1995
DOI: 10.2172/88576
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Trapping of radiation in plasmas

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Cited by 3 publications
(5 citation statements)
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“…This radiation trapping [45][46][47][48] can lengthen the effective radiative lifetime of the excited state that produces the photon dramatically. This, in turn, gives nonradiative quenching processes much more time to quench the excited state before it emits a VUV photon.…”
Section: Resultsmentioning
confidence: 99%
“…This radiation trapping [45][46][47][48] can lengthen the effective radiative lifetime of the excited state that produces the photon dramatically. This, in turn, gives nonradiative quenching processes much more time to quench the excited state before it emits a VUV photon.…”
Section: Resultsmentioning
confidence: 99%
“…From about 20% xenon concentration and higher, the dimer emission is stronger than emission from the resonant line. The emission from the resonant line is reduced because of enhanced radiation trapping by the collisional broadening of the resonance line [20,21]. At these pressures, collisional broadening is the dominant broadening mechanism of the resonance lines in the helium-xenon mixture [21].…”
Section: Resultsmentioning
confidence: 99%
“…The emission from the resonant line is reduced because of enhanced radiation trapping by the collisional broadening of the resonance line [20,21]. At these pressures, collisional broadening is the dominant broadening mechanism of the resonance lines in the helium-xenon mixture [21]. Although emission from the transitions from higher excited states to the [6s] and [6s ] states which emit in the range from about 450 nm in the blue extending into the infrared does exist, the details of those lines are beyond the scope of the present model.…”
Section: Resultsmentioning
confidence: 99%
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