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 …

The solar corona is two to three orders of magnitude hotter than the underlying photosphere,
and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over …

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 …

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

Slow magnetoacoustic waves observed in the solar corona are used as seismological
probes of plasma parameters. It has been shown that the dispersion properties of such …

There is intense interest in determining the precise contribution of Alfvénic waves
propagating along solar structures to the problems of coronal heating and solar wind …

We review novel data analysis techniques developed or adapted for the field of coronal
seismology. We focus on methods from the last ten years that were developed for extreme …

Context. Large-scale fast waves with perturbation of the EUV emission intensity are well
resolved in both temporal and spatial scale by SDO/AIA. These waves are prone to …

The processes of coronal plasma heating and cooling were previously shown to significantly
affect the dynamics of slow magnetoacoustic (MA) waves, causing amplification or …