Author/Authors :
Muinonen، نويسنده , , K and Shkuratov، نويسنده , , Elena Yu. and Ovcharenko، نويسنده , , A and Piironen، نويسنده , , J and Stankevich، نويسنده , , D and Miloslavskaya، نويسنده , , O and Kaasalainen، نويسنده , , S and Josset، نويسنده , , J.-L، نويسنده ,
Abstract :
The lunar surface reveals a sharp opposition effect, which is to be explained by the shadowing and coherent backscattering mechanisms. Generalizing the radiative transfer theory via Monte Carlo methods, we are carrying out studies of backscattering in regolith-like scattering media. We have also started systematic laboratory measurements of structural simulators of lunar regolith. The SMART-1 AMIE and D-CIXS/XSM experiments provide us a unique opportunity for a simultaneous multiwavelength study of the lunar regolith close to opposition, since the SMART-1 spacecraft will pass over several different types of lunar surface at zero phase angles. Results of our theoretical and laboratory investigations can be used as a basis to interpret the SMART-1 AMIE and D-CIXS/XSM experiments. In particular, it seems to be possible to estimate regional variations of regolith particle volume fraction and their size. A short review of observational, experimental and theoretical works is also presented here.
