- 1Université Paris Cité and Univ Paris Est Creteil, CNRS, LISA, F-75013 Paris, France
- 2Univ Paris Est Creteil and Université Paris Cité, CNRS, LISA, F-94010 Créteil, France
- 3INSA Rouen Normandie, Univ. Rouen Normandie, CNRS, Normandie Univ., CORIA UMR 6614, 76000, Rouen France
- 4Institute of Atmospheric Sciences and Climate, National Research Council of Italy, Bologna, Italy
- 5Aix Marseille Univ., CNRS, CINaM, Marseille, France
- 6Univ. Grenoble Alpes, IRD, CNRS, INRAE, Grenoble INP, IGE, 38000 Grenoble, France
- 7now at: Laboratoire des Sciences du Climat et de l'Environnement, CEA–CNRS–UVSQ, IPSL, Université Paris-Saclay, 91191 Gif-sur-Yvette, France
- 8now at: World Meteorological Organization, Geneva, Switzerland
Black carbon (BC) soot aerosol, produced during the incomplete combustion of fossil fuels, biofuels, and biomasses, is a major light-absorbing species and a key climate forcer. Despite its importance, BC remains challenging to represent in models due to persistent uncertainties in its spectral optical properties. In particular, the formation of non-absorbing coatings on fractal BC soot is a ubiquitous atmospheric process that enhances absorption, yet the magnitude of this enhancement (Eabs) remains highly uncertain and poorly represented in current models.
In order to advance on this topic, a set of experiments were performed using the 4.2 m3 CESAM simulation chamber on BC-soot aerosol generated from a propane diffusion flame. Experiments were conceived to systematically investigate the impact of coating formation and further ageing on soot spectral optical properties. Two chemical systems inducing the formation of a coating by a second scattering aerosol phase produced via the photo-oxidation of SO2 and the ozonolysis of α-pinene were considered.
The resulting dataset quantifies the magnitude and variability of Eabs under varying conditions, highlighting its dependence on soot morphology, soot–coating structure, and particle-to-particle heterogeneous mixing state. We show that the relative importance of these factors evolves with the dynamics of coating formation and ageing. Importantly, the Eabs cannot be reliably predicted using a fixed value or simple core–shell optical models, as commonly assumed in climate simulations.
How to cite: Di Biagio, C., Heuser, J., Yon, J., Cazaunau, M., Bergé, A., Pangui, E., Zanatta, M., Renzi, L., Marinoni, A., Yu, C., Chevaillier, S., Ferry, D., Laj, P., Maillé, M., Formenti, P., Picquet-Varrault, B., and Doussin, J.-F.: Evolution of the spectral optical properties of black carbon soot due to coating and ageing: insights from simulation chamber experiments, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-11876, https://doi.org/10.5194/egusphere-egu26-11876, 2026.