A model of flare-produced magneto-radiative shock with increasing energy

Details A model of flare-produced magneto-radiative shock with increasing energy A model of flare-produced magneto-radiative shock with increasing energy

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78...95v&link_type=abstract

Astrophysics and Space Science, vol. 78, no. 1, Aug. 1981, p. 95-103.

Astronomy and Astrophysics

Astrophysics

1

Energy Transfer, Magnetohydrodynamic Waves, Shock Wave Propagation, Solar Flares, Solar Wind, Stellar Models, Propagation Velocity, Radiant Flux Density, Radiative Transfer, Solar Activity Effects

Scientific paper

An exact solution for a spherically symmetric model of a magneto-radiative shock wave in the solar wind caused by the explosive energy release of a solar flare is obtained in the case when energy released is an increasing function of the time. It is shown that as a result of an increase in energy, the density, pressure, radiation flux, magnetic field, and shock velocity can change considerably.

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