EGU22-5192
https://doi.org/10.5194/egusphere-egu22-5192
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Identifying active magnetic reconnection in simulations and in situ observations of plasma turbulence using magnetic flux transport

Tak Chu Li1, Yi-Hsin Liu1, Yi Qi2,3, and Christopher T. Russell3
Tak Chu Li et al.
  • 1Department of Physics and Astronomy, Dartmouth College, Hanover, United States of America (tak.chu.li@dartmouth.edu)
  • 2Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, United States of America
  • 3Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, United States of America

For decades, magnetic reconnection has been suggested to play an important role in the dynamics and energetics of plasma turbulence by spacecraft observations, numerical simulations and theory. Reliable approaches to study reconnection in turbulence are essential to advance this frontier topic of plasma physics. A new method based on magnetic flux transport (MFT) has been recently developed to identify reconnection activity in turbulent plasmas. Applications to gyrokinetic simulations of two- and three-dimensional (2D and 3D) plasma turbulence, and MMS observations of reconnection events in the magnetosphere have demonstrated the capability and accuracy of MFT in identifying active reconnection in turbulence. In 2D, MFT identifies multiple active reconnection X-lines; two of them have developed bi-directional electron and ion outflow jets, observational signatures for reconnection, while one of the X-line does not have bi-directional electron or ion outflow jets, beyond the category of electron-only reconnection recently discovered in the turbulent magnetosheath. In 3D, plentiful reconnection X-lines are identified through MFT, and a new picture of reconnection in turbulence results. In space, MMS observations have provided first evidence for MFT signatures of active reconnection under varying plasma conditions throughout the Earth's magnetosphere. MFT is applicable to in situ measurements by spacecraft missions, including PSP and Solar Orbiter, and laboratory experiments.

How to cite: Li, T. C., Liu, Y.-H., Qi, Y., and Russell, C. T.: Identifying active magnetic reconnection in simulations and in situ observations of plasma turbulence using magnetic flux transport, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-5192, https://doi.org/10.5194/egusphere-egu22-5192, 2022.

Comments on the display material

to access the discussion