2003
DOI: 10.1088/0022-3727/36/9/311
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VUV emission spectra from binary rare gas mixtures near the resonance lines of Xe I and Kr I

Abstract: Emission spectra of Xe-X (X = He, Ne, Ar and Kr) and of Kr-Y (Y = He, Ne and Ar) mixtures with low concentrations of the heavier gases (0.1-1%) and moderate total pressures (50-200 hPa) have been recorded near each of the two resonance lines of Xe and Kr in DC glow capillary discharges. The recorded intense emissions have narrow spectral profiles with FWHM of about 0.1 nm. The profiles are very similar in shape to profiles of known high resolution absorption spectra recorded at comparable gas pressures. A tent… Show more

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Cited by 12 publications
(6 citation statements)
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“…In the lamp used here, excimer molecules are formed via electron beam excitation of a dense gas . By choosing various rare gases or gas mixtures, different wavelengths can be generated. , The main innovation of the light source is a 0.7 × 0.7 mm 2 , 300-nm-thick SiN x foil, which separates the rare gas volume ( p > 1 bar) from the vacuum chamber containing an electron gun (EG). The EG generates a 13−15-keV electron beam, which is directed into the rare gas through the SiN x foil with low energy loss.…”
mentioning
confidence: 99%
“…In the lamp used here, excimer molecules are formed via electron beam excitation of a dense gas . By choosing various rare gases or gas mixtures, different wavelengths can be generated. , The main innovation of the light source is a 0.7 × 0.7 mm 2 , 300-nm-thick SiN x foil, which separates the rare gas volume ( p > 1 bar) from the vacuum chamber containing an electron gun (EG). The EG generates a 13−15-keV electron beam, which is directed into the rare gas through the SiN x foil with low energy loss.…”
mentioning
confidence: 99%
“…3 and 4) is evidence that narrow-band radiation of the heteronuclear dimers Kr*He is superimposed on the atomic lines. 3 The maximum intensity of this molecular radiation is located close to the center of the atomic line, but the contour of the molecular band is wider and asymmetric. 4 The radiation intensity of the heteronuclear dimers depends on the partial pressures of both gases of the mixture.…”
Section: The Vuv Spectrum Of the Sourcementioning
confidence: 91%
“…A mixture of argon and nitrogen shows an enhanced emission on the C-B band of nitrogen between 300 and 400 nm. Mixtures of rare gases show energy transfer from the light to the heavier rare gas with emission due to the formation of mixed molecules [11] and for higher concentrations of the heavier species on the rare gas excimer band of these heavier species (first and second continuum) [12].…”
Section: Energy Transfer and Gas Kinetic Studiesmentioning
confidence: 99%