Data used to make figures presented in "Modeling Kelvin-Helmholtz Instability at the High-Latitude Boundary Layer in a Global Magnetosphere Simulation" by Michael et al. 2021 submitted to Geophysical Research Letters
International audienceWe present a 3D two-fluid simulation using plasma parameters as measured by MM...
The flow shear-driven Kelvin-Helmholtz (KH) instability is ubiquitous in planetary magnetospheres. A...
The Magnetospheric Multiscale (MMS) mission has presented a new opportunity to study the fine scale ...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
A magnetohydrodynamic simulation of Kelvin‐Helmholtz instability at the magnetospheric boundary is p...
The purpose of this thesis is to examine where the Kelvin-Helmholtz Instability exists in the Mesos...
© 2017 Author(s). The process feeding the development of a large boundary layer at the interface bet...
The Kelvin-Helmholtz (KH) instability has long been suggested as a mechanism for viscous interaction...
We study the Kelvin-Helmholtz (KH) instability at the dayside magnetopause, modeling the flow, the m...
The Kelvin–Helmholtz instability, proposed a long time ago for its role in and impact on the transpo...
International audienceKelvin-Helmholtz (KH) instability plays a fundamental role in the entry of sol...
The Kelvin-Helmholtz (KH) instability can operate in various situations in the solar wind, but at th...
A 3D two-fluid simulation, using plasma parameters as measured by MMS on 8 September 2015, shows the...
International audienceA 3D two-fluid simulation, using plasma parameters as measured by MMS on 8 Sep...
International audienceWe present a 3D two-fluid simulation using plasma parameters as measured by MM...
The flow shear-driven Kelvin-Helmholtz (KH) instability is ubiquitous in planetary magnetospheres. A...
The Magnetospheric Multiscale (MMS) mission has presented a new opportunity to study the fine scale ...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
A two-dimensional magnetohydrodynamic simulation of Kelvin-Helmholtz instability at the terrestrial ...
A magnetohydrodynamic simulation of Kelvin‐Helmholtz instability at the magnetospheric boundary is p...
The purpose of this thesis is to examine where the Kelvin-Helmholtz Instability exists in the Mesos...
© 2017 Author(s). The process feeding the development of a large boundary layer at the interface bet...
The Kelvin-Helmholtz (KH) instability has long been suggested as a mechanism for viscous interaction...
We study the Kelvin-Helmholtz (KH) instability at the dayside magnetopause, modeling the flow, the m...
The Kelvin–Helmholtz instability, proposed a long time ago for its role in and impact on the transpo...
International audienceKelvin-Helmholtz (KH) instability plays a fundamental role in the entry of sol...
The Kelvin-Helmholtz (KH) instability can operate in various situations in the solar wind, but at th...
A 3D two-fluid simulation, using plasma parameters as measured by MMS on 8 September 2015, shows the...
International audienceA 3D two-fluid simulation, using plasma parameters as measured by MMS on 8 Sep...
International audienceWe present a 3D two-fluid simulation using plasma parameters as measured by MM...
The flow shear-driven Kelvin-Helmholtz (KH) instability is ubiquitous in planetary magnetospheres. A...
The Magnetospheric Multiscale (MMS) mission has presented a new opportunity to study the fine scale ...