21 citations · 41 across the 7 of their papers we have counts for
8 papers
Self-constrained Magnetic Reconnection of a Solar Flare Co-spatial with a Non-ejected Filament
Ye Qiu, Changxue Chen, Anqin Chen +11
For flares associated with eruptive filaments, the filament normally rises above the post-flare loops. Here, we report an unusual event in which the post-flare loops instead overli…
Data-constrained magnetohydrodynamic simulation of global solar corona including solar wind effects within 2.5
Yihua Li, Guoyin Chen, Jinhan Guo +6
Total solar eclipses (TSEs) provide a unique opportunity to observe the large-scale solar corona. The solar wind plays an important role in forming the large-scale coronal structur…
The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field
Ye Qiu, Yang Guo, Mingde Ding +3
Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms. Particularly, some geom…
Observational Study of Recurrent Jets: Evolution of Magnetic Flux, Current, and Helicity
Chang Zhou, Yang Guo, Guoyin Chen +2
We observed three recurrent blowout jets in an active regio with Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory (SDO). Using Helioseismic Magnetic Imager…
Astronomical image denoising by self-supervised deep learning and restoration processes
Tie Liu, Yuhui Quan, Yingna Su +9
Image denoising based on deep learning has witnessed significant advancements in recent years. However, existing deep learning methods lack quantitative control of the deviation or…
Failure of a solar filament eruption caused by magnetic reconnection with overlying coronal loops
Leping Li, Hongqiang Song, Yijun Hou +11
Failure of a filament eruption caused by magnetic reconnection between the erupting filament and the overlying magnetic field has been previously proposed in numerical simulations.…
Light Bridges and Solar Active Region Evolution Processes
Fuyu Li, Changhui Rao, Xinhua Zhao +5
The formation mechanism of light bridges (LBs) is strongly related to the dynamic evolution of solar active regions (ARs). To study the relationship between LB formation and AR evo…
Can we detect coronal mass ejections through asymmetries of Sun-as-a-star extreme-ultraviolet spectral line profiles?
Zihao Yang, Hui Tian, Xianyong Bai +8
Coronal mass ejections (CMEs) are the largest-scale eruptive phenomena in the solar system. Associated with enormous plasma ejections and energy release, CMEs have an important imp…