Self-similar flows behind shock wave with increasing energy in magnetogasdynamics. I

Details Self-similar flows behind shock wave with increasing energy in magnetogasdynamics. I Self-similar flows behind shock wave with increasing energy in magnetogasdynamics. I

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..85..427s&link_type=abstract

Astrophysics and Space Science, vol. 85, no. 1-2, July 1982, p. 427-435.

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4

Magnetohydrodynamic Flow, Shock Waves, Solar Wind, Adiabatic Flow, Isothermal Flow, Similarity Theorem

Scientific paper

A self-similar blast wave model is investigated which consists of a strong spherical shock wave that is driven outward by a propelling contact surface, moving into a quiet solar wind region with varying density distribution in the presence of an azimuthal magnetic field for adiabatic and isothermal flows. The total energy of the flow increases with time, and the solutions correspond to a blast wave produced by intense and prolonged solar flare activity when the wave has been driven by freshly erupting solar plasma. The total energy of the flow between the shock and the contact surface is taken to be time-dependent and obedient to a power law.

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