In this brief review we discuss the possibility of studying the solar interior by means of neutrinos , in the light of the enormous progress of neutrino physics in the last few years .
The temperature near the solar center can be extracted from Boron neutrino experiments as : T = ( 1.57 \pm 0.01 ) 10 ^ { 7 } K .
The energy production rate in the Sun from pp chain and CNO cycle , as deduced from neutrino measurements , agrees with the observed solar luminosity to about twenty per cent .
Progress in extracting astrophysical information from solar neutrinos requires improvement in the measurements of ^ { 3 } He + ^ { 4 } He \rightarrow ^ { 7 } Be + \gamma 
and p + ^ { 14 } N \rightarrow ^ { 15 } O + \gamma .