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20162023
most citedContinuous Null-Point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar Active Region~12673

29 citations · 152 across the 14 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2023★ 2 cited

Magnetic Reconnection as the Key Mechanism in Sunspot Rotation Leading to Solar Eruption

Chaowei Jiang, Xueshang Feng, Xinkai Bian +8

The rotation of sunspots around their umbral center has long been considered as an important process in leading to solar eruptions, but the underlying mechanism remains unclear. A…

astro-ph.SR2023

A model of failed solar eruption initiated and destructed by magnetic reconnection

Chaowei Jiang, Aiying Duan, Peng Zou +5

Solar eruptions are explosive disruption of coronal magnetic fields, and often launch coronal mass ejections into the interplanetary space. Intriguingly, many solar eruptions fail…

astro-ph.SR2021

Formation of Magnetic Flux Rope during Solar Eruption. I. Evolution of Toroidal Flux and Reconnection Flux

Chaowei Jiang, Jun Chen, Aiying Duan +5

Magnetic flux ropes (MFRs) constitute the core structure of coronal mass ejections (CMEs), but hot debates remain on whether the MFR forms before or during solar eruptions. Further…

astro-ph.SR2021★ 8 cited

The Causes of Peripheral Coronal Loop Contraction and Disappearance Revealed in a Magnetohydrodynamic Simulation of Solar Eruption

Juntao Wang, Chaowei Jiang, Ding Yuan +1

The phenomenon of peripheral coronal loop contraction during solar flares and eruptions, recently discovered in observations, gradually intrigues solar physicists. However, its und…

astro-ph.SR2020

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.…

astro-ph.SR2020★ 29 cited

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…