HDTenEightyP/NetNews huggingface dataset:
From: beaucham@astro.phy.ulaval.ca (Dominique Beauchamp)
Newsgroups: sci.astro
Subject: OIII filter & planetary nebulae
Keywords: OIII filter, planetary nebulae
Date: 24 Jul 92 19:48:35 GMT
Organization: Universite Laval, Ste-Foy, Quebec (Canada)

Hi everybody!

On Wednesday and Thursday night (Jul 22/23 and 23/24), I've observed 15 planet-
ary nebulae with a SC 8in f/10, from a location 60 km away of a half a million
people city (Quebec City).  My goal was to test an OIII filter (Lumicon) with
a 11nm bandpass.  I had tested it on diffuse nebulae sooner this spring but
I found the result not very convincing.  Then, I tried it again on PN and what
a surprise!  Many of them were few arcseconds large and, with 222x, were only
distinguishable with this filter.  On M27, many details are visible that are
completly masked by the glow without the filter.

I would appreciate to have some other's opinion about the use of the OIII
filter on PN, on any other deppsky object, or the use of other filters like
UHC, Hbeta or "nebula" filter.

Dominique Beauchamp

e-mail : beaucham@phy.ulaval.ca
Newsgroups: sci.astro
From: greg@korg3.columbiasc.ncr.com (Greg Porr)
Subject: Re: August showers...
Organization: NCR Corp, MCPD-Columbia, Columbia, SC
Distribution: usa
Date: Tue, 28 Jul 92 12:22:39 GMT

In article <1992Jul27.214348.22201@mnemosyne.cs.du.edu> aalpert@nyx.cs.du.edu (Arnold Alpert) writes:
>
>I was wondering if anyone had any information about what I've heard is
>going to be a spectacular meteor shower in early august.
>Specifically, I'd like to know what the best conditions (Times, places,
>weather...) are so that I can see the best 'show' possible.  (I live in
>Denver CO, but I can easily escape into the foothills, away from the
>lights of the city...  Any other information about this phenomena would be
>greatly appreciated.

The Perseid meteor shower, which peaks around the 12th, has the potential
to produce more meteors than normal, due to the possible return of its
parent comet, Swift-Tuttle.  Higher activity than normal was seen in Japan
last year.

Unfortunately, escaping from the lights of Denver won't be your major concern.
Unless you can also escape from the light of the full moon, much of the
visual observations will be hampered :(

However, you can try observing a few days before and after the peak as well;
radio observations (which I've never done) are also possible.  See the
August Sky & Telescope for more information.

-- Greg Porr
   (Greg.Porr@ColumbiaSC.NCR.COM)
Newsgroups: sci.astro
From: oler@rho.uleth.ca (Cary Oler)
Subject: Daily Solar Geophysical Data Broadcast for 24 July
Organization: University of Lethbridge
Date: 25 Jul 92 03:29:03 GMT

!!BEGIN!! (1.0) S.T.D. Solar Geophysical Data Broadcast for DAY 206, 07/24/92
10.7 FLUX=100.1  90-AVG=127        SSN=058      BKI=3323 3322  BAI=012
BGND-XRAY=B2.2     FLU1=2.8E+05  FLU10=1.1E+04  PKI=3223 3333  PAI=011
  BOU-DEV=020,024,017,028,022,037,014,014   DEV-AVG=022 NT     SWF=00:000
 XRAY-MAX= B3.5   @ 2037UT    XRAY-MIN= B2.1   @ 1014UT   XRAY-AVG= B2.5
NEUTN-MAX= +002%  @ 2125UT   NEUTN-MIN= -003%  @ 0810UT  NEUTN-AVG= -0.2%
  PCA-MAX= +0.0DB @ 2355UT     PCA-MIN= -0.2DB @ 0050UT    PCA-AVG= -0.0DB
BOUTF-MAX=55244NT @ 2159UT   BOUTF-MIN=55207NT @ 1718UT  BOUTF-AVG=55232NT
GOES7-MAX=P:+109NT@ 1841UT   GOES7-MIN=N:-036NT@ 1146UT  G7-AVG=+082,+048,+007
GOES6-MAX=P:+119NT@ 1842UT   GOES6-MIN=E:-013NT@ 1615UT  G6-AVG=+093,+008,+033
 FLUXFCST=STD:103,110,115;SESC:100,105,110 BAI/PAI-FCST=010,010,010/010,010,010
    KFCST=2234 3222 2234 3222  27DAY-AP=014,020   27DAY-KP=2124 3344 2255 4323
 WARNINGS=
   ALERTS=
!!END-DATA!!
From: flower@hpcc01.corp.hp.com (Graham Flower)
Date: Mon, 27 Jul 1992 23:56:09 GMT
Subject: Stellar Structure References
Organization: the HP Corporate notes server
Newsgroups: sci.astro



      Can somebody recommend a popular or more demanding book that discusses
      the (Bethe) sequence of nuclear reactions that explains the evolution
      of Stars and the distribution of chemical abundances in the universe.

