The 400 meters: Stereo topographic mapping of the bright terrain-dark terrain boundary on Ganymede
P Schenk, K Jones, B Fessler - AAS/Division for Planetary …, 1996 - ui.adsabs.harvard.edu
The resurfacing of Ganymede in the form of bright terrain remains a central issue in
understanding why this body is so different from neighboring Callisto. Few useful constraints
on the elevation of bright terrain relative to dark terrain exist. In 1994, LPI began
development of stereogrammetric auto-correlation software designed to produce
topographic maps of the icy satellites using Voyager images. Reliable DEMs are now
possible on Ganymede. Fault-bounded lanes of bright terrain near the south pole show …
understanding why this body is so different from neighboring Callisto. Few useful constraints
on the elevation of bright terrain relative to dark terrain exist. In 1994, LPI began
development of stereogrammetric auto-correlation software designed to produce
topographic maps of the icy satellites using Voyager images. Reliable DEMs are now
possible on Ganymede. Fault-bounded lanes of bright terrain near the south pole show …
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