Magnetogasdynamic cylindrical shock wave model in an optically thin atmosphere

Details Magnetogasdynamic cylindrical shock wave model in an optically thin atmosphere Magnetogasdynamic cylindrical shock wave model in an optically thin atmosphere

Jul 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.135..175o&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 135, no. 1, July 1987, p. 175-185.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics, Optical Thickness, Shock Wave Propagation, Stellar Atmospheres, Stellar Interiors, Stellar Models, Electrical Resistivity, Ideal Gas, Radiative Transfer, Thermal Radiation

Scientific paper

Similarity solutions for one-dimensional unsteady isothermal flow of a perfect gas behind a magnetogasdynamic shock wave including the effects of thermal radiation has been investigated in a uniform thin atmosphere. The flow is caused by an expanding piston and the total energy of the flow is assumed to be constant. Radiation pressure and energy have been neglected in comparison to radiation heat flux and the gas is assumed to be grey and opaque.

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