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Fig. 12


Saturn’s stratospheric H2O meridional distribution as derived from Herschel-PACS mapping observations on January 2, 2011. Left: mole fraction above the local condensation level as a function of latitude. Right: corresponding column density as a function of latitude. The distribution is a Gaussian centered on the equator with yeq = 1.1 ppb and σ = 25°, corresponding to the PACS map best-fit model (see Fig. 11). Background image credits: NASA/JPL-Caltech/Space Science Institute.

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