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Fig. 4


Top:the different heat transport regimes in the current-state Jupiter given by the density ratio Rρ . Jupiter has three different regimes for the heat transport: stable (Rρ < 0), DDC (0 < Rρ < 1), and convective (Rρ > 1). Since the values of Rρ changes on a very wide range, the y-axis zoom-in the critical range, and the background colors represent the ± log(|Rρ|). Bottom: the adiabatic, radiative and mean molecular weight gradients in the current-state model.

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