DocumentCode
1432658
Title
Generation of 103.75 GHz CW Source With
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