Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data

Data of fully polarimetric synthetic aperture radar onboard Chandrayaan-2 make it feasible to analyze the geometric and physical properties of the lunar soil layer. A specific mission of Chandrayaan-2 is to investigate if there is water–ice in the regolith of the permanently shadowed regi...

Full description

Bibliographic Details
Main Authors: Niutao Liu, Feng Xu, Ya-Qiu Jin
Format: Article
Language:English
Published: IEEE 2022-01-01
Series:IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
Subjects:
Online Access:https://ieeexplore.ieee.org/document/9878095/
_version_ 1828147878718078976
author Niutao Liu
Feng Xu
Ya-Qiu Jin
author_facet Niutao Liu
Feng Xu
Ya-Qiu Jin
author_sort Niutao Liu
collection DOAJ
description Data of fully polarimetric synthetic aperture radar onboard Chandrayaan-2 make it feasible to analyze the geometric and physical properties of the lunar soil layer. A specific mission of Chandrayaan-2 is to investigate if there is water&#x2013;ice in the regolith of the permanently shadowed region (PSR). Volatile substances are likely to accumulate in the ancient regolith media. Volumetric scattering of the regolith media might indicate specific characteristics of the regolith. Scattering from surface, rocks should be excluded. Such flat regions are difficult to identify in the digital elevation model. In this article, Chandrayaan-2 full-pol data at L-band are used for this purpose. The co-pol and cross-pol scattering coefficients and decomposition parameters, such as <italic>H</italic>, <inline-formula><tex-math notation="LaTeX">$\alpha $</tex-math></inline-formula>, degree of polarization, and circular polarization ratio of lunar surface, are studied. High-order scattering from rough surface is numerically simulated and analyzed by the bidirectional analytical ray-tracing code. It is found that rocky rough surface causes high co-pol scatterings. High-order scatterings of the rough surface and volumetric scatterers can enhance cross-pol scattering. Criteria are proposed to select volume scatterings at flat regions at Mare Serenitatis and a PSR crater. Regions with weak co-pol backscattering in a PSR crater at 85.9&#x00B0;N, 111.7&#x00B0;E are classified as flat surface. It is found that a flat region with weak co-pol and high cross-pol terms appears different from surrounding regions. The enhanced cross-pol is likely to be caused by volumetric inhomogeneity in the regolith. This unusual region shows its inhomogeneous soil layer and deserves further study.
first_indexed 2024-04-11T21:06:48Z
format Article
id doaj.art-41cf07e8eb46498498f29fd7a2d8b35e
institution Directory Open Access Journal
issn 2151-1535
language English
last_indexed 2024-04-11T21:06:48Z
publishDate 2022-01-01
publisher IEEE
record_format Article
series IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
spelling doaj.art-41cf07e8eb46498498f29fd7a2d8b35e2022-12-22T04:03:15ZengIEEEIEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing2151-15352022-01-01157657766410.1109/JSTARS.2022.32045349878095Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR DataNiutao Liu0https://orcid.org/0000-0002-2015-7406Feng Xu1https://orcid.org/0000-0002-7015-1467Ya-Qiu Jin2https://orcid.org/0000-0001-6666-9151Key Laboratory of Information Science of Electromagnetic Waves (MoE), Fudan University, Shanghai, ChinaKey Laboratory of Information Science of Electromagnetic Waves (MoE), Fudan University, Shanghai, ChinaKey Laboratory of Information Science of Electromagnetic Waves (MoE), Fudan University, Shanghai, ChinaData of fully polarimetric synthetic aperture radar onboard Chandrayaan-2 make it feasible to analyze the geometric and physical properties of the lunar soil layer. A specific mission of Chandrayaan-2 is to investigate if there is water&#x2013;ice in the regolith of the permanently shadowed region (PSR). Volatile substances are likely to accumulate in the ancient regolith media. Volumetric scattering of the regolith media might indicate specific characteristics of the regolith. Scattering from surface, rocks should be excluded. Such flat regions are difficult to identify in the digital elevation model. In this article, Chandrayaan-2 full-pol data at L-band are used for this purpose. The co-pol and cross-pol scattering coefficients and decomposition parameters, such as <italic>H</italic>, <inline-formula><tex-math notation="LaTeX">$\alpha $</tex-math></inline-formula>, degree of polarization, and circular polarization ratio of lunar surface, are studied. High-order scattering from rough surface is numerically simulated and analyzed by the bidirectional analytical ray-tracing code. It is found that rocky rough surface causes high co-pol scatterings. High-order scatterings of the rough surface and volumetric scatterers can enhance cross-pol scattering. Criteria are proposed to select volume scatterings at flat regions at Mare Serenitatis and a PSR crater. Regions with weak co-pol backscattering in a PSR crater at 85.9&#x00B0;N, 111.7&#x00B0;E are classified as flat surface. It is found that a flat region with weak co-pol and high cross-pol terms appears different from surrounding regions. The enhanced cross-pol is likely to be caused by volumetric inhomogeneity in the regolith. This unusual region shows its inhomogeneous soil layer and deserves further study.https://ieeexplore.ieee.org/document/9878095/Fully polarimetric (full-pol) synthetic aperture radarpermanently shadowed region (PSR)regolith mediasurface and volume scattering
spellingShingle Niutao Liu
Feng Xu
Ya-Qiu Jin
Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing
Fully polarimetric (full-pol) synthetic aperture radar
permanently shadowed region (PSR)
regolith media
surface and volume scattering
title Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
title_full Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
title_fullStr Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
title_full_unstemmed Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
title_short Recognition of Volumetric Scattering of Lunar Regolith Media in the PSR via Fully Polarimetric SAR Data
title_sort recognition of volumetric scattering of lunar regolith media in the psr via fully polarimetric sar data
topic Fully polarimetric (full-pol) synthetic aperture radar
permanently shadowed region (PSR)
regolith media
surface and volume scattering
url https://ieeexplore.ieee.org/document/9878095/
work_keys_str_mv AT niutaoliu recognitionofvolumetricscatteringoflunarregolithmediainthepsrviafullypolarimetricsardata
AT fengxu recognitionofvolumetricscatteringoflunarregolithmediainthepsrviafullypolarimetricsardata
AT yaqiujin recognitionofvolumetricscatteringoflunarregolithmediainthepsrviafullypolarimetricsardata