Analysis of the Martian subsurface from the observation of the Rover Subsurface Penetrating Radar (RoSPR) onboard Tianwen-

IntroductionChinasfirst Mars exploration mission, Tianwen-1, was successfully launched on 23rd July 2020. The mission included an orbiter, a lander, and the Zhurong rover.Zhuronglanded on Marsin the southern part of Utopia Planitia (109.925E, 25.066N)on 15th May 2021 andthen conducted unprecedented in-situ observations with several instruments, including a ground-penetrating radar (GPR)called Rover Subsurface Penetrating Radar (RoSPR) (Liu et al., 2023). The radar (Fig. 1) aimed at probing the subsurfaceat the Zhurong landing site and searching for buried water ice. Utopia Planitia is well known for showing different ice-related landforms (Sjourn et al., 2019). To achieve this goal, RoSPRwas equippedwith two channels: a high-frequency channel providing high-resolution (5 cm, when permittivity is 3) full-polarization radargramof the shallow subsurface (first 10 meters)and a low-frequency channel capable of penetrating the Martian subsurface down to a depth of ~100 meters with a 1-meter vertical resolution.In-situ GPR observation can reveal the structure and permittivity distribution along the cross-section drawn by theroverstraverse. The subsurface structureisinterpretedfrom the radar profile,whichintuitively shows the location of subsurface reflectors, such as buried craters, aeolian deposits, and icy beds. Permittivity is a complex parameter describing the electromagnetic properties of materials. It mainly depends on composition and porosity. Its real part and imaginary part respectively control the wave velocity and signal attenuation rate in the Martian subsurface.Data and MethodsWe use all the 5893 dual-channel radar traces collected by RoSPR during the 325 solar days on Mars. The traverse of the radar is shown in Fig. 2. Those observations covered ~1840 meters with an elevation variation of ~10 meters from the Zhurong landing site southward. Data from ground experiments of RoSPR on glaciers on Earth are also used to provide a comparison between the RoSPR data acquired on different sites.In addition to conventional RoSPR data treatments, advanced data processing methodsare deployedto better reveal subsurface structure.In particular, we adopt a background matrix method (Rashed and Harbi, 2014)whichstatistically removes the systematic clutters.Blind deconvolution methods of the radar B-scanare also tested to address and eliminate theringing effect that commonly exists.In addition, the bandwidth extrapolation technique designed for range resolution enhancement (Oudart et al., 2021) will be applied to further provide clarity among different buried objects.Preliminary Results and Ongoing WorkTo estimate the Martian soil permittivity, we applied a hyperbola fitting method which accounts for theantennasheight (Wang et al. 2021, Oudart et al., 2022), and a centroid frequency shift method (Quan et Harris, 1997)which uses the real-time spectrum of dual-channel RoSPR data to maximize the accuracy (Fig. 3).Loss tangent estimation also reveals upper bounds of ~0.008 and ~0.022 for the first 10metersand 40 meters, respectively.The low-frequency B-scan,as shown in Fig. 4, reveals buried structures and indistinct reflectors in deeper regions.The variation of the B-scan and loss tangent value along the depth implies varied composition at the landing site. The ongoing work focuses on refining data processing techniques to improve the clarity of subsurface imaging and provide robust interpretation and geological analysis.References1 S. Liu et al., Data Pre-Processing and Signal Analysis of Tianwen-1 Rover Penetrating Radar, Remote Sensing, vol. 15, no. 4, p. 966, Feb. 2023, doi: 10.3390/rs15040966.2 N. Oudart et al., Range resolution enhancement of WISDOM/ExoMars radar soundings by the Bandwidth Extrapolation technique: Validation and application to field campaign measurements, Planetary and Space Science, vol. 197, p. 105173, Mar. 2021, doi: 10.1016/j.pss.2021.105173.3 N. Oudart et al., Retrieval of the ground dielectric permittivity by planetary GPR accommodated on a rover: Application to the estimation of the reflectors depth by the WISDOM/ExoMars radar, Planetary and Space Science, vol. 224, p. 105606, Dec. 2022, doi: 10.1016/j.pss.2022.105606.4 Y. Quan and J. M. Harris, Seismic attenuation tomography using the frequency shift method, GEOPHYSICS, vol. 62, no. 3, pp. 895905, May 1997, doi: 10.1190/1.1444197.5 M. Rashed and H. Harbi, Background matrix subtraction (BMS): A novel background removal algorithm for GPR data, Journal of Applied Geophysics, vol. 106, pp. 154163, Jul. 2014, doi: 10.1016/j.jappgeo.2014.04.022.6A. Sjourn et al., Grid Mapping the Northern Plains of Mars: Using Morphotype and Distribution of Ice-Related Landforms to Understand Multiple Ice-Rich Deposits in Utopia Planitia, Journal of Geophysical Research: Planets, vol. 124, no. 2, pp. 483503, Feb. 2019, doi: 10.1029/2018JE005665.7 R. Wang et al., A Novel Approach for Permittivity Estimation of Lunar Regolith Using the Lunar Penetrating Radar Onboard ChangE-4 Rover, Remote Sensing, vol. 13, no. 18, p. 3679, Sep. 2021, doi: 10.3390/rs13183679.Fig. 1 The dual-channel RoSPR onboard Zhurong rover. The low-frequency monopole antennas are mounted in the front of the rover. The high-frequency Vivaldi antennas are tied to the rovers body.Fig. 2 The traverse of Zhurong roverand the elevation at the landing site.Fig. 3 The loss tangent estimation via RoSPR low-frequency data. The figure demonstrates the centroid frequency decay versus time delay relationship, calculated from 160 traces of Low-frequency channel data ranging from ~300 to ~550 ns.Fig. 4 RoSPR low-frequency B-scan section from sol 112 to sol 288.