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A Model for Negative Ion Chemistry in Titan’s Ionosphere

  • Authors: Vrinda Mukundan, and Anil Bhardwaj

2018 The Astrophysical Journal 856 168.

  • Provider: AAS Journals

Caption: Figure 5.

Density profiles of (a) C4H and (b) C5N calculated using the current model compared with the calculations of Vuitton et al. (2009) and Dobrijevic et al. (2016). In the top panel, the symbols connected by the solid line show the profile of C3N obtained when electron density was reduced by half to nullify the effect of overestimation in the electron density. See the text for more details.

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