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Prototype of an ultra-stable optical cavity for space applications
B Argence1, E Prevost, T Lévèque
1Laboratoire national de métrologie et d’essais - Systèmes de Références Temps-Espace, Observatoire de Paris, CNRS, UMR 8630, 61 Av. de l’Observatoire, 75014 Paris, France. berengere.argence@obspm.fr
Optics Express
|November 29, 2012
Summary
This study presents an ultra-stable cavity prototype for space missions, demonstrating excellent thermal and vibration isolation. It achieves remarkable fractional frequency instability, crucial for advanced space applications.
Area of Science:
- Physics
- Optical Engineering
- Space Technology
Background:
- Ultra-stable cavities are essential for high-precision frequency standards.
- Space missions require robust systems resistant to environmental perturbations.
Purpose of the Study:
- To design and characterize an ultra-stable cavity prototype for space applications.
- To optimize thermal and vibration sensitivities for space environments.
- To evaluate the system's performance under operational constraints.
Main Methods:
- Finite element modeling for optimization of thermal and vibration sensitivities.
- Mechanical design featuring rigid mounting for perturbation decoupling.
- Thermal isolation using gold-coated aluminum shields within a stainless steel enclosure.
- Experimental evaluation of vibration sensitivity and fractional frequency instability.
Main Results:
- Achieved axial vibration sensitivity of (4 ± 0.5) × 10⁻¹¹/(m·s⁻²).
- Transverse vibration sensitivity below 1 × 10⁻¹¹/(m·s⁻²).
- Fractional frequency instability of ~1×10⁻¹⁵ at short integration times, reaching 5-6×10⁻¹⁶ at 1 second.
- Designed for transportability, high acceleration tolerance (up to several g), and a wide temperature range [-33°C; 73°C].
Conclusions:
- The prototype demonstrates high stability and robustness suitable for demanding space missions.
- The engineered mechanical interface effectively decouples the cavity from environmental disturbances.
- The achieved performance metrics meet the stringent requirements for future space-based frequency standards.

