One of the major solar transients, coronal mass ejections (CMEs) and their related
interplanetary shocks have severe space weather effects and become the focus of study for …

We perform and analyze the results of a global magnetohydrodynamic simulation of the fast
coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using …

The dynamic process of coronal mass ejections (CMEs) in the heliosphere provides us the
key information for evaluating CMEs' geoeffectiveness and improving the accurate …

We report on the development of MPI-AMRVAC version 2.0, which is an open-source
framework for parallel, grid-adaptive simulations of hydrodynamic and …

We present a first-principles-based coronal mass ejection (CME) model suitable for both
scientific and operational purposes by combining a global magnetohydrodynamics (MHD) …

We extend our earlier Particle Acceleration and Transport in the Heliosphere (PATH) model
to study particle acceleration and transport at a coronal mass ejection (CME)‐driven shock …

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 here a time‐dependent three‐dimensional magnetohydrodynamic (MHD) solar
wind simulation from the solar surface to the Earth's orbit driven by time‐varying line‐of …

We carry out the adaptive mesh refinement (AMR) implementation of our solar–
interplanetary space-time conservation element and solution element (CESE) …

The coronal heating problem has been a major challenge in solar physics, and a
tremendous amount of effort has been made over the past several decades to solve it. In this …