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Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station

Knowledge of the rigidity dependence of the boron to carbon flux ratio (B/C) is important in understanding the propagation of cosmic rays. The precise measurement of the B/C ratio from 1.9 GV to 2.6 TV, based on 2.3 million boron and 8.3 million carbon nuclei collected by AMS during the first 5 year...

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Detalles Bibliográficos
Autores principales: Aguilar, M, Ali Cavasonza, L, Alpat, B, Ambrosi, G, Arruda, L, Attig, N, Aupetit, S, Azzarello, P, Bachlechner, A, Barao, F, Barrau, A, Barrin, L, Bartoloni, A, Basara, L, Başeǧmez-du Pree, S, Battarbee, M, Battiston, R, Bazo, J, Becker, U, Behlmann, M, Beischer, B, Berdugo, J, Bertucci, B, Bindi, V, Boella, G, de Boer, W, Bollweg, K, Bonnivard, V, Borgia, B, Boschini, M  J, Bourquin, M, Bueno, E  F, Burger, J, Cadoux, F, Cai, X  D, Capell, M, Caroff, S, Casaus, J, Castellini, G, Cernuda, I, Cervelli, F, Chae, M  J, Chang, Y  H, Chen, A  I, Chen, G  M, Chen, H  S, Cheng, L, Chou, H  Y, Choumilov, E, Choutko, V, Chung, C  H, Clark, C, Clavero, R, Coignet, G, Consolandi, C, Contin, A, Corti, C, Coste, B, Creus, W, Crispoltoni, M, Cui, Z, Dai, Y  M, Delgado, C, Della Torre, S, Demirköz, M  B, Derome, L, Di Falco, S, Dimiccoli, F, Díaz, C, von Doetinchem, P, Dong, F, Donnini, F, Duranti, M, D'Urso, D, Egorov, A, Eline, A, Eronen, T, Feng, J, Fiandrini, E, Finch, E, Fisher, P, Formato, V, Galaktionov, Y, Gallucci, G, García, B, García-López, R  J, Gargiulo, C, Gast, H, Gebauer, I, Gervasi, M, Ghelfi, A, Giovacchini, F, Goglov, P, Gómez-Coral, D  M, Gong, J, Goy, C, Grabski, V, Grandi, D, Graziani, M, Guerri, I, Guo, K  H, Habiby, M, Haino, S, Han, K  C, He, Z  H, Heil, M, Hoffman, J, Hsieh, T  H, Huang, H, Huang, Z  C, Huh, C, Incagli, M, Ionica, M, Jang, W  Y, Jinchi, H, Kang, S  C, Kanishev, K, Kim, G  N, Kim, K  S, Kirn, Th, Konak, C, Kounina, O, Kounine, A, Koutsenko, V, Krafczyk, M  S, La Vacca, G, Laudi, E, Laurenti, G, Lazzizzera, I, Lebedev, A, Lee, H  T, Lee, S  C, Leluc, C, Li, H  S, Li, J  Q, Li, Q, Li, T  X, Li, W, Li, Z  H, Li, Z  Y, Lim, S, Lin, C  H, Lipari, P, Lippert, T, Liu, D, Liu, Hu, Lu, S  Q, Lu, Y  S, Luebelsmeyer, K, Luo, F, Luo, J  Z, Lv, S  S, Majka, R, Mañá, C, Marín, J, Martin, T, Martínez, G, Masi, N, Maurin, D, Menchaca-Rocha, A, Meng, Q, Mo, D  C, Morescalchi, L, Mott, P, Nelson, T, Ni, J  Q, Nikonov, N, Nozzoli, F, Nunes, P, Oliva, A, Orcinha, M, Palmonari, F, Palomares, C, Paniccia, M, Pauluzzi, M, Pensotti, S, Pereira, R, Picot-Clemente, N, Pilo, F, Pizzolotto, C, Plyaskin, V, Pohl, M, Poireau, V, Putze, A, Quadrani, L, Qi, X  M, Qin, X, Qu, Z  Y, Räihä, T, Rancoita, P  G, Rapin, D, Ricol, J  S, Rodríguez, I, Rosier-Lees, S, Rozhkov, A, Rozza, D, Sagdeev, R, Sandweiss, J, Saouter, P, Schael, S, Schmidt, S  M, Schulz von Dratzig, A, Schwering, G, Seo, E  S, Shan, B  S, Shi, J  Y, Siedenburg, T, Son, D, Song, J  W, Sun, W  H, Tacconi, M, Tang, X  W, Tang, Z  C, Tao, L, Tescaro, D, Ting, Samuel C  C, Ting, S  M, Tomassetti, N, Torsti, J, Türkoğlu, C, Urban, T, Vagelli, V, Valente, E, Vannini, C, Valtonen, E, Vázquez Acosta, M, Vecchi, M, Velasco, M, Vialle, J  P, Vitale, V, Vitillo, S, Wang, L  Q, Wang, N  H, Wang, Q  L, Wang, X, Wang, X  Q, Wang, Z  X, Wei, C  C, Weng, Z  L, Whitman, K, Wienkenhöver, J, Willenbrock, M, Wu, H, Wu, X, Xia, X, Xiong, R  Q, Xu, W, Yan, Q, Yang, J, Yang, M, Yang, Y, Yi, H, Yu, Y  J, Yu, Z  Q, Zeissler, S, Zhang, C, Zhang, J, Zhang, J  H, Zhang, S  D, Zhang, S  W, Zhang, Z, Zheng, Z  M, Zhu, Z  Q, Zhuang, H  L, Zhukov, V, Zichichi, A, Zimmermann, N, Zuccon, P
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevLett.117.231102
http://cds.cern.ch/record/2261135