Accès ouvert déclaré
2025
article
Solar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer
M. Aguilar, B. Alpat, G. Ambrosi, H. R. Anderson, L. Arruda, N. Attig, C. Bagwell, F. Barão, M. Barbanera, L. Barrin, A. Bartoloni, R. Battiston, Ammar Bayyari, N. L. Belyaev, B. Bertucci, V. Bindi, K. Bollweg, J. Bolster, M. Borchiellini, B. Borgia, M. J. Boschini, M. Bourquin, C. Brugnoni, Johanna Bürger, W.J. Burger, N. Burzillà, X.D. Cai, M. Capell, J. Casaus, G. Castellini, F. Cervelli, Yuan-Hann Chang, Guo-Ming Chen, G. R. Chen, H. Chen, H. S. Chen, Y. Chen, Lin Cheng, H. Y. Chou, S. Chouridou, V. Choutko, C. H. Chung, C. Clark, G. Coignet, C. Consolandi, A. Contin, C. Corti, Zheng Cui, S. Kokou Dadzie, Fulvio D’Angelo, Amala Dass, S. Della Torre, B. Demirköz, L. Derome, S. Di Falco, V. Di Felice, C. Díaz, F. Dimiccoli, P. von Doetinchem, Fei Dong, M. Duranti, A. I. Egorov, A. Eline, F. Faldi, D. Fehr, J. H. Feng, E. Fiandrini, P.H. Fisher, V. Formato, R. J. Garcı́a López, Corrado Gargiulo, H. Gast, M. Gervasi, F. Giovacchini, D. M. Gómez-Coral, J. Gong, D. Grandi, M. Graziani, S. Haino, K. C. Han, R. K. Hashmani, Z. H. He, B. Heber, F. Hernández-Nicolás, Timothy H. Hsieh, Jiangyong Hu, B. W. Huang, M. Ionica, M. Incagli, Yi Jia, H. Jinchi, G. Karagöz, Th. Kirn, A. P. Klipfel, O. Kounina, A. Kounine, V. Koutsenko, D. Krasnopevtsev, A. Kuhlman, A. Kulemzin, G. La Vacca, E. Laudi, G. Laurenti, G. LaVecchia, I. Lazzizzera, H. T. Lee, S. C. Lee, H. L. Li, J. H. Li, J. Q. Li, M. Li, Q. Li, Q. Y. Li, S. Li, Shiliang Li, Z. H. Li, M. J. Liang, Pu Liao, Chao‐Hung Lin, Thomas Lippert, J. H. Liu, P. C. Liu, Zhen Liu, S. Q. Lu, Y.S. Lu, Junzhou Luo, Q. Luo, Shan Luo, Xi Luo, C. Mañá, J. Marín, J. Marquardt, G. Martínez, N. Masi, D. Maurin, T. Medvedeva, A. Menchaca-Rocha, Q. Meng, V. V. Mikhailov, P. Mott, L. Mussolin, Y. Najafi Jozani, Riccardo Nicolaidis, N. Nikonov, F. Nozzoli, J. Ocampo-Peleteiro, A. Oliva, M. Orcinha, F. Palmonari, M. Paniccia, A. Pashnin, M. Pauluzzi, Dario Pelosi, S. Pensotti, P. Pietzcker, V. Plyaskin, Stepan Poluianov, D. Pridöhl, Z. H. Qu, L. Quadrani, P.G. Rancoita, D. Rapin, A. Reina Conde, E. Robyn, I. Rodríguez-García, Lisa Romaneehsen, F. Rossi, A. Rozhkov, D. Rozza, R. Z. Sagdeev, S. Schael, A. Schultz von Dratzig, G. Schwering, E. S. Seo, B. S. Shan, A. Shukla, T. Siedenburg, A. Siemko, G. Silvestre, Jiwei Song, Xiaojian Song, R. Sonnabend, Lidia Strigari, T. Su, Qie Sun, Z. T. Sun, L. Tabarroni, M. Tacconi, Zichao Tang, Jie Tian, Y. Tian, Samuel C.C. Ting, S. M. Ting, Nicola Tomassetti, J. Torsti, Alessio Ubaldi, T. Urban, Ilya Usoskin, V. Vagelli, Rami Vainio, P. Väisänen, M. Valencia-Otero, E. Valente, E. Valtonen, Alessandro Costa, M. Vecchi, M. Velasco, C. X. Wang, J. C. Wang, L. Wang, L. Q. Wang, N. H. Wang, Qiuliang Wang, S. Wang, X. Wang, Z. M. Wang, Chuncheng Wei, Z. Weng, H. Wu, Y. Wu, Zhibin Wu, J. N. Xiao, R. Q. Xiong, Xianze Xiong, W. Xu, Qi Yan, H. Yang, Y. Yang, Han Yi, Y. H. You, Young Moon Yu, Z. Q. Yu, C. Zhang, F. Z. Zhang, J. Zhang, J. H. Zhang, Zi-Yan Zhang, Pei Zhao, C. Zheng, Z. M. Zheng, H. L. Zhuang, V. Zhukov, A. Zichichi, M. Zuberi, P. Zuccon
15Citations signalées, ce qui n’est pas une note de qualité
51Institutions déclarées
14Pays d’affiliation déclarés
