% 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},
}