collaborators

6 papers

astro-ph.SR2026

On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage

Jinhan Guo, Y. Guo, H. Wu +9

Observations show that many solar eruptions remain confined within strong overlying magnetic fields, forming a so-called magnetic cage. While confinement by poloidal overlying fiel…

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

COCONUT: A coronal model with an energy decomposition strategy

Haopeng Wang, Stefaan Poedts, Andrea Lani +11

In this paper, we propose an energy decomposition method combined with an HLL Riemann solver that includes an additional dissipation term in the energy equation to improve the nume…

astro-ph.SR2025

High-Resolution Observation of Solar Prominence Plumes Induced by Enhanced Spicular Activity

Wensi Wang, Rui Liu, Runbin Luo +1

Solar prominences are the most prominent large-scale structures observed above the solar limb in emission in chromospheric lines but in absorption in coronal lines. At the bottom o…

astro-ph.SR2025

Size Distributions of Arcsecond-Scale Properties of Solar Flare Ribbons

Yue Zhang, Rui Liu, Wensi Wang +1

Solar flare ribbons are believed to map the footpoints of newly reconnected magnetic flux tubes, therefore shedding light on the reconnecting current sheet, which is rarely observe…

astro-ph.SR2025

Falling Threads During Solar Filament Eruptions

Yidian Wu, Rui Liu, Runbin Luo +1

Mass drainage is frequently observed in solar filaments. During filament eruptions, falling material most likely flows along magnetic field lines, which may provide important clues…