Three-dimensional Magnetohydrodynamic Simulations of Periodic Variations of Ganymede’s Footprint

Three-dimensional Magnetohydrodynamic Simulations of Periodic Variations of Ganymede’s Footprint

Alfvénic power is generated through the interaction between the mini-magnetosphere of Ganymede and the corotating flow of the Jovian plasma, contributing to the formation of the Ganymede auroral footprint at Jupiter’s ionosphere. Using a three-dimensional, high-resolution global magnetohydrodynamic...

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Detaylı Bibliyografya
Asıl Yazarlar: Tao Yan, Binzheng Zhang, Junjie Chen, Zhiqi Zheng, Ziyi Yang, Shengyi Ye, Jun Cui
Materyal Türü: Makale
Dil:English
Baskı/Yayın Bilgisi: IOP Publishing 2024-01-01
Seri Bilgileri:The Astrophysical Journal
Konular:
Alfvén waves
Ganymede
Magnetohydrodynamical simulations
Magnetohydrodynamics
Online Erişim:https://doi.org/10.3847/1538-4357/ad2c8a

Internet

https://doi.org/10.3847/1538-4357/ad2c8a

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