基于自适应f-x E MD的LPR CH-2数据月球风化层结构分析:自适应f-x EMD处理的LPR数据

IF 1.6 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Advances in Astronomy Pub Date : 2019-07-01 DOI:10.1155/2019/1528410
Bin Hu, Deli Wang, Ling Zhang, Z. Zeng
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引用次数: 2

摘要

探月雷达(LPR)是中国嫦娥三号(CE-3)在月球表面以下100米范围内成像的重要科学有效载荷之一。所获得的LPR数据对月球地质结构的研究具有重要意义。根据月球风化层的沉积机制,风化层包含许多大小不等的岩石。这些局部异常在LPR数据中以衍射的形式出现,这降低了数据质量,并限制了月球风化层的结构分析。根据岩石引起衍射的运动学特征,将这些问题转化为陡倾角递减问题。为了达到这一目标,我们首先采用了数据预处理工作流程来提高雷达图像的质量。然后,提出了一种基于自适应f-x经验模式分解(EMD)的倾角滤波器来提取风化层中的岩石,相应的去除的IMF图指示了岩石的富集程度,并突出了风化层-基底界面。模拟和LPR CH-2数据都表现出了良好的性能。最后,根据处理结果,我们定位了每个岩石的位置,并突出了风化层与基岩的接触界面。
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Structural Analysis of Lunar Regolith from LPR CH-2 Data Based on Adaptive f-x E MD: LPR Data Processed by Adaptive f-x EMD
The Lunar Penetrating Radar (LPR) is one of the important scientific payloads in China’s Chang’E-3 (CE-3) to image within 100 m below the lunar surface. The acquired LPR data is significant for the research of lunar geological structure. Based on the sedimentary mechanism of lunar regolith, the regolith contains many rocks with different sizes. These local anomalies appear as diffraction in LPR data, which reduces the data quality and limits the structural analysis of lunar regolith. According to the kinematics characteristics of rock caused diffraction, we transform these problems to a problem of steep dip decreasing. To reach this goal, we adopt a data preprocessing workflow to improve the quality of the radar image, firstly. Then, a dip filter based on adaptive f-x empirical mode decomposition (EMD) is proposed to extract the rocks in the regolith and the corresponding removed IMF map indicates the degree of rock enrichment and highlights regolith-basement interface. Both simulation and LPR CH-2 data present a great performance. Finally, according to the processed result, we locate the position of each rock and highlight the contact interface of regolith and the basement rock.
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来源期刊
Advances in Astronomy
Advances in Astronomy ASTRONOMY & ASTROPHYSICS-
CiteScore
2.70
自引率
7.10%
发文量
10
审稿时长
22 weeks
期刊介绍: Advances in Astronomy publishes articles in all areas of astronomy, astrophysics, and cosmology. The journal accepts both observational and theoretical investigations into celestial objects and the wider universe, as well as the reports of new methods and instrumentation for their study.
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