Topographic profiles for planetary wrinkle ridges have been compiled from LTO topographic maps for the Moon and from monoscopic photoclinometry data for Mars. The topographic data have been used to provide an approximation of the amount of shortening across a ridge due to both folding and faulting.
Lunar and Planetary Science Conference Proceedings
- Pub Date:
- Lunar Surface;
- Mars Surface;
- Lunar and Planetary Exploration