Ion Dynamics in the Meso-scale 3-D Kelvin–Helmholtz Instability: Perspectives From Test Particle Simulations

Over three decades of in-situ observations illustrate that the Kelvin–Helmholtz (KH) instability driven by the sheared flow between the magnetosheath and magnetospheric plasma often occurs on the magnetopause of Earth and other planets under various interplanetary magnetic field (IMF) conditions. It...

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Autores principales: Xuanye Ma, Peter Delamere, Katariina Nykyri, Brandon Burkholder, Stefan Eriksson, Yu-Lun Liou
Formato: article
Lenguaje:EN
Publicado: Frontiers Media S.A. 2021
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Acceso en línea:https://doaj.org/article/54798c8ca6f943e3b92ef29fbbe5aa4e
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