CAVALIÉ, T.; BILLEBAUD, F.; BIVER, N.; DOBRIJEVIC, M.; LELLOUCH, E.; BRILLET, J.; LECACHEUX, J.; HJALMARSON, A.; SANDQVIST, A.; FRISK, U.; OLBERG, M.; ODIN, Equipe; BERGIN, E. A.

doi:10.1016/j.pss.2008.04.013

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CAVALIÉ, T.
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]

BILLEBAUD, F.
Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
Observatoire aquitain des sciences de l'univers [OASU]
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]

BIVER, N.
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]

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Este ítem está publicado en

Planetary and Space Science. 2008, vol. 56, n° 12, p. 1573-1584

Elsevier

Resumen en inglés

The water vapor line at 557 GHz has been observed with the Odin space telescope with a high signal-to-noise ratio and a high spectral resolution on November 8, 2002. The analysis of this observation as well as a re-analysis of previously published observations obtained with the SubmillimeterWavelength Astronomy Satellite seem to favor a cometary origin (Shoemaker-Levy 9) for water in the stratosphere of Jupiter, in agreement with the ISO observation results. Our model predicts that the water line should become fainter and broader from 2007. The observation of such a temporal variablity would be contradictory with an IDP steady flux, thussupporting the SL9 source hypothesis.< Leer menos

Palabras clave en inglés

Jupiter

atmosphere

water

spectroscopy

Odin space telescope

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Observation of water vapor in the stratosphere of Jupiter with the Odin Space Telescope.

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Este ítem está publicado en

Resumen en inglés

Palabras clave en inglés

DOI

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