29 citations · 47 across the 2 of their papers we have counts for
5 papers
Data-driven MHD Simulation of the Formation and Initiation of a Large-scale Pre-flare Magnetic Flux Rope in Solar Active Region 12371
Wen He, Chaowei Jiang, Peng Zou +4
Solar eruptions are the most powerful drivers of space weather. To understand their cause and nature, it is crucial to know how the coronal magnetic field evolves before eruption.…
Continuous Null-Point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar Active Region~12673
Peng Zou, Chaowei Jiang, Fengsi Wei +3
Two X-class solar flares occurred on 2017 September 6 from active region NOAA 12673: the first one is a confined X2.2 flare, and it is followed only hours later by the sec…
A Statistical Study of Solar Filament Eruptions That Forms High-Speed Coronal Mass Ejections
Peng Zou, Chaowei Jiang, Fengsi Wei +2
Coronal mass ejections (CMEs) play a decisive role in driving space weather, especially, the fast ones (e.g., with speeds above ~km~s). Understanding the trigger mechan…
A Two-Step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673
Peng Zou, Chaowei Jiang, Xueshang Feng +3
Solar flares are often associated with coronal eruptions, but there are confined ones without eruption, even for some X-class flares. How such large flares occurred and why they ar…
Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with an Homologous X-shaped Flare
Chaowei Jiang, Xiaoli Yan, Xueshang Feng +4
As a fundamental magnetic structure in the solar corona, electric current sheets (CSs) can form either prior to or during solar flare, and they are essential for magnetic energy di…