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Absolute UV and VUV emission in the 110400nm region from 13.56MHz driven hollow slot microplasmas operating in open air

Identifieur interne : 001695 ( Main/Exploration ); précédent : 001694; suivant : 001696

Absolute UV and VUV emission in the 110400nm region from 13.56MHz driven hollow slot microplasmas operating in open air

Auteurs : A. Rahman [États-Unis] ; A P Yalin [États-Unis] ; V. Surla [États-Unis] ; O. Stan [États-Unis] ; K. Hoshimiya [États-Unis] ; Z. Yu [États-Unis] ; Eric Littlefield [États-Unis] ; G J Collins [États-Unis]

Source :

RBID : ISTEX:80B9739C630A9CABD2B229573C9A8619308348B5

English descriptors

Abstract

We present absolute optical emission spectra in the 110400nm regions from radio-frequency-driven (13.56MHz) hollow slot microplasmas operating in open air at atmospheric pressure. The term microplasma in our research refers to inter-electrode separation (100600m) only, as electrode lengths are scalable from 1 to 30cm. This creates an extended slot plasma and an associated afterglow plume as described herein. Spectra are presented for gas flows through the microelectrodes of argon and helium with small admixtures of hydrogen and nitrogen into open air. The spectra are discussed in terms of species origin and magnitude of the dominant emission lines. Atomic O and N lines dominate the 110200nm region, whereas, in the 200400nm region, NO, N2, and NH molecular lines are strongest. The role of the state in the open air microplasmas is discussed and the second positive system of molecular nitrogen (N2(C 3gB 3g)), is used to measure the rotational (gas) temperature. Finally, we compare the efficiency and magnitude of light emission from the open air microplasmas with values attainable from commercial sealed mercury lamps in the UVB and UVC regions.

Url:
DOI: 10.1088/0963-0252/13/3/021


Affiliations:


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<term>Absolute emission</term>
<term>Absolute intensity</term>
<term>Active discharge</term>
<term>Active discharge region</term>
<term>Active plasma</term>
<term>Active plasma region</term>
<term>Admixture</term>
<term>Afterglow</term>
<term>Afterglow plume</term>
<term>Ambient</term>
<term>Ambient nitrogen</term>
<term>Ambient species</term>
<term>Appl</term>
<term>Argon</term>
<term>Argon dimer</term>
<term>Argon dimers</term>
<term>Argon metastables</term>
<term>Argon plasmas</term>
<term>Argon source</term>
<term>Atmospheric pressure</term>
<term>Atomic hydrogen</term>
<term>Atomic lines</term>
<term>Atomic nitrogen</term>
<term>Atomic nitrogen lines</term>
<term>Atomic oxygen</term>
<term>Atomic oxygen line</term>
<term>Cathode discharges</term>
<term>Chem</term>
<term>Colorado state university</term>
<term>Commercial mercury lamps</term>
<term>Concentration decreases</term>
<term>Continuum emission</term>
<term>Current density</term>
<term>Current work</term>
<term>Detection system</term>
<term>Electrical power</term>
<term>Electrode</term>
<term>Electron impact</term>
<term>Electron impact excitation</term>
<term>Electronic version</term>
<term>Emission spectra</term>
<term>Energy levels</term>
<term>Excitation</term>
<term>External plume</term>
<term>Fort collins</term>
<term>Gure</term>
<term>Gures</term>
<term>Helium metastables</term>
<term>Helium plasmas</term>
<term>Hollow slot</term>
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<term>Hollow slot microplasmas</term>
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<term>Hydrogen admixtures</term>
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<term>Main contributions</term>
<term>Mercury lamps</term>
<term>Metastable</term>
<term>Metastable density</term>
<term>Metastables</term>
<term>Microelectrode device</term>
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<term>Open slot electrodes</term>
<term>Open slots</term>
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<term>Optical emission</term>
<term>Optical emission spectra</term>
<term>Optical output</term>
<term>Optical power</term>
<term>Optical spectra</term>
<term>Peak intensities</term>
<term>Phys</term>
<term>Plasma</term>
<term>Plasma plume</term>
<term>Plasma sources</term>
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<term>Plume region</term>
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<term>Processing applications</term>
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<term>Quenching reactions</term>
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<term>Rotational temperature</term>
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<term>Vertical axis</term>
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<front>
<div type="abstract">We present absolute optical emission spectra in the 110400nm regions from radio-frequency-driven (13.56MHz) hollow slot microplasmas operating in open air at atmospheric pressure. The term microplasma in our research refers to inter-electrode separation (100600m) only, as electrode lengths are scalable from 1 to 30cm. This creates an extended slot plasma and an associated afterglow plume as described herein. Spectra are presented for gas flows through the microelectrodes of argon and helium with small admixtures of hydrogen and nitrogen into open air. The spectra are discussed in terms of species origin and magnitude of the dominant emission lines. Atomic O and N lines dominate the 110200nm region, whereas, in the 200400nm region, NO, N2, and NH molecular lines are strongest. The role of the state in the open air microplasmas is discussed and the second positive system of molecular nitrogen (N2(C 3gB 3g)), is used to measure the rotational (gas) temperature. Finally, we compare the efficiency and magnitude of light emission from the open air microplasmas with values attainable from commercial sealed mercury lamps in the UVB and UVC regions.</div>
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