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NASA NTRS · 20000092087

Orsted Initial Field Model

Abstract

Magnetic measurements taken by the Orsted satellite during geomagnetic quiet conditions around January 1, 2000 have been used to derive a spherical harmonic model of the Earth's magnetic field for epoch 2000.0. The maximum degree and order of the model is 19 for internal, and 2 for external, source fields; however, coefficients above degree 14 may not be robust. Such detailed models exist for only one previous epoch, 1980. Achieved rms misfit is 2 nT for the scalar intensity and 4 nT for the vector components perpendicular to the magnetic field. This model is of higher detail than the IGRF 2000, which for scientific purposes related to the Orsted mission it supersedes.

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Olsen, N., Holme, R., Hulot, G., Sabaka, T., Neubert, T., Toffner-Clausen, L., Primdahl, F., Jorgensen, J., Leger, J.-M., Barraclough, D., Smith, David E.. 2000-01-01. Orsted Initial Field Model. https://ntrs.nasa.gov/citations/20000092087

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