EGU24-11788, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-11788
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Material Barriers to the Diffusion of Magnetic Field Lines

Alex Pablo Encinas Bartos1, Balint Kaszás1, Sergio Servidio2, and George Haller1
Alex Pablo Encinas Bartos et al.
  • 1Institute for Mechanical Systems, ETH Zurich, Zurich, Switzerland
  • 2Dipartimento di Fisica, Università della Calabria, Cosenza, Italy

Recent work has identified objective (frame-indifferent) material barriers that inhibit the flux of dynamically active vectorial quantities (i.e. linear momentum, angular momentum and vorticity) in Navier-Stokes flows. In the context of magnetohydrodynamics (MHD) the magnetic field vector is directly coupled to the evolution of the velocity field through the Lorentz force and therefore qualifies as a dynamically active vector field. In this work, we identify active Eulerian and Lagrangian barriers that block the diffusion of magnetic field lines in two-dimensional (2D) and three-dimensional (3D) MHD turbulence. These distinguished material surfaces provide physics-based and frame-indifferent active magnetic coherent structures that locally divide the space into two regions with minimal diffusion of magnetic field lines. In 2D, these barriers are directly connected to the electric current density. We propose an algorithm for the automated identification of such barriers from 2D and 3D numerical data of MHD turbulence simulations.

How to cite: Encinas Bartos, A. P., Kaszás, B., Servidio, S., and Haller, G.: Material Barriers to the Diffusion of Magnetic Field Lines, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-11788, https://doi.org/10.5194/egusphere-egu24-11788, 2024.