光谱学与光谱分析
光譜學與光譜分析
광보학여광보분석
SPECTROSCOPY AND SPECTRAL ANALYSIS
2014年
5期
1421-1424
,共4页
蔡江辉%杨海峰%赵旭俊%张继福
蔡江輝%楊海峰%趙旭俊%張繼福
채강휘%양해봉%조욱준%장계복
局部离群%光谱特征线%子空间
跼部離群%光譜特徵線%子空間
국부리군%광보특정선%자공간
Local outlier%Spectra characteristic line%Subspace
探索海量的M型恒星中具有磁活动、巨星等较特殊、稀有的天体,对于后续观测、银河系结构、演化等科学研究具有重要的意义,针对M型恒星光谱特征线出现在子空间中的局部偏离,设计并实现了晚型恒星离群数据挖掘系统。首先采用稀疏因子和稀疏度系数度量样本在属性空间上的分布特征,并在此基础上对M型恒星光谱特征线进行离散化、降维等预处理,获得光谱子空间;然后采用微粒群算法搜索离群子空间,并证认子空间内光谱是否离群;此外,选择SDSS M型光谱特征线指数集为样本,实验分析了稀疏因子和稀疏度系数的设置对离群结果的影响,并将离群挖掘结果与SDSS提供光谱型等参数对照,表明利用该系统实现晚型恒星光谱特征线局部离群数据挖掘是可行并有价值的。
探索海量的M型恆星中具有磁活動、巨星等較特殊、稀有的天體,對于後續觀測、銀河繫結構、縯化等科學研究具有重要的意義,針對M型恆星光譜特徵線齣現在子空間中的跼部偏離,設計併實現瞭晚型恆星離群數據挖掘繫統。首先採用稀疏因子和稀疏度繫數度量樣本在屬性空間上的分佈特徵,併在此基礎上對M型恆星光譜特徵線進行離散化、降維等預處理,穫得光譜子空間;然後採用微粒群算法搜索離群子空間,併證認子空間內光譜是否離群;此外,選擇SDSS M型光譜特徵線指數集為樣本,實驗分析瞭稀疏因子和稀疏度繫數的設置對離群結果的影響,併將離群挖掘結果與SDSS提供光譜型等參數對照,錶明利用該繫統實現晚型恆星光譜特徵線跼部離群數據挖掘是可行併有價值的。
탐색해량적M형항성중구유자활동、거성등교특수、희유적천체,대우후속관측、은하계결구、연화등과학연구구유중요적의의,침대M형항성광보특정선출현재자공간중적국부편리,설계병실현료만형항성리군수거알굴계통。수선채용희소인자화희소도계수도량양본재속성공간상적분포특정,병재차기출상대M형항성광보특정선진행리산화、강유등예처리,획득광보자공간;연후채용미립군산법수색리군자공간,병증인자공간내광보시부리군;차외,선택SDSS M형광보특정선지수집위양본,실험분석료희소인자화희소도계수적설치대리군결과적영향,병장리군알굴결과여SDSS제공광보형등삼수대조,표명이용해계통실현만형항성광보특정선국부리군수거알굴시가행병유개치적。
In M star population ,some special objects ,which may be of magnetic activity ,may be giant stars ,or may be of other rare properties ,are very important for the follow-up observation and the scientific research on galactic structure and evolution . For local bias of M-type star spectral characteristic lines contained in subspace ,a late-type star spectra outlier data mining system is given in the present paper .Firstly ,for the sample of M stellar spectral characteristic lines indices ,its distribution characteris-tics in attribute spaces are measured by using the sparse factor and sparsity coefficient ,and then this sample is discretized and di-mension-reduced to the spectral subspace .Secondly ,local outlier subspaces are extracted by PSO (particle swarm optimization ) algorithm and identified .Additionally ,the effects of sparse coefficient and sparse factor on the number of outliers are discussed by experiments on the sample of SDSS M stellar spectral line index set ,and the outliers are compared with spectral type provided by SDSS .In this way ,the feasibility and value of this system were validated .