Open Access Article
Kalliopi Florou
a,
Spiro Jorga†
b,
Agata Blaziak
c,
Christina N. Vasilakopoulou
a,
Petro Uruci
ad,
Rafal Szmigielski
c and
Spyros N. Pandis
*ad
aInstitute of Chemical Engineering Sciences, ICE-HT, 26504, Patras, Greece
bDepartment of Chemical Engineering, Carnegie Mellon University, Pittsburgh, PA 15213, USA
cInstitute of Physical Chemistry, Polish Academy of Sciences, 01-224 Warsaw, Poland
dDepartment of Chemical Engineering, University of Patras, 26504 Patras, Greece. E-mail: spyros@chemeng.upatras.gr
First published on 8th November 2025
Diaterpenylic acid acetate (DTAA) (C10H16O6) is a later-generation biogenic secondary organic aerosol (OA) component, formed during the oxidation of first-generation products of monoterpenes such as α-pinene, and β-pinene. Identified in aerosol in terrestrial and forested environments, DTAA is a product of the oxidation of both terpenylic acid and 1,8-cineole. Here, we present the first comprehensive chamber study investigating DTAA's volatility, gas–particle partitioning, and oxidative transformation under atmospherically relevant conditions through a combination of laboratory measurements, modeling, and chemical analysis. Its physicochemical properties were characterized by using two atmospheric simulation chambers, equipped with a range of particle and gas-phase instrumentation. A high-resolution time-of-flight aerosol mass spectrometer (HR-ToF-AMS) identified DTAA aerosol characteristic peaks at mass-to-charge (m/z) 59, 67, 79, 91, 95, 101, 114 and 139. DTAA aerosol density was estimated to be 1.3 ± 0.2 g cm−3. DTAA was classified as a semi-volatile organic compound (SVOC), with a saturation concentration of 3.6–3.9 µg m−3. Upon hydroxyl (OH) radical exposure, DTAA underwent significant chemical aging, producing secondary organic aerosol (SOA) with distinct spectral features and a little higher oxygen-to-carbon ratio (O
:
C = 0.63). The AMS spectrum of the produced SOA was quite different from that of pure DTAA (R2 = 0.48 or θ = 31°) and resembled to an extent (θ = 14–20°), the spectra of ambient biogenic SOA. A suite of oxidation products were identified via proton transfer reaction mass spectrometry (PTR-MS) and chemical ionization mass spectrometry (CIMS) ranging from small molecules (e.g. acetone) to multifunctional species. A kinetic model incorporating partitioning, wall loss, and oxidation accurately captured SOA production during the DTAA reaction with OH, assuming an effective fragmentation probability of 32%. These results highlight the atmospheric relevance of DTAA as a reactive SVOC and underline the importance of integrating later generation chemical processes in SOA studies.
Environmental significanceThis study investigates the oxidation of DTAA by OH radicals. DTAA can be viewed as a model later-generation product of monoterpene ozonolysis, a major source of secondary organic aerosol on both regional and global scales. This paper shows that DTAA is semivolatile and continues reacting, producing even later-generation products. Even at this late reaction stage, functionalization is the major reaction pathway, average SOA O : C increases and SOA mass increases or decreases depending on temperature. The results show how dynamic the SOA production system is and how important the later-generation processes are for its chemical and physical characteristics.
|
Isoprene, monoterpenes, and sesquiterpenes account for roughly 75% of total global bVOC emissions,6,7 while in certain summer periods their contribution can increase to over 90%.8 Monoterpenes (C10H16) are significant bVOCs (11–15%),7,9,10 particularly in forested regions. Although monoterpenes are emitted in lower quantities compared to isoprene, their potential to form SOA is considerably higher, accounting in certain cases for nearly half of the total fine OA in the atmosphere.11
α-Pinene and β-pinene are the most abundant monoterpenes, with global emissions ranging between 30 and 70 TgC annually.7 Oxidation reactions of α-pinene and β-pinene generate a range of secondary products, with diaterpenylic acid acetate (DTAA) being one of them (Fig. 1). The oxidation process of α-pinene comprises several steps, beginning with the formation of peroxy radicals, followed by reactions that yield terpenylic acid and diaterpenylic acid. Terpenylic acid is mainly formed from the α- and β-pinene ozonolysis and from the photo-oxidation of nopinone during the aging of β-pinene first-generation products.12–14 Mutzel et al. (2016)14 suggested that the oxidation of myrtenal, an α-pinene SOA product, also leads to the formation of terpenylic acid. Yasmeen et al. (2010)15 suggested that terpenylic acid can then undergo acid-catalyzed hydrolysis, resulting in the formation of diaterpenylic acid, a hydroxy-carboxylic acid. Diaterpenylic acid can subsequently undergo acetylation to produce DTAA (C10H16O6; m/z 232). DTAA can also be produced through the oxidation of 1,8-cineole (eucalyptol), a naturally occurring cyclic ether derived from botanical sources such as eucalyptus, rosemary, and camphor laurel. According to Iinuma et al. (2009),16 this formation occurs under both low and high NOx conditions (Fig. 1).
