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@ARTICLE{Aguilar:1008545,
      author       = {Aguilar, M. and Cavasonza, L. Ali 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 Behlmann, M. and Belyaev, N. and Berdugo,
                      J. and Bertucci, B. and Bindi, V. and Bollweg, K. and
                      Bolster, J. 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 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 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 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 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, 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
                      Light, C. 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, 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 Palermo, M. and Palmonari, F. and Paniccia,
                      M. and Pashnin, A. and Pauluzzi, M. and Pensotti, S. 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. Schultz 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 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 Xiong, R. Q. and Xu,
                      W. and Yan, Q. and Yang, Y. and Yashin, I. I. and Yelland,
                      A. 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        = {{T}emporal {S}tructures in {E}lectron {S}pectra and
                      {C}harge {S}ign {E}ffects in {G}alactic {C}osmic {R}ays},
      journal      = {Physical review letters},
      volume       = {130},
      number       = {16},
      issn         = {0031-9007},
      address      = {College Park, Md.},
      publisher    = {APS},
      reportid     = {FZJ-2023-02382},
      pages        = {161001},
      year         = {2023},
      abstract     = {We present the precision measurements of 11 years of daily
                      cosmic electron fluxes in the rigidity interval from 1.00 to
                      41.9 GV based on 2.0×108 electrons collected with the Alpha
                      Magnetic Spectrometer (AMS) aboard the International Space
                      Station. The electron fluxes exhibit variations on multiple
                      timescales. Recurrent electron flux variations with periods
                      of 27 days, 13.5 days, and 9 days are observed. We find that
                      the electron fluxes show distinctly different time
                      variations from the proton fluxes. Remarkably, a hysteresis
                      between the electron flux and the proton flux is observed
                      with a significance of greater than 6σ at rigidities below
                      8.5 GV. Furthermore, significant structures in the
                      electron-proton hysteresis are observed corresponding to
                      sharp structures in both fluxes. This continuous daily
                      electron data provide unique input to the understanding of
                      the charge sign dependence of cosmic rays over an 11-year
                      solar cycle.},
      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       = {37154630},
      UT           = {WOS:000992482700001},
      doi          = {10.1103/PhysRevLett.130.161001},
      url          = {https://juser.fz-juelich.de/record/1008545},
}