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Atmospheric Chemistry and Physics An interactive open-access journal of the European Geosciences Union
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ACP | Articles | Volume 19, issue 3
Atmos. Chem. Phys., 19, 1971-1983, 2019
https://doi.org/10.5194/acp-19-1971-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Chem. Phys., 19, 1971-1983, 2019
https://doi.org/10.5194/acp-19-1971-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Research article 13 Feb 2019

Research article | 13 Feb 2019

A proxy for atmospheric daytime gaseous sulfuric acid concentration in urban Beijing

A proxy for atmospheric daytime gaseous sulfuric acid concentration
Yiqun Lu1, Chao Yan2, Yueyun Fu3, Yan Chen4, Yiliang Liu1, Gan Yang1, Yuwei Wang1, Federico Bianchi2, Biwu Chu2, Ying Zhou5, Rujing Yin3, Rima Baalbaki2, Olga Garmash2, Chenjuan Deng3, Weigang Wang4, Yongchun Liu5, Tuukka Petäjä2,5,6, Veli-Matti Kerminen2, Jingkun Jiang3, Markku Kulmala2,5, and Lin Wang1,7,8 Yiqun Lu et al.
  • 1Shanghai Key Laboratory of Atmospheric Particle Pollution and Prevention (LAP), Department of Environmental Science & Engineering, Jiangwan Campus, Fudan University, Shanghai 200438, China
  • 2Institute for Atmospheric and Earth System Research/Physics, Faculty of Science, University of Helsinki, 00014 Helsinki, Finland
  • 3State Key Joint Laboratory of Environment Simulation and Pollution Control, School of Environment, Tsinghua University, Beijing 100084, China
  • 4Institute of Chemistry, Chinese Academy of Sciences, Beijing 100190, China
  • 5Aerosol and Haze Laboratory, Advanced Innovation Center for Soft Matter Science and Engineering, Beijing University of Chemical Technology, Beijing 100029, China
  • 6Joint International Research Laboratory of Atmospheric and Earth System Sciences (JirLATEST), School of Atmospheric Sciences, Nanjing University, Nanjing 210023, China
  • 7Institute of Atmospheric Sciences, Jiangwan Campus, Fudan University, Shanghai 200438, China
  • 8Shanghai Institute of Pollution Control and Ecological Security, Shanghai 200092, China
Abstract
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Gaseous sulfuric acid (H2SO4) is known as one of the key precursors for atmospheric new particle formation (NPF) processes, but its measurement remains challenging. Therefore, a proxy method that is able to derive gaseous sulfuric acid concentrations from parameters that can be measured relatively easily and accurately is highly desirable for the atmospheric chemistry community. Although such methods are available for clean atmospheric environments, a proxy that works well in a polluted atmosphere, such as that found in Chinese megacities, is yet to be developed. In this study, the gaseous sulfuric acid concentration was measured in February–March 2018, in urban Beijing using a nitrate based – long time-of-flight chemical ionization mass spectrometer (LToF-CIMS). A number of atmospheric parameters were recorded concurrently including the ultraviolet radiation B (UVB) intensity, the concentrations of O3, NOx (sum of NO and NO2), SO2, and HONO, and aerosol particle number size distributions. A proxy for atmospheric daytime gaseous sulfuric acid concentration was derived via a statistical analysis method using the UVB intensity, [SO2], the condensation sink (CS), [O3], and [HONO] (or [NOx]) as the predictor variables, where square brackets denote the concentrations of the corresponding species. In this proxy method, we considered the formation of gaseous sulfuric acid from reactions of SO2 and OH radicals during the daytime, and the loss of gaseous sulfuric acid due to its condensation onto the preexisting particles. In addition, we explored the formation of OH radicals from the conventional gas-phase photochemistry using O3 as a proxy and from the photolysis of HONO using HONO (and subsequently NOx) as a proxy. Our results showed that the UVB intensity and [SO2] are dominant factors in the production of gaseous sulfuric acid, and that the simplest proxy could be constructed with the UVB intensity and [SO2] alone. When the OH radical production from both homogenously and heterogeneously formed precursors were considered, the relative errors were reduced by up to 20 %.

