Abstract
The main instrument for the mapping of theEarth's magnetic field
onboard the Danishgeomagnetic satellite rsted is the
"gondola"consisting og a compact spherical coilfluxgate vector
magnetometer (CSC) and a star image (SIM). The SIM gives the
attitude relativeto the rectascension-declination system bytaking
a snapshot of the sky, the CSCmeasures the magnetic field vector
in aninstrument coordinate system. The attitude relation (gondola
quaternion) between the star camera system and the magnetometer
system is a fundamental instrument constant to be determined by
calibration with arc seconds accuracy. Intercalibration has been
carried out at thegeomagnetic observatory at Brorfelde,
Denmark.Snapshots of the sky was taken with simul-taneous readings
of the CSC magnetometer andthe observatory variometer. The SIM
attitudeis reduced to the local geomagnetic systemby time and
astronomical data and the observatoryfield observation is
transformed to the SIMcoordinate system. By comparison with the
CSC readings the orthogonal transformation can be found. The
procedure is equivalent to a magnetic calibration in a test coil
system and the magnetometer constants can likevise be
determined.Results from the calibration of the Ørsted instrument
is presented.
Original language | English |
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Title of host publication | Small Satellite for Earth Observation |
Place of Publication | Berlin, New York |
Publisher | W de Gruyter |
Publication date | 1996 |
Pages | 152-155 |
Publication status | Published - 1996 |
Event | Small Satellite for Earth Observation - Berlin Duration: 1 Jan 1996 → … |
Conference
Conference | Small Satellite for Earth Observation |
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City | Berlin |
Period | 01/01/1996 → … |