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Wavelength Division Multiplexing



                                                              Wavelength Division Multiplexing  209


                      TABLE 12.3. Performance Characteristics of Typical 40-Channel Arrayed Waveguide Gratings
                      Parameter                       Gaussian                Wideband
                      Channel spacing             100GHz                  100GHz
                      1-dB bandwidth               0.2nm                   0.4nm
                      3-dB bandwidth               0.4nm                   0.6nm
                      Insertion loss               5dB                     7dB
                      Polarization-dependent loss   0.25dB                 0.15dB
                      Adjacent channel crosstalk  30dB                    30dB
                      Passband ripple             1.5dB                   0.5dB
                      Optical return loss         45dB                    45dB
                      Size (L 	 W 	 H)            130 	 65 	 15 (mm)      130 	 65 	 15 (mm)


                      elements, such as narrow parallel slits or grooves, separated by a distance com-
                      parable to the wavelength of light. These diffracting elements can be either
                      reflective or transmitting, thereby forming a reflection grating or a transmis-
                      sion grating, respectively. With diffraction gratings, separating and combining
                      wavelengths is a parallel process, as opposed to the serial process that is used
                      with the fiber-based Bragg gratings.
                        Adjacent-channel crosstalk in a diffraction grating is very low, usually less
                      than 30dB. Insertion loss is also low (typically less than 3dB) and is uniform to
                      within 1dB over a large number of channels. A passband of 30GHz at 1-dB rip-
                      ple is standard. As is the case with other WDM schemes, packaging designs can
                      make the device be athermal, so no active temperature control is needed.
                        Reflection gratings are fine ruled or etched parallel lines on some type of
                      reflective surface. With these gratings, light will bounce off the grating at an
                      angle. The angle at which the light leaves the grating depends on its wave-
                      length, so the reflected light fans out in a spectrum. For DWDM applications,
                      the lines are spaced equally and each individual wavelength will be reflected at
                      a slightly different angle, as shown in Fig. 12.8. There can be a reception fiber
                      at each of the positions where the reflected light gets focused. Thus, individual
                      wavelengths will be directed to separate fibers. The reflective diffraction grat-
                      ing works reciprocally; that is, if different wavelengths come into the device on
                      the individual input fibers, all the wavelengths will be focused back into one
                      fiber after traveling through the device. One also could have a photodiode array
                      in place of the receiving fibers for functions such as power-per-wavelength mon-
                      itoring.
                        One type of transmission grating, which is known as a phase grating, consists
                      of a periodic variation of the refractive index of the grating. These may be char-
                      acterized by a Q parameter which is defined as

                                                         2πλd
                                                   Q                                    (12.4)
                                                       n g Λ cosα
                                                           2

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