BEE-spoke-data/govdocs1-by-extension huggingface dataset:
May 10, 1996
                                                        Linda Stutte

           Minutes from the Meson 120 Working Group Meeting

Attendees: Jeff Appel, Win Baker, Greg Bock, Chuck Brown, Peter Cooper,
           Mike Crisler, Gaston Gutierrez, Dan Kaplan, Valery Kubarovsky,
           Paul Lebrun, Anthony Malensek, Stan Pruss, Sunil Somalwar,
           Linda Stutte

General discussion:  Our charge is to investigate whether experiments using
  largely existing equipment can do competitive physics in the Meson Area
  with 120 GeV beam extracted from the Main Injector, starting around the
  year 2000.  The Meson Area was originally sized for a 200 GeV proton beam, 
  and it's interior layout is quite flexible. Chuck Brown showed secondary 
  flux estimates which demonstrated the advantages of Fermilab over BNL quite
  clearly (orders of magnitide) at higher energies.  Even for 6 GeV Kaons,
  the BNL  x6 protons on target is offset by the Fermilab x6 production rates
  due to enhanced fluxes at low x.  Longer targets can further enhance low
  energy production, and Kaon production, for example, can be optimized
  by running at higher Pt, where beam fractions as high as 1/3 have been
  observed.  

Competition:  Brookhaven is sponsoring a workshop next week (AGS2000) to 
  explore many of these same physics issues, with the possibility of running
  the AGS for other physics after RHIC injection.  Greg Bock will be giving a
  presentation during the first day plenary session on the Fermilab 120 GeV
  program.  The Japanese 50 GeV Kaon Factory is also targetting some of these
  same topics, but on a later time scale (2004/5).  Presumably, the SPS could
  also be competitive. 

So far:  Approximately two dozen individuals have responded to our initial
  solicitation of interest.  Responses ranged from general interest to
  specific topics, such as rare Kaon decays, light quark spectroscopy, exotic
  atom production, polarized physics, tagged neutrino studies and offers 
  of useful existing equipment. Two Expressions of Interest have been received,
  one for a rare kaon decay experiment (CKM), K+ -> pi+ nu nubar, the other for
  a study of exotic atoms using a crystal spectrometer.  Numerous past 
  resources are available to draw on, including the '89 Breckenridge study, 
  three workshops (Santa Fe/Fermilab/BNL) on Future Directions in Particle and
  Nuclear Physics in '93, and the output from the Fermilab Fixed Target 
  Working Group in '95.  

Where do we go from here:  Chuck Brown will set up a home page for our working
  group and get pointers to it.  We will add relevant materials.  We plan to
  meet every other week at 12:30 - 1:30 in WH10NE, with the goal of organizing
  a workshop later this year focussed on the relevant physics issues.  Next
  meeting will include reports from Greg Bock and Gaston Gutierrez on AGS2000,
  a report on the CKM Expression of Interest from Peter Cooper, and a discussion
  of a possible light quark spectroscopy experiment from Paul Lebrun.
%sub file of vmefpga1, as clock, feb_data and sigle/double frame switch 9/26/00%
subdesign sw_mode           
(    v_add[13..6],         %raw vme address %
     st15,                 
     CLK                    %switched clock%
                      :input;
     clk_sel,              %clock select to muxfpga%
     data_sel,             %data select to muxfpga %
     v_control             %double frame indicator to muxfpga%
                     :output;
)
variable
     clk_sw:  latch;
     C_DELAY:  DFF;
     PH     : DFFE; %gated clock with 1/2 CLK rate% 
     data_sw:  latch;
     frame_sw: latch;
begin
     %single/double frame switch%
frame_sw.ena = st15 & ((v_add[13..11] == 5) # (v_add[13..11] == 6)) ;
frame_sw.d   = (v_add[13..11]==5) & ((v_add[9..6]==5) # (v_add[9..6]==6)
              # (v_add[9..6]==7)) 
            # (v_add[13..11] == 6) & (v_add[9..6]==1); 
V_CONTROL =  frame_sw.q;         %V_CONTROL=1, DOUBLE FRAME%

     %clock switch%
 PH.CLK     = CLK; 
 PH.ENA = (v_add[13..11]==5) # (v_add[13..11]==6);
 PH.D       = !PH.Q;
 CLK_SW.ENA =st15 & !CLK & ((v_add[13..11] == 5) # (v_add[13..11] == 6)) ;
 CLK_SW.D   = (v_add[13..11] == 5) & ((v_add[9..6]   == 1) # (v_add[9..6]==3)
               # (v_add[9..6]==7));
  
 C_DELAY.CLK  = PH.Q;
 C_DELAY.D    = CLK_SW.Q;
 CLK_SEL   =  C_DELAY.Q;          %clk_sel=1, offline is selected%

    %data_sel switch%
 data_sw.ena = st15 & ((v_add[13..11] == 5) # (v_add[13..11] == 6));
 DATA_SW.D   = (v_add[13..11] == 5) &((v_add[9..6]== 2) # (v_add[9..6]== 3)
               # (v_add[9..6]==7)); 
 DATA_SEL   =  DATA_SW.Q;        %data_sel=1, offline is selected%
end;
TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  1164
SUBJECT: GRB 011121: J-band observations
DATE:    01/11/29 23:13:15 GMT
FROM:    Saurabh Jha at Harvard-Smithsonian CfA  <sjha@cfa.harvard.edu>

M. M. Phillips (Carnegie), K. Krisciunas (CTIO), P. M. Garnavich,
S. Holland (Notre Dame), S. Jha, K. Z. Stanek (Harvard-Smithsonian
CfA) and P. McCarthy (Carnegie) report:

We have observed the field of GRB 011121 with the 6.5m Magellan I
Baade telescope (+ IR imager) on UT 2001 Nov 29.3 for a total of 
4320s in the Js passband with 0.5" seeing in the combined image.

A finder chart of the combined image is available at:
http://cfa-www.harvard.edu/cfa/oir/Research/GRB/.

The data have been calibrated via three IR standard stars also
observed over the course of the night, from the list of Persson et al.
(1998, AJ, 116, 2475). The Js passband is slightly narrower than the
standard J, but we make no color correction and adopt Js = J because
we lack sufficient data (both for the standard stars and the objects
in the GRB field). The effects of the slight filter mismatch are
expected to be small (see, for example, Krisciunas et al. 2001, AJ,
122, 1616). For the bright stars marked in the finder, we measure J =
17.82 +/- 0.03 (star D) and J = 18.59 +/- 0.03 (star E).

