w Nil 4. 09 216 17

6259.772r |4| 0. 6

6259.93 a 3 0.5 6261.106m 40 7. 0 S Til 1. 43 104

6261.23 m S Vi 0, 27 20 13

6261.293r 2 0. 3

6261.552r 2. 5 0.4

6261.965r 1 0. 2

6262.250r 3 0. 5 —La II? 0. 40 33

0. 4 Ti T 1. 74 144

6265.141S 72 12. 4 s Fei 2. 18 62

6265.600 3 0. 5 u1

6266.015r 1 0. 2 S Til 1. 75 144

6266.326 3 0. 5 S Vi 0. 28 20

6266.834r 1 0. 2

6267.216r |1| 0. 2

6267.62 m 4 0. 6 Atm

6267.845 5 0. 8 Fei 4. 29 1123

6268.225r 0. 5 0. 1

6268.53 m

6268.611r

1 2. 5

1

r 0.1

[ 0.

3

S Til 1. 43 103

6268.872r 3 0. 5 S Vi /O. 30

\0. 29 20

20

6269.422r 0. 5 0. 1

6269.977 6 1. 0 0?

6270.231S 46 8. G s Fei 2. 86 342

6270.420r 1 0. 2

6270.904r 1 0. 2 6271.283m 19 S. C s Fei 3. 33 685

6271.495r 3 0. 5 Fe I p 4. 58 1231

6271.767 3. 5 0. 6 Nil 3. 31 6271 949r 2 0. 3 Atm

6272.415r 3 0. 5 Atm

6272.645 4 0. 6 Nil 4. 26 244

6273.098r 1. 5 0. 2

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(Y)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

6273.39 m S Til 0. 02 1 13

6273.65 m 1 0. 2

6273.949 |3| 0. 5

6274.658 6 1. 1 s Vi 0. 27 19

6275.278 131 0. 5 Atm H2O R6 113 26

6275.72 m 1 0. 2

6276.32 m s Sci 0. 02 2 13

6276.44 m 2 0. 3 Atm H2O R3 113 26

6276.590m

6276.633m

[ 24

1

3. 8

f AtmOa

1 AtmOz

R 15 R 17

2,0

2,0

22

22 6276.818m 21 3. 3 Atm O2 R 13 2,0 22 6276.938m 8 1.3 Atm O2 —

Fei?

R 19 2,0 22

6277.151r 5 0.8 w? Atm?

6277.312m 26 4. 1 Atm O2 R 11 2,0 22 6277.419m >

' 1.8 r Atm O2 R 15 2,0 22

6277.470m > 27 1.6

S,I\

] AtmOsl Til

R 17

1. 73

2,0 144

22

6277.525m . LO Atm O2 R21 2,0 22 6277.638m 19 3. 0 Atm O2 R 13 2,0 22 6277.785m 8 1. 3 Atm O2 R 19 2,0 22

6278.00 m 4 0. 6 Atm H2O R 5 113 26 6278.073m

152

1

1

4. 9 Atm O2 R9 2,0 22 6278.126m 4. 0 Atm O2 R 11 2,0 22

6278.374m 3. 5 0. 6 Atm O2 /R21

IR23

2,0

2,0 |22

6278.878m 22 3. 5 Atm O2 R9 2,0 22

6279. lOlS 27 4.3 Atm O2 R7 2,0 22 6279.233m 4 0. 6 Atm O2 R23 2,0 22

6279.318 12 1. 9 Atm —

Si I 5. 86 6279.506m 2 0. 3 Atm O2 R 25 2,0 22

6279.740 23 3. 7 u Sen 1. 50 28

oz/y.ayoo 3. 7

T? 7 9 ft 99

6280.393S 26 4. 1 Atm O2 R 5 2,0 22

6280.622S 52 8. 3 S Fei 0. 86 13 6280.791 6 1. 0 6280.89 m 1. 5 0. 2 Atm O2 R 27 2,0 22

6281.020r 1 0. 2

6281. 178S 20 3. 2 Atm O2 R5 2,0 22

274
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(i)

Equivalent Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6281.627r 1 0.2 Atm H2O R3 113 26 6295.28im s Til fO. 05

il. I.J 1\ 13 6281.781m 0. 5 0. 1 Atm O2 R27 2,0 22 6295.380r 1. 5 0. 2

6281.956S 22 3. 5 Atm O2 R 3 2,0 22 6295.650r 0. 5 0. 1 Atm

6282.500m 5 0. 8 Atm H2O R4 113 26 6295.960S 24 3. 8 Atm O2 P 7 2,0 22

6282.599r 6 1. 0 s,N Co I 1. 74 37 6296. 149r 4. 5 0. 7 6282.726m 22 3. 5 Atm O2 R3 2,0 22 6296.371r 2. 5 0. 4

6282.816 13 2. 1 u 6296.495 6 1. 1 S,d Vi 0. 30 19

6283.796S 12 1. 9 Atm O2 R 1 2,0 22 6296.66 m 2 0. 3 S Til 0. 00 1

6284.001r 0. 5 0. 1 Fe I p 3. 30 624 6297.262 7 1. 1 Atm H2O R 1 113 26 6284.536m 6 1. 0 Atm O2 R 1 2,0 22 6297.799S 65 11. 0 s Fei 2. 22 62

6285.165 7 1. 1 S Vi 0. 28 19 6298.084r 151 0. 8 Til? 1. 73 144

6285.42 m s 13,16 6298.457m 22 3. 5 Atm O2 P9 2,0 22

6285.801

6286.142

10

19

1. 6

3. 0

w

w

-Atm H2O R3 113 26 6298.60 a]

to 6299.05 a J 9 1. 4

6286.40 a

6286.800r

6287.285r 6287.749m

6287.945r

6288.315

6289.140

6289.398S

6289.581r

6289.95 a

6290.221S

6290.532 6290.974m

6292.162S

6292.362r

6292.614

6292.816

6292.958S

1

1

2. 5

13

3

3. 5

2. 5

|15|

1. 5

1. 5

21

6

66

1191

2

8

9

25

0. 2

0.2

0. 4

2. 1

0. 5

0. 6

0.4

2. 4

0.2

0. 2

3. 3

1. 0

10. 5

3. 0

0. 3

1. 3

1. 9

4. 0

s?

S

Atm

Atm H2O

Atm O2 Atm

Atm H2O

Atm O2

Atm H2O

Atm O2

Fei p

Fei

Atm O2

Atm H2O

Vi

Atm O2

R3

P 1

R2

P3

Q3

P3

2. 69

4. 73 P 5

R2

0. 29 P5

113

2,0

113

2,0

113

2,0

208

1258

2,0

113

19

2,0

26

22

26

22

26

22

22

26

22

6299.228S

6299.414r

6299.588

6300.311

6300.49 m

6300.678

6301.508S

6301.845r 6302.000m

6302. 190r

6302.499S

6302.764S

6302.948r

6303.461

6303.767m.

6304.324

6305.314r

30

3. 5

36

5

1

6

127

1. 5

23

3. 5

83

21

5

4

5

4. 5

5

4. 8

0. 6

5. 7

0. 8

0. 2

1. 0

19. 4

0. 2

3. 6

0. 6

13. 0

3. 3

0. 8

0. 6

0. 8

0. 7

0. 8

u,N

si

w

uS

Atm O2

Atm H2O

[Oi]

Sen

Fei

Fe I p Atm O2

Fei

Atm O2

Fei

Til

Zri?

Fe 11 Atm H2O

P9

R 1

0. 00

1. 51

3. 65

3. 64 P 11

3. 69 P 11

4. 32

1. 44

0. 54

6. 22 Q 1

2,0 113

IF

28

816

863

2,0

816

2,0

1140

104

24

200

113

22

26

25

22

22

15

26

6293.21 a 2 0. 3 6305.667r 3. 5 0. 6 S Sci 0. 02 2

6293.60 a 1. 5 0. 2 6305.810S 18 2. 8 Atm O2 P 13 2,0 22

6293.933 12 1. 9 u,NN Fe I p — 4. 83 1260 6306.04 m 1. 5 0. 2 S Sci 0. 02 3

6294.650 3. 5 0. 6 Atm H2O R 1 113 26 6306.218r 1. 5 0. 2 Fe I p 4. 59 1230

6295.178S |23| 3.6 Atm O2 P7 2,0 22 6306. 565S 17 2. 7 Atm O2 P 13 2,0 22

275
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6306.738r

6307.551r

6307.854

6308.62 m

6308.813

6309.394

6309.886S

2. 5

2. 5

5

6

2. 5

22

0. 4

0. 4

0. 8

1. 0

0. 4

3. 5

s

s

sM

Fe I p

Atm HjO

Atm O2

Sc II

3. 64

Q2

P 15

1. 50

863

113

2,0 28

13

2622

6319.943

6320.429

6320.843

6321.329

6322.169 6322.359m

6322.694S

4. 5

I4| 6

1. 5

19

2

75

0.7

0. 6

0. 9

0. 2

3. 0

0. 3

11. 9

u,N

u

0Iw

s

Atm H2O

La II

Sc II Atm H2O —

Nil

Atm H2O

Fe I

Q3

0. 17

1. 50

Q4

4. 15 Q 2,4

2. 59

113

19

28

113

249

113

207

26

16

17,26

26

6310.266 |13| 2. 1 W 6323.750m 4. 5 0. 7 Atm O2 P 21 2,0 22

6310.636m 12 1. 9 Atm O2 P 15 2,0 22 6323.870m 3. 5 0. 6 Atm H2O P 1 113 26

6311.239 |81 1. 3 S Ti I? 1. 44 103 17 6324.479m 4 0. 6 Atm O2 P 21 2,0 22

6311.504m 23 3. 6 S Fe I 2. 83 342 6325.165 2 0. 3 S Til 0. 02 1

6311.724r 2 0. 3 6326.46 m 1. 5 0. 2 6312.241m 5 0. 8 S Til 1. 46 104 6326.823r 2 0. 6 S Vi L 87 84

6312.758 2. 5 0. 4 6327. 270r 1 0. 2

Do i^.o / oni 1X yj. id Attn TT„0 Q 1 2fi ou 0. 1 S 1> 1 I

11. Do

6313.03 m 1 0. 2 s Zn L 58 65 17 6328.913m 2. 5 0. 4 Atm O2 P 23 2,0 22

6314.235m 10 1. 6 Atm O2 P 17 2,0 22 6329.636m 2. 5 0. 4 Atm O2 P 23 2,0 22

6314.668m 67 10. 8 s Nil / 1.93

1(4.15) P 17

4. 14

4. 14

4. 07

Q2

4. 15 Ql

Q 2

2. 45

1. 43

67 249

6330.096m 25 4.S s Cr I 0. 94 6

6314.977m

6315.314S

6315.412

6315.814S

6316.319

6316.584

6317.214

6317.418

6318.027S

11

52

16

33

3. 5

2

3. 5

4. 5

96

1. 7

8. 2

2. 5

5. 2

0. 6

0. 3

0. 6

0. 7

16. 7

w

s

u

s

Atm O2 Fei

Fe I p Atm

Fe I Atm H2O

Nil

Atm H2O

Atm H2O

Fei

(Til)

2,0

1015

1016

1014

113

248

113

113

168

103

22

26

26

26

6330.852S

6331. 129r

6331.58 m

6331.953

6332.066m

6333.235 6334.358m

6334.687r 6335.072m

6335.337S

32

1

2

11

|5|2

2. 5

1. 5

3. 5

103

5. 0

0. 2

0. 3

1. 7

0. 8

0. 3

0. 4

0. 2

0. 6

16. 1

w

0

s

Fei

Si I Fe II Atm H2O

Atm H2O

Atm O2

Atm O2 Fei

4. 73

5. 08

6. 22 P 2 P 2 P 25

P 25

2. 20

1254

199

113

113

2,0

2,0 62

26

26

2'2

22

6318.311r 3 0. 5 6336.113m 8 1. 3 S Til 1. 44 103

6318.61 49 7. 7 Cai 4. 43 53 27 6336.450r |3.5| 0. 6 Atm?

6318.708 37 5. 9 u Mgi 5. 11 23 6336.830S 121 18. 6 s Fe I 3. 69 816

6318.853m 4. 5 0. 7 Atm O2 P 19 2,0 22 6337.59 m 2 0. 3

6319.242 18 2. 8 w Mgi 5. 11 23 6338.15 a 3 0. 5

6319.490 9. 5 1. 5 Atm

(Mgi) 5. 11 23

6338.45 a 6338.880

2420. 3

6. 6 w Fe I 4. 79 1258 6319.591m 4. 5 0. 7 Atm O2 P 19 2,0 22 6339.118 |44| 6. 9 u Nil 4. 15 248

6319.84 a 2 0.3 6339.92 m s,N 13

276
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

6339.975r 1 0. 2 Fe I p 3. 40 685 6364.706 12 1. 9 w Fe I 4. 58 1229

6341.26 m 2 0. 3 Atm H2O P 3 113 26 6366.356 4 0. 6 S Ti I L 46 103

6342.26 m s 13 6366.491m 26 4. 1 w Ni I 4. 17 230

6342.389 4. 5 0. 7 Atm H2O P 3 113 26 6366. 772r 1.5 0. 2

6342.86 a 2 0. 3 6367.128 2.5 0. 4 0

6343.71 a 70 11. 0 Ca I 4. 44 53 27 6367.418 2.5 0. 4

6344. 155S 56 8. 8 s Fe I 2. 43 169 6367.82 m s,N 13

6344.82 m s Sc I 0. 00 1 13 6367.92 m s 13

6347.095 54 8. 5 0 Sin 8. 12 2 6368.464 2.5 0. 4 Atm H2O P 5 113 26 6347.305m 6 0. 9 Atm H2O P 3 113 26 6368.96 a 1.5 0. 2

6347.860 4 0. 6 Co I 4. 39 200 6369.463 18 2. 8 0 Fe II 2. 89 40

6349.48 m 3 0. 6 s V I I. 85 84 6370.357 11 1. 7 u Nil 3. 54 127

6349.75 m 4. 5 0. 7 6370.61 m 3 0. 5 S 16

6350.495

6350.719

8

4

1. 3

0. 6

Nil—

Atm H2O

4. 16 P4 113 266371.26 m

6371.355m

] 35

)

f 1. 4

{ 4.> 0 Si II 8. 12 2

6351.287 |3| 0. 4 s,NN Fe I p 4. 31 1140 6371.568 14 51 0. 7 Atm H2O P 6 113 26

6352.517r 2. 5 0. 4 6372.231m 1 0. 2 Atm H2O P 5 113 26

6352.944 4. 5 0. 7 s 6374.50 a 2.5 0. 4

yjOOO*000 3. 5 0 fi yj. o UO I i 0 111 1X

.c

KJ

6353.849r 1. 5 0. 2 s Fe I p 0. 91 13 6375.225 3 0. 5 Nil 4. 16

6354.657r 3 0. 5 6375.818 4 0. 6 Atm H2O P 5 113 26

6355.035S 62 9. 8 s Fe I 2. 84 342 6376.198 1.5 0. 2 Fe I p 4. 32 1140

booo.lo/ 17 O '7 S! Atm A +TM XT f\ ri2U "D A 11*?A'O Do/o.^oob Z /

/ / 4. 4 w "Mi -r iNl I A IK 4. 10

6357.29 m 1. 5 0. 2 s V I 1. 85 84 6378.72 a 1 0. 2

6357.86 m 1 0. 2 6378.85 m S Sci 0. 00 1 13

6358.687S 1821 12. 9 s Fe I 0. 86 13 6378.953r 1.5 0. 2

6359.91 m S Til 0. 05 1 13 6379.39 m 1 0. 2 S Vi? 2. 12 16

6360.818 16 2. 5 w Nil 4. 17 229 6379.666r 1 0. 2

6361.07 m s 13 6380.750S 40 7. 2 w Fe I 4. 19 1015

6361.205r

6361.252

4. 5

f 0. 2

1 0. 5

s Atm H2O P 5 113 266380.93 m

6381.142

1.5

2

0. 2

0. 3

s Nil 4. 42

6361.94 89? 14.2? Ca I 4. 45 53 27 6381.44 m s 13,16

6362.350m 23 3. 6 w Zn I 5. 79 6 17 6381.632r 1.5 0. 2 s 6362.876m 30 4. 7 S liCri Fe I

0. 94

4. 19 6 1019

6382.60 a 6383.44 m2 0. 3

s 13 6363.79 m 3 0. 5 [0 I] 0. 02 IF 25 6383.715 8 1. 3 0 Fe II 5. 55

6364.00 a 1. 5 0. 2 6383.906r 2 0. 3 CN Q 20 5,1 12 6364.369m 25 3. 9 Fei 4. 79 1253 6384.42 a 1.5 0. 2

277
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6384.668

6385.458

6385.726

6388.22 a

6388.427

20

2

8

2

2. 5

3. 1

0. 3

1. 3

0. 3

0. 4

wl

u

Mn I —

|Nii

Feii

Fe I p

CN

Fe I p

3. 77

4. 15

5. 55

4. 73

Q21

0. 0/

39 246

1253

5,1 DoO

17

12

6408.682

6410.431r

AJ.1 1 1 1 Q

D'il 1 .DOoo

A/f 1 0 OQQ^ O'iiZ.iiOOr

8

2

A

0

ijy

0

1. 2

0.3

u. y

u. y on 1 ZU. 1

U. 0

s

u

0

1

S

Atm H2O

r e I

r e I

r e I

R' 5

Q ACL 0. 00

Z. 40

311

1 0 CA izoo

CIA olO

1 AO loy

16, 26

Doyu.'iyo o n Q U. o La II 00 D'±io.i'± a u. 0 u. 1 S i 1 1 p U. Uo 1

Doy i.zoyr Ml U. O 0^:10. oZ m 1.0 OC I

f\ no U. Uz 1

ooy^.ooo 1 n J. 0 s i? e I 0 OS 1 no AJ.1 Q CiQQT» Z.O U. 4

D£>9a.iy a

o U. oAA1 Q OQO D^io.yoz 9 U. 0 OA y zo 0,1 1 0Iz

iy. i s rex AAl/l c;qa D'ii4:.0y^ 10 z. 0 w iM I 4. lo OA A z44

6394.223 6 0. 9 6414.987 45 7. ^ W Si I 5. 87

6394.487r 1. 5 0.2 Attn H2O P 8 113 26 6415.424r 5 0. 8 CN Q25 5,1 12 cone 1 AQ D u. y *-^0 I 0, oi i /'I A^ 1 A HQ 1

V

D'lJ.D.Uoir 0 *2 U. 0

6395.47 m

6396.388r

1

1

0. 2

0. 2

S

Cai

CN

Fe I p Q210. oy

5,1 00 1 12

AAl 04 A10. Do ur AAl A QOQrYi 041:10. yzoin

A41 7 AQf^ 0^1 / ,OoO

|4/.f)|

Qy

u. 0

/. 0

1. 4

w

s

r e II Paoa TI

0. oy

4. 44

1 4

6397.545r 1 0. 2 Atm 6417.884r 2.5 0. 4

6397.974 3 0.5 s,d? CN Q 23 5,1 12 6419.09 m 1.5 0. 2 S Til 2. 17 196

6398.917r |3| 0.5 Atm 6419.374r 2 0. 3

6400.009S

6400.323S

6400.811r

D4(Jl.yo m

6402.295r

o4Uo.lz /

6403.698r

181

46

2

1. 5

1

28. 3

7.2

0. 3

0. 2

U. o

0. 2

sS

s

0

Fei

Fei

CN

"V T X I

3. 60

0. 91 Q22

C\ OA

816

13

5,1

0,1

12

1 1? lo

iz

6419.650

6419.956S

6420.75 m

6421.360S

6421.526

6424.862

9

80

2

87

16

11

1. 4

iS. ^

0. 3

13. 5

2. 5

1. 7

u?

w

s

0?u

01

CN

Fe I p Fei

CN

Fe I Nil

Atm H2O

Nil

Q27

3. 94

4. 73 Q26

2. 28

4. 16 R4

4. 17

5,1 958

1258

5,1

111 258

212 227

12

12

17, 26

b4U4.16Ur 11 0. I D4Z0.0o/r Z.o U. 4 0,1 1IZ9

C /f AK AC r,^ D4U5.40 m D 0. y CJN 0,1 A/) OA OQ

1

0

u. 0

Ci^ 07Zl 0,1 1IZ9

6405.763 13 2. 0 u?,NN 6426.683 3 0. 5

6406.07 m 1. 5 0. 2 s 16 6428.174r 1 0. 2 CaT?p 4. 44

6406.28 m 2 0. 3 6428.67 a 0.5 0. 1

6407.113 6 0. 9 Sii?p 5. 87 6429.902 2.5 0. 4 u,N Co I 2. 14 81

6407.291 |26| 4. 0 0 Sii Fe II5. 87

3. 89 74

6430.274r 6430.454r

2 0. 3 Atm

6408.026S |80| 12. 5 s Fei 3. 69 816 6430.50 m } [0. 1 s Vi 1. 95 107

6408.375r |5| 0. 8 CN Q25 5,1 12 6430.856S 106 16. 8 s Fei 2. 18 62

6408.47 m 3 0.5 s Sri 2. 27 8 6431.255r 1.5 0. 2

278
The Solar Spectrum—Continued

Equi- Re- Low RMT Eq ui- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(A) (V) vr J Line Band \XIln.l Line Band

6431.63 m s Vi 1. 95 107 13 6450.654r 1 0. 2 CN Q 31 5,1 12

6431. 679r 1.5 0. 2 — CN Q 29 5,1 12 6451. 573r 3 0. 5 Ni I 4. 16 257

Fe I 3. 69 921

6432.023 1.5 0. 2 CN Q 28 5,1 12 Nil 3. 54 126 6452.08 m s? 13 6432.683m 38 5. 9 W Fe II 2. 89 40 6452.315 6 0. 9 ,S Vi L 19 48

6432.966 4.5 0. 7 Atm H2O R 3 212 26 6452.688r 1.5 0. 2 s Ni I? 4. 09 226

Atm

6433.452 15 2. 3 u,N 17 6453.602r 2.5 0. 4 6433.737r 5 0. 8 6453.92 a 1 0. 2 Atm

6434.571 2 0. 3 0? Atm?

6454.139 4 0. 6 Atm H2O R 6 311 26

6435.049r |1.5| 0. 2 s Yi 0. 07 2 6455.001 11 1. 7 Co I 3. 63 174

6436.25 a 1.5 0. 2 Atm

6455.605S 48 7. 4 s Ca I 2. 52 19 6436.413 7 1. 1 s Fe I 4. 19 1016

6455.90 m 2 0. 3 6436.923r 1.5 0. 2 Atm

6456.391S 57 9. 3 w Fe II 3. 90 74

6437.698 6 0. 9 Eu II — 1. 32 8 6456.58 a 3 0. 5 6438.040r 2 0. 3 CN — Q 29 5,1 12 CN Q 30 5,1 12 6456.865 17 2. 6 wl Fe I p 4. 79 1256

Ca II 8. 44 19 6438.773 7 1. 1 s Fe I 4. 43 1158

6457.114 6 0. 9 s.dl — Atm? 17 6439.083in 156 25.6 s Cai 2. 52 18 6457.380 8 1. 2 6439.53 a r 0.2

2 6458.556r 2 0. 3 CN Q 33 5,1 12 6439.72 a J 1 0.1 6458.682 3 0. 5 Atm

6440.19 a 1.5 0. 2 Atm

6458.892 10 1. 5 Atm H2O R 5 311 26 6440.645 1.5 0. 2 6459.080r 1 0. 2 Atm

6440.934 4 0. 6 s,d? Mn I 3. 77 39 6459.683 5 0. 8 Atm H2O R 5 311 26

6441.624r 1.5 0. 2 Atm

6459.987 3 0. 5 Atm

6442.482r 2 0. 3 6460.223 2.5 0. 4 Atm H2O R 5 311 26 6442.950 3.5 0. 5 Fe II 5. 55

6460.934r 3 0. 5 Atm?

6443.55 a 4 0. 6 Atm'HjO R' 3 311 26

6461.10 m 11.51 0. 2 6444.218r 1 r 0.2 CN Q30 5,1 12

^ 4.5 6461.838 5 0. 8 Atm

6444.41 a 1 1 0.5

6462.032 4.5 0. 7 Atm

6444.71 a 3 0. 5 CN Q31 5,1 12 6462.570 |23. 2 S Ca I 2. 52 18 6445.72?m 1 0. 2 s Zn 1. 00 57 216 (2. 45 6462.749 i 111. 6 s Fe I 168

6446.133r 2 0. 3 Atm 1(0.91) 13

6446.400 5 0. 8 Fe II 6. 22 199 6463.19 m 4 0. 6 Atm H2O R 5 311 26

6447 943 2.5 0. 4 Atm H2O R 3 212 26 6463 493 8 1. 2 Atm

6449.127 34 5. 3

« AT J s,N,a 17 6463.744r 3 0. 5 Atm

6449.601 2.5 0. 4 Atm 6463.955r 1.5 0. 2 6449.820S 98 15. 2 S Cai 2. 52 19 6464.183r 2 0. 3 CN Q 33 5,1 12 6450.179 24 3. 7 s,N Co I 1. 71 37 6464.427 9 1. 4 Atm H2O R 5 311 26 6450.325 20 3. 1 s,N 6464.679 10 1. 5 S Cai 2. 52 19

279
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6465.409r 2 0. 3 Atm? 6478.65 a 4. 5 0. 7 CN Q 35 5,1 12

6465.787r 2.5 0. 4 CN Q34 5,1 12 6479.188 5 0. 8 Atm

6466.138 4 0. 6 Atm II2O R 9 311 26

6479.490 2. 5 0. 4 Atm H2O /R3

IR4

311

311 |26

6466.265

6466.726

6466.997

6467.593

181

|51

5

6

1. 2

0. 8

0. 8

0. 9

s

Atm H2O

Atm H2O

Vi

Atm H2O

R4

R 5

1. 05

R 8

311

311

32

311

2626

26

6480.066

6480.252r

6480.983

9

1

1. 5

1. 4

0. 2

0. 2

Atm H2O

Atm

CN

Atm

R4

Q 36

311

5,1

26

12

6467.83 m s 13 6481.684 1 0. 2 Atm

6467.887 5 0. 8 Atm II2O \W 1

J R 4

3111 311/ 26 6481.878m 63 9. 7 s Fei 2. 28 109

6467.984 14| 0. 6 6482.185 7 1. 1 Fe II? 6. 22 199

6468.363 3 0. 5 Atm H2O R 4 311 26 6482.809S 38 5. 9 s Nil 1. 93 66

6468. 834r 3 0. 5 Fe I p 4. 79 1254 6483.062r 1. 5 0. 2 Atm

6469.192m 52 8. 0 u Fei /4. 83

1(2.40) 1258

168

6483.245

6483 .453r

10

1

1. 5

0. 2

Atm H2O

Atm

R 3 311 26

6469.364 6 0. 9 Atm H2O R 4 311 26 6483.762 5 0. 8 Atm H2O R 2 311 26

6469 989

12

1

1. 8

f 0.77

Atm H2O

Atm H,0

R 7 R 4

311

311

26

26

6483.940 11 1. 7 s |Fei p

Atm H2O

1. 48

R3

34

212 26

6470 02 m > 0 7 6484.470r 2 0. 3 Atm

6470.23 m 111 0. 2 $ Zr I 1. 58 65 6484.672 2. 5 0.4 Atm H2O R2 311 26

6470.896 2.5 0. 4 6485.18 a 3 0. 5

6471.17 m |1.5| 0. 2 6485.559 2. 5 0. 4 Atm H2O R3 311 26

6471.668S

6472.144r

6472.477

6472.605

d47o.183

6473.528r

6474.117

6474.614r

83

2.5

12

6

17

1

4

4

13. 4

0. 4

1. 8

0. 9

2. 6

0. 2

0. 6

0. 6

B Cai

Fe I p Atm H2O

Atm?

A XT r\ Atm HjU

Atm

Fei

2. 52

4. 37 R 6

R 4

3. 63

18

1140

311

311

861

26

26

6486.277r

6486.782

6487.291r

6487.539

6488.025

6489.129

6489.651r

|3|

4. 5

2

1. 5

2

5

6

0. 5

0. 7

0. 3

0. 2

0. 3

0. 8

0. 9 s

CN

Fei?

Atm H2O

Atm

Atm H2O

Atm H2O

Atm H2O

Zri

Q 36

R2

Q3

R2

R 2

1. 55

5,1

311

311

212

311

65

12

26

26

26

26

6475.058

6475.213

18

25

2. 8

3. 9

Atm H2O

Atm H2O

R 3 R 5311

311

26

26

6490.376r

6490.652r

5

2. 5

0. 8

0. 4

Coi

Atm

Atm H2O

Fe II

Till Mn I Atm H2O

Fe II

2. 04 81

26

26

6475.632S

6475.824

6476.568

6477.013

6477.329

57

16

4.5

4

5

8. 8

2. 5

0. 7

0. 6

0. 8

s Fei

Atm H2O

Atm

Atm H2O

Atm —

Fei?

2. 56 R 3

R 3

206

311

311

26

26

6490.793

6491.246r 6491.582m

6491.666

6492.909

6493.06 m

|14|

3. 5

1 45

J

10

6

2. 2

0. 5

f 5.

9

1 ...

1. 5

0. 9

w

s

R2

5. 58

2. 06

3. 76 R 1

5. 58

311

91

39

311

6477.869 6 0. 9 0 Co I 3. 77 174 6493.245 5 0. 8 Atm H2O /R 1 IR 2 212

212 |26

280
The Solar Spectruin—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

6493.788S 133 ^0. 5 s Cai 2. 52 18 6506.39 m s Zr I 0. 63 13

6494.10 a 2 0. 3 Atm 6507.661r 3 0. 5 Atm H2O Ql 212 26

6494.304r 3 0. 5 Atm? 6508.154r 3 0. 5 S Til 1. 43 102

6494.499 34 5. 2 w Fe I p 4. 73 1255 6508.593 14 2. 2 0 Atm H2O Q2 311 26

6494.994S 165 26. 2 s Fei 2. 40 168 6508.846 11 1. 7 s Cai 2. 52 18

6495.740 42 6. 5 wl Fei 4. 83 1253 6509.608 3. 5 0. 5 u,d? Fei p 4. 07 1012 16

6495.862 8 1. 2 Atm H2O R 1 311 26 6510.42 a 2 0. 3 CN Q39 5,1 12

6496.120r 3 0.5 6511.10 m 3 0.5 6496.472m 69 10. 6 wt Fei 4. 79 1258 6511.449r 0. 5 0. 1 Atm

6496.908m 98 15. 4 s Ba II 0. 60 2 6511.999 8 1. 2 Atm H2O Ql 311 26

6497.50 2 0. 3 Atm H2O Q4 311 26 6512.242 8 1. 2 Atm H2O Q4 311 26

6497.594 3 0.5 Atm H2O R 1 311 15,26 6512.921r 0. 5 0. 1

6497.68 a 5 0. 8 S Til 1. 44 102 6513.070r |3| 0. 5 Atm

6498.24 a 2 0.3 6513.602 2 0. 3 Atm H2O Q5 311 26

6498.433r 1.5 0. 2 6514.288 6 0. 9 Atm H2O Q3 311 26

6498.75 m s Bai? 1. 19 6 13 6514.727 33 5. 1 Atm H2O- Q 2 311 26

6498.945S 43 8. 6 S Fei 0. 96 13 6515.23 Ir 0. 5 0. 1

6499.216r 4.5 0.7 6515.73 m 4 0. 6

6499.654S 81 12. 5 S Cai 2. 52 18 6515.848 |12| 1. 8 Atm H2O Q2 311 26

6499.93 m 2 0. 3 Atm? 6516.083S 61 9. 4 w Fe 11 2. 89 40

6500.39 m 3.5 0. 5 6516.437 /

"

Atm H2O Q 3 311 26

6500.839r 2.5 0.4 6516.543 156 < 3. 5 Atm H2O Ql 311 26

6501.203

6501.678

6502.22 a

6502.40 a

650 .95 a

6503.45 a

9

25

7

2

6

4

1. 4

3.6

1. 1

0.3

0. 9

0. 6

S,d

s

CriAtm

Fe I Nil

Atm

Atm

Atm H2O

0. 98

3. 40

Q6

16

311 26

6516.625

6517.082

6517.700r

6518.011

6518.373S

6518.741

|18|

1. 5

12

61

|23|

[ 4. 0

2. 8

0. 2

1. 8

9. 4

3. 5

sw

Atm H2O

Atm H2O

Atm H2O

Fe I

Si I Atm H2O

Q3

Q4

Q 4

2. 83

5. 95

Q6

311

311

311

342

62

311

26

26

26

26

6503.75 a 5 0. 8 Atm H2O Q3 311 26 6519.02 a 131 0. 5

6504.00 m 1.5 0. 2 s Sri 2. 26 8 6519.170 5 0. 8 Atm H2O Q4 311 26

6504.186

6504.472r

6504.92 a

6505.08 a

6505.488r

6506.36 m

17

1.5

|1.5|

1

6

121

2. 6

0. 2

0. 2

0. 2

0. 9

0.3

s IIVi Atm H2O

Atm

CNAtm

Fe II

1. 18 R 0

Q 39

5. 59

48

311

5,1

26

12

6519.452

6519.75 a

6520.124

6521.50 a

to 6521.65 a

6521.891r

6522.192

|20|

3. 5

1. 5

1

3

3. 1

0. 5

0. 2

1. 5

0. 2

0. 5

Atm H2O

Atm H2O

Atm H2O

Q3

Q 6 Q2

311

311

311

26

26

26

281
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6522.913r

6523.327

6523.656

6523.843

6524.7 a

to 6525.3 a

6525.807r

131

3

4

21

} ^

|3.5|

0. 4

0. 5

0. 6

3. 2

0. 8

0. 5

Atm

CN

Atm H2O

Atm H2O

Atm H2O

Fe I p—

Atm H2O

Q41

Q5

Q 1 P 1

5. 01

Q4

5,1

311

212

311

1280

311

12

26

26

26

26

6540.430r

6541.274r

6542.313

6543.044r

6543.51 m

6543.907

6545.781

3. 5

2

14

5

3

34

8

0. 5

0. 3

2. 1

0. 8

0. 6

5. 2

1. 2

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Vi

Atm H2O

Atm H2O

Q2

P 3 P3

Q' 2

1. 19 P 3

fP 3 IQ3

212

212

311

311

48

311

311

212

26

26

26

26

26

26

26

6526.421

6526.653

6526.95 a 6527.215m

6527.30 m

6527.598r

6528.113r

6528.539

6529.187r

6530.10 a

6530.598

6531.077r

6531.429

6532.359

6532.572r

6

28

2

53

4

1

11

2

1

7

2

5

24

3

0. 9

4. 3

0. 3

8. 1

0. 6

0. 2

1. 7

0. 3

0. 2

1. 1

0.3

0. 8

3. 7

0. 5

w,d

0?

s

s

s

u

Sii?p

SiiLa II?

Si I

CN

Fe I Cn

Atm H2O

Atm

Vi

Atm H2O

5. 87

5. 87

0. 23

5. 87

Q41

3. 89

Q3

1. 22 P 2

33

52

5,1

265

311

48

311

17

17

13

12

26

26

6546.252m

6546.94 m

6547.29 m

6547.705

6548.34 m

6548.622

6549.054r

6550.26 m

6550.278r

6550.90 a

6551.701

6552.035

6552.629

6552.77 m

103

2. 5

1

16

3. 5

20

2. 5

} ^

|2|

|8|

3

|19|

1. 5

15. 7

0. 4

0. 2

2. 4

0. 5

3. 0

0. 4

f 0.

4

1 0. 4

0. 3

1. 2

0. 5

2. 9

0. 2

s

u,d1

s

s

S

IIFei Til

Atm

lAtmHaOTii?

Atm H2O

Atm

Sri

Atm

Fe I p

Atm?-

Atm H2O

Atm H2O

Fei

2. 76

1. 43

P 3

P 3

2. 69

0. 99

P 4 Q4

5. 02

268

102

311

311

12

13

311

311 1325

17,26

26

26

26

6532.881 18 2. 8 s Ni I 1. 93 64 6553.785 13 2. 0 Atm H2O P 4 311 26

6533.102r 2. 5 0. 4 6554.238 14 2. 1 s Til 1. 44 102

6533.535r 2 0. 3 6554.843 3 0. 5 s

6533.940

6534.000

1 46

f 5. 2

1 1.9

w,d Fe I Atm H2O4. 56 P 2

1197

311

17

26

6555.11 a

6555.466

3

40

0. 5

6. 1 w

Atm H2O

Si I

P 4

5. 98

212

62

26

6534.236r 7 1. 1 Atm 6555.856r 4 0. 6 s? Fe I p 4. 07 1007

6534.641 2. 5 0. 4 Atm 6556.077 14 2. 1 s Til 1. 46 102

6534.975r 4 0. 6 Atm H2O Q5 311 26 6556.321r 1. 5 0. 2 Atm?

6535.60 a

6535.977r

6536.47 m

6536.720r

6537.431r

2. 5

0. 5

38

2

0. 4

0. 1

0. 5

1. 2

0. 3

s

Atm

Atm H2O

Atm

P 2 311

1626

6556.806

6557.171

6557.37 m

6557.857r

16

15

1. 5

2. 4

2. 3

0. 2

s

FeiAtm

Atm H2O

Yi

Atm

4. 79

P 4

0. 00

1255

311

1

17

26

13

6537.938

6538.538r

2. 5 60. 9

0. 9

S Cn

Atm H2OSi?

1. 00

P 2

8. 04

16 212

1526

6558.03 m

6558.149

1

7

0. 2

1. 1

S,N Vi

Sci?

Atm H2O

1.38

2. 61 P 4

5924

311 26

282
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6558.65 a 1. 5 0. 2 Atm HjO P 4 311 26 6578.28 a 3 0.5

6558.955r 1. 5 0. 2 Atm 6578.96 m 2 0. 3 s Vi 1. 04 32

6559.576 14 2. 1 w Till 2. 05 91 6579.08 m 1 0. 2 s?

6559. 813r

6560.258r

6560.555

3

3

22

0. 5

0. 5

3. 4 w,d AtrnHjO —

Si I P 4

5. 96

31162

17, 26

6580.233r

6580.785

6580.99 a

10

3. 5

2

1. 5

0. 5

0. 3

0

s

NiiAtm

Atm H2O

Cri

4. 42

P 6

1. 03

265

311

16

26

6561.097 151 0. 8 Atm H2O P 4 311 26 6581.218 14 2.4 s Fei 1. 48 34 6562.808m 4020 649 W Ha 10. 20 1 6583.259 1. 5 0. 2 Atm H2O P6 311 26

6563.41 m s Co I 2. 04 80 13 6583.538 1. 5 0. 2 Atm H2O P 6 311 26

6563.521 4. 5 0. 7 Atm H2O P 5 212 26 6583.710 15 2. 3 o?,d Si I 5. 95 17

6564.061 4. 5 0. 7 Atm H2O P 5 311 26 6584.558 3 0.5 Atm

6564.206 14 2. 1 Atm H2O P 5 311 26 6585.529r 1. 5 0.2

6565.545 3 0.5 s Atm H2O- R3 231 26 6585.710r 2 0. 3 Atm H2O Q3 231 26

6565.90 a 1 0.2 s? Vi 1. 18 48 6586.319m 35 5. 3 s Nil 1. 95 64

6567.85 a 2 0. 3 Atm 6586.511 4 0. 6 Atm H2O P7 311 26

6568.806 3. 5 0. 5 Atm H2O P 5 311 26 6586.682 4 0. 6 Atm H2O P6 311 26

6568.90 m 5 0. 8 6587.622 21 3. 7 0 Ci 8. 53 22

6569.224S

6570.052m

6570.630m

6570.84 a 6570.979m

6571.18 a

6572.086

6572.795

71

111

4

3

2

5

1191

1261

11. 9

0.2

0. 6

0.5

0.3

0. 8

2.9

4-1

w

S

Fei

(Sm 11) Atm H2O

Atm H2O

Atm

Fei

Atm H2O

Cai

4. 73

1. 49 R2

P 5

4.29

P 5

0. 00

1253

62

231

311

1121

311

1

26

26

26

6588.590

6589.10 a

6590.01 Ir

6591.326

6591.599r

6591.841r

6592.522

6592.926S

2

2. 5

1

10

1. 5

4

23

123

0. 3

0.4

0.2

1.6

0.2

0. 6

3. 5

18. 8

w

w

s

Atm

Fei

Nil

Fei

(Ti I p)

4. 59

4. 23

2. 73 1.44

1229

248

268

102

6573.526r m 0.2 Atm H2O R4 231 26 6593.63 a 1.5 0.2

6574.254 22 3. 6 s Fei 0. 99 13 6593.884m 89 13. 3 S Fei 2. 43 168

6574.474r |1.5| 0.2 6594.361 8 1. 2 Atm H2O P7 311 26

6574.852

6575.037

6575.18 m

6576.376

19

64

0. 5

5

2.9

9. 7

0. 1

0. 8

s

s

Atm H2O

Fei

Til

Atm H2O

Nil

fP5

IP 6

2. 59

2. 58 P 6

311

311

206

286

311

}26

26

6595.355r

6595.887

6597. 038r

6597.571

4

7

1. 5

44

0. 6

1. 1

0. 2

6. 7

s

0?

w

Til?

