We present a multipoint case study of solar wind and magnetospheric observations during a transient magnetospheric compression at 2319 UT on October 15, 2008. We use high-time resolution magnetic field and plasma data from the THEMIS and GOES-11/12 spacecraft to show that this transient event corresponded to an abrupt rotation in the IMF orientation, a change in the location of the foreshock, and transient outward bow shock motion. We employ results from a global hybrid code model to reconcile the observations indicating transient inward magnetopause motion with the outward bow shock motion
In response to a solar wind dynamic pressure enhancement, the compression of the magnetosphere gener...
We have used the AMR-CESE-MHD model to investigate the influences of the IMF Bz and the upstream sol...
Hot flow anomalies (HFAs) at Earth's bow shock were identified in Time History of Events and Ma...
This study focuses on Time History of Events and Macroscale Interactions During Substorms (THEMIS) o...
International audienceSudden impulses (SI) in the tail lobe magnetic field associated with solar win...
We present a scenario resulting in time-dependent behaviour of the bow shock and transient, local io...
We present a case study of a large deformation of the magnetopause on November 26, 2008. The investi...
Anomaly (HFA) on the dusk flank of the Earth’s bow shock on 4 July 2007, observing it on both sides ...
Solar wind mass, energy and momentum can be transferred to Earth's magnetosphere at the magnetopause...
We investigate the global response of the geospace plasma environment to an interplanetary (IP) sho...
Dissertation (Ph.D.) University of Alaska Fairbanks, 2022Interactions between bow shock-reflected (f...
International audienceThe four Cluster spacecraft were flying very close to the nose of the magnetos...
The foreshock located upstream of Earth's bow shock hosts a wide variety of phenomena related to the...
The foreshock located upstream of Earth's bow shock hosts a wide variety of phenomena related to the...
International audienceWe present a case study of Geotail, Interball-1, IMP-8, and Wind observations ...
In response to a solar wind dynamic pressure enhancement, the compression of the magnetosphere gener...
We have used the AMR-CESE-MHD model to investigate the influences of the IMF Bz and the upstream sol...
Hot flow anomalies (HFAs) at Earth's bow shock were identified in Time History of Events and Ma...
This study focuses on Time History of Events and Macroscale Interactions During Substorms (THEMIS) o...
International audienceSudden impulses (SI) in the tail lobe magnetic field associated with solar win...
We present a scenario resulting in time-dependent behaviour of the bow shock and transient, local io...
We present a case study of a large deformation of the magnetopause on November 26, 2008. The investi...
Anomaly (HFA) on the dusk flank of the Earth’s bow shock on 4 July 2007, observing it on both sides ...
Solar wind mass, energy and momentum can be transferred to Earth's magnetosphere at the magnetopause...
We investigate the global response of the geospace plasma environment to an interplanetary (IP) sho...
Dissertation (Ph.D.) University of Alaska Fairbanks, 2022Interactions between bow shock-reflected (f...
International audienceThe four Cluster spacecraft were flying very close to the nose of the magnetos...
The foreshock located upstream of Earth's bow shock hosts a wide variety of phenomena related to the...
The foreshock located upstream of Earth's bow shock hosts a wide variety of phenomena related to the...
International audienceWe present a case study of Geotail, Interball-1, IMP-8, and Wind observations ...
In response to a solar wind dynamic pressure enhancement, the compression of the magnetosphere gener...
We have used the AMR-CESE-MHD model to investigate the influences of the IMF Bz and the upstream sol...
Hot flow anomalies (HFAs) at Earth's bow shock were identified in Time History of Events and Ma...