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@ARTICLE{Aguilar:902577,
      author       = {Aguilar, M. and Cavasonza, L. Ali and Alpat, B. and
                      Ambrosi, G. and Arruda, L. and Attig, N. and Barao, F. and
                      Barrin, L. and Bartoloni, A. and Başeğmez-du Pree, S. and
                      Battiston, R. and Behlmann, M. and Beranek, B. and Berdugo,
                      J. and Bertucci, B. and Bindi, V. 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, G. R. 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
                      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 Gámez, C. and García-López, R. J. and
                      Gargiulo, C. and Gast, H. 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 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 Incagli, M. and Jang,
                      W. Y. and Jia, Yi and Jinchi, H. and Khiali, B. and Kim, G.
                      N. and Kirn, Th. and Konyushikhin, M. and Kounina, O. and
                      Kounine, A. and Koutsenko, V. and Krasnopevtsev, D. 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 Li, J. Q. and Li, M. and Li, Q. and
                      Li, S. and Li, J. H. and Li, Z. H. and Liang, J. and Light,
                      C. and Lin, C. H. and Lippert, T. and Liu, J. H. and Liu, Z.
                      and Lu, S. Q. and Lu, Y. S. and Luebelsmeyer, K. and Luo, J.
                      Z. and Luo, Xi 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 Medvedeva, T. and Menchaca-Rocha, A.
                      and Meng, Q. and Mikhailov, V. V. and Molero, M. and Mott,
                      P. and Mussolin, L. and Negrete, J. 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 Poluianov, S. and Qin, X. and Qu, Z. Y.
                      and Quadrani, L. and Rancoita, P. G. and Rapin, D. and
                      Conde, A. Reina and Robyn, E. and Rosier-Lees, S. and
                      Rozhkov, A. and Rozza, D. and Sagdeev, R. and Schael, S. and
                      von Dratzig, A. Schulz and Schwering, G. and Seo, E. S. and
                      Shakfa, Z. and Shan, B. S. and Siedenburg, T. and Solano, C.
                      and Song, J. W. and Song, X. J. and Sonnabend, R. and
                      Strigari, L. and Su, T. 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 Valencia-Otero, M. and
                      Valente, E. and Valtonen, E. and Vázquez Acosta, M. and
                      Vecchi, M. and Velasco, M. and Vialle, J. P. and Wang, C. X.
                      and Wang, L. and Wang, L. Q. and Wang, N. H. and Wang, Q. L.
                      and Wang, S. and Wang, X. and Wang, Yu and Wang, Z. M. and
                      Wei, J. and Weng, Z. L. and Wu, H. and Xiong, R. Q. and Xu,
                      W. and Yan, Q. and Yang, Y. and Yashin, I. I. and Yi, H. and
                      Yu, Y. M. 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, C. and Zheng, Z. M. and Zhuang, H.
                      L. and Zhukov, V. and Zichichi, A. and Zuccon, P.},
      title        = {{P}roperties of a {N}ew {G}roup of {C}osmic {N}uclei:
                      {R}esults from the {A}lpha {M}agnetic {S}pectrometer on
                      {S}odium, {A}luminum, and {N}itrogen},
      journal      = {Physical review letters},
      volume       = {127},
      number       = {2},
      issn         = {0031-9007},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {FZJ-2021-04376},
      pages        = {021101},
      year         = {2021},
      abstract     = {We report the properties of sodium (Na) and aluminum (Al)
                      cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on
                      0.46 million sodium and 0.51 million aluminum nuclei
                      collected by the Alpha Magnetic Spectrometer experiment on
                      the International Space Station. We found that Na and Al,
                      together with nitrogen (N), belong to a distinct cosmic ray
                      group. In this group, we observe that, similar to the N
                      flux, both the Na flux and Al flux are well described by the
                      sums of a primary cosmic ray component (proportional to the
                      silicon flux) and a secondary cosmic ray component
                      (proportional to the fluorine flux). The fraction of the
                      primary component increases with rigidity for the N, Na, and
                      Al fluxes and becomes dominant at the highest rigidities.
                      The Na/Si and Al/Si abundance ratios at the source,
                      0.036±0.003 for Na/Si and 0.103±0.004 for Al/Si, are
                      determined independent of cosmic ray propagation.},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {5121 - Supercomputing $\&$ Big Data Facilities (POF4-512)},
      pid          = {G:(DE-HGF)POF4-5121},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {34296911},
      UT           = {WOS:000671590200003},
      doi          = {10.1103/PhysRevLett.127.021101},
      url          = {https://juser.fz-juelich.de/record/902577},
}