      I would like to work on this at the level of Clayton's book but would
      like to read some popular accounts first so that I have some perspective
      before grinding through the trenches. I would be most appreciative.


Graham Flower ms 90-TT               |  Better to have convictions and act on 
Hewlett-Packard  350 W Trimble Rd    |  them, even if they are wrong, than to  
Microwave Semiconductor Division     |  waffle in indecision.
San Jose, California, 95131          |
 graham_flower@sj.hp.com             |


Newsgroups: sci.astro
From: dsc@gemini.tmc.edu (Doug S. Caprette Bldg. 28 W191 x3892)
Subject: Re: ST-4 & PHOTOMETRY
Organization: NASA GSFC CDP VLBI
Date: Mon, 27 Jul 1992 17:28:37 GMT

In article <1992Jul26.231056.7584@usenet.ins.cwru.edu> bx372@cleveland.Freenet.Edu (Mr. Arthur J. Musgrove) writes:
>
>In a previous article, malcolm@hpwin052.uksr.hp.com (Malcolm Porter) says:
>
>> I would be interested in hearing about anyone's experienc
>> (CCD photometry)
>
>I have helped a college professor with the installation of one and we have
>taken a few shots of the sky with it and measured the brightnesses with the
>software..  They were not very accurate as in 1/10th of a magnitude but I

Indeed.  I understand that experienced observers with the AAVSO approach 
1/10th magnitude accuracy visually.  CCD photometry should get you an
order of magnitude or more of improvement.  Did you subtract off a flat 
field, dark current etc?

>believe that this should be accurate enough for a lot of applications..
>Another problem is the small field of view...  

Visual observing is done with a field of view an order of magnitude larger,
in diameter, than what is typical of a CCD chip.   So, use of a CCD camers
for stellar phototmetry with 1/10th magnitude accuracy would seem to be a
big and expensive step backward, unless one is planning on doing automated
observing.  

On the other hand, our experience with the Lynxx Spectra Systems 12 bit camera 
leads me to believe that high accuracy stellar photometry is possible with the
off the shelf equipment available to the amatuer.  This 12 bit camera (with
software) is comparably priced when compared to the 8 bit cameras.  Perhaps
you should look into it.

>                                               In order to get a good
>reduction of noise, light pollution etc.  the comparison star should be on
>the same shot with the ccd chip...
>

Absolutely.
From: pvtmakela@hylkn1.Helsinki.FI (M{kel{ Veikko)
Newsgroups: sci.astro
Subject: Astronomical software available via FTP
Date: 22 Jul 92 12:53:18 GMT
Organization: University of Helsinki


        SOME NEW ASTRONOMICAL MATERIAL AVAILABLE IN FTP SERVER
                      ftp.funet.fi (128.214.6.100)

        There have been some adverticements of astronomical 
        software and other material in sci.astro and comp.
        binaries.ibm.pc.d newsgroups.  Also some programs
        have been posted into comp.binaries.ibm.pc newsgroup.
        
        All these are now available in ftp.funet.fi server
        via ANONYMOUS-FTP:
        
        * COSMOS, a planetarium program by Gene W. Lee,
          version 15
          >>> pub/astro/pc/stars/cosmos15.exe
          
        * ASTRONOMY LAB FOR WINDOWS by Eric Bergman-Terrell, 
          version 1.08
          >>> pub/astro/pc/win/alw108.exe
          
        * ASTRO, a star map program by Malcolm Reeves, version 2.02
          >>> pub/astro/pc/stars/astro202.exe
          
        * SKYGLOBE, a star map program by Mark A. Haney, version 3.1
          >>> pub/astro/pc/stars/skygl31.exe
          
        * A summary of PD/SW star map programs for PC edited by Malcolm
          Reeves
          >>> pub/astro/general/starmap.rev


                                         regards,

                                       Veikko Makela,
                                        moderator of
                                       astronomy files
                                       in ftp.funet.fi          
Newsgroups: sci.astro
From: gliba@scivax.stsci.edu
Subject: Nova Cygni 1992 Update
Organization: Space Telescope Science Institute
Distribution: na
Date: Tue, 28 Jul 1992 21:41:12 GMT

Nova Cygni Update

    Last night I observed Nova Cygni 1992 and made a magnitude estimate.
Using the AAVSO (b) chart, I estimated it to be at 8.6 magnitude; so very
little changed from last time. There does seem to be some small amplitude
fluxuations, but probably a photometer will be needed to accurately see
this. I used my 3 inch f6 newtonian telescope at 21x.