A source at the position of the GRB afterglow is marginally detected,
but because of its faintness, it is difficult to separate a possible
point source from the underlying fuzz. Differential PSF-fitting
photometry relative to the bright stars in the field yields J = 21.9
+/- 0.1 for the source at the position of the GRB afterglow. Because
of the marginal detection, this should be viewed as an upper limit.

Two other sources are detected near the GRB position. One bright
source is located 0.8"S and 2.0"E of the GRB with J = 19.98 +/- 0.04.
This object may be the core of the GRB host galaxy, but it is not
clearly resolved -- it might be a foreground star. The other source
(the "blob") located 1.6"S and 2.6" E of the GRB is clearly detected
at J = 21.57 +/- 0.07, and is possibly extended.

Adopting J ~ 16 mag for the GRB afterglow on Nov 22.36 (GCN 1153), the
reported optical decay slope (GCN 1160) would predict J ~ 21 for the
afterglow at the time of these observations.

This message may be cited.
Comment 0419875

From: xxpankoxx@aol.com
Sent: Wednesday, August 10, 2005 12:39 PM
To: Rulemaking, TTB
Subject: Notice No. 41: Labeling and Advertising of Wines, Distilled
Spirits and Malt Beverages

U.S.  TTB
 

Dear U.S.  TTB,

Today, Americans have more choices than ever when deciding what to drink, whether it's a soda, a beer, a glass of wine, or a cocktail. With so many choices, it's only logical that the bottles and cans they drink from provide consistent and accurate nutritional and serving information on their packaging. 

American consumers have long relied on such information on everything from salad dressings to ice creams and it is time that Americans are provided with important serving information for alcohol beverages also. 

The aim of having serving information on most consumable products is to promote an overall balanced lifestyle. Alcohol cannot be exempt as it is a normal part of many Americans'
lifestyles. With greater understanding of how the drinks they prefer can be consumed responsibly, more Americans could be able to make more informed decisions when enjoying their favorite drink. 

I hope you will allow basic serving information, including serving size, servings per container, alcohol per serving, calories, fat, carbohydrates, and protein values to appear on drink bottles. 

Thank you for your consideration. 

Sincerely,

Miguel Gonzalez
10565 sw 109 st
miami, Florida 33176
 cc: 
Representative Lincoln Diaz-Balart
Senator Bill Nelson
Senator Mel Martinez
Director Pat Parmer
000
WWUS72 KTAE 232106
NPWTAE

URGENT - WEATHER MESSAGE
NATIONAL WEATHER SERVICE TALLAHASSEE FL
506 PM EDT SUN OCT 23 2005

...AN INLAND TROPICAL STORM WARNING IS IN EFFECT FOR DIXIE COUNTY
IN THE SOUTHEAST FLORIDA BIG BEND...

.HURRICANE WILMA...CURRENTLY 210 MILES WEST SOUTHWEST OF KEY WEST
FLORIDA...IS FORECAST TO MAKE LANDFALL IN SOUTHWEST FLORIDA BY
MONDAY MORNING. WILMA IS A LARGE HURRICANE...WITH TROPICAL STORM
FORCE WINDS EXTENDING OUT UP TO 230 MILES FROM THE CENTER. IF
WILMA MAKES LANDFALL AS EXPECTED... SUSTAINED TROPICAL STORM FORCE
WINDS OF 40 MPH COULD AFFECT DIXIE COUNTY TONIGHT AND MONDAY.

FLZ034-242000-
/X.EXT.KTAE.TI.W.0001.051024T0000Z-051024T2000Z/
DIXIE-
INCLUDING THE CITY OF...CROSS CITY
506 PM EDT SUN OCT 23 2005

...INLAND TROPICAL STORM WARNING NOW IN EFFECT FROM 8 PM THIS
EVENING TO 4 PM EDT MONDAY FOR DIXIE COUNTY IN THE SOUTHEAST 
FLORIDA BIG BEND...

THE NATIONAL WEATHER SERVICE IN TALLAHASSEE HAS CONTINUED THE
INLAND TROPICAL STORM WARNING...WHICH IS IN EFFECT FROM 8 PM THIS
EVENING UNTIL 4 PM MONDAY AFTERNOON. AS LARGE HURRICANE WILMA
APPROACHES THE SOUTHWEST FLORIDA COAST TONIGHT...SUSTAINED
TROPICAL STORM FORCE WINDS OF 40 MPH...WITH HIGHER GUSTS...WILL
BE POSSIBLE ACROSS DIXIE COUNTY...ESPECIALLY ALONG THE IMMEDIATE
COAST. IF WILMA MOVES A LITTLE FARTHER SOUTH THAN CURRENTLY
FORECAST...TROPICAL STORM CONDITIONS WILL LIKELY NOT REACH DIXIE
COUNTY.

AN INLAND TROPICAL STORM WARNING MEANS WINDS OF 39 TO 73 MPH ARE
EXPECTED DUE TO A LANDFALLING HURRICANE OR TROPICAL STORM. IN THIS
CASE...THE HIGHEST WINDS ARE NOT EXPECTED TO EXCEED 45 MPH. WINDS
OF THIS MAGNITUDE TYPICALLY CAUSE SPORADIC POWER OUTAGES... A FEW
FALLEN TREES...AND HAZARDOUS DRIVING CONDITIONS FOR HIGH PROFILE
VEHICLES.

$$

GODSEY
SJ_GR850   
St. Joseph, MO    Tue Feb 10, 2009    USDA-MO Dept Ag Market News

Daily National Grain Market Summary

   Grain and soybean bids were slight to moderate lower despite supportive USDA 
supply/demand report.  Wheat was pressured by the sharp declines in the stock 
market, along with lower crude oil.  Corn and soybeans retreated as rain was 
forecasted in Argentina.  Wheat was 4-9 cents lower.  Corn was mostly 1-2 cents 
lower.  Sorghum was 1 cent lower.  Soybeans were 6-11 cents lower.

