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基于光谱融合的火星表面相关矿物分类方法研究
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  • 英文篇名:Classification and Discrimination of Martian-Related Minerals Using Spectral Fusion Methods
  • 作者:徐伟杰 ; 武中臣 ; 朱香平 ; 张江 ; 凌宗成 ; 倪宇恒 ; 郭恺琛
  • 英文作者:XU Wei-jie;WU Zhong-chen;ZHU Xiang-ping;ZHANG Jiang;LING Zong-cheng;NI Yu-heng;GUO Kai-chen;Institute of Space Sciences,Shandong Provincial Key Laboratory of Optical Astronomy & Solar Terrestrial Environment,Shandong University;State Key Laboratory of Transient Optics and Photonics,Chinese Academy of Sciences;
  • 关键词:可见近红外光谱 ; 拉曼光谱 ; 光谱融合 ; 软独立建模分类法 ; 主成分分析-K值最邻近分类法
  • 英文关键词:Visible-near infrared spectroscopy;;Raman spectroscopy;;Spectral fusion;;Soft Independent Method of Class Analogy;;Principal Component Analysis-K-Nearest Neighbor
  • 中文刊名:GUAN
  • 英文刊名:Spectroscopy and Spectral Analysis
  • 机构:山东大学空间科学研究院及山东省光学天文与日地空间环境重点实验室;中国科学院西安光学精密机械研究所瞬态光学与光子技术国家重点实验室;
  • 出版日期:2018-06-15
  • 出版单位:光谱学与光谱分析
  • 年:2018
  • 期:v.38
  • 基金:国家自然科学基金项目(41573056,41473065);; 山东省自然科学基金项目(ZR2015DM001,JQ201511);; 西安光机所瞬态光学与光子技术国家重点实验室(开放基金)研究课题(SKLST201504)资助
  • 语种:中文;
  • 页:GUAN201806055
  • 页数:7
  • CN:06
  • ISSN:11-2200/O4
  • 分类号:272-278
摘要
多源数据融合能在一定程度上扩展数据信息量,更利于建立准确和稳健的分析模型。行星探测中常采用多个载荷协同分析同一目标,因此利用多载荷数据融合辨别分析火星矿物具有重要科学意义和应用前景。分别采用可见近红外(Vis-NIR)反射光谱和拉曼(Raman)散射光谱两种技术手段测量了火星表面主要矿物(硅酸盐、硫酸盐、碳酸盐)的光谱特征曲线,并对获取的光谱数据进行基线校正、Savitzky-Golay平滑以及标准矢量归一化(SNV)等必要的数据预处理。根据光谱特征,首先选取样品Vis-NIR和Raman数据信息丰富、信噪比高、光谱信号重叠小的波段(Vis-NIR:430~2 430nm,Raman:130~1 100cm~(-1)),然后运用软独立建模分类法(SIMCA)、主成分分析法-K最邻近分类法(PCA-KNN)分别建立基于Vis-NIR,Raman及两者融合(累加融合、串联融合)的矿物聚类分析模型。采用SIMCA算法的矿物聚类准确率由单一光谱建模的72.6%(Vis-NIR),90.7%(Raman)提升为融合建模的96.3%(累加融合)和98.1%(串联融合);采用PCA-KNN的准确率由单一光谱建模的68.9%(Vis-NIR),72.9%(Raman)提升为融合后的80.3%(累加融合)和92.6%(串联融合)。实验结果表明:光谱融合能够发挥Vis-NIR,Raman各自的数据优势,所建火星表面相关矿物分类模型的预测准确度更高。该研究为我国火星探测任务奠定了岩石分类方法基础。
        Multi-source data fusion is a powerful method to combine data from multiple sources to improve the potential values and interpretation performances of the source data.Multi-payload collaborative analysis is regularly used to detect the same target in planetary exploration.Therefore,it is of great significance and potential application to use spectral fusion to establish a more accurate and robust clustering analysis model for Martian minerals identification.In this paper,the spectral characteristics of the main Martian-related minerals were analyzed by using both visible near-infrared(Vis-NIR)reflectance spectroscopy and Raman spectroscopy.And some data pre-processing methods such as baseline correction,Savitzky-Golay smoothing,standard normal variate(SNV)scaling were used