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Article
Report number arXiv:1810.10783
Title Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
Author(s)

Agafonova, N. (Moscow, INR) ; Alexandrov, A. (INFN, Naples) ; Anokhina, A. (SINP, Moscow) ; Aoki, S. (Kobe U.) ; Ariga, A. (U. Bern, AEC) ; Ariga, T. (U. Bern, AEC ; Kyushu U.) ; Bertolin, A. (INFN, Padua) ; Bozza, C. (INFN, Salerno ; Salerno U.) ; Brugnera, R. (INFN, Padua ; Padua U.) ; Buonaura, A. (INFN, Naples ; Naples U.) ; Buontempo, S. (INFN, Naples) ; Chernyavskiy, M. (Lebedev Inst.) ; Chukanov, A. (Dubna, JINR) ; Consiglio, L. (INFN, Naples) ; D'Ambrosio, N. (Gran Sasso) ; De Lellis, G. (INFN, Naples ; Naples U.) ; De Serio, M. (Bari U. ; INFN, Bari) ; del Amo Sanchez, P. (Annecy, LAPP) ; Di Crescenzo, A. (INFN, Naples ; Naples U.) ; Di Ferdinando, D. (INFN, Bologna) ; Di Marco, N. (Gran Sasso) ; Dmitrievsky, S. (Dubna, JINR) ; Dracos, M. (Strasbourg, IPHC) ; Duchesneau, D. (Annecy, LAPP) ; Dusini, S. (INFN, Padua) ; Dzhatdoev, T. (SINP, Moscow) ; Ebert, J. (Hamburg U.) ; Ereditato, A. (U. Bern, AEC) ; Fini, R.A. (INFN, Bari) ; Fornari, F. (INFN, Bologna ; U. Bologna, DIFA) ; Fukuda, T. (Nagoya U.) ; Galati, G. (INFN, Naples ; Naples U.) ; Garfagnini, A. (INFN, Padua ; Padua U.) ; Gentile, V. (GSSI, Aquila) ; Goldberg, J. (Technion) ; Gorbunov, S. (Lebedev Inst.) ; Gornushkin, Y. (Dubna, JINR) ; Grella, G. (INFN, Salerno ; Salerno U.) ; Guler, A.M. (Middle East Tech. U., Ankara) ; Gustavino, C. (INFN, Rome) ; Hagner, C. (Hamburg U.) ; Hara, T. (Kobe U.) ; Hayakawa, T. (Nagoya U.) ; Hollnagel, A. (Hamburg U.) ; Ishiguro, K. (Nagoya U.) ; Iuliano, A. (INFN, Naples ; Naples U.) ; Jakovčić, K. (Boskovic Inst., Zagreb) ; Jollet, C. (Strasbourg, IPHC) ; Kamiscioglu, C. (Middle East Tech. U., Ankara ; Ankara U.) ; Kamiscioglu, M. (Middle East Tech. U., Ankara) ; Kim, S.H. (Gyeongsang Natl. U.) ; Kitagawa, N. (Nagoya U.) ; Kliček, B. (Boskovic Inst., Zagreb) ; Kodama, K. (Aichi U. of Education) ; Komatsu, M. (Nagoya U.) ; Kose, U. (INFN, Padua) ; Kreslo, I. (U. Bern, AEC) ; Laudisio, F. (INFN, Padua ; Padua U.) ; Lauria, A. (INFN, Naples ; Naples U.) ; Ljubičić, A. (Boskovic Inst., Zagreb) ; Longhin, A. (INFN, Padua ; Padua U.) ; Loverre, P. (INFN, Rome) ; Malgin, A. (Moscow, INR) ; Mandrioli, G. (INFN, Bologna) ; Matsuo, T. (Toho U.) ; Matveev, V. (Moscow, INR) ; Mauri, N. (INFN, Bologna ; U. Bologna, DIFA) ; Medinaceli, E. (INFN, Padua ; Padua U.) ; Meregaglia, A. (Strasbourg, IPHC) ; Mikado, S. (Nihon U., Narashino) ; Miyanishi, M. (Nagoya U.) ; Mizutani, F. (Kobe U.) ; Monacelli, P. (INFN, Rome) ; Montesi, M.C. (INFN, Naples ; Naples U.) ; Morishima, K. (Nagoya U.) ; Muciaccia, M.T. (Bari U. ; INFN, Bari) ; Naganawa, N. (Nagoya U.) ; Naka, T. (Nagoya U.) ; Nakamura, M. (Nagoya U.) ; Nakano, T. (Nagoya U.) ; Niwa, K. (Nagoya U.) ; Ogawa, S. (Toho U.) ; Okateva, N. (Lebedev Inst.) ; Ozaki, K. (Kobe U.) ; Paoloni, A. (Frascati) ; Paparella, L. (Bari U. ; INFN, Bari) ; Park, B.D. (Gyeongsang Natl. U.) ; Pasqualini, L. (INFN, Bologna ; U. Bologna, DIFA) ; Pastore, A. (INFN, Bari) ; Patrizii, L. (INFN, Bologna) ; Pessard, H. (Annecy, LAPP) ; Podgrudkov, D. (SINP, Moscow) ; Polukhina, N. (Lebedev Inst. ; Moscow Phys. Eng. Inst.) ; Pozzato, M. (INFN, Bologna) ; Pupilli, F. (INFN, Padua) ; Roda, M. (INFN, Padua ; Padua U.) ; Roganova, T. (SINP, Moscow) ; Rokujo, H. (Nagoya U.) ; Rosa, G. (INFN, Rome) ; Ryazhskaya, O. (Moscow, INR) ; Sato, O. (Nagoya U.) ; Schembri, A. (Gran Sasso) ; Shakiryanova, I. (Moscow, INR) ; Shchedrina, T. (Lebedev Inst.) ; Shibayama, E. (Kobe U.) ; Shibuya, H. (Toho U.) ; Shiraishi, T. (Nagoya U.) ; Simone, S. (Bari U. ; INFN, Bari) ; Sirignano, C. (INFN, Padua ; Padua U.) ; Sirri, G. (INFN, Bologna) ; Sotnikov, A. (Dubna, JINR) ; Spinetti, M. (Frascati) ; Stanco, L. (INFN, Padua) ; Starkov, N. (Lebedev Inst.) ; Stellacci, S.M. (INFN, Salerno ; Salerno U.) ; Stipčević, M. (Boskovic Inst., Zagreb) ; Strolin, P. (INFN, Naples ; Naples U.) ; Takahashi, S. (Kobe U.) ; Tenti, M. (INFN, Bologna) ; Terranova, F. (Milan Bicocca U.) ; Tioukov, V. (INFN, Naples) ; Vasina, S. (Dubna, JINR) ; Vilain, P. (Brussels U., IIHE) ; Voevodina, E. (INFN, Naples) ; Votano, L. (Frascati) ; Vuilleumier, J.L. (U. Bern, AEC) ; Wilquet, G. (Brussels U., IIHE) ; Yoon, C.S. (Gyeongsang Natl. U.)

Publication 2019-10-01
Imprint 2018-10-25
Number of pages 15
In: JCAP 1910 (2019) 003
DOI 10.1088/1475-7516/2019/10/003
Subject category physics.ins-det ; Detectors and Experimental Techniques ; hep-ex ; Particle Physics - Experiment
Accelerator/Facility, Experiment CERN SPS ; OPERA CNGS1
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 of its correlation with the seasonal variation of the atmospheric temperature are reported.
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 Element opprettet 2018-10-31, sist endret 2024-05-02


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