Yuhong Fan | High Altitude Observatory

Synthetic Lyman-α Emissions for the coronagraph aboard the ASO-S mission I: an Eruptive Prominence-cavity System

Lyman-alpha emission

Coronal Cavities in CoMP Observations

Cavity widths observed by SDO/AIA

Validation of the PDFI SS method for electric field inversions using magnetic flux emergence simulations

3D MHD simulation of the emergence of a twisted magnetic flux tube

Designing a New Coronal Magnetic Field Energy Diagnostic

Non-potentiality diagnostics of the energized flux-rope simulation at time step 89

Magnetic fields in the solar convection zone (major update)

3D view of the magnetic field lines in a simulation of the solar convective dynamo

Simulations of prominence eruption preceded with large amplitude longitudinal oscillations and draining

An MHD simulation of the evolution of a prominence-forming twisted coronal flux rope, for which large amplitude longitudinal (LAL) oscillations are excited during the quasi-static rise phase, followed by prominence draining towards the flux rope foot-points and the eventual eruption of the flux rope and the prominence

Probing the Solar Meridional Circulation using Fourier Legendre Decomposition

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