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

Dayside transients, such as hot flow anomalies, foreshock bubbles, magnetosheath jets, flux
transfer events, and surface waves, are frequently observed upstream from the bow shock …

We report on the in‐flight performance of the Solar Wind Ion Analyzer (SWIA) and
observations of the Mars‐solar wind interaction made during the Mars Atmosphere and …

Global hybrid (electron fluid, kinetic ions) and fully kinetic simulations of the magnetosphere
have been used to show surprising interconnection between shocks, turbulence, and …

Abstract The Moon and Mercury are airless bodies, thus they are directly exposed to the
ambient plasma (ions and electrons), to photons mostly from the Sun from infrared range all …

The magnetometer instrument MPO-MAG on-board the Mercury Planetary Orbiter (MPO) of
the BepiColombo mission en-route to Mercury is introduced, with its instrument design, its …

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 …

Using 2008–2011 data from the five Time History of Events and Macroscale Interactions
during Substorms (THEMIS) spacecraft in Earth's subsolar magnetosheath, we study high …

Both heliophysics and planetary physics seek to understand the complex nature of the solar
wind's interaction with solar system obstacles like Earth's magnetosphere, the ionospheres …

The ion foreshock is a source of energy for magnetospheric ULF waves, but it is usually only
considered effective at driving ULF waves with frequencies above the Pc5 (2–7 mHz) range …