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Wavelength Division Multiplexing



                                                              Wavelength Division Multiplexing  207


                        AWG Operation The AWG shown in Fig. 12.5 works as follows:
                        ■ Starting from the left, the input slab waveguides in region 1 are connected to the
                         planar star coupler (region 2) which acts as a lens.
                        ■ The lens distributes the entering optical power among the different waveguides in
                         the grating array in region 3.
                        ■ Adjacent waveguides of the grating array in region 3 differ in path length by a pre-
                         cise length ∆L. The path length differences ∆L can be chosen such that all input
                         wavelengths emerge at point 4 with different phase delays
                                                             ∆L
                                                   ∆Φ   2πn eff                          (12.2)
                                                              λ c
                         Here n eff is the effective refractive index of the waveguides, and λ c is the center
                         wavelength.
                        ■ The second lens in region 5 refocuses the light from all the grating array waveguides
                         onto the output slab waveguide array in region 6.
                        ■ Thus each wavelength is focused into a different output waveguide in region 6.
                        Note that the demultiplexing function of the AWG is periodic. Thus an import-
                      ant property of the AWG is the free spectral range (FSR), which also is known
                      as the  demultiplexer periodicity. This periodicity is due to the fact that con-
                      structive interference at the output star coupler can occur for a number of
                      wavelengths. Basically the FSR specifies the extent of a spectral width that will
                      be separated across the output waveguides. The next chunk of higher or lower
                      spectral width having an equal width will be separated across the same output
                      waveguides.

                        Example of Free Spectral Range For example, as shown in Fig. 12.6, suppose an AWG
                        is designed to separate light in the 4-THz-wide frequency range in the C-band running
                        from 195.00THz (1537.40nm) to 191.00THz (1569.59nm) into forty 100-GHz chan-
                        nels. Then it also will separate the next-higher-frequency S-band and lower-frequency



                       187 THz    191 THz   195 THz     199 THz
                      (1603.16 nm)  (1569.59 nm)  (1537.40 nm)  (1506.49 nm)
                                       4-THz FSR




                          Forty 100-GHz  Forty 100-GHz  Forty 100-GHz
                         L-band channels   C-band channels   S-band channels
                            go into     go into     go into
                          fibers 1 to 40  fibers 1 to 40  fibers 1 to 40
                      Figure 12.6. The FSR specifies the spectral width that
                      will be separated across the output waveguides of an
                      AWG.




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