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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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| Autores principales: | , |
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| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Academy of Science of South Africa
2011-01-01
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| Colección: | South African Journal of Science |
| Materias: | |
| Acceso en línea: | http://archive.sajs.co.za/index.php/SAJS/article/view/275 |
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