Self-similar flows with increasing energy. III: Radiation-driven shock wave

DOI10.1016/0020-7225(73)90016-5zbMath0269.76047OpenAlexW2073864499MaRDI QIDQ758394

Melam P. Ranga Rao, Bandaru V. Ramana

Publication date: 1973

Published in: International Journal of Engineering Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0020-7225(73)90016-5

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05)

Related Items (8)

Magnetohydrodynamic effects on radiation-driven shock waves ⋮ Magnetogasdynamic cylindrical shock wave model in an optically thin atmosphere ⋮ Self-similar MHD shock waves for a rotating atmosphere under the force of gravitation ⋮ Cylindrical magnetohydrodynamic model of shock waves with radiation heat flux ⋮ Self-similar flows behind a spherical radiation-driven shock wave. II ⋮ An approximate analytical solution for self-isothermal flow behind a radiation driven shock wave. II ⋮ An approximate analytical solution for self-similar flow behind a radiation driven shock wave ⋮ Spherical radiation-driven shock waves in a non-uniform atmosphere

Cites Work

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• Über die instationäre homotherme Bewegung eines durch einen Kolben verdrängten Gases
• Self-similar flows with increasing energy

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