2013
DOI: 10.1109/lpt.2013.2250948
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High Stability Er-Doped Superfluorescent Fiber Source Incorporating an Er-Doped Fiber Filter and a Faraday Rotator Mirror

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Cited by 17 publications
(7 citation statements)
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“…The DPB (Fig. 2b) configurations reported nearly flat [14], [20], [22] or even negative temperature dependency of the mean wavelength [9], [29], [33], [34], which is achieved by a combination of the bare SFS parameters and characteristics of the reflector at the unpumped fiber end. In DPB configuration, the forward ASE is totally or partially reflected and amplified.…”
Section: Principlesmentioning
confidence: 99%
See 1 more Smart Citation
“…The DPB (Fig. 2b) configurations reported nearly flat [14], [20], [22] or even negative temperature dependency of the mean wavelength [9], [29], [33], [34], which is achieved by a combination of the bare SFS parameters and characteristics of the reflector at the unpumped fiber end. In DPB configuration, the forward ASE is totally or partially reflected and amplified.…”
Section: Principlesmentioning
confidence: 99%
“…So far, many approaches have been proposed to enhance the SFS mean wavelength temperature stability, such as long period grating [15], fiber Bragg grating [16], [28], photonic bandgap filter [17], thin film filter [11], [29], Er-doped fiber filter [8], [14], [22], [23], also photonic crystal Er-doped fiber [18], Faraday rotator mirror [19], [20], [30], or variable parameters control [24].…”
Section: Introductionmentioning
confidence: 99%
“…where K t filter is the TC of the central wavelength of the OL caused by the temperature dependence of the central wavelength of the temperature-compensating spectral filter. The long-period fibre grating [12][13][14], the fibre Bragg grating [15][16][17], the unpumped EDF [18][19][20], and thin-film filters [15,16,21] are implemented as temperaturecompensating spectral filters. However, in many cases, it is necessary to create unique spectral filters and choose the optimal parameters (the optimal length of the EDF and/or the optic power of the pump laser) for each optic scheme of the EDFS [5,17,[22][23][24][25].…”
Section: Problematicsmentioning
confidence: 99%
“…The long‐period fibre grating [12–14], the fibre Bragg grating [15–17], the unpumped EDF [18–20], and thin‐film filters [15, 16, 21] are implemented as temperature‐compensating spectral filters. However, in many cases, it is necessary to create unique spectral filters and choose the optimal parameters (the optimal length of the EDF and/or the optic power of the pump laser) for each optic scheme of the EDFS [5, 17, 22–25].…”
Section: Problematicsmentioning
confidence: 99%
“…where K t filter is the TC of the central wavelength of the OL caused by the temperature dependence of the central wavelength of the temperature-compensating spectral filter. The long-period fibre grating [12][13][14], the fibre Bragg grating [15][16][17], the unpumped EDF [18][19][20], and thin-film filters [15,16,21] are implemented as temperature-compensating spectral filters. However, in many cases, it is necessary to create unique spectral filters and choose the optimal parameters (the optimal length of the EDF and/or the optic power of the pump laser) for each optic scheme of the EDFS [6,17,[22][23][24][25].…”
Section: Problematicsmentioning
confidence: 99%