Fig. 13
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Dust extinction κext [cm2 g-1] pressure isobars at φ = 90° (left), 270° (right), θ = 0° (equatorial dayside-nightside terminator regions). Triangles denote the values from Dobbs-Dixon & Agol (2013) assumed additional Rayleigh slope opacity κext ∝ λ-4. Isobars follow an absorption profile κext ∝ λ-2 at the upper atmosphere ≲10-1 bar. Isobars flatten deeper than ≳10-1 bar.
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