On the oxidation of SO2 to sulfate in atmospheric aerosols

This paper presents the results of a study to investigate the atmospheric oxidation of sulfur dioxide (SO₂). A detailed model of gas-phase chemistry, aerosol thermodynamics and aerosol chemistry is employed to simulate atmospheric sulfate formation. The calculations indicate that, in addition to the gasphase oxidation by hydroxyl (OH) radicals, SO₂ oxidation in aqueous aerosols may also contribute significantly to sulfate formation. Reactions of SO₂ with hydrogen peroxide (H₂O₂) and O₂ (catalyzed by Fe³⁺ and Mn²⁺) are identified as principal aqueous-phase oxidation mechanisms. The results of this study confirm the conclusions drawn from the analysis of ambient aerosol data qualitatively. However, some discrepancies also exist between the results of our modeling study and field data. Such discrepancies emphasize the need for the collection of ambient data for a more rigorous and quantitative evaluation of atmospheric aerosol models.     

Sources of hydrogen peroxide in cloudwater

Results of a theoretical investigation of H₂O₂ formation in cloud droplets arising from gaseous HO₂ radical scavenging are presented. It is shown that this process is pH dependent with the maximum rate of H₂O₂ production occurring below pH 3. This dependence arises as a result of the dissociation of HO₂ in water (pK_a = 4.9) and the subsequent disproportionation reaction of HO₂ and O₂⁻ to form hydrogen peroxide. O₂⁻ is also removed by reaction with O₃ to produce OH radicals and this process becomes more competitive as both the pH and $\text{O}{}_2{}^{\mathrm{-}}\text{HO}{}_2$ ratio increase. The presence of soluble organic species, such as aldehydes, in cloudwater counteracts the effect of ozone by converting OH back to HO₂. For low pHs (< 3) the net contribution of organic solutes of H₂O₂ production is predicted to be relatively small, being limited by the availability of OH radicals scavenged from the gas phase. Existing cloud chemistry models may overestimate the rate of aqueous oxidation of formaldehyde by OH radicals.Under conditions where scavenging of gas-phase free radicals by cloud droplets is efficient, uptake of HO₂ radicals may be reversible. The aqueous concentration of OH is unlikely to approach thermodynamic equilibrium with the gas phase (H ∼-30 M atm⁻¹ and can be treated as irreversible. In clouds with a small mean droplet radius, efficient scavenging of precursor OH radicals should result in a decrease in gas-phase HO₂ production with a reduction in the yield of aqueous H₂O₂, although this is offset by the presence of soluble organic species. A similar effect is predicted for clouds with a high liquid water content.The supply of HO₂ and OH radicals to cloud droplets is controlled by gas-phase ozone chemistry which is in turn dependent on the solar u.v. radiation intensity. The u.v. density in clouds may be higher than in clear air when the solar zenith angle is small, thus enhancing H₂O₂ production, but falls off markedly as the solar zenith angle becomes larger. Predicted rates of H₂O₂ formation in clouds based on midday conditions are likely to be considerably higher than the average daytime value, particularly in summer. Diurnal and seasonal effects on H₂O₂ generation are expected to be more marked in clouds than in clear air.     

Scientific uncertainties in atmospheric mercury models II: Sensitivity analysis in the CONUS domain

