# Computed linear and circular polarization rates of solar spectral lines after Delbouille's atlas in the frame of the weak field theory from λ 3700 Å to λ 8800 Å

Jean-Marie Malherbe

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Jean-Marie Malherbe. Computed linear and circular polarization rates of solar spectral lines after Delbouille's atlas in the frame of the weak field theory from λ 3700 Å to λ 8800 Å. Observatoire Paris-PSL. 2024. hal-04560120

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Submitted on 26 Apr 2024

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# Computed linear and circular polarization rates of solar spectral lines after Delbouille's atlas in the frame of the weak field theory from $\lambda$ 3700 Å to $\lambda$ 8800 Å

J.-M. Malherbe, Observatoire de Paris, Université de Recherche PSL, CNRS, LESIA, Meudon, France

Email: Jean-Marie.Malherbe@obspm.fr

ORCID: https://orcid.org/0000-0002-4180-3729

## Abstract

We present in this paper a computation of the polarization rates of solar spectral lines from $\lambda$ 3000 Å to $\lambda$ 8800 Å using Delbouille's atlas (at disk centre) and the weak field theory of the Zeeman effect. Linear and circular polarization profiles and rates are calculated in the frame of this theory using equivalent Lande factors $g*$. Lines are identified by the Moore table.

## Keywords

Solar spectrum, visible, disk centre, linear polarization, circular polarization.

## Description of the spectra

We used the solar atlas of Delbouille et al (1973), from $\lambda$ 3000 Å to $\lambda$ 10000 Å (step 2 mÅ) at disk centre ($\mu$ = 1.0), taken at the Jungfraujoch station (Switzerland, a very high and dry site). We restricted the wavelength range to $\lambda$ 3700 - 8800 Å for which we have the line identification provided by the Moore table (Moore et al, 1966) and the equivalent Lande factors $g*$. We quantified the sensitivity to the Zeeman effect using the weak field theory (Landi, 1992, Stenflo, 1994). In that frame, the Stokes V and $(Q^2+U^2)^{1/2}$ profiles are given by:

for a longitudinal field (along the line of sight):

$$V(\lambda) = - \Delta\lambda_B \frac{dI}{d\lambda}$$

for a transverse field (orthogonal to the line of sight):

$$(Q(\lambda)^2 + U(\lambda)^2)^{1/2} = 1/4 \Delta\lambda_B^2 \left|\frac{d^2I}{d\lambda^2}\right|$$

where $\Delta\lambda_B = [e / (4\pi m C)] \lambda^2 g* B = 4.67 \ 10^{-13} \lambda^2 g* B$ (numerically with B in Gauss and $\lambda$ in Angström) is the Zeeman splitting (which must be small in comparison to the Doppler width of the considered line).

The circular polarization rate is $V/I$; it is maximum (in absolute value) at the inflexion points of the line profiles. The linear polarization rate is $(Q^2+U^2)^{1/2}/I$; it is maximum in the line centre.

The spectra are displayed by pages of 100 Å, each displaying bands of 10 Å. Delbouille's spectrum is shown in **black**. Intensities are normalized to the adjacent continuum $I_c$. The **blue numbers** are equivalent Lande factors $g*$. The line identification follows the convention of the Moore et al (1966) table (slash for main contributors in case of a blend, dash for blends, parenthesis for masked lines, p for predicted line, see page XVIII of their book for details). The circular polarization spectrum $V/I$ is drawn in **red**; it was calculated using the first formula above for $B = 1000 \text{ G} (10^{-4} \text{ T})$ and for $g*=1.0$; the **red vertical bars** provide the minima and the maxima of $V/I$ (located at line inflexion points) for $B = 1000 \text{ G}$ and take into account the equivalent Lande factor $g*$ of each line ($V/I$ is proportional to $g*$ and to $B$). The linear polarization spectrum $(Q^2+U^2)^{1/2}/I$ is drawn in **green**; it was computed using the second formula above for $B = 1000 \text{ G} (10^{-4} \text{ T})$ and for $g*=1.0$; the **green vertical bars**
## Computed linear and circular polarization rates of solar spectral lines after Delbouille's atlas in the frame of the weak field theory from $\lambda$ 3700 Å to $\lambda$ 8800 Å

