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) …

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 …

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 …

Spectral lines in the extreme ultraviolet (EUV) observed on the Sun can originate either from
the hot corona or the cooler chromosphere to corona transition region. In the present paper …

A quiescent prominence was observed by several instruments on 2007 April 25. The
temporal evolution was recorded in Hα by the Hinode SOT, in X-rays by the Hinode XRT …

Previous works have shown that dark and wide EUV filament channels observed at Å are
due to absorption of EUV lines in cool plasma condensations that are not observed in. We …

Context. Prominences are large magnetic structures in the corona filled by cool plasma with
fast evolving fine structure. Aims. We aim to better understand the plasma conditions in the …

From the Hα archive of the Big Bear Solar Observatory (BBSO) we have selected three
examples showing fibril structures that change their orientation, over 1 or 2 days, from nearly …

We present the main current issues concerning prominence studies. We recall the large
range of plasma parameters found in prominences which makes the work of the MHD …

We study a polar-crown prominence with a bubble and its plume observed in several
coronal filters by the SDO/AIA and in Hα by the MSDP spectrograph in Białków (Poland) to …