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Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence
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Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence
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We develop a framework for studying the statistical properties of current sheets in numerical simulations 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 separately 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 populations are different in general. We compare the scaling of these properties to phenomenological predictions obtained for the inertial range of MHD turbulence. Finally, we test whether the reconnecting current sheets are consistent with the Sweet-Parker model.
Forward citations
Cited by 1 Pith paper
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Emergence and Detection of Electron-Scale Current Sheets in Turbulence with MMS Observations and fully kinetic 3D simulations
Electron-scale current sheets dominate 3D kinetic turbulence widths (peak ~2 d_e, broken power law), and PVI detects them but inflates sizes via oblique crossings.
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