activity
20152026
most citedStructure, Stability, and Evolution of Magnetic Flux Ropes from the Perspective of Magnetic Twist

315 citations · 662 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.SR2026

Parametric Study of the Torus Instability Threshold

Jun Chen, Bernhard Kliem, Rui Liu

The torus instability of an arched current channel has been suggested to initiate and drive major solar and stellar eruptions. Its threshold, given by the critical decay index of t…

astro-ph.SR2026

FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis

Jun Chen, Thomas Wiegelmann, Li Feng +2

We present a new version of FastQSL for locating quasi-separatrix layers (QSLs) -- regions characterized by strong magnetic connectivity gradients, preferential current buildup, an…

astro-ph.SR2023

Observations of a Failed Solar Filament Eruption Involving External Reconnection

Yuehong Chen, Xin Cheng, Jun Chen +2

We report a failed solar filament eruption that involves external magnetic reconnection in a quadrupolar magnetic configuration. The evolution exhibits three kinematic evolution ph…

astro-ph.SR2023★ 24 cited

A Model for Confined Solar Eruptions Including External Reconnection

Jun Chen, Xin Cheng, Bernhard Kliem +1

The violent disruption of the coronal magnetic field is often observed to be restricted to the low corona, appearing as a confined eruption. The possible causes of the confinement…

astro-ph.SR2022★ 33 cited

FastQSL: A Fast Computation Method for Quasi-separatrix Layers

Peijin Zhang, Jun Chen, Rui Liu +1

Magnetic reconnection preferentially takes place at the intersection of two separatrices or two quasi-separatrix layers, which can be quantified by the squashing factor Q, whose ca…

astro-ph.SR2021

Formation of Magnetic Flux Rope during Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux

Chaowei Jiang, Jun Chen, Aiying Duan +5

Magnetic flux ropes (MFRs) constitute the core structure of coronal mass ejections (CMEs), but hot debates remain on whether the MFR forms before or during solar eruptions. Further…