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ELISA: A cryocooled 10 GHz oscillator with 10 − 15 frequency stability
This article reports the design, the breadboarding, and the validation of an ultrastable cryogenic sapphire oscillator operated in an autonomous cryocooler. The objective of this project was to demonstrate the feasibility of a frequency stability of 3 × 10 − 15 between 1 and 1000 s for the European...
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Published in: | Review of scientific instruments 2010-02, Vol.81 (2), p.025102-025102-7 |
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Main Authors: | , , , , , , , , , , |
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Language: | English |
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container_end_page | 025102-7 |
container_issue | 2 |
container_start_page | 025102 |
container_title | Review of scientific instruments |
container_volume | 81 |
creator | Grop, S. Bourgeois, P. Y. Bazin, N. Kersalé, Y. Rubiola, E. Langham, C. Oxborrow, M. Clapton, D. Walker, S. De Vicente, J. Giordano, V. |
description | This article reports the design, the breadboarding, and the validation of an ultrastable cryogenic sapphire oscillator operated in an autonomous cryocooler. The objective of this project was to demonstrate the feasibility of a frequency stability of
3
×
10
−
15
between 1 and 1000 s for the European Space Agency deep space stations. This represents the lowest fractional frequency instability ever achieved with cryocoolers. The preliminary results presented in this paper validate the design we adopted for the sapphire resonator, the cold source, and the oscillator loop. |
doi_str_mv | 10.1063/1.3290631 |
format | article |
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3
×
10
−
15
between 1 and 1000 s for the European Space Agency deep space stations. This represents the lowest fractional frequency instability ever achieved with cryocoolers. The preliminary results presented in this paper validate the design we adopted for the sapphire resonator, the cold source, and the oscillator loop.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.3290631</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>American Institute of Physics</publisher><ispartof>Review of scientific instruments, 2010-02, Vol.81 (2), p.025102-025102-7</ispartof><rights>2010 American Institute of Physics</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2321-4c45b6758406647fdc2d7480705cbb50517540759330ff90519d3d242984377d3</citedby><cites>FETCH-LOGICAL-c2321-4c45b6758406647fdc2d7480705cbb50517540759330ff90519d3d242984377d3</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/10.1063/1.3290631$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>314,780,782,784,795,27924,27925,76255</link.rule.ids></links><search><creatorcontrib>Grop, S.</creatorcontrib><creatorcontrib>Bourgeois, P. Y.</creatorcontrib><creatorcontrib>Bazin, N.</creatorcontrib><creatorcontrib>Kersalé, Y.</creatorcontrib><creatorcontrib>Rubiola, E.</creatorcontrib><creatorcontrib>Langham, C.</creatorcontrib><creatorcontrib>Oxborrow, M.</creatorcontrib><creatorcontrib>Clapton, D.</creatorcontrib><creatorcontrib>Walker, S.</creatorcontrib><creatorcontrib>De Vicente, J.</creatorcontrib><creatorcontrib>Giordano, V.</creatorcontrib><title>ELISA: A cryocooled 10 GHz oscillator with 10 − 15 frequency stability</title><title>Review of scientific instruments</title><description>This article reports the design, the breadboarding, and the validation of an ultrastable cryogenic sapphire oscillator operated in an autonomous cryocooler. The objective of this project was to demonstrate the feasibility of a frequency stability of
3
×
10
−
15
between 1 and 1000 s for the European Space Agency deep space stations. This represents the lowest fractional frequency instability ever achieved with cryocoolers. The preliminary results presented in this paper validate the design we adopted for the sapphire resonator, the cold source, and the oscillator loop.</description><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp1kM9KxDAQxoMoWFcPvkGuHrpO_jWNeCnLul0oeFDPoU1bjNSNJhWpT-DZR_RJzLoLnpzLzDd8DN_8EDonMCeQsUsyZ1TFgRyghECuUplRdogSAMbTTPL8GJ2E8ASxBCEJKpfV-q64wgU2fnLGuaFrMQG8Kj-wC8YOQz06j9_t-Lhdf39-YSJw77vXt25jJhzGurGDHadTdNTXQ-jO9n2GHm6W94syrW5X60VRpYYySlJuuGgyKXIOWcZl3xraxlQgQZimETGUFBykUIxB36uoVctayqnKOZOyZTN0sbtrvAvBd71-8fa59pMmoLcINNF7BNF7vfPGR8Z6tG7zv_mXgy70Hwb2A24QXi0</recordid><startdate>20100212</startdate><enddate>20100212</enddate><creator>Grop, S.</creator><creator>Bourgeois, P. Y.</creator><creator>Bazin, N.</creator><creator>Kersalé, Y.</creator><creator>Rubiola, E.</creator><creator>Langham, C.</creator><creator>Oxborrow, M.</creator><creator>Clapton, D.</creator><creator>Walker, S.</creator><creator>De Vicente, J.</creator><creator>Giordano, V.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20100212</creationdate><title>ELISA: A cryocooled 10 GHz oscillator with 10 − 15 frequency stability</title><author>Grop, S. ; Bourgeois, P. Y. ; Bazin, N. ; Kersalé, Y. ; Rubiola, E. ; Langham, C. ; Oxborrow, M. ; Clapton, D. ; Walker, S. ; De Vicente, J. ; Giordano, V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2321-4c45b6758406647fdc2d7480705cbb50517540759330ff90519d3d242984377d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Grop, S.</creatorcontrib><creatorcontrib>Bourgeois, P. Y.</creatorcontrib><creatorcontrib>Bazin, N.</creatorcontrib><creatorcontrib>Kersalé, Y.</creatorcontrib><creatorcontrib>Rubiola, E.</creatorcontrib><creatorcontrib>Langham, C.</creatorcontrib><creatorcontrib>Oxborrow, M.</creatorcontrib><creatorcontrib>Clapton, D.</creatorcontrib><creatorcontrib>Walker, S.</creatorcontrib><creatorcontrib>De Vicente, J.</creatorcontrib><creatorcontrib>Giordano, V.</creatorcontrib><collection>CrossRef</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Grop, S.</au><au>Bourgeois, P. Y.</au><au>Bazin, N.</au><au>Kersalé, Y.</au><au>Rubiola, E.</au><au>Langham, C.</au><au>Oxborrow, M.</au><au>Clapton, D.</au><au>Walker, S.</au><au>De Vicente, J.</au><au>Giordano, V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>ELISA: A cryocooled 10 GHz oscillator with 10 − 15 frequency stability</atitle><jtitle>Review of scientific instruments</jtitle><date>2010-02-12</date><risdate>2010</risdate><volume>81</volume><issue>2</issue><spage>025102</spage><epage>025102-7</epage><pages>025102-025102-7</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>This article reports the design, the breadboarding, and the validation of an ultrastable cryogenic sapphire oscillator operated in an autonomous cryocooler. The objective of this project was to demonstrate the feasibility of a frequency stability of
3
×
10
−
15
between 1 and 1000 s for the European Space Agency deep space stations. This represents the lowest fractional frequency instability ever achieved with cryocoolers. The preliminary results presented in this paper validate the design we adopted for the sapphire resonator, the cold source, and the oscillator loop.</abstract><pub>American Institute of Physics</pub><doi>10.1063/1.3290631</doi><oa>free_for_read</oa></addata></record> |
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source | American Institute of Physics:Jisc Collections:Transitional Journals Agreement 2021-23 (Reading list); AIP_美国物理联合会现刊(与NSTL共建) |
title | ELISA: A cryocooled 10 GHz oscillator with 10 − 15 frequency stability |
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