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  1. Article ; Online: Properties of Cosmic-Ray Sulfur and Determination of the Composition of Primary Cosmic-Ray Carbon, Neon, Magnesium, and Sulfur: Ten-Year Results from the Alpha Magnetic Spectrometer.

    Aguilar, M / Ali Cavasonza, L / Alpat, B / Ambrosi, G / Arruda, L / Attig, N / Bagwell, C / Barao, F / Barrin, L / Bartoloni, A / Başeğmez-du Pree, S / Battiston, R / Belyaev, N / Berdugo, J / Bertucci, B / Bindi, V / Bollweg, K / Bolster, J / Borchiellini, M /
    Borgia, B / Boschini, M J / Bourquin, M / Bueno, E F / Burger, J / Burger, W J / Cai, X D / Capell, M / Casaus, J / Castellini, G / Cervelli, F / Chang, Y H / Chen, G M / Chen, G R / Chen, H / 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 / Dass, A / 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 / Faldi, F / Feng, J / Fiandrini, E / Fisher, P / Formato, V / 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 / Guracho, A N / Haino, S / Han, K C / Hashmani, R K / He, Z H / Heber, B / Hsieh, T H / Hu, J Y / Huang, B W / Incagli, M / Jang, W Y / Jia, Yi / Jinchi, H / Karagöz, G / Khiali, B / Kim, G N / Kirn, Th / Kounina, O / Kounine, A / Koutsenko, V / Krasnopevtsev, D / Kuhlman, A / Kulemzin, A / La Vacca, G / Laudi, E / Laurenti, G / LaVecchia, G / Lazzizzera, I / Lee, H T / Lee, S C / Li, H L / Li, J Q / Li, M / Li, Q / Li, Q Y / Li, S / Li, S L / Li, J H / Li, Z H / Liang, J / Liang, M J / Lin, C H / Lippert, T / Liu, J H / Lu, S Q / Lu, Y S / Luebelsmeyer, K / Luo, J Z / Luo, S D / Luo, Xi / Machate, F / Mañá, C / Marín, J / Marquardt, J / Martin, T / Martínez, G / Masi, N / Maurin, D / Medvedeva, T / Menchaca-Rocha, A / Meng, Q / Mikhailov, V V / Molero, M / Mott, P / Mussolin, L / Negrete, J / Nikonov, N / Nozzoli, F / Ocampo-Peleteiro, J / Oliva, A / Orcinha, M / Ottupara, M A / Palermo, M / Palmonari, F / Paniccia, M / Pashnin, A / Pauluzzi, M / Pensotti, S / Plyaskin, V / Poluianov, S / Qin, X / Qu, Z Y / Quadrani, L / Rancoita, P G / Rapin, D / Reina Conde, A / Robyn, E / Romaneehsen, L / Rozhkov, A / Rozza, D / Sagdeev, R / Schael, S / Schultz von Dratzig, A / Schwering, G / Seo, E S / Shan, B S / Siedenburg, T / 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 / Tian, Y / Ting, Samuel C C / Ting, S M / 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, 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 / Wu, Y / Xiao, J N / Xiong, R Q / Xiong, X Z / Xu, W / Yan, Q / Yang, H T / Yang, Y / Yashin, I I / Yelland, A / Yi, H / You, Y H / Yu, Y M / Yu, Z Q / Zannoni, M / Zhang, C / Zhang, F / Zhang, F Z / Zhang, J / Zhang, J H / Zhang, Z / Zhao, F / Zheng, C / Zheng, Z M / Zhuang, H L / Zhukov, V / Zichichi, A / Zuccon, P

    Physical review letters

    2023  Volume 130, Issue 21, Page(s) 211002

    Abstract: We report the properties of primary cosmic-ray sulfur (S) in the rigidity range 2.15 GV to 3.0 TV based on 0.38×10^{6} sulfur nuclei collected by the Alpha Magnetic Spectrometer experiment (AMS). We observed that above 90 GV the rigidity dependence of ... ...

