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arxiv: 1401.2522 · v1 · pith:PO5WLSBNnew · submitted 2014-01-11 · ⚛️ physics.space-ph · astro-ph.SR

Weibel, Firehose and Mirror mode Relations

classification ⚛️ physics.space-ph astro-ph.SR
keywords weibel-likeadditionanisotropicconditionsfieldfirehosemagneticmirror
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Excitation of Weibel magnetic fields in an initially non-magnetized though anisotropic plasma may trigger other low-frequency instabilities fed by pressure anisotropy. It is shown that under Weibel-like-stable conditions the Weibel-like thermal fluctuation magnetic field allows for restricted Firehose-mode growth. In addition, low frequency Whistlers can also propagate in the plasma under certain anisotropic conditions. When the Weibel-like mode becomes unstable, Firehose instability ceases but Mirror modes take over. This will cause bubble structures in the Weibel-like field in addition to filamentation.

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