  The geodesics in various spherical Rindler frames are investigated. A display
of some kinematical quantities of the spacetime is given. The constant
acceleration from the metric acts as the surface gravity of the horizon $r =
0$. The radial geodesics are computed both for the Balasubramanian et al. form
of the spherical Rindler space and for the non-diagonal metric of Huang and
Sun.
