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Magnetic Field of Rotating Bodies

Published online by Cambridge University Press:  19 July 2016

A.Z. Dolginov
A.Z. Dolginov*
Affiliation:
A.F. Ioffe Physical-Technical Institute Academy of Sciences Politechnical str. 26 194021 Leningrad USSR

Abstract

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Difficulties of the dynamo and alternative theories of the magnetic field generation are briefly discussed. The correlation between η = lg μ/μo and ζ = lg J/Jo for rotating celestial bodies is considered. μ is the magnetic and J the angular momentum of the body. Existing theories do not explain such a correlation, and it may be an evidence for some new fundamental interaction.

Type
1. A Survey of Magnetic Phenomena near the Solar Photosphere, in the Corona, and in Stellar Winds
Information
Symposium - International Astronomical Union , Volume 140: Galactic and Intergalactic Magnetic Fields , 1990 , pp. 27 - 28
Copyright
Copyright © Kluwer 1990 

References

Dolginov, A.Z. (1988) “Magnetic field generation in celestial bodies”, Phys. Rep. 162, No. 6, 337–415.Google Scholar