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# Photolytic radical persistence due to anoxia in viscous aerosol particles

## Abstract

In viscous, organic-rich aerosol particles containing iron, sunlight may induce anoxic conditions that stabilize reactive oxygen species (ROS) and carbon-centered radicals (CCRs). In laboratory experiments, we show mass loss, iron oxidation and radical formation and release from photoactive organic particles containing iron. Our results reveal a range of temperature and relative humidity, including ambient conditions, that control ROS build up and CCR persistence in photochemically active, viscous organic particles. We find that radicals can attain high concentrations, altering aerosol chemistry and exacerbating health hazards of aerosol exposure. Our physicochemical kinetic model confirmed these results, implying that oxygen does not penetrate such particles due to the combined effects of fast reaction and slow diffusion near the particle surface, allowing photochemically-produced radicals to be effectively trapped in an anoxic organic matrix.

## Introduction

Aerosol particles suspended in the atmosphere can take up water and initiate the formation of liquid or ice clouds, impact Earth’s radiative balance1,2, and cause oxidative stress when inhaled affecting respiratory health3,4. Atmospheric aerosol components that generate radicals and reactive oxygen species (ROS) in lungs are linked to toxicity, inflammation, lung disease, and thus, loss of human life4,5,6. Species of ROS include the hydroxyl radical, OH, the hydroperoxyl radical, HO2, the superoxide radical anion, $${\mathrm{O}}_2^ -$$, and hydrogen peroxide, H2O2, among others. Of particular interest are carbon-centered radicals (CCRs), such as the methyl radical, CH3, or the triphenylmethyl radical, C(C6H5)3, with very different lifetimes. They are some of the many types of radicals that are present in aerosol particles produced from combustion sources, like biomass burning or cigarette smoke; photochemical reactions and aqueous aerosol chemistry; ozonolysis of certain biogenic or anthropogenic gaseous compounds; and biogenic aerosol sources, such as pollen proteins4,5,6,7,8. The lifetimes of ROS and CCRs are typically short due to their high reactivity. Yet, some CCRs can have a lifetime on the order of a day, termed environmentally persistent free radicals (EPFR), which are stabilized with the help of aromatic species or by forming organo-metal complexes in particles or on surfaces5,6,7.

In cold and dry air, aqueous aerosol particles that are dominated by organic solutes may attain a high viscosity9,10 and become solid-like, which slows molecular transport and thus radical chemistry11,12,13. Organic matter is abundant in atmospheric particles and frequently mixes with inorganic and trace metal compounds3,4,6,8,14,15. In atmospheric particles, iron can undergo rapid photochemical cycling leading to radical formation and driving chemical change7,8,16,17,18,19,20,21. Photochemical reactions in aerosol particles occur throughout their bulk and produce CCRs, but we hypothesize that subsequent processes, such as ROS production, evaporation, or gas phase O2 uptake and reaction with CCRs can be significantly stunted by molecular diffusion limitations. Iron(III)-citrate (FeIIICit) photochemistry is representative of iron-carboxylate photochemistry22, which is thought to be a dominant source of OH radicals in atmospheric aerosol particles and the dominant sink of carboxylic acids18,23. FeIIICit undergoes ligand to metal charge transfer (LMCT), iron reduction, and decarboxylation in the same way as many other atmospherically important photoactive iron(III) carboxylate compounds18,23,24. Citric acid is also a well-known proxy for atmospheric organic aerosol particles in terms of composition and viscosity25. Photochemically generated radicals that build up and persist may affect lifetimes of other aerosol-bound species such as pathogens or toxins, with health-related impacts.

Here, we show that photochemically produced CCRs are immobilized in highly viscous organic aerosol particles and act as a major sink for O2 inside particles, thereby inducing anoxia. Atmospheric aerosol anoxia is highly unexpected since the time it takes for small molecules, such as water and possibly oxygen, to diffuse and mix throughout non-reactive viscous particles is thought to be on the order of seconds to minutes at ambient conditions11,13,26,27. However, we found that it is the combined effects of reaction and diffusion limitations that ROS and CCRs can persist and accumulate in viscous aerosol particles and completely overwhelm O2 in their interior. This occurs under both cold and warm conditions, but largely depending on the relative humidity, RH, particles are exposed to. Persistent ROS and CCR species can then be released under more humid conditions, e.g., upon inhalation, which will exacerbate the negative health effects of aerosol exposure beyond what is expected when assuming a well-mixed and a highly reactive aerosol matrix during their airborne trajectory.

