Scatter plots as per Fig. 4, and Spectra-derived TiO2 as per Fig. 7

F. Zhang, J. W. Head, C. Wöhler, R. Bugiolacchi, L. Wilson, A. T. Basilevsky, A. Grumpe, Y. L. Zou. Ring-Moat Dome Structures (RMDSs) in the Lunar Maria: Statistical, Compositional, and Morphological Characterization and Assessment of Theories of Origin. Journal of Geophysical Research: Planets, 125, e2019JE005967. https://doi.org/10.1029/2019JE005967 Figure 4. Scatter plots of diameters, heights, and volumes of the 532 RMDSs measured from NAC-derived DTMs: (a) diameter vs. height; (b) diameter vs. volume Figure 7. M3-spectra-derived TiO2 contents of RMDSs and global maria (latitude range +/- 75 degrees). (a) Mean TiO2 wt% vs. diameter for 2407 RMDSs in seven large mare regions indicated in Figure 2; (b) The TiO2 content histogram of the measured 2407 RMDSs (green color), compared with the global TiO2 distribution of all lunar mare regions (red color). Both histograms are normalized to 1, such that the sum of all red or green histogram bins is 1, respectively. The global Ti abundance was taken from the complete lunar mare surface at a latitude range +/- 75 degrees