It is shown that the collisionless transformation of locally trapped and pa
ssing particle orbits in the optimized stellarators of the Wendelstein line
results in stochastic diffusion of energetic ions. This diffusion can lead
to the loss of a significant fraction of the energetic ion population from
the region where the characteristic diffusion time is small compared to th
e slowing down time. The loss region and losses can be minimized by shaping
the plasma temperature and density profiles so that they satisfy certain r
equirements. The predictions of the theory developed here are in agreement
with the results of numerical modeling of alpha -particle confinement in a
Helias reactor, which has been carried out with the use of an orbit followi
ng code. (C) 2001 American Institute of Physics.