首页|基于迁移成分分析的火星LIBS光谱数据定量分析方法

基于迁移成分分析的火星LIBS光谱数据定量分析方法

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火星土壤中的元素成分及其含量是地质演化历史的重要记录载体,可以反映火星环境、气候等信息,因此对火星土壤进行检测和分析具有重要意义.本研究提出了一种迁移成分分析(TCA)结合随机森林(RF)的LIBS定量分析方法,用于预测火星在轨标样的K2O质量分数.选取了383种标样在模拟火星环境下的光谱数据作为训练集,6种在轨标样在真实火星环境下的光谱数据作为测试集.使用训练集建立决策树为250棵的RF模型,其平均绝对误差(EMA)、均方根误差(ERMS)和平均相对误差(EMR)分别为1.117、1.148和10.104,预测性能较差.为了缩短训练集和测试集光谱数据之间的分布距离,建立TCA-RF模型并调整参数.相较于RF模型,TCA-RF模型的EMA、ERMS和EMR分别降低了90.7%、88.1%和94.1%.而与参考模型MOC(一种偏最小二乘法结合独立成分分析的模型)对比,TCA-RF模型在预测测试集中K2O质量分数≥0.15%的样品时,其准确性高于MOC模型.因此TCA-RF模型可以为探测火星土壤元素含量提供新的技术手段.
Quantitative analysis method of Mars LIBS spectral data based on transfer component analysis
The elemental composition and content in Martian soil are important record carrier of geological evolutionary history,which can reflect the Martian environment,climate,and other information,so it is of great significance to detect and analyze Martian soil.A LIBS quantitative analysis method based on the combination of transfer component analysis(TCA)with random forest(RF)is proposed to predict the K2O mass fraction of Mars on-orbit standards.The spectral data of 383 standard samples in simulated Martian environment were selected as the training set,and the spectral data of 6 on-orbit standard samples in real Martian environment were selected as the test set.The RF model with 250 decision trees was established using the training set,and the mean absolute error(EMA),the root mean square error(ERMS)and the mean relative error(EMR)were 1.117,1.148 and 10.104,respectively,indicating poor prediction performance.To shorten the distribution distance between the spectral data of the training set and the test set,the TCA-RF model is established and the parameters are adjusted.Compared with the RF model,the EMA ERMS and EMR of the TCA-RF model are reduced by 90.7%,88.1%and 94.1%respectively.Compared with the reference model MOC,a model based on the partial least squares regression combined with independent component analysis,the TCA-RF model is more accurate than the MOC model in predicting samples with K2O mass fraction higher than or equal to 0.15%in the test set.Therefore,it is indicated that the TCA-RF model can provide a new technical means for detecting the content of soil elements on Mars.

spectroscopylaser-induced breakdown spectroscopyMars explorationtransfer component analysisquantitative analysis

吴敏浩、陈靖、郑子宇、李宣佑、王爽、丁宇

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南京信息工程大学江苏省大数据分析技术重点实验室,江苏 南京 210044

南京信息工程大学江苏省大气环境与装备技术协同创新中心,江苏 南京 210044

南京信息工程大学江苏省气象能源利用与控制工程技术研究中心,江苏 南京 210044

光谱学 激光诱导击穿光谱 火星探测 迁移成分分析 定量分析

国家自然科学基金福建省自然科学基金江苏省大型科学仪器开放共享课题

621051602023J05303TC2023A020

2024

量子电子学报
中国光学学会基础光学专业委员会 中国科学院合肥物质科学研究院

量子电子学报

CSTPCD北大核心
影响因子:0.67
ISSN:1007-5461
年,卷(期):2024.41(3)
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