Медицинская библиотека · Physical review letters · 2026
Properties of Heavy Cosmic Nuclei Phosphorus, Chlorine, Argon, Potassium, and Calcium: Results from the Alpha Magnetic Spectrometer.
Aceituno A, Aguilar M, Alpat B, Ambrosi G, Anderson H, Antunes J, Arruda L, Attig N, Bagwell C, Barao F, Barbanera M, Barrin L, Bartoloni A, Battiston R, Bayyari A, Belyaev N, Bertucci B, Bindi V, Bollweg K, Bolster J, Borchiellini M, Borgia B, Boschini M J, Bourquin M, Brugnoni C, Burger W J, Cai H Y, Cai X D, Capell M, Casaus J, Cassidy J, Castellini G, Cervelli F, Chang Y H, Chen G M, Chen G R, Chen H, 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 Y X, Cui Z, Dadzie K, D'Angelo F, 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, Dotson M, Duranti M, Egorov A, Ellison A, Faldi F, Fehr D, Feng J, Fiandrini E, Fisher P, Formato V, García-López R J, Galdames A, Gargiulo C, Gast H, Ge T T, Gervasi M, Ghezzer L E, Giovacchini F, Gómez-Coral D M, Gong J, Grandi D, Graziani M, Guidetti R, Guan C, He Z H, Heber B, Hernández-Nicolás F, Höfer L, Hsieh T H, Hu J Y, Huang B W, Ionica M, Incagli M, Jia Yi, Jinchi H, Kappe T, Karadöller E, Karagöz G, Kastelic J, Kirn Th, Kounina O, Kounine A, Koutsenko V, Krasnopevtsev D, Kuhlman A, Kulemzin A, La Vacca G, Laudi E, Laurenti G, Lazzizzera I, Lee H T, Lee S C, Li H L, Li J H, Li J Q, Li M, Li Q, Li Q, Li Q Y, Li S L, Li Z H, Liao P, Lin C H, Lippert T, Liu P C, Liu Z, Lu S Q, Luo J Z, Luo Q, Luo S D, Luo Xi, Mañá C, Marín J, Martínez G, Masi N, Maurin D, Medvedeva T, Menchaca-Rocha A, Meng Q, Mikhailov V V, Molero M, Mott P, Mussolin L, Najafi Jozani Y, Nicolaidis R, Nikonov N, Nozzoli F, Ocampo-Peleteiro J, Oliva A, Orcinha M, Palmonari F, Paniccia M, Pashnin A, Pauluzzi M, Pelosi D, Pensotti S, Perez D, Pietzcker P, Plyaskin V, Poluianov S, Pridöhl D, Puccetti N, Qu Z Y, Quadrani L, Rafiei M M, Rancoita P G, Rapin D, Robyn E, Rodríguez-García I, Romaneehsen L, Rossi F, Rozhkov A, Rozza D, Sagdeev R, Schael S, Schultz von Dratzig A, Schwering G, Seo E S, Shan B S, Shukla A, Siedenburg T, Siemko A, Silvestre G, Schledewitz D, Song J W, Song X J, Sonnabend R, Strekalovsky A, Strigari L, Stuzhin A, Su T, Sun Q, Sun Z T, Tabarroni L, Tacconi M, Tang Z C, Teoh J J, Tian J, Tian Ye, Tian Y, Ting Samuel C C, Ting S M, Tomassetti N, Torsti J, Ubaldi A, Usoskin I, Vagelli V, Vainio R, Väisänen P, Valencia-Otero M, Valente E, Valtonen E, Van Hove E, Vázquez Acosta M, Vecchi M, Velasco M, Wang J C, Wang L Q, Wang N H, Wang S, Wang X, Wang Z M, Waqas M, Weng Z L, Wu H, Wu Z B, Xiao J N, Xiong R Q, Xiong Y Z, Xu W, Yan Q, Yan Z X, Yang H T, Yang Y, Yi H, You Y H, Yu M, Yu Y M, Yu Z Q, Yuan B Q, Zhang C, Zhang F Z, Zhang J, Zhang J H, Zhang Z, Zhao P W, Zheng Z M, Zhou H F, Zhuang H L, Zhukov V, Zou L K, Zuberi M, Zuccon P, AMS Collaboration
СтатьяПеревод в очереди
Аннотация
We report the unique properties of cosmic phosphorus (P), chlorine (Cl), argon (Ar), potassium (K), and calcium (Ca) fluxes in the GV to TV rigidity range collected by the Alpha Magnetic Spectrometer (AMS) on the International Space Station. With a total of one million events collected over 13.5 years, we observed that the rigidity dependencies of the five fluxes are well described by the sums of a primary cosmic ray component and a secondary cosmic ray component. The abundance ratios of all five elements to Si at the source are accurately determined independent of cosmic ray propagation. The source abundance of Ar and Ca (even-Z elements) is larger than P, Cl, and K (odd-Z elements). The secondary components of the P and the Cl fluxes are each ∼1/3 of the F flux, and the secondary components of the Ar, K, and Ca fluxes are each ∼1/2 of the F flux. The twenty elements measured by AMS, from He to Ca and Fe, can be categorized into four classes, two primary and two secondary, based on their rigidity dependence.
