A comparison of the physical properties of desert dust retrieved from the sunphotometer observation of major events in the Sahara, Sahel, and Arabian Peninsula

The objective of this work is to assess the variability of the size-distribution, real (n) and imaginary (k) parts of the refractive index, asymmetry parameter (g), and single scattering albedo (SSA) of desert dust events observed in the Sahara, Sahel, and Arabian Peninsula areas. For this we use the level-2 inversions of 14 AERONET sunphotometers representative of the area of study. In the dataset, the dust-dominated events are discriminated on the basis of their large optical depth and low (<0.3) Angstrom exponent (alpha) calculated between 440 nm and 870 nm. In all the volume size-distributions a coarse mode (CM) of particles is observed but a fine mode (FM) of particles with radii <0.2 mu m is also present. The volume fraction represented by the FM is lower (3%) during the most intense dust storms than during moderate ones (12%). The inter-site variability of the characteristics of the CMdominated situations is found to be non-significant and at 440, 675, 870, and 1020 nm a common set of values can be adopted for n (1.54 +/- 0.03, 153 +/- 0.02, 1.50 +/- 0.02, 1.48 +/- 0.02), k (0.0037 +/- 0.0007, 0.0012 +/- 0.0002, 0.0011 +/- 0.0002, 0.0012 +/- 0.0002), g (0.77 +/- 0.01, 0.74 +/- 0.01, 0.73 +/- 0.01, 0.74 +/- 0.01), and the SSA (0.90 +/- 0.02, 0.97 +/- 0.01, 0.98 +/- 0.01, 0.98 +/- 0.01). However; during the less intense dust-events the growing influence of the FM leads to regional differentiation of the dust properties and 2 main areas can be distinguished: 1) the relatively clean central Sahara/Sahel, and 2) the more polluted continuum constituted by the Mediterranean coast and the Arabian Peninsula. (c) 2015 Elsevier B.V. All rights reserved.