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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 27, issue 6
Ann. Geophys., 27, 2331–2339, 2009
https://doi.org/10.5194/angeo-27-2331-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 27, 2331–2339, 2009
https://doi.org/10.5194/angeo-27-2331-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

  08 Jun 2009

08 Jun 2009

On a magnetosphere disturbed by solar wind; observations of macroelectrons

E. B. Wodnicka E. B. Wodnicka
  • Space Reaserch Centre, PAS, Bartycka 18a, 00716 Warsaw, Poland

Abstract. Three-dimensional electromagnetic full kinetic particle code (a version of TRISTAN) is used to study the interaction of a weakly-magnetized object with a solar wind of low density. The details of two magnetospheric processes – wave activity and energetic electrons appearing at the flanks of the magnetosphere – are presented. The results of the simulation are compared with known magnetospheric data.

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