2.1 Sampling site description

Shenzhen (113.9^∘ E, 22.6^∘ N) is located on the southeastern coast of China, in the southeastern corner of the Pearl River Delta region with Hong Kong neighboring to the south and Dongguan (a famous industrial city in China) to the north. The climate in Shenzhen is a subtropical oceanic climate that is deeply influenced by the monsoon. The sampling site was located on the campus of Shenzhen Graduate School, Peking University in the western urban area of Shenzhen. The area surrounding the sampling site was mostly covered by subtropical plants, and there was only a local road that was approximately 100 m away, which can be regarded as an anthropogenic emission source. The measurement was taken from 31 December 2014 to 23 January 2015 in winter, which is the season with the highest air pollution due to regional transportation from northwestern and northeastern China. The average ambient temperature was 15.9±4.2 ^∘C, and the relative humidity was 62.9±17.5 %. The wind was mostly from the northeast and northwest with an average speed of 0.8±0.7 m s⁻¹.

2.2 Instruments and methodology

The aerosol volatility measurements were conducted with a TD-AMS system. The thermodenuder and the high-resolution time-of-flight aerosol mass spectrometer (HR-ToF-AMS, referred to hereafter as AMS) were both manufactured by Aerodyne Research Inc., US. The principle theory of an AMS can be found in previous studies (DeCarlo et al., 2006; Canagaratna et al., 2007). The AMS was set into two sampling ion optical modes: the V mode with unit mass resolution (UMR) was used for quantification of the UMR mass concentration and size distribution of the non-refractory species (including organics, sulfate, nitrate, ammonium, and chloride); the W mode was used to obtain the high-resolution mass spectra (∼3000 m Δm⁻¹), and the ions with a m∕z up to 170 could be separated properly in this study. The calibrations were conducted at the beginning and end of the campaign with the method described previously (Jayne et al., 2000; Jimenez et al., 2003; Drewnick et al., 2005), including the inlet flow rate, ionization efficiency calibration (IE), and particle size calibrations. The relative ionization efficiencies (RIEs) used in the study were 1.2 for sulfate, 1.1 for nitrate, 1.3 for chloride, 1.4 for organics, and 4.0 for ammonium (Jimenez et al., 2003). The TD used in this experiment is based on the design of Huffman et al. (2008). It consists of two parts: the heating section and the denuder section. The stainless steel heating section is 22.25 inches (56.5 cm) in length with a 1 inch OD (2.5 cm) and a 0.875 inch ID (2.2 cm), wrapped with three fiberglass-coated heating tapes. The heating section is then joined to a 22 inch (56 cm) denuder section. The denuder section is filled with activated charcoal at room temperature to adsorb the gas-phase species evaporated from particles. The temperature in the heating section was set at 48, 95, 143, and 192 ^∘C to make the real temperature at the centerline, measured with a thermocouple, reach 50, 100, 150, and 200 ^∘C, respectively. The full configuration of temperatures in the TD software was 35 min at 50 ^∘C, 5 min for the temperature increasing to 100 ^∘C, 22 min at 100 ^∘C, 5 min for the temperature increasing to 150 ^∘C, 24 min at 150 ^∘C, 5 min for the temperature increasing to 200 ^∘C, 25 min at 200 ^∘C, and then 15 min for the temperature decreasing to 50 ^∘C. The complete temperature cycle lasted about 136 min. The TD was placed upstream of the AMS. The aerosol flow can go through the heating and denuder sections (TD path) before being sampled by the AMS or flowing directly (bypass path) into the AMS. The residence time of aerosols in the heating section was approximately 27.9 s with a flow rate of 0.45 L min⁻¹. The AMS was set with four menus: bypass path in V mode, TD path in V mode, TD path in W mode and bypass path in W mode, with 2 min in each menu. Only the data sampled during the stable temperature plateau (1839 points for V mode and 1842 points for W mode in TD path) were selected for the calculation of volatility.

