'
CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR MISSION_NAME = MARS_GLOBAL_SURVEYOR; SPACECRAFT_NAME = MARS_GLOBAL_SURVEYOR; DATA_SET_ID = STATUS_REPORT; FILE_NAME = INSTRPT_MAG_20050926_000000; PRODUCER_ID = MGS_MAG_TEAM; PRODUCER_FULL_NAME = "MONTE KAELBERER, EVER GUANDIQUE"; PRODUCT_CREATION_TIME = 2005-09-26T15:40:00.000; END CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ MAG TEAM REVIEW: This MGS MAG/ER status report covers the period: 18-24 September 2005 (DOYs 261-267) MAG/ER instrument temperatures, currents, and voltages are within nominal ranges. A gif plot of the instrument parameters for the week is located at: http://mgs-mager.gsfc.nasa.gov/status/sr05261-267.html Previous status reports for the magnetometer and electron reflectometer instruments can be selected for viewing at: http://mgs-mager.gsfc.nasa.gov/status/index.html The plotted quantities are: MCP_V-->micro-channel plate voltage A_MA--->controller current A_TEMP--->controller temperature ER_TEMP-->ER temperature IB_TEMP-->inboard temperature OB_TEMP-->outboard temperature There were no instrument commands radiated this period. Gaps on DOY 261 occurred because the recorders were not yet being used. Background sequences, with recorder schedules, were first started at 0000 UTC on DOY 262. According to DSN status reports, the large (~2.5 hr) gap on DOY 263 is due to DSN problems. The slight temperature variations in IB_TEMP and OB_TEMP on DOY 262 were due to a MOC CPROTO event. The temperature variations on DOYs 264 and 267 were due to the MOLA earth-pointing experiments. The slight rise in A_TEMP on DOY 266 was due to the TES turn-on. $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA
Last Modified: Mon Sep 26 12:04:59 EDT 2005
Curator: Monte Kaelberer, L-3 Communications
Email: Monte.S.Kaelberer@gsfc.nasa.gov
Responsible NASA Representative: Mario Acuņa
Email: Mario.H.Acuna@nasa.gov