  An updated analysis of all available neutrino oscillation evidence in Solar
experiments (SK day and night spectra, global rates from Homestake, SAGE and
GALLEX) including the latest SNO CC and NC data is presented. Assuming that the
shape of the SNO CC energy spectrum is undistorted and using the information
provided by SNO we obtain, for the fraction of electron neutrinos remaining in
the solar beam at energies $\gsim 5$ MeV:
$\phi_{CC}/\phi_{NC}=0.34^{+0.05}_{-0.04},$ which is nominally $\sim 30\sigma$
away from the standard value. The fraction of oscillating neutrinos which into
active ones is computed to be:
  $ (\Phi_{NC}-\Phi_{CC})/(\Phi_{SSM}-\Phi_{CC})=0.92^{+0.39}_{-0.20} $ nearly
$5\sigma$ deviations from the pure sterile oscillation case. The data is still
compatible with an important fraction of sterile component in the solar beam
(up to 20% of the total). In the framework of two active neutrino oscillations
we determine individual neutrino mixing parameters and their errors in the
region of no spectrum distortion ($\Delta< T_e> <1%$), we obtain $\Delta m^2=
4.5^{+2.7}_{-1.4}\times 10^{-5} \eV^2, \quad \tan^2\theta=0.40^{+0.10}_{-0.08}.
$ This is in agreement with the best $chi^2$ solution in the LMA region.