Co I Atm H2O

Fei

(Cri)

3. 71 P 7

4. 79

4. 17

174

311

1253 282

26

6576.59 m 2 0. 3 s 6598.38 m 3 0. 5 Nil

Til

Atm H2O

6576.894

6577.60 a

1. 5

9

q. 2

1.4

6598.611

6599.113

6599.324

26

8. 5

4

3. 8

1.4

0. 6

w

S

4. 23

0. 90

P 8

249

49

311 26

283
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6600.65 a

6601.20 a

6601.48

6601.98

6602.134r

6603.25

6603.43

6603.65

6604.40

6604.600

6604.80 a

6605.574r

4

1

2

}

^

1. 5

1. 5

3

1

36

1. 5

6

0. 6

0. 2

0. 3

0. 5

0. 2

0. 2

0. 4

0. 2

5. 6

0. 2

0. 9

s

w

s

O?

r Atm H2O

1 Atm

Fei ?p

Atm

Fe I p

Sen

Cri

Atm H2O

P7

3. 64

3. 63

1. 36

4. 14 P8

311

862

860

19

282

311

26

1726

6617.14

6617.27

6617.60

66l7.743r

6618.349r

6619.12

6619. 588r

6621.11

6621. 204r

6622.402r

6622.94

6623.22 a

3

0. 5

2. 5

3. 5

2. 5

2. 5

|3|

1

2. 5

|3|

2

2

0. 5

0. 1

0. 4

0. 5

0. 4

0. 4

0. 5

0. 2

0. 4

0. 5

0. 3

0. 3

s

S

Atm?

Nil

Sri

Co I? 0?

0?

Atm?

Sii?p

Nil?

Fe I p

Atm?

4. 23

2. 25

4. 47

5. 96

3. 60

4. 39

248

8

97

1157

17

6605.924r

6606.04 a

5

3

0. 8

0. 5

S Vi 1. 19 48 6623.82

6623.924r 1

' 0. 8

f Feip

1 0?

4. 07 1010

6606.75 2 0. 3 0? 6624.368r 2 0. 3 0?

6606.979r 8 1. 5 0 Ti II p 2. 06 91 6624.840r 4 0. 6 S Vi 1. 22 48

6607.40 a 5 0. 8 6625.039r 1. 8 s Fe I 1. 01 13

6607.90 s Vi 1. 35 59 13 6626.267r 1. 5 0. 2 Atm

6608.044r 18 2. 7 s Fe I 2. 28 109 6626.43 |1| 0. 2 Atm H2O P 10 311 26

6609. 11 8S 76 10. 9 s Fe I 2. 56 206 6627.32 2. 5 0. 4 Fe II 7. 27 210

6609. 582r 13 2. 0 s,N Fe I 6627.560r 24 3. 9 w Fei 4. 55 1174

6609.693r 5 0. 8 s Fe I p 0. 99 13 6628.165r 1 0. 2 Atm?

66l0.079r 3 0. 5 6629.390r 1 0. 2 Atm

6610.82 a 4 0. 6 Nil? 5. 28 6629.686r 1 0. 2 0

6611.50 a 3 0. 5 6630.032r 6 0. 9 S Cri 1. 03 16

6611.96 1 0. 2 Atm 6630.73 a 2 0. 3

66l2.237r 5 0. 8 s Cri 4. 16 282 6631. 087r 1. 5 0. 2 Sii?p 5. 98 62

6612.553r 0. 5 0. 1 Atm H2O P9 311 26 6631. 773r 1. 5 0. 2 Atm?

6613.420 10 1. 5 w 6632.029r 4 0. 6

6613.73 4 0. 6 w,N Yii 1. 75 26 6632.472r 5 0. 8 u Co I 2. 28 111

6613.83 5 0. 8 s Fe I p 1. 01 13 16 6632.73 1 0. 2 0?

6614.71 1 0. 2 Atm? 6633.427r 30 4- 1 w Fe I 4. 83 1258

6615.01 2 0. 3 Fe I p 4. 47 1155 6633.758m 70 10. 4 w Fe I 4. 56 1197

6615.63 3 0. 5 0? 6634.123r 40 5. 6 w Fe I 4. 79 1258

6616.20 |2.5 0. 4 Sii?p 5. 95 6635.137r 19 3. 6 w Ni I 4. 42 264

6616.83 3 0. 5 0? 6635.398r 1 0. 2 CN? R 10 7,3 12

6616.95 a 2 0. 3 6635.702r 7 1. 1 w Si I Fe I p

5. 86

4. 43 1155

284
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/\

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6636.332r 2 0. 3 Cri 4. 14 282 6659.00 a 1 0. 2

6637.24 S G 13 6659.866r 3 0. 5 0? O

6638.14 a 4 0. 6 6660.32 0. 5 0. 1 Atm?

6639.45 a 2 0. 3 CN Q 5 7,3 12 6661. 081r 10 1. 5 s Cri 4. 19 282

6639.717r 17 2. 6 w Fe I p 4. 61 1195 6661. 341r 6 1.2 w Ni I 4. 23 246

6639. 897 11 1. 7 s Fel 4. 07 1007 6662.580r 1. 5 0. 2 O?

6640.95 a 1. 5 0. 2 6663.01 13

0. 5 C I 8. 85

6641.63 a 1 0. 2 6663.246 31 4. 7 w Fe I 4. 56 1195

6642.272r 1. 5 0. 2 Atm? 6663.448 76 11. 9 s Fe I 2. 42 111

6642.53 1 0. 2 Atm? 6663.84 a 2 0. 3

6643.00 2 0. 3 Cri 3. 84 256 6664.310r 1 0. 2 CN? R19 7,3 12

6643.638S 83 13. 6 s Ni I 1. 68 43 6665.06 1 0. 2 1 O

6643.864r 2 0.3 O? 6665.27 5 0. 8 } 6644.35 a 2 0. 3 CN R 15 7,3 12 6665.47 2 0. 3 S Fe I p 1. 56 34

6645.127r 4 0. 6 Eu II 1. 38 8 6665.83 1. 5 0. 2 Atm?

6645.41 a 1 0. 2 6666.540r 2 0. 3 S Til 1. 46 101

6646.20 s O 13 6666.73 1. 5 0. 2 Atm?

6646.966r

6647.856r

6648.121r

|7|

2. 5

5

1. 2

0.4

0. 8

s

S

Fe I Fe I p Fe I p

2. 61

3. 24

1. 01

206

551

13

6667.23

6667.455r

1. 5

3. 5

0. 2

0. 5 s

CN?

Fei

fP 6 IR20

2. 45

7,3 7,3 168

|12

6649.20 2 0. 3 O

6667.740r 7 1. 2 s Fe I 4. 58 1228

6649.51

6650.60

6651. 132r

6652.361r

6653.04 a

€653.37 a

6653.67

€653.911r

6655.531r

1

1. 5

3

1

1

0. 5

8

3

0. 2

0. 2

0. 5

0. 2

0. 2

0. 1

^. 4

0. 5

S

w

O

Atm

O

Sii?:p

CN?

O

Fe I Atm

Ci

5. 96 Rl

4. 15

8. 53

7,3

1052

13

12

6668.400r

6668.801r

6669.01 a

6669.310r

6671.82

6672.675r

6673.88

6674.19

6676.89

6677.24

3

HI

1. 5

5

6

2. 5

1

1

1

2

0. 6

0. 1

0. 2

0. 7

0. 9

0. 4

0. 1

0. 1

0. 1

0. 3

s

u

S

O

Si i?p

Cri

Ci

O

Fe I p Ci?

Fe I p Til

5. 96

4. 17

8. 85

4. 73

8. 84

4. 56

2. 49

282

1254

1194

274

6656.36

6656.65

6657.00 a

6657.43

1. 5

1. 5

1. 5

0. 5

0. 2

0. 2

0. 2

0. 1

o

oCN?

Cn

Atm?

R 16

4. 16

7,3 282

12

6677.54

6677.997S

6678.576r

6678.849r

3

122

2

5

0. 4

19. 0

0. 3

0. 7

s

s

Fe I p Fe I p Fe I Til

Co I

3. 21

5. 01

2. 69

2. 25

1. 96

551 1280

268

213

54 6657.639r 2 0. 3 6679.58 1 0. 1 Ci?p 8. 85 6657.95 1 0. 2 Atm? 6680.155r 6 0. 9 w,N Cri 4. 16 282

285
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Banc

Notes

6680.32 a 2. 5 0. 4 6703.97 a 2. 5 0. 4 CN P 16 7,3 12

6681.30

6682.00 a

3

1. 5

0. 4

0. 2

CN?-

Fe I p Q 16

4. 39

7,3 1155

12 6704.500r

6705.105

5

42

0. 7

6. 6

sw

Fei

Fei

(Feip)

4. 22

4. 61

4. 95

1052

1197 1280

6682.24 111 0. 1 Fe I p 4. 07 1008 6705.507r 1. 5 0. 2 O?

6682.78 2 0. 3 6706.75 1 0. 1 CN? Q 22 7,3 12

6683.69 1 0. 1 Atm? 6707.05 1. 5 0. 2 Si i?p 5. 95 61

6684.05 2 0. 3 Atm 6707.449r |5| 0. 7 s? O

6684.8901-

6685.04

]

1 ' 0. 3

[ Co I

1 O

2. 72 140 6707.76

6707.98

1. 5

0. 5

0. 2

0. 1

S

S,N

Li I

Li I

0. 00

0. 00

1

1

6687.26 a 1 0. 1 6708.32 0. 5 0. 1 O

6687.508r 3 0. 4 S Yi 0. 00 1 6708.80 1 0. 1 u,NN O

6687.74 2 0. 3 O? 6709.10 a 2 0. 3 0 CN? P 17 7,3 12

6687.96 1 0. 1 CN Q20 7,3 12 6709.87 m s Cai 2. 93 45 13

6688.83 a

6689.30

6690.61

6690. 825r

6691.61

6692.304r

6692.50 a

6692.856r

6694.62

6696.032

6696.322r

6696.69

6696.92 a

1. 5

1

0. 5

3

1

0. 2

0. 1

0. 1

0. 4

0. 1

C I? CN?

o?

o?

Nil

O

Fei?

Fe I CN?

CN?

All

Fe I p O?

8. 85 Q 18

3. 63

7,3

140

12

6709.935r

6710.323r

671 0 542r

6710.70 a

6711.282r

6711.58

2

12

\

1. 5

2

1

0. 3

1. 8

0. 1

0. 2

0. 3

0. 1

s Fe I

Fe I p

O

1. 48

4. 58

34

1220

2

1. 5

0. 3

0. 2

0. 4

0. 1

5. 1

2. 4

0. 2

0. 4

4. 56 Q 19 P 14

3. 14

4. 83

1192

7,3

7,3

5

1255

12

12

67ll.847r

6712.467r

3

2. 5

0.4

0. 4

CN?

Fe I p

Q23

4. 99

7,3

1279

12

3

1

33

16

1. 5

3

sw

6713.044

67l3.207r

6713.745

6714.80

6715.386

24

7

23

2

33

3. 6

1. 0

3.6

0.3

4.6

0

sw

u

Fei

Fei

Fei

Atm

Fei

(Cri)

4. 61

4. 14

4. 79

4. 61

4. 17

1195

1013

1255

1174 282

6697.406r 4 0. 6 O 6715.70 a 2. 5 0. 4 6698.00 1. 5 0. 2 CN Q22 7,3 12 67l6.252r 15 2. 4 w Fe I 4. 58 1225

6698.669r 21 S. 1 s All 3. 14 5 67l6.666r 2 0. 3 S Til 2. 49 273

6699.136r 7 1. 0 u Fe I 4. 59 1228 6716.95 a 1 0. 1 O

6700.56 a 1 0. 1 O 6717.19 a 1. 5 0. 2 CN Q 24 7,3 12 6700.919r 1. 5 0. 2 Nil

Fe I p

4. 26

/4. 47

15. 07

248

1156

1333

6717.38 a

67l7.527r

2

11

0. 3

1. 9 0? Fe I 4. 61 1194

6701. 377r 1. 5 0. 2 671 7 687S 1JL 20 17. 7 Ca I 2. 71 Q9

6702.55 1 0. 1 o? 6719.62 21 3. 1 s,N O

6703.37 a 1 0. 1 CN Q 23 7,3 12 6720.77 2 0. 3 O

6703.576m 32 6. 2 s Fei 2. 76 268 6721.844m 55 7. 5 0 Si I 5. 86 38

286
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent W lutn AX

(mA)

Re- duced

Vv idth

AX/X

(F)

bpOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

W Kith

AX/X

(F)

tapOt Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Uand

Notes

6722.82 a 2 0. 3 CN? Q 25 7,3 12 6744.50 2. 5 0. 4 G

6724.685r 4 0. 7 0? O 6745. 113r 7 1. 0 U Fei 4. 58 1227 6725.364m 17 2. 5 w Fe I 4. 10 1052 6745.547r 4 0. 6 S Ti I p 2. 24 226

6725.710r - - O 6745.984 8 1. 2 s? Fei 4. 07 1005

6726.282 1 0. 1 0 I 9. 14 2 6746.20 a 2 0.3

6726.673m 50 7. 6 w Fei 4. 61 1197 6746.36 0. 5 0. 1 Til 1. 89 152

6729.05 a 9 1. 3 s Fei 6746.975r 5 0. 7 Fei 2. 61 205

6729.745r

6730.307r

6731.89 a

6732.068r

5

5

3

8

0. 7

0. 7

0. 4

1. 2 u,N

Atm

Cri

Sm II? Fe I

4. 39

1. 17

4. 58

301

59

1225

6747.40 a CT A ''7 CO „ 6747.62 a

6748. 139r

674».4£55r

3

2

4

11

0. 4

0. 3

0. 6

1. 6

OJN G

1 Atm

Ti I?

Q 29

1. 88

7,3

1.52

-I oIz

6732.669r 1 0. 1 Atm? 6748.65 a 5 0. 7 6733.153m 25 S. 7 w Fe I 4. 64 1195 6748.779r 5 0. 7 Si 7. 87 8

6733.531r 5 0. 7 O 6748.870r 17 2. 5 Cr I 4. 39

6734.272r |7| 1. 0 Cri?- 4. 19 282 6749.541r 1 0. 1 Fe I p 3. 64 860

6734.67 2 0. 3 Atm 6749.88 3 0. 4 Atm?

6735.025r 2 0. 3 Fe I p 4. 43 1157 6750.164 75 11. 1 s Fei 2. 42 111

6735.456r 5 0. 7 SI O 6751 .440r OU 0. 4 Cri 5. 28 315

6735.847r 3 0. 4 O 6752.43 2 0. 3 Atm

6736.546r 1. 5 0. 2 Fe I p 4. 29 1122 6752.716m 42 5. 9 w Fei 4. 64 1195

6737.28 1. 5 0. 2 Fe I p 3. 26 551 6753.470r 5 0. 7 Fe I p 4. 56 1196

6737.978r 24 S.4 u Fe I 4. 56 1192 6754.44 2 0. 3 G?

6738.233 10 1. 5 O 6754.68 0. 5 0. 1 Atm

6738.62 5 0. 7 O? 6754.939r 4 0. 6 G

6738.828r 8 1. 2 o1 G 6755.605r 12 1. 8 u Fei

6739.21 1 0. 1 Sii?p 5. 96 61 6755.82 a 3 0. 4

6739.524r 11 1. 6 s Fe I 1. 56 34 6756.568r 5 0. 7 Fe I p 4. 29 1120

6740.11 a 3 0. 4 6757.08 5 0. 7 G?

6740.95 a 3 0. 4 CN? Q 28 7,3 12 6757.195r 19 2. 8 0 Si 7. 87 S

6741.629r 18 2.4 o1 Si I 5. 98 6757.660r 1 0. 1 Atm

6741.92 a 2 0. 3 6758.27 0. 4 Atm

6742.284r 1. 5 0. 2 o 6758.897r 7 1. 0 G

6742. 565r 1 0. 1 Atm?-

Ni I? O?

Ti I Si

G

4. 42

0. 90

7. 86

6759.46 1. 5 0. 2 Nil 4. 23 245

6742.90 6743.127m

6743.575r

6743.89

1

19

12

2. 5

0. 1

2.4

1. 8 0.4

S

0

48

8

6761.011r

6762.156r

6762.398r

6763.690r

3. 5

2

2

1

0. 5

0. 3

0. 3

0. 1

S

Fe I p CN?

Zri

G

4. 58 Q 32

0. 00

1227

7,3

1

12

287
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6763.95 a 1. 5 0. 2

6764.11 a 2 0. 3 Fe I p 4. 59 1225

6766.16 1 0. 1 G?

6766.50 m S,N V I 1. 06 31 13

6767.784 83 12. 1 s Nl I 1. 83 57

6768.83 1 0. 1 CN? Q 32 7,3 12

6769.682r 3 0. 4 Fe I p 4. 58 1226

6770.97 5 0. 7 1

f Co I 1. 88 54

A771 1 9 ± u 1. 6 1 O

Gil1.6^1 ol /. O u Mi T iv 1 I Q AA O. DO

6773.37 1 0. 1 o

6774.33 2 0. 3 La II 0. 13 2

6774.800r 2. 5 0. 4 O

6776.26 2 0. 3 o

6776.42 a 1 0. 1 CN? Q 33 7,3 12

6777.15 1. 5 0. 2 O

6777.406r 6 1. 2 w Fei r4. 14

\4. 19 1010

1013

6777. 775r 11.51 0. 2 O?

6780.25 1 0. 1 Atm

6780.925r 1. 5 0. 2 G?

6781. 81 5r 1. 5 0. 2 G

6782.219r 4 0. 6 G

6782. 502r 4 0. 6 Ni I 5. 34

6783.28 2 0. 3 Fe I p 2. 56 206

6783 7l4r 191 1. 3 s Fe I 2. 59 205

6784. 214r 11 1. 6 s,NN G

6785.00 a 3 0. 4 V I 1. 05 31

6785.76 2. 5 0. 4 Fe I 4. 58 1226

6785.88 1. 5 0. 2 Fe I p 4. 07 1007

6786.204 2 0. 3

6786.46 4 0. 6 Fe I p 3. 24 551 6786.860m 16 2. 8 w ? Fe I 4. 19 1052

6787.16 2 0. 3 Zr II? 2. 49 135

6787.604r 1 0. 1 Fe I p 4. 47 1156

6789.154r 3 0. 4 Cn 3. 84

6789.530r 1. 5 0. 2 Atm

6789.960r 2 0. 3

VV fxVc" length

(A)

EquiVdlcllU Width

(ml)

ReducGci Width

liA/ A

(F)

Spot Identification

Low

or

xvOt. Line

RMT

i\ 0. or

V ID. Band

Notes

1. O

6790.686r 1. 5 0. 2 G?

6792.330r 0. 5 0. 1 G?

6793.273r 10 1. 5 s,N Fei 4. 07 1005

6793.628r 12 1. 8 w? Fe'iYi 0. 07 1

6794.313r 4 0. 6 G

6794.623r 3 0. 4 Fe 1 p 4. 95 1279

6795.428r 3 0. 4 Y II ri. 72

1 1 74

26

9fi

6795 798r 5 0. 9 6796 1 2Sr 8 1X . 9^ s TTp X C TX 4T^. 14Xr± 1 flfl7 X Uu i 6796 49nr 3 OrV/JL TX 4 40 oux 6796 SI 4r oq fl 4

6798 1

5

u. o 0. 1 Cr I 6798 4fi7r u. u o Cn T 9 71 ox^1

6798 S8Sr O fl 4

6799 05 1. o 0. 2 6800 607r Q 1X. o V)

6801 202r f) 1 \J. X 98

6801 849r 1X 0\J. 1X Fg I p

1X. fil Ui ^4

fiSflQ 27 1X 0 1 \/. X Fe I p

4 ^fi 1X1X Q9

680*^ 854r 2. 5 0. 4 Fg I p

1X1X Qlc/X

fifi04 m Or 1X 4t; 11 Fp t 4 fi^ 1X1X 741 ^

fiSn4 9Q7r X u J/ . iyQ u Fp t 4 f>8 199*^

0 4

\J, o nO. 1X PrV^l XT o. oo

UOWU. OtJ U111 94. s FaX c tX 9 7'? ^oo

UOU 1 .oc/Oi u. o AA+mtill

uouo. 1 uyi n 1 U. X Fe I p

9 8'? ^4fl

yj, o W, X \y uouy .uo ui 11 U. X

X. o n 9

4.9 0. o s FoX G T1 4 fil 1 1 Q7

1X yj. X

6812.356r 2 Vi? 1. 04 31

6813.00 0. 5 0. 1 Cr I 3. 85

6813.54 1. 5 0. 2 Fe I? p 4. 98 1288

6813.616r 4 1 0. 6 Nil 5. 34 288 -

288
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6813.911r 2 0. 3

6814.83 1. 5 0. 2 O?

6814.961r 12 1. 9 s Co I 1. 96 54

6815.96 0. 5 0. 1 Atm

6816.96 a 0. 5 0. 1

6817.653r 0. 5 0. 1 O

6819.49 1. 5 0. 2 Fe I p 3. 02 463

6819.595r 5 0. 7 s Fe I 4. 10 1051

6820.374m- 37 5.4 s Fe I 4. 64 1197

6822.042r 1 0. 1 s Fe I (2. 48

14. 58

110 1220

6823.67 1 0. 1 0?

6824.52 1 0. 1 o?

6824.857r 2 0. 3 Fe I p 4 99 1280

6826.04 1 0. 1 O

6827.15 1. 5 0. 2 O?

6827.277r 1 0. 1

6827.963r 7 1. 0 O

6828.193r 5 0. 7 Ci 8. 53 21

6828.37 3 0. 4 o

6828.596 56 8. 0 u Fe I 4. 64 1195

6728.97a 1 0.1

6829.13a 1. 5 0.2

6829.580r 3 0. 4 O

6830.04 1 0. 1 Vi? 1. 08 31

6830.846r 0. 5 0. 1 Atm

6831.478r 1 0. 1 Fe I? p 3. 21 550

6831.74 a 1 0. 1

6832.18 2 0. 3 O?

6832.474r 0. 5 0. 1 Vi?

Yii?

1. 06

1. 75

3126

6833.08 3 0. 4 Zri? 0. 07 1

6833.248r 8 1. 2 0? Fe I 4. 64 1194

6833.592r 3 0. 4 O

6834.11 1 0. 1 O?

2. 5 0. 4 0

6835.12 7 1. 0

6835.368r 2 0. 3 o

6835.75 3 1 0. 4 o?

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6836.702r 5 0. 7 O

6837.013 15 2. S 0? Fe I 4. 59 1225

6837.39 4 0. 6 O

6838.04 a 4 0. 6

6838.357r 5 0. 7 O?

6838.70 a 3. 5 0. 5

6838.85 a 31 4.5 w Fe I

6839.15 a 5 0. 7 O

6839.835 30 4.S 5 Fe I 2. 56 205

6840.443r 3 0. 4 Atm

6841.19 8 1. 2 Mgi p 5. 75

6841.341 65 9. 6 S Fei 4. 61 1195

6841.642r 3 0. 4 Fe I p 5. 10 1333

6841.85 a 4 0. 6 Vi? 1. 05 31 6842.043m 26 3. 9 w Nil 3. 66 126

6842.40 a 5 0. 7 Siilp 5. 98 61 6842.689m 41 6. 0 u Fe I 4 64 1197

6843. 164r 4 0. 6 O?

6843.655 59 8. 9 w Fe I 4 55 1173

6844.683r |3| 0. 4 Fe I 1. 56 34

6845.22 3. 5 0. 5 s Yi

Atm

2. 37 16

6845.57 1 0. 1 O?

6845.98 3. 5 0. 5 Fe I p AtmHaO

4 56 R71190

103 26

6846.33 1 0. 1 G?

6847.06 2 0. 3 Atm H2O- R 5 103 26

6847.603r |5| 0. 7 Atm

Fe I 4 26 1078

6848.566r 15 2. 2 Si I 5. 86 37

6848.87 3 0. 4 Fe I p 4 61 1192

6849.302r 2 0. 3 G?

6850.439 10 1. 5 Ni I 3. 68 157

6851.47 |3| 0. 4 G

6851.652r 4. 5 0. 7 Fe I 1. 61 34

6852.28 1. 5 0. 2 Atm

6852.722r |4| 0. 6 Atm

6853.50 1 0. 1 G?

68o3.851r |2| 0. 3 G?

289
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6854.332r |4.5| 0. 7 O 6865.645r 6 0. 9 Atm H2O R 5 103 26

6854.538r 4 0. 6 o 6866.01 5 0. 7 Atm H2O R4 103 26

6854.850 12 1. 7 0? Fe I 4 59 1224a 6866.342r 6 0.9

6855.166 85 12. 1 s Fe I 4. 56 1195 6866.56 3 0. 4 0?

6855.723m 23 S. 1 u Fe I 4. 61 1194 6866.775r 2 0.3 0?

6856.13 13.51 0. 5 6867.05 3 0. 4 0?

6856.64

6856.87

3

3. 5

0. 4

0. 5

O?

O?

6867.187m

6867.252m

[ 153 22. 3

r Atm O2

1 Atm O2

R 21 R 19

1,0

1,0

22

22

6857.251 27 3. 6 w Fe I 4. 07 1006 6867.394m 29 4. 2 Atm O3 R 23 1,0 22

6857.850r 3 0. 4 O 6867.547m 154 22. 5 Atm O2 R 17 1,0 22

6858.155S 57 8. 2 u Fe I 4. 61 1173 6867.856m 32 4. 7 Atm O2 R25 1,0 22

6858.29 5 0. 7 Y II? 1. 74 26 6868.105m 137 20.0 Atm O2 R15 1,0 22

6858.47 a 4 0. 6 6868.245m 174 25. 4 Atm O2 R19 1,0 22

6859.03 a 3 0. 4 O? 6868.421m 35 5. 1 Atm O2 R23 1,0 22

6859.23 a

6859.493r

1.5

1. 5

0.2

0. 2 Fe I p 2. 84 340

6868.525m

6868.577m 1 149 21. 7

f Atm O2

1 Atm O2

R17

R27

1,0

1,0

22

22

6859.748r

6860.099r

6860.327

6860.46 a

6860.80

6860.953r

6861.268r

6861.50

6861.753r

6861.945

6862.496

6862.858r

6863.00

6863.18

6863.41

6863.787r

6863.95

6864.17

6864.324r

6864.514r

6865.24

6865.443r

2

2

7

3. 5

7

6

5

12

4

22

39

|3|

2

2

2

2

3

2

9

3

5

1. 5

0. 3

0. 3

1. 0

0. 5

1. 0

0. 9

0. 7

1. 7

0. 6

2. 8

5. 1

0. 4

0. 3

0. 3

0. 3

0. 3

0. 4

0. 3

1. 3

0. 4

0.7

0. 2

SI

siu1

O

Fe I p Fe I

O

Fe I Ni I

Ti I O

Fe I Fe I O?

O?

o?

o?

o?

o?

Atm

Fe 1 p O?

G

O

4. 83

2. 61

2. 83

5. 36

2. 27

2. 42

4. 56

4. 56

1255

205

341

293

237

109

1191

1186

6868.915m

6869.096m

6869.567m

6869.627m

6869.887m

6870.007m

6870.620m

6870.819m

6870.946S

6871.285m

6871.872m

6872.247m

6872.44 6872.843m

6873.392m

6873.798m

6874.653m

6875.45 6875.590m

6875.995

6876.38

216

216

6

9

1 382

7

6

233

264

6

257

5 272

l75 258

268

4

249

12

10

3L 4

31. 4

0. 9

1. 3

55. 6

1. 0

0. 9

34. 0

38. 5

0. 9

37.4

0. 7

39. 6

0. 2

37. 6

39. 0

0. 6

36. 2

1. 7

1. 5

Atm O2 Atm O2 Atm O2 Atm O2

f Atm O2

1 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Co I Atm O2

. Atm O3 Atm O2 Atm O2 Fei

Atm O2 Fei

Si I?

fR13

1R25

R15

R29

R27

R 13 Rll

R29

R31

R 11 R9

R31

R9

2. 01 R7

R33

R7

R5

2. 45 R5

4. 19

5. 98

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

1,0

54

1,0

1,0

1,0

1,0

167

1,0 1013

|22

22

22

22

22

22

22

22

22

22

22

22

22

22

22

22

22

290
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6876.715m

6876.972m

6877.637m

6877.991m

241

7

200

6

35. 1

1. 0

29. 1

0. 9

Atm O2 Atm O2 Atm O2 Atm O2

R3

R 17 R 3 /R14

IR17

1,0

1,0

1,0

1,0

1,0

22

23

22

6885.754m

6886.048m

6886.131 6886.209m

175

0. 5

}

'

25. 4

0. 1

0. 1

Atm O2 (Fe i) Atm O2

r Atm

I Atm O2

P3

4. 65 R 3

R 20

1,0 1173

1,0

1,0

22

23

24

6878.315m 3 0. 4 Atm O2 R 16 1,0 23 6886.303m r Atm O2 R 21 1,0 24

6878.436m

6878.630m

6879.041m

t5o/ y.^Dor

1. 5

5

[ 191

J

U. ^

0. 7

27. 8

Atm O2 Atm O2

r Atm O2

L

R 13 R 15 Rl

1,0

1,0

1,0

23

23

22

6886.372m

6886.476m 1

1±

0. 3

0. 1

0 1

[ Atm O2 Atm O2

/R 19 IR 22 R 18 /R 14 IR 17

1,0

1,0

1,0

1,0

1,0

}24

24

|24

Do/ y.oo 1 n

117 ill

i. o

17 0

Fe I p —

Atm H2O

Fe I p

A A1 R 5

0. .iD R 1

lio/ 103

ooi

1 0 1,U

26

99

6886.743m

6887.000m

208

3

30. 2

0. 4

Atm O2

Atm O2

P 3 fR 3 R13

IR 16

1,0

1,0

1,0

1,0

22

23

Rftsn DooU.UoOft mm A 0 fi rv tin \J2 It iU 1 0

1,0 9Q 6887.154m

1

2. 5 0.4

r Atm O2 R 2 1,0 23 6880.446m 4 0. 6 Atm O2 R 11 1,0 23 6887.196m 1 Atm O2 R 15 1,0 24

6880.637 14 9 Fei 4. 15 1051 6887.476m 4 0. 6 Atm O2 R 12 1,0 24

6880. 757m |2| 0. 3 Atm O2 R9 1,0 23 6887.564m 475 0. 7 Atm O2 R 14 1,0 24 6881.054 4. 5 0. 7

0 A

Fe I p Atm O2

4. 65 R 10 1174

1,0 23 6887.75 6888.000m

3

5

0. 4

0. 7 Atm O2 fR 2 LR 13

1,0

1,0

1,0

23 I24 1^4

Oooi.'iDo

6881.716

1 1 li

28

1. D

s?

-f e I Atm O2 Cri

(.Atm U2;

R8

3. 44

xt y

1,0 222

1,0

23

Z6

6888.323m

6888.457m

6888.612m

1

1. 5

2. 5

0. 1

0. 2

0. 4

Atm O2 Atm O2 Atm O2

R 1 R 12 R 10

1,0

1,0

1,0

23

24

24

Uoc5.<i.Z/ / in 9 U. c) Atm U2 K / 1,0 16 6888.948m 190 27. 6 Atm O2 P 5 1,0 22

fi009 cn9

4- 0 s L/r I

*? y1 /I 009 6889.271m 2. 5 0. 4 Atm O2 R 9 1,0 24

fiOQO 7^ Q *i. 0 U. D Atm n.2\J T> 0

K. 0 2d 6889.585m 2. 5 0. 4 Atm O2 R 10 1,0 24

fiSlR*^ vIOOO .^J0701 U O -L s Cr T ^ AA 999 6889.903m 222 32. 2 Atm O2 P 5 1,0 22 6883.230m 5 0. 7 Atm O2 R7 1,0 23 6890.10 m 3 0. 4 Atm O2 R 8 1,0 24

K)000 .Oil Qo 6890.240m 3 0. 4 Atm O2 R 9 1,0 24 6883.833m 146 21. 2 Atm O2 P 1 1,0 22 6890.760m 2 0. 3 Atm O2 R7 1,0 24

6884.041m

6884.78 a

941. 3

0. 6 Atm O2 /R 5

1 T? fi 1,0 1,0 I23

J 6890.948m

6891.593m

2

2. 5

0. 3

0. 4

Atm O2 Atm O2

R 8 R 6

1,0

1,0

24

24

6885.004m 4 0. 6 Atm O2 fR4

IR 5

1,0

1,0 |23 6891.719 2 0. 3 Atm Oo 0

R 7 1,0 24

6885.279m 2 0. 3 Atm O2 l'R20 \R 21

1,0 1,0

1,0

1,0

1,0

I24 6892.369m 208 30. 2 Atm O2 P 7 1,0 22

6885.349m 2 0. 3 Atm O2 /R 19 IR 22 R 18

|24

6892.57 m 1 0. 1 Atm O2 /R 5 IR6

1,0

1,0 |24

6885.477m 2. 5 0. 4

1 Atm O2 24 6893.309m

6893.40 m

213

3

30. 9

0. 4

Atm O2 Atm O2

P7

R 5

1,0

1,0

22

24

291

761-925—66 21
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

leiig til V\ IQIII VV IuIjII Identii— or or "Mn+pc 1ICilg An (T+Ti til Width VV ILL IjLI VV iciLn OpOL XtlcllLl- or or xN oies

Li A fi no "fl /~»n ilL'Cl tlUi-l XVUl. V ID. LsAl A llLdllUIX xtoi. V ID. (A) (mA) ('-r-l^ Line Pn n rl (A) (mA) (F) Line Band

2 V/. 0 169 24. 5 XIA+mtill On PX 1X 0 1x,ufl 99

fiQ05 317 14 9 0 Atm Ov, R 4 1x,u0 24

fiqO'i 4Q4m 4 0 fi xi-tixi A+m 0«1^/2 PX 4 1x,u(\ 94

9 u. 0 R 3 x,u 24

fiQO^i \jij\jKi m 7Sfim i OxJlii r. 0 0 7 xiA+mtill OnW2 Px^ Qy 1x,ufl 9^ n 4. fiQOfi \JU\J\Jm\J\J\J nnn 4 n 7 xitiil A + m TTnO XX2^ P ^ xuo 9fi

i"l n ci u. y IVTo- T 5. 75 34

fiQOfi 05Qm 0 0 4 xii/iix A + m 0«\»/2 PX 05 1 0 24

n 7

fiQflfi 27 Ru 0^J, qy xii Al J. ; JJn 4. 02

coop; 9R9m A u. u Afm 0^ R 3 1x,un 24

fiQOfi fiO Doy 1111 9 flu. 0 A + m On 1 0 24

fiQOfi 728m 10 1. 4 < A+m On P 10 1x,u0 23

DoyO. / 0

A

rr u. 0 xS. A +LIm11 1 fiQOfi 830 1 Atm HO R 2 103 26

DoyO.Uo / 111 ^y. 0 Atm 0« 1 0 22

fiQ07 023m X. 0 9 A + m On P 5 1x,u0 24

i. 0 n 9 A+m n« R 2 x,u 24

fiQ07 3Q 2. 5 0. 4 Atm

AQQA UoyO.DOrtlll AAilm 11 ji. A +Llii m 0«Vy2 R 1 1 0 24

fiQ07 fi55m 3 0. 4 A+m On P 6 1x,u0 24 AQOA QACirY-i Doyo.yDOin 91 f; OX. rVUIll A+m n«Vy2 P Q 1 0J 22 6Q08 28 2 0. 3 Atm

AOQ7 p;A9m Doy / .00^111 u. 0 n 1 A+m 0« R 1 1x,u0 24 6Q08 534m 137 19. 8 Atm Oo P 15 1x,u0 22

11 n 1 U. i XXA+mnil fiQOS 7^ fl 3 5 0 'i DOy / .ooD 9 u. 0 Atm

fiQOQ 32 m 0. 1 Xiuiii A +m OnV-/2 P 7 1 0 24

ACn*7 0/1 Atyi Doy /.y-iDm 1 n 1 U. X iA+m V till n«\J2 IT 0 1X,Ufl 9^

fiQOQ 431 m 143 20. 7 Atm On P 15 1x,u0 22 AQnQ 1 A Q 9 u. 0

3 5 0 5 Doyo.oU/ 1 1D| i^. u 1/1? 4- 99

2 0 3 Xi. A+,m Llll On'^2 P 7 1 0 24

Doyy.o^ Si U. D

0. 1 jrx, A tmmil Onv-'2 P 12 1x,w0 23

boyy.ouu r A+m TT«n P 9 1xuofl*? 9fl I 2 5 fl 4 fiQIO 72Sr '4

0. 6 G?

ooyy.oyDm J

1 ii. A+mtill On\J2 P 6 1 0 23

fiQ1 1 01 5m 5 0. 7 Atm O2 P 8 1x,u0 24 Doyy.yo4m ly 1

9*7 7 A+m n P 1

1

JT 1 X

1x,ufl 99

fiQI 1 3fiQ 6 0. 9 Atm H2O R 7 103 26

oyuu.o^oni U. D iillll A+m r)„ vy2 PIT fiU 1 n> 9"? fiQIX 1X tO^^ ^99 14 2. 0 Fe I 2. 42 109

£inr\f\ qaQtv-4 91 1 ^fl R OU. D iA+m 1 mi 0«^2 P 1 1 J: X X 1x,ufl 22

fiQI 1 79 2. 5 0. 4 DyUl.lU a

n 7 U. / fiQI 1 Q'^9m .£1- Atmu 111 0^V/2 Q 0 4 P 8 x,u 1 0 24

byUl.ii /Im U. 0 Aim KJ2 P 1

X: X

1x,ufl 94. fiQI uy X 9^. 97^ i 0. 5 0 1 \J» X 0

oyUl.DU/m 7 X. u xxtlll A+m n«\J2 PX 9^ 1x,ufl 94

fiQI 9 3 0. 4 Fe I? p 2. 84 341

byui.yu a D n 0 u. y 0. OD

fiQI 9 xi. A +,m iiiJ-i On^^2 oy X ^. 7*^

/ 0 m111 1X 0 1 \J. X P 13 1 0 23 D9U2.zoUm 11 U. 1 Aim ^^2 PX^ 7/ 1x,ufl 9^

fiQI uy X 9^. 75^fim 1 ouijx Q0 0 4 A +,m On P 9 1 0 24 CAAO AOA-*vT. Q U. 4 iixm A+m nv^2 x^P 9^ 1x,ufl 94

fiQI 9n0m 112 16. 2 Atm Oo P 17 1x,w0 22

byuJ.o/4 0. z, AT "PQ T

x* e 1 fiQI oy xo.o^711 X f) 7 Atm

b9(Jo.U4Um U. 4 Atm rP 0 1x,ufl 9/1 6913.615m 4 0. 6 Atm O2 P 13 1,0 23

6903.149 2 0. 3 Atm H2O R 3 400 26 6913.713m 6 0. 9 Atm O2 P 9 1,0 24

6903.828 1. 5 0. 2 Atm

6913.88 a 2. 5 0. 4 6904.117m 165 23. 9 Atm O2 P 13 1,0 22 6914.090m 107 15. 5 Atm O2 P 17 1,0 22 6904.531m 4. 6 0. 7 Atm O2 P4 1,0 24

292
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

A\

(ml)

Ee- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Eot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6914.26

6914.564

6915.004r

4

83

1

0. 6

11. 9

0. 1

Atm

Ni I G?1. 95 62

6923.369

6923.44 a i 93

f 11. 2

1. 7

Atm O2 |Atm HjOP 14 E8

1,0 103 24

26

6915.19 3 0. 4 Fei? 6923.50 a I 0. 6

6915.43 1 0. 1 Atm 6923.756 5 0. 7 6915.533m 3 0. 4 Atm O2 P 10 1,0 24 6923.86 6 0. 9 Atm

6915.670 3 0. 4 Atm 6924.164m 95 13. 7 Atm O2 P 21 1,0 22

6916.475

6916.686

6917.018 6917.409m

6917.505

6917.815

6918.122S

6918.429m

6918.592r

6919.002S

6919.327

4

60

6

4

7

6

89

13

7

97

7

0. 6

5. S

0. 9

0. 6

1. 0

0. 9

12. 9

1. 9

1. 0

14. 0

1. 0

w

|Atm

Atm O2 Fe I

Atm O2 Atm H2O

(Fe I p)

Atm

Atm O2 Atm O2 0?

