We perform numerical simulations of rods and spheroids undergoing Jeff
ery orbits in a variety of shear flows. The numerical simulations are
based on the boundary element method, which allows for the accurate mo
deling of the problem geometry. We compare the period of rotation for
spheroids and rods, both far from walls and very close to walls. We fi
nd that the wall effects in three dimensions are minimal, even for flo
w in gaps not much larger than the longest dimension of the particle.
We also show that two-dimensional simulations grossly overpredict the
wall effects seen in three dimensions. Results are similar for both li
near and nonlinear shear flows. We also briefly look at the orbital mo
tion of a particle in close proximity to another particle, and show th
at, again, there is very little effect on the period of rotation, alth
ough the resulting centroid trajectories are very different from that
of an isolated particle.