Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination
owing to their threadlike features and dynamic behaviors. Utilizing data from the New …

Prominences are intriguing, but poorly understood, magnetic structures of the solar corona.
The dynamics of solar prominences has been the subject of a large number of studies, and …

Quiescent solar prominences are highly dynamic structures which, among other features,
display oscillatory motions. The presence of these oscillations has been confirmed by …

High-resolution observations of solar filaments and prominences reveal that these large-
scale coronal structures are formed by a myriad of long and thin ribbons, here called …

We report an unusual set of observations of waves in a large prominence pillar that consist
of pulses propagating perpendicular to the prominence magnetic field. We observe a huge …

Solar prominences are subject to all kinds of perturbations during their lifetime, and
frequently demonstrate oscillations. The study of prominence oscillations provides an …

Seismology has become a powerful tool in studies of the magnetic structure of solar
prominences and filaments. Reversely, analytical and numerical models are guided by …

Quiescent solar prominences are cool and dense plasma clouds located inside the hot and
less dense solar corona. They are highly dynamic structures displaying flows, instabilities …

Context. High resolution observations have permitted the resolution of solar
prominences/filaments into sets of threads/fibrils. However, the values of the physical …

Context. Quiescent solar prominence fine structures are typically modelled as density
enhancements, called threads, which occupy a fraction of a longer magnetic flux tube. This …