Page 113 - Fiber Bragg Gratings
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92                               Chapter 3 Fabrication of Bragg Gratings

        where n av is the average index of the mode. It follows, therefore, from
        Eqs. (3.1.20) and (3.1.21) that the new grating periods A~ and Ajr corres-
        ponding to the superscripted Bragg wavelengths are









            From Eqs. (3.1.4) and (3.1.22), it follows that the spacing AA between
        the reflected wavelengths in any such superstructure is





        Depending on the shape of the composite structure (and thus the magni-
        tudes of the individual Fourier components), higher order components
        can appear [87].
            Superstructure gratings represent a number of types of gratings: the
        DFB with a single phase step 4> < ZTT [85,86]; the grating Fabry-Perot
        with (f> > 2 77 resulting in multiple high-finesse transmission peaks [89];
        cascaded grating Fabry-Perots in which the phase steps  (f> > 277- [87],
        leading to replicated multi-band-pass transmission spectra; gratings with
        multiple-flat-top reflection spectra, fabricated with unequal grating
        lengths as well as phase steps [90]; and truly flat-top reflection gratings
        fabricated by introducing regular 77/2 phase shifts (A/4) at equal intervals,
        while altering the strength of the grating amplitude in each section to
        mimic a sine function [91].
            There are several methods of making these gratings. In order to
        introduce a specific phase step, the simplest and most reliable is via the
        replication of a phase mask with the appropriately prerecorded phase
        steps [92]. Another method successfully used for introducing a 77/2 phase
        step in a grating is by UV postprocessing [84]. After the grating has been
        written, the small central section is illuminated with UV radiation to
        introduce a phase shift. As the refractive index of the exposed region of
        length SI increases by Sn, the transmission spectrum of the grating is
        monitored to stop the exposure when SnSl = A/4. A disadvantage of post-
        UV exposure is that it not only changes the phase between the two halves
        of the grating, but also alters the local n eff of the fiber. This in turn
        shifts the Bragg wavelength of the already-written grating exposed to UV
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