▪ Abstract Turbulence affects the structure and motions of nearly all temperature and density
regimes in the interstellar gas. This two-part review summarizes the observations, theory …

The magnetosheath lies between the bow shock and the magnetopause and is formed
mainly from decelerated and deflected solar wind, with a small contribution of plasma from …

Magnetic field fluctuations in the frequency range [0.02–12.5] Hz are studied with the four
Cluster satellites in the Earth magnetosheath downstream of a quasi‐perpendicular bow …

Scale interactions in Hall magnetohydrodynamics (MHDs) are studied using both the mean
field theory derivation of transport coefficients, and direct numerical simulations in three …

We report on the development of a computational framework for the parallel, mesh-adaptive
solution of systems of hyperbolic conservation laws like the time-dependent Euler equations …

The Cluster satellites crossed the Earth's bow shock several times on 31 March 2001. For all
these crossings the bow shock was supercritical and quasi‐perpendicular. We present here …

Context. Solar Orbiter is expected to have flown close to the tail of comet C/2019 Y4 (ATLAS)
during the spacecraft's first perihelion in June 2020. Models predict a possible crossing of …

The nonlinear dynamics of ideal, incompressible Hall magnetohydrodynamics (HMHD) is
investigated through classical Gibbs ensemble methods applied to the finite Galerkin …

Waves in the foreshock region are studied on the basis of a hypothesis that the linear
process first excites the waves and further wave-wave nonlinearities distribute scatter the …

The proton velocity distribution functions (VDFs) observed in the solar wind often show
beam components. In this study, by means of one‐dimensional hybrid simulation, parametric …