Solar prominences are one of the most common features of the solar atmosphere. They are
found in the corona but they are one hundred times cooler and denser than the coronal …

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) …

This review paper outlines background information and covers recent advances made via
the analysis of spectra and images of prominence plasma and the increased sophistication …

The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The
review starts from discussing the properties of driven resonant MHD waves. The dissipative …

Solar prominences are long-lived cool and dense plasma curtains in the hot and rarefied
outer solar atmosphere or corona. The physical mechanism responsible for their formation …

We present observations and magnetic field modeling of the large polar crown prominence
that erupted on 2010 December 6. Combination of Solar Dynamics Observatory …

Context. Prominences show a surprising amount of fine structure and it is widely believed
that their threads, as seen in Hα observations, provide indirect information concerning …

Context. The dynamics of prominence fine structures present a challenge to our
understanding of the formation of cool plasma prominence embedded in the hot corona …

Context. Determining the magnetic field vector in quiescent solar prominences is possible by
interpreting the Hanle and Zeeman effects in spectral lines. However, observational …

We analyze solar quiescent prominence bubble characteristics and instability dynamics
using Hinode/Solar Optical Telescope data. We measure the bubble expansion rate …