## Results

### Looking inside single particles for their chemical morphology

The FeIIICit photochemically reactive system shown in Fig. 1a was employed to produce CCRs in the presence of O2, the gas phase reactant of interest. We used a triad of photochemical experiments to observe photochemical reaction cycles on the nanoscale and microscale in single particles and films including scanning transmission X-ray microscopy coupled with near-edge X-ray absorption fine structure (STXM/NEXAFS) spectroscopy, a single particle electrodynamic balance (EDB), and a coated-wall flow tube (CWFT). Our multifarious observations were supported by a recent photochemical reaction and diffusion (PRAD) model28,29. We observed that photochemically produced CCRs induce anoxia in the interior of viscous particles, effectively preserving CCRs under dry conditions. Figure 1 shows viscous FeIIICit particles during photochemical cycling, where an oxidized shell and unoxidized core is depicted by the color gradient (Fig. 1a). This oxidation configuration was directly observed using STXM/NEXAFS to image iron(III) fraction, β, acquired minutes after photoreduction and reoxidation (Fig. 1b). These low β values are indicative of LMCT, i.e., charge transfer from the citrate ligand to Fe3+, forming Fe2+ and a primary radical product, which immediately decays by decarboxylation (i.e., the removal of a carboxyl group via loss of CO2). Then, an organic, carbon-centered radical, the primary CCR, is left behind28. Following the reaction steps in Fig. 1a, ROS is generated when O2 is taken up by the particle and reacts with photochemically generated CCRs, through mostly a first generation of peroxy radicals. Finally, iron(II) can be reoxidized by ROS or O2, then complexed again with citric acid. Low values of β observed within particles also imply an absence of the O2 and ROS needed for oxidation and thus a persistence of CCRs. We observed 2-D column integrated profiles (i.e., in the same dimension as the 2-D microscope image) of β in aerosol particles evolving in the dark at RH = 40, 50, and 60%, Fig. 1c–e respectively, to discover where oxidation occurred inside single particles. At RH = 40%, β remained low and indicated that CCRs remained at high concentrations and unreacted. Gradients in β were observed at all RH, but most discernable for RH ≤ 50% and extended throughout the interior of particles. At RH = 60%, profiles of β were relatively flat from the perimeter to the center of particles (Fig. 1e). This indicates a transition from an inhomogeneous state, characterized by anoxic conditions at RH = 40%, to homogeneous, well-mixed conditions enhancing O2 concentrations in the bulk. Therefore, we conclude that altering RH significantly alters the diffusion coefficients of reactants and products, and so controls whether or not radicals are built up or reacted away quickly.

X-ray imaging shows that oxidation occurred near particle surfaces, but not in their bulk. Therefore, photochemically generated CCRs present in the bulk must have had long lifetimes due to slow molecular transport and reaction with O2 as their main reaction partner. Additional images that support this finding acquired at the start and end of STXM/NEXAFS experiments are given in Supplementary Fig. 1. We used the PRAD model28 to simulate radical persistence due to photochemical reduction and dark reoxidation experiments performed with STXM/NEXAFS (solid lines in Fig. 1c–e). Modeled profiles of β reproduce our observations only when the modeled O2 concentration drops to zero just nanometers beneath the surface of an aerosol particle as shown in the radial profiles in Supplementary Fig. 2. The accumulation of CCRs in anoxic particle interiors is the necessary condition to explain the spectroscopically observed iron oxidation state, pointing to long radical lifetimes in photoactive, viscous aerosol particles. When particles with high radical concentration are inhaled, they may release CCRs and ROS in the respiratory tract. It is conceivable that the saturated lung environment lets non-organic and iron species undergo chemical cycling to produce even more ROS and CCRs, exacerbating lung tissue damage.

