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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Auteurs principaux: | , , , , , |
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Format: | article |
Langue: | EN |
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Frontiers Media S.A.
2021
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Accès en ligne: | https://doaj.org/article/54798c8ca6f943e3b92ef29fbbe5aa4e |
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