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Quantitative mapping of arid alluvial fan surfaces using field spectrometer and hyperspectral remote sensing

机译:使用现场光谱仪和高光谱遥感对干旱冲积扇面进行定量制图

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Mapping and dating of arid and semi-arid alluvial fans are of great importance in many Quaternary studies. Yet the most common mapping method of these features is based on visual, qualitative interpretation of air-photos. In this study we examine the feasibility of mapping and alluvial surfaces by using airborne hyperspectral reflective remote sensing methodology. This technique was tested on Late Pleistocene to Holocene alluvial fan surfaces located in the hyperarid southern Arava valley, Israel. Results of spectral field measurements showed that the surface reflectance is controlled by two main surficial processes, which are used as relative age criteria: the degree of desert pavement development (gravel coverage %) controls the absorption feature depths, while the rock coating development influences significantly the overall reflectance of the surface, but its effect on the absorption feature depths is limited. We show that as the percent of the surface covered by gravels increases, the absorption feature depth of the common gravels, in this case carbonate at 2.3.3 μm, increases as well; whereas the absorption features depth of the fine particle in-between the gravels, decrease (hydroxyl and ferric absorption features at 2.21 μm, and 0.87 μm, respectively), as the fines are removed from the surface. Using these correlations we were able to map the surface gravel coverage (%) on the entire alluvial fan, by calculating the gravel coverage (%) in each pixel of the hyperspectral image. The prediction of gravel coverage (%) is with accuracy of ±15% (e.g. gravel coverage of 50% can be predicted to be 3.5% to 65%). Using extensive accuracy assessment data, we show that the spectral based mapping maintained high accuracy degree (R{sup}2 = 0.57 to 0.83). The quantitative methodology developed in this study for mapping alluvial surfaces can be adapted for other surfaces and piedmonts throughout the arid regions of the world.
机译:在许多第四纪研究中,干旱和半干旱冲积扇的测绘和测年非常重要。然而,这些特征最常见的映射方法是基于对航空照片的视觉,定性解释。在这项研究中,我们通过使用机载高光谱反射遥感方法研究了制图和冲积表面的可行性。这项技术在位于以色列阿拉瓦河谷南部高干旱地区的晚更新世至全新世冲积扇表面进行了测试。光谱场测量的结果表明,表面反射率受两个主要的表面过程控制,这两个过程被用作相对年龄标准:沙漠路面的发展程度(砾石覆盖率%)控制着吸收特征深度,而岩石涂层的发展则对其影响很大。表面的总反射率,但是它对吸收特征深度的影响是有限的。我们发现,随着砾石覆盖表面的百分比增加,普通砾石(在本例中为2.3.3μm的碳酸盐)的吸收特征深度也随之增加;但是,随着细粒从表面去除,细粒在砾石之间的吸收特征深度减小(羟基和铁的吸收特征分别为2.21μm和0.87μm)。使用这些相关性,我们可以通过计算高光谱图像每个像素中的砾石覆盖率(%)来绘制整个冲积扇的砾石覆盖率(%)。砾石覆盖率(%)的预测精度为±15%(例如,砾石覆盖率50%可以预测为3.5%至65%)。使用大量的精度评估数据,我们表明基于频谱的映射保持了较高的精度(R {sup} 2 = 0.57至0.83)。这项研究中开发的用于测绘冲积表面的定量方法可以适用于世界干旱地区的其他表面和山麓。

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