Sources of nitrous acid (HONO) in the upper boundary layer and lower free troposphere of the North China Plain: insights from the Mount Tai Observatory
- 1Environment Research Institute, Shandong University, Qingdao, Shandong, 266237, China
- 2School of Atmospheric Sciences, Nanjing University, Nanjing, 210023, China
- 3Taishan National Reference Climatological Station, Tai'an, Shandong, 271000, China
- 4Collaborative innovation Center for Climate Change, Jiangsu Province, Nanjing, 210023, China
Correspondence: Likun Xue (firstname.lastname@example.org)
Nitrous acid (HONO) is a significant precursor of atmospheric “detergent” OH radicals and plays a vital role in tropospheric chemistry. The current knowledge about daytime HONO sources is incomplete, and its impact on the tropospheric radical chemistry has not been fully quantified. Existing observational studies of HONO were mostly conducted at the surface, with few efforts focusing on the high-elevation atmosphere. In order to better understand the characteristics and sources of HONO in the upper boundary layer and lower free troposphere, two intensive field observations were carried out at the summit of Mt. Tai (1534 m a.s.l.), the peak of the North China Plain (NCP), in winter 2017 and spring 2018. HONO showed moderate concentration levels (average ± standard deviation: 0.15±0.15 and 0.13±0.15 ppbv), with maximum values of 1.14 and 3.23 ppbv in winter and spring, respectively. Diurnal variation patterns with broad noontime maxima and lower nighttime concentrations were observed during both campaigns, which is distinct from most of the previous studies at the ground level. The Lagrangian particle dispersion model (LPDM, WRF-FLEXPART v3.3) simulations indicated the combined effects of the planetary boundary layer evolution and valley breeze on the daytime HONO peak. A photostationary state (PSS) analysis suggested a strong unknown daytime HONO source with production rates of 0.45±0.25 ppb h−1 in winter and 0.64±0.49 ppb h−1 in spring. Correlation analysis supported the important role of photo-enhanced heterogeneous conversion of NO2 to HONO on the aerosol surface at this high-elevation site. HONO photolysis is the predominant primary source of OH radical and plays a major role in the radical chemistry at Mt. Tai. The model only considering a homogenous HONO source predicted much lower levels of the HOx radicals and atmospheric oxidation capacity than the model constrained with measured HONO data. This study sheds light on the characteristics, sources, chemistry, and impacts of HONO in the upper boundary layer and lower free troposphere in the NCP region.
Nitrous acid (HONO) is an important reactive trace gas in the Earth's atmosphere and plays a pivotal role in tropospheric oxidation chemistry. Photolysis of HONO by sunlight releases the hydroxyl radical (OH), which initiates the oxidation reaction cycles, resulting in the degradation of various primary contaminants and formation of secondary pollutants such as ozone (O3) and secondary aerosols (Alicke et al., 2003). HONO can react with amines to form nitrosamines, which are mutagenic and carcinogenic, and thus affects human health (Sleiman et al., 2010). HONO is also a key player in biosphere–atmosphere interactions and the biogeochemical cycle via dry and wet depositions as well as soil microbial processes (Sörgel et al., 2015). Therefore, it is of high significance to better understand the characteristics, sources, sinks, and environmental consequences of tropospheric HONO.
In comparison to the sink processes that have been relatively well understood, the sources of ambient HONO are still under extensive exploration and discussion. In the ambient atmosphere, HONO can be either directly emitted from various processes, such as combustion and soil emissions (Su et al., 2011; Nie et al., 2015), or formed from the photolysis and chemical reactions of reactive nitrogen-containing substances. The gas-phase reaction of NO with OH (Reaction R1) has long been known as a significant formation pathway of HONO (Platt et al., 1980), which forms a pseudo-steady state with the fast photolysis of HONO in sunlight (Reaction R2) and the reactions with OH (Reaction R3) during the daytime. HONO concentrations in photostationary state (PSS; [HONO]PSS) can be calculated by Eq. (1). However, the field observations in the last decade have indicated that the [HONO]PSS can only account for a small portion of the measured concentrations in a variety of environments (Kleffmann et al., 2005; Zhou et al., 2007; Michoud et al., 2014), suggesting the action of additional daytime HONO sources. To explain the observed HONO levels, some new formation mechanisms have been proposed and tested in the lab or through field studies (Bejan et al., 2006; Monge et al., 2010; Su et al., 2011; Li et al., 2014). Among them, a widely well-received HONO source is the heterogeneous reactions of NO2 on various wet surfaces (Reaction R4), including the ground, buildings, urban grime, and aerosol surfaces (Villena et al., 2011; Wong et al., 2012; Liu et al., 2014; Baergen and Donaldson, 2016). However, the contributions of the individual surface types to ambient HONO formation have not been figured out. Most previous studies have suggested the dominance of the ground surface in heterogeneous HONO formation at the ground level (Alicke et al., 2003; Elshorbany et al., 2009; Ziemba et al., 2010), while some studies have argued that aerosol surface may also play an important role (Colussi et al., 2013; Liu et al., 2014; Tong et al., 2016; Lu et al., 2018).