Atm O2 |Atm

Atm O2

P 11

4. 15

P 11 E 6

4. 56

P 19 P 12

P 19

P 12

1,0

1052

1,0

103 1190

1,0

1,0

1,0

1,0

24

24

26

22

24

22

24

6924.450 6924.597m

6924.820

6925.280

6925.497

6926.097

6926.385

6926.567

6926.767

6926.91

6927.120

6927.261

10

2

4

45

1

21

2

5

20

3

4

2

1. 4

0. 3

0. 6

S. 9

0. 1

2. 9

0. 3

0. 7

2. 9

0. 4

0. 6

0. 3

s

s

Atm H2O

Atm O2 Atm

Cr 1 Atm O2 Atm

Cri

Fe I p Atm

Atm H2O

Atm

Atm

Atm H2O

E7

P 15

3. 45

P 15

3. 45

4. 58

R 8

R 3

103

1,0

222

1,0

222

1222

103

400

26

24

24

26

26

6919.77

6919.97 }

^ 0. 7 Atm

6927.675m

6927.89

1. 5

1

0. 2

0. 1

Atm O2 0?

P 16 1,0 24

6920.149

6920.168

6920.274

1

2

1. o

0. 3

flAtm

1 Atm O2 [Feip

0?

P 16

4. 61

1,0

1192

23 6928.330

6928.491

6928.728S

4

5

42

0. 6

0. 7

6. 1

Ni I? Atm

Atm O2

3. 70

P 23

110

1,0 22

6920.426m 4 0. 6 Atm O2 P 13 1,0 24 6928.88 4 0. 6

6920.672 1. 5 0. 2 Atm 6929.091 30 4. 3 Atm H2O R 6 103 26

6920.900 4 0. 6 Atm 6929.310 47 6. 8 Atm H2O R 5 103 26

6921.168 0. 5 0. 1 Atm 6929.599m 45 6. 5 Atm O2 P 23 1,0 22 6921.338m 4 0. 6 Atm O2 P 13 1,0 24 6929.839

' 30 4. 3 Atm H2O R 7 103 26

6921.577 5 0. 7 Atm 6929.938 |13| 1. 9 Atm H2O R 7 103 26

6921.924 4 0. 6 Atm H2O E2 103 26 6930.384 1. 5 0. 2 Fei? p 4. 56 1186

6922.243

6922.260 1

'

J

0. 7 rL Atm

P 14

6930.605

6930.837

17

2

2. 5

0. 3

Fe 1 |Atm

Atm

4. 58 1221

6922.661

Qo

2

1 9

0. 3

Atm On |Atm

0?

1 0 24

6931.103

6931.323

2

19

0. 3

2. 7 Atm H2O R 5 103 26

6923.05 a 5 0. 7 6931.769 1121 1. 7 Atm H2O /R 5 IR 4

103 103 |26

293
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6932.042 3 0. 4 Atm

6932.150 10 1. 4 Atm H2O R 5 103 26

6932.498r 3 0. 4 Atm

(Fe I p) 4. 58 1220

6932. 757r 3 0. 4 Atm

6933.026 16 2. 3 w,N Fe I 4. 19 1051

6933.163 3 0. 4 0

6933.467 7 1. 0 Atm H2O R 6 103 26

6933.605 54 7. 8

1 A J. TT |Atm H2U

Fei

R 4

f2. 43

\4. 14

103

167 1005

26

6933.817 29 4. 2 Atm H2O R 6 103 26

6934.422S 35 5. 0 Atm O2 P 25 1,0 22

6934.531m 2 0. 3

Ax Atm O2 P 19 1,0 z4

6934.886r 2. 5 0. 4 Atm

6935.113 3 0. 4 Atm H2O R 1 103 26 6935.280m 33 4. 8 Atm O2 P 25 1,0 22

6935.422 7 1. 0

A i Atm

6935.818 8 1. 2 Atm II 2O R 4 400 2d

6936.066m 1. 5 0. 2 Atm O2 P 20 1,0 24

6936.496 6 0. 9 Fe I 4. 61 1196

6936.80 a 1 0. 1 6936.962m 0. 5 0. 1

A J. /*\ Atm O2 P 20 1,0 24

6937.17 a 1 0. 1 AT AT s,NN

6937.703 |38| 5. 5 Atm H2O R 5 103 26

6938.199 1. 5 0. 2 Atm

6938.269 10 1. 4 Atm H2O R 5 IO3 26

6938.548m 2 0. 3 Atm O2 P 21 1,0 24

6938.737 3 0. 4 s K I 1. 62

6939.277 0. 5 0. 1 0?

6939.40 a 2 0. 3

6939.613 31 4. 5 Atm H2O R 4 103 26

6939.738 6 0. 9 Atm H2O R4 103 26

6940.192 37 5. 3 Atm H2O R3 103 26 6940.375m 23 3. 3 Atm O2 P 27 1,0 22

6940.62 a 1 0. 1 6940.77 a 0. £ 0. 1 6940.998 6 0. s Atm

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6941.218 26 3. 8 |Atm HoO

Atm 62 R4

P 27

103

1,0 26

22

6941.356 2. 5 0. 4 Atm

6941.72 a 1. 5 0. 2

6942.153 29 4. 2 Atm H2O R 3 103 26

6942.372 20 2. 9 Atm H2O R 4 103 26

6942.488 3 0. 4 Atm

6942.84 1. 5 0. 2 Fe I? p 4. 14 1008

6943.18 1. 5 0. 2 0

6943.637 1 0. 1 CN Q 9 3,0 12

6943.803 39 5. 6 Atm H2O R 4 103 26

6944.90 a 3. 5 0. 5

6945.210 82 11. 4 u Fe I 2. 42 111

6945.520 2 0. 3

6945.900 3 0. 4 0?

6946.330 2 0. 3 Co I? 2. 28 110

6946.590m 7 1. 0 Atm O2 P29 1,0 22

6946.728 1. 5 0. 2 Atm

6947.139r '5

0. 7

6947.48 a

( ^'^ Atm H2O

|Atm H2O

R 5 R 3 103

103 26

26

6947.55 a i 88 I 11. 5 Fe r /4. 58

\4. 59 1221 1224

6947.64 [ 0. 9 Atm H2O R 3 103 26

6947.879 "5

0. 7 Atm H2O R5 103 26

6948.979 16 2. 3 Atm H2O R 2 103 26

6949.086 |27| 3. 9 Atm H2O R 3 103 26

6949.782 1 0. 1 Atm H2O R4 400 26

6949.921r 1 0. 1 Atm?

6950.749 |19| 2. 7 Atm H2O R 3 103 26

6951.237 |60| 8. 8 Atm H2O

Fe I R 3

/4. 56

\4. 56

103 1186

1193

26

oyoi.ooD 7 i. u r c 1 Atm H2O

Art. 98Zo Q 51iu/f>7S0

103 26

6952.33

6952.920

2

1

0.

3

0.

1

s,N 10

Aim XI2'-' Atm

y D

1 AC? lUo ZD

6953.057 2 0.

3

w,N Fe I p — 3. 60 815

6953.072m 27 3.

9

Atm O2 P 31 1,0 22

6953.576 24 3.

5

Atm H2O R 2 103 26

294
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

6953.776 10 1. 4 Atm H2O R 2 103 26 6965.052 6 0. 9 Atm 11,0 Q4 103 26 6953.912m 3 0. 4 Atm O2 P 31 1,0 22 6965.408 25 3. 6 0 Mg I 5. 75 33 6954.014m 1 0. 1 Atm O2 R 17 2,1 22 6965.925 8 1. 1 CN Q 12 3,0 12

6954.22 0. 5 0. 1 0? 6966.75 a 2. 5 0. 4 CN Q 16 3,0 12 6954.494m 2 0. 3 Atm O2 R 15 2,1 22 0966.95 a 2. 5 0. 4

6955.040

6955.241

13

2

1. 9

0. 3

0? Nil

Atm H2O

3. 70 Q4157

103 26

6967.650m

6967.743

0. 2 fAtm O2-

1 Atm

P35 1,0 22

6955.521m 0. 5 0. 1 Atm O2 R 15 2,1 22 6967.999 3 0. 4 0?

6955.641 1. 5 0. 2 Atm H2O R 4 103 26 6968.265 1 0. 1 G?

6955.818 0. 5 0. 1 Atm H2O R 5 400 26 6968.582 2 0. 3 CN? Q 13 3,0 12

6956.214m 1. 5 0. 2 Atm O2 /R 11 IR 13

2,1 2,1 |22 6969.015 2 0. 3 Atm H2O Q 7 103 26

6956.401 56 8. 0 Atm H2O R 2 103 26

6970.495 11 1. 6 w Fe I p Atm H2O

3. 02 R2

463 400 26

6956.487 30 4. 3 Atm H2O R 2 103 26 6970.874 10 1. 4 Atm H2O RO 103 26

6957.009 2 0. 3 Atm H2O R 3 400 23 6971.136 6 0. 9 Atm H2O R 2 400 26

6957.204m 1 0. 1 Atm O2 R 11 2,1 22 6971.51 3 0. 4 CN Q 14 3,0 12

oy 0 < .^Urt 1. o 9fi 1i n 1 U. i 0?

Fei

11 r\'i 00

6957.703 2 0. 3 CN fQ8

IR 19

3,0

3,0 }- 6971.917 17 2. 3 s? 3. 02 404

6958.247 0. 5 0. 1 Atm H2O fQ2

IQ5

103

103 }26

6973.027 1. 5 0. 2 Atm

6958.462m

6958.936

6959.452S 6959.812m

6959.946m

6960.330

6960.476 6960.647m

6960.746m

6960.89

6961.260S

0. 5

1. 5

33

7

0. 5

13

1

2

}

^

51

0. 1

0. 2

2. 8

1. 0

0. 1

1. 7

0. 1

0. 3

0. 3

7. 3

0?

Atm O2 Atm H2O

Atm H2O

Atm O2 Atm O2 Fe I Atm

Atm O2 [Atm O2 [Atm

Atm H2O

Atm O2 0?

R9

R 5 R 1 P33

R 7

4. 59

P 33 R 5

R 1 R 5

2,1

103

103

1,0

2,1

1222

1,0

2,1

103

2,1

22

26

26

22

22

22

22

26

22

6973.374

6973.52 a

6974.32 a

6974.489

6974.763 6975.239m

6975.440

6975.754

6976.24

6976.504

6976.708

6976.908

0. 5

3. 5

1. 5

1

2

2

22

1

11

47

16

0. 1

0. 5

0. 2

0. 1

0. 3

0. 3

2. 9

0. 1

1. 6

6. 3

0. 3

2. 3

W

0W

Atm H2O

Ni I

Atm H3O

Atm H2O

Atm O2 Fe I 0?

Fe I

Si I Atm

Fe I

R 2

5. 30

R 5 Q6

P 5

4. 64

5. 95

4. 58

400

400

103

2,1

1194

60

1221

26

26

26

22

6961.707m

6961.808r

2

1

0. 3

0. 1 6977.466 48 6. 9 u |Atm H2O

Fe I Q 2

4. 59 103 1225

26

6961 .946r 2 0. 3 Atm? 6978.045r 3 0. 4 0

6962.804m 2 0. 3 Atm O2 R3 2,1 22 6978.383 08 9. 3 s Cri 3. 46 222

6963.01 2 0. 3 Fe I p 4. 19 1007 6978.862S 90 12. 2 s Fei 2. 48 111

6963.622

6964.538

6

18

0. 9

2. 6

Atm H2O

Atm H2O

R3

R 1

400

1 103

26

26

6979.156

6979.251 }

^ 1. 3

r Fe I p lAtm H2O

2. 83 R3

340

400 26

295
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

^F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

6979.45 a

6979 806

6980 369

6980 \j \j %j \j • 910 ij i. \j

6981 464

1. 5

41

2

8

23

0. 2

0. 3

1. 1

3. 3

-S

s?

Cr I O ? Cr I Atm H2O —3. 46

3. 46 0 1

222

222

103 26

6994.05

6994.110m6994.371r

6994.622

1

38

8

13

0. 1

5. 4

1. 1

1. 9

Si?

Atm H2O

Atm H2O

CN

Si?

Atm H2O

8. 04

R4

Q 3 Q 20

8. 04

R 3

400

103

3,0

400

26

26

12

26

6981 601r 8 1. 1 0 6994.83 2. 5 0. 4 CN? 0 22 3,0 12

6981 946 3 0. 4 0? 6994.958 8 1. 1 Atm

6982.285 '5

0. 7 0? 6995.378 2 0. 3 Atm O2 P 15 2,1 22 6982.501m 2 0. 3 A-tm O9 P 9 2 1 22 6995.92 a 1 0. 1

6983.52 5 0. 7 Fei?p 4. 59 1220 6996.310 2 0. 3 Atm O2 P 15 2,1 22

6984.114 4 0. 6 Atm H2O /R 2 \R3

400

103

"I}26

6996.634

6997.080

4

7

0. 6

1. 0

Til

Fe I p

2. 33

4. 95

256

1273

6984.606r

6984.936

2

13

0. 3

1. 9

0

Atm?

Atm H2O 0 4 103 26

6997.811r

6998.012

4

17

0. 6

2. 4 S

Atm H2O

Atm H2O

0

Q 6 R4

400

103

26

26

6985.512 2 0. 3 Atm? 6998.236r 3 0. 4 Atm H2O R 3 400 26

6985.812 1. 1 6998.718 15 2. 1 Atm H2O Q 3 103 26

6986.087 1. 5 0. 2 6998.962 79 11. 3 Atm H2O Q 3 103 26

6986.579S 75 10. 7 Atm H2O Qi 103 26 6999.228r 8 1. 1 Atm H2O Q4 103 26

6987.482 1 0. 1 Atm O2 P 11 2,1 22 6999.563r 8 1. 1 Atm H2O R 2 400 26

6987.731 3 0. 4 Atm 6999.885 71 9. 1 u Fei 4. 10 1051

6987.866

6988.272r

6988.533

6988.986S

6989.561r

6989.72

11

36

75

4

1

1. 6

A 7

10. 7

0. 6

0. 1

g

Atm H2O

0?

Fe I Atm H2O

Fe I p

/R 1 IQ3

2. 40

Q2

4. 61

400

103

167

103

1191

|26

26

7000.291r

7000.623

7000.91 a

7001.215r

7001.551

7001.92

5

23

5

3

11

1. 5

0. 7

3. 3

0. 7

0. 4

1. 6

0. 2

w

s,N

CN

Fez

Atm H2O

Nil

Atm?

Oi?

Q 23

4. 14 Q4

1. 93

10. 99

3,0

1005

103

64

21

12

26

6990.073

6990.370

6990.90 a

6991.026

6991.804

6992.00 a

6992.50 a

6992.846

6993.521

4

32

2

8

9

1. 5

X. 0

1

29

48

0. 6

4. 6

0. 3

1. 1

1. 3

0. 2

u. z

0. 1

4. 2

6. 9

0?

Atm H2O

Atm O2?

Atm H2O

Atm H2O

Atm

Atm H2O

Atm H2O

Q 2 P 13 R 1 R4

Q 2 P 1

103

2,1 400

400

103

103

26

22

26

26

26

26

7002.128

7002.62

7003.574

7003.977r

7004.314

7004.41

7004.745

7005.119

7005.37

18

4

81

4

23

6

65

27

9

2. 6

0. 6

10. 4

0. 6

3. 3

0. 9

9. 3

3. 8

1. 3

w,N

Atm H2O

(0 I) Atm H2O

Si I CN?

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Q3

10. 99 Q5

5. 96 Q 22 Q4

Q4

P2

P2

Q3

103

21

103

60

3,0 400

400

103

103

400

26

26

12

26

26

26

26

26

296
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

xte- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMi

No.

or Vib. Band

Notes Wavelength

(A)

Jiqui- valont Width

AX

(mi)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

No.

or

Vib. Band

Notes

7005.61 23 3. 3 Atm H2O Rl 400 26 7017.45 13 1. 9 Atm H2O Q3 400 26

7005.900 89 12. 7 W,N Si I 5. 98 GO 7017.666 51 7. 3 0? Si I 5. 87 51

7006.156 11 1. 6 Atm H2O R 2 400 26 7018.06 5 0. 7 CN Q26 3,0 12

7006.31 5 0. 7 Atm H2O Q 5 400 26 7018.79 6 0. 9 Atm II2O QG 103 26

7006.876 12 1. 7 Atm 7019.10 6 0. 9 0

7007.115 8 1. 1 Atm H2O Q3 400 26 7019.356 20 2. 8 Atm H2O Q3 400 26

7007.75 a

7007.976

7008.265

4

31

7

0. 6

4.0

1. 0

wl

s,N

Atm H2O

Fei

Atm H2O

Til

Q6

4. 18 Q3

2. 33

400

1078

400

256

26

26

7020.14

7020. 63

7020.83

7

8

10

1. 0

1. 1

1. 4

Atm H2OCN

Atm

Atm H2O

Q3

Q25

Q2

103

3,0

400

26

12

26

7008.42 2 0. 3 Atm? 7021.54 5 0. 7 Atm H2O Q!4 400 26

7009.18 a

7009.26 a

7009.90 a

7010.37 a

7010.62

7010.71

7010.99 a

3

5

16

13

1

16

0. 4

0. 7

2. 3

1. 9

1. 0

2. 3

0?

s

Atm H2O

CN?

Atm

Atm H2O

Fei

r Atm

lAtm H,0

Atm

Til

Q2

Q23

P2

4. 58

Q5

2. 33

400

3,0

103

1221

103

256

26

12

26

26

7022.035r

7022.395r

7022.52

7022.957S

7023. 504S

7023.73

7024.065

7024.392r

2

16

8

72

65

5

31

2

0. 3

2. 3

1. 1

9. 8

9. 3

0. 7

4.3

0. 3

s

w

Atm?

Fe I p Atm H2O

Fei

Atm H2O

Atm

Fe I CN?

4. 30

Q!l

4. 19 P3

4. 07 Q"27

1078

400

1051

103

1003

3,0

26

26

12

7011.323

7011.92 a

60

5

8. 5

0. 7

Atm H2O

(Fei)

CN

Q4

4. 59 Q 25

103

1221

3,0

26

12

7024.644

7024.86

51

34

7. 6 4 8

w,N

u

Fei

Ni I (Atm H2O)

4. 56

4. 54 P 3

1187

271

103 26

7012.229r 9 1. 3 Atm H2O Q 4 400 26 7025.58 1. 5 0. 2 0?

7012.612 |47| 6. 7 0 7025.75 1. 5 0. 2 0?

7013.31

7013.816r

7014.08

7014.28

10

5

2

2

1. 4

0. 7

0. 3

0. 3

Atm H2O

Atm

Atm

Atm?

RO 400 26 7026.18

7026.394

7026.61

2

18

13

0. 3

2. 6

1. 8

Atm

CN?

Atm H2O

|Atm H2O

Si I

Q26

R 3 0 5

5. 86

3,0 400

103

12

26

26

7014.546r 2 0. 3 CN Q 24 3,0 12 7026.937 37 5. 3 Atm H2O P 3 103 26

7014.996 13 1. 9 u Fei 2. 45 167 7027.478S 62 8. 8 Atm H2O P 4 103 26

7015.295

7015.536r

7015.77

7015.915r 7016.067

7016.442

7016.62

12

4

2

862

146

1. 7

0. 6

0. 3

1. 1

9. 8

20. 8

su

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Fe I Fe I Atm H2O

J Co I

Q 5 Q 2 R 1 P 3

2. 42

4. 15 P 3

2. 01

103

103

400

103

109 1051

10354

26

26

26

26

26

7027.65 .

7027.859

7028. 196r

7028.59

7029.05

2

28

2

5

20

0. 3

4. 0

0. 3

0. 7

2. 8 u,N

Fe I Atm?

Atm H2O

0?

Fe I p Nil

Ni I Atm H2O

4. 58

P 4

3. 07

3. 70

1 93 Q5

1221

103

463

156

61 103

26

26

7016.72 1 38 5. 4 1 Si I 5. 96 60 7029.712r 1. 5 0. 2 0?

7017.312r 12 1. 7 0? Si I 5. 87 51 7030.021 23 3. 0 w Nil 3. 54 126

297
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

/ 9 \ (A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7030.386r 1. 5 0. 2 Atm 7045.038r 2 0. 3 CN Q 30 3,0 12

7030.68 4 0. 6 Atm H2O Q 6 103 26 7045.233 6 0. 8 0?

7030.944 r 5 0. 7 Atm 7045.44 2 0. 3 CN? Q 29 3,0 12

7031.09

7031.40

7032.09

7032.319

7032.51

7033.40 a

7034.090

4

1. 5

1. 5

33

3

2

7

0. 6

0. 2

0. 2

4. 1

0. 4

0. 4

1. 0

10

CN

Fe I p

Fe I p

0?

0

Atm

Fe I p

Q 28

4. 65

4. 99

1 4. 00

\4. 61

3,0 1173

1278

1190 1190

12 7045.781r

7046.863

7047.08

7047.349

7048.00

7048.22

7048.68

7048.996

1

17

5

5

2

3

2

3

0. 1

2. 4

0. 7

0. 7

0. 3

0. 4

0. 3

0. 4

0?

Atm H2O

0?

Atm H2O

Atm H2O

Atm H2O

Atm

Atm H2O

P 4

P 4 P 2 P 1

Q 6

103

103 400

400

103

26

26

26

26

26

7034.380 11 1. 6 ul Nil 3. 54 97 7049.41 1 0. 1 Atm

7034.910S |80| 10. 6 w Si I 5. 87 50 7049.60 a 1. 5 0. 2 Ni I? 5. 28

7035.22 a 10 1. 4 7050.50 9 1. 3 Atm H2O P 5 103 26

7035.856r 3 0. 4 s,N Ti I 3. 14 307 7050.78 2 0. 3 s Til 2. 34 256

7036.96 0. 5 0. 1 Fe I? p 2. 22 61 7050.853 28 4. 0 Atm H2O P 5 103 26

7037.196 21 3. 0 Atm H2O P 4 103 26 7051.22 5 0. 7 Atm

7037.38 6 0. 9 Ni I 5. 49 288 7051.72 3 0. 4 0?

7037.534 31 4. 4 Atm H2O P 4 103 26 7051.85 3 0. 4 Atm H2O P 4 400 26

7037.98

7038.220

7038.765

3

76

40

0. 4

9. 8

6. 3

s

s

CN

Fei

|Fei

Til

Q 29

4. 22

4. 26

2. 34

3,0

1051

1078 256

12 7052.34

7052.404

7052.60

1. 5

13

6

0. 2

1. 8

0. 9

CN

Atm H2O

Atm H2O

/Q 30

IQ 31 P 6 Q 3

3,0

3,0

103 400

26

26

7039.284

7039.793

7040.587r

7040.81

7041.095

7041.751

7042.13

7042.44

7042.96

7043.40

7043.74

7043.990r

21

62

2

1

1

10

3

4

1. 5

2

3

3

3. 0

8. 8

0. 3

0. 1

0. 1

1. 4

0. 4

0. 6

0. 2

0. 3

0. 4

0. 4

Atm H2O

(Ti i) Atm H2O

Atm

0?

Atm

Atm H2O

Atm

Atm?

Atm

0?

Atm

Atm H2O

P5

3. 15 P 5

P 4

Q 6

103 307

103

103

103

26

26

26

26

7052.776

7052.87

7053.484

7053.85

7054.000

7054.58

7054.706

7054.98 a

7055.80

7055.927

7056.30

7056.474r

7056.65

52

13

2

1

5

6

7

|3|

|3| 20

4

4

2. 5

7. 4

1. 8

0. 3

0. 1

0. 7

0. 8

1. 0

0. 4

0. 4

2. 8

0. 6

0. 6

0. 4

s

0?

Atm H2O

Co I Atm

Atm H2O?

Co I Atm

Atm H2O

0?

Atm H2O

Atm

0?

0?

P 6

1. 96

P 3

2. 72

Q 3

P3

103

54

103

140

400

400

26

26

26

26

7044.50

7044.65

7044.93

7

14

2

1. 0

2. 0

0. 3

Atm H2O

Fei

0?

Q 2

4. 95

400

1276

26

7056.997

7057.20 a

26

1. 5

3. 7

0. 2

|AtmH20- P5 103 26

298
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7057.35 a

7057.544r

7057.92

7058.20

1. 5

1

4

8

0. 2

0. 1

0. 6

1. 1

Atm

Fe I p Atm IIjO3. 65 P 2815

400 26

7067.83

7068.07

7068.423

7068.64

7068.84

7069.06

7069.54

7069.80

4

7

64

0. 6

1. 0

8.4 u

CN?

Atm H2O

Fe I p Fei

Fe I p Atm

Ti I Fe I Atm

Q 33 P3

4. 99

4. 07

4. 91

3. 18

2. 56

.3,0 400

1276

1004

1276

307

205

1226

7058.632

7058.96 a

5

2. 5 9

O

0. 7

0. 4

ft *?

n 4. U. t:

Atm H2O

0?

(J !

P 5 103 26

1 9

11

2

3

4. 5

1. 5

1. 6

0. 3

0. 4

0. 6

0. 2

s

7059.64 4 0. 6 Atm H2O

IR 7 103

301 |26 7070.10 1 0. 1 s Sri 1. 85 3

7060.00 5 0. 7 CN Q 32 3,0 12 7070.35 1 0. 1 Atm H2O R 5 301 26

7060.446 47 6. 7 M? |Atm H2O

Mgi

fP 5 IQ 2

5. 75

103 400

32

|26

7070.663r

7071.63

4

2

0. 6

0. 3

Atm H2O

Atm

R 6 301 26

7060.62 a 11 1. 6 7071.866 35 4.8 0 Fe I 4. 61 1194

7060.85 a 3 0. 4 7072.07 3. 5 0. 5 Atm H2O /P 5 IP 6 103

103 }26

7061.35

7061.507

/ UO^.O i

7062.473r

7062.79

|2|

11

1. 0

1. 5

3

0. 3

1. 6 n 9 u. z

0. 2

0. 4

Atm H2O

A+m "FT r» 0?

Atm

Fe I p

P 3 n 7

4. 99

400

1iUo

1273

269A

7072.46

7072.80

7073.21

7073.49

7073.618r

5

6

1

3

2

0. 7

0. 8

0. 1

0. 4

0. 3

0?

Atm H2O

Fe I Atm H2O

Atm H2O

Atm H2O

P 6

4. 07

P 4 P 6 R 6

103

1003

400

400

301

26

26

26

26

7062.978r

7063.36

7063.483

7063.60 a

7064.12

7064.64

7064.88

7065.24

13

1

17

5

4

5

4

1. 5

1. 8

0. 1

2. 5

0. 7

0. 6

0. 7

0. 6

0. 2

MM?Ni I 0?-

Atm H2O

Nil

Atm H2O

Atm H2O

Atm

1. 95

P 6

4. 54 Q 4 P 6

64

103

270

400

103

26

26

26

7074.50

7074.90

7075.08

7075.27

7075.63

7075.89

7

6

3

3

11

2

3

1. 0

0. 8

0. 4

0. 4

0 1

0. 3

0.

0? Atm H2O?

Fe I p — CN

Atm H2O

Atm H2O

Atm H2O

iltm XI2V-' Atm H2O

CN

P 4

4. 61 Q 33 P 4 Q 3 Q 5

Q4

Q 34

103 1173

3,0 400

400

400 AOO

400

3,0

26

12

26

26

26

9fi

26

12

7065.642

7065.91

7066.218r

21

1

6

3. 0

0. 1

0. 8 w1

Atm H2O

Ci?p

Fe I? p

fp 7 IP 7

8. 64

4. 99

103

1277

|26

7n7fi in

707 ^.A.

7076.52

1

\ 3. 5

J

2

0. 5

0.

ii 1111 X12VJ

l_ /\ L 1 1

Atm?

Ci

/P 6 IP 7

8. 64

1 1 fl"?

r J.UO ^0

7066.29 5 0. 7 Atm H2O Q 5 400 26 7076.815r 3 0.

Atm?

7066.60

7066.933r

1

8

0. 1

1. 1

Atm?

Atm H2O P 5 400 26

7077.22

7077.61

1

3

0.

0. 4

Atm H2O

(Eu 11) Atm

R 4

1. 25 3018 26

7067.04 4 0. 6 Atm II2O Q 3 400 26 7077.81 8 1.

Atm H2O P 2 400 26

7067.460 13 1. 8 w Fe II 7078.05 3 0.

Atm H2O Q 3 400 26

761-925—66——22 299
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7078.252

7078.841

7079.27

7079.51

15

10

5

1. 5

2. 1

1. 4

0. 7

0. 2

Atm H2O

Atm H2O

Fe I p

Atm

P 4 P 7

4. 91

400

103

1278

26

26

7092.31

7092.59

7092.848

1. 5

0. 5

8

0. 2

0. 1

1. 1

CN

Ca I? p

Atm H2O

CNFe I

R 10

2. 93 P 8 Q 36

4. 56

4,1

103

3,0 1187

12

26

12

7079.591 11 1. 6 Atm H2O P 8 103 26 7093.09 18 2. 5 w? Fe I 4. 56 1189

7079.89 3 0. 4 Atm 7093.34 4 0. 6 Ci 8. 64

7080.970 7 1. 0 w Atm H2O P 2 400 26 7093.68 2 0. 3 CN R 11 4,1 12

7082.168r 4 0. 6 s,N 7094.05 5 0. 7 Atm H2O P 9 103 26

7082.480

7082.827r

7083.394

7083.716r

5

5

27

6

0. 7

0. 7

3. 8

0. 8

s,N

W

Atm

CN

Fe I

Q 34

4. 91

3,0

1277

12 7094.334

7095.01

7095.18

7095.407

5

3

1. 5

32

0. 7

0. 4

0. 2

3. 9 0?

Fe I p

Atm

CN

Ni I?-

ilFei

3. 57

R 12

5. 28

4. 21

778

4,1 276

1105

12

7083.960

7084.254r

21

7

3. 0

1. 0

w

sAll

Si I CN

ITiip

4. 02

5. 98

Q 35

1. 43

60

3,0 99

12

7095.58

7095.859

7096.383r

2

7

2

0. 3

1. 0

0. 3

Atm

Atm H2O

Atm

P 7 103 26

7084.656 17 2. 4 All 4. 02 7096.63 1 0. 1 0?

7084.975

7085.533r

61

3

8. 1

0. 4

s? Co I Atm H2O

Ci

1. 88 P7

8. 64

54

103 26

7096.93 a

7097.123

2

20

0. 3

2. 8

CN

Atm

R 13 4,1 12

7086.319 5 0. 7 Atm H2O Q 5 400 26 7097.45 a 2. 5 0. 4 Siip 5. 98 60

7086.730 23 3. 0 w Fei /3. 60

15. 08

815

1311 7097.666 3. 5 0. 5 Atm H2O R 4 301 26

7087.35

7087.59

7087.822r

7088.154

7088.23

7088.64

7089.04

7089.71

7090.390

7090.69

7090.92

7091.18

7091.363r

7091.942

3

3

7

24

2

|2|

3

6

73

4. 5

1

5

1

16

0. 4

0. 4

1. 0

3.4

0.3

0. 3

0. 4

0. 8

9. 7

0. 6

0. 1

0. 7

0. 1

2. 3

u

s0

Ci

Atm H2O

Atm H2O

Atm H2O

Fei?p

Fe I CN

CN

Atm H.,0

Fe I p Fe I

8. 64

/P 7 IP 5

P 3

P 5

4. 58

4. 23 Q 35

R9

P 5

4. 95

4. 95

103 400

400

400

1220

1051

3,0

4,1 400

1277 1278

j26

26

26

12

1226

7097.76 m

7098.02

7098.63

7098.80

7098.91

7099.22

7099.38

7099. 540r

7100.130

7100.75 a

7101.09

7101.31

7101.59

7101.69

7101.96

7102.279

1

6

1. 5

1

5

2

2

2

16

4

1. 5

1

}

'

78

0. 1

0. 8

0. 2

0. 1

0. 7

0. 3

0. 3

0. 3

2. 3

0. 6

0. 2

0. 1

0. 7

1. 0

1. 1

s

w1

Zri

Atm H2O

Atm?

Atm?

Atm H2O

CN?

Atm H2O

Atm H2O

Atm H2O

C I Atm H2O

CN

Fe r p

r Atm

LAtm H2O

CN

Atm

Atm H2O

0. 69 Q 6

P 4 Q 36

R 5 Q4

Q 4

8. 64 R 5 R 15

2.20

P 6 Q 37

P 6

42

400

400

3,0

221

400

400

301

4,1

61

400

3,0

400

26

26

12

26

26

26

26

12

26

12

26

300
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

V/idth

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7102.89 m

7103.150 6 0. 8

s s,NZri

Atm

|Fe I p

0. 65

2. 43

42

167

13 7113.90

7ll4.041r

/114.1 /or

1

'

1

0. 8

(J. 1

r Atm?

[Atm H2O

Atm

R6 221 26

7103.47 3 0. 4 CN R 16 4,1 12 7114.574 8 1. 1 u,N Fe I 2. 69 267

7103.80 1. 5 0. 2 s Zri 0. 62 42

7115.05 2 0. 3 0

7103.90 1. 5 0. 2 Atm

rS 64

18. 64 26

7104.39 1 0. 1 Atm H2O P 8 103 26

7115.17 33 4. 6 0 C I

7104.71 1 0. 1 Atm H2O P 7 103 26 7115.33 3. 5 0. 5 Fe I? p 4. 61 1186

7105.28 0. 5 0. 1 Atm H2O R 4 301 26 7115.47 5 0. 7 Atm H2O P7 400 26

7105.61 1 0. 1 0? 7115.66 1 0. 1 Atm?

7105.87 2. 5 0. 4 Fe I p 4. 19 1008 7115.83 a 1. 5 0. 2 CN RO 4,1 12

7106.164 11 1. 5 Atm H2O R 5 301 26 7116.388 3 0. 4 Atm H2O P7 103 26

7106.44 0 8 Atm TT„0

0

owl 26 7116.963

7117.25 a

21

2

2. 9

0. 3

0? Ci

CN

8. 64 R 17 4,1 12

7107.01

7107.25

3

1

0. 4

0. 1 Fe I p 5. 02 1324

7117.669r 0. 6 Atm?

Q 1 4,1

7107.468 24 3. 4 s Fei 4. 19 1005

Vl 1 C 1 {\^

i i io.i UO Id z. / u J? e I 0. yji 1 97Q

7107.65 1. 5 0. 2

1

9 9 0

XV 0

QHl 9fi

7107.909r 3 0. 4 CN? Q 37 3,0 12 7118.42 5 0. 7 Atm

7108.109r 2 0. 3 Atm? 7118.975r 4 0. 6 CN R21 4,1 12 7108.92 3. 5 0. 5 C I 8. 64 7119.38 3 0. 4 CN Q 6 4,1 12 7109.06 6 0. 8 Atm H2O P 9 103 26 71/ 1. 1i. Q0 • 704 i vj^ 9 7 Atm TT«0 (Ci) 8. 64 26

7109.23 2. 5 0. 4 Atm H2O P 10 103 26

7109.32 3. 5 0. 5 Atm H2O

Dy II? Q 6 400 26

7120.03 13 1. 8 Atm

Fe I CN4 56 Q7

1187

4,1 12

7109.70 2 0. 3 Fe I p 4. 61 1190 7120.58 1. 5 0. 2 Fe I p 4. 14 1006

7109.96 1 0. 1 7120.96 a 1. 5 0. 2

7110.14 1 0. 1 CN 7121.67 1. 5 0. 2 CN P 9 4,1 12

7110.33 2 0. 3

/ 122.20D& 107 s Nil 3. 54 126

7110.46 1. 5 0. 2 7122.50 13 1. 8 Atm H2O R 3 301 26

7110.905 41 5. 2 Nil 1. 93 64 7122.75 . 5 0. 7 CN

Atm?

R 22 4,1 12

7111.14 3 0. 4 Atm H2O P3 400 26 '7100 A-t 0 U. 0 CiN 14 4,1 12 7111.450 23 3. 2 Ci 8. 64 26

i iZo.oU a 1 U. i CN Q 9 4,1 12

71 1 1 0/1

( ill .y* / i. U Zri? 0. 52

j.nn 'iUU 23OP. ZD 7124.00 a 2 0. 3 Atm H2O P 4 400 26

7112.170 33 4. 6 u Fe I 2. 99 404 7124.70 a 3. 5 0. 5 Atm

7113.171 30 4. 2 0 Ci 8. 64 26

7ll3.422r

7ll3.592r }

^ 0. 7

7125.02 a

7125.33

3

1

0. 4

0. 1 s

Fe I p

Fe I p Atm?

3. 69

4. 59

815

1220

301
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7125.84 a

7126.06 a

1. 5

4

0. 2

0. 6

CN

Atm H2O

Q 10 fP7

\R 6

4,1 400

301

12

|26

7139.20

7139.55

2

1

0. 3

0. 1

CN

Atm?

Atm?

P 9 4,1 12

7126.25 a 1. 5 0. 2 Atm 7139.68 2. 5 0. 4 CN? Q 41 3,0 12

7126.71

7127.37

7127.573

7127.76

5

1

29

4

0. 7

0. 1

4. 1

0. 6 W

Ni I CN

CN

Fe I 0-

Atm H2O

3. 54 Q 15 P 5

4. 99

P 4

97

4,1 4,1

1273

400

12

12

26

7139.80 a

7140.279

7141.03

7141.14

3

10

1 '

0. 4

1. 4

0. 3

u,N

CN

Atm H2O?

0?

r CN?

1

/Q 15 IR 24 R4

P 13

4,1

4,1

202

4,1

}-

26

12

7128.150 9 1. 3 Atm H2O R 4 301 26 7141.64 3 0. 4 Ni I? 5. 30 283

7l28..528r 1 0. 1 Atm H2O P 9 103 26 7142.16 3 0. 4 Atm

7129.129 7 1. 0 Atm H2O

Fe I? p

R 4 301 26 7142.517 44 5. 9 w Fe I 4. 95 1274

7129.23 5 0. 7 4. 59 1219 7142.987 15 2. 1 0? Atm H2O R 4 202 26

7129.47

7129.87

4

10

0. 6

1. 4

Atm?

Atm?

Si I? p 5. 86

7143.382

7143.96

3

3

0. 4

0. 4

Atm

CN

CN

Q 16 R 25

4,1

4,1

12

12

7130.12 4 0. 6 Atm 7144.754 1. 5 0. 2 Atm?

7130.64

7130.925

7131.360

3

105

11

0. 4

13. 6

1. 5

u

CN

Fe I CN

Q 12

4. 22 Q 16

4,1

1051

4,1

12

12

7145.14

7145.312

3

42

0. 4

5. 9 w?

Atm H2O

CN?

Fe I

R 2 Q 19

r4. 61

14. 61

301

4,1

1186

1193

26

12

7131.63 2 0. 3 Atm H2O R 4 202 26 7145.55 3 0. 4

7131.82

7132.21

7132.985

7133.389

7134.116

7134.32

7134.61

7135.03

2

3

44

6

10

2

1. 5

2

0. 3

0. 4

5. 9

0. 8

1. 4

0. 3

0. 2

0. 3

w

Hf 1? Atm?

C I? Fe I CN

Atm

Co-i? Atm?

Atm

0. 00

8. 64

4. 07 Q 13

4. 06

26

1002

4,1

179

12

7145.90

7146.16

7146.57

7147.28

7147.634

7148.150

7148.50 a

7148.704

1. 5

2. 5

12

3

28

157

3

14

0. 2

0. 4

1. 7

0. 4

3. 9

20. 3

0. 4

2. 0

s

w

Atm?

Atm H2O

Atm H2O

CN

Atm H2O

Ca I CN

Fe I

P 6 P 4 Q 17 R 3

2. 71 R 26

r4. 28

15. 07

400

400

4,1

301

30

4,1

1078

1339

26

26

12

26

12

7135.58

7135.83

7136.56

7137.21

7137.469

7137.88

7138.08

7138.926

2

5

1. 5

4

26

2

4

5

0. 3

0. 7

0. 2

0. 6

3. 6

0. 3

0. 6

0. 7

s?S

CN?

Atm

Atm

Atm

Atm H2O

Atm H2O

Atm

Ti I p

Ti I

Q 40

R 2 R 3

1. 43

1. 44

3,0

301

301

98

99

12

26

26

7149.33

7149.750

7150.172

7150.680

7151.143

7151.464

7151.80 a

7152.22

7152.51

3

6

12

11

18

24

2

2. 5

1. 5

0. 4

0. 8

1. 7

1. 5

2. 5

3. 4

0. 3

0. 3

0. 2

0?

CN

CN—

Atm H2O

Atm H2O

Fe I 0?

0?

Atm?

Q 42 Q 20 R 5 R 3

2. 48

3,0

4,1 202

202

109

12

12

26

26

302
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7153.06

/ lOO.OOU

7153.746

7154.707

2. 5

7

6

4. 5

0. 3

11. nu

0. 8

0. 6

Atm?

