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Infrared-Laser Induced Fluorescence and Instrumental Design Michael W. Morton Geoffrey A. Blake Division of Geology and Planetary Science California Institute.

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Presentation on theme: "Infrared-Laser Induced Fluorescence and Instrumental Design Michael W. Morton Geoffrey A. Blake Division of Geology and Planetary Science California Institute."— Presentation transcript:

1 Infrared-Laser Induced Fluorescence and Instrumental Design Michael W. Morton Geoffrey A. Blake Division of Geology and Planetary Science California Institute of Technology Pasadena, CA 91125

2 Stable Isotope Studies Applications include Atmospheric chemistry Geochemistry Bio-geochemistry  Planetary Exploration Specific examples Atmospheric photochemistry Climate studies Biological influences

3 Instrumentation Mass Spectrometers Utilize mass differences in isotopes, Great for laboratory studies, but not in situ Limitations in planetary exploration: Size, weight Remote operation Sample preparation Sample destruction Isotopomers/ – N 15 NO 15 NNO NN 17 O Isotopologues in situ Stable Isotope Ratio Spectrometer ? Utilize spectroscopic differences in isotopes

4 A Brief Look at Photoacoustic Detection Figures courtesy of – Miklos, A. & P, Hess (2001). Am. Inst. Phys., 72, 1938, 1951.

5 Photoacoustic Considerations Indirect absorption technique signal strength depends on Beer’s law and cell geometry Cell volume and sample size Non-selective detection of mixed samples HDO - D 2 O Short path length Good sensitivity

6 Sensitivity of PA Detection Show high laser power spectrum with small peak detection cm -1

7 IR-LIF Technique Small instrument size Remote operation Little to no sample preparation non-destructive Isotopomer resolution Small sample size Figure courtesy of – Geoff Blake

8 Instrumental Setup chopper PA cell dewar detector filter wheel lock-in amplifier scope PC wavemeter PC

9 HDO Transitions 1 – OD stretch2726.73 cm -1  – bend1402.2 3 – OH stretch3707.47 Pump v1+v3 near 1550 nm (can use telecommunications diode lasers). cm -1 6434 2727 3707 0 0 1 1 0 1 1 0 0 0 0 0 0 2 1 6512 0 2 0

10 HDO Vapor Spectrum S/N ~ 90 ~1 pMole HDO in volume imaged onto detector.

11 Signal and Noise Analysis 1 Why is the signal ~independent of pressure in a pure gas?

12 Signal and Noise Analysis S/N a √ t out to ~10 sec Microphonic peak (vibrations)

13 Signal and Noise Analysis Figure from – Bernath, P.F. (1995). Oxford University Press, Inc., 8. Limited by warm window?

14 Future Work Characterize noise H 2 O quenching of HDO emissions FM modulation instead of chopper wheel New integrated sample cell on the order of < cm 3 Measure isotopic fractionation of water Low pressure studies < 100 mtorr New detector, lasers 12347561234756

15 Acknowledgements Professor Geoff Blake Vadym Kapinus Dr. Pin Chen Dr. Keith Matthews The Blake Group


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