Static effects of differential rotation on Jupiter’s shape, gravity field, and interior structure

Open Access

Fig. 4

Results for the rotating n = 1 polytrope of Jupiter: calculated mean radii $R_{m}^{f i t}$ $Mathematical equation: $\[R_{\mathrm{m}}^{\mathrm{fit}}\]$$ and even gravitational harmonics for rigid rotation and six differential rotation scenarios (Cases 1–6). For the cases of differential rotation, the intensity parameter A ranges from 0.0005 to 0.010.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.