Atm H2O

Atm

Co I

R 4

2. 04

202

89

26

7106.27

7166.57

7166.71

7166.96

7

5

4

14

1. 0

0. 7

0. 6

2. 0 0

Atm

0?

CN

Atm

Nil

Q 23

3. 74

4,1

109

12

7155.09

7155.37 a

7155.634

7156.422

71 Pi7 7Q

7158.776

5

3

45

21

7

1 4.

20

0. 7

0. 4

6. 1

2. 9

11. nu

2. 8

w,d

inW) iVMMiV

tij i v

u,d

Atm

CN

Atm H2O

Fe I Atm

TPo T J? e 1 G

|Atm H2O

/Q 42 \Q 21 R 3

5. 01

0. DO R7

3,0

4,1 202

1276

oi 0

301

26

26

7167.10

7167.360

7167.904

7168.73

7169.063

7169.11 m

7169.895

7170.086

23

46

132

6

21

18

40

3. 2

6. 4

18. 4

0. 8

2. 9

2. 5

5. 6

0?

u,N

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Zri

Atm H2OAtm H2O

fR3

IR8

R7

R 5

R7

0. 73 R 2 R 6

202

301

301

301

301

42

202

301

|26

2626

26

13

26

26

7159.310 15 2. 1 Atm H2O R 3 202 26 7170.33 23 3. 2 Atm

7160.20 a

7160.35 a

3

4

0. 4

0. 6 S,N

CN

|Tii

Atm

/Q 43 IP 14

1. 43

3,0

4,1

98

7170.568

7170.869

7171.038

80

25

12

11. 2

3. 5

1. 7

Atm H2O

Atm

Atm

R 8 301 26

7160.859

71 fil 11

4

9

0. 6

U. O

CN

Fg I p

I\A fbill m

Fe I p

Q22

0. Uo

4. 64

4,1

1lOiU '^1 n

1190

12 7171.33 a

7171.75

7171.954

2

1. 5

23

0. 3

0. 2

3. 2 Atm

7161.57 4 0. 6 Atm H2O P 5 400 26 7172.714 126 17. 6 Atm H2O R 5 301 26

7162.053 21 2. 9 Atm H2O R 6 301 26 7172.90 36 5. 0 Atm H2O R 6 301 26

7162.34

7162.731

7163.13

7163.27

7163.54

7163.82

7164.23

7164.432

15

7

2. 5

2. 5

3

15

2. 1

1. 0

0. 3

0. 3

0. 4

2. 1

0? Atm H2O?

Fe I p Atm H2O

Atm?

Atm?

Atm H2O

Atm H2O

P 5

5. 02 R6

R 13

IR 12

400

1278

301

301

ou 1 301

26

26

26

1|26

7173.417

7173.774

7174.166

7174.45 a

7174.84

7175.316

71 yrr CA

120

62

66

3

2

7. 5

1 ^

16. 7

8. 6

9. 2

0. 4

0. 3

1. 0

Atm H2O

Atm H2O

Atm H2O

Mn I? Atm

Pi?-

iVXIIl

R7

R 6 R 5

3. 76

8. 15

IX 0

301

301

301

oUl

26

26

26

zo

3

153

0. 4

21. 4 u Fe I 4. 19 1051

71 7 K QRfl i L i o.you 70 i11i. nu w T -T e I —

Atm H2O

4. OD R3

1 1 00 lloo

202 26

7164.62 33 5. 0 0 Si I 5. 87 49 7176.146 64 8. 9 Atm H2O R4 301 26

7164.83 3 0. 4 7176.37 a 2. 5 0. 3

7165.14 12 1. 7 Siip 5. 87 49 7176.59 2 0. 3 Pi? 8. 13

7165.578 93 0 Si I 5. 87 48 7176.878 44 6. 1 u Fe I 4. 99 1276

7165.71 8 1. 3 u7 7177.112 22 3. 1 Atm H2O /R6

IR 6 301

301 [26 7166.09 15 2. 1 Atm H2O R 10 301 26

7177.367 48 6. 7 Atm H2O R6 301 26

303
The Solar Spectrum—^Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7177.618 30 4. 2 Atm H2O R4 301 26 7189.860 |13| 1. 8 S Ti I 2. 58 285

7178.422 13 1. 8 Atm H2O R5 301 26 7190.128 15 2. 1 u Fe I 3. 11 463

7178.765 4 0. 6 CN Q25 4,1 12 7190.42 1. 5 0. 2 Atm H2O Q 1 301 26

7178.97 0. 5 0. 1 0? 7190.96 1 0. 1 Atm H2O Q7 301 26

7179.298 15.51 0. 8 Atm H2O R5 301 26 7191.497 115 16. 0 Atm H2O R 3 301 26

7179.61

7180.004

7180.202

1

19

3

0. 1

2. 6

0. 4

S

Atm H2O

Zr II? Fei

CN?

Atm

CN

R5

1. 74

1. 48

R33

221

33

4,1

26

12

7191.67

7191.868

5

37

0. 7

5. 1 A A

w? Fe I Atm H2O

Fe I |Atm H2O

4. 99 R 3

R 3

1274

301

202

26

26

7180.56

7180.79

2. 5

2

0. 3

0. 3 R 32 4,1 12

7192.759r

7193.183

4

60

0. 6

8. 3 0? Mg I 5. 75 31

7181.198

7181.520

7181.760

71

67

30

9. 9

9. 3

4. 2

s Fei

Atm H2O

Atm H2O

4. 22 R 5 R5

1078

301

301

26

26

7193.561

7193.768

75

54

10. 4

7. 5

Atm H2O

(Si I) Atm H2O

(Six)

/R 4 IR 2

5. 61 R 3

5. 61

301

30125

301

25

}26

26

7181.955

7182.400

7182.825

7183.46

81

3

2

1

11. 3

0. 4

0. 3

0. 1

w

s?

Nil

(Fei)

Atm?

Atm

CN

Atm?

3. 74

4. 91

P 20

126

1274

4,1 12

7194.07

7194.38

7194.569r

7194.93

7195.044

7

4

1

33

26

1. 0

0. 6

0. 1

4. 6

3. 6

w

Fe X p

CN

Fe I Fei

Atm H2O

5. 03 P 20

5. 02 R 3

1307

4,1

1273

301

12

26

7184.38 2. 5 0. 3 Atm H2O R 5 301 26 7195.27 a 2 0. 3 Atm H2O Q 6 202 26

7184.526 146 20. 4 Atm H2O /R4

IR3

301

301 }26

7195.525r 10 1. 4 Crx ? 4. 19

7184.90 24 3. 3 w,N llSii Atm H2O

5. 61 R 5 25

301 26

7195.797

7196.48

1121

2

1. 7

0. 3

Atm H2O

Atm?

R 3 301 26

7185.15

7185.29 }

^ 0. 8

r CN

[Atm H2O

Q26

P5

4,1 400

12

26

7197.020

7197.231

70

25

9. 7

3. 5

s Ni I Atm H2O1. 93 R 2

62

202 26

7185.56 171 1. 0 s Cri 3. 89 264

7197.41 6 0. 8 Atm H2O /Q 5 IQ 6 R 2 R 2 Q 28

Q 6

301

301 |26

7185.70 a

7186.141

7186.384

7187.010

7187.388

5

45

73

43

240

0. 7

6. 3

10. 2

6. 0

33. 5 u,d

Atm H2O

Atm H2O

Atm H2O

FeiAtm H2O

R 4 R 3 R 4

4. 10 R 4

301

301

301

1051 301

26

26

26

26

7197.865

7198.440

7198.86

7199.07 a

7199.42

22

|35|

4

1. 5

2

3. 1

4. 9

0. 6

0. 2

0. 3

Atm H2O

Atm H2O

CN

Atm

Atm H2O

301

301

4,1

301

26

26

12

26

7188.00

7188.27 a

t ±oo.

7188.99

7189.141

7189.45 a

8

3

Q

4

43

3

1. 1

0. 4

1 ^

0. 6

6. 8

0.4

.c

U

Atm H2O

Cr I?

Ti T Atm H2O

Fax

Q 8

3. 89

R 5

3. 07

301 264

301

463

26

26

7199.80

7200.027

7200.097r

7200.22 a

7200.37

7200.56

8

4

3

5

9

73

1. 1

0. 6

0. 4

0. 7

1. 2

10. 2

0?

Atm H2O

G?

CN

Atm H2O

Atm H2O

Q 4

Q 27 R2

R 2

301

4,1

221

301

26

12

26

26

304
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

ite- duced

Width

AX/X

(F)

Spot

Solar

Identification

JjOW

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

KM J. No.

or

Vib. Band

Notes

7201.197 100 13. 9 Atm H2O R 2 301 26 7215. .539 6 0. 8 Atm H2O

0

Ti I

R 2 202 20

c0 U. / Atm A +m XT r\ xlaU /Q 3 IQ7

.301 301 )26 7216.19 22 3. 0 S 1. 44 98

7201.63 1. 5 0. 2 Atm H2O Q 2 301 26 7216.527 24 3. 3 Atm H2O R 0 301 20

7201.80 3 0. 4 Atm H2O R 2 320 26 7216.63 20 2. 8 0? Fei .5. 01 1273

7202.208

7202.543

7202.900a

7203.10 a

7203.27

124

1. 5

|1. 51

1. 5

1

16. 6

0. 2

0. 2

0. 2

0. 1

s Ca 1 Atm H2O

Atm II2O

Atm H2O

2. 71 Q4

R3

P6

29

202

202

400

26

26

26

7217.28

7217.63

7218.022

7218.47

0. 5

4

7

31

0. 1

0. 6

1. 0

4. 3 0?

Atm H2O

Co I? Atm

Atm H2O

0-

Atm H2O

Q7

2. 54

Q 3

Q 3

301

126

301

202

26

26

26

7203.850 12 1. 7 Atm H2O R 1 202 26 7218.65 4 0. 6 Atm H2O R 6 221 20

7204.08 1. 5 0. 2 Atm H2O Q5 301 26 7219.056 3 0. 4 Atm H2O R 5 221 26

7204.308 |82| 11. 4 Atm H2O R 1 301 26 7219.40 m s 13

7204.85 a 2. 5 0. 3 Atm H2O Q 4 202 26 7219.680 53 7. 1 s Fe I 4. 07 1001

7205.22 a 1 0. 1 Atm 7220.12 1. 5 0. 2 Atm

7205.536

7206.15

7206.421

7206.861r

7207.131

2

3

102

1

72

0. 3

0. 4

14. 2

0. 1

10. 4 u

Atm H2O

Fe I p Atm

Atm H2O

CN

Fe I

Q 6

4. 73

R 1 Q28

4. 07

202

1251

301

4,1

1001

26

26

12

7220.786

7221.204

7221.586r

7222.397

7222.90 a

10

49

0. 5

27

24

1. 4

6. 1

0. 1

S. 3

3. 3

w

0

Ni I Fe I Atm H2O

Fe II

Fe I

5. 36

4. 56 Q 5

3. 89

r4. 61

\5. 06

294

1189

202

73

1187

1311

26

7207.396 150 21. 0 u Fe r 4. 15 1051 7223.00 2 0. 3 Atm H2O Q 6 301 26

7207.90 a

7208.220

7208.60 a

7209.504

4

8

1. 5

81

0. 6

1. 1

0. 2

11. 2 u,d

Atm H2O

Si I CN

Ti I-

|Atm H2O

Q2

5. 62 R 37

1. 46 R 1

202

25

4,1

99

301

26

12

26

7223.636

7224.129r

7224.464

7225.056

101

3

28

3. 5

14. 0

0. 4

3. 9

0. 5

u?

0

s?

Atm H2O

|Fei

Atm?

Fe II Ni I?

Q 2

3. 02

3. 89

5. 61

301 463

73

26

7210.08 3 0. 4 Atm? 7225.85 a 5 0. 7 Fe I p 4. 99 1278

7210.37 a 6 0. 8 Atm H2O R 6 221 26 7226.05 5 0. 7

7211.203 12 1. 7 Atm H2O Q4 301 26 7226.208 46 6. 4 0 Six 5. 61 26

7212.037 4 0. 6 Atm H2O RO 202 26 7227.493 42 5. 8 Atm H2O Q 1 301 26

7212.440 34 4. 3 iu,N Fei 4. 95 1273 7227.63 1. 5 0. 2 Atm H2O R 5 221 26

7212.91 1 0. 1 CN P 24 4,1 12 7228.243 4. 5 0. 6 Atm H2O Q5 301 26

7213.28 1 0. 1 Atm? 7228.700 29 4. 0 u Fe I 2. 76 267

7213.41 m

7213.51

7213.847

3

9

0. 4

1. 2

S

10, N

Til

CN

Fe I

1. 74 Q 30

4. 26

143

4,1

1105

13

12

7229.121

7229.46

15

7

2. 1

1. 0

CN

Atm H2O —

fP 26 IQ 32 R 5

4,1

4,1

301

},2

26

7214.74 25 3. 5 0? Ti n p 2. 59 101 7230.06 3 0. 4 0?

7214.93 13 1. 8 s Til 3. 70? 314 7230.56 2 0. 3 Cri? 4. 62

305
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(nil)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7230.677 2. 5 0. 3 Atm H2O R 3 301 26 7245.40 2 0. 3 Atm H2O P5 301 26

7231.06 a 2 0. 3 Atm H2O R 6 221 26 7245.676 41 5. 7 Atm H2O Q 4 301 26

7231.50 a 3. 5 0. 5 7245.90 a 2 0. 3 CN Q 34 4,1 12

7231.69 0. 5 0. 1 Atm H2O R 3 202 26 7246.09 2 0. 3 Atm H2O P 2 202 26

7232.234 26 3. 6 Atm H2O Q 4 301 26

(Z'ko.oi a

Q0 A A fP 27 IP 28

4,1

4,1 )12

7232.55 a

7232.902

7233.33

2

89

2. 5

0. 3

12. 3

0. 3

CN

Atm H2O

CN

R 40 Q 1 Q49

4,1

301

3,0

12

26

12

7246.794

7247.07

4

5

0. 6

0. 7 s

Atm II2O Atm II2O10

R 6 Q 6221

301

26

26

7234.09 1. 5 0. 2 Atm 7247.210 20 2. 8 Atm II2O ro 4 IQ5301

301 j26

7234.400

7234.738

7235.325

18

100

47

2. 5

13. 8

6. 5 W

Atm H2O

Atm H2O

Si I

Q 3 Q2

5. 61

301

301

26

26

26

7247.39

7248.26 a

2

3

0. 3

0. 4

Atm H2O

0?

R4 221 26

7235.85 31 4. 3 w Si I 5. 61 25 7248.924 13 1. 8 Atm H2O /Q4\R 4

301

221 |26

7236.136

7236.425

38

7

5. 3

1. 0

Atm H2O

Atm H2O

Q2

R 5

301

221

26

26

7249.34

7249.47 }

^ 0. 6 JAtm H2O

1 0

Q 3 221 26

7237.40

7237.84

7237.946

7238.24

7238.58

4. 5

2

5

3

3

0. 6

0. 3

0. 7

0. 4

0. 4

|CN

Hf I? Atm H2O

Atm H2O

Atm?

CN

Atm?

Q 33

0. 57 R 4 R4

R 40

4,1

221

221

4,1

12

26

26

12

7249.90 a

7250.216

7250.64

7250.68

7251.717

7252.075

1. 5

23

} "

34

3

0. 2

3. 2

9. 3

4. 1

0. 4

0

s u?,N

CN

Atm H2O

J

Six

lAtm H2O

Ti I -Atm H2O

R 42 Q 3

5. 62 R 5

1. 43 R 4

4,1

301

25

221

99

221

12

26

26

26

7239.042 8 1. 1 Atm H2O R7 221 26 7252..374 |77| 10. 6 Atm H2O P 2 301 26

7239.50 1. 5 0. 2 Atm H2O R 5 221 26 7252.853 |18| 2. 5 Atm H2O Q 5 301 26

7239.848

7240.53

7240.62

7240.822

7241.26

75

2

86

67

2

10. 4

0. 3

11. 9

9. 3

0. 3

u,N

u?

|Atm H2OFe I Atm H2O

Atm H2O

Atm H2O

Atm H2O

Ci

Q 2

4. 21 R 5 P 1 Q 3 Q 8

9. 00

301 1105

221

301

301

301

26

26

26

26

26

7253.224

7253.42

7253.728

7254.648

7254.93 a

34

2

42

32

1. 5

4. 7

0. 3

5. 8

4. 4

0. 2

u

Atm H2O

Atm H2O

Atm H2O

(Til)

Fe I CNP 2 Q 3 Q 4

ri. 75

\2. 16

P 28

301

202

301

143

4,1

26

26

26

12

7242.24 7 1. 0 0 7255.29 3 0. 4 Si I p 5. 96 59

7242.49 3 0. 4 Si? 8. 04 15 7255.42 4 0. 6 CN P 29 4,1 12

7243.09 6 0. 8 Si 8. 04 15 7255.79 5 0. 7 CN R 42 4,1 12

7243.48 26 3. 6 Atm H2O Q3 301 26 7256.142 17 2. 3 w? Fe I 4. 95 1278

7243.72 88 12. 2 Atm HoO Q 3 301 26 7256 58 a 2. 5 0. 3 Atm H2O R 1 221 26

7244.48 4 0. 6 CN Q 33 4,1 12 7256.80 a 0. 5 0. 1 Ni I 3. 60 97

7244.850 63 8. 6 S |Tii Fe I (Si)1. 44

4. 95

8. 04

99 1276

15

7256.99

7257.104

2

9

0. 3

1. 2

Atm H2O

Atm H2O

P 3 Q 5202

301

26

26

306
The Solar Spectrum-—Continued

Wavelength

(A)

Equivalent Wiutn

AX

(mA)

Re- duced

Width

AX/X

(F)

bpot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Ecjui- valcnt Width

AX

(ml)

Reducttd Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7257.371 20 2. 8 Atm HoO Q 5 301 26 7269.05 a 8 1. 1

7257.934

7258.45

7258.65

7258.90 a

7259.10

7259.556

7260.Uoo 7260 266

31

2. 5

4. 5

3

5

1

6

3

4. 3

0. 3

0. 6

0. 4

0. 7

0. 1

U. 4

0. 4

©?-

|Atm H2O

Atm?

Atm H2O

Atm

Atm H2O

Atm H2O

A 4.^ TT Atm i±2(J Atm H2O

P 2

R 3

R 3 P 2 R 4 R 7

301

221

221

202

221

221

26

26

26

26

26

26

7269.752

7269.94

7270.131

7270.300

7270.60 a

7270.95 a

7271.18

7271.40 a

7271.55

15

2

12

5

3

4

0. 5

6

2. 1

0. 3

1. 6

0. 7

0. 4

0. 6

0. 1

0. 4

0. 8 8

Atm IhO

Atm H2O

Atm H2O

Atm H2O

Atm

Atm?

Til

R 3 R3

R 5 R 5

1. 44

221

221

221

221

97

26

26

26

26

7260.730 12 1. 7 Atm H2O fQ 5 IQ 6 301

301 |26 7272.112 10 1. 4

7261.016 19 2. 6 Fe I 2. 73 267 7272.973 100 13. 8 Atm H2O fP 3 IP 3

.301 301 |26

7261.30

7261.45

7261.52

7261.97

7262.01

7262.272r

7262.47 7262 973

7263.380

9

1 45

1

78

1

0. 5

14

3

1. 2

6. 2

r 9.

1 1.

0. 1

0. 1

1. 9

0. 4

U

s

Fe I p fAtm H2O

1 Fei

Ni I Atm H2O

0?

Fei? p Atm H2O

Atm H2O

4. 91 R 4

4. 56

1. 95 Q 5

3. 64 P 3 Q4

1273

221

1188

62

301

859

202

301

26

26

26

26

7273.835

7274.259

7274.73 a

7275.33

7275.398

7275.819

7276.316

7276.560

7276.850

8

3

1. 5

1 94

9

19

11

14

1. 1

0. 4

0. 2

12. 9

1. 2

2. 6

1. 5

1. 9

0?

Atm H2O

Atm

Atm H2O

fSi I Utm H2O

Atm H2O

Atm H2O

Atm

Atm H2O

Q7

Q 5

5. 61 P 3 R 4 R4

P4

301

221

24

301

221

221

202

26

26

26

26

26

26

o n 7 CN /Q 36 \P 29

4,1 4,1 )l2

7277.148 9 1. 2 Atm H2O /Q4 \R2

301 221 }26

7264.04

7264.20 a

1

4

0. 1

0. 6

0?

Yii 1. 84 33 7277.402

7278.085

73

25

10. 0

3. 4

Atm H2O

Atm H2O

P 4 P 4

301

301

26

26

7264.390

7264.598

7264.90 a

7265.149

11

44

3

2

1. 5

6. 0

0. 4

0. 3

Atm HoO

Atm A 4--^ XT r\ MaU

Atm

(Fe 11)

/R 3 IR 6 r 6

6. 22

221

221

301

197

|26

ZD

7278.526

7278.792

7279.03 a

7279.38

16

4

6

5

2. 2

0. 6

0. 8

0. 7

Atm

Fe I p Atm H2O

Atm H2O

CN

4. 99 Q 5 Q 5 Q 37

1274

301

202

4,1

26

26

12

7265.594 89 12. 2 Atm H2O P3 301 26 7279.698 8 1. 1 Atm H2O R 2 221 26

7265.86 8 1. 1 Atm H2O Q4 202 26 7280.32 1. 5 0. 2 Atm H2O Q 5 202 26

7266.28 12 1. 6 s Ti I 1. 73 143 7280.671 9 1. 2 Atm H2O Q 3 221 26

7266.96 2 0. 3 Fe I p 2. 18 61 7280.967 4 0. 5 Atm H2O R 2 221 26

7267.75 6 0. 8 0? 7281.540 2 0. 3 Atm K2O P 4 320 26

7268.05 1 0. 1 Atm H2O Q 5 202 26 7282.02 4 0. 5 Atm

7268.217

7268.566

3

8

0. 4

1. 1

Atm H2O

Atm H2O

Fe I p

Q7

Q 3

3. 88

301

202

957

26

26

7282.302

7282.844

48

68

6. 6

9. 3 w,N

Atm H2O

(Fe I) SiiR 3

5. 01

6. 20

221 1274

26

307
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7283.220 14 1. 9 Atm H2O R 3 221 26

7283.61 8 1. 1

7283.770 13 1. 8 0? Mn I 4. 42 50

7284.18 2 0. 3 0?

7284.56 0. 5 0. 1 0?

7284.842 41 5. 6 u Fe I 4. 14 1004

7285.09 1 0. 1 s?,N

7285.305 25 3. 4 u',N Fe I 4. 61 1188

7285.78 a 0. 5 0. 1 Atm?

7285.98 4 0. 5 Si 1 ? 5. 96 58

7286.52 5 0. 7 Ni I 3. 77 109

7286.90 a 1. 5 0. 2 CN? R 16 5,2 12

7287.378 46 6. 3 Atm H2O

(Fe II) P 46. 22

301

197 26

7287.858 6 0. 8 Atm H2O Q 5 301 26

7288.132 28 3. 8 Atm H2O P 4 301 26

7288.47 3 0. 4

7288.741 70 9. 3 u,N Fe I 4. 22 1077

7289.188 116 14. 6 w,N Si I 5. 62 24

7289.53 9 1. 2 Atm

7289.818 8 1. 1 Atm H2O R 2 221 26

7290.25 a 4 0. 5 Si I 5. 62 24

7290.415 91 12. 5 Atm H2O rP5

\P 5 301 301 }.e

7290.895 16 2. 2 Atm?

Ni I 5. 34 287

7291.098 25 3. 4 Atm H2O

(Mgi)

R 2

5. 39

221 26

7291.438 47 6. 5 u Atm H2ONi I P 5

1. 93 20263

26

7291.75

7292.172

4

19

0. 5

2. 6

Atm

H2O?

Atm H2O

P 3 P 4

202

301

26

26

7292.695 7 1. 0 Atm H2O Q 5 221 26

7292.841 47 6. 7 u Fe I 4. 56 1189

7293.052 85 12. 0 u Fe I 4. 26 1077

7293.372 8 1. 1 Atm H2O R 1 221 26

3 0. 4 Atm HoO 0 7 301 26

7294.20 1 0. 1 Atm H2O Q4 301 26

7294.364 4 0. 5 Atm H2O P5 202 26

7294.863 2 0. 3 Atm H2O Q 6 301 26

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7295.031 39 5. 4 Atm H2O P4 301 26

7295.28 4 0. 5 Fei p 4. 61 1189

7295.610 6 0. 8 Atm H2O P 4 301 26

7295.78 a 2 0. 3 CN Q 9 5,2 12

7296.265 6 0. 8 Atm H2O Q 6 221 26

7297.072 1. 5 0. 2 Atm H2O Q4 221 26

7297.33 2 0. 3 Atm H2O Q 5 301 26

7297.70 10 1. 4 Atm?

Nil? 5. 63 293

7297.93 2 0. 3 CN? R47 4,1 12

7298.169 8 1. 1 Atm H2O R 1 320 26

7298.51 5 0. 7 CN Q 39 4,1 12

7299.33 a 5 0. 7

7299.643 14 1. 9 s |Atm H2O

Ti I R 11. 43

221

97 26

7299.77 1 0. 1 Atm H2O R 1 221 26

7299.926 19 2. 6 Atm H2O R4 221 26

7300.50 33 4. 5 Fe IFe I4. 99

4. 14 1275

1003

7300.63 6 0. 8 Atm H2O Q 7 221 26

7300.874 8 1. 1 Atm H2O Q 6 301 26

7301.262 4 0. 5 Atm H2O Q 6 202 26

7301.577 7 1. 0 0 Fe II 3. 89 72

7302.129 8 1. 1 Atm H2O P 5 301 26

7302.348 3 0. 4 CN

Atm H2O

Q 40 Q 5

4,1 221

1226

7302.603 4 0. 5 Atm H2O Q 5 221 26

7302.777

7302.88 } " 2. 2

0

JAtm H2O

I Mn I

P 3

4. 43

202

50

26

7303.197 42 5. 8 Atm H2O P 5 301 26

7303.76 7 1. 0 Atm H2O P 6 202 26

7304.134 15 2. 1 Atm H2O P 6 301 26

7304.214 42 5. 8 Atm H2O P 6 301 26

7304.80 1 0. 1 Atm H2O Q 5 202 26

7304.954 3 0. 4 s Atm H2O Q 6 221 26

^ OVy (J. vfwO 0 0. 4 Atm HoO P 3 301 26

7305.873 3 0. 4 s Ti I 1. 73 143

7306.03 1. 5 0. 2 Atm H2O Q 3 221 26

7306.570 43 5. 6 u Fe I 4. 18 1077

308
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7307.48

7307.960

7308.08

7308.50 a

7d0».757

7309.518

7310.201

4

52

26

4. 5

-I 'y 17

37

23

0. 5

7.4

3. 7

0. 6

2. 3

5. 1

3. 2

u

u

O

Fei

Fe n O

CN

Atm H2O

Atm H2O

Atm H2O

Fe 11

4. 14

3. 89

Q 40 Q 3 P 5 0 4

3. 89

1002

73

4,1

221

301

221

73

12

26

26

26

7320.689

7320.846

7321.27 a

7321.44

7321.52

7322.201

7323.10

72

19

2. 5

1

2

4

3

10. 1

2. 7

0. 3

0. 1

0. 3

0. 5

0. 4

W

s

Fei

Fe II Atm H2O

Vi

Atm?

Atm

Atm H2O

r4. 56

\4. 91

3. 89 Q3

2. 12

Q6

1188

1276

73

221

117

221

26

26

7310.402

7310.62

7310.73 a

2

3

2. 5

0. 2

0. 4

0. 3

Atm H2O

Atm H2O

R 0 Q 6

221

221

26

26

7323.354

7323.972

9

31

1. 2

4. 2

CN

Fe I? p |Atm H2O

0

Q 42

3. 64 Q 1

4,1 859

221

12

26

7311.080 67 9. 2 Fe I 4. 28 1077 7324.29 5 0. 7 CN R49 4,1 12

7311.265 28 4. 0 Fe I p Atm H2O4. 26 Q41105

221 26

7324.680 10 1. 4 u Atm H2O P6 202 26

7311.484

7311.64

7311.80 a

7312.08

7312.270

1

5

2

6

1

0. 1

0. 7

0. 2

0. 8

0. 1

Atm H2O

0?

CN

Fei p

Atm H2O

Q4

P 34

5. 03 Q7

221

4,1

1310

301

26

12

26

7325.28

7325.56

^ 0 0 C OCX — 7325.89 a

7326.160

2

4

1

136

0. 3

0. 5

0. 1

16. 9 S

CN?

Fe I p 0?

CN

Ca I

Q 56

3. 93

P 36

2. 93

.3,0 980

4,1 44

12

12

7312.616 20 2. 7 Atm H2O P 5 301 26

7326. 4o6 25 3. 4 u,N Mn I Atm

4. 43 50

7312.962 6 0. 8 Atm H2O Q 6 202 26 7326.713 2 0. 3 Atm H2O P7 202 26

7313.176 6 0. 8 Atm H2O Q 2 221 26 7327.104 11 1. 5 Atm H2O P6 301 26

7313.50 a 2. 5 0. 3 Atm H2O P 5 202 26 7327.370 11 1. 5 Atm H2O P 6 301 26

7313.72 a 1 0. 1 CN R 48 4,1 12 7327.650 18 2. 5 Ni I 3. 80 140

7314.545 5 0. 7 Atm H2O Q 3 221 26 7328.25 1. 5 0. 2 Atm H2O Q4 221 26

7314.96 1 0. 1 ON P 35 4,1 12 7328.45 a 1. 5 0. 2

7315.516

7315.886

32

2. 5

4. 4

0. 3

IIAtmHsO Fe I Atm H2O

Q 2

4. 28

Q 5

221 1105

221

26

26

7328.828

7329.30 a

5

5

0. 7

0. 7

CN

Atm H2OCN

Q21

P4

Q 42

5,2 202

4,1

12

26

12

7316.41

7316.739

7316.858

3

16

5

0. 4

2. 2

0. 7

G

Atm H2O

Fei

Atm H2O

P 3

2. 69 Q 2

202

267

221

26

26

7o30.150

7330.34

7330.859

17

5

68

2. 3

0. 7

9. 3

Fe I G?

Atm H2O

4. 64

fP 6 IQ2

1187

301 221 |26

7317.291 21 2. 9 Atm H2O P 6 301 26 7331.04 0. 5 0. 1 s Ti I 1. 74 143

7317.43 13 1. 8 Fei 5. 01 1278 7332.28 1. 5 0. 2 s,N Til 1. 75 143

7^18 no ± o 1 8 Atm HoO \Q 1 301

221 |26

7332.49 2 0. 3 Cn? 5. 15

7318.382 17 2. 3 s,d ||Atm H2O

Ti I P 7

2. 25

301 21226

7332.74

7332.905

1. 5

6

0. 2

0. 8

Atm H2O

Atm H2O

P3

P7

301

301

26

26

7318.692 33 4. 5 Atm H2O P 7 301 26 7333.049 8 1. 1 Atm H2O P7 301 26

309
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

N0I

7333.58 36 4. 9 Fe I 4. 26 1078

7333.684 24 3. 3 Atm HjO P 8 301 26

A

'4 U. 0 rq 43 \Q 20

4,1 5,2 |12

7334.62 1. 5 0. 2 Fe II CN7. 27 Q 22 209

5,2 12

7334.91 1. 5 0. 2 O?

7335.335 16 2. 2 Atm HjO rP6

IPl

301

221 |26

7335.712 6 0. 8 Atm HjO P 6 301 26

7336.02 1. 5 0. 2 O?

7337.043 5 0. 7 Atm

CN P 37 4,1 12

7337.78 |2| 0. 3 s Ti I p 2. 24 212

7338.07 1. 5 0. 2 CN R 29 5,2 12

7338.94 2 0. 3 s Vi 2. 14 117

7339.340 3 0. 4 Atm H,0

CN

Q 5 Q 21 221

5,2 26

12

7339.67 1. 5 0. 2 CN? Q 57 3,0 12

7339.90 1. 5 0. 2 O?

7340.188 |2.5| 0. 3 u Atm H2O

CN

P 6 Q 43301

4,1 26

12

7340.60 1. 5 0. 2 CN Q 23 5,2 12

7341.351 3 0. 4 Atm H2O Q 3 221 26

7341.78 1 0. 1 s Atm H2O

Fe I p P 5

4. 99 202

1307 26

7342.317 6 0. 8 CN R 31 5,2 12

7343.226 20 2. 7 G

7343.52 a 2.5 0. 3

7343.63 a 1 0. 1 Atm?

7343.939 21 2. 9 Atm H2O P 2 221 26

7344.200 14 1. 9 u Fe I —

Attn H2O

2. 73 P 7 266

301 26

7344.46 1 0. 1 CN P 16 5,2 12

7344.759 40 5. 4 S,d TiiAtm H2O

1. 46 P 7 97 301 26

7345.21 5 0. 7 Dy 11?

7345.42 4 0. 5 CN Q 44 4,1 12

7346.37 a 2 0. 3

7346.56 1. 5 0. 2 CN R 51 4,1 12

7346.87 a 2 0.3 CN

Fe I p

Q 24

3. 30

5,2 12

7347.17 a 4 0. 5 Fe I p 2. 76 266

Wavelength

(A)

7347.309

7348.047

7348.214

7348.51

7348.76

7349.249

7349.493

7350.088

7350.49

7351.113

7351.519

7352.14

7352.72 a

7352.791

7352.90 a

7353.03

7353.213

7353.379

7353.507

7353.923

7354.26 a

7354.606

7355.108

7355.457

7355.891

7356.262

7356.40

7358.76

7356.95 a

7357.097

73.57.739

7358.26

Equivalent Width

AX

(ml)

1

|3.5|

3

5

0. 5

7

8

5

"5

48

62

6

i3|

5

3

1. 5

2.5

2. 5

37

7

Re- duced

Width

AX/X

(F)

4

22

79

10

4

|2|

2. 5

|5i

26

3. 5

0. 1

0. 5

0. 4

0. 7

0. 1

1. 0

1. 1

0. 7

0. 7

6. 5

8. 4

0. 8

0.4

0. 7

0. 4

0. 2

0. 3

0. 3

5. 0

1. 0

0. 3

0. 8

0. 5

3. 0

9. 8

1. 4

0. 5

0. 3

0. 3

0. 7

3. 5

0. 5

Spot

ww

S

u,d?

s? w,N

S

Solar

Identification

Atm

Atm H2O

Atm

CN?

Fe I p Atm

Atm H2O

Atm H2O

Atm H2O

CN

Fe I p Fe I Fe I Til

O

Atm H2O

Atm H2O

Atm H2O

CN

Atm H2O

Fe I |Atm H2O

0?

CN

Atm H2O

Co I O

Atm H2O

Tiiip

Cri

Atm H2O

CNV I Fe I p CN

Ti I? p |Atm H2O

Til

O?

Low

E P

or Rot. Line

P 2

P 38

4. 14

'P 8 .P2

P 9 P 7 Q 23

3. 05

4. 99

4. 95

2. 49

P 7

P 5 P 4

.Q 6 Q 25 P 4

4. 73 P7

Q 58 P 3

1. 88

P5

2. 60

2. 89 P3

Q24

2. 13

4. 64 Q45

1. 05 P3

1. 44

RMT

No.

or Vib. Band

221

4,1 1004

301

221

301

301

5,2 509

1273

1275

272

301

202

202

221

5,2 202

1251

301

3,0

221 "53

301

101

93

221

5,2 117

1187

4,1

221

97

Notes

26

12

\26

26

26

12

26

26

^26

1226

26

12

26

26

26

12

12

26

310
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7358.856

7359.983

5

6

0. 7

0. 8

Atm H2O

0?

Fei

P 3

4. 99

320

1310

26 7370.798

7371.496

7372.13 a

0. 5

7

2

0. 1

1. 0

0. 3

Atm II2O Atm II2O CNP8

P 4 P40

301

221

4,1

26

26

12 7360.13 a

7360.347

7360.70

3

9

0. 5

0. 4

1. 2

0. 1 s

CN

Atm H2O

0

TP "^Q

1 i oy IQ26

P3

A 1

J 5,2

221

}12

26

7372.383

7373.011

1

42

0. 1

5. 7 w,N

Atm?

IN Ij it

llSii- Fe I p

1. 41

5. 98

2. 28

58

108

7361.029 4 0. 5 Atm H2O P4 221 26 7373.25 4 0. 5 Atm H2O P8 301 26

7361.782

7361.994

4

3

4. 4

0. 5

0. 4

s II||AI Al TI Tiip

Atm H2O

2. 25

P5

1

1

212

301 26

7^7^ R99

TV!A 9Q

7374.45 a

l»l

7

2. 5

1 1

1 0

0. 3

JO

iWilH Atm TT„n IJ 2Vy PN — CNAtm?P 4 0 A(\ Q 28

221

4 1

5,2

26

12

12

7362.291 43 6. 8 s All 4. 02 11 7375.251 45 6. 1 s,7V 0

OK! CN

Atm H2O

Q 25 P8

A 1 5,2 3011 91226

lot O.vO^

7376.275 2

n 7

0. 3 0? CN

0 97 P 21

'-'7

5,2

12

12

7362.95 8 1. 1 Atm H2O

Si I? Q3

5. 98

221 26 7376.494 39 5. 3 0? Fe 11 Fe I

7363.742

7363.916

7364.106

7364.38

11

41

24

0. 5

1. 5

5. 8

3. 4

0. 1

0S

Atm H2O

Fei

Til

Atm?

P3

4. 95

1. 43

221

1274

97

26 7377.01

7377.57

7377.865

6

3

5

0. 8

0. 4

0. 7

CN?

CN?

|Atm H2O

G?

fR 54

1 R 35 R 36 P 4

4,1

5,2

221

J

12

26

7364.75

70CK orvc

1 000. OUO

tf 000. 1 «J

5

D

00

0. 7

U. 0

i.. 1

CN

P T?

Atm

R 53

Qy. nnuu V Q

4,1 12 7378.332

7378.77

7380.10

7380.492

4

1. 5

2

1

0. 5

0. 2

0. 3

0. 1

Atm H2O

CN

Atm H2O

Atm H2O

P 5 P 40 Q5

P9

221

4,1

221

301

26

12

26

26

7366.036 1 0.

Atm? 7380.73 3 0. 4 CN Q47 4,1 12

7366.367 19 2. 6 Fei 4. 64 1188 7381.342 10 1. 4 G

7366.602

7366.83

7367.21

7367.76

3

7

1. 5

2. 5

0. 4

1. 0

0. 2

0. 3

S,N Atm

Til

CN

CN

G?

1. 43 P 39 Q2796

4,1

5,2

12

12

7381.504

7381 Q42

7382.357 7382 fil 4

2

26

3

11

0. 3

3. 5

0. 4 W

u

Atm H2O

Ni I Atm HjO

Fe I Atm H2O

P 6

5. 36 P5

2 69 P 5

221

292

221

266

221

26

26

26

7368.468 6 0. 8 Atm H2O P 4 221 26 7382.933 35 4. 7 u Fe I r4. 59

14. 61 1188

7368.75 a 2. 5 0. 3 CN Q46 4,1 12 CN Q28 5,2 12

7368.97 a 2 0. 3 7383.350 1. 5 0. 2 Atm H2O P 11 301 26

7369.206

7369.60

7369.88

7370.119

1181

1

6

24

2. 4

0. 1

0. 8

3. 2

Atm H2O

Atm H2O?

CN — CN

AtmH20-

P4

P 5 R 53 R 35 ;q4

IQ5

4. 73

221

202

4,1 5,2

221

221

26

26

12

12

|26

7383.54

7383.721

7384.45

1. 5

9

5

0. 2

1. 2

0. 7

CN

Atm?

Atm H2O

CN

P 22

P 5 fQ 60 <^P41 LR 36

5,2

221

3,0

4,1 5,2

12

26

Fe I 1250 7384.77 1 0. 1

311
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X fication Rot. Vib. AX AX/X fication Rot. Vib.

(A) (ml) (F) Line Band (A) (ml) (F) Line Band

7385.244 52 7. 0 u Ni I 2. 74 84 7398.96 2 0. 3 Fe I p 4. 99 1306

7385.51 3 0. 4 UN R 37 5,2 12 7399.308 2 0. 3 Atm II2O P 7 221 26 Fe I p 4. 79 1251 7400.188 89 11. 1 S Cr I 2. 90 93

7385.89 6 0. 8 0? M i C\r\ A Cl 7400.48 1 0. 1 7386.201 16 2. 8 JNi I 5. 34 286

7400.851 8 1. 1 Fe I p 2. 61 204

7386.336 94 12. 7 w Fe I 4. 91 1275

7401.134 19 2. 6 w Ni I 5. 36 291 7386.66 3 0. 4 Atm?

7401.46 0. 5 0. 1 Atm H2O P 3 221 26

7387.00 a 5 0. 7 Mg I 5. 75 Atm H2O P 7 301 26 7401.691 48 6. 5 u Fe I 4. 19 1004

7387.25 a 2. 5 0. 3 7401.96 2 0. 3 Atm?

