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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| Autori principali: | , |
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| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Science Press
2020-02-01
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| Serie: | Earth and Planetary Physics |
| Soggetti: | |
| Accesso online: | http://www.eppcgs.org/article/doi/10.26464/epp2020014?pageType=en |
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