Up to now, field observational studies of HONO have mainly been conducted at the surface level, with few efforts made at high elevations such as the upper planetary boundary layer (PBL) and lower free troposphere (FT). This has hindered a thorough understanding of the characteristics, processes, and environmental impacts of tropospheric HONO. First, it can be easily expected that the HONO concentrations should be rather low in the upper PBL and lower FT, given the short lifetime of HONO under sunlight. This has been confirmed by the limited measurement studies at mountaintops and aboard aircraft (Acker et al., 2006; Zhou et al., 2007; Ye et al., 2016, 2018). Field observations at high-elevation sites could provide direct constraints for better understanding the vertical distribution and transport processes of HONO. Second, the upper PBL and lower FT are free from the terrestrial (especially ground) surfaces and hence provide an ideal opportunity to evaluate the role of aerosol particles in the heterogeneous formation of HONO. Third, the impacts of HONO on the atmospheric oxidation capacity (AOC) in the upper PBL and lower FT have not been fully quantified. Existing modeling studies may underestimate the AOC of the high-altitude atmosphere owing to the lack of observational data constraints (Kukui et al., 2014). Consequently, in situ observations of HONO in the upper PBL and lower FT are very important to achieve a comprehensive understanding of tropospheric oxidation chemistry.
To investigate the chemical and physical processes in the upper PBL and lower FT over the North China Plain (NCP), one of the most urbanized and polluted regions in China, two intensive field campaigns were carried out at Mt. Tai, the highest mountain over the region, in winter 2017 and spring 2018. This is a part of the Integrated Measurement Campaigns of Air Pollution Complex over the coastal regions of East China (iMAPEC), which aimed to deploy multiple advanced measurement platforms to investigate the three-dimensional distributions and processes governing the formation of regional air pollution over eastern China. A large suite of chemical species and physical properties were measured during the campaigns. This paper describes the measurement results of HONO and related parameters, which are the first report of HONO chemistry in the upper PBL and lower FT in the NCP region. Several models including WRF-FLEXPART, PSS calculation, and the Master Chemical Mechanism (MCM) box model were used to illustrate the origins, formation, and impacts of HONO. Overall, this study demonstrates the moderate pollution levels of HONO in the upper PBL and lower FT in the NCP, and provides some new insights into the roles of aerosol surface in HONO formation as well as the significant effects of HONO photolysis on the atmospheric oxidation capacity in the high-altitude atmosphere.
2.1 Site description
The Mt. Tai Observatory has been widely used as a sampling location to investigate the regional air pollution in the North China Plain region in the past decade (e.g., Gao et al., 2005; Sun et al., 2016; Wen et al., 2018). It stands at the summit of Mount Tai (36∘16′ N, 117∘6′ E, 1534 m a.s.l.), which is at the center of the NCP (see Fig. 1). The geographical location and altitude of Mount Tai make it representative of the regional background air of the region, and it is well within the upper planetary boundary layer during daytime on sunny days and in the residual layer or free troposphere at night. There are some local emissions from small restaurants and temples at the mountain, but the station is situated in the less frequently visited eastern part of the summit, and thus the impact of local anthropogenic emissions can be ignored (Gao et al., 2005). The city of Tai'an (population: over 5.5 million) is located at the foot of Mt. Tai, about 15 km to the south, and the capital city of Shandong province, Ji'nan (population: over 7.4 million), is situated ∼60 km to the north. It should be noted that a 1-year continuous HONO measurement campaign was conducted from September 2015 to August 2016 at an urban site in Ji'nan using the same instrument (D. Li et al., 2018), and its results are compared here with those at Mt. Tai to infer the vertical distributions of HONO in the NCP region. Details of the Mt. Tai Observatory can be found in Gao et al. (2005), Zhou et al. (2010), and Sun et al. (2016). Two intensive field measurement campaigns were conducted during 1–31 December in 2017 and from 5 March to 8 April in 2018.
2.2 Measurement techniques
A large suite of chemical, physical, and meteorological parameters were measured in real time during the campaigns. Here we briefly describe the measurement techniques for the species that were used in the present study. HONO was measured by a long-path absorption photometer (LOPAP-03, QUMA GmbH, Germany). It detects HONO based on the wet chemistry theory, and two channels are designed to eliminate the possible interferences. The detailed description of the LOPAP instrument has been provided by Heland et al. (2001), and it has been successfully applied in various environments (Kleffmann et al., 2005; D. Li et al., 2018; Wen et al., 2019; Y. Liu et al., 2019). During the present study, manual calibrations were performed using 1000 mg L−1 nitrite standard solutions every 4 d to examine the sensitivity of the detector, and the small drift of the baseline was corrected by regular automatic flushing with ultrapure nitrogen (purity of 99.999 %), which was done for 30 min at a time interval of 11 h 30 min. The detection limit is 3 ppt at a time resolution of 30 s, and the measurement precision and accuracy are 1 % and 10 %, respectively.
