Page 450 - Fiber Bragg Gratings
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9.3 Phase and temporal response of Bragg gratings               427

         been used to locate gratings. In the next section we will consider the
         OLCR method and side-scatter as two techniques to assess Bragg gratings.

         Optical low-coherence reflectometry

         The scheme is based on a fast scanning Michelson interferometer, with
         the grating as the mirror in one arm, and a scanning broadband mirror
         (BBM) in the reference arm. Reflected light from the grating and the
         mirror interferes at a photodiode. The source has a large bandwidth so
         that the coherence length is short, and therefore interference is only
         visible over a short region of the grating when the path lengths are within
         the coherence length. The path difference between the arms is adjusted
         by moving the reference mirror so that different points within the grating
         are sampled. A schematic of the apparatus is shown in Fig. 9.20 [37]. The
         moving reference mirror is mounted on a motorized stage with a long
         scan length to allow easy adjustment of the paths. The phase modulator
         is provided to derive a lock-in signal. With reference to a 100% reflection,
         a cleaved end with approximately 4% end reflection registers a signal at
         — 14 dB. The measurement has range with a noise floor at —140 dB with
         a bandwidth of 1 Hz.
             The source should have low spectral ripple to avoid artifacts. The
         coherence length, and therefore the resolution of the measurement in the
         fiber is

























        Figure 9.20: A schematic of the OLCR apparatus (after Ref. [37]).
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