How has the solar wind evolved to reach what it is today? In this review, I discuss the long-
term evolution of the solar wind, including the evolution of observed properties that are …

The Sun's outer atmosphere is heated to temperatures of millions of degrees, and solar
plasma flows out into interplanetary space at supersonic speeds. This paper reviews our …

Coronal holes are areas on the Sun with open magnetic field lines. They are a source region
of the solar wind, but how the wind emerges from coronal holes is not known. We observed …

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 …

As the interface between the Sun's photosphere and corona, the chromosphere and
transition region play a key role in the formation and acceleration of the solar wind …

One of the most important early results from the Parker Solar Probe (PSP) is the ubiquitous
presence of magnetic switchbacks, whose origin is under debate. Using a three-dimensional …

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

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 …

Alfvén wave turbulence models lie at the heart of many investigations into the winds and
extreme-ultraviolet and X-ray emission from cool, solar-like stars. The models provide …

Context. Current models of the solar wind must approximate (or ignore) the small-scale
dynamics within the solar atmosphere; however, these are likely important in shaping the …