Sun glint correction of airborne AISA images for mapping shallow-water benthos

E. Vahtmae, T. Kutser
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引用次数: 2

Abstract

Airborne sensors have higher spatial and spectral resolution than satellite sensors, providing greater accuracy in benthic habitat mapping in case of high spatial heterogeneity. Nevertheless, the effect of wave-induced sun glint may obscure the radiance originating from within the water. Such glint is particularly noticeable due to the high spatial resolution of the sensor and may impede mapping of benthic features. This paper describes the application of the sun glint correction schemes on to airborne hyperspectral AISA measurements acquired on the area of the West-Estonian archipelago during the campaign in July 2006. Currently proposed sun glint removal procedures assume zero water leaving signal in near infrared part of spectrum. This assumption is not true in waters less than about 2 m deep where part of the water leaving signal is originated from the bottom. As a result the shallow water pixels are overcorrected during glint removal procedure and the shapes of reflectance spectra are distorted. This has serious implications on shallow water bottom classification results, especially if spectral libraries of in situ measured or modelled reflectance spectra are used in classification of remote sensing imagery. Therefore, it is important to preserve spectral signatures of these areas if sun glint removal is necessary. We propose an alternative sun glint removal procedure where the amount of glint in each pixel is estimated from the depth of oxygen absorption feature at 760 nm relative to a baseline. The new method removes sun glint successfully and at the same time preserves the shape and magnitude of shallow water reflectance spectra.
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用于测绘浅水底栖生物的机载AISA图像的太阳闪烁校正
机载传感器比卫星传感器具有更高的空间和光谱分辨率,在高空间异质性的情况下,为底栖生物栖息地测绘提供更高的精度。然而,波浪引起的太阳闪光的影响可能会掩盖从水中发出的光芒。由于传感器的高空间分辨率,这种闪烁特别明显,并且可能阻碍底栖生物特征的映射。本文描述了2006年7月在西爱沙尼亚群岛地区的运动期间,太阳闪烁校正方案在机载高光谱AISA测量中的应用。目前提出的太阳闪光去除方法,在近红外光谱中假定零水残留信号。在水深不到2米的水域中,这种假设是不成立的,因为部分水的信号来自底部。在去除闪烁过程中,浅水像元被过度校正,导致反射光谱形状失真。这对浅水底分类结果有严重影响,特别是在遥感图像分类中使用现场测量或模拟反射光谱的光谱库时。因此,如果需要去除太阳闪烁,保存这些区域的光谱特征是很重要的。我们提出了一种替代的太阳闪烁去除程序,其中每个像素中的闪烁量是根据相对于基线的760 nm处的氧吸收特征深度估计的。新方法成功地消除了太阳闪烁,同时保留了浅水反射光谱的形状和大小。
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