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 …

The fast solar wind that fills the heliosphere originates from deep within regions of open
magnetic field on the Sun called 'coronal holes'. The energy source responsible for …

Magnetic reconnection, topological changes in magnetic fields, is a fundamental process in
magnetized plasmas. It is associated with energy release in regions of magnetic field …

Magnetohydrodynamic turbulence regulates the transfer of energy from large to small scales
in many astrophysical systems, including the solar atmosphere. We perform three …

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

Magnetic reconnection is a universal process that powers explosive energy-release events
such as solar flares, geomagnetic substorms and some astrophysical jets. A characteristic …

Phenomenological models of cosmic ray (CR) transport in the Milky Way can reproduce a
wide range of observations assuming that CRs scatter off of magnetic-field fluctuations with …

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 …

In strongly magnetized astrophysical plasma systems, magnetic reconnection is believed to
be the primary process during which explosive energy release and particle acceleration …