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@ARTICLE{Aguilar:877692,
author = {Aguilar, M. and Ali Cavasonza, L. 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 Becker, U. and Behlmann, M. and Beischer, B. and
Berdugo, J. and Bertucci, B. and Bindi, V. and de Boer, W.
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, 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 Dai, Y. M. 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 Gebauer, I. 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
Guo, K. H. 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, Z. C. 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, T. X.
and Li, Z. H. and Light, C. and Lin, C. H. and Lippert, T.
and Liu, Z. and Lu, S. Q. and Lu, Y. S. and Luebelsmeyer, K.
and Luo, J. Z. 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 Mo, D. C. and Molero, M.
and Mott, P. and Mussolin, L. and Ni, J. Q. 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 Qi, X. M. and Qin,
X. and Qu, Z. Y. and Quadrani, L. and Rancoita, P. G. and
Rapin, D. and Reina Conde, A. and Rosier-Lees, S. and
Rozhkov, A. and Rozza, D. and Sagdeev, R. and Schael, S. and
Schmidt, S. M. and Schulz von Dratzig, A. and Schwering, G.
and Seo, E. S. and Shan, B. S. and Shi, J. Y. and
Siedenburg, T. and Solano, C. and Sonnabend, R. and Song, J.
W. 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 Valente, E. and Valtonen, E. and Vázquez Acosta, M.
and Vecchi, M. and Velasco, M. and Vialle, J. P. and
Wallmann, C. and Wang, L. Q. and Wang, N. H. and Wang, Q. L.
and Wang, S. and Wang, X. and Wang, Z. X. and Wei, J. and
Weng, Z. L. and Wu, H. and Xiong, R. Q. and Xu, W. and Yan,
Q. and Yang, Y. and Yi, H. and Yu, Y. J. 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, Z. M. and
Zhuang, H. L. and Zhukov, V. and Zichichi, A. and
Zimmermann, N. and Zuccon, P.},
title = {{P}roperties of {N}eon, {M}agnesium, and {S}ilicon
{P}rimary {C}osmic {R}ays {R}esults from the {A}lpha
{M}agnetic {S}pectrometer},
journal = {Physical review letters},
volume = {124},
number = {21},
issn = {1079-7114},
address = {College Park, Md.},
publisher = {APS},
reportid = {FZJ-2020-02402},
pages = {211102},
year = {2020},
abstract = {We report the observation of new properties of primary
cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si),
measured in the rigidity range 2.15 GV to 3.0 TV with
1.8×106 Ne, 2.2×106 Mg, and 1.6×106 Si
nuclei collected by the Alpha Magnetic Spectrometer
experiment on the International Space Station. The Ne and Mg
spectra have identical rigidity dependence above 3.65 GV.
The three spectra have identical rigidity dependence above
86.5 GV, deviate from a single power law above 200 GV, and
harden in an identical way. Unexpectedly, above 86.5 GV the
rigidity dependence of primary cosmic rays Ne, Mg, and Si
spectra is different from the rigidity dependence of primary
cosmic rays He, C, and O. This shows that the Ne, Mg, and Si
and He, C, and O are two different classes of primary cosmic
rays.},
cin = {JSC / JARA-HPC},
ddc = {530},
cid = {I:(DE-Juel1)JSC-20090406 / $I:(DE-82)080012_20140620$},
pnm = {513 - Supercomputer Facility (POF3-513) / Cosmic-ray
physics with the AMS experiment on the International Space
Station $(jara0052_20150501)$},
pid = {G:(DE-HGF)POF3-513 / $G:(DE-Juel1)jara0052_20150501$},
typ = {PUB:(DE-HGF)16},
pubmed = {pmid:32530660},
UT = {WOS:000536404500001},
doi = {10.1103/PhysRevLett.124.211102},
url = {https://juser.fz-juelich.de/record/877692},
}
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