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hal.structure.identifierDépartement Electronique, Optronique et Signal [DEOS]
dc.contributor.authorMURDOCH, Naomi
dc.contributor.authorCHIDE, Baptiste
hal.structure.identifierLos Alamos National Laboratory [LANL]
dc.contributor.authorLASUE, J.
hal.structure.identifierDépartement Electronique, Optronique et Signal [DEOS]
dc.contributor.authorCADU, Alexandre
hal.structure.identifierDépartement Electronique, Optronique et Signal [DEOS]
dc.contributor.authorSOURNAC, Anthony
hal.structure.identifierDépartement Electronique, Optronique et Signal [DEOS]
dc.contributor.authorBASSAS-PORTÚS, Marti
dc.contributor.authorJACOB, X.
hal.structure.identifierThe mars simulation laboratory
dc.contributor.authorMERRISON, J.
dc.contributor.authorIVERSEN, J.J.
hal.structure.identifierLaboratoire de l'Accélérateur Linéaire [LAL]
dc.contributor.authorMORETTO, C.
hal.structure.identifierDepartment of Microbiology
dc.contributor.authorVELASCO, C.
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorPARÈS, L.
dc.contributor.authorHYNES, A.
dc.contributor.authorGODIVER, V.
hal.structure.identifierJohns Hopkins University Applied Physics Laboratory [Laurel, MD] [APL]
dc.contributor.authorLORENZ, R.D.
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorCAIS, Ph.
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorBERNADI, P.
dc.contributor.authorMAURICE, S.
hal.structure.identifierLos Alamos National Laboratory [LANL]
dc.contributor.authorWIENS, R.C.
hal.structure.identifierDépartement Electronique, Optronique et Signal [DEOS]
dc.contributor.authorMIMOUN, David
dc.contributor.authorWIENS, C.
dc.date.issued2019-01
dc.identifier.issn0032-0633
dc.description.abstractEnThe SuperCam instrument suite onboard the Mars 2020 rover will include the Mars Microphone, an experiment designed to record the sounds of the SuperCam laser strikes on rocks and also aeolian noise. In order to record shock waves produced by the laser blasts, the Mars Microphone must be able to record audio signals from 100 Hz to 10 kHz on the surface of Mars, with a sensitivity sufficient to monitor a laser impact at distances up to 4 m. The Aarhus planetary simulator facility has been used to test the Mars 2020 rover microphone in a controlled Martian environment. The end-to-end tests performed in a 6 mbar CO2 atmosphere, with wind, and also with the microphone at −80° C have demonstrated that the SuperCam/Mars Microphone requirements are satisfied. Tests were also performed on Martian soil simulant targets showing that the variation of the acoustic energy of the shock wave depends on the level of compaction of the target.
dc.language.isoen
dc.publisherElsevier
dc.subject.enLaser-induced breakdown spectroscopy
dc.subject.enMars microphone
dc.subject.enMars 2020
dc.subject.enSuperCam
dc.subject.enAtmosphere
dc.subject.enSoil compaction
dc.title.enLaser-induced breakdown spectroscopy acoustic testing of the Mars 2020 microphone
dc.typeArticle de revue
dc.identifier.doi10.1016/j.pss.2018.09.009
dc.subject.halSciences de l'ingénieur [physics]/Optique / photonique
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalPlanetary and Space Science
bordeaux.page260-271
bordeaux.volume165
bordeaux.peerReviewedoui
hal.identifierhal-02000690
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02000690v1
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