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

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

Publishing date

Jul 1982

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..437s&link_type=abstract

Journals

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 437-441.

Science

Physics

Additional info 2

5

Additional info 3

Atmospheric Physics, Gas Flow, Shock Wave Interaction, Shock Wave Propagation, Pressure Distribution, Radiation Absorption

Type

Scientific paper

Abstract

The self-similar flows behind a radiation-driven shock wave are
investigated for the case of a nonuniform atmosphere, where the total
energy content of the flow behind the shock increases due to the
absorption of radiation and is assumed to be time-dependent. The values
used in the calculation are those of Ranga Rao and Ramana (1973).

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