BEE-spoke-data/govdocs1-by-extension huggingface dataset:
Karen W. Davis								May 1, 1995
Goddard Space Flight Center
Visitor Center
Greenbelt Md.  20771
(301) 286-3979

Jim Sahli
Goddard Space Flight Center
Office of Public Affairs
Greenbelt, Md.  20771
(301) 286-0697

Release No. 95 - 78 

NOTE TO THE EDITORS:

GODDARD SPACE FLIGHT CENTER MAY ACTIVITIES

	The Goddard Space Flight Center Visitor Center provides 
excellent opportunities for learning. May's activities include model 
rocket launches, a "star watch", video and lecture presentations, and 
tours of the Visitor Center and Goddard Space Flight Center facilities.

	The Goddard Space Flight Center Visitor Center is located in 
Greenbelt, Md., on Soil Conservation Road.  All events are free. For 
more information on these and other Goddard Visitor Center activities 
all, (301) 286-8981.  Interpreters will be provided for the hearing 
impaired with seven days' notice through TDD (301) 286-8103.

	The following are brief descriptions for inclusion in your calendar of events:

Sunday, May 7 and 21, 1 p.m.  

MODEL ROCKET LAUNCH

Model rockets will reach new heights at the Goddard Space Flight Center Visitor Center on Sunday, May 7 and 21, at    1 p.m. Bring your own rocket or just come out and enjoy watching the other rocket enthusiasts. All launches are monitored for safety and are held weather permitting.
Saturday, May 13, 8 to p.m.
STAR WATCH
May's warm weather provides excellent conditions for enjoying an evening of stargazing. Come enjoy the night skies at the Goddard Space Flight Center Visitor Center's Star Watch Program on Saturday, May 13, from 8 p.m. to 
10 p.m.  Tour the sky through the Visitor Center's telescope, or through any telescope or binoculars you bring. Rain or cloudy weather conditions will result in cancellation, with the make-up date scheduled for May 20.
	
Saturday, May 13, 1 p.m.

SATURDAY VIDEOS:  "The Atmosphere Below"

The Earth's atmosphere is continuously being bombarded by a stream of particles originating from the Sun and other objects in space. Find out more about these particles and the Earth's atmosphere at the Goddard Space Flight Center Visitor Center's showing of the video "The Atmosphere Below" on Saturday, May 13, at 1 p.m. This video is appropriate for all ages.

Sunday, May 28, 1 p.m.  

DISCOVER GODDARD PRESENTATION:  "How Do We Study Ozone?"

The Total Ozone Mapping Spectrometer (TOMS), to be launched in 1995, on board an Earth Probe Satellite (TOMS-EP), will continue NASA's long term daily mapping of the global distribution of the Earth's atmospheric ozone.  TOMS-EP will extend the high resolution measurement of ozone from space which began with NASA's Nimbus-7 satellite in 1978, and continued with the launch of TOMS instrument on board a Russian Meteor-3 satellite in 1991.  Join Philip A. Sabelhaus, Project Manager for the TOMS Project, as he discusses how studying ozone creation and depletion has helped scientists understand how man and nature are affecting the environment, the importance of ozone and steps being taken worldwide to stop ozone depletion.

###
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JOP098 -- SOHO Joint Observation Programme.

submitted by:
Neale Ranns                 e-mail;  ndrr@mssl.ucl.ac.uk

CDS/EIT/MDI/TRACE/YOHKOH  03-Feb-1999

Multi-Wavelength Observations of Solar Flares.

The principle aim of this Joint Observation Programme is to examine the
morphological and temporal relationships between flare loop footpoint
emissions in Hard X-ray and Extreme Ultraviolet radiation. Flare loop
footpoint emission has been observed up to thirty minutes before a flare
(Cheng,84) and during the impulsive phase (Cheng,81). The impulsive phase
emission was observed to spatially correlate with the HXR emission and the
preflare emission in some examples originated from future flare kernels. 

To accomplish our aim this observing program will incorporate TRACE,
Yohkoh and SOHO-CDS-EIT-MDI in a combined continuous observation of an
active region as it traverses the solar disk. This will ensure the
acquisition of preflare data. Using the wide temporal coverage and high
time resolution of the TRACE instrument we aim to observe EUV brightenings
from Transition region or Chromospheric lines, during the preflare and
impulsive phases of a solar flare and use Yohkoh-HXT to determine the
location of the HXR source. Our intention is to determine the nature of
the preflare burst i.e. whether they are the cause or a consequence of the
X-ray flare. Using the improved spatial resolution of both instruments we
will study the morphological relationships between the EUV and HXR sources
and investigate any relationships between the intensity of the two photon
energy domains. HXT will enable us to accomplish this in a higher energy
band ($53-93keV$) than previously available.

The further employment of SOHO-CDS/NIS, Yohkoh-SXT and SOHO-EIT will
provide information on the densities and temperatures involved within the
flare loops, and with CDS we can measure the velocities of the flare
plasma. Inclusion of the MDI will allow the association of flare kernels
with photospheric magnetic features, and aid with the determination of
loop orientation.


Yohkoh

Continuous tracking of a single active region.

TRACE

Continuous tracking of a single active region. Cycle through filters,
$1550\AA$, $1600\AA$, $WL$ and $171\AA$ to gain high time resolution CIV
and FeIX images.

CDS

Continuous tracking of a single active region. Imaging in FeXVI, FeXIV, OV
and HeI lines.


EIT

Tracking of a single active region, all filters.


