Fig. 3

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Entropy percentage difference between the revised and the original AQUA EoS (background colors). Negative values (blue-ish) imply higher revised entropies. Coloured lines show adiabatic interior profiles of a Uranus-like planet with upper and lower envelope water abundances of Z1 = 0.360 and Z2 = 0.844, respectively, and surface (1 bar) temperatures of 70,100 and 200 K. Solid and dashed lines indicate adiabatic models computed with the revised and original AQUA, respectively.
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