Introduction
Black carbon (BC) has been identified as the second most important anthropogenic global warming agent in the atmosphere by virtue of its strong absorption of solar radiation and its role as cloud condensation nuclei (CCN) in cloud formation (Ramanathan and Carmichael, 2008; Bond et al., 2013; Wang et al., 2013; Jacobson, 2014). BC climatic effects are significantly influenced by the BC aging process in the atmosphere, which transforms BC from an external to internal mixing state (Schwarz et al., 2008; China et al., 2013) and increases its hygroscopicity (Zhang et al., 2008; Popovicheva et al., 2011) and light absorption (Jacobson, 2001; Shiraiwa et al., 2010; Qiu et al., 2012; Scarnato et al., 2013).
Freshly emitted BC particles are mostly hydrophobic and externally mixed with other aerosol constituents (Zuberi et al., 2005; Zhang et al., 2008). BC agglomerates shortly after emission to form irregular aggregates because of multi-phase processes (Zhang et al., 2008; Pagels et al., 2009; Xue et al., 2009). Early studies have found that BC particles age in the atmosphere through condensation and coagulation processes (e.g., Heintzenberg and Covert, 1984; Heintzenberg, 1989). Recent studies have confirmed that BC becomes coated by water-soluble material during atmospheric aging, including condensation of sulfate, nitrate, and organics (Moteki et al., 2007; Shiraiwa et al., 2007), coagulation with preexisting aerosols (Johnson et al., 2005; Kondo et al., 2011), and heterogeneous reactions with gaseous oxidants (Zuberi et al., 2005; Khalizov et al., 2010; Zhang et al., 2012). At the same time, BC aggregates also exhibit considerable restructuring and compaction (Weingartner et al., 1997; Saathoff et al., 2003; Zhang et al., 2008), which significantly alters BC morphology (Adachi and Buseck, 2013; China et al., 2015). Aged BC particles experience hygroscopic growth and activate efficiently as CCN (Zuberi et al., 2005; Zhang et al., 2008). The hygroscopic growth of BC particles depends on their initial size, condensed soluble material mass, surface chemical property, and ambient relative humidity (RH) (Zhang et al., 2008; Khalizov et al., 2009b; Popovicheva et al., 2011).
A number of laboratory experiments have been conducted to investigate the effects of atmospheric aging on BC radiative properties. Gangl et al. (2008) showed that internal BC–wax mixture amplifies the BC absorption coefficient by 10–90 %, depending on the amount of coating. Shiraiwa et al. (2010) found that BC absorption enhancement due to organic coating varies significantly for various BC sizes and coating thickness, with up to a factor of 2 enhancement for thick coatings. Under different experimental conditions, relatively small increases ( 30 %) in BC absorption have also been observed for BC coated by sulfuric acid (Zhang et al., 2008) and some organics (Saathoff et al., 2003). Furthermore, Xue et al. (2009) and Qiu et al. (2012) showed a less than 20 % increase in BC absorption for organic coating, which depends on organic species and coating thickness. Thus, the resulting large variation among different experimental studies indicates that the aging effects on BC radiative properties strongly depend on coating material and thickness as well as BC particle size. It is clear, therefore, that experimental details are critically important in making meaningful and appropriate comparisons among various experimental studies involving BC absorption enhancement associated with coating.
Field measurements have also revealed substantial variation in BC optical properties during atmospheric aging. Bond and Bergstrom (2006) showed that observed BC mass absorption cross sections (MAC) vary by more than a factor of 2 (mostly 5–13 m g under different atmospheric conditions. Based on direct measurements at a suburban site in Japan, Naoe et al. (2009) showed that coating increases BC absorption by a factor of 1.1–1.4 with a larger increase for thicker coatings. Knox et al. (2009) found an absorption enhancement of up to 45 % due to BC coating based on measurements in downtown Toronto. Similar increases in absorption have also been directly observed for the internal mixing of biomass-burning BC (Lack et al., 2012). However, Cappa et al. (2012) reported that the observed BC absorption increased only by 6 % due to internal mixing based on direct in situ measurements over California. This suggests that coating effects on BC absorption are rather complex in reality, which depends on different coating material, mass, and structure influenced by emission sources and atmospheric processes.
Adachi et al. (2010) found that many BC particles embedded within host material are chainlike aggregates locating in off-center positions, based on transmission electron microscope (TEM) observations for samples collected from Mexico City. Using the discrete dipole approximation (DDA) method developed by Draine and Flatau (1994), Adachi et al. showed that a more realistic BC coating morphology results in 20–40 % less absorption at visible wavelengths than a concentric core-shell shape. Based on ground-based measurements during the California Research at the Nexus of Air Quality and Climate Change (CalNex) campaign, Adachi and Buseck (2013) further observed that many BC particles are only attached to host material instead of being fully embedded within them, leading to only a slight increase in BC absorption. They concluded that the complex mixing structure of BC particles could explain a smaller absorption amplification by BC coating determined from observations than the results computed from an idealized core-shell model. China et al. (2013, 2015) classified the observed irregular BC coating shapes into four types: embedded (heavily coated), thinly coated, partly coated, and partially encapsulated. These complex coating structures substantially affect BC optical properties (e.g., Videen et al., 1994; Liu and Mishchenko, 2007; Kahnert et al., 2013), which is one of the most important uncertainty sources in evaluating BC direct radiative forcing (DRF) (Bond et al., 2013). Thus, a reliable estimate of BC DRF requires a quantitative understanding of the evolution of BC radiative properties under the influence of various morphology during atmospheric aging.
