  We consider the implications of the recent results of SAGE and GALLEX
experiments for the solution of the solar neutrino problem in the framework of
the resonant neutrino spin-flavor precession scenario. It is shown that this
scenario is consistent with all the existing solar neutrino data including the
gallium results. The quality of the fit of the data depends crucially on the
magnetic field profile used which makes it possible to get information about
the magnetic field in the solar interior. In particular, the magnetic field in
the core of the sun must not be too strong ($<3 \times 10^6$ G). The detection
rate in the gallium detectors turns out to be especially sensitive to the
magnitude of $\Delta m^2$. Predictions for forthcoming solar-neutrino
experiments are made.