![]() | ||
| Fig. 1 Simplified schematic representation of the reaction pathways leading to the formation of DTAA. | ||
Several studies have measured the levels of DTAA in various ambient environments, providing insights into its spatial and temporal distribution. DTAA has been detected in aerosol samples from forested areas with significant monoterpene emissions. Gómez-González et al. (2012)17 reported ambient concentrations of DTAA ranging from 0.10 to 0.64 ng m−3 during the summer of 2007 at a forest site in Brasschaat, Belgium. Similarly, measurements in the spring of 2008 at a coniferous forest near Silkeborg, Denmark, recorded an average DTAA concentration of 0.4 ng m−3, with peak values reaching 1.4 ng m−3.18 At a ponderosa pine plantation in the Sierra Nevada Mountains, California, DTAA concentrations were 5 ng m−3 during measurements conducted at the cold period of 2007, increasing to 6.5 ng m−3 during a warmer period in 2009.19 At a rural background station in Vavihill, Sweden, characterized by a mix of pastures, forests, and agricultural land, Martinsson et al. (2017)20 observed a mean DTAA concentration of 0.84 ng m−3. Amarandei et al. (2023)21 recorded average DTAA values ranging from 0.6 ng m−3 during the colder months to 1.7 ng m−3 in the warmer months in an urban site in Iasi, Romania. At a marine site surrounded by grasslands (Cape Grim, Australia), Cui et al.22 (2019) measured a mean DTAA concentration of 0.11 ng m−3, with peak values of up to 0.36 ng m−3. Over a 24-year period, DTAA has been found to be the most abundant monoterpene-derived SOA component in Cape Grim, followed by terpenylic acid, terebic acid, MBTCA, and pinic acid.22 Research conducted at Zeppelin Mountain (Svalbard) and Station Nord (Greenland) showed that DTAA was present in considerable amounts, particularly during periods of Arctic haze.23 Hansen et al.23 (2014) reported DTAA concentrations of 0.03–0.16 ng m−3 at Zeppelin Mountain and 0.01–0.05 ng m−3 at Station Nord during these events. These findings contribute valuable data on the role of DTAA in SOA formation across diverse environments.
Even though DTAA has been detected in various field campaigns, there are limited studies about its physicochemical properties.24 DTAA is expected to react with hydroxyl (OH) radicals, though its subsequent reaction pathways remain unclear. These reactions may yield more oxidized products or result in fragmentation into smaller, volatile products. A deeper understanding of these oxidation processes for DTAA and other similar SOA compounds is essential for enhancing atmospheric chemical transport models and better constraining the contribution of biogenic SOA to total OA.
In this study, we employed two distinct atmospheric simulation chambers in conjunction with advanced online instrumentation to characterize the physicochemical properties of aerosol composed of pure DTAA. Using high-resolution mass spectrometry, we characterized the aerosol's OA spectrum and determined key physicochemical parameters, including density, saturation vapor concentration, and enthalpy of vaporization. Furthermore, we investigated the chemical aging processes of DTAA by examining its reaction with hydroxyl radicals, under low- and high-NOx conditions, followed by a detailed particle and gas phase analysis of the resulting oxidation products.
Aerosol samples were generated by atomizing an aqueous solution of DTAA. For selected experiments, ammonium sulfate was added to the solution to create mixed DTAA-ammonium sulfate particles. These aerosols were introduced into two atmospheric simulation chambers: the Foundation of Research and Technology-Hellas Atmospheric Simulation Chamber (FORTH-ASC) in Patras, Greece, and the Carnegie Mellon University Atmospheric Simulation Chamber (CMU-ASC) in Pittsburgh, USA. Initial characterization of the aerosol was conducted under dark conditions. Subsequently, atmospherically relevant levels of OH radicals were generated and allowed to react with DTAA.
Both chambers utilized a 10 m3 Teflon reactor for the experiments. In the FORTH-ASC, the chamber walls were equipped with ultraviolet (UV) lamps (Osram, L 36W/73), achieving a JNO2 of 0.59 min−1 when fully illuminated. The CMU-ASC featured similar UV lamps, resulting in a JNO2 of 0.2 min−1. Using two different chambers enhanced the robustness of the results, ensuring that potential wall-related artifacts were accounted for. Relative humidity (RH) in the chambers was maintained between 10% and 30%.
A constant output TSI atomizer (model 3076) was employed to produce aerosols from the prepared aqueous solutions. Experiments were conducted either in the absence of an aerosol seed or using ammonium sulfate seeds. In cases where the aerosol contained both DTAA and ammonium sulfate, the aerosol was generated from a single solution and introduced into the chamber. Prior to entering the chamber, the aerosol droplets were dried using a diffusion dryer.
