Coherent telescope array with self-homodyne interferometric detection for optical communications

Coherent telescope array with self-homodyne interferometric detection for optical communications
Opt. Eng., Vol. 42, 3139 (2003); DOI:10.1117/1.1612512
Online Publication Date: 31 October 2003

ABSTRACT
REFERENCES (28)
CITING ARTICLES
Bernard Eng-Kie Souw

BMS Enterprise, P.O. Box 5524, Herndon, Virginia 20172-5524
E-mail: souw1@juno.com

The performance of a coherent telescope array (CTA) as an optical communications receiving system is analyzed with regards to the benefits and disadvantages in comparison to monolithic large-aperture single telescopes and conventional photon bucket systems, especially in terms of background photons. The bit error rates for differential phase-shift keying (DPSK) and binary pulse position modulation (BPPM) schemes are derived, the former using self-homodyne interferometry as a novel demodulation technique, in which the background photons interact incoherently. The possibility of further dividing the receiver’s aperture into N>2 smaller subtelescopes is explored, and its adaptability for implementing the N binary phase-shift keying (N-BPSK) technique with optical code division multiplexing (OCDM) is discussed. An N-CTA receiver system with an N-BPSK/OCDM technique is envisioned not only to achieve multiterabit per second data transfer capability, but also to adapt a novel noise suppression technique based on photon correlations, which would render a need for expensive and complicated adaptive optics obsolete. Further combined with significant reduction in weight and overall costs, an N-CTA system with an N-BPSK/OCDM technique could serve in deep space communications as well as in defense to achieve information dominance in the battlefield.

©2003 Society of Photo-Optical Instrumentation Engineers.
History: Received Feb. 6, 2003; revised May 6, 2003; accepted May 12, 2003
DOI Link: http://dx.doi.org/10.1117/1.1612512

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