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20242026
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astro-ph.SR2026

Unprecedent fast winking of solar flares triggered by bursty magnetic reconnection

Ting Li, Xuchun Duan, Yijun Hou +13

Flare ribbons form as a result of energy deposition associated with particles accelerated in low layers of the solar atmosphere. The fine-scale structures of flare ribbons, also ca…

astro-ph.SR2026

Fine Structure and Formation Mechanism of a Sunspot Bipolar Light Bridge in NOAA AR 13663

Fangfang Qiao, Hao Li, Jiasheng Wang +3

Bipolar Light Bridges (BLBs) are bright regions located between sunspot umbrae of opposite magnetic polarity. They are typically characterized by strong magnetic fields and intense…

astro-ph.SR2025

Sympathetic Eruption of Two Filaments and Associated Solar Coronal Jet

Jiayan Yang, Leping Li, Huadong Chen +4

Combining the high-quality observations from the {\it Solar Dynamics Observatory} (SDO), the Global Oscillation Network Group (GONG), and the Chinese H Solar Explorer (CHASE), w…

astro-ph.SR2025

Responses of a Coronal Hole to a Fast Flare-Driven Coronal Wave

Xiaofan Zhang, Huadong Chen, Guiping Zhou +12

Coronal waves, significant solar phenomena, act as diagnostic tools for scientists studying solar atmosphere properties. Here, we present a novel observation detailing how a corona…

astro-ph.SR2024

Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops

Leping Li, Hongqiang Song, Yijun Hou +11

Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…

astro-ph.SR2024

Alpha-Proton Differential Flow of A Coronal Mass Ejection at 15 Solar Radii

Xuechao Zhang, Hongqiang Song, Xiaoqian Wang +4

Alpha-proton differential flow () of coronal mass ejections (CMEs) and solar wind from the Sun to 1 au and beyond could influence the instantaneous correspondence of absolu…