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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 25, issue 3
Ann. Geophys., 25, 769–777, 2007
https://doi.org/10.5194/angeo-25-769-2007
© Author(s) 2007. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 25, 769–777, 2007
https://doi.org/10.5194/angeo-25-769-2007
© Author(s) 2007. This work is distributed under
the Creative Commons Attribution 3.0 License.

  29 Mar 2007

29 Mar 2007

Geotail observations of temperature anisotropy of the two-component protons in the dusk plasma sheet

M. N. Nishino1, M. Fujimoto1, T. Terasawa2, G. Ueno3, K. Maezawa1, T. Mukai4, and Y. Saito1 M. N. Nishino et al.
  • 1ISAS/JAXA, Kanagawa 228-8510, Japan
  • 2Tokyo Institute of Technology, Tokyo 152-8551, Japan
  • 3Institute of Statistical Mathematics, Tokyo 106-8569, Japan
  • 4JAXA, Tokyo 100-8260, Japan

Abstract. In search for clues towards the understanding of the cold plasma sheet formation under northward IMF, we study the temperature anisotropy of the two-component protons in the plasma sheet near the dusk low-latitude boundary observed by the Geotail spacecraft. The two-component protons result from mixing of the cold component from the solar wind and the hot component of the magnetospheric origin, and may be the most eloquent evidence for the transport process across the magnetopause. The cold component occasionally has a strong anisotropy in the dusk flank, and the sense of the anisotropy depends on the observed locations: the parallel temperature is enhanced in the tail flank while the perpendicular temperature is enhanced on the dayside. The hot component is nearly isotropic in the tail while the perpendicular temperature is enhanced on the dayside. We discuss possible mechanism that can lead to the observed temperature anisotropies.

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