All existing measurements of the solar neutrino flux are compared with
the predictions of the most recent solar model by Bahcall and Pinsonn
eault, modified by introducing the hypothesis of neutrino oscillations
with mass differences large enough to render energy-independent any q
uantity observable on earth. It is concluded that the data are consist
ent with this hypothesis and that, at least for the time being, any en
ergy-dependence of the solar neutrino deficit should not be regarded a
s a compelling reality.