    Abstract We report the properties of primary cosmic-ray sulfur (S) in the rigidity range 2.15 GV to 3.0 TV based on 0.38×10^{6} sulfur nuclei collected by the Alpha Magnetic Spectrometer experiment (AMS). We observed that above 90 GV the rigidity dependence of the S flux is identical to the rigidity dependence of Ne-Mg-Si fluxes, which is different from the rigidity dependence of the He-C-O-Fe fluxes. We found that, similar to N, Na, and Al cosmic rays, over the entire rigidity range, the traditional primary cosmic rays S, Ne, Mg, and C all have sizeable secondary components, and the S, Ne, and Mg fluxes are well described by the weighted sum of the primary silicon flux and the secondary fluorine flux, and the C flux is well described by the weighted sum of the primary oxygen flux and the secondary boron flux. The primary and secondary contributions of the traditional primary cosmic-ray fluxes of C, Ne, Mg, and S (even Z elements) are distinctly different from the primary and secondary contributions of the N, Na, and Al (odd Z elements) fluxes. The abundance ratio at the source for S/Si is 0.167±0.006, for Ne/Si is 0.833±0.025, for Mg/Si is 0.994±0.029, and for C/O is 0.836±0.025. These values are determined independent of cosmic-ray propagation.
    MeSH term(s) Magnesium ; Neon ; Carbon ; Sulfur ; Magnetic Phenomena
    Chemical Substances Magnesium (I38ZP9992A) ; Neon (4VB4Y46AHD) ; Carbon (7440-44-0) ; Sulfur (70FD1KFU70)
    Language English
    Publishing date 2023-05-26
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.130.211002
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  2. Article ; Online: Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer.

    Aguilar, M / Ali Cavasonza, L / Ambrosi, G / Arruda, L / Attig, N / Barao, F / Barrin, L / Bartoloni, A / Başeğmez-du Pree, S / Battiston, R / Becker, U / 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, 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 / Dai, Y M / 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 / Gebauer, I / Gervasi, M / Giovacchini, F / Gómez-Coral, D M / Gong, J / Goy, C / Grabski, V / Grandi, D / Graziani, M / Guo, K H / Haino, S / Han, K C / Hashmani, R K / He, Z H / Heber, B / Hsieh, T H / Hu, J Y / Huang, Z C / 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, T X / Li, Z H / Light, C / Lin, C H / Lippert, T / Liu, Z / Lu, S Q / Lu, Y S / Luebelsmeyer, K / Luo, J Z / Lyu, S S / Machate, F / Mañá, C / Marín, J / Marquardt, J / Martin, T / Martínez, G / Masi, N / Maurin, D / Menchaca-Rocha, A / Meng, Q / Mo, D C / Molero, M / Mott, P / Mussolin, L / Ni, J Q / 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 / Qi, X M / Qin, X / Qu, Z Y / Quadrani, L / Rancoita, P G / Rapin, D / Reina Conde, A / Rosier-Lees, S / Rozhkov, A / Rozza, D / Sagdeev, R / Schael, S / Schmidt, S M / Schulz von Dratzig, A / Schwering, G / Seo, E S / Shan, B S / Shi, J Y / Siedenburg, T / Solano, C / Sonnabend, R / Song, J W / 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 / Valente, E / Valtonen, E / Vázquez Acosta, M / Vecchi, M / Velasco, M / Vialle, J P / Wallmann, C / Wang, L Q / Wang, N H / Wang, Q L / Wang, S / Wang, X / Wang, Z X / Wei, J / Weng, Z L / Wu, H / Xiong, R Q / Xu, W / Yan, Q / Yang, Y / Yi, H / Yu, Y J / Yu, Z Q / Zannoni, M / Zhang, C / Zhang, F / Zhang, F Z / Zhang, J H / Zhang, Z / Zhao, F / Zheng, Z M / Zhuang, H L / Zhukov, V / Zichichi, A / Zimmermann, N / Zuccon, P

    Physical review letters

    2020  Volume 124, Issue 21, Page(s) 211102

    Abstract: We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8×10^{6}  Ne, 2.2×10^{6}  Mg, and 1.6×10^{6}  Si nuclei collected by the Alpha ... ...

    Abstract We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8×10^{6}  Ne, 2.2×10^{6}  Mg, and 1.6×10^{6}  Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.
    Keywords covid19
    Language English
    Publishing date 2020-06-12
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.124.211102
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  3. Article ; Online: Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer.

