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Evolutionarity of MHD Discontinuities

Part of the Astrophysics and Space Science Library book series (ASSL, volume 341)

Abstract

A discontinuity cannot exist in astrophysical plasma with magnetic field if small perturbations disintegrate it into other discontinuities or transform it to a more general nonsteady flow.

Keywords

Shock Wave Discontinuity Surface Tangential Discontinuity Dissipative Wave Unstable Node 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media, LLC 2006

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