Applications to Lunar Remote Sensing - 3D Computer Vision: Efficient Methods and Applications - page 331

Fig. 8.18 Lunar Orbiter images of lunar mare domes. Image credit: NASA/USGS. ( a )LunarOr-
biter image IV-178-H1, showing an oblique view on Mare Undarum with its dome field. North is
indicated by the arrow in the upper right of the image , the undistorted image scale in the lower
right .( b ) Lunar Orbiter image IV-163-H2, showing the lunar dome complex Mons Rümker. The
labels R1-R6 indicate individual volcanic edifices

Fig. 8.19 Section from Apollo 15 orbital image AS15-97-13252, showing an oblique view of the
lunar dome complex Mons Rümker from southern direction. Image credit: NASA

pixel resolution of 140 m. 6 The original images were mapped to a simple cylindrical
projection. A detailed description of the M 3 instrument is given by Pieters et al.
( 2009 ). Figures 8.20 c, e, and f are excerpts from the Lunar Reconnaissance Orbiter
Camera (LROC) WAC global mosaic. 7 A detailed description of the LROC WAC

6 The Chandrayaan-1 M 3

hyperspectral image data archive is accessible at http://m3.jpl.nasa.gov/

m3data.html .
7 The LROC WAC image archive is accessible at http://wms.lroc.asu.edu/lroc . TheLROCWAC
global mosaic is available at http://wms.lroc.asu.edu/lroc/wac_mosaic .