activity
20242026
collaborators

5 papers

astro-ph.SR2026

Three-dimensional evolution of a solar filament with multipoint observations

Qingmin Zhang, Jun Dai, Beili Ying +6

In this paper, we first devise a geometrical model, featuring a torus-like flux rope based on the shape of 3DCORE model. The global shape of the torus is an ellipse, while the cros…

astro-ph.SR2025

Early Evolution of the Cavity and Core of a Coronal Mass Ejection in the Inner Corona

Shuting Li, Li Feng, Beili Ying +5

Coronal mass ejections (CMEs) typically exhibit a three-component structure in white-light (WL) coronagraphs. Utilizing the seamless observations of the inner corona ( 3 R$_\o…

astro-ph.SR2025

Understanding the Lyα Emission Observed by the Solar Disk Imager Aboard the Advanced Space-based Solar Observatory

Yiliang Li, Ping Zhang, Zhengyuan Tian +12

The H I Lyman-alpha (Ly) emission, with a wavelength of 1216 Ã , is the brightest solar ultraviolet (UV) line. However, comprehensive observations of the Ly emission line a…

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…

astro-ph.SR2024

Sympathetic solar eruption on 2024 February 9

Shu-Yue Li, Qing-Min Zhang, Bei-Li Ying +3

In this paper, we perform a follow-up investigation of the solar eruption originating from active region (AR) 13575 on 2024 February 9. The primary eruption of a hot channel (HC) g…