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@ARTICLE{Aguilar:1037648,
      author       = {Aguilar, M. and Ali Cavasonza, L. and Alpat, B. and
                      Ambrosi, G. and Arruda, L. and Attig, N. and Bagwell, C. and
                      Barao, F. and Barrin, L. and Bartoloni, A. and Başeğmez-du
                      Pree, S. and Battiston, R. and Belyaev, N. and Berdugo, J.
                      and Bertucci, B. and Bindi, V. and Bollweg, K. and Bolster,
                      J. and Borchiellini, M. and Borgia, B. and Boschini, M. J.
                      and Bourquin, M. and Bueno, E. F. and Burger, J. and Burger,
                      W. J. 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. 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 Dass, A. 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 Faldi, F. and Feng, J. and
                      Fiandrini, E. and Fisher, P. and Formato, V. 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 Guracho, A. N. 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, B. W. and Incagli, M. and
                      Jang, W. Y. and Jia, Yi and Jinchi, H. and Karagöz, G. and
                      Khiali, B. and Kim, G. N. and Kirn, Th. 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 LaVecchia, G. and Lazzizzera, I. and
                      Lee, H. T. and Lee, S. C. and Li, H. L. and Li, J. Q. and
                      Li, M. and Li, M. and Li, Q. and Li, Q. and Li, Q. Y. and
                      Li, S. and Li, S. L. and Li, J. H. and Li, Z. H. and Liang,
                      J. and Liang, M. J. and Lin, C. H. and Lippert, T. and Liu,
                      J. H. and Lu, S. Q. and Lu, Y. S. and Luebelsmeyer, K. and
                      Luo, J. Z. and Luo, S. D. 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 Ocampo-Peleteiro, J. and
                      Oliva, A. and Orcinha, M. and Ottupara, M. A. and Palermo,
                      M. and Palmonari, F. and Paniccia, M. and Pashnin, A. and
                      Pauluzzi, M. and Pensotti, S. and Plyaskin, V. and
                      Poluianov, S. and Qin, X. and Qu, Z. Y. and Quadrani, L. and
                      Rancoita, P. G. and Rapin, D. and Reina Conde, A. and Robyn,
                      E. and Romaneehsen, L. and Rozhkov, A. and Rozza, D. and
                      Sagdeev, R. and Schael, S. and Schultz von Dratzig, A. and
                      Schwering, G. and Seo, E. S. and Shan, B. S. and Siedenburg,
                      T. 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
                      Tian, Y. and Ting, Samuel C. C. and Ting, S. M. and
                      Tomassetti, N. and Torsti, J. 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 Wu, Y. and Xiao, J.
                      N. and Xiong, R. Q. and Xiong, X. Z. and Xu, W. and Yan, Q.
                      and Yang, H. T. and Yang, Y. and Yashin, I. I. and Yelland,
                      A. and Yi, H. and You, Y. 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. 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 {C}osmic-{R}ay {S}ulfur and {D}etermination
                      of the {C}omposition of {P}rimary {C}osmic-{R}ay {C}arbon,
                      {N}eon, {M}agnesium, and {S}ulfur: {T}en-{Y}ear {R}esults
                      from the {A}lpha {M}agnetic {S}pectrometer},
      journal      = {Physical review letters},
      volume       = {130},
      number       = {21},
      issn         = {0031-9007},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {FZJ-2025-00813},
      pages        = {211002},
      year         = {2023},
      abstract     = {We report the properties of primary cosmic-ray sulfur (S)
                      in the rigidity range 2.15 GV to 3.0 TV based on 0.38×106
                      sulfur nuclei collected by the Alpha Magnetic Spectrometer
                      experiment (AMS). We observed that above 90 GV the rigidity
                      dependence of the S flux is identical to the rigidity
                      dependence of Ne-Mg-Si fluxes, which is different from the
                      rigidity dependence of the He-C-O-Fe fluxes. We found that,
                      similar to N, Na, and Al cosmic rays, over the entire
                      rigidity range, the traditional primary cosmic rays S, Ne,
                      Mg, and C all have sizeable secondary components, and the S,
                      Ne, and Mg fluxes are well described by the weighted sum of
                      the primary silicon flux and the secondary fluorine flux,
                      and the C flux is well described by the weighted sum of the
                      primary oxygen flux and the secondary boron flux. The
                      primary and secondary contributions of the traditional
                      primary cosmic-ray fluxes of C, Ne, Mg, and S (even 𝑍
                      elements) are distinctly different from the primary and
                      secondary contributions of the N, Na, and Al (odd 𝑍
                      elements) fluxes. The abundance ratio at the source for S/Si
                      is 0.167±0.006, for Ne/Si is 0.833±0.025, for Mg/Si is
                      0.994 ±0.029, and for C/O is 0.836 ±0.025. These values
                      are determined independent of cosmic-ray propagation.},
      cin          = {JSC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)JSC-20090406},
      pnm          = {5111 - Domain-Specific Simulation $\&$ Data Life Cycle Labs
                      (SDLs) and Research Groups (POF4-511) / 5112 - Cross-Domain
                      Algorithms, Tools, Methods Labs (ATMLs) and Research Groups
                      (POF4-511) / 5121 - Supercomputing $\&$ Big Data Facilities
                      (POF4-512) / 5122 - Future Computing $\&$ Big Data Systems
                      (POF4-512)},
      pid          = {G:(DE-HGF)POF4-5111 / G:(DE-HGF)POF4-5112 /
                      G:(DE-HGF)POF4-5121 / G:(DE-HGF)POF4-5122},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {37295095},
      UT           = {WOS:001025975200016},
      doi          = {10.1103/PhysRevLett.130.211002},
      url          = {https://juser.fz-juelich.de/record/1037648},
}