R. P. Wilkerson, D. L. Rickman, J. R. McElderry, S. R. Walker, K. M. Cannon | 2024 | Icarus
DOI 10.1016/j.icarus.2024.115963Review state
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The paper discusses the challenges and considerations in analyzing shape data from planetary surfaces, focusing on the use of advanced statistical methods to improve the accuracy of geological interpretations. It highlights the importance of accounting for measurement uncertainties and the need for robust data processing techniques to extract meaningful insights from complex datasets. This paper focuses on the measurement of shape in lunar regolith, with applications to lunar regolith analysis. It references various studies and standards related to particle shape and size distribution, but does not introduce new simulants or samples. The provided text appears to be a series of URLs and file paths related to image assets (thumbnails, high-resolution images, etc.) associated with a scientific or technical paper or article. The URLs follow a consistent pattern, with the following components: The paper discusses the analysis of particle shape and size distribution for various powders, including lunar simulants and Apollo regolith. It presents contour plots of particle aspect ratio versus form factor for JSC-1A, JSC-2A, and NU-LHT-4M simulants, highlighting differences in their morpholo
These are the records this paper contributes to the simulant, returned sample, method, and property browsers.
Used to compare regolith and simulant morphology across different particle size ranges.
Morphological Descriptors | Used to analyze the relationship between particle size and shape characteristics.
Apollo 16 | sample
67941 | Luna | reference
68501 | Luna | reference
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open_access
CC BY-NC-ND license license
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US Depart of Energy funding
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