activity
20242026
collaborators

5 papers

astro-ph.SR2026

Apparent magnetic field decay in a solar flare from Zeeman splitting of the Mg 12.32 microns observations

Yuanyong Deng, Xianyong Bai, Jie Hong +23

The magnetic field is the most fundamental observable in solar physics, while solar flares are the most violent, rapid magnetic energy-release events in the solar atmosphere. Decad…

astro-ph.SR2026

Detection and analysis of white-light emission in solar flares through light curve diagnostics

Shuanghong Li, Yongliang Song, Kun Wang +4

White-light flares (WLFs) are crucial for understanding the energy transport and heating processes in the lower solar atmosphere. Systematic studies are highly necessary. However,…

astro-ph.SR2025

Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament

Hechao Chen, Hui Tian, Quanhao Zhang +8

Filament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly af…

astro-ph.SR2024

Observation of a large-scale filament eruption initiated by two small-scale erupting filaments pushing out from below

Yongliang Song, Jiangtao Su, Qingmin Zhang +9

Filament eruptions often result in flares and coronal mass ejections (CMEs). Most studies attribute the filament eruptions to their instabilities or magnetic reconnection. In this…

astro-ph.SR2024

Persistent Upflows and Downflows at Active Region boundaries Observed by SUTRI and AIA

Yuchuan Wu, Zhenyong Hou, Wenxian Li +6

Upflows and downflows at active region (AR) boundaries have been frequently observed with spectroscopic observations at extreme ultraviolet (EUV) passbands. In this paper, we repor…