Abstract

On October-November 2003 complex interplanetary structures, originated by a series of solar eruptions, hit the Earth, triggering violent Sun-Earth connection events. In this paper we analyze the low frequency geomagnetic field fluctuations detected on the ground during Oct. 29-31, 2003, a time period characterized by extremely high solar wind speed values and by out-of-ecliptic interplanetary magnetic field orientation for intervals of several hours. We analyze geomagnetic field measurements at four high latitude stations located in the polar cap, three in the southern and one in the northern hemisphere. From a comparison with simultaneous measurements at low latitude, we address the question of the global character of the observed phenomena. The results show, for selected time intervals, the occurrence of simultaneous fluctuations at all the stations, with high coherence even between high and low latitude; it is interesting that these fluctuations are detected during open magnetospheric conditions, when the high latitude stations are situated well within the polar cap, i.e. far from closed field lines.

Highlights

  • Several studies analyzed the interaction between coronal ejecta, characterized by long periods of out-of-ecliptic interplanetary magnetic field (IMF) orientation, and the Earth’s magnetosphere

  • From a comparison with simultaneous measurements at low latitude, we address the question of the global character of the observed phenomena

  • Fluctuations with different characteristics are observed: - broadband fluctuations at the onset of strong geomagnetic storms, which are observed at all high latitude stations but are not spatially coherent; - fluctuations observed only at some of the stations, corresponding to local phenomena; - fluctuations simultaneously observed at all stations which are spatially coherent, even between high and low latitude

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Summary

Introduction

Several studies analyzed the interaction between coronal ejecta, characterized by long periods of out-of-ecliptic interplanetary magnetic field (IMF) orientation, and the Earth’s magnetosphere.

Results
Conclusion
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