Magnetic waves are a relevant component in the dynamics of the solar atmosphere. Their
significance has increased because of their potential as a remote diagnostic tool and their …

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

Alfvén waves, transverse incompressible magnetic oscillations, have been proposed as a
possible mechanism to heat the Sun's corona to millions of degrees by transporting …

We employ a sequence of Doppler images obtained with the Coronal Multi-channel
Polarimeter (CoMP) instrument to perform time–distance seismology of the solar corona. We …

Outwardly propagating intensity disturbances are a common feature in large, quiescent
coronal loop structures. In this paper, an overview is given of the observed properties and …

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 …

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 use images of high spatial, spectral, and temporal resolution, obtained using both
ground-and space-based instrumentation, to investigate the coupling between wave …

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 present the first Hinode/EUV Imaging Spectrometer observations of 5 minute quasi-
periodic oscillations detected in a transition-region line (He ii) and five coronal lines (Fe x …