Abstract
Results from the entire 1496 live days of solar neutrino data from Super-Kamiokande-I's 1996–2001 run are presented. These results include our measurements of the Sun's absolute Boron-8 neutrino flux and energy spectrum, as well as studies of their variation with respect to the solar zenith angle (day/night asymmetry) and Earth's distance to the Sun. The possibility of neutrino oscillations is discussed in light of these results and those of other experiments, and the MSW Large Mixing Angle solution is found to be strongly favored.
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