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 …

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 …

Context. A complex and long-lasting solar eruption on 17 April 2021 produced a widespread
solar energetic particle (SEP) event that was observed by five longitudinally well-separated …

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 …

We present first observations of a dome-shaped large-scale extreme-ultraviolet coronal
wave, recorded by the Extreme Ultraviolet Imager instrument on board STEREO-B on 2010 …

The nature of coronal mass ejection (CME)-associated low corona propagating
disturbances," extreme ultraviolet (EUV) waves," has been controversial since their …

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

In Fall 2008 NASA selected a large international consortium to produce a comprehensive
automated feature-recognition system for the Solar Dynamics Observatory (SDO). The SDO …

We report on the detection of EUV wave reflection from a coronal hole, as observed by the
Solar Terrestrial Relations Observatory mission. The EUV wave was associated with a …

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 …