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Vertical Water Vapor Distribution In The Atmospheres Of Uranus And Neptune As Obtained From Herschel Observations

dc.contributor.authorJARCHOW, Christopher
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorHARTOGH, P.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorLELLOUCH, E.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]
dc.contributor.authorMORENO, R.
dc.contributor.authorFEUCHTGRUBER, H.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorCAVALIÉ, T.
dc.contributor.authorHSSO TEAM
dc.date.issued2010-10
dc.date.conference2010
dc.description.abstractEnAs part of the guaranteed time key programme "Water and related chemistry in the Solar System" (KP-GT HssO) about twenty different rotational water vapor transitions have been observed in the atmospheres of Uranus and Neptune with the PACS instrument of the European Space Agency's Herschel Space Observatory. In addition the 110-101 ground-state transition of H2O at 557 GHz has been observed in both planets at the very high resolution of 1 MHz using the Herschel/HIFI instrument. Using a line-by-line radiation transfer model in combination with the Optimal Estimation Method as retrieval technique we analyze the data in terms of information content to derive the vertical distribution of water vapor. The resulting distribution, which is obtained from a simultaneous fit of the whole set of transitions, will be presented for both planets.
dc.language.isoen
dc.source.titleBulletin of the American Astronomical Society
dc.title.enVertical Water Vapor Distribution In The Atmospheres Of Uranus And Neptune As Obtained From Herschel Observations
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.page1022
bordeaux.volume42
bordeaux.conference.titleAmerican Astronomical Society, DPS meeting #42, #11.26
bordeaux.countryUS
bordeaux.title.proceedingBulletin of the American Astronomical Society
bordeaux.conference.cityPasadena, CA
bordeaux.peerReviewedoui
hal.identifierhal-00521670
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00521670v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=Bulletin%20of%20the%20American%20Astronomical%20Society&rft.date=2010-10&rft.volume=42&rft.spage=1022&rft.epage=1022&rft.au=JARCHOW,%20Christopher&HARTOGH,%20P.&LELLOUCH,%20E.&MORENO,%20R.&FEUCHTGRUBER,%20H.&rft.genre=unknown


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