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  • General Chemistry  (77,717)
  • SPACE SCIENCES  (12,837)
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  • 1
    Publication Date: 2024-02-26
    Description: Identifcation of ontogenetic age classes plays an important role in the felds of zoology, palaeontology and archaeology, where accurate age classifcations of (sub)fossil remains are a crucial component for the reconstruction \nof past life. Textural ageing\xe2\x80\x94the identifcation of age-related bone surface textures\xe2\x80\x94provides a size-independent \nmethod for age assessment of vertebrate material. However, most of the work so far is limited to qualitative results. \nWhile qualitative approaches provide helpful insights on textural ageing patterns, they are heavily subject to observer \nbias and fall short of quantitative data relevant for detailed statistical analyses and cross-comparisons. Here, we present a pilot study on the application of 3D surface digital microscopy to quantify bone surface textures on the long \nbones of the grey heron (Ardea cinerea) and the Canada goose (Branta canadensis) using internationally verifed \nroughness parameters. Using a standardised measuring protocol, computed roughness values show a strong correlation with qualitative descriptions of textural patterns. Overall, higher roughness values correspond to increased numbers of grooves and pits and vice versa. Most of the roughness parameters allowed distinguishing between diferent \nontogenetic classes and closely followed the typical sigmoidal animal growth curve. Our results show that bone \ntexture quantifcation is a feasible approach to identifying ontogenetic age classes.
    Keywords: General Physics and Astronomy ; General Environmental Science ; General Biochemistry ; Genetics and Molecular Biology ; General Materials Science ; General Chemistry ; Roughness ; Surfaces ; Taphonomy ; Topography ; Bone ; Ontogeny ; Digital microscopy
    Repository Name: National Museum of Natural History, Netherlands
    Type: info:eu-repo/semantics/article
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  • 2
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    In:  CASI
    Publication Date: 2009-12-22
    Description: Impact attenuation methods for manned spacecraft
    Keywords: SPACE SCIENCES
    Type: Proceedings of the National Meeting on Manned Space Flight: Unclassified Portion
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  • 3
    Publication Date: 2009-12-22
    Description: Hypersonic vehicle skin development
    Keywords: SPACE SCIENCES
    Type: Proceedings of the National Meeting on Manned Space Flight: Unclassified Portion
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  • 4
    Publication Date: 2009-12-22
    Description: Design requirements for self-erecting manned space station configuration for use in Apollo program
    Keywords: SPACE SCIENCES
    Type: Proceedings of the National Meeting on Manned Space Flight: Unclassified Portion
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  • 5
    Publication Date: 2009-12-22
    Description: Parabolic manned reentry design comparison of lunar return configurations
    Keywords: SPACE SCIENCES
    Type: Proceedings of the National Meeting on Manned Space Flight: Unclassified Portion
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  • 6
    Publication Date: 2008-08-25
    Description: Spacecraft look-angle problem - instrument orientation
    Keywords: SPACE SCIENCES
    Type: JPL-TR-32-311
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  • 7
    Publication Date: 2008-08-25
    Description: Nuclear electric spacecraft for unmanned planetary and interplanetary missions - powerplants
    Keywords: SPACE SCIENCES
    Type: JPL-TR-32-281
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  • 8
    Publication Date: 2010-10-12
    Description: Rocket exhaust jet interaction with lunar surface dust layer
    Keywords: SPACE SCIENCES
    Type: AGARD THE FLUID DYN. ASPECTS OF SPACE FLIGHT, VOL. 2 1966; P 269-290
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  • 9
    Publication Date: 2011-10-14
    Description: Electric drag of spherical satellites with conducting surfaces
    Keywords: SPACE SCIENCES
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  • 10
    Publication Date: 2010-01-11
    Description: Spacecraft and launch vehicle performance - ma-7
    Keywords: SPACE SCIENCES
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  • 11
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    Publication Date: 2004-12-06
    Description: Apollo 12 photographs from lunar orbit, EVA, and transearth flight
    Keywords: SPACE SCIENCES
    Type: APOLLO 12- PRELIM. SCI. REPT. 1 JUN. 1970; P 7-27
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  • 12
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    Publication Date: 2004-12-06
    Description: Apollo 12 crew observations of moon, earth, lunar surface geology, and EVA
    Keywords: SPACE SCIENCES
    Type: APOLLO 12- PRELIM. SCI. REPT. 1 JUN. 1970; P 29-38
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  • 13
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    Publication Date: 2005-11-27
    Description: Meteoroid density, velocity, flux-mass relation, and impact on spacecraft
    Keywords: SPACE SCIENCES
    Type: SPACE MATER. HANDBOOK 1969; P 63-75
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  • 14
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    Publication Date: 2005-11-17
    Description: Far infrared measurement of galactic center
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 169-171
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  • 15
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    Publication Date: 2005-11-17
    Description: Red supergiant evolution, death, and accelerating changes with neutrino emission
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 161-164
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  • 16
    Publication Date: 2005-11-17
    Description: Far ultraviolet photometric observation of intense extraterrestrial sources at 296 kilometers
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 156-160
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  • 17
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    Publication Date: 2005-11-17
    Description: Qualitative photometric analysis system for metal-rich and metal-poor cepheid variable stars
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 146-149
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  • 18
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    Publication Date: 2005-11-17
    Description: Solar radio bursts
