Modeling Bell's Non-resonant Cosmic Ray Instability

Details Modeling Bell's Non-resonant Cosmic Ray Instability Modeling Bell's Non-resonant Cosmic Ray Instability

2008-01-29

arxiv.org/abs/0801.4486v2

Astronomy and Astrophysics

Astrophysics

12 pages, 4 figures, accepted to ApJ

Scientific paper

10.1086/529579

We have studied the non-resonant streaming instability of charged energetic
particles moving through a background plasma, discovered by Bell (2004). We
confirm his numerical results regarding a significant magnetic field
amplification in the system. A detailed physical picture of the instability
development and of the magnetic field evolution is given.

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