Analysis of the remanent field on the basis of a Cosmos-49 model

Details Analysis of the remanent field on the basis of a Cosmos-49 model Analysis of the remanent field on the basis of a Cosmos-49 model

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975kosis..13..236a&link_type=abstract

Kosmicheskie Issledovaniia, vol. 13, Mar.-Apr. 1975, p. 236-241. In Russian.

Mathematics

Cosmos Satellites, Geomagnetism, Magnetic Field Configurations, Remanence, Spherical Harmonics, Amplitudes, Harmonic Functions, Magnetic Measurement, Mathematical Models, Satellite Observation

Scientific paper

Ben'kova (1973) has calculated the distribution of the remanent magnetic field as the difference between the measurements onboard the Cosmos 49 satellite and the values obtained with a Cosmos-49 model, using nine terms of a series in spherical harmonic functions. The possibility of improving modular models by increasing the number of terms of the series is studied by analyzing the distribution of the remanent magnetic field.

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