Small perturbations (e.g. temperature
variations) in both interferometer arms modify the optical path length
difference (OPLD) and determine the phase drifts. Typical variations of 2p in the OLCR or
laser phase signal are possible in a few seconds. For complex OLCR
measurements, these phase drifts have to be either limited by very fast
measurements or compensated by another reference laser signal when the
measurements are slow. Two main complex OLCR measuring methods has been studied
:
-
Dynamic method : moving the mirror at
constant speed produces a Doppler frequency used to measure the real part
amplitude; the imaginary part is calculated by an Hilbert transformation and
subsequently the complex response is obtained [4-2]
-
Static method : for a given mirror
position, the OPLD is ramp modulated over a multiple of the interference period
producing a quasi sinusoidal signal (Fig. 4-8); a dual-phase lock-in
amplifier then directly derives the amplitude and phase signals
Both methods have their own advantages and
drawbacks :
-
Dynamic method : the main advantages
are the high speed (e.g. 42-m/s with rotating mirror cubes [4-9]) and the
small phase drifts; on the other hand, the signal to noise ratio (S/N) is
limited by the shot noise of the detectors, the phase reconstruction using the
Hilbert transform is not optimal for small signals and a constant mirror speed
is needed; moreover, a high precision reference distance and an OPLD resolution
that fulfills the Nyquist criteria (under l/2) are required
-
Static method : the main advantages
are the high dynamic range (only limited by the fiber Raleigh scattering around
-120 dB) and an OPLD resolution that is not limited by the Nyquist
criteria as only the phase difference between the laser and the OLCR phases is
measured, which is slowly varying with the OPLD; on the other hand the
measurement is slow (3 min/mm in our set-up) due to the ramp modulation
process at each position (150 Hz maximal frequency for piezoelectric
plates) that limits the measurement speed and then requires to compensate the
important phase drifts
The static method has been chosen for
its high dynamic range that enables the measurement of weak FBGs. Fig. 4-8a
shows the interference amplitude for the OPLD, z. The period is given by
half the low coherence light source wavelength l/2. For a given mirror
position z (stationary condition), the OPLD is ramp modulated at frequency f
as seen in Fig. 4-8b. The time dependent signal measured by the detector
(Fig. 4-8c) is a piecewise reconstructed sinus function obtained by
concatenation of the interference signal over a period. The amplitude a(z) corresponds to
the OLCR envelope amplitude and the phase difference b(z) between the ramp excitation
and the signal minima gives the OLCR phase. The transition time between two
ramps (between dotted and dashed lines) explains induced signal distortions
that limit the modulation frequency. The reference laser signal is similar but
the amplitude is nearly constant over the measurement range due to the much
longer coherence length.
Fig. 4-8 Signal generation for OLCR set-ups with static method
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