
The results of a detailed calculation of the effects of resonant neutrino oscillations in the sun on the current and proposed solar neutrino experiments are presented. Analytic results are used for the electron-neutrino survival probability so that a sophisticated model for both the production distribution of the solar neutrino sources and the solar electron-number density can be employed. Contour plots for the electron-neutrino capture rate, in the mass-difference-squared versus vacuum-mixing-angle plane, are given for the current /sup 37/Cl experiment and the proposed /sup 71/Ga detector.
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