The propagation of strong-plane magnetogasdynamic shock waves in an optically-thin atmosphere

Details The propagation of strong-plane magnetogasdynamic shock waves in an optically-thin atmosphere The propagation of strong-plane magnetogasdynamic shock waves in an optically-thin atmosphere

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..87..297v&link_type=abstract

Astrophysics and Space Science, vol. 87, no. 1-2, Oct. 1982, p. 297-304.

Astronomy and Astrophysics

Astrophysics

Atmospheric Density, Magnetohydrodynamic Waves, Optical Thickness, Plane Waves, Shock Wave Propagation, Equations Of Motion, Pressure Distribution, Radiation Distribution, Temperature Distribution, Velocity Distribution

Scientific paper

The propagation of plane magnetogasdynamic shock waves in an optically-thin grey atmosphere of non-uniform density has been discussed by the use of the similarity method, by use of Planck's diffusion approximation. The distributions of pressure, density, magnetic field, velocity, temperature, and radiation flux have been illustrated through graphs. The numerical integration has been done on a DEC-1090 computer under a RKGS programme

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