9 citations · 11 across the 6 of their papers we have counts for
6 papers
A Model of Solar Magnetic Flux Rope Eruption Initiated Primarily by Magnetic Reconnection
Qingjun Liu, Chaowei Jiang, Xinkai Bian +3
There is a heated debate regarding the specific roles played by ideal magnetohydrodynamic (MHD) instability and magnetic reconnection in the causes of solar eruptions. In the conte…
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…
Data-driven MHD simulation of a sunspot rotating active region leading to solar eruption
Chaowei Jiang, Xueshang Feng, Xinkai Bian +8
Solar eruptions are the leading driver of space weather, and it is vital for space weather forecast to understand in what conditions the solar eruptions can be produced and how the…
A fundamental mechanism of solar eruption initiation in multipolar magnetic field
Xinkai Bian, Chaowei Jiang, Xueshang Feng +2
Recently we established a fundamental mechanism of solar eruption initiation, in which an eruption can be initiated from a bipolar field through magnetic reconnection in the curren…
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…
MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation
Xinyi Wang, Chaowei Jiang, Xueshang Feng +2
The relationship between solar eruption and sunspot rotation has been widely reported, and the underlying mechanism requires to be studied. Here we performed a full 3D MHD simulati…