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Initial geomagnetic field model from MAGSATMagsat 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.
Document ID
19800017470
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Langel, R. A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Estes, R. H.
(Business and Technological Systems Seabrook, Md., United States)
Mead, G. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Fabiano, E. B.
(USGS Denver, Colo., United States)
Lancaster, E. R.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 4, 2013
Publication Date
April 1, 1980
Subject Category
Geophysics
Report/Patent Number
NASA-TM-80679
Report Number: NASA-TM-80679
Accession Number
80N25967
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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