ELISA: A cryocooled 10 GHz oscillator with 10-15 frequency stability

被引：45

作者：

Grop, S. ^{[1
]}

Bourgeois, P. Y. ^{[1
]}

Bazin, N. ^{[1
]}

Kersale, Y. ^{[1
]}

Rubiola, E. ^{[1
]}

Langham, C. ^{[2
]}

Oxborrow, M. ^{[2
]}

Clapton, D. ^{[3
]}

Walker, S. ^{[3
]}

De Vicente, J. ^{[4
]}

Giordano, V. ^{[1
]}

机构：

[1] CNRS ENSMM, UMR 6174, FEMTO ST Inst, Dept Time & Frequency, F-25044 Besancon, France

[2] Natl Phys Lab, Teddington TW11 0LW, Middx, England

[3] Oxford Instruments Plc, Tubney Woods, Abingdon OX13 5QX, Oxon, England

[4] European Space Agcy, ESOC, D-64293 Darmstadt, Germany

来源：

REVIEW OF SCIENTIFIC INSTRUMENTS | 2010年 / 81卷 / 02期

关键词：

cryogenic electronics; frequency stability; oscillators; resonators; sapphire; CRYOGENIC SAPPHIRE OSCILLATOR; RESONATOR; STABILIZATION; DESIGN; PHASE; NOISE; DRIFT;

D O I：

10.1063/1.3290631

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

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 3x10(-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.

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