A self-similar flow behind an exponential shock with radiative heat flux. II

DOI10.1007/BF00651764zbMath0533.76063OpenAlexW2049708077MaRDI QIDQ789967

J. B. Singh, P. R. Vishwakarma

Publication date: 1983

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

Full work available at URL: https://doi.org/10.1007/bf00651764

zbMATH Keywords

self-similar solutionsmagnetogasdynamicstime-dependentenergy content of flow between shock front and contact surfacehomothermalincreasing energynonuniform atmosphere at restone-dimensional unsteady flow of a perfect gas behind an exponential shockpropelling contact surfaceradiation fluxRoche's model caseself- gravitatingspherical wave

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

• Propagation of spherical shock waves in an exponential medium with radiation heat flux
• Propagation of magnetogasdynamic spherical shock waves in an exponential medium

This page was built for publication: A self-similar flow behind an exponential shock with radiative heat flux. II