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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 plane of the mass difference squared versus vacuum mixing angle, are given for the current ³⁷Cl experiment and the proposed ⁷¹Ga detector.
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Parke et al. (1986) studied this question.
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