Simplifying the calculation of light scattering properties for black carbon fractal aggregates
Black carbon fractal aggregates have complicated shapes that make the calculation of their optical properties particularly computationally expensive. Here, a method is presented to estimate fractal aggregate light scattering properties by optimising simplified models to full...
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Copernicus Publications
2014-08-01
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Series: | Atmospheric Chemistry and Physics |
Online Access: | http://www.atmos-chem-phys.net/14/7825/2014/acp-14-7825-2014.pdf |
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doaj-2c5f7048ab794cbdb99c56b2d95d8d152020-11-24T23:25:34ZengCopernicus PublicationsAtmospheric Chemistry and Physics1680-73161680-73242014-08-0114157825783610.5194/acp-14-7825-2014Simplifying the calculation of light scattering properties for black carbon fractal aggregatesA. J. A. Smith0R. G. Grainger1Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Oxford, OX1 3PU, UKAtmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Oxford, OX1 3PU, UKBlack carbon fractal aggregates have complicated shapes that make the calculation of their optical properties particularly computationally expensive. Here, a method is presented to estimate fractal aggregate light scattering properties by optimising simplified models to full light scattering calculations. It is found that there are no possible spherical models (at any size or refractive index) that well represent the light scattering in the visible or near-thermal infrared. As such, parameterisations of the light scattering as a function of the number of aggregate particles is presented as the most pragmatic choice for modelling distributions of black carbon when the large computational overheads of rigorous scattering calculations cannot be justified. This parameterisation can be analytically integrated to provide light scattering properties for lognormal distributions of black carbon fractal aggregates and return extinction cross sections with 0.1% accuracy for typical black carbon size distributions. Scattering cross sections and the asymmetry parameter can be obtained to within 3%.http://www.atmos-chem-phys.net/14/7825/2014/acp-14-7825-2014.pdf |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
A. J. A. Smith R. G. Grainger |
spellingShingle |
A. J. A. Smith R. G. Grainger Simplifying the calculation of light scattering properties for black carbon fractal aggregates Atmospheric Chemistry and Physics |
author_facet |
A. J. A. Smith R. G. Grainger |
author_sort |
A. J. A. Smith |
title |
Simplifying the calculation of light scattering properties for black carbon fractal aggregates |
title_short |
Simplifying the calculation of light scattering properties for black carbon fractal aggregates |
title_full |
Simplifying the calculation of light scattering properties for black carbon fractal aggregates |
title_fullStr |
Simplifying the calculation of light scattering properties for black carbon fractal aggregates |
title_full_unstemmed |
Simplifying the calculation of light scattering properties for black carbon fractal aggregates |
title_sort |
simplifying the calculation of light scattering properties for black carbon fractal aggregates |
publisher |
Copernicus Publications |
series |
Atmospheric Chemistry and Physics |
issn |
1680-7316 1680-7324 |
publishDate |
2014-08-01 |
description |
Black carbon fractal aggregates have complicated shapes that make the
calculation of their optical properties particularly computationally
expensive. Here, a method is presented to estimate fractal aggregate
light scattering properties by optimising simplified models to full
light scattering calculations. It is found that there are no possible
spherical models (at any size or refractive index) that well represent
the light scattering in the visible or near-thermal infrared. As
such, parameterisations of the light scattering as a function of the
number of aggregate particles is presented as the most pragmatic
choice for modelling distributions of black carbon when the large
computational overheads of rigorous scattering calculations cannot be
justified. This parameterisation can be analytically integrated to
provide light scattering properties for lognormal distributions of
black carbon fractal aggregates and return extinction cross sections
with 0.1% accuracy for typical black carbon size distributions.
Scattering cross sections and the asymmetry parameter can be obtained
to within 3%. |
url |
http://www.atmos-chem-phys.net/14/7825/2014/acp-14-7825-2014.pdf |
work_keys_str_mv |
AT ajasmith simplifyingthecalculationoflightscatteringpropertiesforblackcarbonfractalaggregates AT rggrainger simplifyingthecalculationoflightscatteringpropertiesforblackcarbonfractalaggregates |
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