Fig. 19
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Albedo retrievals of an Earth-like planet for different noise levels (Nmax = ∞ is noise-free), using the optimal configuration from Fig. 17. The architecture from Fig. 18 for total flux curves computed using Lambertian reflecting model planets is used. The actual Earth albedo map is shown in Fig. 16. The MSE is computed by comparing the retrieved map with the map of the model Earth.
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