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Mare Crisium area topography - A comparison of earth-based radar and Apollo mapping camera resultsAn earth-based radar topography (ERT) map has been constructed of the Mare Crisium area. Systematic and random sources of error are discussed. A comparison between the ERT map and Lunar Topographic Orthophotomaps shows a random mean discrepancy of less than 100 m between the two maps, except for small-scale (20 km or less in diameter) features, where systematic smoothing reduces the ERT elevation contrast
Document ID
19790048493
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Zisk, S.
(Haystack Observatory Westford, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Mare Crisium: The view from Luna 24; Conference
Location: Houston, TX
Start Date: December 1, 1977
End Date: December 3, 1977
Sponsors: NSF
Accession Number
79A32506
Funding Number(s)
CONTRACT_GRANT: NSG-7197
CONTRACT_GRANT: NSF AST-75-14701
Distribution Limits
Public
Copyright
Other

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