Constraints on the depth and variability of the lunar regolith

163 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

The variability of crater identification among expert and community crater analysts (2014, methodology): “ margin of Mare Crisium and the neighboring rim/highlands to the south (Fig. 2). It has a solar incidence angle of 59°, which is on the boundary of what is considered ideal for crater identification (Wilcox et al., 2005; Ostrach et al., 2011; Robbins et al., 2012). Each image was downloaded from the”
How old are young lunar craters (2012, methodology): “…be due to several reasons, including the effects of different illumination conditions in images used for measurements [Soderblom, 1970; Young, 1975; Wilcox et al., 2005; Ostrach et al., 2011], multiphase volcanism [Strom and Fielder, 1968a, 1968b], self-secondary cratering [Shoemaker et al., 1968;…”