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 …

We present the final Sloan Digital Sky Survey IV (SDSS-IV) quasar catalog from Data
Release 16 of the extended Baryon Oscillation Spectroscopic Survey (eBOSS). This catalog …

In this paper, we present the imaging and spectroscopic observations of the simultaneous
horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an …

Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …

Using Fourier and wavelet analysis, we critically re-assess the significance of our detection
of periodic pulsations in coronal loops. We show that the proper identification of the …

The dynamics of a filament channel are observed with imaging and spectroscopic
telescopes before and during the filament eruption on 2011 January 29. The extreme …

We present the first stereoscopic and Doppler observations of simultaneous transverse
oscillations of a prominence and a filament and longitudinal oscillation of another filament …

Winking (oscillating) filaments have been observed for many years. However, observations
of successive winking filaments in one event have not yet been reported. In this paper, we …

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

Solar filaments often exhibit rotation and deflection during eruptions, which would
significantly affect the geoeffectiveness of the corresponding coronal mass ejections …