可視・近赤外リモートセンシングによる造岩鉱物の定量的分析 珪酸塩鉱物を例として;可視・近赤外リモートセンシングによる造岩鉱物の定量的分析 珪酸塩鉱物を例として;Quantitative Analysis of Rock-Forming Minerals by Visible and Near-Infrared Remote Sensing. Silicate Minerals as Examples.

Takahiro Hiroi
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引用次数: 1

Abstract

Most of rock-forming minerals show characteristic absorption features in the visible and near-infrared wavelength regions. Especially, silicates such as olivine and pyroxene show clear absorption bands due to Fe2+, which change in wavelength position and strength as their Fe/Mg ratios change. Also, structural change by shock can alter absorption band shapes as seen in plagioclase-muskelynite series. Such changes can be readily quantified using the Modified Gaussian Model. Also, mineral mixing ratios and grain size and shape of each mineral cause specific changes in reflectance spectra, which can be simulated by photometric models. As a special complication of planetary surface regoliths, spaceweathering effects have to be removed from the reflectance spectra.
以硅酸盐矿物为例,通过可视、近红外遥感对造岩矿物进行定量分析;以硅酸盐矿物为例,通过可视、近红外遥感对造岩矿物进行定量分析;Quantitative Analysis of Rock-Forming Minerals by Visible and Near-Infrared Remote Sensing. SilicateMinerals as Examples。
大多数造岩矿物在可见光和近红外波段表现出特有的吸收特征。特别是橄榄石和辉石等硅酸盐,由于Fe2+的作用,呈现出清晰的吸收带,其波长位置和强度随其Fe/Mg比的变化而变化。此外,由冲击引起的结构变化可以改变吸收带的形状,如在斜长石-肌鞘岩系列中所见。这种变化可以很容易地用修正高斯模型量化。此外,矿物混合比例以及每种矿物的粒度和形状都会引起反射光谱的特定变化,这些变化可以通过光度模型来模拟。作为行星表面风化层的特殊复杂性,空间风化效应必须从反射光谱中去除。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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