Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station

Aguilar M.; Cavasonza L. Ali; Alpat B.; Ambrosi G.; Arruda L.; Attig N.; Aupetit S.; Azzarello P.; Bachlechner A.; Barao F.; Barrau A.; Barrin L.; Bartoloni A.; Basara L.; Basegmez-du Pree S.; Battarbee M.; Battiston R.; Becker U.; Behlmann M.; Beischer B.; Berdugo J.; Bertucci B.; Bindel K. F.; Bindi V.; de Boer W.; Bollweg K.; Bonnivard V.; Borgia B.; Boschini M. J.; Bourquin M.; Bueno E. F.; Burger J.; Burger W. J.; Cadoux F.; Cai X. D.; Capell M.; Caroff S.; Casaus J.; Castellini G.; Cervelli F.; Chae M. J.; Chang Y. H.; Chen A. I.; Chen G. M.; Chen H. S.; Cheng L.; Chou H. Y.; Choumilov E.; Choutko V.; Chung C. H.; Clark C.; Clavero R.; Coignet G.; Consolandi C.; Contin A.; Corti C.; Creus W.; Crispoltoni M.; Cui Z.; Dadzie K.; Dai Y. M.; Datta A.; Delgado C.; Della Torre S.; Demakov O.; Demirkoz M. B.; Derome L.; Di Falco S.; Dimiccoli F.; Diaz C.; von Doetinchem P.; Dong F.; Donnini F.; Duranti M.; DUrso D.; Egorov A.; Eline A.; Eronen T.; Feng J.; Fiandrini E.; Fisher P.; Formato V.; Galaktionov Y.; Gallucci G.; Garcia-Lopez R. J.; Gargiulo C.; Gast H.; Gebauer I.; Gervasi M.; Ghelfi A.; Giovacchini F.; Gomez-Coral D. M.; Gong J.; Goy C.; Grabski V.; Grandi D.; Graziani M.; Guo K. H.; Haino S.; Han K. C.; He Z. H.; Heil M.; Hoffman J.; Hsieh T. H.; Huang H.; Huang Z. C.; Huh C.; Incagli M.; Ionica M.; Jang W. Y.; Jia Yi; Jinchi H.; Kang S. C.; Kanishev K.; Khiali B.; Kim G. N.; Kim K. S.; Kirn Th.; Konak C.; 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.; Leluc C.; Li H. S.; Li J. Q.; Li Q.; Li T. X.; Li Y.; Li Z. H.; Li Z. Y.; Lim S.; Lin C. H.; Lipari P.; Lippert T.; Liu D.; Liu Hu; Lordello V. D.; Lu S. Q.; Lu Y. S.; Luebelsmeyer K.; Luo F.; Luo J. Z.; Lyu S. S.; Machate F.; Mana C.; Marin J.; Martin T.; Martinez G.; Masi N.; Maurin D.; Menchaca-Rocha A.; Meng Q.; Mikuni V. M.; Mo D. C.; Mott P.; Nelson T.; Ni J. Q.; Nikonov N.; Nozzoli F.; Oliva A.; Orcinha M.; Palmonari F.; Palomares C.; Paniccia M.; Pauluzzi M.; Pensotti S.; Perrina C.; Phan H. D.; Picot-Clemente N.; Pilo F.; Pizzolotto C.; Plyaskin V.; Pohl M.; Poireau V.; Quadrani L.; Qi X. M.; Qin X.; Qu Z. Y.; Raeihae T.; Rancoita P. G.; Rapin D.; Ricol J. S.; Rosier-Lees S.; Rozhkov A.; Rozza D.; Sagdeev R.; Schael S.; Schmidt S. M.; von Dratzig A. Schulz; Schwering G.; Seo E. S.; Shan B. S.; Shi J. Y.; Siedenburg T.; Son D.; Song J. W.; Tacconi M.; Tang X. W.; Tang Z. C.; Tescaro D.; Ting Samuel C. C.; Ting S. M.; Tomassetti N.; Torsti J.; Turkoglu C.; Urban T.; Vagelli V.; Valente E.; Valtonen E.; Vazquez Acosta M.; Vecchi M.; Velasco M.; Vialle J. P.; Vitale V.; Vitillo S.; Wang L. Q.; Wang N. H.; Wang Q. L.; Wang X.; Wang X. Q.; Wang Z. X.; Wei C. C.; Weng Z. L.; Whitman K.; Wu H.; Wu X.; Xiong R. Q.; Xu W.; Yan Q.; Yang J.; Yang M.; Yang Y.; Yi H.; Yu Y. J.; Yu Z. Q.; Zannoni M.; Zeissler S.; Zhang C.; Zhang F.; Zhang J.; Zhang J. H.; Zhang S. W.; Zhang Z.; Zheng Z. M.; Zhuang H. L.; Zhukov V.; Zichichi A.; Zimmermann N.; Zuccon P.

