水溶液中乳胶珠的光学偏振研究:冰壳中的雷达散射模拟

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Planetary and Space Science Pub Date : 2024-03-26 DOI:10.1016/j.pss.2024.105891
Antoine Bourget , Parvathy Prem , David Blewett , Michael G. Daly , Isaac B. Smith
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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>. 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引用次数: 0

摘要

本研究利用定制的多轴测角仪(MAGI),对冰质行星碎屑模拟材料的偏振特性进行了0°-5°低相角测量。我们展示了水溶液(λ=0.8μm)中不同大小和体积浓度(v/v)的球形乳胶(非染料)珠子的同感(SC)和反感(OC)反向散射圆偏振系数、圆偏振比(CPR)和线性偏振光度(DLP)。我们还介绍了在 λ=1.064μm 时对空气中氧化铝粉末的测量结果。测量结果表明,在低入射角(i=0°)时,背向散射主要由表面镜面单跳散射引起,掩盖了其他散射过程。在高入射角(i=15°)下,表面单跳散射变得可以忽略不计,从而可以检测到漫反射、二面(多次反弹)散射。我们发现,经典的米氏氧化铝颗粒(2.1μm,4.0μm)与较大的米氏颗粒(30μm)相比,由于空隙较大而增强了次表层散射,使雷达信号从小缺陷处向前散射,保持了信号的极化特性,并产生高 CPR。代表杂质的乳胶珠展示了各向同性和各向异性散射对雷达信号的影响。这项研究还发现,散射介质的各向异性与珠子的大小相关,而介质的空隙与珠子的大小和体积浓度(v/v)成反比。与较大的杂质相比,雷利珠由于散射截面减小而产生各向同性散射,且透明度较高,因此会从样品平台产生次表层单弹跳散射,从而产生 OC≫SC,并在所有 v/v 条件下产生较低(<0.5)的 CPR。透明水冰中的瑞利杂质模拟了来自底层的单弹跳散射。相反,经典的和大的米珠会产生各向异性散射,在高 CPR(与体积浓度成反比)的情况下会加强正向散射。这项研究有助于解释太阳系中冰体的雷达观测结果,为雷达波和冰层碎石成分之间的相互作用提供了见解。
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Optical polarization studies of latex beads in aqueous solution: An analog for radar scattering in icy regolith

This study presents low phase angle 0°5° measurements of polarimetric properties of icy planetary regolith analog materials acquired using the custom-built Multi-Axis- Goniometer-Instrument (MAGI). We present same sense (SC), and opposite sense (OC) backscatter circular polarization coefficients, circular polarization ratio (CPR), and degree linear polarization (DLP) of spherical latex (non-dye) beads of varying sizes and volume concentrations (v/v) in aqueous solutions (λ=0.8μm) in water. We also present measurements of alumina powder in air at λ=1.064μm. Measurements showed that at a low incidence angle (i=0°), backscatter is dominated by surface specular single-bounce scattering, that hides other scattering processes. At high (i=15°) 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 (2.1μm,4.0μm) enhance subsurface scattering due to a larger void space relative to larger Mie particles (30μm), that cause the radar signal to scatter forward off small imperfections, maintaining the polarization properties of the signal and generating high >1 CPR. 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 OCSC and a low (<0.5) CPR 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 CPR, 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.

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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
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
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