Coronal loops are the building blocks of the X-ray bright solar corona. They owe their
brightness to the dense confined plasma, and this review focuses on loops mostly as …

Observations and models of solar prominences are reviewed. We focus on non-eruptive
prominences, and describe recent progress in four areas of prominence research:(1) …

I have felt the need for a book on the theory of solar magnetic fields for some time now. Most
books about the Sun are written by observers or by theorists from other branches of solar …

ABSTRACT A three-dimensional magnetohydrodynamic (MHD) model for the propagation
and dissipation of Alfvén waves in a coronal loop is developed. The model includes the …

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally
attributed to the presence of a magnetic corona that contains plasma at temperatures …

The corona is a layer of hot plasma that surrounds the Sun, traces out its complex magnetic
field, and ultimately expands into interplanetary space as the supersonic solar wind …

We demonstrate that a three-dimensional magnetohydrodynamic (MHD) simulation of the
corona can model its global plasma density and temperature structure with sufficient …

Intended for graduate students and astronomers seeking an introduction to coronal physics,
this textbook strikes a balance between the observational and theoretical aspects of the …

We have used the ASCA and ROSAT X-ray satellites to probe the coronae of a sample of
nine solar-like G stars. These stars are all ostensibly single with ages ranging from 70 Myr to …

The solar transition region, which spans the temperature range from about 20,000 to
1,000,000 K, separates the chromosphere from the corona. All the energy that heats the …