Global Observations of Acetyl Peroxynitrate (PAN) in the Remote Troposphere
Creators
- Lee, Young Ro1
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Huey, L. Gregory1
- Tanner, David J.1
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Roberts, James M.2
- Wang, Yuhang1
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Wennberg, Paul O.3
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Crounse, John D.3
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Allen, Hannah3
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Apel, Eric C.4
- Hills, Alan J.4
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Hornbrook, Rebecca S.4
- Elkins, James W.5
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Hintsa, Eric5, 6
- Moore, Fred5, 6
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Hall, Samuel R.4
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Ullmann, Kirk4
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McKain, Kathryn5
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Sweeney, Colm5
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Ryerson, Thomas B.2
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Peischl, Jeff2, 6
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Tompson, Chelsea R.2, 6
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Bourgeois, Ilann2, 6
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Ray, Eric2, 6
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Newman, Paul A.7
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Strode, Sarah7, 8
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1.
Georgia Institute of Technology
- 2. NOAA Chemical Sciences Laboratory
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3.
California Institute of Technology
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4.
National Center for Atmospheric Research
- 5. NOAA Global Monitoring Laboratory
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6.
Cooperative Institute for Research in Environmental Sciences
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7.
Goddard Space Flight Center
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8.
Morgan State University
Abstract
We present global airborne observations of acetyl peroxynitrate (CH3C(O)OONO2, PAN) in the remote troposphere from the Atmospheric Tomography (ATom) campaign. These observations show that biomass burning is the dominant source of PAN in the Southern Hemisphere (SH). In the Northern Hemisphere, anthropogenic emissions from Asia and Europe also contribute significantly to PAN over the Pacific and Atlantic Oceans. Model simulations underestimate PAN in the lower troposphere, in part, due to the underestimation of local production driven by acetaldehyde oxidation and βNO2 (the ratio of acetyl peroxy radicals reacting with NO2 relative to other pathways). The significant impacts of biomass burning evident in the ATom PAN observations suggest that improving model treatment of plume transport and the conversion of NOx to PAN in biomass burning plumes is a viable focus for better simulating PAN. Global observations of PAN provide a benchmark for the evaluation of satellite observations and model simulations of PAN.
Copyright and License
© 2025. The Author(s). This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
Acknowledgement
The PAN observations and analysis were supported by NASA Grants NNX15AT90G and 80NSSC23K0826. This material is based upon work supported by the NSF National Center for Atmospheric Research, which is a major facility sponsored by the U.S. National Science Foundation under Cooperative Agreement No. 1852977. The GMI CTM was supported by the NASA Modeling, Analysis and Prediction (MAP) program. The NASA High-End Computing Program (HEC) provided computational resources through the NASA Center for Climate Simulation (NCCS) for the GMI CTM simulation.
Data Availability
The data used in this work is available from the ATom campaign archive at https://doi.org/10.3334/ORNLDAAC/1925 (Wofsy et al., 2021). The GMI modelling results for the ATom campaign are available at https://doi.org/10.3334/ORNLDAAC/1897 (Strode et al., 2021).
Supplemental Material
Supporting Information S1 (DOCX)
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Additional details
Related works
- Is supplemented by
- Supplemental Material: https://agupubs.onlinelibrary.wiley.com/action/downloadSupplement?doi=10.1029%2F2025GL115001&file=2025GL115001-sup-0001-Supporting+Information+SI-S01.docx (URL)
- Dataset: 10.3334/ORNLDAAC/1925 (DOI)
- Dataset: 10.3334/ORNLDAAC/1897 (DOI)
Funding
- National Aeronautics and Space Administration
- NNX15AT90G
- National Aeronautics and Space Administration
- 80NSSC23K0826
- National Science Foundation
- 1852977
Dates
- Accepted
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2025-07-28
- Available
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2025-08-18Version of record online
- Available
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2025-08-18Issue online