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ИСТИНА ЦЭМИ РАН |
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In this study, an attempt is made to study the Sun on the basis of modern equipment and the latest advances in the study of solar neutrino fluxes. In particular, a neutrino telescope based on the ANRI effect is used. This made it possible to start the problem of the internal structure of the Sun within the framework of the model of a neutrino source of the central zone. The first results obtained from the flow pattern are in good agreement with the cavitation radiation neutrino model.