collaborators

6 papers

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

Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona

Suli Ma, Eduard P. Kontar, Daniel L. Clarkson +2

Solar radio bursts exhibit complex fine structures that reveal intricate coronal plasma dynamics. Here, we report detection of spike-like repeating burst pairs, characterized by tw…

astro-ph.SR2026

Solar Energetic Particle Events and Associated Type II Radio Bursts from Different Source Regions

Xuchun Duan, Ting Li, Yingli Cui +7

Large solar energetic particle (SEP) events are thought to originate from the shocks driven by fast coronal mass ejections (CMEs) and thus generally accompanied by type II radio bu…

astro-ph.SR2026

A Major Geomagnetic Storm in 2024 October Linked to Sympathetic CME--Prominence Eruptions

Rui Wang, Huidong Hu, Xiaowei Zhao +11

Improving predictions of the geomagnetic impact of coronal mass ejections (CMEs) requires understanding how solar source properties relate to in-situ measurements at Earth. However…

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.SR2025

Tracking an eruptive intermediate prominence originating from the farside of the Sun

Qingmin Zhang, Wenwei Pan, Beili Ying +7

In this paper, we carry out multiwavelength and multiview observations of the eruption of an intermediate prominence originating from the farside of the Sun on 2023 March 12. The s…