  The results of the entire Super-Kamiokande-I solar neutrino data are
presented. The measured interaction rate is 47+-2% of the rate expected by the
standard solar model and 133+-5% of the rate implied by the SNO charged-current
interaction rate. There is no evidence for spectral distortion or a time
dependent neutrino flux. Together with the rates of other experiments, the
Super-Kamiokande results imply active solar neutrino oscillations and restrict
neutrino mixing and mass square difference to lie within the LMA solution area.
