  We review the status of the neutrino oscillation physics (as of June 2003),
with a particular emphasis on the present knowledge of the neutrino mass-mixing
parameters in a three generation approach. We consider first the nu_mu-->nu_tau
flavor transitions of atmospheric neutrinos. It is found that standard
oscillations provide the best description of the SK+K2K data, and that the
associated mass-mixing parameters are determined at 1 sigma (and dof=1) as:
Delta m^2=(2.6 +-0.4) x 10^-3 eV^2 and sin^2(2theta)=1.00+0.00-0.05. Such
indications, presently dominated by SK, could be strengthened by further K2K
data. Then we analyze the energy spectrum of reactor neutrino events recently
observed at KamLAND and combine them with solar and terrestrial neutrino data.
We find that the solution to the solar neutrino problem at large mixing angle
(LMA) is basically split into two sub-regions, that we denote as LMA-I and
LMA-II. The LMA-I solution, characterized by lower values of the squared
neutrino mass gap, is favored by the global data fit. Finally, we briefly
illustrate how prospective data from the SNO and KamLAND can increase our
confidence in the occurrence of standard matter effects in the Sun, which are
starting to emerge from current data.
