RIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface
dc.contributor.author | Casademont, T.M. | |
dc.contributor.author | Eide, S. | |
dc.contributor.author | Shoemaker, E.S. | |
dc.contributor.author | Liu, Y. | |
dc.contributor.author | Nunes, D.C. | |
dc.contributor.author | Russell, P. | |
dc.contributor.author | Dypvik, H. | |
dc.contributor.author | Amundsen, H.E.F. | |
dc.contributor.author | Berger, T. | |
dc.contributor.author | Hamran, S.-E. | |
dc.date.accessioned | 2024-08-03T03:13:26Z | |
dc.date.available | 2024-08-03T03:13:26Z | |
dc.date.issued | 2023-03-21 | |
dc.identifier.citation | Casademont, 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.issn | 2169-9097 | |
dc.identifier.doi | 10.1029/2022JE007598 | |
dc.identifier.uri | http://hdl.handle.net/10150/673008 | |
dc.description.abstract | The 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.iso | en | |
dc.publisher | John 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.uri | https://creativecommons.org/licenses/by-nc/4.0/ | |
dc.subject | bulk rock density | |
dc.subject | dielectric permittivity | |
dc.subject | FMCW radar | |
dc.subject | GPR | |
dc.subject | Mars | |
dc.subject | shallow subsurface | |
dc.title | RIMFAX Ground Penetrating Radar Reveals Dielectric Permittivity and Rock Density of Shallow Martian Subsurface | |
dc.type | Article | |
dc.type | text | |
dc.contributor.department | Lunar and Planetary Laboratory, University of Arizona | |
dc.identifier.journal | Journal of Geophysical Research: Planets | |
dc.description.note | Open access article | |
dc.description.collectioninformation | This 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.version | Final Published Version | |
dc.source.journaltitle | Journal of Geophysical Research: Planets | |
refterms.dateFOA | 2024-08-03T03:13:26Z |