1 Introduction
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Gaseous sulfuric acid (H2SO4) is a key precursor for atmospheric new particle formation (NPF) processes (Kerminen, 2018; Kirkby et al., 2011; Kuang et al., 2008; Kulmala and Kerminen, 2008; Sipilä et al., 2010). A number of atmospheric nucleation mechanisms including H2SO4H2O binary nucleation (Benson et al., 2008; Duplissy et al., 2016; Kirkby et al., 2011), H2SO4NH3H2O ternary nucleation (Kirkby et al., 2011; Korhonen et al., 1999; Kürten et al., 2015), and H2SO4–DMA (dimethylamine)–H2O ternary nucleation (Almeida et al., 2013; Jen et al., 2014; Kürten et al., 2014; Petäjä et al., 2011; Yao et al., 2018) involve the participation of gaseous sulfuric acid molecules. In addition, the condensation of gaseous sulfuric acid onto newly formed particles contributes to their initial growth (Kuang et al., 2012; Kulmala et al., 2013). Quantitative assessments of the contribution of gaseous sulfuric acid to both the NPF rates and the particle growth rates require real-time measurements of gaseous sulfuric acid concentrations prior to and during the NPF events (Nieminen et al., 2010; Paasonen et al., 2010).

Measurements of gaseous sulfuric acid in the lower troposphere are challenging because its ambient concentration is typically quite low (106107 molecule cm−3) (Kerminen et al., 2010; Mikkonen et al., 2011). Reported real-time measurements of gaseous sulfuric acid are currently based on chemical ionization mass spectrometry with NO3- and its ligands as reagent ions (nitrate CIMS) because nitrate CIMS with an atmospheric pressure interface (API) has a low detection limit for the atmospheric concentration range of gaseous sulfuric acid (Jokinen et al., 2012); furthermore, a constant fraction of sulfuric acid present in the air sample will be ionized by excessive nitrate ions in CIMS under constant instrumental conditions (Kürten et al., 2012; Zheng et al., 2010), which makes the quantification of gaseous sulfuric acid feasible.

Arnold and Fabian (1980) measured the negative ions in the stratosphere and derived the concentration of stratospheric gaseous sulfuric acid from the fractional abundances of a series of stratospheric negative ions as well as the rate constants. Later, real-time measurement of sulfuric acid in the lower troposphere was performed using nitrate CIMS (Eisele and Tanner, 1993), with laboratory calibrations performed via the production of known concentrations of OH radicals that were titrated into gaseous sulfuric acid. Since this work, measurements of sulfuric acid using CIMS have been performed around the world (e.g., Berresheim et al., 2000; Bianchi et al., 2016; Chen et al., 2012; Jokinen et al., 2012; Kuang et al., 2008; Kürten et al., 2014; Kurtén et al., 2011; Petäjä et al., 2009; Weber et al., 1997; Zheng et al., 2011), and CIMS has been proven to be a robust tool for gaseous sulfuric acid detection. However, sulfuric acid measurements are still rather sparse due to the high cost of the CIMS instrument and the extensive demand for specialized expertise with respect to instrument calibration, maintenance, and data processing, etc. Therefore, a proxy for gaseous sulfuric acid concentration is highly desirable.

Proxies for the estimation of atmospheric gaseous sulfuric acid concentrations were previously developed to approximate measurement results of sulfuric acid in Hyytiälä, southern Finland (Petäjä et al., 2009), assuming that gaseous sulfuric acid is formed from reactions between SO2 and OH radicals, and lost due to its condensation onto preexisting particles. The derived simplest proxy can be written as Eq. (1) below, where the square brackets denote the concentration, and the authors recognize that the proxies might be site-specific and should be verified prior to utilization in other environments.

(1)H2SO4=kSO2(UVBorGlobalradiation)CS

Mikkonen et al. (2011) later developed a couple of statistical proxies based on measurements of sulfuric acid at six European and North American sites, including urban, rural, and forest areas. Their results showed that the radiation intensity and [SO2] are the most important factors to determine the concentration of sulfuric acid, and that the impact of the condensation sink (CS) for gaseous sulfuric acid, is generally negligible. In several proxies developed by Mikkonen et al. (2011), the correlation between the gaseous sulfuric acid concentration and the CS is positive, which is contrary to what one would expect because a larger CS normally leads to a faster loss for gaseous sulfuric acid. In addition, the performance of a proxy equation is site-specific due to varying atmospheric conditions from one site to another, which implies that the proxy suggested by Mikkonen et al. (2011) might not work well in locations with atmospheric environments different to those at the six sites in that study.

