Hall magnetohydrodynamics (MHD) near a two-dimensional (2D) X-type magnetic neutral line is considered. The Hall effects are shown to be able to sustain the hyperbolicity of the magneticfield (and hence a more open X-point configuration) near the neutral line in the steady state. This result is predicated on considering the steady Hall MHD state as the temporal asymptotic limit of the corresponding time-dependent problem. For the time-dependent Hall MHD problem, the Hall effects are shown to have a negligible impact on the current-sheet formation process near the X-type magnetic neutral line at short times but, subsequently, to quench the finite-time singularity exhibited in ideal MHD and, hence to prevent the plasma collapse, in consistenc...
A theoretical mean field closure for Hall magnetohydrodynamics (Hall-MHD) is developed to investigat...
Two-dimensional resistive Hall magnetohydrodynamics (MHD) code is used to investigate the dynamical ...
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic field...
Hall magnetohydrodynamics (MHD) near a two-dimensional (2D) X-type magnetic neutral line is consider...
Hall magnetohydrodynamics (MHD) properties near a two-dimensional (2D) X-type magnetic neutral line ...
The Hall Magnetohydrodynamic (MHD) model is a new paradigm for describing fast magnetic reconnection...
An exact self-similar solution is used to investigate current sheet formation at a magnetic neutral ...
The formation of a current sheet in a weakly collisional plasma can be modelled as a finite-time sin...
Current-sheet formation near a hyperbolic magnetic neutral line in the MHD model is investigated. In...
Current-sheet formation near a hyperbolic magnetic neutral line in the MHD model is investigated. In...
The framework for the Hall magnetohydrodynamic (MHD) model for plasma physics is built up from kinet...
An exact solution for the magnetohydrodynamic (MHD) equations for a time-dependent, two-dimensional ...
An exact solution for the magnetohydrodynamic (MHD) equations for a time-dependent, two-dimensional ...
An exact solution for the magnetohydrodynamic equations for a time-dependent, two-dimensional flow o...
A theoretical mean field closure for Hall magnetohydrodynamics (Hall-MHD) is developed to investigat...
A theoretical mean field closure for Hall magnetohydrodynamics (Hall-MHD) is developed to investigat...
Two-dimensional resistive Hall magnetohydrodynamics (MHD) code is used to investigate the dynamical ...
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic field...
Hall magnetohydrodynamics (MHD) near a two-dimensional (2D) X-type magnetic neutral line is consider...
Hall magnetohydrodynamics (MHD) properties near a two-dimensional (2D) X-type magnetic neutral line ...
The Hall Magnetohydrodynamic (MHD) model is a new paradigm for describing fast magnetic reconnection...
An exact self-similar solution is used to investigate current sheet formation at a magnetic neutral ...
The formation of a current sheet in a weakly collisional plasma can be modelled as a finite-time sin...
Current-sheet formation near a hyperbolic magnetic neutral line in the MHD model is investigated. In...
Current-sheet formation near a hyperbolic magnetic neutral line in the MHD model is investigated. In...
The framework for the Hall magnetohydrodynamic (MHD) model for plasma physics is built up from kinet...
An exact solution for the magnetohydrodynamic (MHD) equations for a time-dependent, two-dimensional ...
An exact solution for the magnetohydrodynamic (MHD) equations for a time-dependent, two-dimensional ...
An exact solution for the magnetohydrodynamic equations for a time-dependent, two-dimensional flow o...
A theoretical mean field closure for Hall magnetohydrodynamics (Hall-MHD) is developed to investigat...
A theoretical mean field closure for Hall magnetohydrodynamics (Hall-MHD) is developed to investigat...
Two-dimensional resistive Hall magnetohydrodynamics (MHD) code is used to investigate the dynamical ...
Plasma processes such as magnetic reconnection, turbulent regimes or dynamo-generated magnetic field...