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- W4285143649 abstract "Research on lunar basalt thickness and subsurface features is of great significance to conclude the magma evolution history and explore the thermal evolution process of the Moon. The mission of Lunar Radar Sounder (LRS) made subsurface detection within all major lunar maria. Nevertheless, determining the actual depth of reflector needs to estimate the dielectric constants of the uppermost basalt layer. In this letter, we use Maxwell-Garnett theory to determine the unique dielectric constant values of the fifth oldest unit in Mare Humorum(unit H5) and use the two-layer model to calculate the basalt layer thickness. The result shows that the thickness of basalt in the upper layer of unit H5 is 180m and 120m at the border between unit H5 and H7. It points out that the basalt in adjacent units may intrude below the boundary of unit H5" @default.
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- W4285143649 date "2022-01-01" @default.
- W4285143649 modified "2023-10-01" @default.
- W4285143649 title "Estimation of the Thickness of the Lunar Uppermost Basalt Layer Based on Lunar Radar Sounder Observations" @default.
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- W4285143649 doi "https://doi.org/10.1109/jstars.2022.3173790" @default.
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