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Study of Forbush Effects during Powerful Solar Flares by the URAGAN Muon Hodoscope Data

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

Abstract

Forbush effects caused by powerful X-class solar flares are studied using URAGAN muon hodoscope data for the period 2007–2019. The URAGAN muon hodoscope registers the cosmic ray muon flux on the Earth’s surface from different directions simultaneously. This allows study of the energy, angular, and space–time characteristics of variations in the cosmic ray muon flux during Forbush effects. The dependence of the measured Forbush effects on the parameters of heliospheric and geomagnetic disturbances is analyzed.

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ACKNOWLEDGMENTS

This work was performed with data from the Unique Scientific Facility NEVOD.

Funding

This work was supported by the Russian Science Foundation, project no. 17-17-01215.

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Authors and Affiliations

  1. National Research Nuclear University (MEPhI), 115409, Moscow, Russia

    A. A. Kovylyaeva, N. S. Barbashina, A. N. Dmitrieva, Yu. N. Mishutina, V. V. Shutenko, E. I. Yakovleva & I. I. Yashin

  2. Geophysical Center, Russian Academy of Sciences, 119296, Moscow, Russia

    A. A. Kovylyaeva, V. G. Getmanov, A. N. Dmitrieva, M. N. Dobrovolsky, A. A. Soloviev, V. E. Chinkin & I. I. Yashin

  3. Schmidt Institute of Physics of the Earth, Russian Academy of Sciences, 123995, Moscow, Russia

    V. G. Getmanov & A. A. Soloviev

Authors
  1. A. A. Kovylyaeva
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  2. N. S. Barbashina
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  3. V. G. Getmanov
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  4. A. N. Dmitrieva
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  5. M. N. Dobrovolsky
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  6. Yu. N. Mishutina
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  7. A. A. Soloviev
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  8. V. E. Chinkin
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  9. V. V. Shutenko
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  10. E. I. Yakovleva
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  11. I. I. Yashin
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Corresponding author

Correspondence to A. A. Kovylyaeva.

Additional information

Translated by A. Nikol’skii

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Kovylyaeva, A.A., Barbashina, N.S., Getmanov, V.G. et al. Study of Forbush Effects during Powerful Solar Flares by the URAGAN Muon Hodoscope Data. Bull. Russ. Acad. Sci. Phys. 85, 464–467 (2021). https://doi.org/10.3103/S1062873821030126

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  • DOI: https://doi.org/10.3103/S1062873821030126

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