the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Measurement report: Stoichiometry of dissolved iron and aluminum as an indicator of the factors controlling the fractional solubility of aerosol iron – results of the annual observations of size-fractionated aerosol particles in Japan
Aya Sakaguchi
Yoshiaki Yamakawa
Chihiro Miyamoto
Minako Kurisu
Yoshio Takahashi
The atmospheric deposition of iron (Fe) promotes primary production in the surface ocean, which results in the enhanced uptake of carbon dioxide into surface seawater. Given that microorganisms in seawater utilize dissolved Fe (d-Fe) as a nutrient, the bioavailability of Fe in aerosol particles depends on its solubility. However, the factors controlling fractional Fe solubility (Fesol %) in aerosol particles have not been fully understood. This study performed annual observations of the total and dissolved metal concentrations in size-fractionated (seven fractions) aerosol particles at Higashi-Hiroshima, Japan. The feasibility of the molar concentration ratio of d-Fe relative to dissolved Al ([d-Fe] [d-Al]) as an indicator of sources of d-Fe in aerosol particles was investigated because this ratio is likely dependent on the emission sources of Fe (e.g., mineral dust, fly ash, and anthropogenic Fe oxides) and their dissolution processes (proton- and ligand-promoted dissolutions). Approximately 70 % of the total Fe in total suspended particulates (TSPs) was present in coarse aerosol particles, whereas about 70 % of d-Fe in TSPs was mainly found in fine aerosol particles. The average Fesol % in fine aerosol particles (11.4 ± 7.0 %) was higher than that of coarse aerosol particles (2.19 ± 2.27 %). In addition, the average ratio of [d-Fe] [d-Al] in coarse aerosol particles (0.408 ± 0.168) was lower than that in fine aerosol particles (1.15 ± 0.80). The range of [d-Fe] [d-Al] ratios in the coarse aerosol particles (0.121–0.927) was similar to that obtained by proton-promoted dissolution of mineral dust (0.1–1.0), which indicates that the d-Fe in coarse aerosol particles was derived from mineral dust. The [d-Fe] [d-Al] ratios of fine aerosol particles ranged from 0.386 to 4.67, and [d-Fe] [d-Al] ratios greater than 1.50 cannot be explained by proton- and ligand-promoted dissolutions (1.00 < [d-Fe] [d-Al] < 1.50). The [d-Fe] [d-Al] ratio correlated with the enrichment factor of Fe in fine aerosol particles (r: 0.505), which indicates that anthropogenic Fe with a high [d-Fe] [d-Al] ratio was the source of d-Fe in fine aerosol particles. The high [d-Fe] [d-Al] ratio was attributed to anthropogenic Fe oxides emitted from high-temperature combustions. Finally, the fraction of anthropogenic Fe oxides to d-Fe in TSPs was calculated based on the [d-Fe] [d-Al] ratio of aerosols and their emission source samples. As a result, the fraction of anthropogenic Fe oxides to d-Fe in TSPs varied from 1.48 % to 80.7 %. A high fraction was observed in summer when air masses originated from industrial regions in Japan. By contrast, approximately 10 % of d-Fe in the TSPs collected in spring and during Asian dust events was derived from anthropogenic Fe oxides when air masses were frequently transported from East Asia to the Pacific Ocean. Thus, mineral dust was the dominant source of d-Fe in Asian outflow to the Pacific Ocean.
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Primary production in high-nutrient, low-chlorophyll regions, such as the North Pacific, eastern Equatorial Pacific, and Southern Ocean, is limited by the depletion of dissolved Fe (d-Fe, Martin and Fitzwater, 1988; Boyd et al., 2007; Moore et al., 2013; Tagliabue et al., 2017). The atmospheric deposition of Fe activates primary production in surface seawater, which enhances the oceanic uptake of atmospheric CO2 (Martin, 1990; Martin et al., 1994; Falkowski et al., 2000; Jickells et al., 2005). In the last glacial–interglacial period, the atmospheric CO2 concentration was inversely correlated with the supply of mineral dust to the Southern Ocean (Martínez-Garcia et al., 2009, 2011, 2014). Thus, the fertilization of d-Fe in surface seawater via aerosol deposition is an important driver of the global climate system. Given that phytoplankton in surface seawater utilizes d-Fe as a nutrient, the bioavailability of Fe in aerosol particles depends on its solubility (Moore et al., 2013). Iron in aerosols has low solubility in water, and the solubility of fractional Fe (Fesol % = (d-Fe total Fe) ×100) in marine aerosols ranges from 0.1 % to 90 % (Sholkovitz et al., 2012; Mahowald et al., 2018). Factors controlling Fesol % include the differences in the Fesol % among emission sources (e.g., mineral dust versus anthropogenic aerosol) and atmospheric processes of Fe-bearing particles (Sedwick et al., 2007; Sholkovitz et al., 2009; Mahowald et al., 2018; Ito et al., 2019, 2021). In addition, previous studies revealed that the factors have size dependencies because fine aerosol particles yield higher Fesol % than coarse aerosol particles derived from either or both anthropogenic Fe and atmospheric processes (Buck et al., 2010a; Chance et al., 2015; Sakata et al., 2018; Kurisu et al., 2021; Baker and Jickells, 2006, 2017; Baker et al., 2020; Gao et al., 2019). However, the factors controlling Fesol % in aerosol particles have not been fully understood.
Source apportionment of d-Fe in aerosol particles has been conducted based on the correlation analysis of Fesol % with the concentrations and enrichment factors (EFs) of coexisting elements. The EFs of vanadium (V) and lead (Pb) are used as tracer elements of heavy-oil and coal combustion processes, respectively (Sholkovitz et al., 2009; Conway et al., 2019; Hsieh et al., 2022). The correlations of Fesol % with the EFs of V and Pb are useful for evaluating the presence of anthropogenic Fe. However, quantitative evaluation of the fraction of anthropogenic Fe in d-Fe in aerosol particles is difficult. Therefore, an indicator that can estimate the fraction of anthropogenic Fe in d-Fe in aerosols is required to evaluate quantitatively the Fe supply from aerosols to the ocean surface. The fraction of anthropogenic Fe was recently estimated using the Fe isotope ratio (δ56Fe); anthropogenic Fe has a lower δ56Fe than mineral dust (Kurisu et al., 2016a, b, 2019, 2021; Conway et al., 2019). Although the δ56Fe of total Fe in marine aerosol particles has been reported by previous studies, data on the δ56Fe of d-Fe in marine aerosol particles are limited due to analytical difficulties, including high filter blanks (Conway et al., 2019; Kurisu et al., 2021). Given that the fraction of anthropogenic Fe in d-Fe depends on the Fesol % of anthropogenic Fe and mineral dust, the contribution of anthropogenic Fe to the total Fe is not always the same as that of d-Fe. Therefore, attaining the capability to produce indicators for source estimation of d-Fe in aerosol particles with low analytical difficulty is ideal.
The stoichiometry of the mineral dissolution of major elements (e.g., Si, Al, Fe, and Mg) has been investigated to understand the dissolution processes of minerals in the environment (Acker and Bricker, 1992; Brantley et al., 2008; Bibi et al., 2011; Bray et al., 2015). The stoichiometry of mineral dissolution is controlled by acid type, pH, and ionic strength and the presence or absence of organic ligands (Brantley et al., 2008; Bray et al., 2015). Therefore, the ratios of dissolved concentrations of major elements vary depending on their dissolution processes from minerals (Acker and Bricker, 1992; Brantley et al., 2008; Bibi et al., 2011; Bray et al., 2015). However, studies on Fe dissolution from aerosols have focused exclusively on Fe and neglected other dissolved metals in aerosol particles. In general, although the stoichiometry of mineral dissolution is discussed based on the ratio of the dissolution rate of major elements versus that of Si (Acker and Bricker, 1992; Brantley et al., 2008; Bibi et al., 2011; Bray et al., 2015), the data on total and dissolved Si concentrations in aerosol particles are limited relative to those on Fe and Al concentrations (Jickells et al., 2016). Discussion of the dissolution processes of mineral dust using Mg concentration is difficult because Mg in marine aerosol particles is usually derived from sea spray aerosol. Therefore, this study focused on the molar ratio of d-Fe to dissolved Al ([d-Fe] [d-Al]) as an indicator of the sources of d-Fe in aerosol particles because (i) previous studies have frequently determined d-Fe and d-Al concentrations in aerosol particles and (ii) mineral dust is the dominant source of Fe and Al.