The data analysis was performed with SQUIRREL 1.57 and PIKA 1.16 (http://cires1.colorado.edu/jimenez-group/ToFAMSResources/ToFSoftware/index.html) with the method in DeCarlo et al. (2006). The mass concentration was corrected with composition-dependent collection efficiency (Middlebrook et al., 2012). All the elemental ratios calculated here were based on the “Improved-Ambient” (I-A) method (Canagaratna et al., 2015) while the previous “Aiken-Ambient” (A-A) method was also used for comparison in Table S1 in the Supplement (Aiken et al., 2008). An aethalometer (AE-31, Magee, US) coupled with a PM_2.5 cyclone was used to measure the mass concentration of black carbon (BC) with a time resolution of 5 min. The wavelength of 880 nm was used to calculate the BC mass concentration in the data processing. The total BC (BC_total) measured by the aethalometer can be separated into BC emitted by traffic (BC_tr) and biomass burning (BC_bb) based on the aerosol absorption as described in the Supplement (Sandradewi et al., 2008). A scanning mobility particle sizer (SMPS, TSI, Inc.) was used to measure the particle number size distribution (mobility diameter: 15–600 nm) with a time resolution of 5 min. By assuming the densities of the components obtained in the literature (Kuwata et al., 2012; Poulain et al., 2014; Hu et al., 2017), the corresponding mass concentration can be calculated from the particle number size distribution. The AE-31 and SMPS were used only for ambient sampling.

2.3 Particle loss correction

The particle losses through the TD should be of concern for quantitative measurements with the TD, as they can decrease the transmission efficiency through the TD. There are three mechanisms of particle loss inside the TD: sedimentation, thermophoretic, and diffusional processes (Burtscher et al., 2001; Wehner et al., 2002). Burtscher et al. (2001) determined that the dominant effects would be determined by the temperature and particle size: sedimentation increases as the particle size increases and would be negligible when the TD is vertical; diffusive losses increase with decreasing particle size; thermophoresis is not strongly dependent on particle size, is important in the denuder section, and will partly compensate for diffusion in the heating section.

The transmission efficiency in this research was calculated via an experiment. CsCl was chosen as the standard chemical species for the test of the transmission efficiency of TD due to its thermal stability as discussed by Huffman et al. (2008). The CsCl solution was atomized and then measured using a differential mobility analyzer (DMA, TSI, Inc.) and condensation particle counter (CPC, TSI, Inc.) before and after the TD. The transmission efficiency of the bypass path was regarded as 1. The average transmission efficiency through the TD is approximately 90 % at 50, 100, 150, and 200 ^∘C, as shown in Fig. 1, which is similar to previous studies (Huffman et al., 2008; Xu et al., 2016a). The transmission efficiency would be applied in the calculation of the mass concentration of particles flowed through the TD.

Figure 1Temperature-related transmission efficiency through the TD.

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2.4 Source apportionment method

PMF was applied to the high-resolution organic mass spectra using the PMF evaluation tool developed by Ulbrich et al. (2009). The data and error matrices were processed according to the signal-to-noise ratio (SNR) as reported in previous papers (Ulbrich et al., 2009; Huang et al., 2010; He et al., 2011). Weak ions (0.2 < SNR <2) were downweighted by a factor of 2, bad ions (SNR <0.2) were removed from the analysis (Paatero and Hopke, 2003), and ${\mathrm{CO}}_{\mathrm{2}}^{+}$-related ions (O⁺, HO⁺, H₂O⁺, and CO⁺) were also downweighted (Ulbrich et al., 2009).

The PMF analysis was based on the full high-resolution organic dataset (including both data sampled under ambient temperature and data that were thermally denuded) for 1 to 10 factors with f_peak varying from −1 to 1 (seed =0), increasing with a step of 0.1, and seed varying from 0 to 250 (f_peak =0) in steps of 10. The diagnostic plots of the solutions are shown in Fig. S1 in the Supplement, including the Q ∕ Q_expected ratio, the characteristics of the different mass spectra, the scaled residuals, and the correlation of the component time series with the external tracers. The solutions with more than five factors showed no distinct information but splitting of the factors. The Q ∕ Q_expected showed the lowest value at f_peak =0; the varied f_peak did not improve the results. The varied value of seed also made no significant difference of the solution. Therefore, the solution of five factors, f_peak =0, and seed =0 was determined as the optimal solution for this experiment, and the five factors are hydrocarbon-like OA (HOA), cooking OA (COA), BBOA, less-oxidized oxygenated OA (LO-OOA), and more-oxidized oxygenated OA (MO-OOA).

