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 …

Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …

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 …

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 …

A magnetic field modifies the properties of waves in a complex way. Significant advances
have been made recently in our understanding of the physics of sunspot waves with the help …

We studied a blowout jet that occurred at the west limb of the Sun on 2014 August 29 using
high-resolution imaging/spectroscopic observations provided by the Solar Dynamics …

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

Three-minute oscillations over a sunspot's umbra in AR 11131 were observed
simultaneously in UV/EUV emission by the Solar Dynamics Observatory (SDO)/Atmospheric …

The joint effect of gravity and thermal misbalance on the dynamics of acoustic-gravity waves
(AGW) in the solar atmosphere is considered. It is shown that the heating and cooling taken …