Regular ArticleHigh-Resolution Radar Imaging of Mercury's North Pole
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Medical image fusion algorithm based on multi-resolution analysis coupling approximate spare representation
2019, Future Generation Computer SystemsConstraining the thickness of polar ice deposits on Mercury using the Mercury Laser Altimeter and small craters in permanently shadowed regions
2018, IcarusCitation Excerpt :Furthermore, in some craters, surface volatiles exhibit a cratered texture similar to the sunlit portion of the crater floor, suggesting that the surficial ice was emplaced after the formation of the underlying small craters (Chabot et al., 2014). This is also more consistent with Case I. Finally, regolith gardening models (Crider and Killen, 2005) suggest that the ice deposits were emplaced <50 Myr ago in order to explain the enhanced radar backscatter (Slade et al., 1992; Harmon and Slade, 1992; Butler et al., 1993; Harmon et al., 1994, 2001, 2011; Harmon, 2007). It is possible, however, that there are examples of both Case I and Case II craters within the PSRs.
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