A NATURAL EXPLANATION OF ALL SOLAR-NEUTRINO DATA BY THE RESONANT SPIN-FLAVOR PRECESSION SCENARIO

It is emphasized that the E(nu) (neutrino energy) spectrum of the nu(e ) survival probability in the Resonant Spin-Flavor Precession (RSFP) s cenario has very desirable shape to reconcile all existing solar neutr ino data. As the result, the RSFP scenario is shown to have rather bro ad allowed region to reconcile the data in the (B, Delta m(2)) plane, with B being the magnetic field strength inside the Sun. The sensitivi ty of the allowed region on the different choices of the B profile, an d the time variations of the solar neutrino event rates in the RSFP sc enario are also discussed in some detail.