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Cited 14 time in webofscience Cited 13 time in scopus
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Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector

Authors
Agafonova, N.Alexandrov, A.Anokhina, A.Aoki, S.Ariga, A.Ariga, T.Bertolin, A.Bozza, C.Brugnera, R.Buonaura, A.Buontempo, S.Chernyavskiy, M.Chukanov, A.Consiglio, L.D'Ambrosio, N.De Lellis, G.De Serio, M.Sanchez, P. del AmoDi Crescenzo, A.Di Ferdinando, D.Di Marco, N.Dmitrievsky, S.Dracos, M.Duchesneau, D.Dusini, S.Dzhatdoev, T.Ebert, J.Ereditato, A.Fini, R. A.Fornari, F.Fukuda, T.Galati, G.Garfagnini, A.Gentile, VGoldberg, J.Gorbunov, S.Gornushkin, Y.Grella, G.Guler, A. M.Gustavino, C.Hagner, C.Hara, T.Hayakawa, T.Hollnagel, A.Ishiguro, K.Iuliano, A.Jakovcic, K.Jollet, C.Kamiscioglu, C.Kamiscioglu, M.Kim, S. H.Kitagawa, N.Klicek, B.Kodama, K.Komatsu, M.Kose, U.Kreslo, ILaudisio, F.Lauria, A.Ljubicic, A.Longhin, A.Loverre, P.Malgin, A.Mandrioli, G.Matsuo, T.Matveev, VMauri, N.Medinaceli, E.Meregaglia, A.Mikado, S.Miyanishi, M.Mizutani, F.Monacelli, P.Montesi, M. C.Morishima, K.Muciaccia, M. T.Naganawa, N.Naka, T.Nakamura, M.Nakano, T.Niwa, K.Ogawa, S.Okateva, N.Ozaki, K.Paoloni, A.Paparella, L.Park, B. D.Pasqualini, L.Pastore, A.Patrizii, L.Pessard, H.Podgrudkov, D.Polukhina, N.Pozzato, M.Pupilli, F.Roda, M.Roganova, T.Rokujo, H.Rosa, G.Ryazhskaya, O.Sato, O.Schembri, A.Shakiryanova, IShchedrina, T.Shibayama, E.Shibuya, H.Shiraishi, T.Simone, S.Sirignano, C.Sirri, G.Sotnikov, A.Spinetti, M.Stanco, L.Starkov, N.Stellacci, S. M.Stipcevic, M.Strolin, P.Takahashi, S.Tenti, M.Terranova, F.Tioukov, VVasina, S.Vilain, P.Voevodina, E.Votano, L.Vuilleumier, J. L.Wilquet, G.Yoon, C. S.
Issue Date
Oct-2019
Publisher
IOP PUBLISHING LTD
Keywords
cosmic rays detectors; neutrino detectors; neutrino experiments
Citation
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, no.10
Indexed
SCIE
SCOPUS
Journal Title
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Number
10
URI
https://scholarworks.gnu.ac.kr/handle/sw.gnu/73263
DOI
10.1088/1475-7516/2019/10/003
ISSN
1475-7516
Abstract
The OPERA experiment discovered muon neutrino into tau neutrino oscillations in appearance mode, detecting tau leptons by means of nuclear emulsion films. The apparatus was also endowed with electronic detectors with tracking capability, such as scintillator strips and resistive plate chambers. Because of its location in the underground Gran Sasso laboratory, under 3800 m.w.e., the OPERA detector has also been used as an observatory for TeV muons produced by cosmic rays in the atmosphere. In this paper the measurement of the single muon flux modulation and its correlation with the seasonal cycle of atmospheric temperature is reported.
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