2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/147320It is pointed out that the enhancement of the solar neutrino rate in a real time detector like Super-Kamioka, SNO or Borexino due to neutrino oscillations in the moon during a partial or total solar eclipse may be observable. The enhancement is calculated as a function of the neutrino parameters in the case of three flavor mixing. This enhancement if seen, can further help to determine the neutrino parameters.16 Pages Revtex, 5 figures as one ps file. Typos correctedAstrophysicsHigh Energy Physics - Phenomenologytext