文献

J-GLOBAL ID：202002256547604346   整理番号：20A1570657

2宇宙船BepiColomboミッションによる水銀環境の調査【JST・京大機械翻訳】

Investigating Mercury’s Environment with the Two-Spacecraft BepiColombo Mission

著者 (83件)： Milillo A. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Fujimoto M. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, Japan) ,  Murakami G. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, Japan) ,  Benkhoff J. (Science and Operations Department, Directorate of Science, ESA/ESTEC, Noordwijk, The Netherlands) ,  Zender J. (Science and Operations Department, Directorate of Science, ESA/ESTEC, Noordwijk, The Netherlands) ,  Aizawa S. (Institut de Recherche en Astrophysique et Planetologie, CNRS, CNES, Universite de Toulouse, Toulouse, France) ,  Dosa M. (Department of Space Research and Space Technology, Wigner Research Centre for Physics, Budapest, Hungary) ,  Griton L. (Institut de Recherche en Astrophysique et Planetologie, CNRS, CNES, Universite de Toulouse, Toulouse, France) ,  Heyner D. (Institut fuer Geophysik und extraterrestrische Physik, Technische Universitaet Braunschweig, Braunschweig, Germany) ,  Ho G. (The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA) ,  Imber S. M. (Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA) ,  Imber S. M. (Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK) ,  Jia X. (Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA) ,  Karlsson T. (Space and Plasma Physics, School of Electrical Engineering and Computer Science, KTH Royal Institute of Technology, Stockholm, Sweden) ,  Killen R. M. (Goddard Space Flight Centre, Maryland, USA) ,  Laurenza M. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Lindsay S. T. (Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK) ,  McKenna-Lawlor S. (Space Technology Ireland, Ltd., Maynooth, Kildare, Ireland) ,  Mura A. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Raines J. M. (Department of Climate and Space Sciences and Engineering, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA) ,  Rothery D. A. (School of Physical Sciences, The Open University, Milton Keynes, UK) ,  Andre N. (Institut de Recherche en Astrophysique et Planetologie, CNRS, CNES, Universite de Toulouse, Toulouse, France) ,  Baumjohann W. (Space Research Institute, Austrian Academy of Sciences, Graz, Austria) ,  Berezhnoy A. (Sternberg Astronomical Institute, Moscow State University, Moscow, Russia) ,  Berezhnoy A. (Institute of Physics, Kazan Federal University, Kazan, Russia) ,  Bourdin P. A. (Space Research Institute, Austrian Academy of Sciences, Graz, Austria) ,  Bourdin P. A. (Institute of Physics, University of Graz, Graz, Austria) ,  Bunce E. J. (Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK) ,  Califano F. (University of Pisa, Pisa, Italy) ,  Deca J. (University of Colorado, Boulder, USA) ,  de la Fuente S. (ESA/ESAC, Villanueva de la Canada, Spain) ,  Dong C. (Department of Astrophysical Sciences and Princeton Plasma Physics Laboratory, Princeton University, Princeton, NJ, USA) ,  Grava C. (SWRI, San Antonio, TX, USA) ,  Fatemi S. (Swedish Institute of Space Physics, Kiruna, Sweden) ,  Henri P. (Laboratoire de Physique et Chimie de l’Environnement et de l’Espace, CNRS/Universite d’Orleans/CNES, Orleans, France) ,  Ivanovski S. L. (Osservatorio Astronominco di Trieste, INAF, Trieste, Italy) ,  Jackson B. V. (University of California San Diego, La Jolla, USA) ,  James M. (Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK) ,  Kallio E. (School of Electrical Engineering, Department of Electronics and Nanoengineering, Aalto University, Helsinki, Finland) ,  Kasaba Y. (Planetary Plasma and Atmospheric Research Center, Tohoku University, Sendai, Miyagi, Japan) ,  Kilpua E. (Department of Physics, University of Helsinki, Helsinki, Finland) ,  Kobayashi M. (Planetary Exploration Research Center, Chiba Institute of Technology, Narashino, Japan) ,  Langlais B. (Laboratoire de Planetologie et Geodynamique, CNRS, Universite de Nantes, Universite d’Angers, Nantes, France) ,  Leblanc F. (LATMOS/IPSL, CNRS, Sorbonne Universite, Paris, France) ,  Lhotka C. (Space Research Institute, Austrian Academy of Sciences, Graz, Austria) ,  Mangano V. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Martindale A. (Space Research Centre, Department of Physics and Astronomy, University of Leicester, Leicester, UK) ,  Massetti S. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Masters A. (The Blackett Laboratory, Imperial College London, London, UK) ,  Morooka M. (Swedish Institute of Space Physics (IRF), Uppsala, Sweden) ,  Narita Y. (Institute of Physics, University of Graz, Graz, Austria) ,  Oliveira J. S. (Science and Operations Department, Directorate of Science, ESA/ESTEC, Noordwijk, The Netherlands) ,  Oliveira J. S. (CITEUC, Geophysical and Astronomical Observatory, University of Coimbra, Coimbra, Portugal) ,  Odstrcil D. (Goddard Space Flight Centre, Maryland, USA) ,  Orsini S. (Institute of Space Astrophysics and Planetology, INAF, Rome, Italy) ,  Pelizzo M. G. (Institute for Photonics and Nanotechnologies, CNR, Padova, Italy) ,  Plainaki C. (Italian Space Agency, Rome, Italy) ,  Plaschke F. (Space Research Institute, Austrian Academy of Sciences, Graz, Austria) ,  Sahraoui F. (Laboratoire de Physique des Plasmas, CNRS, Ecole Polytechnique, Sorbonne Universite, Universite Paris-Saclay, Observatoire de Paris, Meudon, France) ,  Seki K. (Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, Tokyo, Japan) ,  Slavin J. A. (Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, MI, USA) ,  Vainio R. (Space Research Laboratory, Department of Physics and Astronomy, University of Turku, Turku, Finland) ,  Wurz P. (Physics Institute, University of Bern, Bern, Switzerland) ,  Barabash S. (Swedish Institute of Space Physics, Kiruna, Sweden) ,  Carr C. M. (Department of Physics, Imperial College London, London, UK) ,  Delcourt D. (University of Orleans, Orleans, Paris, France) ,  Glassmeier K.-H. (Institut fuer Geophysik und extraterrestrische Physik, Technische Universitaet Braunschweig, Braunschweig, Germany) ,  Grande M. (Institute of Mathematical and Physical Sciences, University of Wales, Aberystwyth, Wales, UK) ,  Hirahara M. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan) ,  Huovelin J. (Department of Physics, University of Helsinki, Helsinki, Finland) ,  Korablev O. (IKI, Moscow, Russia) ,  Kojima H. (Research Institute for Sustainable Humanosphere, Kyoto University, Kyoto, Japan) ,  Lichtenegger H. (Space Research Institute, Austrian Academy of Sciences, Graz, Austria) ,  Livi S. (SWRI, San Antonio, TX, USA) ,  Matsuoka A. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, Japan) ,  Moissl R. (Science and Operations Department, Directorate of Science, ESA/ESTEC, Noordwijk, The Netherlands) ,  Moncuquet M. (LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universite, UPMC, Universite Paris Diderot, Sorbonne Paris Cite, Meudon, France) ,  Muinonen K. (Department of Physics, University of Helsinki, Helsinki, Finland) ,  Quemerais E. (LATMOS, Universite Versailles Saint-Quentin, Guyancourt, France) ,  Saito Y. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, Japan) ,  Yagitani S. (Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan) ,  Yoshikawa I. (Department of Complexity Science and Engineering, University of Tokyo, Tokyo, Japan) ,  Wahlund J.-E. (Swedish Institute of Space Physics (IRF), Uppsala, Sweden)
資料名： Space Science Reviews  (Space Science Reviews)
巻： 216  号： 5  ページ： 93  発行年： 2020年 
JST資料番号： W4958A  ISSN： 1572-9672  資料種別： 逐次刊行物 (A)
記事区分： 文献レビュー  発行国： ドイツ (DEU)  言語： 英語 (EN)

