The structure of MHD shock waves in a thermally-radiating gas at high Mach numbers

Details The structure of MHD shock waves in a thermally-radiating gas at high Mach numbers The structure of MHD shock waves in a thermally-radiating gas at high Mach numbers

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179..171b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 2, May 1991, p. 171-176.

Mathematics

Asymptotic Methods, High Temperature Gases, Magnetohydrodynamic Waves, Optical Thickness, Shock Waves, Integral Equations, Transformations (Mathematics)

Scientific paper

Asymptotic expansion is used to study the structure of a strong MHD
shock wave which radiates thermally downstream of the shock. The exact
integral equation for radiation is adopted for the study, making
possible a comparison of the optically thick (and thin), the general
differential approximate, and the exact integral equation solutions.

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