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

M. A. Gurwell·D. O. Muhleman
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Abstract

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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M. A. Gurwell, D. O. Muhleman. 2000-02-16. CO on Titan: More Evidence for a Well-Mixed Vertical Profile. https://doi.org/10.1006/icar.2000.6424

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