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

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.; Galper, 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.; Krutkov, S. Y.; Leonov, A. A.; Marcelli, L.; Martucci, M.; Maiorov, A. G.; Malakhov, V. V.; Menn, W.; Mergè, M.; Mikhailov, V. V.; Mocchiutti, E.; Monaco, A.; Mori, N.; MUNINI, RICCARDO; Osteria, G.; Palma, F.; Panico, B.; Papini, P.; Pearce, M.; Picozza, P.; Ricci, M.; Ricciarini, S. B.; Rosetto, M. L.; Simon, M.; Sarkar, R.; Scotti, V.; Sparvoli, R.; Spillantini, P.; Formato, V.; Yurkin, Y. T.

doi:10.1134/S0021364015040086

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.

Titolo:	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
Autori:	A. V. Karelin O. Adriani G. C. Barbarino G. A. Bazilevskaya R. Bellotti M. Boezio E. A. Bogomolov M. Bongi V. Bonvicini S. Bottai A. Bruno A. Vacchi E. Vannuccini G. I. Vasil’ev S. A. Voronov A. M. Galper C. De Donato C. De Santis N. De Simone V. Di Felice G. Zampa N. Zampa F. Cafagna D. Campana R. Carbone P. Carlson M. Casolino G. Castellini A. N. Kvashnin S. V. Koldashov S. A. Koldobskii S. Y. Krutkov A. A. Leonov L. Marcelli M. Martucci A. G. Maiorov V. V. Malakhov W. Menn M. Mergè V. V. Mikhailov E. Mocchiutti A. Monaco N. Mori MUNINI, RICCARDO G. Osteria F. Palma B. Panico P. Papini M. Pearce P. Picozza M. Ricci S. B. Ricciarini M. L. Rosetto M. Simon R. Sarkar V. Scotti R. Sparvoli P. Spillantini V. Formato Y. T. Yurkin mostra contributor esterni nascondi contributor esterni
Data di pubblicazione:	2015
Rivista:	JETP LETTERS
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.
Handle:	http://hdl.handle.net/11368/2847406
Digital Object Identifier (DOI):	http://dx.doi.org/10.1134/S0021364015040086
URL:	http://dx.doi.org/10.1134/S0021364015040086
Appare nelle tipologie:	1.1 Articolo in Rivista

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