Wave and oscillatory activity of the solar corona is confidently observed with modern
imaging and spectral instruments in the visible light, EUV, X-ray and radio bands, and …

Quasi-periodic pulsations (QPP) are a common feature of flaring energy releases in the
solar atmosphere, observed in all bands, from radio to hard X-ray. In this review we …

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

Solar flare emission is detected in all EM bands and variations in flux density of solar
energetic particles. Often the EM radiation generated in solar and stellar flares shows a …

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 …

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 …

Observations revealed that various kinds of oscillations are excited in solar flare regions.
Quasi-periodic pulsations (QPPs) in flare emissions are commonly observed in a wide range …

Solar flares often display pulsating and oscillatory signatures in the emission, known as
quasi-periodic pulsations (QPP). QPP are typically identified during the impulsive phase of …

In this study, we investigate motions in the hot plasma above the flare loops during the 2017
September 10 X8. 2 flare event. We examine the region to the south of the main flare arcade …

A number of theoretical and observational considerations suggest that coronal loops are
bundles of unresolved, impulsively heated strands. This" nanoflare" model, as it is …