                             DATE           CHANGE              YEAR AGO
TRUCK BIDS:                  02/10/09       02/09/09            02/12/08

Wheat:                                                           
   Kansas City (HRW ORD)     5.49-5.52      dn 6               10.06
   Minneapolis (DNS)         6.95 1/2       dn 5 3/4           17.32 1/2
   Portland (SWW)            5.65-5.71      dn 5-14             n/a
   St. Louis (SRW)           4.56           dn 4                9.24
 
Corn, US No 2 Yellow:    
   Kansas City               3.70-3.74      dn 1                4.93
   Minneapolis               3.48 3/4       dn 3/4              4.64 3/4
   So. Iowa               3.49 3/4-3.62 3/4 dn 3/4-up 1 1/4 4.74 3/4-4.75 3/4
   Omaha                     3.62-3.67      up 1-dn 1           4.63-4.76
             
Soybeans, US No 1 Yellow:                
   Kansas City               9.89           dn 8               12.36
   Minneapolis               9.49           dn 8               No Bid
   So. Iowa                  9.63-9.71      dn 8-11            12.56
   Cent. Il Processor        9.89-10.09     dn 8               12.71-12.85

FUTURES:                                                                
   Kansas City (Mar) Wheat     5.89         dn 6               10.45 1/2
   Minneapolis (Mar) Wheat     6.53 1/4     dn 5               16.73
   Chicago     (Mar) Wheat     5.56         dn 9               10.07
   Chicago     (Mar) Corn      3.76 3/4     dn 3/4              4.97 3/4
   Chicago     (Mar) Soybeans  9.94         dn 8               13.21

*EXPORT BIDS:  Barge bids out of the Port of New Orleans, or Rail out of the 
North Texas Gulf.  Bids per bushel, except sorghum per cwt.

US 1 HRW Wheat, Ord Protein:            
     Rail    6.12-6.54               dn 6                  10.85 1/2-10.95 1/2
US 2 Soft Red Winter Wheat:                                 
     Barge   5.11-5.16               dn 6-9                    10.17-10.37
2 Yellow Corn:                
     Barge   4.26 3/4-4.29 3/4       dn 3/4-2 3/4           5.39 3/4-5.41 3/4
US 2 Sorghum    
     Rail    6.73-6.91               dn 1                       9.51-9.69
     Barge   6.67 1/2-6.72 3/4       dn 1 1/4               9.33 1/2-9.87
US 2 Yellow Soybeans   
     Barge   10.54-10.57             dn 7-6                    13.61-13.66

SOURCE:  USDA- MO Dept OF Ag Market News Service, St. Joseph, MO
         Baldemar Ortiz, Market Reporter (816)238-0678
         www.ams.usda.gov/LSMarketNews 
              
1516     bro

.
FBSUB (Mar97)                  ftools.xte                  FBSUB (Mar97)

NAME
    fbsub -- Subtracts a baseline (unpulsed  contribution)  from  an  fB
    histogram.
    
    
USAGE
    fbsub infile outfile phasemin phasemax clobber
    
    
DESCRIPTION
    fbsub  allows  the  user to specify one or two phase ranges that are
    considered to be  free  of  pulsed  signal,  and  to  use  these  to
    determine  the  background,  or baseline (unpulsed), spectrum.  This
    spectrum is then subtracted from the counts stored in  the  fB  file
    to   yield   a  background-  subtracted  pulsed  lightcurve/spectrum 
    two-dimensional histogram.
    
    Input is an fB file; output is an fB file, too.  It does not hurt to
    apply fbsub multiple times, though it does not do much good, either:
    the result is the same as when the  last  fbsub  run  was  performed
    directly  on  the  original  input  fB  file.  Errors are propagated
    rigourously.
    
    
PARAMETERS
    
    infile [string]
        Name of the input fB file (produced by fasebin).
    
    outfile = fBsub.pha [string]
        Name of the baseline-subtracted fB file.
    
    phasemin = 0.0 [double] 
        With phasemax, sets the range of phases to be used to  determine
        the unpulsed contribution.
    
    phasemax = 1.0 [double] 
        With  phasemin, sets the range of phases to be used to determine
        the unpulsed contribution.   phasemax  should  be  greater  than
        phasemin and may exceed 1.0.
    
    (phasemin2 = -100.0) [double]
        With  phasemax2,  sets  an optional second range of phases to be
        used to determine the  unpulsed  contribution.   Negative  value
        indicates that no second range is to be used.
    
    (phasemax2 = -100.0) [double] 
        With  phasemin2,  sets  an optional second range of phases to be
        used to determine the unpulsed contribution.   phasemax2  should
        be greater than phasemin2 and may exceed 1.0.
    
    (clobber = yes) [boolean]
        Should a pre-existing output file be overwritten?
    
    (mode = ql) [string]
        FTOOLS internal -- users should not need to change.
    
    
EXAMPLES
    
    
NOTES:
    See the help file for FASEBIN for details.
    
    
BUGS
    
    Please report problems to xtehelp@athena.gsfc.nasa.gov.
    
    
SEE ALSO
    FASEBIN FBADD FBFSUM FBSSUM
#
# Specify some environment variables to adjust ciod behavior
#

# Set buffer size for reads and writes.
# working values:
# up to 14680064 has been tested sucessfully.  16777216 does not work,
# presumably because it's too much memory for a 512 MB IO node servicing 32
# compute nodes (512/32 = 16). 

# 4MB is a good everyday setting, and gives good performance
export CIOD_RDWR_BUFFER_SIZE=4194304
# this larger value will give you somewhat better perfomrance for large bulk
# i/o transfers, but consumes a lot (50%) of memory
# export CIOD_RDWR_BUFFER_SIZE=8388608

# Startup debug sockets.
#export DEBUG_SOCKET_STARTUP=ALL

# are there any other environment variables we can set?
# there appear to be two undocumented environment variables (based on 'strings
# ciod_fl.440):
# CIOD_TREE_RECV_RETRY
# CIOD_TREE_TIMEOUT
Comments for Review of NuMI Primary Beamline
                        System Design and Instalation
                           July 18, 2001

                   from  Dave Pushka
                       ------------------------

1. Overall Remarks

Well, I didn't see any obvious holes or gaps in what was presented.
Clearly this is a work in progress and as long as progress continues
(especially on the engineering of the stands in the NuMI stub) we should
be okay in that the stands should never be on the critical path.

However, it is troubling and should be considered a warning that the
individual who is charged with working on the engineering of the NuMI Stub
stands was not able to present his own material at the review because of
other problems in the tunnel needing his attention.  I note that this area
is also the only place where any problems were identified (the stand
occluding the door).  Hmm.