Nitric oxide (NO) and total nitrogen oxides (NOy) were measured by a commercial instrument (Model T200U, Advanced Pollution Instrumentation (API), USA), equipped with an externally placed molybdenum oxide catalytic converter. Nitrogen dioxide (NO2) was monitored using cavity-attenuated phase-shift spectroscopy, which is highly selective for true NO2 (Model T500U, API, USA). O3 was measured by a UV photometric analyzer (Model T400, API, USA). CO was measured by a gas filter correlation, non-dispersive infrared analyzer (Model 300EU, API, USA). SO2 was measured by an ultraviolet fluorescence analyzer (Model 43C, Thermo Electron Corporation, USA). The fine-particle (PM2.5) mass concentration was measured using a Synchronized Hybrid Ambient Real-time Particulate monitor (SHARP; Thermo Scientific Model 5030). Inorganic water-soluble ions (e.g., , , ) in PM2.5 together with acid and alkaline gases (e.g., HNO3, NH3) were detected by a Monitor for AeRosols and GAses (MARGA, ADI20801, Applikon-ECN, the Netherlands). The particle number size distributions (5–10 000 nm) were measured by a Wide-range Particle Spectrometer (WPS, Model 1000XP, MSP Corporation, USA) and were used to calculate the aerosol surface area density with the assumption that the particles are of a spherical shape. Methane and C2–C10 non-methane hydrocarbons (NMHCs) were measured by taking ambient air samples in stainless-steel canisters on selected days, followed by chemical analysis by GC-FID/ECD/MS in the laboratory of University of California at Irvine (Simpson et al., 2010). C1–C8 carbonyl compounds were observed offline by absorbing ambient air into a 2,4-DNPH sorbent cartridge followed by HPLC analysis (Yang et al., 2018). Meteorological data including temperature, relative humidity (RH), pressure, and wind speed and direction were provided by the Taishan National Reference Climatological Station. Photolysis frequency of NO2 (J(NO2)) was monitored by a filter radiometer (Meteorologie Consult GmbH, Germany), and the measurements were only available during the spring campaign. All of these techniques have been successfully used in many previous studies, where details of the operation, quality assurance, and quality control procedures can be found (e.g., D. Li et al., 2018; Wen et al., 2018).
The photolysis frequencies of J(NO2), J(HONO), and J(O1D) were computed with the NCAR Tropospheric Ultraviolet and Visible (TUV) radiation model (http://cprm.acom.ucar.edu/Models/TUV/Interactive_TUV/, last access: 16 March 2020), with the O3 column density obtained from the Total Ozone Mapping Spectrometer (TOMS, data available at https://giovanni.gsfc.nasa.gov/giovanni/#service=TmAvMp&starttime=&endtime=, last access: 16 March 2020). In spring when the measured J(NO2) was available, the calculated J(HONO) and J(O1D) were scaled with the ratio of measured J(NO2) to calculated J(NO2). In winter, without direct observations of J(NO2), the TUV-calculated J values were approximated by multiplying the average ratio of measured J(NO2) to calculated J(NO2) obtained in spring (i.e., 0.7). It should be noted that such estimation of J values is subject to some uncertainties, especially for those in winter, when direct J(NO2) measurements were unavailable. Nonetheless, scaling the TUV-calculated clear-sky J values with the same ratio should not alter the major conclusion of this study regarding the impacts of HONO photolysis on the HOx sources and atmospheric oxidation capacity.
2.3 Lagrangian particle dispersion model
A Lagrangian particle dispersion model (LPDM, WRF-FLEXPART v3.3) was utilized to investigate the provenance and trajectory of the air masses sampled at Mt. Tai. The Weather Research and Forecasting (WRF) Model, driven by the NCEP FNL reanalysis data (https://rda.ucar.edu/datasets/ds083.3/index.html#sfol-fw?g=201608, last access: 9 March 2020), was run to produce the high-spatial-resolution meteorological field. The horizontal resolution of the WRF model simulations was 20 km, and the vertical direction was divided into 30 layers under 100 hPa, including 18 layers below an altitude of 2 km. In the LPDM simulations, 3000 particles were released for 3 d backward trajectories from the observational station at an altitude of 1400 m a.g.l. The domain was in the range of 25.5–43.5∘ N, 105–126∘ E with grids. The residence time of particles for a thickness of 100 m above the surface in all grid cell was calculated as the “footprint” retroplume, which indicated the distribution of probability or residence time of a simulated air mass at the surface level. This method has been widely applied in previous studies (Stohl et al., 2003; Ding et al., 2009; Pan et al., 2014).
2.4 Chemical box model
A chemical box model was used to simulate the in situ tropospheric oxidation chemistry and quantify the contributions of HONO to the OH source and atmospheric oxidative capacity. It was set up based on the MCM (v3.3.1), a nearly explicit chemical mechanism describing the degradation of 143 primary volatile organic compounds (VOCs) in addition to the latest inorganic reactions (Jenkin et al., 2003; Saunders et al., 2003). The model was constrained with the measured concentrations of NO, NO2, CO, SO2, O3, VOCs, and carbonyls as well as the meteorological conditions at a time interval of 5 min. For VOCs and carbonyls for which the measurements were not in real time, the high-resolution data were approximated as follows. During the daytime when multiple VOC and carbonyl samples were available, the measurement data were interpolated to a time resolution of 5 min. For the period when measurement data were unavailable, the VOC concentrations (except for isoprene) were estimated with the real-time CO data by assuming a linear regression relationship between VOCs and CO (note that the regression was established with the available measurement data of VOCs and CO). The same method was applied for isoprene and carbonyls, but ambient temperature was used instead of CO for isoprene, and multi-linear regression with CO and O3 was used for carbonyls to account for the primary and secondary sources of carbonyls (Yang et al., 2018; Xue et al., 2016). Such approximation may be subject to some uncertainties but should not significantly interfere in the estimation of the role of HONO photolysis in OH sources (Yang et al., 2018). The model computed the major primary production rates of ROx radicals (), including photolysis of O3, HONO, HCHO and other oxygenated VOCs (OVOCs), and the ozonolysis reactions of unsaturated VOCs (Xue et al., 2016). Also calculated by the model was the AOC by OH, which is defined here as the sum reaction rate of OH with NO, NO2, SO2, CO, and VOCs (AOC =Σ(kOH[OH][Xi]): [Xi] is the concentration of the individual reactant species, and KOH is the rate coefficient of OH with Xi). The model simulations were performed for the two campaigns, and a 4 d pre-run was made with constraints of campaign-average data to facilitate the model to a chemical steady state for the unconstrained species. Two model scenarios with and without the measured HONO constraints were constructed to assess the contribution of the unknown HONO sources to the OH chemistry (note that the model only contained the homogeneous source of HONO). This model has been extensively adopted to simulate the radical chemistry and ozone formation in our previous studies (Xue et al., 2014, 2016; Yang et al., 2018).
