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Page 5638, results 140926 - 140950

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Publication Extents

Not all publications have extents, not all extents are completely accurate
Photogeology: Part F: reinterpretations of the northern Nectaris Basin
Don E. Wilhelms
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
Geologic units of the Nectaris Basin rim have been interpreted as partly impact and partly volcanic in origin (refs. 29-4, 29-21, 29-35, 29-38, and 29-39). An exclusively volcanic origin was proposed for the material in the vicinity of the Apollo 16 landing site, slightly northwest of the Nectaris Basin (ref....
Photogeology: Part W: Apollo 16 landing site: summary of Earth-based remote sensing data
S.H. Zisk, Harold Masursky, D.J. Milton, G. G. Schaber, R.W. Shorthill, T.W. Thompson
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The purpose of the infrared (IR) and radar study of the Apollo data is to establish lunar surface conditions in the vicinity of the orbital tracks of the Apollo command modules during the J-series missions. Correlations and comparisons between the Earth-based radar observations, IR observations, and other data will be...
Photogeology: Part Y: physical and geological aspects of heiligenschein measurements
Robert L. Wildey
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
Heiligenschein is the upsurge in reflected brightness as zero-phase angle is approached. For the first time, an effort has been made to investigate the diagnostic value of the heiligenschein photometric magnitude on a statistically significant scale. This investigation was performed by using the vertical photography of the Apollo 16 metric...
Photogeology: Part X: calibration of radar data from Apollo 16 results
S.H. Zisk, H. J. Moore
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
Orbital and surface photography collected during the Apollo 16 mission can be used to calibrate existing Earth-based, high-resolution radar maps of the lunar surface. The absence of any theoretical treatment of the radar backscatter from irregular rocks has prevented the assignment of radar-echo cross sections to specific size distributions of...
Orbital-science investigation: Part F: regional geology of Hadley Rille
Keith A. Howard, James W. Head
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
Study of the sinuous Hadley Rille (fig. 25-45) was a primary goal of the Apollo 15 mission. Local geology of the rille near the landing site is described in section 5 of this report. Preliminary study of orbital photography from Hasselblad, metric, and panoramic cameras makes possible a description of...
Photogeology: Part J: ranger and other impact craters photographed by Apollo 16
H. J. Moore
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The Apollo 16 crew photographed an unusual variety of impact craters, including the two craters produced by the impacts of Ranger 7 and 9 spacecraft, small craters produced by boulders as they bounced downslope, craters with marked bilateral symmetry, and primary craters with a wide range of morphologies and sizes....
Orbital-science investigation: Part J: preliminary geologic map of the region around the candidate Proclus Apollo landing site
Don E. Wilhelms
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
The Proclus Crater region was mapped to test the value, for photogeologic mapping purposes, of Apollo 15 metric photographs and to estimate the scientific value of the area as a potential landing site. A metric photographic frame (fig. 25-67) serves as a base for a map of the region around...
Photogrammetry and altimetry: Part B: photogrammetry using Apollo 16 orbital photography
Sherman S.C. Wu, Francis J. Schafer, Raymond Jordan, Gary M. Nakata
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The Apollo 15 and 16 metric and panoramic cameras have provided photographs for accurate topographic portrayal of the lunar surface using photogrammetric methods. In turn, quantitative morphologic analyses of topographic results are invaluable aids in the interpretation of the geologic processes....
Photogrammetry and altimetry: Part C: frequency distributions of lunar slopes
Sherman S.C. Wu, H. J. Moore
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The metric and panoramic cameras aboard the Apollo 16 spacecraft provided photographs on which photogrammetric techniques may be used to obtain precise measurements of horizontal distances and elevations. These measurements of horizontal distances and elevations. These measurements may in turn be used to obtain slope-frequency distributions of lunar surfaces at...
Photogeology: Part L: crater morphometry
Richard J. Pike
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
Morphometric analysis of lunar craters (ref. 29-75) complements the more traditional photointerpretive study of crater morphology. These two indirect approaches to the scientific investigation of lunar craters continue to be productive because the preferred alternative method, direct field examination of specific large craters, is not being undertaken in the current...
Orbital-science investigation: Part C: photogrammetry of Apollo 15 photography
Sherman S.C. Wu, Francis J. Schafer, Raymond Jordan, Gary M. Nakata, James L. Derick
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
Mapping of large areas of the Moon by photogrammetric methods was not seriously considered until the Apollo 15 mission. In this mission, a mapping camera system and a 61-cm optical-bar high-resolution panoramic camera, as well as a laser altimeter, were used. The mapping camera system comprises a 7.6-cm metric terrain...
Principal facts for gravity stations in the Bearpaw Mountains and vicinity, Montana
Donald L. Peterson, William L. Rambo
1972, Report
Observed gravity values, station locations, terrain corrections, and Bouguer gravity data are provided in tabular form for approximately 500 gravity observations in north-central Montana. These data were used in preparation of -- Peterson, Donald L. and Rambo, William L., 1967, Bouguer gravity anomaly map of the Bearpaw Mountains and vicinity,...