J.-M. Malherbe, Observatoire de Paris, Université de Recherche PSL, CNRS, LESIA, Meudon, France

Email: Jean-Marie.Malherbe@obspm.fr

ORCID: https://orcid.org/0000-0002-4180-3729

## Abstract

We present in this paper a computation of the polarization rates of solar spectral lines from $\lambda$ 3000 Å to $\lambda$ 8800 Å using Delbouille's atlas (at disk centre) and the weak field theory of the Zeeman effect. Linear and circular polarization profiles and rates are calculated in the frame of this theory using equivalent Lande factors $g*$. Lines are identified by the Moore table.

## Keywords

Solar spectrum, visible, disk centre, linear polarization, circular polarization.

## Description of the spectra

We used the solar atlas of Delbouille et al (1973), from $\lambda$ 3000 Å to $\lambda$ 10000 Å (step 2 mÅ) at disk centre ($\mu$ = 1.0), taken at the Jungfraujoch station (Switzerland, a very high and dry site). We restricted the wavelength range to $\lambda$ 3700 - 8800 Å for which we have the line identification provided by the Moore table (Moore et al, 1966) and the equivalent Lande factors $g*$. We quantified the sensitivity to the Zeeman effect using the weak field theory (Landi, 1992, Stenflo, 1994). In that frame, the Stokes V and $(Q^2+U^2)^{1/2}$ profiles are given by:

for a longitudinal field (along the line of sight):

$$V(\lambda) = - \Delta\lambda_B \frac{dI}{d\lambda}$$

for a transverse field (orthogonal to the line of sight):

$$(Q(\lambda)^2 + U(\lambda)^2)^{1/2} = 1/4 \Delta\lambda_B^2 \left| \frac{d^2I}{d\lambda^2} \right|$$

where $\Delta\lambda_B = [e / (4\pi m C)] \lambda^2 g* B = 4.67 \ 10^{-13} \lambda^2 g* B$ (numerically with B in Gauss and $\lambda$ in Angström) is the Zeeman splitting (which must be small in comparison to the Doppler width of the considered line).

The circular polarization rate is $V/I$; it is maximum (in absolute value) at the inflexion points of the line profiles. The linear polarization rate is $(Q^2+U^2)^{1/2}/I$; it is maximum in the line centre.

The spectra are displayed by pages of 100 Å, each displaying bands of 10 Å. Delbouille's spectrum is shown in **black**. Intensities are normalized to the adjacent continuum $I_c$. The **blue numbers** are equivalent Lande factors $g*$. The line identification follows the convention of the Moore et al (1966) table (slash for main contributors in case of a blend, dash for blends, parenthesis for masked lines, p for predicted line, see page XVIII of their book for details). The circular polarization spectrum $V/I$ is drawn in **red**; it was calculated using the first formula above for $B = 1000 \text{ G} (10^{-4} \text{ T})$ and for $g*=1.0$; the **red vertical bars** provide the minima and the maxima of $V/I$ (located at line inflexion points) for $B = 1000 \text{ G}$ and take into account the equivalent Lande factor $g*$ of each line ($V/I$ is proportional to $g*$ and to $B$). The linear polarization spectrum $(Q^2+U^2)^{1/2}/I$ is drawn in **green**; it was computed using the second formula above for $B = 1000 \text{ G} (10^{-4} \text{ T})$ and for $g*=1.0$; the **green vertical bars**
provide the maxima of $(Q^2+U^2)^{1/2}/I$ (located at line centre) and use the equivalent Lande factor $g^*$ of each line ;
$(Q^2+U^2)^{1/2}/I$ is proportional to $g^{*2}$ and to $B^2$ and is, in general, much smaller than $V/I$. For a given magnetic field
$B$, the maximum polarization rates of $V/I$ and $(Q^2+U^2)^{1/2}/I$ can be easily deduced from the plots : just multiply by the
factors $(B/1000)$ or $(B/1000)^2$, respectively.

