Equatorial propagation of axisymmetric magnetogasdynamic shocks with thermal radiation

Details Equatorial propagation of axisymmetric magnetogasdynamic shocks with thermal radiation Equatorial propagation of axisymmetric magnetogasdynamic shocks with thermal radiation

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..96..153s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 96, no. 1, Oct. 1983, p. 153-158.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Stability, Magnetohydrodynamic Waves, Radiant Cooling, Shock Wave Propagation, Stellar Flares, Piston Theory, Similarity Theorem, Solar Wind, Spherical Waves, Thermal Radiation

Scientific paper

Similarity solutions, for one-dimensional unsteady motion of a perfect gas behind a spherical shock wave produced on account of a sudden explosion or driven out by an expanding piston including the effects of radiative cooling and an idealised azimuthal magnetic field, are studied. The shock is assumed to be strong and it is propagating into a transparent medium at rest with varying density. The magnetic field is proportional to r-1. The total energy of the wave is time dependent obeying a power law.

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