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Fig. 1


Different HCN rotational cooling-rate profiles extending to the exobase, calculations assume LTE conditions. The red full and dashed lines are taken from De La Haye et al. (2008) and present night and day conditions for one of the Cassini flybys (T5), respectively, and the blue full and dashed lines are the same for the second flyby (Ta). The dark green curve is taken from Bell et al. (2010). Results of this work under LTE are shown as the black curve with squares.

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