The complex reflection amplitude rfbg(n) is calculated
from the slowly varying complex OLCR response through a FFT algorithm after a
deconvolution from the broad-band spectral power density S(n). As the OLCR
measurement is not calibrated, a subsidiary calibration of rfbg(n) is required,
using an independent transmission measurement of the grating.
The inverse Fourier transform is performed
with the FFT algorithm. Nevertheless, the spectral resolution possible with
such kind of algorithm strongly depends on the OPLD range. For this reason we
artificially increase the x range by padding zeros after the last measured point (a resolution
of 3.6 pm is found at 1309 nm with an OPLD range of 52 cm). This
zero padding is equivalent to consider the OLCR signal equal to zero for values
under -120 dB. The total number of points is set to a power of two for
optimal FFT algorithm use. The Fourier transform of the slowly varying OLCR
function produces a frequency shifted spectral response. The frequency shift
corresponds to the laser frequency.
The complex slowly varying OLCR
function f(x) is related to the grating complex spectral response r(n) and the
effective broadband power spectral density S(n) that includes some
spectral filtering of the interferometer
|
(4-48) |
where the symbol "~" is used in the meaning of "proportional to" and n0 is the laser frequency. The frequency shifted inverse Fourier
transform F(n) of f(x) is proportional to S(n)×r(n). The deconvolution of the interferometer
signature is in the frequency domain a simple division, i.e. F(n)/S(n). The function
S(n)
is obtained when the FBG is replaced by cleaved fiber end, for which the
reflectivity is constant over the light source frequency range. We can then
write the following relation
|
(4-49) |
where rnc represents the FBG
reflection spectral response that is not calibrated and FT means "Fourier
transform of" and FT-1 "inverse Fourier transform".
We have to notice that S(n) is supposed to
be a real function and that the remaining dispersion, which can appear in the
interferometer is assumed to be very small and thus neglected. For this reason
we use the absolute value of FT-1(fcleaved fiber(x)). In the case
where the dispersion cannot be neglected, a more complicated deconvolution is
required, based on equations (4-33).
Finally, it remains to normalize the
complex reflection amplitude. We have chosen not to calibrate the OLCR
measurement as the polarization rotation drifts makes such calibration hard to
maintain. We prefer an independent measurement of the FBG transmission
intensity with the tunable laser to determine the maximal reflection intensity
Rfbg,max
|
(4-50) |
As long as the induced refractive index
modulation of the grating is not modified (e.g. high temperature), the impulse
response amplitude at the entrance |h(t=0)| remains constant for different
environmental conditions of temperature and strains. This property allows to
perform a single calibration of |h(0)| in a given state of strain and
temperature to calibrate the grating in other environmental states.
|