### Photochemical evolution of particle mass loss and radical release

Finally, the CWFT experiments shown in Fig. 2b show a steady-state production and release of HO2 radicals, $$P_{{\mathrm{HO}}_2}$$, demonstrating continual ROS production from photochemical cycling of FeIIICit. This radical source was due entirely to O2 uptake and reaction. Increasing the FeIIICit to citric acid mole ratio, Mr, led to an increase in $$P_{{\mathrm{HO}}_2}$$, which was expected since a greater number of photochemically active reactants should increase ROS and CCR. At our lowest investigated Mr = 0.01, the PRAD model still predicts anoxic conditions and CCR persistence as seen in Supplementary Fig. 5. We also show a typical time-resolved radial profile of HO2 concentration in Supplementary Fig. 5c, where the maximum occurs when CCR and O2 concentration within particles drops significantly. We also observed that $$P_{{\mathrm{HO}}_2}$$ increased by a factor of 1.5 for film thicknesses 0.18–0.89 µm; however, this is far less than our error estimate from the HO2 loss rate. If there were a large gradient in O2 concentration over this range, we would expect $$P_{{\mathrm{HO}}_2}$$ would significantly depend on film thickness. As this was not the case, O2 penetration must have been much smaller than 0.18 µm, in agreement with STXM and EDB observations and modeling results. Recent ambient observations of soluble iron and ligand concentration in aerosol particles20,21 discussed later have shown that the mole ratio between iron organic complexes and organic compounds can be on the order of Mr = 10−1, which is consistent with the range in our CWFT and EDB experiments.

The observation of steady-state $$P_{{\mathrm{HO}}_2}$$ was the key observable of ensuing peroxy radical chemistry in the condensed phase. The PRAD model over predicted $$P_{{\mathrm{HO}}_2}$$ when using a HO2 self-reaction rate coefficient, kSR = 8.3 × 105 M−1 s−1, from dilute aqueous solution or using a previous parameterization by Dou et al.28 as a function of RH. Here, M is molarity in units of mole L−1. It appears that the condensed phase HO2 sink was greater than only considering its self-reaction and iron reoxidation by roughly 1 order of magnitude, indicating a central role of the organic peroxy radicals in the photochemical cycling, which are presently not known and not included in detail in the PRAD model. The PRAD model captured observed $$P_{{\mathrm{HO}}_2}$$ only when fitting the HO2 loss rate as described in the Supplementary Discussion (see Supplementary Fig. 6). Measurements of $$P_{{\mathrm{HO}}_2}$$ in dependence of film thickness and O2 partial pressure (Supplementary Fig. 6), measurements as a function of RH from Dou et al.28, and PRAD model results all allowed to confine primary peroxy radical formation to the outermost surface where O2 was still present. This reveals that H2O2 and likely second-generation peroxy radicals penetrated over depths larger than expected from its self-reaction. Supplementary Fig. 7 shows that H2O2, in particular, is a large contributor to the overall ROS concentration in the PRAD model. This is because the 1st order chemical loss rate of H2O2 is slow (on the order of 10−4 s−1) and its solubility is high. Therefore, it has a high concentration in the condensed phase and enough time to diffuse through the particle. Calculated depth profiles of HO2 concentrations in films are shown in Supplementary Figs. 5 and 7 along with organic CCR, ROS, and O2 concentrations. Again, the PRAD model predicts complete O2 depletion at a short depth beneath the surface. Despite this limitation, any peroxy radical or hydroperoxides would contribute to the total ROS concentration, giving confidence to our quantification of ROS production for reoxidation and photochemical cycling. As mentioned above, HO2 peaked where O2 and CCRs were depleted, highlighting the importance of the reaction between them. In addition to EDB and STXM/NEXAFS experiments with high CCR concentrations, CWFT experiments further indicate that ROS existed at high concentrations, apparently replenished by the accelerating photochemical cycling.

