Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with 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.; Cai X. D.; Capell M.; Caroff S.; Casaus J.; Castellini G.; Cervelli F.; Chang Y. H.; Chen A. I.; Chen G. M.; Chen H. S.; Chen Y.; 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.; Demirkoz M. B.; Derome L.; Di Falco S.; Dimiccoli F.; Diaz C.; von Doetinchem P.; Dong F.; Donnini F.; Duranti M.; 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.; Hsieh T. H.; Huang H.; Huang Z. C.; Incagli M.; Jia Yi; Jinchi H.; Kanishev K.; Khiali B.; 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 Z. H.; Li Z. Y.; Lin C. H.; Lipari P.; Lippert T.; Liu D.; Liu Hu; Liu Z.; 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.; Mussolin L.; Nelson T.; Ni J. Q.; Nikonov N.; Nozzoli F.; Oliva A.; Orcinha M.; Palermo M.; Palmonari F.; Palomares C.; Paniccia M.; Pauluzzi M.; Pensotti S.; Perrina C.; Phan H. D.; Picot-Clemente N.; Pilo F.; 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.; Song J. W.; Tacconi M.; Tang X. W.; Tang Z. C.; Tescaro D.; Tian J.; Ting Samuel C. C.; Ting S. M.; Tomassetti N.; Torsti J.; Urban T.; Vagelli V.; Valente E.; Valtonen E.; Vazquez 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 C. C.; Wei J.; Weng Z. L.; Whitman K.; Wu H.; Xiong R. Q.; Xu W.; Yan Q.; 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 >Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station

【24h】

Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station

机译：国际空间站上的阿尔法磁谱仪精确测量宇宙射线氮及其主要和次要成分

获取原文

获取原文并翻译 | 示例

掌桥外文数据库（机构版） >>

开具论文收录证明 >>

文献代查 >>

页面导航

摘要
著录项
相似文献
相关主题

摘要

A precision measurement of the nitrogen flux with rigidity (momentum per unit charge) from 2.2 GV to 3.3 TV based on 2.2 x 10(6) events is presented. The detailed rigidity dependence of the nitrogen flux spectral index is presented for the first time. The spectral index rapidly hardens at high rigidities and becomes identical to the spectral indices of primary He, C, and O cosmic rays above similar to 700 GV. We observed that the nitrogen flux Phi(N) can be presented as the sum of its primary component Phi(P)(N) and secondary component Phi(S)(N), Phi(N) = Phi(P)(N) + Phi(S)(N), and we found Phi(N) is well described by the weighted sum of the oxygen flux Phi(O) (primary cosmic rays) and the boron flux Phi(B) (secondary cosmic rays), with Phi(P)(N) = (0.090 +/- 0.002) x Phi(O) and Phi(S)(N) = (0.62 +/- 0.02) x Phi(B) over the entire rigidity range. This corresponds to a change of the contribution of the secondary cosmic ray component in the nitrogen flux from 70% at a few GV to 30% above 1 TV.

机译：提出了基于2.2 x 10（6）事件的从2.2 GV到3.3 TV的具有刚性（每单位电荷动量）的氮通量的精确测量。首次给出了氮通量光谱指数与刚性的关系。光谱指数在高刚度下迅速硬化，并变得与高于700 GV的主要He，C和O宇宙射线的光谱指数相同。我们观察到氮通量Phi（N）可以表示为其主要成分Phi（P）（N）和次要成分Phi（S）（N）之和，Phi（N）= Phi（P）（N） + Phi（S）（N），我们发现Phi（N）由氧气通量Phi（O）（一次宇宙射线）和硼通量Phi（B）（二次宇宙线）的加权和很好地描述了，在整个刚性范围内，Phi（P）（N）=（0.090 +/- 0.002）x Phi（O）和Phi（S）（N）=（0.62 +/- 0.02）x Phi（B）。这对应于二次宇宙射线分量在氮通量中的贡献从几GV时的70％变为高于1 TV时的<30％。

