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  • 1
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    Unknown
    In:  Other Sources
    Publication Date: 2011-08-12
    Description: Photon bunching effect in spatially coherent noise field enhanced by superposing monochromatic coherent signal and/or shaping incident noise spectra
    Keywords: COMMUNICATIONS
    Type: ; ADEMIE DES SCIENCES
    Format: text
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  • 2
    Publication Date: 2019-07-20
    Description: Ammonia concentrations reached minimal levels (approximately 0.1 ppb) in early winter, followed by a sudden later winter increase. A direct relationship between ambient ammonia levels and air temperature was inferred from the data (linear correlation coefficient r=0.53). Ammonia concentrations were determined to be directly related to the absolute humidity of the air (r=0.72); a weaker relationship between ammonia concentrations and relative humidity was discovered (r=0.37). The data also indicated that ammonia levels were generally higher within continental air masses than those of maritime origin. Soil parameters such as pH and moisture content were found to have a major bearing on the release of gaseous ammonia from soils in the region.
    Keywords: METEOROLOGY AND CLIMATOLOGY
    Type: NASA-CR-164188
    Format: application/pdf
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  • 3
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    Unknown
    In:  CASI
    Publication Date: 2019-06-27
    Description: Mathematical model of communication systems including quantum effects
    Keywords: COMMUNICATIONS
    Type: NASA-TM-X-61522
    Format: application/pdf
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  • 4
    Publication Date: 2019-08-14
    Description: An investigation was made to determine the optimum detection scheme for a star-field mapping system that uses coded detection resulting from starlight shining through specially arranged multiple slits of a reticle. The computer solution of equations derived from a theoretical model showed that the greatest probability of detection for a given star and background intensity occurred with the use of a single transparent slit. However, use of multiple slits improved the system's ability to reject the detection of undesirable lower intensity stars, but only by decreasing the probability of detection for lower intensity stars to be mapped. Also, it was found that the coding arrangement affected the root-mean-square star-position error and that detection is possible with error in the system's detected spin rate, though at a reduced probability.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: NASA-TN-D-5972 , L-6477
    Format: application/pdf
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