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

The dual spacecraft mission BepiColombo is the first joint mission between the European
Space Agency (ESA) and the Japanese Aerospace Exploration Agency (JAXA) to explore …

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

Due to its ubiquitous presence, turbulence is often invoked to explain the origin of
nonthermal particles in astrophysical sources of high-energy emission. With particle-in-cell …

The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of
current microphysical CR transport models in magnetohydrodynamic (MHD) turbulence are …

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 …

We present a new theoretical picture of magnetically dominated, decaying turbulence in the
absence of a mean magnetic field. With direct numerical simulations, we demonstrate that …

Using 2.5 dimensional kinetic particle-in-cell simulations, we simulate reconnection
conditions appropriate for the magnetosheath and solar wind, ie, plasma beta (ratio of gas …

We investigate the spectral properties of the electromagnetic fluctuations of sub-ion scale
turbulence in weakly collisional, low-beta plasmas using a two-field isothermal gyrofluid …

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