The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

Characterized by cyclic axisymmetric perturbations to both the magnetic and fluid
parameters, magnetohydrodynamic fast sausage modes (FSMs) have proven useful for …

Global extreme-ultraviolet (EUV) waves are spectacular traveling disturbances in the solar
corona associated with energetic eruptions such as coronal mass ejections (CMEs) and …

We present observations of a blowout jet that experienced two distinct ejection stages. The
first stage started from the emergence of a small positive magnetic polarity, which was …

Quasi-periodic, fast-mode propagating (QFP) wave trains in the corona have been studied
intensively over the last decade, thanks to the full-disk, high spatio-temporal resolution, and …

Abstract We present Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA)
observation of three types of fast-mode, propagating, magnetosonic waves in a GOES C3. 0 …

Abstract Quasi-periodic pulsations (QPPs), which usually appear as temporal pulsations of
the total flux, are frequently detected in the light curves of solar/stellar flares. In this study, we …

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

Context. We present a new event of quasi-periodic wave trains observed in EUV wavebands
that rapidly propagate away from an active region after a flare. Aims. We measured the …

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 …