3.1 Concentration levels and temporal variations
Table 1 summarizes the statistics of major trace gases, PM2.5, and meteorological parameters observed at Mt. Tai during the two campaigns, and the detailed time series of HONO and related species are shown in Figs. S1–S2. The atmospheric conditions at Mt. Tai were dominated by cold and dry weather (especially in winter with average (± standard deviation; SD) temperature and RH of ∘C and 48±20 %, respectively) as well as relatively lower concentrations of air pollutants. This was due to the high elevation of the station, which is primarily located in the lower FT and/or upper PBL during the measurement periods. The sampled air masses at Mt. Tai were rather chemically aged, as indicative of the low NOx∕NOy ratios with average values (±SD) of 0.45±0.21 and 0.25±0.19 in winter and spring, respectively. The average concentrations of NOx (4.64±3.78 ppbv), SO2 (3.8±4.2 ppbv), and PM2.5 (41.1±28.2 µg m−3) in winter were significantly higher than those in spring (2.18±2.09 ppbv for NOx, 1.6±1.6 ppbv for SO2, and 33.7±26.7 µg m−3 for PM2.5), while an opposite seasonal pattern was found for O3 (49±12 ppbv in winter vs. 63±14 ppbv in spring). The ambient levels of HONO were comparable in both seasons, with average mixing ratios (±SD) of 0.15±0.15 and 0.13±0.15 ppbv in winter and spring, respectively. Despite the relatively low average concentration levels, spikes in HONO (and NOx, NOy, CO, and PM2.5) concentrations were frequently encountered throughout the measurement periods (see Figs. S1–S2 in the Supplement), indicating the transport of polluted plumes to the mountaintop. The maximum HONO mixing ratios were recorded at 1.14 and 3.23 ppbv in winter and spring, respectively. The above inspection of data reveals the overall moderate HONO concentration levels as well as the frequent occurrence of HONO-laden plumes in the upper PBL and lower FT of the NCP region.
Table 2 compares the HONO concentration levels at Mt. Tai with those measured at various surface sites as well as in the high-elevation atmosphere around the world. Obviously, the HONO concentrations at Mt. Tai were significantly lower than those observed at the polluted surface sites in China. For example, the ambient HONO levels at Mt. Tai were approximately an order of magnitude lower than those at urban or suburban sites in the NCP and Pearl River Delta (PRD) regions. This is within the realm of expectation considering the height of Mt. Tai and the short lifetime of HONO. A detailed comparison against the measurement results at a nearby urban site will be made in Sect. 3.2 to infer the vertical distribution of HONO in this region. Despite the lower absolute levels, a noteworthy result is that the HONO∕NO2 ratios at Mt. Tai (0.059±0.091 in winter and 0.072±0.080 in spring) are well within the reported ranges (0.041–0.093) obtained at these surface sites (Su et al., 2008b; X. Li et al., 2012; Wang et al., 2017; D. Li et al., 2018; Y. Liu et al., 2019), implying that NO2 might be the key factor governing the regional distribution (or formation) of HONO. Another important finding from the comparison is that the HONO concentrations at Mt. Tai are substantially higher than those measured from the high-elevation atmosphere, e.g., Whiteface Mountain, USA (Zhou et al., 2007); Summit, Greenland (Dibb et al., 2002); Hohenpeissenberg, Germany (Acker et al., 2006); Brocken, Germany (Acker et al., 2001); and aboard research aircraft over the North Atlantic Ocean (Ye et al., 2016), northern Michigan (Zhang et al., 2009), and the southeastern USA (Ye et al., 2018). This demonstrates the higher pollution levels of HONO in the upper PBL and lower FT in the NCP region, which may further lead to a stronger supply of OH radicals and higher atmospheric oxidation capacity in the high-elevation atmosphere. It is very important to pin down the sources of the elevated HONO and fully evaluate their impacts on OH radicals and AOC in the upper PBL and lower FT of the NCP region, which will be detailed in the following sections.