Once the engineering is completed, the cost estimates should be quite
firm, but not before.


2. Itemized suggestions, questions and concerns

(1) It is not clear what mechanism is to be used for safety reviews of
the stands and material handling equipment.  It would be nice to be able
to provide the engineering note (calculations, assembly drawings, etc) to
a safety committee for an independant review.



(2) While not really a hugh deal nor anywhere near a potential show
stopper, the installation equipment used for installing the pre-target
magnets needs to be identified, procedures written, and hazard analysis
performed.  This will likely use a custom designed cart with a cable to
pull it up hill and a built in crane to lift the magnets into position and
set tehem down on to the stands.  Use of a rack and pinion drive (cogged
railroad) would be extreamly costly.  Still, there is 6 months + of
engineering effort here.



(3) A hazard analysis and installation procedure in needed for installing
the magnets in the NuMI Stub and the extension.


(4) No obvious objections were raised about our decision to use completely
manual cranes for handling the magnets in the stub.  Good.  However, I
note the complete absence of technicians on this review committee: no
John Voirin, Dave Erickson, Dave Augustine types.  Opinions from people
with DIRECT hands on experience using cranes to install magnets would have
been most welcome.


(5) Vertical orientation of the adjusters for the angled magnets avoid
putting ANY horizontal load on to the adjusters.  Not only is this good,
it is necessary.
*Pages 1--2 from  Microsoft Word - 40584*
 PUBLIC  NOTICE
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 DA  04-  2317  July  27,  2004
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 REGION  7  (COLORADO)  700  MHz  PUBLIC  SAFETY  PLANNING  COMMITTEE  ANNOUNCES  PLANNING  MEETING
 The  Region  7  (Colorado)  700  MHz  Public  Safety  Planning  Committee  announces  that  the  next  planning  meeting  will  be  held  on  Wednesday,  September  8,  2004  at  3:  30  p.  m.,  at  the  Montrose
 Fire  Department,  441  South  Uncompahgre  Avenue,  Montrose,  Colorado.  The  purpose  for  this  meeting  is  to  review  the  regional  plan  for  700  MHz  and  4.9  GHz  spectrum  use  as  prepared  by  the
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 Administrators  who  are  not  oriented  in  the  communications  field  should  delegate  someone  with  this  knowledge  to  attend,  participate  and  represent  your  agencys  needs.
 All  interested  parties  wishing  to  participate  in  the  planning  for  the  use  of  either  the  new  public  safety  spectrum  in  the  700  MHz  band  and/  or  the  newly  allocated  4.9  GHz  band  within  Region  7
 are  encouraged  to  attend.  Those  planning  to  attend  are  asked  to  RSVP  one  of  the  contact  persons  listed  below.  For  further  information  about  the  meeting,  please  contact:
 Emery  L.  Reynolds,  Chairman  Region  7  700  MHz  Public  Safety  Planning  Committee
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 Phone:  720-  898-  6667  Email:  mark-  s@  arvadaagov.  org
 -  FCC  -
2
STS-97
Report # 16 
 Friday, Dec. 8, 2000  9 a.m. CST 
 
 The International Space Station recorded another milestone today  the
arrival of its first houseguests.

The crew of the Space Shuttle Endeavour and the stations Expedition 1
crew opened the hatches of their respective spacecraft at 8:36 a.m. CST
Friday.  Station Commander Bill Shepherd, Pilot Yuri Gidzenko and Flight
Engineer Sergei Krikalev shook hands with their first station guests in 38
days -- STS-97 Commander Brent Jett, Pilot Mike Bloomfield and Mission
Specialists Marc Garneau, Carlos Noriega and Joe Tanner.

The meeting was the first face-to-face contact between the crews, even
though their spacecraft have been docked together since last Saturday,
orbiting the planet at an altitude of 230 statute miles. At least one
hatch remained closed at all times to maintain different atmospheric
pressures so that the shuttle crew could conduct three spacewalks and
succeed in its primary mission objectives, the delivery, installation and
activation of the first U.S. solar power system for the International
Space Station.

The new solar arrays are working well, converting the Suns rays into
electricity and providing an average of 13 kilowatts of additional energy
for use by the space station, supplementing the power supplied by solar
arrays on the Russian Zarya and Zvezda modules. Other station systems,
including a carbon-dioxide removal system and an air conditioner that
failed earlier in the week but were repaired by the station crew, are
working well.

After a short welcoming ceremony and safety briefing, the eight
spacefarers got right to work conducting joint activities including
structural tests of the station and its solar arrays, transfer of
equipment, supplies and refuse back and forth between their two spacecraft
and checking out a television camera cable that will help the next shuttle
crew deliver and install the stations first laboratory module, Destiny.

A joint crew news conference is scheduled for 10:31 a.m. CST today.

The space station crew is scheduled to go to bed about 6 p.m. CST, and the
shuttle crew a little later about 10 p.m.

The next STS-97 status report will be issued Friday evening.
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","001q.gif","1","1","","001r.jpg|001a.tif"
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","002q.gif","2","2","","002a.tif"
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","003q.gif","3","3","","003a.tif"
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","004q.gif","4","4","","004a.tif"
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","005q.gif","5","5","","005a.tif"
"The campaign polka / composed and respectfully dedicated to the Philadelphia Liberty Cornet Band by Mary E. Walsh.","","scsm018/scsm0189","006q.gif","6","6","","006a.tif"
Seelye, J. G., Marking, L. L., King, E. L. Jr., Hanson, L. H.,, and Bills, T. D.,
1987, Toxicity of TFM lampricide to early life stages of walleye: North American
Journal of Fisheries Management, v. 7, no. 4, p. 598-601.

Abstract: 

The authors studied the effects of the lampricide 3-trifluoromethyl-4-nitrophenol
(TFM) on gametes, newly  fertilized eggs, eyed eggs, larvae, and swim-up fry of
the walleye Stizostedion vitreum . When gametes from  sexually mature walleyes
were stripped into solutions of TFM, no effects were observed during the
fertilization  process at concentrations up to 3.0 mg/L - three times the
concentration lethal to 99.9% of larval sea lampreys  Petromyzon marinus  held
12 h (LC99.9) under the same test conditions. Newly fertilized eggs likewise were 
unaffected during water hardening by concentrations of TFM that were lethal to
sea lamprey ammocoetes. Eyed  eggs, sac fry, and swim-up fry yielded LC25
values that were 2.5 to 5 times greater than the 12-h LC99.9 for sea  lamprey
ammocoetes. The data thus indicated that all of the early life stages of walleyes
tested were considerably  more resistant than sea lamprey ammocoetes to TFM,
and that it is unlikely they would be adversely affected by  standard stream
treatments to kill sea lamprey ammocoetes.

