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Fig. 4.

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Density profiles of various components of Saturn’s upper atmosphere obtained from forward modelling of the Cassini UVIS δ-Ori stellar occultation on 2005 DOY 103 at a latitude of −42.7°. From the book Saturn from Cassini-Huygens (M.K. Dougherty et al. eds.), Chapter 8 by Nagy et al. (2009).

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