vestifmИзвестия Национальной академии наук Беларуси. Серия физико-математических наукProceedings of the National Academy of Sciences of Belarus. Physics and Mathematics Series1561-24302524-2415The Republican Unitary Enterprise Publishing House "Belaruskaya Navuka"10.29235/1561-2430-2023-59-2-147-157vestifm-714Research ArticleФИЗИКАPHYSICSПредсказание солнечных вспышек с помощью нейтринных детекторов второго поколенияPrediction of solar flares using neutrino detectors of the second generationhttps://orcid.org/0000-0003-3880-6918БояркинО. М.BoyarkinO. M.

Бояркин Олег Михайлович – доктор физико-математических наук, профессор

пр. Независимости, 4, 220030, Минск

Oleg M. Boyarkin – Dr. Sc. (Physics and Mathematics),Professor

4, Nezavisimosti Ave., 220030

oboyarkin@tut.byБояркинаИ. О.BoyarkinaI. O.

Бояркина Ирена Олеговна – кандидат наук, ассистент, инженерно-экономический факультет

ул. Парадизо, 47, 01100, Витербо

Iren O. Boyarkina – Ph. D., Assistant, Department ofEconomics, Engineering, Society and Business Organisation

47, Paradise Str., Viterbo, Italy, 01100

estel20@mail.ruБелорусский государственный университетBelarusian State UniversityУниверситет ТускииUniversity of Tuscia202306072023592147157Copyright © Бояркин О.М., Бояркина И.О., 20232023Бояркин О.М., Бояркина И.О.Boyarkin O.M., Boyarkina I.O.Данная работа распространяется под лицензией Creative Commons Attribution 4.0.This work is licensed under a Creative Commons Attribution 4.0 License.https://vestifm.belnauka.by/jour/article/view/714

Предлагается физически обоснованный метод прогнозирования суперсолнечных вспышек с помощью нейтринных детекторов, работа которых основана на использовании когерентного упругого рассеяния нейтрино на ядрах. Исследуется поведение нейтринных пучков, проходящих через спаренные солнечные пятна, которые являются источниками будущих солнечных вспышек. Рассматривается эволюция пучка левосторонних электронных нейтрино и пучка левосторонних мюонных нейтрино, которые образовались в конвективной зоне после прохождения резонанса Михеева – Смирнова – Вольфенштейна. Предполагается, что нейтрино обладает такими мультипольными моментами, как зарядовый радиус, магнитный и анапольный моменты, в то время как магнитное поле спаренных солнечных пятен является вихревым, неоднородным и обладает скручиванием. Даются оценки ослабления нейтринных пучков после прохождения резонансных переходов. Показывается, что в случае суперсолнечных вспышек эти ослабления могут быть зарегистрированы нейтринными детекторами второго поколения только тогда, когда нейтрино имеет дираковскую природу. 

In this paper, we propose a physics-based method of prediction high-energy solar flares (SFs) with the help of neutrino detectors utilizing coherent elastic neutrino-nucleus scattering (CEνNS). The behavior of neutrino beams passing through coupled sunspots (CSs) being the sources of future SFs is investigated. We consider the evolution of left-handed electron neutrino νeL and muon neutrino νμL beams formed in the convective zone after the passage of the Micheev – Smirnov – Wolfenstein resonance. It is assumed that the neutrinos possess the charge radius, the magnetic and anapole moments while the CS magnetic field is vortex, nonhomogeneous and has twisting. Estimations of the weakening of the neutrino beams after traversing the resonant layers are given. It is shown that for SFs this weakening could be registered by neutrino detectors of the second generation only when neutrinos have the Dirac nature. 

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The authors declare that there are no conflicts of interest present.