MDI

Normal synoptic imaging.
Salary Table 2003-MFL (LEO)
	INCORPORATING THE 3.10% GENERAL SCHEDULE INCREASE AND A LOCALITY PAYMENT OF 13.81%
                 FOR THE LOCALITY PAY AREA OF MIAMI-FORT LAUDERDALE, FL
		
                                (Total Increase: 4.35%)

                                Effective January 2003

                             Annual Rates by Grade and Step

GS     1          2         3         4         5        6          7        8        9       10

1     17315     17893     18469     19042     19619     19958     20524    21098    21122    21659
2     19468     19930     20576     21122     21359     21987     22615    23243    23872    24500
3     25489     26197     26905     27613     28320     29028     29736    30444    31152    31860
4     28612     29406     30201     30995     31789     32584     33378    34173    34967    35761
5     32901     33790     34679     35568     36457     37346     38234    39123    40012    40901
6     34695     35686     36678     37669     38660     39651     40643    41634    42625    43617
7     37454     38555     39657     40759     41860     42962     44064    45165    46267    47369
8     39039     40259     41479     42699     43919     45139     46359    47579    48799    50019
9     41772     43119     44467     45814     47162     48509     49857    51204    52552    53899
10    46001     47485     48969     50453     51937     53421     54905    56389    57874    59358
11    48911     50542     52173     53804     55435     57065     58696    60327    61958    63589
12    58621     60575     62529     64484     66438     68392     70346    72300    74254    76208
13    69710     72034     74358     76682     79006     81330     83654    85978    88302    90626
14    82377     85123     87869     90616     93362     96108     98854    101600    104347    107093
15    96898     100128     103358     106588     109818    113047    116277   119507   122737   125967


* Includes Special Salary Rates At GS-3 Through GS-10
"Two Polish dances","sm/sm1885/15100","15143","001.gif","1","1","","001.tif"
"Two Polish dances","sm/sm1885/15100","15143","002.gif","2","2","","002.tif"
"Two Polish dances","sm/sm1885/15100","15143","003.gif","3","3","","003.tif"
"Two Polish dances","sm/sm1885/15100","15143","004.gif","4","4","","004.tif"
"Two Polish dances","sm/sm1885/15100","15143","005.gif","5","5","","005.tif"
"Two Polish dances","sm/sm1885/15100","15143","006.gif","6","6","","006.tif"
"Two Polish dances","sm/sm1885/15100","15143","007.gif","7","7","","007.tif"
"Two Polish dances","sm/sm1885/15100","15143","008.gif","8","8","","008.tif"
"Two Polish dances","sm/sm1885/15100","15143","009.gif","9","9","","009.tif"
000
NWUS54 KHUN 300957
LSRHUN

PRELIMINARY LOCAL STORM REPORT
NATIONAL WEATHER SERVICE HUNTSVILLE AL
456 AM CDT THU AUG 30 2007

..TIME...   ...EVENT...      ...CITY LOCATION...     ...LAT.LON...
..DATE...   ....MAG....      ..COUNTY LOCATION..ST.. ...SOURCE....
            ..REMARKS..

0630 PM     LIGHTNING        4 NW HUNTSVILLE         34.77N 86.64W 
08/29/2007                   MADISON            AL   NEWSPAPER       

            LIGHTNING SPARKED A SMALL ATTIC FIRE AT A RESIDENCE. 
            DAMAGES UNKNOWN. TIME ESTIMATED

0630 PM     LIGHTNING        6 WNW OWENS CROSSROADS  34.61N 86.55W 
08/29/2007                   MADISON            AL   NEWSPAPER       

            LIGHTNING STRUCK A POWER SUBSTATION ON CHANEY THOMPSON 
            ROAD CAUSING A POWER OUTAGE AFFECTING 1900 CUSTOMERS. 
            LIGHTNING ALSO STRUCK A SUBSTATION IN DOWNTOWN HUNTSVILLE
            AFFECTING 300 CUSTOMERS. TIME ESTIMATED.

0700 PM     FLASH FLOOD      1 S HUNTSVILLE          34.72N 86.59W 
08/29/2007                   MADISON            AL   BROADCAST MEDIA 

            FLASH FLOOD WITH KNEE DEEP WATER IMPACTING RESIDENCES ON 
            AUBURN AND STANFORD STREETS. TIME ESTIMATED.

0700 PM     HEAVY RAIN       3 SSW HUNTSVILLE        34.69N 86.60W 
08/29/2007  M3.40 INCH       MADISON            AL   MESONET         

            MEASURED AT SPRING BRANCH...STATION ID SBHA1. ONE HOUR 
            RAINFALL FROM 6 TO 7 PM OF 3.40 INCHES. 30 MINUTE 
            RAINFALL FROM 6 TO 630 PM OF 2.41 INCHES. 20 MINUTE 
            RAINFALL FROM 615 PM TO 635 PM OF 2.18 INCHES...AVERAGING
            0.55 INCHES EACH 5 MINTES.

0730 PM     FLASH FLOOD      3 S HUNTSVILLE          34.69N 86.58W 
08/29/2007                   MADISON            AL   NEWSPAPER       

            FLASH FLOODING PROMPTED A SECTION OF BALMORAL DRIVE TO BE
            BLOCKED OFF. FLASH FLOODING WAS ALSO REPORTED ON SEVERAL 
            HUNTSVILLE STREETS INCLUDING MERIDIAN STREET...WHITESBURG
            DRIVE...SOUTH MEMORIAL PARKWAY...AND UNIVERSITY DRIVE. 
            TIME ESTIMATED. 

&&

$$

KULA
114
A LITTLE TOUR IN FRANCE.
degree of entertainment to be  derived.    If they are
tolerably old, they are often touching; but they must
have a relative antiquity,  for I confess I can do no-
thing with works of art of which the badness is of
recent origin.    The   cool,   still,   empty chambers in
which indifferent collections are apt to be preserved,
the red brick tiles, the diffused light, the musty odor,
the mementos around you of dead fashions, the snuffy
custodian in a black skull cap,   who pulls  aside  a
faded curtain to show you the lustreless gem of the
museum,these things have a mild historical quality,
and the sallow canvases after all illustrate something.
Many of those in the museum of Nantes illustrate the
taste of a successful warrior; having been bequeathed
to the city by Napoleon's marshal,   Clarke (created
Duc de Feltre).    In   addition  to these there  is the
usual number of specimens ofthe contemporary French
school, culled from the annual Salons and presented
to the museum by the State.    Wherever the traveller
goes, in France, he is reminded of this very honorable
practice,the purchase by the Government of a cer-
tain number of "pictures of the year," which are pre-
sently distributed in the provinces.    Governments suc-
ceed   each   other   and bid   for  success  by   different
devices; but the "patronage of art" is a plank, as we
should say here, in every platform.    The works of art
are often ill-selected,there is an official taste which
you immediately recognize,but the custom is essen-
tially liberal, and a government which should neglect
it would be felt to be painfully common.   The only
PUBLIC INFORMATION OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION 
PASADENA, CALIF. 91109. TELEPHONE (818) 354-5011

Contact:  Mary Beth Murrill, (818) 354-6478               

FOR IMMEDIATE RELEASE                         December 18, 1995

A NEW SPACECRAFT COMES TO LIFE

     In the midst of the excitement surrounding the arrival of 
the Galileo spacecraft at Jupiter, technicians and engineers 
presided over the birth of a new spacecraft, in a white-walled 
clean room at NASA's Jet Propulsion Laboratory, Pasadena, CA.

