  The data from all solar neutrino experiments presented at the Neutrino 98
conference has been analyzed and a brief summary of the status of the two most
popular neutrino solutions of the solar neutrino problem, the MSW mechanism and
vacuum oscillations, is presented here. The inclusion of the recoil-electron
data and of the zenith angle distribution of events in the SuperKamiokande
detector, together with the routine analysis of the rates, into a global
$\chi^2$ fit impose stringent constraints on these neutrino oscillation
scenarios.
