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@ARTICLE{Aguilar:891401,
      author       = {Aguilar, M. and Cavasonza, L. Ali and Allen, M. S. 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
                      Galaktionov, Y. 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 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 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 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 Mikhailov, V. V. and Mo,
                      D. C. 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 Piandani, R. and Plyaskin, V. 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 Schulz von Dratzig, A. 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 {H}eavy {S}econdary {F}luorine {C}osmic
                      {R}ays: {R}esults from the {A}lpha {M}agnetic
                      {S}pectrometer},
      journal      = {Physical review letters},
      volume       = {126},
      number       = {8},
      issn         = {1079-7114},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {FZJ-2021-01489},
      pages        = {081102},
      year         = {2021},
      abstract     = {Precise knowledge of the charge and rigidity dependence of
                      the secondary cosmic ray fluxes and the secondary-to-primary
                      flux ratios is essential in the understanding of cosmic ray
                      propagation. We report the properties of heavy secondary
                      cosmic ray fluorine F in the rigidity R range 2.15 GV to 2.9
                      TV based on 0.29 million events collected by the Alpha
                      Magnetic Spectrometer experiment on the International Space
                      Station. The fluorine spectrum deviates from a single power
                      law above 200 GV. The heavier secondary-to-primary F/Si flux
                      ratio rigidity dependence is distinctly different from the
                      lighter B/O (or B/C) rigidity dependence. In particular,
                      above 10 GV, the F/SiB/O ratio can be described by a power
                      law Rδ with δ=0.052±0.007. This shows that the
                      propagation properties of heavy cosmic rays, from F to Si,
                      are different from those of light cosmic rays, from He to O,
                      and that the secondary cosmic rays have two classes.},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {512 - Supercomputing $\&$ Big Data Infrastructures
                      (POF4-512)},
      pid          = {G:(DE-HGF)POF4-512},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {33709764},
      UT           = {WOS:000621595400002},
      doi          = {10.1103/PhysRevLett.126.081102},
      url          = {https://juser.fz-juelich.de/record/891401},
}