The corona of the Sun is a unique environment in which magnetohydrodynamic (MHD)
waves, one of the fundamental processes of plasma astrophysics, are open to a direct study …

Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

Decayless kink oscillations of solar coronal loops (or decayless oscillations for short) have
attracted great attention since their discovery. Coronal bright points (CBPs) are mini-active …

Using data obtained by the EUV Imaging Spectrometer on board Hinode, we have
performed a survey of obvious and persistent (without significant damping) Doppler shift …

Outwardly propagating intensity disturbances are a common feature in large, quiescent
coronal loop structures. In this paper, an overview is given of the observed properties and …

Context. Rapidly decaying slow magnetoacoustic waves are regularly observed in the solar
coronal structures, offering a promising tool for a seismological diagnostics of the coronal …

Recent observations have revealed two types of decayless transverse oscillations in short
coronal loops: one with short periods scaling with loop lengths, and the other with longer …

The presence and interplay of continuous cooling and heating processes maintaining the
corona of the Sun at the observed one million K temperature were recently understood to …

Strongly damped Doppler shift oscillations are observed frequently associated with flarelike
events in hot coronal loops. In this paper, a review of the observed properties and the …