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Change Detection in Sequences of SAR Sub-Aperture Images

机译:SAR子光圈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:在过去几年中,已经为旨在提高几何分辨率的太空载SAR系统开发了图像采集模式。这为计算所谓的子光圈图像及其分析提供了新的机会。由于照明时间的增加,可以将一个单个图像细分为多个子孔,其暂时紧密地布置成与原始图像较低的几何分辨率较低的几何分辨率。专注于这种照明时间的增加,德国Terrasar-X(TSX)和TANDEM-X(TDX)卫星星座的凝视射灯(ST)模式是由可编来的。这里,方位角带宽可以被分成子集图像,其中例如车辆或船舶仍然很明显。因此,可以在不利用SAR原始数据的情况下检测移动目标。为此,只需要考虑单个外观复杂(SLC)图像。在本研究中,计算由子孔图像组成的不同堆叠,其用于不连贯的变化检测。该检测作为在早期开发的SAR时间序列数据中改变分析方法的适应。该方法包括改变的详细描述,关于它们的分类和分类。因此,必须计算合适的特征,导致不同变化类别的清晰区别。作为测试数据,使用TSX SLC图像,其在ST和高分辨率聚光灯(HS)模式下获取。给出了施加到亚孔的不连贯改变检测方法的适用性的评估。随着未来的研究,它将被测试,是否可以有意义地考虑变更分类步骤。为此,所谓的高活动对象的概念,即先前开发的改变分析方案的基础,这可能是对分析子孔径序列的变化的相关性。

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