Extension of the Electron Dissipation Region in Collisionless Hall MHD Reconnection
Brian P. Sullivan, A. Bhattacharjee, Yi-Min Huang

TL;DR
This study uses scaling arguments and numerical experiments within hyper-resistive Hall MHD to analyze the length of the electron dissipation region in collisionless reconnection, revealing its dependence on hyper-resistivity and electron inertia.
Contribution
It extends the understanding of electron dissipation region length in collisionless reconnection by incorporating hyper-resistivity and electron inertia effects, which previous models did not predict.
Findings
Electron dissipation region length depends on hyper-resistivity.
Region length remains below one ion skin depth even with high hyper-resistivity.
Region length scales with electron inertia as (me/mi)^{3/8}.
Abstract
This paper presents Sweet-Parker type scaling arguments in the context of hyper-resistive Hall magnetohyrdodynamics (MHD). The predicted steady state scalings are consistent with those found by Chac\'on et al. [PRL 99, 235001 (2007)], though as with that study, no prediction of electron dissipation region \emph{length} is made. Numerical experiments confirm that both cusp-like and modestly more extended geometries are realizable. However, importantly, the length of the electron dissipation region, which is taken as a parameter by several recent studies, is found to depend explicitly on the level of hyper-resistivity. Furthermore, although hyper-resistivity can produce more extended electron dissipation regions, the length of the region remains smaller than one ion skin depth for the largest values of hyper-resistivity considered here. These electron dissipation regions are significantly…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Magnetic confinement fusion research · Solar and Space Plasma Dynamics
