Self-similar solutions for the blast wave problem in magnetogasdynamics. II

Details Self-similar solutions for the blast wave problem in magnetogasdynamics. II Self-similar solutions for the blast wave problem in magnetogasdynamics. II

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.114..289s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 114, no. 2, Sept. 1985, p. 289-294.

Astronomy and Astrophysics

Astrophysics

Blast Loads, Cylindrical Waves, Equations Of Motion, Gas Explosions, Magnetohydrodynamic Waves, Shock Wave Propagation, Adiabatic Flow, Density Distribution, Magnetic Field Configurations, Radii, Runge-Kutta Method, Time Dependence

Scientific paper

The problem of explosion along a line in a gas cloud in the presence of transverse magnetic field has been considered. Similarity solutions of the adiabatic motion of a gas behind an infinitely strong cylindrical shock wave propagating into an infinitely conducting medium at rest is obtained. Shock radius varies exponentially with time and density is inversely proportional to fourth power of shock radius just ahead of the shock front.

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