文献

J-GLOBAL ID：201902284717854039   整理番号：19A0548253

国際宇宙ステーションにおけるアルファ磁気スペクトロメータによる二次宇宙線リチウム,ベリリウム及びホウ素の新しい性質の観測【JST・京大機械翻訳】

Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station

著者 (120件)： Aguilar M. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  Ali Cavasonza L. (I. Physics Institute and JARA-FAME, RWTH Aachen University, D-52056 Aachen, Germany) ,  Ambrosi G. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Arruda L. (Laboratorio de Instrumentacao e Fisica Experimental de Particulas (LIP), P-1000 Lisboa, Portugal) ,  Attig N. (Juelich Supercomputing Centre and JARA-FAME, Research Centre Juelich, D-52425 Juelich, Germany) ,  Aupetit S. (Laboratoire de Physique Subatomique et de Cosmologie (LPSC), CNRS/IN2P3 and Universite Grenoble-Alpes, F-38026 Grenoble, France) ,  Azzarello P. (DPNC, Universite de Geneve, CH-1211 Geneve 4, Switzerland) ,  Bachlechner A. (I. Physics Institute and JARA-FAME, RWTH Aachen University, D-52056 Aachen, Germany) ,  Barao F. (Laboratorio de Instrumentacao e Fisica Experimental de Particulas (LIP), P-1000 Lisboa, Portugal) ,  Barrau A. (Laboratoire de Physique Subatomique et de Cosmologie (LPSC), CNRS/IN2P3 and Universite Grenoble-Alpes, F-38026 Grenoble, France) ,  Barrin L. (European Organization for Nuclear Research (CERN), CH-1211 Geneva 23, Switzerland) ,  Bartoloni A. (INFN Sezione di Roma 1, I-00185 Roma, Italy) ,  Basara L. (INFN TIFPA, I-38123 Povo, Trento, Italy) ,  Basegmez-du Pree S. (Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing 100049, China) ,  Battarbee M. (Space Research Laboratory, Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland) ,  Battiston R. (INFN TIFPA, I-38123 Povo, Trento, Italy) ,  Battiston R. (Universita di Trento, I-38123 Povo, Trento, Italy) ,  Becker U. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Behlmann M. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Beischer B. (I. Physics Institute and JARA-FAME, RWTH Aachen University, D-52056 Aachen, Germany) ,  Berdugo J. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  Bertucci B. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Bertucci B. (Universita di Perugia, I-06100 Perugia, Italy) ,  Bindel K. F. (Institut fuer Experimentelle Teilchenphysik, Karlsruhe Institute of Technology (KIT), D-76131 Karlsruhe, Germany) ,  Bindi V. (Physics and Astronomy Department, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  de Boer W. (Institut fuer Experimentelle Teilchenphysik, Karlsruhe Institute of Technology (KIT), D-76131 Karlsruhe, Germany) ,  Bollweg K. (National Aeronautics and Space Administration Johnson Space Center (JSC), Jacobs Engineering, and Business Integra, Houston, Texas 77058, USA) ,  Bonnivard V. (Laboratoire de Physique Subatomique et de Cosmologie (LPSC), CNRS/IN2P3 and Universite Grenoble-Alpes, F-38026 Grenoble, France) ,  Borgia B. (INFN Sezione di Roma 1, I-00185 Roma, Italy) ,  Borgia B. (Universita di Roma La Sapienza, I-00185 Roma, Italy) ,  Boschini M. J. (INFN Sezione di Milano-Bicocca, I-20126 Milano, Italy) ,  Bourquin M. (DPNC, Universite de Geneve, CH-1211 Geneve 4, Switzerland) ,  Bueno E. F. (Instituto de Fisica de Sao Carlos, Universidade de Sao Paulo, CP 369, 13560-970 Sao Carlos, Sao Paulo, SP, Brazil) ,  Burger J. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Burger W. J. (INFN TIFPA, I-38123 Povo, Trento, Italy) ,  Cadoux F. (DPNC, Universite de Geneve, CH-1211 Geneve 4, Switzerland) ,  Cai X. D. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Capell M. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Caroff S. (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), CNRS/IN2P3 and Universite Savoie Mont Blanc, F-74941 Annecy-le-Vieux, France) ,  Casaus J. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  Castellini G. (CNR-IROE, I-50125 Firenze, Italy) ,  Cervelli F. (INFN Sezione di Pisa, I-56100 Pisa, Italy) ,  Chae M. J. (Department of Physics, Ewha Womans University, Seoul 120-750, Korea) ,  Chang Y. H. (National Central University (NCU), Chung-Li, Tao Yuan 32054, Taiwan) ,  Chen A. I. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Chen G. M. (Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing 100049, China) ,  Chen H. S. (Institute of High Energy Physics (IHEP), Chinese Academy of Sciences, Beijing 100049, China) ,  Chen H. S. (University of Chinese Academy of Sciences (UCAS), Beijing 100049, China) ,  Cheng L. (Shandong University (SDU), Jinan, Shandong 250100, China) ,  Chou H. Y. (National Central University (NCU), Chung-Li, Tao Yuan 32054, Taiwan) ,  Choumilov E. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Choutko V. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Chung C. H. (I. Physics Institute and JARA-FAME, RWTH Aachen University, D-52056 Aachen, Germany) ,  Clark C. (National Aeronautics and Space Administration Johnson Space Center (JSC), Jacobs Engineering, and Business Integra, Houston, Texas 77058, USA) ,  Clavero R. (Instituto de Astrofisica de Canarias (IAC), E-38205 La Laguna, and Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain) ,  Coignet G. (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), CNRS/IN2P3 and Universite Savoie Mont Blanc, F-74941 Annecy-le-Vieux, France) ,  Consolandi C. (Physics and Astronomy Department, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Contin A. (INFN Sezione di Bologna, I-40126 Bologna, Italy) ,  Contin A. (Universita di Bologna, I-40126 Bologna, Italy) ,  Corti C. (Physics and Astronomy Department, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Creus W. (Institute of Physics, Academia Sinica, Nankang, Taipei 11529, Taiwan) ,  Crispoltoni M. