2007
DOI: 10.1007/s00340-007-2604-z
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Diode-laser-based sensor for ultraviolet absorption measurements of atomic mercury

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Cited by 35 publications
(40 citation statements)
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References 27 publications
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“…Such commercial instruments use highly stabilised light sources and electronics, which our instrument does not. Nevertheless, our detection limit is significantly better than the 0.1 ppbv (800 ng m −3 ) detection limit reported by Anderson et al 23 , using sum-frequency generation and two diode laser systems, or the 200 ng m −3 estimated by Thiebaud et al 24 with a Hg vapour lamp combined with a UV LED. Both of these systems were designed for the high Hg levels of continuous emission monitoring and made use of additional spectral information to discriminate the absorption of Hg from background absorption.…”
Section: Resultscontrasting
confidence: 58%
“…Such commercial instruments use highly stabilised light sources and electronics, which our instrument does not. Nevertheless, our detection limit is significantly better than the 0.1 ppbv (800 ng m −3 ) detection limit reported by Anderson et al 23 , using sum-frequency generation and two diode laser systems, or the 200 ng m −3 estimated by Thiebaud et al 24 with a Hg vapour lamp combined with a UV LED. Both of these systems were designed for the high Hg levels of continuous emission monitoring and made use of additional spectral information to discriminate the absorption of Hg from background absorption.…”
Section: Resultscontrasting
confidence: 58%
“…The three cells include an Hg cell filled with metallic Hg at ambient pressure (∼ 80 kPa within cell; green line); an Hg cell filled with metallic Hg under low pressure (1.33 × 10 −5 Pa within cell; blue line); and the spectrum of an Hg cell filled with an isotopically enriched, metallic 200 Hg (94 % + isotopic purity) under low pressure (1.33 × 10 −5 Pa within cell; red line). In the lowpressure GEM spectrum (blue line), five of seven known stable Hg isotopes (Schroeder and Munthe, 1998;Spuler et al, 2000) can be seen as individual hyperfine structures, which are commonly observed when atmospheric pressure broadening is eliminated (Anderson et al, 2007;Spuler et al, 2000;Schweitzer, 1963). Differences between the external Hg cell at ambient pressure (green line) and low pressure (blue line) result from collisions of Hg atoms with air molecules, shortening their radiative lifetime or resulting in a phase shift and causing collision-induced/pressure broadening of the absorption line (Demtröder, 2003).…”
Section: Wavelength Locking and Stabilization Using An External Hg Cellmentioning
confidence: 99%
“…For the TDLAS technique, at least 80-GHz (three times the absorption linewidth of mercury vapor) of mode-hop-free tuning range is required to extract the whole absorption feature of mercury out of the broadband attenuation due to absorption of other species or particulate scattering [10,12]. However, for the MDL-COSPEC method, there is no special request on mode-hop-free tuning range; instead, the mode hop is used to increase the wavelength coverage and thus obtain an off-resonant baseline.…”
Section: Selectivitymentioning
confidence: 99%
“…An alternative technique for elemental mercury detection is the employment of laser absorption spectroscopy. Various techniques have been developed to generate laser radiation at 253.7 nm, including sum-frequency generation (SFG) by two diode lasers (DLs) [10][11][12], frequency doubling pulsed dye lasers or optical-parametric-oscillator lasers [13][14][15] and frequency quadrupling diode lasers or solid-state lasers [16,17]. By comparison, SFG-DL based systems possess the merits of agile tunability, simplicity and low-cost.…”
Section: Introductionmentioning
confidence: 99%
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