Stochastic scattering in Cen A radio lobes

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dc.contributor.authorSydorenko, M.V.
dc.contributor.authorMarchenko, V.V.
dc.contributor.authorSushchov, O.B.
dc.contributor.authorKobzar, O.O.
dc.date.accessioned2017-06-07T18:51:36Z
dc.date.available2017-06-07T18:51:36Z
dc.date.issued2013
dc.description.abstractThe 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 influence of stochastic scattering in Cen A radio lobes on correlation of the ultra high energy cosmic rays (UHECR) events registered by Auger observatory with Cen A is studied. Typical radio lobe regions, which UHECR of different chemical composition are supposed to come from, are estimated by applying numerical modelling of UHECR scattering with Fermi II mechanism in the turbulent regions.uk_UA
dc.identifier.citationStochastic 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.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119647
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleStochastic scattering in Cen A radio lobesuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2013, вип. 2