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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

Chiba, M. and Tosa, M.: 1990, Mon. Not. R. astr. Soc. 244, 714–726 Google Scholar
Hanasz, M., Lesch, H. and Krause, M.: 1991, Astr. Astrophys. 243, 381–385 Google Scholar
Landau, L.D. and Lifschitz, E.M.: 1969, Mechanics , Pergamon: Oxford Google Scholar
Ruzmaikin, A.A., Shukurov, A.M. and Sokoloff, D.D.: 1988, Magnetic Fields In Galaxies , Kluwer:Dordrecht Google Scholar
Schmitt, D. and Rüdiger, G.: 1992, Astr. Astrophys. , in press Google Scholar