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We describe a mechanism for the new solution of the solar neutrino problem with natural anticorrelation with the solar magnetic-field activity in the convection zone. Our mechanism requires the simultaneous presence of the neutrino flavor mixing and the magnetic (or transition) moment as large as {μ}B{~}10^-10 ({μ} in units of Bohr magneton, B in kG).
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Minakata et al. (1989) studied this question.
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