A self-similar flow of self-gravitating gas behind a spherical shock wave in magnetogasdynamics

Details A self-similar flow of self-gravitating gas behind a spherical shock wave in magnetogasdynamics A self-similar flow of self-gravitating gas behind a spherical shock wave in magnetogasdynamics

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.124...53v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 124, no. 1, July 1986, p. 53-62. Sponsorship: Council of Scientific and In

Physics

Gravitational Collapse, Magnetohydrodynamics, Shock Waves, Spherical Waves, Stellar Physics, Similarity Theorem, Stellar Magnetic Fields, Stellar Motions, Wave Propagation

Scientific paper

This paper considers a spherical shock, in a conducting gas, of self-gravitating gas propagating in a non-uniform atmosphere at rest. Similarity principle has been used to reduce the equations governing the flow to ordinary differential equations under the assumption that the density varies as an inverse-power of distance from the point of explosion. The total energy of the wave is variable.

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