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An updated analysis of all available neutrino oscillation evidence in Reactor(Kamland, first 145 days of data) and Solar experiments (SK day and nightspectra, global rates from  Homestake, SAGE and GALLEX) including the $SNO CC$ and $NC$ data ispresented. In the framework of two active neutrino oscillations we determinethe allowed regions in neutrino parameter space, we obtain, from the Kamlandspectral shape and global signal, the following antineutrino best solutionparameters, $ \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 thatthe LMA region remains the only one which is still favored.  Combining Kamland and Solar data and assuming CPT invariance, i.e. the samemass matrix for neutrino and antineutrinos, we obtain the followingantineutrino best solution parameters (LMAI solution), $ \Delta m^2= 7.1\times10^{-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 determineadditionally individual neutrino mixing parameters and their errors from fitsto marginal likelihood distributions, the values are compatible with previousresults. In both methods, $\chi^2$ minimization and marginal likelihood, thecombined analysis of solar and Kamland data concludes that maximal mixing isnot favored at the $\sim 3\sigma $ level at least

Neutrino mass parameters from Kamland, SNO, and other solar evidence