Prediction of solar flares using neutrino detectors of the second generation. (arXiv:2307.16249v1 [astro-ph.SR])
<a href="http://arxiv.org/find/astro-ph/1/au:+Boyarkin_O/0/1/0/all/0/1">Oleg Boyarkin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Boyarkina_I/0/1/0/all/0/1">Iren Boyarkina</a>

The physics-based method of forecasting the high energy solar flares (SFs)
with the help of the neutrino detectors utilizing the coherent elastic
neutrino-nucleus scattering (CE$nu$NS) is considered. The behavior of the
neutrino beams traveling through the coupled sunspots (CSs) being the sources
of the future SFs is investigated. Two neutrino beams are included into
consideration, namely, the $nu_{eL}$ beam and the $nu_{mu L}$ beam which
have been produced 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 demonstrated, that
this weakening could be registered by the detectors employing CE$nu$NS only
when the neutrinos have the Dirac nature.

The physics-based method of forecasting the high energy solar flares (SFs)
with the help of the neutrino detectors utilizing the coherent elastic
neutrino-nucleus scattering (CE$nu$NS) is considered. The behavior of the
neutrino beams traveling through the coupled sunspots (CSs) being the sources
of the future SFs is investigated. Two neutrino beams are included into
consideration, namely, the $nu_{eL}$ beam and the $nu_{mu L}$ beam which
have been produced 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 demonstrated, that
this weakening could be registered by the detectors employing CE$nu$NS only
when the neutrinos have the Dirac nature.

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