Abstract
The Swedish micro-satellite Astrid-2 was successfully launched
into a near polar orbit last December 98. Despite the fact that
its primary mission was the research of Auroral phenomena, the
magnetic instrumentation has been designed to accomplish high
resolution vector field magnetic measurements and therefore the
mapping of the Earth's magnetic field may be possible. The
spinning of the spacecraft about a certain axis makes the
stabilisation in space possible. This fact and the well
distributed data over the globe makes the magnetic data well
suited for the estimation of the magnetic field model at the
spacecraft altitude (circa 1000km). Several methods for field
modelling are presented in this paper with the assumption that the
direction of the spin axis is nearly constant. In any case the
orientation of the magnetometer is to bedetermined simultaneously
with the instrument calibration and main field model coefficients.
Hence, apart from the scientific use of the magnetic data, the
attitude recovery of the spacecraft may be estimated with more
precision.
Original language | English |
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Journal | Eos Trans. AGU, Fall Meet. Suppl. |
Volume | 80 |
Issue number | 17 |
Pages (from-to) | F892 |
Publication status | Published - 1999 |
Event | AGU 1999 Fall Meeting - San Francisco, United States Duration: 13 Dec 1999 → 17 Dec 1999 |
Conference
Conference | AGU 1999 Fall Meeting |
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Country/Territory | United States |
City | San Francisco |
Period | 13/12/1999 → 17/12/1999 |