Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station

Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/105595

Title:	Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
Authors:	張元翰;Vitale, V;Beischer, B;Bizzaglia, S;Barrau, A;Shan, Y H;Yu, Y J;Consolandi, C;Nozzoli, F;Schmidt, S M;Battarbee, M;Lee, H T;Lee, S C;Xin, G M;Vecchi, M;Wang, Z X;Bachlechner, A;He, Z H;Chen, H;Berdugo, J;Yan, Q;García, B;Hsieh, T H;Battiston, R;Yi, H;Corti, C;Cui, Z;Luo, J Z;Rancoita, P G;Chou, H Y;Sbarra, C;Heil, M;Tang, X W;Gargiulo, C;Fiasson, A;Grandi, D;Li, H L;Qu, Z Y;Paniccia, M;Choumilov, E;Aisa, D;Qin, X;Spinella, F;Zhuang, H L;Guo, K H;Gillard, W;Ionica, M;Levi, G;von Doetinchem, P;Shi, Y M;Huang, Z C;Xu, W;Bizzarri, M;Lim, S;Du, W J;Wienkenhöver, J;Cheng, G M;Di Masso, L;Lv, S S;García-López, R;Xu, N S;Zhang, M T;Crispoltoni, M;Pereira, R;Zichichi, A;Kim, G N;Mo, D C;Li, Z H;Lin, C H;Marín, J;Quadrani, L;Eronen, T;Sagdeev, R;Rosier-Lees, S;Eline, A;Bartoloni, A;Fan, Y Y;Vitillo, S;Galaktionov, Y;Martínez, G;Putze, A;Gebauer, I;Li, W;Velasco, M;Li, Q;Lippert, T;Bollweg, K;de Boer, W;Nunes, P;Wu, X;Menchaca-Rocha, A;Müller, M;Jang, W Y;Poireau, V;Wang, N H;Lu, Y S;Tao, L;Alpat, B;Li, T X;Tang, C P;Rozza, D
Contributors:	理學院物理學系
Keywords:	Alpha Magnetic Spectrometer;Astrophysics;Astrophysics and Astronomy;Cosmic rays;Cosmology and Extra-Galactic Astrophysics;Detectors and Experimental Techniques;Flux;Instrumentation and Methods for Astrophysic;Origins;Physics;Primary cosmic rays;Rigidity;Spectra;Television
Date:	2015-04-30
Issue Date:	2026-04-23 12:40:42 (UTC+8)
Publisher:	American Physical Society;United States: American Physical Society
Abstract:	摘要： A precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin, acceleration, and propagation of cosmic rays. We present the detailed variation with rigidity of the flux spectral index for the first time. The spectral index progressively hardens at high rigidities. 其他題名： Phys Rev Lett 出版者： United States: American Physical Society 出版日期： 2015-04-30 出處： Physical review letters, 2015-04, Vol.114 (17), p.171103-171103, Article 171103 資源來源： American Physical Society Journals 版權： licence_http://creativecommons.org/publicdomain/zero 識別號： ISSN: 0031-9007 識別號： ISSN: 1092-0145 識別號： ISSN: 1079-7114 識別號： EISSN: 1079-7114 識別號： DOI: 10.1103/PhysRevLett.114.171103 識別號： PMID: 25978222
Appears in Collections:	[Department of Physics] journal & Dissertation

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