  An updated analysis of all available neutrino oscillation evidence in Reactor
(Kamland, first 145 days of data) and Solar experiments (SK day and night
spectra, global rates from
  Homestake, SAGE and GALLEX) including the $SNO CC$ and $NC$ data is
presented. In the framework of two active neutrino oscillations we determine
the allowed regions in neutrino parameter space, we obtain, from the Kamland
spectral shape and global signal, the following antineutrino best solution
parameters, $ \Delta m^2_{kl}= 7.7\times 10^{-5} \eV^2, \tan^2\theta_{kl}=
0.98.$ The overall effect of the measured observed ratio $R\sim 0.6$ is that
the LMA region remains the only one which is still favored.
  Combining Kamland and Solar data and assuming CPT invariance, i.e. the same
mass matrix for neutrino and antineutrinos, we obtain the following
antineutrino best solution parameters (LMAI solution), $ \Delta m^2= 7.1\times
10^{-5} \eV^2,\tan^2\theta= 0.47.$ A second solution (LMAII) appears for values
$ \Delta m^2= 1.5\times 10^{-4} \eV^2, \tan^2\theta= 0.48.$ We determine
additionally individual neutrino mixing parameters and their errors from fits
to marginal likelihood distributions, the values are compatible with previous
results. In both methods, $\chi^2$ minimization and marginal likelihood, the
combined analysis of solar and Kamland data concludes that maximal mixing is
not favored at the $\sim 3\sigma $ level at least.
