Fig. 18
Latitudinal variations in the water vapor column density observed by PFS berween Ls = 205° and 215° in the case of MY 29, corresponding to a dust opacity lower than 0.4 (stars), and M34, a great dust storm (crosses). The color bar on the right of the figure indicates the integrated dust opacity. The figure is taken from Giuranna & Wolkenberg (2019).
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