Oxidation experiments were performed under low- and high-NOx conditions. Under low-NOx conditions, hydrogen peroxide (H2O2) photolysis served as the source of OH radicals, whereas in high-NOx experiments, OH was generated through the photolysis of nitrous acid (HONO). Aqueous HONO was prepared by mixing fresh sulfuric acid (H2SO4) (4.9 g L−1) with sodium nitrite (NaNO2) (6.9 g L−1) in a glass bulb, and HONO was introduced into the chamber using dry zero air and a bubbler. In specific experiments, isotopically labelled butanol d-9 (98%, Cambridge Isotope Laboratories, Inc.) was used to quantify OH levels. The chambers were thoroughly cleaned by flushing with clean air overnight prior to each experiment.
Initial concentrations of DTAA aerosol are shown in Table 1. DTAA was examined using two systems: (i) ammonium sulfate seed particles mixed with DTAA, forming internally mixed particles, and (ii) pure DTAA (e.g. Exp. 7). This dual approach was chosen to both assess the impact of impurities and also to isolate the behavior and oxidation chemistry of DTAA while minimizing interference from other organic components. In the atmosphere, DTAA coexists with a complex mixture of organic species formed during monoterpene oxidation. Nevertheless, the simplified framework employed here provides essential insight into DTAA-specific processes and mechanisms, representing a necessary step toward understanding its behavior and role within more compositionally complex atmospheric environments. In our experiments, the equivalent ambient exposure of DTAA to OH varied from 0.6 to 0.9 days.
| Exp. | Experimental conditions | Initial conditions | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Type | Chamber | RH [%] | T [°C] | OA [µg m−3] | Sulfate [µg m−3] | Total PM1 [µg m−3] | O : C |
H : C |
OA density [g cm−3] | |
| 1 | Reference | FORTH | 22 | 27 | 56 | 12 | 71 | 0.54 | 1.57 | 1.30 |
| 2 | Reference | FORTH | 18 | 25 | 29 | 7 | 39 | 0.57 | 1.64 | 1.29 |
| 3 | HONO/UV | FORTH | 10 | 24 | 34 | 9 | 47 | 0.55 | 1.64 | 1.28 |
| 4 | HONO/UV | FORTH | 14 | 25 | 25 | 37 | 78 | 0.57 | 1.63 | 1.30 |
| 5 | HONO/UV | FORTH | 31 | 19 | 59 | 14 | 79 | 0.53 | 1.58 | 1.29 |
| 6 | H2O2/UV | FORTH | 38 | 25 | 50 | 20 | 77 | 0.55 | 1.64 | 1.28 |
| 7 | HONO/UV | FORTH | 9 | 24 | 81 | 0 | 81 | 0.53 | 1.62 | 1.28 |
| 8 | HONO/UV | CMU | 10 | 21 | 24 | 10 | 37 | 0.55 | 1.53 | 1.32 |
| 9 | HONO/UV | CMU | 10 | 22 | 54 | 27 | 88 | 0.53 | 1.50 | 1.32 |
| 10 | HONO/UV | CMU | 14 | 20 | 41 | 33 | 85 | 0.56 | 1.51 | 1.34 |
| Average values ± SD | 17.6 ± 10.0 | 23.1 ± 2.6 | 0.55 ± 0.02 | 1.59 ± 0.06 | 1.30 ± 0.02 | |||||
Time-of-Flight Aerosol Mass Spectrometer (HR-ToF-AMS, Aerodyne Research Inc., Billerica, USA) was utilized in both experimental setups, sampling at a flow rate of approximately 0.1 L min−1. This instrument provided continuous, real-time data on the size and chemical composition of non-refractory PM1 aerosol particles (those with diameters less than 1 µm). Data from the HR-ToF-AMS were processed using standard AMS software toolkits: SeQUential Igor data RetRiEvaL (SQUIRREL) v1.57I and Peak Integration by Key Analysis (PIKA) v1.16I, within Igor Pro 6.37 (Wave Metrics). Elemental ratios, including the oxygen-to-carbon (O
:
C) ratio, were calculated using the enhanced method described by Canagaratna et al. (2015).25
The aerosol number distribution was measured using a TSI scanning mobility particle sizer (SMPS; classifier model 3080, DMA model 3081, CPC model 3787) over the size range of 14–710 nm every 3 min. The SMPS operated with a sheath flow rate of 3 L min−1 and an aerosol sample flow rate of 0.6 L min−1. To characterize OA volatility, a thermodenuder26 was employed. The thermodenuder was integrated with the SMPS and AMS to determine the aerosol mass fraction remaining (MFR) across temperatures ranging from 25 °C to 150 °C. Aerosol alternated between passing through the thermodenuder and a bypass line every 3 min, with both streams subsequently analyzed by the HR-AMS and SMPS. The aerosol had a centerline residence time of 15 s within the thermodenuder.
