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

Show full item record



Permalink

http://hdl.handle.net/10138/161560

Citation

Shah , V , Jaegle , L , Gratz , L E , Ambrose , J L , Jaffe , D A , Selin , N E , Song , S , Campos , T L , Flocke , F M , Reeves , M , Stechman , D , Stell , M , Festa , J , Stutz , J , Weinheimer , A J , Knapp , D J , Montzka , D D , Tyndall , G S , Apel , E C , Hornbrook , R S , Hills , A J , Riemer , D D , Blake , N J , Cantrell , C A & Mauldin III , R L 2016 , ' Origin of oxidized mercury in the summertime free troposphere over the southeastern US ' Atmospheric Chemistry and Physics , vol. 16 , no. 3 , pp. 1511-1530 . DOI: 10.5194/acp-16-1511-2016

Title: Origin of oxidized mercury in the summertime free troposphere over the southeastern US
Author: Shah, V.; Jaegle, L.; Gratz, L. E.; Ambrose, J. L.; Jaffe, D. A.; Selin, N. E.; Song, S.; Campos, T. L.; Flocke, F. M.; Reeves, M.; Stechman, D.; Stell, M.; Festa, J.; Stutz, J.; Weinheimer, A. J.; Knapp, D. J.; Montzka, D. D.; Tyndall, G. S.; Apel, E. C.; Hornbrook, R. S.; Hills, A. J.; Riemer, D. D.; Blake, N. J.; Cantrell, C. A.; Mauldin III, R. L.
Contributor: University of Helsinki, Department of Physics
Date: 2016
Language: eng
Number of pages: 20
Belongs to series: Atmospheric Chemistry and Physics
ISSN: 1680-7316
URI: http://hdl.handle.net/10138/161560
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 +/- 0.16 ngm(-3), model: 1.51 +/- 0.08 ngm(-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: 58-228 pgm(-3)), consistent with model-calculated Hg(II) concentrations of 0-196 pgm(-3). However, for observations above the detection limit we find that modeled Hg(II) concentrations are a factor of 3 too low (observations: 212 +/- 112 pgm-3, model: 67 +/- 44 pgm(-3)). The high-est Hg(II) concentrations, 300-680 pgm(-3), were observed in dry (RH <35 %) and clean air masses during two flights over Texas at 5-7 km altitude and off the North Carolina coast at 1-3 km. 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 5 months in the base simulation to 2.8-1.2 months 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).
Subject: REACTIVE GASEOUS MERCURY
ATMOSPHERIC MERCURY
ELEMENTAL MERCURY
GLOBAL-MODEL
METHYLMERCURY EXPOSURE
INITIATED REACTIONS
BOUNDARY-LAYER
UNITED-STATES
NORTH-AMERICA
OXIDATION
114 Physical sciences
Rights:


Files in this item

Total number of downloads: Loading...

Files Size Format View
acp_16_1511_2016.pdf 5.574Mb PDF View/Open

This item appears in the following Collection(s)

Show full item record