{"id":433,"date":"2018-02-23T18:10:47","date_gmt":"2018-02-23T17:10:47","guid":{"rendered":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/?p=433"},"modified":"2018-02-28T13:29:34","modified_gmt":"2018-02-28T12:29:34","slug":"programmes-dobservation-en-cours","status":"publish","type":"post","link":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/2018\/02\/23\/programmes-dobservation-en-cours\/","title":{"rendered":"Programmes d’observation en cours"},"content":{"rendered":"\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Titre<\/b><\/strong><\/td>\nT\u00e9lescope<\/b><\/strong><\/td>\nType<\/b><\/strong><\/td>\nR\u00f4le<\/b><\/strong><\/td>\n<\/tr>\n
Jupiter System<\/td>\nJWST<\/td>\nERS<\/td>\nScience Team<\/td>\n<\/tr>\n
Are the Enceladus geysers the source of Saturn\u2019s water\u00a0?<\/td>\nALMA<\/td>\nCycle 5<\/td>\nPI<\/td>\n<\/tr>\n
Constraining Jupiter’s atmospheric chemistry and dynamics from H2<\/sub>O mapping in ALMA band 5<\/td>\nALMA<\/td>\nCycle 5<\/td>\nPI<\/td>\n<\/tr>\n
The first direct measurement of Saturn\u2019s stratospheric winds<\/td>\nALMA<\/td>\nCycle 5<\/td>\nCo-I<\/td>\n<\/tr>\n
Constraining the internal and external sources of CO in Saturn’s atmosphere<\/td>\nIRTF<\/td>\nStandard<\/td>\nCo-I<\/td>\n<\/tr>\n
Constraining Jupiter’s atmospheric chemistry and dynamics from post-SL9 species mapping<\/td>\nALMA<\/td>\nCycle 4<\/td>\nPI<\/td>\n<\/tr>\n
HCN emission: a diagnostic of Enceladus cryovolcanic activity and torus dynamics<\/td>\nALMA<\/td>\nCycle 2<\/td>\nCo-I<\/td>\n<\/tr>\n
Probing the vertical structure of Saturn’s storm with ALMA<\/td>\nALMA<\/td>\nCycle 0<\/td>\nPI<\/td>\n<\/tr>\n
Water and related chemistry in the Solar System<\/td>\nHerschel<\/td>\nGuaranteed Time<\/p>\n

Key Program<\/td>\n

Associate Scientist<\/td>\n<\/tr>\n
Probing the temperature and chemistry of Saturn’s storm with Herschel<\/td>\nHerschel<\/td>\nOpen Time<\/td>\nPI<\/td>\n<\/tr>\n
Probing the Enceladus torus with Herschel<\/td>\nHerschel<\/td>\nOpen Time<\/td>\nCo-I<\/td>\n<\/tr>\n
Variability in Ice Giant Stratospheres: Implications for Radiative, Chemical and Dynamical Processes<\/td>\nHerschel<\/td>\nOpen Time<\/td>\nCo-I<\/td>\n<\/tr>\n
The spatial distribution of CO in Saturn<\/td>\nSMA<\/td>\nStandard<\/td>\nPI<\/td>\n<\/tr>\n
Observation of an equatorial jet in the atmosphere of Jupiter<\/td>\nIRAM-30m<\/td>\nStandard<\/td>\nPI<\/td>\n<\/tr>\n
The origin of CO in Saturn\u2019s atmosphere<\/td>\nVLT<\/td>\nShort Program<\/td>\nCo-I<\/td>\n<\/tr>\n
Jupiter\u2019s stratospheric HCN, hydrocarbon and temperature fields<\/td>\nSOFIA<\/td>\nCycle 3<\/td>\nCo-I<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n

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Titre T\u00e9lescope Type R\u00f4le Jupiter System JWST ERS Science Team Are the Enceladus geysers the source of Saturn\u2019s water\u00a0? ALMA Cycle 5 PI Constraining Jupiter’s atmospheric chemistry and dynamics from H2O mapping in ALMA band 5 ALMA Cycle 5 PI The first direct measurement of Saturn\u2019s stratospheric winds ALMA Cycle 5 Co-I Constraining the internal … <\/p>\n

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