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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 17, issue 4
Ann. Geophys., 17, 490–496, 1999
https://doi.org/10.1007/s00585-999-0490-x
© European Geosciences Union 1999
Ann. Geophys., 17, 490–496, 1999
https://doi.org/10.1007/s00585-999-0490-x
© European Geosciences Union 1999

  30 Apr 1999

30 Apr 1999

Pc3 pulsations during variable IMF conditions

U. Villante1, S. Lepidi2,1, P. Francia1, M. Vellante1, A. Meloni2, R. P. Lepping3, and F. Mariani4 U. Villante et al.
  • 1Dipartimento di Fisica, Università dell'Aquila, L'Aquila, Italy
  • 2Istituto Nazionale di Geofisica, Roma, Italy
  • 3Laboratory for Extraterrestrial Physics, NASA/GSFC, Greenbelt, USA
  • 4Dipartimento di Fisica, Universita' di Roma-Tor Vergata, Italy

Abstract. Pc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) during the passage of a high velocity solar wind stream, characterized by variable interplanetary magnetic field conditions, are analyzed. Higher frequency resonant fluctuations and lower frequency phenomena are simultaneously observed; the intermittent appearance and the variable frequency of the longer period modes can be well interpreted in terms of the variable IMF elements; moreover their polarization characteristics are consistent with an origin related to external waves propagating in antisunward direction. A comparison with simultaneous observations performed at Terra Nova Bay (Antarctica) provides additional evidence for a clear relationship between the IMF and Pc3 pulsations also at very high latitudes.

Key words. Magnetospheric physics (MHD waves and instabilities; solar wind · magnetosphere interactions)

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