In this study, we have developed a theoretical BC aging model based on the current understanding of the BC aging process, which accounts for three major stages, namely, freshly emitted aggregates, BC coated by soluble material, and BC particles undergoing further hygroscopic growth. We apply the geometric-optics surface-wave (GOS) approach to compute light absorption and scattering of BC particles at each aging stage. The theoretical calculations are compared with laboratory measurements, followed by a systematic evaluation of uncertainties associated with BC morphology and refractive index. Finally, we discuss the implication of model results for BC radiative effect assessment.
Methods
A theoretical BC aging model
Based on the current knowledge of BC atmospheric aging, we have developed a theoretical model accounting for three major BC aging stages, as depicted in Fig. 1. Stage I represents freshly emitted BC aggregates that are externally mixed with other particles. Stage II represents BC particles coated by water-soluble aerosol constituents through condensation, coagulation, and/or heterogeneous oxidations. Stage III represents BC particles coated by both soluble material and water through hygroscopic growth. In this study, six typical BC coating structures (Fig. 1) have been considered for Stages II and III to approximately represent observations in the real atmosphere or laboratory, including embedded (i.e., concentric core-cell, off-center core-shell, and closed-cell), partially encapsulated, and partly coated (i.e., open-cell and externally attached) structures following the classification presented in China et al. (2013, 2015). The concentric and off-center core-shell structures (Martins et al., 1998; Sedlacek et al., 2012) are a result of considerable collapse of BC aggregates into more compact and spherical clusters when fully engulfed in coating material (Zhang et al., 2008). The closed-cell structure is an example of where coating material not only covers the outer layers of BC aggregates but also fills the internal voids among primary spherules (Strawa et al., 1999). The partially encapsulated structure is formed when only a part of BC aggregate merges inside coating material (China et al., 2015). The open-cell and externally attached structures are produced by coating material sticking to a part of BC aggregates' surface (Stratmann et al., 2010; China et al., 2015). We wish to note that the six coating structures used in this study, including closed-cell and open-cell structures, are theoretical models and as such, they may not completely capture detailed BC coating structures from aircraft and ground-based observations. Further hygroscopic growth of BC particles after Stage III could lead to the formation of cloud droplets, a subject beyond the scope of the present study.
A theoretical model that accounts for three BC aging stages and the associated BC structures, including freshly emitted aggregates (Stage I), BC coated by soluble material (Stage II), and BC after further hygroscopic growth (Stage III). Six typical structures for coated BC at Stages II and III are considered based on atmospheric observations, including embedded (i.e., concentric core-shell, off-center core-shell, and closed-cell), partially encapsulated, and partly coated (i.e., open-cell and externally attached) structures. See text for details.
[Figure omitted. See PDF]
Laboratory measurements
The physical and radiative properties of BC particles during aging after exposure to sulfuric acid (HSO under various RH conditions (5–80 %) have been measured in the laboratory by Zhang et al. (2008) and Khalizov et al. (2009a). BC aggregates were generated by incomplete combustion of propane in a laminar diffusion burner (Santoro et al., 1983) and were sampled by a pinhole diluter (Kasper et al., 1997). A tandem differential mobility analyzer (TDMA) system was used to produce singly charged mobility-classified BC particles, followed by a coating chamber with controlled RH and HSO vapor concentrations at room temperatures (299 1 K). The BC mass and size growth due to HSO and water vapor (HO) condensation during aging were measured by an aerosol particle mass (APM) analyzer and TDMA, respectively. The effective density and fractal dimension ( of BC particles were derived from the measured BC mobility diameter ( and mass (see Eqs. 1 and 2 in Zhang et al., 2008). The compaction and restructuring of BC aggregates were captured by a TEM (see Fig. 1 in Zhang et al., 2008). BC extinction and scattering cross sections were measured at 532 nm wavelength by a cavity ring-down spectrometer (CRDS) and an integrating nephelometer, respectively. The absorption cross section was determined from the resulting difference between extinction and scattering cross sections. Khalizov et al. (2009a) showed that uncertainty in measured optical cross sections of coated BC particles is within 10 %, which primarily represents uncertainty in relative humidity, particle size, number density, and instrument calibration. This uncertainty, however, does not include the contribution from multiply charged particles. For freshly emitted BC aggregates, measured scattering cross sections involve relatively large uncertainties. More details on laboratory experiments have been presented in Zhang et al. (2008) and Khalizov et al. (2009a). Three experimental cases with initial of 155, 245, and 320 nm were used in this study (see Table 1). In each case, BC particles exposed to HSO vapor (1.4 10 molecules cm at 5 and 80 % RH were used to represent coated BC at Stages II and III (see Sect. 2.1), respectively.
