SHARAD sounding radar on the Mars Reconnaissance Orbiter

By Roberto Seu, Roger J. Phillips, Daniela Biccari, R. Orosei, A. Masdea, G. Picardi, A. Safaeinili, B. Campbell, Jeffrey J. Plaut, L. Marinangeli and 2 more. 2007

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The High Resolution Imaging Science Experiment (HiRISE) during MRO’s Primary Science Phase (PSP) (2010, methodology): “These map projections do not use the full MOLA DTM – we do not want to orthorectify (remove terrain distortions) because that is the information anaglyphs are supposed to capture.”
Selection of the InSight Landing Site (2017, methodology): “Subsurface detections at landing sites with SHARAD data have thus far been confined to the ‘Green Valley’ of the PHX site, with returns from ∼25 m depth mapped over 2900 km2 that may represent the base of ground ice (Putzig et al. 2014).”
SHARAD detection and characterization of subsurface water ice deposits in Utopia Planitia, Mars (2016, methodology): “After processing, SHARAD’s cross-track resolution is 3–6 km and the along-track resolution is 0.3–1 km [Seu et al., 2007].”