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

IF 4 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Haoqiu Zhou, Xuan Feng, Zejun Dong, Wenjing Liang, Cai Liu
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引用次数: 0

摘要

本文报道了中国天文一号(TW-1)任务的朱荣火星车采集的全极化火星探测器穿透雷达(RoPeR)数据的结果。将改进的Freeman分解方法应用于RoPeR数据的分析。通过分离不同的极化散射分量,确定了以前被不同散射信号遮挡的难以察觉的界面。此外,通过相关分析,识别了地面与车体之间的双时间反射信号产生的信号中存在伪影。因此,揭示了3米深的火星风化层的双层结构。浅层和深层分别表现出较强的体积散射能力和双弹跳散射能力,说明它们的结构存在差异。数值试验结果表明,火星表面的高强度信号是由稠密的岩石和起伏的地形产生的,而风化层中强烈的体积散射分量是由砾石堆积产生的。此外,在风化层中还发现了一种表面光滑、切线损失大的孤立致密岩石,可解释为观察到的由水活动形成的板状硬壳。结果表明,TW-1着陆点的火星风化结构是高度不均匀的,水活动可能对其有重要贡献。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Dense Rocks With Smooth Surfaces in Martian Regolith Revealed by Polarimetric Analysis of GPR Data: A Case at Tianwen-1 Landing Site, Mars

Dense Rocks With Smooth Surfaces in Martian Regolith Revealed by Polarimetric Analysis of GPR Data: A Case at Tianwen-1 Landing Site, Mars

Dense Rocks With Smooth Surfaces in Martian Regolith Revealed by Polarimetric Analysis of GPR Data: A Case at Tianwen-1 Landing Site, Mars

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.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
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.
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