Estimating minerals abundance from reflectance spectra is one of the fundamental goals of remote sensing lunar exploration, and the main difficulties are the complicated mixing law of minerals spectrum and spectral features being sensitive to several kinds of factors such as topography, particle size and roughness etc. A method based on spectral unmixing was put forward and tested in the present paper. Before spectra are unmixed the spectral continuum is removed for clarifying and strengthening spectral features. The absorption features and reflectance features (the upward curving parts of spectra between absorption features) are integrated for unmixing to improve the unmixing performance. The Hapke model was used to correct unmixing error due to nonlinear mixing of minerals spectra. Forty three mixed spectra of olivine, clinopyroxene, hypersthene and plagioclase were used to validate the above method. The four minerals abundance was estimated under the conditions of being unaware of endmember spectra used to mix, granularity and chemical composition of minerals. Residual error, abundance error and correlation coefficient between retrieved and true abundance were 5. 0 Vol%, 14. 4 Vol% and 0. 92 respectively. The method and result of this paper could be referred in the lunar minerals mapping of imaging spectrometer data such as M3.%室内测量了十六种浮游植物的吸收-衰减光谱,及其粒径分布和叶绿素a浓度.研究结果表明,粒径和单位细胞叶绿素浓度是影响浮游植物吸收和衰减系数量值的两个重要因素;粒径是决定衰减光谱形状的重要因子之一,粒径与衰减光谱斜率之间存在非单调的变化关系;粒径不是影响浮游植物吸收光谱的蓝-红波段比和光谱斜率的决定性因子,但是,藻细胞密度与粒径平方的乘积是决定吸收光谱斜率的关键量.适用于均匀球体颗粒的Mie散射理论能对粒径与浮游植物吸收光谱和衰减光谱间的相关关系进行阐释,该文研究的藻类其非均匀球体结构并没有从根本上改变粒径与吸收—衰减光谱间存在的内在规律.
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