Beijing is a location with typical CS values (e.g., 0.01–0.24 s−1 in the 5 %–95 % percentiles in this study) that are 10–100 times higher (Herrmann et al., 2014; Wu et al., 2007; Xiao et al., 2015; Yue et al., 2009; Zhang et al., 2011) and typical SO2 concentrations that are 1–10 times higher (M. Wang et al., 2011; Wu et al., 2018) than those in Europe and North America (Dunn et al., 2004; Mikkonen et al., 2011), yet measured gaseous sulfuric acid concentrations are relatively similar in these environments (Chen et al., 2012; Smith et al., 2008; Z. B. Wang et al., 2011; Zheng et al., 2011). Whether previous proxies developed for European and North American sites work in Beijing remains to be tested. Furthermore, in addition to the gas-phase reaction between O(1D) and water molecules (Crutzen and Zimmermann, 1991; Logan et al., 1981), photolysis of HONO could potentially be an important source of OH radicals in the atmosphere in the early morning (Alicke et al., 2002, 2003; Elshorbany et al., 2009; Li et al., 2012) and during the daytime (Acker et al., 2005; Aumont et al., 2003; Kleffmann, 2007). An experimental study measuring HONO near the surface layer estimated that HONO was a main contributor to OH production in Beijing, with HONO's contribution being larger than 70 % at around 12:00–13:00 UTC/GMT+08:00, except for in summer when the contribution of O3 dominated (Hendrick et al., 2014). Given the distinct characteristics of these two OH radical formation pathways, they should both be included and evaluated separately when a proxy for atmospheric gaseous sulfuric acid concentration is being built. The reactions between SO2 and Criegee intermediates formed from the ozonolysis of atmospheric alkenes could be a potential source of sulfuric acid only in the absence of solar radiation (Boy et al., 2013; Mauldin et al., 2012); therefore, these reactions are expected to provide a minor contribution to the formation of gaseous sulfuric acid during the daytime in urban Beijing.

In this study, the gaseous sulfuric acid concentration was measured using a long time-of-flight chemical ionization mass spectrometer (LToF-CIMS) in February–March 2018, in urban Beijing. A number of atmospheric parameters were recorded concurrently, including the ultraviolet radiation B (UVB) intensity, the concentrations of O3, NOx, SO2, and HONO, and particle number size distributions. The objective of this study is to develop a robust daytime gaseous sulfuric acid concentration proxy for Beijing, a representative Chinese megacity with an urban atmospheric environment.

2 Ambient measurements
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An intensive campaign was carried out from 9 February to 14 March 2018 on the fifth floor of a teaching building on the west campus of Beijing University of Chemical Technology (3994 N, 11630 E). This monitoring site is 2 km to the west of the West Third Ring Road and is surrounded by commercial properties and residential dwellings. Hence, this station can be regarded as a representative urban site.

The sulfuric acid concentration was measured using a LToF-CIMS (Aerodyne Research, Inc.) equipped with a nitrate chemical ionization source. Ambient air was drawn into the ionization source through a 1.6 m stainless-steel tube with a 3∕4 inch diameter. A mixture of a 3 standard cubic centimeter per minute (sccm) ultrahigh purity nitrogen flow containing nitric acid and a 20 standard liter per minute (slpm) pure air flow supplied by a zero-air generator (Aadco 737, USA), together as a sheath flow, was introduced into a PhotoIonizer (Model L9491, Hamamatsu, Japan) to produce nitrate reagent ions. This sheath flow was then introduced into a coaxial laminar flow reactor concentric to the sample flow. Nitrate ions were pushed to the middle of the sample flow under an electric field and subsequently charged sample molecules. For example, the atmospheric H2SO4 molecules would be charged by nitrate reagent ions NO3-(HNO3)0-2 and would mainly produce HSO4- ions (m/z=96.9601 Th), HSO4-HNO3 ions (m/z=159.9557 Th), and HSO4-(HNO3)2 ions (m/z=222.9514 Th). In addition, HSO4-H2SO4 ions (m/z=194.9275 Th) were formed from ion-induced clustering of neutral sulfuric acid and bisulfate ions within the LToF-CIMS ion reaction zone, and also from the evaporation of DMA and the replacement of one molecule of H2SO4 with one bisulfate ion, HSO4-, during the NO3- reagent ion charging of a stabilized neutral sulfuric acid dimer in the real atmosphere in the presence of DMA or a molecule that works in the same way as DMA. During the campaign, the sample flow rate was kept at 8.8 slpm, as mass flow controllers fixed the sheath flow rate and the excess flow rate, and the flow into the mass spectrometer (around 0.8 slpm) was fixed by the size of a pinhole between the ionization source and the mass spectrometer. The concentration of gaseous sulfuric acid was then determined by Eq. (2):

