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Investigation of Atmospheric Fronts by Means of Cosmic Ray Muon Flux

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Abstract

New method of investigation of atmospheric fronts by means of cosmic ray muon flux is considered. The method is based on searches of changes in the muon flux in the atmosphere, caused by waves from atmospheric fronts. For search of such waves 105 atmospheric fronts passing over Moscow were analyzed. The method allows determining the directions of the waves and their periods.

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Funding

The work was carried out at the Unique Scientific Facility ‘‘Experimental Complex NEVOD’’ and supported by the Ministry of Science and Higher Education of the Russian Federation (State Assignment no. FSWU-2023-0068, project ‘‘Fundamental and Applied Research of Cosmic Rays’’).

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Authors and Affiliations

  1. National Research Nuclear University MEPhI, Moscow, Russia

    S. S. Timakov, A. A. Petrukhin & V. R. Epifanov

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  1. S. S. Timakov
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  2. A. A. Petrukhin
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  3. V. R. Epifanov
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Correspondence to S. S. Timakov.

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Timakov, S.S., Petrukhin, A.A. & Epifanov, V.R. Investigation of Atmospheric Fronts by Means of Cosmic Ray Muon Flux. Phys. Atom. Nuclei 86, 1114–1118 (2023). https://doi.org/10.1134/S1063778824010551

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  • DOI: https://doi.org/10.1134/S1063778824010551

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