Haoqiu Zhou, Xuan Feng, Zejun Dong, Wenjing Liang, Cai Liu
{"title":"GPR数据偏振分析揭示火星风化层致密光滑岩石——以火星“天文一号”着陆点为例","authors":"Haoqiu Zhou, Xuan Feng, Zejun Dong, Wenjing Liang, Cai Liu","doi":"10.1029/2024JE008748","DOIUrl":null,"url":null,"abstract":"<p>This article reports the results of full-polarimetric Mars Rover Penetrating Radar (RoPeR) data acquired by the Zhurong rover of China's Tianwen-1 (TW-1) mission. A modified Freeman decomposition method is applied to the analysis of RoPeR data. By separating different polarimetric scattering components, an imperceptible interface previously obscured by different scattering signals is determined. Besides, an artifact in the signals generated by the double-time reflected signals between the ground and the rover body is identified via correlation analysis. Consequently, a double-layered structure of the Martian regolith to a depth of 3 m is revealed. The shallow layer and deep layer show strong volume scattering power and double-bounce scattering power, respectively, indicating their differences in structure. According to the results of the numerical test, the high-strength signals from the Martian surface are generated by the dense rocks and the undulating terrain, whereas the strong volume scattering components in the regolith are generated by piles of gravel. Besides, a kind of isolated dense rocks with a smooth surface and high loss tangents is identified in the regolith, which is interpreted as the platy duricrusts observed to be formed by aqueous activities. The results demonstrate that the Martian regolith structure at the TW-1 landing site is highly heterogeneous and that aqueous activities may have contributed significantly to it.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"130 7","pages":""},"PeriodicalIF":4.0000,"publicationDate":"2025-07-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Dense Rocks With Smooth Surfaces in Martian Regolith Revealed by Polarimetric Analysis of GPR Data: A Case at Tianwen-1 Landing Site, Mars\",\"authors\":\"Haoqiu Zhou, Xuan Feng, Zejun Dong, Wenjing Liang, Cai Liu\",\"doi\":\"10.1029/2024JE008748\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>This article reports the results of full-polarimetric Mars Rover Penetrating Radar (RoPeR) data acquired by the Zhurong rover of China's Tianwen-1 (TW-1) mission. A modified Freeman decomposition method is applied to the analysis of RoPeR data. By separating different polarimetric scattering components, an imperceptible interface previously obscured by different scattering signals is determined. Besides, an artifact in the signals generated by the double-time reflected signals between the ground and the rover body is identified via correlation analysis. Consequently, a double-layered structure of the Martian regolith to a depth of 3 m is revealed. The shallow layer and deep layer show strong volume scattering power and double-bounce scattering power, respectively, indicating their differences in structure. According to the results of the numerical test, the high-strength signals from the Martian surface are generated by the dense rocks and the undulating terrain, whereas the strong volume scattering components in the regolith are generated by piles of gravel. Besides, a kind of isolated dense rocks with a smooth surface and high loss tangents is identified in the regolith, which is interpreted as the platy duricrusts observed to be formed by aqueous activities. The results demonstrate that the Martian regolith structure at the TW-1 landing site is highly heterogeneous and that aqueous activities may have contributed significantly to it.</p>\",\"PeriodicalId\":16101,\"journal\":{\"name\":\"Journal of Geophysical Research: Planets\",\"volume\":\"130 7\",\"pages\":\"\"},\"PeriodicalIF\":4.0000,\"publicationDate\":\"2025-07-14\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Geophysical Research: Planets\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008748\",\"RegionNum\":1,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Planets","FirstCategoryId":"89","ListUrlMain":"https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2024JE008748","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
Dense Rocks With Smooth Surfaces in Martian Regolith Revealed by Polarimetric Analysis of GPR Data: A Case at Tianwen-1 Landing Site, Mars
This article reports the results of full-polarimetric Mars Rover Penetrating Radar (RoPeR) data acquired by the Zhurong rover of China's Tianwen-1 (TW-1) mission. A modified Freeman decomposition method is applied to the analysis of RoPeR data. By separating different polarimetric scattering components, an imperceptible interface previously obscured by different scattering signals is determined. Besides, an artifact in the signals generated by the double-time reflected signals between the ground and the rover body is identified via correlation analysis. Consequently, a double-layered structure of the Martian regolith to a depth of 3 m is revealed. The shallow layer and deep layer show strong volume scattering power and double-bounce scattering power, respectively, indicating their differences in structure. According to the results of the numerical test, the high-strength signals from the Martian surface are generated by the dense rocks and the undulating terrain, whereas the strong volume scattering components in the regolith are generated by piles of gravel. Besides, a kind of isolated dense rocks with a smooth surface and high loss tangents is identified in the regolith, which is interpreted as the platy duricrusts observed to be formed by aqueous activities. The results demonstrate that the Martian regolith structure at the TW-1 landing site is highly heterogeneous and that aqueous activities may have contributed significantly to it.
期刊介绍:
The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.