CN R 39 5,2 12 7387.700 118 16. 0 w Mgi .5. 75 30

7402.155 8 1. 1 CN R 56 4,1 12

7388.15 a 7 1. 0 7403.33 1 0. 1 CN? P 42 4,1 12 7388.605 13 1. 8 s,N Atm H2O — P 7 221 26 Co I 2. 72 139 7403.857 1. 5 0. 2 Atm H2O P 6 221 26

7389.391 144 18. 1 w Fe I p — 4. 91 1274 7405.17 1 0. 1 Atm?

|Fe I 4. 30 1077 7405.790 108 IS. 6 W Si I 5. 61 23 7389.66 a 3. 5 0. 5 7406.289 4. 5 0. 6 CN Q 32 5,2 12 7389.88 9 1. 2 CN Q 30 5,2 12 Atm H2O P 6 221 26

7390.241 7 1. 0 Atm H2O P 5 221 26 7406.61 1. 5 0. 2 Atm H2O P 8 221 26

7390.88 1 0. 1 Atm? 7407.06 |1.5| 0. 2 Atm?

CN? P 41 4,1 12 7408.135 1 0. 1 Atm H2O P 7 301 26

7391.270 6 0. 8 Atm H2O P 5 221 26

7408.43 3 0. 4 CN R 39 5,2 12 7391.48 2 0. 3 Atm?

7408.78 0. 5 0. 1 Atm?

7391.717 7 1. 0 Atm H2O P6 221 26 7409.100 72 10. 2 W,N Si I 5. 61 23

7392.13 4 0. 5 CN? R 37 5,2 12 7409.352 98 12. S W Ni I 3. 80 139

7392.654 2 0. 3 Atm H2O P 5 202 26 7409.99 2 0. 3 CN P 43 4,1 12

7393.111 4 0. 5 CN Q 48 4,1 12 7410.324 3 0. 4 Atm H2O P 7 221 26

7393.609 |112| 14. 1 w Ni I 3. 61 109 7410.733 4 0. 5 Atm H2O P 7 221 26

7393.85 a 6 0. 8 7411.162 140 17. 1 w I'e I 4. 28 1077

7394.06 a 3 0. 4 7413.06 4 0. 5 0?

7395.539 1. 5 Atm 7413.52 1. 5 0. 2 Atm?

(Si I) 5. 95

7414.00 3 0. 4 CN Q 32 5,2 12 7396.053 6 0. 8 Atm II2O P 6 221 26

7414.514 76 9. 6 u Nil 1. 99 62 7396.526 14 1. 9 ol Fe I p 4. 99 1278

7414.93 3 0. 4 CN Q33 5,2 12 7396.752 2 0. 3 Atm H2O P 6 221 26 7415.193 13 1. 8 u Fe I p 4. 99 1308

7397.123 5 0. 7 Atm HaO P 6 221 26 CN? P 26 5,2 12

7397.535 1 0. 1 7415.363 28 3. 8 0? Si I 5. 61 23

7397.939 4 0. 5 CN Q31 5,2 12 7415.68 3 0. 4

7398.52 2 0. 3 CN Q 48 4,1 12 7415.958 118 U. 3 W,N Si I 5. 61 22

7398.76 2 0. 3 Fe r p 3. 43 684 7417.06 1. 5 0. 2 CN R 40 5,2 12 CN? P 24 5,2 12 1 Tiip 1. 07
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

IjOw

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7417.39 12 1. 6 Co I 2. 04 89 7435.584 32 4. 3 W,N 0

7418.330 4 0. 5 Fei p 4. 14 1002 7435.95 2 0. 3 0?

7418.672 49 6. 3 IV Fei 4. 14 1001 7437.07 3 0. 4 Co I? 1. 9G 53

7419.31 6 0. 8 Ni I 5. 49 287 7437.608 7 0. 9 0

7419.670 4 0. 5 CN R 41 5,2 12 7437.87 1 0. ] Atm?

7420.241

7420.75 a

7421.030

7421.560

7421.86

4

1. 5

2

20

1

0. 5

0. 2

0. 3

2. 7

0. 1

s

0

Fe I p

Atm H2O

Fe I 0?

5. 08

P7

4. 64

1307

221

1188

26

7438.38

7439.24

7439.87 m

7440.253

2

0. 5

7

0. 3

0. 1

0. 9

s,N

S

CN

Fei?

Zr I CNAtm?

R 43

0. 54 Q35

5,2

23

5,2

12

13

12

7422.286 106 IS. 4 w Nil 3. 63 139 7440.58 3 0. 4 S Ti I 2. 25 225

7422.77

7423.16

7423.509

13|

1. 5

120

0. 4

0. 2

15. 2

sW

0?-

Atm H2O

Ti I

Si I (Ni)

P 4

1. 44

5. 62

10. 32

221

97

23

0

26

7440.919

7441.81

7442.23

7442.47

68

2

3

2

8.4

0. 3

0. 4

0. 3

w

s?

Fe I 0?

N I CN

4. 91

10. 33 Q 36

1273

3

5,2 12

7424.27

7424.647

1 n

o

22

1. 3

0. 3

3. 0 u,N

Atm?

ISi I Atm H2O

/Q 50 IQ34

5. 62 P8

4,1 5,2

23

221

)l2

26

7442.71

7443.026

7443.25

7444.47

1

38

7

11.51

0. 1

5. 1

0. 9

0. 2

w

Atm H2O

Fei

Fe I p CN

P 8

4. 19

5. 08 R 43

221

1002

1309

5,2

26

12

7425.048 0. 5 0. 1 -Fe II? p 7. 27 209 7445.758 178 21. 4 w Fe I 4. 26 1077

7425.560 1 0. 1 Atm 7446.99 1. 5 0. 2 Atm?

7425.850 1 0. 1 Atm H2O P8 221 26 7447.400 38 5. 1 s Fei 4. 95 1273

7427.562 8 1. 1 w 7447.912 20 2. 7 0 — Fe I p 5. 52 1352

7429.78 a

7430.553

7430.846

7431.19

7431.599

7431.97

7432.19 a

7432.44

7432.98 a

2

14

32

2

14

1. 5

4

4

2

0. 3

1. 9

4. 3

0. 3

1. 9

0. 2

0. 5

0. 5

0. 3

s

0

u

s

0

1 w,N

Fei

Fe IFe I Siip

CN?

CN?

ITiip

Fe I p CN?

0?

CN

2. 59

5. 48

4. 61

5. 61 Q34

Q 51

1. 74

4. 64 Q 63

Q 35

204

1351 1189

23

5,2

4,1 142 1189

3,0

5,2

12

12

12

12

7448.20

7448.92

7449.338

7450.33

7451.478

7452.110

7452.96

7454.004

7455.389

7456.28 a

2. 5

2. 5

24

11

3

11

2. 5

11

8

1. 5

0. 3

0. 3

3. 2

1. 5

0. 4

1. 5

0. 3

1. 5

1. 1

0. 2

w

0

w

0SI

CN

Ca I G?

Fe II Yii

CNFe I p CN

Fe I

Si I CNTiip

R 44

3. 91

3. 89 L 75 P 30

5. 06 P 31

4. 19

5. 96 P 46

0. 82

5,2

73

25

5,2

1303

5,2

1001

4,1

12

12

12

12

7433.460 161 0. 8 u,N Ni I 5. 41 280 7457.354 '5

0. 7 Coi ? 3. 93

7434.58

7435.08

10.5

2

0. 1

0. 3

s

s

Ti I p 0

0

0. 81 7458.00

7458.384

7459.00 a

1. 5

1

2

0. 2

0. 1

0. 3

G?

Atm H2O

CN

P 10 Q 37221

5,2

26

12

313
The Solar Spectrum—Continued

length

(A)

EquivaV 1 PTi f. Cl> J. ^Li. K) Width

AX

(ml)

Rerl 1 1 pf^rl Width

AX/X

(F)

Spot

Solar

Identifi t,inn

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

ReH 1 1 paH

Width

(F)

Spot

Solar

Identifi pfi ti on

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7459.33 a 0. 5 0. 1 CN Q 53 4,1 12 7483.415 9 1. 2 Ci 8. 77

7460.549 4 0. 5 O 7484.308 9 1. 2 0? Fe I p 5. 08 1306

7461.25 2 0. 3 CN —

Fe I p

P 31

5. 51

5,2

1.352 12 7484.68 1. 5 0. 2 CN

CN

P 48 P 34

4 1 5,2 12

12

7461.527 26 3. 5 s Fei 2. 56 204 7485.00 <2. 5 <0. 3 O?

7462.342 119 15. 0 s Cri

(Fe ii)

2. 91

3. 89

93

73 7485.14 1. 5 0. 2 CNCN

R 47 R 62

5,2

4,1 12

12

7463.19

7463.395 7463 QQ

7464.268

7465.85

7466.533

1

8

1. 5

12

3

5

0. 1

1. 1

0. 2

1. 6

0. 4

0. 7

0?

0

s,NN

CN

Atm?

Fe I p

S i?p

o

TiipP 32

5. 06

8. 04

1. 74

5,2

1307

142

12 7486.118

7486.667

7488.00

7488.706

7488.92

7489.569

5

13

2

3

1. 5

|9|

0. 7

1. 8

0. 3

0. 4

0. 2

1. 2

Fe I p O

CN

Nil

Atm?

CNITii

3. 88

Q55

3. 83

Q40

2. 25

980

4,1

157

5,2 225

12

12

7467.51

7468.27

7468.927

7470.05

7470.61

7471.34

7471.757

7472.755

7473.563

7474.513

1

4

2

1

1

2

2

16

23

6

0. 1

0. 5

0. 3

0. 1

0. 1

0. 3

0. 3

2. 2

3. 1

0. 8

0

sS

s

w

Atm?

N I CN

Tiip

CN

Tiip

Fe I p

O

Fe I Fe I p —

Fe I p

10. 33 Q 38

0. 84 R 61

0. 81

2. 73

4. 61

3. 98

3. 93

3

5,2

4,1

267

1188

957

980

12

12

7490.84

7491.08

7491.652

7492.333

7492.941

7493.11 7493 58

74Q3 Q40

7494.404

7494.74

4

3

71

2

2

1. 5

2

3

13

1. 5

0. 5

0. 4

9. 1

0. 3

0. 3

0. 2

0. 3

0. 4

1. 7

0. 2

s

0

Fe I p —

Six ?

Si I p

Fe I CN

O?

Atm?

CN

CN

o

Fe I p

3. 30

6. 12

5. 96

4. 30 P 34

P 49 D 41

1. 56

1077

5,2

4 1

33

12

12

12

7474.92 1. 5 0. 2 s,N Til 1. 75 142 7495.077 174 22.6 u Fe I 4. 22 1077

7475.87

7476.149

7476.376

7477.595

7478.84

0. 5

12

18

21

3

0. 1

1. 6

2. 4

2. 8

0. 4

s

0

s u,N

s,N

O

Ci

Fei

Fe I p

CN

Fe 1 p

8. 77

4. 79

3. 88 P48

3. 37

1251

957

4,1 683

12

7495.66

7496.12 74Q7 44

7498.535

7498.78

1

6

\

21

1

0. 1

0. 8

0. 1

2. 8

0. 1

g

u

Fe I p CN

Ti T

Fe I O?

4. 99 P35

2. 24

4. 14

1275

5,2

1001

12

7479.10 2 0. 3 s CN- Q 39 5,2 12 7499.18 4 0. 5 CN P 49 4,1 12 7479.701

7480.816

7481.478

7481.736

7481.934

11

5

13

5

15

1. 5

0. 7

1. 8

0. 7

2. 0

0

w

s,N?

Fe II p

Atm HoO

Nil

Fe I p Fe I

3. 89 P 5

5. 49

2. 76

4. 79

72

221

286

266

1250

26

7500.242

7500.55

7501.280

7501.76

4 <3

3

5

0. 5

<0. 4

0. 4

0. 7

CN

O?

Fe I p

CN —

Nil?

/R 63 IQ41

4. 19 R 49

5. 59

4,1 5,2

1002

5,2 282

}-

12

7482.213

7482.871

20

131

2. 7

0. 4

u Si I Fe I p O5. 86

5. 08 1308

7502.78

7503.31

1. 5

2

0. 2

0.3

S CNCN

Q 56 P 35

4,1

5,2

12

12

314
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7503.94 2. 5 0. 3 O

7504.276 8 1. 1 O

7504.940 10 1. 3 0? Sii?p 5. 96

7505.19 3 0. 4 CN Q 42 5,2 12

7506.030 26 3. 5 u,N Fe I 5. 06 1306

7507.273 67 8. 1 u Fe I 4. 41 1137

7507.80 a 2 0.3

7508.60 2 0. 3 CN

Fe I p

P 50

4. 99

4,1 1274

12

7511.031 221 27. 3 u Fe I 4. 18 1077

7511.51 3 0. 4 O?

7511.80 1 0. 1 O?

7512.166 5 0. 7 Fe I p

r2. 28

\4- 14 108 1001

7512.77 1. 5 0. 2 O?

7513.16 1. 5 0. 2 CN R 50 5,2 12

7514.205 19 2. 5 w O

7514.54 1. 5 0. 2 CN

Atm?

P 36 5,2 12

7515.10 4 0. 5 O?

7515.43 1. 5 0. 2 O?

7515.837 15 2. 0 0 Fe II 3. 90 73

7516.21 2 0.3 CN? Q 20 6,3 12

7516.623 3 0. 4 CN Q 43 5,2 12

7516.82 6 0. 8 O?

7517.96 a 2 0. 3 CN

Atm?

Q 57 4,1 12

7518.66 2 0. 3 CN /Q 68 \R 50

3,0

5,2 }12

7519.89 5 0. 7 Fe I

7521.06 |5| 0. 7 w,N Nil 5. 51 282

7521.58 2 0.3 CN? Q 21 6,3 12

7522.778 84 10. 8 u Nil 3. 66 126

7523.217 20 2. 7 w O

7523.93 1 0. 1 CN P 51 4,1 12

7525.118 73 9. 7 s Nil 3. 63 139

7526.10 1. 5 0. 2 CN P 37 5,2 12

7526.43 1 0. 1 O?

7526.67 3 0. 4 Fe I p 5. 51 1352

7527.26 1 0. 1 CN? Q 22 6,3 12

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7528.18 4 0. 5 s Fe I p — CN5. 03 Q 44

1307

5,2 12

7528.41 2 0. 3 O?

7529.48 2. 5 0. 3 CN /P 51 IQ24

4,1 6,3

7530..58 2 0. 3 Atm

7531.153 101 12. 9 s Fei 4. 37 1137

7531.789 20 2. 7 0 O

7532.12 2 0. 3 O?

7533.373 18 2. 4 u CN —

Fe II Q 583. 90

4,172

12

7534.28 3 0. 4 O

7534.60 a 2. 5 0.3 Nil? 5. 51

7534.85 3 0. 4 Fe II p 3. 94 87

7536.25 a 1. 5 0. 2

7537.475 6 0. 8 Fe I? 4. 07 1000

7537.96 1. 5 0. 2 CNFe I p P 38

5. 52

5,2 1352

12

7538.17 a 1. 5 0. 2

7539.52 2 0. 3 CN?

CN?

P 52 Q24

4,1 6,3 12

12

7540.444 8 1. 1 s Fei 2. 73 266

7541.57 3 0. 4 Fe I 3. 94 957

7541.920 9 1. 2 w O

7545.63 a 5 0. 7 -Nix 5. 61 287

7546.183 40 5. 3 s Fe I

7546.63 1. 5 0. 2 O?

7547.00 4 0. 5 O?

7547.38 4 0. 5 o?

7547.904 24 3. 2 w Fei 5. 10 1306

7549.08 1 0. 1 CN Q 59 4,1 12

7549.82 1 0. 1 CN R 53 5,2 12

7550.13 a 1 0. 1 CN P 39 5,2 12

7551.108 9 1. 2 w Fe I p 5. 08 1303

7552.501 9 1. 2 u Ni I p 5. 61 286

7552.795 2 0. 2 s Fe I p—

CN

5. 03 Q 46

1303

5,2 12

7553.42 1. 5 0. 2

7553.953 4 0. 5 Co I? 3. 95 1S3

7554.841 13 1. 7 u,N O

7555.607 98 12. 7 u Ni I 3. 85 187

315
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7557.695

7558.16

7558.87

9

6

1. 2

0. 8 0?

0?

7583.12 1. 5 0. 2 CN?

Si I p

Fei

rQ30

IQ31

5. 98

6,3

6,3

1. 5 0. 2 7583.796 81 11. 0 M 3. 02 402

7559.705

7561.00 a

7562.62

7563.016

34

0. 5

1

16

4. 5

0. 1

0. 1

2. 1

u,d

u

|Fei

Ni I Atm?

CN

Fei

5. 06

5. 52

P 40

4. 83

1308 292

5,2

1251

12

7584.29

7584.77

7586.027S

7586.52

1. 5

1

132

0. 5

0. 2

0. 1

17.6

0. 1

W

0?

Atm?

Fei

0?

4. 31 1137

7563.66 1 0. 1 0?

7586.70 a

7586.92

7588.310

7588.849

2 0. 3

0. 1

3. 7

1. 2

Co I Atm?

Fei

Fei?

2. 87 139

c0

X. 0

n 7

n 9

k)

1

28

9

?iU

5. 03 1306

7565.21

7565.534

1. 5

8

0. 2

1. 1

0?

CN? — Q 47 5,2 12 7590.76 |21 0. 3 Atm?

CN? Q 31 6,3 12

7 nee OA 0q nu. 4^ PM? KjX\ .' n 9Q u,o 12 7tiQ1 '?9 9 0. 0 7CC7 1 70 7CC7 G1

91

9

9 R

u. 0

0/1 W, 1\MAIiV 7c:qi on „ A

u. 0 Atm?

rt "^9 1 9

n 9 9 12 7593.695m 193 25. 4 Atm O2 fR 271

1_ PXX 9Q^y

0,0 0 n )22

J 7KRQ Qneq on 11,1 T 4. 9R 1 n77 1 OiJO.OOVLlX Q 0yj. 4 P "^1 0 n 99

7569.556 10 1. 3 w 7593.997m 226 29. 8 Atm O2 R 25 0,0 22

7569.95 a 2. 5 0. 3 0? 7594.287m 11 1. 4 Atm O2 R 24 0,0 24

11. 0 n 9 W f i oyrt.ou i ill 9SS ^7 Q A +mtill OnW2 P 9'^ n 0 22

7570.79 1

1 t% !• 0

0. 1

0 9 Cn? 5. 18 7594.974m 139 18. 3 Atm O2 rR27

IR29

0,0 0,0 |22

7=79 Qo 1 ^ n 9 7595.235m 446 58. 7 Atm O2 rR21

1 P 9^

0,0 0 0 )22

J

tut O.ttiiU

7^:70 79 i. 0 D 9

u TTa t

Fe I p 0. yo 7595.590m 5 0. 7 Atm O2 fP 9c; <R 26 P 97

0 0

0,0 i24

J

/Of '±.U'±oo 0. 4 zt IN 1 i 0. 00 1X 00 7c:qc 770^1 / OyO. / i Uo 9QQ zyy oy. 'it A +m n P 9"? Xv ^0 99 7=74 oc 9i^. 0 u. 0 7KQC 99Qm A9^ 00. KK Qy A tm n Pxi 1xyQ 99

7574.58 1 0. 1 CN? Q30 6,3 12 7596.503m 485 63. 8 Atm O2 R 21 0,0 22

7574.88 1 0. 1 CN? Q 29 6,3 12 7596.768m 8 1. 1 Atm O2 R 18 0,0 24

7t;7c; on

t 0 i o.ov u. 0 <! AT OIN — P At c; 9 1X.J9 7t;QO n7rm / oyo.y / om e0 U. 0 Aim A tm n\J2 PXy 90iiU U,VJ 94

7577.30

7f;7q 47

1

i. 0

0. ]

n 9

s 0

Atm

7597.438m 845 111. 2 Atm O2 /R 17 \R 19

0,0

0,0 |22

7r;7Q 707 |0| nU. 0s 0 : 7598.006m 25 3. 3 Atm O2 rR16

1 p 1

«

Lxv Xo

0,0 u,u )24

J 7579.08

7580.28

1

1

0. 1

0. 1

s,N

S Til 2. 23 211

7598.650m

7598.847m

|ll20 147

r Atm O2

1 Atm O2

R 17 R 15

0,0

0,0

22

22

7582.120 8 1. 1 u Fe I p 4. 95 1274 7599.228m 14 1. 8 Atm O2 R 16 0,0 24

7582.48 1 0. 1 0? 7599.462S 17 2. 2 Atm O2 R 14 0,0 24

316
The Solar Spectrum^—Continued

Wavelength

(A)

Equivalent Width AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7599.550m 1 0. 1 Atm O2 R 17 0,0 23 7612.578m 26 3. 4 Atm O2 R 2 0,0 24 7600.066m

7600.493m

> 1530 201

r Atm O2

1 Atm O2

R 15 R 13

0,0

0,0

22

22

7012.745m

7613.194m

3

1120

0. 4

147

Atm O2 Atm O2

R3

R3

0,0

0,0

23

22 7601.127m 17 2. 2 Atm O2 R 12 0,0 24 7613.705m 14 1. 8 Atm O2 R2 0,0 24 7601.240m 1. 5 0. 2 Atm O2 R 14 0,0 23 7014.026m 20 2. 6 Atm O2 R 1 0,0 24 7601.470m ? 2. 6 Atm O2 R 13 0,0 24, 28 7614.15 m 2 0. 3 Atm O2 R2 0,0 23 7601.697m 1210 159 Atm O2 R 13 0,0 22 7614.516 8 1. 1 s Ti I 2. 24 211 7602.036m ? 3. 0 Atm O2 R 11 0,0 24, 28 7615.061m 985 129 Atm 0» R 1 0,0 22 7602.363m 1430 188 Atm O2 R 11 0,0 22 7615.552m 17 2. 2 Atm O2 R 0 0,0 24

7602.995S 30 3. 9 Atm O2 R 10 0,0 24 7616.146m 833 109 Atm O2 R 1 0,0 22 7603.216m 25 3. 3 Atm O2 R 11 0,0 24 7616.980S 120 74 8 s Ni I .3. 65 139 7603.556m 1250 164 Atm O2 R 11 0,0 22 7617.245 12 1. 6 w Fei 5. 06 1304

7604.013m 32 4. 2 Atm O2 R 9 0,0 24 7617.985 9 1. 2 u Fe I 4. 19 1001 7604.453m 1500 197 Atm O2 R 9 0,0 22 7618.28 a 2 0. 3 7605.076m 33 4. 3 Atm O2 R 8 0,0 24 7619.214S 69 8. S s Ni I 3. 68 156 7605.186m 33 4. 3 Atm O2 R9 0,0 24 7619.698m 20 1. 6 Atm O2 P 1 0,0 24 7605.635m

7606.198m

7606.238m

7606. /67m

1480

\ 64

J 1530

195

8. 4

201

Atm O2 (Fei)

r Atm O2

[ Atm O2 Atm O2

R 9

5. 03 R7

R 8 R 7

0,0 1308

0,0

0,0

0,0

22

24

24

22

7620.077m

7620.322m

7620.513 7620.996m

7621.323m

16

2. 5

72

1030

27

2. 1

0. 3

9. 4

135

3. 5

s

Atm O2 Atm O2 Fei

Atm O2 Atm O2

P 2 P 1

4. 73 P 1 P2

0,0

0,0 1250

0,0

0,0

24

23

22

24 7607.366m 46 6. 0 Atm O2 fR 6 \R7

0,0

0,0 |24 7621.802S 24 3. 2 Atm O2 P3 0,0 24 7607.933m 1510 199 Atm O2 R 7 0,0 22 7621.9S8m 7 0. 9 Atm O2 P 2 0,0 23 7608.530m

7608.586m

8. 0

r Atm O2

1 Atm02

R 6 R 5

0,0

0,0

24

24

7622.29 7622.503m2. 5

5

0. 3

0. 7 0

Atm O2 P 3 0,0 23

7608.82 m

1. 1

f Atm O2 R 6 0,0 23 7623.012m 30 3. 9 Atm O2 P 3 0,0 24

7608.91 m 1

' 1 Atm O2 R 5 0,0 23 7623.288m 1055 138 Atm O2 P 3 0,0 22 7609.302m 1450 191 Atm O2 R 5 0,0 22 7623.552m ? 4. 0 Atm O2 P 4 0,0 24, 28 7609.746m 24 3. 2 Atm O2 R 5 0,0 24 7623.715m 12 1. 6 Atm O2 P 3 0,0 23 7609.868m

7610.06 m

7610.455m

7611.007m

7611. 194S

7611.364m

7611.584m

7612.060m

7612.314m

25

4

1330

22

24

5

7

1390

?

3. 3

0. 5

175

2. 9

3. 2

0. 7

0. 9

183

2. 6

Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2

R4

R 5 R5

R4

R 3 R4

R 3 R 3 R 3

0,0

0,0

0,0

0,0

0,0

0,0

0,0

0,0

0,0

24

23

22

24

24

23

23

22

24, 28

7624.500m

7625.354S

7625.475m

7626.157m

7626.524m

7627.054m

7628.225m

7629.092m

1240

36

6

6

40

1165

1490

40

163

4. 7

0. 8

0. 8

5. 2

153

195

5. 2

Atm O2

(Nil)

Atm O2 Atm O2 Atm O2 Atm O2 Atm O2 Atm O2

Atm O2

P 3

5. 63 P 5 P 4 P 5 P 5 P 5 P 5 P7

0,0 292

0,0

0,0

0,0

0,0

0,0

0,0

0,0

22

24

23

23

24

22

22

24

317
The Solar Spectrum—Continued

Equi- Re- Low RMT Equi- Re- Low RMT

Wave- valent duced Solar E P No. Wave- valent duced Solar E P No.

length Width Width Spot Identi- or or Notes length Width Width Spot Identi- or or Notes AX AX/X Rot. Vib. AX AX/X fl + 1011 (A) (ml) (F) Line Band (A) (mA) (F) Line Band

7A9Q 1 Qfim 3 0. 4 Atm P 6 0,0 23 1f Atm 0.. P 17 0,0 24

\ 54 7. 1 7fi9Q QRRm Q 0. 8 Atm O9 P 7 0,0 23 7fi=i0 975 J 1 Fe I 2. 69 266

i \jO\J • ilA 37 4. 9 IX. uliJ. v/2 P 7 0,0 24 7651 50 1. 5 0. 2

1310 172 Atm C^^ P 7 0,0 22 20 2. 6 Atm Oo P 17 0,0 24

1500 197 Atm Oo P 7 0 0 22 4. 5 0. 6 A tin 0.- P 17 0 0 23

44 5. 8 A t,rn 0fi P 9 0,0 24 13 1. 7 .^i Atmuin Oov^2 P 18 0 0 24 7633.131m 3 0. 4 Atm O2 P 8 0,0 23 7653.47 m 2 0. 3 Atm O2 P 17 0,0 23 7634.052m 4 » 0. 5 Atm O2 P 9 0,0 23 7653.757 49 6. 4 Fei 4. 79 1250 7634.170m 43 5. 6 Atm O2 P 9 0,0 24 7654.094m 756 98. 8 Atm O2 P 17 0,0 22 7635.192m 1310 172 Atm O2 P 9 0,0 22 7654.428m 24 3. 1 s,N |Atm O2 P 18 0,0 24

Ti I 2. 25 211 7636.328m 1350 177 Atm O2 P 9 0,0 22 7655.182m 747 97. 5 Atm O2 P 17 0,0 22 7637.183m 41 5. 4 Atm O2 P 11 0,0 24

7655.48 15 2. 0 0? Fe II 3. 89 73 7637.276m 2 0. 3 Atm O2 P 10 0,0 23 7655.847m 11 1. 4 Atm O2 P 19 0,0 24

7638. 306S 46 6. 0 Atm O2 P 11 0,0 24

7656.00 m 2 0. 3 Atm O2 P 18 0,0 23 7639.339m 30 3. 9 Atm O2 P 12 0,0 24 7656.940m 15 2. 0 Atm O2 P 19 0,0 24 7639.585m 1170 155 Atm O2 P 11 0,0 22 7657.26 7 0. 9 Ni I 5. 41 278 7640.457m 31 4. 1 Atm O2 P 12 0,0 24

76.57. 606S 142 16. 1 u,N Mgi 5. 11 22 29 7640.707m 1220 160 Atm O2 P 11 0,0 22 7658.03 1 0. 1 7641.535m 36 4. 7 Atm O2 P 13 0,0 24 7658.420m 13 1. 7 Atm O2 P 20 0,0 24 7641.644m 4 0. 5 Atm O2 P 12 0,0 23 7658.60 1 0. 1 Atm O2 P 19 0,0 23 7642.651m 37 4. 8 Atm O2 P 13 0,0 24

7659.148 17 2. 2 Mgi 5. 11 22 7642.786m 4. 5 0. 6 Atm O2 P 13 0,0 23 7659.370m 657 85. 8 Atm O2 P 19 0,0 22 7643.793m 23 3. 0 Atm O2 P 14 0,0 24

7659.91 31 4. 0 0 Mgi 5. 11 22 7644.200m 1010 132 Atm O2 P 13 0,0 '^2 7660.454m 645 84. 1 Atm O2 P 19 0,0 22 7644.900m 28 3. 7 Atm O2 P 14 0,0 24

Atm O2 0,0 7661.05 m 8 1. 0 Atm O2 P 21 0,0 24 7645.312m 1060 139 P 13 22

29 Atm O2 P 15 7661.198 79 10. 3 u Fe I 4. 26 10777646.098m 3. 8 0,0 24

0. 7 Atm O2

7661.48 13 1. 7 Fe I p 5. 08 1309

7646.209m 5 P 14 0,0 23

7647.2028 29 3. 8 Atm O2 P 15 0,0 24 7662.122m 9 1. 2 Atm O2 P 21 0,0 24

0. 8 Atm O2 P 15 7662.42 a 8 1. 0 C I 8. 77 7647.460m 6 0,0 23

7647.84 1. 2 Fe I 4. 44 1137 7662.84 m 2 0. 3 Atm O2 P 21 0,0 239

7648.12 2 0. 3 7663.00 a 1. 5 0. 2

7648.454m 21 2. 8 Atm O2 P 16 0,0 24 7663.22 0. 5 0. 1 7663.726m 5 0. 7 Atm O2 P 22 0,0 24 7648.580m 2 0. S Atm O2 P 15 0,0 23 7663.90 m 1 0. 1 Atm O2 P 21 0,0 23 7649.035m 842 110 Atm O2 P 15 0,0 22 7664.15 a 7 0. 9 Fe I p 4. 83 1250

7649.553S 25 3. 3 Atm O2 P 16 0,0 24 7664.294 120 U. 1 s Fe I 2. 99 402

7664.872 521 68. 0 S UK I 0. 00 1 7650.135m 918 120 Atm O2 P 15 0,0 22 Atm O2 P 21 0,0 22

318
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent

Vv icltn AX

(mA)

Re- duced

TTT4 _1 i-U VViath AX/X

(F)

opOt

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. oand

Notes Wavelength

(A)

E<jui- valent

Wlflth AX

(mA)

Re- duced

VVKltn AX/X

(F)

opol

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib.

rsanci

Notes

7665.944S 468 61. 0 Atm O2 P 21 0,0 22 7686.830m 2 0. 3 Atm O2 R 17 1,1 22

7666.44 4. 5 0. 6 Atm O2 P 23 0,0 24 7687.034 m 1. 5 0. 2 Atm O2 R 19 1,1 22 7666.669m 0. 5 0. 1 Atm O2 P 22 0,0 23 7687.51 6 0. 8 CN? Q 16 7,4 12 7667.518m

7668.399m

7668.93 a 7669.233m

5-

|1|

1. 5

5

0. 7

0. 1

0. 2

0. 7

Atm O2 Atm O2

Atm O2

P 23 P 23

P 24

0,0

0,0

0,0

24

23

24

7688.127m

7688.40

i Do J.U'l

7

17

1 0

0. 9

2. 2

1. y

0?

Atm O2

Si IP

Fe I p

fR 17

1. 1 L 15

6. 19

r 4y

r>. 10

1 1 f 1,1 J

o,z 1304

22

1 01 z

7669.47 m

7669.668

> DO o o o. Z w

r Atm O2 l-Sii

P 23

6. 19

0,0 23 7689.177m

7689.387m

107

2

13. 9

0. 3

Atm O2 Atm O2

P 29 R 15

0,0

1,1

22

22

7670.31 m 3 0. 4 Atm O2 P 24 0,0 24 7689.703m 3 0, 4 Atm O2 R 13 1,1 22 7670.600m 307 40. 1 Atm O2 P 23 0,0 22 7690.218S 95 12. 4 Atm O2 P 29 0,0 22

7671.669S 307 40. 1 Atm O2 P 23 0,0 22 7690.939m 4 0. 5 Atm O2 R 13 1,1 22

7672.09 m

7672.32 m

3

1

0. 4

0. 1

Atm O2 Atm O2

P 25 P 24

0,0

0,0

24

23

7691.487

7691.569

I

> I1791 Z, L ( . 0 w,N

r Atm O2

1 Mgi

R 11

5. 75

1,1

29

22

7673.127m 3 0. 4 Atm O2 P 25 0,0 24 7691.95 a 17 2. 2 7674.183m 1 0. 1 Atm O2 P 25 0,0 23 7692.722m 3. 5 0. 5 Atm O2 Rll 1,1 22 7674.962m <2 <0. 3 Atm O2 P 26 0,0 24 7693.530m 4. 5 0. 6 Atm O2 R9 1,1 22 7675.240m 1 0. 1 Atm O2 P 25 0,0 23 7694.748m 4 0. 5 Atm O2 R 9 1,1 22

7675.82 a 1. 5 0. 2 7695.62 12 1. 6 7676.026m 1 0. 1 Atm O2 P 26 0,0 24 7695.838S 64 8. 3 Atm O2 P 31 0,0 22

7676.565S 196 25. 6 Atm O2 P25 0,0 22 7696.72 a 2. 5 0. 3 S I 7. 87 7

7677.619S 214 27. 9 Atm O2 P 25 0,0 22 7896.869S 57 7. A Atm O2 P 31 0,0 22 7678.953m 1 0. 1 Atm O2 P 27 0,0 24 7696.996m 2 0. 3 Atm O2 R7 1,1 22

7679.60 4 0. 5 S I 7. 86 7 7698.322m 4 0. 5 Atm O2 R 5 1,1 22

7680.267 106 12. 1 w,N Si I (Mn i)

5. 86

5. 49 36

55

7698.977 7699.506m

154

3

19. It

0. 4

S Ki

Atm O2

0. 00 R5

1

1,1 22 7680.912m

7681.953m

7682.758S

1

10.5

124

0. 1

0. 1

16. 2

Atm O2 Atm O2 Atm O2

P 28 P28

P 27

0,0

0,0

0,0

24

24

22

7701.078m

7702.240m

7702.739m

3

2. 5

26

0. 4

0. 3

3. 4

Atm Oj

Atm O2 Atm O2

R3

R 3 P33

1,1

1,1

0,0

22

22

22 7683.47 a

7683.8020

7684.331m

7684.964m

1. 5

133

1

0. 5

0. 2

1 /. 4

0. 1

0. 1

CN?

Atm O2 Atm O2 Atm O2

Q15

"D 07

J It zi VP 29

7,4

1 1 1,1

0,0

12

zz

zz

24

7703.759in

7704.076m

7705.207m

7709.70 a

27

1. 5

0. 5

2

3. 5

0. 2

0. 1

0. 3

Atm O2 Atm O2 Atm O2

P33

Rl

R 1

0,0

1,1

1,1

22

22

22

7685.12 6 0. 8 s,NN 0 7709.871m 9 1. 2 Atm O2 P 35 0,0 22 7685.281m 0. 5 0. 1 Atm O2 R 25 1,1 22 7710.099m 2 0. 3 Atm O2 P 1 1,1 22 7685.764m 1 0. 1 Atm O2 R19 1,1 22 7710.367 70 8. 7 u Fe I 4. 22 1077

7686.13 6 0. 8 S I 7. 87 7 7710.874m 11 1. 3 Atm O2 P 35 0,0 22

7686.203m 1 0. 1 Atm O2 R 21 1,1 22 7711.731 48 6. 1 1 w Fe II 3. 90 73

319
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AN

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

7712.416m

7712.66 7713.658m

7714.310S

7714.59

7714.91 a

7715.219

7715.591 7716.251m

7717.251m

7717.450m

7718.257m

7719.046 7720.304m

7720.72

4

8

4

103

9

1. 5

12

48

4

3

4

3

27

4

6

0. 5

1. 0

0. 5

1. 2

0. 2

1. 6

6. 2

0. 5

0. 4

0. 5

0. 4

3. 5

0. 5

0. 8

s

w

w

w,N

Atm O3 (Mn I) Co I Atm O2 Nil

Fe I?

Nil

Atm O2 Atm O2 Atm O2 Atm O2 Fe I Atm O2 Fe I p — CN

P3

5. 52

2. 54 P 3

1. 93

3. 70 P5

P37

P5

P37

5. 03 P7

5. 08 P 51

1,1 55

126

1,1

62

109

1,1

0,0

0,0

0,0

1304

1,1 1304

5,2

22

22

22

22

22

22

22

12

7735.94

7737.65 7738.848m

7739.978m

7740.50

7741.44

7742.722 7744.080m

7745.202m

7745.521

7746.605

7747.58

7748.284S

7748.894 7749.554m

7750.670m

4

3

|2|

2

2

4

126

1. 5

2

22

18

1

103

92

1. 5

1

0. 5

0. 4

0. 3

0. 3

0. 3

0. 5

14. 6

0. 2

0. 3

2. 8

2. 3

0. 1

13. 2

11. 3

0. 2

0. 1

w

u

u

Nil?

Fe I p Atm O2 Atm O2 Atm?

G

Fe I Atm O2 Atm O2 Fe I Fe I p

0?

Fe I Ni I Atm O2 Atm O2

5. 29

4. 41 P 15 P15

4. 99 P17

Pl7

5. 08

5. 06

2. 95

3. 70

P 19 P 19

281

1137

1,1

1,1

1306

1,1

1,1

1305

1309

402

156

1,1

1 1

22

22

22

22

22

22 7721.482m 4 0. 5 Atm O2 P 7 1 1 22 7751. 116S 46 B. 8 W Fe I 4. 99 1304

7722.64 16 2. 1 w,N Me I 5. 94 44 7755.275m 0. 5 0. 1 Atm O2 P 21 1.1 22

7723.210 41 5. 2 Fe I 2. 28 108 7755.36 10 1. 3 u,NN

7724 586m 3 0. 4 Atm O2 P 9 1 1 22 7756 378m 0. 5 0. 1 A tiin Oo P 21 1 1 ')^ 22

7724 S80m 1. 5 0. 2 Atm O2 P 39 0,0 22 7759 37 a 7 0. 9 u,NN Ma: I? 5. 93

7725.17 4 0. 5 7760.641 17 2. 2 0? Si I p 6. 20 7725 746m 5 0. 6 Atm O2 P 9 1 1 22 7761 232m 0. 5 0. 1 AAf.m JL \J i.J. J Oo\_/ 2 P 23 1 1 22 7725 862m 2 0. 3 Atm O2 P 39 0,0 22 7764.66 4 0. 5 Mn I 5. 37 54 7727 61 6S 94 11. 8 Ni I 3. 68 156 7765.19 I 0. 1 7729 1 01m 3 0. 4 Atm O2 P 11 1 1

, 22 7766 62 0. 5 0. 1 Fg I p 3. 94 957

7729.40 1 0. 1 7767 458m 0. 5 0. 1 A f.TTl Oo P 25 1 1

J^j J- 22

77'^0 03 a 0. 5 0. 1 7768 51 3m 0. 5 0 1 Atm 0^ P 25 1 1 22 7730 254m 4 0. 5 Atm O2 P 11 1 1 22 7771.954 75 Q J, W,N 0 I 9. 14 I

7730.97 2 0. 3 7772.68 2 \j. 0 \y 1

7732.49 13 1. 7 0 7774.177 66 8. 6 W,N Oi 9. 14 1 7732.746m 0. 5 0. 1 Atm O2 P41 0,0 22 7775.395 50 6. 8 W,N Oi 9. 14 1

7733.12 2. 5 0. 3 Mn I 5. 38 54 7777.10 a 3 0. 4 7733.738m

7733.854m

7734.40

10

2. 5

111

1. 3

0. 3

0. 1

S Atm O2 Fe I p

Atm O2 Mm?

