11 citations · 18 across the 8 of their papers we have counts for
6 papers · 1 filter
Electron acceleration by turbulent reconnection in solar flares
Zining Ren, Xin Cheng, Yulei Wang +1
Solar flares can release magnetic energy explosively in the corona and produce high-energy particles on short timescales. However, how and where these particles are accelerated rem…
Unprecedent fast winking of solar flares triggered by bursty magnetic reconnection
Ting Li, Xuchun Duan, Yijun Hou +13
Flare ribbons form as a result of energy deposition associated with particles accelerated in low layers of the solar atmosphere. The fine-scale structures of flare ribbons, also ca…
Discussion on the vanishment of solar atmospheric structures during magnetic reconnection
Jun Zhang, Tao Ding, Yulei Wang
In solar atmosphere, magnetic reconnection alters the topological connectivity, and magnetic energy is released. However, the length change of the reconnecting structures has rarel…
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…
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…
A Method for Determining the Locations and Configurations of Magnetic Reconnection within 3D Turbulent Plasmas
Yulei Wang, Xin Cheng, Yang Guo +2
Context. Three-dimensional (3D) reconnection is an important mechanism for efficiently releasing energy during astrophysical eruptive events, which is difficult to be quantitativel…