activity
20162021
most citedThe role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

62 citations · 149 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202128 cited

Magnetic Twists of Solar Filaments

Jinhan Guo, Yiwei Ni, Ye Qiu +3

Solar filaments are cold and dense materials situated in magnetic dips, which show distinct radiation characteristics compared to the surrounding coronal plasma. They are associate…

astro-ph.SR2021

Data-constrained Magnetohydrodynamic Simulation of a Long Duration Eruptive Flare

Yang Guo, Ze Zhong, M. D. Ding +3

We perform a zero- magnetohydrodynamic simulation for the C7.7 class flare initiated at 01:18 UT on 2011 June 21 using the Message Passing Interface Adaptive Mesh Refinement Ver…

astro-ph.SR202162 cited

The role of non-axisymmetry of magnetic flux rope in constraining solar eruptions

Ze Zhong, Yang Guo, Mingde Ding

Whether a solar eruption is successful or failed depends on the competition between different components of the Lorentz force exerting on the flux rope that drives the eruption. Th…

astro-ph.SR2020

The Magnetic Topology and Eruption Mechanism of a Multiple-ribbon Flare

Ye Qiu, Yang Guo, M. D. Ding +1

Multiple-ribbon flares are usually complex in their magnetic topologies and eruption mechanisms. In this paper, we investigate an X2.1 flare (SOL2015-03-11T16:22) that occurred in…

astro-ph.SR202029 cited

Imaging and spectral study on the null point of a fan-spine structure during a solar flare

Shuhong Yang, Qingmin Zhang, Zhi Xu +3

Using the multi-instrument observations, we make the first simultaneous imaging and spectral study on the null point of a fan-spine magnetic topology during a solar flare. When mag…

astro-ph.SR201830 cited

Transition from circular-ribbon to parallel-ribbon flares associated with a bifurcated magnetic flux rope

Z. Zhong, Y. Guo, M. D. Ding +2

Magnetic flux ropes play a key role in triggering solar flares in the solar atmosphere. In this paper, we investigate the evolution of active region NOAA 12268 within 36 hours from…