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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 23, issue 9
Ann. Geophys., 23, 3095-3101, 2005
https://doi.org/10.5194/angeo-23-3095-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.

Special issue: 1st European Space Weather Week (ESWW)

Ann. Geophys., 23, 3095-3101, 2005
https://doi.org/10.5194/angeo-23-3095-2005
© Author(s) 2005. This work is distributed under
the Creative Commons Attribution 3.0 License.

  22 Nov 2005

22 Nov 2005

Predictions of local ground geomagnetic field fluctuations during the 7-10 November 2004 events studied with solar wind driven models

P. Wintoft1, M. Wik1, H. Lundstedt1, and L. Eliasson2 P. Wintoft et al.
  • 1Swedish Institute of Space Physics, Lund, Sweden
  • 2Swedish Institute of Space Physics, Kiruna, Sweden

Abstract. The 7-10 November 2004 period contains two events for which the local ground magnetic field was severely disturbed and simultaneously, the solar wind displayed several shocks and negative Bz periods. Using empirical models the 10-min RMS and at Brorfelde (BFE, 11.67° E, 55.63° N), Denmark, are predicted. The models are recurrent neural networks with 10-min solar wind plasma and magnetic field data as inputs. The predictions show a good agreement during 7 November, up until around noon on 8 November, after which the predictions become significantly poorer. The correlations between observed and predicted log RMS is 0.77 during 7-8 November but drops to 0.38 during 9-10 November. For RMS the correlations for the two periods are 0.71 and 0.41, respectively. Studying the solar wind data for other L1-spacecraft (WIND and SOHO) it seems that the ACE data have a better agreement to the near-Earth solar wind during the first two days as compared to the last two days. Thus, the accuracy of the predictions depends on the location of the spacecraft and the solar wind flow direction. Another finding, for the events studied here, is that the and models showed a very different dependence on Bz. The model is almost independent of the solar wind magnetic field Bz, except at times when Bz is exceptionally large or when the overall activity is low. On the contrary, the model shows a strong dependence on Bz at all times.

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