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

Preprint

16 February 2000

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0002331

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).

Keywords

INTERFEROMETRIC OBSERVATIONS
MIXED VERTICAL
NEW INTERFEROMETRIC
ROTATIONAL TRANSITION
SPECTRUM
TITAN
UNIFORM PROFILE
VERTICAL PROFILE
WELL MIXED

All Related Versions

Version 1, 2000-02-16, ArXiv
Published version: Icarus, 145 (2), 653.

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