Title :
WDM coherent optical star network
Author :
Glance, Bernard S. ; Pollock, K. ; Burrus, Charles A. ; Kasper, Bryon L. ; Einstein, G. ; Stulz, Lawrence W.
Author_Institution :
AT&T Bell Labs., Holmdel, NJ, USA
fDate :
1/1/1988 12:00:00 AM
Abstract :
The results obtained with a fiber-optical star network using densely-spaced wavelength division multiplexing (WDM) and heterodyne detection techniques are reported. The system consists of three lasers transmitting at optical frequencies around 234000 GHz, spaced at a frequency interval of 300 MHz. The lasers are frequency-shift-key (FSK) modulated at 45 Mb/s. A 4×4 optical star coupler combines the three optical signals. The WDM signals received from one of the four outputs of the star coupler are demultiplexed by a heterodyne receiver. The minimum received optical power needed to obtain a bit-error rate of 10-9 is -61 dBm or 113 photon/bit, which is 4.5 dB from the shot noise limit. The degradation caused by co-channel interference was measured and found to be negligible when the channels, modulated at 45 Mb/s, are spaced by more than 130 MHz in the IF domain. These results indicate that a WDM coherent optical star network of this type has a potential throughput of 4500 Gb/s
Keywords :
frequency division multiplexing; frequency shift keying; optical couplers; optical fibres; optical links; 234000 GHz; 45 Mbit/s; 4500 Gbit/s; IF domain; WDM; bit-error rate; co-channel interference; fiber-optical star network; frequency-shift-key lasers; heterodyne detection techniques; heterodyne receiver; laser modulation; minimum received optical power; optical frequencies; optical signals; wavelength division multiplexing; Fiber lasers; Frequency modulation; Frequency shift keying; Optical coupling; Optical fiber networks; Optical mixing; Optical modulation; Optical noise; Optical receivers; Wavelength division multiplexing;
Journal_Title :
Lightwave Technology, Journal of