Pis'ma v Zh. Èksper. Teoret. Fiz., 2015 Volume 101, Issue 4, Pages 246–249
(Mi jetpl4552)
ASTROPHYSICS AND COSMOLOGY 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. Karelin a ,
O. Adriani bc ,
G. Barbarino de ,
G. A. Bazilevskaya f ,
R. Bellotti gh ,
M. Boezio i ,
E. A. Bogomolov j ,
M. Bongi c ,
V. Bonvicini i ,
S. Bottai c ,
A. Bruno hg ,
S. Vacchi i ,
E. Vannuccini c ,
G. I. Vasiliev j ,
S. A. Voronov a ,
A. M. Gal'per a ,
C. De Donato kl ,
K. De Santis kl ,
N. De Simone kl ,
V. Di Felice k ,
G. Zampa i ,
N. Zampa i ,
F. Cafagna g ,
D. Campana d ,
R. Carbone ld ,
P. Carlson m ,
M. Casolino k ,
G. Castellini n ,
A. N. Kvashnin f ,
S. V. Koldashov a ,
S. V. Koldobskii a ,
S. Yu. Krut'kov j ,
A. A. Leonov a ,
L. Marcelli k ,
M. Martucci ko ,
A. G. Maiorov a ,
V. V. Malakhov a ,
W. Menn p ,
M. Mergè kl ,
V. V. Mikhailov a ,
E. Mocchiutti i ,
A. Monaco g ,
N. Mori bc ,
R. Munini iq ,
G. Osteria d ,
F. Palma kl ,
B. Panico d ,
P. Papini c ,
M. Pearce m ,
P. Picozza kl ,
M. Ricci o ,
S. Ricciarini c ,
M. L. Rosetto m ,
M. Simon p ,
R. Sarkar i ,
V. Scotti ed ,
R. Sparvoli kl ,
P. Spillantini cb ,
V. Formato iq ,
Yu. T. Yurkin a a National Research Nuclear University MEPhI, Kashirskoe sh. 31, Moscow, 115409, Russia b University of Florence, I-50019, Sesto Fiorentiono, Florence, Italy c INFN, Sezione di Florence, I-50019, Sesto Fiorentiono, Florence, Italy d INFN, Sezione di Naples, I-80126, Naples, Italy e University of Naples "Federico II", I-80126, Naples, Italy f Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia g INFN, Sezione di Bari, I-70126, Bari, Italy h University of Bari, I-70126, Bari, Italy i INFN, Sezione di Trieste, I-34149, Trieste, Italy j Ioffe Physical Technical Institute, Russian Academy of Sciences, Politekhnicheskaya ul. 26, St. Petersburg, 194021, Russia k INFN, Sezione di Rome "Tor Vergata", I-00133, Rome, Italy l University of Rome "Tor Vergata", I-00133, Rome, Italy m KTH, Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics AlbaNova University Centre,
SE-10691 Stockholm, Sweden n IFAC, I-50019, Sesto Fiorentino, Florence, Italy o INFN, Laboratori Nazionali di Frascati, I-00044, Frascati, Italy p University of Siegen, D-57068 Siegen, Germany q University of Trieste, I-34147 Trieste, Italy 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.
Received: 22.12.2014
DOI:
10.7868/S0370274X15040037
© , 2024
Fulltext:
PDF file (188 kB)