Star formation is a complex multi-scale phenomenon that is of significant importance for
astrophysics in general. Stars and star formation are key pillars in observational astronomy …

The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their
interaction is governed by complex physical processes and creates heliospheric regions …

We present results from three-dimensional hybrid-kinetic simulations of Alfvénic turbulence
in a high-β, collisionless plasma. The key feature of such turbulence is the interplay between …

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 …

Pressure anisotropy can strongly influence the dynamics of weakly collisional, high-beta
plasmas, but its effects are missed by standard magnetohydrodynamics (MHD). Small …

The modeling of multi-scale and multi-physics complex systems typically involves the use of
scientific software that can optimally leverage extreme scale computing. Despite major …

We study properties of magnetohydrodynamic (MHD) eigenmodes by decomposing the data
of MHD simulations into linear MHD modes—namely, the Alfvén, slow magnetosonic, and …

Magnetic fields grow quickly, even at early cosmological times, suggesting the action of a
small-scale dynamo (SSD) in the interstellar medium (ISM) of galaxies. Many studies have …

To comprehensively understand the saturation of two-dimensional (2D) magnetized Kelvin–
Helmholtz-instability-driven turbulence, energy transfer analysis is extended from the …

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 …