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This article describes the seven experiments Homestake, Kamiokande, SAGE, GALLEX, Super-Kamiokande, GNO and SNO which have so far provided data on the measurement of the solar neutrino fluxes. The detection mechanism, the salient features of the detectors and the results of each experiment are presented. How the solar neutrino problem has evolved and became more focused with each experimental data is summarized. The goals for the future experiments are outlined.

生成讲解博客的中文版本

生成AI智能校验的中文版本