Effect of four-wave mixing on optimal placement of optical amplifier in WDM star networks

被引：13
|
作者：
Singh, SP
Kar, S
Jain, VK
机构：
[1] Netaji Subhash Inst Technol, Dept ECE, New Delhi 110075, India
[2] Indian Inst Technol, Dept Elect Engn, New Delhi 110016, India
来源：
FIBER AND INTEGRATED OPTICS | 2006年 / 25卷 / 02期
关键词：
four-wave mixing (FWM); amplified spontaneous emission (ASE) noise; amplifier placement; probability of error;
D O I：
10.1080/01468030500466289
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
In this article, the effect of four-wave mixing (FWM) and amplified spontaneous emission (ASE) noise on WDM optical star networks has been investigated. Analysis for the evaluation of probability of error has been carried out (a) when only FWM is present and (b) when both FWM and ASE noise are present. Numerical results are presented in the graphical and tabular forms for the practical values of parameters. Finally, optimal location of the amplifier in the network has been identified as being before the star coupler preceding the receiver.
引用
收藏
页码：111 / 140
页数：30
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