Keywords: 

TFM, toxicity, eggs, larvae, pesticides, fry, Stizostedion-vitreum, fish-eggs,
fish-larvae, lampricides
000
NOUS42 KFFC 051933
PNSFFC
GAZ001>009-011>016-019>025-027-030>039-041>062-066>076-078>086-
089>098-102>113-060745-

PUBLIC INFORMATION STATEMENT
NATIONAL WEATHER SERVICE PEACHTREE CITY GA
333 PM EDT THU APR 5 2007

...PUBLIC INFORMATION STATEMENT...

...RECORD OR NEAR RECORD LOWS EXPECTED THIS WEEKEND...

A STRONG COLD FRONT PUSHED THROUGH THE AREA ON WEDNESDAY...AND A
VERY STRONG CANADIAN HIGH IS MOVING INTO THE REGION FOR THE
WEEKEND. EXTREMELY COLD LOW TEMPERATURES ARE FORECAST FOR THE
AREA THAT MAY BREAK RECORDS THAT HAVE HELD FOR MORE THAN HALF A
CENTURY AT SOME LOCATIONS...AND MORE THAN A CENTURY FOR ATLANTA.

THE FOLLOWING IS A LIST OF RECORD LOWS FOR THIS WEEKEND FOR THE
CLIMATE STATIONS IN THE PEACHTREE CITY FORECAST AREA.

FOR ATLANTA...RECORDS HAVE BEEN KEPT SINCE 1878.
APRIL 5...28 DEGREES SET IN 1881
APRIL 6...28 DEGREES SET IN 1891
APRIL 7...29 DEGREES SET IN 1982
APRIL 8...32 DEGREES SET IN 1886
APRIL 9...32 DEGREES SET IN 2000

FOR ATHENS...RECORDS HAVE BEEN KEPT SINCE 1898.
APRIL 5...29 DEGREES SET IN 1944 
APRIL 6...27 DEGREES SET IN 1944 
APRIL 7...28 DEGREES SET IN 1950 
APRIL 8...32 DEGREES SET IN 1990
APRIL 9...32 DEGREES SET IN 2000

FOR MACON...RECORDS HAVE BEEN KEPT SINCE 1899.
APRIL 5...32 DEGREES SET IN 2000
APRIL 6...32 DEGREES SET IN 1944 
APRIL 7...31 DEGREES SET IN 1950 
APRIL 8...30 DEGREES SET IN 1990 
APRIL 9...32 DEGREES SET IN 2000

FOR COLUMBUS..RECORDS HAVE BEEN KEPT SINCE 1948.
APRIL 5...34 DEGREES SET IN 1987
APRIL 6...35 DEGREES SET IN 1966 
APRIL 7...28 DEGREES SET IN 1950 
APRIL 8...32 DEGREES SET IN 1950 
APRIL 9...34 DEGREES SET IN 2000

$$
FIFTH GROUP OF INTERVIEWEES PARTICIPATE IN SELECTION PROCESS

December 1, 1997

Eileen M. Hawley
Johnson Space Center
(281) 483-5111

<h4>Release: J97-40</h4> <h3>Fifth Group of Interviewees Participate 
in Selection Process</h3> 

The fifth of several groups of prospective astronauts will visit the 
Johnson Space Center (JSC) the week of December 5 for interviews, 
orientation and medical evaluations as the astronaut selection 
process continues.

Approximately 100 candidates selected from more than 2,600 applicants, 
are expected to be interviewed through December for a chance to be 
among those named as astronaut candidates for the class of 1998. The 
final selections will be announced in early 1998 with the new class 
reporting next summer.

The fifth group of 21 applicants includes: Christopher A. Apblett, 
Ph.D., Austin, TX; Tucker R. Balch, Atlanta, GA; Michael R. Barratt, 
M.D., League City, TX; Barbara K. Craig, Ph.D., Austin, TX; Richard 
M. Davis, League City, TX; Michael P. DeMasie, Houston, TX; John F. 
Donovan, Ph.D., Manchester, MO; William A. Ehrenstrom, Houston, TX; 
E. Michael Engle, Houston, TX; Deborah L. Falley, San Diego, CA; 
Ellis C. Gayles, Ph.D., Aurora, CO; Gardell G. Gefke, Bethesda, MD; 
Laura H. Hembree, League City, TX; Gregory C. Johnson, Friendswood, 
TX; Smith L. Johnston, M.D., Houston, TX; Stanley N. Koszelak, Ph.D., 
Riverside, CA; Christopher K. Salvino, M.D., Orland Park, IL; William 
J. Spiesman, Ph.D., Austin, TX; Richard S. Stapp (Major, USAF), 
Colorado Springs, CO; Joseph S. Stich, League City, TX; and Thomas A. 
Sullivan, Ph.D., Houston, TX.

Astronaut candidate selections are conducted approximately every two 
years with the number of candidates selected depending on Space 
Shuttle flight rates, overall program requirements and astronaut 
attrition rates.

