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Optical Amplifiers



                                                                          Optical Amplifiers  187























                      Figure 11.10. Gain spectrum for a multiple-stage EDFA config-
                      uration with and without gain-flattening filters.


                      TABLE 11.3. Typical Performance Values of Different Coupler Types That Combine a 980-nm
                      Pump Wavelength with a C-Band Signal
                      Parameter                                       Specification

                      Device technology                    Fused fiber            Thin-film filter
                      Pump channel λ range                 970–990nm              965–995nm
                      Pass channel λ range                 1535–1565nm            1520–1610nm
                      Pump channel insertion loss          0.2dB                  0.6dB
                      Pass channel insertion loss          0.2dB                  1.0dB
                      Polarization-dependent loss           0.1dB                 0.1dB
                      Polarization mode dispersion         0.05ps                 0.05ps
                      Optical power capability             500mW                  500mW


                        ■ There is the shot noise in the photodetector that originates from the signal photons.
                         This is a major noise term, and its associated mean-square noise current is given by
                                              i 2 shot      σ 2 shot -s    2qGP in B     (11.3)
                                                             R
                         where q is the electron charge, R is the photodiode responsivity, G is the amplifier
                         gain, P in is the input power to the amplifier, and B is the front-end receiver electri-
                         cal bandwidth.
                        ■ There is the extra photodetector shot noise due to the addition of ASE-generated pho-
                         tons to the mean optical signal power. However, by using a narrow optical filter at the
                         receiver, most of this noise can be filtered out with the remainder being negligible.
                        ■ The thermal noise of the photodetector generally can be neglected when the ampli-
                         fier gain is large enough.


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