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EVALUATION OF WORLDVIEW-1 STEREO SCENES

机译:评估WorldView-1立体声场景

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This paper describes the investigations carried out at ETH Zurich on the very-high resolution optical satellite sensor WorldView-1. The dataset includes a stereopair acquired in November 2007 over Morrison, Colorado, USA, consisting of a quasi-nadir scene with mean GSD close to 51cm and an off-nadir scene, with GSD up to 73cm. The radiometry of the images was evaluated through the estimation of the noise level (standard deviation of the digital number) in non-homogeneous areas. For the orientation of the scenes, we used ground control points to estimate the parameters of an affine transformation and improve the orientation related to the Rational Polynomial Coefficients (RPC) provided in the metadata files. The next step included the automatic DSM generation with quality assessment. In all our tests the matching and the final DSM generation was realized with our in-house software package SAT-PP (Satellite Image Precision Processing) which has already been successfully used for other satellite sensors like IKONOS, ALOS/PRISM, Cartosat-1 and airborne linear and frame cameras. For the evaluation of the potential of a WorldView-1 stereo image pair for DSM generation, reference data are fundamental. As no DSM with a suitable resolution was available in this dataset, we generated the reference DSM from 1:15'000 scale infrared aerial images purchased from USGS. The aerial images were acquired in April 2002 with an analogue camera and scanned with a resolution of 14(mu)m. No GCPs were available for the area covered by the aerial images. Therefore we defined a sufficient number of well-defined texture points in the oriented stereo pair of WorldView-1 as GCPs and determined their 3D coordinates using the orientation parameter of the satellite stereo pair. These points were used for the image orientation of the aerial images, which leads to a good relative orientation between the two different image sets. By this we investigated the quality of the matching process with WorldView-1 stereo image data mostly independent of the exterior orientation parameters. We will present here our accuracy assessment by visual and quantitative analysis (3D residuals distribution and statistics). The difference between the acquisition times of the two data sets (about 2.5 years) caused changes in the land cover, e.g. in correspondence of vegetation and buildings. In order to avoid the influence of temporal differences in our analysis, we compared the surface models in areas where no significant time depending changes could be expected. In addition, we evaluated the potential of the scenes for 3D building model extraction. The results are presented and discussed.
机译:本文介绍了在非常高分辨率光学卫星传感器世界观-1上的Eth苏黎世进行的调查。 DataSet包括2007年11月在美国科罗拉多州莫里森收购的立体声,由Quasi-Nadir场景组成,该场景与近51厘米的平均GSD和一个离Nadir场景,GSD高达73厘米。通过估计非均匀区域中的噪声水平(数字数的标准偏差)来评估图像的辐射测定。对于场景的方向,我们使用地面控制点估计仿射变换的参数,提高了元数据文件提供了关于有理多项式系数(RPC)的方向。下一步包括具有质量评估的自动DSM生成。在所有测试的匹配,最终DSM生成用我们的内部软件程序包SAT-PP(卫星图像精密加工),其已经成功地用于其他卫星传感器等IKONOS,ALOS / PRISM,的Cartosat-1和实现空中线性和框架摄像头。为了评估DSM生成的WorldView-1立体声图像对的潜力,参考数据是基本的。由于在该数据集中提供了具有合适分辨率的DSM,因此我们从USGS购买的1:15'000规模的红外空中图像生成了参考DSM。航空图像于2002年4月获得模拟摄像机,并扫描了14(mu)m的分辨率。没有GCP可用于航空图像所覆盖的区域。因此,我们在面向的立体声对WorldView-1中定义了足够数量的定义纹理点作为GCP,并使用卫星立体对的方向参数确定其3D坐标。这些点用于空中图像的图像取向,这导致两个不同图像集之间的良好相对取向。由此,我们调查了与世界观-1立体图像数据的匹配过程的质量,大多数与外部方向参数无关。我们将通过视觉和定量分析(3D残差分布和统计)在这里展示我们的准确性评估。两种数据集的采集时间(约2.5岁)之间的差异导致陆地盖的变化,例如,植被和建筑物的对应关系。为了避免对我们分析中的时间差异的影响,我们将表面模型与根据更改的重要时间的区域进行比较。此外,我们还评估了3D建筑模型提取的场景的潜力。提出和讨论了结果。

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