Fig. 2
Pressure–temperature profiles influenced by low and high clouds for four different coverages (Kitzmann et al. 2010): 0% (solid lines), 30% (dotted), 70% (dash-dot), and 100% (dashed). Planets are modeled around typical F (olive green), G (brown), K (orange), and M (blue) star types. The location of the low- (top) and high-level (bottom) clouds is also illustrated.
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