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Jets downstream of collisionless shocks
The magnetosheath flow may take the form of large amplitude, yet spatially localized,
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …
transient increases in dynamic pressure, known as “magnetosheath jets” or “plasmoids” …
Review of solar wind entry into and transport within the plasma sheet
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 …
mechanisms are examined:(1) double cusp or double lobe reconnection,(2) Kelvin …
The link between shocks, turbulence, and magnetic reconnection in collisionless plasmas
Global hybrid (electron fluid, kinetic ions) and fully kinetic simulations of the magnetosphere
have been used to show surprising interconnection between shocks, turbulence, and …
have been used to show surprising interconnection between shocks, turbulence, and …
Anti-sunward high-speed jets in the subsolar magnetosheath
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 …
during Substorms (THEMIS) spacecraft in Earth's subsolar magnetosheath, we study high …
In situ observations of a magnetosheath high‐speed jet triggering magnetopause reconnection
Magnetosheath high‐speed jets—localized dynamic pressure enhancements typically of∼
1 Earth radius in size—impact the dayside magnetopause several times per hour. Here we …
1 Earth radius in size—impact the dayside magnetopause several times per hour. Here we …
Supermagnetosonic subsolar magnetosheath jets and their effects: From the solar wind to the ionospheric convection
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 …
interplanetary magnetic field (IMF) may produce local high speed flows in the …
Magnetosheath dynamic pressure enhancements: Occurrence and typical properties
The first comprehensive statistical study of large-amplitude (> 100%) transient
enhancements of the magnetosheath dynamic pressure reveals events of up to~ 15 times …
enhancements of the magnetosheath dynamic pressure reveals events of up to~ 15 times …
Solar wind control of magnetosheath jet formation and propagation to the magnetopause
Magnetosheath jets are localized high‐dynamic pressure pulses originating at Earth's bow
shock and propagating earthward through the magnetosheath. Jets can influence …
shock and propagating earthward through the magnetosheath. Jets can influence …
Magnetosheath pressure pulses: Generation downstream of the bow shock from solar wind discontinuities
We present multipoint Time History of Events and Macroscale Interactions during Substorms
(THEMIS) observations of transient dynamic pressure pulses in the magnetosheath 3–10 …
(THEMIS) observations of transient dynamic pressure pulses in the magnetosheath 3–10 …
Observational properties of dayside throat aurora and implications on the possible generation mechanisms
Observational properties of throat aurora are investigated in detail by using 7 year
continuous auroral observations obtained at Yellow River Station (magnetic latitude 76.24° …
continuous auroral observations obtained at Yellow River Station (magnetic latitude 76.24° …