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- Editorial & advisory board
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**Research article**
05 Jun 2019

**Research article** | 05 Jun 2019

Optically effective complex refractive index

^{1}Key Laboratory of Meteorological Disaster, Ministry of Education (KLME)/Collaborative Innovation Center on Forecast and Evaluation of Meteorological Disasters (CIC-FEMD)/Joint International Research Laboratory of Climate and Environment Change (ILCEC)/Earth System Modeling Center (ESMC)/Key Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing University of Information Science & Technology, Nanjing, 210044, China^{2}School of Atmospheric Physics, Nanjing University of Information Science & Technology, Nanjing, 210044, China

^{1}Key Laboratory of Meteorological Disaster, Ministry of Education (KLME)/Collaborative Innovation Center on Forecast and Evaluation of Meteorological Disasters (CIC-FEMD)/Joint International Research Laboratory of Climate and Environment Change (ILCEC)/Earth System Modeling Center (ESMC)/Key Laboratory for Aerosol-Cloud-Precipitation of China Meteorological Administration, Nanjing University of Information Science & Technology, Nanjing, 210044, China^{2}School of Atmospheric Physics, Nanjing University of Information Science & Technology, Nanjing, 210044, China

Abstract

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Aerosol complex refractive index (ACRI) is an important microphysical
parameter used for the studies of modeling their radiative effects. With
considerable uncertainties related to retrieval based on observations, a
numerical study is a powerful method, if not the only one, to provide a
better and more accurate understanding of retrieved optically effective ACRIs
of aged black carbon (BC) particles. Numerical investigations of the
optically effective ACRIs of polydisperse coated BC aggregates retrieved from
their accurate scattering and absorption properties, which are calculated by
the multiple-sphere T-matrix method (MSTM), without overall particle shape
variations during retrieval, are carried out. The aim of this study is to
evaluate the effects of aerosol microphysics, including shell∕core
ratio *D*_{p}∕*D*_{c}, BC geometry, BC position inside coating,
and size distribution, on retrieved optically effective ACRIs of coated BC
particles. At odds with expectations, retrieved optically effective ACRIs of
coated BC particles in coarse mode are not merely impacted by their chemical
compositions and shell∕core ratio, being highly complicated functions
of particle microphysics. However, in accumulation mode, the coated BC
optically effective ACRI is dominantly influenced by particle chemical
compositions and the shell∕core ratio. The popular volume-weighted
average (VWA) method and effective medium theory (EMT) provide acceptable
ACRI results for coated BC in accumulation mode, and the resulting
uncertainties in particle scattering and absorption are both less than
approximately 10 %. For coarse coated BC, the VWA and EMT, nevertheless,
produce dramatically higher imaginary parts than those of optically effective
ACRIs, significantly overestimating particle absorption by a factor of nearly
2 for heavily coated BC with a large BC fractal dimension or BC close to the
coating boundary. Using the VWA could introduce significant overestimation in
aged BC absorption analysis studies, and this may be one of the reasons why
modeled aerosol optical depth is 20 % larger than observed, since it is
widely employed in the state-of-the-art aerosol–climate models. We propose a
simple new ACRI parameterization for fully coated BC with
${D}_{\mathrm{p}}/{D}_{\mathrm{c}}\ge \mathrm{2.0}$ in coarse mode, which can serve as a
guide for the improvement of ACRIs of heavily coated BC, and its scattering
and absorption errors are reduced by a factor of nearly 2 compared to the
VWA. Our study indicates that a reliable estimate of the radiative effects of
aged BC particles in coarse mode would require accounting for the optically
effective ACRI, rather than the ACRI given by the VWA, in aerosol–climate
models.

How to cite

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How to cite.

Zhang, X., Mao, M., and Yin, Y.: Optically effective complex refractive index of coated black carbon aerosols: from numerical aspects, Atmos. Chem. Phys., 19, 7507-7518, https://doi.org/10.5194/acp-19-7507-2019, 2019.

1 Introduction

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The largest uncertainty in estimates of the effects of atmospheric aerosols on climate stems from uncertainties in the determination of their microphysical properties, which in turn determines their optical properties. As one of the most significant microphysical properties, aerosol complex refractive index (ACRI) should be known for modeling their radiative effects, and the magnitude of radiative forcing is very sensitive to the ACRI, especially the imaginary part (Raut and Chazette, 2008a). The ACRI is determined by particle chemical composition governing its inherent scattering and absorption properties.

Black carbon (BC), emitted from incomplete fossil fuel combustion and biomass burning, can be coated with secondary aerosol species (e.g., organics and sulfate) through the aging process, being one of the largest uncertainties in estimating aerosol radiative forcing due to their complicated geometry and mixing state (Ramanathan and Carmichael, 2008; Myhre, 2009; Bond et al., 2013; Zhang et al., 2015). As a strong absorptive aerosol, pure BC particles have a large ACRI, whereas our understanding of the ACRI of aged BC is still limited because of its internal mixing with weakly absorptive coatings (Shiraiwa et al., 2010; Cui et al., 2016; Peng et al., 2016). The ACRIs of BC internal mixtures, named effective ACRIs, are normally obtained based on the volume-weighted average (VWA) method and effective medium theory (EMT), and the choice of both approaches is driven by high dependency of ACRIs on particle chemical compositions (e.g., Kandler et al., 2009). The state-of-the-art aerosol–climate models employ the VWA method extensively, approximating the effective ACRIs of internally and externally mixed aerosol ensembles at each mode for calculating their optical and radiative properties (e.g., Stier et al., 2005; Kim at al., 2008; Zhang et al., 2012). Nonetheless, the performances of the VWA and EMT are open questions, as several studies have questioned the validity of both approximations in some questions (e.g., Voshchinnikov et al., 2007).

