Energetic ion acceleration in Saturn's magnetotail: Substorms at Saturn?

  • D. G. Mitchell
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • P. C. Brandt
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • E. C. Roelof
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • J. Dandouras
    Centre D'Etude Spatiale Des Rayonnements Toulouse France
  • S. M. Krimigis
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • B. H. Mauk
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • C. P. Paranicas
    Applied Physics Laboratory Johns Hopkins University Laurel Maryland USA
  • N. Krupp
    Max‐Planck‐Institut für Sonnensystemforschung Lindau Germany
  • D. C. Hamilton
    University of Maryland College Park Maryland USA
  • W. S. Kurth
    Department of Physics and Astronomy University of Iowa Iowa City Iowa USA
  • P. Zarka
    Observatory of Paris Meudon France
  • M. K. Dougherty
    Space and Atmospheric Physics Imperial College London U.K
  • E. J. Bunce
    Department of Physics & Astronomy University of Leicester Leicester U.K
  • D. E. Shemansky
    Department of Aerospace Engineering University of Southern California Los Angeles California USA

書誌事項

公開日
2005-06-25
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1029/2005gl022647
公開者
American Geophysical Union (AGU)

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説明

<jats:p>The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth‐like substorms occur within Saturn's magnetosphere.</jats:p>

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