Invited Article: Design techniques and noise properties of ultrastable cryogenically cooled sapphire-dielectric resonator oscillators
We review the techniques used in the design and construction of cryogenic sapphire oscillators at the University of Western Australia over the 18 year history of the project. We describe the project from its beginnings when sapphire oscillators were first developed as low-noise transducers for gravi...
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Veröffentlicht in: | Review of scientific instruments 2008-05, Vol.79 (5), p.051301-051301-12 |
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creator | Locke, C. R. Ivanov, E. N. Hartnett, J. G. Stanwix, P. L. Tobar, M. E. |
description | We review the techniques used in the design and construction of cryogenic sapphire oscillators at the University of Western Australia over the
18
year
history of the project. We describe the project from its beginnings when sapphire oscillators were first developed as low-noise transducers for gravitational wave detection. Specifically, we describe the techniques that were applied to the construction of an interrogation oscillator for the PHARAO Cs atomic clock in CNES, in Toulouse France, and to the 2006 construction of four high performance oscillators for use at NMIJ and NICT, in Japan, as well as a permanent secondary frequency standard for the laboratory at UWA. Fractional-frequency fluctuations below
6
×
10
−
16
at integration times between 10 and
200
s
have been repeatedly achieved. |
doi_str_mv | 10.1063/1.2919944 |
format | Article |
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18
year
history of the project. We describe the project from its beginnings when sapphire oscillators were first developed as low-noise transducers for gravitational wave detection. Specifically, we describe the techniques that were applied to the construction of an interrogation oscillator for the PHARAO Cs atomic clock in CNES, in Toulouse France, and to the 2006 construction of four high performance oscillators for use at NMIJ and NICT, in Japan, as well as a permanent secondary frequency standard for the laboratory at UWA. Fractional-frequency fluctuations below
6
×
10
−
16
at integration times between 10 and
200
s
have been repeatedly achieved.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.2919944</identifier><identifier>PMID: 18513054</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><ispartof>Review of scientific instruments, 2008-05, Vol.79 (5), p.051301-051301-12</ispartof><rights>2008 American Institute of Physics</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c368t-4d09054a99ff8d2119c6b42ee9fd7932ac8b5edcade25e4769036a5a9c77f6383</citedby><cites>FETCH-LOGICAL-c368t-4d09054a99ff8d2119c6b42ee9fd7932ac8b5edcade25e4769036a5a9c77f6383</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/rsi/article-lookup/doi/10.1063/1.2919944$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,780,784,794,1559,4512,27924,27925,76384,76390</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/18513054$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Locke, C. R.</creatorcontrib><creatorcontrib>Ivanov, E. N.</creatorcontrib><creatorcontrib>Hartnett, J. G.</creatorcontrib><creatorcontrib>Stanwix, P. L.</creatorcontrib><creatorcontrib>Tobar, M. E.</creatorcontrib><title>Invited Article: Design techniques and noise properties of ultrastable cryogenically cooled sapphire-dielectric resonator oscillators</title><title>Review of scientific instruments</title><addtitle>Rev Sci Instrum</addtitle><description>We review the techniques used in the design and construction of cryogenic sapphire oscillators at the University of Western Australia over the
18
year
