Coronal mass ejections (CMEs) are the largest-scale eruptive phenomenon in the solar
system, expanding from active region-sized nonpotential magnetic structure to a much larger …

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

The basic idea of the paper is to present transparently and confront two different views on
the origin of large-scale coronal shock waves, one favoring coronal mass ejections (CMEs) …

This article broadly reviews our knowledge of solar flares. There is a particular focus on their
global properties, as opposed to the microphysics such as that needed for magnetic …

We investigate the properties of two" classical" EUV Imaging Telescope (EIT) coronal waves.
The two source regions of the associated coronal mass ejections (CMEs) possess opposite …

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 …

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 …