Stochastic scattering in Cen A radio lobes

The results of direct numerical modelling of the cosmic ray acceleration in strongly excited turbulence, where quasi-linear theory is non-applicable, are presented. We model turbulent plasma by a set of randomly propagated Alfvén waves with Kolmogorov spectrum of magnetic field fluctuations. The inf...

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Datum:2013
Hauptverfasser: Sydorenko, M.V., Marchenko, V.V., Sushchov, O.B., Kobzar, O.O.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2013
Schriftenreihe:Advances in Astronomy and Space Physics
Online Zugang:http://dspace.nbuv.gov.ua/handle/123456789/119647
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Stochastic scattering in Cen A radio lobes / M.V. Sydorenko, V.V. Marchenko, O.B. Sushchov, O.O. Kobzar // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 2. — С. 126-130. — Бібліогр.: 14 назв. — англ.

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