Magneto-radiative shock wave propagation in a conducting plasma

Details Magneto-radiative shock wave propagation in a conducting plasma Magneto-radiative shock wave propagation in a conducting plasma

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss..90..169s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 90, no. 2, April 1992, p. 169-176.

Astronomy and Astrophysics

Astrophysics

Plasma Conductivity, Plasma-Electromagnetic Interaction, Shock Wave Propagation, Earth Atmosphere, Heat Flux, Magnetic Fields, Numerical Integration, Runge-Kutta Method

Scientific paper

The problem of propagation of magnetoradiative shock wave in a conducting plasma is considered with particular attention given to the problem of explosion along a line in a gas cloud. Similarity solutions are developed describing the propagation of a cylindrical and a spherical shock in a nonuniform atmosphere with magnetic effect, taking into account counter gas pressure and radiation heat flux (but ignoring the radiation pressure and radiation energy) and assuming the total energy of the explosion to be constant. It is noted that the solutions are applicable only to a gaseous medium where the undisturbed pressure falls as the inverse square of the distance from the line of explosion.

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