Для цитирования: Aceituno A, Aguilar M, Alpat B, Ambrosi G, Anderson H, Antunes J, Arruda L, Attig N, Bagwell C, Barao F, Barbanera M, Barrin L, Bartoloni A, Battiston R, Bayyari A, Belyaev N, Bertucci B, Bindi V, Bollweg K, Bolster J, Borchiellini M, Borgia B, Boschini M J, Bourquin M, Brugnoni C, Burger W J, Cai H Y, Cai X D, Capell M, Casaus J, Cassidy J, Castellini G, Cervelli F, Chang Y H, Chen G M, Chen G R, Chen H, 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 Y X, Cui Z, Dadzie K, D'Angelo F, 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, Dotson M, Duranti M, Egorov A, Ellison A, Faldi F, Fehr D, Feng J, Fiandrini E, Fisher P, Formato V, García-López R J, Galdames A, Gargiulo C, Gast H, Ge T T, Gervasi M, Ghezzer L E, Giovacchini F, Gómez-Coral D M, Gong J, Grandi D, Graziani M, Guidetti R, Guan C, He Z H, Heber B, Hernández-Nicolás F, Höfer L, Hsieh T H, Hu J Y, Huang B W, Ionica M, Incagli M, Jia Yi, Jinchi H, Kappe T, Karadöller E, Karagöz G, Kastelic J, Kirn Th, Kounina O, Kounine A, Koutsenko V, Krasnopevtsev D, Kuhlman A, Kulemzin A, La Vacca G, Laudi E, Laurenti G, Lazzizzera I, Lee H T, Lee S C, Li H L, Li J H, Li J Q, Li M, Li Q, Li Q, Li Q Y, Li S L, Li Z H, Liao P, Lin C H, Lippert T, Liu P C, Liu Z, Lu S Q, Luo J Z, Luo Q, Luo S D, Luo Xi, Mañá C, Marín J, Martínez G, Masi N, Maurin D, Medvedeva T, Menchaca-Rocha A, Meng Q, Mikhailov V V, Molero M, Mott P, Mussolin L, Najafi Jozani Y, Nicolaidis R, Nikonov N, Nozzoli F, Ocampo-Peleteiro J, Oliva A, Orcinha M, Palmonari F, Paniccia M, Pashnin A, Pauluzzi M, Pelosi D, Pensotti S, Perez D, Pietzcker P, Plyaskin V, Poluianov S, Pridöhl D, Puccetti N, Qu Z Y, Quadrani L, Rafiei M M, Rancoita P G, Rapin D, Robyn E, Rodríguez-García I, Romaneehsen L, Rossi F, Rozhkov A, Rozza D, Sagdeev R, Schael S, Schultz von Dratzig A, Schwering G, Seo E S, Shan B S, Shukla A, Siedenburg T, Siemko A, Silvestre G, Schledewitz D, Song J W, Song X J, Sonnabend R, Strekalovsky A, Strigari L, Stuzhin A, Su T, Sun Q, Sun Z T, Tabarroni L, Tacconi M, Tang Z C, Teoh J J, Tian J, Tian Ye, Tian Y, Ting Samuel C C, Ting S M, Tomassetti N, Torsti J, Ubaldi A, Usoskin I, Vagelli V, Vainio R, Väisänen P, Valencia-Otero M, Valente E, Valtonen E, Van Hove E, Vázquez Acosta M, Vecchi M, Velasco M, Wang J C, Wang L Q, Wang N H, Wang S, Wang X, Wang Z M, Waqas M, Weng Z L, Wu H, Wu Z B, Xiao J N, Xiong R Q, Xiong Y Z, Xu W, Yan Q, Yan Z X, Yang H T, Yang Y, Yi H, You Y H, Yu M, Yu Y M, Yu Z Q, Yuan B Q, Zhang C, Zhang F Z, Zhang J, Zhang J H, Zhang Z, Zhao P W, Zheng Z M, Zhou H F, Zhuang H L, Zhukov V, Zou L K, Zuberi M, Zuccon P, AMS Collaboration. Properties of Heavy Cosmic Nuclei Phosphorus, Chlorine, Argon, Potassium, and Calcium: Results from the Alpha Magnetic Spectrometer.. Physical review letters. 2026. DOI: 10.1103/d2vf-fw3v.
Подготовка и перевод публикацииОбработка статьи · этапы, ошибки и управление
Загрузка состояния…
Ошибки и ограничения
История · было → стало
Состояние обновляется каждые 5 секунд, пока блок открыт. Процент показывается только там, где известен объём работы. Пауза останавливает продолжение этапа; текущий запрос к источнику может завершиться.
Тип публикации указан по данным источника. Уровень доказательности автоматически не присваивается.