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Orsted Initial Field ModelMagnetic 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.
Document ID
20000092087
Acquisition Source
Goddard Space Flight Center
Document Type
Preprint (Draft being sent to journal)
Authors
Olsen, N.
(Danish Space Research Inst. Copenhagen, Denmark)
Holme, R.
(GeoForschungsZentrum Potsdam, Germany)
Hulot, G.
(Institut de Physique du Globe Paris, France)
Sabaka, T.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Neubert, T.
(Danish Meteorological Inst. Copenhagen, Denmark)
Toffner-Clausen, L.
(Danish Meteorological Inst. Copenhagen, Denmark)
Primdahl, F.
(Technical Univ. of Denmark Lyngby, Denmark)
Jorgensen, J.
(Technical Univ. of Denmark Lyngby, Denmark)
Leger, J.-M.
(Commissariat a l'Energie Atomique Paris, France)
Barraclough, D.
(Geological Survey of Britain Edinburgh United Kingdom)
Smith, David E.
Date Acquired
September 7, 2013
Publication Date
January 1, 2000
Subject Category
Geophysics
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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