activity
20152026
most citedWhy does the apparent mass of a coronal mass ejection increase?

32 citations · 302 across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.SR2026

Spatio-temporal Characteristics of Very Long-periodic Pulsations in Solar Metrewave Bursts: Implications for their Origins

Dong Li, Lei Lu, Jingye Yan +5

We traced the origin of very long-periodic pulsations (VLPs) in type-I burst chains on 2024 February 14. Seven successive and repetitive pulsation structures appeared in radio dyna…

astro-ph.SR2026★ 2 cited

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

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 Å, is the brightest solar ultraviolet (UV) line. However, comprehensive observations of the Ly emission line acro…

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…

astro-ph.SR2024★ 1 cited

Parameter effects on the total intensity of H I Lyα line for a modelled coronal mass ejection and its driven shock

Beili Ying, Guanglu Shi, Li Feng +5

The combination of the H I Lyα (121.6 nm) line formation mechanism with ultraviolet (UV) Lyα and white-light (WL) observations provides an effective method for determining the elec…