  It 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.
