The Influence of Space Weathering on the Far-Ultraviolet Reflectance of Apollo-era Soils

The files listed here contain the data used for Figures 3, 4, 5, and 6 and Supplemental Figures S1b, S2, and S3 of the paper titled "The Influence of Space Weathering on the Far-Ultraviolet Reflectance of Apollo-era Soils." The experimentally derived phase curve data from Figure 3 are contained in the .txt files which have the material name (Apollo 10084, 68501, or 71061) followed by "BRDF," the wavelength in Angstroms (1216, 1400, or 1600), and "Data" in the file name. Files with the fitted Hapke photometric model curves have "Hapke" in place of "Data" in the name. All files with "Hapke" in the file name are the Hapke photometric model (Hapke, 2012) fitted phase curves for the associated experimental data. Figure 4 TEM images are included as .tiff files, with the sample indicated followed by which image pane the image belongs to ("FullGrain" for the first wide field image in line, 1, 2, or 3). The Apollo 71061 images also include "G1" or "G2" for the two different grains presented. Particle size distribution data as presented in Figure 4 is contained in the .txt files with "Fig4" in the file name. The nested sampling results used in Figure 5 are in the .csv file with "Fig5" in the name, with the supplementary examples for Apollo 68501 and 71061 similarly identified with "FigS3a" and "FigS3b," respectively. Figure 6 contains datapoints already listed in supplemental tables S1, S2, and S3. The Hapke "hockeystick" curve data plotted in Figure 6D is included in this dataset as Fig6d_HapkeHockeystickCurve.txt. Elemental maps presented in Figure S1b are included as .tiffs with the sample name and the element mapped indicated in the file name. X-ray counts associated with these maps are included in .txt files with "FigS1b" and the sample name in the title. The supplemental images in Figure S2 are included as .tiffs with the sample name, "SEM," and "W" or "N" for the wide angle and zoomed fields, respectively.