Geometric-optics surface-wave (GOS) approach
We employed the GOS approach developed by Liou et al. (2011, 2014), which explicitly treats fractal aggregates and various coating structures, to compute absorption and scattering properties of BC particles at three aging stages. In the GOS approach, a stochastic procedure developed by Liou et al. (2011) is applied to simulate homogeneous aggregates and coated particles with different shapes in a 3-D coordinate system. In this study, we have extended the original stochastic process to generate more complex coating morphology, including the partially encapsulated and externally attached structures (see Figs. S1–S6 in the Supplement). Once the particle shape and composition are determined by the stochastic procedure, the reflection and refraction of particles are computed with the hit-and-miss Monte Carlo photon tracing technique. The extinction and absorption cross sections are derived following a ray-by-ray integration approach (Yang and Liou, 1997). Diffraction by randomly oriented nonspherical particles is computed on the basis of Babinet's principle (Born and Wolf, 1999) and photon-number-weighted geometric cross sections. The GOS approach accounts for the interaction of incident waves at grazing angles near the particle edge and propagating along the particle surface into shadow regions, referred to as the surface wave, using the formulation developed by Nussenzveig and Wiscombe (1980) for spheres as the basis for physical adjustments and application to nonspherical particles (Liou et al., 2010, 2011). The concept of the GOS approach is graphically displayed in Fig. 2 and it is designed for computations of absorption and extinction cross sections and asymmetry factors in line with experimental results.
A graphical representation of the geometric-optics surface-wave (GOS) approach for light scattering and absorption by coated BC aggregates. The GOS components include the hit-and-miss Monte Carlo photon tracing associated with internal and external refractions and reflections, diffraction following Babinet's principle for randomly oriented irregular particles, and surface waves traveling along the particle edges and propagating into shadow regions. See text for details.
[Figure omitted. See PDF]
Liou et al. (2010, 2011) and Takano et al. (2013) demonstrated that the single-scattering properties of aerosols with different sizes and shapes determined from the GOS approach compare reasonably well (differences < 20 %) with those determined from the finite-difference time-domain (FDTD) method (Yang and Liou, 1996) and DDA (Draine and Flatau, 1994) for column and plate ice crystals, the superposition -matrix method (Mackowski and Mishchenko, 1996) for fractal aggregates, and the Lorenz–Mie model (Toon and Ackerman, 1981) for a concentric core-shell shape. Moreover, compared with other numerical methods, the GOS approach can be applied to a wider range of particle sizes, shapes, and coating morphology with a high computational efficiency, including very large particles (e.g., 100–1000 m snowflakes) and complex multiple inclusions of aerosols within irregular snow grains (Liou et al., 2014; He et al., 2014), in which the FDTD, DDA, and -matrix methods have not been able to be applied. As stated previously, the GOS approach has been developed specifically for optical cross sections (i.e., extinction, absorption, and scattering) and the asymmetry factor. Also, due to the approximation in the use of geometric photon tracing, the GOS approach has limitation and uncertainty for application to size parameters much smaller than 1. To supplement GOS, we have developed the Rayleigh–Gans–Debye (RGD) approximation coupled with GOS for very small particles, which has been cross-validated with the superposition -matrix method (Takano et al., 2013). Takano et al. (2013) showed that the coupled GOS–RGD and superposition -matrix results are both close to the observed specific absorption of BC aggregates for the range of size parameter considered in the present study. The coupled GOS–RGD approach can be applied to size parameters covering 0.1 to 1000. In the present study, the coupled GOS–RGD approach is used for fresh BC aggregates (Stage I), while the GOS approach without RGD coupling is used for coated BC particles (Stages II and III).
BC physical properties used in theoretical calculations.
Aging stage | Pure BC | Coating material | Standard calculation | Sensitivity calculation | |||
---|---|---|---|---|---|---|---|
Mobility | Mass | Species | Mass | ||||
diameter (nm) | (10g) | (10g) | |||||
155 | 5.13 | BC aggregates with a fractal dimension of 2.1, reactive index of | (1) BC refractive index of 1.75–0.63; (2) fractal | ||||
I | 245 | 13.0 | – | – | 1.95–0.79, and primary spherules with diameters | dimension of 2.5; (3) primary spherule diameter of 20 nm; | |
320 | 20.3 | of 15 nm for three experimental cases, respectively | (4) single volume-equivalent BC sphere | ||||
155 | 5.13 | 3.67 | Concentric core-shell coating structures | (1) BC refractive index of 1.75–0.63; (2) off-center core-shell structure; | |||
II | 245 | 13.0 | Sulfuric acid (HSO | 11.0 | with BC refractive index of 1.95–0.79 | (3) closed-cell structure; (4) open-cell structure; (5) partially encapsulated | |
320 | 20.3 | 17.9 | structure; (6) externally attached structure | ||||
155 | 5.13 | Sulfuric acid and water | 7.59 | Concentric core-shell coating structures | (1) BC refractive index of 1.75–0.63; (2) off-center core-shell structure; | ||
III | 245 | 13.0 | (HSO–HO) | 20.7 | with BC refractive index of 1.95–0.79 | (3) closed-cell structure; (4) open-cell structure; (5) partially encapsulated | |
320 | 20.3 | 33.6 | structure; (6) externally attached structure |
Particle properties are derived from measurements in laboratory experiments (Zhang et al., 2008) with initial BC mobility diameters of 155, 245, and 320 nm. See text for details. See Fig. 1 and text for details.