In addition, the PMF results with the data obtained only under ambient temperatures were also explored and the best solution was presented in Fig. S2 in the Supplement. Compared to the results including the thermally denuded data, the HOA and OOA were mixed to some extent, with a signature of the high fraction of ${\mathrm{CO}}_{\mathrm{2}}^{+}$ in the HOA mass spectrum. Therefore, the PMF solution with the inclusion of the thermally denuded data was confirmed as the final result for later discussion. Huffman et al. (2009b) also suggested that the PMF solution of all data collected both with and without TD processing could facilitate the separation of different OA factors by enhancing the contrast of the time series of these factors.

3.1 PM₁ chemical compositions

Figure 2 shows the chemical compositions for only bypass conditions. Figure 2a shows the time series of the mass concentration of non-refractory species measured by the AMS and BC measured with an aethalometer during the experiment. Sulfate showed a relatively stable time series, with a relative SD (RSD) of 38.8 %, compared to the other species, such as organics (RSD =56.1 %), nitrate (RSD =69.6 %), and black carbon (RSD =70.2 %), indicating that sulfate was less affected by local emission sources. However, all the species decreased their concentrations largely during 12–13 January due to a heavy rain event. The sum of the non-refractory species and BC was regarded as PM₁, which showed a high correlation (R²=0.94, slope =1.1; in Fig. S3) with the mass concentration derived from the particle number concentration measured by SMPS. As a result, the average mass concentration of PM₁ was 42.7±20.1 µg m⁻³, ranging from 3.9 to 134.1 µg m⁻³, while organics were the most abundant PM₁ component, contributing 43.2 % to the total PM₁ mass concentration, followed by sulfate (21.2 %), BC (12.2 %), nitrate (11.4 %), ammonium (10.4 %), and chloride (1.6 %). The measured and predicted ammonium showed a high correlation (R²=0.97) with a slope of 0.85, implying that the aerosols showed some acidity (Zhang et al., 2007b).

The diurnal variation in the PM₁ species is shown in Fig. 2b. The two peaks in the diurnal variation in BC obviously match the traffic rush hours at approximately 08:00 in the morning and the activities of heavy duty vehicles in the evening. When BC source apportionment was applied for our BC dataset, the results indicated that biomass-burning-emitted BC also made a small contribution to the evening peak of BC (Fig. S4). Nitrate showed a significant peak about 2 h after the morning peak of BC, which was likely a result of photochemical oxidization of NO_x emitted from the morning traffic. Then, the concentration of nitrate decreased because of both the lifting of the planetary boundary layer (PBL) and its evaporation at higher ambient temperatures (also shown in Fig. 2b). Nitrate maintained a stable concentration level in the evening. Similar to ammonium nitrate, ammonium chloride is also quite semi-volatile as revealed in Sect. 3.3. Therefore, its diurnal variation was largely influenced by the ambient temperature, as well as the height of the PBL. Also, according to Sect. 3.3, sulfate is a less-volatile species and thus would not lose significant particulate mass when the ambient temperature increases. As a secondary species from SO₂ oxidation, sulfate showed a slight diurnal variation, indicating that it was less affected by the variation in the PBL. This implies that sulfate was not a typical ground-emitted species and could be better mixed in the PBL. Actually, aerosol sulfate in Shenzhen has been proven to be a species mostly from regional air mass transport (He et al., 2011; Huang et al., 2014). Since ammonium exists mostly in the forms of (NH₄)₂SO₄, NH₄NO₃, and NH₄Cl, its diurnal variation should be significantly affected by the formation processes of all these inorganic salts, in addition to atmospheric physical processes and semi-volatility. The measured and predicted ammonium showed a similar correlation (R²=0.96–0.97) with a similar slope of 0.84–0.85 for both the ambient temperatures and 50 ^∘C (Fig. S5), implying that the aerosols showed some acidity in the real ambient temperature range (Zhang et al., 2007b). The diurnal variation in organics showed more fluctuation and a few peaks, consistent with its complex origins, e.g., vehicles, biomass burning, and secondary formation (He et al., 2011; Elser et al., 2016), which will be discussed in detail in Sect. 3.2.

The average values of O ∕ C and H ∕ C of OA were 0.52 and 1.61, respectively. The average O ∕ C value in this campaign is within the typical O ∕ C range of 0.28–0.56 previously observed under polluted urban environments in China (Huang et al., 2011, 2012; He et al., 2011; Xu et al., 2016b; Hu et al., 2016; Lee et al., 2013). The diurnal variation in O ∕ C plotted in Fig. 2c shows elevated values during the daytime, which is a clear indicator of the formation of secondary OA with more oxygen, while H ∕ C reasonably showed an opposite diurnal trend, with decreased values during the daytime. The quick elevation of H ∕ C in the evening should be a combined result of various primary emissions, e.g., traffic, cooking, and biomass burning, which is supported by the source apportionment results discussed in Sect. 3.2.

