activity
20182025
collaborators

5 papers

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

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…

astro-ph.SR2025

The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active Regions

Jinhan Guo, Y. W. Ni, B. Schmieder +9

Coronal mass ejections (CMEs) are the eruptions of magnetised plasma from the Sun and are considered the main driver of adverse space weather events. Hence, undrstanding its format…

astro-ph.SR2024

Periodic Coronal Rain Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic Simulation

Zekun Lu, Feng Chen, J. H. Guo +5

The periodic coronal rain and in-phase radiative intensity pulsations have been observed in multiple wavelengths in recent years. However, due to the lack of three-dimensional coro…

astro-ph.SR2018

Three-dimensional MHD Simulations of Solar Prominence Oscillations in a Magnetic Flux Rope

Yu-Hao Zhou, C. Xia, R. Keppens +2

Solar prominences are subject to all kinds of perturbations during their lifetime, and frequently demonstrate oscillations. The study of prominence oscillations provides an alterna…