Preliminary geologic investigation of the Apollo 16 landing site
W.R. Muehlberger, R. M. Batson, E. L. Boudette, C.M. Duke, R. E. Eggleton, D. P. Elston, A. W. England, V. L. Freeman, M. H. Hait, T.A. Hall, J.W. Head, C. A. Hodges, H. E. Holt, E.D. Jackson, J.A. Jordan, K.B. Larson, D.J. Milton, V. S. Reed, J. J. Rennilson, G. G. Schaber, J.P. Schafer, L. T. Silver, D. Stuart-Alexander, R. L. Sutton, G.A. Swann, R.L. Tyner, G. E. Ulrich, H. G. Wilshire, E.W. Wolfe, J.W. Young
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The Apollo 16 landing site in the lunar central highlands encompassed terra plains and adjacent mountainous areas of hilly and furrowed terra. These morphologic units, representing important terrane types in the lunar highlands, had been interpreted as volcanic on most premission geologic maps. However, it became apparent during the mission...
Photogeology: Part A: relative ages of some near-side and far-side terra plains based on Apollo 16 metric photography
Laurence A. Soderblom, Joseph M. Boyce
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
The materials of most light or terra plains predate the lunar maria and postdate the Imbrian event. In the vicinity of the Imbrium Basin, these materials have been called the Cayley Formation (ref. 29-3) but because of the subtle diversity of the terra plains over the near side, Whilhelms and...
Principal facts for gravity stations in the area north of the Grand Canyon in Arizona
Peter Popenoe
1972, Report
Observed gravity values, station location, terrain corrections, and Bouguer gravity data are provided in tabular form for approximately 610 gravity observations in northern Arizona. These data were used in preparation of - - Popenoe, Peter, 1968, Complete Bouguer gravity anomaly map of the area north of the Grand Canyon in...
Orbital-science investigation: Part O: regional variations in the magnitude of heiligenschein and causal connections
Robert L. Wildey
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
Approximately 35 reasonably good candidates for specialized photometric studies were found during a thorough examination of the frames exposed by the Apollo 15 metric camera. Of these, the majority was of value in heiligenschein studies (refs. 25-36 to 25-38). A few were of value for limited-interval delineation of the photometric...
Orbital-science investigation: Part G: lineaments that are artifacts of lighting
Keith A. Howard, Bradley R. Larsen
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
Many Apollo 15 orbital photographs, particularly those taken at low Sun-elevation angles, reveal grid patterns of lineaments. In some circumstances, the grid pattern is present in areas where structural control seems unlikely. For example, in an oblique view (fig. 25-52), the ejecta blankets of two fresh impact craters seem to...
Preliminary geologic investigation of the Apollo 15 landing site
G.A. Swann, N. G. Bailey, R. M. Batson, V. L. Freeman, M. H. Hait, J.W. Head, H. E. Holt, K. A. Howard, J.B. Irwin, K.B. Larson, W.R. Muehlberger, V. S. Reed, J. J. Rennilson, G. G. Schaber, D.R. Scott, L. T. Silver, R. L. Sutton, G. E. Ulrich, H. G. Wilshire, E.W. Wolfe
1972, Book chapter, Apollo 15 preliminary science report (NASA SP-289)
The Apollo 15 lunar module (LM) landed at longitude 03°39'20'' E, latitude 26°26'00'' N on the mare surface of Palus Putredinis on the eastern edge of the Imbrium Basin. The site is between the Apennine Mountain front and Hadley Rille. The objectives of the mission, in order of decreasing priority,...
Preliminary examination of lunar samples: Part A: a petrographic and chemical description of samples from the lunar highlands
The Lunar Sample Preliminary Examination Team
1972, Book chapter, Apollo 16 preliminary science report (NASA SP 315)
More than four-fifths of the surface of the Moon consists of a profoundly cratered irregular surface designated terra or highlands by analogy with the terrestrial continents. These terra regions have much higher albedos than the physiographically lower and much smoother mare regions. The difference in albedo can now be ascribed...
Principal facts for gravity stations for the Central Arizona Project
Donald L. Peterson
1972, Report
Observed gravity values, station locations, terrain corrections, and Bouguer gravity data are provided in tabular form for approximately 2460 gravity observations in south-central Arizona. "These data were used in preparation of -- Peterson, Donald L., 1968, Bouguer gravity map of parts of Maricopa, Pima, Pinal, and Yuma Counties, Arizona: U.S....
Principal facts for gravity stations in the Death Valley region, California
Don R. Mabey
1972, Report
Observed gravity values, station locations, terrain corrections, and Bouguer gravity data are provided in tabular form for approximately 1,500 gravity observations in eastern California. Coverage includes Saline Valley, Panamint Valley, Searles Basin, Death Valley, the southern Amargosa Desert and the enclosed and adjoining highlands. These data were used in preparation...