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Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer

Precise knowledge of the charge and rigidity dependence of the secondary cosmic ray fluxes and the secondary-to-primary flux ratios is essential in the understanding of cosmic ray propagation. We report the properties of heavy secondary cosmic ray fluorine F in the rigidity $R$ range 2.15 GV to 2.9...

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Autores principales:	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, Beranek, B, Berdugo, J, Bertucci, B, Bindi, V, 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, Schulz von Dratzig, A, 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, Zuccon, P
Lenguaje:	eng
Publicado:	2021
Materias:	Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1103/PhysRevLett.126.081102 http://cds.cern.ch/record/2757354

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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 Beranek, B Berdugo, J Bertucci, B Bindi, V 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 Schulz von Dratzig, A 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 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 Beranek, B Berdugo, J Bertucci, B Bindi, V 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 Schulz von Dratzig, A 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 Zuccon, P
author_sort	Aguilar, M
collection	CERN
description	Precise knowledge of the charge and rigidity dependence of the secondary cosmic ray fluxes and the secondary-to-primary flux ratios is essential in the understanding of cosmic ray propagation. We report the properties of heavy secondary cosmic ray fluorine F in the rigidity $R$ range 2.15 GV to 2.9 TV based on 0.29 million events collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The fluorine spectrum deviates from a single power law above 200 GV. The heavier secondary-to-primary F/Si flux ratio rigidity dependence is distinctly different from the lighter B/O (or B/C) rigidity dependence. In particular, above 10 GV, the $^{\textrm{F/Si}}_{\textrm{B/O}}$ ratio can be described by a power law $R^δ$ with $δ=0.052±0.007$. This shows that the propagation properties of heavy cosmic rays, from F to Si, are different from those of light cosmic rays, from He to O, and that the secondary cosmic rays have two classes.
id	oai-inspirehep.net-1849433
institution	Organización Europea para la Investigación Nuclear
language	eng
publishDate	2021
record_format	invenio
spelling	oai-inspirehep.net-18494332021-03-19T22:31:32Zdoi:10.1103/PhysRevLett.126.081102http://cds.cern.ch/record/2757354engAguilar, MCavasonza, L AliAllen, M SAlpat, BAmbrosi, GArruda, LAttig, NBarao, FBarrin, LBartoloni, ABaşeğmez-du Pree, SBattiston, RBehlmann, MBeranek, BBerdugo, JBertucci, BBindi, VBollweg, 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, SSchulz von Dratzig, ASchwering, 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, AZuccon, PProperties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic SpectrometerAstrophysics and AstronomyPrecise knowledge of the charge and rigidity dependence of the secondary cosmic ray fluxes and the secondary-to-primary flux ratios is essential in the understanding of cosmic ray propagation. We report the properties of heavy secondary cosmic ray fluorine F in the rigidity $R$ range 2.15 GV to 2.9 TV based on 0.29 million events collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The fluorine spectrum deviates from a single power law above 200 GV. The heavier secondary-to-primary F/Si flux ratio rigidity dependence is distinctly different from the lighter B/O (or B/C) rigidity dependence. In particular, above 10 GV, the $^{\textrm{F/Si}}_{\textrm{B/O}}$ ratio can be described by a power law $R^δ$ with $δ=0.052±0.007$. This shows that the propagation properties of heavy cosmic rays, from F to Si, are different from those of light cosmic rays, from He to O, and that the secondary cosmic rays have two classes.oai:inspirehep.net:18494332021
spellingShingle	Astrophysics and Astronomy 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 Beranek, B Berdugo, J Bertucci, B Bindi, V 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 Schulz von Dratzig, A 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 Zuccon, P Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title	Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title_full	Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title_fullStr	Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title_full_unstemmed	Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title_short	Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer
title_sort	properties of heavy secondary fluorine cosmic rays: results from the alpha magnetic spectrometer
topic	Astrophysics and Astronomy
url	https://dx.doi.org/10.1103/PhysRevLett.126.081102 http://cds.cern.ch/record/2757354
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propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT fengj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT fiandrinie propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT fisherp propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT formatov propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT freemanc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT galaktionovy propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gamezc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT garcialopezrj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gargiuloc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gasth propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gervasim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT giovacchinif propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gomezcoraldm propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT gongj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT goyc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT grabskiv propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT grandid propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT grazianim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hainos propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hankc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hashmanirk propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hezh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT heberb propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hsiehth propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT hujy propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT incaglim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT jangwy propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT jiayi propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT jinchih propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kanishevk propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT khialib propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kimgn propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kirnth propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT konyushikhinm propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kouninao propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kouninea propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT koutsenkov propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kuhlmana propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT kulemzina propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lavaccag propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT laudie propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT laurentig propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lazzizzerai propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lebedeva propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT leeht propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT leesc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lijq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT liq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lis propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lijh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lizh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT liangj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lightc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT linch propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lippertt propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT liujh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT liuz propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lusq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT luys propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT luebelsmeyerk propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT luojz propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT luoxi propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT lyuss propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT machatef propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT manac propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT marinj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT marquardtj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT martint propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT martinezg propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT masin propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT maurind propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT menchacarochaa propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT mengq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT mikhailovvv propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT modc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT molerom propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT mottp propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT mussolinl propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT negretej propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT nikonovn propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT nozzolif propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT olivaa propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT orcinham propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT palermom propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT palmonarif propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT panicciam propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT pashnina propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT pauluzzim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT pensottis propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT phanhd propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT piandanir propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT plyaskinv propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT poluianovs propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT qinx propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT quzy propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT quadranil propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT rancoitapg propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT rapind propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT condeareina propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT robyne propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT rosierleess propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT rozhkova propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT rozzad propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT sagdeevr propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT schaels propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT schulzvondratziga propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT schweringg propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT seoes propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT shakfaz propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT shanbs propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT siedenburgt propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT solanoc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT songjw propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT songxj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT sonnabendr propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT strigaril propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT sut propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT sunq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT sunzt propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tacconim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tangxw propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tangzc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tianj propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tingsamuelcc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tingsm propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tomassettin propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT torstij propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT tuysuzc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT urbant propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT usoskini propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT vagelliv propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT vainior propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT valenciaoterom propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT valentee propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT valtonene propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT vazquezacostam propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT vecchim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT velascom propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT viallejp propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangcx propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangl propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wanglq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangnh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangql propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangs propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangx propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangyu propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wangzm propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT weij propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wengzl propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT wuh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT xiongrq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT xuw propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yanq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yangy propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yashinii propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yih propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yuym propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT yuzq propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zannonim propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhangc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhangf propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhangfz propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhangjh propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhangz propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhaof propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhengc propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhengzm propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhuanghl propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zhukovv propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zichichia propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer AT zucconp propertiesofheavysecondaryfluorinecosmicraysresultsfromthealphamagneticspectrometer

Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer

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