Spontaneous reconnection at a separator current layer. I. Nature of the reconnection
Julie E. H. Stevenson, Clare E. Parnell

TL;DR
This paper investigates the detailed process of magnetic reconnection at a separator in three-dimensional resistive magnetohydrodynamic simulations, revealing a two-phase process with rapid initial energy release followed by slow, bursty reconnection.
Contribution
It provides the first detailed analysis of separator reconnection dynamics, highlighting the two-phase process and asymmetric reconnection behavior in 3D MHD simulations.
Findings
Rapid initial reconnection reduces current by 2.3 times
75% of magnetic energy converts to internal energy during the first phase
Reconnection occurs along most of the separator, asymmetrically, and in bursts later
Abstract
Magnetic separators, which lie on the boundary between four topologically-distinct flux domains, are prime locations in three-dimensional magnetic fields for reconnection, especially in the magnetosphere between the planetary and interplanetary magnetic field and also in the solar atmosphere. Little is known about the details of separator reconnection and so the aim of this paper, which is the first of two, is to study the properties of magnetic reconnection at a single separator. Three-dimensional, resistive magnetohydrodynamic numerical experiments are run to study separator reconnection starting from a magnetohydrostatic equilibrium which contains a twisted current layer along a single separator linking a pair of opposite-polarity null points. The resulting reconnection occurs in two phases. The first is short involving rapid-reconnection in which the current at the separator is…
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