## Discussion

The range of atmospheric conditions under which ROS and CCRs can persist in aerosol populations is shown in Fig. 3 as a function of temperature, T, RH, Mr, and the photochemical reaction rate, j. Conditions at which RH = 40–50% over T = 0–25 °C marks a transition between CCR buildup and depletion in aerosol particles entirely due to changing diffusion coefficients. Trends in [ROS] and [CCR] were similar as seen in Supplementary Fig. 9. At constant T and RH, [ROS] increased with Mr and reached a maximum of about 7 mM between Mr = 0.04–0.3. Inhaled particles with this level of exogenously produced ROS may contribute significantly to the total production in lungs (exogenous and endogenous), which is discussed in more detail in the Supplementary Information. When Mr increased further, [ROS] sharply decreased as seen in Fig. 3b. This was because O2 loss from CCR reaction became so extreme that O2 penetration, and thus ROS production became limited to <0.3 nm beneath the surface, i.e., the molecular scale. Additionally, an excess of Fe2+ resulted in a short ROS lifetime. In the PRAD model, diffusion coefficients for Mr > 0.05 decrease, which is evident from measured viscosities at Mr = 1.0 and 0.05 (Supplementary Fig. 11), contributing to this sub-nanometer penetration depth. Overall, we argue that ROS and CCR build-up in aerosol particles at the Earth’s surface are controlled, in part, by meteorological conditions and aerosol composition.

The rectangles in Fig. 3 allow comparing our estimates of ROS and CCR build-up with those previous field studies17,19,20,21,39, which detail aerosol composition, and specifically iron concentration, solubility, or speciation. We estimated Mr from previous studies using measured aerosol composition and 3 conservative assumptions, (i) that a fraction of iron in particles is soluble, (ii) that a fraction of soluble iron is in complex with carboxylate compounds, and (iii) that only a fraction of total particles (by number) contain iron. More details on estimates of Mr are in the Supplementary Information and Supplementary Table 2. In more continental and drier climates, as was the case for field studies in central China19 and the Great Plains of the USA17 (shown as the blue and purple boxes), T and RH were sufficiently low on average to promote radical buildup. In other field studies in Okinawa Island39, multiple urban sites in Canada20 and in the Po Valley of Italy21, climates are more humid on average. This implies that high [CCR] and [ROS] should occur across the Earth where aerosol particles are more viscous with long mean equilibrium mixing times, as previously reported40. Even under warm or humid average meteorological conditions, cold or dry weather spells can still lead to episodes of high radical concentrations. In the Po Valley of Italy21, metal concentrations were similar to other European urban areas with abundant iron carboxylate complexes (green box in Fig. 3). Therefore, we argue that iron carboxylate complexes are an ubiquitous aerosol component, in line with previous studies quantifying organic matter with carboxyl functions and iron in ambient particles10,18,39. These can lead to aerosol anoxia and a consistent source of aerosol-borne CCRs and ROS.

A large radical source due to iron carboxylate photochemistry has important implications for other atmospheric photoactive aerosol components and the lifetime of air mass tracer compounds, pathogens or toxic compounds posing a health risk. Common atmospheric brown carbon compounds such as imidazoles41,42, quinone containing compounds6,43, or humic-like substances (HULIS)44 are photoactive and may limit O2 penetration if they produce sufficient radical numbers with low diffusion coefficients. Secondary organic aerosol particles are highly viscous11,12,25,40 and photochemical aging may generate radical compounds within them that are preserved. Therefore, we strongly suggest that radical production and persistence along with anoxia may be possible with all photoactive aerosol compounds given sufficient concentration and aerosol viscosity to cause anoxia due to both reaction and diffusion limitations. The transition region for CCRs and ROS at intermediate RH as revealed in Fig. 3 and Supplementary Fig. 9 delineates conditions where radical concentration within particles is still high, but their mobility is substantial enough to exert a significant role in condensed phase aging, e.g., impacting the chemical turnover of harmful organic toxins or tracer compounds for aerosol source apportionment. This transition also coincides with the RH range where the lifetime of viruses suspended in exhaled human respiratory particles is shortest45. Exhaled particles of lung-lining fluid are composed of, in part, proteins, saccharides, and iron, which may be highly viscous, susceptible to photochemical radical buildup and impact pathogen viability. Quantifying the link between environmental parameters and aerosol photochemistry as done for the iron carboxylate complexes here will greatly improve our understanding of condensed phase chemistry, radical process, and controls on human exposure to particulate matter that are detrimental to health.

