Large-scale, globally propagating wave-like disturbances have been observed in the solar
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …

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 a case study for the global extreme-ultraviolet (EUV) wave and its
chromospheric counterpart the Moreton-Ramsey Wave associated with the second X-class …

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 …

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 …

The solar atmosphere is full of complicated transients manifesting the reconfiguration of the
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …

This paper presents a study of a large sample of global disturbances in the solar corona with
characteristic propagating fronts as intensity enhancement, similar to the phenomena that …

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 …

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. A flare-driven quasi-periodic extreme ultraviolet wave train totally reflected at a
coronal hole boundary was well imaged on both temporal and spatial scales by AIA/SDO …