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Published February 25, 2020 | Supplemental Material + Published
Journal Article Open

An unexpected catalyst dominates formation and radiative forcing of regional haze

Abstract

Although regional haze adversely affects human health and possibly counteracts global warming from increasing levels of greenhouse gases, the formation and radiative forcing of regional haze on climate remain uncertain. By combining field measurements, laboratory experiments, and model simulations, we show a remarkable role of black carbon (BC) particles in driving the formation and trend of regional haze. Our analysis of long-term measurements in China indicates declined frequency of heavy haze events along with significantly reduced SO₂, but negligibly alleviated haze severity. Also, no improving trend exists for moderate haze events. Our complementary laboratory experiments demonstrate that SO₂ oxidation is efficiently catalyzed on BC particles in the presence of NO₂ and NH₃, even at low SO₂ and intermediate relative humidity levels. Inclusion of the BC reaction accounts for about 90–100% and 30–50% of the sulfate production during moderate and heavy haze events, respectively. Calculations using a radiative transfer model and accounting for the sulfate formation on BC yield an invariant radiative forcing of nearly zero W m⁻² on the top of the atmosphere throughout haze development, indicating small net climatic cooling/warming but large surface cooling, atmospheric heating, and air stagnation. This BC catalytic chemistry facilitates haze development and explains the observed trends of regional haze in China. Our results imply that reduction of SO₂ alone is insufficient in mitigating haze occurrence and highlight the necessity of accurate representation of the BC chemical and radiative properties in predicting the formation and assessing the impacts of regional haze.

Additional Information

© 2020 the Author(s). Published by PNAS. This open access article is distributed under Creative Commons Attribution-NonCommercial-NoDerivatives License 4.0 (CC BY-NC-ND). Contributed by Mario J. Molina, December 24, 2019 (sent for review November 7, 2019; reviewed by Russell R. Dickerson and Manish Shrivastava). PNAS first published February 10, 2020. This work was supported by the National Natural Science Foundation of China (Grants 41675141 and 41975174), the National Basic Research Program of China (Grant 2017YFC1501702), and the Robert A. Welch Foundation (Grant A-1417). We thank Zipeng Dong for assistance with the radiative forcing data analysis. Data and Materials Availability: All data needed to evaluate the conclusions in the paper are present in the paper and/or the SI Appendix. Additional data related to this paper may be requested from the authors. Author contributions: F.Z. and R.Z. designed research; F.Z., Yuan Wang, J.P., L.C., Y.S., and R.Z. performed research; X.G., X.Z., G.Z., Y.P., Yuesi Wang, M.H., and M.J.M. contributed new reagents/analytic tools; F.Z., J.P., Y.S., L.D., Y.L., J.Z., C.L., Y.J., G.W., and M.J.M. analyzed data; and F.Z., A.L.Z., and R.Z. wrote the paper. Reviewers: R.R.D., University of Maryland; and M.S., Pacific Northwest National Laboratory. The authors declare no competing interest. This article contains supporting information online at https://www.pnas.org/lookup/suppl/doi:10.1073/pnas.1919343117/-/DCSupplemental.

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Additional details

Created:
August 22, 2023
Modified:
October 19, 2023