Solar neutrino oscillations
Abstract
The author considers the behavior of an electron neutrino beam in solar matter and presents a method for predicting high-energy solar flares, based on the attenuation of an electron neutrino beam when passing through the magnetic field of paired sunspots.
About the Authors
O. Boyarkin
Международный государственный экологический институт им. А.Д. Сахарова БГУ
Belarus
Belarus
V. Makhnach
БГУИР
Belarus
Belarus
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Review
For citations:
Boyarkin O., Makhnach V. Solar neutrino oscillations. Science and Innovations. 2024;(4):45-49. (In Russ.)
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