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Sea Clutter Modeling Improvement and Target Detection by Tsallis Distribution

机译:Tsallis分布的海杂波建模改进和目标检测

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Sea clutter is the backscattered returns from a patch of sea surface illuminated by a radar pulse and it's one of difficult domains in radar clutter modeling. A lot of efforts have been made to fit various distributions to the observed amplitude data of sea clutter. However, the fitting of those distributions to real sea clutter data is not good, and using parameters estimated from those distributions is not very effective for detecting targets within sea clutter. This may be due to the fact that sea clutter is highly non-stationary. Tsallis distribution is one of distributions that recommend in recent year for sea clutter modeling. This distribution is obtained by maximizing the Tsallis entropy. The Tsallis entropy is a generalization of the Shanon entropy. In this paper was found two weak points, by accomplished simulation analyses: a) By reason of using small step in parameters estimation, the time of modeling is long. b) By reason of using short segment of clutter data, decrease the target detection accuracy. By using the bigger step in this paper, increase the parameter estimation quickness and by using all sea clutter data and decrease performance, was improving the target detection accuracy.
机译:海杂波是由雷达脉冲照射的海面斑点的背散射回报,它是雷达杂波建模中的难度域之一。已经进行了许多努力,以适应各种分布到观察到的海洋杂波的幅度数据。然而,将这些分布到真正的海洋杂波数据的拟合不好,并且使用从这些分布估计的参数对于检测海杂波内的目标不是很有效。这可能是由于海洋杂波高度静止的事实是由于。 Tsallis分配是近年推荐海杂波建模的分布之一。通过最大化Tsallis熵获得该分布。 Tsallis熵是Shanon熵的概括。本文发现了两个弱点,通过完成模拟分析:a)由于使用小步骤在参数估计中,建模时间很长。 b)由于使用杂波数据的短段,降低目标检测精度。通过使用本文的更大步骤,增加参数估计速度,并通过使用所有海杂波数据并降低性能,提高目标检测精度。

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