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Using Data from a Ground-Based Network of Detectors and the PAMELA and AMS-02 Experiments to Compare Long-Term Variations in the Cosmic Ray Flux

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

Abstract

Results are presented from comparing long-term changes in the flux of cosmic rays, using data obtained by a network of ground-based detectors, direct measurements of fluxes made with the PAMELA and AMS-02 magnetic spectrometers, and a series of stratospheric balloon soundings.

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ACKNOWLEDGEMENTS

This work was performed on equipment at the CRSN (Cosmic Ray Station Network) research facility.

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Authors and Affiliations

  1. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, 108840, Moscow, Russia

    A. V. Belov, R. T. Gushchina, N. S. Shlyk & V. G. Yanke

Authors
  1. A. V. Belov
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  2. R. T. Gushchina
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  3. N. S. Shlyk
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  4. V. G. Yanke
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Corresponding author

Correspondence to V. G. Yanke.

Additional information

Translated by A. Kobkova

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Belov, A.V., Gushchina, R.T., Shlyk, N.S. et al. Using Data from a Ground-Based Network of Detectors and the PAMELA and AMS-02 Experiments to Compare Long-Term Variations in the Cosmic Ray Flux. Bull. Russ. Acad. Sci. Phys. 85, 1039–1041 (2021). https://doi.org/10.3103/S1062873821090045

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  • DOI: https://doi.org/10.3103/S1062873821090045

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