Obs SatTrackCam Leiden (Cospar 4353): 33490 09 001A 4353 F 20111023181732300 17 75 2334410-082560 56 35815 09 047A 4353 F 20111023181702300 17 75 2312494-073780 56 35815 09 047A 4353 F 20111023181732300 17 75 2313192-073780 56 35815 09 047A 4353 F 20111023182102300 17 75 2316497-073780 56 35815 09 047A 4353 F 20111023182302300 17 75 2318499-073790 56 Hellas-sat 2: 27811 03 020A 4353 F 20111023181702300 17 75 2312526-073780 56 27811 03 020A 4353 F 20111023181732300 17 75 2313228-073770 56 27811 03 020A 4353 F 20111023182102300 17 75 2316533-073770 56 27811 03 020A 4353 F 20111023182302300 17 75 2318535-073800 56 Express AM-1: 28463 04 043A 4353 F 20111023181702300 17 75 2317161-087230 56 Paksat 1R: 37779 11 042A 4353 F 20111023181702300 17 75 2308250-073500 56 Thuraya 2: 27825 03 026A 4353 F 20111023181732300 17 75 2335091-083190 56 Turksat 3A: 33056 08 030B 4353 F 20111023181732300 17 75 2326242-073100 56 Turksat 2A: 26666 01 002A 4353 F 20111023181732300 17 75 2326168-073490 56 Block DM-SL r/b: 32405 08 001B 4353 F 20111023181702300 17 75 2300588-085250 56 ------------------------------------------------------------------------- Canon EOS 450D + Carl Zeiss Sonnar MC 2.8/180, 800 ISO + ASTRORECORD astrometric software. What these numbers mean: http://www.satobs.org/position/IODformat.html ------------------------------------------------------------------------- Reasonable if not entirely perfect sky. PAN and Hellas-sat 2 are a very close pair: I have assumed that the most west (right) one is PAN, but analysts, please check this. - Marco ----- Dr Marco Langbroek - SatTrackCam Leiden, the Netherlands. e-mail: sattrackcam@wanadoo.nl Cospar 4353 (Leiden): 52.15412 N, 4.49081 E (WGS84), +0 m ASL Cospar 4354 (De Wilck): 52.11685 N, 4.56016 E (WGS84), -2 m ASL SatTrackCam: http://home.wanadoo.nl/marco.langbroek/satcam.html Station (b)log: http://sattrackcam.blogspot.com Twitter: @Marco_Langbroek ----- _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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