Iron-bearing particles derived from mineral dust and anthropogenic Fe have different chemical compositions and mineralogy. Mineral dust is mainly composed of crystalline aluminosilicates (Jeong and Achterberg, 2014; Jeong et al., 2014; Jeong, 2020). The fly ash emitted from anthropogenic high-temperature combustion processes can be categorized into two groups: non-magnetic and magnetic particles. Non-magnetic particles in fly ash consist of aluminosilicate glass (Furuya et al., 1987; Rivera et al., 2015). This fraction is dominated by poorly ordered polymerized hydroxyl Fe(III) (Rivera et al., 2015). The magnetic fraction is composed of crystalline Fe oxides (e.g., hematite and magnetite) formed through the condensation of evaporated Fe during gas cooling (Kukier et al., 2003; Fomenko et al., 2019; Czech, 2022). Magnetic and non-magnetic particles have been found in ambient aerosol particles (Li et al., 2021; Y. Zhu et al., 2020; Zhu et al., 2022). Therefore, differences in the mineralogy and chemical composition of mineral dust, magnetic, and non-magnetic particles possibly affect the [d-Fe] [d-Al] ratio in aerosol particles. The [d-Fe] [d-Al] ratio of clay minerals ranges from 0.100 to 1.00 (Kodama and Schnitzer, 1973; Lowson et al., 2005; Bibi et al., 2011; Bray et al., 2015), whereas that of fly ash emitted from coal and municipal solid-waste incinerators (MSWIs) is less than 0.100 (Seidel and Zimmels, 1998; Kim et al., 2003; Huang et al., 2007). In addition, the [d-Fe] [d-Al] ratio of aggregates of Fe oxide nanoparticles derived from anthropogenic emissions is expected to be higher than that of mineral dust and fly ash because Fe oxide nanoparticles contain minimal amounts of coexisting elements (Kukier et al., 2003; Fomenko et al., 2019). If the [d-Fe] [d-Al] ratio of mineral dust and anthropogenic Fe is generalized, the fractions of mineral dust and anthropogenic Fe in d-Fe in aerosol particles can be estimated based on the [d-Fe] [d-Al] ratio.
In 2013, the annual observation of Fe, Al, and other trace metal concentrations and their fractional solubilities in size-fractionated aerosol particles (seven fractions) was conducted in Higashi-Hiroshima, Hiroshima, Japan (Fig. 1). Air masses at the sampling site in summer were mainly derived from the domestic region of Japan, whereas air masses passing over East Asia arrived at the site in winter and spring (Fig. S1 in the Supplement). Our sample set included samples affected by Asian dust and serious haze events associated with anthropogenic emissions, which allowed us to obtain aerosol samples with considerable differences depending on the size dependence and seasonal variation expected for Fe chemistry and d-Fe sources. Ground-based long-term observations of Fesol % are important to complement the observed data on Fesol % in marine aerosols because (i) mineral dust and anthropogenic Fe (excluding ship emissions) are emitted in continental regions and (ii) the representativeness of Fesol % data obtained by ship-board observation is often problematic due to difficulties in the long-term observation of marine aerosol particles at fixed stations (Mahowald et al., 2018). In addition, mineral dust and anthropogenic Fe internally mixed with sulfate, nitrate, and organics are frequently found in the continental atmosphere, which indicates that chemical aging of Fe-bearing particles begins during transport in continental regions. Previous studies reported that atmospheric processing after passing over Japan has a small effect on the Fesol % of marine aerosol particles in the case of Fe-bearing particles during their transport from East Asia to the Pacific Ocean (Buck et al., 2013; Sakata et al., 2022). Japan is located at the rim of East Asia (or the entrance of the North Pacific Ocean), and thus it can accumulate mineral dust and anthropogenic Fe aged during their transport from East Asia to Japan. Therefore, Japan can be an important observation site for the characterization of aerosols transported to the North Pacific Ocean. This study aimed to evaluate the availability of source identification of d-Fe in aerosol particles based on [d-Fe] [d-Al] ratios and gain insights into the seasonal variability of the fractions of mineral dust and anthropogenic Fe in d-Fe in aerosols.
2.1 Aerosol sampling
Aerosol sampling was performed at Higashi-Hiroshima, Hiroshima, Japan (Fig. 1; 34.40∘ N, 132.71∘ E). Size-fractionated aerosol particles were collected using a high-volume air sampler (model 123-SL, Kimoto, Japan) with a Sierra-type cascade impactor (TE-236, Tisch Environmental Inc., USA) installed on a roof 10∘ m a.g.l. The cascade impactor had seven stages, and the aerodynamic diameters of the aerosol particles collected in each stage from stage 1 to stage 7 followed the order >10.2, 4.2–10.2, 2.1–4.2, 1.3–2.1, 0.69–1.3, 0.39–0.69, and <0.39 µm. The coarse aerosol particles were coarser than 1.3 µm (stages 1–4), whereas the fine aerosol particles were finer than 1.3 µm (stages 5–7). Aerosol particles were collected onto cellulose filters (stages 1–6: TE-230WH, Tisch Environmental Inc., USA; stage 7: Whatman 41, 8×10 in2, GE Healthcare, USA). Aerosol samplings during non-dust events were conducted every month from December 2012 to December 2013 (Table S1 in the Supplement). The flow rate of the air sampler was fixed at 0.566 m3 min−1. The typical sampling period was 2 weeks. However, if the sampling flow rate decreased due to clogging of the stage 7 filter, aerosol sampling was immediately stopped. Aerosol samplings were also performed during two dust events associated with haze and Asian dust on 31 January to 1 February 2013 and on 4 to 9 March 2013, respectively. Aerosol mass concentrations in China exceeded 600 µg m−3 at the end of January 2013 (Tian et al., 2014; Wang et al., 2014), and their transported particles can be collected during the haze event. The sampling periods for the haze and Asian dust events were 1 and 5 d, respectively. The sampling periods for haze and Asian dust events were decided based on a chemical weather forecasting system, which predicted the mass concentrations of Asian dust and sulfate aerosols (Uno et al., 2004). Backward trajectories at the altitude of 100 m were calculated using the Hybrid Single-Particle Lagrangian Integrated Trajectory model (Stein et al., 2015). The Global Data Assimilation System (GDAS 0.5∘ archive) was used to collect meteorological data. The total run time was 72 h, and the backward trajectory was calculated every 6 h. Figures S1 and S2 show the backward trajectories for non-dust and dust events, respectively.
2.2 Major ion concentrations
Aerosol particles on approximately one-fourth of the filter strips were used for the extraction of major ions (Na+, NH, K+, Mg2+, Ca2+, Cl−, NO, and SO using 5 mL ultrapure water (MQ, Merck Millipore, USA) in polypropylene vials with ultrasonication for 30 min. Suspended particles in the extract were removed using a hydrophilic polytetrafluoroethylene (PTFE) filter (φ: 0.20 µm, Dismic, Advantec, Toyo Roshi Kaisha, Ltd., Japan). All materials used for the extraction of major ions were rinsed thrice with ultrapure water before use.
Major ion concentrations were determined through ion chromatography (ICS–1100, Dionex Japan, Japan). The guard columns for cations and anions were Dionex IonPac CG12A and AG22, respectively. The separation columns for cations and anions were Dionex CS12A and AS22, respectively. The eluents for cations and anions were methanesulfonic acids and a mixed solution of 4.5 mmol L−1 Na2CO3 and 1.4 mmol L−1 NaHCO3, respectively. The detailed procedure of ion chromatography was described in the work of Sakata et al. (2014).
Non-sea-salt (nss) K+, Mg2+, Ca2+, and SO concentrations were estimated as follows:
where X is the molar concentration of either K+, Mg2+, Ca2+, or SO. The molar ratios of [K+] [Na+], [Mg2+] [Na+], [Ca2+] [Na+], and [SO] [Na+] were 0.0213, 0.113, 0.0213, and 0.0596, respectively (Nozaki, 2001).
