Propagation of Magneto-Radiative Shock Waves - Part Two

Details Propagation of Magneto-Radiative Shock Waves - Part Two Propagation of Magneto-Radiative Shock Waves - Part Two

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.146...79s&link_type=abstract

Astrophysics and Space Science, Volume 146, Issue 1, pp.79-88

Astronomy and Astrophysics

Astrophysics

Scientific paper

Self-similar motion of a perfect gas behind a cylindrical shock wave with radiation heat flux in the presence of an azimuthal magnetic field have been discussed. The shock is assumed to be propagating in a medium at rest with non-uniform density. The conductivity of the gas is infinite and magnetic permeability is one everywhere. Also, the shock is assumed to be transparent and isothermal.

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