Mostrar el registro sencillo del ítem

WISDOM GPR designed for shallow and high-resolution sounding of the martian subsurface

hal.structure.identifierESTER - LATMOS
dc.contributor.authorCIARLETTI, Valérie
hal.structure.identifierLaboratoire Atmosphères, Milieux, Observations Spatiales [LATMOS]
dc.contributor.authorCORBEL, Charlotte
hal.structure.identifierTechnische Universität Dresden = Dresden University of Technology [TU Dresden]
dc.contributor.authorPLETTEMEIER, Dirk
hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorCAIS, Ph.
hal.structure.identifierLunar and Planetary Institute [Houston] [LPI]
dc.contributor.authorCLIFFORD, S. M.
hal.structure.identifierUniversity of Oslo [UiO]
dc.contributor.authorHAMRAN, Svein-Erik
dc.date.issued2011
dc.identifier.issn0018-9219
dc.description.abstractEnThe Water Ice Subsurface Deposit Observation on Mars (WISDOM) Ground Penetrating Radar (GPR) is one of the instruments that have been selected as part of the Pasteur payload of the European Space Agency's (ESA's) 2018 ExoMars Rover mission. The main scientific objectives of the mission are to search for evidence of past and present life and to characterize the nature of the shallow subsurface. The Rover is equipped with a drill that can sample the subsurface down to a depth of approximately 2 m. The WISDOM GPR is the only instrumentation capable of obtaining information about the nature of the subsurface along the Rover path before drilling. WISDOM has been designed to explore the first $sim$3 m of the subsurface with a vertical resolution of a few centimeters. The paper presents a description of the WISDOM instrument with a particular emphasis on the electronic architecture and antenna design that have been chosen to meet the challenging technical objectives. Some preliminary measurements obtained with the prototype are given to illustrate the instrument's potential performance.
dc.language.isoen
dc.publisherInstitute of Electrical and Electronics Engineers
dc.title.enWISDOM GPR designed for shallow and high-resolution sounding of the martian subsurface
dc.typeArticle de revue
dc.identifier.doi10.1109/JPROC.2010.2100790
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.journalProceedings of the IEEE
bordeaux.page824-836
bordeaux.volume99
bordeaux.issue5
bordeaux.peerReviewedoui
hal.identifierhal-00566259
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00566259v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Proceedings%20of%20the%20IEEE&rft.date=2011&rft.volume=99&rft.issue=5&rft.spage=824-836&rft.epage=824-836&rft.eissn=0018-9219&rft.issn=0018-9219&rft.au=CIARLETTI,%20Val%C3%A9rie&CORBEL,%20Charlotte&PLETTEMEIER,%20Dirk&CAIS,%20Ph.&CLIFFORD,%20S.%20M.&rft.genre=article


Archivos en el ítem

ArchivosTamañoFormatoVer

No hay archivos asociados a este ítem.

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo del ítem