The Nitrogen Chemistry of Titan’s Upper Atmosphere Revealed

By V. Vuitton, R. Yelle, V. Anicich. 2006

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Analysis of Titan's neutral upper atmosphere from Cassini Ion Neutral Mass Spectrometer measurements in the Closed Source Neutral mode (2009, unknown): “…based on INMS have already been presented in Waite et al. (2005, 2007), Cravens et al. (2006), Yelle et al. (2006, 2008), De La Haye et al. (2007a, 2007b), Lavvas et al. (2008a, 2008b), Vuitton et al. (2006, 2007, 2008), Cui et al. (2008), Müller-Wodarg et al. (2006, 2008) and Hörst et al. (2008).”
Ion chemistry and N-containing molecules in Titan's upper atmosphere (2007, methodology): “In the following, we extend the study by Vuitton et al. (2006a) to the heavier mass end of the INMS spectrum (m/z > 60).”
Formation and distribution of benzene on Titan (2008, methodology): “[34] On the night-side, Vuitton et al. [2007] showed that because the ionization rate by magnetospheric electrons is”
Negative ion chemistry in Titan's upper atmosphere (2008, methodology): “Yet, the model includes the complete formation of positive ions as well, the details of which along with a complete description of the model can be found in Vuitton et al. (2007).”