## Methods

### Scanning transmission X-ray microscopy coupled to near-edge X-ray absorption fine structure (STXM/NEXAFS) spectroscopy experiments

We recently developed a photochemical reactor at the PolLux beamline46 of the Swiss Light Source to expose particles containing citric acid and FeIIICit to UV light under atmospherically relevant RH and T47,48. The main advantage of STXM/NEXAFS spectroscopy is the coupling of high-spatial resolution and chemical selectivity for organic carbon functionality and iron oxidation state, and effectively mapping chemical reactions in particles in real-time and in situ46,49,50. All particles in the three STXM/NEXAFS experiments were exposed to O2 at a partial pressure of 112, 107, and 104 mbar, at RH = 40, 50, and 60%, respectively. Helium was the carrier gas for O2 and H2O with a total flow of 20 mL min−1 at standard temperature and pressure. The total pressure in the environmental chamber was 150 mbar. The iron oxidation state within single particles containing FeIIICit and citric acid was measured using STXM/NEXAFS. A solution having Mr = 1.0 was prepared and nebulized to generate droplets that were subsequently dried at RH < 30% and impacted onto X-ray transparent membranes51. These particles on membranes were then placed in an environmental chamber set inside the X-ray microscope47. At all steps, we avoided ambient light and humidity exposure and kept particles in a dry, dark vacuum container prior to use. The time between particle generation and use in STXM/NEXAFS experiments was <2 h. We used STXM/NEXAFS to measure transmitted X-ray photons through a square spot, or pixel, 35 × 35 nm2 in size46. A 5 × 5 µm2 image contained 20,400 pixels, each making up either the transmitted photon count mapped across a particle, I, or quantifying the background signal, I0. From this, the optical density, OD = -ln(I/I0), at each pixel was determined. Acquiring multiple images as a function of X-ray energy yielded a NEXAFS spectrum, which was used to obtain absorption peaks of FeIIICit over the L-edge of iron (700–735 eV) and the K-edge of carbon (280–320 eV). Additionally, we imaged OD at two X-ray energies, 707.8 and 709.5 eV, which correspond to the peak resonant X-ray absorption by iron(II) and iron(III) species, respectively. Energy calibration and determination of non-resonant absorption followed previous work, including a procedure to evaluate X-ray beam damage and avoid it entirely51. Image analysis was based on publicly available software tools50. Using the parameterization in Moffet et al.39 and following an imaging procedure in Alpert et al.51, we mapped the iron(III) fraction out of the total iron, β, with a time resolution on the order of minutes. Maps were used to derive 2-D β-profiles (Fig. 1c, d) following Alpert et al.51, by averaging β over the perimeter pixels (1 pixel from the perimeter) and those concentric pixels toward the center (>2 pixels from the perimeter). In line with previous studies51,52,53,54,55,56, our particles were determined to be half-spheres, evident from their morphology and OD profiles of particles compared with known spherical polystyrene particles. We note that a single profile, i.e., one color in Fig. 1c, d correspond to a single image of multiple particles (5–20) with >10,000 pixels, where each pixel quantifies iron oxidation state over an area of 1.2 × 10−3 µm2. Uncertainty in β was determined as, Δβ = ±0.07 or propagated from the photon counting error, whichever was larger51. Prior to illumination, initial β-profiles were determined. A UV-LED fiber optic coupling to the STXM chamber was custom-built utilizing UV compatible components and optics, which resulted in a uniformly illuminated sample area with a measured power density of 3.6 ± 0.6 mW mm−2 in the narrow wavelength range of 364–370 nm, equivalent to j = 2.2 ± 0.04 × 10−3 s−1 when accounting for the absorption cross section. Illumination for all samples then lasted for 15 min with a UV LED. Immediately after the light was switched off, we continually mapped β over multiple particles while re-oxidation took place under a constant RH and O2 gas phase concentration, unless otherwise specified. A different procedure is outlined in the Supplementary Information for the data specific to Supplementary Fig. 4 in order to elucidate the radical lifetime. Briefly, this involved photochemical reduction in helium, without the presence of O2, and waiting 35 min or 9 h before O2 was introduced.

