Variations in the Cosmic Ray Flux at the End of Solar Cycle 24

Variations in the Cosmic Ray Flux at the End of Solar Cycle 24

Data from most neutron monitor stations show that the intensity of cosmic rays has not yet reached the level observed at them in 2009. At a number of stations (e.g., Barentsburg, Thule, Kerguelen, and Moscow), however, the intensity has already surpassed the 2009 level. This anomalous effect could b...

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Veröffentlicht in:Bulletin of the Russian Academy of Sciences. Physics 2021-03, Vol.85 (3), p.230-233
Hauptverfasser: Balabin, Yu. V., Belov, A. V., Gushchina, R. T., Yanke, V. G., Yankovsky, I. V.
Format: Artikel
Sprache:eng
Schlagworte:
Cosmic rays
Hadrons
Heavy Ions
Neutron flux
Nuclear Physics
Physics
Physics and Astronomy
Solar activity
Solar cycle
Stations
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Zusammenfassung:Data from most neutron monitor stations show that the intensity of cosmic rays has not yet reached the level observed at them in 2009. At a number of stations (e.g., Barentsburg, Thule, Kerguelen, and Moscow), however, the intensity has already surpassed the 2009 level. This anomalous effect could be associated with the unusual behavior of solar activity in cycle 24.
ISSN:1062-8738
1934-9432
DOI:10.3103/S1062873821030035