157 citations · 1.7k across the 69 of their papers we have counts for
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Numerical Simulation of a Fundamental Mechanism of Solar Eruption with Different Magnetic Flux Distributions
Xinkai Bian, Chaowei Jiang, Xueshang Feng +3
Solar eruptions are explosive release of coronal magnetic field energy as manifested in solar flares and coronal mass ejection. Observations have shown that the core of eruption-pr…
Investigations of Sizes and Dynamical Motions of Solar Photospheric Granules by a Novel Granular Segmenting Algorithm
Liu Yanxiao, Jiang Chaowei, Yuan Ding +3
Granules observed in solar photosphere are believed to be convective and turbulent, but the physical picture of granular dynamical process remains unclear. Here we performed an inv…
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…
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…
Light Bridges Can Suppress the Formation of Coronal Loops
Yuhu Miao, Libo Fu, Xian Du +5
A light bridge is a magnetic intrusion into a sunspot, it interacts with the main magnetic field and excites a variety of dynamical processes. In the letter, we studied magnetic co…
MHD Modeling of Solar Coronal Magnetic Evolution Driven by Photospheric Flow
Chaowei Jiang, Xinkai Bian, Tingting Sun +1
It is well known that magnetic fields dominate the dynamics in the solar corona, and new generation of numerical modelling of the evolution of coronal magnetic fields, as featured…