Figure 2 shows the average diurnal variation patterns of HONO and related parameters during the two measurement campaigns. Overall, most pollutants including NO2, NOy, CO, O3, and PM2.5 showed well-defined diurnal profiles with a daytime concentration peak, compared to lower levels during the nighttime (note that the exact peak time varied among the individual pollutants with different lifetimes and photochemical behaviors). This can be explained by the evolution of the PBL, mountain–valley breeze, and atmospheric photochemistry (Sun et al., 2016). Similar diurnal patterns were also found for HONO, showing noontime concentration peaks with relatively lower mixing ratios during the night in both seasons. Such a pattern is quite different from those determined by most previous studies at the ground level, which generally show higher nighttime concentrations but with a daytime trough (Lee et al., 2016; D. Li et al., 2018; Y. Liu et al., 2019; Fu et al., 2019). The noontime HONO maximum (e.g., ∼11:00–15:00 LT) at Mt. Tai suggested the potential upslope transport of HONO to the mountaintop and/or the presence of “additional” daytime sources. The almost coincident noontime concentration peak of CO (e.g., ∼12:00–15:00 LT) confirmed the upslope transport of boundary layer air to the mountaintop. We also examined the diurnal variations of HONO∕NO2, the ratio commonly used to indicate the efficiency of HONO formation from the reactions involving NO2 (Yu et al., 2009). From Fig. 2c, the HONO∕NO2 ratio shows an increasing trend throughout the nighttime together with an extra peak during the midday in both seasons. This indicates nighttime HONO formation and accumulation from the heterogeneous reactions of NO2 as well as the presence of some “additional” daytime sources. The higher daytime HONO∕NO2 ratios in spring than in winter suggest the action of photo-enhanced heterogeneous formation of HONO. The daytime HONO sources will be diagnosed via a detailed PSS calculation in Sect. 3.3.
3.2 Potential transport by PBL evolution and mountain–valley breeze
In this section, we compare our observations at Mt. Tai with the recent year-round measurement results obtained at a surface site in Ji'nan to infer the vertical gradient of HONO over the NCP region, and we examine the vertical transport of HONO with the LPDM modeling. The surface site is located in the downtown of Ji'nan, which is about 60 km to the north of Mt. Tai (Fig. 1), and the measurement data have been reported by D. Li et al. (2018). It should be noticed that both measurements were not conducted at the same time, and only the average conditions of HONO and NO2 in the same season were compared here.
Figure 3 presents the average diurnal variations of HONO, NO2, and HONO∕NO2 at both the surface and mountaintop in winter and spring. Several interesting aspects are clearly illustrated in the figure. First, the diurnal variation patterns are distinct between the surface and the mountaintop. HONO showed higher concentrations at nighttime and lower levels during the day at the surface, which is opposite to the profile at the mountaintop. Second, the HONO and NO2 concentrations at the surface were overall almost an order of magnitude higher than those at Mt. Tai, but the vertical gradient (as indicative of the mountaintop / surface (M / S) concentration ratio) showed a clear diurnal dependence. The M / S ratios of HONO at nighttime (18:00–6:00 LT; with averages of 0.05±0.01 and 0.07±0.02 in winter and spring, respectively) were significantly lower than those during midday (11:00–15:00 LT; 0.28±0.04 and 0.23±0.03). This is also the case for NO2 and should be ascribed to the efficient mixing within the PBL and upslope transport driven by the valley breeze during the daytime. Third, although the HONO∕NO2 ratios were almost comparable at both the surface and Mt. Tai during the night, the daytime ratios were significantly higher at the mountaintop (0.065±0.093 and 0.093±0.094) than at the surface (0.047±0.090 and 0.052±0.040). This implies enhanced HONO formation from the NO2-involved sources at the mountaintop, especially in spring (see Fig. 3).
Can the PBL mixing and mountain–valley breeze transport HONO from the ground level to the mountaintop with an altitude of ∼1.5 km, given its quite short lifetime? The vertical transport distance (σ) driven by the turbulent diffusion can be estimated by the following Eq. (2) (Jacob, 1999):
where Kz is the turbulent diffusion coefficient, and τHONO is the chemical lifetime of HONO. In the early morning when the boundary layer is stable, Kz is usually within the range of 102∼105 cm2 s−1 and increases with the temperature (Zhang et al., 2009). Assuming an overall τHONO of 60 min in the early morning (corresponding to a J(HONO) of s−1), the vertical transport distance of the ground-level HONO is estimated in the range of 9–268 m, far below the altitude of Mt. Tai. This explains the huge difference in the HONO concentrations between the surface site and the mountaintop in the early morning and during the nighttime. Around noontime, the PBL has been developed and Kz is generally on the order of 106 cm2 s−1 (Zhang et al., 2009). Adopting a median value of Kz (5×106 cm2 s−1) and τHONO (25 min; refer to Sect. 3.3 for the lifetime estimation), the maximum transport distance of HONO can be up to 1200 m, which is still below the peak of Mt. Tai. If we further consider the mountain–valley breeze, by adopting a mean upslope wind speed of 1 m s−1 (Kalthoff et al., 2000; Wang et al., 2015), the transport height of HONO by the valley breeze is estimated to be 1500 m. Note that the transported HONO from the ground level may be subject to extensive dilution and more photolysis at higher altitudes. Therefore, the PBL evolution and valley breeze should play an important role in the regional transport of HONO in the mountainous areas.
The LPDM modeling results also support the upslope transport of surface pollution to Mt. Tai. Figure 4 shows the average distributions of the footprint retroplume of the 3 d backward trajectories, computed by the WRF-FLEXPART model, arriving at Mt. Tai during both daytime and nighttime. During the night and early morning (02:00–8:00 LT), obviously, the air masses sampled at Mt. Tai mainly originated from long-range transport and were less affected by the PBL air from the NCP region (Fig. 4a and c). This can be explained by the fact that Mt. Tai is in the free troposphere (or residual layer) and under the influence of a downslope mountain breeze during the nighttime. In comparison, the air masses reaching Mt. Tai in the afternoon (12:00–18:00 LT) primarily came from the boundary layer in the nearby regions (i.e., Ji'nan, Tai'an, and Ji'ning: major cities surrounding Mt. Tai; Fig. 4b and d). Note that the footprint retroplume denotes the residence time of particles within the lowest 100 m near the surface. This demonstrates the efficient transport of regional surface air pollution to the mountaintop with the development of PBL and valley breeze.
