An advanced thermal roughness model for airless planetary bodies - Implications for global variations of lunar hydration and mineralogical mapping of Mercury with the MERTIS spectrometer

Open Access

Fig. 16

Measured radiance (points) across a titanium-rich region of Oceanus Procellarum vs. various modeling approaches (solid lines). The data points correspond to a subsample of profile 30_C1 in Fig. 6. To avoid clutter, we offset the profile groups by 1 W m⁻² sr⁻¹ µm⁻¹.

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