The wavelength multiplexing OLCR design
is presented in Fig. 4-11.
Fig. 4-11 Wavelength multiplexing OLCR set-up : wavelength division
multiplexer (WDM), cleaved fiber end (PC)
The low coherence light source around
1318 nm and the reference laser around 1550 nm are launched together
in the reference and test arms. The FBG (in the 1300 nm range) has very
low reflectivity at the laser wavelength, and then another laser reference
point in the test arm is required and a cleaved fiber end behind the grating is
used for this purpose. The distance between the FBG and the PC has to be as
small as possible to limit the laser phase noise (i.e. the interference of
lights emitted at different time). The laser wavelength is calibrated with a
wavemeter to improve the distance accuracy (relative distance uncertainty less
than 10-6).
Fig. 4-12 Measurement chronology for the wavelength multiplexing OLCR set-up
The cross talk between the low
coherence and reference laser signals is reduced by using 1310/1550 nm
wavelength division multiplexers with isolation greater than 45 dB. The
remaining cross talk disappears with the different levels used in the balanced
detection of both signals. Spectral variation of the laser and broadband
sources are kept below 2 pm with temperature control. Two dual-phase
lock-in amplifiers extract amplitude (Ioclr, Ilaser) and
phase (jolcr, jlaser) of the OLCR and laser signals. Ix and jx are measured at each mirror (MIR) position. The perfect symmetry of
the set-up allows measuring FBG's at 1550 nm with a matching broadband
source and a laser source at 1310 nm. The OPLD is sampled in order to
fulfill the Nyquist criteria for the reference laser phase. The absolute
distance without phase drifts for the OLCR phase is then calculated (i.e.
OPLD = llaser×jlaser/2p). From the absolute distance, a linear resampling is applied to the
OLCR amplitude and phase.
The measurement chronology is presented
in Fig. 4-12. A small time delay of 4 ms is observed between both
phase measurements.
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