     The Cassini spacecraft, bound for a launch to Saturn in 
1997,  was successfully "powered on" for the first time last week 
as its cousin spacecraft Galileo began its historic mission at 
Jupiter.   Cassini is scheduled for launch from Cape Canaveral, 
FL, on October 6, 1997 and will reach Saturn in July 2004.

     "This is the first time the major elements of the spacecraft 
have been electrically linked together, and it all worked," said 
Richard J. Spehalski, Cassini program manager at JPL.   
     
     Support equipment supplied the 30 volts of electricity on 
which the spacecraft and its science instruments will operate.  
No problems were found as the power flowed through the seven 
miles of cabling that will link Cassini's computers, science 
instruments and mechanical and propulsion systems.

     Cassini, a joint mission of NASA, the European Space Agency 
(ESA) and the Italian Space Agency (ASI), is similar in concept 
to the Galileo mission.  Cassini will send a parachuted probe, 
called Huygens, into the atmosphere and to the surface of 
Saturn's large moon Titan.  The main Cassini spacecraft will 
orbit Saturn to provide four years of close-up data on the moons, 
rings, planet and Saturn's magnetic environment.  Huygens is 
provided by ESA, and Cassini's sophisicated radio antenna is 
provided by ASI.  The Cassini program is managed by JPL.

     Assembly and testing of the spacecraft will continue at JPL 
through mid-1997 when the spacecraft will be shipped to Cape 
Canaveral, FL, for launch preparations.

                            #####

12-18-95 MBM
#9588
From owner-nwchem-users@emsl.pnl.gov Wed Apr 21 14:52:51 2004
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Date: Wed, 21 Apr 2004 17:51:03 -0400
From: "Harrison, Robert J." <harrisonrj@ornl.gov>
Subject: RE:
To: jmsulliv@chem.northwestern.edu, nwchem-users@emsl.pnl.gov
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I tossed this together, so don't take the numbers
as gospel, but the below computes the corrected
and uncorrected He-Ne interaction energy

The main tricks are specifying the ghost
centers with bq before the atomic symbol,
and inserting the atom name in the basis
set specification for the ghost center.
The extra scf;vectors atomic;end is just
to force the SCF initial guess to be used
since the old vectors from another fragment
won't be appropriate.

Robert




start

# He--Ne MP2/aug-cc-pdz interaction energy at 3 angstrom

# BSSE corrected interaction energy = +2.4 uH
#    uncorrected interaction energy = -65.4 uH

basis spherical
  he library aug-cc-pvdz
  ne library aug-cc-pvdz
  bqhe library he aug-cc-pvdz
  bqne library ne aug-cc-pvdz
end

mp2
  tight
  print low
  freeze core atomic
end

geometry
  he 0 0 0
  ne 0 0 3
end
scf; vectors atomic; end
task mp2 energy     # -131.585955808294


geometry
  he 0 0 0
  bqne 0 0 3
end
scf; vectors atomic; end
task mp2 energy    # -2.882686515578


geometry
  bqhe 0 0 0
  ne 0 0 3
end
scf; vectors atomic; end
task mp2 energy    # -128.703271690657

geometry
  ne 0 0 3
end
scf; vectors atomic; end
task mp2 energy    # -128.703223239222

geometry
  he 0 0 0
end
scf; vectors atomic; end
task mp2 energy    # -2.882667179282



-----Original Message-----
From: owner-nwchem-developers@emsl.pnl.gov on behalf of Jay Sullivan
Sent: Wed 4/21/2004 4:35 PM
To: nwchem-users@emsl.pnl.gov
Subject: 
 
Would anyone care to send me a simple (complete) example of how to make a
BSSE correction with NWChem. 

I am having some difficulty figuring it out from the manual.

Thanks,
JMS
264
HISTORY OF ST. DOMINGO.
also commanded a division.    To them were added Generals
Kerversan and Boudet, with a force of twenty thousand men.
The two sons of Toussaint L'Ouverture who had been educated
in France, were sent as hostages for the reception of the French
army by their father, under the care of the tutors who had ac-
companied them. Admiral Villaret (who was in the service of the
regal government of France) commanded the fleet, under whom
were Rear-Admiral Latouche, and Captain Magon.    The fleet
consisted of some of the best ships of the line, and a propor-
tionable number of frigates, transports, &c.    The prevalent sen-
timent seemed to be, that after the first attack, a compromise
would be effected with Toussaint and the different chiefs, which
would enable the French force to establish itself throughout the
island, and complete the subjugation of the armed blacks.%
In the month of December the expedition sailed, amidst the
acclamations of all, who were either interested in its success, or
* The absurdity of this idea, when the state of St. Domingo at the time is considered, and
the accumulated strength which the General in Chief had acquired from the defeat of every
enemy as well as the experience which the different contentions had afforded him, is a suf-
ficient proof of the inconsideration with which Bonaparte was hurried into tins rll-contrived
and ruinous measure.    The writer did not omit any means, both with those in power
and otherwise, to convince them of the futility of the scheme, and to caution the British
government against the temptation afforded to Admiral Villaret, to turn his course to a mor
accessible destination.   But such was the predetermined state of the public ^1     h
opinions and his cautions were alike disregarded.   Both have, however, been fullyeonroho
rated  and if the "feeble and divided" blacks had not given a better account of the French
expedition, worse effects of such an inattention might have been experienced. As a curiosity,
when compared with the French General's dispatches, the anticipation of h.s  ate, as pub-
lished at the Military Library in London in the beginning of 1802, will be found in the
Appendix to this work.                     g                                                  imagined
Resolutions to he Addressed to the State Legislature
By Local JVleetings
WHEREAS Taxation without representation is tyranny, and
WHEREAS The women of this and all other states pay a rapidly increasing amount of taxes> therefore
RESOLVED That justice demands that their present disability be removed, and that they be enfranchised upon the same, terms as the men in the States, and
RESOLVED That, as a means to this end, we ask that Congress
shall, at the coming session, submit to the voters a Sixteenth Amendment to the Constitution of the United States, to be submitted to the Legislatures of the several States for ratification, prohibiting dis-franchisement of United States Citizens on account of sex.
RESOLVED That we respectfully request the Legislature of the
State of New York to adopt a memorial to Congress urging the submission to the several States of such sixteenth Amendment to the Constitution of the United States, and
RESOLVED That the Secretary of this meeting is hereby requested to forward a copy of this resolution to the Governor and to the Senator and Representatives of this district.
FXUS65 KPIH 052124
AFDPIH

