6 papers
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…
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…
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…
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…
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…
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…