Fig. 16
Latitudinal section of the beam-convolved column density of water as derived from the 66.4 μm map. Only the pixels within the planetary disk are represented here. The peak values around 15 °S can most probably be attributed to the warmer temperatures observed around this latitude. The marginal increase seen around 30 °N could be due to the bright band detected at these latitudes in 2010 in the IRTF/MIRSI observations (see Fig. 14).
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