• DocumentCode
    1432658
  • Title

    Generation of 103.75 GHz CW Source With 5.10^{-16} Frequency Instability Using Cryogenic Sapphire Oscillators

  • Author

    Bara, Romain ; Floch, Jean-Michel Le ; Tobar, Michael E. ; Stanwix, Paul L. ; Parker, Stephen R. ; Hartnett, John G. ; Ivano, Eugene N.

  • Author_Institution
    Sch. of Phys., Univ. of Western Australia, Crawley, WA, Australia
  • Volume
    22
  • Issue
    2
  • fYear
    2012
  • Firstpage
    85
  • Lastpage
    87
  • Abstract
    We report the generation of millimeter wave signals with frequency instability of a few parts in 1016. Such performance was achieved at 103.750 GHz by frequency multiplication of two nominally identical 12.969 GHz oscillators based on liquid helium cooled sapphire dielectric resonators. The multiplication stages were shown to only add a small amount of noise at averaging times less than 10 s, resulting in a minimum of frequency instability of 5×10-16 at 20 s averaging time. Such ultra-stable signal sources operating at frequencies of 100 GHz are very important for many applications including high frequency radio astronomy.
  • Keywords
    cryogenics; dielectric resonators; frequency multipliers; millimetre wave generation; millimetre wave oscillators; sapphire; CW source; cryogenic sapphire oscillators; frequency 103.75 GHz; frequency 12.969 GHz; frequency instability; frequency multiplication; liquid helium cooled sapphire dielectric resonators; millimetre wave generation; Cryogenics; Noise; Oscillators; Resonant frequency; Stability criteria; Time frequency analysis; ATACAMA; CW source; EHF; SKA; cryogenic sapphire oscillators (CSO); doubler; high-q; mm-wave; multiplication; oscillator; sapphire; stability; synthesis; very long baseline interferometry (VLBI);
  • fLanguage
    English
  • Journal_Title
    Microwave and Wireless Components Letters, IEEE
  • Publisher
    ieee
  • ISSN
    1531-1309
  • Type

    jour

  • DOI
    10.1109/LMWC.2011.2181347
  • Filename
    6140593