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 …

Magnetopause position is controlled mainly by the solar wind dynamic pressure and north‐
south interplanetary magnetic field component and these quantities are included in different …

In the analysis of in-situ space plasma and field data, an establishment of the coordinate
system and the frame of reference, helps us greatly simplify a given problem and provides …

High‐speed plasma jets downstream of Earth's bow shock are high velocity streams
associated with a variety of shock and magnetospheric phenomena. In this work, using the …

Abstract This White Paper outlines the importance of addressing the fundamental science
theme “How are charged particles energized in space plasmas” through a future ESA …

Magnetosheath jets are plasma entities that feature a significantly enhanced dynamic
pressure with respect to the ambient plasma. They occur more often downstream of the …

We investigate and evaluate the possibility of using local magnetosheath measurements to
classify the plasma according to upstream conditions. In order to do this, we use …

Magnetosheath jets represent localized enhancements in dynamic pressure observed within
the magnetosheath. These energetic entities, carrying excess energy and momentum, can …

Magnetosheath jets are localized plasma structures with high dynamic pressure which are
frequently observed downstream of the Earth's bow shock. In this work we analyze …