  We discuss the nature of the radial and azimuthal components of centrifugal
force associated with fluid flows in the equatorial plane of black hole space
times. The equations of motion are solved for the radial and azimuthal
components of the 3-velocity V^i which are then used in evaluating the nature
of the various components of inertial accelerations. It is shown that the
reversal of centrifugal force is governed mainly by the dominance of the
azimuthal velocity and the reversal occurs for r, mostly at 2m <~ r <~ 3m,
depending upon the boundary condition.
