Three-dimensional (3-D) maps of the nearside and polar regions of the Moon
can be obtained with an Earth-based radar interferometer. This paper descri
bes the theoretical background, experimental setup, and processing techniqu
es for a sequence of observations performed with the Goldstone Solar System
Radar in 1997. These data provide radar imagery and digital elevation mode
ls of the polar areas and other small regions at similar to 100 m spatial a
nd similar to 50 m height resolutions. A geocoding procedure relying on the
elevation measurements yields cartographically accurate products that are
free of geometric distortions such as foreshortening.