2004
DOI: 10.1016/j.sab.2004.09.003
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Influence of ambient gas pressure on laser-induced breakdown spectroscopy technique in the parallel double-pulse configuration

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Cited by 145 publications
(74 citation statements)
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“…shielding for the ablation pulse [29,30]. Higher sensitivity was also evident in the double pulse pre-spark configuration, than when compared to all other experimental data, due to the resolution of emission line Ti II 336.12 nm.…”
mentioning
confidence: 58%
“…shielding for the ablation pulse [29,30]. Higher sensitivity was also evident in the double pulse pre-spark configuration, than when compared to all other experimental data, due to the resolution of emission line Ti II 336.12 nm.…”
mentioning
confidence: 58%
“…Lower gas pressure can lead to a shift toward smaller particle size distributions of ablated aerosol [36][37][38] and therefore it is natural to consider that stability of the signal intensity could be improved. To test this, signal intensity profiles were obtained from a metallic sample using the present low gas-pressure cell.…”
Section: Signal Intensity Profilementioning
confidence: 99%
“…The effect of the gas pressure in the sample cell onto the data was well studied in laserinduced breakdown spectroscopy (LIBS) and enhancement of the signal intensity could be achieved by laser ablation under low-pressure conditions. 35 The gain in the signal intensity in LIBS is basically explained by better plasma expansion due to low local pressure, 36,37 or by a shift toward a smaller particle size distribution of ablated particles. 23 Moreover, the level of sample re-deposition after ablation can be reduced by laser ablation under low gas-pressure conditions.…”
Section: Introductionmentioning
confidence: 99%
“…recently in Refs. [1][2][3][4][5][6][7][8]. A significant number of experimental studies have been dedicated to the investigation of the Ar I total Stark full-width at half-intensity maximum (FWHM) (W t ) and total Stark shift (d t ) of the 751.465 nm, 763.511 nm and 772.376 nm spectral lines from 4s-4p transition and 696.543 nm, 727.294 nm, 706.722 nm and 738.398 nm spectral lines from 4s -4pV transition.…”
Section: Introductionmentioning
confidence: 99%