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 108-112
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  • 19
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    Publication Date: 2005-11-17
    Description: Electronic techniques applied to Hansen theory for satellite position determination
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 96-99
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  • 20
    Publication Date: 2005-11-17
    Description: Scattering effects on thermal emission and cloud structure of Venus atmosphere
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 78-81
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  • 21
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    In:  CASI
    Publication Date: 2005-11-17
    Description: Evolution and nature of Venus atmosphere
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 71-73
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  • 22
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    Publication Date: 2005-11-17
    Description: Solar corona analysis from X ray emissions
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 100-102
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  • 23
    Publication Date: 2005-11-17
    Description: Venus surface composition as determined from atmospheric composition
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 74-77
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  • 24
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    Publication Date: 2005-11-17
    Description: Radical and ion emission phenomena in comets
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 82-84
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  • 25
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    Publication Date: 2005-11-17
    Description: Real time orbit determination for Mariner 5
    Keywords: SPACE SCIENCES
    Type: THE MARINER 5 FLIGHT PATH AND ITS DETERMINATION FROM TRACKING DATA 1 JUL. 1969; P 1-26
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  • 26
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    Publication Date: 2005-11-17
    Description: Long-wavelength radio astronomy from Explorer 38 satellite with spatial distribution
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 165-168
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  • 27
    Publication Date: 2005-11-17
    Description: Ultraviolet spectra by rocket observations of Zeta Puppis and Gamma Velorum
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 150-155
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  • 28
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    Publication Date: 2005-11-17
    Description: Solar wind and solar corona models
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACCOMPLISHMENTS IN SCI., 1968 1969; P 117-120
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  • 29
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    In:  CASI
    Publication Date: 2005-11-17
    Description: Evolution of life in universe
    Keywords: SPACE SCIENCES
    Type: SCHOOL OF AEROSPACE MED. BIOASTRONAUT. AND THE EXPLORATION OF SPACE NOV. 1968; P 569-593
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  • 30
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    Publication Date: 2005-11-17
    Description: Planetology research in 1967, with data on planet atmospheres and origins, moon, meteorites, impact cratering, and metamorphism
    Keywords: SPACE SCIENCES
    Type: NIFICANT ACHIEVEMENTS IN SPACE SCI. 1967 1968; P 303-437
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  • 31
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    Publication Date: 2005-11-17
    Description: Stellar astronomy progress in 1967, including X ray, gamma ray, ultraviolet, and infrared region results
    Keywords: SPACE SCIENCES
    Type: NASA, WASHINGTON SIGNIFICANT ACHIEVEMENTS IN SPACE SCI. 1967 1968; P 1-39
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  • 32
    Publication Date: 2005-11-30
    Description: Infrared and radar studies of the Apollo 16 landing site are summarized. Correlations and comparisons between earth based remote sensing data, IR observations, and other data are discussed in detail. Remote sensing studies were devoted to solving two problems: (1) determining the physical difference between Cayley and Descartes geologic units near the landing site; and (2) determining the nature of the bright unit of Descartes mountain material.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 5 p
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  • 33
    Publication Date: 2005-11-30
    Description: Problematic causes and characteristics of light colored sinuous markings on the lunar surface are explored. Two processes, exogenetic and endogenetic, are examined in detailed. During the endogenetic process it is suggested that impact ejecta deposition and surface disturbances cause the markings. During the endogenetic process, it is suggested that extrusive volcanism and sublimation and/or alteration cause the markings.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 4 p
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  • 34
    Publication Date: 2005-11-30
    Description: Probable causes, distributions, and nature of fracture patterns of Type 3 craters around the margins of major maria are investigated.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
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  • 35
    Publication Date: 2005-11-30
    Description: Metric camera photographs are used to analyze volcanic and surficial features of the lunar surface between Mare Smythii and King Crater. Patterns created by lava flows, ejecta blankets, impact debris, and fissures are discussed in detail. Possible causes of each phenomena are suggested.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
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  • 36
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    Publication Date: 2005-11-30
    Description: Morphometric analysis of lunar craters complements the more traditional photointerpretive study of crater morphology. A sampling is presented of morphometric results for five selected medium-sized craters photographed on the Apollo 16 mission: Madler, Langrenus B, Isidorus, Capella, and King. Apollo metric camera data present the first real opportunity to evaluate previous topographic measurements in terms of accuracy rather than in terms of precision. This method of generating crater measurements furnishes far more complete data than does the shadow-length method that yielded most of the previous morphometric information on lunar craters.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 6 p
