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Optical Fibres in Radioastronomy

Published online by Cambridge University Press:  19 July 2016

Alan C. Young*
Affiliation:
CSIRO Radiophysics Laboratory, PO Box 76, Epping 2121, Australia

Abstract

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Within the recently completed Australia Telescope, optical fibres are used extensively to carry wideband IF data, LO reference signals, timing signals and computer communications. This paper discusses the various options considered in the design of the optical fibre system.

Type
Impact of Technology I: Radio and Millimeter Waves
Copyright
Copyright © Kluwer 1994 

References

Primus, L.E., Lutes, G.F., and Sydnor, R.L. “Stabilized Fiber- Optic Frequency Distribution System” The Telecommunications and Data Acquisition Progress Report, J an-Mar 1989, pp8897, NASA JPL.Google Scholar
Lutes, G and Primus, L “State-of-the-Art Fiber Optics for Short Distance Frequency Reference Distribution” The Telecommunications and Data Acquisition Progress Report, J an-Mar 1989, pp8187, NASA JPL.Google Scholar
Primus, L.E., Logan, R.T., Lutes, G.F., and Maleki, L. “Distributuion of Ultra Stable Reference Frequency Signals Over Fiber Optic Cable” AFCEA Department of Defense Fiber optics conference proceedings McLean Virginia 20 March 1990 pp352356.Google Scholar
Sarma, N.V.G. “Optical Fibre Link For Reference Frequency Distribution” Australia Telescope technical report AT/23.2/020, Feb 1988.Google Scholar
Cooper, R. “Fiber Optic Insertion Loss Measurements… How They Relate to System Use” Technical paper P 270–83, 1983, pp20814–20827 AMP Incorporated, Harrisburg, PA.Google Scholar
Epworth, R.E. “Modal Noise - Causes and Cures” Laser Focus, Sept. 1981, pp109115 Google Scholar