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在镜面反射条件下,除亮度对比反转外,对AISA波段差异进行精细运用以识别浮油。

Refined use of AISA band-differences for oil slick identification beyond brightness contrast reversal under sunglint.

作者信息

Jin Song, Lu Yingcheng, Liu Yongxue, Wei Xianglin, Lu Wanyun, Wang Difeng, Mao Zhihua

出版信息

Opt Express. 2018 Dec 24;26(26):33748-33755. doi: 10.1364/OE.26.033748.

Abstract

Marine oil slicks show brighter or darker than surrounding oil-free seawater under different sunglint, which can be observed by satellite optical sensors. Although this has been interpreted using a critical angle concept and simulated using the Cox-Munk model, it has not been demonstrated in high spatial resolution images from airborne sensors. In this study, an AISA (airborne imaging spectrometer for applications) image was used to determine the characteristics of non-emulsion oil slicks under sunglint in high spatial resolution images. Although a similar positive or negative contrast between non-emulsion oil slicks and oil-free seawater can be observed, it is difficult to directly model sunglint reflectance due to the different remote sensing scale effect. There are many sun glitter pepper noise produced by various micro-mirror facets of ocean surface in high spatial resolution images. Based on the optical image characteristics, a normalized noise index (ξ) was designed to evaluate the pepper noise in 1830 band-difference results. Then a level segmentation method was used to delineate the oil slicks under various sunglint from a minimum pepper noise image. Our study provides a preliminary reference for airborne optical remote sensing of oil slicks under various levels of sunglint.

摘要

在不同的镜面反射条件下,海面油膜比周围无油海水显得更亮或更暗,这可以通过卫星光学传感器观测到。尽管这已使用临界角概念进行了解释,并使用Cox-Munk模型进行了模拟,但尚未在机载传感器的高空间分辨率图像中得到证实。在本研究中,利用AISA(应用机载成像光谱仪)图像来确定高空间分辨率图像中镜面反射条件下非乳化油膜的特征。尽管在非乳化油膜和无油海水之间可以观察到类似的正或负对比度,但由于不同的遥感尺度效应,很难直接对镜面反射率进行建模。在高空间分辨率图像中,海洋表面的各种微镜面会产生许多太阳耀斑胡椒噪声。基于光学图像特征,设计了归一化噪声指数(ξ)来评估1830波段差值结果中的胡椒噪声。然后采用水平分割方法从最小胡椒噪声图像中勾画出不同镜面反射条件下的油膜。我们的研究为不同镜面反射条件下油膜的机载光学遥感提供了初步参考。

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