  We present a solution of the solar neutrino deficit using three flavors of
neutrinos within the R-parity non-conserving supersymmetric model. In vacuum,
mass and mixing is restricted to the nu(mu)-nu(tau) sector only, which we
choose in consistency with the requirements of the atmospheric neutrino
anomaly. The nu(e) is massless and unmixed. The flavor changing and flavor
diagonal neutral currents present in the model and an energy-dependent
resonance-induced nu(e)-nu(mu) mixing in the sun result in the new solution to
the solar neutrino problem. The best fit to the solar neutrino rates and
spectrum (1258-day SK data) requires a mass square difference of 10^{-5} eV^2
in vacuum between the two lightest neutrinos. This solution cannot accommodate
a significant day-night effect for solar neutrinos.
