Open Access
Fig. 13
Effect of the inner boundary of the 3D GCM models on the (Tgas, pgas)-profiles and the localcloud properties J*,
, and ρd ∕ρ
for the giant gas planet example WASP-43b. Left: based on the 1D thermodynamic profiles from Parmentier et al.
Right: based on the 1D thermodynamic profiles from Carone et al.
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