Radiative decay behind strong M.H.D. shocks

Details Radiative decay behind strong M.H.D. shocks Radiative decay behind strong M.H.D. shocks

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.159..165s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 159, no. 1, Sept. 1989, p. 165-168.

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamic Waves, Plasma Decay, Radiation Effects, Shock Fronts, Bremsstrahlung, Magnetic Fields, Plasma Density, Radiant Cooling

Scientific paper

The effect of radiation up on the state of gas behind strong MHD shock front has been studied. The jump conditions for flow variables across the shock boundary have been obtained and temperature decay behind the shock front is determined for an optically-thin brehmsstrahlung radiation plasma. It has been found that, for a shock within strong magnetic field, the temperature decay is much quicker.

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