Strong resemblance between surface and deep zonal winds inside Jupiter revealed by high-degree gravity moments

Jupiter's atmosphere-interior is a coupled fluid dynamical system strongly influenced by the rapid background rotation. While the visible atmosphere features east-west zonal winds on the order of 100 m/s (Tollefson et al. 2017), zonal flows in the dynamo region are significantly slower, on the...

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Veröffentlicht in:arXiv.org 2023-11
Hauptverfasser: Cao, Hao, Bloxham, Jeremy, Park, Ryan S, Militzer, Burkhard, Yadav, Rakesh K, Kulowski, Laura, Stevenson, David J, Bolton, Scott J
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Sprache:eng
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