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On the Gyrotropic Magnetohydrodynamic Turbulence

Published online by Cambridge University Press:  19 July 2016

M. Hnatich  and
M. Stehlik
M. Hnatich
Affiliation:
Institute of Experimental Physics of Slovak Academy of Sciences, Košice, Czecho-Slovakia
M. Stehlik
Affiliation:
Institute of Experimental Physics of Slovak Academy of Sciences, Košice, Czecho-Slovakia

Extract

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1. The reflective non-symmetric (gyrotropic) stochastic magnetic hydrodynamics (MHD) turbulence is investigated by a quantum-field (QF) theory method including a renormalization group (RG), that has been successfully applied to the fully developed HD turbulence [1,2] and to the ordinary (reflective symmetric) MHD turbulence [3].

Type
6. General Aspects of Dynamo Theory
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 243 - 244
Copyright
Copyright © Kluwer 1993 

References

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3. Adzhemyan, L. Ts., Vasilev, A.N., Hnatich, M. Teor. Mat. Fiz. (Russian J.) 64 (1985) 196.Google Scholar
4. Hnatich, M., Stehlik, M. in Renormalization Group'91 , Eds. Shirkov, D.V., Priezzhev, V.B., World Scientific Publishing Co. Pte. Ltd., Singapore, 1992.Google Scholar
5. Adzhemyan, L. Ts., Vasilev, A. N., Hnatich, M. Teor. Mat. Fiz. (Russian J.) 72 (1987) 369.Google Scholar
6. Hnatich, M. Stationary turbulent dynamo as spontaneous symmetry breaking , these Proceedings.Google Scholar