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

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

2000-02-16

arxiv.org/abs/astro-ph/0002331v1

Astronomy and Astrophysics

Astrophysics

Submitted to as a Note to Icarus. Uses emulateapj.sty under Latex, 6 text pages, 2 figs (includes with psfig)

Scientific paper

10.1006/icar.2000.6424

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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