1998
DOI: 10.1109/68.681305
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Output intensity noise of lightwave transmitters employing chirp demodulation

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Cited by 3 publications
(5 citation statements)
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“…j 0 is proportional to laser-emitted power and suggests that operation at low laser powers (low bias) is more vulnerable to noise, Downloaded by [Northeastern University] at 13:03 20 November 2014 as expected. The noise has a resonant behavior due to the involvement of the IM transfer function inŝ ω ,ν ω , andˆ ω as explained in Yabre [4]. A low FSR is required for good signal linearity in PM to IM conversion [4], creating a tradeoff between linearity and noise.…”
Section: Theoretical Analysismentioning
confidence: 98%
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“…j 0 is proportional to laser-emitted power and suggests that operation at low laser powers (low bias) is more vulnerable to noise, Downloaded by [Northeastern University] at 13:03 20 November 2014 as expected. The noise has a resonant behavior due to the involvement of the IM transfer function inŝ ω ,ν ω , andˆ ω as explained in Yabre [4]. A low FSR is required for good signal linearity in PM to IM conversion [4], creating a tradeoff between linearity and noise.…”
Section: Theoretical Analysismentioning
confidence: 98%
“…The noise has a resonant behavior due to the involvement of the IM transfer function inŝ ω ,ν ω , andˆ ω as explained in Yabre [4]. A low FSR is required for good signal linearity in PM to IM conversion [4], creating a tradeoff between linearity and noise. For the wavelength converter, the choice of FSR would depend on the magnitude of phase or frequency modulation induced on the converter laser through XPM, a parameter that is well under the control of the system designer by varying the laser power and SMF length.…”
Section: Theoretical Analysismentioning
confidence: 98%
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“…It contains three terms, the classical RIN, a term proportional to the power spectral density of the frequency noise and a term resulting from the cross correlation between the two noise sources and is given below [6] FSR ΪΙ j] (3) in which 9Ί denotes the real part, the star symbol represents the complex conjugate, ω is the angular modulation frequency, RIN(co) is the classical relative intensity noise of a laser, ν ω is the Fourier transform of the laser frequency variation (ν ω = jvfyj, § ω is the Fourier transform of the normalized photon density and Τκ where -· <*=<»· · · · > (2) T(v) is the transmission of the Mach-Zender interferometer given by [7] where is the free spectral range of the MZI most conveniently defined as the frequency offset between a maximum transmission and the next neighboring minimum. In the OXC, interferometric intensity noise is due to PM-IM conversion in the wavelength converter.…”
Section: Optical Cross-connect Noise Modelmentioning
confidence: 99%