2017
DOI: 10.1039/c7ja00185a
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Evaluation of a compact VUV spectrometer for elemental imaging by laser-induced breakdown spectroscopy: application to mine core characterization

Abstract: This work introduces a new approach to perform LIBS elemental imaging in the vacuum ultraviolet (VUV) wavelength range by using an argon purged probe coupled to a compact spectrometer.

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Cited by 29 publications
(6 citation statements)
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“…An argon flow of 1.3 L/ min blowing through the plasma was used both to prevent surface contamination due to ablated material deposition from previous laser shots and to enhance the emission signal. 25 The laser pulse energy and its focus onto the sample were strictly controlled.…”
Section: Libs Imaging Setupmentioning
confidence: 99%
“…An argon flow of 1.3 L/ min blowing through the plasma was used both to prevent surface contamination due to ablated material deposition from previous laser shots and to enhance the emission signal. 25 The laser pulse energy and its focus onto the sample were strictly controlled.…”
Section: Libs Imaging Setupmentioning
confidence: 99%
“…In addition, this technique is associated with interesting analytical performances, such as multi-element detection, detection of light elements, limits of detection in the range of ppm for most of the elements and microscopic-scale resolution [ 62 ]. It also has quantitative capabilities through the use of reference samples or various calibration strategies [ 209 , 210 , 211 , 212 ]. All these advantages make LIBS imaging very promising with the potential to become a reference technique in the panel of space-resolved elemental approaches, also including electron probe micro-analysis, laser ablation inductively coupled plasma mass spectrometry and synchrotron radiation microanalysis [ 213 , 214 , 215 ].…”
Section: Laser-induced Breakdown Spectroscopy (Libs)mentioning
confidence: 99%
“…Due to the intended application of in-situ S assessment in coal mining, the experiments were conducted in ambient air with a N 2 -filled spectrometer. For other publications reporting on the VUV emission lines of S I around 180 nm, different atmospheric conditions have been employed, mainly argon at different pressures, but none of them involves a pressure below 200 Pa [27,105,107,128,129].…”
Section: Detection and Quantification Of Sulfur In Lunar Analoguesmentioning
confidence: 99%