G.W. Gliba - 'I would rather see starlight than streetlights'
From: weemba@sagi.wistar.upenn.edu (Matthew P Wiener)
Newsgroups: sci.astro
Subject: Re: On the formation of black holes
Date: 23 Jul 92 19:37:06 GMT
Reply-To: weemba@sagi.wistar.upenn.edu (Matthew P Wiener)
Distribution: sci
Organization: The Wistar Institute of Anatomy and Biology
In-reply-to: cpyy@vax5.cit.cornell.edu

In article <1992Jul23.101505.13947@vax5.cit.cornell.edu>, cpyy@vax5 writes:
>I am not interested in clarification.

That's pretty obvious.
-- 
-Matthew P Wiener (weemba@sagi.wistar.upenn.edu)
Newsgroups: sci.astro
From: gliba@scivax.stsci.edu
Subject: Re: Phobos and Deimos
Organization: Space Telescope Science Institute
Distribution: na
Date: Mon, 27 Jul 1992 21:59:07 GMT

>From: frisbee@jpl-devvax.jpl.nasa.gov (Tyler Brown)
>Subject: Phobos and Deimos
>Date: Fri, 24 Jul 1992 19:19:33 GMT

>I know that the moon Phobos means "fear" and was a consort of the God
>of war (Mars/Ares), but I forget what "Deimos" means. Could someone
>remind me?

>			frisbee@devvax.jpl.nasa.gov


   My Vote is for PANIC!


GWG - 'I would rather see starlight than streetlights'


Newsgroups: sci.astro
From: bic@cgl.ucsf.edu (Bruce Cohen%CGL)
Newsgroups: sci.astro
Subject: First Telescope: Astroscan, C4.5
Date: 26 Jul 92 23:47:35 GMT
Organization: Computer Graphics Laboratory, UCSF
Originator: bic@socrates.ucsf.edu

I am interested in buying my first telescope.  Any comments on the Edmunds
Scientific Astro scan would be appreciated.  I am also considering (the
most costly, less portable) Celestron C4.5 Newtonian.

Thanks.
-- 
=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-=-
"	Bruce Cohen                    |  UUCP:     ..ucbvax!ucsfcgl!bic
"	Computer Graphics Lab          |  INTERNET: bic@cgl.ucsf.edu
"	S-926                          |  BITNET:   bic@ucsfcgl
Newsgroups: sci.astro
From: tomrice@netcom.com (Tom R. Rice)
Subject: Re: laser guide star 07/30/92
Date: Fri, 31 Jul 92 01:12:25 GMT
Organization: Netcom - Online Communication Services  (408 241-9760 guest) 

Thank you for the info.  I was driving through Livermore about
1:00 AM and was treated to a genuine "HOLY COW!" experience, seeing
that beam zapping into the sky.  Tried a few time exposures....
Unfortunately, I guess it was turned off when I got home (in the
mountains 30 miles south of LLNL).

I'm sure many folk would appreciate some advance notice when it
is next turned on;  it's a real phenomenon from nearby locations.
Who sez science ain't pretty?

TRR   WB6BYH


-- 
==============================================================
tomrice@netcom.com              Holler Observatory 
CIS:71160,1122                  Longitude: 121 d  30 m  20 s W 
WB6BYH                          Latitude:   37 d  25 m  10 s N
From: j.jahn@abbs.hanse.de (Jost Jahn)
Newsgroups: sci.astro
Subject: Sunspots at 24.07.1992.
Date: 26 Jul 92 07:40:26 GMT
Reply-To: j.jahn@abbs.hanse.de
Distribution: sci
Organization: ABBS AstroMail, D-W 2121 Dahlenburg / Germany
X-Version: ZerUU V6.45c

Sunspots at 24.07.1992., 0 h UT.