In this study, we present the response of model results to different scientific treatments in an effort to quantify the uncertainties caused by the incomplete understanding of mercury science and by model assumptions in atmospheric mercury models. Two sets of sensitivity simulations were performed to assess the uncertainties using modified versions of CMAQ-Hg in a 36-km Continental United States domain. From Set 1 Experiments, it is found that the simulated mercury dry deposition is most sensitive to the gaseous elemental mercury (GEM) oxidation product assignment, and to the implemented dry deposition scheme for GEM and reactive gaseous mercury (RGM). The simulated wet deposition is sensitive to the aqueous Hg(II) sorption scheme, and to the GEM oxidation product assignment. The inclusion of natural mercury emission causes a small increase in GEM concentration but has little impact on deposition. From Set 2 Experiments, it is found that both dry and wet depositions are sensitive to mercury chemistry. Change in model mercury chemistry has a greater impact on simulated wet deposition than on dry deposition. The kinetic uncertainty of GEM oxidation by O₃ and mechanistic uncertainty of Hg(II) reduction by aqueous HO₂ pose the greatest impact. Using the upper-limit kinetics of GEM–O₃ reaction or eliminating aqueous Hg(II)–HO₂ reaction results in unreasonably high deposition and depletion of gaseous mercury in the domain. Removing GEM–OH reaction is not sufficient to balance the excessive mercury removal caused by eliminating the HO₂ mechanism. Field measurements of mercury dry deposition, better quantification of mercury air-surface exchange and further investigation of mercury redox chemistry are needed for reducing model uncertainties and for improving the performance of atmospheric mercury models.     

Aqueous h2o2 production from o3 in glass impingers

The aqueous generation of H₂O₂ from bubbling ozonized air through water in glass impingers is investigated. O₃ loss is monitored throughout each experiment. Aqueous H₂O₂ is measured at the end of each experiment. The mole quantities of O₃ lost (ΔO₃) and H₂O₂ formed (ΔH₂O₂) are calculated. There is a stoichiometric relationship between ΔO₃ and ΔH₂O₂ which is independent of bubbling time, solution acidity and initial O₃ concentration but is dependent upon the liquid water content of each impinger. For 10 ml of water in each impinger, the AO₃ to ΔH₂O₂ mole ratio is between 2:1 and 3:1 and for 20 ml is between 1:1 and 1:2. Increasing the solution acidity increases the rates of O₃ loss and H₂O₂ generation. This result contradicts mechanisms in which a O₃ + HO⁻ reaction is used to initiate radical formation and H₂O₂ production.These results are interpreted through a combination of glass surface chemistry and bulk aqueous chemistry. The O₃-H₂O₂ impinger mechanisms involve O₃ adsorption and/or reaction on the impinger surface and its surface products subsequent reaction with water or trace impurities in the water. Experiments using tetrafluorethylene (TFE) impingers in place of glass impingers are conducted to examine the role of surface chemistry. The TFE impingers are found to substantially increase ΔO₃ and ΔH₂O₂ without changing their mole ratio. This is attributed to an enhanced O₃-H₂O surface chemistry or O₃ reaction with unsaturated Teflon linkages or impurities in the Teflon from machining.     

An assessment of the polar HOx photochemical budget based on 2003 Summit Greenland field observations

An interpretative modeling analysis is conducted to simulate the diurnal variations in OH and HO₂+RO₂ observed at Summit, Greenland in 2003. The main goal is to assess the HO_x budget and to quantify the impact of snow emissions on ambient HO_x as well as on CH₂O and H₂O₂. This analysis is based on composite diurnal profiles of HO_x precursors recorded during a 3-day period (July 7–9), which were generally compatible with values reported in earlier studies. The model simulations can reproduce the observed diurnal variation in HO₂+RO₂ when they are constrained by observations of H₂O₂ and CH₂O. By contrast, model predictions of OH were about factor of 2 higher than the observed values. Modeling analysis of H₂O₂ suggests that its distinct diurnal variation is likely controlled by snow emissions and loss by deposition and/or scavenging. Similarly, deposition and/or scavenging sinks are needed to reproduce the observed diel profile in CH₂O. This study suggests that for the Summit 2003 period snow emissions contribute ∼25% of the total CH₂O production, while photochemical oxidation of hydrocarbon appears to be the dominant source. A budget assessment of HO_x radicals shows that primary production from O(¹D)+H₂O and photolysis of snow emitted precursors (i.e., H₂O₂ and CH₂O) are the largest primary HO_x sources at Summit, contributing 41% and 40%, respectively. The snow contribution to the HO_x budget is mostly in the form of emissions of H₂O₂. The dominant HO_x sink involves the HO₂+HO₂ reaction forming H₂O₂, followed by its deposition to snow. These results differ from those previously reported for the South Pole (SP), in that primary production of HO_x was shown to be largely driven by both the photolysis of CH₂O and H₂O₂ emissions (46%) with smaller contributions coming from the oxidation of CH₄ and the O(¹D)+H₂O reaction (i.e., 27% each). In sharp contrast to the findings at Summit in 2003, due to the much higher levels of NO_x, the SP HO_x sinks are dominated by HO_x–NO_x reactions, leading to the formation and deposition of HNO₃ and HO₂NO₂. Thus, a comparison between SP and Summit studies suggests that snow emissions appear to play a prominent role in controlling primary HO_x production in both environments. However, as regards to maintaining highly elevated levels of OH, the two environments differ substantially. At Summit the elevated rate for primary production of HO_x is most important; whereas, at SP it is the rapid recycling of the more prevalent HO₂ radical, through reaction with NO, back to OH that is primarily responsible.     

