Antoine Bourget , Parvathy Prem , David Blewett , Michael G. Daly , Isaac B. Smith
{"title":"Optical polarization studies of latex beads in aqueous solution: An analog for radar scattering in icy regolith","authors":"Antoine Bourget , Parvathy Prem , David Blewett , Michael G. Daly , Isaac B. Smith","doi":"10.1016/j.pss.2024.105891","DOIUrl":null,"url":null,"abstract":"<div><p>This study presents low phase angle <span><math><mrow><mn>0</mn><mo>°</mo><mtext>–</mtext><mn>5</mn><mo>°</mo></mrow></math></span> measurements of polarimetric properties of icy planetary regolith analog materials acquired using the custom-built Multi-Axis- Goniometer-Instrument (MAGI). We present same sense <span><math><mrow><mo>(</mo><mi>S</mi><mi>C</mi><mo>)</mo></mrow></math></span>, and opposite sense <span><math><mrow><mo>(</mo><mi>O</mi><mi>C</mi><mo>)</mo></mrow></math></span> backscatter circular polarization coefficients, circular polarization ratio <span><math><mrow><mo>(</mo><mi>C</mi><mi>P</mi><mi>R</mi><mo>)</mo></mrow></math></span>, and degree linear polarization <span><math><mrow><mo>(</mo><mi>D</mi><mi>L</mi><mi>P</mi><mo>)</mo></mrow></math></span> of spherical latex (non-dye) beads of varying sizes and volume concentrations (v/v) in aqueous solutions (<span><math><mrow><mi>λ</mi><mo>=</mo><mn>0</mn><mo>.</mo><mn>8</mn><mspace></mspace><mi>μ</mi><mi>m</mi></mrow></math></span>) in water. We also present measurements of alumina powder in air at <span><math><mrow><mi>λ</mi><mo>=</mo><mn>1</mn><mo>.</mo><mn>064</mn><mspace></mspace><mi>μ</mi><mi>m</mi></mrow></math></span>. Measurements showed that at a low incidence angle <span><math><mrow><mo>(</mo><mi>i</mi><mo>=</mo><mn>0</mn><mo>°</mo><mo>)</mo></mrow></math></span>, backscatter is dominated by surface specular single-bounce scattering, that hides other scattering processes. At high <span><math><mrow><mo>(</mo><mi>i</mi><mo>=</mo><mn>15</mn><mo>°</mo><mo>)</mo></mrow></math></span> incidence angle, surface single-bounce surface scattering becomes negligible, allowing for the detection of diffuse, dihedral (multiple bounces) scattering. We find that classical Mie alumina particles <span><math><mrow><mo>(</mo><mn>2</mn><mo>.</mo><mn>1</mn><mspace></mspace><mi>μ</mi><mi>m</mi><mo>,</mo><mn>4</mn><mo>.</mo><mn>0</mn><mspace></mspace><mi>μ</mi><mi>m</mi><mo>)</mo></mrow></math></span> enhance subsurface scattering due to a larger void space relative to larger Mie particles <span><math><mrow><mo>(</mo><mn>30</mn><mspace></mspace><mi>μ</mi><mi>m</mi><mo>)</mo></mrow></math></span>, that cause the radar signal to scatter forward off small imperfections, maintaining the polarization properties of the signal and generating high <span><math><mrow><mo>></mo><mn>1</mn></mrow></math></span> <span><math><mrow><mi>C</mi><mi>P</mi><mi>R</mi></mrow></math></span>. Latex beads, representing impurities, demonstrate the impact of isotropic and anisotropic scattering on radar signatures. This study also found that the scattering medium’s anisotropy correlates to the size of the beads, while the void space of the medium inversely correlates with the bead size and the volume concentration (v/v) of the beads. Rayleigh beads, due to isotropic scattering from the reduced scattering cross-section and higher transparency relative to larger impurities, generate subsurface single bounce scattering from the sample platform, producing <span><math><mrow><mi>O</mi><mi>C</mi><mo>≫</mo><mi>S</mi><mi>C</mi></mrow></math></span> and a low <span><math><mrow><mo>(</mo><mo><</mo><mn>0</mn><mo>.</mo><mn>5</mn><mo>)</mo></mrow></math></span> <span><math><mrow><mi>C</mi><mi>P</mi><mi>R</mi></mrow></math></span> across all v/v. Rayleigh impurities in transparent water-ice simulate single bounce scattering from underlying layers. Conversely, classical and large Mie beads generate anisotropic scattering that intensifies scattering in the forward direction with high <span><math><mrow><mi>C</mi><mi>P</mi><mi>R</mi></mrow></math></span>, inversely proportional to the volume concentration. This study aids in interpreting radar observations of icy bodies in the solar system, providing insights into the interplay between radar waves and icy regolith compositions.</p></div>","PeriodicalId":20054,"journal":{"name":"Planetary and Space Science","volume":"244 ","pages":"Article 105891"},"PeriodicalIF":1.8000,"publicationDate":"2024-03-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S0032063324000552/pdfft?md5=c513602ff4b1c6ccdd84378188bdef1d&pid=1-s2.0-S0032063324000552-main.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Planetary and Space Science","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0032063324000552","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
This study presents low phase angle measurements of polarimetric properties of icy planetary regolith analog materials acquired using the custom-built Multi-Axis- Goniometer-Instrument (MAGI). We present same sense , and opposite sense backscatter circular polarization coefficients, circular polarization ratio , and degree linear polarization of spherical latex (non-dye) beads of varying sizes and volume concentrations (v/v) in aqueous solutions () in water. We also present measurements of alumina powder in air at . Measurements showed that at a low incidence angle , backscatter is dominated by surface specular single-bounce scattering, that hides other scattering processes. At high incidence angle, surface single-bounce surface scattering becomes negligible, allowing for the detection of diffuse, dihedral (multiple bounces) scattering. We find that classical Mie alumina particles enhance subsurface scattering due to a larger void space relative to larger Mie particles , that cause the radar signal to scatter forward off small imperfections, maintaining the polarization properties of the signal and generating high . Latex beads, representing impurities, demonstrate the impact of isotropic and anisotropic scattering on radar signatures. This study also found that the scattering medium’s anisotropy correlates to the size of the beads, while the void space of the medium inversely correlates with the bead size and the volume concentration (v/v) of the beads. Rayleigh beads, due to isotropic scattering from the reduced scattering cross-section and higher transparency relative to larger impurities, generate subsurface single bounce scattering from the sample platform, producing and a low across all v/v. Rayleigh impurities in transparent water-ice simulate single bounce scattering from underlying layers. Conversely, classical and large Mie beads generate anisotropic scattering that intensifies scattering in the forward direction with high , inversely proportional to the volume concentration. This study aids in interpreting radar observations of icy bodies in the solar system, providing insights into the interplay between radar waves and icy regolith compositions.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research