文献

J-GLOBAL ID：201802224187588488   整理番号：18A1425480

下向き雷リーダーとの同時計数における地上レベルで観測されたガンマ線シャワー【JST・京大機械翻訳】

Gamma Ray Showers Observed at Ground Level in Coincidence With Downward Lightning Leaders

著者 (120件)： Abbasi R. U. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Abu-Zayyad T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Allen M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Barcikowski E. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Belz J. W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Bergman D. R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Blake S. A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Byrne M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Cady R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Cheon B.G. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seoul, Korea) ,  Chiba J. (Department of Physics, Tokyo University of Science, Noda, Japan) ,  Chikawa M. (Department of Physics, Kinki University, Higashi-osaka, Japan) ,  Fujii T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Fukushima M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Fukushima M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, The University of Tokyo, Kashiwa, Japan) ,  Furlich G. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Goto T. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Hanlon W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Hayashi Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Yokohama, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Japan) ,  Ikeda D. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Inoue N. (The Graduate School of Science and Engineering, Saitama University, Saitama, Japan) ,  Ishii T. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Japan) ,  Ito H. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Japan) ,  Ivanov D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Jeong S. (Department of Physics, Sungkyunkwan University, Suwon, Korea) ,  Jui C. C. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Kadota K. (Department of Physics, Tokyo City University, Tokyo, Japan) ,  Kakimoto F. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Tokyo, Japan) ,  Kalashev O. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Kasahara K. (Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan) ,  Kawai H. (Department of Physics, Chiba University, Chiba, Japan) ,  Kawakami S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Kido E. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Kim H. B. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seoul, Korea) ,  Kim J. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Kim J. H. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, Ulsan, Korea) ,  Kishigami S. S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Krehbiel P. R. (Langmuir Laboratory for Atmospheric Research, New Mexico Institute of Mining and Technology, Socorro, NM, USA) ,  Kuzmin V. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Kwon Y. J. (Department of Physics, Yonsei University, Seoul, Korea) ,  Lan J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  LeVon R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Lundquist J. P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Machida K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, The University of Tokyo, Kashiwa, Japan) ,  Matuyama T. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Matthews J. N. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Minamino M. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Mukai K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Japan) ,  Myers I. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Japan) ,  Nakamura R. (Department of Computer Science and Engineering, Shinshu University, Nagano, Japan) ,  Nakamura T. (Faculty of Science, Kochi University, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Ogio S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Ohoka H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Oki K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Kusatsu, Japan) ,  Ono M. (Department of Physics, Kyushu University, Fukuoka, Japan) ,  Onogi R. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Oshima A. (Engineering Science Laboratory, Chubu University, Kasugai, Japan) ,  Ozawa S. (Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan) ,  Park I. H. (Department of Physics, Sungkyunkwan University, Suwon, Korea) ,  Pshirkov M. S. (Department of Physics, Tokyo City University, Tokyo, Japan) ,  Pshirkov M. S. (Sternberg Astronomical Institute Moscow M.V.Lomonosov State University, Moscow, Russia) ,  Remington J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Rison W. (Langmuir Laboratory for Atmospheric Research, New Mexico Institute of Mining and Technology, Socorro, NM, USA) ,  Rodeheffer D. (Langmuir Laboratory for Atmospheric Research, New Mexico Institute of Mining and Technology, Socorro, NM, USA) ,  Rodriguez D. C. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Rubtsov G. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Ryu D. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, Ulsan, Korea) ,  Sagawa H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Saito K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Sakaki N. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Seki T. (Department of Computer Science and Engineering, Shinshu University, Nagano, Japan) ,  Sekino K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Shah P.D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Shibata F. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Japan) ,  Shibata T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Shimodaira H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Shin B. K. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Shin H. S. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Smith J. D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Sokolsky P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Springer R. W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Stokes B. T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Stroman T. A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Takai H. (Brookhaven National Laboratory, Upton, NY, USA) ,  Takeda M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Takeishi R. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Taketa A. (Earthquake Research Institute, University of Tokyo, Tokyo, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Japan) ,  Tameda Y. (Department of Engineering Science, Faculty of Engineering, Osaka Electro-Communication University, Neyagawa, Japan) ,  Tanaka H. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Tanaka K. (Graduate School of Information Sciences, Hiroshima City University, Hiroshima, Japan) ,  Tanaka M. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Japan) ,  Thomas R. J. (Langmuir Laboratory for Atmospheric Research, New Mexico Institute of Mining and Technology, Socorro, NM, USA) ,  Thomas S. B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Thomson G. B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Tinyakov P. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Tinyakov P. (Universite Libre de Bruxelles, Brussels, Belgium) ,  Tkachev I. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Tokuno H. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Tokyo, Japan) ,  Tomida T. (Department of Computer Science and Engineering, Shinshu University, Nagano, Japan) ,  Troitsky S. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Tsunesada Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Uchihori Y. (National Institute of Radiological Science, Chiba, Japan) ,  Udo S. (Faculty of Engineering, Kanagawa University, Yokohama, Japan) ,  Urban F. (Universite Libre de Bruxelles, Brussels, Belgium) ,  Vasiloff G. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Wong T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA) ,  Yamamoto M. (Department of Computer Science and Engineering, Shinshu University, Nagano, Japan) ,  Yamane R. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Yamaoka H. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Japan)
資料名： Journal of Geophysical Research: Atmospheres  (Journal of Geophysical Research: Atmospheres)
巻： 123  号： 13  ページ： 6864-6879  発行年： 2018年 
JST資料番号： C0294B  ISSN： 2169-897X  CODEN： JGREA2  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： ガンマ線シャワーのバーストは,望遠鏡アレイ表面検出器(TASD)による雷放電における下向き伝搬負リーダと一致して観測された。TASDは米国南西部に位置する700km2宇宙線観測所である。2014年と2016年の間に収集されたデータにおいて,3つのシャワー生成フラッシュの構造と時間的発達を示す相関観測を,3D電光マッピングアレイで得た。そして,TASDと共配置された両方のケースにおいて,追加の7つのフラッシュに対して電場変化測定を得た。また,国家雷検出ネットワーク情報を全体的に使用した。シャワーは数百マイクロ秒の時間間隔にわたって2~5の短期間(≦10μs)バーストのシーケンスに到着し,雲から地上への落雷の開始における下向きの負のリーダ破壊の最初の1~2msの間に地上レベルの約3~5kmの高度で生じた。シャワーフットプリント,関連波形および大気伝搬の影響は,シャワーが主に下向きビーム化ガンマ線から成ることを示した。これはGEANTシミュレーション研究により支持され,16°半角度ビームに対する約10~12~10~14光子の一次源フラックスを示した。著者らは,シャワーが衛星によって観測されたものと類似しているが,地上観測が時間的なソース活動をより代表しており,衛星観測より敏感であり,最も強力な地上ガンマ線フラッシュを検出することを結論した。Copyright 2018 Wiley Publishing Japan K.K. All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 雷放電 ,  検出器 ,  ネットワーク ,  *シャワー ,  *γ線 ,  *同時計数 ,  バースト ,  光子 ,  三次元 ,  電場 ,  シミュレーション ,  宇宙線 ,  望遠鏡
準シソーラス用語： 衛星観測 ,  地上観測 , 【Automatic Indexing@JST】

分類 (3件)： その他の気象  (DC05130I) ,  放電一般  (BJ03010I) ,  宇宙線・天体物理観測技術  (DB01000N)

タイトルに関連する用語 (7件)： 雷 ,  リーダー ,  同時計数 ,  地上 ,  観測 ,  ガンマ線 ,  シャワー