Electronic Resource
Springer
Astrophysics and space science
82 (1982), S. 307-309
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract 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.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00651441
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