International audienceUsing 5 years of Cluster data, we present a detailed statistical analysis of magnetic fluctuations associated with mirror structures in the magnetosheath. We especially focus on the shape of these fluctuations which, in addition to quasi-sinusoidal forms, also display deep holes and high peaks. The occurrence frequency and the most probable location of the various types of structures is discussed, together with their relation to local plasma parameters. While these properties have previously been correlated to the ? of the plasma, we emphasize here the influence of the distance to the linear mirror instability threshold. This enables us to interpret the observations of mirror structures in a stable plasma in terms of b...
International audienceWe show evidence for mirror mode structures at comet Giacobini-Zinner. These a...
Spacecraft observations confirm the existence of mirror fluctuations in the magnetosheath. The mirro...
International audienceBetween December 1997 and March 1998 Equator-S made a number of excursions int...
International audienceUsing 5 years of Cluster data, we present a detailed statistical analysis of m...
Mirror modes are large amplitude non-propagating structures frequently observed in the magnetosheath...
International audienceNon-propagating magnetic hole solutions in anisotropic plasmas near the mirror...
[1] An examination of the magnetic field and plasma observed by the inner THEMIS‐D spacecraft (P3) c...
International audienceThe evolution of structures associated with mirror modes during their flow in ...
We performed two-dimensional (2D) and three-dimensional (3D) hybrid simulations in open boundary mod...
International audienceA model for the nonlinear dynamics of mirror modes near the instability thresh...
International audienceThe Cluster spacecraft have returned the first simultaneous four-point measure...
The relationship between a decaying strong turbulence and the mirror instability in a slowly expandi...
We present a statistical analysis of 5 years of Cluster mission data in the magnetosheath. Our prima...
Nonpropagating mirror-mode structures are commonly observed in many regions of natural plasma such a...
A global stability analysis of mirror modes in the magnetosheath is presented. The analysis is based...
International audienceWe show evidence for mirror mode structures at comet Giacobini-Zinner. These a...
Spacecraft observations confirm the existence of mirror fluctuations in the magnetosheath. The mirro...
International audienceBetween December 1997 and March 1998 Equator-S made a number of excursions int...
International audienceUsing 5 years of Cluster data, we present a detailed statistical analysis of m...
Mirror modes are large amplitude non-propagating structures frequently observed in the magnetosheath...
International audienceNon-propagating magnetic hole solutions in anisotropic plasmas near the mirror...
[1] An examination of the magnetic field and plasma observed by the inner THEMIS‐D spacecraft (P3) c...
International audienceThe evolution of structures associated with mirror modes during their flow in ...
We performed two-dimensional (2D) and three-dimensional (3D) hybrid simulations in open boundary mod...
International audienceA model for the nonlinear dynamics of mirror modes near the instability thresh...
International audienceThe Cluster spacecraft have returned the first simultaneous four-point measure...
The relationship between a decaying strong turbulence and the mirror instability in a slowly expandi...
We present a statistical analysis of 5 years of Cluster mission data in the magnetosheath. Our prima...
Nonpropagating mirror-mode structures are commonly observed in many regions of natural plasma such a...
A global stability analysis of mirror modes in the magnetosheath is presented. The analysis is based...
International audienceWe show evidence for mirror mode structures at comet Giacobini-Zinner. These a...
Spacecraft observations confirm the existence of mirror fluctuations in the magnetosheath. The mirro...
International audienceBetween December 1997 and March 1998 Equator-S made a number of excursions int...