activity
20242026
most citedParameter effects on the total intensity of H I Lyα line for a modelled coronal mass ejection and its driven shock

1 citations · 2 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

Simulation study of the cosmic ray Sun shadow with a time-dependent solar magnetic field model

Jie Xia, Ming-Yang Cui, Qiang Yuan +3

During the propagation of cosmic rays in the solar system, the Sun will block those particles and form a shadow whose position and depth are very important probe of the magnetic fi…

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

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

astro-ph.SR2024★ 1 cited

Improving image quality of the Solar Disk Imager (SDI) of the Lyman-alpha Solar Telescope (LST) onboard the ASO-S mission

Hui Liu, Hui Li, Sizhong Zou +11

The in-flight calibration and performance of the Solar Disk Imager (SDI), which is a pivotal instrument of the Lyman-alpha Solar Telescope (LST) onboard the Advanced Space-based So…

astro-ph.SR2024

Inflight Performance and Calibrations of the Lyman-alpha Solar Telescope on board the Advanced Space-based Solar Observatory

Bo Chen, Li Feng, Guang Zhang +40

The Lyman-alpha Solar Telescope (LST) on board the Advanced Space-based Solar Observatory (ASO-S) is the first payload to image the full solar disk and the solar corona in both whi…

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…

astro-ph.SR2024

Refinement of global coronal and interplanetary magnetic field extrapolations constrained by remote-sensing and in-situ observations at the solar minimum

Guanglu Shi, Li Feng, Beili Ying +2

Solar magnetic fields are closely related to various physical phenomena on the sun, which can be extrapolated with different models from photospheric magnetograms. However, the Ope…

astro-ph.SR2024

Spectral and Imaging Observations of a C2.3 White-Light Flare from the Advanced Space-Based Solar Observatory (ASO-S) and the Chinese H Solar Explorer (CHASE)

Qiao Li, Ying Li, Yang Su +27

Solar white-light flares are characterized by an enhancement in the optical continuum, which are usually large flares (say X- and M-class flares). Here we report a small C2.3 white…

astro-ph.SR2024

A Statistical Study of Solar White-Light Flares Observed by the White-light Solar Telescope of the Lyman-alpha Solar Telescope on the Advanced Space-based Solar Observatory (ASO-S/LST/WST) at 360 nm

Zhichen Jing, Ying Li, Li Feng +26

Solar white-light flares (WLFs) are those accompanied by brightenings in the optical continuum or integrated light. The White-light Solar Telescope (WST), as an instrument of the L…