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Volume 16, issue 3
Atmos. Chem. Phys., 16, 1511-1530, 2016
https://doi.org/10.5194/acp-16-1511-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.
Atmos. Chem. Phys., 16, 1511-1530, 2016
https://doi.org/10.5194/acp-16-1511-2016
© Author(s) 2016. This work is distributed under
the Creative Commons Attribution 3.0 License.

Research article 10 Feb 2016

Research article | 10 Feb 2016

Origin of oxidized mercury in the summertime free troposphere over the southeastern US

V. Shah1, L. Jaeglé1, L. E. Gratz2, J. L. Ambrose3,a, D. A. Jaffe1,3, N. E. Selin4, S. Song4, T. L. Campos5, F. M. Flocke5, M. Reeves5, D. Stechman5, M. Stell5, J. Festa6, J. Stutz6, A. J. Weinheimer7, D. J. Knapp7, D. D. Montzka7, G. S. Tyndall7, E. C. Apel7, R. S. Hornbrook7, A. J. Hills7, D. D. Riemer8, N. J. Blake9, C. A. Cantrell10, and R. L. Mauldin III10,11 V. Shah et al.
  • 1Department of Atmospheric Sciences, University of Washington, Seattle, WA, USA
  • 2Environmental Program, Colorado College, Colorado Springs, CO, USA
  • 3School of Science, Technology, Engineering and Mathematics, University of Washington-Bothell, Bothell, WA, USA
  • 4Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
  • 5Earth Observing Laboratory, National Center for Atmospheric Research, Boulder, CO, USA
  • 6Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA, USA
  • 7Atmospheric Chemistry Observations and Modeling Laboratory, National Center for Atmospheric Research, Boulder, CO, USA
  • 8Rosenstiel School of Marine and Atmospheric Science, University of Miami, Miami, FL, USA
  • 9Department of Chemistry, University of California, Irvine, CA, USA
  • 10Department of Atmospheric and Oceanic Sciences, University of Colorado, Boulder, CO, USA
  • 11Department of Physics, University of Helsinki, Helsinki, Finland
  • anow at: College of Engineering and Physical Sciences, University of New Hampshire, Durham, NH, USA

Abstract. We collected mercury observations as part of the Nitrogen, Oxidants, Mercury, and Aerosol Distributions, Sources, and Sinks (NOMADSS) aircraft campaign over the southeastern US between 1 June and 15 July 2013. We use the GEOS-Chem chemical transport model to interpret these observations and place new constraints on bromine radical initiated mercury oxidation chemistry in the free troposphere. We find that the model reproduces the observed mean concentration of total atmospheric mercury (THg) (observations: 1.49 ± 0.16ng m−3, model: 1.51 ± 0.08ng m−3), as well as the vertical profile of THg. The majority (65%) of observations of oxidized mercury (Hg(II)) were below the instrument's detection limit (detection limit per flight: 58–228pg m−3), consistent with model-calculated Hg(II) concentrations of 0–196pg m−3. However, for observations above the detection limit we find that modeled Hg(II) concentrations are a factor of 3 too low (observations: 212 ± 112pg m−3, model: 67 ± 44pg m−3). The highest Hg(II) concentrations, 300–680pg m−3, were observed in dry (RH < 35%) and clean air masses during two flights over Texas at 5–7km altitude and off the North Carolina coast at 1–3km. The GEOS-Chem model, back trajectories and observed chemical tracers for these air masses indicate subsidence and transport from the upper and middle troposphere of the subtropical anticyclones, where fast oxidation of elemental mercury (Hg(0)) to Hg(II) and lack of Hg(II) removal lead to efficient accumulation of Hg(II). We hypothesize that the most likely explanation for the model bias is a systematic underestimate of the Hg(0) + Br reaction rate. We find that sensitivity simulations with tripled bromine radical concentrations or a faster oxidation rate constant for Hg(0) + Br, result in 1.5–2 times higher modeled Hg(II) concentrations and improved agreement with the observations. The modeled tropospheric lifetime of Hg(0) against oxidation to Hg(II) decreases from 5months in the base simulation to 2.8–1.2months in our sensitivity simulations. In order to maintain the modeled global burden of THg, we need to increase the in-cloud reduction of Hg(II), thus leading to faster chemical cycling between Hg(0) and Hg(II). Observations and model results for the NOMADSS campaign suggest that the subtropical anticyclones are significant global sources of Hg(II).

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We present airborne observations of mercury over the southeastern USA during summer. Higher concentrations of oxidized mercury were observed in clean, dry air masses descending in the subtropical anti-cyclones. We used an atmospheric model to simulate the chemistry and transport of mercury. We found reasonable agreement with the observations when the modeled oxidation of elemental mercury was increased, suggesting fast cycling between elemental and oxidized mercury.
We present airborne observations of mercury over the southeastern USA during summer. Higher...
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