Page 161 - Fiber Bragg Gratings
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138                            Chapter 4 Theory of Fiber Bragg Gratings

        there is no intersection with the outer or inner circles. There is a gap in
        the spectrum, in which no phase matching is possible. At some point the
        arrowhead meets the vertical dotted line for the radiation modes on line
        a, and phase matching to the radiation modes begins. This will couple to
        the lowest-order modes. With an infinite cladding, free-space radiation
        mode phase matching occurs. As the wavelength becomes even shorter,
        the angle of the radiation modes increases, and only when the vector 6
        meets the n clad circle is radiation mode coupling at an angle of ff b. After
        this point, the angle of the radiation mode increases beyond ff b. We now
        note that the change in the mode index is 8n from the RH side of the
        figure, so that we can calculate the wavelength at which the radiation
        loss starts to occur.
            Figure 4.6 shows the phase-matching diagram for coupling to the
        guided and radiation modes and fields with a tilted grating, known as
        side-tap-grating (STG, also see Chapter 6). This grating has a period
        similar to Bragg gratings but does not have its grating planes normal to
        the fiber axis, and it is tilted at an angle, 6 g. The diagram specifically
        deals with the case of coupling to counterpropagating fields.
            In the first interaction with n g, we have Bragg reflection at A Bragg.
        We assume that the grating angle d g = 0, and that when the wavelength
                                                 s rt
        is tuned, the effective index of the mode is n ^  at the point indicated by
        a on Fig. 4 6, so that mathematically, this is simply phase matching to a
        mode with the cladding index as





        where start indicates the wavelength at which the radiation mode coupling
        begins.
                                                             s
                                                               rt
            Rearranging and using the approximation n eff ^ n *^  «* n^ agg , it
        follows that




        Therefore, radiation loss begins at a wavelength slightly shorter than the
        Bragg wavelength, governed by the ratio in the brackets in Eq. (4.2.32).
        For example, in a fiber with a large core-cladding index difference with
        a tightly confined Bragg wavelength (1550 nm) mode (n eff = 1.475), the
        start wavelength will be at —1537 nm, some 13 nm away.
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