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...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Academy of Science of South Africa
2011-01-01
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| Series: | South African Journal of Science |
| Subjects: | |
| Online Access: | http://192.168.0.108/index.php/sajs/article/view/9888 |