Vertical abundance profiles of hydrocarbons in Titan's atmosphere at 15° S and 80° N retrieved from Cassini/CIRS spectra

By S. Vinatier, B. Bézard, T. Fouchet, Nicholas A. Teanby, Remco J. de Kok, P. Irwin, B. Conrath, C. Nixon, P. Romani, E. M. Flasar and 1 more. 2007

200 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/a86dff396d7a471a8d3020d3cdc9d5eaf603fda0

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In Astronomy and Astrophysics

1. V. Vuitton
2. M. McEwan
3. R. Yelle
4. Nicholas A. Teanby
5. B. Bézard
6. J. Cui
7. J. Owen
8. V. Krasnopolsky

In Atmospheric Science

1. M. McEwan
2. V. Vuitton
3. R. Yelle

Citations in the corpus

• Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles (2010, background): “It was not inferred in our previous study (Vinatier et al., 2007a) because the limb spectra in the previous version of the calibration were then noisier. Below 46 N, we were only able to infer a 3-r upper limit of 0.3 ppb in the 5–2 mbar pressure range. This value at low latitude is consistent with ”
• Ion chemistry and N-containing molecules in Titan's upper atmosphere (2007, methodology): “ter (CIRS) on Cassini retrieves stratospheric abundance vertical profiles of C2H4, C4H2, C6H6, HCN and HC3N (Teanby et al., 2006; Vinatier et al., 2007).”