Gene, Danny: Here is the time line for the MEX BSR on 25 April. This experiment looks very much like the one conducted on 19 April. The spacecraft is near apoapsis, the echo is narrow, and it barely moves in frequency. The downside is that the echoes will be weak, especially at S-Band because of the high spacecraft altitude; and the X-Band carrier will be outside the 25 kHz window while you are watching the echo. I'm building this timeline using fairly old predict files; but I doubt the final files would lead to any significant changes. Let me know if you notice any problems. Thanks and good luck, Dick 2009/115 (UTC) - - - - - - - 03:45 Begin Pre-cal at DSS 14 FGAIN = 60 dB (all channels, including X-RCP) FRO_X = 0; FRO_S = 0 (all SCHAN) Start 4-channel 25 kHz recordings after Step 4 Stop 25 kHz recording after Step 18 05:45 Begin track (X-Band may be ON; S-Band should be OFF) 06:03 S-Band Tx ON 06:19 Resume 25 kHz recording (SCHAN 3) Ask station to prepare for switching to planetary coordinates 06:29 Begin SLEW #1 06:30 Ask station to switch to "planetary pointing" (center of Mars) 06:34 FRO_X = +21000 Hz (SCHAN 3) FRO_S = +3000 Hz (SCHAN 3) FRO_X = +11000 Hz (SCHAN 4) 06:35 Begin Minical #1 06:50 End Minical #1 (end of Step 5) 06:59 End SLEW #1 Begin 4-channel 100 kHz recordings (SCHAN 4) Begin surface reflections Expect X-RCP and X-LCP to have similar magnitudes Expect S-RCP and S-LCP to have similar magnitudes, both weaker than X Echoes drift slowly to right during the hour; RCP should get stronger 08:04 End surface reflections Begin SLEW #2 End 100 kHz recordings 08:05 Begin Minical #2 08:20 End Minical #2 (end of step 5) 08:25 FRO_X = 0 FRO_S = 0 08:34 End SLEW #2 08:44 EOT (16 minutes early) Move antenna to zenith Begin post-cal when ready 10:00 End post-cal (or earlier, if post-cal complete) End 25 kHz recordings End of Activity