Improved methods for signal processing in measurements of mercury by Tekran® 2537A and 2537B instruments

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Abstract

Atmospheric Hg measurements are commonly carried out using Tekran® Instruments Corporation's model 2537 Hg vapor analyzers, which employ gold amalgamation preconcentration sampling and detection by thermal desorption (TD) and atomic fluorescence spectrometry (AFS). A generally overlooked and poorly characterized source of analytical uncertainty in those measurements is the method by which the raw Hg atomic fluorescence (AF) signal is processed. Here I describe new software-based methods for processing the raw signal from the Tekran® 2537 instruments, and I evaluate the performances of those methods together with the standard Tekran® internal signal processing method. For test datasets from two Tekran® instruments (one 2537A and one 2537B), I estimate that signal processing uncertainties in Hg loadings determined with the Tekran® method are within ±[1%+ 1.2 pg] and ±[6%+0.21 pg], respectively. I demonstrate that the Tekran® method can produce significant low biases (≥5 %) not only at low Hg sample loadings (<5 pg) but also at tropospheric background concentrations of gaseous elemental mercury (GEM) and total mercury (THg) (~1 to 2 ng m-3/ under typical operating conditions (sample loadings of 5-10 pg). Signal processing uncertainties associated with the Tekran® method can therefore represent a significant unaccounted for addition to the overall ~10 to 15% uncertainty previously estimated for Tekran®- based GEM and THg measurements. Signal processing bias can also add significantly to uncertainties in Tekran®-based gaseous oxidized mercury (GOM) and particle-bound mercury (PBM) measurements, which often derive from Hg sample loadings <5 pg. In comparison, estimated signal processing uncertainties associated with the new methods described herein are low, ranging from within ±0.053 pg, when the Hg thermal desorption peaks are defined manually, to within ±[2%C0.080 pg] when peak definition is automated. Mercury limits of detection (LODs) decrease by 31 to 88% when the new methods are used in place of the Tekran® method. I recommend that signal processing uncertainties be quantified in future applications of the Tekran® 2537 instruments.

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APA

Ambrose, J. L. (2017). Improved methods for signal processing in measurements of mercury by Tekran® 2537A and 2537B instruments. Atmospheric Measurement Techniques, 10(12), 5063–5073. https://doi.org/10.5194/amt-10-5063-2017

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