activity
20182022
most citedA fundamental mechanism of solar eruption initiation

156 citations · 272 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR202221 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.SR2021156 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.SR20217 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…

astro-ph.SR202113 cited

The Source Locations of Major Flares and CMEs in the Emerging Active Regions

Lijuan Liu, Yuming Wang, Zhenjun Zhou +1

Major flares and coronal mass ejections (CMEs) tend to originate from the compact polarity inversion lines (PILs) in the solar active regions (ARs). Recently, a scenario named as "…

astro-ph.SR20209 cited

Variation of Magnetic Flux Ropes Through Major Solar Flares

Aiying Duan, Chaowei Jiang, Zhenjun Zhou +2

It remains unclear how solar flares are triggered and in what conditions they can be eruptive with coronal mass ejections. Magnetic flux ropes (MFRs) has been suggested as the cent…

astro-ph.SR2020

The Relationship between Chirality, Sense of Rotation, and Hemispheric Preference of Solar Eruptive Filaments

Zhenjun Zhou, Rui Liu, Xing Cheng +4

The orientation, chirality, and dynamics of solar eruptive filaments is a key to understanding the magnetic field of coronal mass ejections (CMEs) and therefore to predicting the g…