AREA FORECAST DISCUSSION...CORRECTION
NATIONAL WEATHER SERVICE POCATELLO ID
230 PM MST FRI MAR 05 2004

.DISCUSSION...
LATEST H2O SATIMG SHOWING NEXT PAC WAVE PUSHING ACROSS BC WITH 140KT 
300MB JET NOSING INTO VC ISLAND.  MODELS TRENDING FURTHER NORTH THAN 
PREVIOUS 12Z RUN WITH WAVE SLICING ESE INTO NRN MONTANA TONIGHT.  
INCREASING 700MB FLOW ALONG WITH APPROACHING SURFACE FRONT AND 
STRONG FLOW ALOFT EXPECTED TO GENERATE ADVISORY LEVEL WINDS STARTING 
LATE TONIGHT AND CONTINUING THROUGH A GOOD PORTION OF THE DAY 
SATURDAY. HENCE HAVE ISSUED A WIND ADVISORY FOR VALLEY ZONES.  
OVERNIGHT LOWS LIKELY TO FALL BEFORE MIDNIGHT TONIGHT AND HAVE 
ADJUSTED GRIDS TO REFLECT THIS.  BROAD FLAT UPPER RIDGE GRADUALLY 
BUILDS OVER PAC NW SUNDAY THROUGH MONDAY WITH CORRESPONDING DECREASE 
IN PRECIPITATION POTENTIAL AND INCREASE IN DAY TIME TEMPERATURES 
THROUGH THE PERIOD. HUSTON 

IN THE EXTENDED FOR MONDAY NGT THROUGH FRIDAY NGT...MODEL RUNS FOR 
EXTENDED SUITES ARE MUCH DRIER THAN PREVIOUS DAY.  MAIN FEATURE OF 
THE PERIOD IS LOW AMPLITUDE U/L RIDGING OVER THE WRN US WITH THE 
STORM TRACK STAYING NEAR THE US-CAN BORDER.  THIS DOES ALLOW FOR 
SOME OCCASIONAL CLOUDINESS WITH SLIGHT CHC OF PRECIP ALONG THE 
CONTDIVID AND EXTRM NRN ZONES.  THE ONE LONE EXCEPTION IS THE 
STRONGEST S/W OF THE PERIOD WHICH MOVES THROUGH SERN ID DURING THE 
DAY WED.  HOWEVER EURO/UK PRODUCTS DO NOT HAVE THIS S/W AS INTENSE 
AS THE GFSX...SO THIS FEATURE MAY BE OVERDONE.  BY FRI/FRI 
NGT...GFSX MOS GUIDANCE BRINGS BACK SLT CHC/LOW CHC POPS FOR THE 
AREA.  PATTERN DOES NOT SUPPORT THIS WITH LARGE LOW IN ERN PAC AND 
ANOTHER IN THE CENTRAL GREAT PLAINS...CAN ONLY ASSUME CLIMATOLOGY 
INFLUENCE IN EQUATIONS HAS OVERPOWERED THE SYNOPTIC SITUATION.  WILL 
LOWER ZERO FOR MOST LOCATIONS EXCEPT ALONG NRN BORDER WHERE SLT CHC 
MAY RULE WITH WEAK ZONAL FLOW AND POSSIBLE UPSLOPE SHOWERS IN 
FAVORABLE TERRAIN.  MESSICK
&&

.PIH WATCHES/WARNING/ADVISORIES...WIND ADVISORY ZONES 17/20/21 LATE 
TONIGHT THROUGH SATURDAY.  SEE LATEST BULLETING FOR FURTHER 
INFORMATION.
&&

$$
000
WWUS84 KOHX 191650
SPSOHX
SPECIAL WEATHER STATEMENT
NATIONAL WEATHER SERVICE NASHVILLE TN
1050 AM CST SAT JAN 19 2008
TNZ005>011-022>034-056>066-075-077>080-093>095-192300-
STEWART-MONTGOMERY-ROBERTSON-SUMNER-MACON-CLAY-PICKETT-BENTON-
HOUSTON-HUMPHREYS-DICKSON-CHEATHAM-DAVIDSON-WILSON-TROUSDALE-
SMITH-JACKSON-PUTNAM-OVERTON-FENTRESS-PERRY-HICKMAN-LEWIS-
WILLIAMSON-MAURY-MARSHALL-RUTHERFORD-CANNON-DEKALB-WHITE-
CUMBERLAND-BEDFORD-COFFEE-WARREN-GRUNDY-VAN BUREN-WAYNE-LAWRENCE-
GILES-
INCLUDING THE CITIES OF...DOVER...CLARKSVILLE...SPRINGFIELD...
GALLATIN...LAFAYETTE...CELINA...BYRDSTOWN...CAMDEN...ERIN...
WAVERLY...DICKSON...ASHLAND CITY...KINGSTON SPRINGS...NASHVILLE...
LEBANON...MOUNT JULIET...HARTSVILLE...CARTHAGE...GAINESBORO...
COOKEVILLE...LIVINGSTON...JAMESTOWN...ALLARDT...LINDEN...
LOBELVILLE...CENTERVILLE...HOHENWALD...FRANKLIN...BRENTWOOD...
COLUMBIA...LEWISBURG...MURFREESBORO...WOODBURY...SMITHVILLE...
SPARTA...CROSSVILLE...FAIRFIELD GLADE...SHELBYVILLE...TULLAHOMA...
MANCHESTER...MCMINNVILLE...TRACY CITY...ALTAMONT...COALMONT...
SPENCER...WAYNESBORO...LAWRENCEBURG...PULASKI
1050 AM CST SAT JAN 19 2008
...FRIGID ARCTIC AIR WILL COVER MIDDLE TENNESSEE BY NIGHTFALL...
A FRIGID ARCTIC AIR MASS WILL SETTLE ACROSS MIDDLE TENNESSEE THIS
AFTERNOON AND EVENING...SENDING TEMPERATURES INTO THE LOW TO MID
TEENS BY SUNDAY MORNING. TEMPERATURES THIS COLD MAY BE DANGEROUS
TO OUTDOOR PETS...AND PET OWNERS MAY WANT TO CONSIDER BRINGING
ANIMALS INDOORS FOR THE NIGHT. TEMPERATURES THIS COLD CAN ALSO
FREEZE EXPOSED WATER PIPES...AND HOME OWNERS MAY WANT TO CONSIDER
INSULATING OUTDOOR WATER SPICKETS...AND CLOSING CRAWL SPACE VENTS
TO PREVENT PIPES FROM FREEZING.
TEMPERATURES ON SUNDAY PROBABLY WILL NOT RISE ABOVE THE FREEZING
MARK... WITH TEMPERATURES IN THE LOW TO MID TEENS AGAIN SUNDAY
NIGHT.
THE COLDEST TEMPERATURE SO FAR THIS WINTER IN NASHVILLE HAS BEEN
11 DEGREES ON JANUARY 3RD. LAST WINTER...THE COLDEST TEMPERATURE
WAS ALSO 11 DEGREES ON JANUARY 29TH.
THE LAST TIME THE TEMPERATURE WAS BELOW ZERO IN NASHVILLE WAS BACK
ON FEBRUARY 4TH AND 5TH IN 1996...WHEN IT FELL TO 3 DEGREES BELOW
ZERO.
THE ALL TIME RECORD LOW IN NASHVILLE WAS BACK ON JANUARY 21ST 1985
WHEN THE TEMPERATURE FELL TO A MINUS 17 DEGREES BELOW ZERO.
$$
BOYD
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Date: Sun, 01 Aug 1999 15:13:04 -0500
To: Jeff Squyres <jsquyres@lsc.nd.edu>
From: William Gropp <gropp@mcs.anl.gov>
Subject: Re: MPI-2 MPI_Comm_spawn inconsistency 
Cc: mpi-core@mcs.anl.gov
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At 06:26 PM 7/30/99 -0500, Jeff Squyres wrote:
I think we came across a conflict in the MPI-2 standard today (gasp!).

