EGU2020-3523
https://doi.org/10.5194/egusphere-egu2020-3523
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Scaling of magnetic reconnection with a limited x-line extent

Kai Huang1,2,3, Yi-Hsin Liu3, Quanming Lu1,2, and Michael Hesse4
Kai Huang et al.
  • 1CAS Key Lab of Geospace Environment, School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, China
  • 2CAS Center for Excellence in Comparative Planetology, China
  • 3Dartmouth College, Hanover, NH 03750, USA
  • 4University of Bergen, Bergen, Norway

Contrary to all the 2D models, where the reconnection x-line extent is infinitely long, we study magnetic reconnection in the opposite limit. The scaling of the average reconnection rate and outflow speed are modeled as a function of the x-line extent. An internal x-line asymmetry along the current direction develops because of the flux transport by electrons beneath the ion kinetic scale, and it plays an important role in suppressing reconnection in the short x-line limit; the average reconnection rate drops because of the limited active region, and the outflow speed reduction is associated with the reduction of the J×B force, that is caused by the phase shift between the J and B profiles, also as a consequence of this flux transport.

How to cite: Huang, K., Liu, Y.-H., Lu, Q., and Hesse, M.: Scaling of magnetic reconnection with a limited x-line extent, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-3523, https://doi.org/10.5194/egusphere-egu2020-3523, 2020

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