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. Author manuscript; available in PMC: 2020 Dec 17.
Published in final edited form as: Nat Astron. 2020 May 11;4:756–761. doi: 10.1038/s41550-020-1080-9

Extended Data Fig. 1 — Frequency of temperature and water vapor pressure pairings.

Extended Data Fig. 1 —

In Figure 1, the Mars-relevant pairings of surface temperature and atmospheric water vapor pressure are contained between the cyan lines. Here we show the frequency (in color) of each combination of surface temperature and water vapor pressure predicted by MarsWRF in support of the presented analysis in Figure 1. Frequency here is the log base 10 of the number of hours across the surface of Mars at a 5° × 5° latitude/longitude grid and one-hour temporal resolution. For the purposes of counting, temperature and water vapor pressure were binned in increments of 1 K and 1 Pa. Here the cyan lines from Figure 1 are in black