Formation and distribution of benzene on Titan

By V. Vuitton, R. Yelle, J. Cui. 2008

191 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/90790fb126486c2245dee98d6e3bd7e3a54d6818

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Jon Fortney
2. M. Marley
3. A. Showman
4. N. Madhusudhan
5. R. Freedman
6. V. Parmentier
7. N. Lewis
8. Adam Burrows

In Atmospheric Science

1. M. Marley
2. J. Cui
3. V. Vuitton
4. P. Lavvas
5. M. McEwan
6. Jon Fortney
7. R. Yelle
8. A. Showman

Citations in the corpus

• Analysis of Titan's neutral upper atmosphere from Cassini Ion Neutral Mass Spectrometer measurements in the Closed Source Neutral mode (2009, background): “The candidate neutrals include N2, CH4, H2, C2H2, C2H4, C2H6, C3H4, C3H8, C4H2, C4H6, C6H6, C7H8, NH3, HCN, CH3CN, HC3N, C2H3CN, C2H5CN, C2N2, H2O, CO2 and 40Ar.”
• Negative ion chemistry in Titan's upper atmosphere (2008, methodology): “Furthermore, it was used for the investigation of the ion–neutral chemical processes controlling the formation of the observed thermospheric benzene abundance (Vuitton et al., 2008).”
• AN ESTIMATE OF THE CHEMICAL COMPOSITION OF TITAN's LAKES (2009, methodology): “The precipitation rates used here are given in Table 2 and derive from the photochemical models of Lavvas et al. (2008a,b) and Vuitton et al. (2008) and correspond to the main products of CH4 and N2 photolysis.”
• Ion chemistry and N-containing molecules in Titan's upper atmosphere (2007, methodology): “This is in good agreement with the detection of C6H6 obtained by INMS in the neutral mode for lowaltitude flybys (Vuitton et al., 2007).”
• DISEQUILIBRIUM CARBON, OXYGEN, AND NITROGEN CHEMISTRY IN THE ATMOSPHERES OF HD 189733b AND HD 209458b (2011, background): “…ions and photochemically produced aerosols through a Titan-like ion-chemistry process (e.g., Waite et al. 2007, 2009; Imanaka & Smith 2007; Vuitton et al. 2007, 2008), although it is also possible that the high abundance of H2O and/or CO and the low abundance of CH4 at high altitudes on…”
• Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles (2010, methodology): “This value at low latitude is consistent with the prediction of the photochemical model of Vuitton et al. (2008) .”