基于实例的支持向量机遗传算法在太阳耀斑预测中的应用

Y. Taniguchi, Y. Kubota, S. Tsuruta, Yoshiyuki Mizuno, T. Muranushi, Yuko Hada Muranushi, Yoshitaka Sakurai, R. Knauf, Andrea Kutics
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引用次数: 0

摘要

异常强烈的太阳耀斑可能造成严重的灾难,如电力/核电站的损坏。因此,由于现有数据的不平衡特性,预测强烈的太阳耀斑是非常需要的,但也是相当困难的。为了解决这一问题,我们开发并应用了一种基于案例的遗传算法(CBGALO),该算法包含一个局部优化器,即支持向量机(SVM)。然而,预测性能在很大程度上依赖于学习的输入数据。在此基础上,对CBGALO进行了进一步扩展,提出了一种基于案例的学习特征和输入数据自动可重启的Good组合搜索遗传算法(CBRsGcmbGA)。即使是强大但计算成本昂贵的深度学习也不能自动(在我们的方法中是进化的)搜索学习数据。我们的方法通过基于案例的方法更好地解决了这个问题。然而,很明显,即使是这项工作也会受到典型的遗传效应的影响,陷入局部最优。为了改善结果,我们开发了一种新的多样性维持方法,将具有较大汉明距离的优秀个体作为精英个体插入到GA群体的病例库中。在3类太阳耀斑中的2类中,我们的新方法的表现达到了传统世界最高纪录中的最佳表现。也就是说,即使在≥C级的太阳耀斑中,我们采用汉明距离增加多样性的方法的性能也高达0.662,而传统的世界最高纪录为0.650。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Maintaining Diversity in an SVM integrated Case Based GA for Solar Flare Prediction
Unusually intense solar flares may cause serious calamities such as damages of electric/nuclear power plants. It is thereupon highly demanded, but is quite difficult, to predict intense solar flares due to the imbalanced character of the available data. To cope with this problem, we have heretofore developed and applied a Case Based Genetic Algorithm (CBGALO) that contains a Local Optimizer, which is a Support Vector Machine (SVM). However, the prediction performance significantly depends on input data for learning. Hereupon, CBGALO is further extended by a Case Based automatically restartable Good combination searching GA for both learning features and input data (CBRsGcmbGA). Even the powerful but computationally expensive Deep Learning cannot automatically (evolutionarily, in our approach) search the learning data. Our approach solved this problem a little better by the case-based approach. However, it became obvious that even this work suffers from the typical GA effect in falling into local optima. To improve the results, we hence developed newly a diversity maintenance approach that inserts good individuals with large Hamming distance into the case base as elite individuals in GA’s population. In 2 out of 3 classes of solar flares, the performance of our new approach became as high as the best ones among the conventional world top records. Namely, even in those ≥ C class solar flares, our approach applying the Hamming distance to increase diversity had as high a performance 0.662 as compared with the conventional world top record 0.650.
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