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
Link To Document :
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