Abstract. The formation of black carbon fractal aggregates (BCFAs) from
combustion and subsequent ageing involves several stages resulting in
modifications of particle size, morphology, and composition over time. To
understand and quantify how each of these modifications influences the BC
radiative forcing, the optical properties of BCFAs are modelled. Owing to
the high computational time involved in numerical modelling, there are some
gaps in terms of data coverage and knowledge regarding how optical
properties of coated BCFAs vary over the range of different factors (size,
shape, and composition). This investigation bridged those gaps by following
a state-of-the-art description scheme of BCFAs based on morphology,
composition, and wavelength. The BCFA optical properties were investigated
as a function of the radius of the primary particle (ao), fractal dimension (Df), fraction of organics (forganics), wavelength (λ), and mobility diameter (Dmob). The optical properties are
calculated using the multiple-sphere T-matrix (MSTM) method. For the first
time, the modelled optical properties of BC are expressed in terms of
mobility diameter (Dmob), making the results more relevant and
relatable for ambient and laboratory BC studies. Amongst size, morphology,
and composition, all the optical properties showed the highest variability
with changing size. The cross sections varied from 0.0001 to
0.1 µm2 for BCFA Dmob ranging from 24 to 810 nm. It has been shown that MACBC and single-scattering albedo (SSA) are sensitive to morphology, especially for larger particles with Dmob > 100 nm. Therefore, while using
the simplified core–shell representation of BC in global models, the
influence of morphology on radiative forcing estimations might not be
adequately considered. The Ångström absorption exponent (AAE) varied from
1.06 up to 3.6 and increased with the fraction of organics
(forganics). Measurement results of AAE ≫ 1 are
often misinterpreted as biomass burning aerosol, it was observed that the AAE of purely black carbon particles can be ≫ 1 in
the case of larger BC particles. The values of the absorption enhancement
factor (Eλ) via coating were found to be between 1.01 and 3.28 in the
visible spectrum. The Eλ was derived from Mie calculations for
coated volume equivalent spheres and from MSTM for coated BCFAs. Mie-calculated enhancement factors were found to be larger by a factor of 1.1 to 1.5 than their corresponding values calculated from the MSTM method. It is shown that radiative forcings are highly sensitive to modifications in morphology and composition. The black carbon radiative forcing ΔFTOA (W m−2) decreases up to 61 % as the BCFA becomes more compact, indicating that global model calculations should account for changes in morphology. A decrease of more than 50 % in ΔFTOA was observed as the organic content of the particle increased up to 90 %. The changes in the ageing factors (composition and morphology) in tandem result in an overall decrease in the ΔFTOA. A parameterization scheme for optical properties of BC fractal aggregates was developed, which is applicable for modelling, ambient, and laboratory-based BC studies. The parameterization scheme for the cross sections (extinction, absorption, and scattering), single-scattering albedo (SSA), and asymmetry parameter (g) of pure and coated BCFAs as a function of Dmob were derived from tabulated
results of the MSTM method. Spanning an extensive parameter space, the
developed parameterization scheme showed promisingly high accuracy up to
98 % for the cross sections, 97 % for single-scattering albedos (SSAs), and 82 % for the asymmetry parameter (g).
Cross sections of electron collisions with noble gases atoms