This PDF document is based on 2280 x 3324 pixel images and must be zoomed to see the details. Original plates
(GIF format) are available here:

<https://www.lesia.obspm.fr/perso/jean-marie-malherbe/spectrevisible/spectreZE/index.html>

The spectra are displayed below from 3700 Å to 8800 Å, by pages of 100 Å bandpass, each page showing 10 bands of 10 Å.

Wavelength intervals [λ1, λ2] (in Å), see page number :

3700-3800 : 3 / 3800-3900 : 4 / 3900-4000 : 5

4000-4100 : 6 / 4100-4200 : 7 / 4200-4300 : 8 / 4300-4400 : 9 / 4400-4500 : 10

4500-4600 : 11 / 4600-4700 : 12 / 4700-4800 : 13 / 4800-4900 : 14 / 4900-5000 : 15

5000-5100 : 16 / 5100-5200 : 17 / 5200-5300 : 18 / 5300-5400 : 19 / 5400-5500 : 20

5500-5600 : 21 / 5600-4700 : 22 / 5700-5800 : 23 / 5800-5900 : 24 / 5900-6000 : 25

6000-6100 : 26 / 6100-6200 : 27 / 6200-6300 : 28 / 6300-6400 : 29 / 6400-6500 : 30

6500-6600 : 31 / 6600-6700 : 32 / 6700-6800 : 33 / 6800-6900 : 34 / 6900-7000 : 35

7000-7100 : 36 / 7100-7200 : 37 / 7200-7300 : 38 / 7300-7400 : 39 / 7400-7500 : 40

7500-7600 : 41 / 7600-7700 : 42 / 7700-7800 : 43 / 7800-7900 : 44 / 7900-8000 : 45

8000-8100 : 46 / 8100-8200 : 47 / 8200-8300 : 48 / 8300-8400 : 49 / 8400-8500 : 50

8500-8600 : 51 / 8600-8700 : 52 / 8700-8800 : 53

References

Delbouille, L. Roland, G. and Neven, L., 1973, Atlas photometrique du spectre solaire de [lambda] 3000 a
[lambda] 10000, https://bass2000.obspm.fr/Atlas visible.pdf, also available on line at
https://bass2000.obspm.fr/solar spect.php

Landi, E., 1992, Magnetic field measurements, in Solar observations, techniques and interpretation, Sanchez,
Collados and Vasquez editors, Cambridge University Press, page 73

Moore, C., Minnaert, M., Houtgast, J., 1966, the solar spectrum 2835-8770 Å, second revision of Rowland's
preliminary table of solar spectrum wavelengths, monograph 61, US department of commerce, national bureau
of standards

Stenflo, J.O., 1994, Solar magnetic fields, Polarized radiation diagnostics, Kluwer academic publishers
provide the maxima of $(Q^2+U^2)^{1/2}/I$ (located at line centre) and use the equivalent Lande factor $g^*$ of each line ;
$(Q^2+U^2)^{1/2}/I$ is proportional to $g^{*2}$ and to $B^2$ and is, in general, much smaller than $V/I$. For a given magnetic field
$B$, the maximum polarization rates of $V/I$ and $(Q^2+U^2)^{1/2}/I$ can be easily deduced from the plots : just multiply by the
factors $(B/1000)$ or $(B/1000)^2$, respectively.

This PDF document is based on 2280 x 3324 pixel images and must be zoomed to see the details. Original plates
(GIF format) are available here:

<https://www.lesia.obspm.fr/perso/jean-marie-malherbe/spectrevisible/spectreZE/index.html>

The spectra are displayed below from 3700 Å to 8800 Å, by pages of 100 Å bandpass, each page showing 10 bands of 10 Å.

