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 betw...
International audienceAn analysis of the low frequency geomagnetic field fluctuations at an Antarcti...
On October-November 2003 complex interplanetary structures, originated by a series of solar eruption...
Daytime Pc 3-4 pulsation activities observed at globally coordinated low-latitude stations [SGC (L=1...
Pc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) during the passage of ...
International audiencePc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) ...
An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nova Bay) an...
An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nova Bay) and...
Based on a detailed study of Pc3 events at an array between L = 1.5 and 3 in Central Europe, the au...
We conducted a statistical analysis of the physical characteristics of the micropulsation activity ...
Geomagnetic pulsation in the Pc3–4 bands have been studied at high Antarctic latitudes during the lo...
Abstract. Energy for the Earth’s magnetospheric processes is provided by solar wind. Pc3 Geomagnetic...
Abstract. Geomagnetic pulsations recorded on the ground are the signa-tures of the integrated signal...
On October-November 2003 complex interplanetary structures, originated by a series of solar eruption...
Abstract. An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nov...
The results are presented of a statistical study of the occurrence, strength, frequency and polariza...
International audienceAn analysis of the low frequency geomagnetic field fluctuations at an Antarcti...
On October-November 2003 complex interplanetary structures, originated by a series of solar eruption...
Daytime Pc 3-4 pulsation activities observed at globally coordinated low-latitude stations [SGC (L=1...
Pc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) during the passage of ...
International audiencePc3 geomagnetic field fluctuations detected at low latitude (L'Aquila, Italy) ...
An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nova Bay) an...
An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nova Bay) and...
Based on a detailed study of Pc3 events at an array between L = 1.5 and 3 in Central Europe, the au...
We conducted a statistical analysis of the physical characteristics of the micropulsation activity ...
Geomagnetic pulsation in the Pc3–4 bands have been studied at high Antarctic latitudes during the lo...
Abstract. Energy for the Earth’s magnetospheric processes is provided by solar wind. Pc3 Geomagnetic...
Abstract. Geomagnetic pulsations recorded on the ground are the signa-tures of the integrated signal...
On October-November 2003 complex interplanetary structures, originated by a series of solar eruption...
Abstract. An analysis of the low frequency geomagnetic field fluctuations at an Antarctic (Terra Nov...
The results are presented of a statistical study of the occurrence, strength, frequency and polariza...
International audienceAn analysis of the low frequency geomagnetic field fluctuations at an Antarcti...
On October-November 2003 complex interplanetary structures, originated by a series of solar eruption...
Daytime Pc 3-4 pulsation activities observed at globally coordinated low-latitude stations [SGC (L=1...