The dynamic mass transfer model developed by Riipinen et al. (2010)27 was employed to estimate the volatility of OA. This model simulates the evaporation of particles within both the heating and cooling sections of the thermodenuder. Evaporation also occurs in the cooling section as organic vapors are removed by adsorption onto the activated carbon walls. The model estimates the mass fraction remaining (MFR), the OA saturation concentration (C*) at 298 K and its effective vaporization enthalpy (ΔHvap). For these simulations, the effective mass accommodation coefficient was assumed to be unity. The best estimates for C* and ΔHvap were derived from the top 1% of parameter combinations, which showed the lowest errors when comparing the measured MFR to model predictions.
Gas-phase compounds were monitored using a Proton Transfer Reaction Mass Spectrometer (PTR-MS 500, Ionicon Analytik), with H3O+ as the reagent ion. The PTR-MS operated at 600 V with a constant pressure of 2.2–2.3 mbar and a sampling flow rate of 0.5 L min−1. Calibration was conducted according to the procedure outlined by Kaltsonoudis et al. (2016)28 using VOC standards from Ionicon. The OH radical levels were determined based on the decay of butanol-d9, monitored at m/z 66 using the PTR-MS, and employing a reaction rate constant with OH of 3.4 × 10−12 cm3 per molecule per s.29
DTAA reaction products were analyzed in the CMU-ASC using a time-of-flight chemical ionization mass spectrometer (ToF-CIMS, Aerodyne Research Inc.) with two reagent ions: iodide (I−) and nitrate (NO3−), depending on the experimental setup. The NO3− reagent ion has been widely employed for studying the composition of highly oxidized organics in laboratory and ambient air studies.30–32 It has been particularly effective for probing nitrogen-containing oxidized monoterpenes, as demonstrated by Draper et al. (2019).33 NO3− clusters selectively with highly oxidized compounds containing at least two hydrogen bond donor sites, making it invaluable for identifying the formation of such products in oxidation experiments. In contrast, iodide (I−) has been extensively used to detect oxidized organic compounds and inorganic nitrogen species.34–37 The dual use of I− and NO3− reagent ions offers complementary insights, enhancing the mechanistic understanding of oxidation processes by capturing a broader range of oxidized products.
To determine the AMS collection efficiency (CE) and the OA density, we utilized the algorithm developed by Kostenidou et al. (2007),38 which involves comparing the volume distributions obtained from the SMPS with the mass distributions obtained from the AMS. For addressing particle wall losses in both chambers, we applied a size-dependent particle wall loss rate constant, using ammonium sulfate seeds, as recommended by Wang et al. (2018).39 Ammonium sulfate particles were generated using the constant output TSI atomizer, dried, and then introduced into the chamber either before or after each experiment. The wall-loss rate constant, kc, was consistent across all experiments, with a value of kc = 0.08 ± 0.05 h−1 in both the FORTH-ASC and CMU-ASC chambers.
To assess the variability in the OA and SOA mass spectra measured by the AMS across different experiments, we employed the theta angle (θ). The theta angle method treats the AMS OA spectra as n-dimensional vectors, where n represents the number of mass-to-charge ratios (m/z), and calculates the angle between these vectors in the n-dimensional space.40 A theta angle of less than 10° denotes a high degree of similarity between the spectra, whereas angles exceeding 25° indicate significant differences between the examined spectra.
In most experiments, ammonium sulfate seeds were introduced with DTAA in the same solution, and during the characterization period, sulfate levels were observed to be up to 34 µg m−3. In Exp. 7, only DTAA was injected into the chamber. Relative humidity (RH) remained low in all experiments, varying from 9% to 38%, while the average temperature was maintained at 23 ± 3 °C (Table 1).
The HR spectrum of DTAA was characterized by oxygenated fragment ions (58%), with contribution from the CxHyO+ family at 39.7% and the CxHyOz+ family at 18.5% (Fig. 2). Significant CxHyO+ ions were detected at m/z 43 (C2H3O+), 59 (C3H7O+), 71 (C4H7O+), 85 (C5H9O+), 95 (C6H7O+), 108 (C7H8O+), 109 (C7H9O+), and 157 (C11H9O+). Major CxHyOz+ ions included those at m/z 45 (CH4O2+), 60 (C2H4O2+), 86 (C4H6O2+), 101 (C5H9O2+), 114 (C5H6O3+), 126 (C7H10O2+), 127 (C7H11O2+), 139 (C7H7O3+), and 154 (C8H10O3+). The CxHy family contributed 38.4% to the total OA signal, and the main m/z peaks included 53 (C4H5+), 65 (C5H5+), 67 (C5H7+), 68 (C5H8+), 77 (C6H5+), 79 (C6H7+), 81 (C6H9+), and 91 (C7H7+). The average unit resolution OA mass spectra from all experiments, along with the standard deviation, are shown in Fig. S2. The HR spectrum of DTAA exhibits a distinct profile, largely due to the significant number of detected m/z values, particularly those above m/z 100.
The O
:
C ratio for DTAA (C10H16O6) is 0.6, and its H
:
C ratio is 1.6. Following the method of Canagaratna et al. (2015),25 the AMS O
:
C and H
:
C ratios were estimated to be 0.55 ± 0.02 and 1.59 ± 0.06, which are consistent with the expected values. The Van Krevelen diagram of the OA for all experiments is shown in Fig. S3.
