CO on Titan: More Evidence for a Well-Mixed Vertical Profile

Caltech); D.O. Muhleman (Division of Geological; M.A. Gurwell (Harvard-Smithsonian Center for Astrophysics); Planetary Sciences

arxiv: astro-ph/0002331 · v1 · submitted 2000-02-16 · 🌌 astro-ph

CO on Titan: More Evidence for a Well-Mixed Vertical Profile

M.A. Gurwell (Harvard-Smithsonian Center for Astrophysics) , D.O. Muhleman (Division of Geological , Planetary Sciences , Caltech) This is my paper

classification 🌌 astro-ph

keywords profiletitanbesterrorsestimatedevidencefindinterferometric

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We report new interferometric observations of the CO (2-1) rotational transition on Titan. We find that the spectrum is best fit by a uniform profile of 52 ppm, with estimated errors of 6 ppm (40 to 200 km) and 12 ppm (200 to 300 km).

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CO on Titan: More Evidence for a Well-Mixed Vertical Profile

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