The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …

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 …

We present a comprehensive model of the global properties of Alfvén waves in the solar
atmosphere and the fast solar wind. Linear non-WKB wave transport equations are solved …

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 …

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

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 …

We propose a new model for quasi-periodic modulation of solar and stellar flaring emission.
Fast magnetoacoustic oscillations of a non-flaring loop can interact with a nearby flaring …

Quasi-periodic pulsations (or QPPs) are periodic intensity variations in the flare emission
that occur across all wavelength bands. In this article, we review the observational and …

Quasi-periodic, fast-mode propagating (QFP) wave trains in the corona have been studied
intensively over the last decade, thanks to the full-disk, high spatio-temporal resolution, and …