EGU25-10154, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-10154
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Wednesday, 30 Apr, 10:45–12:30 (CEST), Display time Wednesday, 30 Apr, 08:30–12:30
 
Hall X5, X5.32
Advancements in the incorporation of complex soot morphology within atmospheric sciences
Baseerat Romshoo1, Thomas Müller1, Sascha Pfeifer1, Jorge Saturno2, Andreas Nowak2, Yifan Yang1, Ajit Ahlawat3, Gazala Habib4, Arun S. Babu1, Anil Madariya6, Andrea Cuesta1, Shravan Deshmukh1, Jaikrishna Patil5, Tobias Michels5, Marius Kloft5, and Mira Pöhlker1
Baseerat Romshoo et al.
  • 1Leibniz Institute for Tropospheric Studies(TROPOS), Experimental aerosol and cloud microphysics, Leipzig, Germany (baseerat@tropos.de)
  • 2Physikalisch-Technische Bundesanstalt, Braunschweig, Germany
  • 3Delft University of Technology, Delft, Netherlands
  • 4Indian Institute of Technology, Delhi, India
  • 5University of Kaiserslautern-Landau, Germany
  • 6Univ Paris Est Creteil and Université Paris Cité, CNRS, LISA, F–94010, Créteil, France

Soot, also commonly known as black carbon (BC) aerosol, is an important short-lived climate forcer. Although global anthropogenic BC emissions from fossil fuel combustion are expected to decrease, BC remains a significant concern in air pollution hotspots in Asia and Africa. Estimates of the global black carbon direct radiative forcing are still subject to considerable uncertainties, ranging from 0.20 to 0.42 Wm⁻². To reduce these uncertainties, it is crucial to improve the representation of the complex soot morphology in simulations of their optical properties and global models. We have investigated various aspects of the optical properties of morphologically complex soot particles, including field and laboratory measurements, and optical simulations of BC as ‘realistic’ fractal aggregates. Investigations conducted in Delhi, a highly polluted urban environment in Asia, confirmed that fractal morphology is important in reducing the overestimation of aerosol light absorption by commonly used light simulation models by 10 to 80%.

To address the computationally expensive nature of fractal simulations, we propose a new metric known as the morphology index (MI). Additionally, to reduce the computational burden of optical simulations of fractal BC particles, we developed a fast and accurate machine learning-based tool for predicting the optical properties of BC fractal aggregates. We have highlighted the importance of the lack of representation of complex soot particles in global models, and offer methods to facilitate their integration into the atmospheric science community.

How to cite: Romshoo, B., Müller, T., Pfeifer, S., Saturno, J., Nowak, A., Yang, Y., Ahlawat, A., Habib, G., Babu, A. S., Madariya, A., Cuesta, A., Deshmukh, S., Patil, J., Michels, T., Kloft, M., and Pöhlker, M.: Advancements in the incorporation of complex soot morphology within atmospheric sciences, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10154, https://doi.org/10.5194/egusphere-egu25-10154, 2025.