Modeling study of the potential importance of heterogeneous surface reactions for NOx transformations in plumes

A parametric model of gas-particle surface reactions is incorporated into a reactive plume model and used to assess the potential importance of heterogeneous surface reactions on gas phase plume chemistry. Heterogeneous loss of the following species is found to be potentially significant: H₂O₂, PAN, NO₃, N₂O₅, OH, HO₂ and in cold weather HO₂NO₂. This simple model is unable to account for equilibrium/capacity effects in the condensed phase and therefore cannot be used for SO₂ and HNO₃ reaction with aerosol surface.     

South Pole Antarctica observations and modeling results: New insights on HOx radical and sulfur chemistry

Measurements of OH, H₂SO₄, and MSA at South Pole (SP) Antarctica were recorded as a part of the 2003 Antarctic Chemistry Investigation (ANTCI 2003). The time period 22 November, 2003–2 January, 2004 provided a unique opportunity to observe atmospheric chemistry at SP under both natural conditions as well as those uniquely defined by a solar eclipse event. Results under natural solar conditions generally confirmed those reported previously in the year 2000. In both years the major chemical driver leading to large scale fluctuations in OH was shifts in the concentration levels of NO. Like in 2000, however, the 2003 observational data were systematically lower than model predictions. This can be interpreted as indicating that the model mechanism is still missing a significant HO_x sink reaction(s); or, alternatively, that the OH calibration source may have problems. Still a final possibility could involve the integrity of the OH sampling scheme which involved a fixed building site. As expected, during the peak in the solar eclipse both NO and OH showed large decreases in their respective concentrations. Interestingly, the observational OH profile could only be approximated by the model mechanism upon adding an additional HO_x radical source in the form of snow emissions of CH₂O and/or H₂O₂. This would lead one to think that either CH₂O and/or H₂O₂ snow emissions represent a significant HO_x radical source under summertime conditions at SP. Observations of H₂SO₄ and MSA revealed both species to be present at very low concentrations (e.g., 5 × 10⁵ and 1 × 10⁵ molec cm^?3, respectively), but similar to those reported in 2000. The first measurements of SO₂ at SP demonstrated a close coupling with the oxidation product H₂SO₄. The observed low concentrations of MSA appear to be counter to the most recent thinking by glacio-chemists who have suggested that the plateau's lower atmosphere should have elevated levels of MSA. We speculate here that the absence of MSA may reflect efficient atmospheric removal mechanisms for this species involving either dynamical and/or chemical processes.     

