Author/Authors :
Glenn Y. Yokota، نويسنده , , J. Haruyama، نويسنده , , Makio C. Honda، نويسنده , , T. Morota، نويسنده , , M. Ohtake ، نويسنده , , H. Kawasaki، نويسنده , , S. Hara، نويسنده , , K. Hioki، نويسنده , , the LISM Working Group، نويسنده ,
Abstract :
Quantifying surface roughness may contribute significantly in the stratigraphic study of the Moon. We demonstrate the root mean square (RMS) deviation method as an indicator of topographic roughness on a kilometer scale, using stereo images from an Apollo Mapping Camera in a Digital Terrain Model, and compare three regions in the lunar highlands.