No.    Pos.  Cl.  Ar.  Mag. SF  F  M  X
---------------------------------------
7229 24N 79W Hax   50   a
7234 17S 81W Cao   70   b    1
7235 05S 72W Hsx   40   a
7236 18N 16W Dao   60   b
7237 05N 50W Cro   30   b

Explanations of spot columns:
No.  Running number of sunspot group.
Pos. Position in Latitude and Longitude.
     N - North, S- South, E - East, W- West.
Cl.  MacIntosh classification.
Ar.  Area in 10-6 of visible hemisphere.
Mag. Magnetic Classification.
     a - alpha, b - beta, bg - beta/gamma,
     g - gamma, bd - beta/delta, bg - gamma/delta
     bgd - beta/gamma/delta.
SF   Number of subflares.
F    Number of optical flares. (importance > 1).
M    Number of medium x-ray eruptions.
X    Number of strong x-ray eruptions.


No optical or x-ray flares yesterday observed.


 
--
------------------------------------------------------------------------------
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------------------------- for amateur astronomers ----------------------------
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Newsgroups: sci.astro
From: metares@well.sf.ca.us (Tom Van Flandern)
Subject: Re: B-O Effect (was Re: Proof of quasar non-locality?)
Organization: Whole Earth 'Lectronic Link
Date: Sun, 26 Jul 1992 21:01:31 GMT



Earlier, I wrote:

>> The universe derived by the Meta Model is infinite in five dimensions:
>> three of space plus time and scale..

and dwells@fits.cv.nrao.edu (Don Wells) replied:

> Infinite in time means steady-state, i.e. no creation. This is, of course,
> in contradiction to the B-O Effect, and to a number of other observations,
> such as radio source counts.

     Only if they are interpreted with the standard model.  If you assume the
premises of the Meta Model, then you can see whole new meanings to this and
many other effects which contradict nothing; for example, the two-population
idea I described earlier.

> I reassert: "The B-O objects are unquestionably *galaxies*." That assertion
> is an observational *fact*, which is why I said "unquestionably". I have
> personally acquired imagery of the distant clusters, and I can tell you
> that these objects are *resolved*, they are not point sources as quasars
> are. Spectra of the B-O objects have been obtained, and they are seen to be
> similar to spectra of nearby spiral galaxies. The "blue" galaxies of the
> B-O Effect are not exotic objects which need special explanations, they are
> merely galaxies which have been forming stars recently.

     Can you put together an air-tight argument to the effect that most B-O
objects are galaxies?  Their merely being resolved is inconclusive, since
they might be nebulae around supermassive stars.  And some normal galaxies
are bluer than others.  But what is the argument that *most* of the B-O
objects *must* be galaxies?  -|Tom|-

-- 
Tom Van Flandern / Washington, DC / metares@well.sf.ca.us
Meta Research was founded to foster research into ideas not otherwise
supported because they conflict with mainstream theories in Astronomy.
Newsgroups: sci.astro
From: gak@wrs.com (Richard Stueven)
Subject: Re: Crosser 1992 Aug. 03 - 10.
Reply-To: gak@wrs.com
Organization: Wind River Systems, Inc.
Date: Wed, 29 Jul 1992 19:48:02 GMT

What's this?  An astronomy-related posting on sci.astro?

It's a miracle!

---
gak
107/H/3&4

Newsgroups: sci.astro
From: turner@bigbang.astro.indiana.edu (George Wm Turner)
Subject: Re: Heavy Boots
Reply-To: turner@bigbang.astro.indiana.edu (George Wm Turner)
Organization: Indiana University
Date: Fri, 31 Jul 92 19:08:10 GMT


>In article <1992Jul31.071337.14623@omen.UUCP>, caf@omen.UUCP (Chuck Forsberg WA7KGX) writes:
>
>Were any of your students sharp enough to choose a moon light
>enough that one could drop the pen hard enough that its rebound
>would exceed escape velocity?  It would have been a matter of
>honor in my 3rd semester physics recitation section at RPI.


on any moon it would, at best, only bounce as high as it had been dropped from.
any friction at all would cause it to rise to a height something less than 
what it was dropped from.

george wm turner     turner@bigbang.astro.indiana.edu
Newsgroups: sci.astro
From: frisbee@jpl-devvax.jpl.nasa.gov (Tyler Brown)
Subject: Re: Phobos and Deimos
Organization: Jet Propulsion Laboratory (NASA)
Date: Fri, 24 Jul 1992 23:54:54 GMT

I asked recently on this net what "Deimos" meant. So far I have received the
following responses:

		Translation		Number of Votes
		___________		_______________

		Terror				5
		Panic				3

Terror is currently beating out panic, but by a slim margin...