### Electrodynamic balance (EDB) experiments

Experiments using an EDB28,57 were performed to measure the mass loss of aqueous particles irradiated by a frequency-doubled diode laser with a wavelength of 473 nm in the visible. In the experiments, the power density was 40 mW mm−2 at all RH except for RH = 47%, where it was 20 mW mm−2 (j = 4.3 × 10−3 and 2.2 × 10−3 s−1, respectively). Aqueous solutions having Mr = 0.05 were prepared and used to generate an aqueous particle injected into the RH and T controlled EDB chamber. The injected particle was given ample time to equilibrate with water vapor in an O2 atmosphere at a pressure of 800 mbar. The aqueous solution and particle were kept in the dark at all steps prior to irradiation. Before and after the laser was switched on, the particle radius change was monitored over time and the mass loss determined. For each investigated RH, a new particle from a freshly prepared solution was used. The EDB applies a high AC voltage across two electrode rings and a DC voltage across hyperbolic end-caps to generate an electric field to levitate particles. The electric field was adjusted automatically to compensate the gravitational force on the particle as its size changed. The refractive index and size of spherical particles were determined from measurements of backscattered light from a broad-band LED centered around 640 nm. The radius loss in Fig. 2a was determined from the ratio between the particle radius over time, r(t), and the radius prior to illumination, r0 = r (t = 0). Due to the high accuracy of determining mass and radius loss, the main source of error was due to the unknown change in refractive index from any changes in composition during irradiation.

### Coated wall flow tube (CWFT) experiments

The release of HO2 into the gas phase was measured in CWFT experiments through the efficient scavenging reaction with excess NO42,58,59. Films were generated by dispensing a known volume of aqueous FeIIICit and citric acid solutions with Mr from 0.01 to 0.11 in Duran glass tubes 1.2 cm in diameter and 50 cm long. The error on Mr, ΔM, was ±7% on its measured value. Solutions and prepared films were always kept in the dark prior to use. Calculated film thickness was between 0.2–1.8 µm with an approximate ±20% uncertainty and accounted for water uptake at a given RH. When thickness was varied, Mr = 0.0784 and RH = 38.5%. When Mr was varied, thickness was 1.1 µm and RH = 37%. Films were allowed to equilibrate to RH prior to the start of an experiment. Uncertainty in RH was ΔRH = ±2%. A constant flow rate of N2 and O2 was used, typically at a 20% O2 content. We also performed O2-dependent experiments by varying the partial flow rates, but maintaining a constant total flow, either 1.0 or 0.5 L min−1. Prior to illumination, a baseline NO concentration was determined. Illumination using up to 7 fluorescent tubes were then switched on simultaneously causing a drop in NO concentration. This drop was used to calculate the HO2 release from the film following a previous procedure42. The NO conversion was routinely checked to exclude processes involving NO and HO242,58, such as a loss due to O3 formation, a production due to the photolysis of NO2 and the return of HO2 to the film. We note, gas phase loss of HO2 with volatile organic compounds is highly unlikely to affect NO conversion as known reaction rates are far too slow. We cycled all films with intervals of UV light switched off and on for approximately 0.5–2 h per interval. Loss of NO and recovery were reproducible to within about 10%, which emphasizes the robustness of our system and our instrument precision. The light output of our fluorescent tubes had a broadband spectrum >300 nm in wavelength and extended into the visible spectrum. Utilizing the measured wavelength-dependent irradiance42, absorption cross section33, and the quantum yield28, we calculated that j = 9.1 × 10−3 s−1, which is higher than that used in STXM or EDB experiments.

