Observational analysis showed cosmic ray flux changes during geomagnetic disturbances, suggesting varied effects on cosmic rays.
We presented the results of the analysis of solar and geomagnetic activity, variations in cosmic ray fluxes in the period May 9–15, 2024. Data from a network of ground-based neutron monitors, data from measurements of cosmic rays by CARPET instruments and neutron detectors located at the Dolgoprudnenskaya Scientific Station of the LP1 RAS, at the Eurasian National University (Astana, Republic of Kazakhstan) and at the astronomical complex KASLEO are used (The Argentine Andes). We studied the characteristics of the Forbush decrease in cosmic ray fluxes on May 10, 2024, and the subsequent increase in cosmic rays on May 11. The results obtained indicate the different nature of these effects.
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V. S. Makhmutov (2025) studied this question.
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