Figure 2d shows the average size distribution of the five non-refractory species. The peaks of all the species were at approximately 500–700 nm in the accumulation modes, while organics apparently had more mass distribution at smaller sizes down to ∼100 nm. The inorganic aerosol species showed a similar average size distribution during the experiment as described in previous studies in Shenzhen (He et al., 2011). Compared to other species, the peak of organics was slightly smaller, which was a result of the much broader size distribution of organics towards smaller sizes. This character of organic size distribution implies that urban fresh primary emissions contributed significantly to OA (Canagaratna et al., 2004; He et al., 2011). The peak of sulfate was slightly larger than the other species, suggesting that sulfate was mostly associated with more aged particles that had grown during air mass transport (Zhang et al., 2005; Huang et al., 2008).

Figure 2Chemical composition for only bypass conditions: (a) time series and the mass percentages of PM₁ composition; (b) diurnal variation in PM₁ species and ambient temperature; (c) diurnal variation in H ∕ C ratio and O ∕ C ratio; (d) average size distribution of non-refractory PM₁ species.

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3.2 Source apportionment

Organics are one of the most important chemical species in aerosol pollution in Shenzhen, contributing 43.2 % to the total PM₁ mass loading. As discussed in Sect. 2.4, PMF modeling was applied to the high-resolution mass spectra of organics and five factors were identified with their mass spectrometer profiles shown in Fig. 3a. Under ambient temperatures, HOA, COA, BBOA, LO-OOA, and MO-OOA averagely accounted for 13.5, 20.6, 8.9, 39.1, and 17.9 % of the total organic mass, respectively (Fig. 3d).

HOA is most often dominated by long-chain hydrocarbon ion series of ${\mathrm{C}}_n{\mathrm{H}}_{\mathrm{2}n+\mathrm{1}}^{+}$ and ${\mathrm{C}}_n{\mathrm{H}}_{\mathrm{2}n-\mathrm{1}}^{+}$ in previous findings (Canagaratna et al., 2004; Mohr et al., 2009; Ng et al., 2010), which is also the case in this campaign. The average O ∕ C of HOA was 0.10 in this campaign, which was in its range (0.03 to 0.17) reported in previous publications (e.g., Aiken et al., 2009; Huang et al., 2010; Mohr et al., 2012). BC is regarded as a tracer of HOA and can be significantly emitted from both fossil fuel combustion and biomass burning (Zhang et al., 2007a; Lanz et al., 2007; Lan et al., 2011). The good correlation (R²=0.82) of HOA and BC_tr (Fig. 3b) suggested that HOA was mainly from traffic emissions. The diurnal variation in HOA was influenced by PBL dynamics and also showed peaks that matched the rush hours, further supporting the dominant role of traffic emissions in the HOA.

The O ∕ C ratio of COA is 0.18, which is similar to the previous results shown in Mohr et al. (2012). The mass spectral signature of COA is dominated by the ion series of ${\mathrm{C}}_n{\mathrm{H}}_{\mathrm{2}n+\mathrm{1}}^{+}$ and ${\mathrm{C}}_m{\mathrm{H}}_{\mathrm{2}m+\mathrm{1}}{\mathrm{CO}}^{+}$ (m∕z 29, 43,57,71, 85…) and ${\mathrm{C}}_n{\mathrm{H}}_{\mathrm{2}n-\mathrm{1}}^{+}$ and ${\mathrm{C}}_m{\mathrm{H}}_{\mathrm{2}m-\mathrm{1}}{\mathrm{CO}}^{+}$ (m∕z 41, 55, 69, 83…), which are mainly ionized from alkanes, alkenes, and, possibly, long-chain fatty acids (He et al., 2010; Huang et al., 2010; Mohr et al., 2009, 2012). Mohr et al. (2012) also identified COA from HOA by comparing the signals of m∕z 55 and m∕z 57 and determined that the differentiation between COA and HOA is mainly driven by the oxygen-containing ions of C₃H₃O⁺ and C₃H₅O⁺; especially if the signal ratio of m∕z 55 to m∕z 57 is larger than 2, it can probably be recognized as COA. In this study, COA showed much more C₃H₃O⁺ than HOA, and the ratio of m∕z 55 to m∕z 57 showed values larger than 2, indicating the origin of cooking emissions. The diurnal variation in COA in Fig. 3c shows a small peak at approximately 8:00 UTC+8 (UTC+8 for all times following), breakfast time, and the second peak at approximately 14:00 corresponds with lunch time. The mass concentration of COA also rises after 17:00, which is the time for dinner and partly because of the decreasing PBL height. The good correlation of COA with the tracer ion C₆H₁₀O (R²=0.91) (Sun et al., 2011; Crippa et al., 2013; Elser et al., 2016) also demonstrated the presence of COA.

