Exploring the deep atmospheres of HD 209458b and WASP-43b using a non-gray general circulation model

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Fig. 8

Evolution of the temperature profile at the substellar point (like Fig. 6). Three time steps (100 d, 5000 d and 12 000 d) of the nominal model of WASP-43b are compared to a model of WASP-43b with a rotation period equal to the rotation period of HD 209458b. The color scale is the same as in Fig. 6.

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