Strong spherical magnetogasdynamic shock waves in rotating stellar atmosphere

Details Strong spherical magnetogasdynamic shock waves in rotating stellar atmosphere Strong spherical magnetogasdynamic shock waves in rotating stellar atmosphere

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..82..307v&link_type=abstract

Astrophysics and Space Science, vol. 82, no. 2, Mar. 1982, p. 307-309.

Astronomy and Astrophysics

Astrophysics

3

Interplanetary Medium, Magnetohydrodynamic Waves, Rotating Fluids, Shock Wave Propagation, Spherical Waves, Stellar Atmospheres, Coriolis Effect, Equations Of Motion, Stellar Magnetic Fields

Scientific paper

An analytic expression for the velocity of magnetogasdynamic shock wave, propagating in rotating inter stellar atmosphere has been obtained by using the method of characteristics and considering the effect of coriolis force. It has been shown that in the outer convective layer of the star Coriolis force and magnetic field both have significant effect on the shock velocity

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