Spherical shock waves in viscous magnetogasdynamics

Details Spherical shock waves in viscous magnetogasdynamics Spherical shock waves in viscous magnetogasdynamics

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..253v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 2, April 1985, p. 253-263. Sponsorship: Council of Scientific and

Astronomy and Astrophysics

Astrophysics

2

Magnetohydrodynamics, Shock Wave Propagation, Spherical Waves, Viscosity, Astrophysics, Inviscid Flow, Magnetic Fields, Point Sources, Shock Discontinuity, Viscous Flow

Scientific paper

The point-source, spherical magnetogasdynamics shock wave moving into a constant density γ-law gas is considered in the limit of infinite shock strength, from the point of view of the Richtmyer-Von Neumann viscosity technique. Numerical solutions of this problem has been obtained in viscous and non-viscous regions. A similarity solution of this problem is shown to exist. The authors have shown that field variables change rapidly when the magnetic field is imposed in both the viscous and non-viscous regions.

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