E3S Web of Conferences
Volume 1, 2013Proceedings of the 16th International Conference on Heavy Metals in the Environment
|Number of page(s)||3|
|Section||GMOS I (Global Mercury Observation System)|
|Published online||23 April 2013|
222Rn calibrated mercury fluxes from terrestrial surfaces of southern Africa derived from observations at Cape Point, South Africa
1 Max-Planck-Institut für Chemie, P.O.Box 3060, D-55020 Mainz, GERMANY
2 South African Weather Service c/o CSIR, P.O.Box 320, Stellenbosch 7599, SOUTH AFRICA
3 ANSTO Environment, PMB 1, Menai, NSW 2234, AUSTRALIA
4 Helmholtz-Zentrum Geesthacht, Institute of Coastal Research, Max-Planck-Strasse, D-21502 Geesthacht, GERMANY
Gaseous elemental mercury (GEM) and 222Rn, a radioactive gas of primarily terrestrial origin with a half-life of 3.8 days, have been measured simultaneously at Cape Point, South Africa, since March 2007. Between March 2007 and December 2009 altogether 59 events with high 222Rn concentrations were identified. GEM correlated with 222Rn in 41 of the events and was constant during the remaining events without significant correlation. The average GEM/222Rn emission ratio of all events was −0.0047 ± 0.0054 pg mBq−1, with ± 0.0054 being the standard error of the average. With an emission rate of 1.1 222Rn atoms cm−2 s−1 and a correction for the transport duration, this emission ratio corresponds to a radon calibrated flux of about −0.53 ± 0.62 ng m−2 h−1 which is statistically not distinguishable from zero. With wet deposition, which is not included in this estimate, the terrestrial surface of southern Africa appears to be a net mercury sink.
Key words: Heavy metals / mercury / emission / deposition / flux / terrestrial surface
© Owned by the authors, published by EDP Sciences, 2013
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 2.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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