	
-end-
Submitted Data file =  98081dat.wb1 (renamed to nutrients-proc-1998-081.txt)
Cruise: PROC-1998-081
Ship: R/V Laurentian
Cruise Dates:  March 22 - April 3, 1998
PI: Tom Johengen   Ph#: 734-741-2203   Email:  tom.johengen@noaa.gov
Data type: 
Particulate and dissolved nutrients on discrete water samples
Total Dissolved Phosphorus (TDP) : molybdate/ascorbic acid method on 
   AutoAnalyzer II, after persulfate digestion of 0.2 uM filtered samples
Particulate Phosphorus (PP) : molybdate/ascorbic acid method on AutoAnalyzer II, 
   after combustion, boiling HCL extraction of particles retained on a GFF filter
Bioavailable Phosphorus (AVP) : molybdate/ascorbic acid method on AutoAnalyzer II, 
   after NaOH digestion of particles retained on 0.2 uM nucleopore filter
Particulate Silica  (PSiO2) : molybdate/ascorbic acid method on AutoAnalyzer II, 
   after NaOH digestion of particles retained on 0.2 uM nucleopore filter
Soluble Reactive Phosphorus (SRP) : molybdate/ascorbic acid method on AutoAnalyzer II, 
   of  0.2 uM filtered samples
Nitrate + Nitrite (NO3): cadium reduction method on AutoAnalyzer II, of 0.2 uM 
   filtered samples
Ammonium (NH4): phenol method on AutoAnalyzer II, of 0.2 uM filtered samples
Particulate Organic Carbon (POC): Perkin Elmer CHN elemental analyzer
Particulate Organic Nitrogen (PON): Perkin Elmer CHN elemental analyzer
TDP coeff of variance on field reps = 7.6%  (n=9)
PP coeff of variance on field reps = 6.0%    (n=7)
AVP coeff of variance on field reps = 2.5%    (n=4)
NO3 coeff of variance on duplicates = 0.7% (n=4)
NH4 coeff of variance on duplicates = 17.2% (n=4)
SRP coeff of variance on duplicates = 32.1% (n=4)
POC coeff of variance on duplicates = 13.7%   (n=9 pairs)
PON coeff of variance on duplicates = 17.7%   (n=9 pairs)
Bruce G. Bills  
			Bruce.G.Bills@nasa.gov	858-822-0767

CURRENT POSITION

	Geophysicist, Planetary Geodynamics Laboratory
	Visiting Research Geophysicist, Scripps Institution of Oceanography

RESEARCH AREAS

	Planetary geodynamics, geodetic paleolimnology, 
      orbital, rotational and climatic interactions

EDUCATION  

	1973  B.S. (mathematics/physics) Brigham Young University, Provo, UT
	1981  Ph.D. (planetary science) California Institute of Technology, Pasadena, CA
		Thesis: A Harmonic and Statistical Analysis of the Topography of 
		            the Earth, Moon and Mars

PREVIOUS POSITIONS 
 
1977-1979	Senior Engineer, Tracking and Orbit Determination Group, 
        Jet Propulsion Laboratory, Pasadena, CA	
      1979-1984	Senior Scientist, Planetary Dynamics and Geophysics Group, 
        Jet Propulsion Laboratory, Pasadena, CA
      1984-1990	Staff Scientist, 
        Lunar and Planetary Institute,   Houston, TX
	1990-1992	Supervisory Geophysicist, Geodynamics Branch,
	  NASA Goddard Space Flight Center, Greenbelt, MD
      1992-present	Geophysicist, Geodynamics Branch,
	  NASA Goddard Space Flight Center, Greenbelt, MD
1991-1998	Adjunct Professor, Department of Earth and Planetary Sciences,
	  Johns Hopkins University, Baltimore, MD
1998-present	Visiting Research Geophysicist
			  Scripps Institution of Oceanography, La Jolla, CA

 
SELECTED PUBLICATIONS  

1994	Bills, B.G., D.R. Currey, and G.A. Marshall,
Viscosity estimates for the crust and upper mantle from patterns
  of lacustrine shoreline deformation in the eastern Great Basin,
    J. Geophys. Res., 99, 22,059-22,086.
1999	Adams, K.D.,  S.G. Wesnousky,  and B.G. Bills,
  Isostatic rebound, active faulting, and potential geomorphic effects
    in the Lake Lahontan Basin, Nevada and California
      Geol. Soc. Amer. Bull. 111, 1739-1756.
2003	Comstock, R.L., and B.G. Bills (2003),
  A solar system survey of forced librations in longitude,
    J. Geophys. Res. Planets, 108, 5100. 
2004	Egbert, G.D., R.D. Ray, and B.G. Bills,
  Numerical modeling of the global semidiurnal tide in 
    the present day and in the last glacial maximum,
      J. Geophys. Res. Oceans, 109, C03003. 
2005	B.G. Bills,
  Free and forced obliquities of the Galilean satellites of Jupiter,
    Icarus, 175, 233-247	
2005	B.G. Bills, and R.L. Comstock,
  Spatial and temporal patterns of solar eclipses by Phobos on Mars,
    J. Geophys. Res. Planets, 110, E04004.
2005	B.G. Bills, and R.L. Comstock,
  Forced obliquity variations of Mercury,
    J. Geophys. Res. Planets, 110, E04006.
2005	Bills, B.G., G.A. Neumann, D.E. Smith, and M.T.Zuber,
  Improved estimate of tidal dissipation within Mars from 
    MOLA observations of the shadow of Phobos,
      J. Geophys. Res. Planets, 110, E07004.
QUESTION:
Have you ever tried to use a different colored filter other then
red, green or blue?  and would it give us different information?

ANSWER from David Soderblom on May 6, 1996:
The amount of light from an object at different wavelengths provides vital
information on how that light was created and was has happened to it since.
The best way to analyze the distribution of light with wavelength is to
pass the light through a spectrograph; this disperses the light by color,
making it possible to see details in the spectrum.  These details reveal
what elements may be in a star and how much of them, how hot a star is,
the kinds of stars making up the core of a galaxy (for example), and so on.

For very faint objects (distant galaxies, for instance), there isn't enough
light to be able to use a spectrograph, so we use a crude approximation:
pictures through filters.  If we can take, say, pictures through blue,
yellow, and red filters, we can get an idea of where most of the energy
is coming from and what the sources might be.

The filters we use in astronomy aren't just colored glass, they are
specially manufactured to high tolerance to have specific characteristics.
There are a few filters that are very frequently used, but there are
also many specialized filters.  Some of these isolate very narrow bands
of wavelength, making it possible to get a "spectrum" in a rough sense.
For example, gaseous nebulae often emit light of specific wavelengths
from hydrogen and oxygen atoms, but not at other wavelengths.  Filters for
those specific wavelengths make it possible to see the object as though
you'd obtained a spectrum of the whole thing at once.

Other filters allow us to measure how much iron is in stars without having
to take the time to get a detailed spectrum; this makes observing more
efficient.  Still others are tailored to other specific problems.

There are maybe a dozen "standard" filters that are heavily used in
ground-based observing and in HST, but there are dozens more used for
particular purposes.
What the Commuity Can Do for You

Panelists 

- Reverend C.B. Akins, Community Leader, Lexington, KY 
- Lieutenant Dan Schiele, Sacramento (CA) Police Department 
- Phillip Osborne, Preston-Osborne, Lexington, KY 

The workshop discussed how to engage the 
community in partnership with the police 
department/sheriffs office in support of 
recruiting efforts. 


