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  • ASTROPHYSICS  (172)
  • INSTRUMENTATION AND PHOTOGRAPHY  (40)
  • 2015-2019
  • 1985-1989  (212)
  • 1980-1984
  • 1987  (212)
  • 1
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    X-rays from the radio halo of M87 (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-12
    Description: The Einstein Observatory and the VLA were used to scan the radio halo of the galaxy M87 to detect the presence, if any, of inverse Compton X-ray (ICX) emissions. The scans revealed a coincidence of an asymmetrical X-ray structure with a luminosity near 4 x 10 to the 41st ergs/sec and dominant symmetrical emission from the hot interstellar gas. The emission can be attributed to ICX if the magnetic field of the proposed halo varies between 3-8 times below equipartition levels of 2-5 micro-gauss, which would imply that the confinement is produced by an outside medium. The necessary characteristics of the confining mechanism are discussed.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 312; 101-110
    Format: text
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    NASA TECHNICAL REPORTS
  • 2
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    Airborne and groundbased spectrophotometry of comet P/Halley from 5-13 micrometers (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-12
    Description: Spectrophotometry of comet Halley from 5-13 microns was obtained from the Kuiper Airborne Observatory and from the Lick Observatory Nickel Telescope, revealing a strong broad emission band at 10 microns and a weak feature at 6.8 microns. The 10-micron band is identified with silicate materials, and the primary component of the silicate emission is suggested to be due to olivine. The 6.8 micron feature may be due either to carbonates or the C-H deformation mode in organic molecules. The data indicate that small particles are abundant in the coma and that the dust contains at least two physically separate components. Significant spatial and temporal variations are also noted in the spectrum.
    Keywords: ASTROPHYSICS
    Type: Astronomy and Astrophysics (ISSN 0004-6361); 187; 1-2
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  • 3
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    A simple device for the preparation of embedded materials science specimens for ultramicrotomy (1987)
    In:  Other Sources
    Details
    Publication Date: 2011-08-19
    Description: A simple hand-held grinding fixture is discussed which can produce microtome mounts of hard materials, oriented interfaces, and powders embedded in a 5/16-in plastic rod. The device has been used for the ultramicrotomy of meteorite samples, 10-50 micron interplanetary dust particles, and thin films on plastic. Results are presented for a layer lattice silicate from the Murchison carbonaceous chondrite, illustrating the resolution and structural detail that can be obtained with the method.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Journal of Electron Microscopy Technique (ISSN 0741-0581); 6; 305
    Format: text
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  • 4
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    Collisional and dynamical processes in moon and planet formation (1987)
    In:  CASI
    Details
    Publication Date: 2013-08-31
    Description: Research on a variety of dynamical processes relevant to the formation of planets, satellites and ring systems is discussed. The main focus is on studies of accretionary formation of early protoplanets using a numerical model, structures and evolution of ring systems and individual bodies within planetary rings, and theories of lunar origin.
    Keywords: ASTROPHYSICS
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 112-114
    Format: application/pdf
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  • 5
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    Simultaneous temperature and concentration measurement in front of solidifying monotectic systems using the two wavelength holographic technique (1987)
    In:  Other Sources
    Details
    Publication Date: 2013-08-29
    Description: A holographic technique for the simultaneous measurement of temperature and concentration in solidifying transparent model alloy systems was developed. Its application to the study of the interactions between the temperature, concentration, and fluid flow fields in such systems at 1 g and micro-g conditions is discussed.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: ESA, Proceedings of the Sixth European Symposium on Material Sciences under Microgravity Conditions; p 309-311
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  • 6
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    Noncontact temperature pattern measuring device (1987)
    In:  CASI
    Details
    Publication Date: 2019-06-28
    Description: This invention relates to a noncontact imagine pyrometer system for obtaining the true temperature image of a given substance in a contactless fashion without making assumptions about localized emissivity of the substance or the uniformity of the temperature distribution. Such a contactless temperature imaging system has particular application in the study and production of many materials where the physical contact required to make a conventional temperature measurement drastically effects or contaminates the physical process being observed. Two examples where accurate temperature profiles are of critical interest are: (1) the solid-liquid phase change interface in the production of electronic materials and (2) metastable materials in the undercooling region. The apparent novelty resides in the recognition that an active pyrometer system may be advantageously adapted to perform contactless temperature imaging so that an accurate temperature profile can be obtained.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: NAS 1.71:NPO-17024-1-CU
    Format: application/pdf
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  • 7
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    Design, calibration and error analysis of instrumentation for heat transfer measurements in internal combustion engines (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: The paper reports the methodology and uncertainty analyses of instrumentation for heat transfer measurements in internal combustion engines. Results are presented for determining the local wall heat flux in an internal combustion engine (using a surface thermocouple-type heat flux gage) and the apparent flame-temperature and soot volume fraction path length product in a diesel engine (using two-color pyrometry). It is shown that a surface thermocouple heat transfer gage suitably constructed and calibrated will have an accuracy of 5 to 10 percent. It is also shown that, when applying two-color pyrometry to measure the apparent flame temperature and soot volume fraction-path length, it is important to choose at least one of the two wavelengths to lie in the range of 1.3 to 2.3 micrometers. Carefully calibrated two-color pyrometer can ensure that random errors in the apparent flame temperature and in the soot volume fraction path length will remain small (within about 1 percent and 10-percent, respectively).
