Abstract
Satellite magnetic anomaly maps derived by different techniques from Magsat/POGO data vary by more than a
factor of 2 in the deduced strength of the lithospheric magnetic field. Here, we present a first anomaly map from new CHAMP
scalar magnetic field data. After subtracting a recent Ørsted main and external field model, we remove remaining unmodeled
large-scale external contributions from 120 track segments by subtracting a best-fitting uniform field. In order to preserve
N/S trending features, the data are not filtered along-track. Direct integration of the spherically gridded data yields the final
degree 14-65 spherical harmonic expansion of the total intensity anomaly at the mean satellite altitude of 438 km. Apart from
enhanced long wavelength features and a smoother general appearance, our initial map is strikingly similar to one of the lower
strength Magsat/POGO maps.
| Original language | English |
|---|---|
| Journal | Geophyical Research Letters |
| Volume | 29 |
| Issue number | 14 |
| ISSN | 0094-8276 |
| Publication status | Published - 2002 |
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