Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …

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

Taking advantage of both the high temporal and spatial resolutions of the Atmospheric
Imaging Assembly on board the Solar Dynamics Observatory, we studied a limb coronal …

Large-scale, globally propagating wave-like disturbances have been observed in the solar
chromosphere and by inference in the corona since the 1960s. However, detailed analysis …

A major, albeit serendipitous, discovery of the SOlar and Heliospheric Observatory mission
was the observation by the Extreme Ultraviolet Telescope (EIT) of large-scale extreme …

Global extreme-ultraviolet (EUV) waves are spectacular traveling disturbances in the solar
corona associated with energetic eruptions such as coronal mass ejections (CMEs) and …

We present the first unambiguous detection of quasi-periodic wave trains within the broad
pulse of a global EUV wave (so-called EIT wave) occurring on the limb. These wave trains …

This paper presents a study of a large sample of global disturbances in the solar corona with
characteristic propagating fronts as intensity enhancement, similar to the phenomena that …

We report on the first simultaneous observation of an Hα Moreton wave, the corresponding
EUV fast coronal waves, and a slow and bright EUV wave (typical EIT wave). We observed a …

For the first time, the kinematic evolution of a coronal wave over the entire solar surface is
studied. Full Sun maps can be made by combining images from the Solar Terrestrial …