157 citations · 1.3k across the 36 of their papers we have counts for
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MHD Equilibria and Triggers for Prominence Eruption
Yuhong Fan
Magneto-hydrodynamic (MHD) simulations of the emergence of twisted magnetic flux tubes from the solar interior into the corona are discussed to illustrate how twisted and sheared c…
Differential Rotation in Solar Convective Dynamo Simulations
Yuhong Fan, Fang Fang
We carry out a magneto-hydrodynamic (MHD) simulation of convective dynamo in the rotating solar convective envelope driven by the solar radiative diffusive heat flux. The simulatio…
Numerical Study on Emergence of Kinked Flux Tube for Understanding of Possible Origin of Delta-spot Regions
Shinsuke Takasao, Yuhong Fan, Mark. C. M. Cheung +1
We carried out a magnetohydrodynamics simulation where a subsurface twisted kink-unstable flux tube emerges from the solar interior to the corona. Unlike the previous expectations…
-Sunspot Formation in Simulation of Active-Region-Scale Flux Emergence
Fang Fang, Yuhong Fan
-sunspots, with highly complex magnetic structures, are very productive in energetic eruptive events, such as X-class flares and homologous eruptions. We here study the formatio…
Effects of Radiative Diffusion on Thin Flux Tubes in Turbulent Solar-like Convection
Maria A. Weber, Yuhong Fan
We study the combined effects of convection and radiative diffusion on the evolution of thin magnetic flux tubes in the solar interior. Radiative diffusion is the primary supplier…