'
CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR MISSION_NAME = MARS_GLOBAL_SURVEYOR; SPACECRAFT_NAME = MARS_GLOBAL_SURVEYOR; DATA_SET_ID = STATUS_REPORT; FILE_NAME = INSTRPT_MAG_20030902_000000; PRODUCER_ID = MGS_MAG_TEAM; PRODUCER_FULL_NAME = "MONTE KAELBERER, EVER GUANDIQUE"; PRODUCT_CREATION_TIME = 2003-09-02T19:45:00.000; END CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ MAG TEAM REVIEW: This MGS MAG/ER status report covers the period: 24-30 August 2003 (DOY's 236-242) MAG/ER instrument temperatures, currents, and voltages are within nominal ranges. A gif plot of the instrument parameters for the week is located at: http://mgs-mager.gsfc.nasa.gov/status/sr03236-242.html Previous status reports for the magnetometer and electron reflectometer instruments can be selected for viewing at: http://mgs-mager.gsfc.nasa.gov/status/index.html The plotted quantities are: MCP_V-->micro-channel plate voltage A_MA--->controller current A_TEMP--->controller temperature ER_TEMP-->ER temperature IB_TEMP-->inboard temperature OB_TEMP-->outboard temperature There were no instrument commands radiated this period. The slight rise in the A_TEMP and ER_TEMP temperatures during DOYs 238-241 was due to the Mars Relay UHF Experiment. The large gaps at the end of DOYs 236, 237, 240, and 242 are due to a lack of data playback (mapping sequence 308-310). According to DSN status reports, the small (~40 min) gap in DOY 239 is due to DSN problems. $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA
Last Modified: Tue Sep 2 15:53:49 EDT 2003
Curator: Monte Kaelberer, L-3 Communications
Email: Monte.S.Kaelberer@gsfc.nasa.gov
Responsible NASA Representative: Mario Acuņa
Email: Mario.H.Acuna@nasa.gov