Observations of cyanogen bromide (BrCN) in the global troposphere and their relation to polar surface O₃ destruction
- Creators
- Roberts, James M.
- Wang, Siyuan1, 2
- Veres, Patrick R.3
- Neuman, J. Andrew1, 2
- Robinson, Michael A.1, 2
- Bourgeois, Ilann1, 2, 4
- Peischl, Jeff1, 2
- Ryerson, Thomas B.
- Thompson, Chelsea R.
- Allen, Hannah M.5
- Crounse, John D.5
- Wennberg, Paul O.5
- Hall, Samuel R.6
- Ullmann, Kirk6
- Meinardi, Simone7
- Simpson, Isobel J.7
- Blake, Donald7
- 1. Cooperative Institute for Research in Environmental Sciences, CIRES, University of Colorado, and NOAA, Boulder, CO, USA
- 2. National Oceanic and Atmospheric Administration
- 3. Earth Observing Laboratory, National Center for Atmospheric Research, Boulder, CO, USA
- 4. Université Savoie Mont Blanc
- 5. California Institute of Technology
- 6. National Center for Atmospheric Research
- 7. University of California, Irvine
Abstract
Bromine activation (the production of Br in an elevated oxidation state) promotes ozone destruction and mercury removal in the global troposphere and commonly occurs in both springtime polar boundary layers, often accompanied by nearly complete ozone destruction. The chemistry and budget of active bromine compounds (e.g., Br2, BrCl, BrO, HOBr) reflect the cycling of Br and affect its environmental impact. Cyanogen bromide (BrCN) has recently been measured by iodide ion high-resolution time-of-flight mass spectrometry (I− CIMS), and trifluoro methoxide ion time-of-flight mass spectrometry (CF3O− CIMS) during the NASA Atmospheric Tomography Mission second, third, and fourth deployments (NASA ATom), and could be a previously unquantified participant in active Br chemistry. BrCN mixing ratios ranged from below the detection limit (1.5 pptv) up to as high as 36 pptv (10 s average) and enhancements were almost exclusively confined to the polar boundary layers in the Arctic winter and in both polar regions during spring and fall. The coincidence of BrCN with active Br chemistry (often observable BrO, BrCl and O3 loss) and high CHBr3/CH2Br2 ratios imply that much of the observed BrCN is from atmospheric Br chemistry rather than a biogenic source. Likely BrCN formation pathways involve the heterogeneous reactions of active Br (Br2, HOBr) with reduced nitrogen compounds, for example hydrogen cyanide (HCN/CN−), on snow, ice, or particle surfaces. Competitive reaction calculations of HOBr reactions with Cl−/Br− and HCN/CN− in solution, as well as box model calculations with bromine chemistry, confirm the viability of this formation channel and show a distinct pH dependence, with BrCN formation favored at higher pH values. Gas-phase loss processes of BrCN due to reaction with radical species are likely quite slow and photolysis is known to be relatively slow (BrCN lifetime of ∼ 4 months in midlatitude summer). These features, and the lack of BrCN enhancements above the polar boundary layer, imply that surface reactions must be the major loss processes. The fate of BrCN determines whether BrCN production fuels or terminates bromine activation. BrCN reactions with other halogens (Br−, HOCl, HOBr) may perpetuate the active Br cycle; however, preliminary laboratory experiments showed that BrCN did not react with aqueous bromide ion (< 0.1 %) to reform Br2. Liquid-phase reactions of BrCN are more likely to convert Br to bromide (Br−) or form a C–Br bonded organic species, as these are the known condensed-phase reactions of BrCN and would therefore constitute a loss of atmospheric active Br. Thus, further study of the chemistry of BrCN will be important for diagnosing polar Br cycling.
Copyright and License
© Author(s) 2024. This work is distributed under the Creative Commons Attribution 4.0 License.
Code Availability
Statistical analyses were performed using the standard routines for averaging and ODR fitting provided by Igor Pro Version 8 software. The box model code is available on request.
Data Availability
Data are available in the main text and Supplement as well as from the Atmospheric Tomography Mission archives in the Oak Ridge National Laboratory Distributed Active Archive Center (ORNL DAAC) at https://doi.org/10.3334/ORNLDAAC/1925 (Wofsy et al., 2021).
Contributions
JMR wrote the paper with assistance from co-authors. JMR, PRV, JAN, MAR, JDC, and POW worked on BrCN calibration. SW performed model analyses on Br chemistry. PRV, JAN, IB, JP, TBR, CRT, HMA, JDC, POW, SRH, KU, DB, and SM conducted the ATom measurements.
This paper was edited by Markus Ammann and reviewed by two anonymous referees.
Acknowledgement
We thank William D. Neff and Matthew Shupe for helpful discussions. We acknowledge the ATom Science Team who contributed to this mission. We also gratefully acknowledge the NASA and ESPO project personnel who participated in this campaign. This work was supported by the NOAA cooperative agreement with CIRES: NA17OAR4320101.
The ATom project is an EVS-2 investigation under NASA Research Announcement (NRA) NNH13ZDA001N-EVS2, Research Opportunities in Space and Earth Science (ROSES-2013), and is funded through NASA agreement NNH15AB12I to NOAA.
Contributions from Caltech were funded through NASA agreements NNX15AG61A and 80NSSC21K1704.
The National Center for Atmospheric Research is sponsored by the National Science Foundation under cooperative agreement 1852977.
Funding
This research has been supported by the National Oceanic and Atmospheric Administration (grant no. NA17OAR4320101), the National Aeronautics and Space Administration (grant nos. NNH13ZDA001N-EVS2, NNH15AB12I, NNX15AG61A, and 80NSSC21K1704), and the National Science Foundation (grant no. 1852977).
Additional Information
The supplement related to this article is available online at: https://doi.org/10.5194/acp-24-3421-2024-supplement.
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Additional details
- National Oceanic and Atmospheric Administration
- NA17OAR4320101
- National Aeronautics and Space Administration
- NNH13ZDA001N-EVS2
- National Aeronautics and Space Administration
- NNH15AB12I
- National Aeronautics and Space Administration
- NNX15AG61A
- National Aeronautics and Space Administration
- 80NSSC21K1704
- National Science Foundation
- 1852977
- Accepted
-
2024-01-18Accepted
- Available
-
2024-03-20Published online
- Publication Status
- Published