Abstract
From the data (uncorrected for temperature effect) of the global network of neutron monitors (GNNM), along with the data of the Yakutsk muon telescope suite and the URAGAN muon hodoscope (Moscow), we applied a modified spectrographic global survey (SGS) for the 2018 Aug event to split cosmic ray variations into components of primary, magnetospheric, and atmospheric origin. Obtained were the time evolutions for the different-rigidity primary particle isotropic flux, pitch-angle anisotropy of cosmic rays (CRs), and interplanetary magnetic field (IMF) orientation. We provide variations in the rigidity of the geomagnetic cutoff (RGC) in Irkutsk and in the average bulk temperature at the points that observe charged components.
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ACKNOWLEDGMENTS
The authors are grateful to Pyotr Gololobov and Sergey Starodubtsev (Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences) for providing the data of the Yakutsk muon telescope suite.
The results were obtained by using the facilities at the Angara Multi-Access Center (Angara MAC) and at the “Russian National Ground-Based Network of Cosmic Ray Stations” (CRS Network) Unique Research Facilities (URFs).
Funding
The study was supported by the RF Ministry of Science and Higher Education (project no. 075-00964-20-01).
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Kovalev, I.I., Olemskoy, S.V., Sdobnov, V.E. et al. Monitoring Heliosphere, Magnetosphere, and Atmosphere via Cosmic Ray Effects in 2018 August. Bull. Russ. Acad. Sci. Phys. 87, 958–961 (2023). https://doi.org/10.3103/S1062873823702556
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DOI: https://doi.org/10.3103/S1062873823702556