The estimates of the ACRI of coated BC can also be made from observed optical properties, and the ACRI is inferred by obtaining a best fit to numerical simulations with Mie theory assuming a spherical particle shape, which is called optically effective ACRI. For instance, the optically effective ACRIs are retrieved based on simultaneous measurements of surface aerosol scattering and absorption coefficients, as well as size distributions (Abo Riziq et al., 2007; Schkolnik et al., 2007; Mack et al., 2010; Stock et al., 2011). Meanwhile, the airborne in situ measurements of particle optical properties from a particle soot absorption photometer (PSAP), spectral optical absorption photometer (SOAP), sunphotometer, or lidar, combined with a Mie theory-based data analysis scheme, are also applied for the retrieval of optically effective ACRIs (Raut and Chazette, 2008a, b; Petzold et al., 2009; Muller et al., 2009). Muller et al. (2010) even compare retrieved optically effective ACRIs from different techniques and reveal only partly a reasonable agreement with significant differences for the spectra of imaginary part remaining, indicating uncertainties during retrieval. The uncertainties may be that those retrieval methods are based on unrealistic spherical shape assumption, inaccurate numerical modeling, or without considering the errors in aerosol optical measurements, and then sizeable errors in retrieved optically effective ACRIs are posed. Moreover, these uncertainties significantly limit our ability to understand the relationships between the optically effective ACRI and aerosol other microphysical properties, and furthermore to improve radiation simulations in aerosol–climate models. Therefore, a systematic theoretical investigation on optically effective ACRIs of internally mixed particles retrieved from exactly calculated optical properties without particle shapes changed is a must, which is generally missing, and will benefit our understanding of these relationships. For coated BC particles with several chemical compositions, their optically effective ACRIs are not only affected by their compositions, but are also possibly impacted by their other microphysics. However, the effects of coated BC microphysics on their optically effective ACRIs are still under discussion and need more investigation.

Here, numerical investigations of the optically effective ACRIs of
polydisperse coated BC aggregates as examples are systematically presented
based on our current understanding, and the optically effective ACRI
influences are decomposed into that due to particle microphysical
properties, including shell∕core ratio, BC fractal dimension, BC position
inside coating, and size distribution. An exact multiple-sphere *T*-matrix
method (MSTM) is employed to numerically calculate the absorption properties
of coated BC aggregates while the Mie method is applied for the retrieval of
optically effective ACRI. The objective is to evaluate the effects of
coating microphysics on the optically effective ACRIs of aged BC particles,
which hopefully benefits our understanding of the mechanism responsible for
the model–observation discrepancies and refining estimates of aerosol
radiative forcing. The performances of the VWA and EMT approximations are
also studied for comparison.

2 Methodology

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Freshly emitted BC particles often exist as loose cluster-like aggregates with hundreds or even thousands of small spherical monomers (e.g., Li et al., 2016), and the concept of fractal aggregate has shown great success and wide applications in representing realistic BC geometries (e.g., Sorensen, 2001). The fractal aggregate can be mathematically described by the well-known statistic scaling rule following

$$\begin{array}{}\text{(1)}& N={k}_{\mathrm{0}}{\left({\displaystyle \frac{{R}_{\mathrm{g}}}{a}}\right)}^{{D}_{\mathrm{f}}},\end{array}$$

$$\begin{array}{}\text{(2)}& {R}_{\mathrm{g}}=\sqrt{{\displaystyle \frac{\mathrm{1}}{N}}\sum _{i=\mathrm{1}}^{N}{r}_{i}^{\mathrm{2}}},\end{array}$$

where *N* is the monomer number in an aggregate, *a* the mean monomer
radius, *k*_{0} the fractal prefactor, *D*_{f} the fractal
dimension, and *R*_{g} the gyration radius.

After being emitted into the atmosphere, BC aggregates tend be coated by
other materials, such as sulfate and organics (e.g., Schwarz et al.,
2008a; Tritscher et al., 2011), through the aging
process, and their chain-like structures tend to collapse into more compact
clusters (Zhang et al., 2008; Coz and Leck, 2011). The aged BC particles can
have BC *D*_{f} of almost 3, while the fresh BC aggregates generally
show lacy structures with *D*_{f} less than 2 (Liu et al., 2008).
While the fractal aggregates have been successfully employed to model the
geometries of BC particles (e.g., Dlugach and Mishchenko, 2015; Mishchenko et
al., 2016), their coating geometries are generally complicated in ambient
air. Some observations of individually aged BC particles actually show
spherical coating geometry (e.g., Schnaiter et al., 2005; Alexander et al., 2008; Zhang et al., 2008; Wu et al., 2016),
while others depict complex irregular geometries. Meanwhile, it is found that
the simple spherical coatings on BC particles have similar effects on
scattering and absorption properties to those with more complicated coating
structures (e.g., Dong et al., 2015; F. Liu et al., 2015; C. Liu et al.,
2017). To avoid the influence of overall particle shape variations on
retrieval results of optically effective ACRIs and to use the fast Mie theory
for retrieval, this study therefore considers an aggregate as the BC core,
and a spherical coating is added as the coating material, which is assumed to
be the weakly absorbing sulfate, following the numerical model developed by
Zhang et al. (2017). The sketch map of the BC aggregates coated by sulfate
with an overall spherical shape is shown in Fig. 1.