Gosh, doesn't that sound like a baseball game in Hell?

			frisbee@devvax.jpl.nasa.gov


Newsgroups: sci.astro
From: edwards@andy.bgsu.edu (Bruce Edwards)
Subject: Re: Structure of Time, please stop
Organization: Bowling Green State University B.G., Oh.
Date: Wed, 29 Jul 1992 14:38:36 GMT

Please stop posting these discussions to sci.astro, they
are not appropriate to the group, they are not contributing
anything interesting or new at this point, and they are beginning
to become annoying. Thank you.


edwards@andy.bgsu.edu

-- 

<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<<
edwards@andy.bgsu.edu  (ken jenkins as guest of Bruce Edwards)
century marketing corporation
From: baalke@kelvin.jpl.nasa.gov (Ron Baalke)
Newsgroups: sci.astro
Subject: Re: Comet Shoemaker Levy 1991a1
Date: 22 Jul 92 05:37:11 GMT
Reply-To: baalke@kelvin.jpl.nasa.gov
Organization: Jet Propulsion Laboratory
News-Software: VAX/VMS VNEWS 1.3-4

In article <1992Jul21.182723.12131@linus.mitre.org>, chaloux@mandolin.mitre.org (Dave Chaloux) writes...
>Has there been any internal structure or tail that could be seen on better
>nights elsewhere?

The Hubble Space Telescope made three observations of Comet Shoemaker Levy
yesterday using its Faint Object Camera.  There was no mention of any
tail, but good spectra data was obtained.   
     ___    _____     ___
    /_ /|  /____/ \  /_ /|     Ron Baalke         | baalke@kelvin.jpl.nasa.gov
    | | | |  __ \ /| | | |     Jet Propulsion Lab |
 ___| | | | |__) |/  | | |__   M/S 525-3684 Telos | Most of the things you 
/___| | | |  ___/    | |/__ /| Pasadena, CA 91109 | worry about will never
|_____|/  |_|/       |_____|/                     | happen.
Organization: Georgia Tech Research Institute
Date: Saturday, 18 Jul 1992 00:30:24 EDT
From: <LABBEY@GTRI01.GATECH.EDU>
Newsgroups: sci.astro
Subject: Re: Mirror Coatings ???

John, the main difference between the various coatings is price.

For a first mirror, regular aluminum is OK.  It is cheap, and if you later
decide to go for a better coating, you can easily have the old one removed,
in face that is part of the process.

I have been using the same coating on my 10" since 1966.  A good one lasts
forever!

Leonard Abbey, F.R.A.S.
Georgia Tech Research Institute
Atlanta, Georgia, USA
labbey@gtri01.gatech.edu
From: slb@slced1.nswses.navy.mil (Shari L Brooks)
Newsgroups: sci.astro
Subject: Re: On the formation of black holes
Date: 30 Jul 92 23:14:59 GMT
Distribution: na
Organization: Naval Satellite Operations Center, Point Mugu, CA, USA

What is a Penrose diagram?
--
  Shari L Brooks                   |   slb%suned1.nswses.navy.mil@nosc.mil
  NAVSOC code NSOC323D             |   shari@caspar.nosc.mil
  NAWS Pt Mugu, CA 93042-5013      |   
--> All statements/opinions above are mine and mine only, not the US Navy's.
Newsgroups: sci.astro,rec.radio.shortwave,rec.radio.amateur.misc
From: jan@world.std.com (Joshua A Natarajan)
Subject: Apparant Stasis
Organization: The World Public Access UNIX, Brookline, MA
Distribution: usa
Date: Wed, 29 Jul 1992 16:06:57 GMT


Sci.astro -  Mostly answering questions like Is the universe closed, Cold dark
matter - what of it? Is there an astronomy program? What is Relativity and what
are black holes.

Frankly I am beginning to get tired of it all. We know only so much but we
keep discussing these things over and over again.

I have just test flown an FTL space ship that works on Pure Ignorance and since
the space ship can hold only one please give me a list of experiments to try
when I am near  a) molecular clouds b) planetary nebulas c) T Tauri,  the
next time.

