Abstract
It is shown that from the data of future solar neutrino experiments (SNO and Super-Kamiokande), in which high-energy neutrinos will be detected, it will be possible in a model independent way: 1) To reveal the presence of sterile neutrinos in the flux of solar neutrinos on the earth; 2) To obtain the initial flux of 's; 3) To determine the probability of 's to survive as a function of neutrino energy.
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