85 citations · 316 across the 13 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…
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…
Scaling of Turbulent Viscosity and Resistivity: Extracting a Scale-dependent Turbulent Magnetic Prandtl Number
Xin Bian, Jessica K. Shang, Eric G. Blackman +2
Turbulent viscosity and resistivity are perhaps the simplest models for turbulent transport of angular momentum and magnetic fields, respectively. The associated turbul…
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…