Cosmic ray propagation in a fractal galactic medium

Simple cosmic ray diffusion in magnetic fields is often discussed in terms of a characteristic scattering mean free path or equivalent diffusion coefficient. This assumes very simple properties of the structure of astrophysical magnetic fields. A better approximation is to assume that the magnetic s...

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Bibliografiska uppgifter
Huvudupphovsmän: Hamid A. Kermani, Jalileldin Fatemi
Materialtyp: Artigo
Språk:Inglês
Publicerad: Academy of Science of South Africa 2011-01-01
Serie:South African Journal of Science
Ämnen:
cosmic ray
diffusion
fractal
magnetic field
Länkar:http://archive.sajs.co.za/index.php/SAJS/article/view/275
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