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  • 37
    Publication Date: 2005-11-30
    Description: Photogeologic analysis was attempted on a strip of Apollo 16 metric photographs; the superior quality and stereographic properties of the photography permitted this reevaluation. Geologic contacts, as redrawn closely resemble those of earlier maps, but some differences resulted because of improved photographic quality and a conscious attempt to test fully the impact hypothesis. All or most of the nonmare material of the region of the northern Nectaris Basin rim can be explained by the formation of impact basins. This interpretation seems strained only for some irregular and clustered craters north of Mare Nectaris and for the southern facies of the Descartes material. If the latter material is shown to have been sampled and to be of impact origin, then extensive hill and crater-forming volcanic material of Imbrian or younger age probably does not exist on the lunar terra.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 4 p
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  • 38
    Publication Date: 2005-11-30
    Description: The distribution of subtle but definite color variations on the lunar surface is analyzed using Apollo 16 photographs. Results show the strongest color variations and most distinct boundaries are concentrated in the northwest quadrant of the moon, where major boundaries correspond with distal fronts of a complex and prominent series of lava flows.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
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  • 39
    Publication Date: 2005-11-30
    Description: Stereoscopic lunar photographs were used to study the form of mare ridges and arches, their relative ages, and their association with fractures and sinuous rilles in the Southern Oceanus Procellarum.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 3 p
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  • 40
    Publication Date: 2005-11-30
    Description: Additional evidence of the volcanic origin of mare ridges and sinuous rilles is provided by near-terminator photography of the Herigonius Rille area (12 deg S 37 deg W) northeast of Gassendi Crater. A possible genetic relationship between ridges and rilles is illustrated. From the figure, the following relationships are evident. (1) The most prominent rille crosses several ridges without distortion, which indicates that the mare ridges did not form after the sinuous rilles. (2) The rilles could not have formed by flow up and over the ridges. (3) The rilles extend from their widest ends toward distinctly lower elevations, and the largest one branches both north and south from the vent area. Elevations are evident in stereographic views that clearly indicate the local slopes. (4) The wider end of each rille is marked by an elongate vent (?) near the summit of the mare ridge from which the rille appears to issue. (5) The two most prominent rilles join south of the vent area and continue southward for more than 130 km.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 1 p
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  • 41
    Publication Date: 2005-11-30
    Description: The Apollo 16 panoramic camera photographed the impact locations of the Ranger 7 and 9 spacecraft and the S-4B stage of the Apollo 14 Saturn launch vehicle. Identification of the Ranger craters was very simple because each photographed its target point before impact. Identification of the S-4B impact crater proved to be a simple matter because the impact location, as derived from earth-based tracking, displayed a prominent and unique system of mixed light and dark rays. By using the criterion of a dark ray pattern, a reexamination of the Apollo 14 500 mm Hasselblad sequence taken of the Apollo 13 S-4B impact area was made. This examination quickly led to the discovery of the ray system and the impact crater. The study of artificial lunar impact craters, ejecta blankets, and ray systems provides the long-needed link between the various experimental terrestrial impact and explosion craters, and the naturally occurring impact craters on the moon. This elementary study shows that lunar impact crater diameters are closely predictable from a knowledge of the energies involved, at least in the size range considered, and suggests that parameters, such as velocity, may have a profound effect on crater morphology and ejecta blanket albedo.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 6 p
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  • 42
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    Publication Date: 2005-11-30
    Description: Apollo 16 metric photographs taken at low to high sun angles provided the first stereographic coverage of the distinctive landforms collectively referred to as Imbrium sculpture. The sculpture consists of a series of nearly linear ridges and troughs extending radially outward for more than 1000 km from the rim of the Imbrium Basin. The origin of the ridges and troughs, whether by deposition and impact scoring by fluidized clouds of ejecta from the Imbrium Basin or by faulting and volcanism during and subsequent to basin formation, is controversial. Evidence indicative of the mode of origin of Imbrium sculpture is summarized as follows. Evidence of volcano-tectonic mode of origin is favored by: (1) wide variation in relative age of parts of the sculpture; (2) furrows without rims; (3) absence of ballistic shielding; (4) asymmetry of sculpture; (5) absence of randomly oriented clusters; and (6) association with other features of structural origin. An origin by ejecta scoring and deposition is favored by the gradational ejecta with a Fra Mauro-type texture. Features that are ambiguous as to mode or origin are furrows made of coalesced crater chains and prominent rims on furrows.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 2 p
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  • 43
    Publication Date: 2005-11-30
    Description: The Apollo 16 lunar surface magnetometer (LSM) activation completed the network installation of magnetic observatories on the lunar surface and initiated simultaneous measurements of the global response of the moon to large-scale solar and terrestrial magnetic fields. Fossil remanent magnetic fields have been measured at nine locations on the lunar surface, including the Apollo 16 LSM site in the Descartes highlands area. This fossil record indicates the possible existence of an ancient lunar dynamo or a solar or terrestrial field much stronger than exists at present. The experimental technique and operation of the LSM are described and the results obtained are discussed.
