Collisionless magnetic reconnection is often associated with time-dependent behavior. Specifically, current layers in the diffusion region can become unstable to tearing-type instabilities on one hand, or to instabilities with current-aligned wave vectors on the other. In the former case, the growth of tearing instabilities typically leads to the production of magnetic islands, which potentially provide feedback on the reconnection process itself, as well as on the rate of reconnection. The second class of instabilities tend to modulate the current layer along the direction of the current flow, for instance generating kink-type perturbations, or smaller-scale turbulence with the potential to broaden the current layer. All of these processes...
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic rec...
The role of turbulence in producing fast reconnection rates is an important unresolved question. Sca...
Magnetic reconnection is recognized as a dominant mechanism for converting magnetic energy into the ...
The question of whether the micro scale controls the macroscale or vice-versa remains one of the mos...
The role of turbulence in the process of magnetic reconnection has been the subject of a great deal ...
International audience<p><span>Observations of Earth&#8217;s magnetosheath from the ...
The question of whether the microscale controls the macroscale or vice-versa remains one of the most...
Reconnection is a ubiquitous energy conversion process operating in current sheets. It appears in a ...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
International audience<p>The Earth&#8217;s magnetosheath is filled with small-scale curren...
We study the evolutions of collisionless magnetic reconnection with full kinetic particle-in-cell si...
In near-collisionless plasmas, which are ubiquitous in astrophysics, entropy production relies on fu...
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic rec...
Context. Forced magnetic reconnection, a reconnection event triggered by external perturbation, shou...
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic rec...
The role of turbulence in producing fast reconnection rates is an important unresolved question. Sca...
Magnetic reconnection is recognized as a dominant mechanism for converting magnetic energy into the ...
The question of whether the micro scale controls the macroscale or vice-versa remains one of the mos...
The role of turbulence in the process of magnetic reconnection has been the subject of a great deal ...
International audience<p><span>Observations of Earth&#8217;s magnetosheath from the ...
The question of whether the microscale controls the macroscale or vice-versa remains one of the most...
Reconnection is a ubiquitous energy conversion process operating in current sheets. It appears in a ...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
International audience<p>The Earth&#8217;s magnetosheath is filled with small-scale curren...
We study the evolutions of collisionless magnetic reconnection with full kinetic particle-in-cell si...
In near-collisionless plasmas, which are ubiquitous in astrophysics, entropy production relies on fu...
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic rec...
Context. Forced magnetic reconnection, a reconnection event triggered by external perturbation, shou...
Turbulent plasmas generate a multitude of thin current structures that can be sites for magnetic rec...
The role of turbulence in producing fast reconnection rates is an important unresolved question. Sca...
Magnetic reconnection is recognized as a dominant mechanism for converting magnetic energy into the ...