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Modelling Reflectance Spectra of Muscovite as Function of Aluminium Content and Grain Size Using Hapke Model

机译:用Hapke模型建模葡萄干的反射光谱作为铝含量和晶粒尺寸的函数

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Muscovite is an important mineral commonly found in hydrothermal systems of Earth and Mars. Reflectance spectra of muscovite has several diagnostic absorption features in wavelength range 0.4-2.5 μm. The absorption feature near 2.20 μm is sensitive to alumina content variations. In this study, we use reflectance spectra of powdered muscovite and geochemical datasets to quantify the relationship between spectral shift and alumina content. Imaginary index of refraction (k) was derived from reflectance spectra and a linear model was proposed relating alumina content and k. Reflectance spectra of muscovite was modelled for varying alumina content and grain size using Hapke model. Modelled spectra shows shift in wavelength position of 2.20 μm with varying alumina content and deepening of absorption features with increase in grain size. The results shall be helpful in interpretation of reflectance spectra acquired from space borne and airborne platforms.
机译:Muscovite是一种重要的矿物,常见于地球和火星的水热系统。 Muscovite的反射光谱具有波长范围0.4-2.5μm的若干诊断吸收特征。 2.20μm附近的吸收特征对氧化铝含量变化敏感。在这项研究中,我们使用粉末状葡萄质和地球化学数据集的反射光谱来量化光谱移位和氧化铝含量之间的关系。折射折射率(K)源自反射光谱,提出了与氧化铝含量和k相关的线性模型。使用Hapke模型的氧化铝含量和晶粒尺寸的模型模拟了Muscovite的反射光谱。建模光谱显示波长位置的换档2.20μm,具有不同的氧化铝含量和吸收特征的加深,随着晶粒尺寸的增加。结果应有助于解释从太空和空中平台获得的反射谱。

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