In this article we analyze the geodesics of test particles and light in the
five dimensional (charged) doubly spinning black ring spacetime. Apparently it
is not possible to separate the Hamilton-Jacobi-equation for (charged) doubly
spinning black rings in general, so we concentrate on special cases: null
geodesics in the ergosphere and geodesics on the two rotational axes of the
(charged) doubly spinning black ring. We present analytical solutions to the
geodesic equations for these special cases. Using effective potential
techniques we study the motion of test particles and light and discuss the
corresponding orbits.Comment: arXiv admin note: substantial text overlap with arXiv:1208.254