A model of flare-produced magneto radiative shock with increasing energy

DOI10.1007/BF00654025zbMath0474.76062MaRDI QIDQ1159041

B. G. Verma, R. C. Srivastava

Publication date: 1981

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

zbMATH Keywords

similarity solutionincreasing energyflare-produced magneto radiative shockMcVittie solution

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05)

Related Items (1)

An isothermal shock wave in a perfectly-conducting and non-homogeneous stellar interior

Cites Work

• Unnamed Item
• On the propagation of shock waves in regions of non-uniform density
• On the propagation of shock waves through regions of non-uniform area or flow
• SIMILARITY FLOWS BEHIND STRONG SHOCK WAVES
• The formation of a blast wave by a very intense explosion I. Theoretical discussion
• Spherically symmetric solutions of the equations of gas dynamics

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