Title: Solar Neutrino Results from Super-Kamiokande


Neutrino oscillations have long been suggested to explain the discrepancy between predicted and measured solar neutrino flux. Depending on the oscillation parameters, this may lead to day-night or seasonal variations or an energy dependence of the suppresion of the solar neutrino flux. I will present the result of a search for these effects in Super-Kamiokande's 1117-day solar neutrino data sample.