  The first results of the solar neutrino flux measurement from
Super-Kamiokande are presented. The results shown here are obtained from data
taken between the 31st of May, 1996, and the 23rd of June, 1997. Using our
measurement of recoil electrons with energies above 6.5 MeV, we infer the total
flux of 8B solar neutrinos to be
2.42+-0.06(stat.)+0.10-0.07(syst.)*10^6/cm^2/s. This result is consistent with
the Kamiokande measurement and is 36% of the flux predicted by the BP95 solar
model. The flux is also measured in 1.5 month subsets and shown to be
consistent with a constant rate.
