As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …

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 …

We present a new version of the Alfvén wave solar model, a global model from the upper
chromosphere to the corona and the heliosphere. The coronal heating and solar wind …

We present a new method for performing differential emission measure (DEM) inversions on
narrow-band EUV images from the Atmospheric Imaging Assembly (AIA) on board the Solar …

Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events
are of particular interest, not only because of the scientific challenges they pose, but also …

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 …

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 …

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 …

We describe, analyze, and validate the recently developed Alfvén Wave Solar Model, a
three-dimensional global model starting from the top of the chromosphere and extending …