Bi-Directional Spectro-Polarimetry of Olivine Sand

IF 2.6 3区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Earth and Space Science Pub Date : 2025-01-17 DOI:10.1029/2024EA003928
Chris H. Lee, Charles M. Bachmann, Nayma Binte Nur, Rachel M. Golding
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Abstract

We characterized the bi-directional spectro-polarimetry of olivine sands of varying grain size distributions for a comprehensive set of measurement and illumination angles over a wavelength range of 350–2,500 nm. Our laboratory instrumentation included a hyperspectral goniometer, a broadband linear polarizer, and a tungsten-halogen illumination source. Three distinct grain size distributions of olivine sand samples were used in our experiments. As a function of azimuth, we measured a significant degree of anisotropic scattering, that depends directly on polarization angles, resulting in a distribution that cannot be accurately described solely using phase angle. For media of uniform or similar composition, we observed robust separability of grain size distributions using spectro-polarimetry. We compared Hapke's polarimetric model for semi-infinite granular media with a new empirical polarimetric model that we developed. This empirical model more accurately replicates the scattering of unpolarized incident light as a function of all view azimuth, view zenith, and polarization angles for all incident zenith angles. Parameters of our empirical polarimetric model that determine the magnitude of polarization correlate linearly with the inverse diffuse reflectances of the olivine sand samples, exhibiting phenomenology that is most likely due to the Umov effect. Because of the linearity of the correlations, our results show that polarimetry can be used to retrieve medium parameters, such as grain size distributions. We provide our data online and freely available in a Zenodo/GitHub repository.

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橄榄石砂的双向光谱极坐标测量法
在350 - 2500 nm波长范围内,我们对不同粒度分布的橄榄砂进行了双向光谱偏振测定。我们的实验室仪器包括一个高光谱测角仪,一个宽带线性偏振器和一个钨卤照明光源。实验中采用了三种不同粒度分布的橄榄石砂样品。作为方位角的函数,我们测量了很大程度的各向异性散射,这直接取决于偏振角,导致仅使用相位角无法准确描述分布。对于均匀或相似成分的介质,我们使用光谱偏振法观察到粒度分布的可分离性。我们将hake的半无限颗粒介质的极化模型与我们开发的新的经验极化模型进行了比较。这个经验模型更准确地复制了非偏振入射光的散射,作为所有视点方位角、视点天顶和所有入射天顶角的偏振角的函数。我们的经验极化模型的参数决定了极化的大小与橄榄石砂样品的反向漫反射呈线性相关,表现出很可能是由于Umov效应造成的现象。由于相关性的线性,我们的结果表明,偏振法可以用来检索介质参数,如粒度分布。我们在Zenodo/GitHub存储库中提供在线和免费的数据。
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来源期刊
Earth and Space Science
Earth and Space Science Earth and Planetary Sciences-General Earth and Planetary Sciences
CiteScore
5.50
自引率
3.20%
发文量
285
审稿时长
19 weeks
期刊介绍: Marking AGU’s second new open access journal in the last 12 months, Earth and Space Science is the only journal that reflects the expansive range of science represented by AGU’s 62,000 members, including all of the Earth, planetary, and space sciences, and related fields in environmental science, geoengineering, space engineering, and biogeochemistry.
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