Weibel, Firehose and Mirror mode Relations
Space Physics
2014-01-23 v1 Solar and Stellar Astrophysics
Abstract
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.
Keywords
Cite
@article{arxiv.1401.2522,
title = {Weibel, Firehose and Mirror mode Relations},
author = {R. A. Treumann and W. Baumjohann},
journal= {arXiv preprint arXiv:1401.2522},
year = {2014}
}
Comments
6 pages, no figures, in press