The vertical profile of CO in the atmosphere of Neptune from JCMT and IRAM observations

Details The vertical profile of CO in the atmosphere of Neptune from JCMT and IRAM observations The vertical profile of CO in the atmosphere of Neptune from JCMT and IRAM observations

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..881c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.881

Physics

Scientific paper

In this paper, we will present a new observation of CO in the atmosphere of Neptune, obtained with the James Clerck Maxwell Telescope (JCMT) in the CO(6-5) line at 691.473GHz. We will present a joint analysis of this line and the CO(2-1) and CO(3-2) lines (published previously in [5, 6]) with the photochemical model we have developed in [10]. We will derive new constraints on the CO vertical profile in the upper atmosphere of Neptune and thus on the origin of this species.

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