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astro-ph.SR2024
A New Approach of Data-driven Simulation and Its Application to Solar Active Region 12673
Zhi-Peng Liu, Chao-Wei Jiang, Xin-Kai Bian +3
The solar coronal magnetic field is a pivotal element in the study of eruptive phenomena, and understanding its dynamic evolution has long been a focal point in solar physics. Nume…
astro-ph.SR2024
Why are non-radial solar eruptions less frequent than radial ones?
Qingjun Liu, Chaowei Jiang, Xuesheng Feng +2
Coronal mass ejections from the Sun are not always initiated along a radial trajectory; such non-radial eruptions are well known to be caused by the asymmetry of the pre-eruption m…
astro-ph.SR2024
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…