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Mars Global Surveyor Magnetic Field Experiment

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MGS MAG/ER Status Report for Year 2002 DOYs 069-075 Mars Global Surveyor MAG/ER
MGS MAG/ER Investigation Status

MGS MAG/ER Status Report for Year 2002 DOYs 069-075

plots of Volts vs. MCP_V and A_MA, and Degrees C vs IB_TEMP,
OB_TEMP, A_TEMP, and ER_TEMP

CCSD3ZS0000111111111NJPL3KS0L015MOMAGDSR
MISSION_NAME          = MARS_GLOBAL_SURVEYOR;
SPACECRAFT_NAME       = MARS_GLOBAL_SURVEYOR;
DATA_SET_ID           = STATUS_REPORT;
FILE_NAME             = INSTRPT_MAG_20020318_000000;
PRODUCER_ID           = MGS_MAG_TEAM;
PRODUCER_FULL_NAME    = "MONTE KAELBERER, EVER GUANDIQUE";
PRODUCT_CREATION_TIME = 2002-03-18T20:00:00.000;
END
CCSD3RE00000MOMAGDSRNJPL3IS00175GSFCACNA
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MAG TEAM REVIEW:

This MGS MAG/ER status report covers the period: 
10-16 March, 2002 (DOY's 69-75)

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/sr02069-075.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 commands were radiated this period.

The temperature increase in A_TEMP on DOY 71 was due to the TES 
instrument turn-on.

The temperature increase in OB_TEMP on DOY 73 corresponds to the return to
beta-supplement mapping.

According to DSN status reports, gaps in DOY's 71 and 73 are due to DSN
problems.

Gaps in DOY's 72, 74 and 75 are unexplained.

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CCSD3RE00000MOMAGDSRCCSD3RE00000GSFCACNA


Last Modified: Mon Mar 18 15:08:01 EST 2002

Curator: Monte Kaelberer, L3 Analytics
Email: Monte.S.Kaelberer@gsfc.nasa.gov

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

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MGS MAG/ER is an international collaboration by: