The shallow subsurface structures of Chang'E-3 landing site based on the wavefield characteristics of LPR Channel-2B data

被引:7
|
作者
Zhao, Na [1 ,2 ]
Zhu, Peimin [2 ]
Yuan, Yuefeng [2 ]
Zhang, Bingzheng [3 ]
Deng, Jian [2 ]
机构
[1] Ningbo Univ Finance & Econ, Coll Informat Engn, Ningbo 315175, Zhejiang, Peoples R China
[2] China Univ Geosci, Inst Geophys & Geomat, Wuhan 430074, Peoples R China
[3] Zhejiang Engn Prospecting Inst, Ningbo 315012, Zhejiang, Peoples R China
关键词
Moon; LPR waveform profile; Lunar shallow subsurface; Rocks; EXPERIMENT ON-BOARD; REGOLITH THICKNESS; RADAR; SERENITATIS; MARIA; LAYER; MOON;
D O I
10.1016/j.asr.2018.05.023
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Lunar Penetrating Radar (LPR) carried by the Yutu rover has imaged the shallow subsurface of the Chang'E-3 (CE-3) landing site at the northern Mare Imbrium. In this paper, by processing LPR Channel-2B data we obtained radar waveform profile. According to the radar wavefield characteristics in the profile, three evident strata can be discovered in the lunar shallow subsurface below the CE-3 site. Most notably, many arc-shaped reflection and/or diffraction events are observed in the profile, especially more in the second layer. In order to find out what caused those arc-shaped events, we conducted radar wavefield numerical simulation. The numerical simulation results reveal that those arc-shaped events are most possibly resulted in by the rocks of different sizes and shapes from the craters surrounding the landing site, especially the C-1 crater. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:884 / 889
页数:6
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