Theoretical calculations
We used BC physical properties measured from laboratory experiments (see Sect. 2.2) as input to theoretical calculations (see Table 1). In standard calculations, the freshly emitted BC aggregates (Stage I) were assumed to be comprised of primary spherules with a diameter () of 15 nm measured from the experiments and were constructed by the GOS stochastic procedure to reproduce the measured mass and fractal dimension (i.e., 2.1) of BC aggregates. The BC mass was the product of measured BC effective densities and mobility volumes. The mass of HSO coating on BC at Stage II was derived from the observed relationship between condensed HSO mass and particle diameter at 5 % RH. The mass of HO condensed on HSO-coated BC at Stage III was derived from the measured hygroscopic mass growth ratio of HSO-coated BC at 80 % RH. In standard calculations, we used a concentric core-shell structure for coated BC particles at Stages II and III because of the strong particle compaction during aging based on laboratory observations (Zhang et al., 2008). Thus, BC core size and coating thickness were computed from the mass of BC and HSO/HO coating. The refractive index (RI) of HSO–HO coating at Stage III was derived as the volume-weighted RI of HSO and HO. We used a BC RI of 1.95–0.79 (upper bound) recommended by Bond and Bergstrom (2006) and a BC density of 1.77 g cm suggested by Zhang et al. (2008). Under the preceding conditions, computations of BC optical properties at 532 nm wavelength were carried out for comparison with laboratory measurements. The comparison between GOS and experimental results in this study provides an additional dimension of validation/cross-check of the GOS approach.
In addition, we conducted four sensitivity calculations for Stage I and six sensitivity calculations for Stages II and III to quantify uncertainties associated with BC RI and morphology (see Table 1). In the first sensitivity calculation for each aging stage, a lower bound of BC RI of 1.75–0.63 recommended by Bond and Bergstrom (2006) was used. For the other three sensitivity tests on morphology effects at Stage I, we increased BC fractal dimension from 2.1 to 2.5 and primary spherules diameter from 15 to 20 nm without changing BC mass, and replaced BC aggregates with a single volume-equivalent sphere. We then applied five types of BC coating structures, including off-center core-shell, closed-cell, open-cell, partially encapsulated, and externally attached structures (see Fig. 1 and Sect. 2.1), and conducted five additional sensitivity calculations for both Stages II and III. Specifically, the off-center core-shell structure assumes a spherical BC core internally tangent to the particle surface with the same size as the concentric core-shell structure used in standard calculations. The closed-cell structure assumes that all primary spherules have the same concentric core-shell shape with a BC core diameter of 15 nm. The open-cell structure also assumes a diameter of 15 nm for all primary spherules, which are either pure BC or pure coating material. Both closed- and open-cell structures were constructed to have the same fractal dimension as measured in the experiments. The partially encapsulated structure assumes that a random part of BC aggregates is inside a spherical coating particle (Figs. S1–S6), while the externally attached structure assumes that a single spherical coating particle is randomly sticking to a part of the BC aggregate's surface (Figs. S1–S6). BC primary spherules in both structures have diameters of 15 nm. We note that assuming a cluster of spheres for the above-mentioned coating structures may not be sufficiently realistic and that nonspherical morphology models without restrictions to composite of spheres appear to be more plausible (Adachi et al., 2010), a challenging subject to be investigated in future work.
Results and discussions
Fresh BC aggregates (Stage I)
Figure 3 shows the extinction, absorption, and scattering cross sections (at 532 nm) of fresh BC aggregates at Stage I based on laboratory measurements and theoretical calculations using different BC RI and morphology. For comparison with experimental measurements, theoretical results with BC RI of 1.95–0.79 (i.e., standard calculations) are used unless stated otherwise. The calculated extinction cross sections are consistent (differences 20 %) with measurements for fresh BC aggregates at Stage I with different sizes (i.e., 155, 245, and 320 nm). However, theoretical calculations tend to overestimate and underestimate extinction for the smallest and largest BC aggregates, respectively. The discrepancies between theoretical and measured BC absorption cross sections at Stage I increase from 7 % (overestimate) to 15 % (underestimate) as BC size becomes larger (Fig. 3). Although the calculated scattering cross sections at Stage I are consistently overestimated for different BC sizes compared with measurements, the absolute discrepancies are small. This overestimate is partly because of the uncertainty associated with extinction and absorption calculations for small particles, where theoretical results overestimate (underestimate) extinction cross sections more (less) than absorption cross sections for of 155 nm ( of 245 and 320 nm). The scattering measurements also contribute to the discrepancy in view of the fact that the integrating nephelometer misses light scattering signals at near-forward directions (Anderson and Ogren, 1998). We note that the calculated single scattering albedo (SSA; 0.16) of BC aggregates at Stage I is within the range of 0.15–0.3 measured for BC from different combustion sources (Bond and Bergstrom, 2006), while the experimentally measured SSA is smaller than 0.10 due to the relatively open and loosely connected BC aggregate structures (Khalizov et al., 2009a).
