An exact similarity solution in radiation magneto-gas-dynamics for the flows behind a spherical shock wave

Details An exact similarity solution in radiation magneto-gas-dynamics for the flows behind a spherical shock wave An exact similarity solution in radiation magneto-gas-dynamics for the flows behind a spherical shock wave

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.129...45v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 129, no. 1, Jan. 1987, p. 45-52.

Astronomy and Astrophysics

Astrophysics

2

Magnetohydrodynamic Flow, Radiant Flux Density, Radiation Pressure, Shock Wave Propagation, Similarity Theorem, Spherical Waves, Radiation Distribution, Radiative Heat Transfer, Time Dependence

Scientific paper

An exact similarity solution for a spherical magnetogasdynamic shock is obtained in the case when radiation energy, radiation pressure and radiative heat flux are important. The total energy of the shock wave increases with time. The authors have shown that due to the magnetic field the flow variables are considerably changed. Also, due to increases in radiation pressure number the radiation flux is increased.

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