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Rapid Communication
01 January 1992

Fundamental phase noise limit in optical fibres due to temperature fluctuations

Abstract

Theoretical results are presented for the power and RMS amplitude spectra of phase noise in optical fibres due to thermodynamic temperature fluctuations, including the effects of finite fibre outside diameter and retardation. For a fibre optic Mach–Zehnder interferometer with 20m of 125μm diameter fibre in each arm, the (0–25) kHz phase noise is (5.1–1.3) × 10−7rad RMS/√(Hz) at 1300nm.

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References

1.
Bucholtz F., Coluander J.E., and Dandridge A. Thermal noise spectrum of a fiber-optic magnetostrictive transducer Opt. Lett. 16 432-434 1991
2.
Yartv A. Optical electronics 3rd edn 315-317 Holt, Rinehart, and Winston Orlando, FL 1985
3.
Shapiro J.H., Shepard S.R., and Wong N.C. Ultimate quantum limits on phase measurement Phys. Rev. Lett. 62 2377-2380 1989
4.
Kersey A.D. Private conversation Proc. Conf. Lasers and Electro Optics (CLEO) 1990 Anaheim, CA
5.
Landau L. and Lifshitz E.M. Fluid mechanics 523-529 Pergamon Oxford 1959
6.
Wanser K.H. Interferometric sensor length limitations due to distributed phase modulation Proc. SPIE 718 256-258 1986
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Glenn W.H. Noise in interferometric optical systems an optical Nyquist theorem IEEE J. Quantum Electron. QE-25 1218-1224 June1989

Information and Authors

Information

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History

Published online: 01 January 1992
Published in print: 02 January 1992

Inspec keywords

  1. fibre optic sensors
  2. light interferometers
  3. optical fibres

Keywords

  1. optical fibres
  2. temperature fluctuations
  3. power
  4. RMS amplitude spectra
  5. phase noise
  6. fibre outside diameter
  7. retardation
  8. fibre optic Mach-Zehnder interferometer
  9. 1300 nm
  10. 20 m

Keywords

  1. Noise
  2. Optical fibres

Authors

Affiliations

K.H. Wanser
Department of Physics, California State University Fullerton, Fullerton, WCA 92634, USA

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