Similarity solution of the propagation of spherical shock waves in a magnetogasdynamic self-gravitating system

Details Similarity solution of the propagation of spherical shock waves in a magnetogasdynamic self-gravitating system Similarity solution of the propagation of spherical shock waves in a magnetogasdynamic self-gravitating system

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146..175n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 146, no. 1, July 1988, p. 175-182.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Waves, Shock Wave Propagation, Similarity Theorem, Spherical Waves, Stellar Atmospheres, Interstellar Gas, Magnetic Field Configurations, Stellar Magnetic Fields, Wave Equations

Scientific paper

The self-similar model of propagation of spherical strong shock waves
into non-uniform stellar atmosphere under self-gravitation and
non-uniform magnetic field is investigated. The disturbances are headed
by a shock surface of variable strength. Gas is assumed to be grey and
opaque and the shock to be transparent.

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