collaborators

6 papers

astro-ph.SR2025

Multiwavelength Observations for a Double-decker Filament Channel in AR 13102

Yin Zhang, Baolin Tan, Quan Wang +8

We present the observational evidence of the existence of a double-decker filament channel (FC) by using observations in extreme ultraviolet and Hα wavelengths. For both FCs, the…

astro-ph.SR2025

Probing Solar Polar Regions

Yuanyong Deng, Hui Tian, Jie Jiang +45

The magnetic fields and dynamical processes in the solar polar regions play a crucial role in the solar magnetic cycle and in supplying mass and energy to the fast solar wind, ulti…

astro-ph.SR2025

Radio dimming associated with filament eruptions in the meter and decimeter wavebands

Zhenyong Hou, Hui Tian, Jingye Yan +12

Filament eruptions are considered to be a common phenomenon on the Sun and other stars, yet they are rarely directly imaged in the meter and decimeter wavebands. Using imaging data…

astro-ph.SR2025

Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament

Hechao Chen, Hui Tian, Quanhao Zhang +8

Filament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly af…

astro-ph.SR2024

Ubiquitous Small-scale EUV Upflow-Like Events above Network Regions Observed by the Solar Orbiter/Extreme Ultraviolet Imager

Yadan Duan, Hechao Chen, Zhenyong Hou +2

Universal small-scale solar activity in quiet region are suggested to be a potential source of solar wind and the upper solar atmosphere. Here, with the high-resoltion 174 Ã ~imagi…

astro-ph.SR2024

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.…