  Even after the confirmation of the large mixing angle (LMA) solution of the
solar neutrino problem, the scope for resonant spin- flavor precession (RSFP)
transitions as a subdominant effect still exists. In this work,we have
considered suitably suppressed RSFP transitions in addition to the dominant LMA
flavor transitions and translated the bounds on the antineutrino flux into the
bounds on the product of neutrino magnetic moment and solar magnetic field. The
low and intermediate energy neutrinos have been included in the analysis by
obtaining indirect bounds on the corresponding antineutrino fluxes for these
components. It is assumed that the missing beryllium neutrinos are being
converted into muon antineutrinos via RSFP transitions in the Sun.
