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 history and present state of large-scale magnetohydrodynamic modeling of the solar
corona and the solar wind with steady or quasi-steady coronal physics is reviewed. We put …

The Space Weather Modeling Framework (SWMF) provides a high‐performance flexible
framework for physics‐based space weather simulations, as well as for various space …

Aims. We study the evolution of stellar rotation and wind properties for low-mass main-
sequence stars. Our aim is to use rotational evolution models to constrain the mass loss …

Numerical three‐dimensional magnetohydrodynamic models are capable of predicting large‐
scale solar wind structures at Earth, provided that appropriate time‐dependent boundary …

The magnetic field of the Sun is the underlying cause of the many diverse phenomena
combined under the heading of solar activity. Here we describe the magnetic field as it …

We present a three‐dimensional (3‐D) numerical ideal magnetohydrodynamics (MHD)
model describing the time‐dependent expulsion of a coronal mass ejection (CME) from the …

We present a new global model of the solar corona, including the low corona, the transition
region, and the top of the chromosphere. The realistic three-dimensional magnetic field is …

The objective of this paper is to explore the application of a six-component overset grid to
solar wind simulation with a three-dimensional (3D) Solar-InterPlanetary Conservation …

This two-part book is devoted to classic fundamentals and current practices and
perspectives of modern plasma astrophysics. This second part discusses the physics of …