Abstract
The current experimental data on the solar-neutrino problem are reviewed. The possibilities offered by the radiochemical lithium detector for solving this problem, in particular, for determining the contribution of medium-energy and boronneutrinos in chlorine and gallium detectors, are discussed. A brief description is given of the prototype of the lithium detector containing a target of 300 kg of metallic lithium, which is presently under construction at the Nuclear Research Institute of the Russian Academy of Sciences.
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