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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 28, issue 10
Ann. Geophys., 28, 1877–1878, 2010
https://doi.org/10.5194/angeo-28-1877-2010
© Author(s) 2010. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 28, 1877–1878, 2010
https://doi.org/10.5194/angeo-28-1877-2010
© Author(s) 2010. This work is distributed under
the Creative Commons Attribution 3.0 License.

  07 Oct 2010

07 Oct 2010

Corrigendum to "Substorm activity in Venus's magnetotail" published in Ann. Geophys., 27, 2321–2330, doi:10.5194/angeo-27-2321-2009, 2009

M. Volwerk1, M. Delva1, Y. Futaana2, A. Retinò1, Z. Vörös3, T. L. Zhang1, W. Baumjohann1, and S. Barabash2 M. Volwerk et al.
  • 1Space Research Institute, Austrian Academy of Sciences, 8042 Graz, Austria
  • 2Swedish Institute of Space Physics, Kiruna, 98128, Sweden
  • 3Institute of Astro- and Particle Physics, University of Innsbruck, 6020 Innsbruck, Austria

Abstract. A re-evaluation of the reconnection event reported by Volwerk et al. (2009) shows that the original interpretation of the magnetic field data as quadrupolar Hall-current signatures around a reconnection site was mistaken. It could be interpreted as the signature of reconnection in the presence of a guide field. The path of VEX through the active region in Venus's magnetotail is re-evaluated and the strongly energized ions associated to this event are now in agreement with the magnetic field data.

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