TY - JOUR
T1 - Influence of shape on the optical properties of hematite aerosol
AU - Veghte, Daniel P.
AU - Moore, Justin E.
AU - Jensen, Lasse
AU - Freedman, Miriam Arak
N1 - Funding Information:
We would like to thank the staff of the shared instrumentation facilities at the University Park campus of the Pennsylvania State University for the use of TEM and ball milling facilities along with helpful discussions. We thank the Material Characterization Lab for the use of the SWECO mill and the Microscopy and Cytometry Facility for use of the JEOL JEM 1200 EXII. We addi tionally acknowledge the staff of Research Computing and Cyberinfrastructure, a unit of ITS at Penn State, for the computational time and helpful discussions. D.P.V. and M. A.F. were supported by startup funding from the Pennsylvania State University. L.J. and J.E.M acknowledge the CAREER program of the National Science Foundation (grant CHE-0955689) for financial support. Data for this paper are available upon request from the corresponding author (Miriam Freedman, maf43@psu.edu). The program used to create roughened spheres and spheroids can be found at https://github. com/jensengrouppsu/ddscat-inputgen.
Publisher Copyright:
© 2015. American Geophysical Union. All Rights Reserved.
PY - 2015
Y1 - 2015
N2 - Mineral dust particles are the second highest emitted aerosol type by mass. Due to changes in particle size, composition, and shape that are caused by physical processes and reactive chemistry, optical properties vary during transport, contributing uncertainty in the calculation of radiative forcing. Hematite is the major absorbing species of mineral dust. In this study, we analyzed the extinction cross sections of nigrosin and hematite particles using cavity ring-down aerosol extinction spectroscopy (CRD-AES) and have measured particle shape and size distributions using transmission electron microscopy. Nigrosin was also used in this study as a spherical standard for absorbing particles. The size-selected nigrosin particles have a narrow size distribution, with extinction cross sections that are described by Mie theory. In contrast, the size distribution of size-selected hematite particles is more polydisperse. The extinction cross sections were modeled using Mie theory and the discrete dipole approximation (DDA). The DDA was used to model more complex shapes that account for the surface roughness and particle geometry. Of the four models used, Mie theory was the simplest to implement, but had significant error with a 26.1% difference from the CRD-AES results. By increasing the complexity of the models using the DDA, we determined that spheroids had a 14.7% difference, roughened spheres a 12.8% difference, and roughened spheroids a 11.2% difference from the experimental results. Using additional parameters that account for particle shape is necessary to model the optical properties of hematite particles and leads to improved extinction cross sections for modeling aerosol optical properties.
AB - Mineral dust particles are the second highest emitted aerosol type by mass. Due to changes in particle size, composition, and shape that are caused by physical processes and reactive chemistry, optical properties vary during transport, contributing uncertainty in the calculation of radiative forcing. Hematite is the major absorbing species of mineral dust. In this study, we analyzed the extinction cross sections of nigrosin and hematite particles using cavity ring-down aerosol extinction spectroscopy (CRD-AES) and have measured particle shape and size distributions using transmission electron microscopy. Nigrosin was also used in this study as a spherical standard for absorbing particles. The size-selected nigrosin particles have a narrow size distribution, with extinction cross sections that are described by Mie theory. In contrast, the size distribution of size-selected hematite particles is more polydisperse. The extinction cross sections were modeled using Mie theory and the discrete dipole approximation (DDA). The DDA was used to model more complex shapes that account for the surface roughness and particle geometry. Of the four models used, Mie theory was the simplest to implement, but had significant error with a 26.1% difference from the CRD-AES results. By increasing the complexity of the models using the DDA, we determined that spheroids had a 14.7% difference, roughened spheres a 12.8% difference, and roughened spheroids a 11.2% difference from the experimental results. Using additional parameters that account for particle shape is necessary to model the optical properties of hematite particles and leads to improved extinction cross sections for modeling aerosol optical properties.
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U2 - 10.1002/2015JD023160
DO - 10.1002/2015JD023160
M3 - Article
AN - SCOPUS:84939255553
VL - 120
SP - 7025
EP - 7039
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
SN - 2169-897X
IS - 14
ER -