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M. F. Thomsen Saturn's magnetospheric dynamics Geophysical Research Letters 40

Version of Record online: 30 OCT 2013 | DOI: 10.1002/2013GL057967

Key Points

  • Centrifugal interchange and tail reconnection move plasma toward the solar wind
  • Cassini observations and numerical simulations illuminate these processes
  • Ultimate loss processes for Saturnian plasma are not yet quantitatively known

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