The most abundant signals in BBOA are m∕z 29 (CHO⁺) and m∕z 43 (C₂H₃O⁺), and there are more fragments in the range of $m/z>\mathrm{100}$ for BBOA than for COA and HOA (He et al., 2010). BBOA can be identified by the contribution of m∕z 60 (mostly ${\mathrm{C}}_{\mathrm{2}}{\mathrm{H}}_{\mathrm{4}}{\mathrm{O}}_{\mathrm{2}}^{+}$), which is a distinct fragment of ionized levoglucosan, the molecular marker of biomass burning (Alfarra et al., 2007; Aiken et al., 2009; Mohr et al., 2009). Some previous studies have shown that the background level of m∕z 60 ∕ OA is approximately 0.3 % in urban areas without biomass-burning impacts (DeCarlo et al., 2008; Docherty et al., 2008). The signal of m∕z 60 in BBOA is 1.36 % in this study, indicating the presence of BBOA during this experiment, and the BBOA correlated well with m∕z 60 (R²=0.83). The O ∕ C ratios of BBOA varied a lot in previous studies. Laboratory studies reported O ∕ C ratios of 0.18–0.26 for six types of biomass-burning emissions (He et al., 2010), O ∕ C ratios of 0.31 for lodgepole pine burning, and 0.42 for sage/rabbitbrush burning (Aiken et al., 2008). DeCarlo et al. (2010) reported an O ∕ C ratio of 0.42 for ambient biomass-burning aerosol. The BBOA in this study showed an O ∕ C ratio of 0.33, which is within the range of previous studies. The diurnal trend in BBOA showed a large peak in the evening, consistent with the diurnal peak of BC_bb in Fig. S4.

OOA is recognized by the most intense signal of m∕z 44 (${\mathrm{CO}}_{\mathrm{2}}^{+}$), and the signals at higher values of m∕z are lower relative to those of other OA factors (Ng et al., 2010). Furthermore, the OOA can be divided into two factors, LO-OOA (typically named semi-volatile OOA) and MO-OOA (typically named less-volatile OOA), according to the O ∕ C ratios and f₄₄ (Jimenez et al., 2009; Ng et al., 2010; Xu et al., 2015). The factor with a relatively higher O ∕ C ratio (0.95) of OOA and higher f₄₄ than f₄₃ is identified as MO-OOA. It showed a good correlation (R²=0.64) with sulfate, which was less volatile and had been identified as a regional pollutant in Shenzhen (He et al., 2011; Huang et al., 2014), implying MO-OOA could also be aged aerosol from regional transport. The correlation of MO-OOA with nitrate (R²=0.27) is much lower than with sulfate, which is a typical result. Meanwhile, LO-OOA, which is less oxygenated ($\mathrm{O}/\mathrm{C}=\mathrm{0.76}$), showed a narrow gap between f₄₃ and f₄₄. The correlation of LO-OOA with sulfate (R²=0.59) was indeed a little bigger than with nitrate (R²=0.46), which could be a combined result of the precursors, formation mechanisms, and volatility of LO-OOA. Unlike the primary organic components, which had lower concentrations during the daytime due to the elevated PBL, the diurnal variations in both LO-OOA and MO-OOA showed higher concentrations during the daytime, suggesting that photochemical secondary production should be their main source. The diurnal variation in MO-OOA was relatively stable compared to that in LO-OOA, which is consistent with MO-OOA being a more aged and regional component. The contribution of the two OOA to total OAs is 57.0 %, indicating that OOA contributes the majority of the OA pollution in wintertime in Shenzhen.

Figure 3(a) MS profiles of the five OA factors identified by PMF; (b) time series of the five OA factors and the correlation with the relevant species during the experiment; (c) the diurnal variation in the five OA factors; (d) the average contributions of the five OA factors to total OA. The time series, diurnal variation, and pie chart display the results only for ambient conditions.

