The observations are ~4 min late per Ted's 79001, thus within the limits he suggested. I had a hunch this figure would be the most probable - by the indications from radio obs the separation from USA 186 was shorter than ususal, but if 161 had its MM lowered by 0.042 a day earlier, it would increase the separation between the two to more normal values at maneuvre time. 26934 01 044A 5919 G 20080327215843490 17 25 2041255+520014 29 S 26934 01 044A 5919 G 20080327215912020 17 25 2142768+515290 68 S 26934 01 044A 5919 G 20080327215927130 17 25 2211183+504999 97 S The first two are less accurate appulses. (As usual in IOD format: http://www.satobs.org/position/IODformat.html) -- Björn Gimle -- -- COSPAR 5917, STAR, +18.05447 (E), +59.34185 (N), 33 m -- -- COSPAR 5918 WGS84, +18.10127 (E), +59.29813 (N), 44 m -- -- COSPAR 5919, MALMA, +18.6206 (E), +59.2615 (N), 33 m -- ----- Original Message ----- > Possible/probable obs at 21:58 UTC near the following adjusted elset: > > USA 161 4m+Ted 1 15.0 4.0 0.0 5.2 v > 1 79001U 08079.70595140 .00001495 00000-0 30000-4 0 08 > 2 79001 97.8833 192.4394 0471000 25.5066 1.7800 14.75900000 07 > ------------------------------------------------------------------------- Subscribe/Unsubscribe info, Frequently Asked Questions, SeeSat-L archive: http://www.satobs.org/seesat/seesatindex.html
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