3.3 Daytime HONO sources
Exploration of the potential daytime source has been a major objective of the recent HONO observational studies. Here we diagnose the possible daytime sources of HONO in the upper PBL and lower FT by performing a PSS analysis for the measurement data collected at Mt. Tai. According to the measurement-derived J(HONO) (with noontime averages of 6.4±3.5 and s−1 in winter and spring, respectively; see Fig. S3) and the model-simulated OH concentrations (with noontime averages of 2.5±0.7 and molecules cm−3; Fig. S3), the average lifetime of HONO was estimated as 25.7±1.4 and 21.8±16.9 min during noontime (11:00-14:00 LT) in winter and spring, respectively. Given such short lifetimes, the air masses arriving at Mt. Tai at noon should facilitate a steady state for HONO. The PSS concentrations of HONO ([HONO]pss) can be deduced from Eq. (1) if we only take the homogeneous formation from OH+NO reactions, HONO photolysis, and OH+HONO reactions into account. Note that the OH concentrations were simulated with the observation-constrained MCM model as described in Sect. 2.4 (see Fig. S3 for detailed time series of OH). The PSS approach has been widely used in previous studies (Zhou et al., 2002; Kleffmann et al., 2005; Elshorbany et al., 2012).
Figure 5 shows the campaign-average [HONO]pss at noontime and the comparison with the measured HONO concentrations in the two seasons. It is evident that the [HONO]pss was significantly lower than the measured data. On average, [HONO]pss only accounted for 18 and 12 % of the ambient HONO levels at Mt. Tai in winter and spring (see Fig. S4), respectively, demonstrating the existence of strong HONO sources other than the homogeneous OH+NO reactions. To maintain the observed HONO levels, an additional “source” is needed, and its source strength (hereafter referred to as Pother) can be calculated from Eq. (3).
In the present study, the Pother was calculated in the range of 0.01–1.24 and 0.01–4.26 ppb h−1, with average (±SD) values of 0.45±0.25 and 0.64±0.49 ppb h−1 in winter and spring, respectively. In comparison, the noontime HONO production rates from the OH+NO reactions were 0.13±0.10 and 0.09±0.08 ppb h−1, much lower than Pother. The additional source strengths of daytime HONO at Mt. Tai are much lower than those previously reported at the surface sites in Ji'nan (2.95 ppb h−1; D. Li et al., 2018), Beijing (1.83 ppb h−1; Hou et al., 2016), and Santiago, Chile (1.69 ppb h−1; Elshorbany et al., 2009), and are comparable to those derived from the rural or mountain sites, such as Hohenpeissenberg (0.40 ppb h−1; Acker et al., 2006), Whiteface Mountain (0.38 ppb h−1; Zhou et al., 2007), and a forest site in Jülich, Germany (0.50 ppb h−1; Kleffmann et al., 2005). Some studies have reported much lower Pother values obtained from aircraft studies in Michigan (0.057 ppb h−1; Zhang et al., 2009) and in the southern USA (0.17 ppb h−1; Ye et al., 2018).
Recent field and laboratory studies have proposed some potential sources that may help explain the observed higher-than-PSS daytime HONO levels. Among them, direct emissions from vehicle exhaust and soil microbiological processes, heterogeneous conversion of NO2 to HONO on surfaces, and photolysis of adsorbed and aqueous-phase nitrate are relatively well accepted to be relevant in the ambient atmosphere (Zhou et al., 2003; Su et al., 2011; VandenBoer et al., 2013; Y. Liu et al., 2019). It is believed that vehicle and soil emissions should be of minor importance at Mt. Tai, which is free from anthropogenic activities and soil surfaces. We thus diagnosed the potential action of heterogeneous formation of HONO on both ground and aerosol surfaces as well as photolysis of nitrate by examining the relationship between Pother and a variety of indicators for the specific HONO sources. Such a correlation analysis method has been widely applied in many previous studies to identify the most likely additional daytime HONO source, despite the inherent uncertainty in the statistical approach (Su et al., 2008b; Lee et al., 2016; Lu et al., 2018).
Figure 6 shows the scatterplots of Pother against several HONO source indicators during the two campaigns. As illustrated in the figure, Pother shows weak correlation with NO2 (the commonly used indicator for the heterogeneous NO2-to-HONO conversion on the ground surface, assuming that the ground surface density is uniform in the PBL), with correlation coefficients (r) of 0.26 and 0.24 in winter and spring, respectively. This indicates that the heterogeneous reactions on the ground should not be the dominant HONO source at Mt. Tai. When the aerosol surface area density ((S∕V)a) was included, the correlations were significantly improved (Fig. 6b and e), with r values of 0.52 and 0.43, respectively, for Pother and NO2 × (S∕V)a (an indicator of the heterogeneous NO2-to-HONO conversion on the aerosol surface). Furthermore, the correlations were further improved after J(NO2) (an indicator of sunlight) was considered, with r being 0.54 and 0.48 for Pother and J(NO2) × NO2 × (S∕V)a (Fig. 6c and f), respectively. These results suggest that the photo-enhanced heterogeneous reactions of NO2 on the aerosol surface should be a significant daytime HONO source at Mt. Tai. This is different from most previous studies conducted at the ground level showing the dominant role of ground surface in heterogeneous HONO formation (Kleffmann et al., 2003; Su et al., 2008a; Xu et al., 2015; D. Li et al., 2018), and it highlights the importance of the aerosol surface in HONO formation in the upper PBL and lower FT. Furthermore, Fig. S5 shows the relatively weak correlation between Pother and J(NO2) × (the indicator for the photolysis of particulate nitrate), with r of 0.17 and 0.03, respectively, indicating that the nitrate photolysis is relatively insignificant to the ambient HONO at Mt. Tai.