    Keywords: SPACE SCIENCES
    Type: Apollo 16 Prelim. Sci. Rept.; 14 p
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  • 44
    Publication Date: 2005-11-30
    Description: Preliminary results of examining the lunar rock samples from the Apollo 16 flight are reported. Topics discussed include: premission geologic studies, geologic objectives, description of the site and traverse routes, superficial deposits, and station descriptions.
    Keywords: SPACE SCIENCES
    Type: Apollo 16 Prelim. Sci. Rept.; 81 p
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  • 45
    Publication Date: 2005-11-30
    Description: Two pieces of the Surveyor 3 spacecraft recovered during the Apollo 12 mission were examined for secondary lunar ejecta and micrometeorite impacts. One piece was section E of the aluminum strut; the other was the nickel-coated beryllium television camera mirror.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 151-153
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  • 46
    Publication Date: 2005-11-30
    Description: The mirror and middle shroud were extracted for organics by washing the surfaces with solvents. The techniques are discussed. Ion microprobe analyses of the primarily atomic species are presented. The sources of the organic contaminants are: (1) hydrocarbons from lubricating oils and general terrestrial contamination, (2) dioctyl phthalate, probably from polyethylene bagging material (the plasticizer), (3) carboxylic acids from decomposition of grease and general terrestrial contamination, (4) silicones from sources such as lubricating oil, (5) outgassing of electronics and plasticizer, (6) vinyl alcohol and styrene copolymer, probably from electronic insulation, and (7) nitrogenous compounds from the lunar module and possibly Surveyor 3 engine exhaust.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 127-142
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  • 47
    Publication Date: 2005-11-30
    Description: Material removed from the spacecraft and returned to earth remained on the lunar surface for 31.9 lunations. None of the returned parts received the maximum 10,686 hours of exposure because of shadowing by the planar array antenna, solar panel, thermal control compartments, or other parts of the spacecraft. To determine the actual exposure of specific parts to sunlight, six series of photographs were taken. A one-fifth-scale model spacecraft was oriented to a collimated light source simulating the orientation of Surveyor with the sun. Three cameras were set up to view different parts of the spacecraft. The data obtained from these photographs permitted an evaluation of the effects of exposure to solar radiation on the camera and its parts, the surface sampling scoop, and the strut from the radar altimeter and Doppler velocity sensor.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 253-260
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  • 48
    Publication Date: 2005-11-30
    Description: The television housing and a section of the strut of the radar altimeter and Doppler velocity sensor were examined optically and with a scanning electron microscope for particulate impacts. The white surface of the camera was discolored during the months the Surveyor 3 was on the moon; however, most of the craters must have occurred as a result of lunar dust sandblasted by the LM exhaust. The polished section of the strut exhibits contamination which appears brown and seems to be partially composed of crystals. Electron microscopic analysis of the strut section indicated no craters of hypervelocity impact origin, confirmed pitting density results of the optical scans, and indicated that material in the craters is of lunar origin. No meteorite impacts larger than 25 microns were detected on the tubing section.
    Keywords: SPACE SCIENCES
    Type: Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 158-167
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  • 49
    Publication Date: 2005-11-30
    Description: Determination of the number of micrometeoroid impact craters on the camera provided an opportunity to make a sensitive direct measurement of the flux of interplanetary dust particles impacting the lunar surface. Optical and scanning electron microscope studies were performed. Low velocity impact and flux analyses are presented.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 143-151
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  • 50
    Publication Date: 2005-11-30
    Description: Two screws and two washers, several small chips of tubing, and a fiber removed from a third screw were examined with the scanning electron microscope and the electron microprobe. The purpose of the examination was to determine the nature of the material on the surface of these samples and to search for the presence of meteoritic material.
