  We analyse a sample of 244 ram-pressure-stripped candidate galaxy members
within the virial radius of 62 nearby clusters, to determine their velocity
anisotropy profile $\beta(r)$. We use previously determined mass profiles for
the 62 clusters to build an ensemble cluster by stacking the 62 cluster samples
in projected phase-space. We solve the Jeans equation for dynamical equilibrium
by two methods, MAMPOSSt and the Jeans inversion technique, and determine
$\beta(r)$ both in parametric form and non-parametrically. The two methods
consistently indicate that the orbits of the ram-pressure-stripped candidates
are increasingly radial with distance from the cluster center, from almost
isotropic ($\beta \simeq 0$) at the center, to very radial at the virial radius
($\beta \simeq 0.7$). The orbits of cluster galaxies undergoing ram-pressure
stripping are similar to those of spiral cluster galaxies, but more radially
elongated at large radii.
