PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM STANDARD_DATA_PRODUCT_ID = HEA DATA_SET_ID = "MEX-M-MRS-1/2/3-PRM-0547-V1.0" PRODUCT_ID = "M00SUE0L1A_HEA_052490421_00.TXT" PRODUCT_CREATION_TIME = 2008-07-01T10:41:25.000 PRODUCER_ID = "SUE" INSTRUMENT_HOST_ID = "MEX" OBJECT = TEXT PUBLICATION_DATE = 2005-09-28 NOTE = "DSN MEX RSR Data Collection: BSR 249" END_OBJECT = TEXT END Miscellaneous ============= This is the first report since HEA5270A.TXT. Joe Twicken reports that he did not receive HEA5266A.TXT, which reported on radio occultation data collection for days 243 to 262 and 100 kHz bistatic radar data collection for day 243. If others have not received this report, please let me know and I will send it again. Open Loop Data ============== Data Collection --------------- We have completed quick-look processing on the following MEX RSR open loop 25 kHz bistatic radar data at Stanford: DOY DSS RSR BAND RSR CH KSPS BT REC RECS RSR MAX START STOP ID RS LEN FILE NAME SNR --- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ ----- 249 63 04:21:00 05:30:00 -/XR 4 3 25 16 25260 16561 5249042A.RSR 3.8 249 63 07:05:00 07:43:00 -/XR 4 3 25 16 25260 9121 5249070A.RSR 72.7 249 63 07:43:00 08:13:00 -/XR 4 3 25 16 25260 7201 5249074A.RSR 74.8 249 63 08:13:00 08:43:00 -/XR 4 3 25 16 25260 7201 5249081A.RSR 39.5 249 63 08:43:00 09:13:00 -/XR 4 3 25 16 25260 7201 5249084A.RSR 74.5 249 63 09:13:00 09:50:00 -/XR 4 3 25 16 25260 8881 5249091A.RSR 3.7 249 63 04:21:00 05:30:00 -/XL 2 3 25 16 25260 16561 5249042C.RSR 4.9 249 63 07:05:00 07:43:00 -/XL 2 3 25 16 25260 9121 5249070C.RSR 46.9 249 63 07:43:00 08:13:00 -/XL 2 3 25 16 25260 7201 5249074C.RSR 48.6 249 63 08:13:00 08:43:00 -/XL 2 3 25 16 25260 7201 5249081C.RSR 28.4 249 63 08:43:00 09:13:00 -/XL 2 3 25 16 25260 7201 5249084C.RSR 48.6 249 63 09:13:00 09:50:00 -/XL 2 3 25 16 25260 8881 5249091C.RSR 4.0 249 63 04:21:00 05:30:00 -/SR 3 3 25 16 25260 16561 5249042B.RSR 3.6 249 63 07:05:00 07:43:00 -/SR 3 3 25 16 25260 9121 5249070B.RSR 53.0 249 63 07:43:00 08:13:00 -/SR 3 3 25 16 25260 7201 5249074B.RSR 53.0 249 63 08:13:00 08:43:00 -/SR 3 3 25 16 25260 7201 5249081B.RSR 24.1 249 63 08:43:00 09:13:00 -/SR 3 3 25 16 25260 7201 5249084B.RSR 52.5 249 63 09:13:00 09:50:00 -/SR 3 3 25 16 25260 8881 5249091B.RSR 4.7 249 63 04:21:00 05:30:00 -/SL 1 3 25 16 25260 16561 5249042D.RSR 4.1 249 63 07:05:00 07:43:00 -/SL 1 3 25 16 25260 9121 5249070D.RSR 26.4 249 63 07:43:00 08:13:00 -/SL 1 3 25 16 25260 7201 5249074D.RSR 29.3 249 63 08:13:00 08:43:00 -/SL 1 3 25 16 25260 7201 5249081D.RSR 14.8 249 63 08:43:00 09:13:00 -/SL 1 3 25 16 25260 7201 5249084D.RSR 30.0 249 63 09:13:00 09:50:00 -/SL 1 3 25 16 25260 8881 5249091D.RSR 3.5 We have completed quick-look processing on the following MEX RSR open loop 100 kHz bistatic radar data at Stanford: DOY DSS RSR BAND RSR CH KSPS BT REC RECS RSR MAX START STOP ID RS LEN FILE NAME SNR --- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ ----- 249 63 08:13:00 08:28:00 -/XR 4 4 100 16 20260 18001 5249081E.RSR 44.8 249 63 08:13:00 08:28:00 -/SR 3 4 100 16 20260 18001 5249081F.RSR 28.2 249 63 08:13:00 08:28:00 -/XL 2 4 100 16 20260 18001 5249081G.RSR 33.9 249 63 08:13:00 08:28:00 -/SL 1 4 100 16 20260 18001 5249081H.RSR 18.4 249 63 08:28:00 08:42:59 -/XR 4 4 100 16 20260 17981 5249082A.RSR 44.2 249 63 08:28:00 08:42:59 -/SR 3 4 100 16 20260 17981 5249082B.RSR 27.9 249 63 08:28:00 08:42:59 -/XL 2 4 100 16 20260 17981 5249082C.RSR 33.5 249 63 08:28:00 08:42:59 -/SL 1 4 100 16 20260 17981 5249082D.RSR 17.7 An egress atmospheric occultation was captured at S-band; but apparently the X-band transmitter was not turned on until after the occultation. The data appear to be of good quality. An operations error resulted in collection of little or no spacecraft calibration data after the HGA slew back to Earth. Instead of monitoring S- and X-band carrier levels until 09:58, the station broke track at 09:10 and began the post-calibration. The reason for this error is not known; if the pre-experiment spacecraft calibration data are good, there should be little or no impact on the science. We are now up to date in collection and quick-look processing of radio occultation and bistatic radar data.