    Aguilar, M / Ali Cavasonza, L / Ambrosi, G / Arruda, L / Attig, N / Bachlechner, A / Barao, F / Barrau, A / Barrin, L / Bartoloni, A / Başeğmez-du Pree, S / Battiston, R / Becker, U / 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 / Cai, X D / Capell, M / Caroff, S / Casaus, J / Castellini, G / Cervelli, F / Chang, Y H / Chen, G M / Chen, H S / Chen, Y / Cheng, L / Chou, H Y / Choutko, V / Chung, C H / Clark, C / Coignet, G / Consolandi, C / Contin, A / Corti, C / Cui, Z / Dadzie, K / Dai, Y M / Datta, A / 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 / Galaktionov, Y / Gámez, C / García-López, R J / Gargiulo, C / Gast, H / Gebauer, I / Gervasi, M / Giovacchini, F / Gómez-Coral, D M / Gong, J / Goy, C / Grabski, V / Grandi, D / Graziani, M / Guo, K H / Haino, S / Han, K C / He, Z H / Hsieh, T H / Huang, H / Huang, Z C / 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 / Kulemzin, A / La Vacca, G / Laudi, E / Laurenti, G / Lazzizzera, I / Lebedev, A / Lee, H T / Lee, S C / Li, J Q / Li, Q / Li, T X / Li, Z H / Light, C / Lin, C H / Lippert, T / Liu, Z / Lu, S Q / Lu, Y S / Luebelsmeyer, K / Luo, F / Luo, J Z / Luo, Xi / Lyu, S S / Machate, F / Mañá, C / Marín, J / Martin, T / Martínez, G / Masi, N / Maurin, D / Menchaca-Rocha, A / Meng, Q / Mo, D C / Molero, M / Mott, P / Mussolin, L / Nelson, T / Ni, J Q / Nikonov, N / Nozzoli, F / Oliva, A / Orcinha, M / Palermo, M / Palmonari, F / Paniccia, M / Pashnin, A / Pauluzzi, M / Pensotti, S / Phan, H D / Plyaskin, V / Poireau, V / Poluianov, S / Popkow, A / Qi, X M / Qin, X / Qu, Z Y / Quadrani, L / Rancoita, P G / Rapin, D / Reina Conde, A / Rosier-Lees, S / Rozhkov, A / Rozza, D / Sagdeev, R / Schael, S / Schmidt, S M / Schulz von Dratzig, A / Schwering, G / Seo, E S / Shan, B S / Shi, J Y / Siedenburg, T / Solano, C / Song, J W / 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 / Valente, E / Valtonen, E / Vázquez Acosta, M / Vecchi, M / Velasco, M / Vialle, J P / Wang, L Q / Wang, N H / Wang, Q L / Wang, X / Wang, X Q / Wang, Z X / Wei, J / Weng, Z L / Wu, H / Xiong, R Q / Xu, W / Yan, Q / Yang, Y / Yi, H / Yu, Y J / Yu, Z Q / Zannoni, M / Zeissler, S / Zhang, C / Zhang, F / Zhang, J H / Zhang, Z / Zhao, F / Zheng, Z M / Zhuang, H L / Zhukov, V / Zichichi, A / Zimmermann, N / Zuccon, P

    Physical review letters

    2019  Volume 123, Issue 18, Page(s) 181102

    Abstract: Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of ^{3}He and ^{4}He fluxes are presented. The measurements are based on 100 million ^{4}He nuclei in the rigidity range from 2.1 to 21 GV and 18 million ^{ ...

    Abstract Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of ^{3}He and ^{4}He fluxes are presented. The measurements are based on 100 million ^{4}He nuclei in the rigidity range from 2.1 to 21 GV and 18 million ^{3}He from 1.9 to 15 GV collected from May 2011 to November 2017. We observed that the ^{3}He and ^{4}He fluxes exhibit nearly identical variations with time. The relative magnitude of the variations decreases with increasing rigidity. The rigidity dependence of the ^{3}He/^{4}He flux ratio is measured for the first time. Below 4 GV, the ^{3}He/^{4}He flux ratio was found to have a significant long-term time dependence. Above 4 GV, the ^{3}He/^{4}He flux ratio was found to be time independent, and its rigidity dependence is well described by a single power law ∝R^{Δ} with Δ=-0.294±0.004. Unexpectedly, this value is in agreement with the B/O and B/C spectral indices at high energies.
    Language English
    Publishing date 2019-11-25
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.123.181102
    Database MEDical Literature Analysis and Retrieval System OnLINE

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