Page 201 - Fiber Bragg Gratings
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178                             Chapter 4 Theory of Fiber Bragg Gratings

        where r is the Fresnel amplitude reflection coefficient at the cladding
        surface, and L b is the distance between the successive reflections at the
        cladding surface.



        4.8 Grating simulation


        4.8.1   Methods for simulating gratings
        Many of the techniques for simulating fiber Bragg gratings were intro-
        duced at the beginning of the chapter [10,58,9,19]. All the techniques
        have varying degrees of complexity. However, the simplest method is
        the straightforward numerical integration of the coupled-mode equations
        such as Eqs. (4.3.9) and (4.3.10). While this method is direct and capable
        of simulating the transfer function accurately, it is not the fastest. Another
        technique is based on the Gel'Fand-Levitan-Marchenko inverse scatter-
        ing [58] method. This is again a powerful scheme based on integral coupled
        equations but has the primary disadvantage of obscuring the problem
        being solved. It has, however, the advantage of allowing a grating with
        particular characteristics to be designed. Perhaps the most attractive
        method is based on techniques developed for the analysis of metal wavegu-
        ides by Rouard [11] and carries his name as a result. This technique,
        extended by Weller-Brophy and Hall [12], works on the principle that the
        waveguide may be segmented into subwavelength thin films. Standard
        thin-film techniques for calculating the amplitude and phase of the trans-
        mitted and reflected electric fields at each interface are propagated back-
        ward from the output end of the grating. The method is slow, but is one
        of the few that offers complete piecemeal control of the spatial variation
        in the refractive index modulation of the grating. For example, the transfer
        function of a grating with a sawtooth modulation is analyzed equally as
        well as a square or sinusoidal profile. The influence on the phase and
        amplitude response of the grating cannot be fully characterized if the
        Fourier coefficient of the phase-synchronous term for phase matching as
        shown in Eq. (4.2.27) alone is used. Thus, it is a laborious and time-
        intensive computation; however, the results accurately simulate the char-
        acteristics of complex-shaped grating periods with reasonable reflectivi-
        ties, being limited by the rounding errors in the computation.
            A fast and accurate technique is based on the T-matrix (transfer) for
        calculating the input and output fields for a short section SI of the grating
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