著录项

来源
《Physical review letters》 |2018年第5期|051103.1-051103.8|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.; Cai X. D.; Capell M.; Caroff S.; Casaus J.; Castellini G.; Cervelli F.; Chang Y. H.; Chen A. I.; Chen G. M.; Chen H. S.; Chen Y.; 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.; Demirkoz M. B.; Derome L.; Di Falco S.; Dimiccoli F.; Diaz C.; von Doetinchem P.; Dong F.; Donnini F.; Duranti M.; 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.; Hsieh T. H.; Huang H.; Huang Z. C.; Incagli M.; Jia Yi; Jinchi H.; Kanishev K.; Khiali B.; 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 Z. H.; Li Z. Y.; Lin C. H.; Lipari P.; Lippert T.; Liu D.; Liu Hu; Liu Z.; 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.; Mussolin L.; Nelson T.; Ni J. Q.; Nikonov N.; Nozzoli F.; Oliva A.; Orcinha M.; Palermo M.; Palmonari F.; Palomares C.; Paniccia M.; Pauluzzi M.; Pensotti S.; Perrina C.; Phan H. D.; Picot-Clemente N.; Pilo F.; 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.; Song J. W.; Tacconi M.; Tang X. W.; Tang Z. C.; Tescaro D.; Tian J.; Ting Samuel C. C.; Ting S. M.; Tomassetti N.; Torsti J.; Urban T.; Vagelli V.; Valente E.; Valtonen E.; Vazquez 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 C. C.; Wei J.; Weng Z. L.; Whitman K.; Wu H.; Xiong R. Q.; Xu W.; Yan Q.; 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.;
展开▼
作者单位

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

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

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

Res Ctr Julich, Julich Supercompu 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 1, D-52056 Aachen, Germany;

Lab Instrumentacao & 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;

Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy;

Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Trento, Italy;

METU, Dept Phys, TR-06800 Ankara, Turkey;

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

Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Trento, Italy;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

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

Ist Nazl Fis Nucl, 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;

Jacobs Engn & Business Integra, Natl Aeronaut & Space Adm Johnson Space Ctr ( JS, Houston, TX 77058 USA;

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

Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy;

Ist Nazl Fis Nucl, 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 Paulo, SP, Brazil;

MIT, Cambridge, MA 02139 USA;

Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Trento, Italy;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

CNRS IN2P3, LAPP, F-74000 Annecy, France;

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

CNR IROE, I-50125 Florence, Italy;

Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy;

NCU, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

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

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

NCU, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Jacobs Engn & Business Integra, Natl Aeronaut & Space Adm Johnson Space Ctr ( JS, Houston, TX 77058 USA;

IAC, E-38205 San Cristobal la Laguna, Spain;

CNRS IN2P3, LAPP, F-74000 Annecy, France;

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

Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy;

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

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

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

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, IEE, Beijing 100190, Peoples R China;

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

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

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

METU, Dept Phys, TR-06800 Ankara, Turkey;

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

Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy;

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

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

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

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

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

Ist Nazl Fis Nucl, 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;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy;

IAC, E-38205 San Cristobal la Laguna, Spain;

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

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

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

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

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

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

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

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

CNRS IN2P3, LAPP, F-74000 Annecy, France;

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

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

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

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

NCSIST, Longtan 32546, Tao Yuan, Taiwan;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy;

MIT, Cambridge, MA 02139 USA;

NCSIST, Longtan 32546, Tao Yuan, Taiwan;

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

NCU, Chungli 32054, Tao Yuan, Taiwan;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

METU, 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;

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

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

Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy;

Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Trento, Italy;

MIT, Cambridge, MA 02139 USA;

ASGC, 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;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy;

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

NCU, Chungli 32054, Tao Yuan, Taiwan;

MIT, Cambridge, MA 02139 USA;

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

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

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

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

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

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

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

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

Jacobs Engn & Business Integra, Natl Aeronaut & Space Adm Johnson Space Ctr ( JS, Houston, TX 77058 USA;

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

Ist Nazl Fis Nucl, 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 Paulo, SP, Brazil;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Jacobs Engn & Business Integra, Natl Aeronaut & Space Adm Johnson Space Ctr ( JS, Houston, TX 77058 USA;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