P41

0. ORUD P 13

5. 54

0,0

i OUD

1,1

55

22

22

7777.91 a

7780.568S

7788.933S

7797.588S

2

102

82

79

0. 3

14. 8

10. 8

9. 9

s

s

s

Siip

Fe I Ni I Ni I

6. 08

4. 47

1. 95

3. 90

1154

62

201 7734.995m 2. 5 0. 3 Atm O2 P 13 1,1 22 7798.86 5. 5 0. 7 Fei?p 3. 02 403

320
The Solar Sp cctrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Ifienti- fication

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

7799.21 7800 000

7800.29

7801.16

10

61

5

1. 5

1. 3

7. 1

0. 6

0. 2

W,N

S

0

Si I Rb I O

6. 18

0. 00

81

1

7852.71

7854.692

785.5.16

5

0. 5

6

0. 6

0. 1

0. 8

S,d CN?-

Tiip

Atm H2O

Ni I Fci

R' 9

0. 85 R 6

4. 54

2,0 34

013

267

12

26

7802.51 12 1. 5 u Fe I p 5. 08 1303

7555.405 25 3. 6 w 5. 06 1305

7804.70 a

7807.91 6S

1

64

0. 1

7. 7 u Fe I 4. 99 1303

7855.822

7860.76

3

5

0. 4

0. 6

0wCo I? C I Atm

4. 11

8. 85 32

7810.815 13 1. 7 w Fe I 5. 03 1303 7861.045 12 1. 5 w Nil 3. 70 156

7811.16 46 5. 9 W,N Mgi 5. 94 43 7861.32 3 0. 4 Atm

7813.67 3 0. 4 Fei?p 5. 10 1305 7862.28 1 0. 1 Atm?

7815.82 2 0. 3 O 7863.193 2 0. 3 Atm

7820.81 5 0. 6 Fe I p 4. 29 1118 7863.799 |15| 1. 9 w Nil 4. 54 268

7821.73 3 0. 4 Si I? 6. 08 7864.437S 6 0. 8 Atm H2O R 7 013 26

7826.77 11 1. 4 u Nil 3. 70 109 7865.71 2 0. 3 Atm

7830.78 a 2 0. 3 7866.080 8 1. 0 Atm H2O R 5 013 26

7832.208S 150 18. 5 a Fei 4. 43 1154 7866.710 3 0. 4 Atm H2O R 10 013 26

7832.68 a 5 0. 6 Ci 8. 84 7869.635 26 3. 3 w Fe I 4. 37 1137

7833.06 a

7835.317

7836.130S

7837.10 a

7838.15

7839.64

4

42

64

|2|

5

1. 5

0. 5

6.4

7. 5

0. 3

0. 6

0. 2

s,N

s,N

Siip

All

All

Ci

Co I Fe II p

O?

6. 08

4. 02

4. 02

8. 85

3. 97

3. 97

68

10

10

32

87

7869.94

7870.50

7871.30 a

7871.67 a

7872.79

10

1

2

1. 5

11

1. 3

0. 1

0. 3

0. 2

1. 4

s

s

Zri

|Atm H2O

Atm H2O

Co I

Atm H2O

(CN)

(CN)

0. 69 R 5 R 9

4. 17

R 6 R5

R6

41 013

013

189

013

2,0

2,0

26

26

26

12

12

7840.05 a 2 0. 3 Co I 4. 11 7873.34 3 0. 4 CN R7 2,0 12

7841.37 3 0. 4 Fe II p 3. 90 72 7873.96 1 0. 1 CN R 8 2,0 12

7843.04 13 1. 7 0? O 7874.84 1. 5 0. 2 CN R9 2,0 12

7844.569 11 1. 4 w Fe I 4. 83 1250 7875.320 "8

1. 0 Atm H2O R 8 013 26

7845.27

7846.272

7846.52

2

1

2

0. 3

0. 1

0. 3

Atm

Atm H2O

Atm?

Fe i?p

R7

5. 02

013

1323

26

7876.114

7876.570

7876.705

6

11

1. 5

0. 8

1. 4

0. 2

Atm H2O

(CN)

Atm H2O

Atm

R 5 R 10 R 5

013

2,0

013

26

12

26

7848.20 a 1. 5 0. 2 Ci 8. 85 7877.059 20 2. 6 0 Mg II 9. 99 8

7848.74

7849.38

7849.984

7850.88

7851.95

2

1. 5

|66|

3. 5

2

0. 3

0. 2

7. 8

0. 4

0. 3

s W,N

s?

Atm H2O

Zri

Si I CN?

0?

R' 3

0. 69

6. 19

R' 11

013

40

81

2,0

26

12

7877.45 a

7877.80 a

7878.89

7879.78

7879.86

im

3

2

8

3

1. 4

0. 4

0. 3

1. 0

0. 4

Coi?-

(CN)

CN

Fe I Atm H2O

R 11

R 12

5. 03 R4

2,0

2,0

1306

013

12

12

26

321
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

IdentificTtion

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7880.699 7 0. 9 Attn H2O R 7 013 26 7898.12 a 1 0. 1 CN R 14 2,0 12

7880.847

7881.67

7881.92

7882.30

7882.84

3

8

17

1. 5

1. 5

0. 4

1. 0

2. 2

0. 2

0. 2

i w,N

J

CN

J Mgi

[Atm H2O

CN

CN

R 13

5. 93 R 5 Q4

R 14

2,0

013

2,0

2,0

12

26

12

12

7898.38

7899.53

7899.86

7900.797

2

1

3

13

0. 3

0. 1

0. 4

1. 6

CNCN

Atm H2O

CN

Atm H2O

(CN)

Q 10 P 6 R4

R 15 R 4 R 20

2,0

2,0

112

2,0

013

2,0

12

12

26

12

26

12

7884.44 2 0. 3 CN Q 5 2,0 12 7901.16 0. 5 0. 1

7885.014S

7885.18 a

5

4

0. 6

0. 5

S |Atm H2O

Tiip

CN

R4

0. 84 R 15

01334

2,0

26

12

7901.780 40 5. 1 Atm H2O

(CN)

/R 4 \R3

/Qll

IR 16

013

013

2,0

2,0

J26

}-

7885.72

7886.202

0. 5

2

0. 1

0. 3

Atm?

CN

Atm H2O

P3

R4

2,0

013

12

26

7902.880

7903.160

2

6

0. 3

0. 8 s

Atm H2O

Atm H2O

CN

R 3 R 3 P7

013

013

2,0

26

2612

7886.802 6 0. 8 Atm H2O R 6 013 26 7903.794 2 0. 3 Atm H2O R 3 112 26

7887. 117S 12 1. 5 Atm H2O R 6 013 26 7904.18 4 0. 5 CN

Fe I? p

CN

CN

R 17

2. 99 R21

Q 12

2,0 12

7887.78

7889.339

2

7

0. 3

0. 9 CN

Atm H2O

(CN)

R 16 R4

Q7

2,0

013

2,0

12

26

12

7904.53

7905.60

3

3

0. 4

0. 4

uu

403

2,0

2,0

12

12

7890.12

7890.420

7890.63 a

7890.99

5

1. 5

2

1. 5

0. 6

0. 2

0. 3

0. 2

u,N

u,N

Ni I

CN

Atm H2O

rs. 90

\4. 54

Pl 17 R 4

200

267

2,0

013

12

26

7906.33

7906.80

7907.46

7908.14

0. 5

1. 5

0. 5

3

0. 1

0. 2

0. 1

0. 4

Atm H2O

CN

Atm H2O

CN

Cr I?

Q 6 R 18 Q 5 P8

5. 62

013

2,0

013

2,0 316

26

12

26

12

7891.144 3. 5 0. 4 Atm H2O R4 013 26 7908.750 42 5. 3 Atm H2O R3 013 26

7891.90 14 1. 8 Atm H2O R, 4 013 26 7909.05 1. 5 0. 2 CN Q 4 2,0 12

7892.10 a

7892.57 a

7893. 51 2S

3

2. 5

19

0. 4

0. 3

2. 4

CN

Atm H2O

Q 8

R 5

2,0

013

12

26

7909.370

7909.610

8

17

1. 0

2. 2

s,N |Atm H2O

Tiip

CN

R 2

3. 32 fQ 13 \R 19

013

308

2,0

2,0

26

12

12

7893.62 3 0. 4 CN R 18 2,0 12 7910.684 13 1. 6 Atm H2O R 3 013 26

7894.15 6 0. 8 CNCN

CN

R9

R 8 R 10

2,0

2,0

2,0

1212

12

7911.84 a

7912.004

2

5

0. 3

0. 6 s

CN

Atm H2OSi I

Q 7 R 2

2,0 013

12

26

7894.849 |6| 0. 8 Atm II2O CN

R 5 Rll

013

2,0 26

12 7912.384 15 1. 9 w 6. 10 68

7895.13 2. 5 0. 3 CN Q 9 2,0 12 7912. 870S 40 5. 1 S Fe I 0. 86 12

7895.515

7896.035

23

27

2. 9

3. 4

u Atm H2O

(Tiip)

(CN)

Atm H2O

R 3

0. 83 R 12 R3

01334

2,0

013

26

12

26

7913.12 a

7913.438

3

17

0. 4

2. 2 w

CN

Si I CNCN

R 23

5. 86 P9

Q8

2,0

35

2,0

2,0

12

12

12

7896.378 28 3. 6 0 Mg II 10. 00 8 7913.80 5 0. 6 s CN Q 14 2,0 12

7896.66 3 0. 4 CN R 13 2,0 12 7915.35 6 0. 8 CN Q9 2,0 12

7897.06 2 0. 3 CN R 19 2,0 12 7915.634S 14 1. 8 Atm H2O R2 013 26

322
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

E()ui- valent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Tdttnti- fication

Low

E P

or Rot. Line

RAIT

No.

or

Vib. Band

Notes

7916.32

7916.532

7916.79

2. 5

2. 5

1. 5

0. 3

0. 3

0. 2

CN

Atm H2O

Atm H2O

R 21 R 4 Q 3

2,0

112

013

12

26

26

7933.12

7933.48

22

6

2. 8

0. 8

s?

s

Cu I (CN)

CNCN

3. 78 Q 18 R 27 Q 15

f; 2,0

2,0

2,0

12

1212

7917.428 31 3. 9 s Nil 3. 74 109 7934.11 2. 5 0. 3 0?

7917.561 10 1. 3 Atm H2O rR4

\R 2 112 013 )26

J 7934.90 a 4 0. 5 CN P 9 2,0 12

7917.78 7 0. 9 CN \R 24

2 0

2,0 )12

7936.39

7937. 150S

3

166

0. 4

20. 7 u

CN

Fei

P 13

4. 31

2,0

1136

12

7918.383 100 11. 9 W Si I 5. 95 57 7937.65 3 0. 4 CN Q 16 2,0 12

7920.03 2 0. 3 CN R22 2,0 12 7938.05 3 0. 4 CN R 26 2,0 12

7920.24

7920.666S

7922.77 a

7922.98

7923.81

7924.169

7924.348

7925.30

3

32

2

7

3

16

21

2

0. 4

4. 0

0. 3

0. 9

0. 4

2. 0

2. 7

0. 3

s,NN

o1

0?

CN

Atm H2O

CN

CNCN

IS I CN

Fei

CN

Atm H2O

(CN)

Atm?

Si I? p

Q 11 R 2 R25

Q 16 Q 12

8. 41 P 6

4. 79 R23

R 1 P 11

6. 20

2,0

013

2,0

2,0

2,0

22

2,0

1250

2,0 013

2,0

81

12

26

12

12

12

12

12

26

12

7938.61

7938.96

7939.23

7941.096S

7941.79

7942.00

7942.74

7943.28

6

1

6

38

11

8

4

2. 5

0. 8

0. 1

0. 8

4. 8

1. 4

1. 0

0. 5

0. 3

s

s

s

u1

ITiip- CN

Atm H2O

CN

Fei

Atm H2O

Fe I

|Cri

CN

Atm H2O

(CN)

CN

1. 88 Q 19 Q 3 fP 10 \R28

3. 27 RO

3. 05

4. 39 Q 17 Q 5 P 14 R 27

151

2,0 013

2,0 2,0 623

013

508

300

2,0

013

2,0

2,0

12

26

26

12

26

12

12

7925.82

7926.29

15

5

1. 9

0. 6

Q Si I CN

Til

6. 22 Q 13

3. 28

2,0 308

12

7944.001

7944.38

147

2

17. 6

0. 3

w,N Si I (Til)

CN

5 98

3. 29 Q 20

57 308

2,0 12

7926.54 5 0. 6 0 7945.27 2 0. 3 CN R 29 2,0 12

7927.14 1 0. 1 CN P 7 2 0 12 7945. 858S 185 22. 6 s Fe I 4. 39 1154

7927.928 8 1. 0 CN /Q 17

\tx Zo

2,0 2,0 )l2

J 7946.744 5 0. 6 Atm H2O

(CN

)

Q 3 ^ IS 112

0 0 26

1

7928.24 2 0. 3 Atm H2O Q 4 013 26 7947.63 2. 5 0. 3 s Rb I 0. 00 1

7928. 618S 27 3. 4 Atm H2O

(Si)

R 1

8. 41 01322 26 7947.726 10 1. 3 Atm H2O Q 2 013 26

7929.20 0. 5 0. 1 Atm H2O R3 112 26 7948.78 6 0. 8 u CN fP 12 \R 28

2,0

2,0 )12

7929.339 4 0. 5 Atm H2O R 3 112 26 7949.149 9 1. 1 S Ti I 1. 50 125

7929.81 3 0. 4 CN Q 14 2,0 12 7949.38 a 2 0. 3

7929.939 1 0. 1 Atm H2O R 4 112 26 7950.42 7 0. 9 s CN Q 21 2,0 12

7930.28 2 0. 3 Gd II CNSi

P 12

8. 41

2,0 22

12 7950.889

7951.176

9

10

1. 1

1. 3

Atm H2O

Atm H2O

Q4

R 3

013

112

26

26

/yoU.oiy

7931.772

7932.351

AA

5

90

O. 0

0. 6

11. 3

tt AT

W,N

Mg I Atm H2O

(Si)

Si I

K dA

R 1

8. 42

5. 96

013

22

57

26

/ yoi. / 0

7953.07

iU; n

2.

5

1. 0

0. 3

s CN

Atm?

Nil

R 30

4. 54

9 n

2,0

266

1 912

323

761-925—66

—23
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

ReducGcl Width

AX/X

(F)

Spot

ooitir Identification

Low

or Rot. Line

RMT

IN 0. or Vib. Band

Notes

vv tivt;- length

(1)

EquiV laltJIl \j Width

AX

(ml)

Re-

(luC6(i Width

AX/X

(F)

Spot

ooitir Identification

Low

or Rot. Line

RMT

IN 0. or

Vib. Band

Notes

1. 5 0. 2 O ? 7970.11 2 0. 3

\ w,N

r CN Q 24 2 0 12

7953.64 10 1. 3 Atm? 7970.300 35 4. 4 1 Si I 5. 96 57

7953.84 8 1. 0 Atm H2O Q 1 013 26 7970.81 1. 5 0. 2 CN P 18 2,0 12

7954.12 2 0. 3 CN P 13 2,0 12 7971. 522S 30 3. 8 Atm H2O P 1 013 26

7954.57

7954.97

7955.71

7956.19

3

7

27

10

0. 4

0. 9

3. 4

1. 3

I s,N

J w

fCN

LFe ip

Fe I Atm H2O

(CN)

R 29

2. 99

5. 03

Q 3 P 16

2,0

402

1305

013

2,0

12

26

12

7971.86

7972.15

7973.79

7974.136

47

3

6

0. 5

0. 9

0. 4

0. 8

0?

Atm

CN

CN

CN

Atm H2O

P 16 R 33 R 32 P 2

2,0

2,0

2,0

112

12

12

12

26

7956.71

7957.01

7957.77

7958.21 7958.492S

7959.148

7959.70

7960.270

7

6T

3

52

23

1. 5

15

0. 9

0. 8

0. 5

0. 4

6. 6

2. 8

0. 2

1. 9

s

s

w

Zr I CN

CN

Atm

CN

Atm H2O

Fei

CN

Atm H2O

0. 65 Q 22 Q20

R 31 Q 2

5. 03

P 14 Q 2

41

2,0

2,0

2,0

013

1304

2,0 013

12

12

12

26

12

26

7974.69

7975.002

7975.58

7976.30

7976.586

7977.215

7977.995

7978.46 a

7

6

6

2

4

4

6

0. 9

0. 8

0. 8

0. 3

0. 5

0. 5

0. 4

0. 5

CN

Atm H2O

Si I 0?

Atm H2O

CN

Atm

CNCN

Q 23 Q 5

6. 08

Q 5 Q 25

P 17 P 19

2,0 013

68

112

2,0

2,0

2,0

12

26

26

12

12

12

7960.734 49 6. 2 Atm H2O Q 1 013 26 7978.834 13 1. 6 Til ri. 89

\3. 32

151 308

7961.604

7962.606

7962.861

27

12

14

3. 4

1. 5

1. 8

s |Atm ii20 Til

CN

Atm H2O

/R 2 IQ5

3. 30 Q 21 Q 3

112 013

308

2,0 013

|26

12

26

7979.00 a

7979.81

7980.008

3

3

9

0. 4

0. 4

1. 1 u

CN

Atm H2O

Fe I p

R 34

Q3

5. 08

2,0 013

1304

1226

7963.00 a

7963.132

7963.42 a

8

43

6

1. 0

5. 4

0. 8

Atm H2O

Atm H2O

CN

CN

/Q 4 lR2

Q3

Q 23 P 17

013

112

013

2,0

2,0

|26

26

12

12

7980.452

7980.79

7981.150

7981.54

13

4

6

1

1. 6

0. 5

0. 8

0. 1

s

Atm H2O

CN

CN

0?

Q 3 R 33 Q 24

112

2,0

2,0

26

12

12

7964.349 27 3. 4 Atm H2O Q 3 013 26 7982.06 a 1. 5 0. 2

7964.970 24 3. 0 w,d |Atm H2O

Fe I p (CN)

Q 4

5. 06 R 32

013

1303

2,0

26

12

7982.87

7983.65

1. 5

1

0. 2

0. 1

Atm

Atm

7965.55

7966.43

7967.10

7967.70

3

1. S

3

2

0. 4

0. 2

0. 4

0. 3

s,N

s

Fe I p — CN

Atm

CN

Atm H2O

5. 08

P 15

R 31 Q 5

1305

2,0

2,0 013

12

12

26

7984.00

7984.615

7985.17

7986.264

3

oU^0

8

1. 5

13

0. 4

0. 0

1. 0

0. 2

1. 6

Atm H2O

Attn H„0

CN

CN

Atm H2O

Q 5 P 9 Q 26 P IS P 2

013

013

2,0

2,0 013

26

26

12

12

26

7968.121 30 3. 8 Atm H2O ro 5 IQ4

013

013 |26 7986.48 a 3 0. 4 CN P 20 2,0 12

7968.473

7968.765

14

6

1. S

0. S

Atm H2O

CN

Atm H2O

Q 2 Q 22 Q 5

013

2,0 013

26

12

26

7987.24

7987.391 1 22 2. 8

f s,N

I .

0

Atm

Co I 2. 08 89

324
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent W lutu AX

(mA)

Re- duced

Wiutn

AX/X

(F)

opot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

7987.97 5 0. 6 5? CN Q 25 2,0 12 8004.971 7 0. 9 Atm H2O P 3 013 26

7988.113

7988.40 a

7990.729

7990.90

/yy i.oz

7991.71

11

1

15

7

1

2

1. 4

0. 2

1. 9

0. 9

U. 1

0. 3

Atm H2O

(CN)

Atm H2O

Atm?

A J. 0 Atm

0?

P 3 R 34

P 2

112

2,0

013

26

12

26

8006.46

8006.62

8006.97

8007.470

8007.720

8008.455

8009.38

14

4

5

95

14

14

4

1. 8

0. 5

0. 6

11. 9

1. 8

1. 8

0. 5

0?

Atm H2O

0?

Atm H2O

Atm H2O

CN

Siip

Q5

P 3 P 3 Q 29

6. 12

112

013

013

2,0

74

26

26

26

12

7992.322 9 1. 1 S CN fP 19 IQ 27

2,0 2,0 8010.088 6 0. 7 CN Q 28 2,0 12

7993.048

7993.43

7993.86

7994.02 a

'JCiCiA AQQQl

/ yy4.4ooo

7994.75 a

7995.019

5

3

4

6

OU

3. 5

12

0. 6

0. 4

0. 5

0. 8

0. U

0. 4

1. 5

u,N

s

w

u

All

Atm H2O

Ci?

Atm H2O0

Atm H2O

r e I CN

CN

Siip

4. 08

R 6

9. 33 R 5

R 1

P 21 0 2fi

5. 61

211

112

112

2,0

2 0

21

26

26

26

12

12

8010.896

8011.72

8011.98

8012.273

8012.484

8012.940S

8013.384

8013.81

|10|

4

3

10

15

43

17

3

1. 2

0. 5

0. 4

1. 2

1. 9

5. 4

2. 1

0. 4

0?

w

Atm H2O

CN

CN

Si ?p

Atm H2O?

-CN

Atm H2O

Atm H2O

Atm H2O

Q3

R 37 P 23

7. 87 R 3 R 38 P4

Q4

R7

112

2,0

2,0

112

2,0

013

112

211

26

12

12

26

12

26

26

26

7995.63

7995.809

6

2. 5

0. 8

0. 3

\ t N

r CN

1 0

rR35

IR36

2,0

2,0 }- 8014.051

8014.713

25

6

3. 1

0. 7

Atm H2O

Atm H2O

P4

R2

013

112

26

26

7996.485 11 1. 4 S Til 3. 34 308 8015.03 a 3 0. 4

7996.80 2 0. 3 Co I? 2. 14 79 8015.652 4 0. 5 Atm?

CN P 22 2 0 12

7997.572

7998.247

1. 5

23

0. 2

2. 9

Atm

Atm H2O R 1 112 26

SOI fi 'i9'? 7 Kit U Atm Hod

Fe I p 0 4

4. 79

1 1

1249

26

7998.499 15 1. 9 Atm H2O P3 013 26 8017.04 8 1. 0 CN Q 30 2,0 12

7998.953 172 20. 4 u Fe I 4. 37 1136 8017 425 12 1. 5 Atm H2O Q 5 112 26

7999.88 3 0. 4 CN P 20 2,0 12

SOI s 04.4 10 i.. u Cr I —

|CN Q 29 9QQ

2,0 12 8000.300S 57 7. 1 Atm H2O

(CN)

P 3 Q28

013

2,0 26

12 8018.304 6 0. 7 Atm H2O Q 3 112 26

8000.52 2 0. 2 Atm? 8018.64 a 2 0. 2

8000.959 4 0. 5 Atm H2O R 4 112 26 8020.240 . |6| 0. 7 s CN R 38 2,0 12

8001.40 1. 5 0. 2 Atm? 8020.709 23 2. 9 Atm H2O P 4 013 26

8002 OKjyj ^ 40

5 0. 6 CN 0 27 1 2 8021.07 a 5 0. 6 CN P24 2,0 12

8002.56 7 0. 9 Fei 4. 58 1217 8021.44 2 0. 2 CN R 39 2,0 12

8003.237 14 1. 8 Atm H2O

(CN)

R 4 P 22112

2,0 26

12

8022.055

8022.52

14

2

1. 8

0. 2 u

Atm H2O

Atm HoO

Q 2 R 6

112

211

26

26- 8003.53 6 0. 7 Atm?

CN R 36 2,0 12 8022.971 10 1. 2 Atm H2O Q 5 112 26

8003.93 |3| 0. 4 CN R37 2,0 12 8023.166 20 2. 5 Atm H2O R 1 112 26

8004.588 3. 5 0. 4 Atm 1 8023.852 14 1. 8 Atm H2O P4 013 26

325
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Reduced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

8024.178

8024.547

8024.861

8025.193

8025.865

8026.09

8026.38

12

14

11

8

8

6

6

1. 5

1. 8

1. 4

1. 0

1. 0

0. 7

0. 7

0&

Atra H2O

Ti I Atm H2O

Atm H2O

CN

Atm

CN

R 2

1. 88

P 4 P 4 Q 31

Q 30

112

151

013

013

2,0

2,0

26

26

26

12

12

8041.77

8042.321

8043.169

o04o.Diz

8043.874

5044. o9o

131

9

1231

|7|

17

loci |25|

0. 4

1. 1

2. 9 n A u. y

2. 1

0. 1

u

CNAtm H2O

Atm H2OAtm H2O

Atm A 4-«rt XT r\ XI2U CN

Atm ii2U

Atm

(CN)

P25

P5

Q 2 P 6

tr D Q 32 P 5

Q33

2,0

013

112

013

013

2,0 013

2,0

1226

26

26

0£? 26

1226

12

8026.925 |41| 5. 1 w llSii Atm rl2U

6. 26

T> A li 4Oil ZD 8045.530S |39| 4. 8 Atm H2O /Q 1 LR 3 112 211 I26

J 8027.39 lot |2| 0. 2 C A7 V I 1. Uo on 5U4d.Uooo t Ad.

7d>. 0 u Fe I

A At

4. 41 1136

8027.838 13 1 a1. 6 W 0

on AC ACi / A A Atm A +TM XT r\ s±2\) P 5 A 1 0 013 OCZD

8027.93 19 Z. 4 W r e I 0 OK 6. Zo Clf\AC! OA '7i U. y 01 I p

10 D. Iz 7o

8028.318 70 P. 5 w Fe I

A A"? 4. 47 1154 OA A'y iiO CQ o047.6zoD |58|

ct Fe I A Oct 0. 80 12

8028.544 A A 44 5. 5 Atm H2U r 5 Olo ZO OA A 0 AOA o04o.9o0 lU 1 0 1. z Atm A +TM XT r\ XI2U T)R /i 4 211 o£i ZD

8029.02 a 3 0. 4 UN R 39 0 A

2,0 Iz OA Art 00 8049.33 |18| 0 0 z. z W,JM N

8029.21 a 2. 5 0. 3 Uo I 4. 05 OA /I A C A « 8049.54 a

1

0

Iz "1 c1. 0

8029.453 3. 5 0. 4 Atm I12U K 5

011 ZO 0A /) A AA

8049.yu A 0 4Z K 0 0. z Mg I 5. yo

8030.36 2 0. 2 ON T> 0 C r zo 0 c\ 2,0 Iz 0 A C A 0 /I b0ou.z4 a

T>1 relate jjeiect

8030.67 3 0. 4 ON R 40 0 f\ 2,0 1 0Iz 8051.12 0z

A 0 u. z OJN T> O^i if ZD 0 A

2,0 1 012

o r» o I o c; rv 8031.269 9 1. 1

A 4.TM XT r\ Atm HjO (ci 2

1 1 0 112 ZD OA CO /IOC »05z.4do 11 1. 4 Atm A +TM XTXI2U if 0 Ulo OAZO

8032.04 1 0. 1 Atm? 8052.88 2 0. 2 0?

8032.77 3 0. 4 CN P24 2,0 12 8053.098 8 1. 0 s CN- Q33 2,0 12

8033.606 18 2. 2 Atm H2O Q 5 112 26 8053.81 2 0. 2 0?

8034.293

8034.50 a

23

3

2. 9

0. 4

Atm H2O

Nil

Q 3

3. 74

112

109

26 8054.311

8054.903

52

8

6. 5

1. 0

Mgi

(CN)

Atm H2O

5. 93

Q 34

P6

2,0

013

12

26

1 7 s PN /Q 31 IQ 32

2,0 2,0 8055.995 7 0. 9 s? Co I? 4. 15 193

8035.36 9 1. 1 Atm H2O /R 2 IQ4

5. 98

112

112 |26

8056.36 3 0. A 0 !

8035.608 32 4 0 w,N Si I 57 8056 67

8056.95

2

3

0. 2

0. 4

0?

G?

8036.460S 35 4. 4 Atm H2O fQB

\P 5 112 013 }26 8057.27 4 0. 5 s CN R 42 2,0 12

8037.878 3 0. 4 Atm H2O /R 1 \Q6

R 40 P 5 P 26 R 41

112 013 }26

8057.91 2. 5 0. 3 Sii?p 6. 10 68

8038.15

8039.600S

8040.00

8040.28

8041.038

3

25

2. I

3

3

0. 4

3. 1

) 0. S

0. A

0. ^

t

1

[

Atm?

CN

Atm H2O

CN

CN

Atm

2,0

013

2,0

2,0

12

26

12

12

8058.54

8058.74

8059.538

8060.249

8060.70

6

7

13

11

2

0. 7

0 9

1. 6

1. 4

0. 2

0?

Atm

Ci

Atm H2O?

Atm H2O

Atm H2O

CN

CN

8. 85 P 6 P 7 P7

fP 28 \R43

P27

013

013

013

2,0

2,0

2,0

26

26

26

]n

12

326
The Solar Spectrum—Continued

WaveIcngtb.

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

8061 16 m Cr I 4. 41 300 13

8062.161 10 1. 2 Atm H2O

Atm H2O

P 6 P 6 013

013

26

26

8062.594 8 1. 0 s CN Q34 2,0 12

8062.89 1. 5 0. 2 Atm H2O P 6 013 26

8063.10 m s Zri 0. 62 40 13

8063.286S 14 1. 7 Atm H2O R 5 211 26

8064.106 7 0. 9 CN Q 35 2,0 12

8064.61 1. 5 0. 2 Atm?

8065.226 8 1. 0 Atm

8065.876 6 0. 7 Al I 4. 08 16

8066.07 m 5 Til 1. 89 151 13

8067.08 a 1. 5 0. 2 CN fR4

\R 5

3,1 3 1 }l2

8067.26 6 0. 7 CN f R 43 IR6

2 0

3^1 }l2

8067.78 5 0. 6 CN R 7 3 1 12 8068 261 7 0. 9 s Ti I 1. 87 151

8068.50 3 0. 4 Q Sm II CN

1. 75 R 8 68

3,1 12 8069 34 2 0. 2 8069 79 9 1. 1 Si I? p 6. 27

8070.016 25 3. 1 0? Atm H2O? Q 1 112 26

8070.34 7 0. 9 s Zri 0. 73 40

8070.620 29 3. 6 SiiCN

Ci

6. 08

rp 28 ^R44

[R 10

8. 85

2 0

2,0 30,11 J

8071.262 |21| 2. 6 0 Si I 6. 10 32

8071.50 a 2 0. 2

8072.162 12 1. 5 s Fe I 2. 42 108

8072.381 6 0. 7 CN Q 35 2,0 12

8073.029 |14| 1. 7 w,N 0

8073.80 1. 5 0. 2 CN R 12 3,1 12

8074.430 6 0. 7 CN Q 36 2,0 12

8074.744 4 0. 5

8075.158S 33 5. 8 S Fei 0. 91 12

8075.35 a 5 0. 6 Al I 4. 09 16

8075.549 6 0. 7 0

8075.75 a 3, 5 0. 4 CN R 13 3,1 12

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

A\/X

(F)

Spot

Solar

IdentiLow

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

•

8076.293 10 1. 2 Atm H2O fP 8 \P8

013

013 |2G

8077.012 2 0. 2 CN Q4 .3,1 12 R077 0\J 1 1 .uo fiS yj, 0 CN R 44 12

oU / / . yO Q0 fl0. 4T CN R 14 3 1 12

OUI O.iJOi 1 1 T 4 Ci

R 4

8. 85

211 26

8079.00 a 1 0. 1

8079.252 3 0. 4 Atm H2O P2 112 26

8079.597 3 0. 4 Atm H2O P7 013 26

8080.00 a 1 0. 1

8080.30 a 1. 5 0. 2

8080.582

8080.69

28

12

5. 3

1. 5

Ti I p Fei2. 17

3. 30

195

623

8080.97 a 2. 5 0. 3 CN P29 2,0 12

8081.523 12 1. 5 Atm H2O

CN — CN

P 1 R 45 P 30

112

2 0

2)0

26

12

12

11 U. 1 Atm Fr„o P 7 yj XO 26 S089 U Q 1. 1 CN 0 3fi 2 0 12

A

\j. 0 Atm H2O P3 112 26

8083.19 3 0. 4 CN R 16 3,1 12

8083.82 5 0. 6 Ci 8. 85

8084.807 1. 5 0. 2 Atm XI2U R 4 310 26

ouoo. 140 |iOU| Fe I 4. 44 1136

8085.431 14 1. 7 Atm H2O fR 4 IQ3

211

112

1j26

8085.82 5 0. 6 Atm H2O R4 310 26

8086.18 6 0. 7 CN R 17 3,1 12

8087.46 2. 5 0. 3 CN Q 8 3,1 12

8088.31 3 0. 4 CN R45 2,0 12

8088.56 . 2 0. 2 Atm?

8089.361 13 1. 6 CN? R 18 3,1 12

8089.76 6 0. 7 CN

CNCN

R 9 R 8 R 10

3,1

3,1

3,1

12

12

12

8090.30 a 12 1. 5 Fe I 4. 58 1218

8090.464 15 1. 9 w,N Atm H2OCN

CN

R 3 R 11 Q 9

211

3,1

3,1

26

12

12

8091.082 |2| 0. 2 Atm H2O R2 211 26

8091.50 |3i 0. 4 CN P 30 2,0 12

327
The Solar Spectrum—Continued

WavC"

length

(A)

Equivalent Width

AX

(mA)

Recluced Width

AX/X

CF)

Spot Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8092.00 a 4 0. 5 CN R 5 3,1 12 8107.32 9 1. 1 0

8092.640 38 4. 7 w Cu I 3. 82 6 8107.842S 20 2. 5 Atm H2O R7 211 26

8093.04 5 0. 6 CN Q 37 2,0 12 8108.312 11 1. 4 Fe I 2. 73 265

8093.232

8093.76

8093.937

66

1

25

8. 2

0. 1

2. 9

W,N

w

llSii V 1? Atm H2O?

Co I

5. 86

1. 05

P 9

4. 02

34

30 013

189

26

8109.018

8109.65 a

8109.840

7

2

8

0. 9

0. 2

1. 0

Atm H2O

CN

CNCN

R 5 R 20 Q 8 R 23

310

3,1

3,1 3 1

26

12

12

12

8094.270 12 1. 5 Atm H2O P2 112 26 8110.090 7 0. 9 CN Q 14 3,1 12

8094.836 6 0. 7 0? 8110.568 13 1. 6 Atm H2O R7 211 26

8095.352 2. 5 0. 3 Atm H2O Q 2 112 26 8111.01 2 0. 2 Atm?

8096.02

8096.580S

8096.874

8097.524

8098.00 a

8098.746

12

16

36To

4

114

1. 5

2. 0

4. 0

1. 2

0. 5

14. 1

u

u

IV, N

CN

CN

Atm H2O

Fe I -CN

CN

liMgi

Atm H2O

Q38

R 15 P 3

4. 07 Q 11 R 16

5. 94

0 4

2,0

3,1

112

999

3,1

3,1

41 112

1212

26

12

12

26

8111.85

8112.179

8112.406

8113.28 a

8113.631

8113.948

8114.21 a

3

18

16

3

22

27

4

0. 4

2. 2

2. 0

0. 4

2. 7

3. 3

0. 5

CN

Fe I Atm H2O

CN

Atm H2O

Atm H2O

CN

Q9

2. 69 R3

R 21 R 8 R 7 0 10

3,1

265

211

3 1

211

211

3 1

12

26

12

26

26

12

8098.90

8099.418

8099.75 a

6

1161

4

0. 8

2. 0

0. 5

CN

Atm

CN

P 7

R 1

3,1

3 1

12

12

8114.69

8114.890

\ 35

J

4. 3 w

u

f 0

I CN

CN

Q 39 fQ 15 \R 24

2,0

3^1 3 1

12

J 8100.43 4 0. 5 CN R 17 3,1 12 811.5.70 a 2. 5 0. 3 CN R 48 2,0 12

8100.90 a 3 0. 4 CN R 21 3,1 12 8115.931 4 0. 5 s CN P33 2,0 12

8101.09 12 5 0. 3 8116.38 a 2. 5 0. 3 Co I 4. 02

8101.382

8101.86

8102.285

10

1. 5

6

1. 2

0. 2

0. 7

Atm

Atm?

CN P 31 2 0 12

8116.94 a

8117.301

161

5

0. 7

0. 6

V I—

CN

CNCN

1 08 Q 11 R 22 P 5

30

3,1

3,1 30,11

12

12

12

8103. 165S 9 1. 1 Atm H2O Q 3 112 26 8118.105 6 0. 7 Atm H2O P2 112 26

8103.764 8 1. 0 CN Q 38 2,0 12 8118.446 2 0. 2 Atm H2O R 10 211 26

8103.95 a 3 0. 4 CN R 47 2,0 12 8118.72 a 3. 5 0. 4 CN Q40 2,0 12

8104.14 a

8104.709

8105.25 a

8105.69

4

8

1. 5

5

0. 5

1. 0

0. 2

0. 6

CN

CN

Atm H2O

CN

CN

CN

P8

P 32 R 8 R 2 Q 13 0 5

3,1 2,0

211

3,1

3,1

3,1

12

12

26

12

12

12

8118.910S

8119.70

8119.992

8120.661

11

4

8

14

1. 4

0. 5

1. 0

1. 7

g

Atm H2O

CN

Atm

CN

CN

Atm HoO

P 4 0 16

Q 12 R 25 R 6

112

3 1

3,1 3 1

211

26

12

12

12

26

olUo.yo/ 1 f; 1. 0 n o U. ^ 8121). 95 a i A 1 U. 1 ^AT TJ 1 1 P 11 3,1 8106.385 5 0. 6 Atm H2O P 3 112 26 8121.248 6 0. 7 Atm H2O R 7 211 26

8106.708 8 1. 0 CN Q 6 3,1 12 8121.499 14 1. 7 Atm H2O R 6 211 26

8107.12 8 1. 0 CN Q 39 2,0 12 8122.22 3 0. 4 CN R 48 2,0 12

328
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8122.576 15 1. 8 Atm liaO Atm H2O

Atm H2O

Atm H2O

Atm?-

-CN

Atm ii2'-'

CN

/R 0 \P2

R 9 R 3 R 6

P 33

JX 0

T> OA Q40

211

112

211

310

211

2,0

2,0

}26 8139.718S 22 2. 7 Atm JI2O R 9 211 2G

8122.820

8123.316

8123.579

8124.289

8125.054

Q1 OA 997

10

10

7

1

19

1991

1. 2

1. 2

0. 9

0. 1

2. 4

9 7

1. 0

u,N

s,N

s

26

26

26

12

ZD

1 912

8140.674

8140.82 a

8141.936

8142.761

8143.56

8143.794

8144.193

8144.515

135

22

|152|

7

7

65

30

20

16. 6

2. 7

18. 7

0. 9

0. 9

8. 0

3. 7

2. 5

Atm IIjO

Atm H2O

Atm H2O

CN

Atm H2O

Atm

Atm

|Atm H2O

R 0 R 5 R 5 Q 42 P 4

fR 5 \R 7

211

211

211

2,0

112

131

131

20

26

26

12

26

|26

8126.48 5 0. 6 Fe I? 4. 58 1218 Vi 1. 04 30

8126.852 23 2. 8 Atm H2O R 8 211 26 8144.76 5 0. 6 CN Q 18 3,1 12

8127.130

8127.70 a

8127.94

8129.35

8130.01

8130.460

8131.00

9

1. 5

4

4

22

51

7

1. 1

0. 2

0. 5

0. 5

2. 7

6. 3

0. 9

s,N

Atm H2O

CN

CN

CN

CN

Fe I p

Atm H2O

Atm

Atm H2O

CNCN

P 5 P 12 R49

P 34 P8

2. 76 P5

R 6 Q 15 R 25

112

3,1

2,0

2,0

3,1 265

112

211

3,1

3,1

26

12

12

12

12

26

26

12

12

8145.478

8146.213S

8146.67

8147.188S

8147.55 a

8147.80 a

8148.078

8148.392

8149.269

18

83

15

|96|

6

5

48

145

55

2. 2

10. 2

1. 8

11. 8

0. 7

0. 6

5. 9

18. 8

6. 8

s Fei

Atm H2O

CN

Fe I p Atm

CN

Atm?

Atm H2O

Atm H2O

R 5 P 12

3. 27

R 28

R 7 R 7

310

3,1 623

3,1

211

211

26

12

12

26

26

8131.213

8131.38

24

7

3. 0

0. 9

Atm H2O

CN

Atm H2O

R7

R 27 P 3

211

3,1 112

26

1226

8149.58 a

8149.689

16

140

2. 0

17. 2

Fe I

Atm H2O

r4. 58 14 58 fR 4

L-tt 0

1217

1218

211

91 1 )26

J 8131.709 1. 5 0. 2

U. 0

Atm H2O

Atm

R 12

13 K

sr 0

211 26

9A 8149.876 63 7. 7 Atm H2O R4 211 26

01 QQ r\A 1 A 1 sV*. T ZjT I u. oy 8150.05 a 4 0. 5 CN fQ 42 2,0 }12

8133.209S 24 3. 0 Atm H3O ) ri 0 \R7

91 1 211 |26Q1 KC\ KA 0 01 I CN

0. Di R 30 9n

3,1 12

8133.564 13 1. 6 Atm H3O R 11 211 26 8151.336 3 0.

