Estimation of lunar surface dielectric constant using MiniRF SAR data
Nidhi Verma, Pooja Mishra, Neetesh Purohit

TL;DR
This paper introduces a novel SAR-based model to estimate the lunar surface's dielectric constant, leveraging MiniRF data and coherency matrices, avoiding parallax errors and prior material knowledge.
Contribution
The paper presents a new method to estimate lunar surface dielectric constant using SAR data and coherency matrices, eliminating the need for prior surface composition information.
Findings
Estimates are comparable with previous methods.
The model avoids parallax errors in dielectric estimation.
Applicable to other celestial bodies like Mars.
Abstract
A new model has been developed to estimate the dielectric constant of the lunar surface using Synthetic Aperture Radar (SAR) data. Continuous investigation on the dielectric constant of the lunar surface is a high priority task due to future lunar mission's goals and possible exploration of human outposts. For this purpose, derived anisotropy and backscattering coefficients of SAR images are used. The SAR images are obtained from Miniature Radio Frequency (MiniRF) radar onboard Lunar Reconnaissance Orbiter (LRO). These images are available in the form of Stokes parameters, which are used to derive the coherency matrix. The derived coherency matrix is further represented in terms of particle anisotropy. This coherency matrix's elements compared with Cloud's coherency matrix, which results in the new relationship between particle anisotropy and coherency matrix elements (backscattering…
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Taxonomy
TopicsPlanetary Science and Exploration · Soil Moisture and Remote Sensing · Scientific Research and Discoveries
