activity
20162026
most citedA Circular White-Light Flare with Impulsive and Gradual White-Light Kernels

43 citations · 112 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2026

Back Reaction of the Untwisting Solar Corona Scars Sunspots

Chen Xing, Xin Cheng, Guillaume Aulanier +1

The evolution of magnetic fields in the tenuous solar corona is predominantly governed by the motions of the underlying dense photosphere. Despite, coronal magnetic restructuring d…

astro-ph.SR2025

Two-stage primary acceleration in filament initial eruption under a fan-spine magnetic configuration

Haitang Li, Ke Yu, Chang Zhou +6

Understaning the filament rising process is crucial for unveiling the triggering mechanisms of the coronal mass ejections and forecasting the space weather. In this paper, we prese…

astro-ph.SR2025

High-Resolution Modelling of Coronae and Winds in Solar-type Stars with Varying Rotation Rates I. X-ray Coronae

Yue-Hong Chen, Julián D. Alvarado-Gómez, Xin Cheng +8

Stellar coronae are believed to be the main birthplace of various stellar magnetic activities. However, the structures and properties of stellar coronae remain poorly understood. U…

astro-ph.SR2024

Eruption of a million-Kelvin warm magnetic flux rope on the Sun

Leping Li, Hongqiang Song, Hardi Peter +4

Solar magnetic flux rope (MFR) plays a central role in the physics of coronal mass ejections (CMEs). It mainly includes a cold filament at typical chromospheric temperatures (10000…

astro-ph.SR2024★ 18 cited

A model for heating the super-hot corona in solar active regions

Zekun Lu, Feng Chen, M. D. Ding +3

What physical mechanisms heat the outer solar or stellar atmosphere to million-Kelvin temperatures is a fundamental but long-standing open question. In particular, the solar corona…

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…