We have updated the results on atmospheric and solar neutrinos from Super-K
amiokande. The zenith-angle distributions of atmospheric neutrinos are pres
ented. We have done a new analysis to distinguish nu(mu) <-> nu(tau) and nu
(mu) <-> nu(s) oscillations. The preliminary result disfavored nu(mu) <-> n
u(s) oscillations at about 2 sigma level. We also present the updated resul
ts on the energy spectrum and day-night variation of solar neutrinos. (C) 2
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