Fig. 3

Illustration of viewing geometries and effect of microtopography. Panel a: relations between the viewing angles. i, e, and g are the incidence angle, emission angle, and phase angle, respectively, and i′ and e′ are the incidence and emission angles after topographical correction. θ1 and θ2 are the slope angles along and perpendicular to the rover viewing direction, respectively. Panel b: corrected angles. φ is the relative azimuth angle between the rover and the Sun, p1 is the length of the projection of the normal vector onto the YOZ plane, p2 is the length of the projection of the normal vector onto the XOZ plane, and p3 is the length of the projection of the normal vector onto the Z-axis.
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.