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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 29, issue 4
Ann. Geophys., 29, 701–716, 2011
https://doi.org/10.5194/angeo-29-701-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: Cluster 10th anniversary workshop

Ann. Geophys., 29, 701–716, 2011
https://doi.org/10.5194/angeo-29-701-2011
© Author(s) 2011. This work is distributed under
the Creative Commons Attribution 3.0 License.

  27 Apr 2011

27 Apr 2011

Observations of an auroral streamer in a double oval configuration

O. Amm1, R. Nakamura2, T. Takada3, K. Kauristie1, H. U. Frey4, C. J. Owen5, A. Aikio6, and R. Kuula6 O. Amm et al.
  • 1Finnish Meteorological Institute, Arctic research unit, P.O. Box 503, 00101 Helsinki, Finland
  • 2Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • 3Kochi National College of Technology, Nankoku, Japan
  • 4Space Sciences Laboratory, University of California, Berkeley, USA
  • 5Mullard Space Science Laboratory, Dorking, UK
  • 6University of Oulu, Oulu, Finland

Abstract. During the late evening and night of 14 September 2004, the nightside auroral oval shows a distinct double oval configuration for several hours after a substorm onset at ~18:45 UT. This structure is observed both by the IMAGE satellite optical instruments focusing on the Southern Hemisphere, and by the MIRACLE ground-based instrument network in Scandinavia. At ~21:17 UT during the recovery phase of the substorm, an auroral streamer is detected by these instruments and the EISCAT radar, while simultaneously the Cluster satellites observe a bursty bulk flow in the conjugate portion of the plasma sheet in the magnetotail. Our combined data analysis reveals significant differences between the ionospheric equivalent current signature of this streamer within a double oval configuration, as compared to previously studied streamer events without such a configuration. We attribute these differences to the presence of an additional poleward polarization electric field between the poleward and the equatorward portions of the double oval, and show with a simple model that such an assumption can conceptually explain the observations. Further, we estimate the total current transferred in meridional direction by this recovery phase streamer to ~80 kA, significantly less than for previously analysed expansion phase streamer events. Both results indicate that the development of auroral streamers is dependent on the ambient background conditions in the magnetosphere-ionosphere system. The auroral streamer event studied was simultaneously observed in the conjugate Northern and Southern Hemisphere ionosphere.

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