'
CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR MISSION_NAME = MARS_GLOBAL_SURVEYOR; SPACECRAFT_NAME = MARS_GLOBAL_SURVEYOR; DATA_SET_ID = STATUS_REPORT; FILE_NAME = INSTRPT_MAG_20040202_000000; PRODUCER_ID = MGS_MAG_TEAM; PRODUCER_FULL_NAME = "MONTE KAELBERER, EVER GUANDIQUE"; PRODUCT_CREATION_TIME = 2004-02-02T16:00:00.000; END CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ MAG TEAM REVIEW: This MGS MAG/ER status report covers the period: 25-31 January 2004 (DOY's 025-031) MAG/ER instrument temperatures, currents, and voltages are within nominal ranges. A gif plot of the instrument parameters for the week is located at: http://mgs-mager.gsfc.nasa.gov/status/sr04025-031.html Previous status reports for the magnetometer and electron reflectometer instruments can be selected for viewing at: http://mgs-mager.gsfc.nasa.gov/status/index.html The plotted quantities are: MCP_V-->micro-channel plate voltage A_MA--->controller current A_TEMP--->controller temperature ER_TEMP-->ER temperature IB_TEMP-->inboard temperature OB_TEMP-->outboard temperature There were no instrument commands radiated this period. According to DSN status reports, the large (~1 hr) gap in DOY 027 is due to DSN problems. The change in OB_TEMP starting on DOY 028 was caused by switching the solar array elevational offset angle from 25 degrees to 0 degrees (this is to increase electrical power margins as the spacecraft/sun distance increases). The slight temperature variation in IB_TEMP and OB_TEMP on DOY 030 was due to a MOC CPROTO event. $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA
Last Modified: Mon Feb 2 11:47:51 EST 2004
Curator: Monte Kaelberer, L-3 Communications
Email: Monte.S.Kaelberer@gsfc.nasa.gov
Responsible NASA Representative: Mario Acuņa
Email: Mario.H.Acuna@nasa.gov