Josh   jan@world.std.com

Newsgroups: sci.astro,sci.space
From: cyamamot@kilroy.Jpl.Nasa.Gov (Cliff Yamamoto)
Subject: Nachos (Ted Molczan elements) mirror/backup site
Summary: A mirror/backup site is now available
Keywords: nachos, mirror, orbital, elements
Organization: Jet Propulsion Laboratory, Pasadena, CA
Date: Wed, 22 Jul 1992 21:41:14 GMT


Please add this to the FAQ.

A mirror/backup site has been created for nachos.ssesco.com which typically
carries Ted Molczan's orbital elements from his BBS.  The anonymous FTP
site is as follows:

Name:     kilroy.jpl.nasa.gov
Address:  128.149.1.165
Aliases:  jpl-fmc-gw.jpl.nasa.gov

The nasa elements will be located in:

~ftp/pub/space/elements/nasa

Ted Molczan's elements will be located in:

~ftp/pub/space/elements/molczan

This site is NOT temporary.  Once nachos is repaired, kilroy will be a mirror
site to reduce loading on nachos and to perhaps archive the elements sets for
a longer period (there are no foreseen disk usage problems on kilroy).

Chris Elmquist will be fowarding the elements to kilroy which are automagically
placed into the appropriate FTP directory.

If you have any questions/comments/complaints about this mirror site, please
email me.

Regards,
Cliff Yamamoto
---------------------------------------+---------------------------------------
Internet: cyamamot@kilroy.Jpl.Nasa.Gov | MaBell: 1 (818) 354-1242 - office
          cyamamot@grissom.Jpl.Nasa.Gov|         1 (818) 354-2825 - fax
          cky@vermithrax.Jpl.Nasa.Gov   ---------------------------------------
Bitnet:	  cyamamot%kilroy.Jpl.Nasa.Gov@Hamlet.Bitnet
Uucp:     uunet!kilroy.Jpl.Nasa.Gov!cyamamot@uunet.UU.NET
          ames!elroy!jato!jpl-mil!kilroy.jpl.nasa.gov!cyamamot
Packet:   KA6JRG@W6VIO.#SOCA.CA.USA.NA
-------------------------------------------------------------------------------
USnail:   Clifford K. Yamamoto - KA6JRG      Jet Propelled La-bore-atore-ee
          4800 Oak Grove Drive               M/S 238-737, Section 333
          Pasadena, Calif.  91109
From: j.jahn@abbs.hanse.de (Jost Jahn)
Newsgroups: sci.astro
Subject: Sunspots at 19.07.1992.
Date: 21 Jul 92 06:26:24 GMT
Reply-To: j.jahn@abbs.hanse.de
Distribution: sci
Organization: ABBS AstroMail, D-W 2121 Dahlenburg / Germany
X-Version: ZerUU V6.45c

Sunspots at 19.07.1992., 0 h UT.

No.    Pos.  Cl.  Ar.  Mag. SF  F  M  X
---------------------------------------
7220 13S 98W Hsx  120   a
7222 11S 81W Fai  290   b    5
7225 09S 41W Cao   50   b
7226 24S 69W Dao  100   b    2
7227 13N 24W Bxo   20   b    1     1
7229 23N 17W Dao   80   b
7230 13S 08E Bxo   10   b
7232 16N 33E Dao   70   b    2
7233 06N 79W Bxo   20   b    2


Optical and x-ray flares in 18.07.92.

Date     Beg. Max. End   Posit. Xray Opt
----------------------------------------
18.07.92 0242 0250 0255 09N 13W M1.0 SF
18.07.92 1338 1344 1356 17S 90W M2.0
18.07.92 2031 2038 2045 16N 40E C5.6 1N


 
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From: banshee@cats.ucsc.edu (Wailer at the Gates of Dawn)
Newsgroups: sci.astro
Subject: Another bolide
Date: 27 Jul 92 23:22:39 GMT
Distribution: usa
Organization: University of California, Santa Cruz
NNTP-Posting-Host: am.ucsc.edu


	Last evening ~9:30 PST  30deg west of zenith passing through
cygnus for 20+ degrees.  Several magnitudes brighter than vega.  Pulsated
two or three times as it fell.

-- 
The Wailer at the Gates of Dawn              | banshee@cats.UCSC.EDU       |
Just who ARE you calling a FROOFROO Head?    |                             |
DoD#0667  "Just a friend of the beast."      | banshee@ucscb.UCSC.EDU      |
2,3,5,7,13,17,19,31,61,89,107,127,521,607....| banshee@ucscb.BITNET        |
Newsgroups: sci.astro