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. 2014 Sep 26;119(9):2132–2147. doi: 10.1002/2013JE004514

Figure 13.

Figure 13

Atmospheric water content (in precipitable water as of micrometers) inferred from the in situ Mini-TES observations on board the Spirit (15°S) and Opportunity (2°S) rovers at the Martian surface. The black points are individual Mini-TES retrievals; the red line is a smoothed curve. The blue points are from the TES climatology for the rover sites [Smith et al., 2006].