0?

8133.777 94 11. 6 Atm H2O R 5 211 26 8151.95 1 0.

Co I 4. 07 193

8134.520 7 0. 9 Atm H2O R 2 211 26 8152.498 142 17. 4 Atm H2O fR 1 \R 4 211

211 j26

8135.047

8136.207

8136.525

8137.149

8137.47

8137.974

76

17

25

|10|

3

5

9. 4

2. 1

3. 1

1. 2

0. 4

0. 6

s

s

Atm H2O

Atm H2O

Atm H2O

Atm H2O

CNCN

R 5 R 10 R 5 R 5 R 28 Q41

211

211

211

211

3,1

2,0

26

26

26

26

12

12

8153.06

8153.703

8154.409

8154.63 a

8154.70 a

8154.90 a

16

99

. 240

2. 0

12. 2

5. 4

27. 5

6. 7

1. 0

CN

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Si I

P 36 R 4 R 3 R 6 R 6

6. 10

2,0 211

310

211

211

12

26

26

26

26

8138.777 16 2. 0 Atm H3O R 6 230 26

329
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8155.22 7 0. 9 Atra CN — CN

0 22 Q 43

3,1 2,0 12

12

8169.386S

8169.995

114

309

13. 9

37. 8

Atm H2O

Atm H2O

R3

;q6

\R 4

211

211

211

26

)26

J 8155.467 13 1. 6 Atm

o? 8170.75 a 1 0. 1 CN P 16 3 1 12

8155 85 3 0. 4 Atm H2O P 3 112 26 8171.239 23 2. 8 Si I 6. 10

8156.13 a 1. 5 0. 2 8171.647 6 0. 7 Atm H2O P 4 112 26

8156.51 1 0. 1 Atm H2O? Q 9 211 26 8172.00 2 0. 2 CN R 52 2 0 12

8156.854 8 1. 0 Atm H2O P 3 112 26 8172.36 2. 5 0. 3 CN R 33 3,1 12

8157.57 1. 5 0. 2 CN R 31 3,1 12 8172.80 a 2 0. 2

8158.019 205 25. 2 Atm H2O R 4 211 26 8173.008 12 1. 5 Atm H2O R 1 310 26

8158.84

8159.15

2. 5

9

0. 3

1. 1 s,N

0 —

Atm H2O

Mgi

CN

Q 4

5. 93 R 51

211

2 0

26

12

8173.36

8173.754

8174.12

3

10

7

0. 4

1. 2

0. 9

Atm H2O

CN

Q 6 Q 23

211

3 1

26

12

8159.38 a 1. 5 0. 2 8174.678 31 3, 8 Atm H2O Q 5 211 26

8159.60 a 1 0. 1 8175.12 6 0. 7 CN Q 44 2 0 12

8159 88 a 1 0. 1 8175.72 2 0. 2 Atm?

8160 16 2 0. 2 CN R 30 3,1 12 8176.20 a 4 0. 5

8160.78 1. 5 0. 2 8176.32 4 0. 5

8160.98 0. 5 0. 1 S,N Vi 1. 06 30 8176.975 350 42. 8 Atm H2O R 3 211 26

8161.434 239 29. 3 Atm H2O R 5 211 26 8177.40 a 9 1. 2

8161.972

8162.35

oi CO om

8163.02

8163.776

116

257

y

8

7

14. 2

31. 5

1. i

1. 0

0. 9

s,N

Atm H2O

Atm H2O

Atm rl2U Atm

Cri

Atm

R 5 R 3

4. 39

211

211

298

26

26

8177.60 a

8177.932S

8178.491S

8179.056

8179.48

3. 5

190

104

190

?

0. 4

23. 3

12. 7

23. 3

0. 6

CN

Atm H2O

Atm H2O

Atm H2O

(Fei)

Siip

fP 17 IP 19 R 2 R 2 R 3

4. 31

5. 86

3,1

3,1

211

211

211 1136

33

}-

26

26

26

8164.157 16 2. 0 Atm H2O rR4

IR6

131

131 j26 8179.913 16 2. 0 Atm H2O Q4 211 26

8164.54 350 42. 8 Atm H2O fR 3 \R 3 211 211 j26

8180.23 4 0. 5 CN R34 3,1 12

8165.337S

8165.79

8166.06

8166.450

8166.75

52

3

2

151

|3|

6. 4

0. 4

0. 2

0. 6

0. 4

Atm H2O

CN

CN

Atm H2O

Cr I?

R 3 R 52 P 37 P 6

4. 41

211

2 0

2 0

112

299

26

12

12

26

8180.878

8181.273

8181.848S

8182.25

8182.48

6

6

219

10

8

0. 7

0. 7

26. 8

1. 2

1. 0

CN

CN

Atm H2O

Atm H2O

Atm

0

Q24

Q45

R2

Q5

3,1

2,0

211

310

12

12

26

26

8166.88 a 2 0. 2 CN R 31 3,1 12 8183.12 19 2. 3 Atm H2O Q 3 211 26

OlD/.lOO D U. i Atra a Zj. U JNa I 0 1 A 4

8167.660

8168.107

8168.820

6

8

163

0. 7

1. 0

20. 0

CN

CN

Atm HjO

Q22

Q44

R4

3,1

2,0 211

12

12

26

8184.207

8184.50

8

5

1. 0

0. 6

0

Atm H2O

CN

Q 2 Q 26

211

3,1

26

12

330
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Ec|ui- valent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

EP

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8184.78

8185.34

8

3

1. 0

0. 4

Atm

CN

CN

P 18 R 53

3,1

2,0

12

12

8202.94

8203.230

3

5

0. 4

0. 6 0?

V I? CN

Si I?

3. 13 Q 27 3,1 12

8185.67 3 0. 4 Cr I? 4. 41 299 8203.48 a 1. 5 0. 2 CN P 22 3,1 12

8186.371 193 23. 6 Atm H2O R 2 211 26 8204.09 4 0. 5 ,S Fe I p 0. 91 12

8186.791

8187.852

|50|

12

6. 1

1. 5

s Fe I (Vi)

II Atm H2O

N I

4. 91

1. 05 Q 5

10. 32

127230

211

2 26

8204.827

8204.95

8205.31

21

14

3

2. 6

1. 7

0. 4

Atm H2O

Fei

CN

Q6

0. 96 R 36

211

12

3,1

20

12

8188.11

8188.38 a

8189.272

8190.83

8191.02

8192.069

13

2

359

4

3. 5

3

1. 6

0. 2

43. 9

0. 5

0. 4

0. 4

s,N CNCN

CN

Atm H2O

Atm H2O

Atm H2O

Q 25 Q 45 R 35 R 2

R 2 P 4

3,1 2,0

3,1

211

310

112

12

12

12

26

26

26

8205.67

8206.785

8207.04

8207.749S

8208.15

8208.56

2

4

2

64

1. 5

|5|

0. 2

0. 5

0. 2

8.4

0. 2

0. 6

s

CN

Atm

CN

Fe I CN

CN —

Co I

R 37

P 40

4. 44 P 21 Q 47

4. 24

3,1

2,0

1136

3,1

2,0 193

12

12

12

12

8192.24 4 0. 5 CN P 19 3,1 12 8209.559 38 4. 6 Atm H2O Q3 211 26

8192.55 3 0. 4 CN Q 27 3,1 12 8209.85 6 0. 7 Mgi 5. 75

8193.113 290 35. 4 Atm H2O R 1 211 26 8210.321 22 2. 7 Atm H2O R 0 310 26

8193.738 4 0. 5 Atm H2O Q 7 211 26 8210.96 a 1. 5 0. 2 N I? 10. 33 2

8194.233 1 0. 1 Atm 8211.151 |3. 5| 0. 4 Atm H2O P 5 112 26

8194.836S

8195.452

304

4

S4. S

0. 5

S,N Nai

(Na i)

Si I? CN

2. 10

2. 10

5. 96 Q 26

4

4

3,1 12

8211.32 a

8211.57

8212.132S

2

1

93

0. 2

0. 1

11. 3

CN

Si I Atm H2O

Q28

5. 61 R 0

3,1

19

211

12

26

8196.51 5 0. 6 Fe I 4. 59 1217 8212.55 2. 5 0. 3 <S? Zr I 0. 65 40

8196.96

8197.704

5

320

0. 6

39. 1

CN

CN

Atm H2O

R 35 R 36 R 1

3,1 3,1

211

12

12

26

8213.041

8213.85

157

10

17. 3

1. 2

w,N

s,N

Mg I Atm H2OMg II?

5. 75 Q 3

9. 99

28 310

7 26

8198.278 8 1. 0 8214.413 18 2. 2 Atm H2O Q 5 211 26

8198.98

8199.49

129

0. 5

15. 8

0. 1

S IIFei Atm H2O

Vi

Atm

4. 43 Q 4

1. 04

1154

21130

26

8214.71

8215.155

6

35

0. 7

4. 2

0? w,NCN

llSii CN — CN

R 38

6. 26 P 40 Q47

3,1

2,0

2,0

12

12

12

8199.989 69 8. 4 Atm II2O R 1 310 26 8215.798 8 1. 0 0

8200.694S 138 16. 9 Atm H2O R 1 211 26 8216.303 7 0. 9 0 Ni 10. 33 2

8200.99 8 1. 0 CN Q 28 3,1 12 8216.975 2 0. 2 Atm

8201.20 1. 5 0. 2 CN P 39 2,0 12 8218.114S 180 21. 9 Atm H2O Q2 211 26

8201.57

8201.695

10

42

1. 2

5. 1 w

Atm

(CN)

Atm

jCa n

Q 46

7. 50

2,0

13

12 8218.51

8219.710

8220.388

6

5

221

0. 7

0. 6

25. 8 s

-CN

CN

Fe I

Q30

Q29

4. 32

3,1

3,1

1130

12

12

8202.14 2 0. 2 8221. 553S 112 13. 6 Atm H2O Q4 211 26

331
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

oolar

Identification

Low

thtr or

itot. Line

RMT

iNO. or

V ID. Band

Notes

8222.24 1 0. 1 CN P 24 3,1 12

8222.70 2 0. 2 CN Q48 2,0 12

8222.88 5 0. 6 Atm H2O Q 1 310 26

1

0

iz

oZZo.xv a i. O U. Z JN I in 00 iU. 00 0

loo lb. Z Atm A ^-»^ TT r\ 112<J Q 1 oil ocZO

OZZ4.4DU oo Z. t Atm rl2^ H ^ oil Zl 1 Oft ZD OOO /I o o i U. 1 Jr^t 1 1 0 TO z. / z

8225.124 3 0. 4 Atm?

8225.688S 88 10. 7 Atm H2O Q3 211 26

Qoo^; f\ciO oZzo.yoZ o4/ /I O O Atm XI2U y 2oil Zi 1 26 0007 OQA

8228.32

8228.761

1 CiP. iyo

463

218

OQ Q

56. 2

26. 5 J

Atm H2O

I Atm H2O

Atm XI2'-' I Atm H2O

0 Q 3 Q 3 H 4 Q 2

oil Zl 1 211

211

oil Zl L 211

.26

8228.86 20 2. 4 Atm H2O Q 6 211 26

8229.27 5 0. 6 CN rP 41 IQ 48

2,0

2,0 }12

1/0 Atm XI2U H 4

oil zl 1 ocZ6 OOOn AQCi. ooZZ O ^7 Atm XI2U Q 5 211 26

ozoU.oo 1 oIz 1. 6 bl I 5. 62 19 QOQ oZo oy. y Atm A +rT^ TT r\ ±i2U oil zl 1 26

8231.703 197 24. 0 Atm H2O Q 5 211 26

8232.319 91 10. 8 s Fe I 4. 41 1136

8233.906S 213 25. 9 Atm H2O Q 3 211 26

OZO'i.DZoO OO D. 4 Atm JI2V-' (Mg II) Q 6

10. 00

211

7 26

8235.34 2. 5 0. 3 Ca I? 4. 45

8235.81 9 1. 1 Cr I Atm A tiiij TT ^

4. 40

Q 7 298

211 26

8236.121 29 3. 5 Atm H2O Q 7 211 26 OOQ7 yu 10. y Atm H2U Q 5 211 26

8238.538 6 0. 7 Atm H2O Q 8 211 26 Q090 1 QOQ dy 4. 6 s r e 1 2. 42 108

d4 A J. TT Atm H2U Q 2 211 26 8240.379 3 0. 4 Atm H2O Q 8 211 26 8241.277 1 0. 1 Atm H2O Q 8 211 26 8241.60 m Vi 1. 05 30 13 8241.765 3. 5 0. 4 s? CN R 40 3,1 12 8242.14 a 1. 5 0. 2 CN P 26 3,1 12 8242.365 18 2. 2 Atm H2O Q7 211 26

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

oolar

Identification

Low

EP

or Rot. Line

RMT AT ^ No.

or

Vib. Band

Notes

8242.50 a 11 1. 3 N I 10. 33 2 00^0 1 OA 8243.130 66 A f\ 4. U Atm H2O Q 4 211 26

Oct A 0 A 00 8243.488 278 33. 8 Atm H2O T> 1 P 1 211 26

8z44.05 A4 0. 0 Atm

CN fP 25 \R 41

3,1

3,1 }l2

J

oci A c c ori 8246. DZy 9 1. 1 Atm H2O Q 6 211 26

OCi A 0 01 8246.81 6 0. 7

AT CN Q 32 3,1 12

8247.307 0 A n0. 7 CN Q 33 3,1 Iz 00 /I 0 c 8247.85 1 0. 1 Atm

8248.137S 81 a 3 w Fe I 4. 37 1136

8248.802S 98 11. 3 W Ca II 7. 51 13

8249.620 5 0. 6 Atm

8250.38 |3| 0. 4 Atm

8250. yy 5

A £? 0. fa AT CN P 43 2,0 12 00 cr 1 COG 8251. o3o 5 0. 6

/I AT CN R 41 3,1 12

8252.02 8 1. 0 CN Q50 2,0 12

8252.727S 104 12. 6 Atm H2O Q3 211 26

00 C 0 C(\ n\ 8zoo,dU m CI AT b,N \7 T V I1 AO

1. 08 OA30 1 0 lo

8253.81 4 0. 5

/~1 AT CN

Fei?p

P 26

4. 58

3,1 1216

12

8254.32 2 0. 2 CN

Fe I p

R 42

3. 05

3,1 508

12

A col 8254.681 0 A 24 0 C\ 2. 9

TXT w Ca II 7. 51 13

8255.57 4 0. 5 0?

8256.00 0. 5 0. 1 S,N V I 1. 06 30

8256.515 294 35. 6 Atm II2O P 2 211 26

8257.283 8 1. 0

8257.51 8 1. 0 CN Q 34 3,1 12

8257.860 14 1. 7 Atm H2O P 2 310 26

8258.40 4 0. 5 CN Q 50 2,0 12

8258.72 2 0. 2 CN P 43 2,0 12

8259. 692S |130| 15. 8 Atm H2O P 2 211 26

8260.355 11 1. 3 Atm H2O Q 7 211 26

8260.79 3 0. 4 Atm?

8261.00 1. 5 0. 2 Atm

8261.849 6 0. 7 Atm

8262.733 4 0. 5 Atm

8263.445S 107 12. 9 Atm H2O P2 211 26

332
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8263.850 32 3. 9 u Fei 4. 95 1272

8264.276 26 3. 1 0? Fe I 5. 10 1332

8264.642 6 0. 7 Atm H2O Q2 310 26

8264.969 9 1. 1 Atm H2O Q3 310 26

8265.69 1. 5 0. 2 0?

8266.433 11 1. 3 s CNCNP 44 Q34

2,0

3,1 12

12

8267.118 6 0. 7 u CN Q 51 2,0 12

8268.073 12 1. 4 CN Q 35 3,1 12

8268.47 3 0. 4 Atm

8268.83 4 0. 5 Atm

10

8269.186 19 2. 3 |Atm H2O Q 4 211 26

8269.32 a 5 0. 6 Co I 5. 15

8269.644 16 1. 9 w Fe I 4. 59 1218

8270.16 1 0. 1 0

8272.G42S 124 15. 0 Atm H2O P 3 211 26

8272.47 8 1. 0 CN R 43 3,1 12

8273.076 15 1. 8 Atm H2O Q' 2 211 26

8273.475 10 1. 2 s CN Q 51 2,0 12

8274.354 296 35. 8 Atm H2O

(Fei)

P 3

5. 07

211 133226

8275.553 4 0. 5 Atm H2O Q 6 211 26

8275.899 36 4. 3 w Fe I 4. 95 1270

8276.54 76 9. 2 Atm H2O P 3 211 26

8276.69 118 14. 3 Atm H2O P 3 310 26

8278.19 2 0. 2

8278.710 19 2. 3 u Atm HjO

CN

Q' 3 Q 36

211

3,1 26

12

8279.600S 203 24. 5 Atm H2O P 3 211 26

8282.024 311 37. 6 Atm H2O P 3 211 26

8282.67 4 0. 5 CN Q 52 2,0 12

8283.06 2 0. 2 Atm?

8283.42 |2.5| 0. 3 Atm?-

CN R 44 3,1 12

8284.53 6 0. 7 Atm

8285.17 14 1. 7 |CN

Atm

P 29 3,1 12

8285.40 a 2 0. 2

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8285.71 4 0. 5 CN P 30 3,1 12

8286.17 3 0. 4 Atm

8287.233 18 2. 2 Atm

8287.50 6 0. 7 Atm H2O

CN

Q 3 fQ 36 \R45

310

3,1

3,1

26

8287.940 290 35. 0 Atm H2O P 4 211 26

8288.221 23 2. 8 Atm H2O Q 5 211 26

8288.63 1. 5 0. 2

8288.955 9 1. 1 s CN Q 52 2,0 12

8289.535 140 16. 9 Atm H2O P 4 211 26

8290.01 9 1. 1 CN Q 37 3,1 12

8290.45 2. 5 0. 3

8290.98 1. 5 0. 2

8291.229 6 0. 7 Atm H2O R 4 131 26

8292.07 2 0. 2 CN Q8 4,2 12

8292.806 15 1. 8 w |o Atm H2O Q4 310 26

8293.52 52 6. 5 s Fei 3. 30 623

8294.160 193 23. 3 Atm H2O P 4 211 26

8294.541 106 12. 8 Atm H2O P 4 211 26

8295.299 39 4. 7 Atm H2O P 4 211 26

8295.668 11 1. 3 Atm H2O Q 7 211 26

8296.028 15 1. 8 Atm H2O Q 4 310 26

8296.562 5 0. 6 Atm

10

8297.37 1. 5 0. 2 CN P 31 3,1 12

8297.65 4 0. 5 Cr I?-

Si I?

4. 41

6. 12 297

8298.066 7 0. 8 Atm H2O Q 5 310 26

8298.454 12 1. 4 CNCN

Q 37 Q 53

3,1 2,0 12

12

8298.973 7 0. 8 Atm HjOCN

P 4 R 46 310

3,1 26

12

8299.45 1 0. 1 Atm

8299.985 12 1. 4 Fe I 5. 07 1331

8300.408S |170| 20. 5 Atm H2O fP 4 \P 4

211

211 |26

8301.49 5 0. 6 0 CN Q38 3,1 12 8302.681 1. 5 0. 2 8303.17 3 0. 4 Fe I p Cn?

2. 73

2. 71 265

57

333
The Solar Spectrum—Continued

Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.I

or Vib. Band

Notes

8303.39 10 1. 2 Mgi 5. 93 8320.90 a 4 0. 5 CN Q 54 2,0 12

8303.65 a 1. 5 0. 2 CN? R 16 4,2 12 8321.242 168 20. 2 Atm H2O P 6 211 26

8304.300S 89 10. 7 Atm H2O P5 211 26 8321.587 190 22. 8 Atm H2O fP5

\P 6 211

211 |26

8305.092

8305.617

8306.20

8306.699

8307.12

8307.54 m

8307.603

213

31

4

6

1

15

25. 7

3. 7

0. 5

0. 7

0. 1

1. 8

0

s

s

Atm H2O

Mgi

Zr I?-

CN

Til?

Atm

(Sir)

Atm?

Til

Atm H2O

Fe I p

P 5

5. 93

0. 62 R 46

3. 44

5. 61

0. 83 P 5

0. 99

211

40

3,1

19

33

310

12

26

12

13

26

8322.527

8322.924

8323.42

8324.142

8324.608

8324.99

8325.450

8325.737

5

4

3

8

10

3

5

2

0. 6

0. 5

0. 4

1. 0

1. 2

0. 4

0. 6

0. 2

e?

CN

0

Atm

10

Cai

CN

Atm H2O

R 48

4. 53 Q 40 P 4

3,1

3,1 310

12

12

26

8308.670 3 0. 4 Atm H2O Q 6 211 26 8326.03 a 1. 5 0. 2

8309.39 2. 5 0. 3 CN P 32 3,1 12 8326.316 13 1. 6 Atm H2O P' 3 211 26

8309.71 8 1. 0 CN Q 38 3,1 12 8326.68 2 0. 2 Atm

8310.115 30 3. 6

1

> w,d

Atm H2O P 5 310 26 8327.061S 193 S4. 0 5 Fe I 2. 20 60

8310.252 60 7. 2 Mgi 5. 93 8328.474 12 1. 4 Atm H2O P 6 211 26

8310.829 19 2. 3 Atm H2O Q' 6 211 26 8328.950 17 2. 1 0? G

8311.28 11 1. 3 8329.254 12 1. 4 Atm I-I2O Q 7 211 26

8311.767 29 3. 5 w |Atm H2O

0

Atm H2O

P 5 211 26 8329.682S 125 1. 5 Atm H2O P 6 211 26

8311.956S 97 11. 7 rP5

\P 5 211211 |26

nOQA OA oooU.Zo c0

12

n R U. D

1. 4 ^i. Atmtill PToO R 4

3,1

131

1LZ

26

8312.44

8312.874

7

4

0. 8

0. 5 Atm H2O P3 310 26

8331.20 4 0. 5 CN

Atm H2O

P 48 P 6

2,0

310

1226

8313.301 5 0. 6 CN Q39 3,1 12 8331.432 12 1. 4 CN fQ 55 \P 33

2,0 3 1 )l2

J 8313.873 30 3. 6 Atm H2O P5 211 26 8331.926 130 16. 1 Fe I 4. 39 1153

8314.45 2 0. 2 0? CN P47 2,0 12 8332.145 35 4. 2 Atm H2O P 6 211 26

QQ-\A 77 0 U. D OAT H 54 2,0 8332.55 a 10 1. 2 ooiO.O / Q i. 1 Atm 8332.726 11 1. 3 Atm H2O P 6 211 26

QO-i c 097 1. 0 Atm XI2V/ f\' R 01

1

8332.88 8 1. 0 WyN

Atm

oo inn iU. u Atm ±i2U r 0 OR

U. U U. 1 8333.584S |58| 7. 0 Atm H2O P 6 211 26

8317.394 4 0. 5 Si I 5. 61 19 8333.891 9 1. 1 Atm

8318.139 172 20. 7 Atm H2O P 5 211 26 8334.20 a 6 0. 7

8319.36 3 0. 4 CN P 32 3,1 12 000^.00 ux 1

1

1. 3 Sito Ti T 0. 82 33

8319.90 a 1. 5 0. 2 8334.50 a 22 2. 6 Atm H2O R 5 131 26

8320.183 7 0. 8 0 8335.150 114 13. 7 0 Ci 7. 68 10

8320.443 8 1. 0 CN R 62 2,0 12 8335.508 40 4. 8 Atm H2O P 6 211 26

334
The Solar Spectrum—CoTitiruicd

Wavelength

(A)

Equivalent Width

A\

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8335.80 a

8336.108

8336.236

8336.98

o O OT OA 8o37.c54

3

9

18

0. 5

7

0. 4

1. 1

2. 2

0. 1

0. 8

w

Atra H2O

0?

CN —

CN

P 7

Q 18 Q 55 ;Q 41 IQ 15

4. 53

310

4,2

2,0

26

12

12

8352.43

8353.123

8353.55

8353.642

3

9

9

12

30

0. 4

1. 1

1. 1

1. 4

4. 3

S

CN

Ca I Atm

Ti I Atm IIjO

Atm H2O

CN

Atra II2O

Q 18

4. 53

0. 81 P 7 P 7

4,2

33

211

310

12

26

26

8337.916 7 0. 8 CN

Cai?

3,1 4,2 8354.36

8354.723

6

18

0. 7

2. 2

Q 56 P 7

2,0

211

12

26 OOOO O /I o 8oo8.o4o

8338.666

8338.902

19

28

28

2. 3

3. 4

3. 4

CN

Si I Atm H3O

Atm H2O

P 48

5. 86 P 6 P 7

2,0 33

211

211

12

26

26

8355.15

8355.36

8356.02

1. 5

1. 5

4

0. 2

0. 2

0. 5

Fe I p CN

CN

Fe I p

4. 10 P 49 R 28

4. 29

1050

2,0

4,2 1117

1

12

8339.034 111 13. 3 Atm H2O P 7 211 26 8356.37 4. 5 0. 5 CN Q 21 4,2 12

8339.413 109 13. 1 w Fei 4. 43 1153 8356.70 a 3 0. 4 CN P 35 3,1 12

8340.500 8 1. 0 w? Ni I p 3. 80 139 8357.040S 72 8. 6 Atm H2O P 8 211 26

8341.443 7 0. 8 Atm H2O P 3 211 26 8357.441 29 3. 5 Atm H2O P 8 211 26

8341.874 11 1. 3 Atra H2O P 3 211 26 8357.873 17 2. 0 0? -CN Q 19 4,2 12

8342.290S

8342.866

8343.33

8343.716

8343.932

8344.765

50

19

1. 5

7

7

2

6. 0

2. 3

0. 2

0. 8

0. 8

0. 2

w

0

Atm H2O

(Feip)

Fei

CN

Atra H2O

Atra

P6

2. 95

4. 99 Q 19

P7

211 401

1270

4,2

131

26

12

26

8358.504

8359.542

8360.795

8362.000

8362. 302B

8362.56

21

15

50

35

45

5

2. 5

1. 8

6. 1

4. 2

5. 4

0. 6

u,N

u

Fei

Atm H2O

Fe I Atm H2O

Atra H2O

CN2. 99 R 4

4. 47 P 7 P 7 /R 51 \R 29

401

131

1153

211

211

3,1 4,2

26

26

26 y8345.19 |4| 0. 5 Fe I p 2. 69 265 8363.254 2 0. 2 CN Q 4,2 12

8345.73 1 0. 1 CN Q41 3,1 12 8363.58 m S Ti I p 2. 09 182 13

8346.131

8346.39

8347.326

146

1. 5

13

16. 1

0. 2

1. 6

wl,N

s

Mg I

Atra CN

Atm H2O

5. 94

Q 17 P 7

40

4,2 310

1226

8363.8o7

8384.243

8364.948

7

16

1. 5

0. 8

1. 9

0. 2

S

CN

CN

Ti I 0?

Q 43 Q 20

0. 84

3,1 4,2

33

12

12

8347.829

8348.304

8349.02 m

8349.162S

4

12

57

0. 5

1. 4

6. 8

w

S

c

/b

Atra H2O

Cri

Fe I p Atm H2O

P 7

2. 71

0. 91 P 7

310

50

12

211

26

13

26

8305.640

8366.022

8366.542

8367.022

8367.331S

51

3

10

3

51

6. 7

0. 4

1. 2

0. 4

6. 1

u Fe I Atm

Atm H2O

Atm H2O

Atm H2O

3. 25

P 8 P 8 P 8

623

211

131

211

26

26

26 8349.383 29 3. 5 Atm H2O fP 7 \P7

211

211 |26 8369.06 0. 5 0. 1 Atm H2O R 4 131 26

8349.77

8349.964

8350.733

8352.18

2

3

4

1. 5

0. 2

0. 3

0. 5

0. 2

W

CN

Atm H2O

CN

Atm

Q20

R4

Q42

4,2

131

3,1

12

26

12

8369.25

8369.77

8369.858

2

5

5

0. 2

0. 6

0. 6

CNCN

Atm H2O

CN

Fe I p

R 51 R 30 R 7 P 36

4. 91

3,1 4,2

131

0,1 1271

1212

26

12

335
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

8370.472 5 0. 6 Atm H2O P 8 230 26 8385.48 13 1. 6 u Atm H2O

0?

Atm

CN

R 5 131 26

8370.802

8371.457

1. 5

5

0. 2

0. 6

Atm H2O

CNCN

P 8 Q 43 Q 57

211

3,1 2,0

26

1212

8385.63

8385.95 a

5

2

0. 6

0. 2 Q25 4,2 12

8372.177 8 1. 0 Atm H2O P 9 131 26 8386.182 4 0. 5 Atm H2O P 9 211 26

8372.55 a 2 0. 2 8386.35 m s Tiip 2. 10 182 13

8372.777

8373.236

8373.711

8373.95 a

8374.27 a

8374.546

11

4

43

8

4

10

1. 3

0. 5

5. 1

1. 0

0. 5

1. 2

CN

Co I Atm

Atm B.2O Cai

CN

Atm H2O

P 50

4. 07

P 8

4. 44 P 37 Q 4

2,0 193

211

3,1

131

12

26

12

26

8386.53

8386.933

8387.782

8388.328

8389.19

8389.521

3

9

170

10

4

6

0. 4

1. 1

£0. 8

1. 2

0. 5

0. 7

s

S

CN

Atm H2O

Fe 1 CN

CN

IITii Zri

P 19 P 9

2. 18 P 38 Q 58

2. 09

0. 60

4,2

211

60

3,1

2,0

18240

12

26

12

12

8374.80 a 1 0. 1 8390.459 7 0. 8 CN rP51

IQ24

2,0

4,2 }-

8375.35 a

8375.713

8376.187

8376.381S

8376.594

8376.90

8377.160

8377.39

8377.870

8378.25

8379.37

8381.440

8382.217

8382.541

1. 5

5

12

38

9

4

16

4

25

8

1. 5

8

8

29

0. 2

0. 6

1. 4

4. 5

1. 1

0. 5

1. 9

0. 5

3. 2

1. 0

0. 2

1. 0

1. 0

3. 5

0S

S

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Atm H2O

CNTi I

AtmHoO

Co I Atm H2O

Fe I p

Ti I

R 6 Q 5 P 9 Q 6

P 9 Q 44

0. 83

P8

4. 21 P8

0. 99

0. 82

131

131

211

131

211

3,1

33

211

193

211

12

33

26

26

26

26

26

12

26

26

8391.185

8393.72 a

8394.020S

8394.518

8394.882

8395.134

8396.900

8397.152S

8397.635

8397.99

8398.481

8399.12

8399.947

4. 5

2

18

4

|41

12

23

15

4

2. 5

4

4

9

0. 5

0. 2

2. 2

0. 5

0. 4

1. 4

2. 8

1. 8

0. 5

0. 3

0. 5

0. 5

1. 1

S

CN

Atm H2O

Atm H2O

Atm H2O

Atm H2O

Fei?

Til

Atm H2O

Atm H2O

CN

Sii?p

CN

|Atm H2O

Fei?

Q45

P 9 R4

P 5 R4

0. 81 P 10 P 10 Q 25

5. 61 Q45

P9

3,1

211

131

211

131

33

211

211

4,218

3,1

211

12

26

26

26

26

26

26

12

12

26

8382.781 23 2. 8 s Til 0. 81 33 8400.640 8 1. 0 Atm H2O R2 131 26

8383.302 7 0. 8 CN fQ 58

LQ 23

2,0

3,1 4,2

8401.15 a

8401.401

2

25

0. 2

3. 0 s Fei 2. 48 108

oooo. uo 0. 5 0. 1 CN P 51 2 0 12 g 1. 1 Fg I p 4. 44 1136

8383.861

8384.170

7

17

0. 8

2. 0

Atm H2O

Atm II2O

P 5 R 3310

131

26

26

8402.629 5 0. 6 s Ti I |CN

2. 25 fP 39 IQ 27224

3,1 4,2

8384.40 a 1. 5 0. 2 8403.001 2. 5 0. 3 Atm H2O P 9 211 26

8384.831

8385.03 a

|7|

1. 5

0. 8

0. 2

Atm H2O

CN

R 5 Q44

131

3,1 26

12 8404.182

8404.382

6

11

0. 7

1. 3 u,N

Atm H2O R 3 131 26

8404.73 1. 5 0. 2 CN R 54 3,1 12

336
The Solar Spectrum—Continued

Wave-

\A)

Equivalent Width

AX

KUXA)

Re- duced

Width

AX/X

Spot

Solar

Tr) pn f.i- fication

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

WaveEquivalent Width

AX vmA;

Re- duced

Widtli AX/X

Kb)

Spot

Solar

Tflpn t.i- fication

Low

E P

or Rot. Line

RMT

No.

or Vib. BandNotes

8405.374 |22| 2. 6 Atm H2O R 3 131 26 8424.44 0. 4 ,s Ti I 2. 10 182

8405.665 11 1. 3 Atm H2O P 10 211 26 8425.62 2 0. 2 CN Q 00 2,0 12

8407.257 6 0. 7 CN Q 59 2,0 12 8425.889 5 0. 6 Fe I p 1. 01 12

8408.229 10 1. 2 Atm H2O P 9 211 26 8426.126 6 0. 7 CN R 37 4,2 12

8408.550 10 1. 2 Atm H2O Q 3 131 20 8426.514S 43 5. 1 Ti I 0. 83 33

8408.755 26 3. 1 Atm H2O Q 3 131 26 8426.997 10 1. 2 CN- Q47 3,1 12

8409.585 12 1. 4 Atm H2O Q4 131 26 8427.769 2 0. 2 Atm H2O R 1 131 26

8409.88 a 2 0. 2 Mn I? 5. 13 8428.107 1 0. 1 Atm H2O P 11 211 26

8410.12 a 3 0. 4 CN? P 20 4,2 12 8429.595 4 0. 4 Atm H2O Q 4 131 26

8410.43 1 0. 1 8429.967 3 0. 4 CN Q 30 4,2 12

8411.127 4 0. 5 Atm H2O Q4 131 26 8430.798 18 2. 1 Atm H2O Rl 131 26

8411.36

8411.62

8412.356

8413.33

8414.084

8414.59

8415.450

84.1 fi 89 n

84.1 fi 0*^4

841 7 999

5

3

44

4

12

1

37

4

5

15

0. 6

0. 4

6. 0

0. 5

1. 4

0. 1

4. 4

0. 4

0. 6

1. 8

s,NN

S

u,d

g

CNCN

0

Til

Atm?

Zr I Fe I p —

Atm H2O

Atm?

Atm H2O

CN

Ti I

|Ni I Atm H2O

P 39 Q 28

0. 82

0. 69

4. 47 P 10

R 2 R 36

2. 24

3 83 R 2

3,1 4,2

33

40

1154

211

131

4 9

224

156

131

12

12

26

26

12

26

8431.236

8432.389

8433.23

8434.509

8434.968S

8435.28

8435.655

8436.376

8437.232

8437.462

8437.96

8438.054

6

3

2

15

57

4

52

18

4

5

5

0. 7

0. 4

0. 2

1. 8

6. 8

0. 4

6. 3

2. 1

0. 4

0. 6

0. 6

w

S

S

u,N

CN

CN

CN

Fe I

Ti I

Si I

Ti I Atm H2O

0?

0?

H I Atm H2O

Q29

P41

P24

5. 01

0. 85

4. 93

0. 84 Q2

12. 08 Q2

4,2

3,1

4,2

1270

33

8

33

131

10

131

12

12

12

26

31

26

8417.51 m S,N Til 2. 12 182 13 8438.64 3. 5 0. 4 CN Q61 2,0 12

8417.96 1 0. 1 Si I 5. 62 18 8438.920 11 1. 3 S Til 2. 25 224

8418.408 9 1. 1 Atm H2O R 1 131 26 8439.581S 79 9. 1 u Fe I 4. 55 1172

8418.639 9 1. 1 Atm H2O P 11 211 26 8440.02 2 0. 2

8419.292 18 2. 1 w,N 0 8440.40 2 0. 2 CN Q 30 4,2 12

8419.59

8419.872

8420.496

1. 5

7

6

0. 2

0. 8

0. 7 u,d

CN

CN

CN

R 55 Q 47 Q 29

3,1

3,1

4,2

12

12

12

8440.751

8441.480

8441.765

|7|

4

4

0. 8

0. 4

0. 4

|Atm H2O

CN

CN

Atm H2O

Til

Si I

Si I Atm H2O

P 12 P41

Q48

Q3

2. 25

5. 87

5. 87 Q2

211

3,1

3,1

131 210

46

46

131

26

12

12

26

13

26

8421.443 10 1. 2

8422.06

8422.923

8423.14

1

21

13

0. 1

n 9

Z. 0

1. 5

u

SI

0?

r e I

Ti I Cai?

n 98

A "i A

i. 14

1. 88

4. 45

4 9

yyy

150

1 9

8442.476

8443.00 m

8443.975

8444.377

8444.783

11

32

3

3

1. 3

3. 8

0. 4

0. 4

s

0

8424.139 32 3. 7 0 Fei 4. 95 1272 8445.278 1. 5 0. 2 CN R39 4,2 12

337
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes Wavelength

(1)

Equivalent Width

AX

(ml)

Re- duced

Width

AX/X

^F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8445.729

8446.359

8446.741

4

|74|

50

0. 4

8. A

5. 0

W

0

O?

Oi

0 I (Fei)

Oi

(Feip)

9. 52

9. 52

4. 99

9. 52

4. 91

4

4 1272

4 1267

8468.418S

8468.839

8469.20

8469.892

128

10

7

3

15. 1

1. 2

0. 8

0. 4

S, Fei

(Ti I) Mg I Atm H2O

CN

2. 22

1. 89

5. 93 Q 2 Q 33

60 150

131

4,2

26

12

8447.34 1 0. 1 Fe I p 4. 91 1266 8470.377 6 0. 7 G?

8447.678

8448.60

8450.022

8450.247

8450.880

8452.086

4

1 U

4

8

5

0. 4

0. 1

1. 3

0. 4

0. 9

0. 6

s

u,N

sS

Fe I p —

CN

Atm H2O

CN

Cr I Til

S I Atm HoO

0. 96

P 42 P 12 Q 49

2. 71

2. 25

8. 04

12

3,1

211

3,1

56

224

14

131

12

26

12

26

8470.949

8471.28

8471.744S

8472.399 QA70 aaQ

8474.12 a 8474 362

4

0. 5 44

8

1

1

1

4

0. 4

0. 1

6. 2

0. 9

1. 0

0. 1

0. 4

w

0

CN

Atm?

Fe I CN

Mg I

Atm

Q34

4. 95

Q 50

0. yo

4,2

1270

3,1

12

12

8453.661 7 0. 8 w,N 8476.35 1 0. 1 CN P 28 4,2 12

8455.295 4 0. 4 S Cri 2. 71 56 8476.69 1 0. 1 CN R42 4,2 12

8456.01 11.51 0. 2 CN P 42 3,1 12 8477.127 5 0. 6

8456.945

8457.15

5

2.5

0. 6

0. 3 S

Atm

CN

Ti I

Q 49

1. 75

3,1

141

12 8477.54

8477.999

1. 5

6

0. 2

0. 7 oi

CN

0

Atm H2O

Q63

P4

2,0

131

12

26

8457.88 2.5 0. 3 8478.456 3 0. 4 CN P56 2,0 12

8458.70 1 0. 1 CN P 55 2,0 12 8478.890 3. 5 0. 4 Atm H2O P4 131 26

8458.99 4 0. 4 Fe I p 4. 99 1270 8479.67 2 0. 2 CN P44 3,1 12

8459.734

8460.245

8461.472

3.5

24

3

0. 4

2. 8

0. 4

CN

Atm H2O

Fe I p —

Si I

Q 32 Qi

3. 60

5. 96

4,2

131

814

12

26

8479.864

8480.18 a

8480.42 a

13

2

2. 5

1. 5

0. 2

0. 3

w,N CN

Atm H2O

CN

R43

P 1

Q34

4,2 131

4,2

1226

12

8462.39 4 0. 4 0? 8480.636 16 1. 9 V) Fe I p 4. 99 1272

8462.90 1 0. 1 Atm H2O Q 5 131 26 8481.22 0. 5 0. 1

8463.539 4 0. 4 CN P 43 3,1 12 8481.60 2. 5 0. 3 CN Q 51 3,1 12

8464.03 1.5 0. 2 Fe I p 5. 07 1330 8481.986 22 2. 6 u Fei 4. 19 999

8464.69 m s Zn 0. 65 40 13 8482.412 3 0. 4 Atm HjO Q 3 131 26

8465.173 7 0. 8 Fe I p 5. 01 1270 8482.876 4 0. 4 Atm

0

CN

|Tii

8465.634

8466.102

|41

5

0. 4

0. 6

CN

Fe I p

Q 50

4. 99

3,1 1269

12

8483.16 4. 5 0. 5 s,N Q 63

1. 87

2,0 150

12

8466.510

8467.158

8467.26

8

4

0. 9

0. 4 S

MgiFg I p Til

H I

5. 93

4. 1 4.

