In this study we analyzed a long-duration ULF wave event detected on 18–19 February 2005 by Cluster satellites, upstream of the nose of the bow shock. The availability of simultaneous data from Geotail satellite, located in the foreshock region close to the dawn flank of the bow shock, allowed us to make a comparison between the observations at the two different sites. The results can be explained in terms of local wave generation, depending on the orientation of the interplanetary magnetic field with respect to the local bow shock normal. In addition, simultaneous data from Polar satellite in the inner magnetosphere and from ground stations in the southern polar cap and at low latitude allowed us to investigate the transmission of the exte...
We examined several events of geomagnetic field fluctuations related to upstream waves, focusing the...
The occurrence of Pcl-2 ULF waves in Scott Base and Casey Antarctic magnetometer data has been exami...
Ultra-low frequency (ULF) waves in the 1-100 mHz band are ubiquitous in the magnetosphere. They are ...
On 5 September 2002 the Geotail satellite observed the cone angle of the Interplanetary Magnetic Fie...
Based on magnetic field measurements from the satellite CHAMP, a detailed picture could be obtained...
We examine the characteristics of a train of ULF waves observed in the magnetosphere and at ground ...
International audienceWe study two examples of broadband ultra-low frequency (ULF) waves observed ne...
We examine the characteristics of a train of ULF waves observed in the magnetosphere and at ground a...
Hot flow anomalies (HFAs), which are frequently observed near Earth's bow shock, are phenomena ...
For the intrusion of the solar wind energy into the magnetosphere the polar cusp has been believed t...
We studied the occurrence of upstream waves in the foreshock region and their relationship with the ...
We have used 1-year's data from the recently installed Magnetometer Array for Cusp and Cleft Studies...
Research Doctorate - Doctor of Philosophy (PhD)ULF waves (0.001-5 Hz) in the Earth's magnetosphere a...
International audienceThe multi-spacecraft missions (Cluster and THEMIS) observations allowed to col...
A one dimensional, computational model for the propagation of ultra low frequency (ULF; 1-100 mHz) ...
We examined several events of geomagnetic field fluctuations related to upstream waves, focusing the...
The occurrence of Pcl-2 ULF waves in Scott Base and Casey Antarctic magnetometer data has been exami...
Ultra-low frequency (ULF) waves in the 1-100 mHz band are ubiquitous in the magnetosphere. They are ...
On 5 September 2002 the Geotail satellite observed the cone angle of the Interplanetary Magnetic Fie...
Based on magnetic field measurements from the satellite CHAMP, a detailed picture could be obtained...
We examine the characteristics of a train of ULF waves observed in the magnetosphere and at ground ...
International audienceWe study two examples of broadband ultra-low frequency (ULF) waves observed ne...
We examine the characteristics of a train of ULF waves observed in the magnetosphere and at ground a...
Hot flow anomalies (HFAs), which are frequently observed near Earth's bow shock, are phenomena ...
For the intrusion of the solar wind energy into the magnetosphere the polar cusp has been believed t...
We studied the occurrence of upstream waves in the foreshock region and their relationship with the ...
We have used 1-year's data from the recently installed Magnetometer Array for Cusp and Cleft Studies...
Research Doctorate - Doctor of Philosophy (PhD)ULF waves (0.001-5 Hz) in the Earth's magnetosphere a...
International audienceThe multi-spacecraft missions (Cluster and THEMIS) observations allowed to col...
A one dimensional, computational model for the propagation of ultra low frequency (ULF; 1-100 mHz) ...
We examined several events of geomagnetic field fluctuations related to upstream waves, focusing the...
The occurrence of Pcl-2 ULF waves in Scott Base and Casey Antarctic magnetometer data has been exami...
Ultra-low frequency (ULF) waves in the 1-100 mHz band are ubiquitous in the magnetosphere. They are ...