    Keywords: SPACE SCIENCES
    Type: NASA, Washington Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 89-90
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  • 51
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    Publication Date: 2005-11-30
    Description: The ionopause of the Venus ionosphere, as indicated by Mariner 5 electron density data, and which occurs at 500km on the day side, and 2500km on the night side is discussed in terms of the solar wind interaction with the ionosphere. It is concluded that for a source of stabilization by heating to be effective, a small horizontal magnetic field is required to reduce the downward heat conduction of charged particles, and it has been shown that such a magnetic field is present.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 63-70
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  • 52
    Publication Date: 2005-11-30
    Description: As part of the investigation of Surveyor 3 materials, a study was conducted to determine the effect of the lunar environment on some of the painted and unpainted exterior surfaces. Examination of the camera parts and tube sections was conducted using three techniques: (1) optical and scanning electron microscopy, (2) energy dispersive X-ray probe analysis, and (3) spectral reflectance measurements.
    Keywords: SPACE SCIENCES
    Type: Analysis of Surveyor 3 Mater. and Phot. Returned by Apollo 12; p 76-88
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  • 53
    Publication Date: 2005-11-30
    Description: Photographs and geologic maps of the area around Littrow rilles and eastern edge of Mare Serenitatis are presented, along with variations in the features and compositions of the region.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 3 p
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  • 54
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    Publication Date: 2005-11-30
    Description: Some astronomical results, obtained by very long baseline interferometry, on quasi-stellar sources are reported. Data cover variations in optical luminosity, radio brightness variations, and observations of quasi-stellar nuclei.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 238-247
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  • 55
    Publication Date: 2005-11-30
    Description: Reflectivity and polarization laws for the powder sample and its spectrum are close to the mean for the lunar maria. Solid samples show a marked absorption feature at 1 micron. The low albedo appears to be due to a surface coating on dust grains rather than volume absorption. The high frequency electrical properties resemble those of a fine powder made from typical dense terrestrial rocks, and are consistent with previous ground-based radar estimates. The differential mass spectrum is almost constant from 100 micron particles down to 0.1 micron; most particles are smaller than 0.3 micron. Their shapes disclose a variety of generation processes.
    Keywords: SPACE SCIENCES
    Type: Res. on Lunar Mater.; p 25-39
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  • 56
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    Publication Date: 2005-11-30
    Description: An attempt was made to build a model for the observed continuous emission from extragalactic radio sources. The data, measured by RAE spacecraft, are compared to deduced measurements. The difference between the two is taken as the model for observed emission. Data also cover spectra for the anticenter, north halo minimum region, RAE low frequency observations, and ground based high frequency observations.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 227-230
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  • 57
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    Publication Date: 2005-11-30
    Description: Two independent methods for measuring the electron intensity in interstellar space are proposed. The positron method involves the production of pions in proton-proton collisions, the decay of the pions into muons, and the subsequent decay of the muons into positrons. Results from detailed calculations of these processes are given in graphical form. The second method involves cosmic electron emitted synchrotron radiation in the interstellar magnetic field. These two methods are also used to analyze the spatial and temporal constancy of cosmic ray electrons in the galaxy.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 217-221
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  • 58
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    Publication Date: 2005-11-30
    Description: The use of special detectors to measure and classify spectral X-ray sources in the region of a few keV and above, is discussed. Two sources, Cygnus X-2 and Cygnus X-3 were measured.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 196-199
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  • 59
    Publication Date: 2005-11-30
    Description: A quantitative discussion is presented of the lifetime against photodecomposition, or the probability of photodecomposition, of interstellar molecules. In addition to photodissociation, molecules can also be destroyed by interaction with high energy radiation and energetic particles. These processes are much less effective than destruction by ultraviolet radiation. However, when the ultraviolet is highly attenuated in clouds, the energetic radiation and particles will persist and will become relatively more important and the ultimate lifetimes in clouds may depend upon these processes.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 125-128
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  • 60
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    Publication Date: 2005-11-30
    Description: An example is given of the capture orbit for the general problem of three bodies and how it may be related to some practical problems in the solar system.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 107-111
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  • 61
    Publication Date: 2005-11-30
    Description: A preliminary quantitative analysis was conducted of four frames exposed by the Apollo 15 metric camera. Two of the frames show the zero-phase surge on maria and the other two show the surge on terrae. It was found that the curves resulting from brightness plotted as a function of phase angle, differ markedly according to which terrain type is involved. The magnitude of the heiligenschein was found to be significantly greater for the maria than for the terrae.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 1 p
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  • 62
    Publication Date: 2005-11-30
    Description: An Apollo 15 panoramic camera frame was used as a base for a geologic sketch map of an area near Proclus Crater. The map was prepared to investigate the usefulness of the panoramic camera photography in large-scale geologic mapping and to assess the geologic value of the area as a potential Apollo landing site. The photographs, taken under high solar illumination, resulted in good definition of albedo features, and stereoscopic viewing provided extreme clarity of topographic relief with terrain units easily delineated. The geological characteristics of the area as evidenced by the high-resolution photographs is discussed. It is concluded that the panoramic camera photographs reveal a wealth of detail and are eminently suited for geologic mapping purposes. In addition, the Proclus area, as a potential landing site, offers relatively rough plains terrain.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 5 p
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  • 63
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    Publication Date: 2005-11-30
    Description: The distance from the sun to the center of the star, Gamma Velorium, is determined in an effort to draw a physical model and identify the ionized energy source of the Gum nebula. The distance is calculated from the local hydrogen density of radio astronomy studies and the hydrogen measure.
