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, Oscar; Barbarino, G. C.; Bazilevskaya, G. A.; Bellotti, R.; Boezio, M.; Bogomolov, E. A.; Bongi, Massimo; 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. Y. U.; 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, Nicola; Munini, R.; 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. U. 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.

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.; 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.; Marcelli, L.; Martucci, M.; Maiorov, A.G.; Malakhov, V.V.; Menn, W.; Mergè, M.; Mikhailov, V.V.; Mocchiutti, E.; Monaco, A.; Mori, N.; Munini, R.; 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, Yu. T.. - In: JETP LETTERS. - ISSN 0021-3640. - ELETTRONICO. - 101:(2015), pp. 228-231. [10.1134/S0021364015040086]