Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA

Spectral hole burning (SHB) effects in a gain-flattened erbium-doped fiber amplifier (EDFA) are demonstrated to be significant in the presence of large signal power around the 1530-1532-nm wavelength range. These are the first effects reported in a setup employing equivalent power level distribution...

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Auteurs principaux: Sarmani, A.R., Sheih, S.J., Adikan, Faisal Rafiq Mahamd, Mahdi, M.A.
Format: Article
Publié: 2011
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author Sarmani, A.R.
Sheih, S.J.
Adikan, Faisal Rafiq Mahamd
Mahdi, M.A.
author_facet Sarmani, A.R.
Sheih, S.J.
Adikan, Faisal Rafiq Mahamd
Mahdi, M.A.
author_sort Sarmani, A.R.
collection UM
description Spectral hole burning (SHB) effects in a gain-flattened erbium-doped fiber amplifier (EDFA) are demonstrated to be significant in the presence of large signal power around the 1530-1532-nm wavelength range. These are the first effects reported in a setup employing equivalent power level distribution of 40 channels ranging from 1530 to 1561 am. To explain this, the introduction of a new local population variable into the laser equation is required to support the original inversion ratio that is determined by the pump lasers. In the analysis section, spectroscopic parameters and high signal powers are considered to be other contributing parameters to the change in the gain characteristics. An improvement to this theoretical basis is suggested by implementing mathematical modeling to validate similarities between the gain shape of simulation to that obtained in the experiment.
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spelling um.eprints-46562018-10-11T02:19:15Z http://eprints.um.edu.my/4656/ Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA Sarmani, A.R. Sheih, S.J. Adikan, Faisal Rafiq Mahamd Mahdi, M.A. TK Electrical engineering. Electronics Nuclear engineering Spectral hole burning (SHB) effects in a gain-flattened erbium-doped fiber amplifier (EDFA) are demonstrated to be significant in the presence of large signal power around the 1530-1532-nm wavelength range. These are the first effects reported in a setup employing equivalent power level distribution of 40 channels ranging from 1530 to 1561 am. To explain this, the introduction of a new local population variable into the laser equation is required to support the original inversion ratio that is determined by the pump lasers. In the analysis section, spectroscopic parameters and high signal powers are considered to be other contributing parameters to the change in the gain characteristics. An improvement to this theoretical basis is suggested by implementing mathematical modeling to validate similarities between the gain shape of simulation to that obtained in the experiment. 2011 Article PeerReviewed Sarmani, A.R. and Sheih, S.J. and Adikan, Faisal Rafiq Mahamd and Mahdi, M.A. (2011) Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA. Chinese Optics Letters, 9 (2). ISSN 1671-7694,
spellingShingle TK Electrical engineering. Electronics Nuclear engineering
Sarmani, A.R.
Sheih, S.J.
Adikan, Faisal Rafiq Mahamd
Mahdi, M.A.
Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title_full Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title_fullStr Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title_full_unstemmed Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title_short Spectral hole burning effects initiated by uniform signal intensities in a gain-flattened EDFA
title_sort spectral hole burning effects initiated by uniform signal intensities in a gain flattened edfa
topic TK Electrical engineering. Electronics Nuclear engineering
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AT adikanfaisalrafiqmahamd spectralholeburningeffectsinitiatedbyuniformsignalintensitiesinagainflattenededfa
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