A story of regolith told by Lunar Penetrating Radar

被引:28
作者
Zhang Ling [1 ,2 ]
Zeng Zhaofa [1 ,2 ]
Jing Li [1 ,2 ]
Huang Ling [3 ]
Huo Zhijun [1 ,2 ]
Zhang Jianmin [1 ,2 ]
Huai Nan [1 ,2 ]
机构
[1] Jilin Univ, Coll Geoexplorat Sci & Technol, Changchun 130026, Jilin, Peoples R China
[2] Minist Land & Resources, Key Lab Appl Geophys, Changchun 130026, Jilin, Peoples R China
[3] Chinese Acad Sci, Inst Elect, Beijing 100190, Peoples R China
关键词
Lunar Penetrating Radar; Lunar exploration; Regolith; Data processing; Forward modeling; MICROWAVE BRIGHTNESS TEMPERATURE; DIELECTRIC-PROPERTIES; THICKNESS; LAYER; SURFACE; WAVES;
D O I
10.1016/j.icarus.2018.11.006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Knowledge of the lunar regolith not only provides important information about lunar geology, but is also critical to quantifying potential resources for lunar exploration and engineering for human outposts. The Lunar Penetrating Radar (LPR) onboard China's Chang'E-3 (CE-3) provides a unique opportunity for mapping the subsurface structure and the near-surface stratigraphic structure of the regolith. A radar image with high resolution can be produced using a data processing pipeline. The contact interface of the regolith and the basement rock is explored according to forward simulation results. F-K (Frequency-wavenumber) filtering that highlights the contact surface of the regolith and the basement rock is carried out. The energy distribution of the LPR data helps to stratify the lunar regolith. Finally, by combining this with the history of the Moon, regional geology, and particularly the LPR data, we deduce the evolution of the regolith on the CE-3 landing site.
引用
收藏
页码:148 / 160
页数:13
相关论文
共 45 条
[21]  
Kroupenio N.N., 1973, COSPAR SPACE RES, VXIII, P969
[22]   Structural analysis of lunar subsurface with Chang'E-3 lunar penetrating radar [J].
Lai, Jialong ;
Xu, Yi ;
Zhang, Xiaoping ;
Tang, Zesheng .
PLANETARY AND SPACE SCIENCE, 2016, 120 :96-102
[23]   A Study on Lunar Regolith Quantitative Random Model and Lunar Penetrating Radar Parameter Inversion [J].
Li, Jing ;
Zeng, Zhaofa ;
Liu, Cai ;
Huai, Nan ;
Wang, Kun .
IEEE GEOSCIENCE AND REMOTE SENSING LETTERS, 2017, 14 (11) :1953-1957
[24]  
Muhleman D. O., 1969, SURVEYORPROGRAMRESUL, V184, P203
[25]   SHALLOW LUNAR STRUCTURE DETERMINED FROM PASSIVE SEISMIC EXPERIMENT [J].
NAKAMURA, Y ;
DORMAN, J ;
DUENNEBIER, F ;
LAMMLEIN, D ;
LATHAM, G .
MOON, 1975, 13 (1-3) :57-66
[26]   DIELECTRIC PROPERTIES OF FIRST 100 METERS OF MOON [J].
OLHOEFT, GR ;
STRANGWAY, DW .
EARTH AND PLANETARY SCIENCE LETTERS, 1975, 24 (03) :394-404
[27]   THICKNESS DETERMINATIONS OF LUNAR SURFACE LAYER FROM LUNAR IMPACT CRATERS [J].
QUAIDE, WL ;
OBERBECK, VR .
JOURNAL OF GEOPHYSICAL RESEARCH, 1968, 73 (16) :5247-+
[28]   Total transmission of electromagnetic waves at interfaces associated with an indefinite medium [J].
Shen, Nian-Hai ;
Wang, Qin ;
Chen, Jing ;
Fan, Ya-Xian ;
Ding, Jianping ;
Wang, Hui-Tian ;
Tian, Yongjun .
JOURNAL OF THE OPTICAL SOCIETY OF AMERICA B-OPTICAL PHYSICS, 2006, 23 (05) :904-912
[29]   Regolith layer thickness mapping of the moon by radar and optical data [J].
Shkuratov, YG ;
Bondarenko, NV .
ICARUS, 2001, 149 (02) :329-338
[30]   MIGRATION BY FOURIER-TRANSFORM [J].
STOLT, RH .
GEOPHYSICS, 1978, 43 (01) :23-48