首页> 外文期刊>Physical review letters >Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station

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Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station

机译：国际空间站上的Alpha磁谱仪观测高刚度He，C和O宇宙射线的相同刚度依赖性

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摘要

We report the observation of new properties of primary cosmic rays He, C, and O measured in the rigidity (momentum/charge) range 2 GV to 3 TV with 90 x 10(6) helium, 8.4 x 10(6) carbon, and 7.0 x 10(6) oxygen nuclei collected by the Alpha Magnetic Spectrometer ( AMS) during the first five years of operation. Above 60 GV, these three spectra have identical rigidity dependence. They all deviate from a single power law above 200 GV and harden in an identical way.

机译：我们报告观察到的主要宇宙射线He，C和O的新特性在90 G（10）（6）氦，8.4 X 10（6）的氦，2 GV至3 TV的刚度（动量/电荷）范围内测量在运行的头五年中，Alpha电磁光谱仪（AMS）收集到7.0 x 10（6）氧核。高于60 GV，这三个光谱具有相同的刚度依赖性。它们都偏离200 GV以上的单一功率定律，并且以相同的方式硬化。

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来源
《Physical review letters》 |2017年第25期|251101.1-251101.8|共8页
作者
Aguilar M.; Cavasonza L. Ali; Alpat B.; Ambrosi G.; Arruda L.; Attig N.; Aupetit S.; Azzarello P.; Bachlechner A.; Barao F.; Barrau A.; Barrin L.; Bartoloni A.; Basara L.; Basegmez-du Pree S.; Battarbee M.; Battiston R.; Becker U.; Behlmann M.; Beischer B.; Berdugo J.; Bertucci B.; Bindel K. F.; Bindi V.; de Boer W.; Bollweg K.; Bonnivard V.; Borgia B.; Boschini M. J.; Bourquin M.; Bueno E. F.; Burger J.; Burger W. J.; Cadoux F.; Cai X. D.; Capell M.; Caroff S.; Casaus J.; Castellini G.; Cervelli F.; Chae M. J.; Chang Y. H.; Chen A. I.; Chen G. M.; Chen H. S.; Cheng L.; Chou H. Y.; Choumilov E.; Choutko V.; Chung C. H.; Clark C.; Clavero R.; Coignet G.; Consolandi C.; Contin A.; Corti C.; Creus W.; Crispoltoni M.; Cui Z.; Dadzie K.; Dai Y. M.; Datta A.; Delgado C.; Della Torre S.; Demakov O.; Demirkoz M. B.; Derome L.; Di Falco S.; Dimiccoli F.; Diaz C.; von Doetinchem P.; Dong F.; Donnini F.; Duranti M.; DUrso D.; Egorov A.; Eline A.; Eronen T.; Feng J.; Fiandrini E.; Fisher P.; Formato V.; Galaktionov Y.; Gallucci G.; Garcia-Lopez R. J.; Gargiulo C.; Gast H.; Gebauer I.; Gervasi M.; Ghelfi A.; Giovacchini F.; Gomez-Coral D. M.; Gong J.; Goy C.; Grabski V.; Grandi D.; Graziani M.; Guo K. H.; Haino S.; Han K. C.; He Z. H.; Heil M.; Hoffman J.; Hsieh T. H.; Huang H.; Huang Z. C.; Huh C.; Incagli M.; Ionica M.; Jang W. Y.; Jia Yi; Jinchi H.; Kang S. C.; Kanishev K.; Khiali B.; Kim G. N.; Kim K. S.; Kirn Th.; Konak C.; 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.; Leluc C.; Li H. S.; Li J. Q.; Li Q.; Li T. X.; Li Y.; Li Z. H.; Li Z. Y.; Lim S.; Lin C. H.; Lipari P.; Lippert T.; Liu D.; Liu Hu; Lordello V. D.; Lu S. Q.; Lu Y. S.; Luebelsmeyer K.; Luo F.; Luo J. Z.; Lyu S. S.; Machate F.; Mana