    Keywords: SPACE SCIENCES
    Type: Significant Accomplishments in Sci., 1970; p 190-195
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  • 64
    Publication Date: 2005-11-30
    Description: Apollo 15 orbital photographs, particularly those taken at low sun elevation angles, are examined revealing grid patterns of lineaments. Preliminary results of experiments demonstrate that spurious lineaments and grid patterns can be produced and that the directions are dependent in part upon the position of the light source. The experiments were designed to duplicate the effect of bright sunlight reflecting from a hummocky surface with little or no diffuse light in the shadowed areas.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 5 p
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  • 65
    Publication Date: 2005-11-30
    Description: The three cameras (stellar, mapping, and panoramic) together with the laser altimeter are included in the scientific instrument module bay, representing an integrated photogrammetric system. Data analysis objectives and procedure are presented, along with deformation of second generation negatives and heighting accuracy of panoramic photographs. Mapping camera photographs and stellar photography are evaluated. Rectified prints from panoramic camera photographs are produced, as well as enlarged prints from the mapping camera pictures.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 9 p
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  • 66
    Publication Date: 2005-11-30
    Description: A preliminary analysis of magnetometer data from Apollo 15 subsatellite is concluded. Remanent magnetization is a characteristic property of the moon, and the distribution is such that a complex pattern is produced. A mapping of the distribution is feasible with the present experiment. Lunar induction fields produced by transients in interplanetary magnetic field are detectable at satellite orbit. Magnetometer data will provide estimates of the latitude and longitude dependences of interior conductivity. The plasma void extends to some altitude below the satellite orbit and probably the lunar surface. Solar wind near the limbs is usually strongly disturbed.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spaceflight Center Apollo 15 Prelim. Sci. Rept.; 9 p
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  • 67
    Publication Date: 2005-11-30
    Description: Near-terminator photography from the Apollo 14 and 15 missions is used as a basis to evaluate the processes by which craters disappear from the lunar surface. From observations and analyses it is concluded that: (1) The erosion of lunar craters in the size range of 10 m to 1 km is effected principally by small impacts producing minute changes in crater form up to the point where the crater is worn to an interior slope of approximately 1 degree. Below that slope, the annihilation process is dominated by the formation of younger overlapping craters. (2) The distribution of shapes of craters in this size range can be explained as resulting from impact generated processes.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 5 p
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  • 68
    Publication Date: 2005-11-30
    Description: The Apollo 15 metric camera photography provided a number of spectacular views of most of the southern and central portions of the unique systems of major lava flows that stretch diagonally across Mare Imbrium from the general area of Euler Crater to a point east of Le Verrier Crater. A preliminary examination of the photographs indicates that the source of the material comprising the major flows is situated to the west of Euler Crater and south of the limits of the photographic coverage. The photographs also show clearly that most, if not all, the mare ridges included were formed after the solidification of the flows. Few color boundaries exist in the area of metric photography where the illumination angle is low enough to show the fronts of some of the very thin flows. However, patches of redder material lying northeast of Mt. Lahire are found to be enclosed by low flow fronts, confirming the theory that the redder material represents an earlier filling of the Imbrium basin.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 2 p
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  • 69
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    Publication Date: 2005-11-30
    Description: A dark-colored mare unit within the southwestern corner of the Taurus Mountains is discussed. The geologic characteristics of this unit, the intricate relationship between it and the surrounding features, and the probable source of the unit were the objects of visual observations during the Apollo 15 flight. The results of these observations made from orbit indicate that the unit probably consists of volcanic ash or pyroclastic deposits that came to the surface through a multitude of cinder cones. The local setting of the area and the relationship of the dark deposit to other nearby geologic units are examined in light of data obtained from the Apollo 15 panoramic camera photographs.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 6 p
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  • 70
    Publication Date: 2005-11-30
