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Remote sensing and photogrammetric studies: Part C: comparison between photogrammetric and bistatic-radar slope-frequency distributions

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Abstract

Stereoscopic photographs taken by the metric and panoramic cameras can be used to obtain information on the roughness and slope-frequency distributions of lunar surfaces (see appendix to this part). Bistatic radar on board Apollo 14, 15, and 16 spacecraft may also be used to obtain information on lunar surface roughness at two wavelengths—13 cm (S-band) and 116 cm (VHF).

Additional Publication Details

Publication type:
Book chapter
Publication Subtype:
Book Chapter
Title:
Remote sensing and photogrammetric studies: Part C: comparison between photogrammetric and bistatic-radar slope-frequency distributions
Series number:
330
Year Published:
1973
Language:
English
Publisher:
National Aeronautics and Space Administration
Publisher location:
Washington, D.C.
Contributing office(s):
Astrogeology Science Center
Description:
10 p.
Larger Work Type:
Report
Larger Work Subtype:
Federal Government Series
Larger Work Title:
Apollo 17 preliminary science report (NASA SP-330)
First page:
33-17
Last page:
33-26
Other Geospatial:
Moon