For this inhomogeneous internally mixed particle, the BC aggregates are
generated based on a tunable particle-cluster aggregation algorithm from
Skorupski et al. (2014). The *k*_{f} of BC is assumed to be 1.2
based on Sorensen (2001). The *D*_{f} can characterize the shape of
BC aggregates reasonably well, and its variation reflects BC aging processes
(Wang et al., 2017). The radius *a* of BC aggregate monomers is observed to
vary over a range of about 10–25 nm (Bond and Bergstrom, 2006), while the
monomer number *N* can alter up to approximately 800 (Adachi and Buseck,
2008). Since the monomer size has a rather weak effect on BC scattering and
absorption as *D*_{f} is fixed (Liu and Mishchenko, 2007; He et al.,
2015), we consider two *N* values of 200 and 800 as examples of accumulation
and coarse particles, respectively, and compare three *D*_{f} values
of 2.6, 2.8, and 2.98 for aged BC aggregates. After BC geometry is defined,
the shell∕core ratio *D*_{p}∕*D*_{c} of coated BC is
assumed to be in the range of 1.1–2.7 on the basis of the SP2 measurements
in London (D. Liu et al., 2015) and Beijing (Zhang et al., 2016). It should
be noted that some small *D*_{p}∕*D*_{c} values might not be
used, because we only study the cases for BC aggregates fully coated by
sulfate. An incident wavelength of 550 nm is considered in this study, and
related refractive indices of BC and sulfate are assumed to be 1.85−0.71*i*
(Bond and Bergstrom, 2006) and $\mathrm{1.52}-\mathrm{5.0}\times {\mathrm{10}}^{-\mathrm{4}}i$ (Aouizerats et al.,
2010), respectively. With the internally mixed coated BC model defined, which
depicts quite realistic geometries, its random-orientation scattering and
absorption properties are exactly calculated with the robust multiple-sphere
*T*-matrix method (Mackowski, 2014).

For ambient atmospheric applications, it is meaningful to consider bulk
particle optical properties averaged over a certain size distribution. This
study explores an ensemble of BC aggregates with different sizes but the same
sulfate coating fraction (i.e., same *D*_{p}∕*D*_{c}), and a
lognormal size distribution is assumed with the form of

$$\begin{array}{}\text{(3)}& n\left(r\right)={\displaystyle \frac{\mathrm{1}}{\sqrt{\mathrm{2}\mathit{\pi}}r\mathrm{ln}\left({\mathit{\sigma}}_{\mathrm{g}}\right)}}\mathrm{exp}\left[-{\left({\displaystyle \frac{\mathrm{ln}\left(r\right)-\mathrm{ln}\left({r}_{\mathrm{g}}\right)}{\sqrt{\mathrm{2}}\mathrm{ln}\left({\mathit{\sigma}}_{\mathrm{g}}\right)}}\right)}^{\mathrm{2}}\right],\end{array}$$

where *σ*_{g} is the geometric standard deviation and
*r*_{g} is the geometric mean radius (e.g., Yurkin and Hoekstra,
2007; Schwarz et al., 2008b). As particles in
accumulation and coarse modes contribute dominated light scattering and
absorption, we only consider coated BC in both modes. For the accumulation
mode, the radius range is set as 0.05–0.5 µm in steps of
0.005 µm, while the coarse radius range is assumed to be
0.5–2.5 µm in steps of 0.05 µm as ambient aerosols with
sizes larger than 5 µm are few (Zhang et al., 2014, 2018; Zhang and
Mao, 2015). Note that the exact sizes of BC aggregates are known based on
these coated BC sizes and shell∕core ratios. To better understand the
behavior at different particle size modes, size distributions in accumulation
and coarse modes are utilized separately, which are similar to those applied
in the aerosol–climate models (Zhang et al., 2012). In this study, we
consider the size distributions of coated BC aggregates (i.e., BC–sulfate
internal mixtures) with *r*_{g} of 0.075 and 0.75 µm, and
*σ*_{g} of 1.59 and 2.0 in accumulation and coarse modes,
respectively (Zhang et al., 2012). With given particle size distributions,
the bulk scattering cross section (*C*_{sca}) and absorption cross
section (*C*_{abs}) of coated BC follow the equations of

$$\begin{array}{}\text{(4)}& \u2329{C}_{\mathrm{sca}}\u232a=\underset{{r}_{min}}{\overset{{r}_{max}}{\int}}{C}_{\mathrm{sca}}\left(r\right)n\left(r\right)d\left(r\right),\end{array}$$

$$\begin{array}{}\text{(5)}& \u2329{C}_{\mathrm{abs}}\u232a=\underset{{r}_{min}}{\overset{{r}_{max}}{\int}}{C}_{\mathrm{abs}}\left(r\right)n\left(r\right)d\left(r\right).\end{array}$$

With the inhomogeneous coated BC model defined and its exact scattering and absorption properties obtained, it is possible to retrieve its optically effective ACRI with more details.