    Description: In the Apollo 15 mission, a mapping camera system and a 61 cm optical bar, high resolution panoramic camera, as well as a laser altimeter were used. The panoramic camera is described, having several distortion sources, such as cylindrical shape of the negative film surface, the scanning action of the lens, the image motion compensator, and the spacecraft motion. Film products were processed on a specifically designed analytical plotter.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 12 p
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  • 71
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    Publication Date: 2005-11-30
    Description: A bistatic-radar study during the Apollo 15 flight is reviewed, with the orbiting command module as one terminal. Bistatic-radar slopes are compared to geological maps of Copernicus and Riphaeus mountain regions and Kepler region. Basic theory is discussed, including the radar echoes composed of the sum of the reflections from the moon area that is mutually visible from the spacecraft and earth. A signal receiving system and data processing system are outlined schematically.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spacecraft Center Apollo 15 Prelim. Sci. Rept.; 10 p
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  • 72
    Publication Date: 2005-11-30
    Description: The preliminary results from the Sco X-1 and Cyg X-1 obtained from the Apollo 15 X-ray detector data are presented along with preliminary results of the X-ray fluorescence spectrometric data of the lunar surface composition. The production of the characteristic X-rays following the interaction of solar X-rays with the lunar surface is described along with the X-ray spectrometer. Preliminary analyses of the astronomical X-ray observation and the X-ray fluorescence data are presented.
    Keywords: SPACE SCIENCES
    Type: Apollo 15 Prelim. Sci. Rept.; 17 p
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  • 73
    Publication Date: 2005-11-30
    Description: The Apollo program techniques for studying elemental and isotopic abundances in the solar wind are described. During Apollo 11, 12, 14 and 15 missions, aluminum foils were deployed on the lunar surface as targets for collecting solar wind ions. The foils were returned to earth, and the implanted solar wind particles were analyzed. The preliminary results showing the helium and neon concentrations are presented.
    Keywords: SPACE SCIENCES
    Type: NASA. Manned Spaceflight Center Apollo 15 Prelim. Sci. Rept.; 7 p
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  • 74
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    Publication Date: 2005-11-30
    Description: Previously developed models for trapped electron radiation belts and trapped proton radiation belts in the Jovian magnetosphere are described. The spatial distribution of flux and the L shell dependence of the characteristic energy are displayed for both models. Based on these models, the fluence accumulated by a Jupiter flyby spacecraft is given in terms of the equivalent 3-MeV fluence for electrons and the equivalent 20-MeV proton fluence. Finally, some impacts of these fluences on outer planet missions are described.
    Keywords: SPACE SCIENCES
    Type: JPL Quart. Tech. Rev., Vol. 1, No. 4; p 78-88
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  • 75
    Publication Date: 2005-11-30
    Description: The objective grating technique is discussed. From the investigation of actual material, it is established that the effect of coma varies significantly from plate to plate, also that a model linear in diameter and/or coordinate may be inadequate for its removal, and even introduce systematic errors. From this standpoint, the requirements of reference star systems are discussed.
    Keywords: SPACE SCIENCES
    Type: Conf. on Phot. Astrometric Technique; p 241-248
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  • 76
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    Publication Date: 2005-11-30
    Description: Proper motions formed with the use of positions in the AGK3 and other, older catalogues are investigated for systematic trends.
    Keywords: SPACE SCIENCES
    Type: Conf. on Phot. Astrometric Technique; p 169-172
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  • 77
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    Publication Date: 2005-11-30
    Description: The arrival times of the pulses from each pulsar are measured by a cesium clock. The observations are all made at a frequency of 2388 MHz (12.5 cm wavelength) on a 26 m dish antenna. The effect of interstellar charged particles is a random one that increases the noise level on the arrival time measurements. The variation in clock rate is shown consisting of two effects: the time dilation effect of special relativity and the red shift effect of general relativity.
    Keywords: SPACE SCIENCES
    Type: Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 65-67
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  • 78
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    Publication Date: 2005-11-30
    Description: Cosmic helium abundance was studied through the interior structure of young stars, profiles of helium absorption lines in the photospheric spectra of hot young stars, and emission-line spectrum of ionized gas. It is concluded that helium occurred before galaxies were formed. Inconsistencies found in the quasar spectra are briefly mentioned.