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Figure 4 showed the mass fractions of the five factors at different TD temperatures. It is found that when the temperature increased, the fraction of MO-OOA quickly increased up to 67.6 % at 200 ^∘C, while LO-OOA showed a reverse trend, accounting for only 2.9 % at 200 ^∘C, indicating that they had quite different volatilities. HOA, COA, and BBOA also exhibited different volatilities, with HOA accounting for only 5–7 % above 100 ^∘C, while the fraction of COA did not change much with the increasing temperature. The different volatilities of different OA factors will be discussed in more detail in the following section.

Figure 4The average compositions of the total OA at different TD temperatures.

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3.3 Volatility of PM₁ species and OA factors

Figure 5 shows the mass fraction remaining (MFR) of the non-refractory species. The MFR is calculated as the ratio of the species mass concentrations with and without TD processing. The narrow average MFR ± SD regions show that the volatilities of these species were stable during the measurement. The MFRs of the total non-refractory species and organics both showed nearly linear correlations with the TD temperature, which is consistent with the fact that they include various compounds with a wide range of volatilities. For organics, the MFR was 0.88 at 50 ^∘C, 0.63 at 100 ^∘C, 0.32 at 150 ^∘C, and, finally, 0.16 at 200 ^∘C. Based on the linear relationship of the MFR of organics and the TD temperature, the evaporation rate of organics is approximately 0.45 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$. The relationship of the O ∕ C, H ∕ C, and N ∕ C ratios with the TD temperature is also shown in Fig. 5. It can be seen that O ∕ C kept increasing as the temperature increased, especially after 150 ^∘C, which is consistent with previous studies (Xu et al., 2016a). When examining the organic mass spectra at difference temperatures (in Fig. S6), the elevation of O ∕ C with increasing temperature was found to be reasonably related to increasing of ${\mathrm{CO}}_{\mathrm{2}}^{+}$. Previous PMF results usually correlated higher volatility with reduced species and lower volatility with more oxygenated species (Ng et al., 2010; Huang et al., 2012). In this study, the elevation of O ∕ C with increasing temperature was closely related to the evaporation of more reduced organic components, as the PMF results indicated. Conversely, H ∕ C showed a reasonable reverse trend relative to that of O ∕ C. N ∕ C generally had an increasing trend with the TD temperature increasing, but N ∕ C varied largely at the different TD temperatures, suggesting that the volatilities of N-containing compounds are complex.

Figure 5 also shows the MFRs of inorganic species with different temperature, and all the inorganic species showed trends similar to the results shown by Huffman et al. (2008). Nitrate and chloride show similar trends: they both decreased sharply from ambient temperature to 50 ^∘C, reaching approximately 0.57; then they decreased at a lower rate from 50 to 150 ^∘C. When the TD temperature increased to 200 ^∘C, the MFRs of nitrate and chloride were at approximately 0.08, which is lower than those of all the other species. Sulfate is the least volatile species among all PM₁ species. The MFR of sulfate does not show a significant decreasing trend with temperature below 100 ^∘C (0.93 at 50 ^∘C and 0.89 at 100 ^∘C); when the temperature reached 150 ^∘C, the MFR decreased sharply to 0.43, with 11 % left at 200 ^∘C. The trend in MFR of sulfate is consistent with the discussion in Burtscher et al. (2001): sulfuric acid would evaporate under temperatures of 30–125 ^∘C, while ammonium sulfate and bisulfate would evaporate between 125 and 175 ^∘C.

Figure 5Variation in the average mass fraction remaining (MFR) of the total of non-refractory species and the ratios of O ∕ C, H ∕ C, and N ∕ C with the TD temperature. The shaded regions indicate the average ±SD.

