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Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
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. Beca...
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| Lenguaje: | eng |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2019/10/003 http://cds.cern.ch/record/2645401 |
| _version_ | 1780960440211210240 |
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| author | 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. del Amo Sanchez, P. Di 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, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Ljubičić, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, 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, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. |
| author_facet | 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. del Amo Sanchez, P. Di 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, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Ljubičić, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, 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, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. |
| author_sort | Agafonova, N. |
| collection | CERN |
| description | 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. |
| id | cern-2645401 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2018 |
| record_format | invenio |
| spelling | cern-26454012023-04-04T03:13:18Zdoi:10.1088/1475-7516/2019/10/003http://cds.cern.ch/record/2645401engAgafonova, 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.del Amo Sanchez, P.Di 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, V.Goldberg, J.Gorbunov, S.Gornushkin, Y.Grella, G.Guler, A.M.Gustavino, C.Hagner, C.Hara, T.Hayakawa, T.Hollnagel, A.Ishiguro, K.Iuliano, A.Jakovčić, K.Jollet, C.Kamiscioglu, C.Kamiscioglu, M.Kim, S.H.Kitagawa, N.Kliček, B.Kodama, K.Komatsu, M.Kose, U.Kreslo, I.Laudisio, F.Lauria, A.Ljubičić, A.Longhin, A.Loverre, P.Malgin, A.Mandrioli, G.Matsuo, T.Matveev, V.Mauri, 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, I.Shchedrina, T.Shibayama, E.Shibuya, H.Shiraishi, T.Simone, S.Sirignano, C.Sirri, G.Sotnikov, A.Spinetti, M.Stanco, L.Starkov, N.Stellacci, S.M.Stipčević, M.Strolin, P.Takahashi, S.Tenti, M.Terranova, F.Tioukov, V.Vasina, S.Vilain, P.Voevodina, E.Votano, L.Vuilleumier, J.L.Wilquet, G.Yoon, C.S.Measurement of the cosmic ray muon flux seasonal variation with the OPERA detectorphysics.ins-detDetectors and Experimental Techniqueshep-exParticle Physics - ExperimentThe 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.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.arXiv:1810.10783oai:cds.cern.ch:26454012018-10-25 |
| spellingShingle | physics.ins-det Detectors and Experimental Techniques hep-ex Particle Physics - Experiment 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. del Amo Sanchez, P. Di 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, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Ljubičić, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, 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, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title | Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title_full | Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title_fullStr | Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title_full_unstemmed | Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title_short | Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector |
| title_sort | measurement of the cosmic ray muon flux seasonal variation with the opera detector |
| topic | physics.ins-det Detectors and Experimental Techniques hep-ex Particle Physics - Experiment |
| url | https://dx.doi.org/10.1088/1475-7516/2019/10/003 http://cds.cern.ch/record/2645401 |
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