Self-similar cylindrical shock waves with radiation heat flux

Details Self-similar cylindrical shock waves with radiation heat flux Self-similar cylindrical shock waves with radiation heat flux

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.102..263s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 102, no. 2, July 1984, p. 263-268.

Astronomy and Astrophysics

Astrophysics

5

Cylindrical Waves, Gas Explosions, Radiative Heat Transfer, Shock Wave Propagation, Earth Atmosphere, Runge-Kutta Method, Stellar Atmospheres

Scientific paper

Similarity solutions describing the flow of a perfect gas behind cylindrical shock waves with radiation heat flux are investigated. The total energy of the expanding waves has been supposed to remain constant. The solution, however, is only applicable to a gaseous medium where the undisturbed pressure falls as the inverse square of the distance from the line of explosion.

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