2. 12

12. 08

QQQ

182

10 31

8483.447

8486.914

8487.62

10

13

1. 5

1. 2

1. 5

0. 2

Atm H2O

CN

P2

P44

131

3,1

26

12

8467.734 3? 0. 4? 0? 8487.92 7 0. 8 CN fP 28

IP 29

4,2

4,2 }i2

338
The Solar Spectrum—^Continued

Wavelength

(A)

Equivalent Wiutn

AX

(ml)

Re- duced

Vv lutu A\/\

(F)

opot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(1)

Equivalent wmtn

AX

(ml)

Re- duced

Wicitn AX/X

(F)

Spot

Solar mentification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8488.306 8 0. 9 Atm HjO P 3 131 26 8514. 082S 108 12. 9 .s Fei 2. 20 60

8491.291

8491.735

o ^ no on

3

13

lU

Z. 0

1

0. 4

1. 5

1 o 1. z n o

1 o

1. 0 w

CN

Atm H2O

bl I

Fe I p Atm H2O

Q 35 P3

0. 00 y 3d

A n c 4. 95 P 2

4,2

131

4,2

1269

131

12

26

1

iz

26

8514.63

8515.122S

8515.63

8516.007

8516.75

4

79

1. 5

6

0. 5

0. 4

8. 9

0. 2

0. 7

0. 1

u

CN

Si 1? p Fei

AtmlijOQ 53

5. 61

3. 02

P 6

3,118

401

131

12

26

8494.44 m S Til 1. 74 141 13 8517.295 |11| 1. 3 CN- Q 38 4,2 12

8495.73 2 0. 2 8518.011 6 0. 7 S Ti I 2. 13 182

8496.075 3 0. 4 S ITiiCN

/2. 25

\3. 70?

P 45

209 313

3,1 12

8518.397

8519.10

21

3

2. 5

0. 4

s Til

Fe I p

1. 88

4. 95

150

1267

8496.483

8490. yy4

8498.062

5

O A o4

1470

0. 7

uS

Atm H2O

Fe I p

r e I Ca II

P2

4. 41

4. Dl

1. 69

131 1136

1 1 'TO 117/

2

26 8519.640

8520.73

8521.219

8522.01

19

1. 5

|4.5|

2

2. 2

0. 2

0. 5

0. 2

s,N

Atm H2O

CN

CNCN

P 4 P 46 Q 53 R 61

131

3,1

3,1

3,1

26

12

12

12

8499.326 7 1. 1 0 CN- /P 29 IR44

4,2

4,2 }- 8522.99 ? 0. 7 s,NN CN- P 31 4,2 12

8499.883

8500.330

8501.553

8501.803

8502.228

8502.49

8502.50 a

8502.76

8503.145

8503.54

8503.966

8504.536

8505.112

6

1. 5

34

17

50

5

4

12

3

4

5

6

0. 7

0. 2

4.0

2. 1

(5. 6

0. 6

0. 4

1. 4

0. 4

0. 4

0. 6

0. 7

w

0?W

Atm H2O

0

Si I Ni I

Si I (Hi)

CN

Atm H2O

CN

CN

CN

P5

5. 87

3. 85

5. 87

12. 08 Q 36

P 3

P 45 Q 52 Q 37

131

47

18646

10

4,2

131

3,1

3,1

4,2

26

31

12

26

12

12

12

8523.46

8524.72

8525.008

8525.50

8525.72

8525.97 a

8526.32

8526.676S

8526.994

qf;97 QA'7

8529.90

2

3

13

3

4. 5

3

7

58

10

1 1 1 1

4

0. 2

0. 4

1. 5

0. 4

0. 5

0. 4

0. 8

7. S

1. 2

1 Q X. 0

U. '1

0. 4

w

s

w

CN

CN

Zni0?

Cai

CN

Atm H2O

Fe 1 Atm

x e I p

Atm H2O

/Q 65 IR 46 P 32

2. 41

4. 43 Q 38 P 4

4. 91

c; no

r\ on ^ oy

P4

2,0 4,2

4,2

4,2

131

1270

1izo7n/ U

131

12

12

26

1 0

26

8505.852 |12| 1. 4 Atm H2O P 4 131 26 8530.17 3 0.

CN P 47 3,1 12

8509.65

8510.253

8510.92

8511.912

8512.97

4

8

1. 5

28

on

3

0. 4

0. 9

0. 2

3. 3 o c

Z. D

0. 4

Fe I p

Si I CN

Atm II2U Atm riz^J CN

Fe I p

4. 37

6. 18 P 30

"D 0 r 3

T> 0 r 6 P 46

3. 02?

1136

4,2

131

1 0

131

3,1 462

12

OA

OA

12

8531.51

8531.71

8533.34

8534.781

8535.50

8536.163

4

4

1

6

2

58

0. 4

0.

0.

0. 7

0. 2

(?. e

s,d

5?

w

Ti IAtm

CN

CN

Atm H2O

0?

Si I

1. 73

Q 54 R 62 P 5

6. 18

141

3,1

3,1

131

80

12

12

26

8513.26 3 0. 4 AtmHaO- P 4 131 26 8536.45 a 3 0. 4

8513.45 2 0. 2 0? 8536.68 3 0. 4 Atm

761-925—66-^24 339
The Solar Spectrum—Continued

Wavelength.

(A)

Equivalent

Wirl + Vi VV IQT/n AX

Re- duced w iQin

AX/X

(F)

opOT' Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib.

IN 0 oes

8538.021 |31| S. 7 w Fe I 4. 91 1266

O coo OK n z V/iN y oy A 0

4,2 O CO O '77

U. 0 U. 1 s y 00 0 n z,u IZ

o c on o

O

i U. 1 oo Til

T? AO

2. 24 209

1 0

8539.888 3. 5 0. 6 Atm HoO P 6 131 26

8540.817 8 0. 9 Atra H2O P 5 131 26

8542.144 3670 S98 s Ca II L 70 2

8545.38 (Hi) 12. 08 10 31

8546.222 5 0. 6 Atra H2O P 5 131 26

8547.19 1. 5 0. 2 Atm

804/. /

4

O. 0 U. 0

"Pr AQ45 Q 1 1 0iZ

Qt^AQ n7Q oo

n Q u. y

eo 111 1I. Q701 lOU OKAQ C AO U. o

o AT' PAT Cri

xt I0

2. 71

A 05611 0z

8549.188 3 0. 4 CN Q55 3,1 12

8549.74 1. 5 0. 2

8550.366 9 1. 1 w Siip 6. 22 88

8550.52 m Til 1. 75 141 13

8550.85 a 5 0. 6 CN Q40 4,2 12

8553.762 9 1. 0 Atm H2O P 6 131 26

8554.271 3. 5 0. 4

8555.000 7 0. 8 Atm H2O — P 6 131 26

8555.569 7 0. 8 s |Cr I CN

2. 71

J y 00 IQ41

56

Q 1 3,1 4,2 }12

8555.96 a 4 0. 5 Si I? 5. 61 18

8556.32 2 0. 2 Atm H2O P 6 131 26

8556.797S 134 15. 1 W,N Si I 5. 87 45

8558.563 3 0. 4

o c c A nc 1 8559. Uol 7 U. &

O C CO 7 C 1 c0 U. D

o cen AO o U. Z J? e I CN

K no 0. UZ Q 671 Q01 ioZi

2,0 12

8560.639 3 0. 4

8561.05 2 0. 2 CN P 34 4,2 12

8561.61 7 0. 8 0

8562.109 16 1. 9 wl Fe I 4. 47 1153

8562.365 5 0. 6

8563.83 1. 5 0. 2 CN Q 41 4,2 12

Wavelength

(A)

Equivalent

"ITT"; j + v, Wiatxi AX

(ml)

Re- duced

W idtn AX/X

(F)

Spot

Solar

T 1 J.

• Identification

Low

E P

or Rot. Line

RMT

No.

or Vib. Band

Notes

8564.62 1. 0

ri 0 U. 2 CN P 35 4,2 12 8565.456 1. 5 0. 2 s Ti I CN

1. 74 Q 67 141

2,0 12

8567. 043 3 0. 4 CN Q 56 3,1 12

8567. 776 7 0. 8 Fe I p 4. 91 1269

8568. 724 ^ 0. 4 Atm

8569. 02 1. 5 0. 2 CN Q 42 4,2 12

8569. 25 a 1 0. 1 CN? R 64 3,0 12

8569. 67 1 0. 1 s Til 2. 23 209

8571. 08 3 0. 4

8571. 328 6 0. 7 Siip 6. 19

8571. 807S 36 4. 2 W Fe I 5. 01 1272

8572. 55 a 4 0. 4

8573. 141 9 1. 0 Atm H2O P 7 131 26

8573. 47 1 niU 1 0 1. z U,J\

8573. 96 2 0. 2

8574. 538 7 0. 8 s,N CN

Co I P 352. 70

4,2 12

8575. 268 7 o 0

U. 0 CN —

Co I R 642. 79

3,1 12

8575. 75 5 0. 6 CN R 50 4,2 12

8576. 48 2.

5

0. 3 Fe I p 4. 59 1215

8577. 19 2.

5

0. 3 CN Q 42 4,2 12

8578. 43 m s Til 1. 73 141 13

8579. 08 4 0. 4 Si I 5. 98 56

8581. 76 2 0. 2 CN? Q 68 2,0 12

8582. 271S 86 9. 4 s Fe I 2. 99 401

8582.857 8 0. 9 CN Q 43 4,2 12

8583.310 22 2. 6 S Cai 4. 44

8584.09 2. 5 0. 3 CN P 50 3,1 12

8584.791 5 0. 6 Fe I p 5. 01 1270

8585.27 2 0. 2 CN Q 57 3,1 12

8585.577 13 1. 5 0? S I

8586.211 11 1. 3 w Nii?p 5. 45 296

8586.64 1 0. 1 Co I? 4. 15

8586.90 0. 5 0. 1 Atm

8587.04 2. 5 0. 3 CN Q 68 2,0 12

8587.93 2 0. 2 CN R 65 3,1 12

8588.34 5 0. 6 CN P 36 4,2 12

340
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8589.59 10 1. 2 -Co I? 4. 15 193

8590.327 3 0. 4

8590.86 a 2. 5 0. 3 CN Q 43 4,2 12

8591.191 3 0. 4

S591.54 6 0. 7 CN Q 57 3,1 12

«592.119 3 0. 4 Fe I p 5. 01 1269

8592.969 |48| 6. 1 w Fe I 4. 95 1267

8595.968S 54 6. 5 w,N Si I 6. 19 80

S597.059 |36| 4. 2 w,N Si I 6. 19 80

8598.17 1 0. 1 S Ti I 2. 27 236

8598.39 H I 12. 08 9 31

«598.836S 54 6. 6 w Fei 4. 39 1153

8601.03 2 0. 2 S Ti I ri. 73

\2. 25

141 209

8602.18 |4| 0. 4 O?

^602.77 8 0. 9 S CarTi I? p

4. 44

2. 49

8603.82 9 1. 0 u CN Q 58 3,1 12

8604.92 2 0. 2 CN Q 44 4,2 12

8605.74 1. 5 0. 2 Atm?

^606.00 9 1. 0 0 Si I 5. 95 55

8606.383 8 0. 9 0? Ni I 5. 28 275

8607.075 19 2. 2 w Fe I p 5. 01 1272

«607.78 3 0. 4 s O

8608.337 12 1. 4 w O

^608.98 m s 13

8610.10 4 0. 4 CN Q 58 3,1 12

8610.609 26 S. 6 w Fe I p 4. 43 1153

8611.11 m s 13

8611.812S 99 11. 7 s Fe I 2. 84 339

8612.90 m s,N Ti I 1. 74 141 13

8613.9468 33 4. 2 W Fe I p 4. 99 1272

8615.314 8 0. 9 u,N O

.8616.284S 42 6. 3 w Fe I 4. 91 1266

8616.99 4 0. 4 -CN P 38 4,2 12

.8618.41 |2| 0. 2 s,N Til 2. 24 209

8619.10 8 0. 9 u,N

8619.45 7 0. 8 u,N CN- Q45 4,2 12 8621.618 75 9. 0 s Fe I 2. 95 401

Wavelength

(A)

Equivalent Width

AX (mA)

Re- duced

Width

AX/X

(F)

Spot

oolar

Idonti- ncation

Low

h, tr or Rot. Line

RMT

JNo. or

VlD. Band

Notes

8622.05 2. 5 0. 3 CN r 5Z .3,

1 o

8622.753 17 2. 0 w,N o

8623.738 A4 0. 4

8624.46 2 0. 2 Atm?

8626.26 a 5 0. 6 CN R67 3,0 12

8626.59 5 0. 6 CN Q46 4,2 12

8629.16 7 0. 8 N I 10. 69 H 59

8

3,1 1 o

8631.25 3 0. 4

8631.92 3 0. 4 CJN

K d7 3,1 1 O

8632.424 15 1. 7 w Fe I p

y1 1 A 4. lU iUoU

8633.10 7 0. 8 0

8633.956 17 2. 0 s Oa I 4. 40

8634.16 5 0. D y 4D 1 9

8636.26 1 0. 1 JO s,df KjV I /. / I 00

8637.003 13 1. 5 w Nil 3. 85 186

OC A t f\ A « 8641.94 a 2 0. I (c^ 4/ 1 9

8642.35 a 2 0. 2

D < O Art 8643.00

8643.35

3

3

0. 4

0. 4 J

i^r I Fe I p

O 71 Z. / i

4. yi

DO

1 OAl

8646.358 9 1. 0 0 bl I

8647.88 7 0. 8 o?

("1 A 4 ^0(~1 8648.472S 161 18. 7 W bl I

ft OA

8650.91 3 0. 4 Atm?

8652.475 6 0. 7 Fe I p 4. 10 iUOU

8654.04 3. 5 0. 4 O !

8654.436 9 1. 0 w Fe I p

O QA

8655.20 2 0. 2

8656.672 9 1. 0 w re I K AO

8657.57

3 0. 4 OAT9 y 48 1 9

8658.94 a 1 0. 1

8661.97 40 11. 6 s? I'e I O OO ft A

8662.170 2600 297 w Ca n 1. 69 2

oooo*

RD 0

Fg I p 4. 99 1270

8664.90 a 1 0. 1 CN Q 48 4,2 12

8665.02 (Hi) 12. 08 9 31 8667.366 8 0. 9 u Fe I? p—

Si I

2. 45

5. 96 16655

8668.07 a 2 0. 2

341
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

(mA)

Reduced. Width

Zaa/ a

(F)

Spot

ooiar

Identification

Low

Hi IT or

XVO t. Line

RMT

XNMr.0. or

V ID. Band

Notes

ODD0.40D y 1. u u

OO/U./U QO u. y 0 I 7 HP, 0

oc'rn AO'? 1 o 1. 4 0 OC7 1 o no 50/ l.oUo cD ID I 7 SR D

oo/l.o/y 1. 0 If Fe I p 0. yjij 1 979

OD /4. / 00C3 I/O S

TP121 T -T e I 9 ooy

1 Qla /. 1 11

1

1 n7 Do

8675.88 6 0. 7

8677.12 2. 5 0. 3

Qo u. y 0 I 7 S7 p.0

o0/y.D4D 41 4. / W ] r e I p —

S I

•i. yo

7. 87

1 9RR

6

8680.097 19 2. 2 0 Si IIn I

5. 86

lU. 00 1

ODSU.4UO 9 0 0 Q I 7 Q7 u

y 1. J Fe I p

A 1 0 4. iy y y y

3 U. 4 p f^p; ir 00 6,L 1

9

8682.45 3 0. 4 CN Q G2 3,1 12

8682.987 12 1. 4 s Ti I 1. 05 68

8D00.084 oO n n u. y w TS.T T iN I iU. 00 11

BDOO.ODS 0'± 0, 0 vv 01 I p (Ni)

0. 10. 32 OUSin1

8686.75 7 0. 8 S,N Feip r3. 88

1^4. yy 956

i^Dy

9 r\ 0 U. Z 0 I

8687.49 5 0. 6 Slip 6. 20 80

000/ .yu 4 u. 4 QGQQ CiAO 0000.04^ c AT r e I 9 1 Qio fin

oooy./u a ocon oo ^ oooy.oo a

QO

11U|

n 0 U. y

1. 1

1

I tv,N

J

Fe I p

I* e I p

0. uo

in 0. iU

i^n7

icS.jU

oDyZ,o4Z PI u. 0

e0 111 i. uo Do

obyo.io oo u. 4 Q T 0 I 7 Q7 D

o c no n K

o

oDyo.yoo 1 r 0 0 I 7 Q7 D

8094.041 o4 0. y 0

C3 T b I 7 07 /. 0/ 0

8d96.45 a 1. c

f\ 0 u. z

8697.20 a 11.5 0. 2 CN Q 50 4,2 12

8698.717 20 2.

3

u Fe I p 2. 99 400

8699.461S 73 5.

0

W Fe I 4. 95 1267

8700.314 4 0.

4

0? Fe I p 4. 95 1266

^Wavelength

(A)

Equivalent Width

AA

(ml)

Re- duced

Width

A \ /\ llA/ A

(F)

Spot

DOiar

Identification

Low

TP iJ or

rtot. Line

RMT

AT^or

VlD. Band

Notes

Q7nn QAQ 0 i uu.y4y 0 A U. 0 w,N Mn I A A'i 4. 4o A C\ 4y

8701.15 a 2. 5 1

8701.73 2 0. 2 CN? Q74 2,0 12

8702.510 9 1. 0 Nil 2. 74 83

8703.15 8 0. 9 CN-

\r T iN I Q63

1 n '39 iU. oZ

3,1

11 12

Q7nQ 7^ 0 / Uo. / 0 9Q Z. 0

^, AT U,l\ Mn I 4. 4c> 4y

1. 0 n 9 T> AADO 0 n

o/Uo.lo 0

C\ A U. 0

0 ( UO.UOO c0

fl A U. 0

r\ 9

o/UD.oy CS. 0 U. 4 <cj oi 4,2 1 0

07A7 Q1 7 U. 0 (^r I 9 71 00 Q7n7 OA 9 b (^U/ .y4^ c0 n A U. D K^V I 4. oy jyo

c 7Afi 9Q 4

0 /I U. 4

8710.21 21 2. 5 5. 93

8710.398 82 10. 4 w Fei 4. 91 1267

8711.671 4. 5 0. 5 Ni 10. 33 1

8712.701 57 5. 9 W Mg I 5. 93

8713.208S 58 6. 6 u Fei f2. 95

\ A OQ

l_4. yy 400

IZO/

C 7 1 0 K A r> 0/ io.oD aQ n A

U. 4 0710 00 Q0

O /I U. 4 y 01 /I 0 1 0IZ 07 1 G CO Q

U. 4 Atm '.

8717.833S 105 W,N Mgi 5. 93

8718.76 5 0. 6 N I 10. 33 1

8719.66 m S Ti I 1. 74 140 13

8724.13 3 0. 4 CN- Q 52 H 644,2

3,1 12

1 0

070 C 01 A 8725.210 A4 U. 4

9

8725.95 2 0. 2 Ti I? 1. 73 139

8727.19 4 0. 4 Fe I p 4. 19 999

8728.024 107 11. 6 0 Si I 6. 18 79

8728.604 16 1. 8 0 Si I

/ \T T \ 6. 18inlU. 66 79

1

8/29.171 9 K

Z. 0 u Fe I p 6. 41 71 Q

8729.35 a

pr r\ A

(J. D bl I p D. lo

8730.22 3 0. 4 0?

8734.74 0. 4 S Ti I 1. 05 68

8736.040 289 W,N Mgi 5. 94 39

8737.40 4 0. 4 u Mn I 4. 43 49

342
The Solar Spectrum—Continued

Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes Wavelength

(A)

Equivalent Width

AX

(mA)

Re- duced

Width

AX/X

(F)

Spot

Solar

Identification

Low

E P

or Rot. Line

RMT

No.

or

Vib. Band

Notes

8738.76 1. 5 0. 2 Atm? 8751.198 14 1. 6 0? Si I 5. 87 44

8739.50 1. 5 0. 2 Atm? 8752.025 94 11. 8 W,N Si I 5. 87 43

8740.68 a 7 0. 8 8753.11 2 0. 2 C I 9. 00

8741.00 a 7 0. 8 Mn I 4. 43 49 8755.75 6 0. 7 O

8741.68

8742.466

8743.53

8745.34

8745.81

8747.438S

2

97

4

3

3

16

0. 2

11. 3

0. 4

0. 4

0. 4

1. 8

W,N

CN

Pi?

Si I O?

CN?

CN?

Fei

(Ni)

Q 53

7. 96

5. 87

P 58 Q 65

3. 02

10. 33

4,2

44

3,1

3,1

401

1

12

12

12

8757.199

8758.466

8759.72 a

8763.978

8764.94

91

1

0. 5

99

2

10. 0

0. 1

0. 1

6

0. 2

s

u

Fei

Atm H2O

CN

Fe I

Si ir p

2. 84

R' 8 Q 54 4 65

6. 22

339

003

4,2

1172

26

12

wt

8766.417

8766.68

13

5

1. 5

0. 6

w

S

Si I Til5. 96

1. 07

54

68

8747.85 2. 5 0. 3 8767.05 3 0. 4

8750.48

8750.57 1 0. 1

n I CN?12. 08 Q 759

2,0

31

12

8767.68

8770.681

3. 5

11

0. 4

1. 3 w

CN

Fe I p

Ni I

Q 66

3. 65

2. 74

3,1 814

82

12

343
Notes to the Solar Spectrum Ledger (See § 2.8)

Note

Number Designations for molecular lines in the solar spectrum; notes 1, 2, 3, 4, 6:

Spectrum

Electronic TransitionVibration

Band

Spectral Range

(A)

References for Analysis

1 OH A^s + - xm 0, 0

1 1 If 1

2, 2

3021 to 3362

oiUy I/O OoiO

3184 to 3375

G. H. Dieke and H. M. Crosswhite, The Johns Hopkins University

jjumoieDee oeries rtcporo i\o. o/, iio pp. (.ly^oj. See also C. E. Moore and H. P. Broida, J. Research Nat. Bur.

Std. 63A, 279 to 295 (1959). 2 CH + - xm 0, 0

1, 1 3086 to 3219

3119 to 3222

T. Heimer, Zeit. Phys. 78, 771 to 780 (1932).

See, also, C.E. Moore and H. P. Broida, J. Research Nat. Bur.

Std. 63A, 19 to 53 (1959). 3 CH B^s - - xm 0, 0

1, 0

1, 1

3871 to 4084

3627 to 3710

4025 to 4119

L. Gero, Zeit. Phys. 118, 27 to 36 (1941). See also, C. E. Moore and H. P. Broida, Ref. in Note 2.

4 CH A*A - xm 0, 0

1, 1

2, 2

0, 1

4133 to 4413

4185 to 4446

4238 to 4468

4726 to 4941

|l. Gero, Zeit. Phys. 118, 27 to 36 (1941).

N. H. Kiess and H. P. Broida, Astroph. J. 123, 166 to 171 (1956). See also, C. E. Moore and H. P. Broida, Ref. in Note 2.

5 Wavelength measurement by J. L. Greenstein and E. Tanbderg-Hanssen, Astroph. J. 119, 113 to 119 (1954):

Ben 3130.414 A; 3131.058 A. Be I 3321.043 A; 3321.252 A. 3321.430 A.

SpectrumElectronic Transition Vibration

Band

Spectral Range

(A)

References for Analysis

6 NH Am, - z^s- 0, 0

1, 1 3280 to 3487

3307 to 3485

R. N. Dixon, Canadian J. Phvs. 37, 1171 to 1186 (1959). G. W. Funke, Zeit. Phys. 96, 787 to 798 (1935). G. W. Funke, Zeit. Phys. 101, 104 to 112 (1936). A. Fowler and C. C. L. Gregory, Phil. Trans. Roy. Soc. London

[A] 218, 351 to 372 (1919).

Lines recorded in Rowland's Table as double, but not resolved in Atlas. For lines short of 4000 A thel adopted wavelength

is a mean of the Rowland lines weighted according to the estimated Rowland intensity. To longer waves, additional measure- ments are included in the adopted values. Some of these lines are probably single but broadened by hyperfine structure or isotope effect, cf A. Abt, Astroph. J. 115, 199 to 205 (1952).

Recorded

Pair

(A)

\

Adopted

(A)

Recorded

Pair

(A)

Adopted

(A)

Recorded

Pair

(A)

Adopted

(A)

Recorded

Pair

(A)

Adopted

(A)

3310.

3310.

3322.

3322.

3335.

3335.

3340.

3340.

3646. 3346.

3349. 3349.

3372.

3372.

3395.

3395.

3405.

3405.

913rl

923rl

927rl 987rl

168r1 219r|

332r1 391r|

728r1

772rJ

386rl 464rl

765rl

858rl

370rl 409rl

084rl

169rl

3310. 918

3322. 949

3335. 185

3340. 356

3346. 746

3349. 447

3372. 812

3395. 386

3405. 126

3413. 465r

3413. 519r

3433. 028rl 3433. 077r

3472. 544rl 3472. 594r

3502. 255r

3502. 327r

3504. 876r

3504. 917r

3547. 178r

3547. 220r

3564. 936r

3564. 989r

3575. 355r

3575. 394r

3590. 468r

3590. 510r

3413. 492

3433. 048

3472. 558

3502. 291

3504. 892

3547. 199

3564. 959

3575. 374

3590. 489

3602. 068r

3602. lllr

3630. 736rl 3630. 778r

3642. 774r

3642. 827r

3645. 290r

3645. 336r

3847. 826rl 3847. 871r

4018. 085rl 4018. 120r

4030. 729rl 4030. 798r

4052. 453rl 4052. 500r

4187. 785rl 4187. 861r

3602. 085

3630. 754

3642. 806

3645. 313

3847. 848

4018. 104

4030. 763

4052. 482

4187. 812

4526.

4526.

4535.

4535.

5457.

5457.

5782. 5782.

5790. 5791.

412rl 465rl

711r1

741r|

435rl

496r|

099rl 176ri

959r1

028rJ

4526. 442

4535. 712

5457. 474

5782. 136

5790. 990'

344
Notes to the Solar Spectrum Ledger, continued (See § 2.8)

Wavelength measurements of selected solar lines of NH, from A. Fowler and C. C. L. Gregory, Phil. Trans^Roy. Soc. London

[A] 218, 351 to 372 (1919), corrected to present scale adopted for Rowland lines.

Adopted

(A)

Rowland \ Corrected

(A) Remarks

3360. 808m

3364. 651m

3364. 735m

3381. 033m

3427. 086m

3360. 854r

3364. 697r

3381. 065r

Solar line from Higgs

Solar line from Higgs

9 The two components of this line, 4054.815 A and 4054.873 A have in the Atlas and on the plate, intensities which are clearly in the reverse order from that given by Rowland.

10 The Balmer Series of hydrogen extends through Hn. Because of the width and diffuseness of these solar^hnes, the calcu- lated laboratory wavelength is given in column one for the members of this series from Hg through H17: Hi

Calc.X

(A)

Series Member

Multiplet No.

Calc.X

(A)

Series MemberMultiplet No.

3697. 15 Hn 3750. 15 H12

3703. 86 H16 3770. 63 Hn

3711. 97 His 3 3797. 90 Hio 2

3721. 94 H,4 3835. 39 H„

3734. 37 Hl3 3889. 05 Hs

Measurement of the equivalent widths of these difEcult wide lines is described in § 2.2.

345
Notes to the Solar Spectrum Ledger, continued (See § 2.8)

Designations for molecular lines in the solar spectrum, continued; notes 11, 12:

Spectrum

Electronic TransitionVibration

Band

Wavelength

Range

(A)

References for Analysis

CN B 2S+—Z 2S+

CN

0, 0

1, 1

2, 2

3, 3 4,4

0, 1

1, 2

2, 3

3, 4

0, 0

etc

1, 0

etc.

2, 0

3, 1

4, 2

3, 0

4, 1

5, 2

6, 3

5, 1 7,3

3583 to 3883

3961 to 4216

Beyond range

} of present

publication.

7850 to 8798

8044 to 8812

8247 to 9008

6910 to 7593

7072 to 7588

7242 to 7812

7423 to 7801

6320 to 6741 6619 to 7180

H. S. Uhler and R. A. Patterson, Astroph. J. 43, 434 to 468 (1915)

{ Measurement of solar equivalent width (228mA) refers to integrated

first head of CN band, X3883.287.

T. Heurlinger, Lund Dissertation, Chapter VI, pp. I to XXIX

following p. 66 (1918).

J. Genard and J. Weinard, Ann. d' Astroph. 18, 329 to 333 (1955).

J. Weinard, Dissertation, Univ. des Saarlandes, 86 pp. (1955); Ann.

d' Astroph. 18, 334 to 353 (1955).

S. P. Davis and J. G. Phillips, Berkeley Analysis of Molecular

Spectra, Monograph 1, 1963. Referred to below as "Mono".

W. S. Benedict, Unpubl. material, 1964. M. Rigutti and F. Drago-Chiuderi, Ann. d' Astroph. 26, 253 to 262

(1963). (2, 0) and (3, 1). Mono pp. 168 to 174 and unpubl. material 1964. Mono pp. 175 to 182. Mono pp. 183 to 189. Mono pp. 129 to 134. Mono pp. 138 to 144. Mono pp. 145 to 151. Mono pp. 152 to 156. Mono pp. 99 to 104. Mono pp. 118 to 123.

Atomic lines present only in the sun-spot spectrum, based chiefly on work done by C. E. Moore in 1933 from a study of the Mount Wilson spot spectrograms.

X(A) X(A) X(A) X(A) X(A) X(A) X(A) X(A)

3900. 44 4564. 23 4784. 45 5033. 61 t5331. 98 5797. 55 6367. 92 8349. 02

4069. 84

4077. 16

4078. 89?

4116. 60

4573. 09

4575. 48

4578. 47

4581. 30

4787. 64

4851. 35

4861. 19

4862. 26

t5046. 55

t5069. 36

5070. 23

t5077. 55

15332. 14

5335. 24

5335. 36

t5335. 43

5799. 90

5807. 14

5807. 30

5813. 97

6378. 85

6381. 44

6383. 44

6401. 95?

8363. 58

8386. 35

8417. 51

8443. 00

4117. 56

4152. 36

4179. 86

4186. 84

4278. 79

4583. 90

4586. 93

4590. 55

4594. 50?

4599. 79

4862. 90

4863. 75

4881. 24

4893. 92

4895. 99

t5078. 28

5144. 64

t5158. 30

5161. 78

t5190. 19

5339. 82?

t5354. 68

15356. 43

t5356. 60

5359. 05

5879. 79

5955. 16

6032. 60

6058. 76

6077. 37

6431. 63

6452. 08

6467. 83?

6498. 75

6506. 39

8464. 69

8494. 44

8550. 52

8578. 43

8608. 98

4281. 71

4306. 18

4306. 91

4314. 36

4314. 77

4609. 97

4626. 49?

4643. 72

4643. 94

4644. 86

4900. 02?

4904. 30

4908. 45

4924. 56

t4927. 59

15194. 77

15201. 82

t5218. 09

5222. 67

t5222. 98

5361. 71

t5377. 35

t5382. 92

t5392. 06

5401. 92

6106. 78?

6106. 98

6134. 71

6192. 95

6193. 69

6527. 30

6557. 37

6563. 41

6607. 90

6637. 24

8611. 11 8612. 90

8719. 66

4368. 92

4387. 20

4393. 33

4394. 51

4397. 22

4661. 92?

4663. 28?

4679. 73

4683. 44

4684. 28

4930. 21

4937. 16

t4937. 99

t4940. 30

4941. 02

5228. 60

t5231. 52

5232. 82?

t5234. 82

5238. 52

t5403. 98

5444. 85

5465. 75

5470. 48

5481. 71

6230. 85

6241. 31?

6257. 63

6261. 23

6273. 39

6646. 20

6649. 51 6709. 87

6766. 50

7102. 89

4420. 46

4433. 97

4476. 62

4491. 18

4497. 73

4684. 50

4698. 83

4707. 69?

4714. 12

4737. 66

4941. 38

t4944. 82

t4947. 33

4947. 98

t4959. 12

t5252. 36

5273. 43

5288. 40

t5291. 60

t5294. 31

5517. 18

5535. 51

5548. 76

5597. 69

5659. 16

6276. 32

6285. 42

6295. 28

6308. 62

6339. 92

7169. 11 7213. 41

7219. 40

7439. 87

8061. 16

4511. 82

4535. 86

4541. 35

4541. 61

4563. 66

4747. 27

4747. 96

4751. 58

4757. 48

4779. 34

4967. 32

14971. 62

4973. 06

t4994. 99

t4995. 56

5311. 20

5311. 43

t5317. 89

t5323. 93

t5326. 41

5664. 26

5752. 86

5756. 40?

5785. 94

5788. 61

6342. 26

6344. 82

6359. 91

6361. 07

6367. 82

8063. 10

8066. 07

8241. 60

8253. 60

8307. 54

fRounded off wavelength measured by R. S. Richardson (unpublished) and kindly furnished to C.E.M. in 1932. Except

for one line, at 5377 A, all were measured independently by C.E.M.

346
Notes to the Solar Spectrum Ledger, continued (See § 2.8)

14

15

The observed equivalent width, (column two) relates to the combined lines 3968.492 A, (Ca ii) and 3970.076 A, (II i). The

reduced width (column three) for 3968.492 A, Ca ii (/i), has been derived by theory from 3933.682 A, Ca u (K); for 3970.076

A, (He), it has been interpolated between the other Balmer lines. The line may be double.

x(A) x(A) X(A) X(A)

3975. 051 4134. 438 5095. 176 6091. 920

3985. 789 4163. 480 5142. 530 6183. 574

3988. 332 4188. 315 5146. 776 6303. 461

4001. 940 4315. 458 5161. 764 6395. 148

4057. 957 4334. 166 5338. 333 6497. 594

4061. 733 4340. 848 5399. 479 6537. 938

4072. 888 5089. 212 5470. 636

16

17

18

Possibly a molecular line in the sun-spot spectrum.

Blend of a molecular and an atomic line in the sun-spot spectrum.

Special notes pertaining to double lines:

X(A) Remarks

3972. 440

4049. 731

4868. 414

5040. 890

5342. 504

Recorded by Rowland as two lines, but appears as single on Atlas records. Line is a close unresolved double. Line is a close unresolved double in the disk spectrum; two lines seen in the spot spectrum.

Line is an unresolved double in the disk spectrum, with separation 0.05 A (HDB); two lines seen in the spot spectrum.

Line may be a close unresolved double.

Designations for molecular lines in the solar spectrum, continued notes 19, 20, 22, 23, 24, 26.

Spectrum

Electronic Transition Vibration

Band

Wavelength

Range

(A)

References for Analysis

A ^JIi~X 3nu 0, 0

1, 1 2,2

4831 to 5165

4919 to 5129

4972 to 5097

R. C. Johnson, Phil. Trans. Roy. Soc. [A] 336, 157 to 230 (1927).

J. G. Phillips, unpublished material (Nov. 1963). Present identifications can be extended when Berkeley Monograph

on C2 has been completed.

1, 0

2, 1 4671 to 4737

4664 to 4708

0, 1

1, 2

2, 3

5501 to 5635

5499 to 5585

5475 to 5540

Mg H A 2n3/2.1/2—

0, 0 4956 to 5210 R. H. Fowler, Mon. Not. Roy. Astron. Soc. 67, 530 to 534 (1907).

Phil. Trans. Roy. Soc. [A] 209, 447 to 478 (1909). R. S. Richardson, Astroph. J. 73, 216 to 249 (1931). A. Guntsch, Zeit. Phys. 104, 585 to 591 (1936). A. Schadee, Dissertation, Utrecht (1964); Bull. Astron. Inst. Netherlands 17, 311 (1964).

19

20

347
Notes to the Solar Spectrum Ledger, continued (See § 2.8)

There are probably regions of continuous absorption from 4643 A to 4650 A; 4654 A to 4658 A; 4661 A to 4665 A; and also from: 4826 A to 4830 A; 4831 A to 4835 A. The note number appears near the strongest absorption dip in these intervals. The

extent of the absorption is indicated by a vertical dashed line in the note column.

Spectrum

Electronic Transition IsotopeVibration

Band

Wavelength

Range

(A) References for Analysis

Atm Us >S+—SS- U, U / oyo to / / OO H. D. Babcock and L. Herzberg, Astroph. J. 108, 167 to

1, 1 7684 to 7768 190 (1948).

1, 0 6867 to 6967 First line in head of B group: 6867.187 A.

2,1 6954 to 6996

2, 0 6276 to 6353 First line of a group: 6276.590 A.

3, 0 5788 to 5829

Atm Oj 016 on 0, 0 7599 to 7675 H. D. Babcock and L. Herzberg. See above. 1,0 6876 to 6920

Atm Oj QU 013 0, 0 7594 to 7684 H. D. Babcock and L. Herzberg. See above.

1,0 6885 to 6938

[O i] Brackets denote forbidden transition. Identification suggested by I. S. Bowen, Rev. Mod. Phys. 30, 109 to 112 (1948) 5577.341 A, 6300.311 A, 6363.79 A.

Unclassified "Atm" lines are probably due to HjO. They are entered as "Atm" to distinguish them from classified lines in the H2O Band System. In the present work they start at 5393 A and extend to 8739 A. Two short regions in this interval are

free from atmospheric Unes: 5478 A to 5665 A and 6093 A to 6267 A.

All lines identified as "Atm H2O" have been assigned to specific transitions in the vibration-rotation spectrum. The designations are from the detailed analysis kindly furnished in advance of publication by W. S. Benedict (Dec. 1963). These lines occur

in the range 5414 A to 8758 A. The following bands are represented in the solar table: Atm HjO

Vibration-Rotation

Band

Range

(A)

Vibration-Rotation

Band

Range

(A)

Vibration-Rotation

Band

Range

(A)

411 5414 to 5470 212 6424 to 6563 013 7846 to 8093

203 5665 to 5769 231 6565 to 6585 112 7899 to 8211

500 5701 to 5766 103 6845 to 7128 310 8084 to 8383

321 5828 to 6019 400 6903 to 7203 211 7993 to 8448

401 5830 to 5999 301 7059 to 7408 230 8138 to 8370

302 5863 to 5983 221 7099 to 7480 131 8144 to 8573

113 6275 to 6375 202 7131 to 7392 003 8758

311 6408 to 6626 320 7201 to 7358

This Band System is described by W. S. Benedict in the introduction to the Michigan Table on the infrared solar spectrum

:

See 0. Mohler, A Table of Solar Spectrum Wave Lengths, 11984 A to 25578 A, p. 9, Univ. Michigan Press, 83 pp., 1955. A fuller discussion will appear in a forthcoming Table of Identifications in the Solar Spectrum, which is based on The Photometric

Atlas of the Solar Spectrum from \7i98 <o X12016, by L. Delbouille and G. Roland, Mem. Soc. Roy. Sci. Lifege, Special

Volume 4 (1963). For the text and ledger accompanying this Atlas see J. W. Swensson, W. S. Benedict, 0. C. Mohler^

L. Delbouille and G. Roland; ibid 5, in press (1966).

348
Notes to the Solar Spectrum Ledger, continued (See § 2.8)

27 The presence of this Cai multiplet in the solar spectrum was first reported by W. Mitchell and explained by L. Goldberg,

of L. Goldberg, Harvard College Obs. Sci. Report No. 4, 22 pp (1965); W. E. Mitchell, Jr., and 0. C. Mohler, Astroph. .J. 141, 1126 to 1130 (1965). See, also, R. F. Griffin, The Obs. 84, 154 to 156 (1964).

Cai

Solar X (A) Lab. X Multiplet

Mitchell and Mohler (A) No.

6318. 61 6318. 11

6343. 71 6343. 29 53

6361. 94 1 6361. 79

* Equivalent width not measurable; multiplet rules used to determine AX and AX/X.

28 The value of AX/X in column three has been interpolated between neighboring lines of the Atm O2 band: 7601.470 A, 7602.036 A, 7612.314 A, 7623.552 A.

29 This line, 7657.606 A, remeasured from the original plate, yields an equivalent width of 113 mA, corresponding to AX/X= 14.7.

30 The measured intensities correspond to the total area of the band head, 4688.60 A to 4689.00 A.

31 For the members of the Paschen series of H having n=12 through 18, laboratory wavelengths are entered in column one. In the solar spectrum there is a background haze caused by the first of these Paschen lines.

n Lab. X

(A)

Remarks n Lab. X

(A)

Remarks

12 8750. 48 AX 220 mA; AX/X 34 16 8502. 49 masked by Can

13 8665. 02 masked by Can 17 8467. 26

14 8598. 39 18 8437. 96

15 8545. 38 masked by Ca 11

32 The equivalent width refers to the central, symmetric component of this complex line, 8071.262 A.

349

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