Optimizing model performance: variable size resolution in cloud chemistry modeling

Under many conditions size-resolved aqueous-phase chemistry models predict higher sulfate production rates than comparable bulk aqueous-phase models. However, there are special circumstances under which bulk and size-resolved models offer similar predictions. These special conditions include alkaline conditions (when there is a high ammonia to nitric acid ratio or a large amount of alkaline dust) or conditions under which the initial H₂O₂ concentration exceeds that of SO₂. Given that bulk models are less computationally-intensive than corresponding size-resolved models, a model equipped to combine the accuracy of the size-resolved code with the efficiency of the bulk method is proposed in this work. Bulk and two-section size-resolved approaches are combined into a single variable size-resolution model (VSRM) in an effort to combine both accuracy and computational speed. Depending on initial system conditions, bulk or size-resolved calculations are executed based on a set of semi-empirical rules. These rules were generated based on our understanding of the system and from the results of many model simulations for a range of input conditions. For the conditions examined here, on average, the VSRM sulfate predictions are within 3% of a six-section size-resolved model, but the VSRM is fifteen times faster.     

Chemistry of HOx radicals in the upper troposphere

Aircraft observations from three recent missions (STRAT, SUCCESS, SONEX) are synthesized into a theoretical analysis of the factors controlling the concentrations of HO_x radicals (HO_x=OH+peroxy) and the larger reservoir family HO_y (HO_y=HO_x+2H₂O₂+2CH₃OOH+HNO₂+HNO₄) in the upper troposphere. Photochemical model calculations capture 66% of the variance of observed HO_x concentrations. Two master variables are found to determine the variance of the 24 h average HO_x concentrations: the primary HO_x production rate, P(HO_x), and the concentration of nitrogen oxide radicals (NO_x=NO+NO₂). We use these two variables as a coordinate system to diagnose the photochemistry of the upper troposphere and map the different chemical regimes. Primary HO_x production is dominated by the O(¹D)+H₂O reaction when [H₂O]>100 ppmv, and by photolysis of acetone (and possibly other convected HO_x precursors) under drier conditions. For the principally northern midlatitude conditions sampled by the aircraft missions, the HO_x yield from acetone photolysis ranges from 2 to 3. Methane oxidation amplifies the primary HO_x source by a factor of 1.1–1.9. Chemical cycling within the HO_x family has a chain length of 2.5–7, while cycling between the HO_x family and its HO_y reservoirs has a chain length of 1.6–2.2. The number of ozone molecules produced per HO_y molecule consumed ranges from 4 to 12, such that ozone production rates vary between 0.3 and 5 ppbv d⁻¹ in the upper troposphere. Three chemical regimes (NO_x-limited, transition, NO_x-saturated) are identified to describe the dependence of HO_x concentrations and ozone production rates on the two master variables P(HO_x) and [NO_x]. Simplified analytical expressions are derived to express these dependences as power laws for each regime. By applying an eigenlifetime analysis to the HO_x–NO_x–O₃ chemical system, we find that the decay of a perturbation to HO_y in the upper troposphere (as from deep convection) is represented by four dominant modes with the longest time scale being factors of 2–3 times longer than the steady-state lifetime of HO_y.     

Aqueous-phase nitration of phenol by N2O5 and ClNO2

Nitrophenols are present in the atmospheric gas phase and in cloud and rainwater. Their formation via aqueous-phase reactions of phenol with the nitronium ion, NO₂⁺, arising from N₂O₅ and ClNO₂ partitioning into the aqueous phase, has been proposed but not verified experimentally. Here, we demonstrate for the first time that gaseous N₂O₅ and ClNO₂ partitioning into dilute aqueous solutions of phenol yields 2- and 4-nitrophenol (and 4-nitrosophenol), but no dinitrophenol isomers. The rate of nitration does not vary significantly between 5 and 20 °C, presumably because of opposing temperature dependences in Henry's law partitioning and reaction rate coefficients. The rate coefficient for reaction of NO₂⁺ with phenol could not be directly quantified but is evidently large enough for this reaction to compete effectively with the reaction between NO₂⁺ and water and to provide a feasible route to nitrophenol production in the atmosphere.     

