The measurement of the flux of beryllium neutrinos with an accuracy of about 10% and CNO neutrinos with an accuracy of 20-30% will enable one to find the flux of pp neutrinos in the source with an accuracy better than 1% using the luminosity constraint. The future experiments on ve(-) scattering will enable one to measure with very good accuracy the flux of beryllium and pp neutrinos on the Earth. The ratio of the flux of pp neutrinos on the Earth and in the source will enable one to find with very good accuracy a mixing angle theta(circle dot). A lithium detector has high sensitivity to CNO neutrinos and can find the contribution of the CNO cycle to the energy generated in the Sun. This will be a stringent test of the theory of stellar evolution and combined with other experiments will provide a precise determination of the flux of pp neutrinos in the source and a mixing angle theta(circle dot). The work on the development of the technology of a lithium experiment is now in progress. (C) 2004 MAIK "Nauka/Interperiodica".
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机译：准确度约为10％的铍中微子通量和准确度为20-30％的CNO中微子通量的测量将使人们能够利用光度约束找到源中pp中微子的通量，其准确度优于1％ 。未来关于ve（-）散射的实验将使人们能够非常准确地测量地球上铍和pp中微子的通量。 pp中微子在地球上和源中的pp中微子通量之比将使人们能够非常精确地找到混合角theta（圆点）。锂探测器对CNO中微子具有很高的灵敏度，可以发现CNO循环对太阳中产生的能量的贡献。这将是对恒星演化理论的严格测试，并与其他实验相结合，将精确确定源中pp中微子的通量和混合角theta（圆点）。锂实验技术开发的工作目前正在进行中。 （C）2004 MAIK“ Nauka / Interperiodica”。
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