% IMPORTANT: The following is UTF-8 encoded. This means that in the presence % of non-ASCII characters, it will not work with BibTeX 0.99 or older. % Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or % “biber”. @ARTICLE{Aguilar:906806, author = {Aguilar, M. and Cavasonza, L. Ali 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 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 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 Karagöz, G. 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. Schultz 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 Urban, T. and Usoskin, I. and Vainio, R. and Vagelli, V. 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}eriodicities in the {D}aily {P}roton {F}luxes from 2011 to 2019 {M}easured by the {A}lpha {M}agnetic {S}pectrometer on the {I}nternational {S}pace {S}tation from 1 to 100 {GV}}, journal = {Physical review letters}, volume = {127}, number = {27}, issn = {0031-9007}, address = {College Park, Md.}, publisher = {APS}, reportid = {FZJ-2022-01704}, pages = {271102}, year = {2021}, abstract = {We present the precision measurement of the daily proton fluxes in cosmic rays from May 20, 2011 to October 29, 2019 (a total of 2824 days or 114 Bartels rotations) in the rigidity interval from 1 to 100 GV based on 5.5×109 protons collected with the Alpha Magnetic Spectrometer aboard the International Space Station. The proton fluxes exhibit variations on multiple timescales. From 2014 to 2018, we observed recurrent flux variations with a period of 27 days. Shorter periods of 9 days and 13.5 days are observed in 2016. The strength of all three periodicities changes with time and rigidity. The rigidity dependence of the 27-day periodicity is different from the rigidity dependences of 9-day and 13.5-day periods. Unexpectedly, the strength of 9-day and 13.5-day periodicities increases with increasing rigidities up to ~10 GV and ~20 GV, respectively. Then the strength of the periodicities decreases with increasing rigidity up to 100 GV.}, 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 = {35061443}, UT = {WOS:000754466000004}, doi = {10.1103/PhysRevLett.127.271102}, url = {https://juser.fz-juelich.de/record/906806}, }