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 …

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 …

The severe geomagnetic effects of solar storms or coronal mass ejections (CMEs) are to a
large degree determined by their propagation direction with respect to Earth. There is a lack …

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 …

In this paper, we present the imaging and spectroscopic observations of the simultaneous
horizontal and vertical large-amplitude oscillation of a quiescent filament triggered by an …

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