J. Terradas

TL;DR: In this article, a temporal and spatial analysis of oscillations in a quiescent prominence has been performed using time series of two-dimensional Dopplergrams, and the direction of propagation, wavelength and phase speed, together with the damping time and wave period have been quantified and their spatial arrangement has been analyzed.

TL;DR: In this article, the authors established clear evidence for the resonant absorption damping mechanism by analyzing observational data from the novel Coronal Multi-Channel Polarimeter (CoMP), which has established that in the solar corona there are ubiquitous propagating low amplitude ($\approx$1 km s$^{-1}$) Alfv\'{e}nic waves with a wide range of frequencies.

TL;DR: In this paper, the authors studied the excitation and damping of transverse oscillations in a multi-stranded model of a straight line-tied coronal loop, and they found that the mechanism of mode conversion, due to the coupling between fast and Alfv\'en waves, is not compromised by the complicated geometry of the model.

TL;DR: In this article, the authors investigated the dynamics of condensations falling in the solar corona using a simple fully ionized plasma model and found that the presence of a heavy condensation gives rise to a dynamical rearrangement of the coronal pressure that results in the formation of a large pressure gradient that opposes gravity.

TL;DR: In this article, the authors discuss the difficulties found when trying to assess the statistical significance of the North-South asymmetry (hereafter SSNSA) of the most usually considered time series of solar activity.