Derivation of topographic feature names in the Apollo 15 landing region
Location and derivation of nomenclature for lunar topographic features in Apollo 15 landing region
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Location and derivation of nomenclature for lunar topographic features in Apollo 15 landing region
Orthogonal transforms and feature selection using pattern, Harr, Walsh, Fourier and Karhunen- Loeve spaces for providing efficient classification algorithms in pattern recognition
Mars surface features contrast reduction, discussing forward scattering haze as possible cause
Jupiter Red Spot and other photographic features in 1969-1970, noting 90-day oscillation in longitude and south tropical zone disturbance
Lunar volcano-tectonic processes, considering primary circular or polygonal surface features evolution
Vacuum UV emission features dissociative excitation by electron impact on molecular hydrogen and oxygen, measuring excitation cross sections from threshold to 350 eV
Mathematical feature selection transformations by multidimensional rotations, considering character recognition experiment
Walsh functions in image processing, rotational feature selection and pattern recognition, defining set of orthogonal transformations
Mineralogical, petrological and chemical features of four Apollo 12 lunar microgabbros
Lunar rocks 12063,9 and 12004,11 opaque mineralogy and textural feature, comparing to apollo 11 samples
Findings are presented for IRIS data from NIMBUS 3 in mapping the global ozone distribution. The seasonal and regional variations of ozone, especially in the Southern Hemisphere, reveal features that were not evident from the sparse ground-based ozone observation network in this hemisphere. A regression analysis was undertaken for temperature and height fields on radiance data. Spectrum analyses of upper wind data from the North American section and Australia were completed.
To ensure good aerial photography, the effects that factors such as submergence depth, sun angle, film and filter type, exposure, aircraft altitude, and polarization have on the photographic resolution of an underwater object must be determined. Various subjects were photographed, such as the deck of a small submersible, colored and gray scale panels, and natural bottom features. No underwater resolution target was used.
The philosophy and methods used in the design of the DC-10 aircraft to assure structural reliability against cracks under repeated service loads are described in detail. The approach consists of three complementary parts: (1) the structure is designed to be fatigue resistant for a crack-free life of 60,000 flight hours; (2) inasmuch as small undetected cracks could develop from other sources, such as material flaws and manufacturing preloads, the structure also is designed to arrest and control cracks within a reasonable service-inspection interval; and (3) a meaningful service-inspection program has been defined on the basis of analysis and test experience from the design development program. This service-inspection program closes the loop to assure the structural integrity of the DC-10 airframe. Selected materials, fasteners, and structural arrangements are used to achieve these design features with minimum structural weight and with economy in manufacturing and maintenance. Extensive analyses and testing were performed to develop and verify the design. The basic design considerations for fatigue-resistant structure are illustrated in terms of material selection, design loads spectra, methods for accurate stress and fatigue damage analysis, and proven concepts for efficient detail design.
Grating spectra of the North Equatorial Belt of Jupiter between 4.5 and 5.1 microns, obtained with a nominal resolving power of 180, are presented. An absorption feature centered at 4.73 microns and not due to a known constitu ent has been found. Its possible identification is discussed.
Study of the origin and development of lava conduits in terrestrial volcanic regions and the possible association of two important classes of lunar morphological features - i.e., channels and the sinuous rilles on the lunar maria - with stages in the evolution of lava conduits. The study was motivated by observations of some Hawaiian active volcanic regions. The origin of apparent flow channels on steep slopes on the moon is also considered.
A control net of Mars has been computed from measurements of 115 control points identified on the Mariner 6 and 7 pictures. Most of these points are located with respect to topographic features on the surface of Mars, and their areographic coordinates were computed by photogrammetric techniques. These pictures offered the first opportunity to establish a control net of Mars based on topographic detail.
ERTS-1 imagery of geological and structural features of sedimentary basin in France
ERTS-1 imagery and shipboard data on oceanographic features of eastern Caribbean Sea