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Change Detection in Sequences of SAR Sub-Aperture Images

机译:SAR子孔径图像序列中的变化检测

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In the last few years, image acquisition modes have been developed for spaceborne SAR systems aiming on an enhancement of geometric resolution. This offers new opportunities for the calculation of so-called sub-aperture images and their analysis. Due to the increase of illumination time, one single image can be subdivided into multiple sub-apertures, which are temporarily closely arranged to each other with a lower geometric resolution than the original image. Focusing on this increase of illumination time, the Staring Spotlight (ST) mode of the German TerraSAR-X (TSX) and TanDEM-X (TDX) satellite constellation is mentionable. Here, the azimuth bandwidth can be divided into subset images, in which e.g. vehicles or ships are still well observable. Consequently, moving targets can be detected without utilizing SAR raw data. For this, only a Single Look Complex (SLC) image has to be considered. In this study, different stacks consisting of sub-aperture images are calculated, which are used for incoherent change detection. The detection is performed as an adaption of a method for change analysis in SAR time series data developed earlier. This method comprises the detailed description of changes, concerning their categorization and classification. Therefore, suitable features have to be calculated leading to a clear distinction of different change categories. As test data, TSX SLC images are used which were acquired both in ST and in High Resolution Spotlight (HS) mode. An assessment concerning their suitability for the incoherent change detection method applied to the sub-apertures is given. With future studies, it will be tested, whether the temporal aspect can be meaningfully regarded for the change categorization step. For this, the concept of so-called high activity objects, which were the basis of the earlier developed change analysis scheme, might be of relevance for the analysis of changes in sub-aperture sequences.
机译:在过去的几年中,已经针对星载SAR系统开发了图像采集模式,旨在提高几何分辨率。这为所谓的子孔径图像的计算及其分析提供了新的机会。由于照明时间的增加,一个单独的图像可以细分为多个子光圈,这些子光圈以比原始图像更低的几何分辨率彼此暂时紧密排列。着眼于照明时间的增加,德国TerraSAR-X(TSX)和TanDEM-X(TDX)卫星星座的凝视聚光(ST)模式值得一提。在此,方位角带宽可以分为子图像,例如车辆或轮船仍然可以观察到。因此,可以在不利用SAR原始数据的情况下检测运动目标。为此,只需要考虑单一外观复杂(SLC)图像。在这项研究中,计算了由子孔径图像组成的不同堆栈,这些堆栈用于非相干变化检测。该检测是对先前开发的SAR时间序列数据中的变化分析方法的一种改编。此方法包括有关更改的详细描述,涉及更改的分类和分类。因此,必须计算合适的特征,以明确地区分不同的更改类别。作为测试数据,使用在ST模式和高分辨率Spotlight(HS)模式下获取的TSX SLC图像。给出了关于它们适用于子孔径的非相干变化检测方法的适用性的评估。在以后的研究中,将测试在变更分类步骤中是否可以有意义地考虑时间方面。为此,作为早期开发的变化分析方案的基础的所谓的高活动对象的概念可能与子孔径序列变化的分析有关。

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