Add to ORKGRecent studies (Moore et al, 2016, Nature Physics, Moore et al., JGR 2017) have shown that during Kelvin-Helmholtz Instability ion-scale plasma waves are more abundant and are associated with ion heating. In the present paper the Kelvin-Helmholtz (KH) Waves within the flank magnetopause are identified in the Magnetosphere Multi Scale (MMS) data and are sorted with respect to the OMNI solar wind conditions. Large scale KH wave properties and current layer structures are compared with 3-D MHD simulations. A search for high frequency (between ion and electron scales) plasma waves in KH vortices is performed, waves are analyzed and the properties are compared with the ambient plasma characteristic
In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked ...
In this study, we present the first observations from the Magnetospheric Multiscale (MMS) mission of...
The Kelvin-Helmholtz (K-H) waves predominantly excited at the Earth's low-latitude magnetopause were...
Recent studies (Moore et al, 2016, Nature Physics, Moore et al., JGR 2017) have shown that during Ke...
The Kelvin-Helmholtz Instability (KHI), which occurs regularly at Earth’s magnetopause, is known to ...
The Magnetospheric Multiscale (MMS) mission has presented a new opportunity to study the fine scale ...
The Kelvin-Helmholtz Instability (KHI) is common at the magnetopause boundary enclosing Earth’s magn...
The Kelvin-Helmholtz (KH) instability can operate in various situations in the solar wind, but at th...
Understanding the physical mechanisms responsible for the cross-scale energy transport and plasma he...
The Kelvin-Helmholtz instability (KHI) is thought to be an important driver for mass, momentum, and ...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked ...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked ...
In this study, we present the first observations from the Magnetospheric Multiscale (MMS) mission of...
The Kelvin-Helmholtz (K-H) waves predominantly excited at the Earth's low-latitude magnetopause were...
Recent studies (Moore et al, 2016, Nature Physics, Moore et al., JGR 2017) have shown that during Ke...
The Kelvin-Helmholtz Instability (KHI), which occurs regularly at Earth’s magnetopause, is known to ...
The Magnetospheric Multiscale (MMS) mission has presented a new opportunity to study the fine scale ...
The Kelvin-Helmholtz Instability (KHI) is common at the magnetopause boundary enclosing Earth’s magn...
The Kelvin-Helmholtz (KH) instability can operate in various situations in the solar wind, but at th...
Understanding the physical mechanisms responsible for the cross-scale energy transport and plasma he...
The Kelvin-Helmholtz instability (KHI) is thought to be an important driver for mass, momentum, and ...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked ...
In the Earth\u27s magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shock...
In the Earth's magnetosphere, the magnetotail plasma sheet ions are much hotter than in the shocked ...
In this study, we present the first observations from the Magnetospheric Multiscale (MMS) mission of...
The Kelvin-Helmholtz (K-H) waves predominantly excited at the Earth's low-latitude magnetopause were...