抄録/ポイント： ESA-JAXA BepiColmboミッションは,2つの宇宙機から同時測定を提供し,水銀における磁気圏および外圏動力学,ならびに太陽風,放射および惑星間塵とのそれらの相互作用を研究する前例のない機会を提供した。2つの宇宙機を搭載する多くの科学的手段は,完全に,または,それを支配する複雑なプロセスと同様に,水銀の近宇宙環境を研究するために,完全に,あるいは部分的に devotedげられるであろう。多くの問題は,2015年に終了したMESSENGERミッション後でも未解決のままである。2つの宇宙飛行体,MPOとMioの特定の軌道,および包括的な科学的ペイロードは,単独,あるいは以前のミッションによって,個々の機器によって達成できるものより,より広い科学的疑問を対処できる。これらの共同観測は,水銀の環境における多くの現象が時間的および空間的に変動するので,重要な重要性を持つ。本論文では,可能な協調観測の例を述べ,異なるBepiColombo装置センサの必要な幾何学的条件,ポインティング,分解能および操作タイミングを解析した。Copyright The Author(s) 2020 Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 磁気圏 ,  相互作用 ,  太陽風 ,  *水銀 ,  *宇宙飛行体 ,  宇宙環境 ,  分解能 ,  外気圏 ,  ペイロード ,  センサ ,  同時計測
準シソーラス用語： ポインティングデバイス ,  宇宙航空研究開発機構 ,  *BepiColombo , 【Automatic Indexing@JST】

著者キーワード (4件)： 水銀の環境 ,  磁気圏 ,  外気圏 ,  BepiColombo

分類 (2件)： 宇宙飛行体  (QK08000Y) ,  惑星  (DB04020E)

タイトルに関連する用語 (6件)： 宇宙船 ,  BepiColombo ,  ミッション ,  水銀 ,  環境 ,  調査