摘要
分析了矿物在可见光及近红外区光谱生成的机理,介绍了月球表面最为主要的四种矿物———辉石、斜长石、橄榄石、钛铁矿,并分析了它们各自光谱特征及生成原因,讨论了造成同种矿物光谱差异的原因,给出了它们各自的标志性特征.
The mechanism of the mineral spectrum on Visable-NearInfrared regions is analysed. The major four minerals (pyroxenes, plagioclase, olivine, ilmenite) on the surface of lunar and their spectral features are introduced. The reasons to cause the difference of the same kind of mineral spectrum are discussed. The diagnostic features of each minerals are developed.
出处
《地球物理学进展》
CSCD
2004年第3期717-720,共4页
Progress in Geophysics
基金
国家自然科学基金项目(40301031)资助.