Non-linear evolution of unstable acoustic waves in cosmic ray modified shocks

Details Non-linear evolution of unstable acoustic waves in cosmic ray modified shocks Non-linear evolution of unstable acoustic waves in cosmic ray modified shocks

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mnras.401.2799c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 401, Issue 4, pp. 2799-2804.

Astronomy and Astrophysics

Astronomy

1

Hydrodynamics, Instabilities, Shock Waves, Cosmic Rays

Scientific paper

The non-linear evolution of unstable acoustic waves in the precursors of
cosmic ray mediated shocks with large Mach numbers results in the
formation of a host of weak shock waves. These weak shocks heat the
thermal plasma, and therefore change the parameters of the strong
large-scale shock.

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