DocumentCode
1965140
Title
Characterization of an ultra-stable optical cavity developed in the industry for space applications
Author
Argence, B. ; Bize, S. ; Lemonde, P. ; Santarelli, Giorgio ; Prevost, E. ; Le Goff, R. ; Leveque, Thomas
Author_Institution
LNE-SYRTE, Obs. de Paris, UPMC, Paris, France
fYear
2012
fDate
23-27 April 2012
Firstpage
550
Lastpage
553
Abstract
We report the main characteristics and performances of the first - to our knowledge - prototype of an ultra-stable cavity designed and produced by industry with the aim of space missions. Finite element modeling was performed in order to minimize thermal and vibration sensitivities. The system was designed to be transportable, acceleration tolerant (up to several g) and temperature range compatible (ΔT ~ 40 K). The optical axis of the 100 mm long cavity is vertical. The spacer is made from Ultra-Low Expansion (ULE) glass and mirrors substrate from fused silica to reduce the thermal noise limit to 4×10-16. The axial vibration sensitivity was evaluated at (4 ± 0.5) ×10-11 /(ms-2), while the transverse one is <; 1×10-11 /(ms-2). The fractional frequency instability is ~ 1×10-15 from 0.1 to few seconds.
Keywords
Fabry-Perot interferometers; aerospace instrumentation; finite element analysis; laser cavity resonators; laser mirrors; optical glass; thermal noise; ULE; acceleration tolerant; axial vibration sensitivity; finite element modeling; glass; mirror; optical axis; size 100 mm; space mission; thermal noise limit; transportability; ultralow expansion; ultrastable optical cavity;
fLanguage
English
Publisher
ieee
Conference_Titel
European Frequency and Time Forum (EFTF), 2012
Conference_Location
Gothenburg
Print_ISBN
978-1-4673-1924-9
Type
conf
DOI
10.1109/EFTF.2012.6502440
Filename
6502440
Link To Document