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hal.structure.identifierImperial College London
dc.contributor.authorGHAIL, R. C.
hal.structure.identifierDepartment of Atmospheric, Oceanic and Planetary Physics [Oxford] [AOPP]
dc.contributor.authorWILSON, Colin
hal.structure.identifierImperial College London
dc.contributor.authorGALAND, Marina
hal.structure.identifierAstrium [Portsmouth]
dc.contributor.authorHALL, David
hal.structure.identifierImperial College London
dc.contributor.authorCOCHRANE, Chris
hal.structure.identifierImperial College London
dc.contributor.authorMASON, Philippa
hal.structure.identifierGerman Aerospace Center [DLR]
dc.contributor.authorHELBERT, Joern
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorMONTMESSIN, Franck
hal.structure.identifierDepartment of Physics [Madison]
dc.contributor.authorLIMAYE, Sanjay
hal.structure.identifierThe Open University [Milton Keynes] [OU]
dc.contributor.authorPATEL, Manish
hal.structure.identifierDepartment of Atmospheric, Oceanic and Planetary Physics [Oxford] [AOPP]
dc.contributor.authorBOWLES, Neil
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorSTAM, Daphne
hal.structure.identifierSwedish Institute of Space Physics [Uppsala / Kiruna] [IRF]
dc.contributor.authorWAHLUND, Jan-Erik
hal.structure.identifierPolitecnico di Milano [Milan] [POLIMI]
dc.contributor.authorROCCA, Fabio
hal.structure.identifierRoyal Holloway [University of London] [RHUL]
dc.contributor.authorWALTHAM, David
hal.structure.identifierDepartment of Earth Sciences [Oxford]
dc.contributor.authorMATHER, Tamsin A.
hal.structure.identifierUniversity of Bristol [Bristol]
dc.contributor.authorBIGGS, Juliet
hal.structure.identifierImperial College London
dc.contributor.authorGENGE, Matthew
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorPAILLOU, Philippe
hal.structure.identifierJet Propulsion Laboratory [JPL]
dc.contributor.authorMITCHELL, Karl
hal.structure.identifierLancaster University
dc.contributor.authorWILSON, Lionel
hal.structure.identifierNASA Langley Research Center [Hampton] [LaRC]
dc.contributor.authorSINGH, Upendra N.
dc.date.issued2012
dc.identifier.issn0922-6435
dc.description.abstractEnEnVision is an ambitious but low-risk response to ESA's call for a medium-size mission opportunity for a launch in 2022. Venus is the planet most similar to Earth in mass, bulk properties and orbital distance, but has evolved to become extremely hostile to life. EnVision's 5-year mission objectives are to determine the nature of and rate of change caused by geological and atmospheric processes, to distinguish between competing theories about its evolution and to help predict the habitability of extrasolar planets. Three instrument suites will address specific surface, atmosphere and ionosphere science goals. The Surface Science Suite consists of a 2.2 m2 radar antenna with Interferometer, Radiometer and Altimeter operating modes, supported by a complementary IR surface emissivity mapper and an advanced accelerometer for orbit control and gravity mapping. This suite will determine topographic changes caused by volcanic, tectonic and atmospheric processes at rates as low as 1 mm a - 1. The Atmosphere Science Suite consists of a Doppler LIDAR for cloud top altitude, wind speed and mesospheric structure mapping, complemented by IR and UV spectrometers and a spectrophotopolarimeter, all designed to map the dynamic features and compositions of the clouds and middle atmosphere to identify the effects of volcanic and solar processes. The Ionosphere Science Suite uses a double Langmiur probe and vector magnetometer to understand the behaviour and long-term evolution of the ionosphere and induced magnetosphere. The suite also includes an interplanetary particle analyser to determine the delivery rate of water and other components to the atmosphere.
dc.language.isoen
dc.publisherSpringer Link
dc.subject.enLIDAR
dc.subject.enInSAR
dc.subject.enVenus Tectonics
dc.subject.enVenus Atmosphere
dc.subject.enVenus Ionosphere
dc.title.enEnVision: taking the pulse of our twin planet
dc.typeArticle de revue
dc.identifier.doi10.1007/S10686-011-9244-3
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.journalExperimental Astronomy
bordeaux.page337-363
bordeaux.volume33
bordeaux.issue2-3
bordeaux.peerReviewedoui
hal.identifierhal-00620907
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00620907v1
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