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dc.contributor.authorCasademont, T.M.
dc.contributor.authorEide, S.
dc.contributor.authorShoemaker, E.S.
dc.contributor.authorLiu, Y.
dc.contributor.authorNunes, D.C.
dc.contributor.authorRussell, P.
dc.contributor.authorDypvik, H.
dc.contributor.authorAmundsen, H.E.F.
dc.contributor.authorBerger, T.
dc.contributor.authorHamran, S.-E.
dc.date.accessioned2024-08-03T03:13:26Z
dc.date.available2024-08-03T03:13:26Z
dc.date.issued2023-03-21
dc.identifier.citationCasademont, T. M., Eide, S., Shoemaker, E. S., Liu, Y., Nunes, D. C., Russell, P., et al. (2023). RIMFAX ground penetrating radar reveals dielectric permittivity and rock density of shallow Martian subsurface. Journal of Geophysical Research: Planets, 128, e2022JE007598. https://doi.org/10.1029/2022JE007598
dc.identifier.issn2169-9097
dc.identifier.doi10.1029/2022JE007598
dc.identifier.urihttp://hdl.handle.net/10150/673008
dc.description.abstractThe Mars 2020 Perseverance Rover is equipped with the RIMFAX ground penetrating radar instrument which has been continuously surveying the shallow subsurface during the rover's journey. Within the first 379 mission days, we identify hyperbolic patterns in the data, which are thought to be caused by objects such as buried boulders or cavities located in the upper 5 m of the subsurface. To obtain the first detailed estimates of radar wave propagation velocity, we match these scatterer-generated patterns with theoretical traveltime hyperbolas, which take into account the refraction at the surface. We employ these estimates to derive the average dielectric permittivity and bulk rock density of the volume above the scatterer source. The parameters compare well with those obtained through orbital radar measurements and those measured by other instruments onboard the Perseverance Rover. Our findings are consistent with a subsurface dominated by solid rock and mafic material. © 2023. The Authors.
dc.language.isoen
dc.publisherJohn Wiley and Sons Inc
dc.rights© 2023 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License.
dc.rights.urihttps://creativecommons.org/licenses/by-nc/4.0/
dc.subjectbulk rock density
dc.subjectdielectric permittivity
dc.subjectFMCW radar
dc.subjectGPR
dc.subjectMars
dc.subjectshallow subsurface
dc.titleRIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface
dc.typeArticle
dc.typetext
dc.contributor.departmentLunar and Planetary Laboratory, University of Arizona
dc.identifier.journalJournal of Geophysical Research: Planets
dc.description.noteOpen access article
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
dc.eprint.versionFinal Published Version
dc.source.journaltitleJournal of Geophysical Research: Planets
refterms.dateFOA2024-08-03T03:13:26Z


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© 2023 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License.
Except where otherwise noted, this item's license is described as © 2023 The Authors. This is an open access article under the terms of the Creative Commons Attribution-NonCommercial License.