collaborators

5 papers

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

Two-sided-loop jet originates from the filament internal reconnection

Yunxue Huang, Jialin Li, Zhining Qu +4

Magnetic reconnection driving two-sided-loop jet is typically associated with interactions between an emerging bipole and the overlying horizontal magnetic field, or between filame…

astro-ph.SR2025

3D fast-mode Wave Propagation from Corona to Chromosphere: Triggering Mechanism for 3D Oscillations of filaments

Yunxue Huang, Qin Feng, Yuhu Miao +5

Moreton waves are widely regarded as the chromospheric counterpart of extreme ultraviolet (EUV) waves propagating in the corona. However, direct observational evidence confirming t…

astro-ph.SR2024

On the origin of a broad QFP wave train: unwinding jet as the driver

Xinping Zhou, Zehao Tang, Zhining Qu +5

Large-scale extreme-ultraviolet (EUV) waves commonly exhibit as single wavefront and are believed to be caused by coronal mass ejections (CMEs). Utilizing high spatiotemporal resol…

astro-ph.SR2024

Broad and Bi-directional narrow quasi-periodic fast-propagating wave trains associated with a filament-driven halo CME on 2023 April 21

Xinping Zhou, Yuandeng Shen, Yihua Yan +8

This paper presents three distinct wave trains that occurred on 2023 April 21: a broad quasi-periodic fast-propagating (QFP) wave train and a bi-directional narrow QFP wave train.…