EGU24-10581, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-10581
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Topology of turbulence within collisionless plasma reconnection

Bogdan Hnat1, Sandra Chapman1, and Nick Watkins1,2,3
Bogdan Hnat et al.
  • 1University of Warwick, CFSA, Department of Physics, Coventry, United Kingdom of Great Britain – England, Scotland, Wales (b.hnat@warwick.ac.uk)
  • 2Grantham Research Institute on Climate Change and the Environment, LSE, London, WC2A 2AE, UK
  • 3School of Engineering and Innovation, The Open University, Milton Keynes, MK7 6AA, UK

Magnetospheric Multi Scale four-point satellite observations are used to characterize the magnetic field line topology within a single reconnection current layer. We examine magnetopause reconnection where the spacecraft encounter the Electron Diffusion Region (EDR). We find fluctuating magnetic field with topology identical to that found for dynamically evolving vortices in hydrodynamic turbulence. The turbulence is supported by an electron-magnetohydrodynamic (EMHD) flow in which the magnetic field is effectively frozen into the electron fluid. Accelerated electrons are found in the EDR edge where we identify a departure from this turbulent topology, towards two-dimensional sheet-like structures. This is consistent with a scenario in which sub-ion scale turbulence can suppress electron acceleration within the EDR which would otherwise be possible in the electric field at the X-line.

How to cite: Hnat, B., Chapman, S., and Watkins, N.: Topology of turbulence within collisionless plasma reconnection, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-10581, https://doi.org/10.5194/egusphere-egu24-10581, 2024.