PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM STANDARD_DATA_PRODUCT_ID = HEA DATA_SET_ID = "MEX-M-MRS-1/2/3-EXT2-1549-V1.0" PRODUCT_ID = "M00SUE0L1A_HEA_082401854_00.TXT" PRODUCT_CREATION_TIME = 2011-07-21T18:03:48.000 PRODUCER_ID = "SUE" INSTRUMENT_HOST_ID = "MEX" OBJECT = TEXT PUBLICATION_DATE = 2008-08-28 NOTE = "DSN MEX Occultation Data" END_OBJECT = TEXT END Miscellaneous ============= This is the first report since HEA8233A.TXT. No additional MEX open loop data are expected through at least 7 September 2008. Open Loop Data ============== Data Collection --------------- We have completed quick-look processing on the following MEX RSR open loop radio occultation data at Stanford: DOY DSS RSR BAND RSR CH KSPS BT REC RECS RSR MAX START STOP ID RS LEN FILE NAME SNR --- --- -------- -------- ---- --- -- ---- -- ----- ----- ------------ ----- 240 63 18:54:00 19:14:00 X/XR 4 1 2 16 8260 1201 8240185A.RSR 53.6 240 63 18:54:00 19:14:00 X/SR 3 1 2 16 8260 1201 8240185B.RSR 40.6 241 65 15:26:00 15:45:59 X/XR 4 1 2 16 8260 1200 8241152A.RSR 49.1 241 65 15:26:00 15:45:59 X/SR 3 1 2 16 8260 1200 8241152B.RSR 31.9 These observations appear to have been conducted with spacecraft telemetry modulation ON. The DSS 63 carrier signal-to-noise is 5 dB lower than on day 231 when DSS 14 (also 70-m) was used. There are variations of up to +/-0.5 dB in the X-Band carrier level prior to ingress on day 240. These are mimicked (at about +/-0.15 dB) in the S-Band carrier level. The carrier levels on day 241 are very stable by comparison. The S-to-X correlation (with DSS 63 only) suggests that ground antenna pointing may have been the cause. The X-Band power spectra from day 240 show weak spurs at about +/-180 and +/-500 Hz on either side of the carrier. These harmonics are commonly seen at low levels when observing signals at or above 50 dB/Hz. Very weak +/-180 Hz harmonics are seen in the data from day 241.