27 citations · 49 across the 6 of their papers we have counts for
6 papers
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…
MHD simulation of Solar Eruption from Active Region 11429 Driven by Photospheric Velocity Field
Xinyi Wang, Chaowei Jiang, Xueshang Feng
Data-driven simulation is becoming an important approach for realistically characterizing the configuration and evolution of solar active regions, revealing the onset mechanism of…
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…
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…
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…