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.

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 / A. V., K., O., A., G. C., B., G. A., B., R., B., M., B., E. A., B., M., B., V., B., S., B., A., B., A., V., E., V., G. I., V., S. A., V., A. M., G., C., D.D., C., D.S., N., D.S., V., D.F., et al.. - In: JETP LETTERS. - ISSN 0021-3640. - STAMPA. - 101:4(2015), pp. 228-231. [10.1134/S0021364015040086]

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

MUNINI, RICCARDO;
2015-01-01

Abstract

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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11368/2847406
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