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Laboratory for Optical Physics and Engineering CO + and C 2 Spectra Generated by CO 2 Atmospheric Pressure Glow Discharge in MicroChannels Chul Shin, Thomas.

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Presentation on theme: "Laboratory for Optical Physics and Engineering CO + and C 2 Spectra Generated by CO 2 Atmospheric Pressure Glow Discharge in MicroChannels Chul Shin, Thomas."— Presentation transcript:

1 Laboratory for Optical Physics and Engineering CO + and C 2 Spectra Generated by CO 2 Atmospheric Pressure Glow Discharge in MicroChannels Chul Shin, Thomas J. Houlahan, Zhen Dai, Sung-Jin Park and J. Gary Eden University of Illinois 1406 W. Green St., Urbana, IL, 61801 June 16, 2014

2 Laboratory for Optical Physics and Engineering MOTIVATION Microcavity plasmas provide a unique platform for molecular spectroscopy: –Electron temperature of 1-10 eV –Specific power loadings up to 1 MW/cm 3 –Electron densities of 10 13 -10 17 cm -3 –Operating pressures up to and beyond 1 atm Demonstrate microplasma capacity with CO –Ionization potential of CO: ~14 eV Microplasmas are an efficient source of highly-excited diatomic neutrals and ions

3 Laboratory for Optical Physics and Engineering SYSTEM ARRANGEMENT CO 2 Ar H2H2 MFC Manometer Device Port Check Valve Vent Spectrophotometer (ICCD) Premixing Chamber Lens Optical Rail

4 Laboratory for Optical Physics and Engineering DEVICE DIMENSIONS 500 μm 100 μm 160 μm 40 μm Al 2 O 3 Al

5 Laboratory for Optical Physics and Engineering OPERATION AT ONE ATMOSPHERE - f = 20 kHz sine wave - V opeation ~2 kV rms 5 mm

6 Laboratory for Optical Physics and Engineering PANORAMIC: 320-670 nm

7 Laboratory for Optical Physics and Engineering COMET TAIL BAND SYSTEM 5 W, 60 SCCM CO 2

8 Laboratory for Optical Physics and Engineering SWAN SYSTEM 5 W, 60 SCCM CO 2

9 Laboratory for Optical Physics and Engineering POWER DEPENDENCE 60 SCCM CO 2

10 Laboratory for Optical Physics and Engineering POWER DEPENDENCE 60 SCCM CO 2

11 Laboratory for Optical Physics and Engineering SUMMARY Optical emission from dissociating pure CO 2 has been demonstrated CO + Comet Tail Band System dominates ultraviolet/visible emission Microplasmas are an efficient source of highly- excited diatomic neutrals and ions

12 Laboratory for Optical Physics and Engineering Thank You!

13 Laboratory for Optical Physics and Engineering REFERENCES [1] Pearse, R. W. B., Gaydon, A. G., Pearse, R. W. B., & Gaydon, A. G. (1976). The identification of molecular spectra (Vol. 297, p. 293). London: Chapman and Hall.

14 Laboratory for Optical Physics and Engineering OPTICAL EMISSION SPECTRUM OF CO 2 MICROPLASMA


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