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 …

Observations and models of solar prominences are reviewed. We focus on non-eruptive
prominences, and describe recent progress in four areas of prominence research:(1) …

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 …

We present a case study for the global extreme-ultraviolet (EUV) wave and its
chromospheric counterpart the Moreton-Ramsey Wave associated with the second X-class …

We present direct upper limits on gravitational wave emission from the Crab pulsar using
data from the first 9 months of the fifth science run of the Laser Interferometer Gravitational …

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

With modern imaging and spectral instruments observing in the visible, EUV, X-ray, and
radio wavelengths, the detection of oscillations in the solar outer atmosphere has become a …

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

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 …