2010
DOI: 10.1007/s00339-010-5782-1
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Modeling of laser induced breakdown spectroscopy for very low-pressure conditions

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Cited by 14 publications
(6 citation statements)
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“…40 Studies have been performed that show the peak temperatures of laser produced plasma regardless of pressure are the same; however, in reduced pressures, the plasma expands at faster velocities and cools faster. 41,42 Equally consistent with this, our results could also show that the plasma persists for shorter times in reduced pressure and results in reduced line intensities.…”
Section: Description Of the Spectra And Atmospheric Impactssupporting
confidence: 91%
“…40 Studies have been performed that show the peak temperatures of laser produced plasma regardless of pressure are the same; however, in reduced pressures, the plasma expands at faster velocities and cools faster. 41,42 Equally consistent with this, our results could also show that the plasma persists for shorter times in reduced pressure and results in reduced line intensities.…”
Section: Description Of the Spectra And Atmospheric Impactssupporting
confidence: 91%
“…Such an assumption is somehow supported by theoretical papers where it is demonstrated the almost constant plasma temperature and front expansion during the first millimeter of the plasma as long as a certain base pressure has been reached. 19…”
Section: Resultsmentioning
confidence: 99%
“…The plasma passes by the optical eld of view of the spectrographic system with a specic velocity (generally 10 5 to 10 6 cm s À1 ) so this requires fast dynamic detection and gives short temporal duration. 16 Concerning the lifetime of ions presented in the plasma (Fig. 3, top right), the minimum time resolution achievable was 800 ns to allow proper ion extraction.…”
Section: Resultsmentioning
confidence: 99%
“…4a summarizes the data corresponding to the evolution of four atomic species (H, C, N and O) with uence. The signals corresponding to 1 H + , 12 C + , 14 N + and 16 O + were recorded in the mass spectrometer, whereas the emissions at 656.28 nm, 247.82 nm, 746.82 nm and 777.42 nm were used for H, C, N and O, respectively. The four wavelengths selected correspond to emissions from excited states of the neutral atom.…”
Section: Resultsmentioning
confidence: 99%