Self-similar solutions for the blast wave problem in radiative gasdynamics. I

Details Self-similar solutions for the blast wave problem in radiative gasdynamics. I Self-similar solutions for the blast wave problem in radiative gasdynamics. I

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111...79s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 1, April 1985, p. 79-85.

Astronomy and Astrophysics

Astrophysics

Equations Of State, Explosions, Gas Dynamics, Radiative Heat Transfer, Shock Wave Propagation, Spherical Waves, Heat Flux, Runge-Kutta Method, Shock Fronts, Solar Flares, Unsteady Flow, Viscous Flow

Scientific paper

Similarity solutions, describing the flow of a perfect gas behind spherical shock waves, are investigated including the radiation heat flux. The shock is assumed to be propagating in a medium at rest. Shock radius varies exponentially with time and density is inversely proportional to fifth power of the shock radius immediately ahead of the shock front.

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