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Crispoltoni M. (Universita di Perugia, I-06100 Perugia, Italy) ,  Cui Z. (Shandong University (SDU), Jinan, Shandong 250100, China) ,  Dadzie K. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Dai Y. M. (Institute of Electrical Engineering (IEE), Chinese Academy of Sciences, Beijing 100190, China) ,  Datta A. (Physics and Astronomy Department, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Delgado C. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  Della Torre S. (INFN Sezione di Milano-Bicocca, I-20126 Milano, Italy) ,  Demirkoz M. B. (Department of Physics, Middle East Technical University (METU), 06800 Ankara, Turkey) ,  Derome L. (Laboratoire de Physique Subatomique et de Cosmologie (LPSC), CNRS/IN2P3 and Universite Grenoble-Alpes, F-38026 Grenoble, France) ,  Di Falco S. (INFN Sezione di Pisa, I-56100 Pisa, Italy) ,  Dimiccoli F. (INFN TIFPA, I-38123 Povo, Trento, Italy) ,  Dimiccoli F. (Universita di Trento, I-38123 Povo, Trento, Italy) ,  Diaz C. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  von Doetinchem P. (Physics and Astronomy Department, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Dong F. (Southeast University (SEU), Nanjing 210096, China) ,  Donnini F. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Donnini F. (Universita di Perugia, I-06100 Perugia, Italy) ,  Duranti M. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  D’Urso D. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Egorov A. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Eline A. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Eronen T. (Space Research Laboratory, Department of Physics and Astronomy, University of Turku, FI-20014 Turku, Finland) ,  Feng J. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Fiandrini E. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Fiandrini E. (Universita di Perugia, I-06100 Perugia, Italy) ,  Fisher P. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Formato V. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Galaktionov Y. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Gallucci G. (INFN Sezione di Pisa, I-56100 Pisa, Italy) ,  Garcia-Lopez R. J. (Instituto de Astrofisica de Canarias (IAC), E-38205 La Laguna, and Departamento de Astrofisica, Universidad de La Laguna, E-38206 La Laguna, Tenerife, Spain) ,  Gargiulo C. (European Organization for Nuclear Research (CERN), CH-1211 Geneva 23, Switzerland) ,  Gast H. (I. Physics Institute and JARA-FAME, RWTH Aachen University, D-52056 Aachen, Germany) ,  Gebauer I. (Institut fuer Experimentelle Teilchenphysik, Karlsruhe Institute of Technology (KIT), D-76131 Karlsruhe, Germany) ,  Gervasi M. (INFN Sezione di Milano-Bicocca, I-20126 Milano, Italy) ,  Gervasi M. (Universita di Milano-Bicocca, I-20126 Milano, Italy) ,  Ghelfi A. (Laboratoire de Physique Subatomique et de Cosmologie (LPSC), CNRS/IN2P3 and Universite Grenoble-Alpes, F-38026 Grenoble, France) ,  Giovacchini F. (Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas (CIEMAT), E-28040 Madrid, Spain) ,  Gomez-Coral D. M. (Instituto de Fisica, Universidad Nacional Autonoma de Mexico (UNAM), Mexico, D. F. 01000, Mexico) ,  Gong J. (Southeast University (SEU), Nanjing 210096, China) ,  Goy C. (Laboratoire d’Annecy-le-Vieux de Physique des Particules (LAPP), CNRS/IN2P3 and Universite Savoie Mont Blanc, F-74941 Annecy-le-Vieux, France) ,  Grabski V. (Instituto de Fisica, Universidad Nacional Autonoma de Mexico (UNAM), Mexico, D. F. 01000, Mexico) ,  Grandi D. (INFN Sezione di Milano-Bicocca, I-20126 Milano, Italy) ,  Graziani M. (Institut fuer Experimentelle Teilchenphysik, Karlsruhe Institute of Technology (KIT), D-76131 Karlsruhe, Germany) ,  Guo K. H. (Sun Yat-Sen University (SYSU), Guangzhou 510275, China) ,  Haino S. (Institute of Physics, Academia Sinica, Nankang, Taipei 11529, Taiwan) ,  Han K. C. (National Chung-Shan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan 32546, Taiwan) ,  He Z. H. (Sun Yat-Sen University (SYSU), Guangzhou 510275, China) ,  Heil M. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Hsieh T. H. (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Huang H. (Institute of Physics, Academia Sinica, Nankang, Taipei 11529, Taiwan) ,  Huang Z. C. (Sun Yat-Sen University (SYSU), Guangzhou 510275, China) ,  Huh C. (CHEP, Kyungpook National University, 41566 Daegu, Korea) ,  Incagli M. (INFN Sezione di Pisa, I-56100 Pisa, Italy) ,  Ionica M. (INFN Sezione di Perugia, I-06100 Perugia, Italy) ,  Jang W. Y. (CHEP, Kyungpook National University, 41566 Daegu, Korea) ,  Jia Yi (Massachusetts Institute of Technology (MIT), Cambridge, Massachusetts 02139, USA) ,  Jinchi H. (National Chung-Shan Institute of Science and Technology (NCSIST), Longtan, Tao Yuan 32546, Taiwan) ,  Kang S. C. (CHEP, Kyungpook National University, 41566 Daegu, Korea)
資料名： Physical Review Letters  (Physical Review Letters)
巻： 120  号： 2  ページ： 021101  発行年： 2018年 
JST資料番号： H0070A  ISSN： 0031-9007  CODEN： PRLTAO  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： アメリカ合衆国 (USA)  言語： 英語 (EN)

