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J-GLOBAL ID：201802247940528010   整理番号：18A0287187

宇宙線により誘起された空気シャワーのレーダ断面積に対する最初の上限【Powered by NICT】

First upper limits on the radar cross section of cosmic-ray induced extensive air showers

著者 (120件)： Abbasi R.U. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Abe M. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Abou Bakr Othman M. (Department of Electrical and Computer Engineering, University of Utah, Salt Lake City, Utah, USA) ,  Abu-Zayyad T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Allen M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Anderson R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Azuma R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Barcikowski E. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Belz J.W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Bergman D.R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Besson D. (University of Kansas, Lawrence, Kansas, USA) ,  Besson D. (Moscow Engineering and Physics Institute, Moscow, Russia) ,  Blake S.A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Byrne M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Cady R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Chae M.J. (Department of Physics and Institute for the Early Universe, Ewha Womans University, Seodaaemun-gu, Seoul, Korea) ,  Cheon B.G. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea) ,  Chiba J. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Chikawa M. (Department of Physics, Kinki University, Higashi Osaka, Osaka, Japan) ,  Cho W.R. (Department of Physics, Yonsei University, Seodaemun-gu, Seoul, Korea) ,  Farhang-Boroujeny B. (Department of Electrical and Computer Engineering, University of Utah, Salt Lake City, Utah, USA) ,  Fujii T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fukushima M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fukushima M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Chiba, Japan) ,  Gillman W.H. (Gillman & Associates, Salt Lake City, Utah, USA) ,  Goto T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hanlon W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Hanson J.C. (University of Kansas, Lawrence, Kansas, USA) ,  Hayashi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ikeda D. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Inoue N. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Ishii T. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ishimori R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ito H. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Ivanov D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Jayanthmurthy C. (Department of Electrical and Computer Engineering, University of Utah, Salt Lake City, Utah, USA) ,  Jui C.C.H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kadota K. (Department of Physics, Tokyo City University, Setagaya-ku, Tokyo, Japan) ,  Kakimoto F. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, 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, Shinjuku-ku, Tokyo, Japan) ,  Kawai H. (Department of Physics, Chiba University, Chiba, Chiba, Japan) ,  Kawakami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kawana S. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kido E. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kim H.B. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea) ,  Kim J.H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kim J.H. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, Korea) ,  Kitamura S. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kitamura Y. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kunwar S. (University of Kansas, Lawrence, Kansas, USA) ,  Kuzmin V. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Kwon Y.J. (Department of Physics, Yonsei University, Seodaemun-gu, Seoul, Korea) ,  Lan J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Lim S.I. (Department of Physics and Institute for the Early Universe, Ewha Womans University, Seodaaemun-gu, Seoul, Korea) ,  Lundquist J.P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Machida K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Chiba, Japan) ,  Matsuda T. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, Japan) ,  Matsuyama T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Matthews J.N. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Minamino M. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Mukai K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Myers I. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Nagasawa K. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Nakamura T. (Faculty of Science, Kochi University, Kochi, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Nozato A. (Department of Physics, Kinki University, Higashi Osaka, Osaka, Japan) ,  Ogio S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ogura J. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Ohoka H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Oki K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Kusatsu, Shiga, Japan) ,  Ono M. (Department of Physics, Kyushu University, Fukuoka, Fukuoka, Japan) ,  Oshima A. (Engineering Science Laboratory, Chubu University, Kasugai, Aichi, Japan) ,  Ozawa S. (Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan) ,  Park I.H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Prohira S. (University of Kansas, Lawrence, Kansas, USA) ,  Pshirkov M.S. (Sternberg Astronomical Institute, Moscow M.V.Lomonosov State University, Moscow, Russia) ,  Pshirkov M.S. (National Nuclear Research University, Moscow Engineering Physics Institute, Moscow, Russia) ,  Rezazadeh-Reyhani A. (Department of Electrical and Computer Engineering, University of Utah, Salt Lake City, Utah, USA) ,  Rodriguez D.C. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, 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, UNIST-gil, Ulsan, Korea) ,  Sagawa H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Sampson A.L. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Scott L.M. (Department of Physics and Astronomy, Rutgers University - The State University of New Jersey, Piscataway, New Jersey, USA) ,  Schurig D. (Department of Electrical and Computer Engineering, University of Utah, Salt Lake City, Utah, USA) ,  Shah P.D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Shibata F. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Shibata T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shimodaira H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shin B.K. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea) ,  Smith J.D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Sokolsky P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Springer R.W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stokes B.T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stratton S.R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stratton S.R. (Department of Physics and Astronomy, Rutgers University - The State University of New Jersey, Piscataway, New Jersey, USA) ,  Stroman T.A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Suzawa T. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Takai H. (Brookhaven National Laboratory, Upton, New York, USA) ,  Takamura M. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Takeda M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Takeishi R. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Taketa A. (Earthquake Research Institute, University of Tokyo, Bunkyo-ku, Tokyo, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Tameda Y. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Tanaka H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Tanaka K. (Graduate School of Information Sciences, Hiroshima City University, Hiroshima, Hiroshima, Japan) ,  Urban F. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  Thomas S.B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Thomson G.B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA)
資料名： Astroparticle Physics  (Astroparticle Physics)
巻： 87  ページ： 1-17  発行年： 2017年 
JST資料番号： W0658A  ISSN： 0927-6505  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： オランダ (NLD)  言語： 英語 (EN)

抄録/ポイント： TARA(望遠鏡アレイレーダ)はデルタ,米国,ユタ州近傍望遠鏡アレイ,従来の表面シンチレーション検出器(SD)と蛍光望遠鏡検出器(FD)と共通の宇宙線レーダ検出実験であるTARA検出器は,SD配列上と展望のFD場内のレーダキャリアを放送する,250MS/s DAQ受信機に対する40kW,54.1MHz VHF送信機と高利得送信アンテナを組み合わせたものである。TARAは広範な空気シャワー(EAS)のレーダシグネチャを観察することを第一の目的として,2013年以降のデータを収集した。シミュレーションは,エコーは,期間(~ 10 μs)における短いことが期待され,周波数急速に変化を示し,1MHz/μsの速度であることを示した。EASレーダ断面積(RCS)は現在不明である,推測の70年以上の主題である。新しい信号探索技術は,特に空気シャワーの予想されるレーダエコーは整合フィルタテンプレートとして使用を記述し,望遠鏡配列蛍光検出器を用いたレーダDAQの引き金を引くことにより得られた波形と比較した。EASによる無線周波数放射の散乱の証拠は,今日までに得られなかった。望遠鏡配列蛍光検出器を引き起こすEASを用いた最初の定量的RCS上限を報告した。Copyright 2018 Elsevier B.V., Amsterdam. All rights reserved. Translated from English into Japanese by JST.【Powered by NICT】

シソーラス用語： *宇宙線 ,  検出器 ,  送信機 ,  蛍光 ,  高速度 ,  *空気シャワー ,  整合フィルタ ,  送信アンテナ ,  *レーダ断面積 ,  蛍光検出器 ,  周波数 ,  *レーダ ,  望遠鏡 ,  受信機
準シソーラス用語： レーダ検出 , 【Automatic Indexing@JST】

著者キーワード (4件)： 宇宙線 ,  レーダ ,  ディジタル信号処理 ,  レーダ断面積

分類 (1件)： 空気シャワー  (DB02070T)

タイトルに関連する用語 (5件)： 宇宙線 ,  誘起 ,  空気シャワー ,  レーダ断面積 ,  上限