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Radiometric Normalization of Multitemporal Optical Satellite Images using Iteratively-Reweighted Multivariate Alteration Detection

机译:迭代加权多元变化检测对多时相光学卫星图像的辐射归一化

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Radiometric normalization is a fundamental process for multitemporal satellite images. The accuracy of relative normalization depends on the quality of selected Pseudo Invariant Features (PIFs). PIFs represent the ground objects whose reflectance are constant during a period of time. In previous study, an algorithm, called Multivariate Alteration Detection (MAD), was applied to statistically select no-changed pixels within bi-temporal satellite images. However, MAD is sensitive to cloud covers and some clouds may be misclassified as PIFs. For this reason, Iteratively Reweighted MAD (IR-MAD) was introduced to establish an increasingly better no-changed background using iterative scheme. Nonetheless, both MAD and IR-MAD only compute the linear combinations for bi-temporal images, and not applicable for multitemporal images with more than two images. In this study, a novel method called Weighted Generalized Canonical Correlation Analysis (WGCCA) is proposed for the selection of high-quality PIFs in multitemporal and multispectral images, which solves coefficients for the correlations of not only multivariable data but also multitemporal data. Specifically, the proposed method integrates the strengths of Generalized Canonical Correlation Analysis (GCCA) and IR-MAD, and PIFs extraction from a sequence of satellite images is performed at the same time, which leads to a consistent feature extraction. Furthermore, when the high-quality PIFs are determined by the proposed method, the digital numbers of PIFs from multitemporal images are transformed into a predefined radiometric reference level. With this approach, the radiometric resolution of multitemporal images can be preserved, and a better radiometric normalization can be obtained. In experiment. SPOT-5 imagery was tested. Compared with Canonical Correlation Analysis (CCA) which is used in MAD, the proposed method can discriminate no-changed pixels from changed more precisely.
机译:辐射归一化是多时相卫星图像的基本过程。相对归一化的准确性取决于选定的伪不变特征(PIF)的质量。 PIF表示反射率在一段时间内恒定的地面对象。在先前的研究中,一种称为多变量变更检测(MAD)的算法被用于统计地选择双时相卫星图像中的不变像素。但是,MAD对云层很敏感,某些云可能会误分类为PIF。为此,引入了迭代加权MAD(IR-MAD),以使用迭代方案建立越来越好的无变化背景。但是,MAD和IR-MAD都仅计算双时间图像的线性组合,不适用于具有两个以上图像的多时间图像。在这项研究中,提出了一种称为加权广义典范相关分析(WGCCA)的新方法,用于选择多时相和多光谱图像中的高质量PIF,该方法不仅解决了多变量数据而且还涉及了多时相数据的相关系数。具体来说,该方法融合了广义规范相关分析(GCCA)和IR-MAD的优势,同时从一系列卫星图像中提取了PIF,从而实现了一致的特征提取。此外,当通过所提出的方法确定高质量的PIF时,来自多时相图像的PIF的数字数量将转换为预定义的辐射参考水平。使用这种方法,可以保留多时间图像的辐射分辨率,并可以获得更好的辐射归一化。在实验中。测试了SPOT-5图像。与MAD中使用的典范相关分析(CCA)相比,该方法可以更准确地区分出不变像素。

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