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astro-ph.SR2026

Three-dimensional properties of a coronal shock and the longitudinal distribution of its related solar energetic particles

Yue Zhou, Li Feng, Guanglu Shi +6

This study aims to investigate the relationship between the spatial-temporal evolution of shock properties and the longitudinal dependence of SEP intensities and spectra. The shock…

astro-ph.SR2025

The Role of Far-side Magnetic Structures in Modeling 2024 Solar Eclipse

Guanglu Shi, Jiahui Shan, Li Feng +2

The corona is a crucial region that connects the solar surface to the solar wind and serves as the primary site of solar activity. The 2024 total solar eclipse (TSE) provides a uni…

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

Asymmetric Hard X-ray Radiation of Two Ribbons in a Thermal-Dominated C-Class Flare

Guanglu Shi, Li Feng, Jun Chen +9

The asymmetry in hard X-ray (HXR) emission at the footpoints (FPs) of flare loops is a ubiquitous feature closely associated with nonthermal electron transport. We analyze the asym…

astro-ph.SR2024

Association between a Failed Prominence Eruption and the Drainage of Mass from Another Prominence

Jianchao Xue, Li Feng, Hui Li +31

Sympathetic eruptions of solar prominences have been studied for decades, however, it is usually difficult to identify their causal links. Here we present two failed prominence eru…