Aims. To understand the formation mechanism of large plumes in solar prominences, we
investigate the formation process of two such phenomena. Methods. We studied the …

Prominence plumes are evacuated upflows that emerge from bubbles below prominences,
whose formation mechanism is still unclear. Here we present a detailed study of plumes in a …

Observations by the Hinode satellite show in great detail the dynamics of rising plumes, dark
in chromospheric lines, in quiescent prominences that propagate from large (∼ 10 Mm) …

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 …

Prominence bubbles are cavities rising into quiescent prominences from below. The bubble-
prominence interface is often the active location for the formation of plumes, which flow …

We report on a dynamical event observed in a quiescent prominence on 2007 November 8:
a well-formed dark “bubble” with a bright core rose vertically through the prominence without …

Aims. The aim of this work is to analyse the multi-instrument observations of the June 22,
2010 prominence to study its structure in detail, including the prominence-corona transition …

Aims. Solar prominences contain a significant number of neutral species. The dynamics of
the ionised and neutral fluids composing the prominence plasma can be slightly different if …

Prominences in the solar corona are a hundredfold cooler and denser than their
surroundings, with a total mass of 10 13 up to 10 15 g. Here, we report on the first …

We review recent observational and theoretical results on the fine structure and dynamics of
solar prominences, beginning with an overview of prominence classifications, the proposal …