2.3 Estimation of aerosol pH
The aerosol pH of fine aerosol particles was estimated using the thermodynamic E-AIM model IV (Clegg et al., 1998; Friese and Ebel, 2010). The calculation parameters for the model were [H+], [NH], [Na+], [Cl−], [NO], [SO], temperature, and relative humidity (RH). Ammonia gas concentration was not measured during the sampling campaign. Therefore, aerosol pH was calculated through a reverse mode that tended to overestimate aerosol acidity (Song and Osada, 2020). Previous studies have reported that nonvolatile cations (e.g., Mg2+ and Ca2+) affect the calculation results of aerosol pH (Guo et al., 2018; Pye et al., 2020). [Na+] was used as a representative of nonvolatile cations (= [Na+] + [K+] + 2 × [Mg2+] + 2 × [Ca2+]) to estimate aerosol pH because the E-AIM model IV cannot incorporate the concentrations of nonvolatile cations other than Na+ (Tao and Murphy, 2019a). The [H+] concentration in aerosol particles was estimated on the basis of charge balance. Several samples had negative [H+] concentrations and were thus excluded from the estimation of aerosol pH. In addition, E-AIM model IV cannot calculate aerosol pH when the RH is below 60 %. The average RH during each sampling period was higher than 60 %, except for those of aerosol samples collected in April and May 2013. The aerosol pH collected in April and May was calculated under the assumption of 60 % RH because the average RHs of the samples for these months were 59.4 % and 59.5 %, respectively. Aerosol pH was calculated using the following equation:
where and are the molar fraction and activity coefficient of H+, respectively.
2.4 Trace metal concentrations
Approximately one-fourth of the filter strips were used for acid digestion to determine the total trace metal concentrations. Each filter piece was digested with a mixed acid solution of 15.2 mol L−1 HNO3, 9.3 mol L−1 HCl, and 20 mol L−1 HF in a 7 mL perfluoroalkoxyalkane vial heated at 120 ∘C for 12 h (all mineral acids were procured from TAMAPURE AA-100, Tama Chemicals Co., Ltd., Japan). Subsequently, the mixed acid was evaporated to dryness. The dried residue was dissolved in 5 mL of 0.15 mol L−1 HNO3 heated at 120 ∘C for 3 h. The solution was filtered through a hydrophilic PTFE filter (φ: 0.20 µm, Dismic®, 25HP020AN, Advantec, Japan) to prepare the analytical solution. Soluble metals in aerosol particles were extracted using 5 mL ultrapure water with ultrasonication for 30 min. Then, the extracted solution was filtrated with a hydrophilic syringe PTFE filter. The filtrated solution was acidified to prepare a 0.15 mol L−1 HNO3 solution by the addition of 15.3 mol L−1 HNO3. The filtrated solutions for total and dissolved metal concentration analyses were diluted with 0.15 mol L−1 HNO3 by factors of 10–1000.
The total and dissolved metal concentrations of the sample solution were determined via inductively coupled plasma mass spectrometry (ICP–MS, Agilent 7700, Agilent, Japan). The sample introduction system consisted of a borosilicate nebulizer (MicroMist, Agilent, Japan) and a quartz Scott double-pass spray chamber. The elements in the sample solution were ionized by argon plasma (RF power: 1500 W; Ar flow for career gas: 1.0 L min−1). The ions were introduced into the detection system by passing them through nickel sampling and skimmer corns. The ion beam was focused with x-type ion lenses. Helium collision mode was used to reduce interference from oxides (e.g., 40Ar16O+ for 56Fe). Helium gas was injected into a dynamic reaction cell at a rate of 3.6 mL min−1. Then, mass selection was performed on a quadrupole system. Target metal concentrations were measured in pulse (ion-counting) mode. The sensitivity drift during measurements was corrected using the internal standard of 1 ng g−1 indium.
2.5 Estimation of EF of Fe and Fesol %
The total and dissolved metal concentrations in TSPs were calculated by the summation of the target metal concentrations in all sampling stages. Crustal and non-crustal Fe concentrations and the EF of target metals normalized by the average continental crust were calculated by using the following equations:
where M is the target metal. Iron and Al concentrations in the average continental crust (Fe Al: 0.684) were acquired by referring to Taylor (1964). Given the variability of the Fe Al ratio in crustal materials, significant enrichment of the Fe derived from anthropogenic emissions is usually recognized at EF values higher than 10.0. The EF equation suggests that about 90 % of Fe is derived from anthropogenic sources when the EF is 10.0. Given that the emission amount of crustal Fe is an order of magnitude higher than that of anthropogenic Fe, the EF for Fe in aerosol particles is usually below 10.0, except for aerosol samples collected near steel plants and in urban areas. Therefore, classification of Fe as anthropogenic Fe by the criterion EF > 10.0 substantially simplifies the origin of Fe in aerosol particles. If the variation of the Fe Al ratio in natural-source aerosol is limited in a narrow range, aerosols with EF > 2.00 can still be evaluated as aerosol samples containing an anthropogenic Fe component to a certain degree. The small variability of the Fe Al ratio in desert soil in East Asia was confirmed (average ± 1σ standard deviation (avg ± 1σ): 0.555 ± 0.170; range: 0.294–1.05; Nishikawa et al., 2013; Ding et al., 2001; Cao et al., 2008; X. Liu et al., 2022, and references therein). The Fe Al ratio in mineral dust exhibits a small variability, and thus enrichment of anthropogenic Fe is recognized when the EF of Fe is higher than 2.00 (Fe Al > 1.37). The Fesol % in aerosol samples was calculated by using the following equation:
3.1 Total Fe and Al concentrations
The total Fe and Al concentrations in the TSPs collected during the non-dust event were 256–1561 and 170–1716 ng m−3, respectively (Fig. 2a, b). Coarse aerosol particles accounted for 69.4 ± 7.2 % and 72.9 ± 7.6 % of the total Fe and Al in TSPs, respectively. The total Fe and Al concentrations were higher in spring (March to May) and Asian dust events than in other seasons (Fig. 2a, b). A higher Ca2+ concentration, as a marker of Asian dust, was also observed in spring than in other seasons (Fig. S3b). Therefore, the high Fe and Al concentrations in spring were due to the strong influence of Asian dust (Fig. 2a, b). The average EF of Fe in the TSPs collected from summer to fall (June to October) was 2.84 ± 0.83 when air masses mainly originated from Japan (Fig. S6a). By contrast, the average EF of Fe in the TSPs derived from East Asia in winter and spring was 1.57 ± 0.35 (Fig. S6a). Thus, the influences of anthropogenic emission on the total Fe in TSPs are more significant in the air mass derived from Japan than that from East Asia (Figs. S1, S2, and S6a). The total Al concentrations sharply decreased from May to June, whereas the decrease in the total Fe concentrations was not as significant (Fig. 2a, b). This result indicated that the aerosol particles emitted in Japan contained non-crustal Fe. In addition, the total Fe concentration in the haze event was almost the same as that in the Asian dust event, whereas the total Al concentration in the haze event was lower than that in the Asian dust event. This result demonstrated that during haze events, the total Fe concentrations were significantly enhanced by the non-crustal Fe emitted from anthropogenic emissions.
The average EFs of Fe in coarse and fine aerosol particles were 1.99 ± 0.89 and 2.49 ± 1.09, respectively (Figs. 2c and S6a). Therefore, non-crustal Fe may be present in coarse and fine aerosol particles. Non-crustal Fe concentration in coarse aerosol particles correlated with Cu, Zn, and Sb (r>0.500, Table S2). These elements in coarse aerosol particles are known as tracer elements of fragment vehicle-related materials in road dust (brake dust: Cu and Sb; tire wear: Zn) (Adachi and Tainosho, 2004; Wåhlin et al., 2006; Iijima et al., 2007; Gietl et al., 2010; Harrison et al., 2021). The correlation coefficient of non-crustal Fe with Cu as a tracer element of brake pads was the highest among these tracer elements (r: 0.747, Table S2). Fe is the most dominant metal in brake rings (up to 50 wt %), and its concentration is about an order of magnitude higher than that of Al in brake pads. Therefore, brake pads can increase the EF of Fe in aerosol particles. The EF of Fe in road dust (<40 µm) collected from tunnels and roadsides around the sampling site was 3.41 and 6.04, respectively. Therefore, resuspensions of brake pad fragments in road dust can be considered non-crustal Fe in coarse aerosol particles. This result is consistent with the finding of a previous model study, which showed that road dust was the dominant source of Cu and non-crustal Fe in PM10 in the Chugoku–Shikoku area (the locality around the sampling site) (Kajino et al., 2020).
