4.7 Article

Numerical Verification of Full Waveform Inversion for the Chang'E-5 Lunar Regolith Penetrating Array Radar

出版社

IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TGRS.2021.3098104

关键词

Moon; Permittivity; TV; Radar imaging; Mathematical model; Conductivity; Radar antennas; Chang'E-5 (CE-5); full waveform inversion (FWI); lunar regolith penetrating radar; numerical test; total variation (TV)

资金

  1. Natural Science Foundation of China [41874134, 41874120]
  2. Youth Talent Project of China Association for Science and Technology [2019QNRC001]
  3. Technology Development Program of Jilin Province [20200201216JC]

向作者/读者索取更多资源

The LRPR carried by CE-5 has explored the lunar subsurface structure and guided sampling procedures, and a multiscale FWI method with TV regularization has been used to evaluate its performance. The strategy has successfully reduced signal scattering and provided reliable imaging for sampling, demonstrating improved inversion accuracy.
The lunar regolith penetrating array radar (LRPR) carried by Chang'E-5 (CE-5) has explored the subsurface regolith structure of the moon and guided the drill sampling procedures. To evaluate LRPR performance in subsurface imaging and physical-parameter estimation, we apply multiscale full-waveform inversion (FWI) with total variation (TV) regularization to the synthetic CE-5 LRPR data. The time-domain multiscale inversion strategy gives a low-frequency update for the deep region and increases the frequency range for updating the shallow area. The TV regularization reduces the image noise and improves the inversion accuracy of local structures. To mimic the actual scenario, we use an LRPR source wavelet obtained from the LRPR instrument prototype for our FWI test. The LRPR source wavelets include the effect of the antenna radiation patterns and signal scattering from the metallic lander. We test the proposed FWI scheme on two heterogeneous models of the lunar regolith and demonstrate that the scheme effectively reduces the signal scattering from the metallic lander and provides a reliable way to image the lunar regolith structures. These images can be used to estimate the regolith physical parameters.

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