Rattachement africain : es, it, us, pt, de, ch, nl, tw, cn, fr, tr, bd, mx, fi.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
We report the properties of precision time structures of cosmic nuclei He, Li, Be, B, C, N, and O fluxes over an 11-year solar cycle from May 2011 to November 2022 in the rigidity range from 1.92 to 60.3 GV. The nuclei fluxes show similar but not identical time variations with amplitudes decreasing with increasing rigidity. In particular, below 3.64 GV the Li, Be, and B fluxes, and below 2.15 GV the C, N, and O fluxes, are significantly less affected by solar modulation than the He flux. We observe that these differences in solar modulation are linearly correlated with the differences in the spectral indices of the cosmic nuclei fluxes. This shows, in a model-independent way, that solar modulation of galactic cosmic nuclei depends on their spectral shape. In addition, solar modulation differences due to nuclei velocity dependence on the mass-to-charge ratio (A/Z) are not observed.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Solar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer
- Date Crossref
- 03/02/2025
- Éditeur
- American Physical Society (APS)
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
Centro de Investigaciones Energéticas, Medioambientales y TecnológicasIstituto Nazionale di Fisica Nucleare, Sezione di PerugiaMassachusetts Institute of TechnologyLIP - Laboratory of Instrumentation and Experimental Particle PhysicsErnst Ruska CentreEuropean Organization for Nuclear ResearchIstituto Nazionale di Fisica Nucleare, Sezione di Roma IUniversity of TrentoIstituto Nazionale di Fisica Nucleare, Trento Institute for Fundamental Physics And ApplicationsUniversity of Hawaii SystemUniversity of PerugiaNational Aeronautics and Space AdministrationJohnson Space CenterUniversity of GroningenSapienza University of RomeIstituto Nazionale di Fisica Nucleare, Sezione di Milano BicoccaUniversity of GenevaIstituto Nazionale di Fisica Nucleare, Roma Tor VergataIstituto Nazionale di Fisica Nucleare, Sezione di PisaInstitute of Physics, Academia SinicaChinese Academy of SciencesInstitute of High Energy PhysicsUniversity of Chinese Academy of SciencesShandong Institute of Advanced TechnologyZhejiang University-University of Edinburgh InstituteRWTH Aachen UniversityInstitut des langues et cultures d'Europe, Amérique, Afrique, Asie et AustralieUniversité Grenoble AlpesIstituto Nazionale di Fisica Nucleare, Sezione di BolognaUniversity of BolognaShandong UniversityMiddle East Technical UniversitySoutheast UniversitySoutheast UniversityUniversidad de La LagunaUniversity of Milano-BicoccaUniversidad Nacional Autónoma de MéxicoNational Chung Shan Institute of Science and TechnologyChristian-Albrechts-Universität zu KielZhejiang UniversityGenomics Research Center, Academia SinicaAcademia SinicaInstitute of Electrical EngineeringUniversity of OuluEast–West CenterUniversity of Maryland, College ParkBeihang UniversityUniversity of TurkuAgenzia Spaziale ItalianaNational Central UniversityNational Cheng Kung University
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Solar and Space Plasma DynamicsAstro and Planetary ScienceDark Matter and Cosmic Phenomena