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...
| Váldodahkkit: | , |
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| Materiálatiipa: | Artihkal |
| Giella: | English |
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Science Press
2020-02-01
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| Ráidu: | Earth and Planetary Physics |
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| Liŋkkat: | http://www.eppcgs.org/article/doi/10.26464/epp2020014?pageType=en |