In looking at MPI_Comm_spawn[_multiple] the other day, we noticed that one
of the parameters doesn't seem to make sense for non-root ranks.  Let me
refresh your memory of MPI_Comm_spawn (MC_Spawn_multiple is similar, so
we'll just use MC_spawn here):

MPI_Comm_spawn(IN command, IN argv, IN maxprocs, IN info, IN root, IN
               comm, OUT intercomm, OUT array_of_errorcodes)

command, argv, maxprocs, and info are specifically denoted as "significant
only at root".

After calling MPI_Comm_spawn (which is collective across comm), everyone
gets a new intercomm to communicate with the spawned children.  Everyone
is also supposed to also get an array of errorcodes that represent the
return codes from spawning each of the maxprocs children.

MPI-2 88:13 specifically says, "The array_of_errorcodes is an array of
length maxprocs..."  But maxprocs is only significant at the root -- so
the non-root members of comm may not know what maxprocs is.  Hence, they
might not know how long array_of_errorcodes is supposed to be.  Recall
that in true MPI fashion, the user is responsible for allocating
array_of_errorcodes; this can be pretty hard to do if you don't know how
long it needs to be.

So this doesn't seem to make sense.

Significant at the root only means that that argument is ignored except by the designated root process (in order to avoid confusion over which value to use if different processes provided different values).  We can still require that the arrays representing other arguments have the appropriate sizes.

Bill
"Cyclone polka /","sm1883/10100","10130","001.gif","1","1","","001.tif"
"Cyclone polka /","sm1883/10100","10130","002.gif","2","2","","002.tif"
"Cyclone polka /","sm1883/10100","10130","003.gif","3","3","","003.tif"
"Cyclone polka /","sm1883/10100","10130","004.gif","4","4","","004.tif"
"Cyclone polka /","sm1883/10100","10130","005.gif","5","5","","005.tif"
"Cyclone polka /","sm1883/10100","10130","006.gif","6","6","","006.tif"
"Cyclone polka /","sm1883/10100","10130","007.gif","7","7","","007.tif"
"Cyclone polka /","sm1883/10100","10130","008.gif","8","8","","008.tif"
"Cyclone polka /","sm1883/10100","10130","009.gif","9","9","","009.tif"
"Cyclone polka /","sm1883/10100","10130","010.gif","10","10","","010.tif"
"Cyclone polka /","sm1883/10100","10130","011.gif","11","11","","011.tif"
"Cyclone polka /","sm1883/10100","10130","012.gif","12","12","","012.tif"
"Cyclone polka /","sm1883/10100","10130","013.gif","13","13","","013.tif"
"Cyclone polka /","sm1883/10100","10130","014.gif","14","14","","014.tif"
"Cyclone polka /","sm1883/10100","10130","015.gif","15","15","","015.tif"
"Cyclone polka /","sm1883/10100","10130","016.gif","16","16","","016.tif"
"Cyclone polka /","sm1883/10100","10130","017.gif","17","17","","017.tif"
"Cyclone polka /","sm1883/10100","10130","018.gif","18","18","","018.tif"
"Cyclone polka /","sm1883/10100","10130","019.gif","19","19","","019.tif"
"Cyclone polka /","sm1883/10100","10130","020.gif","20","20","","020.tif"
"Cyclone polka /","sm1883/10100","10130","021.gif","21","21","","021.tif"
From: Tatusov, Roman (NIH/NLM/NCBI)
Sent: Monday, November 14, 2005 5:18 PM
To: NLM/NCBI List ncbi-seminar
Subject: CBB seminar, Nov 15
Tuesday, November 15, 11am
Bldg. 38A, B2 conference room
Rank based approach to find phylogenetic neighbors.
The amount of completely sequenced genomes increases exponentially and
floods the protein databases with ever growing numbers of protein. The
majority of proteins from new genomes are close counterparts to already
described ones. Clusters of Orthologous Groups organize proteins into
groups, decreasing number of independent entities considerably.
Traditional COG approach to group orthologous genes uses heuristics to
find the descendants of the same ancestor. The clustering procedure
utilizes the only relationship called organism specific best hit. This
minimalism defines the simplicity of algorithm implementation, but at
the same time degrades the quality of the results with increasing number
of the organisms. The broadened procedure uses ranks of all the BLAST
hits. Those ranks are considered as distances and elements of standard
tree constructing techniques are applied to delineate clusters of
orthologs.
The comparable routine can be applied to a collection of extremely close
organisms like strains of Influenza virus. Each strain differs from
counterparts only by a handful of mutations prompting a significant
effect on the virulence. The appropriately modified rankings help to
differentiate clades of subclades of the Influenza virus.
Roman Tatusov
- Mario generated over the weekend MBR MC. This he compared with minbias
 data. There's a factor of two difference in the means, as well as a much
 longer tail in the data. These differences are SL independent. His MC
 points are consistent with RunI predictions, though. We had some
 discussion as to possible causes which I'll skip here.

