An equation of shear Alfven eigenmodes (AE) in optimized stellarators of We
ndelstein line (Helias configurations) is derived. The metric tensor coeffi
cients, which are contained in this equation, are calculated analytically.
Two numerical codes are developed: the first one, COBRA (COntinuum BRanches
of Alfven waves), is intended for the investigation of the structure of Al
fven continuum; the second, BOA (Branches Of Alfven modes), solves the eige
nvalue problem. The family of possible gaps in Alfven continuum of a Helias
configuration is obtained. It is predicted that there exist gaps which ari
se due to or are strongly affected by the variation of the shape of the pla
sma cross section along the large azimuth of the torus. In such gaps, discr
ete eigenmodes, namely, helicity-induced eigenmodes (HAE(21)) and mirror-in
duced eigenmodes (MAE) are found. It is shown that plasma inhomogeneity may
suppress the AEs with a wide region of localization. (C) 2001 American Ins
titute of Physics.