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 ^−1 , zonal flows in the dynamo region are significantly slower, on the order of ∼cm s ^−1 or l...

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Principais autores:	Hao Cao, Jeremy Bloxham, Ryan S. Park, Burkhard Militzer, Rakesh K. Yadav, Laura Kulowski, David J. Stevenson, Scott J. Bolton
格式:	Artigo
語言:	Inglês
出版:	IOP Publishing 2023-01-01
叢編:	The Astrophysical Journal
主題:	Jupiter Planetary atmospheres Planetary interior Gravitational fields
在線閱讀:	https://doi.org/10.3847/1538-4357/ad0cbb
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