{"id":144,"date":"2018-02-21T14:41:59","date_gmt":"2018-02-21T13:41:59","guid":{"rendered":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/?p=144"},"modified":"2018-02-28T13:29:50","modified_gmt":"2018-02-28T12:29:50","slug":"observation-programs","status":"publish","type":"post","link":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/en\/2018\/02\/21\/observation-programs\/","title":{"rendered":"Current observation programs"},"content":{"rendered":"\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n\n
Title<\/b><\/strong><\/td>\nTelescope<\/b><\/strong><\/td>\nType<\/b><\/strong><\/td>\nRole<\/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

[social_warfare buttons=”Facebook”]<\/p>\n","protected":false},"excerpt":{"rendered":"

Title Telescope Type Role 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

Continue reading “Current observation programs”<\/span><\/a><\/p>\n","protected":false},"author":45,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[34],"tags":[],"class_list":["post-144","post","type-post","status-publish","format-standard","hentry","category-research-en"],"_links":{"self":[{"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/posts\/144","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/users\/45"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/comments?post=144"}],"version-history":[{"count":5,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/posts\/144\/revisions"}],"predecessor-version":[{"id":537,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/posts\/144\/revisions\/537"}],"wp:attachment":[{"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/media?parent=144"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/categories?post=144"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/sites.lesia.obspm.fr\/thibault-cavalie\/wp-json\/wp\/v2\/tags?post=144"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}