Coronal Mass Ejections (CMEs) often travel in the interplanetary space faster than the ambient solar wind. When their relative velocities exceed the local magnetosonic speed, a shock wave forms. The region between the shock front and the leading edge is known as a sheath region. Sheaths are compressed regions characterized by turbulent magnetic field and plasma properties and they can cause significant space weather disturbances. Within the sheath region, it is possible to find fine structures such as planar magnetic structures (PMSs). The magnetic field vectors in a PMS are characterized by abrupt changes in direction and magnitude, but they all remain for a time interval of several hours nearly parallel to a single plane that includes th...
We examine 188 coronal mass ejections (CMEs) measured by the twin Solar Terrestrial Relations Observ...
International audienceWe present a statistical study of interplanetary conditions and geospace respo...
We report a statistical analysis of magnetic field fluctuations in 79 coronal mass ejection- (CME-) ...
Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic...
Coronal Mass Ejections (CMEs) often travel in the interplanetary space faster than the ambient solar...
Context. Sheath regions ahead of coronal mass ejections (CMEs) are large-scale heliospheric structur...
We present a statistical study of interplanetary conditions and geospace response to 89 coronal mass...
In this work, we investigate magnetic field fluctuations in three coronal mass ejection (CME)-driven...
Context. We investigated the plasma and magnetic field characteristics of the upstream regions of in...
Context. The transition of the magnetic field from the ambient magnetic field to the eject...
Mirror mode waves arise from the antiphase, low frequency fluctuations of the magnetic field and pla...
International audienceWe present a statistical study of interplanetary conditions and geospace respo...
We examine 188 coronal mass ejections (CMEs) measured by the twin Solar Terrestrial Relations Observ...
International audienceWe present a statistical study of interplanetary conditions and geospace respo...
We report a statistical analysis of magnetic field fluctuations in 79 coronal mass ejection- (CME-) ...
Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic...
Coronal Mass Ejections (CMEs) often travel in the interplanetary space faster than the ambient solar...
Context. Sheath regions ahead of coronal mass ejections (CMEs) are large-scale heliospheric structur...
We present a statistical study of interplanetary conditions and geospace response to 89 coronal mass...
In this work, we investigate magnetic field fluctuations in three coronal mass ejection (CME)-driven...
Context. We investigated the plasma and magnetic field characteristics of the upstream regions of in...
Context. The transition of the magnetic field from the ambient magnetic field to the eject...
Mirror mode waves arise from the antiphase, low frequency fluctuations of the magnetic field and pla...
International audienceWe present a statistical study of interplanetary conditions and geospace respo...
We examine 188 coronal mass ejections (CMEs) measured by the twin Solar Terrestrial Relations Observ...
International audienceWe present a statistical study of interplanetary conditions and geospace respo...
We report a statistical analysis of magnetic field fluctuations in 79 coronal mass ejection- (CME-) ...