This review covers the techniques, observations, and inferences of solar flare spectroscopy.
It is not a spectroscopist's view of solar flares but rather a solar flare physicist's view of …

Magnetic reconnection is a fundamental physical process in various astrophysical, space,
and laboratory environments. Many pieces of evidence for magnetic reconnection have …

Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …

In this Letter, we present a spectacular eruptive flare (X8. 2) associated with a coronal mass
ejection on 2017 September 10 at the west limb of the Sun. A flux rope eruption is followed …

Context. The origin of the slow solar wind is still an open issue. It has been suggested that
upflows at the edge of active regions are a possible source of the plasma outflow and …

Using 2D particle-in-cell plasma simulations, we study electron acceleration by temperature
anisotropy instabilities, assuming conditions typical of above-the-loop-top sources in solar …

In this article, we measure the mean magnetic shear from the morphological evolution of
flare ribbons, and examine the evolution of flare thermal and nonthermal X-ray emissions …

Magnetic reconnection, a ubiquitous process in space plasmas, is currently cutting-edge
research. This process is usually referred to as the topological reconstruction of the …

Polarisation measurements of solar flares at millimetre-waves were used to investigate the
magnetic field configuration of the emitting sources. We analyse two solar flares (SOL2013 …

Using 2D particle-in-cell plasma simulations, we study electron acceleration by temperature
anisotropy instabilities, assuming conditions typical of above-the-loop-top sources in solar …