Laboratory measurements and theoretical calculations of BC extinction (left column), absorption (middle column), and scattering (right column) cross sections (at 532 nm) at three aging stages for BC with initial mobility diameters ( of 155 nm (top row), 245 nm (middle row), and 320 nm (bottom row). Black circles represent mean values from measurements and black error bars indicate experimental uncertainties reported by Zhang et al. (2008) and Khalizov et al. (2009a). Green squares indicate results from the standard theoretical calculations (see Table 1 for details). Red error bars indicate the range of theoretical calculations using a BC refractive index of 1.95–0.79 (upper bound) and 1.75–0.63 (lower bound). Blue error bars represent the upper and lower bounds of sensitivity calculations using different BC morphology with a refractive index of 1.95–0.79 (see also Fig. 1 and Table 1).
[Figure omitted. See PDF]
Sensitivity calculations show that using a BC RI of 1.75–0.63 narrows the gap between calculated and measured scattering cross sections of fresh BC aggregates by up to a factor of 2 (Fig. 3). Because of using the BC RIs of 1.95–0.79 (upper bound) and 1.75–0.63 (lower bound), the extinction and absorption cross sections of fresh BC aggregates can vary by 25–40 % and 20–30 %, respectively, while the scattering cross section ranges from 50 to 65 % with a higher sensitivity for larger BC sizes. Based on the -matrix calculations using a BC RI of 2–1 and 1.75–0.5, Liu et al. (2008) showed variation of 50–70 % in BC absorption and scattering cross sections depending on aggregate structures, which is comparable to the results derived in this study. Scarnato et al. (2015) also found a strong dependence of BC absorption on BC RI for uncoated aggregates using the DDA method.
Figure 4 shows the extinction, absorption, and scattering cross sections for different aggregate morphology normalized by BC aggregate cross sections determined from standard calculations (i.e., fractal aggregates with a of 2.1 and of 15 nm; see Sect. 2.4) at Stage I. We found that a 20 % increase in (i.e., more compact structure) decreases BC absorption and scattering cross sections by 20–50 %, with greater reductions for larger BC sizes. Using the DDA method, Scarnato et al. (2013) also found a smaller BC absorption of more compact structures. Liu et al. (2008) applied a -matrix calculation to show that as increases from 1.5 to 3, the absorption of BC aggregates either decreases monotonically or decreases until reaches a certain value and then increases, depending on BC RI, size and the number of primary spherules. This is because the amount of BC directly exposed to the incident light becomes smaller as increases, while the growing interaction among primary spherules could increase light absorption (Liu et al., 2008). The present calculations illustrated that BC absorption and scattering are weakly dependent on the size of primary BC spherules. An increase in the spherule diameter from 15 to 20 nm results in less than 10 % variation in BC extinction, absorption, and scattering cross sections (Fig. 4), which is consistent with the -matrix results presented by Liu and Mishchenko (2007) who concluded that the monomer size has a rather weak effect on BC scattering and absorption, if fractal dimension is fixed. Nevertheless, the effect of monomer size on BC optical properties could vary significantly depending on BC aggregate shape, size, the number of primary spherules, and BC RI (Liu et al., 2008; Kahnert et al., 2014). Assuming a volume-equivalent BC sphere instead of fractal aggregates results in 5–25 % weaker absorption and extinction and up to 65 % smaller scattering cross sections for different BC sizes, compared with BC aggregates in standard calculations. The stronger absorption and scattering from aggregate structures is due primarily to the interaction between neighboring primary spherules of BC aggregates (Fuller, 1995). The present calculated increase (5–20 %) in absorption from sphere to aggregate structures is slightly smaller than the value ( 30 %) reported by Bond and Bergstrom (2006), because of different numbers and sizes of primary spherules, aggregate shapes, and fractal dimensions employed in calculations (Iskander et al., 1991; Liu et al., 2008; Kahnert et al., 2014). Using the -matrix method, Kahnert and Devasthale (2011) showed a radiative forcing of BC aggregates that was 2 times higher than the volume-equivalent sphere counterparts.
Extinction (red), absorption (blue), and scattering (orange) cross sections (at 532 nm) for different BC morphology normalized by BC aggregate cross sections determined from standard calculations at aging Stage I for initial BC mobility diameters () of 155 nm (a), 245 nm (b), and 320 nm (c). Results for four BC structures are shown, including BC aggregates in standard calculations (circles) with a fractal dimension () of 2.1 and a primary spherule diameter () of 15 nm, BC aggregates with of 2.5 (triangles; versus 2.1 in standard calculations), BC aggregates with a of 20 nm (squares; versus 15 nm in standard calculations), and a single mass-equivalent BC sphere (crosses; versus fractal aggregate in standard calculations). Dashed horizontal lines indicate a value of 1.
