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Mid-IR ethene detection using a quasi-phase matched LiNbO 3 waveguide 64th OSU International Symposium on Molecular Spectroscopy 23 rd June 2009
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Biogenic sources - Plant Hormone 'ripening hormone' Anthropogenic sources - Organic chemical industry (polyethylene products) - Vehicle exhaust (Ethene as indicator of UV-induced lipid peroxidation) OH ~ 20 hours O3 ~ 9.7 days NO3 ~ 5.2 months Why ethene? Urban Area ~ few ppbv Remote Area < 1 ppbv
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C2H4C2H4 A.M.Parkes et al., Phys. Chem. Chem. Phys., 6 (2004) 5313-53178 HITRAN Database, 2008 Mid-IR vs Near-IR Mid-IRNear-IR DFG (2 to 5 m) QCLs (5 to 11 m)
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C2H4C2H4 HITRAN Database, 2004 3081.002 cm -1 6150.300 cm -1 cm -1 (FWHM) 0.007170.01432 line / cm 2 molecule -1 cm -1 1.124 10 -20 5.08 10 -22 Gain ~ 46 Mid-IR vs Near-IR
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ELECTRONICS LETTERS 17th August 2006 Vol. 42 No. 17 Applied Physics Letters 88, 061101, 2006 pp ss i p s ii Frequency mixing and phase matching d eff = 17 pm/V ksks kpkp kiki
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Bulk vs waveguide Applied Physics Letters 88, 061101, 2006 Waveguide structure improves conversion efficiency with respect to bulk
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PZT Experimental set-up (OA-CEAS) 90 mW 28 mW ~ 200 W
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Characterization of the laser source Conversion efficiency = 12.3 % W -1 Experimental phase matching curve in good agreement with the simulated one Beam profile analysis gave a Gaussian beam waist of ~2 mm.
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Tunability of the laser source Wide tunability range of 35 cm -1 FWHM ~ 7 cm -1
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Multi-pass absorption + WMS 1.29 Torr of C 2 H 4 in Ar (500 ppmv) Slow modulation = 1 Hz Fast modulation = 20 kHz c = 5 ms Idler power = 193 W L = 56 m Modulation depth → b = 2 min (BW)= 1.63 x 10 -8 cm -1 Hz -1/2 (2 )
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OA-CEAS 1.8 Torr of C 2 H 4 in Ar (21.8 ppmv) Slow modulation = 0.8 Hz Chopper frequency = 2.6 kHz = 0.01232 cm -1 = 0.00717 cm -1
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OA-CEAS R = 99.901 ± 0.002 % min (BW)= 1.6 x 10 -8 cm -1 Hz -1/2 (2 ) L = 1110 ± 20 m
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Conclusions and future work Mid-IR light has been characterized. The CONVERSION EFFICIENCY of the waveguide, the BEAM PROFILE and the TUNABILITY of the system have been tested. Applications of the DFG spectrometer as a new laser sources @ 3.2 m for ethene detection have been proved using MULTI-PASS ABSORPTION coupled with WMS, and OA-CEAS. A.M.Parkes et al., Phys. Chem. Chem. Phys., 6 (2004) 5313-53178 Technique [C 2 H 4 ] min / molecule cm -3 (in air) Mixing ratio / ppbv (in air) Near-IR (@ 1.6 m) cw-CRDS 1.6 10 12 64 cw-CRDS + preconc. 4.7 10 10 1.9 Mid-IR (@ 3.2 m) MPA + WMS 5.4 10 11 21.8 OA-CEAS 2.2 10 11 8.9
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Acknowledgements Prof. Andrew Orr-Ewing Dr. Mike Nix Keith Rosser Dr James Smith Charles Murray Bristol Laser Group Prof. Gus Hancock Dr Grant Ritchie Dr Rob Peverall Luca Ciaffoni
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Spectrum analysis of the EDFA output - Fabry-Perot spectrum analyzer → laser bandwidth ~ 500 kHz - 1480 nm pump more noisy than 980 nm - FFT spectrum analyzer → ASE at seeding powers < 1 mW Characterization of the laser source
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Noise Analysis 330-370 kHz
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Noise Analysis Applied Physics B 76, 473-477 (2003) 0.025 (200-500kHz)
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cw-CRDS with Laser Detuning Technique Cavity Signal Laser Current
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