  We perform a global analysis in the framework of two active neutrino
oscillations of all solar neutrino data, including the recent SNO day and night
spectra (comprised of the charged current (CC), elastic scattering (ES) and
neutral current (NC) events), the Super-Kamiokande (SK) day and night spectra
(from 1496 days) and the updated SAGE results. We find that the Large Mixing
Angle (LMA) solution is selected at the 99% C.L.; the best-fit parameters are
\Delta m^2=5.6 \times 10^{-5} eV^2 and \theta=32^{\circ}. No solutions with
\theta\geq \pi/4 are allowed at the 5\sigma C.L. Oscillations to a pure sterile
state are excluded at 5.3\sigma, but a sizeable sterile neutrino component
could still be present in the solar flux.