C.; Marin J.; Martin T.; Martinez G.; Masi N.; Maurin D.; Menchaca-Rocha A.; Meng Q.; Mikuni V. M.; Mo D. C.; Mott P.; Nelson T.; Ni J. Q.; Nikonov N.; Nozzoli F.; Oliva A.; Orcinha M.; Palmonari F.; Palomares C.; Paniccia M.; Pauluzzi M.; Pensotti S.; Perrina C.; Phan H. D.; Picot-Clemente N.; Pilo F.; Pizzolotto C.; Plyaskin V.; Pohl M.; Poireau V.; Quadrani L.; Qi X. M.; Qin X.; Qu Z. Y.; Raeihae T.; Rancoita P. G.; Rapin D.; Ricol J. S.; Rosier-Lees S.; Rozhkov A.; Rozza D.; Sagdeev R.; Schael S.; Schmidt S. M.; von Dratzig A. Schulz; Schwering G.; Seo E. S.; Shan B. S.; Shi J. Y.; Siedenburg T.; Son D.; Song J. W.; Tacconi M.; Tang X. W.; Tang Z. C.; Tescaro D.; Ting Samuel C. C.; Ting S. M.; Tomassetti N.; Torsti J.; Turkoglu C.; Urban T.; Vagelli V.; Valente E.; Valtonen E.; Vazquez Acosta M.; Vecchi M.; Velasco M.; Vialle J. P.; Vitale V.; Vitillo S.; Wang L. Q.; Wang N. H.; Wang Q. L.; Wang X.; Wang X. Q.; Wang Z. X.; Wei C. C.; Weng Z. L.; Whitman K.; Wu H.; Wu X.; Xiong R. Q.; Xu W.; Yan Q.; Yang J.; Yang M.; Yang Y.; Yi H.; Yu Y. J.; Yu Z. Q.; Zannoni M.; Zeissler S.; Zhang C.; Zhang F.; Zhang J.; Zhang J. H.; Zhang S. W.; Zhang Z.; Zheng Z. M.; Zhuang H. L.; Zhukov V.; Zichichi A.; Zimmermann N.; Zuccon P.;
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作者单位

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

INFN, Sez Perugia, I-06100 Perugia, Italy;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Lab Instrumenta & Fis Expt Particulas LIP, P-1000 Lisbon, Portugal;

Res Ctr Julich, Julich Supercomp Ctr, D-52425 Julich, Germany;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Lab Instrumenta & Fis Expt Particulas LIP, P-1000 Lisbon, Portugal;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

European Org Nucl Res, CERN, CH-1211 Geneva 23, Switzerland;

INFN, Sez Roma, I-00185 Rome, Italy;

INFN TIFPA, I-38123 Povo, Trento, Italy;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Univ Turku, Dept Phys & Astron, Space Res Lab, FI-20014 Turku, Finland;

INFN TIFPA, I-38123 Povo, Trento, Italy;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Karlsruhe Inst Technol, Inst Expt Teilchenphys, D-76131 Karlsruhe, Germany;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Karlsruhe Inst Technol, Inst Expt Teilchenphys, D-76131 Karlsruhe, Germany;

NASA, JSC, Jacobs Engn & Business Integra, Houston, TX 77058 USA;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

INFN, Sez Roma, I-00185 Rome, Italy;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Univ Sao Paulo, Inst Fis Sao Carlos, CP 369, BR-13560970 Sao Carlos, SP, Brazil;

MIT, Cambridge, MA 02139 USA;

INFN TIFPA, I-38123 Povo, Trento, Italy;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

CNR, IROE, I-50125 Florence, Italy;

INFN, Sez Pisa, I-56100 Pisa, Italy;

