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The vertical profile of CO in the atmosphere of Neptune from JCMT and IRAM observations
FOUCHET, T.
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
Institut universitaire de France [IUF]
Université Pierre et Marie Curie - Paris 6 [UPMC]
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
Institut universitaire de France [IUF]
Université Pierre et Marie Curie - Paris 6 [UPMC]
HARTOGH, P.
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
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Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
Language
en
Communication dans un congrès
This item was published in
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France., p.881, 2011, EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France., p.881, 2011, EPSC-DPS Joint Meeting 2011, 2011, Nantes. 2011-10p. 881
English Abstract
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 ...Read more >
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.Read less <
Origin
Hal imported