The retrieval approach is similar to the methods described in previous studies (e.g., Mack et al., 2010; Stock et al., 2011; Zhang et al., 2013), with the only differences being that the inherent aerosol optical properties are exactly calculated rather than measured and particle overall shapes are not changed during retrieval. Among all particle optical properties, the scattering and absorption are selected for retrieval, since both are basically governed by the real and imaginary parts of the ACRI, respectively. As coated BC models are overall spherical, the optically effective ACRI is determined by an iterative algorithm based on Mie theory, utilizing particle size distributions and calculated scattering and absorption cross sections. Exploiting all calculations, the designed inversion scheme to retrieve the optically effective ACRI follows.

Based on a guess for a real part, *n*, and an imaginary part, *k*, of the
ACRI at a given wavelength, two look-up tables are built from the database
with known size distribution. One look-up table encompasses the scattering
cross sections and the other contains the absorption cross sections. For
physically based sense, guessed real and imaginary parts of the optically
effective ACRI are within refractive index ranges of known compositions of
simulated internally mixed particles. Thus in our retrieval, the guessed real
part of a refractive index varies from 1.52 to 1.85 with an equidistant space
of 0.001 and the imaginary part changes from $\mathrm{5.0}\times {\mathrm{10}}^{-\mathrm{4}}$ to 0.71 with
a logarithmic interval of 0.005. Then the retrieval algorithm simultaneously
varies *n* and *k* and scans through all physically possible ACRI values
within a selected resolution until it minimizes *χ*^{2}:

$$\begin{array}{ll}{\displaystyle}{\mathit{\chi}}^{\mathrm{2}}(n,k)& {\displaystyle}={\displaystyle \frac{\mathrm{1}}{N}}\sum _{i=\mathrm{1}}^{{N}_{\phantom{\rule{0.33em}{0ex}}}}\left[{\left({\displaystyle \frac{{C}_{\mathrm{sca},\mathrm{calculated}}(n,k)-{C}_{\mathrm{sca},\mathrm{inherent}}}{{C}_{\mathrm{sca},\mathrm{inherent}}}}\right)}_{i}^{\mathrm{2}}\right.\\ \text{(6)}& {\displaystyle}& {\displaystyle}\left.+{\left({\displaystyle \frac{{C}_{\mathrm{abs},\mathrm{calculated}}(n,k)-{C}_{\mathrm{abs},\mathrm{inherent}}}{{C}_{\mathrm{abs},\mathrm{inherent}}}}\right)}_{i}^{\mathrm{2}}\right],\end{array}$$

where *C*_{sca,inherent} and *C*_{abs,inherent} are inherent
scattering and absorption cross sections of simulated internally mixed
particles, *χ*^{2}(*n*,*k*) generates the fractional difference of the
calculated scattering and absorption cross sections relative to the inherent
properties, and *N* is the number of calculations during the retrieval. The
*χ*^{2}(*n*,*k*) values for particle scattering and absorption are minimized
by optimizing initial guess ACRI values, yielding an optically effective ACRI
at this wavelength. Since particle scattering is mainly determined by the
magnitude of *n*, while its absorption is
primarily governed by the magnitude of *k*, the
minimization of *χ*^{2}(*n*,*k*) should retrieve a unique result of optically
effective ACRIs.

As the optically effective ACRIs of coated BC with fixed microphysical parameters (such as shell∕core ratio, BC fractal dimension, size distribution) are retrieved, it is possible to study the impacts of these microphysical parameters on retrieved optically effective ACRI with more details. The optically effective ACRI of internally mixed particles here is defined as an ACRI that provides almost the same scattering and absorption properties as their inherent properties, based on known size distribution and overall particle shapes for homogeneous particles. Please note that aged BC particles have complicated shapes in ambient air (D. Liu et al., 2017), and coated BC considered in this study represents a case study, resembling the findings presented by Schnaiter et al. (2005), to give insights into the effects of particle microphysics on its optically effective ACRI.

3 Results and discussion

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This study focuses on the influence of the microphysics of coated BC
aggregates on their optically effective ACRIs, and, therefore, the properties
of the microphysics are our interest. The coated BC optically effective ACRI
depends not only on the particle shell∕core ratio (i.e.,
*D*_{p}∕*D*_{c}), but also on particle morphology (i.e., the
physical arrangement of BC with respect to other components within a given
particle). With sulfate coating geometry fixed and BC fully coated, we will
consider two other morphological factors: BC geometry and BC position inside
sulfate coating.

To show the effect of BC geometry on coated BC optically effective ACRIs, the concentric core-shell structures (i.e., mass centers located at the coating center) with inside BC aggregates exhibiting fractal dimensions of 2.6, 2.8 and 2.98 are considered. Figure 2 compares retrieved optically effective ACRIs of these coated BC aggregates with different BC geometries at different shell∕core ratios, while the introduced differences of scattering and absorption cross sections are illustrated in Fig. 3. The differences are relative errors of scattering and absorption cross sections induced by retrieved effective ACRIs compared with initial inherent optical properties. The retrieved ACRIs of internally mixed coated BC particles are optically effective, since the relative errors for both scattering and absorption cross sections are within 1 % (see Fig. 3a and b). For comparison, the ACRIs of coated BC aggregates derived from the popular volume-weighted average method and Bruggeman effective medium theory, as well as their induced differences of scattering and absorption, are also shown in Figs. 2 and 3. The properties are averaged over an ensemble of BC–sulfate internally mixed particles with the aforementioned size distributions for accumulation and coarse modes separately.