Ewha Womans Univ, Dept Phys, Seoul 120750, South Korea;

Natl Cent Univ, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

Natl Cent Univ, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

NASA, JSC, Jacobs Engn & Business Integra, Houston, TX 77058 USA;

Univ La Laguna, Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Spain;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

INFN, Sez Bologna, I-40126 Bologna, Italy;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, Inst Elect Engn, Beijing 100190, Peoples R China;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

MIT, Cambridge, MA 02139 USA;

Middle East Tech Univ, Dept Phys, TR-06800 Ankara, Turkey;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

INFN, Sez Pisa, I-56100 Pisa, Italy;

INFN TIFPA, I-38123 Povo, Trento, Italy;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

INFN, Sez Perugia, I-06100 Perugia, Italy;

INFN, Sez Perugia, I-06100 Perugia, Italy;

INFN, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Univ Turku, Dept Phys & Astron, Space Res Lab, FI-20014 Turku, Finland;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Pisa, I-56100 Pisa, Italy;

Univ La Laguna, Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Spain;

European Org Nucl Res, CERN, CH-1211 Geneva 23, Switzerland;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Karlsruhe Inst Technol, Inst Expt Teilchenphys, D-76131 Karlsruhe, Germany;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Karlsruhe Inst Technol, Inst Expt Teilchenphys, D-76131 Karlsruhe, Germany;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

NCSIST, Longtan 32546, Tao Yuan, Taiwan;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

MIT, Cambridge, MA 02139 USA;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

INFN, Sez Pisa, I-56100 Pisa, Italy;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

MIT, Cambridge, MA 02139 USA;

NCSIST, Longtan 32546, Tao Yuan, Taiwan;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

European Org Nucl Res, CERN, CH-1211 Geneva 23, Switzerland;

Natl Cent Univ, Chungli 32054, Tao Yuan, Taiwan;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Middle East Tech Univ, Dept Phys, TR-06800 Ankara, Turkey;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

European Org Nucl Res, CERN, CH-1211 Geneva 23, Switzerland;

INFN, Sez Bologna, I-40126 Bologna, Italy;

INFN TIFPA, I-38123 Povo, Trento, Italy;

MIT, Cambridge, MA 02139 USA;

Acad Sinica Grid Ctr, Taipei 11529, Taiwan;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Natl Cheng Kung Univ, Tainan 70101, Taiwan;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

INFN, Sez Roma, I-00185 Rome, Italy;

Res Ctr Julich, Julich Supercomp Ctr, D-52425 Julich, Germany;

Natl Cent Univ, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

Univ Sao Paulo, Inst Fis Sao Carlos, CP 369, BR-13560970 Sao Carlos, SP, Brazil;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

NASA, JSC, Jacobs Engn & Business Integra, Houston, TX 77058 USA;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

INFN, Sez Bologna, I-40126 Bologna, Italy;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

Univ Nacl Autonoma Mexico, Inst Fis, Mexico City 01000, DF, Mexico;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Univ Sao Paulo, Inst Fis Sao Carlos, CP 369, BR-13560970 Sao Carlos, SP, Brazil;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

NASA, JSC, Jacobs Engn & Business Integra, Houston, TX 77058 USA;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

Lab Instrumenta & Fis Expt Particulas LIP, P-1000 Lisbon, Portugal;

INFN, Sez Bologna, I-40126 Bologna, Italy;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

INFN, Sez Perugia, I-06100 Perugia, Italy;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

MIT, Cambridge, MA 02139 USA;

Univ Maryland, IPST, College Pk, MD 20742 USA;

INFN, Sez Pisa, I-56100 Pisa, Italy;

INFN, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

INFN, Sez Bologna, I-40126 Bologna, Italy;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

CNRS, IN2P3, LPSC, F-38026 Grenoble, France;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Univ Maryland, East West Ctr Space Sci, College Pk, MD 20742 USA;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Res Ctr Julich, Julich Supercomp Ctr, D-52425 Julich, Germany;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Univ Maryland, IPST, College Pk, MD 20742 USA;

Beihang Univ BUAA, Beijing 100191, Peoples R China;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

