A filamentation instability for streaming cosmic rays
We demonstrate that cosmic rays form filamentary structures in the precursors of supernova remnant shocks due to their self-generated magnetic fields. The cosmic ray filamentation results in the growth of a long-wavelength instability, and naturally couples the rapid non-linear amplification on smal...
| Váldodahkkit: | , |
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| Materiálatiipa: | Journal article |
| Giella: | English |
| Almmustuhtton: |
2012
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