Seasonal variation of the main gases in Titan's ionosphere from Cassini INMS data

Open Access

Fig. 4

Upper and lower limits of the transition area between the homosphere and the heterosphere for each flyby from the mole fraction (grey) and the molecular density (red) of N₂. The results from Waite et al. (2005) are in blue and those from Bell et al. (2011) are represented by the dashed grey line.

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