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.190..169s&link_type=abstract

Astrophysics and Space Science, Volume 190, Issue 2, pp.169-176

Astronomy and Astrophysics

Astrophysics

Scientific paper

Similarity solutions describing the flow of a perfect gas behind a spherical and cylindrical shock wave in a magnetic field with radiation heat flux have been investigated. The total energy of the expanding wave has been assumed to remain constant. The solutions, however, are only applicable 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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