To compute the synodic effect you need to know the position of the object's rotation axis, the type of reflecting surface and its angle to the rotation axes - in addition to sun-object-observer positions. To estimate the rotation axis you need three flashes from the same surface, observed in widely separated positions (and within a few weeks for a LEO) I have a graphing program to facilitate DETECTION of synodic effects that vary during one pass, because of the changing sun-object-observer angles (and flashes from additional surfaces). 2013/9/3 Vitaly Mechinsky <lupus_sat@tut.by> > Hi all! > > Could anybody recommend me a software for satellite synodic effect > calculation, that act to observed flash period? > > -- > Best regards, > > Vitaly (Minsk, Belarus). > _______________________________________________ > Seesat-l mailing list > http://mailman.satobs.org/mailman/listinfo/seesat-l > -- ---------------------------------------- Björn Gimle, COSPAR 5919 59.2576 N, 18.6172 E, 23 m Phone: +46 (0)8 571 43 312 Mobile: +46 (0) 704 385 486 -------------- next part -------------- An HTML attachment was scrubbed... URL: http://mailman.satobs.org/mailman/private/seesat-l/attachments/20130903/7dc0e05d/attachment.html _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
This archive was generated by hypermail 2b29 : Tue Sep 03 2013 - 20:49:48 UTC