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. Author manuscript; available in PMC: 2019 Apr 17.
Published in final edited form as: J Geophys Res Planets. 2016 Jul 4;121(7):1293–1320. doi: 10.1002/2015JE004924

Figure 11.

Figure 11.

Nili Fossae. (a) THEMIS daytime image I02007009 8–7-5 DCS, modeled end-members (olivine = olivine-bearing material), and overlapping thermal inertia from THEMIS nighttime image I01327002. Color bar for end-member concentrations 0–100% and thermal inertia 120 to 380 J m–2 K–1 s–1/2. Black lines on modeled olivine image outline area of overlap with thermal inertia image. White boxes show location of CRISM image in Figure 12a. (b) THEMIS-derived thermal inertia bins with average olivine abundance indicate a generally positive correlation between thermal inertia and olivine abundance within the area of overlap.