(2)H2SO4=HSO4-(HNO3)0-2+HSO4-H2SO4NO3-(HNO3)0-2C,

where C is the calibration coefficient, and NO3-(HNO3)0-2, HSO4-(HNO3)0-2 and HSO4-H2SO4 represent the signals of corresponding ions in units of counts per second (cps). The unit of the resulting [H2SO4] is molecule cm−3. The CIMS was calibrated during the campaign using a homemade calibration box that can produce adjustable concentrations of gaseous sulfuric acid from SO2 and OH radicals following the protocols in previous literatures (Kürten et al., 2012; Zheng et al., 2015). We obtain a calibration coefficient of 3.79×109 molecule cm−3 for our instrument and use 1.1×1010 molecule cm−3 as the effective calibration coefficient, after taking the diffusion losses in the stainless-steel tube and the nitrate chemical ionization source into account. The obtained mass spectra were analyzed with a tofTools package based on MATLAB software (Junninen et al., 2010).

Ambient particle number size distributions down to about 1 nm were measured using a combination of a scanning mobility particle sizer spectrometer (SMPS) equipped with a diethylene glycol-based condensation particle counter (DEG-CPC, ∼1–10 nm) and a conventional particle size distribution system (PSD, ∼3 nm–10 µm) consisting of a pair of aerosol mobility spectrometers developed by Tsinghua University (Cai et al., 2017; Jiang et al., 2011; Liu et al., 2016). The values of the CS were calculated following Eq. (3) (Dal Maso et al., 2002):

CS=2πD0DpβmDpnDpdDp(3)=2πDiβiDpiNi,

where Dpi is the geometric mean diameter of particles in the size bin i and Ni is the particle number concentration in the corresponding size bin; D is the diffusion coefficient of gaseous sulfuric acid, and βm represents a transition-regime correction factor dependent on the Knudsen number (Fuchs and Sutugin, 1971; Gopalakrishnan and Hogan Jr., 2011).

SO2, O3, and NOx concentrations were measured using a SO2 analyzer (Model 43i, Thermo, USA), an O3 analyzer (Model 49i, Thermo, USA), and a NOx analyzer (Model 42i, Thermo, USA) with detection limits of 0.1, 0.5, and 0.4 ppbv, respectively. The above instruments were pre-calibrated before the campaign. The UVB (280–315 nm) intensity (UV-S-B-T, KIPP&ZONEN, the Netherlands) was measured on the rooftop of the building. Atmospheric HONO concentrations were measured using a homemade HONO analyzer with a detection limit of 0.01 ppbv (Tong et al., 2016).

Particle number size distributions and concentrations of gaseous sulfuric acid, SO2, O3, NOx, and HONO were recorded with a time resolution of 5 min, and the UVB intensity with a time resolution of 1 min. A linear interpolation method was used for deriving the variables with the same time intervals, i.e., 5 min. Only data between local sunrise and sunset were used in the subsequent analysis.

3 Development of a proxy for atmospheric gaseous sulfuric acid
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We derived the gaseous sulfuric acid concentration proxy on the basis of currently accepted formation pathways of sulfuric acid in the atmosphere (Reactions R1–R3; Finlayson-Pitts and Pitts, 2000; Stockwell and Calvert, 1983):

(R1)OH+SO2HSO3(R2)HSO3+O2SO3+HO2(R3)SO3+2H2OH2SO4+H2O

Reaction (R1) is the rate-limiting step of this formation pathway (Finlayson-Pitts and Pitts, 2000), so our proxy will consider the two major processes that determine the abundance of gaseous sulfuric acid: the formation of gaseous sulfuric acid from reactions between SO2 and OH radicals, and the loss of gaseous sulfuric acid due to its condensation onto preexisting particles (Dal Maso et al., 2002; Kulmala et al., 2012; Pirjola et al., 1999).

The rate of change of sulfuric acid concentration can be written as Eq. (4) (Mikkonen et al., 2011):

(4)dH2SO4/dt=kOHSO2-H2SO4CS,

where k is a temperature-dependent reaction constant given by Eq. (5) (DeMore et al., 1997; Mikkonen et al., 2011).

k=Ak3(A+k3)(5)expk51+log10Ak32-1cm3(molecules)-1,

where A=k1[M]300Tk2, [M] represents the density of the air in molecule cm−3 as calculated by 0.101(1.381×10-23T)-1, k1=4×10-31, k2=3.3, k3=2×10-12 and k5=-0.8.

