I haven't found any TDF-1 data (yet?), but I tediously dug out the following
approximate observations of Gorizont 23 out of my mail boxes:
Flash RA Dec
2002-03-13 05:00 Ed0313 13:46 0.5
2002-03-13 05:19 Ed0313 14:04 -0.4
2002-03-13 06:39 Ed0313 15:24 -2.55
2002-08-26 04:11 PG0826 16:41 -6.3
2002-08-17 04:31 Ed0817 19:47 -11.5
2002-08-17 05:36 Ed0817 22:50 -12.25
2002-08-26 04:11 PG0826 16:41 -6.3
2002-08-26 04:11 PG0826 17:09 -7.2
2002-08-24 04:40 PG0824 18:03 -8.75
2002-08-24 05:00 PG0824 18:23 -9.25
2002-08-24 05:10 Ed0824 18:15 -9.6
2002-08-23 04:49 PG0823 18:12 -9
2002-08-08 04:44 Ed0808 22:44 -12.05
2002-08-08 05:12 Ed0808 23:11 -11.95
2002-08-21 04:49 JH0821 19:03 -11.4
With such long observation periods, I didn't expect very useful solutions, but
it doesn't look so bad.
Axis at 22:50, +79.7, cone angle 86.0 (and 86.9 for the late sessions)
For 2002-08-28, at San Antonio at UTC 09:30, just before shadow entry, flashes
should be getting brighter, and after leaving eclipse at 10:40 they would
decrease, but from a second episode (back side of computed surface)
For Jason Hatton, 08:50 to 09:10
For Ed Cannon, first flash event should be around 03:45, second 04:10 ??
Rob Matson could have the first event 04:00
PG8305 04:15
I am puzzled by the large differences, but too tired to check them out.
>
> >For anyone interested in seeing a flashing geosynch, Gorizont
> >23 has been easy to observe with 10x50 binoculars the last few
> >evenings
>
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This archive was generated by hypermail 2b29 : Mon Aug 26 2002 - 17:50:29 EDT