The Mobility Diameter of Soot Determines Its Angular Light Scattering Distribution
GEORGIOS A. KELESIDIS, Patrizia Crepaldi, Martin Allemann, Aleksandar Duric, Sotiris Pratsinis,
ETH Zurich, Switzerland Abstract Number: 170
Working Group: Carbonaceous Aerosol
AbstractCharacterization of soot agglomerates often relies on the angular distribution of their light scattering cross-section,
C, that is based on the structure factor exponent,
Ds, and asymmetry parameter,
g, and depend on agglomerate mobility,
dm, and constituent primary particle,
dp, size distributions. Here, discrete element modeling (DEM) [1] is interfaced with discrete dipole approximation (DDA) [2] to determine
C in the range of
dm= 60 - 450 nm with mean
dp = 9 - 26 nm that are most prevalent in fire detection, air pollution and climate change. Increasing
dm reduces the effective density,
ρeff, and drastically increases
Ds and
g (by a factor of about 2-20), while increasing
dp or its geometric standard deviation,
σg,p, increases
ρeff but only slightly decreases
Ds (10 - 20 %). Thus, the angular light scattering distribution of soot is largely determined by its
dm. Currently, constant
Ds and
g (obtained for large agglomerates,
dm > 200 nm) are used in laser diagnostics and climate models. This overestimates the
dm for small soot agglomerates by up to a factor of four and underestimates their radiative forcing efficiency by 10 %. So, relations between
Ds,
g and
dm are derived here and validated with data from our premixed flames [3] and literature diffusion flame and field data. These relations cover the evolution of
Ds and
g with
dm and nicely converge to the constant
Ds for
dm > 200 nm. As such, they can facilitate the characterization of soot agglomerates by light scattering and help to quantify accurately the soot contribution to global warming.
References:[1] G.A. Kelesidis, E. Goudeli, S.E. Pratsinis, Morphology and mobility diameter of carbonaceous aerosols during agglomeration and surface growth, Carbon 121 (2017) 527-535, doi.org/10.1016/j.carbon.2017.06.004.
[2] G.A. Kelesidis, S.E. Pratsinis, Soot light absorption and refractive index during agglomeration and surface growth, Proc. Combust. Inst. 37 (2019) 1177-1184, doi.org/10.1016/j.proci.2018.08.025.
[3] G.A. Kelesidis, M.R. Kholghy, J. Zuercher, J. Robertz, M. Allemann, A. Duric, S.E. Pratsinis, Light scattering from nanoparticle agglomerates, Powder Technol. 365 (2020) 52-59, doi.org/10.1016/j.powtec.2019.02.003.