Self-similar strong magnetogasdynamic spherical shock waves in rotating atmosphere

Details Self-similar strong magnetogasdynamic spherical shock waves in rotating atmosphere Self-similar strong magnetogasdynamic spherical shock waves in rotating atmosphere

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jmps...17..641v&link_type=abstract

Journal of Mathematical and Physical Sciences (ISSN 0047-2557), vol. 17, Dec. 1983, p. 641-646.

Physics

Magnetohydrodynamics, Rotating Plasmas, Runge-Kutta Method, Shock Wave Propagation, Spherical Waves, Stellar Atmospheres, Azimuth, Equations Of Motion, Radial Velocity, Supernovae

Scientific paper

The propagation of strong spherical shock waves in a rotating atmosphere
with nonuniform density in a nonuniform conducting medium has been
studied. The energy gain of the flow enveloped by the shock is assumed
to be time dependent. The distribution of flow variables behind the
shock has been obtained.

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