 - Marco seems to have figured out how to combine the different pieces of
 mixing events. It is amazing that this was never done in CDF since
 ~1996. Was working on building an exe. Just now we got a message that he
 has merged jet20 with 5 mbs events. These need checking, and Richard
 will look at the COT part, while Marco will test the Si.

 - Y2K started breaking down JDL's trigger table into its physics
 drivers. She has to incorporate the calibration triggers, and add the
 various remarks, but this is what we want. Mel promised to look at it
 and send his comments today. I think that we should build around this
 approach, i.e. add a short paragraph before it as an introduction etc.

 - I showed plots made by Chris Hays of number of obscured hits for all
 SL's with ttbar+0, 5, 10 15 MBS events. Scary. Time was short. Will get
 back to it next time.

 - Y2K showed worse case scenario of Z->bbbar mass resolution. Nice and
 quick work. She wants to see the sensitivity to cone size (0.7->0.4).
 She'll dig the kind of mass resolution people were assuming in our
 various propaganda Higgs reach plots.

 - Patrizia's back from Tuscany and is re-rerunning the Si track finding
 eff. We need to get some computing resources (MC farm) to do the MC
 generation/simulation for her to be able to turn these into B-tagging
 numbers. She's contacted Pasha & Frank. We'll see.

 We agreed to meet tomorrow, 0900, Trailer 171.

 Avi.
{CaptionsBy}    InDyne, Inc.

{LastEditor}    Anita Barrett

{ScannedBy}     Seven/Still Photo Imaging

{author}        NASA or National Aeronautics and Space Administration

{date}          10-Nov-2000

{description}   From the top of a utility pole, a red-tailed hawk launches into
                flight, perhaps after spotting prey, typically a small rodent.
                Ranging in height from 18 inches to 25 inches, the species has a
                stocky build with a whitish breast and rust-colored tail. It has
                a high-pitched descending scream with a hoarse quality. The hawk
                inhabits mainly deciduous forest and adjacent open country from
                Alaska and Nova Scotia south to Panama. KSC shares a boundary
                with the Merritt Island National Wildlife Refuge, which
                encompasses 92,000 acres that are a habitat for more than 331
                species of birds, 31 mammals, 117 fishes, and 65 amphibians and
                reptiles. The marshes and open water of the refuge provide
                wintering areas for 23 species of migratory waterfowl, as well as
                a year-round home for great blue herons, great egrets, wood
                storks, cormorants, brown pelicans and other species of marsh and
                shore birds, as well as a variety of insects.

{highres}       1787 x 2670

{highsize}      1061544

{hightype}      JPEG

{lowres}        161 x 240

{lowsize}       55417

{lowtype}       GIF

{mediumres}     514 x 768

{mediumsize}    65467

{mediumtype}    JPEG

{number}        KSC-00PP-1740

{slideres}      111 x 156

{slidesize}     25115

{slidetype}     GIF

{tinyres}       67 x 100

{tinysize}      10222

{tinytype}      GIF

{title}         A red-tailed hawk at KSC

{type}          Image

{end}
/* SUMFUNC.C
 *
 * Computes sum-of-squares for lobing model.
 */
#include <math.h>
#include "fitlobes.h"
/* LOCAL FUNCTIONS */
static OneResidualFnAnon oneResidual;
double sumFunc( void *x, const Vector p )
	/* Calculate sum of squares of model for L-M algorithm */
{
	FitData *fd = (FitData *)x;
	/* Set up lobe angles so that once we know which lobe, the rest is easy */
	/* Index corresponds to cusp number */
	setupFitData( fd, p );
	/* Now loop through everything */
	return sumOfSquaresAnon( x, dsLength(&fd->ds), p, oneResidual );
}
#pragma argsused /* const Vector q */
static double oneResidual( void *x, int i, const Vector q )
	/* Calculate one residual for combined model */
{
	const FitData *fd = (FitData *)x;
	const Vector p = fd->fitParms;
	const struct Dataset_ *pts = &fd->ds;
	double x_i, y_i, z_i, r_i, azimuth_i, decl_i;
	double pretravel;
	/* Get spherical coordinates for point i */
	ptInfo( dsAt(pts,i), p, &x_i, &y_i, &z_i, &r_i, &azimuth_i, &decl_i );
	if ( decl_i < fd->capAngle ) {
		/* Within friction cap */
		pretravel = K(p);
	} else {
		/* Outside the friction cap. */
		int lobe;
		double cusp, lobeAngle, sDecl = sin(decl_i);
		/* Get the lobe index and the relative angle of azimuth_i in the lobe */
		lobe = lobeIndex( azimuth_i, decl_i, p, fd, &lobeAngle );
		/* Calculate the "cusp" function (my name) */
		cusp = sDecl * cos(azimuth_i-lobeAngle) + BETA(p) * cos(decl_i);
		pretravel = ALPHA(p) * cusp + GAMMA(p)*fd->bigF[lobe]*sDecl*sDecl / cusp;
	}
	return r_i - RAD(p) + pretravel;
}
000
FLUS44 KLUB 051045
HWOLUB

HAZARDOUS WEATHER OUTLOOK
NATIONAL WEATHER SERVICE LUBBOCK TX
545 AM CDT THU APR 5 2007

TXZ021>044-061045-
PARMER-CASTRO-SWISHER-BRISCOE-HALL-CHILDRESS-BAILEY-LAMB-HALE-
FLOYD-MOTLEY-COTTLE-COCHRAN-HOCKLEY-LUBBOCK-CROSBY-DICKENS-KING-
YOAKUM-TERRY-LYNN-GARZA-KENT-STONEWALL-
545 AM CDT THU APR 5 2007

THIS HAZARDOUS WEATHER OUTLOOK IS FOR THE EXTREME SOUTHERN TEXAS
PANHANDLE...SOUTH PLAINS AND ROLLING PLAINS.