Applying the algorithm of Kostenidou et al.38 (2007), the AMS collection efficiency (CE) was estimated to be 0.8 ± 0.1 and the pure DTAA density was 1.35 ± 0.15 g cm−3. This value is close to the density of 1.30 ± 0.02 g cm−3 that is predicted by the Kuwata et al. (2012)41 parameterization based on the actual O
:
C and H
:
C values for DTAA.
The SMPS mass concentration also demonstrated a consistent decrease, mirroring the trend observed in the AMS data. The data of characterization Exp. 2 were consistent with those of Exp. 1 (Fig. S4). During the characterization period, the AMS OA spectrum showed minimal changes (θ < 3°), and the O
:
C ratio of DTAA remained practically constant (less than 2% change), which is consistent with the minimal variation observed in the high-resolution OA spectrum.
At t = 0 h, the OA-to-sulfate ratio was 4.8, but this value progressively declined, reaching 4.3 after 6 h. Given that sulfate is non-volatile at room temperature, this decrease indicates that DTAA gradually evaporated, with its vapor slowly depositing onto the chamber walls (Fig. 3b).
The observed reduction in OA concentration over time, coupled with the declining OA-to-sulfate ratio, provides evidence that DTAA, once introduced into the chamber, undergoes partial evaporation to establish equilibrium with the gas phase. The vapor wall loss rate will be estimated in a subsequent section.
Kostenidou et al. (2022)43 proposed a different method for calculating the saturation concentration at room temperature. This approach is based on the assumption that the difference between the initial OA concentration and its equilibrium concentration reflects the quantity that has evaporated into the gas phase, which corresponds to the saturation concentration. The proposed equation accounts for several factors, including the OA-to-sulfate ratio, the mass concentrations of OA and sulfate before evaporation, the final OA concentration, as well as adjustments for wall losses and deposition. Employing this methodology, the saturation concentration of DTAA was determined across all experiments during the characterization phase (defined as the 60 min prior to UV light activation in Experiments 3–10) to be 3.9 ± 3.6 µg m−3. While this estimate carries greater uncertainty compared to values obtained from the thermodenuder analysis, both methods provide consistent results within the bounds of their experimental uncertainties. The value of this study is consistent considering the experimental uncertainties with the 1.7 µg m−3 measured by Babar et al. (2020).44 As a result, DTAA can be classified as a semi-volatile organic compound (SVOC) based on these findings.
Assuming a linear loss process, the DTAA vapor wall loss rate constant kwl,DTAA can be estimated by:
![]() | (1) |
Using this expression for the typical characterization experiment, we estimated a vapor wall loss rate of approximately 0.11 h−1, with values ranging from 0.07 to 0.2 h−1, depending on the C* value. These values suggest slow but non-negligible removal of DTAA vapors to the chamber walls and will be used in our model in a subsequent section.
The O
:
C ratio for all oxidation experiments is displayed in Fig. 5. At time zero, the average O
:
C ratio for both the FORTH-ASC and CMU-ASC experiments was 0.55 ± 0.02 (Table 1). Following illumination, the O
:
C ratio remained relatively stable across all experiments, except for Experiment 5, where it decreased by 0.07 units to 0.48 after 6 h. The primary distinction of Exp. 5 is that it occurred predominantly at a significantly higher temperature than the other experiments (Fig. S6). Analysis of the AMS OA spectra revealed a change in the theta angle for the total OA spectrum of up to 8 degrees (Fig. 5b). The pre- and post-oxidation OA spectra exhibited noticeable differences across several m/z values, supporting the observed variation in the theta angle (Fig. S5).
![]() | ||
Fig. 5 The (a) O : C ratio for the aging experiments and (b) theta (θ) angles of the HR OA spectra for Experiments 3–10. | ||
The DTAA reaction with OH resulted in changes in the OA mass concentration in all oxidation experiments. The normalized change in OA concentration relative to the initial OA is illustrated in Fig. 6a. An enhancement of approximately 10% was observed in certain experiments (e.g., Exp. 3 and 4), while others exhibited a moderate (5–16%) decrease (e.g., Exp. 6, 7, and 8). In Experiments 5 and 10, there was a substantial reduction (35–60%) in OA. In Experiments 5 and 10, the observed OA reduction occurred at a much faster rate than the estimated DTAA vapor wall loss rate of 0.4 µg m−3 h−1. For instance, in Experiment 5, the particle wall-loss-corrected OA concentration decreased by 21 µg m−3 over 6 hours, while vapor wall losses accounted for only 2.5 µg m−3 (12%) of this reduction. This pronounced decrease was primarily driven by enhanced evaporation caused by a 15 °C temperature increase in the chamber and the consequent acceleration of gas-phase oxidation processes. The relative contributions of these two effects can be estimated based on the experimental data. If evaporation alone were occurring, the OA loss would correspond to the change in saturation concentration over the 15 °C temperature range, amounting to approximately 5.3 µg m−3. This value was derived from the reported saturation concentration at 298 K and the effective enthalpy of evaporation. Accounting for the estimated vapor wall loss (2.5 µg m−3) and comparing with the total observed decrease in particulate-phase DTAA concentration (21 µg m−3) indicates that most of the reduction was due to the gas-phase reactions.
