Abstract
A comparative analysis is performed of data on variations in the electromagnetic component over a solar cycle (SC) to study increases in gamma radiation in different phases of an SC. Variations in the intensity of cosmic rays are detected in Apatity by different detectors for all main components of secondary cosmic rays: nucleonic, electron–muonic, and electromagnetic (gamma radiation).
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Translated by M. Potapov
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Balabin, Y.V., Germanenko, A.V., Mikhalko, E.A. et al. Effect of Solar Activity on Events of Growing Background Gamma Radiation. Bull. Russ. Acad. Sci. Phys. 86, 290–294 (2022). https://doi.org/10.3103/S1062873822030042
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DOI: https://doi.org/10.3103/S1062873822030042