Derek Breit, Scott Campbell, Kevin Fetter, Marco Langbroek, Jim Nix, Ian Roberts, Peter Wakelin, Mike Waterman, Brad Young, and I, contributed observations used to determine one or more of the following element sets. SDS 3-3 816 X 39531 km 1 28384U 04034A 10244.82916228 .00000000 00000-0 00000-0 0 08 2 28384 63.9590 288.6143 7290618 272.5830 13.8746 2.00649380 02 Arc 20100829.95-0902.09 WRMS resid 0.005 totl 0.003 xtrk AEHF 1 608 X 49995 km 1 36868U 10039A 10244.78501347 .00000000 00000-0 00000-0 0 03 2 36868 21.2710 306.0492 7794810 188.0207 140.2341 1.54002045 08 Arc 20100901.16-0902.15 WRMS resid 0.009 totl 0.006 xtrk If the interval between the first two perigee-raising manoeuvres is indicative of the plan, then the next burn would have occurred near the apogee passage of Sep 02 at 12:09:14 UTC; if so, it will be running several minutes late tonight, and a bit off track. If that is found to be the case, the following estimated post-manoeuvre elements may be helpful in assessing what is observed, or not: 770 X 49995 km 1 70000U 10245.50641205 .00000000 00000-0 00000-0 0 05 2 70000 20.8700 305.8963 7749373 188.3643 180.0000 1.53414000 00 AEHF 1 r 227 X 50115 km 1 36869U 10039B 10244.85771905 .00011580 00000-0 36905-2 0 01 2 36869 21.6590 308.3213 7906308 185.8516 149.6593 1.54959798 08 Arc 20100828.04-0902.13 WRMS resid 0.024 totl 0.014 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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