The nonlinear amplification of magnetic fields by cosmic rays at supernova remnant shocks
A central problem in the theory of cosmic ray acceleration at supernova shock fronts is the generation of turbulent magnetic fields needed to scatter particles across a shock front. In this paper we build on previous studies [1], [2] into the effect of streaming cosmic rays produced by the outer sho...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2006
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