To simplify the calculation, the production and loss of sulfuric acid can be assumed to be in pseudo-steady-state (Mikkonen et al., 2011; Petäjä et al., 2009). Then the sulfuric acid concentration can be written as follows:

(6)H2SO4=kOHSO2CS-1

Atmospheric OH radical measurements also represent a major challenge. As previous studies suggest that the OH radical concentration is strongly correlated with the intensity of UVB, [OH] could be replaced with UVB intensity in the proxy equation (Petäjä et al., 2009; Rohrer and Berresheim, 2006). Although the photolysis of O3 (λ<320 nm) and subsequent reactions with H2O are considered to be the dominant source of OH radicals in the atmosphere (Logan et al., 1981), recent studies argue that photolysis of HONO (λ<400 nm) is a potentially important OH radical formation pathway (Hendrick et al., 2014; Kleffmann, 2007; Su et al., 2011; Villena et al., 2011). Thus, we attempt to introduce both O3 and HONO into the proxy equation and evaluate their effects on the concentration of OH radicals.

In practice, the exponents for variables in nonlinear fitting procedures are rarely equal to one (Mikkonen et al., 2011), so we replaced the factors xi with xiwi in the proxy, where xi can be an atmospheric variable such as UVB and [SO2], and wi defines xi weight in the proxy. As k is a temperature-dependent reaction constant and varies within a 10 % scope in the atmospheric temperature range of 267.6–292.6 K, i.e., the actual atmospheric temperature variation in this study, we approximately regard k as a constant and use a new scaling factor k0. This methodology has been used previously in the proxies of gaseous sulfuric acid in Hyytiälä, southern Finland (Petäjä et al., 2009). As a result, the general proxy equation can be written as Eq. (7), with the UVB intensity, [SO2], the condensation sink (CS), [O3], and [HONO] (or [NOx]) as predictor variables:

H2SO4=fk0,xiωi,(7)xi=UVB,SO2,CS,O3,HONO

The nonlinear curve-fitting procedures using iterative least square estimation for the proxies of gaseous sulfuric acid concentration based on Eq. (7) were performed using a custom-made MATLAB software. In addition to the correlation coefficient (R), the relative error (RE) is used to evaluate the performance of proxies in the statistical analysis and can be written as follows:

(8)RE=1ni=1n|H2SO4proxy,i-H2SO4meas.,i|H2SO4meas.,i
4 Results and discussion
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4.1 General characteristics of daytime sulfuric acid and atmospheric parameters

Table 1 summarizes the mean, median, and 5 %–95 % percentiles of gaseous sulfuric acid concentrations and other variables measured during the daytime in the campaign. The 5 %–95 % percentile ranges of the UVB intensity, [SO2], [NOx], and [O3] were 0–0.45 W m−2, 0.9–11.4, 3.3–61.4, and 3.5–23.3 ppbv, respectively. Compared with the sites in the study by Mikkonen et al. (2011), Beijing was characterized by a factor of 1.4–13.1 higher mean [SO2] but a factor of 3.4–5.4 lower mean [O3]. The 5 %–95 % percentile range of the CS in Beijing was 0.01–0.24 s−1, which is about 10–100 times higher than corresponding value ranges in Europe and North America. The concentration of gaseous sulfuric acid during this campaign was (2.2–10.0) ×106 molecule cm−3 in the 5 %–95 % percentile range, which is relatively similar to that observed elsewhere around the world. A diurnal mean concentration of 0.74 ppbv for HONO was observed in this campaign, consistent with previous long-term HONO measurements of about 0.48–1.8 ppbv (averaged values) in winter in Beijing (Hendrick et al., 2014; Spataro et al., 2013; Wang et al., 2017), which is a factor of 4–10 higher than HONO concentrations measured in Europe (Alicke et al., 2002, 2003). In addition, Beijing is dry in winter and had a mean ambient relative humidity of 28 % during the campaign.

Table 1Mean, median, and 5 %–95 % percentiles of key atmospheric variables and [H2SO4] during the daytime.

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4.2 Correlations between [H2SO4] and atmospheric variables

Table 2 summarizes the correlation coefficients between [H2SO4] and atmospheric variables using a Spearman-type correlation analysis. Clearly, the UVB intensity is an isolated variable that is independent of all the other variables but that imposes a positive influence on O3 due to the photochemical formation of ozone, and a negative influence on HONO because of HONO's photochemical degradation. The sulfuric acid concentration shows positive correlations with all the other variables. The correlation coefficients between [H2SO4] and [SO2] and between [H2SO4] and UVB intensity are 0.74 and 0.46, respectively, which indicate that [SO2] and UVB have important influences on the formation of atmospheric gaseous sulfuric acid. Accordingly, [O3] and [HONO] show positive correlations with [H2SO4] because both O3 and HONO could be precursors of OH radicals. Surprisingly, a high positive correlation coefficient (0.6) was found between [H2SO4] and the CS, which is in contrast to the conventional thought that the CS describes the loss of gaseous sulfuric acid molecules onto preexisting particles and thus should show a negative correlation. The CS correlates well with [SO2] (r=0.83) and [NOx] (r=0.77); thus, a high CS value, as an indicator of atmospheric particle pollution, is usually accompanied by a high concentration of both SO2 and NOx in urban China, indicating co-emissions. A strong correlation between [HONO] and [NOx] (r=0.88) in our measurement is supported by the fact that HONO can either be heterogeneously formed by reactions of NO2 on various surfaces (Calvert et al., 1994) or homogeneously formed by the gas-phase NO + OH reaction, the former of which is likely dominate for the daytime HONO production in urban Beijing (Liu et al., 2014).

