南京大学学报(自然科学版) ›› 2016, Vol. 52 ›› Issue (1): 184–193.

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基于张量动态纹理模型的极光视频分类

宋亚婷1, 韩 冰1,2*, 高新波1,   

  • 出版日期:2016-01-27 发布日期:2016-01-27
  • 作者简介:(1. 西安电子科技大学电子工程学院,西安,710071;2. 遥感科学国家重点实验室,北京,100101)
  • 基金资助:
    基金项目:国家自然科学基金(41031064,61572384),教育部留学回国人员科研启动基金,2010年海洋公益性行业科研专项经费
    (201005017),中央高校基本科研业务费专项资金(K5051302008,K5051202048),遥感科学国家重点实验室开放基金
    (OFSLRSS201415),中国博士后科学基金(2014M560752),陕西省博士后科研项目
    收稿日期:2015-06-29
    *通讯联系人,E-mail:bhan@xidian.edu.cn

Tensor based dynamic textures model for aurora sequences classification

Song Yating1, Han Bing1,2*, Gao Xinbo1   

  • Online:2016-01-27 Published:2016-01-27
  • About author:(1. School of Electronic Engineering, Xidian University, Xian, 710071, China; 2. State Key Laboratory of Remote Sensing Science, Beijing, 100101, China)

摘要: 极光事件的形态与行星际磁场及太阳风等空间物理过程密切相关,通过研究极光形态可以得到大量地球磁层和太阳风活动的信息.随着海量极光的产生,如何借助计算机对极光图像序列进行自动分类成为热点.目前极光分类研究大多是基于单幅图像的特征分析,极光视频的建模和分析仍然有待深入研究.提出一种基于极光视频动态纹理建模的极光视频事件识别方法.首先对四类极光视频进性普适性动态纹理建模.该模型能充分表征极光序列帧间的重复相关性和动态变化特性.然后利用矩阵SVD分解对动态纹理模型求解,最后用模型参数间的马丁距离衡量极光序间差异性,采用最小距离分类器和SVM分类器实现四类典型形态的极光序列的自动分类识别.为进一步提高模型紧凑型,引入张量分解,建立张量动态纹理模型.相比于动态纹理模型只关注序列帧间的重复相关性,张量动态纹理模型还分析图像帧内各个部分间的重复相关性.张量动态纹理模型能从时间和空间维度上同时进行分解,提取模型参数构造极光序列特征,减少模型冗余的同时提高分类准确率.在中国北极黄河站的ASI图像数据库上进行了算法验证,实验结果表明该方法分类准确率可以达到80%以上.算法能有效识别不同形态的极光序列事件.

Abstract: The morphological characteristics of aurora are strongly affected by the contemporaneous solar wind variance and interplanetary magnetic field. Large amounts of information about the magnetosphere and solar wind activities can be got through the study of aurora morphology. With millions of aurora images collected, how to classify the aurora sequences fast and efficiently becomes an important and hot topic. At present, the dynamic features of aurora sequence are seldom extracted compare to the static features of aurora images. In this paper, a method for classifying aurora sequences based on the dynamic texture model is proposed. Linear dynamical texture systems are used to model all four categories of aurora sequences universally. The scheme can acquire the dynamics and correlations between aurora frames. Then SVD decomposition of matrix was used to the solution of dynamic texture model. Finally, the difference between sequences are evaluated by the Martin distance of model parameters. The nearest neighbor(NN) classifier and SVM classifier is applied to classify aurora sequences. In order to reduce the redundancy of the model, tensor dynamic texture models are used based on tucker tensor decomposition. Compare to dynamical texture models which only focus on the correlations between the aurora frames, tensor dynamic texture models also analysis the correlations in one frame, because tensor dynamic texture models decompose the aurora sequences both on spatial and temporal dimensions. Then the parameters are extracted as the features of aurora sequences, which reduce the redundant information while enhance the classification accuracy at the same times. The experimental results on the dataset obtained from All-sky Imager (ASI) at the Chinese Yellow River Station achieve high classification accuracy, and demonstrate the effectiveness of the proposed classification algorithm.

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