a OVOC photolysis denotes the photolysis of OVOCs other than formaldehyde. b Rate is the midday (09:00-15:00 LT) average radical production rate. c Proportion is the ratio of the target radical source to the total quantified radical primary production rates.
There is the possible interference of peroxynitric acid (PNA; HO2NO2) for measuring HONO by the LOPAP especially in cold environments. While the LOPAP instrument has been extensively tested for a variety of interferences (Heland et al., 2001; Kleffmann and Wiesen, 2008), some recent studies have reported that it may be subject to positive interference from HO2NO2 (e.g., Legrand et al., 2014). Due to the thermal instability of HO2NO2, its interference is generally negligible at ambient temperatures at the ground level but may become important in circumstances of low temperature and active photochemistry. Legrand et al. (2014) reported that the interference of HO2NO2 in their HONO measurements was about 15 % according to laboratory experiments. In the present study, we did not conduct in situ measurements of HO2NO2. To estimate the potential interference for our HONO measurements, we simulated the HO2NO2 concentrations at Mt. Tai in both campaigns with the MCM chemical box model constrained with all measured species, including HONO. Figure S6 shows the time series of modeled HO2NO2 and its comparison with the measured HONO and missing HONO (measured HONO minus [HONO]pss) concentrations. Overall, moderate concentration levels of HO2NO2 were predicted by the model at Mt. Tai, with average values (±SD) of 0.07±0.06 ppbv and 0.03±0.04 ppbv in winter and spring, respectively. When we took a HO2NO2 interference of 15 % (Legrand et al., 2014), the potential interference in the missing HONO was 16 %±15 % and 11 %±10 % in winter and spring, respectively. Figure S7 shows the scatterplots of missing HONO versus [NO2] × J(NO2), an indicator of HO2NO2 production. As we can see, the correlation was rather weak between missing HONO and [NO2] × J(NO2), especially in winter (r=0.19). This indicates that the interference from HO2NO2 may not be a major factor in the determined missing HONO, and more experiments are needed to confirm and quantify the possible interferences to the ambient HONO observations.
3.4 Impacts of HONO on OH radical and atmospheric oxidation capacity
The detailed chemical budget of ROx radicals was explored by the observation-based MCM box model. Figure 7 shows the average diurnal profiles of primary production rates of OH, HO2, and RO2 radicals from major sources at Mt. Tai during the two campaigns, and the statistical results are documented in Table 3. Two points are noteworthy here. First, the primary production rates of ROx radicals at Mt. Tai were substantially lower than those derived from most of the ground-level sites over China, such as Beijing (Liu et al., 2012; Yang et al., 2018), Wuhan (Lu et al., 2017), Chengdu (Tan et al., 2018), Hong Kong (Xue et al., 2016; Z. Li et al., 2018), and a rural site in the Yellow River Delta region (Chen et al., 2020). Note that most of these previous studies were based on modeling of the polluted photochemical episodes, but the modeled highest ROx production rates at Mt. Tai were still lower than those in these studies. The model-simulated daily maximum AOC (defined here as the sum of reaction rates of OH with NOx, SO2, CO, and VOCs) at Mt. Tai was in the range of 1.3–3.9×107 and 0.6–10.8×107 molecules cm−3 s−1 in winter and spring (see Fig. S8), respectively, which are still much lower than values at the abovementioned surface sites (Xue et al., 2016; Yang et al., 2018; Z. Li et al., 2018). This demonstrates the relatively lower oxidation capacity of the upper PBL and lower FT atmosphere compared to the polluted surface-layer air. Nonetheless, the primary ROx production rates at Mt. Tai were comparable to those obtained from Hohenpeissenberg, Germany (Acker et al., 2006); Whiteface Mountain (Zhou et al., 2007); and Pinnacle State Park, a rural site in southwestern New York (Zhou et al., 2002).
Second, photolysis of HONO presents the predominant primary OH source, and it is also among the most important sources of ROx at Mt. Tai. In winter, HONO photolysis was overwhelmingly the primary source of ROx radicals, with a midday (09:00–15:00 LT) average production rate 0.520 ppb h−1, followed by photolysis of OVOCs other than formaldehyde (0.210 ppb h−1 for HO2 and 0.182 ppb h−1 for RO2) and formaldehyde (0.193 ppb h−1 for HO2), ozonolysis reactions of unsaturated VOCs (0.036 ppb h−1 for ROx), and O3 photolysis (0.022 ppb h−1 for OH). In spring, in comparison, photolysis of OVOCs other than formaldehyde turns out to be the dominant ROx source (with a midday average rate of 0.434 ppb h−1 for HO2 and 0.407 ppb h−1 for RO2), followed by photolysis of HONO (0.511 ppb h−1 for OH), formaldehyde (0.374 ppb h−1 for HO2) and O3 (0.178 ppb h−1 for OH), and reactions of O3+VOCs (0.057 ppb h−1 for ROx). In percentage, HONO photolysis accounted for 44.4 and 25.8 % of the total primary ROx production at midday at Mt. Tai in winter and spring, respectively. For OH alone, the percentages of the contribution of HONO photolysis to the primary sources were 93.2 and 71.3 % in winter and spring, respectively. Evidently, HONO photolysis plays a very important role in the OH supply and hence jump-start of atmospheric oxidation chemistry in the upper PBL and lower FT in the NCP region.
