Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …

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

The plasma sheet is populated in part by the solar wind plasma. Four solar entry
mechanisms are examined:(1) double cusp or double lobe reconnection,(2) Kelvin …

We investigate localized magnetosheath and solar wind density enhancements, associated
with clear magnetic field changes, and therefore referred to as magnetosheath/solar wind …

Abstract Time History of Events and Macroscale Interactions during Substorms multipoint
observation of the plasma and magnetic fields, conducted simultaneously in the dayside …

We use Cluster multipoint density measurements, using the spacecraft potential, to identify
localized density enhancements (> 50%) in the magnetosheath, and estimate their three …

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

This paper presents in situ observational evidence from the Cluster Ion Spectrometer (CIS)
on Cluster of injected solar wind" plasma clouds" protruding into the day-side high-latitude …

Turbulent fluctuations are omnipresent in the terrestrial magnetosphere as well as in other
planetary plasma systems. While the topic is broad and was largely treated in the past (see …

The penetration of plasma clouds, or plasmoids, across abrupt magnetic barriers (of the
scale less than a few ion gyro radii, using the plasmoid directed velocity) is studied. The …