activity
20002023
most citedObservation of An Evolving Magnetic Flux Rope Prior To and During A Solar Eruption

325 citations · 2.7k across the 88 of their papers we have counts for

collaborators

88 papers

astro-ph.SR2023

Spectral Features of the Solar Transition Region and Chromospheric Lines at Flare Ribbons Observed with IRIS

Lingfang Wang, Ying Li, Qiao Li +2

We report on the spectral features of the Si IV 1402.77 Å, C II 1334.53 Å, and Mg II h or k lines, formed in the layers from the transition region to the chromosphere, in three two…

astro-ph.SR2023

Radiative Magnetohydrodynamic Simulation of the Confined Eruption of a Magnetic Flux Rope: Unveiling the Driving and Constraining Forces

Can Wang, Feng Chen, Mingde Ding +1

We analyse the forces that control the dynamic evolution of a flux rope eruption in a three-dimensional (3D) radiative magnetohydrodynamic (RMHD) simulation. The confined eruption…

astro-ph.SR2023★ 25 cited

Three-dimensional Turbulent Reconnection within Solar Flare Current Sheet

Yulei Wang, Xin Cheng, Mingde Ding +3

Solar flares can release coronal magnetic energy explosively and may impact the safety of near-earth space environments. Their structures and properties on macroscale have been int…

astro-ph.SR2023★ 22 cited

Spectral Observations and Modeling of a Solar White-light Flare Observed by CHASE

De-Chao Song, Jun Tian, Y. Li +11

The heating mechanisms of solar white-light flares remain unclear. We present an X1.0 white-light flare on 2022 October 2 (SOL2022-10-02T20:25) observed by the Chinese \ha\ Solar E…

astro-ph.SR2023★ 5 cited

An Atypical Plateau-like Extreme-ultraviolet Late-phase Solar Flare Driven by the Non-radial Eruption of a Magnetic Flux Rope

Yuehong Chen, Yu Dai, Mingde Ding

Recent observations in extreme-ultraviolet (EUV) wavelengths reveal an EUV late phase in some solar flares, which is characterized by a second peak in the warm coronal emissions (a…

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…