Effects of overtaking disturbances behind the flow in CCW1-3 approach have been included to describe the motion of cylindrical hydromagnetic shock wave in a self-gravitating rotating gas. The magnetic filed is assumed to have only constant axial (HZo = constant) and variable azimuthal (Hqo = r1/2 Hz) components, taking an initial density distribution as r0 = r'e-lr, where r' is the density on the axis of symmetry and l is a non-dimensionalising constant. Cases of reverse trends of variation of flow variables with inclusion of e.o.d have been highlighted.
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S. Kumar; S. Singh; M. Ranau00a0, "Corrections to ccw predictions for the motion of cylindrical hydromagnetic shock waves in a self-gravitating rotating gas ", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 2, Page Number 201-222, 2018Copy the following to cite this URL:
S. Kumar; S. Singh; M. Ranau00a0, "Corrections to ccw predictions for the motion of cylindrical hydromagnetic shock waves in a self-gravitating rotating gas ", Journal of Ultra Scientist of Physical Sciences, Volume 20, Issue 2, Page Number 201-222, 2018Available from: http://ultraphysicalsciences.org/paper/1290/