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Monitoring Space Weather with a System of Ground-Based Cosmic Ray Detectors

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

Abstract

Flicker noise spectroscopy is developed for the remote identification of processes of powerful solar activity in the form of coronal mass ejections (CMEs) directed toward the Earth. Results are presented from analyzing geo-effective events (>G1) using data from the international network of neutron monitors and the URAGAN multidirectional muon hodoscope that indicate the emergence of precursors (1–2 days in advance) of CMEs approaching the Earth’s orbit.

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ACKNOWLEDGMENTS

This work was performed at the NEVOD Research Center of the Moscow Engineering Physics Institute.

Funding

The study was supported by the program “Priority 2030.”

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Authors and Affiliations

  1. Moscow Engineering Physics Institute (MEPhI), 115409, Moscow, Russia

    V. V. Borog, A. N. Dmitrieva & Y. N. Mishutina

Authors
  1. V. V. Borog
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  2. A. N. Dmitrieva
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  3. Y. N. Mishutina
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Corresponding author

Correspondence to V. V. Borog.

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The authors of this work declare that they have no conflicts of interest.

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Translated by E. Seifina

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Borog, V.V., Dmitrieva, A.N. & Mishutina, Y.N. Monitoring Space Weather with a System of Ground-Based Cosmic Ray Detectors. Bull. Russ. Acad. Sci. Phys. 88, 260–264 (2024). https://doi.org/10.1134/S1062873823705342

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  • DOI: https://doi.org/10.1134/S1062873823705342

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