文献

J-GLOBAL ID：201902263119307034   整理番号：19A0548585

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】

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

著者 (91件)： 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)
資料名： Physical Review Letters  (Physical Review Letters)
巻： 120  号： 3  ページ： 031101  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： 著者らは,チベット-III空気シャワーアレイで観測された太陽の影を解析し,影の中心が「離れた」(「離れた」惑星間磁場(IMF)セクター)の光学的太陽円盤中心から北向きにずれることを見出した。太陽磁場モデルに基づく数値シミュレーションと比較することにより,離れた(方向に向かう)セクターにおける平均IMF強度はモデル予測よりも[数式:原文を参照]([数式:原文を参照])時間が大きいことを見出した。これらの結果は,観測された太陽の影が平均太陽磁場の定量的評価のための有用なツールであることを示している。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： *惑星間磁場 ,  宇宙線 ,  空気シャワー ,  円板 ,  *太陽 ,  太陽磁場 ,  モデル予測 ,  数値シミュレーション
準シソーラス用語： 定量的評価 , 【Automatic Indexing@JST】

分類 (3件)： 太陽電池  (NC03084O) ,  重力理論の実験的試験及び観測  (BA07040Q) ,  電磁場と統一ゲージ場  (BF02020A)

タイトルに関連する用語 (5件)： 太陽 ,  宇宙線 ,  影 ,  惑星間磁場 ,  評価