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Stationary Turbulent Dynamo as Spontaneous Symmetry Breaking

Published online by Cambridge University Press:  19 July 2016

M. Hnatich
M. Hnatich*
Affiliation:
Institute of Experimental Physics of Slovak Academy of Sciences, Watsonova 47, 04001 Košice, Czecho-Slovakia

Extract

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The large-scale magnetic field generation by the turbulent motion energy, known as turbulent dynamo [1], is perspective candidate to explain the observed stationary magnetic fields of cosmic objects.

Type
6. General Aspects of Dynamo Theory
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 237 - 241
Copyright
Copyright © Kluwer 1993 

References

1. Vainshtein, S.I., Zeldovich, Ya.B., Ruzmaikin, A. Turbulentnoye dynamo v astrofizike , Nauka (Moscow), (1980), 351 pp.Google Scholar
2. Krause, F., Rädler, K.-H. Mean-field magnetohydrodynamics and dynamo theory, Pergamon, Oxford OX3 0BW (1980), 271 pp.Google Scholar
3. Adzhemyan, L. Ts., Vasilev, A.N., Hnatich, M. Teor. i mat. fizika (Russian J.) 72 (1987) 369.Google Scholar
4. De Dominicis, C., Martin, P.C. Phys. Rev. A 19 (1979) 419.Google Scholar
5. Adzhemyan, L. Ts., Vasilev, A.N., Pis'mak, Ju.M. Teor. i mat. fizika (Russian J.) 57 (1983) 268.Google Scholar
6. Adzhemyan, L. Ts., Vasilev, A.N., Hnatich, M. Teor. i mat. fizika (Russian J.) 64 (1985) 196.Google Scholar
7. Fournier, J.D., Sulem, P.L., Pouquet, A. Phys. Rev. A 15 (1982) 1393.Google Scholar