2018/04/30 by Justin Walker, Stanislav Boldyrev, Nuno Loureiro · 1 citation
Physics and Astronomy · #physics.plasm-ph
paper · pdf · doi:10.1103/physreve.98.033209
published as Phys. Rev. E 98, 033209 (2018) · 5 pages, 7 figures
arxiv created 2018/09/24 · arxiv updated 2018/09/25
It has been proposed recently by Loureiro & Boldyrev [Phys. Rev. Lett. 118, 245101 (2017)] and Mallet et al. [Mon. Not. R. Astron. Soc. 468, 4862 (2017)] that strongly anisotropic current sheets formed in the inertial range of magnetohydrodynamic turbulence become affected by the tearing instability at scales smaller than a critical scale λc, and larger than the dissipation scale of turbulence. If true, this process can modify the nature of energy cascade at smaller scales, leading to a new, tearing-mediated regime of magnetohydrodynamic (MHD) turbulence. In this work we present a numerical study of strongly anisotropic, two-dimensional turbulent eddies, and we demonstrate that the tearing instability can indeed compete with their nonlinear evolution. The results, therefore, provide direct numerical support for the picture that a new regime of MHD turbulence can exist below λc.