As shown in Fig. 2, in accumulation mode, it is expected that, as
*D*_{p}∕*D*_{c} increases (i.e., BC content decreases),
both *n* and *k* of retrieved
optically effective ACRI of concentric coated BC aggregates will decrease. With
*D*_{p}∕*D*_{c} varying from 2.7 to 1.5, the real part of the optically
effective ACRI of accumulation coated BC increases from ∼1.53 to
∼1.60, whilst its imaginary part becomes almost 6 times larger from ∼0.038
to ∼0.216 (see Fig. 2a and c). As BC fractal dimension increases (i.e., BC
becomes more compact), the real part of the optically effective ACRI shows a
slight decrease in accumulation mode, whereas the reverse is true for
the retrieved imaginary part. For mass-center positions of different BC
geometries fixed within sulfate coating, retrieved optically effective ACRIs
of accumulation particles are slightly sensitive to their inside BC
geometries, with differences of less than 1 % and 5 % for *n* and *k*,
respectively. Compared to the optically effective ACRIs of concentric coated
BC aggregates in accumulation mode, the imaginary parts of ACRIs estimated
from the VWA and EMT are lower by 2 %–7 % and 9 %–15 %, respectively,
depending on *D*_{p}∕*D*_{c} and BC fractal dimension, while their real
parts are slightly higher, with differences within 2 %. As a result, the
VWA and EMT overestimate coated BC scattering cross sections by 2 %–7 % and
4 %–11 % and underestimate absorption cross sections by 1 %–4 % and
5 %–11 %, respectively (see Fig. 3c and e). Meanwhile, the VWA performs
slightly better than the EMT for coated BC in accumulation mode.

Unlike accumulation mode, the retrieved optically effective ACRI of
concentric coated BC in coarse mode depicts distinctive patterns, which is
illustrated in Fig. 2b and d. The impact of particle microphysics on the
optically effective ACRIs of coarse concentric coated BC is complicated,
especially for their real parts, which show strong oscillations as a function
of the shell∕core ratio. The imaginary parts of retrieved optically
effective ACRIs of coated BC aggregates in coarse mode generally decrease
with the increase in *D*_{p}∕*D*_{c} or BC fractal dimension.
The imaginary parts of derived ACRIs based on the VWA and EMT can be higher
than those of retrieved optically effective ACRIs by a factor of ∼3,
and the resulting overestimation of absorption cross sections of coarse
concentric coated BC can be as high as ∼75 %. The optically
effective ACRI, producing coated BC scattering and absorption with
differences less than 1 %, performs predominantly better than the VWA and
EMT in coarse mode, and the VWA and EMT result in more uncertainties in
particle absorption than scattering. Furthermore, the VWA and EMT
overestimate more absorption and underestimate more scattering for coarse
coated BC with a larger BC fractal dimension or *D*_{p}∕*D*_{c}.

The simulations discussed above assume coated BC with a concentric core-shell
structure, which does not always represent realistic aerosols, whereas coated
BC with an off-center core-shell structure may be certainly true for some
ambient particles. Figure 4 portrays retrieved optically effective ACRIs of
coated BC aggregates (BC fractal dimension of 2.8) with the aforementioned
size distributions for two different off-center structures compared to the
concentric core-shell structure. For two off-center core-shell structures
assumed, one is BC aggregates located in the middle of a radius of the
coating sphere and the other is BC in an outer position as close as possible
to the coating boundary. It is evident that coated BC optically effective
ACRIs in accumulation mode decrease with increasing
*D*_{p}∕*D*_{c} for various BC inside positions (see Fig. 4a
and c). The optically effective ACRIs of accumulation coated BC aggregates
are generally sensitive to the BC position inside sulfate coating, with
variations of 1 % and 20 % for *n* and *k*, respectively. When BC
aggregates move from the coating center to the boundary, the real parts of
retrieved optically effective ACRIs in accumulation mode are found to
increase slightly, as opposed to the decrease in their imaginary parts. For
accumulation BC aggregates with different core-shell structures, the VWA and
EMT give relatively close ACRIs to their optically effective ACRIs, with *n*
differences both within 1 % and *k* differences less than 11 % and
14 %, respectively. In coarse mode, the real parts of retrieved optically
ACRIs show intricately strong variations in the shell∕core ratio and
BC inside position, and their imaginary parts are generally decreasing, with
BC becoming closer to the coating boundary (see Fig. 4b and d). The imaginary
parts of retrieved optically effective ACRIs of coarse coated BC with
different BC inside positions are significantly lower than those given by the
VWA and EMT, indicating severe overestimation of coarse particle absorption
by the VWA and EMT.

Figure 5 illustrates the differences of scattering and absorption cross sections of coated BC aggregates with different BC inside positions induced by the VWA, EMT and optically effective ACRIs. The optically effective ACRIs cause differences of coated BC scattering and absorption within 1 % compared to its inherent properties in both accumulation and coarse modes, whereas the VWA and EMT induce large particle scattering and absorption differences, especially in coarse mode. One can see that, in coarse mode, the VWA and EMT can overestimate coated BC absorption as high as ∼90 % at some coating states, and they overestimate more for BC closer to coating boundary.

