基于最小误差熵代价的核自适应滤波器预测太阳黑子数

P. Brahma
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引用次数: 3

摘要

自适应滤波中的几种算法都是基于均方误差代价函数的最小化。然而,MSE只是二阶统计量,因此不能捕获有关系统中误差概率分布的全部信息。一种信息论的替代方法是使用最小误差熵(MEE)代价函数。基于这一准则的自适应算法已经被开发出来,并显示出与MSE相比较的优越性。在这项工作中,对其中一些方法的核心版本进行了设计和测试,以预测每年的太阳黑子数。太阳黑子数是太阳表面可见的较暗区域的数量,已被证明是模拟空间天气、电离层状态、气候异常甚至全球变暖的工具。本文提出了用MEE和MSE准则训练的各种线性和核算法在预测这种混沌非线性时间序列方面的比较性能研究。实验结果清楚地显示了基于MEE的核设计的优势,它具有非线性的优点,并且能够从误差分布中获得最大的信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Prediction of Sunspot Number Using Minimum Error Entropy Cost Based Kernel Adaptive Filters
Several algorithms in adaptive filtering are based on the minimization of the mean squared error (MSE) cost function. However, MSE is just a second order statistics and hence does not capture the entire information about the probability distribution of the error in the system. An information theoretic alternative is using the minimum error entropy (MEE) cost function. Adaptive algorithms based on this criterion have been developed and shown to be superior as compared to MSE counterparts. In this work, kernel versions of some of these methods are designed and tested on predicting the annual sunspot number. The sunspot number is the number of visibly darker regions on the solar surface and has been shown to be instrumental in modeling space weather, state of the ionosphere, climatic anomalies and even global warming. A comparative performance study of the various linear and kernel algorithms, trained with both MEE and MSE criteria, in predicting such a chaotic non-linear time series is presented in this paper. Experimental results clearly show the advantage of the MEE based kernel design which is as per expectation given that it has the advantage of being non-linear along with being able to derive maximum information from the error distribution.
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