2007
DOI: 10.1088/0022-3727/40/9/025
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X-ray induced fluorescence measurement of segregation in a DyI3–Hg metal-halide lamp

Abstract: Segregation of elemental Dy in a DyI 3-Hg metal-halide high-intensity discharge lamp has been observed with x-ray induced fluorescence. Significant radial and axial Dy segregation are seen, with the axial segregation characterized by a Fischer parameter value of λ = 0.215 ± 0.002 mm −1. This is within 7% of the value (λ = 0.20 ± 0.01 mm −1) obtained by Flikweert et al (2005 J. Appl. Phys. 98 073301) based on laser absorption by neutral Dy atoms. Elemental I is seen to exhibit considerably less axial and radial… Show more

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Cited by 14 publications
(24 citation statements)
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“…In order to also study the effect of convection, experiments have also been done at hyper-gravity [11] and normal gravity [10], the future plan is to compare numerical results of the model to these experiments.…”
Section: Discussionmentioning
confidence: 99%
“…In order to also study the effect of convection, experiments have also been done at hyper-gravity [11] and normal gravity [10], the future plan is to compare numerical results of the model to these experiments.…”
Section: Discussionmentioning
confidence: 99%
“…The model was run with lamp fillings ranging from 3 to 20 mg Hg. To fix the boundary conditions for the elemental pressure we assume the existence of a cold spot at the bottom corner of the lamp, where the elemental pressure is derived from the x-ray induced fluorescence measurements at 1g of the elemental density of Dy and I at the cold spot [20]. Everywhere else the flux through the wall is zero.…”
Section: Resultsmentioning
confidence: 99%
“…Increase in the temperature by 10 K is enough to raise the vapour pressure to 30%. Using a vapour pressure of 150 Pa rather than the value of 517 Pa measured by x-ray fluorescence (XRF) by Nimalasuriya et al [20] on similar lamps yields a better quantitative match between model and experiment.…”
Section: Discussionmentioning
confidence: 99%
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“…Previous efforts to observe the arc and its characteristics in micro-gravity include emission spectroscopy in the space shuttle Bellows et al 1984Bellows et al , 1985. Besides lab experiments (1g) Nimalasuriya et al 2005Nimalasuriya 2007) we investigated the lamp during parabolic flights. Here the lamp was measured during periods of about 20 s of micro-gravity (0g) and hyper-gravity (∼ 1.8g) .…”
Section: Introductionmentioning
confidence: 99%