[Figure omitted. See PDF]
Coated BC particles (Stages II and III)
The extinction, absorption, and scattering cross sections (at 532 nm) of coated BC particles at aging Stages II and III determined from laboratory measurements and theoretical calculations are depicted in Fig. 3. Theoretical results with the BC RI of 1.95–0.79 are used for comparison with experimental measurements unless stated otherwise. The calculated optical cross sections (i.e., extinction, absorption, and scattering) of coated BC at Stages II and III are in general agreement (differences 30 %) with laboratory measurements, because of the observed efficient structure compaction during aging in laboratory experiments (Zhang et al., 2008). However, theoretical calculations tend to overestimate extinction and absorption for of 155 and 245 nm at both Stages II and III, while the extinction and absorption for the largest particle ( of 320 nm) is underestimated at Stage II. The calculated scattering cross sections are overestimated for the smallest BC size ( of 155 nm) at Stage II, but tend to be underestimated for larger BC sizes at Stage III, particularly for of 320 nm. The present sensitivity calculations show that the discrepancy in scattering for of 320 nm at Stage III cannot be explained by uncertainties associated with BC RI or coating morphology (Fig. 3), which, however, could be attributed to uncertainty associated with the coating mass of HSO and HO. We assumed only HO condensation during BC hygroscopic growth from Stage II to III in the calculation of coating mass, which may not be accurate considering that HSO condenses on BC surface simultaneously along with HO. A sensitivity calculation shows that replacing HO by HSO in the coating material reduces scattering discrepancy to 10 % for of 320 nm at Stage III, since HSO is more reflective than HO, but increases the overestimate in BC absorption from 17 to 25 %.
Theoretical calculations show that using a BC RI of 1.75–0.63 decreases extinction and absorption cross sections of coated BC particles by 10–17 % at Stage II and by 5–15 % at Stage III for different BC sizes, which, however, is smaller compared with the decrease for fresh BC aggregates (20–40 %). The scattering cross sections of coated BC particles decrease by up to 50 % due to the use of smaller BC RI for different BC sizes and aging stages.
Figures 5 and 6 show the extinction, absorption, and scattering cross sections for different coated BC structures normalized by cross sections of the concentric core-shell structure determined from standard calculations. The off-center core-shell structure has little impact on BC optical properties at Stage II (Fig. 5) with differences of less than 10 % compared with the concentric core-shell structure, primarily because of the thin coating layer. As the coating thickness increases after hygroscopic growth, the off-center core-shell structure results in a 5–30 % decrease in extinction, absorption, and scattering cross sections at Stage III (Fig. 6). This finding is consistent with the result presented by Adachi et al. (2010) using the DDA method, where they found up to 30 % reductions in BC absorption depending on the position of BC core inside coating material. A recent -matrix study (Mishchenko et al., 2014) also showed that the absorption of BC–water mixture tends to decrease as a BC particle moves from the droplet center to the boundary.
Extinction (red), absorption (blue), and scattering (orange) cross sections (at 532 nm) for different coating morphology normalized by cross sections of concentric core-shell structures determined from standard calculations at aging Stage II (BC coated by sulfuric acid (HSO for initial BC mobility diameters ( of 155 nm (a), 245 nm (b), and 320 nm (c). Six BC coating structures are considered, including concentric core-shell (circles), off-center core-shell (triangles), closed-cell (squares), open-cell (crosses), partly encapsulated (diamonds), and externally attached (asterisks) structures (see also Fig. 1). Dashed horizontal lines indicate a value of 1.
[Figure omitted. See PDF]
Same as Fig. 5, but for aging stage III where BC particles are coated by both sulfuric acid and water (HSO–HO).
[Figure omitted. See PDF]
Compared with the concentric core-shell structure, the closed-cell structure tends to have stronger absorption and weaker scattering for of 245 and 320 nm at Stages II and III, while the reverse is true for the open-cell structure (Figs. 5 and 6). This is in line with the conclusion presented in Liou et al. (2011) that closed-cell aggregates have larger absorption and smaller SSA than their open-cell counterparts. The closed-cell structure has a larger surface area for the interaction of the incident light with each primary spherule that acts as a coated core-shell unit, leading to a stronger lensing effect and thus stronger absorption compared with the concentric core-shell structure. However, the open-cell structure lacks a closed coating structure to produce efficient lensing effects. The coating spherules sticking to pure BC spherules in the open-cell structure increase the interaction between the incident light and nonabsorbing coating material, resulting in a stronger scattering.
Enhancement in BC absorption (top) and scattering (bottom) during aging from freshly emitted aggregates at Stage I to BC coated by sulfuric acid (HSO at Stage II (circles), and by both sulfuric acid and water (HSO–HO) at Stage III (crosses) for initial BC mobility sizes (D of 155 nm (left), 245 nm (middle), and 320 nm (right). The enhancements for different BC coating morphology are shown, including concentric core-shell, off-center core-shell, closed-cell, open-cell, partly encapsulated, and externally attached structures (see also Fig. 1). The reference case for enhancement calculation is the fresh BC aggregate measured in laboratory experiments, which is used for all six BC coating morphology cases. Thus, the enhancement is computed as the ratio of calculated absorption/scattering cross sections of coated BC particles to observed values of fresh BC aggregates. Also shown is the measured enhancement from laboratory experiments (Obs.). Horizontal dashed lines indicate a value of 1.0.
