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 …

Recent observations have revealed that magnetohydrodynamic (MHD) waves and
oscillations are ubiquitous in the solar atmosphere, with a wide range of periods. We give a …

Context. We investigate the decayless regime of coronal kink oscillations recently
discovered in the Solar Dynamics Observatory (SDO)/AIA data. In contrast to decaying kink …

The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …

The linear theory of MHD resonant waves in inhomogeneous plasmas is reviewed. The
review starts from discussing the properties of driven resonant MHD waves. The dissipative …

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

Since their discovery, spicules have attracted increased attention as energy/mass bridges
between the dense and dynamic photosphere and the tenuous hot solar corona. Mechanical …

Context. Solar flares are often accompanied by kink (transverse) oscillations of coronal
loops. Despite intensive study of these oscillations in recent years, the mechanisms that …

The detection of overtones of coronal loop kink oscillations has been an important advance
in the development of coronal seismology. It has significantly increased the potential of …

Context. Despite intensive studies of kink oscillations of coronal loops in the last decade, a
large-scale statistically significant investigation of the oscillation parameters has not been …