What the Commuity Can Do for You

Overview of Presentations 

- Use data to understand your community and its 
changing demographics. Identify and use decision 
makers and opinion influencers. 

- Stages of working with the community: irritation, 
confrontation, cooperation, collaboration, cross-
fertilization 

- Use community leaders to be community recruiters for 
the police department and sponsor officers who will 
later serve their community. 


What the Commuity Can Do for You

Common/Cross-cutting Themes 

- CEO must be front and center engaging the community. 

- Listen to criticism 

- Give the community a say and ownership in
recruitment, selection, and hiring.

- Problems getting diversity (e.g., citizenship rules)

- The CEO may face resistance working with the 
community. Community leaders often face the same 
resistance. 

- Work with community to make the agency the best it 
can be. 


What the Commuity Can Do for You

Innovative and Promising Practices That Emerged

- Understand your community and changing
demographics through data analysis

- Collaborate and think innovatively about how to deal 
with housing, education, quality of life issues potential 
officers face (e.g., work with lenders to get 0% down on 
homes for officers) 

- Sacramento (CA) Police Department: Community 
members as police recruiters 


What the Commuity Can Do for You

Concluding Takeaway Messages / Lessons 

 Understand and be in touch with your community 
 Promote jointly with the agency that  
 Service is an officer safety issue 
 Having the right people serves a public good
{CaptionsBy}    Information Dynamics, Inc (Kay Grinter, Anita Barrett, and Elaine
                Liston)
{LastEditor}    Anita Barrett
{ScannedBy}     Seven/Still Photo Imaging
{author}        NASA or National Aeronautics and Space Administration
{date}          18-Feb-2000
{description}   Near a road at Kennedy Space Center, a red-tailed hawk perches on
                a weathered tree stump. The red-tailed hawk has a stocky build
                and broad, rounded wings. Its broad range covers Alaska and Nova
                Scotia south to Panama. It can frequently be seen perched in a
                tree at the edge of a meadow, watching for movement in the grass
                below. It feeds mainly on small rodents. The Refuge 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. Kennedy Space Center
                shares a boundary with the Merritt Island National Wildlife
                Refuge, encompassing 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}       1818 x 2670
{highsize}      656708
{hightype}      JPEG
{lowres}        163 x 240
{lowsize}       56018
{lowtype}       GIF
{mediumres}     523 x 768
{mediumsize}    71703
{mediumtype}    JPEG
{number}        KSC-00PP-0244
{slideres}      112 x 156
{slidesize}     25350
{slidetype}     GIF
{tinyres}       68 x 100
{tinysize}      10373
{tinytype}      GIF
{title}         A Red-Tailed Hawk perches on a stump at KSC.
{type}          Image
{end}
000
WWUS84 KSJT 100132
SPSSJT

SPECIAL WEATHER STATEMENT
NATIONAL WEATHER SERVICE SAN ANGELO TX
829 PM CDT SUN OCT 9 2005

TXZ076>078-100230-

CROCKETT TX-SCHLEICHER TX-SUTTON TX-
829 PM CDT SUN OCT 9 2005

...SIGNIFICANT WEATHER ALERT EFFECTIVE UNTIL 930 PM CDT FOR
SCHLEICHER...CROCKETT AND SUTTON COUNTIES...

AT 827 PM CDT...STRONG THUNDERSTORMS WERE INDICATED BY NATIONAL 
WEATHER SERVICE DOPPLER RADAR FROM OZONA SOUTH DOWN STATE HIGHWAY 
163 TO THE VAL VERDE COUNTY LINE...MOVING NORTHEAST AT 45 MPH.

* THE STRONG THUNDERSTORM WILL BE NEAR...
  I-10 NEAR THE CROCKETT-SUTTON COUNTY LINE BY 835 PM CDT            
  US-277 NEAR THE SUTTON-SCHLEICHER COUNTY LINE BY 900 PM CDT        
  ELDORADO BY 910 PM CDT

PEA SIZE HAIL AND WIND GUSTS TO 50 MPH ARE LIKELY WITH THESE STORMS.
RESIDENTS ARE ENCOURAGED TO MONITOR THE SITUATION CLOSELY AND BE
PREPARED TO TAKE THE PROPER ACTIONS SHOULD A WARNING BE ISSUED.

A SEVERE THUNDERSTORM WATCH ALSO REMAINS IN EFFECT UNTIL 300 AM CDT 
MONDAY MORNING FOR WEST CENTRAL TEXAS.

$$
FXUS63 KLOT 161746 CCA
AFDCHI

AREA FORECAST DISCUSSION...CORRECTION 
NATIONAL WEATHER SERVICE CHICAGO IL
1145 AM CST MON FEB 16 2004

.FORECAST DISCUSSION FOR AM ZONES/GRIDS:

THE WEATHER WILL BE COLD WITH LIGHT WINDS TODAY. HIGH PRESSURE OVER 
MICHIGAN WILL MOVE EAST INTO NEW YORK BY MIDNIGHT TUESDAY MORNING. 
WE EXPECT A SOUTH WIND AND WARMER AIR TO MOVE INTO THE REGION. ALL 
THE GUIDANCE SHOW THE TEMPERATURES BECOMING HIGHER THROUGH THE WEEK. 
LOOKING AT THE FORECAST POSITION OF THE 500 MB WAVE TUESDAY NIGHT 
THE AVN AND ETA MODELS ARE SIMILAR. THERE IS NOT MUCH MOISTURE WITH 
THIS WAVE AND ITS SURFACE COLD FRONT. WILL NOT ISSUE ANY FORECAST 
PRECIPITATION AS ALL MOS GUIDANCE POPS ARE LOW. 

A CYCLONE DEVELOPS IN WESTERN KANSAS THURSDAY NIGHT AND MOVES EAST
TO NORTHERN GEORGIA. THE INVERTED TROUGH PASSE THROUGH NORTHERN 
ILLINOIS LATE FRIDAY. THE UPPER AIR WAVE HAS MORE NEGATIVE TILT 
FORECAST BY FRIDAY MORNING. SO WE EXPECT THIS CYCLONE TO BE 
STRONGER. THERE WILL BE A STRONG SOUTH FLOW INTO THE FORECAST AREA 
FROM THE GULF. HENCE WARMING TOWARD THE END OF THE WEEK. 
PRECIPITATION MAY BE IN THE FORM OF RAIN OR A MIXTURE OF BOTH. WHW 
    
&&

.AVIATION DISCUSSION REGARDING 18Z TAFS:

SYNOPSIS...RETREATING SURFACE ANTICYCLONE OVER MICH AND SRN ONTARIO 
WILL ALLOW A WEAK RETURN FLOW TTHIS AFTERNOON AND TONIGHT. ANOTHER 
WEAK TROUGH WIL PASS NORTH OF THE REGION EARLY TUESDAY VEERING THE 
WINDS AROUND TO W OR NW AGAIN.

