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Variations in the Cosmic Ray Flux at the End of Solar Cycle 24

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

Data from most neutron monitor stations show that the intensity of cosmic rays has not yet reached the level observed at them in 2009. At a number of stations (e.g., Barentsburg, Thule, Kerguelen, and Moscow), however, the intensity has already surpassed the 2009 level. This anomalous effect could be associated with the unusual behavior of solar activity in cycle 24.

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Authors and Affiliations

  1. Polar Geophysical Institute, 184209, Apatity, Russia

    Yu. V. Balabin

  2. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, 108840, Moscow, Russia

    A. V. Belov, R. T. Gushchina & V. G. Yanke

  3. Kabardino-Balkarian State University, 360004, Nalchik, Russia

    I. V. Yankovsky

Authors
  1. Yu. V. Balabin
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  2. A. V. Belov
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  3. R. T. Gushchina
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  4. V. G. Yanke
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  5. I. V. Yankovsky
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Corresponding author

Correspondence to Yu. V. Balabin.

Additional information

Translated by A. Kobkova

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Balabin, Y.V., Belov, A.V., Gushchina, R.T. et al. Variations in the Cosmic Ray Flux at the End of Solar Cycle 24. Bull. Russ. Acad. Sci. Phys. 85, 230–233 (2021). https://doi.org/10.3103/S1062873821030035

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  • DOI: https://doi.org/10.3103/S1062873821030035

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