Generally, retrieved optically effective ACRIs of coated BC aggregates show significantly distinctive patterns in accumulation and coarse modes. In accumulation mode, besides the shell∕core ratio, the optically effective ACRIs are slightly sensitive to BC geometry and BC position inside sulfate coating. Their retrieved real parts increase slightly as BC becomes loose or BC is located closer to the coating boundary, whereas the reverse is true for their imaginary parts. Nevertheless, in coarse mode, the real parts of optically effective ACRIs are highly complex functions of the shell∕core ratio, BC fractal dimension and BC inside position, while their imaginary parts generally increase with BC fractal dimension decreasing or BC close to the coating center. Meanwhile, the VWA and EMT show acceptable performance for estimating ACRIs of coated BC in accumulation mode, resulting in uncertainties in scattering and absorption, both within approximately 10 %, whereas in coarse mode, the VWA and EMT, generating dramatically higher imaginary parts than those of optically effective ACRIs, can significantly overestimate coated BC absorption by a factor of nearly 2, particularly for heavily coated BC with a large BC fractal dimension or BC close to the coating boundary.

As demonstrated in Bond et al. (2006), particle size distribution affects
coated BC absorption properties and its BC absorption amplification due to
weakly absorbing coatings. Figure 6 illustrates the variations of retrieved
ACRIs of concentric coated BC aggregates (BC fractal dimension of 2.8) with
different particle size distributions at different shell∕core ratios.
The real parts (panels a–d) and imaginary parts (panels e–h) of retrieved
ACRIs are depicted in Fig. 6, respectively, and the panels from left to right
correspond to the optically effective ACRIs in accumulation and coarse modes,
and the ACRIs given by the VWA and EMT. The lognormal size distributions are
assumed for the coated BC particles with *r*_{g} (*x* axis) ranging
from 0.025 to 0.15 µm and from 0.5 to 1.0 µm in
accumulation and coarse modes, respectively, and *σ*_{g} fixed as
the aforementioned values. Figure 6 clearly shows that the optically
effective ACRIs of coated BC aggregates are sensitive to particle size
distribution and shell∕core ratio. For accumulation coated BC, the
retrieved optically effective ACRI shows weak variation in particle size
distribution, and with *r*_{g} increasing, its imaginary part
increases mildly for thin coating (i.e., small *D*_{p}∕*D*_{c}),
whereas the real part decreases. Nevertheless, in coarse mode, the variation
of retrieved optically effective ACRI becomes strong, and its imaginary part
generally shows a decreasing trend as *r*_{g} increases. Compared to
the results in accumulation mode, retrieved optically effective ACRIs of
concentric coated BC aggregates in coarse mode become more sensitive to
particle size distribution and shell/core
ratio, i.e., showing larger variation. Considering that the BC∕sulfate
volume ratio is a constant as *D*_{p}∕*D*_{c} is fixed, ACRI
results given by the VWA and EMT are not sensitive to particle size
distribution and are expressed by the horizontal lines in the figure. In
accumulation mode, the VWA and EMT provide acceptable ACRI results for
different size distributions with scattering and absorption uncertainties
within ∼10 % (not shown), and the VWA shows mildly better
performance than the EMT in estimating the imaginary part. However, in coarse
mode, the imaginary parts are severely overestimated by the VWA and EMT at
different size distributions when compared to retrieved optically effective
ACRIs, indicating that the VWA and EMT overrate aged BC absorption
significantly. This is consistent with the results of Bond et al. (2006),
which suggest that the VWA for the refractive index is unrealistic, leading
to unphysical results and overestimation of particle absorption.

As discussed above, the VWA approximation employed in the state-of-the-art aerosol–climate models extensively could result in significant errors in the absorption of thickly coated BC aggregates in coarse mode (specifically, ${D}_{\mathrm{p}}/{D}_{\mathrm{c}}\ge \mathrm{2.0})$, although it gives acceptable results for fully coated BC in accumulation mode and thinly coated BC in coarse mode. For thickly coated BC in coarse mode, with all previous microphysical factors considered, it seemingly becomes possible to decompose the influences of coated BC microphysics on their optically effective ACRIs and to do the parameterization. Nonetheless, the optically effective ACRIs of coarse coated BC are highly intricate functions of their microphysical properties parameterized by multiple parameters (e.g., BC fractal parameters, coating parameters and shell∕core ratio), and cannot simply be represented by these microphysical parameters adequately. Because the ACRIs of internally mixed particles are dependent on their chemical compositions, the traditional VWA approach to their determination is to calculate them from their bulk chemical compositions and known values of the refractive indices of the pure components. This may be a reasonable approach for approximation of the real part of ACRIs, whereas the corresponding values for calculation of the imaginary part are not as good as their real counterparts (e.g., Marley et al., 2001). Meanwhile, for heavily coated BC in coarse mode with various microphysics, the VWA generates dramatically higher imaginary parts than those of optically effective ACRIs to varying degrees. Thus, the imaginary part of heavily coated BC in coarse mode is considered to be that given by the VWA divided by a factor, which may show better results, whilst its real part is the same as that approximated by the VWA. To be simple and specific, the factor for dividing the imaginary part given by the VWA is assumed to be 2, and a new assumed parameterization of ACRIs of BC heavily coated by sulfate in coarse mode is expressed by

