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Comparison between photogrammetric and bistatic-radar slope frequency distributionsA comparison was made of the results for lunar surface roughness estimates and slope frequency distributions obtained by using photogrammetric techniques with those obtained by using bistatic radar. Three topics were discussed: (1) the form of the slope frequency distributions, (2) the change of roughness estimates of the lunar surface with scale, and (3) the magnitude of surface roughness.
Document ID
19740010367
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Moore, H. J. (Geological Survey Washington, DC, United States)
Tyler, G. L. (Stanford Univ.)
Date Acquired
August 7, 2013
Publication Date
January 1, 1973
Publication Information
Publication: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.
Subject Category
Communications
Accession Number
74N18480
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19740010315Collected WorksApollo 17 Preliminary Science Report
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