We calculate the self-force acting on a scalar particle which is falling ra
dially into a Schwarzschild black hole. We treat the particle's self-held a
s a linear perturbation over the fixed Schwarzschild background. The force
is calculated by numerically solving the appropriate wave equation for each
mode of the field in the time domain, calculating its contribution to the
self-force, and summing over all modes using Ori's mode-sum regularization
prescription. The radial component of the force is attractive at large dist
ances, and becomes repulsive as the particle approaches the event horizon.