Table 2Correlation coefficients (Spearman type) between [H2SO4] and atmospheric variables during the daytime.

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As the UVB intensity and [SO2] have been reported as the dominating factors for the formation of sulfuric acid (Mikkonen et al., 2011; Petäjä et al., 2009), we further explored the relationship of the measured sulfuric acid concentrations with the UVB intensity and [SO2] using a nonlinear curve-fitting method with a single variable. Figure 1a presents a scatterplot of [H2SO4] against the UVB intensity, color-coded by [SO2]. A good correlation between [H2SO4] and the UVB intensity, laying with [SO2], is evident. A similar scatterplot (Fig. 1b) of [H2SO4] against [SO2], color-coded by the UVB intensity, leads to a similar conclusion.

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Figure 1Correlations (a) between [H2SO4] and UVB intensity, and (b) between [H2SO4] and [SO2] during the 9 February to 14 March 2018 campaign. km is a constant term.

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4.3 Proxy construction

Similar to the nonlinear proxies suggested by Mikkonen et al. (2011), we tested a number of proxies for gaseous sulfuric acid; these proxies are listed in Table 3 with their respective fitting parameters, and their performance summarized in Table 4. The scatterplots of observed [H2SO4] versus predicted values given by proxies are presented in Fig. S1 in the Supplement. In these proxies, the concentration of a gaseous species is in molecule cm−3, the UVB intensity is in W m−2, the CS is in s−1, and k0 is a scaling factor.

Proxy N1 was built using the UVB intensity and [SO2] as the source terms and the CS as the sink term, which follows the conventional idea of H2SO4 formation and loss in the atmosphere. The CS was then removed from this proxy to examine the performance of proxy N2, which then had the UVB intensity and [SO2] as the only predictor variables. As the formation of OH radicals in the atmosphere depends on precursors in addition to UVB, we further attempted to introduce the OH precursor term into the H2SO4 proxy. Proxies N3 and N4 were built by introducing O3 as the only OH precursor to evaluate its influence on the formation of sulfuric acid. Furthermore, we added HONO as another potential precursor for OH radicals, resulting in proxies N5 and N6. Lastly, proxy N7 was built by replacing [HONO] with [NOx] because (1) HONO is not regularly measured, and (2) a good linear correlation between [HONO] and [NOx] was generally observed during the daytime in this campaign, although higher [HONO]∕[NOx] ratios were noted in the morning due to the accumulation of HONO during the night (Fig. 2). The RH was not considered in the current study because a test that introduced RH into the proxies did not result in significantly better performance, which is consistent with conclusions from Mikkonen et al. (2011).

As shown in Table 4, the correlation coefficients are in the range of 0.83–0.86 and REs are in the range of 19.1 %–20.0 %. The exponents for the UVB intensity range from 0.13 to 0.15, and those for [SO2] generally range from 0.38 to 0.41, except in case of proxy N6 (b=0.33). The obtained exponent b for [SO2] is significantly smaller than 1 unlike the assumption in Eq. (6), mainly because [SO2] is also an indicator of air pollution that usually influences the sinks of both OH radicals and sulfuric acid. The exponent for [SO2] ranged from 0.5 to 1.04 in the previous proxy study for European and North American sites (Mikkonen et al., 2011), including values from 0.48 to 0.69 in Atlanta, GA, USA, which was probably quite a polluted site as the measurements were conducted only 9 km from a coal-fired power plant. The obtained value range of the exponent b for [SO2] in our study is probably related to the urban nature of Beijing. The value of exponent c for the CS in proxy N1 is as low as 0.03, which might be due to the covariance of the CS and certain H2SO4 sources that cancels the dependence on the CS, or it might indicate that the CS is actually insufficient in regulating the H2SO4 concentration, as recently suggested by Kulmala et al. (2017). By comparing proxies N1 and N2, we can see that the CS plays a minor role because the exponents of [SO2] and UVB, the overall correlation coefficient, and the REs are almost identical with and without the CS. We can also see the negligible role of the CS when comparing the results of proxies N3 and N4 where O3 is considered. However, the role of the CS becomes evident between proxies N5 and N6 when HONO is introduced: the exponents of [SO2], [O3], and [HONO] significantly increased when taking the CS into account, suggesting that the covariance between HONO and the CS can explain, at least partially, the close-to-zero exponent of the CS in proxies N1–N4. In addition, when [O3] is introduced as the only precursor for OH radicals, minor improvements in the correlation coefficient and RE were obtained, as suggested by comparing proxies N3 and N1. When both [O3] and [HONO] were introduced as OH precursors in proxies N5–N7, the REs show noticeable improvements, and correlation coefficients improved slightly. Altogether, these observations suggest that it is crucial to introduce HONO into the proxy, both in our study and also likely for the previous work where the exponent of the CS is close-to-zero (Mikkonen et al., 2011).

