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  • INSTRUMENTATION AND PHOTOGRAPHY  (6)
  • LASERS AND MASERS  (1)
  • 1975-1979  (7)
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  • 1
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    Infrared heterodyne spectroscopy of astronomical and laboratory sources at 8.5 microns (1975)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: It is pointed out that the first successful infrared heterodyne spectrometer featuring semituneable semiconductor diode lasers was constructed and used near 8.5 micrometers to make laboratory measurements of line profiles in nitrous oxide and to detect thermal emission from Mars and from the moon. Questions of instrument design are discussed along with the significance of the results obtained in the investigation.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Nature; 253; Feb. 13
    Format: text
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  • 2
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    Sensitivity of an astronomical infrared heterodyne spectrometer (1976)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: The factors determining the sensitivity of a real astronomical heterodyne spectrometer are described. The deviation from the ideal heterodyne system for line detection is described in terms of a series of degradation factors. A discussion of degradation due to a low local oscillator power and to line profile detection is presented. Representative values for the degradation factors are given. Even with a total degradation of not less than 30, the heterodyne spectrometer is still found to be a highly sensitive tool in IR astronomy.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
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  • 3
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    Infrared upconversion for astronomical applications (1976)
    In:  Other Sources
    Details
    Publication Date: 2011-08-16
    Description: The performance of an upconversion system is examined for observation of astronomical sources in the low to middle IR spectral range. Theoretical values for the performance parameters of an upconversion system for astronomical observations are evaluated in terms of the conversion efficiencies, spectral resolution, field of view minimum detectable source brightness, and source flux. Experimental results of blackbody measurements and molecular absorption-spectrum measurements using a lithium niobate upconverter with an argon-ion laser as the pump are presented. Estimates are given of the expected optimum sensitivity of an upconversion device that may be built with presently available components.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Applied Optics; 15; Apr. 197
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  • 4
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    Upconversion spectrometry for astrophysical applications (1976)
    In:  Other Sources
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    Publication Date: 2011-08-16
    Description: Black body measurements and absorption spectra of methane near 3.3 microns are presented and used as examples in a discussion of upconversion spectrometry for astrophysical application. Factors determining the system conversion efficiency and the minimum detectable flux for a typical system are presented. The spectrometer described uses an Argon-ion laser and a temperature turned LiNbO3 crystal in a CW mode. Satisfactory agreement between measured and calculated performance parameters is obtained. An estimate of the highest performance parameters attainable using current technology is given.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
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  • 5
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    Precision measurements of NH3 spectral lines near 11 microns using the infrared heterodyne technique (1977)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: Absolute line-center frequencies for eleven lines of ammonia in near coincidence with CO2-laser transitions have been determined to accuracies of + or -3 MHz by infrared heterodyne detection. These results were obtained by heterodyning a blackbody with a stable grating-tuned CO2 gas laser. A discussion of the apparatus and method of calculation, including error analysis, is presented. With these accurately determined line-center positions, the ammonia molecule will be a useful secondary-frequency standard for diode-laser spectroscopy in the 11-micron wavelength region.
    Keywords: LASERS AND MASERS
    Type: Optics Letters; 1; Sept
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  • 6
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    Sensitivity limits of an infrared heterodyne spectrometer for astrophysical applications (1976)
    In:  Other Sources
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    Publication Date: 2011-08-16
    Description: A discussion and an evaluation of the degradation in sensitivity are given for a heterodyne spectrometer employing a HgCdTe photodiode mixer and tunable diode lasers. The minimum detectable source brightness is considered as a function of the mixer parameters, transmission coefficient of the beam splitter, and local oscillator emission powers. The degradation in the minimum detectable line source brightness that results from the bandwidth being a fraction of the line width is evaluated and plotted as a function of the wavelength and bandwidth for various temperature to mass ratios. It is shown that the minimum achievable degradation in the sensitivity of a practical astronomical heterodyne spectrometer is about 30. Estimates of SNRs with which IR line emission from astronomical sources of interest may be detected are given.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Applied Optics; 15; Feb. 197
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  • 7
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    A 10 micron laser heterodyne spectrometer for remote detection of trace gases (1978)
    In:  Other Sources
    Details
    Publication Date: 2011-08-17
    Description: Infrared heterodyne spectroscopy provides a means of measuring the intensity profiles of individual rotation-vibration spectral lines with high sensitivity. Considerable effort has been expended on optimizing these instruments for remote measurements of gases in planetary atmospheres with the result that present-generation spectrometers are beginning to provide new and startling results on the planets. The fundamental principles of laser heterodyne spectroscopy are discussed. Detailed considerations of the optical design and the electronic design of the spectral-line receiver are given. Representative results obtained with this spectrometer are discussed, including precision frequency measurements of NH3 (nu-2) lines, detection of auroral emission from Jupiter, and measurements of terrestrial O3 and CO2.
    Keywords: INSTRUMENTATION AND PHOTOGRAPHY
    Type: Optical Engineering; 17; Jan
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