A comparison of chemical mechanisms based on TRAMP-2006 field data

A comparison of a model using five widely known mechanisms (RACM, CB05, LaRC, SAPRC-99, SAPRC-07, and MCMv3.1) has been conducted based on the TexAQS II Radical and Aerosol Measurement Project (TRAMP-2006) field data in 2006. The concentrations of hydroxyl (OH) and hydroperoxy (HO₂) radicals were calculated by a zero-dimensional box model with each mechanism and then compared with the OH and HO₂ measurements. The OH and HO₂ calculated by the model with different mechanisms show similarities and differences with each other and with the measurements. First, measured OH and HO₂ are generally greater than modeled for all mechanisms, with the median modeled-to-measured ratios ranging from about 0.8 (CB05) to about 0.6 (SAPRC-99). These differences indicate that either measurement errors, the effects of unmeasured species or chemistry errors in the model or the mechanisms, with some errors being independent of the mechanism used. Second, the modeled and measured ratios of HO₂/OH agree when NO is about 1 ppbv, but the modeled ratio is too high when NO was less and too low when NO is more, as seen in previous studies. Third, mechanism–mechanism HO_x differences are sensitive to the environmental conditions – in more polluted conditions, the mechanism–mechanism differences are less. This result suggests that, in polluted conditions, the mechanistic details are less important than in cleaner conditions, probably because of the dominance of reactive nitrogen chemistry under polluted conditions.     

Importance of formaldehyde in cloud chemistry

A physical-chemical model which is an extension of that of Hong and Carmichael (1983) is used to investigate the role of formaldehyde in cloud chemistry. This model takes into account the mass transfer of SO₂, O₃, NH₃, HNO₃, H₂O₂, CO₂, HCl, HCHO, O₂, OH and HO₂ into cloud droplets and their subsequent chemical reactions. The model is used to assess the importance of S(IV)-HCHO adduct formation, the reduction of H₂O₂ by HCHO, HCHO-free radical interactions, and the formation of HCOOH in the presence of HCHO in cloud droplets.Illustrative calculations indicate that the presence of HCHO inhibits sulfate production rate in cloud droplets. The direct inhibition of sulfate production rate in cloud water due to nucleophilic addition of HSO⁻₃ to HCHO_(aq) to form hydroxymethanesulfonate (HMSA) is generally low for concentrations of HCHO typical of ambient air. However, inhibition of sulfate production due to formaldehyde-free radical interactions in solution can be important. These formaldehyde-free radical reactions can also generate appreciable quantities of formic acid.     

Numerical studies of acidification processes within and below clouds with a flow-through chemical reactor model

A flow-through chemical reactor model has been exercised to assess the importance of various oxidation reactions and cloud processes on wet removal and redistribution of atmospheric pollutants and to investigate the effect of in-cloud acidification on precipitation chemistry at the surface. Preliminary results indicate that in-cloud acidification accounts for more than 60% of the wet deposited acids derived from acidification of initial SO₂, that 42–57% of water-soluble, non-reactive NH₃ and HNO₃ are removed by wet deposition. The pseudo-first-order conversion rate of SO₂ to SO₄²⁻ ranges from 3 to 25% h ⁻¹ depending on initial and boundary conditions.Sensitivity studies have been carried out to test the importance of time evolution of clouds on partitioning of pollutants in the atmosphere and to investigate the variability of precipitation chemistry due to changes in rate constants. The distributions of NH₃ and HNO₃ are found to be dependent largely on the cloud microphysical parameters, while the distributions of H₂O₂ and SO₂ depend largely on initial conditions of both species. Individual physical and chemical mechanisms can determine the overall rate of sulfate wet deposition at different stages of cloud evolution.     

Steady-state modelling of hydroxyl radical concentrations at Mace Head during the EASE ’97 campaign,May 1997

Two different steady-state methods are applied to calculate OH radical concentrations based on the rates of known source and sink processes. The first method, which calculates only OH radical concentrations from measured data including HO₂ gives good correlation with measured OH concentrations but overpredicts by 30%. The second method applied calculates OH, HO₂ and RO₂ radical concentrations simultaneously. This second method overestimates the measured concentrations of OH by almost 3 times. This apparent overprediction may be a result of calculated concentrations of HO₂ which appear too high and may be indicative of a gap in our understanding of the relevant peroxy radical chemistry or a result of the limited peroxy radical chemistry assumed by the method.     