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Figure 6 shows the MFRs of the different OA factors identified by PMF. The MFR of HOA was 0.56 at 50 ^∘C and decreased by 1.26 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$ from the ambient temperature to 50 ^∘C and reached only 17.8 % at 100 ^∘C. Then, the evaporation rate slowed down significantly, with a MFR of 7.6 % at 200 ^∘C. BBOA showed significant volatility in this study, with an evaporation rate of 0.37 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$ near the ambient temperature and an MFR of 0.87 at 50 ^∘C. In addition, it was noted that the evaporation rate of BBOA increased when the TD temperature increased from 100 to 150 ^∘C, indicating that BBOA contained more compounds that favor evaporation in this temperature range. COA showed a similar volatility to that of BBOA, with an MFR of 0.85 at 50 ^∘C, but it kept a stable evaporation rate throughout the whole temperature range (∼0.44 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$). The volatility of LO-OOA (MFR =0.70 at 50 ^∘C) was higher than that of MO-OOA (MFR =0.99 at 50 ^∘C), COA, and BBOA but lower than that of HOA. The MFR curve of MO-OOA remained relatively stable below 100 ^∘C and then decreased significantly when the temperature increased further. The MFR of MO-OOA was as high as 51.5 % even at 200 ^∘C. Thus, MO-OOA was the least volatile one among the five factors. The OOA (LO-OOA+MO-OOA) in Fig. 6 presents the MFR variation in the combination of LO-OOA and MO-OOA. The MFR of OOA, which is regarded as a good surrogate of SOA, showed a good linear decline at the temperatures under 150 ^∘C, with an evaporation rate of 0.54 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$. The evaporation rates of the different OA factors identified by PMF in this study provide the first-hand information of semi-volatility of OAs in China, which will be helpful in constraining parameters in the atmospheric chemical models.

Figure 6Average mass fraction remaining (MFR) of the five OA factors and OOA (calculated as the combination of MO-OOA and LO-OOA). The shaded region is the average MFR ± SD.

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Figure 7 compares both the volatilities (MFR at 50 ^∘C) and the O ∕ C ratios of the five factors. The sequence of the volatilities can be summarized as HOA > LO-OOA > COA ≈ BBOA > MO-OOA. It can be easily found that the sequence of the volatilities of the OA factors does not completely follow the sequence of the O ∕ C ratios. For example, although LO-OOA has a higher O ∕ C ratio than BBOA and COA, LO-OOA is also more volatile (or with a lower MFR) than BBOA and COA. This clearly indicates the volatility of the OA factors depends on not only the oxygenation of organic compounds but also other factors, e.g., molecular weight and mixing state. HOA is identified as the most volatile OA factor while MO-OOA is nearly nonvolatile near the real atmospheric temperatures in Shenzhen, which is consistent with the results observed in Mexico and Paris (Cappa and Jimenez, 2010; Paciga et al., 2016). However, LO-OOA is the second most volatile OA factor after HOA in Shenzhen, which is different from that in Mexico, where BBOA is more volatile than LO-OOA. Actually, the volatility of the aerosols directly from biomass burning has been measured to be quite variable, with an evaporation rate of 0.2–1.6 $\mathrm{\%}{}^{\circ }{\mathrm{C}}^{-\mathrm{1}}$, depending on the kinds of wood and combustion conditions (Huffman et al., 2009a). The relatively lower volatility of COA was also identified in previous studies and attributed to the abundant fatty acids of low volatility in COA (Mohr et al., 2009; Paciga et al., 2016). Hong et al. (2017) recently reported the estimation of the OA volatility in a boreal forest in Finland using two independent methods, including using a VTDMA with a kinetic evaporation model and applying PMF to HR-AMS data. Semi-volatile and low-volatility organic mass fractions were determined with both methods, similar to our study in China. This implies that MO-OOA and LO-OOA, with different volatilities, could be popular OA components across the world. Hong et al. (2017) also pointed out that determining extremely low-volatility OAs from AMS data using the PMF analysis should be explored in future studies.

Figure 7Comparison of the volatilities (MFRs at 50 ^∘C) and O ∕ C ratios of the five OA factors in this study. The colorful regions indicate the SDs of the MFRs.

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It should also be noted that as the most volatile species in this study, HOA could be evaporated easily and thus have a larger potential to experience the “evaporation – oxidation in gas phase – condensation” process and then form SOA since previous studies showed that semi-volatile hydrocarbons from diesel exhaust (Robinson et al., 2007) and crude oil (de Gouw et al., 2011) can be easily oxidized in the gas phase to form less-volatile SOA. Huang et al. (2012) also pointed out that HOA could be oxidized to SOA based on the analysis of their diurnal variations. This potential can be further supported by the fact that it was difficult to resolve HOA in downwind regions far from urban and industrial areas in China, implying that HOA had been oxidized during the air mass transport (Huang et al., 2011; Zhu et al., 2016). Therefore, the modeling work needs to consider the process from HOA to SOA in future.