Hi Dave, > I asked pretty much the same question on 16 Oct. '98. How could the > 2.4 to 2.6 mm tether could be seen at 200 km without magnification? My > answer covered about fifteen or so posts, but none were satisfatory. If you dig back a little further -- to March of '96 when TSS was flying -- Rob McNaught explained the optical phenomenon in: http://www2.satellite.eu.org/seesat/Mar-1996/0185.html (with a minor correction in a later post). I also posted a detailed magnitude calculation on tether brightness, but can't seem to find it -- it may have been for an even earlier tether than TSS. SEDS? Anyway, simple solar reflection is all that is required to produce the observed signature. --Rob ----------------------------------------------------------------- Unsubscribe from SeeSat-L by sending a message with 'unsubscribe' in the SUBJECT to SeeSat-L-request@lists.satellite.eu.org http://www2.satellite.eu.org/seesat/seesatindex.html
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