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 …

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 …

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 …

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 …

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 …

ABSTRACT On 2011 May 30, quasi-periodic fast-propagating (QFP) magnetosonic waves
accompanied by a C2. 8 flare were directly imaged by the Atmospheric Imaging Assembly …

We apply a new method to determine the magnetic field in coronal loops, using observations
of coronal loop oscillations. We analyze seven Doppler-shift oscillation events detected by …

There is increasingly strong observational evidence that slow magnetoacoustic modes arise
in the solar atmosphere, either as propagating or standing waves. Sunspots, coronal plumes …

We demonstrate that disturbances observed to propagate along the axis of the arcade in two-
ribbon solar flares at the speed of a few tens of km s− 1, well below the Alfvén and sound …

The goal of this review is to outline some new ideas in the physics of coronal magnetic
loops, the fundamental structural elements of the atmospheres of the Sun and flaring stars …