Geo-referencing and stereo calibration of ground-based Whole Sky Imagers using the sun trajectory

Florian M. Savoy, Soumyabrata Dev, Y. Lee, Stefan Winkler
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引用次数: 9

Abstract

Ground-based Whole Sky Imagers (WSIs) are now commonly used for cloud observations. Upon deployment, they may not be exactly level or precisely face north. This significantly affects subsequent processing of the images, especially for applications where two or more imagers are required, e.g. 3D volumetric cloud reconstruction. We present a method to remove this mis-alignment using the sun position in images captured over a whole day. Coupled with precise coordinates of the device locations, this method also improves the geo-referencing accuracy of the captured images. We detect the sun in the images and compute the corresponding 3D vectors using the lens calibration function. These vectors are compared to the actual sun direction. The mismatch between the two sets of vectors is then corrected using a 3D rotation matrix. The method can also be applied to other celestial bodies, such as stars or the moon.
基于太阳轨迹的地面全日成像仪的地理参考和立体校准
地面全天空成像仪(WSIs)现在通常用于云观测。在部署时,它们可能不是完全水平或完全面向北方。这极大地影响了图像的后续处理,特别是对于需要两个或更多成像仪的应用,例如3D体积云重建。我们提出了一种方法,以消除这种不对准使用太阳的位置在一整天的图像捕获。加上设备位置的精确坐标,该方法还提高了捕获图像的地理参考精度。我们检测图像中的太阳,并使用镜头校准函数计算相应的三维矢量。将这些矢量与实际的太阳方向进行比较。然后使用3D旋转矩阵校正两组矢量之间的不匹配。该方法也可以应用于其他天体,如恒星或月亮。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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