ABSTRACT
Horizontal Surface Esh .................................................................... 165 7.3.5 Total Irradiance on a Horizontal Surface Eh ............................... 165 7.3.6 Binary Coefficient to Control Cast Shadow Θ ........................... 167
7.4 Elevation of the Topographic Correction Results .................................. 167 7.5 Albedo Solving Based on Hapke’s Model .............................................. 168 7.6 Spectral Mixing Analysis .......................................................................... 168 7.7 Results .......................................................................................................... 169 7.8 Conclusion and Discussion ...................................................................... 170 Symbols ................................................................................................................ 171 References ............................................................................................................. 172
7.1.1 Lunar Minerals
Lunar minerals have directly led to the early evolution of lunar crust and interacting geological processes. But the composition of lunar surface is relatively simple, primarily dominated by clinopyroxene, orthopyroxene, plagioclase, olivine, ilmenite, and agglutinitic glass (Papike et al. 1991; Taylor et al. 2001). The recent lunar missions, for example, SELenological and ENgineering Explorer (SELENE) Kaguya, Chang’E-1, and Chandrayaan-1, provided new opportunities to explore and understand these issues (Jin et al. 2013; Wei et al. 2013).
