Statistics – Computation
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..94..127s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 94, no. 1, July 1983, p. 127-132.
Statistics
Computation
Flow Theory, One Dimensional Flow, Radiative Heat Transfer, Shock Wave Luminescence, Computational Fluid Dynamics, Exponential Functions, Heat Flux, Ideal Gas, Similarity Numbers, Unsteady Flow
Scientific paper
The self-similar flow of a perfect gas behind an exponential shock driven out by an expanding surface, that is, the surface of contact discontinuity that moves with time according to an exponential law, is considered. The shock waves propagate in a uniform atmosphere that is assumed to be at rest. The similarity solutions are developed for a situation where the radiation heat flux is more important than the radiation pressure and radiation energy. It is assumed that the gas is gray and opaque and that the shock is transparent and isothermal. The total energy of the wave is found to vary as the cube of the shock radius. Viscosity and the solar gravity are neglected.
Vishwakarma P. R.
~Singh ~B. J.
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