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Figure 21 | Planetary Science

Figure 21

From: Precipitation-induced surface brightenings seen on Titan by Cassini VIMS and ISS

Figure 21

Spectral window changes. Here we compare the relative integrated I/F for clouds, bright terrain, dark terrain, and the T76 Yalaing Terra brightened terrain within the spectral windows and acquired under the same viewing geometry with i=45°, e=19°. This three-dimensional plot shows the total spectral areas for individual pixels in each of these terrains, integrated across the 2, 2.68/2.78, and 5 micron windows. The T76 brightened surfaces plot apart from both dark and bright terrain, and well apart from clouds.

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