探地雷达探测月球次表层的灵敏度分析

Pranay Putrevu, D. Pandey, Tathagata Chakraborty
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摘要

探地雷达(GPR)是表征亚表层介质特性的重要工具。探地雷达可以有效地探测和区分具有显著介电对比度的亚表层。然而,在行星地下,由于缺乏水,各层之间的介电对比度非常低,使得探测极具挑战性。在本研究中,进行了数值模拟来确定低介电对比度情况下的探地雷达信号电平。我们的研究结果表明,在这种情况下,探地雷达仪器的本底噪声水平应至少低于发射功率110dB才能成功探测。这些结果将成为未来任务中以行星表面和地下研究为目标的GPR系统设计和配置的主要输入。
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GPR Sensitivity Analysis for Detection of Subsurface Layers in Lunar Scenario
Ground Penetrating Radar (GPR) is an important instrument to characterize subsurface layers depending on their dielectric properties. GPR can efficiently detect and differentiate subsurface layers with significant dielectric contrast. However, in planetary subsurface, due to lack of water, dielectric contrast between the layers is very low, making the detection extremely challenging. In the present study, numerical simulations are carried out to determine the GPR signal levels in low dielectric contrast scenarios. Our results reveal that, noise-floor level of the GPR instrument should be at least 110dB below transmit power for successful detection in such cases. These results will be major input for GPR system design and configuration targeting planetary surface and subsurface studies for future missions.
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