Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0-20.0 MeV. The measured solar neutrino flux is 2.32+/-0.03\(stat\)+0.08- 0.07\(syst\)×106 cm-2 s-1, which is 45.1+/-0.5\(stat\)+1.6-1.4\(syst\)% of that predicted by the BP2000 SSM. The day vs night flux asymmetry \(Φn-Φd\)/Φaverage is 0.033+/-0.022\(stat\)+0.013-0.012\(syst\). The recoil electron energy spectrum is consistent with no spectral distortion. For the hep neutrino flux, we set a 90% C.L. upper limit of 40×103 cm-2 s-1, which is 4.3 times the BP2000 SSM prediction.