Evaluation of the candidate Main Field model for IGRF 2000 derived from preliminary Ørsted data

On this occasion the selection of the IGRF for 2000 was left to a small Task Force. Before it was accepted by the Task Force as IGRF 2000, the final candidate model (a truncated version of Ørsted(10c/99)) was compared with a comprehensive set of independent surface and satellite data. The method, da...

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Veröffentlicht in:Earth, planets, and space planets, and space, 2000-01, Vol.52 (12), p.1183-1186
Hauptverfasser: Lowes, F. J., Bondar, T., Golovkov, V. P., Langlais, B., Macmillan, S., Mandea, M.
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Sprache:eng
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Zusammenfassung:On this occasion the selection of the IGRF for 2000 was left to a small Task Force. Before it was accepted by the Task Force as IGRF 2000, the final candidate model (a truncated version of Ørsted(10c/99)) was compared with a comprehensive set of independent surface and satellite data. The method, data selection, and results of this comparison are described.
ISSN:1880-5981
1880-5981
DOI:10.1186/BF03352350