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Properties of Daily Helium Fluxes.

Authors :
Aguilar M
Cavasonza LA
Ambrosi G
Arruda L
Attig N
Barao F
Barrin L
Bartoloni A
Başeğmez-du Pree S
Battiston R
Behlmann M
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
Lee HT
Lee SC
Li HL
Li JQ
Li M
Li Q
Li QY
Li S
Li SL
Li JH
Li ZH
Liang J
Liang MJ
Light C
Lin CH
Lippert T
Liu JH
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
Ocampo-Peleteiro J
Oliva A
Orcinha M
Palermo M
Palmonari F
Paniccia M
Pashnin A
Pauluzzi M
Pensotti S
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
Shan BS
Siedenburg T
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 P
Source :
Physical review letters [Phys Rev Lett] 2022 Jun 10; Vol. 128 (23), pp. 231102.
Publication Year :
2022

Abstract

We present the precision measurement of 2824 daily helium fluxes in cosmic rays from May 20, 2011 to October 29, 2019 in the rigidity interval from 1.71 to 100 GV based on 7.6×10^{8} helium nuclei collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The helium flux and the helium to proton flux ratio exhibit variations on multiple timescales. In nearly all the time intervals from 2014 to 2018, we observed recurrent helium 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. In the entire time period, we found that below ∼7  GV the helium flux exhibits larger time variations than the proton flux, and above ∼7  GV the helium to proton flux ratio is time independent. Remarkably, below 2.4 GV a hysteresis between the helium to proton flux ratio and the helium flux was observed at greater than the 7σ level. This shows that at low rigidity the modulation of the helium to proton flux ratio is different before and after the solar maximum in 2014.

Details

Language :
English
ISSN :
1079-7114
Volume :
128
Issue :
23
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
35749176
Full Text :
https://doi.org/10.1103/PhysRevLett.128.231102