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Stereoscopic ground-based determination of the cloud base height: camera position adjusting with account for lens distortion

机译:立体地面确定云底高度:调整镜头位置并考虑镜头变形

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For the reconstruction of the cloud base height a method was developed based on taking pictures of the sky by a pair of digital photo cameras from the ground and subsequent processing of the obtained sequence of stereo frames. Since the directions of the optical axes of the stereo cameras are not exactly known, a procedure of adjusting of obtained frames was developed which use photographs of the night starry sky. In the second step, the method of the morphological analysis of images is used to determine the relative shift of the coordinates of some fragment of cloud. The shift is used to estimate the searched cloud base height. The proposed method can be used for automatic processing of stereo data and getting the cloud base height. The earlier paper described a mathematical model of stereophotography measurement, poses and solves the problem of adjusting of optical axes of the cameras in paraxial (first-order geometric optics) approximation and was applied for the central part of the sky frames. This paper describes the model of experiment which takes into account lens distortion in Seidel approximation (depending on the third order of the distance from optical axis). Based on this model a procedure of simultaneous camera position adjusting and estimation of parameters of lens distortion in Seidel approximation was developed. The first experimental results of its application are shown.
机译:为了重建云底高度,开发了一种方法,该方法基于一对数码相机从地面拍摄天空的图片并随后对获得的立体帧序列进行后续处理。由于立体摄像机的光轴方向尚不完全清楚,因此开发了使用夜空星空照片调整获得的帧的程序。在第二步中,使用图像形态分析的方法确定云的某些片段的坐标的相对移动。该偏移量用于估计搜索到的云底高度。该方法可用于立体数据的自动处理并获得云底高度。较早的论文描述了立体摄影测量的数学模型,提出并解决了以近轴(一阶几何光学)近似值调节摄像机光轴的问题,并将其应用于天空框架的中心部分。本文介绍了一种实验模型,该模型考虑了Seidel近似中的透镜畸变(取决于距光轴距离的三阶)。基于此模型,开发了一种同时调整相机位置和估计Seidel近似值的镜头畸变参数的程序。显示了其应用的第一个实验结果。

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