Table 3Proxy functions for the nonlinear fitting procedure.

* UVB is the intensity of ultraviolet radiation b in W m−2; [SO2] is the concentration of sulfur dioxide in molecule cm−3; CS is the condensation sink in s−1; [O3] is the concentration of ozone in molecule cm−3; [HONO] is the concentration of nitrous acid in molecule cm−3; [NOx] is the concentration of nitrogen oxides in molecule cm−3; and k0 is a scaling factor. The superscript numbers define the variables' weight in the proxy, and their values for the best fit are shown in Table 4.

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Table 4Results of the nonlinear fitting procedure for different proxy functions, in addition to the correlation coefficient (R, Pearson type) and the relative error (RE).

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https://www.atmos-chem-phys.net/19/1971/2019/acp-19-1971-2019-f02

Figure 2Correlation between [HONO] and [NOx] during the 9 February to 14 March 2018 campaign. The black line represents a linear fit with a zero intercept.

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Although so far proxy N5 had the best fitting quality, it is impractical to explicitly include [HONO] because HONO measurements are very challenging. As shown in Fig. 2, [HONO] and [NOx] tended to correlate linearly with each other during the daytime in this campaign, with a linearly fitted [HONO]∕[NOx] ratio of around 0.03 and a relative error of 0.42. Occasionally higher [HONO]∕[NOx] ratios could be seen in the morning, which may have been due to the fact that the HONO concentration could have undergone an accumulation process during the nighttime and lead to a deviation from the steady state. Therefore, due to the good correlation, proxy N7 replaces [HONO] by [NOx], a more easily measured variable, and performs as well as proxy N5.

Clearly, proxy N2 provides the simplest parameterization, but proxies N5 and N7 result in the best fitting quality due to the introduction of [HONO]. Figure 3 presents the RE values for proxies N2 and N7, respectively, as a function of linear bins of measured sulfuric acid concentrations. The performance of proxy N7 is considerably better than that of proxy N2 in the sulfuric acid concentration range of (2.2–10) ×106 molecule cm−3, which covers the 5 %–95 % percentiles of the sulfuric acid concentration in this study. In the worst scenario, the RE of proxy N2 is 1.2 times as high as that of proxy N7, e.g., the REs are 16.75 % and 13.99 %, respectively, in the sulfuric acid concentration bin of (4–5) ×106 molecule cm−3, and 16.71 % and 14.42 %, respectively, in the bin of (7–8) ×106 molecule cm−3.

https://www.atmos-chem-phys.net/19/1971/2019/acp-19-1971-2019-f03

Figure 3Performance assessments of proxy N2 and proxy N7. The REs are used to evaluate the performances of proxy N2 and N7, respectively, as a function of linear bins of measured sulfuric acid concentrations.

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4.4 Comparison of measured and predicted [H2SO4]

A comparison between measured and predicted [H2SO4] was performed. Figure 4 includes calculated results from proxies N2 and N7 as well as from a proxy constructed according to measurement in a boreal forest site, Finland, i.e., Eq. (1) (Petäjä et al., 2009). The measured daytime [H2SO4] on 10 March 2018, was above 4×106 molecules cm−3 when averaged to a time resolution of 5 min. The predicted [H2SO4] using proxies N2 and N7 both track the measured [H2SO4] quite well, even when an unexpected dip in the sulfuric acid concentration was observed at around 10:00–11:00. The performance of proxy N7 is better than that of proxy N2 during the entire day, consistent with our results in Fig. 3. The proxy by Petäjä et al. (2009) underestimated the concentrations of sulfuric acid by a factor of 20 or so, which can be attributed to the very different values of the CS between Beijing and the boreal forest. The fact that [H2SO4]Petäjä et al. does not track the measured [H2SO4] even after including a scaling factor indicates that proxies are site-specific and do not necessarily work well in locations other than the location that they were originally developed for. In addition, the direct performance comparison between proxy N2 and the proxy by Petäjä et al. (2009) indicates the importance of assigning exponential weights to variables in the nonlinear fitting procedures, which is consistent with results from Mikkonen et al. (2011).