Redistribution of free tropospheric chemical species over West Africa: radicals (OH and HO₂), peroxide (H₂O₂) and acids (HNO₃ and H₂SO₄)

The purpose of this paper is to study the redistribution of chemical species (OH, HO₂, H₂O₂, HNO₃ and H₂SO₄) over West Africa, where the cloud cover is ubiquitously present, and where deep convection often develops. In this area, because of these cloud systems, chemical species are redistributed by the ascending and descending flow, or leached if they are soluble. So, we carry out a mesoscale study using the Regional Atmospheric Modelling System (RAMS) coupled to a code of gas and aqueous chemistry (RAMS_Chemistry). It takes into account all processes under mesh. We examine several cases following the period (November and July), with inputs emissions (anthropogenic, biogenic and biomass burning). The radicals OH and HO₂ are an indicator of possibilities for chemical activity. They characterize the oxidizing power of the atmosphere and are very strong oxidants. The acids HNO₃ and H₂SO₄ are interesting in their transformation into nitrates and sulfates in precipitation. In November, when photochemistry is active during an event of biomass burning, concentrations of chemical species are higher than those of November in the absence of biomass burning. The concentrations of nitric acid double and sulfuric acid increases 70 times. In addition, the concentrations are even lower in July if there is a deep convection. Compared to measures of the African Monsoon Multidisciplinary Analysis (AMMA), the results and observations of radicals OH and HO₂ are the same order of magnitude. Emissions from biomass burning increase the concentrations of acid and peroxide, and a deep convection cloud allows the solubility and the washing out of species, reducing their concentration. Rainfalls play a major role in solubility and washing out acids, peroxides and radicals in this region.     

OH and HO2 measurements in a forested region of north-western Greece

Boundary layer concentrations of hydroxyl (OH) and hydroperoxyl (HO₂) radicals were measured at 1180 m elevation in a mountainous, forested region of north-western Greece during the AEROsols formation from BIogenic organic Carbon (AEROBIC) field campaign held in July–August 1997. In situ measurements of OH radicals were made by laser-induced fluorescence (LIF) at low pressure, exciting in the (0, 0) band of the A–X system at 308 nm. HO₂ radicals were monitored by chemical titration to OH upon the addition of NO, with subsequent detection by LIF. The instrument was calibrated regularly during the field campaign, and demonstrated a sensitivity towards OH and HO₂ of 5.2×10⁵ and 2.4×10⁶ molecule cm⁻³, respectively, for a signal integration period of 2.5 min and a signal-to-noise ratio of 1. Diurnal cycles of OH and HO₂ were measured on 10 days within a small clearing of a forest of Greek Fir (Abies Borisi-Regis). In total 4165 OH data points and 1501 HO₂ data points were collected at 30 s intervals. Noon-time OH and HO₂ concentrations were between 4–12×10⁶ and 0.4–9×10⁸ molecule cm⁻³, respectively. The performance of the instrument is evaluated, and the data are interpreted in terms of correlations with controlling variables. A significant correlation (r²=0.66) is observed between the OH concentration and the rate of photolysis of ozone, J(O¹D). However, OH persisted into the early evening when J(O¹D) had fallen to very low values, consistent with the modelling study presented in the following paper (Carslaw et al., 2001, OH and HO₂ radical chemistry in a forest region of north-western Greece. Atmospheric Environment 35, 4725–4737) that predicts a significant radical source from the ozonolysis of biogenic alkenes. Normalisation of the OH concentrations for variations in J(O¹D) revealed a bell-shaped dependence of OH upon NO_x (NO+NO₂), which peaked at [NO_x] ∼1.75 ppbv. The diurnal variation of HO₂ was found to be less correlated with J(O¹D) compared to OH.     

