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hal.structure.identifierPLANETO - LATMOS
hal.structure.identifierESTER - LATMOS
dc.contributor.authorCIARLETTI, Valérie
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorCAIS, Ph.
hal.structure.identifierLaboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS]
dc.contributor.authorBELARBI, Alex
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierUniversité Sciences et Technologies - Bordeaux 1 [UB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
dc.contributor.authorSALIM, Z.
hal.structure.identifierTechnische Universität Dresden = Dresden University of Technology [TU Dresden]
dc.contributor.authorPLETTEMEIER, Dirk
dc.date.created2010
dc.date.issued2010-09
dc.date.conference2010-09-19
dc.description.abstractThe WISDOM (Water Ice Subsurface Deposit Observation on Mars) Ground Penetrating Radar has been selected for inclusion in the payload of the rover for the ESA ExoMars mission (2018) [1]. WISDOM will remotely characterize the shallow subsurface of Mars, providing information essential to understanding the local geological context and the identification of the best locations for obtaining subsurface cores with the rover’s onboard drill.The requirements for the instrument’s performance are driven by the objectives of the mission (a vertical resolution of a few cm and a nominal penetration depth of ~3 m). A series of initial field tests and calibrations have been initiated in simple environments to validate the performance of the instrument. Preliminary results show that WISDOM’s calibrated data should provide reliable contextual and quantitative information about the nature of the Martian shallow subsurface. The instrument’s depth of sounding, vertical resolution and accuracy are consistent with its expected performance.
dc.language.isoen
dc.source.titleEPSC abstracts
dc.title.enInitial Field and Calibration Tests of the WISDOM GPR for the 2018 ExoMars Mission
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.pageEPSC2010-760
bordeaux.volume5
bordeaux.conference.titleEuropean Planetary Science Congress 2010
bordeaux.countryIT
bordeaux.title.proceedingEPSC abstracts
bordeaux.conference.cityRome
bordeaux.peerReviewednon
hal.identifierhal-00594202
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2010-10-24
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00594202v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=EPSC%20abstracts&rft.date=2010-09&rft.volume=5&rft.spage=EPSC2010-760&rft.epage=EPSC2010-760&rft.au=CIARLETTI,%20Val%C3%A9rie&CAIS,%20Ph.&BELARBI,%20Alex&SALIM,%20Z.&PLETTEMEIER,%20Dirk&rft.genre=unknown


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