Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...501..407s&link_type=abstract
Astronomy and Astrophysics, Volume 501, Issue 2, 2009, pp.407-410
Astronomy and Astrophysics
Astrophysics
3
Plasmas, Shock Waves, Magnetohydrodynamics (Mhd), Solar Wind
Scientific paper
Aims: We reinvestigate the parallel pressure-anisotropic MHD shock with an emphasis on the downstream stability of the plasma with respect to the firehose instability. Methods: Aiming to close the underdetermined jump conditions, we take advantage of a kinetic model of the shock transit, based on the Boltzman-Vlasow equation with CGL invariants. In addition, we show that we need to consider plasma waves as an additional component of the system. Results: The system of jump conditions and the kinetic model reduces to a relatively simple form. At first glance, about all parallel magnetosonic shocks must be considerd unstable, at least with respect to plasma-wave generation caused by the firehose instability. In a similar way to this fundamental instability, the system will be also unstable when considering other plasma instabilities.
Fahr Hans Jörg
Siewert Mark
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