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Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer
We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×10$^6$ iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flu...
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Lenguaje: | eng |
Publicado: |
2021
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.126.041104 http://cds.cern.ch/record/2751462 |
_version_ | 1780969239491903488 |
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author | Aguilar, M Cavasonza, L Ali Allen, M S Alpat, B Ambrosi, G Arruda, L Attig, N Barao, F Barrin, L Bartoloni, A Başeğmez-du Pree, S Battiston, R Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Burmeister, S Cai, X D Capell, M Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, G R Chen, H S Chen, Y Cheng, L Chou, H Y Chouridou, S Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Cui, Z Dadzie, K Delgado, C Della Torre, S Demirköz, M B 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 Galaktionov, Y Gámez, C García-López, R J Gargiulo, C Gast, H Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Haino, S Han, K C Hashmani, R K He, Z H Heber, B Hsieh, T H Hu, J Y Incagli, M Jang, W Y Jia, Yi Jinchi, H Kanishev, K Khiali, B Kim, G N Kirn, Th Konyushikhin, M Kounina, O Kounine, A Koutsenko, V Kuhlman, A Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Li, J Q Li, M Li, Q Li, S Li, J H Li, Z H Liang, J Light, C Lin, C H Lippert, T Liu, J H Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Marquardt, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mikhailov, V V Mo, D C 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, H D Piandani, R Plyaskin, V Poluianov, S Qin, X Qu, Z Y Quadrani, L Rancoita, P G Rapin, D Conde, A Reina Robyn, E Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Schael, S von Dratzig, A Schulz Schwering, G Seo, E S Shakfa, Z Shan, B S Siedenburg, T Solano, C Song, J W Song, X J Sonnabend, R Strigari, L Su, T Sun, Q Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Tüysüz, C Urban, T Usoskin, I Vagelli, V Vainio, R Valencia-Otero, M Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Wang, C X Wang, L Wang, L Q Wang, N H Wang, Q L Wang, S Wang, X Wang, Yu Wang, Z M Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yashin, I I Yi, H Yu, Y M Yu, Z Q Zannoni, M Zhang, C Zhang, F Zhang, F Z Zhang, J H Zhang, Z Zhao, F Zheng, C Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P |
author_facet | Aguilar, M Cavasonza, L Ali Allen, M S Alpat, B Ambrosi, G Arruda, L Attig, N Barao, F Barrin, L Bartoloni, A Başeğmez-du Pree, S Battiston, R Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Burmeister, S Cai, X D Capell, M Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, G R Chen, H S Chen, Y Cheng, L Chou, H Y Chouridou, S Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Cui, Z Dadzie, K Delgado, C Della Torre, S Demirköz, M B 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 Galaktionov, Y Gámez, C García-López, R J Gargiulo, C Gast, H Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Haino, S Han, K C Hashmani, R K He, Z H Heber, B Hsieh, T H Hu, J Y Incagli, M Jang, W Y Jia, Yi Jinchi, H Kanishev, K Khiali, B Kim, G N Kirn, Th Konyushikhin, M Kounina, O Kounine, A Koutsenko, V Kuhlman, A Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Li, J Q Li, M Li, Q Li, S Li, J H Li, Z H Liang, J Light, C Lin, C H Lippert, T Liu, J H Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Marquardt, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mikhailov, V V Mo, D C 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, H D Piandani, R Plyaskin, V Poluianov, S Qin, X Qu, Z Y Quadrani, L Rancoita, P G Rapin, D Conde, A Reina Robyn, E Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Schael, S von Dratzig, A Schulz Schwering, G Seo, E S Shakfa, Z Shan, B S Siedenburg, T Solano, C Song, J W Song, X J Sonnabend, R Strigari, L Su, T Sun, Q Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Tüysüz, C Urban, T Usoskin, I Vagelli, V Vainio, R Valencia-Otero, M Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Wang, C X Wang, L Wang, L Q Wang, N H Wang, Q L Wang, S Wang, X Wang, Yu Wang, Z M Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yashin, I I Yi, H Yu, Y M Yu, Z Q Zannoni, M Zhang, C Zhang, F Zhang, F Z Zhang, J H Zhang, Z Zhao, F Zheng, C Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P |
author_sort | Aguilar, M |
collection | CERN |
description | We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×10$^6$ iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class. |
id | oai-inspirehep.net-1844651 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2021 |
record_format | invenio |
spelling | oai-inspirehep.net-18446512021-02-09T22:54:56Zdoi:10.1103/PhysRevLett.126.041104http://cds.cern.ch/record/2751462engAguilar, MCavasonza, L AliAllen, M SAlpat, BAmbrosi, GArruda, LAttig, NBarao, FBarrin, LBartoloni, ABaşeğmez-du Pree, SBattiston, RBehlmann, MBeischer, BBerdugo, JBertucci, BBindi, Vde Boer, WBollweg, KBorgia, BBoschini, M JBourquin, MBueno, E FBurger, JBurger, W JBurmeister, SCai, X DCapell, MCasaus, JCastellini, GCervelli, FChang, Y HChen, G MChen, G RChen, H SChen, YCheng, LChou, H YChouridou, SChoutko, VChung, C HClark, CCoignet, GConsolandi, CContin, ACorti, CCui, ZDadzie, KDelgado, CDella Torre, SDemirköz, M BDerome, LDi Falco, SDi Felice, VDíaz, CDimiccoli, Fvon Doetinchem, PDong, FDonnini, FDuranti, MEgorov, AEline, AFeng, JFiandrini, EFisher, PFormato, VFreeman, CGalaktionov, YGámez, CGarcía-López, R JGargiulo, CGast, HGervasi, MGiovacchini, FGómez-Coral, D MGong, JGoy, CGrabski, VGrandi, DGraziani, MHaino, SHan, K CHashmani, R KHe, Z HHeber, BHsieh, T HHu, J YIncagli, MJang, W YJia, YiJinchi, HKanishev, KKhiali, BKim, G NKirn, ThKonyushikhin, MKounina, OKounine, AKoutsenko, VKuhlman, AKulemzin, ALa Vacca, GLaudi, ELaurenti, GLazzizzera, ILebedev, ALee, H TLee, S CLi, J QLi, MLi, QLi, SLi, J HLi, Z HLiang, JLight, CLin, C HLippert, TLiu, J HLiu, ZLu, S QLu, Y SLuebelsmeyer, KLuo, J ZLuo, XiLyu, S SMachate, FMañá, CMarín, JMarquardt, JMartin, TMartínez, GMasi, NMaurin, DMenchaca-Rocha, AMeng, QMikhailov, V VMo, D CMolero, MMott, PMussolin, LNegrete, JNikonov, NNozzoli, FOliva, AOrcinha, MPalermo, MPalmonari, FPaniccia, MPashnin, APauluzzi, MPensotti, SPhan, H DPiandani, RPlyaskin, VPoluianov, SQin, XQu, Z YQuadrani, LRancoita, P GRapin, DConde, A ReinaRobyn, ERosier-Lees, SRozhkov, ARozza, DSagdeev, RSchael, Svon Dratzig, A SchulzSchwering, GSeo, E SShakfa, ZShan, B SSiedenburg, TSolano, CSong, J WSong, X JSonnabend, RStrigari, LSu, TSun, QSun, Z TTacconi, MTang, X WTang, Z CTian, JTing, Samuel C CTing, S MTomassetti, NTorsti, JTüysüz, CUrban, TUsoskin, IVagelli, VVainio, RValencia-Otero, MValente, EValtonen, EVázquez Acosta, MVecchi, MVelasco, MVialle, J PWang, C XWang, LWang, L QWang, N HWang, Q LWang, SWang, XWang, YuWang, Z MWei, JWeng, Z LWu, HXiong, R QXu, WYan, QYang, YYashin, I IYi, HYu, Y MYu, Z QZannoni, MZhang, CZhang, FZhang, F ZZhang, J HZhang, ZZhao, FZheng, CZheng, Z MZhuang, H LZhukov, VZichichi, AZimmermann, NZuccon, PProperties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic SpectrometerAstrophysics and AstronomyDetectors and Experimental TechniquesWe report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×10$^6$ iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.oai:inspirehep.net:18446512021 |
