In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …

The first self-consistent simulations of electron acceleration during magnetic reconnection in
a macroscale system are presented. Consistent with solar flare observations, the spectra of …

The past decade has seen a dramatic increase in practical applications of microwave
gyrosynchrotron emission for plasma diagnostics and three-dimensional modeling of solar …

Energetic particle populations in the solar corona and in the heliosphere appear to have
different characteristics even when produced in the same solar flare. It is not clear what …

A new computational model, kglobal, is being developed to explore energetic electron
production via magnetic reconnection in macroscale systems. The model is based on the …

The aim of this study is to generate maps of the hard X-ray emission produced by energetic
electrons in a solar flare and compare them with observations. The ultimate goal is to test the …

Abstract We performed 3D Particle-In-Cell simulations to study electron acceleration in the
electron dissipation region of asymmetrical electron magnetic reconnection driven by ultra …

Quantitatively analyzing the role of turbulence in the magnetic fluctuation-induced self-
generating-organization region and the plasma turbulence-induced self-feeding-sustaining …

Twisted magnetic flux ropes are reservoirs of free magnetic energy. In a highly conducting
plasma such as the solar corona, energy release through multiple magnetic reconnections …

We show how some different fundamental plasma processes-the ideal kink instability,
magnetic reconnection and magnetohydrodynamic oscillations-can be causally linked. This …