Magnetic reconnection is a fundamental process whereby microscopic plasma processes
cause macroscopic changes in magnetic field topology, leading to explosive energy release …

High time-resolution solar wind magnetic field data are employed to study statistics
describing intermittency near the first perihelion (∼ 35.6 R⊙) of the Parker Solar Probe …

Based on the unprecedented high‐resolution data from the Magnetospheric Multiscale
mission, we investigate the energy dissipation in turbulent reconnection outflow during …

Magnetic reconnection is believed to be the main driver to transport solar wind into the
Earth's magnetosphere when the magnetopause features a large magnetic shear. However …

Collisionless dissipation in turbulent plasmas such as the solar wind and the solar corona
has been an intensively studied subject recently, with new insights often emerging from …

The energy of turbulence in the universe, which cascades from large fluid scales to small
kinetic scales, is believed to be dissipated through conversion to thermal or nonthermal …

In the context of space and astrophysical plasma turbulence and particle heating, several
vocabularies emerge for estimating turbulent energy dissipation rate, including Kolmogorov …

In the last decades, a few spacecraft missions have been launched to investigate the
process of magnetic reconnection in space, during which magnetic free energy is …

Plasma turbulence at scales of the order of the ion inertial length is mediated by several
mechanisms, including linear wave damping, magnetic reconnection, the formation and …

The properties of the turbulence that develops in the outflows of magnetic reconnection have
been investigated using self-consistent plasma simulations, in three dimensions. As …