Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

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 comprehensive statistical analysis spanning over a solar cycle of the
properties and drivers of traveling fast forward and fast reverse interplanetary shocks. We …

This chapter focuses on the range of low frequency electromagnetic modes observed at and
upstream of collisionless shocks in the heliosphere. It discusses a specific class of whistler …

Transverse, near-circularly polarized, parallel-propagating electromagnetic waves around
the proton cyclotron frequency were found sporadically in the solar wind throughout the …

Large-scale disturbances generated by the Sun's dynamics first propagate through the
heliosphere, influence the heliosphere's outer boundaries, and then traverse and modify the …

We present a nonlinear Monte Carlo model of efficient diffusive shock acceleration where
the magnetic turbulence responsible for particle diffusion is calculated self-consistently from …

The paper reviews the interaction of collisionless interplanetary (IP) shocks with the
turbulent solar wind. The coexistence of shocks and turbulence plays an important role in …

A study of the structure of 145 low‐Mach number (M≤ 3), low‐beta (β≤ 1), quasi‐
perpendicular interplanetary collisionless shock waves observed by the Wind spacecraft has …

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