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. 6

Comparison of the measured radiance (black) with the rough model (red) and the equilibrium model (blue) along the horizontal profiles 30_R1–30_R4 and along the vertical profiles 30_C1–30_C4 indicated in Fig. 5 (bottom). Offsets for clarity.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.