期刊文献+

顾及太空风化效应的虹湾地区矿物含量反演

Lunar Mineral Abundance Inversion of Sinus Iridum Considering Space Weathering Effect
原文传递
导出
摘要 月表矿物含量反演是研究月球地质起源和演化的关键.太空风化作用普遍发生在月球表面,对矿物纯净光谱造成了不可忽视的影响,它弱化光谱吸收特征,降低反射率,影响矿物含量遥感反演精度.基于Relab光谱库和Hapke辐射传输模型,将月表4种矿物(单斜辉石、斜方辉石、斜长石、橄榄石)的二向性反射率转换成同向性的单次散射反照率,然后计算矿物的光学常数;再根据亚微观金属铁SMFe(submicroscopic metallic iron)的质量分数模拟6种不同程度太空风化效应,得到端元矿物的反射率光谱;最后基于上述方法,利用多端元线性分解方法和M3(moon mineralogy mapper,月球矿物绘图仪)高光谱数据反演不同风化程度下的矿物含量,得到月表虹湾地区辉石、斜长石、橄榄石3种矿物的含量分布.实验表明,利用多端元线性分解可以有效模拟太空风化效应对矿物光谱的影响,是研究太空风化效应影响下矿物识别及含量反演的一种行之有效的方法. The inversion of lunar minerals is critical to study the Moon's geological origin and evolution.Space weathering generally occurs on the surface of the Moon with an assignable influence on the pure mineral spectra,which obscures the reflectance spectra feature of minerals and reduces the overall reflectance.The effect of space weathering should be removed when accurately investigating the lunar minerals using remote sensing technology.The level of the space weathering is proportional to the mass fraction of submicroscopic metallic iron(SMFe).In this paper,the authors firstly transform the bidirectional reflectance into the isotropic single scattering albedo of four endmember minerals(clinopyroxene,orthopyroxene,plagioclase and olivine)in the Relab spectral library based on Hapke radiative transfer model,secondly,calculate the optical constants and absorption coefficient of each mineral,then simulate the reflectance spectra of these minerals under six space weathering levels according to SMFe mass fraction,thus we obtain endmember mineral reflectance under different space weathering levels.Finally we inverse mineral abundance with six multi-endmember linear unmixing models and the M3(moon mineralogy mapper)hyperspectral data and obtain the inversion abundance and distribution of pyroxene,plagioclase and olivine in Lunar Sinus Iridum.The results show that using multi-endmember linear unmixing method can effectively simulate the effects of space weathering on mineral spectra,and it is an useful way of mineral identification and abundance inversion with hyperspectral under the space weathering.
作者 郭艳 张琪 李婵 董晓莹 刘福江 Guo Yan Zhang Qi Li Chan Dong Xiaoying Liu Fujiang(College of Computer Science, China University of Geosciences, Wuhan 430074, China Faculty of Information Engineering, China University of Geosciences, Wuhan 430074, China Xinjiang Academy of Surveying and Mapping, Urumqi 830002, China)
出处 《地球科学(中国地质大学学报)》 EI CSCD 北大核心 2016年第12期2100-2108,共9页 Earth Science-Journal of China University of Geosciences
基金 中央高校基本科研业务费专项资金项目(No.CUGL130261) 湖北省2014年面上自然科学基金项目(No.2014CFB911) 国家"十二五"国家高技术研究发展计划课题("863"课题)(No.2014AA123001)
关键词 太空风化 Hapke模型 虹湾 矿物 反演 space weathering Hapke model Sinus Iridum minerals inversion
  • 相关文献

参考文献5

二级参考文献123

  • 1LIU FuJiang,QIAO Le,LIU Zheng,YANG Rong,SHI JinPing,ZHANG Ying,WU WeiLong.Estimation of lunar titanium content: Based on absorption features of Chang’E-1 interference imaging spectrometer (ⅡM)[J].Science China(Physics,Mechanics & Astronomy),2010,53(12):2136-2144. 被引量:8
  • 2薛彬,杨建峰,赵葆常.月球表面主要矿物反射光谱特性研究[J].地球物理学进展,2004,19(3):717-720. 被引量:19
  • 3Mouelic S L, Yangevin Y, Erard S. A New Data Reduction Approach for the Clementine Data Set: Application to Aristillus, Aristarchus and Kepler[J].Journal of Geophysical Research,1999, 104(E2) : 3833-3843.
  • 4Mustard J F, Pieters C M, Photometric Phase Functions of Common Geologic Minerals and Applications to Quantitative Analysis of Mineral Mixture Reflectance Spectra [ J ]. Journal of Geophysical Research, 1989, 94( B10), 13619 - 13634.
  • 5Johnson P E, Smith M O, George S T, et al. Simple Algorithms for Remote Determination of Mineral Abundances and Particle Sizes from Reflectance Spectra [ J ]. Journal of Geophysical Research, 1992, 97 ( E2 ), 2649 - 2657.
  • 6Yan B K, Liu S W, Wang R S, et al, Experiment Study on Quantitative Retrieval of Mineral Abundances from Reflectance Spectra [ A ]. Proceedings of SPIE [ C ]. 2008, 7123 : 7123 - 1 - 7123 - 11.
  • 7Pieters C M, Hiroi T. RELAB ( Reflectance Experiment Laboratory) : A NASA Multispectrat Spectroscopy Facility[ A]. 35th Annual Lunar and Planetary Science Conference[ C ]. 2004, 1721 -1722.
  • 8Lucey P G, Blewett D T, Hawke B R. Mapping the FeO and TiO2 Content of the Lunar Surface with Muhispectral Imagery[J]. Journal of Geophysical Research, 1998,103 (E2) :3679 - 3699.
  • 9Clark R N, Roush T L. Reflectance Spectroscopy: Quantitative Analysis Techniques for Remote Sensing Application[ J]. Journal of Geophysical Research, 1984,89 ( B7 ) : 6329 - 6340.
  • 10Adams J, McCord T. Optical Properties of Mineral Separates, Glass, and Anorthositic Fragments from Apollo Mare Samples [ A]. Proceedings of the Lunar Science Conference[ C]. 1971,2 : 2183 -2195.

共引文献23

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部