$$\begin{array}{ll}{\displaystyle}{n}_{\mathrm{effective}}\left(\mathit{\lambda}\right)& {\displaystyle}=\left({n}_{\mathrm{BC}}\right(\mathit{\lambda})\times {\displaystyle \frac{{V}_{\mathrm{BC}}}{{V}_{\mathrm{BC}}+{V}_{\mathrm{sulfate}}}}+{n}_{\mathrm{sulfate}}(\mathit{\lambda})\\ \text{(7)}& {\displaystyle}& {\displaystyle}\times {\displaystyle \frac{{V}_{\mathrm{sulfate}}}{{V}_{\mathrm{BC}}+{V}_{\mathrm{sulfate}}}})/\mathrm{2},\end{array}$$

$$\begin{array}{ll}{\displaystyle}{k}_{\mathrm{effective}}\left(\mathit{\lambda}\right)& {\displaystyle}={\displaystyle \frac{\mathrm{1}}{\mathrm{2}}}\times \left({k}_{\mathrm{BC}}\right(\mathit{\lambda})\times {\displaystyle \frac{{V}_{\mathrm{BC}}}{{V}_{\mathrm{BC}}+{V}_{\mathrm{sulfate}}}}+{k}_{\mathrm{sulfate}}(\mathit{\lambda})\\ \text{(8)}& {\displaystyle}& {\displaystyle}\times {\displaystyle \frac{{V}_{\mathrm{sulfate}}}{{V}_{\mathrm{BC}}+{V}_{\mathrm{sulfate}}}})/\mathrm{2},\end{array}$$

where *n*_{effective} and *k*_{effective} denote the real part and
imaginary part of parameterized ACRI, *λ* the wavelength of light,
*n*_{BC} and *n*_{sulfate} the real parts of pure BC and sulfate, *k*_{BC} and *k*_{sulfate} the imaginary parts of BC and sulfate, and *V*_{BC}
and *V*_{sulfate} the volumes of BC and sulfate, respectively.

To demonstrate the performance of the simple expressions in approximating ACRIs of fully coated BC aggregates in coarse mode with ${D}_{\mathrm{p}}/{D}_{\mathrm{c}}\ge \mathrm{2.0}$, Fig. 7 compares induced relative errors of scattering and absorption coefficients of coarse coated BC with the aforementioned fixed size distributions based on ACRIs from the popular VWA and Eqs. (7)–(8). The cases of coarse coated BC with BC fractal dimensions of 2.8 and 2.98 are illustrated in panels (a), (b), (e) and (f) and panels (c), (d), (g) and (h) of the figure. It is clear that the assumed new ACRI parameterization method shows a better performance than the VWA in the estimation of scattering and absorption of heavily coated BC with various coating microphysics in coarse mode. Compared to the VWA, the new parameterization method reduces the relative errors in estimating absorption cross sections of coarse coated BC by a factor of nearly 2. Surprisingly, the errors of scattering cross sections of coated BC are also lessened, although the real part of the ACRI in the assumed parameterization method is considered to the same as that in the VWA. As the effects of particle microphysics on optically effective ACRIs of coarse coated BC are rather complicated, it is difficult to find a “best” parameterization for the optically effective ACRI based on its microphysics. However, Fig. 7 indicates that the simple ACRI approximation we assume gives a better estimation than the VWA, which are widely used in aerosol–climate models, on the optical properties of heavily coated BC in coarse mode.

Our theoretical analysis depicts retrieved optically effective ACRI of coated BC sensitive to its shell∕core ratio, BC geometry, BC position inside coating, and size distribution. Due to aged BC particles having complicated coating morphologies in ambient air, which can be provided by individual particle analysis (Adachi and Buseck, 2008; Li et al., 2016; Wang et al., 2017), coated BC considered in this study represents case studies, such as those BC particles observed under polluted urban environments (Peng et al., 2016; Chen et al., 2017), to give insights into the effects of particle microphysics, resembling the findings presented by Schnaiter et al. (2005). The study indicates that retrieved optically effective ACRIs of coated BC aggregates show distinctive patterns in accumulation and coarse modes. In accumulation mode, retrieved optically effective ACRIs of coated BC are more impacted by their chemical compositions and composition ratio, which look like the real ACRI, and the influences by their other microphysics are generally limited. However, in coarse mode, the results challenge conventional beliefs, and retrieved optically effective ACRIs of coated BC are highly complicated functions of particle microphysics. That is to say, the optically effective ACRIs of coarse coated BC are not only affected by their chemical compositions and composition ratio, but are also impacted by their other microphysics (such as size distribution and BC geometry). This makes the notion of refractive index become somewhat ill-defined for internally mixed particles, since it is not the real particle refractive index, but an optically effective refractive index. This study also indicates that the VWA and EMT, giving acceptable ACRIs for internally mixed particles in accumulation mode, produce a higher imaginary part of ACRI than that of optically effective ACRI, and could overestimate heavily coated BC absorption significantly in coarse mode. This may be one of the reasons why modeled aerosol optical depth is 20 % larger than observed (Roelofs et al., 2010), since the VWA approximation is widely employed in the state-of-the-art aerosol–climate models. To reduce the uncertainties, we propose a simple ACRI parameterization method for heavily coated BC in coarse mode (specifically, ${D}_{\mathrm{p}}/{D}_{\mathrm{c}}\ge \mathrm{2.0})$, which reduces the scattering and absorption errors of coated BC by a factor of nearly 2 in comparison with the VWA, although absorption errors of coated BC with some microphysics are still relatively high. As such, in order to produce reliable estimates of BC radiative forcing in aerosol–climate models, the optically effective ACRI, rather than the ACRI given by the VWA, appears to be essential, especially for aged BC in coarse mode.

