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Hydromagnetic turbulence, shock waves and particle acceleration in supernova remnants

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Abstract

A number of mechanisms for generation of the small-scale hydromagnetic turbulence in Supernova remnants is investigated. It is shown that the mechanisms of particle acceleration on the shock waves and on the large-scale turbulence face considerable difficulties.

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Authors and Affiliations

  1. A. F. Ioffe Physical Technical Institute, Leningrad, Russia

    V. N. Fedorenko

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  1. V. N. Fedorenko
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Fedorenko, V.N. Hydromagnetic turbulence, shock waves and particle acceleration in supernova remnants. Astrophys Space Sci 96, 25–36 (1983). https://doi.org/10.1007/BF00661940

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  • DOI: https://doi.org/10.1007/BF00661940

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