The results of all currently operating solar neutrino experiments are
analyzed in the framework of the resonant neutrino spin-flavor precess
ion scenario including the effects of neutrino mixing. Nine different
profiles of the solar magnetic field are used in the calculations. It
is shown that the available experimental data can be accounted for wit
hin the considered scenario. The Ga-Ge data lead to an upper limit on
the neutrino mixing angle: sin 2 theta(0) less than or similar to 0.25
. One can discriminate between small mixing angle (sin 2 theta(0) less
than or similar to 0.1) and moderate mixing angle solutions by studyi
ng the solar <(nu)over bar>(e) flux which is predicted to be sizeable
for moderate mixing angles. The expected signals due to <(nu)over bar>
(e) in the SNO, Super-Kamiokande and Borexino experiments are calculat
ed and found to be detectable for sin 2 theta(0) less than or similar
to 0.1.