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Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer.

Authors :
Aguilar M
Cavasonza LA
Allen MS
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 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
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
Galaktionov Y
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
Kanishev K
Khiali B
Kim GN
Kirn T
Konyushikhin M
Kounina O
Kounine A
Koutsenko V
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
Lyu SS
Machate F
Mañá C
Marín J
Marquardt J
Martin T
Martínez G
Masi N
Maurin D
Menchaca-Rocha A
Meng Q
Mikhailov VV
Mo DC
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
Piandani R
Plyaskin V
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
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 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
Zimmermann N
Zuccon P
Source :
Physical review letters [Phys Rev Lett] 2021 Jan 29; Vol. 126 (4), pp. 041104.
Publication Year :
2021

Abstract

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.

Details

Language :
English
ISSN :
1079-7114
Volume :
126
Issue :
4
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
33576661
Full Text :
https://doi.org/10.1103/PhysRevLett.126.041104