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2 results for “lunar regolith simulants”
Far-Ultraviolet Photometric Characteristics of JSC-1A and LMS-1 Lunar Regolith Simulants: Comparative Investigations with Apollo 10084
<p>The .txt files listed here contain the data used for Figure 3 and Supplemental Figure S3 of the paper titled "Far-Ultraviolet Photometric Characteristics of JSC-1A and LMS-1 Lunar Regolith Simulants: Comparative Investigations with Apollo 10084." The experimentally derived phase curves are contained in the files which have the material name (JSC-1A, LMS-1, or Apollo 10084) followed by the wavelength alone (Lyman-a, 140 nm, 160 nm) in the file name. All files with "Hapke" in the file name are the Hapke photometric model (Hapke, 2012) fitted phase curves for the associated experimental data. Two of the JSC-1A files have either "LT38" or "GT150" included in the file name; these are the sieved grain size category data referenced in S3.</p> <p>Also included are .txt files of the data points used in Figure 4 for the JSC-1A and LMS-1 simulants. These each have "Fig4" in the file name.</p>
Ultrasonic velocity measurements of lunar regolith simulant at low confining pressures with variable ice content
<p>This dataset was created by Christopher Chance Amos during completion of a PhD degree in Space Resources</p><p>at Colorado School of Mines. This data was collected during Spring 2023.</p><p> </p><p>This dataset includes compressional and shear raw collected waveforms as well as interpreted velocities</p><p>from first-break picking. See the README files in subdirectories for explanations of individual files.</p><p> </p><p>The purpose of this dataset is to serve as a foundation and calibration for seismic modeling of the lunar</p><p>near-surface. These models will be used to determine if seismic methods are feasible for characterizing</p><p>the quantity and form of lunar subsurface ice deposits.</p>
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