首页> 外文会议>Conference on Optomechatronic Systems III, Nov 12-14, 2002, Stuttgart, Germany >Mean squared and worst case performance of multi-spacecraft imaging systems: a feature based approach
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Mean squared and worst case performance of multi-spacecraft imaging systems: a feature based approach

机译:多航天器成像系统的均方和最坏情况性能:基于特征的方法

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The problem of quantifying minimum acceptable performance of multi-spacecraft interferometric imaging systems is considered. The noise corrupting the measurements is critical in the design of these systems and is dependent on the motion of the constituent spacecrafts. Minimum acceptable performance is defined in terms of the misclassification error of an image given that the set of images has been partitioned into two distinct classes. Two measures of the noise corrupting the measurements are considered : mean squared error(MSE) and the worst case error(WCE). It is shown that these are consistent with the goal of image classification in the sense that as image estimates converge in the MSE/WCE sense, the probability of misclassifying the image tends to zero. Error bounds are obtained on the MSE/WCE such that some minimum acceptable performance, in terms of the probability of correctly classifying an image, is acheived. An example is presented where the bandedness of the image of a planet is sought to be detected. Bounds on the noise corrupting the measurements are obtained such that a pre-specified level of performance is achieved for this case.
机译:考虑了量化多航天器干涉成像系统的最小可接受性能的问题。破坏测量的噪声在这些系统的设计中至关重要,并且取决于组成航天器的运动。假定图像集已划分为两个不同的类,则根据图像的误分类错误定义最低可接受性能。考虑了噪声破坏测量的两种方法:均方误差(MSE)和最坏情况误差(WCE)。从图像估计在MSE / WCE的意义上收敛的角度来看,这表明与图像分类的目标是一致的,图像误分类的可能性趋于零。在MSE / WCE上获得了误差范围,从而实现了一些将图像正确分类的最低可接受性能。提出了一个示例,其中试图检测行星图像的带状度。获得使测量结果恶化的噪声的界限,从而针对这种情况获得预定的性能水平。

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