How much do the additional HONO sources (other than the homogeneous OH+NO source) affect the atmospheric photochemistry in the upper PBL and lower FT? To evaluate this issue, two modeling scenarios were performed, with and without constraints of the measured HONO data. The model only contains the homogeneous HONO formation from OH+NO reactions, and thus the difference between both scenarios can represent the effects of the additional daytime HONO sources. Figure 8 documents the differences in the model-simulated OH, HO2, AOC, and POH (primary production rate of OH) between the two scenarios in winter and spring. Clearly, the model only considering the homogeneous source and without observational constraints predicted much lower levels of the HOx radicals and AOC at Mt. Tai. Specifically, the discrepancy in the midday (09:00–15:00) average POH, OH, HO2, and AOC can be up to 83.4 % (63.7 %), 47.2 % (27.1 %), 39.7 % (20.3 %), and 46.1 % (26.4 %) in winter (spring), respectively, compared to the base scenario with constraints of the measured HONO data. Given the essential role of HOx radicals in atmospheric chemistry, the models would largely underestimate the atmospheric oxidation processes in the upper PBL and lower FT if the measurement data and/or additional HONO source mechanisms were absent. So far, direct observations of HONO in the high-elevation atmosphere are still lacking, and accurate representation of the HONO sources in atmospheric chemistry models is underway. This study highlights the significance of HONO chemistry in the upper PBL and lower FT in the NCP region, and calls for more efforts to address the tempo-spatial variations and sources of HONO in the high-elevation atmosphere.
We analyzed the characteristics, sources, and impacts on tropospheric oxidation chemistry of ambient HONO in the upper PBL and lower FT of the NCP region, by conducting intensive field observations at Mt. Tai (the peak of the region) followed by detailed modeling analyses. Moderate concentration levels of HONO were observed, which are higher than those measured from other high-elevation areas around the world. HONO showed a distinctive diurnal variation pattern at Mt. Tai with a daytime concentration peak, compared to lower levels at night, which is opposite to the results determined at the ground level. The evolution of PBL and the upslope transport driven by valley breezes explained the observed daytime HONO peak. The data were compared with the year-round continuous measurement results at a nearby surface urban site to infer the vertical gradient of HONO in the NCP region. Strong additional daytime HONO sources other than homogeneous OH+NO reactions existed in the PBL, and the PSS estimation only accounted for 18 and 12 % of the observed HONO in winter and spring, respectively. The photo-enhanced heterogeneous reactions of NO2 on aerosol surface appears to be an important HONO source. HONO photolysis is the predominant primary source of OH radical and plays a major role in the radical chemistry at Mt. Tai. With only inclusion of the OH+NO reactions, significant reductions of the modeled OH (by ∼47.2 %; 27.1 %), HO2 (by ∼39.7 %; 20.3 %), POH (by ∼83.4 %; 63.7 %), and AOC (by ∼46.1 %; 26.4 %) were found, compared with being constrained by observed HONO data. This study elucidates the significant role of HONO in the atmospheric oxidation chemistry in the upper PBL and lower FT of the NCP region, where previous studies mainly focused on HONO at the ground level.
The measurement data and model output used in the present study can be accessed from https://data.mendeley.com/datasets/wcn84cybx9/draft?a=e87e4e3e-4ad2-45e4-96e4-697a7533cb37 (Jiang and Xue, 2020). The code for the MCM model can be downloaded from the MCM website (http://mcm.leeds.ac.uk/MCMv3.3.1/home.htt, last access: 20 October 2020).
The supplement related to this article is available online at: https://doi.org/10.5194/acp-20-12115-2020-supplement.
LX designed the research. YJ performed the field observations, analyzed data, and wrote the paper. RG, LW, PZ, TC, HL, YS, YZ, ZG, YB, and HL carried out the field observations at Mt. Tai. MJ and AD conducted the WRF-FLEXPART analyses. YZ conducted the MCM modeling analyses. LX, AD, QZ, and WW helped in the interpretation of results and revised the original manuscript.
The authors declare that they have no conflict of interest.
The authors thank all the staff of the Taishan National Reference Climatological Station for their logistical support and help during the field observations. We are grateful to the MCM group of the University of Leeds for provision of the MCM model. We thank the three anonymous referees, whose comments were very helpful in improving the original manuscript.
This research has been supported by the National Key Research and Development Program of China (grant no. 2016YFC0200500), the National Natural Science Foundation of China (grant nos. 41922051 and 91544213), the Shandong Provincial Science Foundation for Distinguished Young Scholars (grant no. ZR2019JQ09), the Jiangsu Collaborative Innovation Center for Climate Change, and the Taishan Scholars (grant no. ts201712003).
This paper was edited by James Roberts and reviewed by three anonymous referees.
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