activity
20182023
most citedA fundamental mechanism of solar eruption initiation

156 citations · 444 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2023★ 3 cited

Quantification of the Writhe Number Evolution of Solar Filament Axes

Zhenjun Zhou, Chaowei Jiang, Hongqiang Song +3

Solar filament eruptions often show complex and dramatic geometric deformation that is highly relevant to the underlying physical mechanism triggering the eruptions. It has been we…

astro-ph.SR2023

The Mechanism of Magnetic Flux Rope Rotation During Solar Eruption

Zhenjun Zhou, Chaowei Jiang, Xiaoyu Yu +3

Solar eruptions often show the rotation of filaments, which is a manifestation of the rotation of erupting magnetic flux rope (MFR). Such a rotation of MFR can be induced by either…

astro-ph.SR2022★ 21 cited

The Rotation of Magnetic Flux Rope Formed during Solar Eruption

Zhenjun Zhou, Chaowei Jiang, Rui Liu +3

The eruptions of solar filaments often show rotational motion about their rising direction, but it remains elusive what mechanism governs such rotation and how the rotation is rela…

astro-ph.SR2021★ 1 cited

Resolving Two Distinct Thermal X-ray Components in A compound Solar Flare

Zhenjun Zhou, Rui Liu, Jianqing Sun +6

X-ray emission provides the most direct diagnostics of the energy-release process in solar flares. Occasionally, a superhot X-ray source is found to be above hot flare loops of ~10…

astro-ph.SR2021★ 156 cited

A fundamental mechanism of solar eruption initiation

Chaowei Jiang, Xueshang Feng, Rui Liu +8

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are initiated remains unclear. Prevailing theories often rely on special magnetic topologies t…

astro-ph.SR2021★ 7 cited

The configuration and failed eruption of a complex magnetic flux rope above a δ sunspot region

Lijuan Liu, Jiajia Liu, Jun Chen +4

Aims. We investigate the configuration of a complex flux rope above a δ sunspot region in NOAA AR 11515, and its eruptive expansion during a confined M5.3-class flare. Methods. We…