Effects of mass ratio heterogeneity and coating-related optical characteristics on the light absorption enhancement of black carbon-containing particles
Abstract. Black carbon (BC) is a strong climate forcer, but considerable uncertainty remains in estimating its radiative impact, largely due to persistent gaps between observed and modeled light absorption enhancement (Eabs). In this study, we employed a Centrifugal Particle Mass Analyzer and Single Particle Soot Photometer tandem system to characterize mass ratio (MR, coating-to-BC) of BC-containing particles in Hangzhou, China. Observations across a field campaign revealed low, medium, and high Eabs values under varying atmospheric conditions. The uniform core-shell Mie model overestimated Eabs, particularly during clean periods (low Eabs). To address this, we developed an observationally constrained parameterization for transition-state particles based on MR-dependent optical transitions behaviors. This approach effectively reconciles modeled and measured Eabs across varying pollution conditions. It also emphasizes the importance of incorporating MR heterogeneity and transition-state optical behavior to improve BC light absorption estimates and reduce uncertainties in assessing radiative effects.
Authors
- Zhen Xu (ORCID: https://orcid.org/0000-0003-4269-4226)
- Jinmei Ding
- Yao Song
- Bin-Ye Xu
- Wei Jin (ORCID: https://orcid.org/0000-0003-2671-1989)
- Shutao Xu (ORCID: https://orcid.org/0000-0003-4722-8371)
- Zhibin Wang (ORCID: https://orcid.org/0000-0001-7662-6032)
- Xudong Tian (ORCID: https://orcid.org/0000-0002-3394-4986)
- Xiao-Yuan Wang
- Fei Zhang
- Xiang-Yu Pei
Institutions
- State Key Laboratory of Pollution Control and Resource Reuse (CN)
- Zhejiang Lab (CN)
- Zhejiang Environmental Monitoring Center (CN)
Publication Details
- Journal
- Atmospheric chemistry and physics
- Published
- 2026-02-26
- DOI
- https://doi.org/10.5194/acp-26-2881-2026
- Primary Topic
- Atmospheric chemistry and aerosols
- Type
- article
- Field-Weighted Citation Impact
- 0.00