How to help newbies?
Walter Nissen (dk058@cleveland.Freenet.Edu)
Fri, 28 Jul 1995 22:19:01 -0400
Any comments about the adequacy of the response below?
Date Fri Jul 28 22:03:53 1995
>From dk058@cleveland.Freenet.Edu (Walter Nissen)
Subject Visual Observing of Satellites
To markus@interaccess.com, jjmalley@maui.netwave.net
> From: markus@interaccess.com (mark haas)
> Newsgroups: sci.astro.amateur
> Subject: SATALITE VIEWING
> Date: Mon Jul 24 01:34:54 1995
> I AM INTERESTED IN IDENTIFYING SOME OF THE SATALITES THAT PASS OVER
> ON A GIVEN EVENING. WHATs a good PROGRAM TO USE TO PLOT ELEMENT DATA?
> THANKS..
> From: jjmalley@maui.netwave.net (John J. Malley)
> Newsgroups: sci.astro.amateur
> Subject: Tracking satellites
> Date: Thu Jul 27 23:33:29 1995
> I'm trying to learn to track satellites visually, but I'm not having
> much luck spotting them. I have a program to track them, and it tells
> me when the satellites should be visible. Are there particular
> satellites which are brighter? Which ones?
> What types of things affect their visibility? Altitude? Their
> color??? I know they have to be in sunlight, and I have to be in the
> dark - and I'm afraid that's exactly where I feel I am right now.
> Any help would be appreciated. I'm getting tired of plotting these
> things on the computer and not being able to spot them!
> Thanks!
> John
Three mistakes beginners often make are using old elements, looking for
radio dots, and using a radio-oriented program. A program like Mike
McCants' QuickSat addresses all of these issues. It generates for every
pass a heuristic value that will help you spot an elset that should be
freshened. It contains his photometric catalog which allows you to pick
out only bright candidates, or at least know what you are up against if
you choose to try for fainter objects, or newer objects with no
observations. It can precisely calculate shadow ingress and egress, so
you don't waste effort looking for objects 12 magnitudes fainter than the
limit for your sky, something that radio-oriented programs with some
visual features don't adequately do. QuickSat is available from the
SeeSat-L archive, mentioned just below.
The SeeSat-L mailing list serves visual satellite observers. You may send
subject "subscribe" to seesat-l-request@iris01.plasma.mpe-garching.mpg.de
and also "help" and "archive help". Volume is only maybe 3 messages a
day.
You may wish to access the archive for the many discussions of visual
observing. Recent messages have discussed the merits of the various lists
and catalogs of bright objects, some of which are available from the
archive. Elsets for bright objects are maintained in special files by the
OIG BBS, Celestial BBS, and kilroy. The archive has a search facility
called egrep.
You can obtain information about the mailing list and much other material
of interest to visual observers of Earth satellites, including Web access
to recent traffic on the mailing list, by checking into the Web pages at:
http://www.ipp-garching.mpg.de/~bdp/satintro.html and
http://www.physics.ox.ac.uk/sat/satintro.html.
Cheers.
Walter Nissen dk058@cleveland.freenet.edu 216-243-4980
---
It ain't the cranks, it's the responses to the cranks.
It ain't the FAQs, it's the responses to the FAQs.