Astrophysical plasmas have the remarkable ability to preserve magnetic topology, which
inevitably gives rise to the accumulation of magnetic energy within stressed regions …

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 …

Magnetized turbulence and magnetic reconnection are often invoked to explain the
nonthermal emission observed from a wide variety of astrophysical sources. By means of …

The rate of magnetic reconnection is of the utmost importance in a variety of processes
because it controls, for example, the rate energy is released in solar flares, the speed of the …

This review of scaling theories of magnetohydrodynamic (MHD) turbulence aims to put the
developments of the last few years in the context of the canonical time line (from Kolmogorov …

While observations have suggested that power-law electron energy spectra are a common
outcome of strong energy release during magnetic reconnection, eg, in solar flares, kinetic …

Magnetic reconnection is thought to be one of the main energy-dissipation mechanisms
fueling energy to the plasma in the vicinity of a black hole. Indeed, plasmoids formed …

Magnetic reconnection is a primary driver of particle acceleration processes in space and
astrophysical plasmas. Understanding how particles are accelerated and the resulting …

Magnetic reconnection, a plasma process converting magnetic energy to particle kinetic
energy, is often invoked to explain magnetic energy releases powering high-energy flares in …

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma
phenomenon that plays a key role in energy transport and conversion in space and …