One characteristic trait of space plasmas is the multi-scale dynamics resulting from non-
linear transfers and conversions of various forms of energy. Routinely evidenced in a range …

The solar wind is a magnetized plasma and as such exhibits collective plasma behavior
associated with its characteristic spatial and temporal scales. The characteristic length …

Magnetic reconnection in current sheets is a magnetic-to-particle energy conversion process
that is fundamental to many space and laboratory plasma systems. In the standard model of …

Magnetic reconnection converts, often explosively, stored magnetic energy to particle
energy in space and in the laboratory. Through processes operating on length scales that …

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 …

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 …

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

Data-driven science and technology offer transformative tools and methods to science. This
review article highlights the latest development and progress in the interdisciplinary field of …

An emerging paradigm for the dissipation of magnetic turbulence in the supersonic solar
wind is via localized small-scale reconnection processes, essentially between quasi-2D …

The magnetosheath flow may take the form of large amplitude, yet spatially localized,
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …