NASA NTRS · 19800017470
Initial geomagnetic field model from MAGSAT
Abstract
Magsat data from magnetically quiet days were used to derive a thirteenth degree and order spherical harmonic geomagnetic field model, MGST(3/80). The model utilized both scalar and vector data and fit that data with standard deviations of 8, 52, 55 and 97 nT for the scalar magnitude, B sub r, B sub theta and B sub phi respectively. When compared with earlier models, the Earth's dipole moment continues to decrease at a rate of about 26 nT/year. Evaluation of earlier models with Magsat data shows that the scalar field at the Magsat epoch is best predicted by the POGO(2/72) model but that the AWC/75 and IGS/75 are better for predicting vector fields.
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Langel, R. A., Estes, R. H., Mead, G. D., Fabiano, E. B., Lancaster, E. R.. 1980-04-01. Initial geomagnetic field model from MAGSAT. https://ntrs.nasa.gov/citations/19800017470
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