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![Page 1: Deriving vertical profiles of free tropospheric trace gases from ground based measurements: Implications for oxidation of atmospheric mercury Sean Coburn.](https://reader033.fdocuments.net/reader033/viewer/2022051517/56649e5c5503460f94b540b9/html5/thumbnails/1.jpg)
Deriving vertical profiles of free tropospheric trace gases from ground based measurements:
Implications for oxidation of atmospheric mercury
Sean Coburn1,2, Siyuan Wang 1,2, Barbara Dix2, Arnout terSchure3, and Rainer Volkamer1,2
1Dept. of Chemistry, University of Colorado, Boulder, CO2Cooperative Institute for Research in Environmental Science (CIRES), Boulder,
CO3Electric Power Research Institute (EPRI), Palo Alto, CA,
ESA-SOLAS-EGU Conference28-31 October 2014
Frascati ,Italy
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TORERO Field Study
Outline
Background• Halogens and mercuryInstrumentation/Technique• MAX-DOAS • MeasurementsResults• Derived vertical columns• Implications for
atmospheric oxidationSummary/Conclusions
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Why are halogen important?• Modify oxidative capacity of atmosphere through reaction with O3
• Linked to atmospheric HOx and NOx cycles.• Participate in new particle formation• Involved in mercury oxidation reactions
Pechtl et al., 2006 (ACP); Holmes et al., 2009 (AE)
<2ppt BrO in MBL
What about FT?
Tropospheric Halogens
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BrO overview: observations and models
Theys et al. [2011]
Satellite: 1-3 x1013 molec cm-2
(Chance et al., 1998; Wagner et al., 2001; Richter et al., 2002; Van Roozendael et al., 2002; Theys et al., 2011)
Ground : 0.2-3 x1013 molec cm-2
(Schofield et al., 2004 , Hendrick et al., 2007; Theys et al., 2007; Coburn et al., 2011; Coburn et al., 2014, in prep.)
Balloon: 0.2-0.3 x1013 molec cm-2
(Pundt et al., 2002; Dorf et al., 2008)
Models: 0.2-1.0 x1013 molec cm-2
(~ 0.2-0.5 ppt)(Saiz Lopez et al., 2012; Parrella et al., 2012) – in the tropics
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Mercury
Prevailing winds
• Atmosphere biggest source of mercury to terrestrial environment
Where in the atmosphere is oxidation occurring?
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MAX-DOAS observations of the FT
• Greatest sensitivity at instrument altitude
• Ground based still contains information about layers aloft
• Aircraft can directly probe layers at different altitudes
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MAX-DOAS Platforms/Instrumentation
spectrographs/detectors
Telescope pylon
motionstabilized
Volkamer et al., SPIE 2009, Coburn et al., 2011, Baidar et al., AMT 2013
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MAX-DOAS Data overview
# of meas. days ~300
Periods June – Oct. 2009; March – June 2010; Aug. – Oct. 2010; Feb. 2011
# of spectra >200,000
Trace gases BrO, IO, CHOCHO, HCHO, NO2, O4
% Cloudy <40%
Filters Detection limit, absolute RMS, SZA
Spectral proof for the detection of IO and BrO
BrO = 2.1 ppt IO = 3.1 ppt
MAX-DOAS Measurements
• Long term measurements
• Retrieve multiple species
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optic
al d
ensi
ty [a
.u.]
wavelength [nm]
3.4 ppt BrO @ 14.2km
2.2 ppt BrO @ 9.0km
0.3 ppt BrO @ 4.1km
no BrO @ 0.9km
340 359
BrO measured by CU AMAX-DOAS
18E-4
13E-4
5E-4
<1-2E-4
optic
al d
ensi
ty [a
.u.]
BrO is detectable over most of the tropospheric air column
~ 0.3 ppt BrO in lower FT (4.1km)~ 3.4 ppt BrO above 14km
DOAS detection limit: ~ 0.3 ppt BrO @ 1min data
Spectral proof of BrO in the tropical FT
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CU AMAX/GMAX VCDs: BrO & IO
In line with other free tropospheric observations 1-3x1013 molec cm-2 global background VCD
IO more variable -> background 2-4x1012 molec cm-2 IO VCD?
No BrO in the MBL!
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Vertical profiles: Non-linear Optimal Estimation
Simulated O4 SCDs
Radiative transfer (1)
Inversion
Measured O4 SCDs
convergence?
Weighing function
Measured Trace gas
SCDs
Radiative transfer
Trace gasprofile
Aerosolprofile
Volkamer et al., 2009, SPIE; Baidar et al., 2013, AMT; Rodgers (2000); http://rtm.iup.uni-heidelberg.de/McArtim
Þ Trace gases and aerosol extinction profiles
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CU GMAX/AMAX Profiles: BrO and IO
Converge on 1 profile, independent of a priori
Coburn et al., 2014, in prep; Volkamer Group, unpublished
Now have vertical distribution of BrO in the troposphere -> Use to assess impact on GEM oxidation
Comparison with previous profile measurements
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Comparison with model profiles
Models are under predicting BrO in the free troposphere
Effect on GEM oxidation?
TORERO, GEOS-Chem This study, WACCM
Coburn et al., 2014, in prep; Volkamer Group, unpublished
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Relevance of FT-BrO for mercury
Even with lower amounts from models oxidation by Br radicals is dominant pathway
Modeled Measured
Coburn et al., 2014, in prep
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Relevance of FT-BrO for mercury
Free tropospheric Hg brought to the BL through deep convection
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ConclusionsField observations of halogens:• First simultaneous observations of BrO and IO in the tropical FT
– First vertical profiles of BrO from aircraft in the tropics
• Vertical profiles and VCDs derived from ground-based MAX-DOAS measurements
• IO and BrO are widespread in the FT and detected in NH and SH– 0.1-0.5 ppt IO have been detected in the FT in NH and SH– 2 ppt BrO are measured at altitudes >12km in NH and SH– IO and BrO show different vertical profiles– Some similarities between SH and NH from AMAX and GMAX
Relevance for mercury:• Bromine dominates mercury oxidation rates (chlorine < 1%). • GEM lifetime wrt bromine: ~1 d in upper FT; 8 to 80 d in lower FT
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Volkamer GroupEPA staffNCAR/EOL/RAFthe entire TORERO team
FundingEPRI TI ProgramEPRI Air toxics programNSF-TORERO
Acknowledgements