Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

FDMA-FSK 1 Gb/s Star Network Using LD-Pumped Erbium-Doped Fiber Preamplifiers with Optimal Noise Filtering

Not Accessible

Your library or personal account may give you access

Abstract

A key advantage of a frequency-division-multiple-access (FDMA) optical star network is high-speed simultaneous distribution of information to many users. An attractive implementation [1,2] is to frequency-shift-key (FSK) modulate N laser transmitters (Tx) and use direct-detection receivers (Rx), each consisting of a fiber Fabry-Perot [3] demodulator/demultiplexer. One disadvantage of this simple scheme is the limitation placed on the number of network users due to the inherent (1/N) power splitting losses of the N×N star coupler. These splitting losses as well as substantial component insertion losses can be compensated for by including an Erbium-doped fiber amplifier (EDFA) [4-6] in each receiver [1]. Such amplifiers have the advantages of being compatible with a fiber-based system, providing high gain and output saturation power, and being insensitive to polarization and crosstalk effects.

© 1990 Optical Society of America

PDF Article
More Like This
1.2-Gbit/s closely spaced FDMA- FSK direct-detection star network using two-electrode DFB lasers

A. E. WILLNER, I. P. KAMINOW, M. KUZNETSOV, J. STONE, and L. W. STULZ
CWI3 Conference on Lasers and Electro-Optics (CLEO:S&I) 1990

Active star couplers using multiple erbium-doped fibers pumped with a single laser

A. E. Willner, A. A. M. Saleh, H. M. Presby, D. J. DiGiovanni, and C. A. Edwards
CThJ4 Conference on Lasers and Electro-Optics (CLEO:S&I) 1991

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.