Other
Scientific paper
Sep 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.104..189s&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 104, no. 2, Sept. 1984, p. 189-197.
Other
Adiabatic Flow, Anisotropic Media, Isothermal Flow, Magnetohydrodynamic Waves, Shock Wave Propagation, Spherical Waves, Approximation, Boundary Value Problems, Density Distribution, Equations Of Motion, Magnetic Field Configurations, Propagation Velocity
Scientific paper
The propagation of magnetohydrodynamic spherical shock waves in a decreasing density medium is considered. A series of equations is derived which describe both adiabatic and isothermal flows, using an approximate method similar to Whitham's (1958). The effect of initial magnetic fields on shock velocity is discussed, and a comparison is made between the adiabatic and isothermal cases. The comparison shows that the zero-temperature gradient condition behind the shock has a damping effect on the velocity of the shock waves.
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