Wavelength intervals [λ1, λ2] (in Å), see page number :

3700-3800 : 3 / 3800-3900 : 4 / 3900-4000 : 5

4000-4100 : 6 / 4100-4200 : 7 / 4200-4300 : 8 / 4300-4400 : 9 / 4400-4500 : 10

4500-4600 : 11 / 4600-4700 : 12 / 4700-4800 : 13 / 4800-4900 : 14 / 4900-5000 : 15

5000-5100 : 16 / 5100-5200 : 17 / 5200-5300 : 18 / 5300-5400 : 19 / 5400-5500 : 20

5500-5600 : 21 / 5600-4700 : 22 / 5700-5800 : 23 / 5800-5900 : 24 / 5900-6000 : 25

6000-6100 : 26 / 6100-6200 : 27 / 6200-6300 : 28 / 6300-6400 : 29 / 6400-6500 : 30

6500-6600 : 31 / 6600-6700 : 32 / 6700-6800 : 33 / 6800-6900 : 34 / 6900-7000 : 35

7000-7100 : 36 / 7100-7200 : 37 / 7200-7300 : 38 / 7300-7400 : 39 / 7400-7500 : 40

7500-7600 : 41 / 7600-7700 : 42 / 7700-7800 : 43 / 7800-7900 : 44 / 7900-8000 : 45

8000-8100 : 46 / 8100-8200 : 47 / 8200-8300 : 48 / 8300-8400 : 49 / 8400-8500 : 50

8500-8600 : 51 / 8600-8700 : 52 / 8700-8800 : 53

References

Delbouille, L. Roland, G. and Neven, L., 1973, Atlas photometrique du spectre solaire de [lambda] 3000 a
[lambda] 10000, https://bass2000.obspm.fr/Atlas visible.pdf, also available on line at
https://bass2000.obspm.fr/solar spect.php

Landi, E., 1992, Magnetic field measurements, in Solar observations, techniques and interpretation, Sanchez,
Collados and Vasquez editors, Cambridge University Press, page 73

Moore, C., Minnaert, M., Houtgast, J., 1966, the solar spectrum 2835-8770 Å, second revision of Rowland's
preliminary table of solar spectrum wavelengths, monograph 61, US department of commerce, national bureau
of standards

Stenflo, J.O., 1994, Solar magnetic fields, Polarized radiation diagnostics, Kluwer academic publishers
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3700 Å to 3710 Å

<figure><img src="image_1.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3710 Å to 3720 Å

<figure><img src="image_2.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3720 Å to 3730 Å

<figure><img src="image_3.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3730 Å to 3740 Å

<figure><img src="image_4.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3740 Å to 3750 Å

<figure><img src="image_5.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3750 Å to 3760 Å

<figure><img src="image_6.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3760 Å to 3770 Å

<figure><img src="image_7.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3770 Å to 3780 Å

<figure><img src="image_8.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3780 Å to 3790 Å

<figure><img src="image_9.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3790 Å to 3800 Å

<figure><img src="image_10.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3700 Å to 3710 Å

<figure><img src="image_2.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3710 Å to 3720 Å

<figure><img src="image_3.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3720 Å to 3730 Å

<figure><img src="image_4.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3730 Å to 3740 Å

<figure><img src="image_5.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3740 Å to 3750 Å

<figure><img src="image_6.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3750 Å to 3760 Å

<figure><img src="image_7.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3760 Å to 3770 Å

<figure><img src="image_8.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3770 Å to 3780 Å

<figure><img src="image_9.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3780 Å to 3790 Å

<figure><img src="image_10.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3790 Å to 3800 Å

<figure><img src="image_11.png" /></figure>
<figure><img src="image_11.png" /></figure>

<figure><img src="image_12.png" /></figure>

<figure><img src="image_13.png" /></figure>

<figure><img src="image_14.png" /></figure>

<figure><img src="image_15.png" /></figure>

<figure><img src="image_16.png" /></figure>

<figure><img src="image_17.png" /></figure>

<figure><img src="image_18.png" /></figure>

<figure><img src="image_19.png" /></figure>

<figure><img src="image_20.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3800 Å to 3810 Å

<figure><img src="image_12.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3810 Å to 3820 Å

<figure><img src="image_13.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3820 Å to 3830 Å

<figure><img src="image_14.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3830 Å to 3840 Å

<figure><img src="image_15.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3840 Å to 3850 Å

<figure><img src="image_16.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3850 Å to 3860 Å

