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- J. L. Burch
- Southwest Research Institute, San Antonio, TX, USA.
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- R. B. Torbert
- Southwest Research Institute, San Antonio, TX, USA.
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- T. D. Phan
- University of California, Berkeley, CA, USA.
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- L.-J. Chen
- University of Maryland, College Park, MD, USA.
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- T. E. Moore
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- R. E. Ergun
- University of Colorado LASP, Boulder, CO, USA.
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- J. P. Eastwood
- Blackett Laboratory, Imperial College London, London, UK.
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- D. J. Gershman
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- P. A. Cassak
- West Virginia University, Morgantown, WV, USA.
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- M. R. Argall
- University of New Hampshire, Durham, NH, USA.
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- S. Wang
- University of Maryland, College Park, MD, USA.
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- M. Hesse
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- C. J. Pollock
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- B. L. Giles
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- R. Nakamura
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
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- B. H. Mauk
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA.
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- S. A. Fuselier
- Southwest Research Institute, San Antonio, TX, USA.
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- C. T. Russell
- University of California, Los Angeles, CA, USA.
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- R. J. Strangeway
- University of California, Los Angeles, CA, USA.
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- J. F. Drake
- University of Maryland, College Park, MD, USA.
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- M. A. Shay
- University of Delaware, Newark, DE, USA.
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- Yu. V. Khotyaintsev
- Swedish Institute of Space Physics, Uppsala, Sweden.
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- P.-A. Lindqvist
- Royal Institute of Technology, Stockholm, Sweden.
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- G. Marklund
- Royal Institute of Technology, Stockholm, Sweden.
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- F. D. Wilder
- University of Colorado LASP, Boulder, CO, USA.
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- D. T. Young
- Southwest Research Institute, San Antonio, TX, USA.
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- K. Torkar
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
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- J. Goldstein
- Southwest Research Institute, San Antonio, TX, USA.
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- J. C. Dorelli
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- L. A. Avanov
- NASA, Goddard Space Flight Center, Greenbelt, MD, USA.
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- M. Oka
- University of California, Berkeley, CA, USA.
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- D. N. Baker
- University of Colorado LASP, Boulder, CO, USA.
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- A. N. Jaynes
- University of Colorado LASP, Boulder, CO, USA.
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- K. A. Goodrich
- University of Colorado LASP, Boulder, CO, USA.
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- I. J. Cohen
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA.
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- D. L. Turner
- Aerospace Corporation, El Segundo, CA, USA.
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- J. F. Fennell
- Aerospace Corporation, El Segundo, CA, USA.
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- J. B. Blake
- Aerospace Corporation, El Segundo, CA, USA.
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- J. Clemmons
- Aerospace Corporation, El Segundo, CA, USA.
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- M. Goldman
- University of Colorado, Boulder, CO, USA.
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- D. Newman
- University of Colorado, Boulder, CO, USA.
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- S. M. Petrinec
- Lockheed Martin Advanced Technology Center, Palo Alto, CA, USA.
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- K. J. Trattner
- University of Colorado LASP, Boulder, CO, USA.
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- B. Lavraud
- Institut de Recherche en Astrophysique et Planétologie, Toulouse, France.
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- P. H. Reiff
- Department of Physics and Astronomy, Rice University, Houston, TX, USA.
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- W. Baumjohann
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
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- W. Magnes
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
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- M. Steller
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
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- W. Lewis
- Southwest Research Institute, San Antonio, TX, USA.
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- Y. Saito
- Institute for Space and Astronautical Sciences, Sagamihara, Japan.
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- V. Coffey
- NASA, Marshall Space Flight Center, Huntsville, AL, USA.
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- M. Chandler
- NASA, Marshall Space Flight Center, Huntsville, AL, USA.
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説明
<jats:title>Probing magnetic reconnection in space</jats:title> <jats:p> Magnetic reconnection occurs when the magnetic field permeating a conductive plasma rapidly rearranges itself, releasing energy and accelerating particles. Reconnection is important in a wide variety of physical systems, but the details of how it occurs are poorly understood. Burch <jats:italic>et al.</jats:italic> used NASA's Magnetospheric Multiscale mission to probe the plasma properties within a reconnection event in Earth's magnetosphere (see the Perspective by Coates). They find that the process is driven by the electron-scale dynamics. The results will aid our understanding of magnetized plasmas, including those in fusion reactors, the solar atmosphere, solar wind, and the magnetospheres of Earth and other planets. </jats:p> <jats:p> <jats:italic>Science</jats:italic> , this issue p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" related-article-type="in-this-issue" xlink:href="10.1126/science.aaf2939">10.1126/science.aaf2939</jats:related-article> ; see also p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6290" page="1176" related-article-type="in-this-issue" vol="352" xlink:href="10.1126/science.aaf7269">1176</jats:related-article> </jats:p>
収録刊行物
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- Science
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Science 352 (6290), aaf2939-, 2016-06-03
American Association for the Advancement of Science (AAAS)
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詳細情報 詳細情報について
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- CRID
- 1360283693426160128
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- ISSN
- 10959203
- 00368075
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
