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

We present an overview of solar flares and associated phenomena, drawing upon a wide
range of observational data primarily from the RHESSI era. Following an introductory …

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally
attributed to the presence of a magnetic corona that contains plasma at temperatures …

This paper, a review of the present status of existing models for particle acceleration during
impulsive solar flares, was inspired by a week‐long workshop held in the Fall of 1993 at …

We report on radiative hydrodynamic simulations of moderate and strong solar flares. The
flares were simulated by calculating the atmospheric response to a beam of nonthermal …

The Neupert effect is the name given to the correlation observed in many flares between the
time-integrated microwave and hard X-ray emissions and the soft X-ray emission light curve …

The first flare on the Sun was observed exactly 150 years ago. During most of the long
history, only secondary effects have been noticed, so flares remained a riddle. Now the …

Two-dimensional magnetohydrodynamic (MHD) simulation of a solar flare including the
effect of anisotropic heat conduction and chromospheric evaporation based on the magnetic …

We present new results from the Interface Region Imaging Spectrograph (IRIS) showing the
dynamic evolution of chromospheric evaporation and condensation in a flare ribbon, with …

The temperature T e (s) and density structure ne (s) of active region loops in EUV observed
with TRACE is modeled with a multithread model, synthesized from the summed emission of …