Self-similar flows behind a spherical radiation-driven shock wave. II

DOI10.1007/BF00653465zbMath0511.76121OpenAlexW1994308975MaRDI QIDQ1839175

J. B. Singh, R. N. Lal Srivastava

Publication date: 1982

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

Full work available at URL: https://doi.org/10.1007/bf00653465

zbMATH Keywords

propelling contact surfaceadiabatic and isothermal flowsnon-uniform atmosphereazimuthal magnetic fieldstrongerupting solar plasmaisentropic behind shockoptically thin ahead and thick behind the shock frontquiet solar wind regionradiation-driven spherical shockself-similar blast wave modelsolar flare activitytime- dependent total energy contentvarying density distribution

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Planetary atmospheres (85A20) Ionized gas flow in electromagnetic fields; plasmic flow (76X05) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (3)

Magnetohydrodynamic effects on radiation-driven shock waves ⋮ An approximate analytical solution for self-isothermal flow behind a radiation driven shock wave. II ⋮ Spherical radiation-driven shock waves in a non-uniform atmosphere

Cites Work

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

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