This paper outlines the current understanding of solar flares, mainly focused on
magnetohydrodynamic (MHD) processes responsible for producing a flare. Observations …

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 …

Abstract The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced
Technology demonstration satellite (SATech-01), which was launched to a Sun …

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

Prominences are intriguing, but poorly understood, magnetic structures of the solar corona.
The dynamics of solar prominences has been the subject of a large number of studies, and …

EIT waves and extreme-ultraviolet (EUV) dimmings attract particular attention as they
frequently accompany Coronal Mass Ejections (CMEs). We present several examples of EIT …

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 use combined high-cadence, high-resolution, and multi-point imaging by the Solar-
Terrestrial Relations Observatory (STEREO) and the Solar and Heliospheric Observatory to …

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 …

Early observations by the EUV Imaging Telescope (EIT) on the Solar and Heliospheric
Observatory indicated that propagating diffuse wave fronts, now conventionally referred to …