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Results from the First Field Tests of the WISDOM GPR (2018 ExoMars Mission)

hal.structure.identifierESTER - LATMOS
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorCIARLETTI, Valérie
hal.structure.identifierLunar and Planetary Institute [Houston] [LPI]
dc.contributor.authorCLIFFORD, S.
hal.structure.identifierLaboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS]
dc.contributor.authorVIEAU, André-Jean
hal.structure.identifierLaboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS]
dc.contributor.authorLUSTREMENT, Benjamin
hal.structure.identifierLaboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS]
dc.contributor.authorHASSEN-KHODJA, Rafik
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]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCAIS, Ph.
dc.date.issued2011
dc.date.conference2011-03-07
dc.description.abstractEnIntroduction: The WISDOM (Water Ice Subsur- face Deposit Observation on Mars) Ground Penetrating Radar (GPR) is one of the instruments that have been selected as part of the Pasteur payload of ESA’s 2018 ExoMars Rover mission[1]. The Pasteur payload actu- ally consists of two different sets of instruments: the Panoramic Instruments, which include a wide angle camera and the WISDOM radar, that will be used to perform large-scale scientific investigations of the landing site and the Analytical Laboratory Instruments that will analyze the core samples obtained by the sub- surface drill. WISDOM will help identify the location of sedimentary layers, where organic molecules are the most likely to be found and well-preserved. WISDOM has been designed to investigate the near subsurface environment down to a depth of ~2-3 m with a vertical resolution of a few centimeters [2]. WISDOM is a step frequency radar operating over a wide frequency band between 0.5 and 3 GHz. Particular attention was paid to the design of the antenna system, which needs to be able to conduct polarimetric measurements over the whole bandwidth without significant distortion [3].
dc.language.isoen
dc.title.enResults from the First Field Tests of the WISDOM GPR (2018 ExoMars Mission)
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page2613.pdf
bordeaux.volume42
bordeaux.countryUS
bordeaux.conference.cityThe Woodlands - Texas
bordeaux.peerReviewedoui
hal.identifierhal-00619293
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2011-03-11
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00619293v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2011&rft.volume=42&rft.spage=2613.pdf&rft.epage=2613.pdf&rft.au=CIARLETTI,%20Val%C3%A9rie&CLIFFORD,%20S.&VIEAU,%20Andr%C3%A9-Jean&LUSTREMENT,%20Benjamin&HASSEN-KHODJA,%20Rafik&rft.genre=unknown


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