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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 27, issue 1
Ann. Geophys., 27, 59–64, 2009
https://doi.org/10.5194/angeo-27-59-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: Ninth International Conference on Substorms (ICS9)

Ann. Geophys., 27, 59–64, 2009
https://doi.org/10.5194/angeo-27-59-2009
© Author(s) 2009. This work is distributed under
the Creative Commons Attribution 3.0 License.

  06 Jan 2009

06 Jan 2009


Plasmoid formation for multiple onset substorms: observations of the Japanese Lunar Mission "Kaguya"

T. Nagai1, H. Tsunakawa1, H. Shibuya2, F. Takahashi1, H. Shimizu3, M. Matsushima1, M. N. Nishino4, Y. Yokota4, K. Asamura4, T. Tanaka4, Y. Saito4, and O. Amm5 T. Nagai et al.
  • 1Tokyo Institute of Technology, Tokyo, Japan
  • 2Kumamoto University, Kumamoto, Japan
  • 3University of Tokyo, Tokyo, Japan
  • 4Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan
  • 5Finnish Meteorological Institute, Helsinki, Finland

Abstract. The Japanese Lunar Mission "Kaguya" carried out its first magnetic field and plasma measurements in the Earth's magnetotail on 22 December 2007. Fortuitously, three well-defined multiple onset substoms took place. Kaguya was located in the premidnight magnetotail at radial distances of 56 RE and observed plasmoids and/or traveling compression regions (TCRs). Although the present study is based on limited data sets, important issues on multiple onset substorms can be examined. Each onset in a series of onsets releases a plasmoid, and magnetic reconnection likely proceeds to tail lobe field lines for each onset. Since the duration of each plasmoid is less than 5 min, these observations imply that magnetic reconnection for each onset can develop fully to the tail lobe field lines and be quenched within this timescale.

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