Figure 19
From: Precipitation-induced surface brightenings seen on Titan by Cassini VIMS and ISS
Adiri changes in doublepeak color. Titan’s bright region Adiri (view centered ∼1000 km west of the Huygens Landing Site) as seen by VIMS over the time range discussed in the text. This color scheme, colormapped with red as 2.0 μ m, green as 2.7 μ m, and blue as 2.8um, accentuates the changed areas of the surface due to the relatively greater brightening at 2.0 μ m and 2.8 μ m in the observed spectra (Figure 20).