<figure><img src="image_17.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3860 Å to 3870 Å

<figure><img src="image_18.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3870 Å to 3880 Å

<figure><img src="image_19.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3880 Å to 3890 Å

<figure><img src="image_20.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 3890 Å to 3900 Å

<figure><img src="image_21.png" /></figure>
<figure><img src="image_21.png" /></figure>

<figure><img src="image_22.png" /></figure>

<figure><img src="image_23.png" /></figure>

<figure><img src="image_24.png" /></figure>

<figure><img src="image_25.png" /></figure>

<figure><img src="image_26.png" /></figure>

<figure><img src="image_27.png" /></figure>

<figure><img src="image_28.png" /></figure>

<figure><img src="image_29.png" /></figure>

<figure><img src="image_30.png" /></figure>
<figure><img src="image_22.png" /></figure>

<figure><img src="image_23.png" /></figure>

<figure><img src="image_24.png" /></figure>

<figure><img src="image_25.png" /></figure>

<figure><img src="image_26.png" /></figure>

<figure><img src="image_27.png" /></figure>

<figure><img src="image_28.png" /></figure>

<figure><img src="image_29.png" /></figure>

<figure><img src="image_30.png" /></figure>

<figure><img src="image_31.png" /></figure>
<figure><img src="image_31.png" /></figure>

<figure><img src="image_32.png" /></figure>

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<figure><img src="image_34.png" /></figure>

<figure><img src="image_35.png" /></figure>

<figure><img src="image_36.png" /></figure>

<figure><img src="image_37.png" /></figure>

<figure><img src="image_38.png" /></figure>

<figure><img src="image_39.png" /></figure>

<figure><img src="image_40.png" /></figure>
<figure><img src="image_32.png" /></figure>

<figure><img src="image_33.png" /></figure>

<figure><img src="image_34.png" /></figure>

<figure><img src="image_35.png" /></figure>

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<figure><img src="image_37.png" /></figure>

<figure><img src="image_38.png" /></figure>

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<figure><img src="image_40.png" /></figure>

<figure><img src="image_41.png" /></figure>
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<figure><img src="image_42.png" /></figure>

<figure><img src="image_43.png" /></figure>

<figure><img src="image_44.png" /></figure>

<figure><img src="image_45.png" /></figure>

<figure><img src="image_46.png" /></figure>

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<figure><img src="image_48.png" /></figure>

<figure><img src="image_49.png" /></figure>

<figure><img src="image_50.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4100 Å to 4110 Å

<figure><img src="image_42.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4110 Å to 4120 Å

<figure><img src="image_43.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4120 Å to 4130 Å

<figure><img src="image_44.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4130 Å to 4140 Å

<figure><img src="image_45.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4140 Å to 4150 Å

<figure><img src="image_46.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4150 Å to 4160 Å

<figure><img src="image_47.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4160 Å to 4170 Å

<figure><img src="image_48.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4170 Å to 4180 Å

<figure><img src="image_49.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4180 Å to 4190 Å

<figure><img src="image_50.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4190 Å to 4200 Å

<figure><img src="image_51.png" /></figure>
<figure><img src="image_51.png" /></figure>

<figure><img src="image_52.png" /></figure>

<figure><img src="image_53.png" /></figure>

<figure><img src="image_54.png" /></figure>

<figure><img src="image_55.png" /></figure>

<figure><img src="image_56.png" /></figure>

<figure><img src="image_57.png" /></figure>

<figure><img src="image_58.png" /></figure>

<figure><img src="image_59.png" /></figure>

<figure><img src="image_60.png" /></figure>
<figure><img src="image_52.png" /></figure>

<figure><img src="image_53.png" /></figure>

<figure><img src="image_54.png" /></figure>

<figure><img src="image_55.png" /></figure>

<figure><img src="image_56.png" /></figure>

<figure><img src="image_57.png" /></figure>

<figure><img src="image_58.png" /></figure>

<figure><img src="image_59.png" /></figure>

<figure><img src="image_60.png" /></figure>

<figure><img src="image_61.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4300 Å to 4310 Å

