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...

Descrizione completa

Dettagli Bibliografici

Autori principali:	S. H. Lai, Y.-C. Wang, Y.-H. Yang, W.-H. Ip
Natura:	Artigo
Lingua:	Inglês
Pubblicazione:	IOP Publishing 2024-01-01
Serie:	The Astrophysical Journal
Soggetti:	Planetary magnetospheres Solar wind Magnetohydrodynamical simulations Space plasmas Mercury (planet) Solar-terrestrial interactions
Accesso online:	https://doi.org/10.3847/1538-4357/ad944b
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!