The structure of strong hydromagnetic shock waves in a thermally-radiating gas

Details The structure of strong hydromagnetic shock waves in a thermally-radiating gas The structure of strong hydromagnetic shock waves in a thermally-radiating gas

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.173...53b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 173, no. 1, Nov. 1990, p. 53-67.

Astronomy and Astrophysics

Astrophysics

2

Conducting Fluids, Gas Dynamics, Magnetohydrodynamic Waves, Shock Waves, Thermal Radiation, Hypersonic Flow, Ideal Gas, Mach Number, Mathematical Models, Viscosity

Scientific paper

The evolution of a strong magnetogasdynamic shock wave in a thermally radiating gas with a magnetic field perpendicular to the shock propagation direction is investigated analytically. The approach employed involves an asymptotic expansion (as M goes to infinity) under a differential approximation for radiation in an optically thick medium. The derivation of the solutions is given in detail, and their potential applicability to high-temperature hypersonic flow regimes is indicated.

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