Coupling photochemistry with haze formation in Titan's atmosphere, Part I: Model description

By P. Lavvas, A. Coustenis, I. Vardavas. 2008

209 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/c89429e531c2e7824ce698709a024eb73ea82d06

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. Line
3. J. Lustig-Yaeger
4. T. Greene
5. N. Madhusudhan
6. P. Lavvas
7. C. Montero
8. Kyle L. Luther

In Atmospheric Science

1. Jon Fortney
2. P. Lavvas
3. J. Lustig-Yaeger
4. M. Line
5. V. Vuitton
6. N. Madhusudhan

Citations in the corpus

• AN ESTIMATE OF THE CHEMICAL COMPOSITION OF TITAN's LAKES (2009, background): “At low temperature conditions found in the lower stratophere and troposphere, the formed gases can condense on the aerosols and their precipitation rates (see Table 2). are given by photochemical models (Lavvas et al. 2008a, 2008b; Vuitton et al. 2008).”
• Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles (2010, background): “Wilson and Atreya, 2004; Lavvas et al., 2008a, b, ... ) predict that the molecular vertical mixing ratio profiles increase with height as the molecules are formed in the upper atmosphere, diffuse downwards and generally condense in the lower stratosphere.”
• CHARACTERIZING TRANSITING EXOPLANET ATMOSPHERES WITH JWST (2015, background): “These processes come in a variety of flavors including, but not limited to vertical and horizontal mixing (Prinn & Barshay 1977; Cooper & Showman 2006), photochemistry (Yung & Demore 1999), ion chemistry (Lavvas et al. 2008), and biology (e.g., Holland 1994).”