EGU23-14591, updated on 18 Jul 2023
https://doi.org/10.5194/egusphere-egu23-14591
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Evaluating the Uncertainties of the Global Atmospheric Sulphur Budget in a Multi-Model Framework

Christina Brodowsky1, Valentina Aquila2, Slimane Bekki3, Sandip Dhomse4, Anton Laakso5, Graham Mann4,6, Ulrike Niemeier7, Ilaria Quaglia8, Eugene Rozanov9, Takashi Sekiya10, Simone Tilmes11, Claudia Timmreck7, Pengfei Yu12, Yunqian Zhu13,14, and Timofei Sukhodolov9
Christina Brodowsky et al.
  • 1ETHZ, IAC, D-USYS, Zürich, Switzerland (brodowsc@student.ethz.ch)
  • 2American University, Washington DC, USA
  • 3Laboratoire Atmosphère Observations Spatiales, UVSQ, CNRS, Sorbonne University, Guyancourt, France
  • 4School of Earth and Environment, University of Leeds, Leeds, UK
  • 5Finnish Meteorological Institute, Atmospheric Research Centre of Eastern Finland, 70200 Kuopio, Finland
  • 6UK National Centre for Atmospheric Science, University of Leeds, Leeds, UK
  • 7Max Planck Institute for Meteorology, Bundesstr. 53, 20146 Hamburg, Germany
  • 8Department of Physical and Chemical Sciences, Università dell’Aquila, 67100 L’Aquila, Italy
  • 9Physikalisch-Meteorologisches Observatorium Davos and World Radiation Center, Davos, Switzerland
  • 10Japan Agency for Marine-Earth Science and Technology, Yokohama, Japan
  • 11Atmospheric Chemistry Observations and Modeling Laboratory, National Center for Atmospheric Research, Boulder, USA
  • 12Jinan University, Guangzhou, China
  • 13Laboratory for Atmospheric andSpace Physics, University of Colorado Boulder, Boulder, USA
  • 14University of Colorado Cooperative Institute for Research in Environmental Sciences (CIRES) at the NOAA Chemical Sciences Laboratory, Boulder, CO, USA

Sulphate aerosol in the stratosphere recently became an interactive part of many global climate models and its uncertainties are not yet well constrained. Stratospheric sulphate aerosol is modulated by natural emissions of several sulphur-containing species, including volcanic eruptions, as well as anthropogenic emissions. If not directly injected into the stratosphere by large volcanic eruptions, sulphate aerosols and their precursors are transported into the stratosphere via the tropical tropopause. While there have been some model intercomparison activity for the large volcanic eruptions, the background conditions of sulphur species and in particular the stratospheric aerosol layer have thus far not been addressed at all. Evaluating the background conditions in global models allow to identify modelling issues that are usually masked by larger perturbations such as volcanic eruptions, yet may still be of importance after such a perturbation. Some key factors causing differences between models include different microphysical schemes, chemical schemes, as well as transport and cross-tropopause fluxes. In this work, we use 8 models and available observational data to quantify the full background atmospheric sulphur cycle (burdens, fluxes, and their variability) and investigate its uncertainties within the framework of the Interactive Stratospheric Aerosol Model Intercomparison Project (ISA-MIP). We focus on stratospheric aerosol and its transport with the Brewer-Dobson-Circulation, as well as the influence of the polar vortices. We find significant inter-model variations in the background burden of the major sulphur species. Seasonal cycles agree well in the southern hemisphere, whereas the northern hemisphere shows more inter-model differences due to the individual representations of the northern polar vortex.

How to cite: Brodowsky, C., Aquila, V., Bekki, S., Dhomse, S., Laakso, A., Mann, G., Niemeier, U., Quaglia, I., Rozanov, E., Sekiya, T., Tilmes, S., Timmreck, C., Yu, P., Zhu, Y., and Sukhodolov, T.: Evaluating the Uncertainties of the Global Atmospheric Sulphur Budget in a Multi-Model Framework, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-14591, https://doi.org/10.5194/egusphere-egu23-14591, 2023.