collaborators

5 papers

astro-ph.SR2026

Multiple Extreme Ultraviolet Peaks Attributed to Three-dimensional Magnetic Reconnection in a Long-duration Solar Flare

Shihan Li, Jinhan Guo, Wensi Wang +5

Solar flares are a major driver of hazardous space weather, whose intense electromagnetic emissions and energetic particles can significantly disturb the near-Earth space environme…

astro-ph.SR2026

Rotation of a Solar Jet Driven by Plasma Flow along Helical Magnetic Fields in an Active Region

Lei Huang, Yang Guo, Zhen Li +2

Solar jets, collimated plasma ejections driven by magnetic reconnection, play a vital role in energy transport and coronal heating. While rotational motions in jets are often attri…

astro-ph.SR2025

Particle Acceleration and Transport in the Large-scale Current Sheet under an Erupting Magnetic Flux Rope

Hao Wu, Yang Guo, Rony Keppens +4

We investigate the acceleration and transport of electrons in the highly fine-structured current sheet that develops during magnetic flux rope (MFR) eruptions. Our work combines ul…

astro-ph.SR2025

SIP-IFVM: An observation-based magnetohydrodynamic model of coronal mass ejection

Haopeng Wang, Jinhan Guo, Stefaan Poedts +12

Currently, achieving a balance between computational efficiency, accuracy, and numerical stability in CME simulations, particularly in the sub-Alfv{'e}nic coronal region, remains a…

astro-ph.SR2025

Data-constrained Magnetohydrodynamic Simulation of a Filament Eruption in a Decaying Active Region 13079 on a Global Scale

Yihua Li, Yang Guo, Jinhan Guo +3

Filaments are special plasma phenomena embedded in the solar atmosphere, characterized by unique thermodynamic properties and magnetic structures. Magnetohydrodynamic (MHD) simulat…