Key points are not available for this paper at this time.
The Homestake Solar Neutrino Detector, based on the inverse beta-decay reaction l e ] 37Cl ] 37Ar ] e~, has been measuring the ux of solar neutrinos since 1970. The experiment has operated in a stable manner throughout this time period. All aspects of this detector are reviewed, with particular emphasis on the determination of the extraction and counting efficiencies, the key experimental parameters that are necessary to convert the measured 37Ar count rate to the solar neutrino production rate. A thorough consideration is also given to the systematics of the detector, including the measurement of the extraction and counting efficiencies and the nonsolar production of 37Ar. The combined result of 108 extractions is a solar neutrinoinduced 37Ar production rate of 2. 56 ⁰. l6 (statistical) ⁰. 16 (systematic) SNU.
Cleveland et al. (1998) studied this question.