<figure><img src="image_61.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4310 Å to 4320 Å

<figure><img src="image_62.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4320 Å to 4330 Å

<figure><img src="image_63.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4330 Å to 4340 Å

<figure><img src="image_64.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4340 Å to 4350 Å

<figure><img src="image_65.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4350 Å to 4360 Å

<figure><img src="image_66.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4360 Å to 4370 Å

<figure><img src="image_67.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4370 Å to 4380 Å

<figure><img src="image_68.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4380 Å to 4390 Å

<figure><img src="image_69.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4390 Å to 4400 Å

<figure><img src="image_70.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4300 Å to 4310 Å

<figure><img src="image_62.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4310 Å to 4320 Å

<figure><img src="image_63.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4320 Å to 4330 Å

<figure><img src="image_64.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4330 Å to 4340 Å

<figure><img src="image_65.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4340 Å to 4350 Å

<figure><img src="image_66.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4350 Å to 4360 Å

<figure><img src="image_67.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4360 Å to 4370 Å

<figure><img src="image_68.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4370 Å to 4380 Å

<figure><img src="image_69.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4380 Å to 4390 Å

<figure><img src="image_70.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4390 Å to 4400 Å

<figure><img src="image_71.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4400 Å to 4410 Å

<figure><img src="image_71.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4410 Å to 4420 Å

<figure><img src="image_72.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4420 Å to 4430 Å

<figure><img src="image_73.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4430 Å to 4440 Å

<figure><img src="image_74.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4440 Å to 4450 Å

<figure><img src="image_75.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4450 Å to 4460 Å

<figure><img src="image_76.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4460 Å to 4470 Å

<figure><img src="image_77.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4470 Å to 4480 Å

<figure><img src="image_78.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4480 Å to 4490 Å

<figure><img src="image_79.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4490 Å to 4500 Å

<figure><img src="image_80.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4400 Å to 4410 Å

<figure><img src="image_72.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4410 Å to 4420 Å

<figure><img src="image_73.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4420 Å to 4430 Å

<figure><img src="image_74.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4430 Å to 4440 Å

<figure><img src="image_75.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4440 Å to 4450 Å

<figure><img src="image_76.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4450 Å to 4460 Å

<figure><img src="image_77.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4460 Å to 4470 Å

<figure><img src="image_78.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4470 Å to 4480 Å

<figure><img src="image_79.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4480 Å to 4490 Å

<figure><img src="image_80.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4490 Å to 4500 Å

<figure><img src="image_81.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4500 Å to 4510 Å

<figure><img src="image_81.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4510 Å to 4520 Å

<figure><img src="image_82.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4520 Å to 4530 Å

<figure><img src="image_83.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4530 Å to 4540 Å

<figure><img src="image_84.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4540 Å to 4550 Å

<figure><img src="image_85.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4550 Å to 4560 Å

<figure><img src="image_86.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4560 Å to 4570 Å

<figure><img src="image_87.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4570 Å to 4580 Å

<figure><img src="image_88.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4580 Å to 4590 Å

<figure><img src="image_89.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4590 Å to 4600 Å

<figure><img src="image_90.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4500 Å to 4510 Å

<figure><img src="image_82.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4510 Å to 4520 Å

<figure><img src="image_83.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4520 Å to 4530 Å

<figure><img src="image_84.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4530 Å to 4540 Å

<figure><img src="image_85.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4540 Å to 4550 Å

<figure><img src="image_86.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4550 Å to 4560 Å

<figure><img src="image_87.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4560 Å to 4570 Å

<figure><img src="image_88.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4570 Å to 4580 Å

<figure><img src="image_89.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4580 Å to 4590 Å

<figure><img src="image_90.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4590 Å to 4600 Å

<figure><img src="image_91.png" /></figure>
<figure><img src="image_91.png" /></figure>

<figure><img src="image_92.png" /></figure>

<figure><img src="image_93.png" /></figure>

<figure><img src="image_94.png" /></figure>

<figure><img src="image_95.png" /></figure>

<figure><img src="image_96.png" /></figure>

<figure><img src="image_97.png" /></figure>

<figure><img src="image_98.png" /></figure>

<figure><img src="image_99.png" /></figure>

<figure><img src="image_100.png" /></figure>
<figure><img src="image_92.png" /></figure>