[Figure omitted. See PDF]
The extinction and absorption cross sections of partially encapsulated and externally attached structures are consistently lower than those of the concentric core-shell structure by 30–80 % for different BC sizes (Figs. 5 and 6). This is because the relatively open coating structure leads to inefficient lensing effect for partially encapsulated and externally attached structures, in which a part of BC aggregates is shielded from interaction with incident photons that are backscattered by the attached nonabsorbing coating material. Adachi et al. (2010) showed that the concentric core-shell structure has a 20–30 % stronger absorption than BC aggregates that are fully embedded within host sulfate. Thus, the partially encapsulated structure with only a part of BC aggregates embedded inside coating material in the present study could further decrease the absorption and lead to much smaller absorption values than a concentric core-shell structure. Kahnert et al. (2013) found that the difference in BC absorption between concentric core-shell and encapsulated structures strongly depends on particle size, BC volume fraction, and wavelength, based on the DDA calculation. Interestingly, we found that the absorption of partially encapsulated structure is 10–40 % weaker than that of externally attached structure with larger differences for thicker coating, while their scattering cross sections are similar (differences 5 %). The preceding analysis demonstrates that coating structures exert a significant impact on BC optical properties. Thus, in order to produce reliable and accurate estimates of BC radiative forcing in climate models, the development of a realistic BC coating morphology parameterization appears to be essential, which, however, could be a challenging task in view of limited observations available at the present time.
Evolution of BC absorption and scattering
Figure 7 shows the enhancement in absorption and scattering during BC aging from freshly emitted aggregates (Stage I) to BC coated by HSO (Stage II) and by HSO–HO (Stage III) for different BC coating structures and sizes. The measured BC absorption increases by 10–45 % due to coating, while the concentric core-shell model results in a 20–65 % absorption increase depending on BC sizes and aging stages. This implies that assuming a concentric core-shell shape could overestimate BC radiative forcing. Adachi et al. (2010) found that using a more realistic BC coating morphology from field measurements leads to about 20 % less BC DRF than using a concentric core-shell shape.
Moreover, coated BC particles with closed-cell structures enhance absorption by 50–100 % for Stage II and more than 100 % after hygroscopic growth (Fig. 7). In contrast, the open-cell structures produce less than 10 % increase in absorption during aging for of 245 and 320 nm, while the enhancement tends to be stronger for smaller BC size ( 155 nm). Surprisingly, we found that the partially encapsulated and externally attached BC structures have a weaker absorption than fresh BC aggregates, probably because that the two structures in the absence of fully embedded shape have no efficient lensing effect and that the nonabsorbing coating material blocks the photons coming from behind BC aggregates and produces a shadowing effect (Liu and Mishchenko, 2007). This shadowing effect could also explain the decreasing BC absorption for partially encapsulated, externally attached, and open-cell structures when coating material increases during Stages II to III. Adachi and Buseck (2013) and Scarnato et al. (2013) found that BC particles attached to or partially immersed in host material, instead of fully embedded within them, do not show noticeable increases in BC absorption relative to uncoated aggregates based on DDA calculations. Bond et al. (2006) recommended a 50 % increase in BC absorption to account for the averaged coating effect during atmospheric aging. However, in light of the preceding analysis, the morphology, composition, and amount of coating play significant roles in altering the BC optical properties during aging. It appears that a fixed enhancement factor may not represent the realistic increase in BC absorption due to complex coating, particularly over regions with highly heterogeneous aging conditions.
Compared with absorption enhancement, BC coating results in a much larger increase in scattering, with a greater enhancement for a larger amount of coating material (Fig. 7). The measured scattering cross sections from laboratory experiments for different BC sizes increase by a factor of 5–6 from Stage I to II and a factor of 11–13 from Stage I to III. Theoretical calculations show that the increase in scattering from Stage I to II varies from a factor of 3 to 8 for of 245 and 320 nm depending on coating morphology, while both the magnitude and variation of enhancement are much larger for of 155 nm ranging from a factor of 6 to 15. After hygroscopic growth (Stage III), BC scattering further increases by 20–200 % for different coating structures relative to that at Stage II. Cheng et al. (2009) observed that the increase in BC scattering, due to both the increased amount of coating and the transition of uncoated to coated BC, can reach up to a factor of 8–10 within several hours' aging at a polluted site in northeastern China, which is comparable to laboratory measurements and theoretical calculations presented above.
Atmospheric implications
Our theoretical calculations have shown that BC absorption and scattering are highly sensitive to coating morphology and the amount of coating at different aging stages. This suggests that the change of BC coating states (e.g., coating thickness, morphology, and composition) during the aging process in the real atmosphere could substantially affect BC radiative properties and thus its climatic effects. Metcalf et al. (2012) observed that the mean BC coating thickness increases from 95 nm over urban areas within boundary layers to 150 nm in its downwind regions and 190 nm in the free troposphere, with number fractions of thickly coated BC in the free troposphere and downwind regions higher than near the source by a factor of 2. Such large variations in BC coating thickness and number fraction of thickly coated BC during aging have also been observed over the tropics from the ground to high altitudes (Schwarz et al., 2008), implying a strong dependence of BC coating state on aging condition and timescale that BC particles have experienced. Furthermore, atmospheric observations also suggest large variability in the composition of coating materials (Moteki et al., 2007; Metcalf et al., 2012) and coating morphology (China et al., 2013, 2015) during BC aging under different atmospheric conditions. Thus, better characterizations of BC coating mass, composition, and morphology during aging are critically important to accurately estimate BC radiative effects.
