1995
DOI: 10.1002/ctpp.2150350606
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UV Radiation of Low Pressure XeCl* and KrCl* Glow Discharges

Abstract: The positive column of low pressure DC glow discharges in Xe/CI, and Kr/C1, gas mixtures has been investigated with respect to its UV radiation power and radiative efficiency for a wide range of parameters (total gas pressure: 1 -30 mbar, current 10-30 mA, partial pressure of CI,: 1 -33%). Also the radial distribution of the particle number densities of XeCl* ( B ) and KrCI* (B) has been determined by absolutely calibrated emission spectroscopy. Optimum UV (190-350 nm) output and efficiency has been found in g… Show more

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Cited by 9 publications
(15 citation statements)
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References 20 publications
(11 reference statements)
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“…At low pressure the XeCl emission becomes wider, a shoulder appears on the blue side of the band and the maximum is shifted to shorter wavelengths. The spectrum at 10 mbar is similar to those reported in [23,24] and pressure dependence of the spectra qualitativly agrees with the results in [9]. It is usually assumed [9,24,25] that the difference between the high and low pressure spectra is caused by the formation of the XeCl molecule in vibrationally and rotationally excited states.…”
Section: Variation Of the Xecl Band Shape With Experimental Conditionssupporting
confidence: 81%
See 1 more Smart Citation
“…At low pressure the XeCl emission becomes wider, a shoulder appears on the blue side of the band and the maximum is shifted to shorter wavelengths. The spectrum at 10 mbar is similar to those reported in [23,24] and pressure dependence of the spectra qualitativly agrees with the results in [9]. It is usually assumed [9,24,25] that the difference between the high and low pressure spectra is caused by the formation of the XeCl molecule in vibrationally and rotationally excited states.…”
Section: Variation Of the Xecl Band Shape With Experimental Conditionssupporting
confidence: 81%
“…The spectrum at 10 mbar is similar to those reported in [23,24] and pressure dependence of the spectra qualitativly agrees with the results in [9]. It is usually assumed [9,24,25] that the difference between the high and low pressure spectra is caused by the formation of the XeCl molecule in vibrationally and rotationally excited states. At low pressure the XeCl molecule emits from those vibrationally and rotationally excited www.cpp-journal.org states whereas at high pressures the XeCl molecule is vibrationally relaxed before emission.…”
Section: Variation Of the Xecl Band Shape With Experimental Conditionssupporting
confidence: 81%
“…As already described in [3], at pressures above 10 mbar, the positive column constricts towards the discharge axis. The constricted column has a higher axis temperature and larger radial temperature gradients.…”
Section: N T E R F E R O M E T R I C S E T -U Pmentioning
confidence: 74%
“…In a preceeding paper [3] we reported measurements of the UV radiation power and the radial distribution of the emitting excimer molecules. Also, some characteristics of this discharge type, e.g.…”
Section: Introductionmentioning
confidence: 99%
“…It is clear that at low pressures, up to 30 mbar, which is used for cw XeCl lamps, the harpoon mechanism is dominant [26][27][28]. At high pressures, above atmospheric as in XeCl lasers, ion recombination is much more efficient [29][30][31].…”
Section: Decay Of the Xecl Excimer Radiationmentioning
confidence: 97%