Statistics – Computation
Scientific paper
May 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.155..163n&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 155, no. 1, May 1989, p. 163-167.
Statistics
Computation
2
Computational Astrophysics, Magnetohydrodynamic Waves, Shock Waves, Stellar Physics, Radiation Absorption, Stellar Atmospheres, Stellar Interiors, Stellar Magnetic Fields, Wave Propagation
Scientific paper
This paper considers a theoretical model of cylindrical MHD shock waves in a gas under the action of monochromatic radiation, with such model absorption coefficients for which the problem of interaction of radiation with gas is reducible to a self-similar problem. The gas is assumed to be gray and opaque, and the shock is assumed to be transparent. Special consideration is given to the effects of magnetic field. Results obtained on the variation of flow variables of the gas indicate that the flow velocity increases during the motion toward the line of explosion, whereas the density, pressure, and magnetic field first increase and then decrease.
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