In fine aerosol particles, non-crustal Fe concentrations were correlated with Zn, Sb, Cd, and Pb emitted from high-temperature combustions, including coal combustion, MSWI, and steel/iron industrial processes (r>0.700, Table S3; Pacyna and Pacyna, 2001; Sakata et al., 2000, 2014; Kajino et al., 2020). These high-temperature combustion processes emit nanoparticles of hematite and magnetite, which can increase the EF of Fe in fine aerosol particles. The negative δ56Fe associated with hematite derived from high-temperature combustion processes was detected in aerosol samples collected at the same sampling site (Kurisu et al., 2016a). Therefore, the nanoparticles of hematite and magnetite are likely the dominant sources of non-crustal Fe in fine aerosol particles. In addition, in fine aerosol particles, the non-crustal Fe concentration correlated with V as a tracer element of heavy-oil combustion (Nriagu and Pacyna, 1988); however, the correlation factor between non-crustal Fe and V was lower than those of Zn, Sb, Cd, and Pb (r: 0.601, Table S3). A previous model study predicted that V around the sampling site was derived from vessel emissions in the Seto Inland Sea (Kajino et al., 2020), which is located at the southern part of the sampling site (Fig. 1). Our result also showed that the V concentration in fine aerosol particles collected from July to September when air masses passed through the Seto Inland Sea was higher than that for other periods (Figs. 1 and S7a). At this point, the concentrations of Zn, Sb, and Pb did not increase (Fig. S7b–d). Therefore, in addition to the high-temperature combustion processes mentioned above, heavy-oil combustion processes around the Seto Inland Sea were possible emission sources of the non-crustal Fe in fine aerosol particles collected in summer.
3.2 Size distributions of d-Fe and d-Al concentration and their fractional solubility
The concentrations of d-Fe and Al in the TSPs collected during the non-dust event ranged from 11.4 to 65.0 ng m−3 and from 8.30 to 40.6 ng m−3, respectively (Fig. 3a, d). The Fesol % and Alsol % of the TSPs ranged from 2.00 % to 7.73 % and 1.46 % to 7.39 %, respectively (Fig. S6b, c), which were within the typical range of Fesol % in the TSPs collected from East Asia and the north-western Pacific Ocean (Buck et al., 2006, 2013; Takahashi et al., 2013; Sakata et al., 2022). Although approximately 70 % of the total Fe and Al in the TSPs were present in coarse aerosol particles, high concentrations of d-Fe and d-Al were found in fine aerosol particles (Fig. 3a, d). The average d-Fe and d-Al concentrations of fine aerosol particles were 27.3 ± 17.4 and 14.3 ± 10.9 ng m−3, which accounted for 72.0 ± 8.9 % and 53.1 ± 9.9 % of d-Fe and d-Al in the TSPs, respectively. Enrichment of d-Fe and d-Al in fine aerosol particles has been reported not only in the urban atmosphere (Fang et al., 2017; Hsieh et al., 2022; L. Liu et al., 2022) but also in the marine atmosphere (McDaniel et al., 2019; Baker et al., 2020; Sakata et al., 2022). These previous studies have reported that the higher amounts of d-Fe and d-Al in fine aerosol particles than coarse aerosol particles were caused by either or both (i) contamination of the anthropogenic aerosol with high Fesol % and Alsol % and (ii) solubilization of Fe and Al in fine aerosol particles by atmospheric processes. The average Fesol % in fine aerosol particles in this study (11.4 ± 7.0 %) was about 5 times higher than that of coarse aerosol particles (2.19 ± 2.27 %, Fig. 3b, c). In the case of Al, fine aerosol particles (8.82 ± 6.48 %) yielded about twice as much as the Alsol % of coarse aerosol particles (3.25 ± 3.41 %, Fig. 3e, f). These results indicated that the Fe in fine aerosol particles is more susceptible to dissolution in water by anthropogenic activities and chemical aging than Al. The Fesol % and Alsol % in coarse aerosol particles were higher than those in desert dust soil (typical Fesol % and Alsol %: 0.100 %). Therefore, the Fesol % and Alsol % in coarse aerosol particles increased due to anthropogenic aerosol and/or atmospheric processes, but the effect was not as pronounced as in fine aerosol particles.
3.3 Possible factor controlling Fesol % and Alsol %
3.3.1 Coarse aerosol particles
Non-crustal Fe in coarse aerosol particles was derived from brake pads and tire ware debris in road dust as mentioned above. If road dust is the dominant source of d-Fe in coarse aerosol particles, then the d-Fe concentration correlates with non-crustal Fe concentration. However, no correlation was found between non-crustal Fe and d-Fe concentrations in coarse aerosol particles (r: 0.352). Thus, road dust was not the source of d-Fe in coarse aerosol particles. This result is consistent with that of previous studies in which the Fesol % of brake pads and tire wear debris was lower than 0.01 % (Shupert et al., 2013; Halle et al., 2021).
The Fesol % and Alsol % of coarse aerosol particles increased with the decrease in aerosol diameter (Fig. 3b, c, e, f). Specific surface area is one of the factors controlling Fesol % and Alsol % in aerosol particles (Baker and Jickells, 2006, 2017; McDaniel et al., 2019), and the chemical reactivity of aerosol particles increases with the increase specific surface area (decrease in aerosol diameter). Previous studies have reported that chemical aging of coarse aerosol particles by acidic species, including HNO3 and H2SO4, solubilized Fe in aerosol particles (Takahashi et al., 2011; Zhu et al., 2022). The Fesol % and Alsol % of coarse aerosol particles correlated with the molar concentration ratios of nss-SO relative to the total Al or total Fe (Fig. 4a), [nss-SO] [total Fe], and [nss-SO] [total Al]. This result is consistent with previous findings showing that aluminosilicates in aerosol particles react preferentially with H2SO4 (Sullivan et al., 2007; Fitzgerald et al., 2015). Furthermore, our previous studies showed that the relative abundance of ferrihydrite formed by hydrolysis of Fe in coarse aerosol particles increased with the decrease in diameter (Takahashi et al., 2011; Sakata et al., 2022). These results indicate that atmospheric processes of coarse aerosol particles by H2SO4 promoted the formation of d-Fe via proton-promoted dissolution or hydrolysis of Fe. By contrast, no good correlation of Fesol % and Alsol % with [NO] [total Fe] and [NO] [total Al] was found because HNO3 reacts mainly with Ca-rich particles (e.g., CaCO3) in mineral dust (Fig. 4b, Karydis et al., 2016; Kakavas et al., 2021).
3.3.2 Fine aerosol particles
Unlike the d-Fe in coarse aerosol particles, the d-Fe concentrations in fine aerosol particles correlated with non-crustal Fe concentrations (Fig. 5a). Good correlations of d-Fe in fine aerosol particles with concentrations of V, Zn, Sb, and Pb as tracer elements for high-temperature combustions were also found (Fig. 5b–e). The correlation coefficient between d-Fe and Zn was the largest (Fig. 5c). Zinc in fine aerosol particles from the sampling sites originated from various high-temperature combustions, including those in MSWIs, steel/iron industries, and coal power plants (Kajino et al., 2020). Therefore, the non-crustal Fe emitted from high-temperature combustion is one of the dominant sources of d-Fe in fine aerosol particles, although identification of specific sources of non-crustal d-Fe around the sampling site was difficult. This result is consistent with our previous study, which showed that negative δ56Fe associated with high-temperature combustions was detected in fine aerosol particles (Kurisu et al., 2016a).
