collaborators

5 papers

astro-ph.SR2026

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…

physics.plasm-ph2026

Central Equations and Band Structures of Linear Magnetohydrodynamic Waves in a Magneto-Lattice

Shiyu Sun, Peifeng Fan, Yulei Wang +3

We investigate the band structures and propagation properties of linear ideal magnetohydrodynamic (MHD) waves in a plasma with a spatially periodic background magnetic field (a mag…

astro-ph.SR2025

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…

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…