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On the Parametric Resonance in Thin Disk Galactic Dynamo

Published online by Cambridge University Press:  19 July 2016

K.M. Kuzanyan  and
D.D. Sokoloff
K.M. Kuzanyan
Affiliation:
Lomonosov University of Moscow, Department of Physics, Chair of Mathematics, 119899 Moscow, Russia
D.D. Sokoloff
Affiliation:
Lomonosov University of Moscow, Department of Physics, Chair of Mathematics, 119899 Moscow, Russia

Abstract

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The absence of parametric resonance by generation of the large-scale bisymmetric magnetic field in the framework of the simplest thin disk galactic dynamo model is shown.

Keywords

galactic dynamobisymmetric modeparametric resonance
Type
8. Magnetic Fields in Galaxies: Dynamo Theory
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 381 - 382
Copyright
Copyright © Kluwer 1993 

References

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