4 Conclusions

Back to toptop
This study numerically explores the impacts of coating microphysics on the
optically effective ACRIs of polydisperse coated BC particles, which are
retrieved from exactly calculated scattering and absorption properties
without variations in overall particle shapes during retrieval. The numerical
simulations conducted here have multiple controllable microphysical
variables, i.e., shell∕core ratio, BC geometry, BC position inside
sulfate coating and size distribution, and we attempt to constrain these
variables within realistic ranges as determined by observation-based studies.
The fractal aggregate is employed to model the realistic BC geometry, and
optical properties of spherical coated BC aggregates are calculated by
utilizing the numerically exact multiple-sphere *T*-matrix method. The fast-Mie-theory-based data analysis scheme is applied for retrieving the optically
effective ACRIs of coated BC, and the numerical results are analyzed to
better understand retrieved optically effective ACRIs in relation to the
controllable microphysical variables.

Our results reveal that retrieved optically effective ACRIs of coated BC aggregates depict significantly different patterns in accumulation and coarse modes. With BC becoming loose or close to coating the boundary, the real parts of retrieved optically effective ACRIs of accumulation-coated BC increase slightly, as opposed to the decrease for the imaginary parts. The retrieved optically effective ACRIs of coated BC in accumulation mode are predominantly influenced by their chemical compositions and composition ratio, which makes it reasonable and looks like the real ACRIs, although it is slightly sensitive to BC geometry, BC position inside the coating and particle size distribution. Nonetheless, retrieved optically effective ACRIs of coarse coated BC are highly complicated functions of particle microphysics, and this challenges conventional beliefs given by the VWA and EMT. The VWA and EMT exhibit acceptable performances for estimating ACRIs of coated BC in accumulation mode, and resulting uncertainties in scattering and absorption are both within approximately 10 %. In coarse mode, the VWA and EMT, nevertheless, produce dramatically higher imaginary parts than those of optically effective ACRIs, and can significantly overestimate coated BC absorption by a factor of nearly 2, especially for heavily coated BC with a large BC fractal dimension or BC close to the coating boundary. This is probably one of the reasons why modeled aerosol optical depth is 20 % larger than observed (Roelofs et al., 2010), as the VWA approximation is widely employed in the state-of-the-art aerosol–climate models.

Although the parameterization of the optically effective ACRI of coarse coated BC is difficult and challenging, we propose a simple ACRI parameterization method for heavily coated BC with ${D}_{\mathrm{p}}/{D}_{\mathrm{c}}\ge \mathrm{2.0}$ in coarse mode, and its scattering and absorption errors are decreased by a factor of nearly 2 compared to the VWA. Overall, this work clearly highlights the importance of accounting for the optically effective ACRI, rather than the ACRI given by the VWA, for producing reliable estimates of radiative forcing of coated BC, especially in coarse mode, in aerosol–climate models. However, caution may be taken in interpreting our results as a comprehensive guide, as the closure studies between observation and numerical models on aged BC properties still show poor agreement (Radney et al., 2014).

Data availability

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Data availability.

The data obtained from this study are available upon request from Mao Mao (mmao@nuist.edu.cn) or Xiaolin Zhang (xlnzhang@nuist.edu.cn) and are also available at https://github.com/xiaolinzhang/Data_FOR_ACP-2018-1279 (last access: 19 May, 2019; Zhang, 2019).

Supplement

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Supplement.

The supplement related to this article is available online at: https://doi.org/10.5194/acp-19-7507-2019-supplement.

Author contributions

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Author contributions.

XZ and MM designed the research plan. YY gave some suggestions for the revision. XZ carried it out, performed the simulations, and prepared the manuscript with contributions from all the co-authors.

Competing interests

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Competing interests.

The authors declare that they have no conflict of interest.

Acknowledgements

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Acknowledgements.

We particularly acknowledge the source codes of MSTM 3.0 from Daniel W. Mackowski and Michael I. Mishchenko. We also gratefully appreciate the supports from the Special Program for Applied Research on Super Computation of the NSFC-Guangdong Joint Fund (the second phase) under grant no. U1501501.

Financial support

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Financial support.

This work is financially supported by the National Natural Science Foundation of China (NSFC) (nos. 91644224 41505127, and 21406189), the Natural Science Foundation of Jiangsu Province (no. BK20150901), the Natural Science Foundation of the Jiangsu Higher Education Institutions of China (no. 15KJB170009), and the Key Laboratory of Meteorological Disaster, Ministry of Education (no. KLME201810). This work is also supported by the Startup Foundation for introducing Talent of NUIST (nos. 2015r002 and 2014r011), a China Postdoctoral Science Foundation Funded Project (no. 2016M591883), and Jiangsu Planned Projects for Postdoctoral Research Funds (no. 1601262C).

Review statement

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Review statement.

This paper was edited by Yves Balkanski and reviewed by two anonymous referees.

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Short summary

The understanding of the exactly retrieved optically effective aerosol complex refractive index (ACRI) of aged BC affected by their microphysics is numerically evaluated. A simple new ACRI parameterization for heavily coated BC in coarse mode is then proposed. We suggest that, to produce reliable estimates of BC radiative forcing in aerosol–climate models, the optically effective ACRI, rather than the ACRI given by the VWA, appears to be essential, especially for coarse coated BC particles.

The understanding of the exactly retrieved optically effective aerosol complex refractive index...

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