<figure><img src="image_93.png" /></figure>

<figure><img src="image_94.png" /></figure>

<figure><img src="image_95.png" /></figure>

<figure><img src="image_96.png" /></figure>

<figure><img src="image_97.png" /></figure>

<figure><img src="image_98.png" /></figure>

<figure><img src="image_99.png" /></figure>

<figure><img src="image_100.png" /></figure>

<figure><img src="image_101.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4700 Å to 4710 Å

<figure><img src="image_101.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4710 Å to 4720 Å

<figure><img src="image_102.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4720 Å to 4730 Å

<figure><img src="image_103.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4730 Å to 4740 Å

<figure><img src="image_104.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4740 Å to 4750 Å

<figure><img src="image_105.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4750 Å to 4760 Å

<figure><img src="image_106.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4760 Å to 4770 Å

<figure><img src="image_107.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4770 Å to 4780 Å

<figure><img src="image_108.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4780 Å to 4790 Å

<figure><img src="image_109.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 4790 Å to 4800 Å

<figure><img src="image_110.png" /></figure>
<figure><img src="image_102.png" /></figure>

<figure><img src="image_103.png" /></figure>

<figure><img src="image_104.png" /></figure>

<figure><img src="image_105.png" /></figure>

<figure><img src="image_106.png" /></figure>

<figure><img src="image_107.png" /></figure>

<figure><img src="image_108.png" /></figure>

<figure><img src="image_109.png" /></figure>

<figure><img src="image_110.png" /></figure>

<figure><img src="image_111.png" /></figure>
<figure><img src="image_111.png" /></figure>

<figure><img src="image_112.png" /></figure>

<figure><img src="image_113.png" /></figure>

<figure><img src="image_114.png" /></figure>

<figure><img src="image_115.png" /></figure>

<figure><img src="image_116.png" /></figure>

<figure><img src="image_117.png" /></figure>

<figure><img src="image_118.png" /></figure>

<figure><img src="image_119.png" /></figure>

<figure><img src="image_120.png" /></figure>
<figure><img src="image_112.png" /></figure>

<figure><img src="image_113.png" /></figure>

<figure><img src="image_114.png" /></figure>

<figure><img src="image_115.png" /></figure>

<figure><img src="image_116.png" /></figure>

<figure><img src="image_117.png" /></figure>

<figure><img src="image_118.png" /></figure>

<figure><img src="image_119.png" /></figure>

<figure><img src="image_120.png" /></figure>

<figure><img src="image_121.png" /></figure>
<figure><img src="image_121.png" /></figure>

<figure><img src="image_122.png" /></figure>

<figure><img src="image_123.png" /></figure>

<figure><img src="image_124.png" /></figure>

<figure><img src="image_125.png" /></figure>

<figure><img src="image_126.png" /></figure>

<figure><img src="image_127.png" /></figure>

<figure><img src="image_128.png" /></figure>

<figure><img src="image_129.png" /></figure>

<figure><img src="image_130.png" /></figure>
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<figure><img src="image_141.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5100 Å to 5110 Å

<figure><img src="image_141.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5110 Å to 5120 Å

<figure><img src="image_142.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5120 Å to 5130 Å

<figure><img src="image_143.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5130 Å to 5140 Å

<figure><img src="image_144.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5140 Å to 5150 Å

<figure><img src="image_145.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5150 Å to 5160 Å

<figure><img src="image_146.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5160 Å to 5170 Å

<figure><img src="image_147.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5170 Å to 5180 Å

<figure><img src="image_148.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5180 Å to 5190 Å

<figure><img src="image_149.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5190 Å to 5200 Å

<figure><img src="image_150.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5100 Å to 5110 Å

<figure><img src="image_142.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5110 Å to 5120 Å

<figure><img src="image_143.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5120 Å to 5130 Å

<figure><img src="image_144.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5130 Å to 5140 Å

