Art

J-GLOBAL ID：201902263119307034   Reference number：19A0548585

Evaluation of the Interplanetary Magnetic Field Strength Using the Cosmic-Ray Shadow of the Sun

太陽の宇宙線影を用いた惑星間磁場強度の評価【JST・京大機械翻訳】

Author (91)： Amenomori M. (Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan) ,  Bi X. J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Chen D. (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China) ,  Chen T. L. (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Chen W. Y. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Cui S. W. (Department of Physics, Hebei Normal University, Shijiazhuang 050016, China) ,  Danzengluobu (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Ding L. K. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Feng C. F. (Department of Physics, Shandong University, Jinan 250100, China) ,  Feng Zhaoyang (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Feng Z. Y. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Gou Q. B. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Guo Y. Q. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  He H. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  He Z. T. (Department of Physics, Hebei Normal University, Shijiazhuang 050016, China) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Hotta N. (Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan) ,  Hu Haibing (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Hu H. B. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Huang J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Jia H. Y. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Jiang L. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Kajino F. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Kasahara K. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Katayose Y. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Kato C. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Kozai M. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Kozai M. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210, Japan) ,  Labaciren (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Le G. M. (National Center for Space Weather, China Meteorological Administration, Beijing 100081, China) ,  Li A. F. (School of Information Science and Engineering, Shandong Agriculture University, Taian 271018, China) ,  Li A. F. (Department of Physics, Shandong University, Jinan 250100, China) ,  Li A. F. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Li H. J. (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Li W. J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Li W. J. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Liu C. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Liu J. S. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Liu M. Y. (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Lu H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Meng X. R. (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Miyazaki T. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Mizutani K. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Mizutani K. (Saitama University, Saitama 338-8570, Japan) ,  Munakata K. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Nakajima T. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Nakamura Y. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Nanjo H. (Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan) ,  Nishizawa M. (National Institute of Informatics, Tokyo 101-8430, Japan) ,  Niwa T. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Ohta I. (Sakushin Gakuin University, Utsunomiya 321-3295, Japan) ,  Ozawa S. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Qian X. L. (Department of Physics, Shandong University, Jinan 250100, China) ,  Qian X. L. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Qu X. B. (College of Science, China University of Petroleum, Qingdao 266555, China) ,  Saito T. (Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan) ,  Saito T. Y. (Max-Planck-Institut fuer Physik, Muenchen D-80805, Deutschland) ,  Sakata M. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Sako T. K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Sako T. K. (Escuela de Ciencias Fisicas y Nanotechnologia, Yachay Tech, Imbabura 100115, Ecuador) ,  Shao J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Shao J. (Department of Physics, Shandong University, Jinan 250100, China) ,  Shibata M. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Shiomi A. (College of Industrial Technology, Nihon University, Narashino 275-8576, Japan) ,  Shirai T. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Sugimoto H. (Shonan Institute of Technology, Fujisawa 251-8511, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Tan Y. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Tateyama N. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Torii S. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Tsuchiya H. (Japan Atomic Energy Agency, Tokai-mura 319-1195, Japan) ,  Udo S. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Wang H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Wu H. R. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Xue L. (Department of Physics, Shandong University, Jinan 250100, China) ,  Yamamoto Y. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Yamauchi K. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Yang Z. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Yuan A. F. (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Yuda T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Zhai L. M. (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China) ,  Zhang H. M. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang J. L. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang X. Y. (Department of Physics, Shandong University, Jinan 250100, China) ,  Zhang Y. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang Yi (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang Ying (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhaxisangzhu (Department of Mathematics and Physics, Tibet University, Lhasa 850000, China) ,  Zhou X. X. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China)
Material： Physical Review Letters  (Phys Rev Lett)
Volume： 120  Issue： 3  Page： 031101  Publication year： 2018 
JST Material Number： H0070A  ISSN： 0031-9007  CODEN： PRLTAO  Document type： Article
Article type： 原著論文  Country of issue： United States (USA)  Language： ENGLISH (EN)

Abstract/Point： We analyze the Sun’s shadow ob...

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Thesaurus term： *interplanetary magnetic field ,  cosmic ray ,  air shower ,  circular plate ,  *sun ,  solar magnetic field ,  model prediction ,  Numerical Simulation
Semi thesaurus term： 定量的評価 , 【Automatic Indexing@JST】

JST classification (3)： Solar cell  (NC03084O) ,  Experimental tests and observations of gravitational theory  (BA07040Q) ,  Electromagnetic and unified gauge fields  (BF02020A)

Terms in the title (5)： 太陽 ,  宇宙線 ,  影 ,  惑星間磁場 ,  評価