In addition to the input of non-crustal Fe with high Fesol % in fine aerosol particles, aerosol acidification resulted in the high Fesol % and Alsol % in fine aerosol particles (Fang et al., 2017; Sakata et al., 2022). Along with coarse aerosol particles, Fesol % and Alsol % in fine aerosol particles did not correlate with [NO] [total Fe] and [NO] [total Al] due to the preferential reaction of HNO3 with Ca2+ (Fig. 4d). The Fesol % and Alsol % correlated with [nss-SO] [total Fe] and [nss-SO] [total Al], respectively (Fig. 4c). Moreover, these solubilities increased with the decrease in aerosol pH (Fig. 4e), which indicates that acidification of fine aerosol particles by H2SO4 plays a significant role in Fe solubilization. These results are reasonable and supported by previous studies reporting that mineral dust and anthropogenic Fe in fine aerosol particles were covered by sulfate, and internal mixing of these particles with sulfate promoted the dissolution of Fe (Sullivan et al., 2007; Fitzgerald et al., 2015; Li et al., 2017, Y. Zhu et al., 2020; Zhu et al., 2022). However, compared with the correlation factor of Fesol % with [nss-SO] [total Fe], coarse aerosol particles yielded a higher correlation factor than fine aerosol particles (Fig. 4a, c). Similar results have been reported by previous studies on Fesol % in China, which indicated the presence of anthropogenic Fe with high Fesol % as one of the reasons for the low value of the correlation factor (Zhang et al., 2022, 2023). Therefore, the low correlation between Fesol % and [nss-SO] [total Fe] of fine aerosol particles implied that acidification of mineral dust was not the sole factor controlling Fesol %.
4.1 [d-Fe] [d-Al] ratio in coarse aerosol particles and mineral dust
Correlation analysis between non-crustal Fe and d-Fe concentrations revealed that non-crustal Fe contributed to the source of d-Fe in fine aerosol particles but not in coarse aerosol particles. Correlation analysis is a simple method used to evaluate emission sources of d-Fe in aerosol particles. However, quantitative estimations of the fraction of non-crustal Fe to d-Fe in aerosol particles present a challenge. Therefore, a quantitative indicator is preferable for the assessment of the relative abundance of non-crustal Fe to d-Fe. This study investigated the evaluation of the fraction of non-crustal Fe to d-Fe using the [d-Fe] [d-Al] ratio. One of the reasons is that the [d-Fe] [d-Al] ratio in mineral dust differs from that in non-crustal sources, as will be discussed below (Fig. 6a). In addition, the [d-Fe] [d-Al] ratio may vary depending on the extraction method and aging process of aerosol particles (Fig. 6a, e.g., proton-promoted versus ligand-promoted dissolutions). The [d-Fe] [d-Al] ratio in fine aerosol particles (avg ± 1σ: 1.15 ± 0.80) differed from that in coarse aerosol particles (Fig. 6b, avg ± 1σ: 0.408 ± 0.168). With the evaluation of the fraction of non-crustal Fe to d-Fe in aerosol particles, the [d-Fe] [d-Al] ratios of crustal and non-crustal Fe can be generalized.
Biotite, illite, and Fe-rich chlorite are considered representative mineral species of aluminosilicates in aerosol particles because they are detected in aerosol particles collected in East Asia (Takahashi et al., 2011; Kurisu et al., 2016a; Sakata et al., 2022). When Fe and Al in these aluminosilicates were dissolved by proton-promoted dissolution (pH 1.0–7.0) under oxic conditions, the [d-Fe] [d-Al] ratios of biotite, illite, and Fe-rich chlorite were within 0.427–0.930 (avg ± 1σ: 0.776 ± 0.152), 0.156–0.689 (avg ± 1σ: 0.404 ± 0.189), and 0.142–1.03 (avg ± 1σ: 0.699 ± 0.303), respectively (Fig. 6a; Kodama and Schnitzer, 1973; Lowson et al., 2005; Bibi et al., 2015; Bray et al., 2015). In addition, the average [d-Fe] [d-Al] ratios of Asian dust, Saharan dust, and Arizona test dusts obtained by proton-promoted dissolution were 0.238 ± 0.201, 0.163 ± 0.157, and 0.230 ± 0.009, respectively (Fig. 6a, Desboeufs et al., 2001; Duvall et al., 2008; Shi et al., 2011). The [d-Fe] [d-Al] ratio decreased with the increase in pH due to either or both the preferential retention of Fe in the mineral phase and precipitation of secondary ferrihydrite under near-neutral conditions (Fig. S8, Kodama and Schnitzer, 1973; Desboeufs et al., 2001; Lowson et al., 2005; Bray et al., 2015). Thus, the [d-Fe] [d-Al] ratio obtained from the proton-promoted dissolution of the mineral dust was between 0.100 and 1.00.
Organic ligands promote the dissolution of Fe from the mineral phase through the direct complexation of organic ligands with Fe at the mineral surface and reduction of the saturation index of inorganic Fe in aqueous phase due to the formation of organic complexes of Fe (Chen and Grassian, 2013; Paris and Desboefus, 2013; Wang et al., 2017). The [d-Fe] [d-Al] ratios of biotite and Fe-rich chlorite associated with ligand-promoted dissolution were 0.795–3.83 (avg ± 1σ: 1.20 ± 0.66) and 1.19–1.37 (avg ± 1σ: 1.31 ± 0.06), respectively (Kodama and Schnitzer, 1973; Bray et al., 2015). A previous study showed that the [d-Fe] [d-Al] ratios of coarse aerosol particles extracted by 20 mmol L−1 oxalate at pH 4.7 (1.31 ± 0.42) were higher than that of ultrapure water extraction (0.354 ± 0.714) (“Coarse aerosols (Proton)” and “Coarse aerosols (Ligand)” in Fig. 6a; Kurisu et al., 2019). Thus, the [d-Fe] [d-Al] ratio associated with ligand-promoted dissolution was higher than that associated with proton-promoted dissolution (Fig. 6a). The higher stability constant (log K) of Fe3+ than that of Al3+ with organic ligands (e.g., log K of AlC2O: 7.73; log K of FeC2O: 9.15) caused the preferential dissolution of Fe over Al from mineral dust, which increased the [d-Fe] [d-Al] ratio.
The [d-Fe] [d-Al] ratio of coarse aerosol particles collected by this study (n=60, average: 0.121–0.927) was within the range of [d-Fe] [d-Al] ratios of mineral dust that underwent proton-promoted dissolutions, and it increased with the increase in Fesol % (Fig. 6b, r: 0.552). As previously mentioned, [d-Fe] [d-Al] and Fesol % obtained by proton-promoted dissolution of mineral dust increased with the decrease in pH, which is consistent with the correlation between Fesol % and [nss-SO] [total Fe] in coarse aerosol particles (Fig. 4a). Therefore, the proton-promoted dissolution of mineral dust is the dominant source of d-Fe in coarse aerosol particles. By contrast, no coarse aerosol particles had [d-Fe] [d-Al] ratios higher than 1.0 (Fig. 6b), which indicates that the effect of organic ligands on the solubilization of Fe and Al in coarse aerosol particles was insignificant. In addition, the non-crustal Fe derived from road dust was not a factor controlling the [d-Fe] [d-Al] ratio in coarse aerosol particles due to the lack of correlation between the [d-Fe] [d-Al] ratio and EF of Fe. This result is reasonable because the Fesol % of brake pads and tire wear debris was less than 0.01 % (Shupert et al., 2013; Halle et al., 2021).
