Lower-order zonal gravitational coefficients caused by zonal circulations inside gaseous planets: Convective flows and numerical comparison between modeling approaches

To infer the internal equilibrium structure of a gaseous planet, especially the equation of state (EOS) and size of its inner core, requires accurate determination of lower-order zonal gravitational coefficients. Modeling of the gravitational signature associated with deep zonal circulation depends...

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Detaylı Bibliyografya

Asıl Yazarlar:	DaLi Kong, KeKe Zhang
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	Science Press 2020-02-01
Seri Bilgileri:	Earth and Planetary Physics
Konular:	gaseous planets gravitation zonal circulation
Online Erişim:	http://www.eppcgs.org/article/doi/10.26464/epp2020014?pageType=en
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