WINDS...GRADIENT FAIRLY WEAK AND WITH SNOW COVER AND SHALLOW 
INVERSION AT AROUND 2500FT REMAINING LIGHT SE WINDS UNDER 10 KT 
EXPECTED THROUGH THE DAY. WINDS BECOMING MOVE SW AHEAD OF TROUGH 
DURING THE NIGHT THEN WEST SOMETIME TUESDAY MORNING. ALL SPEEDS 12KT 
OR LESS.

VIS...NO RESTRICTIONS ENTR PERIOD. 

CLOUDS/CIGS...WIDESPREAD CIRRUS WITH SOME LOWER DECKS TO 10K TONIGHT 
AND TUESDAY. LOW LEVEL CONTINUED DRY AND NO MEANINGFUL MOSITURE SEEN 
AHEAD OF APPROACHING TROUGH TUE.

KL

&&

.LOT...WATCHES/WARNINGS/ADVISORIES...
IL...NONE.
IN...NONE.
LK MI...NONE.

&&

$$
Expires:200807130030;Remove:200807130030;444083
WUUS55 KREV 122334
SVRREV

CAC017-130030-
/O.NEW.KREV.SV.W.0020.080712T2331Z-080713T0030Z/
BULLETIN - EAS ACTIVATION REQUESTED
SEVERE THUNDERSTORM WARNING
NATIONAL WEATHER SERVICE RENO NV
431 PM PDT SAT JUL 12 2008
THE NATIONAL WEATHER SERVICE IN RENO HAS ISSUED A
* SEVERE THUNDERSTORM WARNING FOR...
  NORTHEASTERN EL DORADO COUNTY IN CENTRAL CALIFORNIA...
* UNTIL 530 PM PDT
* AT 428 PM PDT...NATIONAL WEATHER SERVICE DOPPLER RADAR INDICATED A
  SEVERE THUNDERSTORM CAPABLE OF PRODUCING PENNY SIZE HAIL...AND
  STRONG WINDS UP TO 60 MPH.  THIS STORM WAS LOCATED NEAR
  EMERALD BAY...OR ABOUT 6 MILES WEST OF SOUTH LAKE TAHOE. THIS STORM
  WAS MOVING NORTH AT LESS THAN 5 MILES AN HOUR.
* THE SEVERE THUNDERSTORM WILL BE NEAR...
  EMERALD BAY AND BLISS STATE PARK BY 445 PM PDT...
BOATERS AND SWIMMERS ON OR NEAR LAKE TAHOE ESPECIALLY ON THE 
SOUTHERN PORTION OF THE LAKE NEAR EMERALD BAY...GET OUT OF THE WATER 
AND MOVE INDOORS OR INSIDE A VEHICLE. DON'T BE CAUGHT ON THE WATER 
IN A THUNDERSTORM! PEOPLE IN OR ON WATER ARE MUCH MORE PRONE TO 
BEING STRUCK BY DEADLY LIGHTNING. STRONG AND ERRATIC WINDS CAN LEAD 
TO BOATS CAPSIZING.
THIS STORM IS CAPABLE OF PRODUCING LOCALLY HEAVY RAINFALL. WATCH FOR
PONDING WATER ON AREA ROADWAYS. DRIVERS SHOULD SLOW DOWN IF
ENCOUNTERING HEAVY RAINS...AND REMEMBER TO TURN ON THEIR HEADLIGHTS.
LAT...LON 3902 12013 3897 11999 3887 12009 3894 12016
TIME...MOT...LOC 2331Z 159DEG 1KT 3893 12009
$$
GMCGUIRE
a44                    VOYAGES
alimenter  un corps   qui  semble  leur  tre  
charge.
Souvent on les rencontre en haute mer, et
on les voit aborder sur les vergues du vaisseau ;
ils s'y laissent prendre, ou paroissenl insensibles
au massacre de leurs semblables, qu'on assomme
 ct d'eux, sans prvoir que le mme sort les
attend. Ils n'ont pas la moindre prudence, et la
mfiance qui caractrise en gnral tous les
oiseaux d'eau.
Les fous, quoique palmipdes, se perchent
facilement; ils sont aussi trs-bons nageurs,
volent avec lgret, enfin sont en tat, sous
tous les rapports, d'viter ou de se soustraire au
danger qui les menace; mais, soit apathie ou
scurit inconsidre, ils ne redoutent point
l'homme, malgr les exemples frquens de ses
cruauts, et ne se troublent point  la vue mme
de ses nouveaux projets de destruction.
Je n'en tuai que deux pendant mon sjour 
Saint-Domingue, mais de si prs, que mon coup
fit balle. Les deux autres cependant prirent le
vol au bruit de l'explosion; ce qui dnote en
faveur de cette classe trop confiante, qu'il existe
des exceptions.
On mange sans rpugnance la chair du fou,
lorsqu'on a eu la prcaution de le dpouiller.
On le prpare alors  la daube ou en salmis.
#
# ChangeLog for /cdat/trunk/Scripts/vcs_icon.xbm 
# 
# Generated by Trac 0.10.5
# 02/23/09 14:12:57
#


09/24/04 03:32:31 doutriau [2798]
	* cdat/trunk/Scripts/vcs_icon.xbm (modified)
	smaller icon

09/21/04 08:23:13 doutriau [2796]
	* cdat/trunk/Packages/browser/Lib/vcs_function.py (modified)
	* cdat/trunk/Packages/vcs/Lib/install_vcs.py (modified)
	* cdat/trunk/Packages/vcs/Src/library/procCanvas.c (modified)
	* cdat/trunk/Scripts/vcs_icon.xbm (added)
	let user specify template for 1D method if graphic method name
	doesn't start with ASD
	on Linux, little icon for vcs windows, seemed to be ignored by Mac
	window manager