Abstract
We present numerical evidence from two dimensional simulations that the growth of the Richtmyer-Meshkov instability is suppressed in the presence of a magnetic field. A bifurcation occurs during the refraction of the incident shock on the density interface which transports baroclinically generated vorticity away from the interface to a pair of slow or intermediate magnetosonic shocks. Consequently, the density interface is devoid of vorticity and its growth and associated mixing is completely suppressed. © 2003 American Institute of Physics.
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CITATION STYLE
Samtaney, R. (2003). Suppression of the Richtmyer-Meshkov instability in the presence of a magnetic field. Physics of Fluids, 15(8). https://doi.org/10.1063/1.1591188
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