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Effect of Artificial Viscosity on the Expansion of Dis-Continuities in a Rotating Interplanetary Medium with Material Pressure
2015
SAMRIDDHI A Journal of Physical Sciences Engineering and Technology
The solution of equations by seeking quasi-similar solution, in which the viscosity coefficient is taken to be at most a function of time but independent of space co-ordinates. an attempt is made to account for the material strength by including Newtonian- Viscosity term. In the present paper the characteristic method (Chester, Witham) is applied to obtain expressions of the density, the pressure, the particle velocity just behind the shock propagating in a rotating atmosphere. The effect of
doi:10.18090/samriddhi.v6i1.1552
fatcat:cwpo5epagbcszgk4cv2onqo6h4