Preprints
https://doi.org/10.5194/egusphere-2026-559
https://doi.org/10.5194/egusphere-2026-559
16 Feb 2026
 | 16 Feb 2026
Status: this preprint is open for discussion and under review for Atmospheric Chemistry and Physics (ACP).

Chromophores and chemical compositions of brown carbon aerosol before and after photooxidation of combustion emissions

Feng Jiang, Jun Zhang, David Bell, Kun Li, Nadine Borduas-Dedekind, Andre S. H. Prevot, Hongbiao Cui, Harald Saathoff, and Thomas Leisner

Abstract. Brown carbon (BrC) aerosols affect earth’s climate and originate mainly from biomass burning. However, chromophores and chemical composition of BrC remain difficult predict, especially considering BrC from different sources and aging e.g. by photooxidation. To address this gap, we studied emissions of burning beech wood, straw, plastics, and cow dung in an oxidative flow reactor allowing to conduct photooxidation aging of fresh emissions. After photooxidation, volatile organic compounds and heavier molecules were oxidized and formed more oxidized products. Phenolic-like substances (PLS) and less oxygenated humic-like substances (LO-HULIS) dominated the fluorescence of primary organic aerosol with 88 ± 7 %. After photooxidation, the PLS chromophore significantly decreased from 45 ± 8 % to 10 ± 6 % and humic-like substance increased from 55 ± 8 % to 90 ± 6 %, especially highly-oxygenated humic-like substance (HO-HULIS). To futher confirm the chromophore variation process during the photooxidation, links between chromophore and chemical composition were inverstigated. The HULIS chromophores were unsaturated and contained high fractions with 5 % –10 % of nitrogen containing molecules. In contrast, the PLS chromophores had low oxidation states and contained lower fraction (2 %) of nitrogen containing molecules. After photooxidation, oxidation of PLS chromophores and volatile organic compounds in presence of NOx were converted into HULIS with the higher fraction of nitrogen containing and unsaturation chromophores. This study extends the current understanding of formation and photochemcial aging of brown carbon chromophorese e.g. PLS, HO-HULIS, and LO-HULIS from open fires including their molecular composition. This will facilitate modelling of brown carbon aerosol e.g. in trasport models.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Atmospheric Chemistry and Physics.

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Feng Jiang, Jun Zhang, David Bell, Kun Li, Nadine Borduas-Dedekind, Andre S. H. Prevot, Hongbiao Cui, Harald Saathoff, and Thomas Leisner

Status: open (until 30 Mar 2026)

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Feng Jiang, Jun Zhang, David Bell, Kun Li, Nadine Borduas-Dedekind, Andre S. H. Prevot, Hongbiao Cui, Harald Saathoff, and Thomas Leisner
Feng Jiang, Jun Zhang, David Bell, Kun Li, Nadine Borduas-Dedekind, Andre S. H. Prevot, Hongbiao Cui, Harald Saathoff, and Thomas Leisner
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Short summary
We studied chemical compositions and chromophores of brown carbon aerosol from combustion emission before and after photooxidation using an oxidative flow reactor. The chromophore and chemical composition of brown carbon were determined by excitation-emission spectroscopy and mass spectrometry. This work helps to get a better understanding of evolution process of the chromophores from primary combustion emissions during the real atmospheric transportation.
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