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GEOPHYSICAL RESEARCH LETTERS,
VOL. 29, NO. 10,
1398,
doi:10.1029/2002GL014947,
2002
Importance of shapes and compositions of wind-blown dust particles for remote sensing at solar wavelengths
Olga V. Kalashnikova
Program in Atmospheric and Oceanic Sciences,
University of Colorado,
Boulder,
CO,
USA
Irina N. Sokolik
Program in Atmospheric and Oceanic Sciences,
University of Colorado,
Boulder,
CO,
USA
Abstract
The quality of satellite aerosol retrievals depends critically upon the modeling accuracy of the aerosol optical properties.
The optical properties of mineral aerosols depend on particle morphology, mineralogy, and state of mixing. Here we investigate
how the realistic morphology and composition of dust particles affect the optical properties of dust mixtures by utilizing
microscopy data that recently become available of dust samples collected in the atmosphere. The data were used to reconstruct
the representative composition-shape-size (CSS) distributions and then the discrete dipole approximation technique was applied
to calculate the optical properties. We demonstrate that the presence of sharp-edge, angular-type particles results in various
differences in the scattering phase function, asymmetry parameter, optical depth and single scattering albedo compared to
those of the volume-equivalent spheres or ellipses. These differences are sufficiently large as to affect the retrievals of
aerosol optical properties from satellite and ground-based remote sensing observations at the solar wavelengths.
Published 23
May
2002.
Index Terms: 0305 Atmospheric Composition and Structure: Aerosols and particles (0345, 4801); 0360 Atmospheric Composition and Structure: Transmission and scattering of radiation; 6969 Radio Science: Remote sensing.
Read Full Article (file size: 213618 bytes) Cited by
Citation: Kalashnikova, O. V., and I. N. Sokolik
(2002),
Importance of shapes and compositions of wind-blown dust particles for remote sensing at solar wavelengths,
Geophys. Res. Lett.,
29(10),
1398,
doi:10.1029/2002GL014947.
Copyright 2002 by the American Geophysical Union.
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