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Noise characteristics of rare-earth-doped fiber sources and amplifiers

Noise characteristics of rare-earth-doped fiber sources and amplifiers
Noise characteristics of rare-earth-doped fiber sources and amplifiers
The A.M. and F.M. noise mechanisms in a number of rare-earth doped fiber devices are reviewed. Spontaneous emission noise presents an ultimate limit to the performance of a number of fiber laser and amplifier devices and the paper concentrates primarily on this area. Important concepts are reviewed and experimental and theoretical data are presented.
9780819404343
Morkel, Paul
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Laming, Richard I.
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Cowle, Gregory J.
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Payne, David N.
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Morkel, Paul
f58fd0b9-846f-4829-ab0e-f82c94e47c46
Laming, Richard I.
7a3db66b-2c54-43e3-bdd8-ab45c9195cd4
Cowle, Gregory J.
eccef571-7712-4b83-9754-2305a6e34ed6
Payne, David N.
4f592b24-707f-456e-b2c6-8a6f750e296d

Morkel, Paul, Laming, Richard I., Cowle, Gregory J. and Payne, David N. (1990) Noise characteristics of rare-earth-doped fiber sources and amplifiers. SPIE 1373 : Fiber Laser Sources and Amplifiers II, San Jose, United States. 16 - 21 Sep 1990. (doi:10.1117/12.24945).

Record type: Conference or Workshop Item (Paper)

Abstract

The A.M. and F.M. noise mechanisms in a number of rare-earth doped fiber devices are reviewed. Spontaneous emission noise presents an ultimate limit to the performance of a number of fiber laser and amplifier devices and the paper concentrates primarily on this area. Important concepts are reviewed and experimental and theoretical data are presented.

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e-pub ahead of print date: January 1990
Venue - Dates: SPIE 1373 : Fiber Laser Sources and Amplifiers II, San Jose, United States, 1990-09-16 - 1990-09-21
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Identifiers

Local EPrints ID: 77468
URI: http://eprints.soton.ac.uk/id/eprint/77468
DOI: doi:10.1117/12.24945
ISBN: 9780819404343
PURE UUID: 1d85ea40-a4b8-48ae-b327-1d8fdc3d9a19

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Date deposited: 11 Mar 2010
Last modified: 13 Mar 2024 23:53

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Contributors

Author: Paul Morkel
Author: Richard I. Laming
Author: Gregory J. Cowle
Author: David N. Payne

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