![]() | ||
| Fig. 6 Normalized change of (a) total OA and (b) pure DTAA (after applying PMF analysis) for the oxidation experiments once compared to initial conditions (time = 0). | ||
Ammonium and sulfate mass concentrations remained stable in all experiments after applying the particle wall loss corrections, indicating that the corrections to AMS measurements, based on the corresponding wall loss characterization experiments, were reliable (Table 2).
| Exp. | Experimental parameters at t = 3 h | |||||
|---|---|---|---|---|---|---|
| OA [µg m−3] | Sulfate [µg m−3] | Total PM1 [µg m−3] | O : C |
H : C |
OA density [g cm−3] | |
| 1 | 55 | 12 | 70 | 0.54 | 1.57 | 1.30 |
| 2 | 26 | 7 | 35 | 0.57 | 1.64 | 1.30 |
| 3 | 37 | 9 | 49 | 0.56 | 1.64 | 1.29 |
| 4 | 28 | 37 | 80 | 0.57 | 1.62 | 1.30 |
| 5 | 50 | 14 | 69 | 0.49 | 1.61 | 1.26 |
| 6 | 49 | 20 | 76 | 0.56 | 1.64 | 1.29 |
| 7 | 79 | 0 | 79 | 0.54 | 1.64 | 1.28 |
| 8 | 23 | 10 | 37 | 0.53 | 1.53 | 1.31 |
| 9 | 49 | 27 | 85 | 0.53 | 1.50 | 1.32 |
| 10 | 18 | 32 | 62 | 0.58 | 1.41 | 1.38 |
| Average values ± SD | 0.55 ± 0.03 | 1.58 ± 0.08 | 1.30 ± 0.03 | |||
A slight temperature increase of 2 °C, coinciding with the activation of UV lights, was observed in all oxidation experiments, with the exception of Experiment 5. In that case, a more pronounced temperature increase of 15 °C was recorded during the experiment because the chamber cooling system was deactivated (Fig. S6). This significant temperature increase may help explain the faster reduction in OA observed in Experiments 5 and 10, compared to the other experiments.
The first factor corresponded to the HR spectrum of fresh DTAA (Fig. 2), measured in the characterization phase, with an AMS O
:
C ratio of 0.55. As chemical aging commenced, the mass concentration of the fresh DTAA factor decreased (Fig. 7), albeit at different rates in each experiment (Fig. 6b). The second factor was attributed to aged DTAA aerosol, hereafter referred to as SOA. SOA had practically zero mass concentration when the UV lights were off and increased once the aerosol was exposed to OH radicals and UV irradiation (Fig. 7). The SOA had an O
:
C ratio of 0.63 (Fig. 8), that is 0.08 units (15%) higher than the fresh DTAA. The SOA AMS spectrum differed significantly from the fresh DTAA spectrum, particularly at m/z 28, 29, 43, 44, 45, 55, 60, 61, 65, 67, 68, 79, 86, 101, 114, 139 and 157 (Fig. S7). Contributions from the CxHyO+ and CxHyOz+ families to the SOA spectrum were 41.1% and 16.8%, respectively. The theta angle between the fresh DTAA and SOA factors was 31 degrees, indicating a substantial chemical transformation during aging.
![]() | ||
| Fig. 7 Time series for total measured OA (dark green line), sulfate (red line), ammonium (orange line) and PMF OA factors for pure DTAA (light green line) and SOA (black line) for Experiments 3–10. | ||
![]() | ||
| Fig. 8 HR mass spectrum of the SOA factor. The most important characteristic m/z ratios were 44, 45, 48, 53, 55, 64, 67, 69, 77, 79, 80, 81, 82, 85, 91, 95, 100, and 111. | ||
The pure DTAA and PMF SOA HR spectra were compared with other biogenic-related and ambient factors reported in the literature (Table 3). The pure DTAA spectrum demonstrated a small similarity (θ = 22°) to SOA formed from β-caryophyllene aging under high NOx conditions.48 Other compared spectra exhibited theta angles ranging from 23° to 46°, while the ambient biogenic factors had theta angles exceeding 32°. In contrast, the SOA factor showed a closer resemblance (theta angle of 14°) to SOA spectra resulting from α-pinene oxidation under high NOx conditions, and around 20° when compared to the biogenic OA factors from two different locations in Greece (Pertouli and Patras).49,50 This suggests a degree of similarity, though also noticeable differences between this SOA factor and the ambient field factors examined.
