Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector
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DOI：
10.1088/1475-7516/2019/10/003
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发表时间：
2018-10
影响因子：
6.4
通讯作者：
N. Agafonova;A. Alexandrov;A. Anokhina;S. Aoki;A. Ariga;T. Ariga;A. Bertolin;C. Bozza;R. Brugnera;A. Buonaura;S. Buontempo;M. Chernyavskiy;A. Chukanov;L. Consiglio;N. D’Ambrosio;G. Lellis;M. Serio;P. Sanchez;A. Crescenzo;D. Ferdinando;N. Marco;S. Dmitrievsky;M. Dracos;D. Duchesneau;S. Dusini;T. Dzhatdoev;J. Ebert;A. Ereditato;R. Fini;F. Fornari;T. Fukuda;G. Galati;A. Garfagnini;V. Gentile;J. Goldberg;S. Gorbunov;Y. Gornushkin;G. Grella;A. Guler;C. Gustavino;C. Hagner;T. Hara;T. Hayakawa;A. Hollnagel;K. Ishiguro;A. Iuliano;K. Jakovčić;C. Jollet;Ç. Kamışcıoğlu;M. Kamiscioglu;S.H. Kim;N. Kitagawa;B. Kliček;K. Kodama;M. Komatsu;U. Kose;I. Kreslo;F. Laudisio;A. Lauria;A. Ljubičić;A. Longhin;P. Loverre;A. Malgin;G. Mandrioli;T. Matsuo;V. Matveev;N. Mauri;E. Medinaceli;A. Meregaglia;S. Mikado;M. Miyanishi;F. Mizutani;P. Monacelli;M. Montesi;K. Morishima;M. Muciaccia;N. Naganawa;T. Naka;M. Nakamura;T. Nakano;K. Niwa;S. Ogawa;N. Okateva;K. Ozaki;A. Paoloni;L. Paparella;B. Park;L. Pasqualini;A. Pastore;L. Patrizii;H. Pessard;D. Podgrudkov;N. Polukhina;M. Pozzato;F. Pupilli;M. Roda;T. Roganova;H. Rokujo;G. Rosa;O. Ryazhskaya;O. Sato;A. Schembri;I. Shakiryanova;T. Shchedrina;E. Shibayama;H. Shibuya;T. Shiraishi;S. Simone;C. Sirignano;G. Sirri;A. Sotnikov;M. Spinetti;L. Stanco;N. Starkov;S. Stellacci;M. Stipčević;P. Strolin;S. Takahashi;M. Tenti;F. Terranova;V. Tioukov;S. Vasina;P. Vilain;E. Voevodina;L. Votano;J. Vuilleumier;G. Wilquet;C. Yoon
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文献类型：
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作者：
N. Agafonova;A. Alexandrov;A. Anokhina;S. Aoki;A. Ariga;T. Ariga;A. Bertolin;C. Bozza;R. Brugnera;A. Buonaura;S. Buontempo;M. Chernyavskiy;A. Chukanov;L. Consiglio;N. D’Ambrosio;G. Lellis;M. Serio;P. Sanchez;A. Crescenzo;D. Ferdinando;N. Marco;S. Dmitrievsky;M. Dracos;D. Duchesneau;S. Dusini;T. Dzhatdoev;J. Ebert;A. Ereditato;R. Fini;F. Fornari;T. Fukuda;G. Galati;A. Garfagnini;V. Gentile;J. Goldberg;S. Gorbunov;Y. Gornushkin;G. Grella;A. Guler;C. Gustavino;C. Hagner;T. Hara;T. Hayakawa;A. Hollnagel;K. Ishiguro;A. Iuliano;K. Jakovčić;C. Jollet;Ç. Kamışcıoğlu;M. Kamiscioglu;S.H. Kim;N. Kitagawa;B. Kliček;K. Kodama;M. Komatsu;U. Kose;I. Kreslo;F. Laudisio;A. Lauria;A. Ljubičić;A. Longhin;P. Loverre;A. Malgin;G. Mandrioli;T. Matsuo;V. Matveev;N. Mauri;E. Medinaceli;A. Meregaglia;S. Mikado;M. Miyanishi;F. Mizutani;P. Monacelli;M. Montesi;K. Morishima;M. Muciaccia;N. Naganawa;T. Naka;M. Nakamura;T. Nakano;K. Niwa;S. Ogawa;N. Okateva;K. Ozaki;A. Paoloni;L. Paparella;B. Park;L. Pasqualini;A. Pastore;L. Patrizii;H. Pessard;D. Podgrudkov;N. Polukhina;M. Pozzato;F. Pupilli;M. Roda;T. Roganova;H. Rokujo;G. Rosa;O. Ryazhskaya;O. Sato;A. Schembri;I. Shakiryanova;T. Shchedrina;E. Shibayama;H. Shibuya;T. Shiraishi;S. Simone;C. Sirignano;G. Sirri;A. Sotnikov;M. Spinetti;L. Stanco;N. Starkov;S. Stellacci;M. Stipčević;P. Strolin;S. Takahashi;M. Tenti;F. Terranova;V. Tioukov;S. Vasina;P. Vilain;E. Voevodina;L. Votano;J. Vuilleumier;G. Wilquet;C. Yoon
OPERA实验发现了μ中微子在τ中微子振荡中的出现模式，通过核乳胶膜检测τ轻子。该仪器还配备了具有跟踪能力的电子探测器，如闪烁体条和电阻板室。由于它位于格兰萨索地下实验室，低于3800 m.w.e.，OPERA探测器也被用作观测大气中宇宙射线产生的TeV μ子的观测站。本文报道了单μ子通量调制的测量及其与大气温度季节循环的关系。
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.