4.2 [d-Fe] [d-Al] ratio in fine aerosol particles and their emissions
The average [d-Fe] [d-Al] ratio of fine aerosol particles (n=45; avg ± 1σ: 1.15 ± 0.80; range: 0.386–4.67) was higher than those of coarse aerosol particles and mineral dust (Fig. 6a, b). The [d-Fe] [d-Al] ratios of several fine aerosol particles exceeded 1.5, which was beyond the range of the ratio of mineral dust that underwent ligand-promoted dissolutions (Fig. 6a, b). Given the good correlation between the [d-Fe] [d-Al] ratio and EF of Fe (r: 0.505), the [d-Fe] [d-Al] ratio higher than 1.5 was attributed to non-crustal Fe (Fig. 6c). The non-crustal Fe in fine aerosol particles was derived from fly ash produced by high-temperature combustions, including steel/iron industrial processes, MSWI, and coal and fuel oil combustion. Fly ash contains two types of particles, namely, magnetic and non-magnetic particles (Kukier et al., 2003; Fomenko et al., 2021). Given the different elemental compositions and Fe species of between magnetic and non-magnetic particles, the influences of these particles on the [d-Fe] [d-Al] ratio and Fesol % in fine aerosol particles were evaluated separately
4.3 [d-Fe] [d-Al] ratio of non-crustal Fe: magnetic particles
The mass fraction of magnetic particles accounts for a small percentage of the total fly ash mass (Hansen et al., 1981), but up to 90 % Fe in fly ash was present as magnetic particles (Kukier et al., 2003). Iron species of magnetic particles in fly ash are mainly composed of Fe oxides, including hematite and magnetite. The iron concentration in magnetic particles reaches up to 60 %–70 %, whereas that of Al typically amounts to up to 10 % (Kukier et al., 2003; Fomenko et al., 2021). This result indicated that Fe in magnetic particles in fly ash can increase the EF of fine aerosol particles.
Previous studies have reported that d-Fe in fine aerosol particles yielded negative δ56Fe (Kurisu et al., 2016a, 2019), and recent research showed negative δ56Fe in magnetic particles in PM2.5 (Zuo et al., 2021). The magnetic particles in fine fractions (<1.0 µm) are considered formed by either or both the fragmentation of large particles and condensation of vaporized Fe. The Fe oxides formed by condensation of vaporized Fe (hereafter high-temp-FeOx) are one of the important sources of d-Fe in fine aerosol particles because the high-temp-FeOx yield negative δ56Fe, which is formed by kinetic Fe isotope fractionation during vaporization (Kurisu et al., 2016a, 2019). The high-temp-FeOx can increase the [d-Fe] [d-Al] ratio of fine aerosol particles because the [d-Fe] [d-Al] ratio of fine aerosol particles with low δ56Fe ( ‰) collected near a steel plant was higher than 1.5 when extracted with proton-promoted (ultrapure water) and ligand-promoted (20 mmol L−1 oxalic acid at pH 4.7) dissolutions (“Anthropogenic Fe in fine aerosols (Proton)” and “Anthropogenic Fe in fine aerosols (Ligand)” in Fig. 6a; Kurisu et al., 2019). However, the Fesol % in magnetic particles in coal fly ash was less than 0.100 % in weakly acidic solutions (Kukier et al., 2003), which was considerably lower than the Fesol % in fine aerosol particles (11.4 ± 7.0 %). As previously mentioned, the Fesol % in fine aerosol particles increased with the increase in [nss-SO] [total Fe] and with the decrease in aerosol pH (Fig. 4c, e, respectively). In addition, at a high Fesol % (>10 %), the aerosol pH was lower than 3.0, which was consistent with previous observations (Tao and Murphy, 2019b). Therefore, aerosol acidification is also a dominant factor that controls Fesol % in fine aerosol particles.
As for fine aerosol particles with [d-Fe] [d-Al] between 1.00 and 1.50, the effect of ligand-promoted dissolution of mineral particles should be considered (Fig. 6b). If ligand-promoted dissolution of mineral dust is the dominant source of d-Fe in fine aerosol particles, the correlation between the [d-Fe] [d-Al] ratio and EF of Fe should not be observed because the EF of mineral dust should be about 1.00. Therefore, the high [d-Fe] [d-Al] ratio in fine aerosol particles was attributed to the presence of high-temp-FeOx rather than ligand-promoted dissolution of mineral dust.
4.4 [d-Fe] [d-Al] ratio of non-crustal Fe: non-magnetic fraction of fly ash
Non-magnetic particles are mainly composed of amorphous aluminosilicate glasses, which are formed by the melting of crystalline aluminosilicate or chemical reactions of melted Al2O3 and SiO2 (Zhang et al., 2007). Although previous studies did not perform the separation of magnetic and non-magnetic particles, the average [d-Fe] [d-Al] ratio of coal and MSWI fly ash under acidic and circumneutral conditions was 0.104 ± 0.075 (Fig. 6a, Seidel and Zimmels, 1998; Praharaj et al., 2002; Kim et al., 2003; Huang et al., 2007; Chang et al., 2009; Gitari et al., 2009; Komonweeraket et al., 2015). Given the high [d-Fe] [d-Al] ratio in the magnetic particles mentioned above, the [d-Fe] [d-Al] ratio of non-magnetic particles should be less than 0.1 (Fig. 6a). Such a low [d-Fe] [d-Al] ratio has not been detected in fine aerosol particles, which indicates that non-magnetic aluminosilicate glass in fly ash is not a dominant source of d-Fe (Fig. 6b). Furthermore, the EF of Fe in non-magnetic aluminosilicate glass emitted from MSWI and coal fly ash is almost 1, which cannot explain the correlation between EF and Fesol % for these particles (Sakata et al., 2022; Li et al., 2022). Therefore, the non-magnetic aluminosilicate glass derived from coal combustion and MSWI is possibly not a dominant source of aerosol particles with high Fesol % and [d-Fe] [d-Al] ratio in fine aerosol particles.
In the case of heavy-oil combustion, Fesol % in oil fly ash can reach 80 % under circumneutral pH conditions due to the presence of water-soluble Fe(III) sulfate (Schroth et al., 2009; Oakes et al., 2012). In addition, the fly ash emitted from heavy-oil combustions may be a source of d-Fe in fine aerosol particles collected in summer. Despite the limited data, the [d-Fe] [d-Al] ratios of oil fly ash reached 0.403, 1.07, and 7.00 at pH 5.7, 4.7, and −0.3, respectively (Akita et al., 1995; Desboeufs et al., 2001). With the assumption of a linear relationship between the dissolution pH and the [d-Fe] [d-Al] ratio of heavy-oil fly ash, the expected [d-Fe] [d-Al] ratio of heavy-oil ash was approximately 4.0 at the average aerosol pH in fine aerosol particles collected in summer (average: 2.11 ± 0.45). However, heavy-oil fly ash was not the source of fine aerosol particles with the high EF of Fe and the [d-Fe] [d-Al] ratio because the EF of Fe in heavy-oil fly ash was almost 1.0 as well as non-magnetic aluminosilicates of coal and MSWI (Sakata et al., 2017).
4.5 Fractions of crustal Fe and high-temp-FeOx in d-Fe and their Fesol %
4.5.1 Estimation method for the fractions of crustal and high-temp-FeOx and their Fesol %
The fractions of d-Fe derived from crustal Fe and high-temp-FeOx in d-Fe in fine aerosol particles were estimated based on the [d-Fe] [d-Al] ratio. Hereafter, the fractions of d-Fe derived from crustal Fe and high-temp-FeOx are denoted as Fcrust and Fanthro, respectively. In consideration of the binary mixing of d-Fe derived from mineral dust and high-temp-FeOx, the Fanthro in fine aerosol particles and Fanthro in TSPs (Fanthro-TSP) were estimated with the following equations:
where ([d-Fe] [d-Al])aerosol is the [d-Fe] [d-Al] ratio in aerosol particles. The ([d-Fe] [d-Al])crust and ([d-Fe] [d-Al])anthro are the representative values of [d-Fe] [d-Al] ratios of mineral dust and anthropogenic Fe, respectively. Here, the ([d-Fe] [d-Al])crust and ([d-Fe] [d-Al])anthro were defined based on our observational results. The average [d-Fe] [d-Al] ratio in coarse aerosol particles (0.408) was used as a representative ([d-Fe] [d-Al])crust, and its value was within the range of proton-promoted dissolution of mineral dust (Fig. 6a, b). Given that the ([d-Fe] [d-Al])anthro has not been reported by previous studies, its two types were used in the calculation. The ([d-Fe] [d-Al])anthro was 4.67, which was the highest value observed in fine aerosol particles. Another ([d-Fe] [d-Al])anthro was the average [d-Fe] [d-Al] ratio of fine aerosol particles with [d-Fe] [d-Al] ratios higher than 1.5. At this time, the ([d-Fe] [d-Al])anthro was 2.08. When the average [d-Fe] [d-Al] was used for the calculation, the Fanthro was higher than the value calculated by the highest([d-Fe] [d-Al]anthro (Fig. S9a, b). Fanthro was calculated using the average ([d-Fe] [d-Al])anthro to avoid underestimation.