### Photochemical reaction and diffusion (PRAD) model

The PRAD model was developed to describe the FeIIICit system constrained with experimental data. It utilizes physical and chemical parameters, such as molecular diffusion coefficients and Henry’s law constants for molecular transport and solubility of the multiple species represented, as well as chemical parameters, such as reaction rates and equilibrium constants. All observables in STXM/NEXAFS, EDB, and CWFT experiments are explicitly modeled and are directly compared. The condensed phase is separated in multiple layers each hosting photochemical reactions, chemical reactions and imposing equilibria conditions first, followed by modeling the flux of molecules between the layers. Details of the PRAD model are given in Dou et al.28, and those pertinent to this study are reviewed below. Diffusion coefficients of all species were scaled with the diffusion coefficient of water, Dw, i.e., the diffusion coefficient of a species x is Dx = DwfDx, where fDx is a species-specific constant. We have observed that solution viscosity increased significantly when Mr > 0.05 (Supplementary Fig. 11), therefore we have decreased Dw with increasing Mr. For example, Dw was parameterized to increase by a factor of ~4 from Mr = 0.05 to 1.028. Known equilibrium coefficients for dissociation and complex formation, photochemical reaction rates, and chemical reaction rate coefficients were determined from previous literature28. Unknown equilibrium coefficients and rate coefficients were globally fit to all STXM/NEXAFS, EDB, and CWFT experimental results simultaneously28. Henry’s law constants for O2, ROS, and other volatile compounds were also adjusted to match observations28 and were typically about 1 order of magnitude higher than those reported in dilute aqueous solution. Dou et al.28 reported an observed mass loss with UV light exposure using a quantum yield, Φ = 1.0, for wavelengths, λ < 400 nm28. In order to reproduce our observations in the EDB, we used Φ(473 nm) = 0.002 following our previous work57. A parameterization of Φ as a function of λ was formulated28 and used to predict j for CWFT experiments and for j due to sunlight reaching the Earth’s surface, which was determined with the online TUV calculator, http://cprm.acom.ucar.edu/Models/TUV/Interactive_TUV/, as a function of solar zenith angle.

## Data availability

The data that support the findings of this study are publicly available at https://doi.org/10.5281/zenodo.3817356.

## Code availability

The PRAD model code that support the findings of this study can be found in Dou et al.28.

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## Acknowledgements

This work was funded by the Swiss National Science Foundation (Grants 163074 and 188662) and by the European Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement (No 701647). The PolLux end station was financed by the German Ministerium für Bildung und Forschung (BMBF) through contracts 05K16WED and 05K19WE2. We acknowledge Mirko Holler for building the UV LED and fiber optic coupling. We further acknowledge Simone Finizio, Katharina Witte, and Blagoj Sarafimov for support at the PolLux end station.

## Author information

Authors

### Contributions

P.A.A. wrote the manuscript. M.A. and U.K.K. conceptualized and planned the study. P.A.A. planned and conducted STXM/NEXAFS experiments supervised by B.W. and M.A. J.D., P.C.A., J.X., T.H., C.N.B., and K.D.H. also conducted STXM/NEXAFS experiments. P.A.A. conducted STXM/NEXAFS data analysis and interpretation and developed the UV-LED fiber optic setup at the PolLux end station supervised by B.W. and J.R. J.D. conducted EDB experiments and data analysis and interpretation supervised by U.K.K. and T.P. P.C.A conducted CWFT experiments and data analysis and interpretation supervised by M.A. F.S. conducted viscosity experiments and data analysis and interpretation supervised by P.A.A. B.L. wrote and developed the PRAD model with the assistance of J.D. and P.A.A. H.H. and T.S. advised on the photochemical reaction mechanisms. All co-authors discussed the results and commented on the manuscript and Supplementary Information.

### Corresponding authors

Correspondence to Peter A. Alpert or Markus Ammann.

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### Competing interests

The authors declare no competing interests.

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Alpert, P.A., Dou, J., Corral Arroyo, P. et al. Photolytic radical persistence due to anoxia in viscous aerosol particles. Nat Commun 12, 1769 (2021). https://doi.org/10.1038/s41467-021-21913-x

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• DOI: https://doi.org/10.1038/s41467-021-21913-x