Spherical MHD shock waves under the action of monochromatic radiation

Details Spherical MHD shock waves under the action of monochromatic radiation Spherical MHD shock waves under the action of monochromatic radiation

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.202..355n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 202, no. 2, p. 355-362.

Astronomy and Astrophysics

Astrophysics

Magnetic Fields, Magnetohydrodynamic Waves, Monochromatic Radiation, Shock Wave Propagation, Stellar Atmospheres, Absorptivity, Boundary Conditions, Differential Equations, Ideal Gas

Scientific paper

Self-similar MHD shock waves have been studied under the action of
monochromatic radiation into a non-uniform stellar atmosphere with a
constant intensity on unit area. It has been assumed that the radiation
flux moves through the gas. Variation of flow variables have been shown
in tables for two different cases.

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