.DAY ONE...TODAY AND TONIGHT

NO HAZARDOUS WEATHER IS EXPECTED AT THIS TIME.

.DAYS TWO THROUGH SEVEN...FRIDAY THROUGH WEDNESDAY

A COLD CANADIAN AIR MASS WILL MOVE INTO THE OUTLOOK AREA FRIDAY
AND SATURDAY. TEMPERATURES BELOW FREEZING WILL BE POSSIBLE BY SATURDAY
MORNING AND MORE LIKELY SUNDAY MORNING ACROSS MUCH OF THE
CAPROCK...AND POSSIBLY INTO PORTIONS OF THE ROLLING PLAINS. WINTRY
PRECIPITATION WILL ALSO BE POSSIBLE ACROSS THE AREA BEGINNING LATE
FRIDAY AND CONTINUING THROUGH SUNDAY MORNING. SNOWFALL
ACCUMULATIONS ARE EXPECTED TO BE LIGHT...BUT ONE OR TWO INCHES IS
POSSIBLE...MAINLY ACROSS THE EXTREME SOUTHERN TEXAS PANHANDLE.

ADDITIONALLY...ABOVE NORMAL TEMPERATURES THE PAST MONTH HAVE CAUSED MANY PLANTS
TO BLOOM OR SPROUT EARLY. SOME OF THESE PLANTS MAY BE SUSCEPTIBLE
TO THE FREEZING TEMPERATURES.

$$
FQCN35 CYQX 131324
NAVTEX FOR LABRADOR VOK AT 10:00 AM NST FRI 13 FEB 2009.
VLD 13/13Z-15/03Z,
WND(KT), VIS(NM) ABV 1 NM UNL IND, FOG IMPL VIS LESS THAN 1 NM.
 SYNOPSIS:
13/13Z LOW 972 MB S OF NFLD. 14/13Z LOW 972 MB SE OF THE MARINE
 DISTRICT.
STRAIT OF BELLE ISLE:
WNG: GALE / FREEZING SPRAY.
WND: NE25-35.
SPRAY: 13/13Z-13/21Z MOD OVR-OW.
VIS: 13/13Z-15/03Z 0-1 SN.
BELLE ISLE BANK:
WNG: GALE.
WND: E15. 13/17Z NE25. 14/00Z NE35. 14/12Z NE25.
VIS: 13/18Z-15/03Z 0-1 LGT-SN.
LAKE MELVILLE:
WNG: NIL.
WND: NE15. 14/09Z NE25.
VIS: 13/13Z-15/03Z 0-1 LGT-SN.
SOUTH LABRADOR COAST, MID LABRADOR COAST, SOUTH LABRADOR SEA:
WNG: NIL.
WND: NE15-20. 14/00Z NE25.
VIS: 13/13Z-15/03Z 0-1 LGT-SN.
NORTH LABRADOR COAST, NORTHWEST LABRADOR SEA-W:
WNG: FREEZING SPRAY.
WND: N25. 14/03Z N15. 14/18Z NW25.
SPRAY: 13/13Z-14/03Z MOD OVR-OW. 14/18Z-15/03Z MOD.
VIS: 13/13Z-14/03Z 0-1 LGT-SN.
NORTHWEST LABRADOR SEA-E:
WNG: NIL.
WND: LGT. 14/21Z N25.
EAST LABRADOR SEA:
WNG: NIL.
WND: LGT. 14/09Z N15.
WAVES(M) VLD 13/09Z-15/03Z
STRAIT OF BELLE ISLE, BELLE ISLE BANK - WESTERN HALF:
MAINLY ICE COVERED.
BELLE ISLE BANK - EASTERN HALF:
2-3 OVR-OW. 13/18Z 3-4
WAVES(M) VLD 13/09Z-15/03Z
SOUTH LABRADOR COAST, MID LABRADOR COAST, NORTH LABRADOR COAST, SOUTH
LABRADOR SEA - WESTERN HALF, NORTHWEST LABRADOR SEA - WESTERN HALF:
MAINLY ICE COVERED.
SOUTH LABRADOR SEA - EASTERN HALF, NORTHWEST LABRADOR SEA - EASTERN
HALF:
2-3 OVR-OW. 13/12Z 1-2. 14/09Z 2-3
EAST LABRADOR SEA:
2-3 13/12Z 1-2
END
FPUS64 KEWX 141351 AAA
SFTEWX

TXZ168>173-183>194-202>209-217>225-228-150451-

TABULAR STATE FORECAST FOR SOUTH CENTRAL TEXAS...UPDATED
NATIONAL WEATHER SERVICE AUSTIN/SAN ANTONIO TX
851 AM CDT THU OCT 14 2004

ROWS INCLUDE...
   DAILY PREDOMINANT DAYTIME WEATHER 6AM-6PM
   FORECAST TEMPERATURES...EARLY MORNING LOW/DAYTIME HIGH
         PROBABILITY OF PRECIPITATION 6AM-6PM
          - INDICATES TEMPERATURES BELOW ZERO
         MM INDICATES MISSING DATA


   FCST     FCST     FCST     FCST     FCST     FCST     FCST     
   TODAY    FRI      SAT      SUN      MON      TUE      WED      
   OCT 14   OCT 15   OCT 16   OCT 17   OCT 18   OCT 19   OCT 20   

......AUSTIN/SAN ANTONIO CORRIDOR......
   AUSTIN
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /73    47/83    57/85    62/90    61/87    64/84    66/84    
   POP 10   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

   GEORGETOWN    
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /71    46/81    58/84    65/88    62/86    65/83    67/82    
   POP 10   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

   NEW BRAUNFELS 
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /74    51/79    58/85    65/87    61/86    65/86    67/84    
   POP 20   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

   SAN ANTONIO   
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /75    54/82    61/85    65/88    62/86    67/84    69/83    
   POP 20   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

   SAN MARCOS    
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /74    49/83    58/86    63/89    61/86    64/85    66/85    
   POP 20   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

......HILL COUNTRY......
   BURNET
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /71    45/82    54/82    63/87    60/84    63/83    65/81    
   POP 10   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   