抄録/ポイント： 国際宇宙ステーションに搭載されている最初の5年間に,AMSによって収集された[数式:原文を参照]核を用いて,1.9GVから3.3TVまでの剛性(単位電荷当たりの運動量)で測定された二次宇宙線Li,Be,およびBの新しい特性の観測について報告する。LiとBフラックスは7GV以上で同一の剛性依存性を有し,3つのフラックスは[数式:原文を参照]の[数式:原文を参照]フラックス比とともに30GV以上で同じ剛性依存性を有した。3つのフラックスは同じ方法で200GV以上の単一べき乗則から逸脱する。二次宇宙線のこの挙動は,一次宇宙線He,C,およびOのAMS測定でも観測されたが,一次宇宙線と二次宇宙線の剛性依存性は明確に異なっている。特に,200GV以上では,二次宇宙線は一次宇宙線よりも多くなる。Copyright 2019 The American Physical Society All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： *磁気スペクトロメータ ,  *ベリリウム ,  *リチウム ,  *二次宇宙線 ,  *ホウ素 ,  運動量 ,  剛性 ,  一次宇宙線 ,  電荷
準シソーラス用語： べき乗則 ,  流量比 ,  *国際宇宙ステーション , 【Automatic Indexing@JST】

分類 (1件)： 宇宙線起源  (DB02020Q)

タイトルに関連する用語 (8件)： 宇宙ステーション ,  磁気スペクトロメータ ,  二次宇宙線 ,  リチウム ,  ベリリウム ,  ホウ素 ,  性質 ,  観測