Finally, the Fesol % of crustal and high-temp-FeOx (crustal-Fesol % and anthro-Fesol %) in fine aerosol particles were estimated through the following equations:
Crustal and non-crustal Fe concentrations were calculated using Eqs. (3) and (4), respectively.
4.5.2 Size dependence and seasonal variation of Fanthro
The annual average Fanthro-TSP was 19.9 ± 19.2 % (Fig. 7a; range: 1.48 %–80.7 %). The Fanthro-TSP was higher in summer–fall with the influence of Japanese air mass (average: 29.4 ± 25.8 %; range: 9.41 %–80.7 %) than in winter–spring with the influence of Asian outflow (Fig. 7a; average: 13.5 ± 10.6 %; range: 1.48 %–34.4 %). The high Fanthro-TSP in summer was attributed to the high EF of Fe and the [d-Fe] [d-Al] ratio in the season. From the viewpoint of size dependence of Fanthro, the largest Fanthro in summer–fall and winter–spring was found in the finest and 0.39–0.69 µm fractions, respectively (Fig. 7b). These results are consistent with the source apportionment of Fe using δ56Fe at the same sampling site because (i) the contribution of anthropogenic Fe to d-Fe in fine aerosol particles was more significant in summer than in spring due to the low δ56Fe and (ii) the lowest δ56Fe was found in the finest and 0.39–0.69 µm fractions in summer and spring, respectively. Thus, the source estimation of Fe using [d-Fe] [d-Al] is consistent with that which uses δ56Fe.
Given the Fe supply to the Pacific Ocean, spring is the most important season throughout the year because approximately half of aerosol transport events from East Asia to the Pacific Ocean occurred in spring between 2007 and 2016, and they were mainly associated with mineral dust events (Q. Zhu, 2020). In addition, atmospheric Fe is supplied to the surface ocean by an episodic dust event that accounts for approximately 30 %–90 % of annual Fe depositions within 5 % of the days in a year (Mahowald et al., 2009). In consideration of these facts with the estimation results of Fanthro-TSP and Fcrust-TSP, mineral dust was the dominant source of d-Fe in aerosol particles deposited in the North Pacific Ocean (Fig. 7a). Nevertheless, the contribution of high-temp-FeOx, as a source of d-Fe in surface seawater during dust events, cannot be disregarded because the average fraction of non-crustal Fe during spring and dust events was 10.2 ± 7.6 %.
4.5.3 Crustal-Fesol % and anthro-Fesol %
The annual average crustal-Fesol % (avg ± 1σ: 14.1 ± 9.3 %) was higher than the anthro-Fesol % (avg ± 1σ: 9.35 ± 10.29 %) when the focus was on fine aerosol particles (Fig. 7c, d). This result is inconsistent with the finding of previous studies where the Fesol % of anthropogenic Fe derived from high-temperature combustion was higher than that of mineral dust (Sedwick et al., 2007; Sholkovitz et al., 2009). One of the reasons is that the Fe oxide nanoparticles were poorly solubilized at the aerosol pH of the samples obtained in this study. Marcotte et al. (2020) showed that the Fesol % of submicron Fe oxides (<1.5 %) was lower than those of submicron illite and kaolinite (about 10 %). Similar results have been obtained from the experiments on Fe dissolution from aluminosilicates and Fe oxides at pH 2.0 (particle diameter <100 µm, Journet et al., 2008). According to the results of this study, the aerosol pH of fine aerosol particles with high Fesol % (>10 %) was lower than 3.0, but almost no fine aerosol samples whose aerosol pH was lower than 1.7 were observed (Fig. 4e). Therefore, even if the Fe oxides were derived from high-temperature combustion, the significant increase in their anthro-Fesol % was unlikely without sufficient acidification. Another reason is that mineral dust with a low Fesol % was mainly present in coarse aerosol particles. The annual average of crustal-Fesol % in TSPs was 6.52 ± 3.05 %, which was lower than that of anthro-Fesol %.
The crustal-Fesol % of fine aerosol particles in the 0.39–0.69 and 0.69–1.3 µm fractions was higher than that in the finest fraction throughout the year (Fig. 7c), which indicates that mineral dust in the 0.39–0.69 and 0.69–1.3 µm fractions was more aged than that in the finest fraction. This result is reasonable because internally mixed particles of Fe and sulfate were found in the fine aerosol particles, whose number fraction relative to the total number of Fe-bearing particles became the largest at around 700 nm rather than finer than 400 nm (Sullivan et al., 2007; Li et al., 2017; Y. Zhu et al., 2020; Zhu et al., 2022). The uptake of Fe-bearing particles into cloud water promotes internal mixing with sulfate (Li et al., 2017; Liu et al., 2018; Lin et al., 2019). However, the sufficient dissolution of Fe in fine aerosol particles at the pH condition of cloud water is unlikely (global average pH: 5.2, Shah et al., 2020), as observed in the relationship between aerosol pH and Fesol % (Fig. 4e). The aerosol pH decreased rapidly with the phase transition from cloud water to the aerosol concentration of protons in a tiny amount of aerosol liquid water content. Furthermore, the uptake coefficient of SO2 by aluminosilicates increases as they experience cloud processes, which is expected to further promote aerosol acidifications (Wang et al., 2019). Considering these facts, crustal-Fesol % in fine aerosol particles was enhanced by the aerosol–cloud water cycle during transport.
The availability of the [d-Fe] [d-Al] ratio for the evaluation of Fcrust and Fanthro in marine aerosol particles was investigated using the observational results of previous studies (Buck et al., 2006, 2010b; Shelley et al., 2018; Baker et al., 2020; Sakata et al., 2022). In general, soluble metals in aerosol particles were extracted with ultrapure water through instantaneous or batch leaching, and only Baker et al. (2020) used ammonium acetate solution with a pH of 4.7. The [d-Fe] [d-Al] ratio of the marine aerosol samples collected in the Pacific and Atlantic oceans was rarely higher than 1.0 (Fig. 8a, b). The Fanthro of TSPs collected from the Atlantic and Pacific oceans was 9.58 % and 13.4 %, respectively (Fig. 8c). In the Pacific Ocean, Fanthro was higher in the region east of 170∘ E because anthropogenic Fe in fine aerosol particles was transported farther than that in coarse mineral dust particles (Fig. 9a, Mahowald et al., 2018). By contrast, the large Fanthro in the Atlantic was detected around the coastal areas in North America and Europe (Fig. 9b). This result was consistent with the estimation of the Fanthro based on δ56Fe, which indicated that more than half of the d-Fe in Fe around the coastal regions was derived from anthropogenic Fe with a negative δ56Fe (Conway et al., 2019). However, the Fanthro of TSPs with negative δ56Fe values, which were estimated on the basis of the [d-Fe] [d-Al] ratio, was 12.4 ± 2.9 % (Fig. 8c). Thus, the Fanthro estimated by the [d-Fe] [d-Al] ratio differed from that estimated by δ56Fe. One of the reasons for this discrepancy was the limited data of the [d-Fe] [d-Al] and δ56Fe ratios for emission source samples, specifically anthropogenic emissions. The [d-Fe] [d-Al] ratio and δ56Fe of high-temp-FeOx were estimated based on the measurement values of aerosol particles due to the lack of reliable reference materials for high-temp-FeOx. By contrast, the [d-Fe] [d-Al] ratios of mineral dust and non-magnetic aluminosilicates of coal combustion and MSWI had a small effect on the uncertainty of Fanthro estimation due to the presence of reference values. Therefore, further studies involving the accumulated data on the [d-Fe] [d-Al] ratio and δ56Fe of high-temp-FeOx collected from various industrial sites are required. Currently, the accurate δ56Fe and [d-Fe] [d-Al] ratio of high-temp-FeOx may be obtained through the separation of magnetic particles, as performed by Zuo et al. (2022). The accumulated data on the previously reported values of [d-Fe] [d-Al] ratio can be used and are expected to provide insights into the time-series variation in the contribution of anthropogenic Fe to aerosols in marine aerosols.