history of the project. We describe the project from its beginnings when sapphire oscillators were first developed as low-noise transducers for gravitational wave detection. Specifically, we describe the techniques that were applied to the construction of an interrogation oscillator for the PHARAO Cs atomic clock in CNES, in Toulouse France, and to the 2006 construction of four high performance oscillators for use at NMIJ and NICT, in Japan, as well as a permanent secondary frequency standard for the laboratory at UWA. Fractional-frequency fluctuations below
6
×
10
−
16
at integration times between 10 and
200
s
have been repeatedly achieved.</description><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp1kcFqGzEURUVpiF0ni_5A0arQxSTSSKMZFbowSdoEAtkkayFLb2IVWZpKcsAf0P-OjAe66tvoIQ6Xd-9F6DMlV5QIdk2vWkml5PwDWlIyyKYXLfuIloQw3oieDwv0KeffpE5H6Tla0KGjjHR8if4-hDdXwOJ1Ks54-I5vIbvXgAuYbXB_9pCxDhaH6DLgKcUJKlg_44j3viSdi954wCYd4isEZ7T3B2xi9FUz62naugSNdeDBlOQMTpBj0CUmHLNx3h_XfIHORu0zXM7vCr38vHu-uW8en3493KwfG8PEUBpuiaxXaynHcbAtpdKIDW8B5Gh7yVpthk0H1mgLbQe8F5IwoTstTd-Pgg1shb6edKuRo7Widi4bqFcEiPuseipaKQSv4LcTaFLMOcGopuR2Oh0UJeqYuaJqzryyX2bR_WYH9h85h1yBHyegGi66uBj-rzbXoeY6VG2DvQOXq5SL</recordid><startdate>20080501</startdate><enddate>20080501</enddate><creator>Locke, C. R.</creator><creator>Ivanov, E. N.</creator><creator>Hartnett, J. G.</creator><creator>Stanwix, P. L.</creator><creator>Tobar, M. E.</creator><general>American Institute of Physics</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope></search><sort><creationdate>20080501</creationdate><title>Invited Article: Design techniques and noise properties of ultrastable cryogenically cooled sapphire-dielectric resonator oscillators</title><author>Locke, C. R. ; Ivanov, E. N. ; Hartnett, J. G. ; Stanwix, P. L. ; Tobar, M. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c368t-4d09054a99ff8d2119c6b42ee9fd7932ac8b5edcade25e4769036a5a9c77f6383</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Locke, C. R.</creatorcontrib><creatorcontrib>Ivanov, E. N.</creatorcontrib><creatorcontrib>Hartnett, J. G.</creatorcontrib><creatorcontrib>Stanwix, P. L.</creatorcontrib><creatorcontrib>Tobar, M. E.</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Locke, C. R.</au><au>Ivanov, E. N.</au><au>Hartnett, J. G.</au><au>Stanwix, P. L.</au><au>Tobar, M. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Invited Article: Design techniques and noise properties of ultrastable cryogenically cooled sapphire-dielectric resonator oscillators</atitle><jtitle>Review of scientific instruments</jtitle><addtitle>Rev Sci Instrum</addtitle><date>2008-05-01</date><risdate>2008</risdate><volume>79</volume><issue>5</issue><spage>051301</spage><epage>051301-12</epage><pages>051301-051301-12</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>We review the techniques used in the design and construction of cryogenic sapphire oscillators at the University of Western Australia over the
18
year
history of the project. We describe the project from its beginnings when sapphire oscillators were first developed as low-noise transducers for gravitational wave detection. Specifically, we describe the techniques that were applied to the construction of an interrogation oscillator for the PHARAO Cs atomic clock in CNES, in Toulouse France, and to the 2006 construction of four high performance oscillators for use at NMIJ and NICT, in Japan, as well as a permanent secondary frequency standard for the laboratory at UWA. Fractional-frequency fluctuations below
6
×
10
−
16
at integration times between 10 and
200
s
have been repeatedly achieved.</abstract><cop>United States</cop><pub>American Institute of Physics</pub><pmid>18513054</pmid><doi>10.1063/1.2919944</doi><tpages>1</tpages><oa>free_for_read</oa></addata></record> |
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ispartof | Review of scientific instruments, 2008-05, Vol.79 (5), p.051301-051301-12 |
issn | 0034-6748 1089-7623 |
language | eng |
recordid | cdi_proquest_miscellaneous_71629664 |
source | AIP Journals Complete; AIP Digital Archive; Alma/SFX Local Collection |
title | Invited Article: Design techniques and noise properties of ultrastable cryogenically cooled sapphire-dielectric resonator oscillators |
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