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

We present a combined observational and theoretical analysis to investigate the nature of
plasma turbulence at kinetic scales in the Earth's magnetosheath. In the first decade of the …

In this paper we use the full armament of the MMS (Magnetospheric Multiscale) spacecraft to
study magnetic reconnection in the turbulent magnetosheath downstream of a quasi …

Collisionless space plasma turbulence can generate reconnecting thin current sheets as
suggested by recent results of numerical magnetohydrodynamic simulations. The …

Heliospheric plasma turbulence plays a key role in transferring the energy of large‐scale
magnetic field and plasma flow fluctuations to smaller scales where the energy can be …

Turbulence properties are examined before, during, and after a coronal mass ejection
(CME) detected by the Wind spacecraft in 2012 July. The power-law scaling of the structure …

The magnetosheath (MSH) plasma turbulence depends on the structure and properties of
the bow shock (BS). Under quasi-parallel (Q||) and quasi-perpendicular (Q⊥) BS …

We use a global hybrid-Vlasov simulation for the magnetosphere, Vlasiator, to investigate
magnetosheath high-speed jets. Unlike many other hybrid-kinetic simulations, Vlasiator …

During the lifetime of the Cluster mission, the inter‐spacecraft distances in the solar wind
have changed from the large, fluid, scales (∼ 104 km), down to the scales of protons (∼ 102 …

Numerical simulations and experimental results have shown that the formation of current
sheets in space plasmas can be associated with enhanced vorticity. Also, in simulations the …