The temporal distribution characteristics of total gaseous mercury at an urban monitoring site in Seoul during 1999-2000

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Abstract

In order to assess the temporal variabilities of atmospheric mercury (Hg) from an area moderately impacted by man-made source processes, the concentrations of total gaseous mercury were measured routinely from an urban monitoring station during January 1999-August 2000. The mean hourly concentration of Hg from overall measurements was computed to be 5.26±3.27ngm-3 (N=11, 572). Using these measurement data, we inspected various aspects on the temporal distribution of Hg. When analyzed over 24h scale, the pattern was characterized by high concentration during nighttime relative to daytime (e.g., values approaching 9ngm-3). This pattern was prominent during winter and seen persistently across fall, spring, and summer. When divided seasonally, the highest mean of 6.01ngm-3 was observed during winter. It appears that such wintertime dominance is most likely to come from the anthropogenic sources such as household heating systems from late fall to early spring. A close inspection of the Hg data however indicated that the seasonal variation proceeded quite dynamically. Inspection of seasonally divided data groups generally showed substantial variabilities among different months. In order to analyze the factors affecting Hg distributions over different time scale, we conducted the correlation analysis. Whereas Hg generally exhibited strong correlations with such parameters as PM, SO2, and NO2, its relationship varied diurnally and seasonally. The overall results of the present study suggest that changes in its source signatures can vary over varying time scale under the influence of strong man-made source processes. Copyright © 2001 Elsevier Science Ltd.

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Kim, K. H., & Kim, M. Y. (2001). The temporal distribution characteristics of total gaseous mercury at an urban monitoring site in Seoul during 1999-2000. Atmospheric Environment, 35(25), 4253–4263. https://doi.org/10.1016/S1352-2310(01)00214-X

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