| Factor from literature vs. DTAA | θ (°) | Factor from literature vs. SOA | θ (°) |
|---|---|---|---|
| SOA: β-caryophyllene + OH (high NOx)48 | 22.2 | SOA: α-pinene + OH (unpublished data) | 14.2 |
| SOA: limonene + OH (unpublished data) | 23.1 | Biogenic OA (Patras)49 | 18.6 |
| α-Humelene initial (30–60 min)51 | 23.7 | Biogenic OA (Pertouli)50 | 20.8 |
| SOA: α-pinene + OH (unpublished data) | 25.2 | Terebic acid52 | 20.8 |
| SOA: β-caryophyllene + O3 (ref. 48) | 26.5 | SOA: β-caryophyllene + O3 (ref. 48) | 23.1 |
| α-Humelene final (4–5 h)51 | 26.9 | SOA: limonene + OH (unpublished data) | 23.9 |
| Terebic acid52 | 29.1 | LO-OOA (Pertouli)50 | 24.1 |
| SOA: β-caryophyllene + OH (low NOx)48 | 30.5 | SOA: β-caryophyllene + OH (high NOx)48 | 25.1 |
| Biogenic OA (Patras)49 | 32.5 | α-Humelene initial (30–60 min)51 | 27.0 |
| Biogenic OA (Pertouli)50 | 33.7 | MBTCA53 | 27.6 |
| LO-OOA (Pertouli)50 | 39.0 | MO-OOA (Pertouli)50 | 27.9 |
| Isoprene-OA (Centreville, Alabama)54 | 39.8 | Isoprene-OA (Centreville, Alabama)54 | 28.0 |
| MBTCA53 | 42.4 | α-Humelene final (4–5 h)51 | 29.5 |
| MO-OOA (Pertouli)50 | 43.0 | Norpinic Acid43 | 34.1 |
| Norpinic acid43 | 46.0 | SOA: β-caryophyllene + OH (low NOx)48 | 35.7 |
The PTR-MS detected increases in several VOCs across all FORTH-ASC experiments, including m/z 57 (butenes), 59 (acetone), 73 (methyl ethyl ketone), 81 (monoterpene fragment), 92 (unidentified), 93 (nominally toluene but also a monoterpene fragment), 95 (nominally phenol but also a monoterpene fragment), 103 (unidentified), 113 (biogenic oxidation product) and 115 (2-heptanone). The most significant increases were observed for m/z 57 (81 ± 31%), 81 (77 ± 37%) and 93 (77 ± 48%), which are commonly identified as monoterpene fragments when H3O+ is used as the reagent ion.55,56 The signal at m/z 92 (increase of 45 ± 21%), previously linked to monoterpene oxidation products in similar studies using H3O+, also showed a consistent increase.56 No increase of m/z 137 (monoterpenes) was detected. Quantitatively, m/z 59 (acetone) exhibited the highest enhancement, as high as 40 ppb, for the case of Experiment 5 (Fig. S9). To ensure this increase was due to the DTAA reactions rather than contamination from chamber walls, three blank experiments were conducted. The chamber was flushed overnight with clean air to ensure thorough cleaning before HONO was injected. UV lights were then activated, and the chamber was monitored for 3 h. In these blank experiments, an average acetone increase of 7 ppb was measured, verifying that the pronounced increase in m/z 59 was mainly due to the oxidation of DTAA. The acetone production observed is consistent with previous studies on α-pinene oxidation by ozone, OH and nitrate radicals, further supporting its attribution to DTAA oxidation processes.57
In order to examine the VOC oxidation products under relevant atmospheric conditions, the Generator for Explicit Chemistry and Kinetics of Organics in the Atmosphere (GECKO-A) (https://geckoa.lisa.u-pec.fr/) chemical mechanism was used to simulate the gaseous oxidation of DTAA.58,59 GECKO-A automatically assigns reactions and rate constants and produces detailed and explicit chemical mechanisms. The generated mechanism included 12 stable oxidation products (Fig. S10). The ToF-CIMS detected three of these 12 oxidation products (m/z 205.8, C3H4O3 and C4H10O9). The PTR-MS did not detect most of these products, mainly because the corresponding m/z ratios were not assigned. This discrepancy between the model-predicted and experimentally identified products could be partially due to limitations of the measurement techniques under the specific experimental conditions. Some predicted products may have been present at concentrations below the detection limits of CIMS and PTR-MS. In addition, highly functionalized species are more likely to be lost to chamber walls or sampling lines, further reducing their detectability. Finally, model predictions include possible products across a broad range of timescales and pathways, and some species may form too slowly to appear within the timeframe of our chamber experiments. As a result, the number of experimentally identified products likely underestimates the true overlap with model predictions.
According to GECKO-A, the reaction rate constant of DTAA with OH is 17 × 10−12 cm3 per molecule per s.
