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