Fig. 2
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Left column: pressure-temperature profiles from the cloudless GCM models (top, cloudless GCM with low Tint; bottom, cloudless GCM with high Tint; grey, profiles at all latitudes and longitudes and light blue, 1D profile from Wiser et al. 2025). The condensation curves of several important species are plotted as dashed lines. Right column: ADAM spectrum plotted with JWST observations in grey (top, emission spectra for cloudless GCM with low and high Tint showing significant overlap, indicating minimal sensitivity to internal heating in the terminator region, plotted along with 1D spectrum from Wiser et al. (2025); bottom, transmission spectra for cloudless GCM with low and high Tint showing significant overlap, indicating minimal sensitivity to internal heating in the terminator region).
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