https://www.atmos-chem-phys.net/19/1971/2019/acp-19-1971-2019-f04

Figure 4Comparison of measured [H2SO4], [H2SO4]N2, [H2SO4]N7, and [H2SO4]Petäjä et al. on 10 March 2018 with a time resolution of 5 min.

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5 Summary and conclusions
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Sulfuric acid is a key precursor for atmospheric NPF. In this study, we constructed a number of proxies for gaseous sulfuric acid concentration according to our measurements in urban Beijing during the winter. According to the obtained proxies and their performance, the UVB intensity and [SO2] were the dominant influencing factors. Hence, the simplest proxy (proxy N2) only involves UVB intensity and [SO2] as shown by Eq. (9). The units for [H2SO4] and [SO2] are molecule cm−3, and the unit for UVB is W m−2.

(9)H2SO4=280.05UVB0.14SO20.40

For a comprehensive consideration of the formation pathways of OH radicals, [O3] and [HONO] as well as the CS should be included (proxy N5), as shown by Eq. (10). The units for [O3] and [HONO] are molecule cm−3 and the unit for the CS is s−1.

H2SO4=0.0072UVB0.15SO20.41CS-0.17(10)(O30.36+HONO0.38)

As HONO measurements are not a regular practice, we can further replace [HONO] with [NOx], shown in Eq. (11), which can be justified by the strong linear correlation between [HONO] and [NOx] observed in this study. The unit for [NOx] is molecule cm−3.

H2SO4=0.0013UVB0.13SO20.40CS-0.17(11)(O30.44+NOx0.41)

We consider this last proxy more reasonable than the others due to the following reasons: it makes the equation physically meaningful as the CS is included as a sink term, and the RE is reduced considerably compared with the other proxies. Overall, this suggests that the photolysis of O3 and HONO are both important OH sources in urban Beijing.

In summary, we recommend using the simplest proxy (proxy N2 as shown in Eq. 9) and a more accurate proxy (proxy N7 as shown in Eq. 11) for calculating daytime gaseous sulfuric acid concentrations in the urban Beijing atmosphere. It is clear that the current proxies are only based on a month-long campaign of sulfuric acid measurements in urban Beijing during winter. Given the dramatic reduction in the concentration of SO2 in recent years (Wang et al., 2018) and the strong dependence of calculated [H2SO4] on [SO2], the performance of the proxies in past and future years remains to be evaluated. Furthermore, the proxies might be site-specific and season-specific. As the proxies were derived with atmospheric parameters in winter, in urban Beijing, the exponents for atmospheric variables in the proxy could have different values for other cities or other seasons. Thus, the proxies in this study should be further tested before their application to other Chinese megacities or other seasons.

Data availability
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Data availability. 

The data in this article are available from the corresponding author upon request (lin_wang@fudan.edu.cn).

Supplement
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Supplement. 

The supplement related to this article is available online at: https://doi.org/10.5194/acp-19-1971-2019-supplement.

Author contributions
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Author contributions. 

LW designed this study. YLu, CY, YF, YC, YLiu, GY, YW, YZ, RY, RB, and CD conducted the field campaign. YLu analyzed data with contributions from LW and all of the other co-authors. YLu and LW wrote the paper with contributions from all of the other co-authors.

Competing interests
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Competing interests. 

The authors declare that they have no conflict of interest.

Acknowledgements
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Acknowledgements. 

This study was financially supported by the National Key R&D Program of China (2017YFC0209505), and the National Natural Science Foundation of China (41575113, 91644213).

Edited by: Timothy Bertram
Reviewed by: two anonymous referees

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Gaseous sulfuric acid is one of the key precursors for atmospheric new particle formation processes, but its measurement remains challenging. This work develops an estimation method for the gaseous sulfuric acid concentration in an urban environment in China using multiple atmospheric variables that are easier to measure. The consideration of the heterogeneous formation of HONO and the subsequent photo-production of OH radicals improves the performance of the estimation method.
Gaseous sulfuric acid is one of the key precursors for atmospheric new particle formation...
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