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...

Full description

Bibliographic Details
Main Authors: A. J. A. Smith, R. G. Grainger
Format: Article
Language:English
Published: Copernicus Publications 2014-08-01
Series:Atmospheric Chemistry and Physics
Online Access:http://www.atmos-chem-phys.net/14/7825/2014/acp-14-7825-2014.pdf
id doaj-2c5f7048ab794cbdb99c56b2d95d8d15
record_format Article
spelling 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
_version_ 1725556865636499456