Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …

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High-resolution images of the solar surface show a granulation pattern of hot rising and
cooler downward-sinking material–the top of the deep-reaching solar convection zone …

We present a comprehensive model of the global properties of Alfvén waves in the solar
atmosphere and the fast solar wind. Linear non-WKB wave transport equations are solved …

Determining the heating mechanism (or mechanisms) that causes the outer atmosphere of
the Sun, and many other stars, to reach temperatures orders of magnitude higher than their …

We investigate the ionization of hydrogen in a dynamic solar atmosphere. The simulations
include a detailed non-LTE treatment of hydrogen, calcium, and helium but lack other …

Magnetism is one of the most pervasive features of the Universe, with planets, stars and
entire galaxies all having associated magnetic fields. All of these fields are generated by the …

Numerical simulations of wave propagation in a two-dimensional stratified magneto-
atmosphere are presented for conditions that are representative of the solar photosphere …

Over the last two decades the uninterrupted, high resolution observations of the Sun, from
the excellent range of telescopes aboard many spacecraft complemented with observations …

Outwardly propagating intensity disturbances are a common feature in large, quiescent
coronal loop structures. In this paper, an overview is given of the observed properties and …