However, many global models tend to use fixed BC optical properties or simplified core-shell models for the computation of BC radiative effects (Bond et al., 2013), which may not be representative and sufficiently accurate in view of various BC coating states in the real atmosphere. This study suggests that a reliable estimate of BC radiative effects in climate models would require the representation of a dynamic BC aging process with realistic coating structures, especially for regional analysis with highly heterogeneous atmospheric conditions.
Conclusions
We developed a theoretical model that accounts for three typical BC aging stages, including freshly emitted aggregates, BC coated by soluble material, and coated BC particles after further hygroscopic growth. The GOS approach was used to compute BC absorption and scattering at each aging stage, which was coupled with a stochastic procedure to construct different BC structures. The theoretical calculations were compared with laboratory measurements, followed by a systematic analysis of uncertainties associated with BC RI and morphology. Finally, we discussed atmospheric implications of our results in the assessment of BC radiative effects.
Theoretical calculations yielded consistent extinction (sum of absorption and scattering) cross sections for fresh BC aggregates at Stage I, with differences of less than 20 % compared with measurements. Theoretical calculations underestimated BC absorption by up to 25 %, while overestimated BC scattering for different sizes, because of uncertainties associated with both theoretical calculations for small particles and scattering measurements in laboratory experiments. Sensitivity calculations showed that variation of the extinction and absorption cross sections of fresh BC aggregates is 20–40 % due to the use of upper and lower bounds of BC RIs, while variation of the scattering cross section ranges from 50 to 65 % with a higher sensitivity for larger BC sizes. We also found that the optical cross sections of BC aggregates are sensitive to fractal dimension, but insensitive to the size of primary spherules. Using volume-equivalent spheres instead of aggregates decreased the BC absorption at Stage I.
The measured extinction, absorption, and scattering cross sections of coated BC were generally captured (differences 30 %) by theoretical calculations using a concentric core-shell structure for Stages II and III. However, theoretical calculations tend to overestimate extinction and absorption for of 155 and 245 nm at Stages II and III, while the scattering tends to be underestimated for larger BC sizes at Stage III, particularly for of 320 nm due partly to the uncertainty associated with HSO–HO coating mass. Sensitivity analyses showed that the effects of BC RI on extinction and absorption for coated BC were much smaller than that for fresh BC aggregates. The off-center core-shell structure resulted in up to 30 % less absorption and scattering cross sections than the concentric core-shell structure. The open-cell structure tended to have weaker absorption and stronger scattering than the concentric core-shell structure, while the reverse is true for the closed-cell structure. Compared with the concentric core-shell structure, the partially encapsulated and externally attached structures had substantially smaller absorption and scattering cross sections due to the lack of efficient lensing effects.
Theoretical calculations showed that using a concentric core-shell structure overestimated the measured enhancement in BC absorption by up to 30 % during aging. The closed-cell structure led to increases in BC absorption higher than measured values by a factor of 2, while the open-cell structure did not show a noticeable increase in absorption for of 245 and 320 nm during aging. The partially encapsulated and externally attached coating structures had a weaker absorption than fresh BC aggregates, likely produced by the shadowing effect from nonabsorbing coating material as well as the lack of efficient lensing effect. The increase in BC scattering during aging was much stronger than absorption, ranging from a factor of 3 to 24 depending on BC size, morphology, and aging stage. Thus, the present analysis showed that BC optical properties are highly sensitive to BC morphology and coating mass at different aging stages.
Our theoretical calculations suggested that the evolution of BC coating states (e.g., coating thickness, morphology, and composition) during aging in the real atmosphere could exert significant impacts on BC radiative properties and thus its climatic effects, particularly over regions with high heterogeneity. Therefore, to accurately estimate BC radiative effects requires the incorporation of a dynamic BC aging process accounting for realistic coating structures in climate models.
The Supplement related to this article is available online at
Acknowledgements
This research was supported by the NSF under grant AGS-0946315 and AGS-1523296, by the DOE Earth System Modeling program under grant DESC0006742, and by subcontract S100097 from the Texas A&M Research Foundation, which is sponsored by NASA under grant NNX11AK39G. Pacific Northwest National Laboratory is operated for DOE by Battelle Memorial Institute under contract DE-AC05-76RL01830. R. Zhang acknowledges the support by the Robert A. Welch Foundation (A-1417). Users can access the data in this study through the corresponding author. Edited by: M. Shiraiwa
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
© 2015. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
Abstract
A theoretical black carbon (BC) aging model is developed to account for three typical evolution stages, namely, freshly emitted aggregates, BC coated by soluble material, and BC particles undergoing further hygroscopic growth. The geometric-optics surface-wave (GOS) approach is employed to compute the BC single-scattering properties at each aging stage, which are subsequently compared with laboratory measurements. Theoretical calculations are consistent with measurements in extinction and absorption cross sections for fresh BC aggregates with different BC sizes (i.e., mobility diameters of 155, 245, and 320 nm), with differences of
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details



1 Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles (UCLA), CA 90095, USA; Joint Institute for Regional Earth System Science and Engineering, University of California, Los Angeles (UCLA), CA 90095, USA
2 Department of Atmospheric Sciences, Texas A&M, College Station, TX 77845, USA
3 Pacific Northwest National Laboratory, Richland, WA 99352, USA