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Theory of a turbulent dynamo

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Radiophysics and Quantum Electronics Aims and scope

Abstract

The Klyatskin-Tatarskii method is used in the article to obtain an equation for the dynamics of a magnetic field in a turbulent medium. The coefficients of diffusion and gyrotropy are obtained in the Markov and the first super-Markov approximations.

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Literature cited

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Authors and Affiliations

  1. Siberian Institute of Terrestrial Magnetism, the Ionosphere, and Radio-Wave Propagation, Siberian Branch, Academy of Sciences of the USSR, USSR

    S. I. Vainshtein

Authors
  1. S. I. Vainshtein
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 21, No.12, pp. 1803–1811, December, 1978.

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Vainshtein, S.I. Theory of a turbulent dynamo. Radiophys Quantum Electron 21, 1256–1262 (1978). https://doi.org/10.1007/BF02121908

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  • DOI: https://doi.org/10.1007/BF02121908

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