2013/02/06 by Vladimir Zhdankin, Dmitri A. Uzdensky, Jean C. Perez +1 · 1 citation
Physics and Astronomy · #astro-ph.HE #physics.plasm-ph #physics.space-ph
paper · pdf · doi:10.1088/0004-637x/771/2/124
published as The Astrophysical Journal, 771, 124 (2013) · 19 pages, 19 figures
arxiv created 2013/02/06 · arxiv updated 2013/06/27
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.