Geoefficiency of Sporadic Phenomena in Solar Cycle 24

A. V. Belov; Белов А. В.; E. A. Belova; Белова Е. А.; N. S. Shlyk; Шлык Н. С.; M. A. Abunina; Абунина М. А.; A. A. Abunin; Абунин А. А.

doi:10.31857/S0016794023600291

Geoefficiency of Sporadic Phenomena in Solar Cycle 24

Authors: Belov A.V.¹, Belova E.A.¹, Shlyk N.S.¹, Abunina M.A.¹, Abunin A.A.¹
Affiliations:
1. Pushkov Institute of Terrestrial Magnetism, the Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences (IZMIRAN)
Issue: Vol 63, No 4 (2023)
Pages: 534-544
Section: Articles
URL: https://journals.rcsi.science/0016-7940/article/view/134744
DOI: https://doi.org/10.31857/S0016794023600291
EDN: https://elibrary.ru/OUBOKI
ID: 134744

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Abstract
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References
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Abstract

The specific features of solar cycle 24 are discussed, including cosmic ray variations, characteristics
of solar flares, proton events, coronal mass ejections, and the level of geomagnetic activity. It is shown
that in terms of the sunspot number and other manifestations of solar activity, cycle 24 turned out to be the
most modest one over the last 100 years of observations. A significant decrease in the geoefficiency of various
solar events is described, which manifested itself in a smaller number and magnitude of Forbush
effects recorded on the Earth, the enhancements of the fluxes of protons and electrons of different energies,
and geomagnetic storms.

References

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