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  • Other Sources  (5)
  • 1
    Publication Date: 2016-06-07
    Description: A 163 micron (1.836 THz) radiometer developed for airplane and/or balloon platforms is described. The laser local oscillator is a CO2 pumped methanol laser operating at a frequency which is approx. 1 GHz from the J = 3/2 - 1/2 transition of OH. The laser is used directly as a local oscillator or is translated in frequency to closer coincidence with the OH emission, depending on achieved detector IF bandwidth. Frequency translation techniques which are described are diode mixing and a method of single sideband generation using an external Stark modulated gas cell. The photoconductive mixer used is a strained Ge crystal, doped with Ga, originally used as an incoherent detector. The uniaxial strain on the Ga doped Ge crystal shifts the threshold for photoconduction from 100/cm to frequencies as low as 50/cm. These detectors are currently being characterized as mixers in the laboratory. Of particular interest are the effect of local oscillator power and strain on IF, bandwidth detector impedance, and conversion loss. Preliminary results of these tests are described and compared with theorectical expectations.
    Keywords: LASERS AND MASERS
    Type: NASA. Langley Res. Center Heterodyne Systems and Technol., Pt. 1; p 241-248
    Format: application/pdf
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  • 2
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    In:  CASI
    Publication Date: 2019-05-11
    Description: Type iii solar radio noise - frequency polarization and drift rate
    Keywords: BIOTECHNOLOGY
    Type: BN-290
    Format: text
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  • 3
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    In:  Other Sources
    Publication Date: 2019-05-22
    Description: Radio noise generation due to plasma oscillations, using the collisionless boltzmann equation
    Keywords: PHYSICS, ATOMIC, MOLECULAR, AND NUCLEAR
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  • 4
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    In:  CASI
    Publication Date: 2019-05-21
    Description: Generation of radio noise by plasma oscillations
    Keywords: PHYSICS, ATOMIC, MOLECULAR, AND NUCLEAR
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  • 5
    Publication Date: 2019-07-12
    Description: This brief describes two monolithic microwave integrated-circuit (MMIC) amplifier chips optimized to function in the frequency range of 90 to 130 GHz, covering nearly all of F-band (90 - 140 GHz). These amplifiers were designed specifically for local-oscillator units in astronomical radio telescopes such as the Atacama Large Millimeter Array (ALMA). They could also be readily adapted for use in electronic test equipment, automotive radar systems, and communications systems that operate between 90 and 130 GHz.
    Keywords: Electronics and Electrical Engineering
    Type: NPO-41481 , NASA Tech Briefs, October 2007; 27
    Format: application/pdf
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