Solar Wind–Magnetosphere Coupling by the Kelvin–Helmholtz Instability at Mercury

The Kelvin–Helmholtz instability (KHI) has been considered important in the energy transfer and momentum coupling between the solar wind and planetary magnetospheres. To explore this issue, we employ a two-dimensional magnetohydrodynamic simulation to study the nonlinear evolution of the KHI at Merc...

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Detalles Bibliográficos

Autores principales:	S. H. Lai, Y.-C. Wang, Y.-H. Yang, W.-H. Ip
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2024-01-01
Colección:	The Astrophysical Journal
Materias:	Planetary magnetospheres Solar wind Magnetohydrodynamical simulations Space plasmas Mercury (planet) Solar-terrestrial interactions
Acceso en línea:	https://doi.org/10.3847/1538-4357/ad944b
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