We develop a framework for studying the statistical properties of current sheets in numerical sim-ulations of 3D magnetohydrodynamic (MHD) turbulence. We describe an algorithm that identifies current sheets in a simulation snapshot and then determines their geometrical properties (including length, width, and thickness) and intensities (peak current density and total energy dissipation rate). We then apply this procedure to simulations of reduced MHD turbulence and perform a statistical analysis on the obtained population of current sheets. We evaluate the role of reconnection by sepa-rately studying the populations of current sheets which contain magnetic X-points and those which do not. We find that the statistical properties of the two p...
General three-dimensional toroidal ideal magnetohydrodynamic equilibria with a continuum of nested f...
The statistical properties of the dissipation process constrain the analysis of large scale numerica...
We investigate using direct numerical simulations with grids up to 15363 points, the rate at which s...
We study the statistics of coherent current sheets, the population of X-type critical points, and re...
We demonstrate that the initial correlation between velocity and current density fluctuations can le...
Temporal evolution of a current sheet with initial perturbations is studied by using the three-dimen...
The statistical study of magnetic reconnection events in two-dimensional turbulence has been perform...
The three-dimensional (3D) Hall magnetohydrodynamics (HMHD) equations are often used to study turbul...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
In collisionless space and astrophysical plasmas dissipation of macroscopic energy into heat in the...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
A two-dimensional reconnecting current sheet is studied numerically in the magnetohydrodynamic appro...
The nonlinear dynamics of magnetic reconnection in turbulence is investigated through direct numeric...
The turbulent solar wind abounds with MHD discontinuities, and such discontinuities are often found ...
Systematic analysis of numerical simulations of two-dimensional magnetohydrodynamic turbulence revea...
General three-dimensional toroidal ideal magnetohydrodynamic equilibria with a continuum of nested f...
The statistical properties of the dissipation process constrain the analysis of large scale numerica...
We investigate using direct numerical simulations with grids up to 15363 points, the rate at which s...
We study the statistics of coherent current sheets, the population of X-type critical points, and re...
We demonstrate that the initial correlation between velocity and current density fluctuations can le...
Temporal evolution of a current sheet with initial perturbations is studied by using the three-dimen...
The statistical study of magnetic reconnection events in two-dimensional turbulence has been perform...
The three-dimensional (3D) Hall magnetohydrodynamics (HMHD) equations are often used to study turbul...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
In collisionless space and astrophysical plasmas dissipation of macroscopic energy into heat in the...
In the presence of turbulence, magnetic field lines lose their dynamical identity and particles entr...
A two-dimensional reconnecting current sheet is studied numerically in the magnetohydrodynamic appro...
The nonlinear dynamics of magnetic reconnection in turbulence is investigated through direct numeric...
The turbulent solar wind abounds with MHD discontinuities, and such discontinuities are often found ...
Systematic analysis of numerical simulations of two-dimensional magnetohydrodynamic turbulence revea...
General three-dimensional toroidal ideal magnetohydrodynamic equilibria with a continuum of nested f...
The statistical properties of the dissipation process constrain the analysis of large scale numerica...
We investigate using direct numerical simulations with grids up to 15363 points, the rate at which s...