to produce a high-quality representation of the spectral data.Firstly,the informationrich spectral bands with higher signal-to-noise ratio and less overlapping were selected(i.e.,Vis-NIR:430~2 430 nm;Raman:130~1 100 cm-1)for the clustering analysis.Secondly,soft independent method of class analogy(SIMCA)and principal component analysis-K-nearest neighbor(PCA-KNN),were respectively built based on selected Vis-NIR,Raman and two kinds of their fusion data(i.e.,coaddition fusion and concatenation fusion),respectively.The accuracy of SIMCA model was enhanced from 72.6%(Vis-NIR)and 90.7%(Raman)to 96.3%(coaddition fusion)and 98.1%(concatenation fusion).The accuracy of PCA-KNN model was improved from 68.9%(Vis-NIR)and 72.9%(Raman)to 80.3%(coaddition fusion)and92.6%(concatenation fusion),respectively.The results indicate that the fused Raman/Vis-NIR data can improve the classification model's accuracy of Martian-related minerals which will lay the foundation of quick rock classification for future Mars exploration.
引文
[1]WU Xiao-li,LI Yan-jun,WU Tie-jun(武晓莉,李艳君,吴铁军).Chinese Journal of Analytical Chemistry(分析化学),2007,35(12):1716.
    [2]LI Zhi-gang,PENG Si-long,YANG Ni,et al(李志刚,彭思龙,杨妮,等).Chinese Journal of Analytical Chemistry(分析化学),2016,44(3):437.
    [3]JIAO Ai-quan(焦爱权).Journal of Food Science and Biotechnology(食品与生物技术学报),2016,35(4):357.
    [4]Casale M,Sinelli N,Oliveri P,et al.Talanta,2010,80(5):1832.
    [5]Bi Y F,Zhang Y,Yan J W,et al.Plasma Science and Technology,2015,17(11):923.
    [6]Wu Z,Wang A,Ling Z.Earth and Planetary Science Letters,2016,452:123.
    [7]Wang A,Freeman J J,Jolliff B L.Journal of Raman Spectroscopy,2015,46(10):829.
    [8]Ling Z C,Wang A,Jolliff B L.Icarus,2011,211(1):101.
    [9]Buzgar N,Buzatu A,Sanislav I V.Analele Stiintifice de Universitatii AI Cuza din Iasi.Sect.2,Geologie,2009,55(1):5.
    [10]Haaland D.Vibrational Spectroscopy,1991,1(3):325.
    [11]Miyake M,Minato I,Morikawa H,et al.American Mineralogist,1978,63(5-6):506.
    [12]Harri A M,Genzer M,Kemppinen O,et al.Journal of Geophysical Research:Planets,2014,119(9):2132.
    [13]Rivera-Valentin E G,Chevrier V F.Icarus,2015,253:156.
    [14]Liu Y,Wang A,Freemen J J.Lunar and Planetary Science Conference,2009,40:2128.
    [15]WANG Wen-xiu,PENG Yan-kun,XU Tian-feng,et al(王文秀,彭彦昆,徐田锋,等).Spectroscopy and Spectral Analysis(光谱学与光谱分析),2016,36(12):4001.
    [16]Moros J,Laserna J J.Talanta,2015,134:627.
    [17]Duca D,Mancini M,Rossini G,et al.Energy,2016,117:251.
    [18]Zhu X,Suk H,Shen D,et al.NeuroImage,2014:91.
    [19]Zhu X,Suk H,Shen D,et al.Computer Vision and Pattern Recognition,2014:3089.

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