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Topographic models of the Humboldtianum Basin and Mare Crisium from Galileo stereo image data

Oberst, J. (1996) Topographic models of the Humboldtianum Basin and Mare Crisium from Galileo stereo image data. International Moon Workshop, Berlin, Jan. 31 - Feb. 2, 1996.

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Abstract

Galileo SSI multi-look angle 1 km/pixel images obtained during the Earth-Moon flyby in 1992 were analyzed to derive a DTM (Digital Terrain Model) of the lunar nearside northern hemisphere. The nominal camera pointing data were corrected by using control points and a bundle block adjustment procedure. Digital image matching was used to measure stereo effects in image pairs. The resulting terrain model features 2000 m grid spacing and 500 m height resolution. Prominent selenographic features visible in the terrain model are the Humboldtianum basin and Mare Crisium. The new topographic data superior to the Clementine Laser Altimeter data in terms of spatial resolution and noise level and may be crucial in our understanding of the formation of these large impact basins.

Document Type:Conference or Workshop Item (Speech)
Additional Information: LIDO-Berichtsjahr=1996,
Title:Topographic models of the Humboldtianum Basin and Mare Crisium from Galileo stereo image data
Authors:
AuthorsInstitution or Email of Authors
Oberst, J.UNSPECIFIED
Date:1996
Status:Published
Event Title:International Moon Workshop, Berlin, Jan. 31 - Feb. 2, 1996
HGF - Research field:UNSPECIFIED
HGF - Program:Space (old)
HGF - Program Themes:W EW - Erforschung des Weltraums
DLR - Research area:UNSPECIFIED
DLR - Program:W EW - Erforschung des Weltraums
DLR - Research theme (Project):UNSPECIFIED
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Institut für Planetenerkundung
Deposited By: elib DLR-Beauftragter
Deposited On:02 Apr 2006
Last Modified:27 Apr 2009 09:50

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