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Empirical Evaluation of S-band Radar Polarimetric Response to Surface Rock Abundance across the Lunar Highlands and Maria

  • Authors: Edgard G. Rivera-Valentín, Caleb I. Fassett, Anne K. Virkki, Santa L. Pérez-Cortés, Tyler Powell, Dylan C. Hickson, Michael C. Nolan, G. Wesley Patterson

Edgard G. Rivera-Valentín et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 6.

CPR as a function of RA on a log-scaled axis for (left) Giordano Bruno and (right) Eimmart A. The top row shows the individual values for (dark gray) a random selection of values outside of three crater radii from the respective crater, and values inside three crater radii with (light gray) −0.6 < ρ < 0.6, (pink) ρ ≥ 0.6, and (green) ρ ≤ −0.6 (i.e., following the color bar in Figures 5(c) and (f)). The bottom row shows the median CPR behavior with RA over 50θ ≤ 60 for (blue) outside of three crater radii of the studied crater, and (orange) inside of three crater radii. The median behavior (solid lines) is shown along with the interquartile range (dashed lines).

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