53 citations · 137 across the 7 of their papers we have counts for
9 papers
Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over Quadrupolar Magnetic Configuration in a Solar Flare
Zhenjun Zhou, Xin Cheng, Lijuan Liu +3
A second emission enhancement in warm coronal extreme-ultraviolet (EUV) lines (about 2-7 MK) during some solar flares is known as the EUV late phase. Imaging observations confirm t…
Why torus-unstable solar filaments experience failed eruption?
Zhenjun Zhou, Xin Cheng, Jie Zhang +5
To investigate the factors that control the success and/or failure of solar eruptions, we study the magnetic field and 3-Dimensional (3D) configuration of 16 filament eruptions dur…
Origin and Structures of Solar Eruptions II: Magnetic Modeling (Invited Review)
Yang Guo, Xin Cheng, M. D. Ding
The topology and dynamics of the three-dimensional magnetic field in the solar atmosphere govern various solar eruptive phenomena and activities, such as flares, coronal mass eject…
A Statistical Study of the Average Iron Charge Distributions inside Magnetic Clouds for Solar Cycle 23
Hongqiang Song, Ze Zhong, Yao Chen +5
Magnetic clouds (MCs) are the interplanetary counterpart of coronal magnetic flux ropes. They can provide valuable information to reveal the flux rope characteristics at their erup…
Bidirectional outflows as evidence of magnetic reconnection leading to a solar microflare
Jie Hong, M. D. Ding, Ying Li +5
Magnetic reconnection is a rapid energy release process that is believed to be responsible for flares on the Sun and stars. Nevertheless, such flare-related reconnection is mostly…
Predicting the Arrival Time of Coronal Mass Ejections with the Graduated Cylindrical Shell and Drag Force Model
Tong Shi, Yikang Wang, Linfeng Wan +3
Accurately predicting the arrival of coronal mass ejections (CMEs) at the Earth based on remote images is of critical significance in the study of space weather. In this paper, we…