2005
DOI: 10.1364/opex.13.007336
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Stimulated Brillouin scattering gain profile characterization by interaction between two narrow-linewidth optical sources

Abstract: We report on results from the characterization of Stimulated Brillouin Scattering (SBS) spectra for standard single-mode fiber produced by the interaction between two counter-propagating tunable laser sources (TLS) using one as the probe signal to measure and the other as the pump, sweeping a wide span around the signal. Assuming TLS linewidth negligible against SBS gain bandwidth, we measure SBS spectrum for a wide range of pump and probe signal power levels and study the evolution of relevant SBS parameters … Show more

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Cited by 34 publications
(20 citation statements)
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“…Since the frequency shift is inversely dependent on lambda, a~6 GHz frequency shift is expected at 1.55 μm in bulk for the same composition. Our measurements differ due to the different pump/saturations conditions used in our experiments [15]. Fig.…”
Section: Resultsmentioning
confidence: 79%
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“…Since the frequency shift is inversely dependent on lambda, a~6 GHz frequency shift is expected at 1.55 μm in bulk for the same composition. Our measurements differ due to the different pump/saturations conditions used in our experiments [15]. Fig.…”
Section: Resultsmentioning
confidence: 79%
“…Therefore, we can stipulate that the actual shape is in-between a Gaussian and Lorentzian function, as shown on the high frequency side of the BGS. Since we are far from the high gain saturation regime as described by Villafranca and Lázaro [15], the presence of a Gaussian nature may indicate inhomogeneous broadening. From the observed maximum gain, we can calculate the Brillouin gain g B , from Eq.…”
Section: Resultsmentioning
confidence: 79%
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“…1(b), which was captured via an optical spectrum analyzer, BOSA 200 by Aragon Photonics. The undithered (S D (t) off) optical spectral at the output of DM and EM resulted in a linewidth of full width at half maximum (FWHM) of ~11.14 MHz, since SBS linewidth is typically around ~30 MHz [4], most propagating signals are back-reflected due to the formation of index grating. From Fig.…”
Section: Resultsmentioning
confidence: 99%
“…An index grating is formed when the propagating signal has a narrower linewidth than the SBS linewidth and subsequently energizes the back-reflecting Stokes wave [4]. An enhanced SBS threshold optical fibre was proposed as a solution in [5], but replacing the existing single mode fibre (SMF) infrastructure would not be cost effective [3].…”
Section: Introduction and The Proposed Systemmentioning
confidence: 99%