activity
20162026
most citedEvolution of A Magnetic Flux Rope toward Eruption

40 citations · 133 across the 13 of their papers we have counts for

collaborators

14 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.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

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★ 1 cited

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…

astro-ph.SR2024

Nonparametric Statistics on Magnetic Properties at the Footpoints of Erupting Magnetic Flux Ropes

Rui Liu, Wensi Wang

It is under debate whether the magnetic field in the solar atmosphere carries neutralized electric currents; particularly, whether a magnetic flux rope (MFR), which is considered t…

astro-ph.SR2023★ 29 cited

Complete replacement of magnetic flux in a flux rope during a coronal mass ejection

Tingyu Gou, Rui Liu, Astrid M. Veronig +5

Solar coronal mass ejections are the most energetic events in the Solar System. In their standard formation model, a magnetic flux rope builds up into a coronal mass ejection throu…

astro-ph.SR2022★ 14 cited

Investigating pre-eruptive magnetic properties at the footprints of erupting magnetic flux ropes

Wensi Wang, Jiong Qiu, Rui Liu +4

It is well established that solar eruptions are powered by free magnetic energy stored in current-carrying magnetic field in the corona. It has also been generally accepted that ma…

astro-ph.SR2021★ 2 cited

Erupting Magnetic Flux Rope Affects Running Penumbral Waves

Wensi Wang, Rui Liu

It is well known that solar flares have broad impacts on the low atmosphere, but it is largely unknown how they affect sunspot waves and oscillations. It is also under debate as to…

astro-ph.SR2020★ 8 cited

Electric Currents through J-shaped and Non-J-shaped Flare Ribbons

Yuwei He, Rui Liu, Lijuan Liu +3

Recently solar flares exhibiting a double J-shaped ribbons in the lower solar atmosphere have been paid increasing attention in the context of extending the two-dimensional standar…

astro-ph.SR2020★ 19 cited

Eruption of Solar Magnetic Flux Ropes Caused by Flux Feeding

Quanhao Zhang, Yuming Wang, Rui Liu +5

Large-scale solar eruptions are believed to have a magnetic flux rope as the core structure. However, it remains elusive as to how the flux rope builds up and what triggers its eru…

astro-ph.SR2018★ 40 cited

Evolution of A Magnetic Flux Rope toward Eruption

Wensi Wang, Chunming Zhu, Jiong Qiu +3

It is well accepted that a magnetic flux rope (MFR) is a critical component of many coronal mass ejections (CMEs), yet how it evolves toward eruption remains unclear. Here we inves…

astro-ph.SR2016★ 20 cited

Tornado-Like Evolution of A Kink-Unstable Solar Prominence

Wensi Wang, Rui Liu, Yuming Wang

We report on the tornado-like evolution of a quiescent prominence on 2014 November 1. The eastern section of the prominence first rose slowly transforming into an arch-shaped struc…