Kyungpook Natl Univ, CHEP, Daegu 41566, South Korea;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Univ La Laguna, Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Spain;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

INFN, Sez Perugia, I-06100 Perugia, Italy;

Univ Turku, Dept Phys & Astron, Space Res Lab, FI-20014 Turku, Finland;

Middle East Tech Univ, Dept Phys, TR-06800 Ankara, Turkey;

NASA, JSC, Jacobs Engn & Business Integra, Houston, TX 77058 USA;

INFN, Sez Perugia, I-06100 Perugia, Italy;

INFN, Sez Roma, I-00185 Rome, Italy;

Univ Turku, Dept Phys & Astron, Space Res Lab, FI-20014 Turku, Finland;

Univ La Laguna, Inst Astrofis Canarias, E-38205 San Cristobal la Laguna, Spain;

Univ Sao Paulo, Inst Fis Sao Carlos, CP 369, BR-13560970 Sao Carlos, SP, Brazil;

Ctr Invest Energet Medioambientales & Tecnol, E-28040 Madrid, Spain;

CNRS, IN2P3, LAPP, F-74941 Annecy Le Vieux, France;

INFN TIFPA, I-38123 Povo, Trento, Italy;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

Shandong Univ SDU, Jinan 250100, Shandong, Peoples R China;

Chinese Acad Sci, Inst Elect Engn, Beijing 100190, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Sun Yat Sen Univ, Guangzhou 510275, Guangdong, Peoples R China;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

MIT, Cambridge, MA 02139 USA;

Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Univ Geneva, DPNC, CH-1211 Geneva 4, Switzerland;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Ewha Womans Univ, Dept Phys, Seoul 120750, South Korea;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Natl Cheng Kung Univ, Tainan 70101, Taiwan;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Chinese Acad Sci, Inst Elect Engn, Beijing 100190, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

INFN, Sez Milano Bicocca, I-20126 Milan, Italy;

Karlsruhe Inst Technol, Inst Expt Teilchenphys, D-76131 Karlsruhe, Germany;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Southeast Univ SEU, Nanjing 210096, Jiangsu, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Beihang Univ BUAA, Beijing 100191, Peoples R China;

Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

INFN, Sez Bologna, I-40126 Bologna, Italy;

Rhein Westfal TH Aachen, Phys Inst, D-52056 Aachen, Germany;

MIT, Cambridge, MA 02139 USA;

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1. Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station [J] . Aguilar M., Cavasonza L. Ali, Alpat B., Physical review letters . 2017,第18a26CD期

机译：国际空间站α磁光谱仪在高刚性下观察He，C和O宇宙射线的相同刚度依赖性
2. Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV to 3 TV with the Alpha Magnetic Spectrometer on the International Space Station [J] . Aguilar M., Aisa D., Alpat B., Physical review letters . 2015,第21期

机译：在国际空间站上使用Alpha磁谱仪精确测量1.9 GV到3 TV的主要宇宙射线中的氦通量
3. Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station [J] . Aguilar M., Aisa D., Alpat B., Physical review letters . 2015,第17期

机译：在国际空间站上使用Alpha磁谱仪精确测量从刚性1 GV到1.8 TV的主要宇宙射线中的质子通量
4. The transition radiation detector of the alpha magnetic spectrometer(AMS-02) on the International Space Station and the precision measurement of the cosmic ray positron fraction [C] . Chung Chan Hoon 2013 IEEE Nuclear Science Symposium and Medical Imaging Conference . 2013

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5. Solar modulation of protons and helium in cosmic rays with the alpha magnetic spectrometer [D] . Corti, Claudio. 2017

机译：用α磁光谱仪在宇宙射线中的质子和氦的太阳能调节
6. The DNA of Bacteria of the World Ocean and the Earth in Cosmic Dust at the International Space Station [O] . T. V. Grebennikova, A. V. Syroeshkin, E. V. Shubralova, 2018

机译：国际空间站宇宙尘埃中世界海洋和地球细菌的DNA
7. Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station [O] . Aguilar, M., Ali Cavasonza, L., Alpat, B., 2017

机译：国际空间站上的Alpha磁谱仪观测高刚度He，C和O宇宙射线的相同刚度依赖性

Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station

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