Detection of a change in the North-South ratio of count rates of particles of high-energy cosmic rays during a change in the polarity of the magnetic field of the Sun

作者:Karelin A V*; Adriani O; Barbarino G C; Bazilevskaya G A; Bellotti R; Boezio M; Bogomolov E A; Bongi M; Bonvicini V; Bottai S; Bruno A; Vacchi A; Vannuccini E; Vasil'ev G I; Voronov S A; Gal'per A M; De Donato C; De Santis C; De Simone N; Di Felice V; Zampa G; Zampa N; Cafagna F; Campana D; Carbone R; Carlson P; Casolino M; Castellini G; Kvashnin A N; Koldashov S V; Koldobskii S A; Krut'kov S Yu; Leonov A A
来源:JETP Letters, 2015, 101(4): 228-231.
DOI:10.1134/S0021364015040086

摘要

A change in the ratio of the intensities of particles of high-energy cosmic rays arriving from the North and South in the time interval of 2010-2014 has been detected with a calorimeter entering into the experimental complex of the PAMELA satellite experiment since June 2006. The polarity of the magnetic field of the Sun changed in a part of this time interval. Thus, the results indicate that the North-South asymmetry of cosmic ray fluxes is related to the magnetic field of the Sun.

  • 出版日期2015-2

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