Night-time radical chemistry during the TORCH campaign

We present one of the most comprehensive studies of night-time radical chemistry to date, from the Tropospheric ORganic CHemistry experiment (TORCH) in the summer of 2003. TORCH provided a wealth of measurements with which to study the oxidizing capacity of the atmosphere. The measurements provided input to a zero-dimensional box model which has been used to study night-time radical chemistry during the campaign. Average night-time predicted concentrations of OH (2.6 × 10⁵ molecule cm^?3), HO₂ (2.9 × 10⁷ molecule cm^?3) and [HO₂+ΣRO₂] radicals (2.2 × 10⁸ molecule cm^?3) were an order of magnitude smaller than those predicted during the daytime. The model under-predicted the night-time measurements of OH, HO₂ and [HO₂+ΣRO₂] radicals, on average by 41%, 16% and 8% respectively. Whilst the model captured the broad features of night-time radical behaviour, some of the specific features that were observed are hard to explain. A rate of radical production assessment was carried out for the whole campaign between the hours of 00:00 and 04:00. Whilst radical production was limited owing to the absence of photolytic reactions, production routes via the reactions of alkenes with O₃ provided an effective night-time radical source. Nitrate radical concentrations were predicted to be 0.6 ppt on average with a peak of 18 ppt on August 9th during a polluted heat wave period. Overall, the nitrate radical contributes about a third of the total initiation via RO₂, mostly through reaction with alkenes.     

Simulation of long-range transport of acidic pollutants in East Asia during the Yellow Sand event

The atmospheric chemical process was simulated using the Carbon Bond 4 (CB-4) model, the aqueous-phase chemistry in Regional Acid Deposition Model and the thermodynamic equilibrium relation of aerosols with the emission inventories of the Emission Database for Global Atmospheric Research, the database of China and South Korea and the Mesoscale Model version 2 (MM5) meteorological fields to examine the spatial distributions of the acidic pollutant concentrations in East Asia for the case of the long-lasting Yellow Sand event in April 1998. The present models simulate quite well the observed general trend and the diurnal variation of concentrations of gaseous pollutants, especially for O₃ concentration. However, the model underestimates SO₂ and NO_x concentration but overestimates O₃ concentration largely due to uncertainty in NO_x and VOC emissions. It is found that the simulated gaseous pollutants such as SO₂, NO_x, and NH₃ are not transported far away from the source regions but show significant diurnal variations of their concentrations. However, the daily variations of the concentrations are not significant due to invariant emission rates. On the other hand, concentrations of the transformed pollutants including SO₄²⁻, NH₄⁺, and NO₃⁻ are found to have significant daily variations but little diurnal variations. The model-estimated deposition indicates that dry deposition is largely contributed by gaseous pollutants while wet deposition of pollutants is mainly contributed by the transformed pollutants.     

Nighttime variations in HO2 radical mixing ratios at Rishiri Island observed with elevated monoterpene mixing ratios

HO₂ radical concentrations were measured by a laser-induced fluorescence instrument for three nighttime periods during the intensive field campaign at Rishiri Island, Japan, in June 2000. The HO₂ mixing ratio had temporal variations around its average of 4.2±1.2 (1σ) pptv and showed a positive correlation with the summed mixing ratio of four monoterpene species, α-pinene, β-pinene, camphene, and limonene, that sometimes reached 1 ppbv. Our model calculations suggested that ozonolysis reactions of monoterpenes were the main source of nighttime radicals and they explained 58% of measured HO₂ concentration levels. The model roughly reproduced the dependence of the HO₂ mixing ratio on the square root of the radical production rate due to the ozonolysis reactions of the monoterpenes. However, the absolute HO₂ mixing ratio was significantly underpredicted by the model. We discuss possible reasons in terms of misunderstood RO₂ chemistry, RO₂ interference with HO₂ observations, unknown radical production process associated by high NO₂ mixing ratio, and the contribution of unmeasured olefinic species to radical production via their reactions with ozone.