Magnetic turbulence is found in most space plasmas, including the Earth's magnetosphere,
and the interaction region between the magnetosphere and the solar wind. Recent …

We study the linear and nonlinear evolution of the tearing instability on thin current sheets by
means of two-dimensional numerical simulations, within the framework of compressible …

We review the current literature on the formation of coherent structures (CoSs) in strongly
turbulent 3D magnetized plasmas. CoSs [Current Sheets (CS), magnetic filaments, large …

Electron and proton acceleration in three-dimensional electric and magnetic fields is studied
through test particle simulations. The fields are obtained by a three-dimensional …

Magnetic reconnection, a fundamentally important process in astrophysics, is believed to be
initiated by the tearing instability of an electric current sheet, a region where magnetic field …

It has been recently shown numerically that there exists an inverse transfer of magnetic
energy in decaying, non-helical, magnetically dominated, magnetohydrodynamic turbulence …

Astrophysical fluids have very large Reynolds numbers and therefore turbulence is their
natural state. Magnetic reconnection is an important process in many astrophysical plasmas …

The present work is devoted to introduce the backward Euler based modular time filter
method for MHD flow. The proposed method improves the accuracy of the solution without a …

The nonlinear behavior of reconnecting modes in three spatial dimensions (3D) is
investigated, on the basis of a collisionless fluid model in slab geometry, assuming a strong …

Three-dimensional numerical simulations of the tearing instability in the framework of
compressible and resistive magnetohydrodynamics are presented. Simulations have been …