<figure><img src="image_145.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5140 Å to 5150 Å

<figure><img src="image_146.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5150 Å to 5160 Å

<figure><img src="image_147.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5160 Å to 5170 Å

<figure><img src="image_148.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5170 Å to 5180 Å

<figure><img src="image_149.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5180 Å to 5190 Å

<figure><img src="image_150.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5190 Å to 5200 Å

<figure><img src="image_151.png" /></figure>
<figure><img src="image_151.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5210 Å to 5220 Å</figcaption></figure>

<figure><img src="image_152.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5220 Å to 5230 Å</figcaption></figure>

<figure><img src="image_153.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5230 Å to 5240 Å</figcaption></figure>

<figure><img src="image_154.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5240 Å to 5250 Å</figcaption></figure>

<figure><img src="image_155.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5250 Å to 5260 Å</figcaption></figure>

<figure><img src="image_156.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5260 Å to 5270 Å</figcaption></figure>

<figure><img src="image_157.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5270 Å to 5280 Å</figcaption></figure>

<figure><img src="image_158.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5280 Å to 5290 Å</figcaption></figure>

<figure><img src="image_159.png" /><figcaption>Atlas from Delbouille et al. (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5290 Å to 5300 Å</figcaption></figure>

<figure><img src="image_160.png" /></figure>
<figure><img src="image_152.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5210 Å to 5220 Å</figcaption></figure>

<figure><img src="image_153.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5220 Å to 5230 Å</figcaption></figure>

<figure><img src="image_154.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5230 Å to 5240 Å</figcaption></figure>

<figure><img src="image_155.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5240 Å to 5250 Å</figcaption></figure>

<figure><img src="image_156.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5250 Å to 5260 Å</figcaption></figure>

<figure><img src="image_157.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5260 Å to 5270 Å</figcaption></figure>

<figure><img src="image_158.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5270 Å to 5280 Å</figcaption></figure>

<figure><img src="image_159.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5280 Å to 5290 Å</figcaption></figure>

<figure><img src="image_160.png" /><figcaption>Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 5290 Å to 5300 Å</figcaption></figure>

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<figure><img src="image_364.png" /></figure>

<figure><img src="image_365.png" /></figure>

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<figure><img src="image_368.png" /></figure>

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<figure><img src="image_362.png" /></figure>

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<figure><img src="image_365.png" /></figure>

<figure><img src="image_366.png" /></figure>

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<figure><img src="image_369.png" /></figure>

<figure><img src="image_370.png" /></figure>

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<figure><img src="image_372.png" /></figure>

<figure><img src="image_373.png" /></figure>

<figure><img src="image_374.png" /></figure>

<figure><img src="image_375.png" /></figure>

<figure><img src="image_376.png" /></figure>

<figure><img src="image_377.png" /></figure>

<figure><img src="image_378.png" /></figure>

<figure><img src="image_379.png" /></figure>

<figure><img src="image_380.png" /></figure>
<figure><img src="image_372.png" /></figure>

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<figure><img src="image_379.png" /></figure>

<figure><img src="image_380.png" /></figure>

<figure><img src="image_381.png" /></figure>
Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7500 Å to 7510 Å

<figure><img src="image_381.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7510 Å to 7520 Å

<figure><img src="image_382.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7520 Å to 7530 Å

<figure><img src="image_383.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7530 Å to 7540 Å

<figure><img src="image_384.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7540 Å to 7550 Å

<figure><img src="image_385.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7550 Å to 7560 Å

<figure><img src="image_386.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7560 Å to 7570 Å

<figure><img src="image_387.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7570 Å to 7580 Å

<figure><img src="image_388.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7580 Å to 7590 Å

<figure><img src="image_389.png" /></figure>

Atlas from Delbouille et al (μ=1.0), V/I & SQRT(Q²+U²)/I for g=1 & B=1000 G, polarization rates for B=1000 G (bars), line identification (Moore table), Lande factors, from 7590 Å to 7600 Å

<figure><img src="image_390.png" /></figure>
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<figure><img src="image_384.png" /></figure>

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