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Developments in experimental techniques in heat transfer and combustion; Aug 09, 1987 - Aug 12, 1987; Pittsburgh, PA; United States
    Format: text
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  • 8
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    Molecular clouds and cloud cores in the inner Galaxy (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-12
    Description: A compilation of CO emission regions and their measured parameters is presented which represents a nearly complete accounting of the molecular clouds in the first quadrant of the Galaxy. Emission regions associated with radio H II regions have systematically brighter CO peaks that are a factor of two to three times larger and have twice the mean velocity dispersion as the general cloud population. Both the H II region clouds and the hot core regions have a Galactic distribution characteristic of a spiral arm population, whereas the colder clouds are much less confined in Galactic azimuthal angle. Virial masses are obtained for the large sample of clouds with assigned kinematic distances. The mean H2 density for a GMC of diameter 40 pc is 180/cm. For these clouds, a linear relationship is found between the H2 column density and the integrated CO emission. The variation in the Z-dispersion of clouds as a function of cloud mass suggests that more massive GMCs have smaller random velocities.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal Supplement Series (ISSN 0067-0049); 63; 821-915
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  • 9
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    Discovery of three new RS Canum Venaticorum-like counterparts to HEAO I X-ray sources (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-12
    Description: The identification of three high-latitude HEAO I Scanning Modulation Collimator X-ray sources with the chromospherically active RS CVn-like stars HD 113816, HD 146413, and HD 39576 is reported. Optical observations, including coude spectroscopy and broad-band and narrow band photoelectric photometry are presented. The Ca II emission strength of all three stars shows that they are chromospherically active. HD 146413 and HD 39576 exhibit variable X-ray emission in the 1-13 keV energy range, while HD 113816 is a softer and steadier source. The level of X-ray flux detected from these three stars is some one to two orders of magnitude higher than predicted empirically from the Ca II emission fluxes. It is proposed that this emission results from flarelike activity.
    Keywords: ASTROPHYSICS
    Type: Astrophysical Journal, Part 1 (ISSN 0004-637X); 315; 273-285
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  • 10
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    Radio emission from RS CVn binaries. II - Polarization and spectral properties (1987)
    In:  Other Sources
    Details
    Publication Date: 2019-07-12
    Description: Multiepoch radio observations of circular polarization and spectral characteristics of several close, late-type stellar binaries are reported. The median luminosity of four well-studied systems ranged from 16.2 to 17.1 ergs/s/Hz. For individual systems, the fractional circular polarization decreases with increasing luminosity, particularly at frequencies above 5 GHz. Eclipsing binaries have significantly lower average circular polarization compared with noneclipsing systems. Helicity reversal is almost always observed between 1.4 and 4.9 GHz for systems with high orbital inclination. Comparison with ten years of previously published polarization observations for two RS CVn stellar systems show that the same helicity occurs at a given frequency for a given source, indicating a very stable, large-scale magnetic field geometry. These spectral and polarization characteristics strongly support a model of inhomogeneous gyrosynchrotron emission arising from electrons with power law energy spectra interacting with inhomogeneous magnetic fields.
    Keywords: ASTROPHYSICS
    Type: Astronomical Journal (ISSN 0004-6256); 93; 1220-122
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