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

DOI10.1007/BF00648925zbMath0501.76050OpenAlexW2050281206MaRDI QIDQ1172495

S. Singh

Publication date: 1982

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00648925

zbMATH Keywords

similarity methodPlanck's diffusion approximationDEC-1090 computerdistributions of pressure, density, magnetic field, velocity, temperature, and radiation fluxnon- uniform densityoptically-thin grey atmosphereplane magnetogasdynamic shock wavesRKGS programme

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Magnetohydrodynamics and electrohydrodynamics (76W05) Planetary atmospheres (85A20) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Software, source code, etc. for problems pertaining to fluid mechanics (76-04) Radiative transfer in astronomy and astrophysics (85A25)

Cites Work

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• On the propagation of shock waves through regions of non-uniform area or flow
• Nonsimilar blast waves with transparent gas radiation
• The ‘piston problem’ with thermal radiation
• Effect of Radiation upon the Post-Shock State
• Self-similar piston problems with radiative heat transfer

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