A019-04
Regional Variability of Dust Single Scattering Albedo due to Mineral Composition.

Monday, 7 December 2020: 10:42
Virtual
Vincenzo Obiso1,2, Ron L Miller3, Maria Gonçalves4,5, Carlos Pérez García-Pando4,6 and Gregory L Schuster7, (1)NASA/GISS, New York, United States, (2)Columbia University CCSR, New York, NY, United States, (3)NASA/GISS, New York, NY, United States, (4)Barcelona Supercomputing Center (BSC), Barcelona, Spain, (5)Technical University of Catalonia, Barcelona, Spain, (6)ICREA, Catalan Institution for Research and Advanced Studies, Barcelona, Spain, (7)NASA Langley Research Center, Hampton, VA, United States
Recorded Presentation
Abstract:
Nearly all Earth System Models (ESMs) assume globally homogeneous dust aerosols, neglecting regional variations of the imaginary refractive index (IRI) due to varying mineral composition. This has led to a range of single scattering albedo (SSA) and direct radiative forcing (DRF) estimates, as models assign global properties using dust measurements from different regions. We use model and observational data to assess to what extent regionally varying mineral composition affects visible-band SSA and short-wave DRF of dust.

We run global simulations with NASA GISS ModelE2.1, using optical properties for minerals based on laboratory-derived empirical relationships between dust IRI at visible wavelengths and the mineral content of iron oxides. When allowing mineral variations instead of homogeneous dust, we find regional differences in dust SSA up to ~0.06 and consequent variations in DRF up to ~6 and ~5 W/m2, at surface and top-of-atmosphere respectively. We compare model SSA with AERONET inversion data (Version 3.0, Level 2), filtered by aerosol size and optical properties to identify pure dust scenes. To investigate possible contamination by biomass burning aerosols, we use the dataset of Schuster et al. (2016, doi:10.5194/acp-16-1565-2016), who separately calculated the contribution of iron oxides and carbonaceous species to AERONET extinction and absorption optical depths. Our results show that: (1) the range of observed SSA (even without carbonaceous species) is larger than that resulting from homogeneous dust; (2) residual amounts of fine mode black and brown carbon may affect AERONET SSA even in seasons with limited biomass burning; (3) model SSA from our mineral scheme exceeds the AERONET range, possibly due also to an uncertain treatment of goethite.

In summary, homogeneous dust cannot explain the variability of observed SSA, so regionally varying optical properties based on mineral content are necessary. Higher accuracy in soil mineralogy maps is needed to better reproduce SSA variations at regional scales. Also, distinct soil maps for hematite and goethite are required, given the high sensitivity of model SSA to their extreme optical properties.

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