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dc.contributor.authorTing, Samuel
dc.date.accessioned2022-05-02T18:53:46Z
dc.date.available2022-05-02T18:53:46Z
dc.date.issued2021
dc.identifier.urihttps://hdl.handle.net/1721.1/142235
dc.description.abstractWe 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 5.5×10^{9} 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.en_US
dc.language.isoen
dc.publisherAmerican Physical Society (APS)en_US
dc.relation.isversionof10.1103/PHYSREVLETT.127.271102en_US
dc.rightsCreative Commons Attribution 4.0 International Licenseen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0en_US
dc.sourceAPSen_US
dc.titlePeriodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GVen_US
dc.typeArticleen_US
dc.identifier.citationTing, Samuel. 2021. "Periodicities in the Daily Proton Fluxes from 2011 to 2019 Measured by the Alpha Magnetic Spectrometer on the International Space Station from 1 to 100 GV." Physical Review Letters, 127 (27).
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Science
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2022-05-02T18:23:47Z
dspace.orderedauthorsAguilar, M; Cavasonza, LA; Ambrosi, G; Arruda, L; Attig, N; Barao, F; Barrin, L; Bartoloni, A; Başeğmez-du Pree, S; Battiston, R; Behlmann, M; Beranek, B; Berdugo, J; Bertucci, B; Bindi, V; Bollweg, K; Borgia, B; Boschini, MJ; Bourquin, M; Bueno, EF; Burger, J; Burger, WJ; Burmeister, S; Cai, XD; Capell, M; Casaus, J; Castellini, G; Cervelli, F; Chang, YH; Chen, GM; Chen, GR; Chen, HS; Chen, Y; Cheng, L; Chou, HY; Chouridou, S; Choutko, V; Chung, CH; Clark, C; Coignet, G; Consolandi, C; Contin, A; Corti, C; Cui, Z; Dadzie, K; Dass, A; Delgado, C; Della Torre, S; Demirköz, MB; Derome, L; Di Falco, S; Di Felice, V; Díaz, C; Dimiccoli, F; von Doetinchem, P; Dong, F; Donnini, F; Duranti, M; Egorov, A; Eline, A; Feng, J; Fiandrini, E; Fisher, P; Formato, V; Freeman, C; Gámez, C; García-López, RJ; Gargiulo, C; Gast, H; Gervasi, M; Giovacchini, F; Gómez-Coral, DM; Gong, J; Goy, C; Grabski, V; Grandi, D; Graziani, M; Haino, S; Han, KC; Hashmani, RK; He, ZH; Heber, B; Hsieh, TH; Hu, JY; Incagli, M; Jang, WY; Jia, Y; Jinchi, H; Karagöz, G; Khiali, B; Kim, GN; Kirn, T; Konyushikhin, M; Kounina, O; Kounine, A; Koutsenko, V; Krasnopevtsev, D; Kuhlman, A; Kulemzin, A; La Vacca, G; Laudi, E; Laurenti, G; Lazzizzera, I; Lebedev, A; Lee, HT; Lee, SC; Li, JQ; Li, M; Li, Q; Li, S; Li, JH; Li, ZH; Liang, J; Light, C; Lin, CH; Lippert, T; Liu, JH; Liu, Z; Lu, SQ; Lu, YS; Luebelsmeyer, K; Luo, JZ; Luo, X; Machate, F; Mañá, C; Marín, J; Marquardt, J; Martin, T; Martínez, G; Masi, N; Maurin, D; Medvedeva, T; Menchaca-Rocha, A; Meng, Q; Mikhailov, VV; Molero, M; Mott, P; Mussolin, L; Negrete, J; Nikonov, N; Nozzoli, F; Oliva, A; Orcinha, M; Palermo, M; Palmonari, F; Paniccia, M; Pashnin, A; Pauluzzi, M; Pensotti, S; Phan, HD; Plyaskin, V; Pohl, M; Poluianov, S; Qin, X; Qu, ZY; Quadrani, L; Rancoita, PG; Rapin, D; Conde, AR; Robyn, E; Rosier-Lees, S; Rozhkov, A; Rozza, D; Sagdeev, R; Schael, S; von Dratzig, AS; Schwering, G; Seo, ES; Shakfa, Z; Shan, BS; Siedenburg, T; Solano, C; Song, JW; Song, XJ; Sonnabend, R; Strigari, L; Su, T; Sun, Q; Sun, ZT; Tacconi, M; Tang, XW; Tang, ZC; Tian, J; Ting, SCC; Ting, SM; Tomassetti, N; Torsti, J; Urban, T; Usoskin, I; Vagelli, V; Vainio, R; Valencia-Otero, M; Valente, E; Valtonen, E; Vázquez Acosta, M; Vecchi, M; Velasco, M; Vialle, JP; Wang, CX; Wang, L; Wang, LQ; Wang, NH; Wang, QL; Wang, S; Wang, X; Wang, Y; Wang, ZM; Wei, J; Weng, ZL; Wu, H; Xiong, RQ; Xu, W; Yan, Q; Yang, Y; Yashin, II; Yi, H; Yu, YM; Yu, ZQ; Zannoni, M; Zhang, C; Zhang, F; Zhang, FZ; Zhang, JH; Zhang, Z; Zhao, F; Zheng, C; Zheng, ZM; Zhuang, HL; Zhukov, V; Zichichi, A; Zuccon, Pen_US
dspace.date.submission2022-05-02T18:23:50Z
mit.journal.volume127en_US
mit.journal.issue27en_US
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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