   FREDERICKSBURG
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /70    49/80    55/84    59/87    57/84    60/82    62/81    
   POP 10   POP 0    POP 0    POP 10   POP 10   POP 10   POP 10   

   KERRVILLE     
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /70    49/80    57/85    59/87    56/83    60/82    62/81    
   POP 10   POP 0    POP 0    POP 10   POP 10   POP 10   POP 10   

......OTHER LOCATIONS IN SOUTH CENTRAL TEXAS......
   DEL RIO
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /77    55/87    62/87    62/89    59/86    64/86    66/85    
   POP 30   POP 0    POP 0    POP 10   POP 10   POP 10   POP 10   

   HONDO         
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /76    49/84    56/85    62/89    58/85    63/85    65/83    
   POP 30   POP 0    POP 0    POP 10   POP 10   POP 10   POP 10   

   LA GRANGE     
   PTCLDY   SUNNY    PTCLDY   PTCLDY   PTCLDY   PTCLDY   PTCLDY   
     /73    51/83    59/84    68/92    68/85    67/86    69/85    
   POP 30   POP 0    POP 0    POP 10   POP 10   POP 10   POP 20   


$$
QUESTION: 
What types of commands will you be able to send to the rover (like forward,
turn, right, stop, etc.)? How detailed will your control be?
 
ANSWER from David Mittman on August 12, 1997:
Good question! Here is a list of many of the commands that the Rover
understands. This listing gives only the letters which represent the command
parameters (for instance, "CAMERA c" where 'c' is Left, Right, or Rear). If
you are interested in additional details for some commands, please let me
know.

ABORT SEQUENCE 
APPLY PATCH SET s LENGTH n 
CALIBRATE HEADING WITH SUN AT h USING CAMERA c BY TIME t 
CALL FUNCTION AT ADDRESS a WITH BANKS b1, b2 [PARAMETERS p1 p2 ...] 
CAPTURE IMAGE WITH CAMERA c AT EXPOSURE t, RETURN REGION FROM (r1,c1) TO 
     (r2,c2) WITH APID a [compressed] 
CLEAR c
DRIVE MOTORS
DEPLOY APXS p 
END OF SEQUENCE
FIND ROCK NEAR x y WITHIN m MINUTES 
GO TO WAYPOINT AT x y WITHIN m MINUTES 
HEALTH CHECK AT LEVEL n
HEAT FOR n MINUTES IN SEQUENCE s [s ...] 
LIMIT-CALIBRATE POSITION SENSORS 
MATERIAL ADHERENCE
MOVE BACKWARD n COUNTS 
MOVE FORWARD n COUNTS 
OUTPUT x TO PORT p
PATCH MEMORY SET s CRC c SEGMENT b ADDRESS a TO x x x ...
POSITION APXS 
READ ANALOG CHANNEL c AT GAIN g [ c AT g ... ]
READ BYTES FROM PORT p p p ...
READ n BYTES FROM SEGMENT s ADDRESS a
RUN MOTOR m FOR t CENTONS 
RUN MOTOR m TO p
SEND APXS COMMAND c
SET CLOCK TO t
SET DEVICE d STATUS s 
SET ERROR MASK TO m
SET MISSION PHASE p 
SET PARAMETER p = value
SET VEHICLE POSITION TO x y, HEADING TO h 
SHUTDOWN UNTIL t
SOIL MECHANICS TEST ON WHEEL w AT POSITION p, RUN FOR n COUNTS, REPEAT k TIMES 
SYNCHRONIZE CLOCK
TEST n BYTES OF MEMORY IN SEGMENT s AT ADDRESS a
TURN LEFT n BAMS 
TURN OFF DEVICES d 
TURN ON DEVICES d 
TURN RIGHT n BAMS 
TURN TO HEADING h 
TURN TOWARD x, y 
UNSTOW p d c l r 
WAIT FOR s SECONDS
WAIT UNTIL LOCAL TIME t
WAIT UNTIL MISSION TIME t
WAIT UNTIL s < v, LIMIT m 
WAIT UNTIL s > v, LIMIT m 
WHEEL ABRASION MEASUREMENT AT GAIN g 
ZERO-CALIBRATE POSITION SENSORS 

ANSWER from Bridget Landry on October 6, 1997: 
We can command the rover at a variety of detail levels.  Because there is
onboard autonomy, there is a command "find rock" and one called "go to way
point".  These commands have parameters which include the coordinates for a
target (either the rock to take a measurement of the the "way point" to aim
for); the rover then computes the best path to get to that target.  However,
we can also give very detailed commands along the lines of "back up one
meter" or "turn 70 degrees to the right". Early in the mission, we used more
detailed commands, but we have now used many of the more general commands,
trusting that the onboard autonomy capabilities will perform properly.

Bridget Landry
Deputy Uplink System Engineer
Mars Pathfinder
WHY MIDAS FAILED
upon the bunk, impatiently. "What about afterwards?"
"We will find a way into Siberia or China where we can enjoy our hard-earned gold," with a sarcastic emphasis upon the three last words of his sentence, but laughing lightly.
"There is no reason you should not do this," was the reply, "but with me it is different. I am ill, and daily growing weaker. This isolation and enforced inaction takes the life out of me; my head grows dizzy from much thinking, and I see forms, spectres, and hobgoblins in all shapes and colors," this was said complainingly and in a weakened voice.
"My dreams are so horrible that I dread the prospect of night."
"You're a fool to worry. Keep a stiff upper lip, and all will be well. See, I'm making a checker-board with which we can kill time when we like."
"I'd like to kill the whole of it before it kills me," was the response. "If I only had something to read or something to do. I'm sick of this infernal hole!"
"Ditto here, but what can we do? If we push on eastward now we will probably be 165
List of files in the package
 ----------------------------

 ga.for - source code for 'main' and other routines including the routine
          that computes the conservation score for each structure

 gtstr.for - source code for generating the inial population of structures

 mga.for - miscellaneous subroutines

 mutat.for - source code for the mutation operation

 xovr.for - source code for the crossover operation

 gtmseq.for - program to read multiple sequences

 efn.for - program to compute the energy (Zuker's program)

 ergparm - energy parameters

 gtrerg.for - program to compute the average random energy and its standard
              deviation based on the base composition

 cf20, f30, cf50, cf100, and cf150 - empiracal energy coefficients used
                                     by the program gtrerg.for