This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

The topology and dynamics of the three-dimensional magnetic field in the solar atmosphere
govern various solar eruptive phenomena and activities, such as flares, coronal mass …

We develop a general description of how information propagates through a
magnetohydrodynamic (MHD) system based on the method of characteristics and use that to …

Current magnetohydrodynamic (MHD) simulations of the initiation of solar eruptions are still
commonly carried out with idealized magnetic field models, whereas the realistic coronal …

This work is devoted to the construction of a data-driven model for the study of the dynamic
evolution of the global corona that can respond continuously to the changing of the …

We present a comprehensive study of the formation and eruption of an active region (AR)
sigmoid in AR 11283. To follow the quasi-static evolution of the coronal magnetic field, we …

Due to the absence of direct measurement, the magnetic field in the solar corona is usually
extrapolated from the photosphere in a numerical way. At the moment, the nonlinear force …

We report our implementation of the magneto-frictional method in the Message Passing
Interface Adaptive Mesh Refinement Versatile Advection Code (MPI-AMRVAC). The method …

The magnetic field in the solar corona is usually extrapolated from a photospheric vector
magnetogram using a nonlinear force-free field (NLFFF) model. NLFFF extrapolation needs …

In order to bridge the gap between heliospheric and solar observations of coronal mass
ejections (CMEs), one of the key steps is to improve the understanding of their …