EGU21-10848, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-10848
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Variability in modelled airborne dust mineralogy derived from global soil composition uncertainties

María Gonçalves Ageitos1,2, Matt Dawson2,3, Vincenzo Obiso4, Martina Klose5, Ron Miller4, Oriol Jorba2, and Carlos Pérez García-Pando2,6
María Gonçalves Ageitos et al.
  • 1Technical University of Catalonia (UPC), Projects and construction engineering department, Terrassa, Spain.
  • 2Barcelona Supercomputing Center (BSC), Barcelona, Spain.
  • 3National Center for Atmospheric Research (NCAR), Boulder, Colorado, USA.
  • 4NASA Goddard Institute for Space Studies (NASA-GISS), New York, USA.
  • 5Karlsruhe Institute of Technology (KIT), Karlsruhe, Germany.
  • 6Catalan Institution for Research and Advanced Studies (ICREA), Barcelona, Spain.

Dust aerosols consist on a variety of minerals with different physic and chemical properties. As such, they interact with short and long wave radiation, potentially form clouds, act as nutrients modulating biogeochemical cycles, or influence atmospheric chemistry, differently. Most current state-of-the-art Earth System Models (ESMs) neglect the complexity in dust composition, mainly due to computational constraints, but also to the existing uncertainties in the size resolved composition of parent soils, the resulting distribution of minerals in airborne dust, and the scarcity of observations to constrain them.

Within this work, we assess the variability of global dust composition due to uncertainties in the characterization of the parent soil mineralogy. To that end, we consider two available global soil mineralogy atlases, developed by Claquin et al. (1999) –C1999- and Journet et al. (2014) –J2014-, which represent respectively 8 and 12 relevant minerals for climate (namely: illite, smectite/montmorillonite, kaolinite, calcite, gypsum, hematite, quartz, and feldspars in C1999, and those plus chlorite, vermiculite, goethite, and mica in J2014). Thanks to a recently developed feature of the MONARCH atmospheric-chemistry model, we are able to explicitly resolve the minerals’ atmospheric cycle. Therefore, we define two global experiments to assess changes on airborne dust composition attributed to the soil mineralogy assumptions and provide a measure of their variability. We also perform a preliminary evaluation of the global mineralogy results against available observations of mineral fractions in surface dust concentration.

Our results will inform the climate modelling community about the potential variability in dust composition, an aspect that will gain relevance as ESMs continue growing in complexity and new processes to better characterize aerosols’ forcing or biogeochemical cycles are added. Further observational constraints, such as those that will derive from the EMIT NASA mission on soil composition or the FRAGMENT experimental campaigns on airborne dust characterization, will be key in the near future to improve our understanding of the impact of dust mineralogy on fundamental climate features.

How to cite: Gonçalves Ageitos, M., Dawson, M., Obiso, V., Klose, M., Miller, R., Jorba, O., and Pérez García-Pando, C.: Variability in modelled airborne dust mineralogy derived from global soil composition uncertainties, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-10848, https://doi.org/10.5194/egusphere-egu21-10848, 2021.

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