collaborators

7 papers

astro-ph.SR2025

The Solar Close Observations and Proximity Experiments (SCOPE) mission

Jun Lin, Jing Feng, Zhenhua Ge +31

The Solar Close Observations and Proximity Experiments (SCOPE) mission will send a spacecraft into the solar atmosphere at a low altitude of just 5 R_sun from the solar center. It…

astro-ph.SR2025

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…

astro-ph.SR2025

Microwave Imaging Spectroscopy Diagnosis of the Slow-rise Precursor of a Major Solar Eruption

Yuankun Kou, Xin Cheng, Sijie Yu +3

In this Letter, taking advantage of microwave data from the Expanded Owens Valley Solar Array and extreme-ultraviolet (EUV) data from the Atmospheric Imaging Assembly, we present t…

astro-ph.SR2025

Initiation Route of Coronal Mass Ejections: II. The Role of Filament Mass

Chen Xing, Xin Cheng, Guillaume Aulanier +1

The thorough understanding on the initiation of coronal mass ejections (CMEs), which is manifested as a slow rise of pre-eruptive structures before the impulsive ejection in kinema…

astro-ph.SR2025

Basic Pattern of Three-dimensional Magnetic Reconnection within Strongly Turbulent Current Sheets

Yulei Wang, Xin Cheng, Mingde Ding

Magnetic reconnection is a fundamental mechanism of driving eruptive phenomena of different scales and may be coupled with turbulence as suggested by recent remote-sensing and in-s…

astro-ph.SR2025

Understanding observational characteristics of solar flare current sheets

Zining Ren, Yulei Wang, Xin Cheng +1

The elongated bright structures above solar flare loops are suggested to be current sheets, where magnetic reconnection takes place. Observations have revealed various characterist…