When the supersonic solar wind encounters the Earth's magnetosphere a shock, called bow
shock, is formed and the plasma is decelerated and thermalized in the magnetosheath …

Magnetosheath jets are localized regions of plasma that move faster towards the Earth than
the surrounding magnetosheath plasma. Due to their high velocities, they can cause …

We use Magnetosphere Multiscale (MMS) mission data to investigate a small number of
magnetosheath jets, which are localized and transient increases in dynamic pressure …

Abstract Using Magnetospheric Multiscale (MMS) data, we find, classify, and analyze
transient dynamic pressure enhancements in the magnetosheath (jets) from May 2015 to …

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

The terrestrial magnetosheath is embedded with coherent high‒speed jets of about 1RE in
scale, predominantly during quasi‒radial interplanetary magnetic field (IMF). When these …

When a magnetosheath jet (localized dynamic pressure enhancements) compresses
ambient magnetosheath at a (relative) speed faster than the local magnetosonic speed, a …

Magnetosheath jets are currently an important topic in the field of magnetosheath physics. It
is thought that 97% of the jets are produced by the shock rippling at quasi‐parallel shocks …

It has recently been proposed that ripples inherent to the bow shock during radial
interplanetary magnetic field (IMF) may produce local high speed flows in the …

Magnetosheath jets travel from the bow shock toward the magnetopause, and some of them
eventually impact it. Jet impacts have recently been linked to triggering magnetopause …