Magnetogasdynamic cylindrical shock wave model in an optically thin atmosphere

DOI10.1007/BF00644472zbMath0623.76072OpenAlexW2038434696MaRDI QIDQ1091888

S. N. Ojha

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1007/bf00644472

zbMATH Keywords

similarity solutionsradiation pressureperfect gasthermal radiationmagnetogasdynamic shock waveone-dimensional unsteady isothermal flowuniform thin atmosphere

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Basic methods in fluid mechanics (76M99) Stability and instability of geophysical and astrophysical flows (76E20)

Cites Work

• Unnamed Item
• Self-similar flows with increasing energy. III: Radiation-driven shock wave
• Similarity solutions for propagation of strong plane shock waves in an optically thin atmosphere
• The ‘piston problem’ with thermal radiation
• Self-similar piston problems with radiative heat transfer
• Propagation of Spherical Shock Waves in Stellar Interiors

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