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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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| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Головна астрономічна обсерваторія НАН України
2013
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| Series: | Advances in Astronomy and Space Physics |
| Online Access: | http://dspace.nbuv.gov.ua/handle/123456789/119647 |
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