    Keywords: SPACE SCIENCES
    Type: JPL Proc. of the Conf. on Exptl. Tests of Gravitation Theories; p 1-3
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  • 79
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    Publication Date: 2005-11-27
    Description: Deep well drilling for lunar gases
    Keywords: SPACE SCIENCES
    Type: NASA, WASHINGTON PROC. OF THE 7TH ANN. WORKING GROUP ON EXTRATERREST. RESOURCES 1970; P 131-133
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  • 80
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    Publication Date: 2005-11-27
    Description: Friction tests of minerals in ultrahigh vacuum simulating lunar environment
    Keywords: SPACE SCIENCES
    Type: NASA, WASHINGTON PROC. OF THE 7TH ANN. WORKING GROUP ON EXTRATERREST. RESOURCES 1970; P 107-111
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  • 81
    Publication Date: 2005-11-27
    Description: Hydrothermally altered rocks as water source on Moon and Mars
    Keywords: SPACE SCIENCES
    Type: NASA, WASHINGTON PROC. OF THE 7TH ANN. WORKING GROUP ON EXTRATERREST. RESOURCES 1970; P 87-92
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  • 82
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    Publication Date: 2005-11-27
    Description: Hygrometer, neutron-induced gamma characteristics, and neutron albedo measurements for lunar water detection
    Keywords: SPACE SCIENCES
    Type: PROC. OF THE 7TH ANN. WORKING GROUP ON EXTRATERREST. RESOURCES 1970; P 53-59
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  • 83
    Publication Date: 2005-11-27
    Description: Astronomical photography of zodiacal light and lunar libration clouds
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 300-302
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  • 84
    Publication Date: 2005-11-27
    Description: High resolution strip photography of lunar surface
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 283-290
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  • 85
    Publication Date: 2005-11-27
    Description: Study of far side upland volcanism of lunar surface using Hasseblad camera
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 267-274
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  • 86
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    Publication Date: 2005-11-27
    Description: Bistatic radar for remote determination of vertical crustal structure of lunar surface
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 257-266
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  • 87
    Publication Date: 2005-11-27
    Description: Apollo 14 command service and lunar module orbital velocity data from radio navigation S-band transponder experiment for lunar gravitation effects
    Keywords: SPACE SCIENCES
    Type: NASA. MANNED SPACECRAFT CENTER APOLLO 14 PRELIM. SCI. REPT. 1971; P 253-256
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  • 88
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    Publication Date: 2005-11-27
    Description: Closeup photographs of soil and rock on lunar surface obtained with Apollo 14 stereoscopic camera
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 239-247
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  • 89
    Publication Date: 2005-11-27
    Description: Aluminum foils for measuring solar wind ion composition
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 221-226
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  • 90
    Publication Date: 2005-11-27
    Description: Lunar portable magnetometer experiment to measure steady magnetic field at different sites in Fra Mauro region - Apollo 14 flight
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 227-237
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  • 91
    Publication Date: 2005-11-27
    Description: Laser ranging retroreflector deployed on lunar surface to study lunar librations for defining precisely lunar orbits and studying earth planetary structure - Apollo 14 flight
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 215-220
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  • 92
    Publication Date: 2005-11-27
    Description: Cold cathode gage for measuring amount of gas present in lunar atmosphere
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 185-191
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  • 93
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    Publication Date: 2005-11-27
    Description: Active seismic signal analysis from Apollo 14 thumper and mortar detonations on lunar surface
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 163-174
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  • 94
    Publication Date: 2005-11-27
    Description: Seismic signal analysis from Apollo 14 passive seismic experiment
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 133-161
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  • 95
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    Publication Date: 2005-11-27
    Description: Mineralogy and petrology of lunar rock and soil samples returned from Apollo 14 landing site
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 109-131
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  • 96
    Publication Date: 2005-11-27
    Description: Lunar soil mechanics and properties based on Apollo 14 observations and data
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 87-108
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  • 97
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    Publication Date: 2005-11-27
    Description: Apollo 14 crew visual observations of earth, moon, lunar topology and geology, and astronaut maneuverability during extravehicular activity
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 33-37
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  • 98
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    Publication Date: 2005-11-27
    Description: Photographic equipment and film used during Apollo 14 flight in command and lunar modules and during extravehicular activity
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 9-32
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  • 99
    Publication Date: 2005-11-27
    Description: Apollo 14 lunar seismographic, geologic, magnetic field, and atmospheric data summary
    Keywords: SPACE SCIENCES
    Type: APOLLO 14 PRELIM. SCI. REPT. 1971; P 1-8
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  • 100
    Publication Date: 2005-11-27
    Description: Perturbation theory using variation of parameters formulation to calculate satellite orbits
    Keywords: SPACE SCIENCES
    Type: THE DEEP SPACE NETWORK, VOL. 1 15 FEB. 1971; P 117-121
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