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@ARTICLE{Aguilar:888870,
      author       = {Aguilar, M. and Ali Cavasonza, L. and Ambrosi, G. and
                      Arruda, L. and Attig, N. and Barao, F. and Barrin, L. and
                      Bartoloni, A. and Başeğmez-du Pree, S. and Bates, J. and
                      Battiston, R. and Behlmann, M. and Beischer, B. and Berdugo,
                      J. and Bertucci, B. and Bindi, V. and de Boer, W. and
                      Bollweg, K. and Borgia, B. and Boschini, M. J. and Bourquin,
                      M. and Bueno, E. F. and Burger, J. and Burger, W. J. and
                      Burmeister, S. and Cai, X. D. and Capell, M. and Casaus, J.
                      and Castellini, G. and Cervelli, F. and Chang, Y. H. and
                      Chen, G. M. and Chen, H. S. and Chen, Y. and Cheng, L. and
                      Chou, H. Y. and Chouridou, S. and Choutko, V. and Chung, C.
                      H. and Clark, C. and Coignet, G. and Consolandi, C. and
                      Contin, A. and Corti, C. and Cui, Z. and Dadzie, K. and Dai,
                      Y. M. and Delgado, C. and Della Torre, S. and Demirköz, M.
                      B. and Derome, L. and Di Falco, S. and Di Felice, V. and
                      Díaz, C. and Dimiccoli, F. and von Doetinchem, P. and Dong,
                      F. and Donnini, F. and Duranti, M. and Egorov, A. and Eline,
                      A. and Feng, J. and Fiandrini, E. and Fisher, P. and
                      Formato, V. and Freeman, C. and Galaktionov, Y. and Gámez,
                      C. and García-López, R. J. and Gargiulo, C. and Gast, H.
                      and Gebauer, I. and Gervasi, M. and Giovacchini, F. and
                      Gómez-Coral, D. M. and Gong, J. and Goy, C. and Grabski, V.
                      and Grandi, D. and Graziani, M. and Guo, K. H. and Haino, S.
                      and Han, K. C. and Hashmani, R. K. and He, Z. H. and Heber,
                      B. and Hsieh, T. H. and Hu, J. Y. and Huang, Z. C. and
                      Hungerford, W. and Incagli, M. and Jang, W. Y. and Jia, Yi
                      and Jinchi, H. and Kanishev, K. and Khiali, B. and Kim, G.
                      N. and Kirn, Th. and Konyushikhin, M. and Kounina, O. and
                      Kounine, A. and Koutsenko, V. and Kuhlman, A. and Kulemzin,
                      A. and La Vacca, G. and Laudi, E. and Laurenti, G. and
                      Lazzizzera, I. and Lebedev, A. and Lee, H. T. and Lee, S. C.
                      and Leluc, C. and Li, J. Q. and Li, M. and Li, Q. and Li, S.
                      and Li, T. X. and Li, Z. H. and Light, C. and Lin, C. H. and
                      Lippert, T. and Liu, Z. and Lu, S. Q. and Lu, Y. S. and
                      Luebelsmeyer, K. and Luo, J. Z. and Lyu, S. S. and Machate,
                      F. and Mañá, C. and Marín, J. and Marquardt, J. and
                      Martin, T. and Martínez, G. and Masi, N. and Maurin, D. and
                      Menchaca-Rocha, A. and Meng, Q. and Mo, D. C. and Molero, M.
                      and Mott, P. and Mussolin, L. and Ni, J. Q. and Nikonov, N.
                      and Nozzoli, F. and Oliva, A. and Orcinha, M. and Palermo,
                      M. and Palmonari, F. and Paniccia, M. and Pashnin, A. and
                      Pauluzzi, M. and Pensotti, S. and Phan, H. D. and Plyaskin,
                      V. and Pohl, M. and Porter, S. and Qi, X. M. and Qin, X. and
                      Qu, Z. Y. and Quadrani, L. and Rancoita, P. G. and Rapin, D.
                      and Reina Conde, A. and Rosier-Lees, S. and Rozhkov, A. and
                      Rozza, D. and Sagdeev, R. and Schael, S. and Schmidt, S. M.
                      and Schulz von Dratzig, A. and Schwering, G. and Seo, E. S.
                      and Shan, B. S. and Shi, J. Y. and Siedenburg, T. and
                      Solano, C. and Song, J. W. and Sonnabend, R. and Sun, Q. and
                      Sun, Z. T. and Tacconi, M. and Tang, X. W. and Tang, Z. C.
                      and Tian, J. and Ting, Samuel C. C. and Ting, S. M. and
                      Tomassetti, N. and Torsti, J. and Tüysüz, C. and Urban, T.
                      and Usoskin, I. and Vagelli, V. and Vainio, R. and Valente,
                      E. and Valtonen, E. and Vázquez Acosta, M. and Vecchi, M.
                      and Velasco, M. and Vialle, J. P. and Wang, L. Q. and Wang,
                      N. H. and Wang, Q. L. and Wang, S. and Wang, X. and Wang, Z.
                      X. and Wei, J. and Weng, Z. L. and Wu, H. and Xiong, R. Q.
                      and Xu, W. and Yan, Q. and Yang, Y. and Yi, H. and Yu, Y. J.
                      and Yu, Z. Q. and Zannoni, M. and Zhang, C. and Zhang, F.
                      and Zhang, F. Z. and Zhang, J. H. and Zhang, Z. and Zhao, F.
                      and Zheng, Z. M. and Zhuang, H. L. and Zhukov, V. and
                      Zichichi, A. and Zimmermann, N. and Zuccon, P.},
      title        = {{T}he {A}lpha {M}agnetic {S}pectrometer ({AMS}) on the
                      international space station: {P}art {II} — {R}esults from
                      the first seven years},
      journal      = {Physics reports},
      volume       = {894},
      issn         = {0370-1573},
      address      = {Amsterdam [u.a.]},
      publisher    = {Elsevier Science, North-Holland},
      reportid     = {FZJ-2020-05280},
      pages        = {1-116},
      year         = {2021},
      abstract     = {The Alpha Magnetic Spectrometer (AMS) is a precision
                      particle physics detector on the International Space Station
                      (ISS) conducting a unique, long-duration mission of
                      fundamental physics research in space. The physics
                      objectives include the precise studies of the origin of dark
                      matter, antimatter, and cosmic rays as well as the
                      exploration of new phenomena. Following a 16-year period of
                      construction and testing, and a precursor flight on the
                      Space Shuttle, AMS was installed on the ISS on May 19, 2011.
                      In this report we present results based on 120 billion
                      charged cosmic ray events up to multi-TeV energies. This
                      includes the fluxes of positrons, electrons, antiprotons,
                      protons, and nuclei. These results provide unexpected
                      information, which cannot be explained by the current
                      theoretical models. The accuracy and characteristics of the
                      data, simultaneously from many different types of cosmic
                      rays, provide unique input to the understanding of origins,
                      acceleration, and propagation of cosmic rays.},
      cin          = {JSC / JARA-HPC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406 / $I:(DE-82)080012_20140620$},
      pnm          = {5121 - Supercomputing $\&$ Big Data Facilities (POF4-512) /
                      Cosmic-ray physics with the AMS experiment on the
                      International Space Station $(jara0052_20200501)$},
      pid          = {G:(DE-HGF)POF4-5121 / $G:(DE-Juel1)jara0052_20200501$},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000608963000001},
      doi          = {10.1016/j.physrep.2020.09.003},
      url          = {https://juser.fz-juelich.de/record/888870},
}