Similarity solutions are obtained for one-dimensional adiabatic flow behind a magnetogasdynamic cylindrical shock wave propagating in a rotating a medium in presence of a variable or constant azimuthal magnetic field. The density of the medium ahead of the shock is assumed to be varying and obeying a power law. In order to obtain the similarity solutions the angular velocity of the ambient medium is assumed to be decreasing as the distance from the axis increases. Effects of an increase of the Alfven-Mach number and the variation of the initial den sity, initial magnetic field and initial angular velocity of the medium, on the flow-field behind the shock, are obtained.
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