Figure 8b shows a scatter plot of the [d-Fe] [d-Al] ratios and Fesol % of size-fractionated aerosol particles collected from the Atlantic and Pacific oceans (Baker et al., 2020; Sakata et al., 2022). The average [d-Fe] [d-Al] ratios of coarse and fine aerosol particles collected offshore of the Sahara were 0.216 ± 0.163 and 0.155 ± 0.055, respectively. These values were similar to the [d-Fe] [d-Al] ratio of Saharan dust (0.108 ± 0.061), which indicates that the d-Fe in these size-fractionated aerosol samples originated from Saharan dust. Iron in the size-fractionated aerosol particles collected in the western Pacific Ocean was also derived from mineral dust regardless of aerosol diameter because the EF of Fe in all size fractions was almost 1.00 (Sakata et al., 2022). The average [d-Fe] [d-Al] ratio of coarse aerosol particles collected above the Pacific Ocean (0.378 ± 0.104) was slightly higher than the average [d-Fe] [d-Al] ratio of Asian dust (0.238 ± 0.201) but was similar to that of coarse aerosol particles collected in this study (0.408 ± 0.168). Therefore, the d-Fe in these samples was derived from the hydrolysis or proton-promoted dissolution of mineral dust. Although the Fe in coarse aerosol particles collected in the Atlantic and Pacific oceans was derived from mineral dust, the [d-Fe] [d-Al] ratios of the coarse and fine aerosol particles above the Atlantic Ocean were lower than that of coarse aerosol particles collected in the Pacific Ocean. The differences in mineralogical compositions of mineral dust in the hinterlands account for differences in the ratios of aerosol particles collected in the Atlantic and Pacific oceans. Therefore, measurement of the [d-Fe] [d-Al] ratio of soil samples around the sampling site is important to determine the representative [d-Fe] [d-Al] ratio of mineral particles in aerosol particles.
The high Fesol % (>10 %) of fine aerosol particles in the Pacific was attributed to ferric organic complexes of humic-like substances (Fe(III)-HULIS, Sakata et al. 2022). The [d-Fe] [d-Al] ratio of fine aerosol particles containing Fe(III)-HULIS was expected to be between 1.0 and 1.5 due to ligand-promoted dissolution. However, the obtained [d-Fe] [d-Al] ratio for these particles was 0.440 ± 0.117 (range: 0.255–0.567), which was consistent with the ratio of Asian dust that underwent proton-promoted dissolution. A previous study reported that aerosol acidification of aluminosilicates enhanced the Fesol % of samples; Fe(III)-HULIS then formed via complexation reactions in cloud water (Sakata et al., 2022). The [d-Fe] [d-Al] ratio may not change even if the Fe species was altered by atmospheric processes after Fe solubilization. However, further investigation of this point is required. Moreover, to evaluate source and dissolution processes using the [d-Fe] [d-Al] ratio, we preferred the determination of the [d-Fe] [d-Al] ratio via ultrapure water extraction without organic ligands (e.g., oxalate and acetate) because the ratio is altered if the extracted solution contains organic ligands (e.g., “Coarse aerosols (Proton)” versus “Coarse aerosols (Ligand)”, Fig. 6a). The data on the [d-Fe] [d-Al] ratio of size-fractionated marine aerosol particles under the effect of high-temp-FeOx up to this point have not been published. Therefore, further studies on the [d-Fe] [d-Al] ratio of marine aerosol particles influenced by high-temp-FeOx are required. If future studies detect high [d-Fe] [d-Al] ratios in marine aerosol samples that are strongly affected by high-temp-FeOx, then the [d-Fe] [d-Al] ratio will be a powerful tool for estimation of the fraction of crustal and non-crustal Fe in d-Fe in marine aerosol particles.
Annual observations of the total and d-Fe and Al concentrations in size-fractionated aerosol particles were conducted at the eastern end of East Asia. The total Fe and Al concentrations were mainly distributed in coarse aerosol particles, whereas d-Fe and d-Al concentrations dominated fine aerosol particles. Given the higher d-Fe concentration and longer residence time of fine aerosol particles than coarse aerosol particles, the atmospheric deposition of fine aerosol particles was the dominant source of d-Fe in the surface ocean. The [d-Fe] [d-Al] ratio of coarse aerosol particles (0.408 ± 0.168) was lower than that of fine aerosol particles (1.15 ± 0.80). Thus, the sources of d-Fe differed between coarse and fine aerosol particles. The [d-Fe] [d-Al] ratio of coarse aerosol particles was similar to that observed for Fe dissolved via proton-promoted dissolution. The Fesol % increased as the surfaces of coarse particles became hygroscopic through the reaction with sulfuric acid. This effect intensified with the reduction in particle size. The fine aerosol particles presented a wide range of [d-Fe] [d-Al] ratios (0.386–4.67). The correlation of the [d-Fe] [d-Al] ratio of the fine aerosol particles with the EF of Fe indicated that the high [d-Fe] [d-Al] ratios (>1.5) can be attributed to non-crustal Fe. High-temp FeOx in magnetic particles were likely the dominant species of non-crustal Fe with high [d-Fe] [d-Al] ratios. The Fcrust and Fanthro were evaluated using the [d-Fe] [d-Al] ratios in aerosol particles and their emission source samples. Approximately 80 % of d-Fe in TSPs collected in spring, when numerous aerosol transport events from East Asia to the North Pacific occurred, originated from mineral particles. The high Fcrust was attributed to the higher crustal-Fesol % than anthro-Fesol %. The Fesol % of submicron mineral dust (e.g., illite) was higher than those of hematite and magnetite of the same size in solutions with pH higher than 1.7. Furthermore, the Fesol % of fine aerosol particles increased with the decrease in aerosol pH, which indicates that the acidification of mineral particles played an important role in the supply of d-Fe to surface seawater in the North Pacific via atmospheric deposition. Thus, the source estimation of d-Fe using the [d-Fe] [d-Al] ratio is a powerful tool for estimation not only of the source of d-Fe in marine aerosols but also the dissolution processes of Fe in aerosol particles. The source estimation of d-Fe using the [d-Fe] [d-Al] ratio also has the advantage of being performed through a simple analytical method, in which Fe and Al are extracted by ultrapure water and their concentrations are measured through ICP–MS. Therefore, this method can be easily conducted not only in future studies but also on aerosol samples collected in previous research. Currently, data on the [d-Fe] [d-Al] ratios of aerosols, which are strongly affected by anthropogenic Fe and emission sources associated with high-temperature combustion processes, are limited. Therefore, collection of data on the [d-Fe] [d-Al] ratios of these samples will enable us to identify the emission sources of d-Fe in marine aerosol particles with increased robustness.
All quantitative data will be available on the ERAN database (https://www.ied.tsukuba.ac.jp/database/00156.html, last access: 23 August 2023, Sakata et al., 2023): https://doi.org/10.34355/CRiED.U.Tsukuba.00156.
The supplement related to this article is available online at: https://doi.org/10.5194/acp-23-9815-2023-supplement.
The study was designed by KS, AS, and YT. Aerosol sampling was performed by KS and YY. Major ion concentrations were determined by KS, YY, and CM. Trace metal concentrations were measured by KS, CM, and MK. The paper was written by KS and YT, and all authors reviewed the manuscript before submission.
The contact author has declared that none of the authors has any competing interests.
Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
We thank Masatomo Fujiwara and Aya Miyahara for collecting the aerosol samples.
This research has been supported by the Japan Society for the Promotion of Science (grant nos. 14J06437, 25550013).
This paper was edited by Fangqun Yu and reviewed by Mingjin Tang and one anonymous referee.
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- Abstract
- Introduction
- Method
- Results and discussion
- Establishment of source estimation method for d-Fe using the [d-Fe] [d-Al] ratio
- Implication for marine aerosol particles
- Conclusions
- Data availability
- Author contributions
- Competing interests
- Disclaimer
- Acknowledgements
- Financial support
- Review statement
- References
- Supplement
- Abstract
- Introduction
- Method
- Results and discussion
- Establishment of source estimation method for d-Fe using the [d-Fe] [d-Al] ratio
- Implication for marine aerosol particles
- Conclusions
- Data availability
- Author contributions
- Competing interests
- Disclaimer
- Acknowledgements
- Financial support
- Review statement
- References
- Supplement