We have performed analysis of the solar neutrino data including results from the SNO salt phase as well as the combined analysis of the solar and the KamLAND results .
The best fit values of neutrino parameters are \Delta m ^ { 2 } = 7.1 \cdot 10 ^ { -5 } eV ^ { 2 } , \tan ^ { 2 } \theta = 0.40 with the boron flux f _ { B } = 1.04 .
New SNO results strongly disfavor maximal mixing and the h-LMA region ( \Delta m ^ { 2 } > 10 ^ { -4 } 
eV ^ { 2 } ) which is accepted now at the 3 \sigma level .
We find the 3 \sigma upper bounds : \Delta m ^ { 2 } < 1.7 \cdot 10 ^ { -4 } eV ^ { 2 } and \tan ^ { 2 } \theta < 0.64 , and the lower bound \Delta m ^ { 2 } > 4.8 \cdot 10 ^ { -5 } eV ^ { 2 } .
Non-zero 13-mixing does not change these results significantly .
The present data determine quantitatively the physical picture of the solar neutrino conversion .
At high energies relevant for SNO and Super-Kamiokande the deviation of the effective survival probability from the non-oscillatory value is about 10 - 14 % .
The oscillation effect contribution to this difference is about 10 % and the Earth regeneration about 3 - 4 % .
At low energies ( E < 1 MeV ) the matter corrections to vacuum oscillation effect are below 5 % .
The predictions for the forthcoming measurements are given which include the spectral distortion and CC/NC ratio at SNO , the Day-Night asymmetry , the KamLAND spectrum and rate .