A current driven instability in parallel, relativistic shocks
Recently, Bell [2] has reanalysed the problem of wave excitation by cosmic rays propagating in the pre-cursor region of a supernova remnant shock front. He pointed out a strong, nonresonant, current-driven instability previously overlooked in kinetic treatments [1, 5] and suggested that it can subst...
| Päätekijät: | , , |
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| Aineistotyyppi: | Journal article |
| Kieli: | English |
| Julkaistu: |
2006
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