Magnetohydrodynamic oscillations in the solar corona and Earth's magnetosphere: towards consolidated understanding
VM Nakariakov, V Pilipenko, B Heilig, P Jelínek… - Space Science …, 2016 - Springer
Magnetohydrodynamic (MHD) oscillatory processes in different plasma systems, such as the
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …
corona of the Sun and the Earth's magnetosphere, show interesting similarities and …
Kelvin Helmholtz instability in planetary magnetospheres
Kelvin–Helmholtz instability plays a particularly important role in plasma transport at
magnetospheric boundaries because it can control the development of a turbulent boundary …
magnetospheric boundaries because it can control the development of a turbulent boundary …
[HTML][HTML] A space hurricane over the Earth's polar ionosphere
In Earth's low atmosphere, hurricanes are destructive due to their great size, strong spiral
winds with shears, and intense rain/precipitation. However, disturbances resembling …
winds with shears, and intense rain/precipitation. However, disturbances resembling …
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 …
Plasma transport driven by the three‐dimensional Kelvin‐Helmholtz instability
X Ma, P Delamere, A Otto… - Journal of Geophysical …, 2017 - Wiley Online Library
It has been well demonstrated that the nonlinear Kelvin‐Helmholtz (KH) instability plays a
critical role for the solar wind interaction with the Earth's magnetosphere. Although the two …
critical role for the solar wind interaction with the Earth's magnetosphere. Although the two …
Magnetized Kelvin–Helmholtz instability: theory and simulations in the Earth's magnetosphere context
M Faganello, F Califano - Journal of Plasma Physics, 2017 - cambridge.org
The Kelvin–Helmholtz instability, proposed a long time ago for its role in and impact on the
transport properties at magnetospheric flanks, has been widely investigated in the Earth's …
transport properties at magnetospheric flanks, has been widely investigated in the Earth's …
Multiple transpolar auroral arcs reveal insight about coupling processes in the Earth's magnetotail
QH Zhang, YL Zhang, C Wang… - Proceedings of the …, 2020 - National Acad Sciences
A distinct class of aurora, called transpolar auroral arc (TPA)(in some cases called “theta”
aurora), appears in the extremely high-latitude ionosphere of the Earth when interplanetary …
aurora), appears in the extremely high-latitude ionosphere of the Earth when interplanetary …
Solar wind ion entry into the magnetosphere during northward IMF
Extended periods of northward interplanetary magnetic field (IMF) lead to the formation of a
cold, dense plasma sheet due to the entry of solar wind plasma into the magnetosphere …
cold, dense plasma sheet due to the entry of solar wind plasma into the magnetosphere …
Interaction of magnetic reconnection and Kelvin‐Helmholtz modes for large magnetic shear: 1. Kelvin‐Helmholtz trigger
X Ma, A Otto, PA Delamere - Journal of Geophysical Research …, 2014 - Wiley Online Library
At the Earth's magnetopause, both magnetic reconnection and the Kelvin‐Helmholtz (KH)
instability can operate simultaneously for southward interplanetary magnetic field conditions …
instability can operate simultaneously for southward interplanetary magnetic field conditions …
Kelvin‐Helmholtz Waves and Magnetic Reconnection at the Earth's Magnetopause Under Southward Interplanetary Magnetic Field
Abstract We present Magnetospheric Multiscale (MMS) observations of a K‐H wave event
under southward IMF conditions, accompanied by ongoing magnetic reconnection. The …
under southward IMF conditions, accompanied by ongoing magnetic reconnection. The …