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dc.contributor.authorCasademont, Titusen_GB
dc.contributor.authorEide, Sigurden_GB
dc.contributor.authorShoemaker, E.S.en_GB
dc.contributor.authorLiu, Y.en_GB
dc.contributor.authorNunes, D.C.en_GB
dc.contributor.authorRussell, P.en_GB
dc.contributor.authorDypvik, Henningen_GB
dc.contributor.authorAmundsen, Hans E. Fossen_GB
dc.contributor.authorBerger, Toren_GB
dc.contributor.authorHamran, Svein-Eriken_GB
dc.date.accessioned2024-02-22T06:22:47Z
dc.date.accessioned2024-10-01T06:14:05Z
dc.date.available2024-02-22T06:22:47Z
dc.date.available2024-10-01T06:14:05Z
dc.date.issued2023-06-02
dc.identifier.citationCasademont T, Eide, Shoemaker, Liu, Nunes, Russell, Dypvik, Amundsen, Berger T, Hamran. RIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface. Journal of Geophysical Research (JGR): Planets. 2023;128(5)en_GB
dc.identifier.urihttp://hdl.handle.net/20.500.12242/3319
dc.descriptionRIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface. Journal of Geophysical Research (JGR): Planets 2023 ;Volum 128.(5)en_GB
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.en_GB
dc.language.isoenen_GB
dc.subjectRadaren_GB
dc.subjectMarsen_GB
dc.subjectTettheten_GB
dc.titleRIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurfaceen_GB
dc.date.updated2024-02-22T06:22:47Z
dc.identifier.cristinID2156203
dc.identifier.doi10.1029/2022JE007598
dc.relation.projectIDNorges forskningsråd: 309835
dc.source.issn2169-9097
dc.source.issn2169-9100
dc.type.documentJournal article
dc.relation.journalJournal of Geophysical Research (JGR): Planets


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