Ground experiments of Chang'e-5 lunar regolith penetrating radar

被引:28
|
作者
Xiao, Yuan [1 ,2 ,3 ]
Su, Yan [1 ,2 ]
Dai, Shun [1 ,2 ]
Feng, Jianqing [1 ,2 ]
Xing, Shuguo [1 ,2 ]
Ding, Chunyu [4 ]
Li, Chunlai [1 ,2 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
[2] Chinese Acad Sci, Key Lab Lunar & Deep Space Explorat, Beijing 100012, Peoples R China
[3] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[4] Sun Yat Sen Univ, Sch Atmospher Sci, Zhuhai 519082, Peoples R China
基金
中国国家自然科学基金;
关键词
Chang'e-5 (CE-5); Lunar Regolith Penetrating Radar; Ground experiments; GPR;
D O I
10.1016/j.asr.2019.02.001
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Lunar Regolith Penetrating Radar (LRPR) is an Ultra-Wideband (UWB) array-based Ground penetrating radar (GPR) onboard the lander of Chang'e-5 (CE-5) mission. The primary scientific objectives of the LRPR are to probe the thickness and structure of lunar regolith of the landing site, and support the drilling and sampling process. In order to evaluate the performance of the LRPR, a series of ground experiments are performed using the LRPR prototype mounted on a CE-5 lander model. The performance of the LRPR is evaluated by comparing the experimental data with the simulated data. Data processing and imaging method are verified, and the interferences from the lander and other aspects are analyzed. The results of the ground experiments and simulation demonstrate that the LRPR is able to meet the design requirement of 2-m detection depth. They also indicate that the upper and lower interfaces of the stratified structure in the lunar regolith can be well distinguished by the LRPR when the dielectric constant difference is greater than 0.3, and the imaging effect of the location under the dense antennas is better than that of other positions. However, the identification capability of the LRPR to the independent blocky objects is relatively poor mainly due to the clutters caused by the lander, the sparsity of the antenna elements compared to the size of the basalt block, the limited aperture of the antenna array, and the tail of the transmitted waveform. (C) 2019 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:3404 / 3419
页数:16
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