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

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Ist Nazl Fis Nucl, TIFPA, I-38123 Povo, Trento, Italy;

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

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

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

Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy;

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

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

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

Ist Nazl Fis Nucl, 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;

Ist Nazl Fis Nucl, Sez Pisa, I-56100 Pisa, Italy;

MIT, Cambridge, MA 02139 USA;

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

CNRS IN2P3, LAPP, F-74000 Annecy, France;

Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Ist Nazl Fis Nucl, 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-74000 Annecy, France;

MIT, Cambridge, MA 02139 USA;

Ist Nazl Fis Nucl, 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 1, D-52056 Aachen, Germany;

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

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Rhein Westfal TH Aachen, Phys Inst 1, 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 1, D-52056 Aachen, Germany;

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

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

IAC, E-38205 San Cristobal la Laguna, Spain;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

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

Jacobs Engn & Business Integra, Natl Aeronaut & Space Adm Johnson Space Ctr ( JS, Houston, TX 77058 USA;

Ist Nazl Fis Nucl, Sez Perugia, I-06100 Perugia, Italy;

Ist Nazl Fis Nucl, Sez Roma 1, I-00185 Rome, Italy;

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

IAC, E-38205 San Cristobal la Laguna, Spain;

Univ Groningen, KVI Ctr Adv Radiat Technol, NL-9700 AB Groningen, Netherlands;

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

CNRS IN2P3, LAPP, F-74000 Annecy, France;

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

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

Chinese Acad Sci, IEE, Beijing 100190, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

SYSU, Guangzhou 510275, Guangdong, Peoples R China;

Acad Sinica, Inst Phys, Taipei 11529, Taiwan;

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

MIT, Cambridge, MA 02139 USA;

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

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

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

MIT, Cambridge, MA 02139 USA;

MIT, Cambridge, MA 02139 USA;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Natl Cheng Kung Univ, Tainan 70101, Taiwan;

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

Chinese Acad Sci, IEE, Beijing 100190, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Ist Nazl Fis Nucl, Sez Milano Bicocca, I-20126 Milan, Italy;

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

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

MIT, Cambridge, MA 02139 USA;

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

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

MIT, Cambridge, MA 02139 USA;

Beihang Univ BUAA, Beijing 100191, Peoples R China;

Chinese Acad Sci, IHEP, Beijing 100049, Peoples R China;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy;

Rhein Westfal TH Aachen, Phys Inst 1, D-52056 Aachen, Germany;

MIT, Cambridge, MA 02139 USA;

展开▼
收录信息
原文格式 PDF
正文语种 eng
中图分类
关键词

相似文献

外文文献
中文文献
专利

1. Precision measurement of the proton and helium flux in primary cosmic rays with the Alpha Magnetic Spectrometer on the International Space Station [J] . M. Heil EPJ Web of Conferences . 2016,第12期

机译：使用国际空间站上的Alpha电磁光谱仪精确测量一次宇宙射线中的质子和氦通量
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

机译：国际空间站的α磁谱仪（AMS-02）的过渡辐射探测器和宇宙射线正电子分数的精确测量
5. Interfacing the Liquid Sampling: Atmospheric Pressure Glow Discharge Ion Source with Orbitrap Mass Spectrometers for High Accuracy High Precision Isotope Ratio Measurements of Uranium [D] . Hoegg, Edward Dexter. 2018

机译：接口液体采样：大气压辉光放电离子源，具有抗纤维素的高精度高精度同位素比率测量铀
6. Bubble-detector measurements of neutron radiation in the international space station: ISS-34 to ISS-37 [O] . M. B. Smith, S. Khulapko, H. R. Andrews, -1

机译：国际空间站中子辐射的气泡探测器测量：ISS-34至ISS-37
7. Precision Measurement of the Proton Flux in Primary Cosmic Rays from 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station [O] . Vitaly Choutko 2016

机译：在国际空间站上的α磁光谱仪从1 GV到1.8电视的初级宇宙射线中质子通量的精确测量

Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station

摘要

著录项

相似文献

相关主题

期刊订阅