Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/87407
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Type: Journal article
Title: Generation of 103.75 GHz CW source with 5.10‾¹⁶ frequency instability using cryogenic sapphire oscillators
Other Titles: Generation of 103.75 GHz CW source with 5.10-bar(16) frequency instability using cryogenic sapphire oscillators
Author: Bara, R.
Le Floch, J.
Tobar, M.
Stanwix, P.
Parker, S.
Hartnett, J.
Ivanov, E.
Citation: IEEE Microwave and Wireless Components Letters, 2012; 22(2):85-87
Publisher: Institute of Electrical and Electronics Engineers
Issue Date: 2012
ISSN: 1531-1309
1558-1764
Statement of
Responsibility: 
Romain Bara, Jean-Michel Le Floch, Michael E. Tobar, Paul L. Stanwix, Stephen R. Parker, John G. Hartnett, and Eugene N. Ivanov
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: ATACAMA; CW source; EHF; SKA; cryogenic sapphire oscillators (CSO); doubler; high-q; mm-wave; multiplication; oscillator; sapphire; stability; synthesis; very long baseline interferometry (VLBI)
Rights: © 2011 IEEE
DOI: 10.1109/LMWC.2011.2181347
Grant ID: http://purl.org/au-research/grants/arc/DP0878108
http://purl.org/au-research/grants/arc/FL0992016
http://purl.org/au-research/grants/arc/DP0878108
Published version: http://dx.doi.org/10.1109/lmwc.2011.2181347
Appears in Collections:Aurora harvest 2
Physics publications

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