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CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR
MISSION_NAME          = MARS_GLOBAL_SURVEYOR;
SPACECRAFT_NAME       = MARS_GLOBAL_SURVEYOR;
DATA_SET_ID           = STATUS_REPORT;
FILE_NAME             = INSTRPT_MAG_20010312_000000;
PRODUCER_ID           = MGS_MAG_TEAM;
PRODUCER_FULL_NAME    = "MONTE KAELBERER, EVER GUANDIQUE";
PRODUCT_CREATION_TIME = 2001-03-12T20:20:00.000;
END
CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA
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MAG TEAM REVIEW:

This MGS MAG/ER status report covers the period: 
4-10 March 2001 (DOY's 63-69)

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/sr01063-069.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

No MAG/ER NIPC's were radiated during this period.

- According to DSN status reports, the first gap in DOY 64 is due to DSN
  problems.  The second gap is due to partition 6 not being played back
  (mapping sequence 119).
- The gap in DOY 65 is due to DSN problems according to DSN status
  reports.
- There are three gaps in DOY 66:  The first gap is due to DSN problems
  (DSN status reports), the second one is due to partition 6 not being
  played back (mapping sequence 120), and the third one is assumed due to
  scheduling conflicts associated with playing back partition 7.
- The two gaps in DOY 68, according to DSN status reports, are due to DSN
  problems.
- DOY 69 has two gaps that are unexplained.  However, the gap at the end 
  of the day is assumed due to scheduling conflicts associated with playing 
  back partition 7. 
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CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA

Last Modified: Mon Mar 12 15:13:04 EST 2001

Curator: Monte Kaelberer, Emergent
Email: Monte.S.Kaelberer@gsfc.nasa.gov

Responsible NASA Representative: Mario Acuña
Email: Mario.H.Acuna.1@gsfc.nasa.gov