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Dynamics of Large-Scale Magnetic Fields

Published online by Cambridge University Press:  14 August 2015

G. V. Kuklin
G. V. Kuklin*
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Irkutsk, U.S.S.R.

Abstract

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A discussion is given of the dynamics of large-scale solar magnetic fields as a joint action of a transport by a regular velocity field, by a generalized diffusion, by coming to the surface and sinking and by sources of origin and destruction of magnetic fields. Also these processes are discussed using the observed picture of magnetic field dynamics.

Type
Part VII: The Polar Fields of the Sun and the Magnetic Activity Cycle
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 737 - 743
Copyright
Copyright © Reidel 1971 

References

Bumba, V. and Howard, R. F.: 1965, Astrophys. J. 141, 1502.CrossRefGoogle Scholar
Leighton, R. B.: 1964, Astrophys. J. 140, 1547.CrossRefGoogle Scholar