  This article summarises the status of the solar neutrino oscillation
phenomenology at the end of 2002 in the light of the SNO and KamLAND results.
We first present the allowed areas obtained from global solar analysis and
demonstrate the preference of the solar data towards the Large-Mixing-Angle
(LMA) MSW solution. A clear confirmation in favor of the LMA solution comes
from the \kl reactor neutrino data. The \kl spectral data in conjunction with
the global solar data further narrows down the allowed LMA region and splits it
into two allowed zones -- a low $\Delta m^2$ region (low-LMA) and high $\Delta
m^2$ region (high-LMA). We demonstrate through a projected analysis that with
an exposure of 3 kton-year (kTy) \kl can remove this ambiguity.