spellingShingle | Astrophysics and Astronomy Detectors and Experimental Techniques Aguilar, M Cavasonza, L Ali Allen, M S Alpat, B Ambrosi, G Arruda, L Attig, N Barao, F Barrin, L Bartoloni, A Başeğmez-du Pree, S Battiston, R Behlmann, M Beischer, B Berdugo, J Bertucci, B Bindi, V de Boer, W Bollweg, K Borgia, B Boschini, M J Bourquin, M Bueno, E F Burger, J Burger, W J Burmeister, S Cai, X D Capell, M Casaus, J Castellini, G Cervelli, F Chang, Y H Chen, G M Chen, G R Chen, H S Chen, Y Cheng, L Chou, H Y Chouridou, S Choutko, V Chung, C H Clark, C Coignet, G Consolandi, C Contin, A Corti, C Cui, Z Dadzie, K Delgado, C Della Torre, S Demirköz, M B 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 Galaktionov, Y Gámez, C García-López, R J Gargiulo, C Gast, H Gervasi, M Giovacchini, F Gómez-Coral, D M Gong, J Goy, C Grabski, V Grandi, D Graziani, M Haino, S Han, K C Hashmani, R K He, Z H Heber, B Hsieh, T H Hu, J Y Incagli, M Jang, W Y Jia, Yi Jinchi, H Kanishev, K Khiali, B Kim, G N Kirn, Th Konyushikhin, M Kounina, O Kounine, A Koutsenko, V Kuhlman, A Kulemzin, A La Vacca, G Laudi, E Laurenti, G Lazzizzera, I Lebedev, A Lee, H T Lee, S C Li, J Q Li, M Li, Q Li, S Li, J H Li, Z H Liang, J Light, C Lin, C H Lippert, T Liu, J H Liu, Z Lu, S Q Lu, Y S Luebelsmeyer, K Luo, J Z Luo, Xi Lyu, S S Machate, F Mañá, C Marín, J Marquardt, J Martin, T Martínez, G Masi, N Maurin, D Menchaca-Rocha, A Meng, Q Mikhailov, V V Mo, D C 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, H D Piandani, R Plyaskin, V Poluianov, S Qin, X Qu, Z Y Quadrani, L Rancoita, P G Rapin, D Conde, A Reina Robyn, E Rosier-Lees, S Rozhkov, A Rozza, D Sagdeev, R Schael, S von Dratzig, A Schulz Schwering, G Seo, E S Shakfa, Z Shan, B S Siedenburg, T Solano, C Song, J W Song, X J Sonnabend, R Strigari, L Su, T Sun, Q Sun, Z T Tacconi, M Tang, X W Tang, Z C Tian, J Ting, Samuel C C Ting, S M Tomassetti, N Torsti, J Tüysüz, C Urban, T Usoskin, I Vagelli, V Vainio, R Valencia-Otero, M Valente, E Valtonen, E Vázquez Acosta, M Vecchi, M Velasco, M Vialle, J P Wang, C X Wang, L Wang, L Q Wang, N H Wang, Q L Wang, S Wang, X Wang, Yu Wang, Z M Wei, J Weng, Z L Wu, H Xiong, R Q Xu, W Yan, Q Yang, Y Yashin, I I Yi, H Yu, Y M Yu, Z Q Zannoni, M Zhang, C Zhang, F Zhang, F Z Zhang, J H Zhang, Z Zhao, F Zheng, C Zheng, Z M Zhuang, H L Zhukov, V Zichichi, A Zimmermann, N Zuccon, P Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title | Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title_full | Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title_fullStr | Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title_full_unstemmed | Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title_short | Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer |
title_sort | properties of iron primary cosmic rays: results from the alpha magnetic spectrometer |
topic | Astrophysics and Astronomy Detectors and Experimental Techniques |
url | https://dx.doi.org/10.1103/PhysRevLett.126.041104 http://cds.cern.ch/record/2751462 |
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