Modeling the Reflectance of the Lunar Regolith by a New Method Combining Monte Carlo Ray Tracing and Hapke’s Model with Application to Chang’E-1 IIM Data
Figure 19
The 1D results of removing the influence of the topography applying our model (in all figures, -axis is wavelength (nm) and -axix is the reflectance). (a) simulated diffusion results; (b) -profile of CE-1 IIM data (nm); (c) the result using the inverse model of our method to CE-1 IIM data. The featuring parts to show the changes after dividing the diffusion are circled.
