'
CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR MISSION_NAME = MARS_GLOBAL_SURVEYOR; SPACECRAFT_NAME = MARS_GLOBAL_SURVEYOR; DATA_SET_ID = STATUS_REPORT; FILE_NAME = INSTRPT_MAG_20030811_000000; PRODUCER_ID = MGS_MAG_TEAM; PRODUCER_FULL_NAME = "MONTE KAELBERER, EVER GUANDIQUE"; PRODUCT_CREATION_TIME = 2003-08-11T16:00:00.000; END CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ MAG TEAM REVIEW: This MGS MAG/ER status report covers the period: 3-9 August 2003 (DOY's 215-221) MAG/ER instrument temperatures, currents, and voltages are within nominal ranges. A gif plot of the instrument parameters for the week is located at: http://mgs-mager.gsfc.nasa.gov/status/sr03215-221.html Previous status reports for the magnetometer and electron reflectometer instruments can be selected for viewing at: http://mgs-mager.gsfc.nasa.gov/status/index.html The plotted quantities are: MCP_V-->micro-channel plate voltage A_MA--->controller current A_TEMP--->controller temperature ER_TEMP-->ER temperature IB_TEMP-->inboard temperature OB_TEMP-->outboard temperature There were no instrument commands radiated this period. According to DSN status reports, the large (~2 hr) gap in DOY 217 is due to DSN problems. The first large (~1.5) gap in DOY 218 is unexplained. The large (~1.5 hr) gap at the end of DOY 218 is due to limited DSN coverage (mapping sequence 303). According to MGS ACE reports, the large (~2 hr) gap in DOY 219 is due to DSN problems. Gaps in DOYs 220-221 are due to limited DSN coverage (mapping sequences 303 and 304). $$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$$ CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA
Last Modified: Mon Aug 11 12:01:10 EDT 2003
Curator: Monte Kaelberer, L-3 Communications EER Corporation
Email: Monte.S.Kaelberer@gsfc.nasa.gov
Responsible NASA Representative: Mario Acuņa
Email: Mario.H.Acuna@nasa.gov