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@ARTICLE{Aguilar:851761,
author = {Aguilar, M. and Ali Cavasonza, L. and Alpat, B. and
Ambrosi, G. and Arruda, L. and Attig, N. and Aupetit, S. and
Azzarello, P. and Bachlechner, A. and Barao, F. and Barrau,
A. and Barrin, L. and Bartoloni, A. and Basara, L. and
Başeğmez-du Pree, S. and Battarbee, M. and Battiston, R.
and Becker, U. and Behlmann, M. and Beischer, B. and
Berdugo, J. and Bertucci, B. and Bindel, K. F. and Bindi, V.
and de Boer, W. and Bollweg, K. and Bonnivard, V. 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 Caroff, S. and Casaus, J. and Castellini, G.
and Cervelli, F. and Chang, Y. H. and Chen, A. I. and Chen,
G. M. and Chen, H. S. and Chen, Y. and Cheng, L. and Chou,
H. Y. and Choumilov, E. and Choutko, V. and Chung, C. H. and
Clark, C. and Clavero, R. and Coignet, G. and Consolandi, C.
and Contin, A. and Corti, C. and Creus, W. and Crispoltoni,
M. and Cui, Z. and Dadzie, K. and Dai, Y. M. and Datta, A.
and Delgado, C. and Della Torre, S. and Demirköz, M. B. and
Derome, L. and Di Falco, S. and Dimiccoli, F. and Díaz, C.
and von Doetinchem, P. and Dong, F. and Donnini, F. and
Duranti, M. and Egorov, A. and Eline, A. and Eronen, T. and
Feng, J. and Fiandrini, E. and Fisher, P. and Formato, V.
and Galaktionov, Y. and Gallucci, G. and García-López, R.
J. and Gargiulo, C. and Gast, H. and Gebauer, I. and
Gervasi, M. and Ghelfi, A. 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 He, Z. H. and Heil, M. and Hsieh, T. H.
and Huang, H. and Huang, Z. C. and Incagli, M. and Jia, Yi
and Jinchi, H. and Kanishev, K. and Khiali, B. and Kirn, Th.
and Konak, C. and Kounina, O. and Kounine, A. and Koutsenko,
V. 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 Leluc, C. and Li, H. S. and Li, J. Q.
and Li, Q. and Li, T. X. and Li, Z. H. and Li, Z. Y. and
Lin, C. H. and Lipari, P. and Lippert, T. and Liu, D. and
Liu, Hu and Liu, Z. and Lordello, V. D. and Lu, S. Q. and
Lu, Y. S. and Luebelsmeyer, K. and Luo, F. and Luo, J. Z.
and Lyu, S. S. and Machate, F. and Mañá, C. and Marín, J.
and Martin, T. and Martínez, G. and Masi, N. and Maurin, D.
and Menchaca-Rocha, A. and Meng, Q. and Mikuni, V. M. and
Mo, D. C. and Mott, P. and Mussolin, L. and Nelson, T. and
Ni, J. Q. and Nikonov, N. and Nozzoli, F. and Oliva, A. and
Orcinha, M. and Palermo, M. and Palmonari, F. and Palomares,
C. and Paniccia, M. and Pauluzzi, M. and Pensotti, S. and
Perrina, C. and Phan, H. D. and Picot-Clemente, N. and Pilo,
F. and Plyaskin, V. and Pohl, M. and Poireau, V. and
Quadrani, L. and Qi, X. M. and Qin, X. and Qu, Z. Y. and
Räihä, T. and Rancoita, P. G. and Rapin, D. and Ricol, J.
S. 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 Song, J. W. and
Tacconi, M. and Tang, X. W. and Tang, Z. C. and Tescaro, D.
and Tian, J. and Ting, Samuel C. C. and Ting, S. M. and
Tomassetti, N. and Torsti, J. and Urban, T. and Vagelli, V.
and Valente, E. and Valtonen, E. and Vázquez Acosta, M. and
Vecchi, M. and Velasco, M. and Vialle, J. P. and Wang, L. Q.
and Wang, N. H. and Wang, Q. L. and Wang, X. and Wang, X. Q.
and Wang, Z. X. and Wei, C. C. and Wei, J. and Weng, Z. L.
and Whitman, K. and Wu, H. and Xiong, R. Q. and Xu, W. and
Yan, Q. and Yang, M. and Yang, Y. and Yi, H. and Yu, Y. J.
and Yu, Z. Q. and Zannoni, M. and Zeissler, S. and Zhang, C.
and Zhang, F. and Zhang, J. and Zhang, J. H. and Zhang, S.
W. and Zhang, Z. and Zheng, Z. M. and Zhuang, H. L. and
Zhukov, V. and Zichichi, A. and Zimmermann, N. and Zuccon,
P.},
title = {{P}recision {M}easurement of {C}osmic-{R}ay {N}itrogen and
its {P}rimary and {S}econdary {C}omponents with the {A}lpha
{M}agnetic {S}pectrometer on the {I}nternational {S}pace
{S}tation},
journal = {Physical review letters},
volume = {121},
number = {5},
issn = {1079-7114},
address = {College Park, Md.},
publisher = {APS},
reportid = {FZJ-2018-05285},
pages = {051103},
year = {2018},
abstract = {A precision measurement of the nitrogen flux with rigidity
(momentum per unit charge) from 2.2 GV to 3.3 TV based on
2.2×106 events is presented. The detailed rigidity
dependence of the nitrogen flux spectral index is presented
for the first time. The spectral index rapidly hardens at
high rigidities and becomes identical to the spectral
indices of primary He, C, and O cosmic rays above
∼700 GV. We observed that the nitrogen flux ΦN can
be presented as the sum of its primary component ΦPN and
secondary component ΦSN, ΦN=ΦPN+ΦSN, and we found ΦN is
well described by the weighted sum of the oxygen flux ΦO
(primary cosmic rays) and the boron flux ΦB (secondary
cosmic rays), with ΦPN=(0.090±0.002)×ΦO and
ΦSN=(0.62±0.02)×ΦB over the entire rigidity range. This
corresponds to a change of the contribution of the secondary
cosmic ray component in the nitrogen flux from $70\%$ at a
few GV to $<30\%$ above 1 TV.},
cin = {JSC / VS-I / JARA-FAME / JARA-HPC},
ddc = {550},
cid = {I:(DE-Juel1)JSC-20090406 / I:(DE-Juel1)VS-I-20090406 /
$I:(DE-82)080023_20140620$ / $I:(DE-82)080012_20140620$},
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:30118280},
UT = {WOS:000440386100003},
doi = {10.1103/PhysRevLett.121.051103},
url = {https://juser.fz-juelich.de/record/851761},
}
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