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. BoyarkinBelarus
V. Makhnach
Belarus
References
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Review
For citations:
Boyarkin O., Makhnach V. Solar neutrino oscillations. Science and Innovations. 2024;(4):45-49. (In Russ.)