Abstract. Black carbon (BC) aerosol is the strongest
sunlight-absorbing aerosol, and its optical properties are fundamental to
radiative forcing estimations and retrievals of its size and concentration.
BC particles exist as aggregate structures with small monomers and are widely
represented by the idealized fractal aggregate model. In reality, BC
particles possess complex and nonideal minor structures besides the overall
aggregate structure, altering their optical properties in unforeseen ways.
This study introduces the parameter “volume variation” to quantify and
unify different minor structures and develops an empirical relationship to
account for their effects on BC optical properties from those of ideal
aggregates. Minor structures considered are as follows: the polydispersity of
monomer size, the irregularity and coating of the individual monomer, and
necking and overlapping among monomers. The discrete dipole approximation is
used to calculate the optical properties of aggregates with these minor
structures. Minor structures result in scattering cross-section enhancement slightly more than that
of absorption cross section, and their effects on the angle-dependent phase matrix as well as asymmetry factor are negligible.
As expected, the effects become weaker with the increase in wavelength. Our results suggest that a correction ratio of 1.05 is
necessary to account for the mass or volume normalized absorption and
scattering of nonideal aggregates in comparison to ideal ones, which also
applies to aggregates with multiple minor structures. In other words, the
effects of minor structures are mainly contributed by their influence on
particle volume/mass that cannot be ignored, and a relative difference of
approximately 5 % is noticed after removing the volume effects. Thus,
accurate knowledge and evaluation of BC volume/mass are more important than
those of the minor structures themselves. Most importantly, the simulations
of optical properties of nonideal aggregates are greatly simplified by
applying the empirical relationship because they can be directly obtained
from those of the corresponding ideal aggregates, a volume/mass difference
parameter, and the correction factor, i.e., 1.05, not the detailed minor
structure information. We expect this convenient treatment to find wide
applications for the accounting for the effects of nonideal minor structures
on BC optical properties.