The mechanism is described using the following set of equations:
![]() | (2) |
![]() | (3) |
![]() | (4) |
![]() | (5) |
The system of eqn (2)–(5) was solved using the following initial conditions:
| Cg,DTAA (t = 0) = C0DTAA | (6) |
| Cp,DTAA (t = 0) = OA | (7) |
| Cg,P (t = 0) = 0 | (8) |
| Cp,P (t = 0) = 0 | (9) |
Model results are compared to experimental data from three representative oxidation experiments—Experiment 6 (low-NOx, FORTH-ASC), Experiment 7 (high-NOx, no ammonium sulfate seeds, FORTH-ASC), and Experiment 9 (high-NOx, CMU-ASC) in Fig. 10. Despite the differences in NOx regimes, presence/absence of seeds and chamber setups, the simple model was able to capture the observed changes in pure DTAA and formed SOA in all cases. This consistency across diverse experimental conditions highlights the robustness and applicability of the proposed framework for describing DTAA behaviour under varying atmospheric scenarios. A fragmentation probability of 0.32 appears to describe its reaction with OH. This probability denotes the fraction of the mass that is converted to high volatility products and therefore does not partition any more to the particle phase.
The model used in this study was designed to capture the dominant partitioning and fragmentation behaviour of DTAA under a range of conditions, and therefore it oversimplifies the gas-phase chemistry and neglects certain processes such as heterogeneous reactions, chamber-specific wall-loss variability, and detailed volatility distributions of the various products. These simplifications likely contribute to the deviations observed between modelled and measured SOA. Particle-phase functionalization or oligomerization could enhance SOA mass beyond model predictions, whereas uncertainties in fragmentation probabilities and product volatilities may also play a role. Sensitivity analyses indicate that increasing the fraction of lower-volatility products or incorporating a modest particle-phase uptake term improves agreement between model results and measurements. These findings suggest that heterogeneous processes and product volatility assumptions are plausible contributors to the observed discrepancies. Although a complete mechanistic reconciliation is beyond the scope of this study, it is acknowledged that a more complex modelling framework is needed to fully reproduce all experimental outcomes.
DTAA at 298 K has a saturation concentration equal to 3.6 µg m−3 and an effective vaporization enthalpy of 61 ± 8 kJ mol−1. It is a semi-volatile organic compound, and its atmospheric lifetime due to the oxidation by OH in the gas phase is estimated to be of the order of 5 h. This makes it a rather poor choice as a tracer for monoterpene SOA and its use will only provide a lower limit of its contribution to total OA.
The oxidation of DTAA by OH led to later-generation SOA that had O
:
C 0.08 units (15%) higher than the parent compound. Its AMS spectrum, determined by applying PMF to the results of all experiments, was significantly different than that of DTAA and had some similarity to other biogenic SOA spectra, particularly those associated with α-pinene SOA produced under high-NOx conditions. Depending on the conditions, the oxidation of DTAA can lead to small increases or significant decreases in the SOA concentration. The sign of the change does depend on temperature, with decreases appearing at higher temperatures.
Analysis of the gas-phase products of the DTAA oxidation using PTR-MS and CIMS revealed the formation of both smaller and multifunctional oxidation products. These gas-phase products covered a wide chemical range, from smaller compounds such as acetone to larger, highly oxidized molecules. An effective fragmentation probability of 32% was estimated using a simple model of the system. The model successfully reproduced key features of our experiments, including the extent and timescale of SOA formation, offering a quantitative tool for understanding DTAA's role in oxidative aerosol production.
The loss rate constant of DTAA vapor to the walls of the FORTH chamber was estimated to be 0.11 h−1 on average, with values ranging from 0.07 to 0.2 h−1. The corresponding losses are non-negligible and should be taken into account in experiments that last several hours, especially if the DTAA concentrations in the particle phase are low.
Together, these results show that DTAA is a reactive SVOC that contributes to SOA formation, but also continues reacting, forming a variety of products, both smaller and larger. Its transformation under OH exposure resembles that of more extensively studied biogenic compounds, but its distinct spectrum adds to the chemical diversity of the ambient aerosol pool. The techniques used here can be used for other later-generation products of atmospheric VOC oxidation in an effort to improve our understanding of the later-generation processes taking place during atmospheric SOA formation.
Supplementary information (SI): (1) theta angles for all experiments during the characterization period, (2) the average DTAA spectrum from all experiments along with their standard deviation, (3) the Van Krevelen diagram of DTAA for the 10 experiments, (4) the volume distributions for every hour and the time series of AMS and SMPS for characterization experiment 2, (5) the comparison of before- and after-UV spectra for the oxidation experiments, (6) the temperature and RH time series for the FORTH-ASC, (7) the comparison of AMS mass spectra for DTAA and SOA, (8) the CIMS time-series for experiment 10, (9) the PTRMS-compounds that increased after injecting OH radicals and started UV irradiation for experiment 5, and (10) the products of the DTAA oxidation by OH predicted by GECKO-A. See DOI: https://doi.org/10.1039/d5ea00086f.
Footnote |
| † Present address: TOFWERK, 3645 Thun, Switzerland. |
| This journal is © The Royal Society of Chemistry 2025 |