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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-25-6991-2025</article-id><title-group><article-title>Understanding summertime H<sub>2</sub>O<sub>2</sub> chemistry in the North China Plain through observations and modeling studies</article-title><alt-title>H<sub>2</sub>O<sub>2</sub> chemistry in the North China Plain</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ye</surname><given-names>Can</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4350-0892</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2">
          <name><surname>Liu</surname><given-names>Pengfei</given-names></name>
          <email>pfliu@rcees.ac.cn</email>
        <ext-link>https://orcid.org/0000-0001-6237-3759</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff3">
          <name><surname>Xue</surname><given-names>Chaoyang</given-names></name>
          <email>ch.xue@mpic.de</email>
        <ext-link>https://orcid.org/0000-0001-6673-7716</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zhang</surname><given-names>Chenglong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Ma</surname><given-names>Zhuobiao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Liu</surname><given-names>Chengtang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Liu</surname><given-names>Junfeng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Lu</surname><given-names>Keding</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9425-9520</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2">
          <name><surname>Mu</surname><given-names>Yujing</given-names></name>
          <email>yjmu@rcees.ac.cn</email>
        <ext-link>https://orcid.org/0000-0002-7048-2856</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Zhang</surname><given-names>Yuanhang</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>School of Environmental Science and Engineering, Tiangong University, Tianjin 300387, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Research Center for Eco-Environmental Sciences, Chinese Academy of Sciences, Beijing 100085, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Aerosol Chemistry Department, Max Planck Institute for Chemistry, Mainz 55128, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>State Key Joint Laboratory of Environment Simulation and Pollution Control, College of Environmental Sciences and Engineering, Peking University, Beijing, 100871, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Pengfei Liu (pfliu@rcees.ac.cn), Chaoyang Xue (ch.xue@mpic.de), and Yujing Mu (yjmu@rcees.ac.cn)</corresp></author-notes><pub-date><day>8</day><month>July</month><year>2025</year></pub-date>
      
      <volume>25</volume>
      <issue>13</issue>
      <fpage>6991</fpage><lpage>7005</lpage>
      <history>
        <date date-type="received"><day>20</day><month>February</month><year>2025</year></date>
           <date date-type="rev-request"><day>25</day><month>March</month><year>2025</year></date>
           <date date-type="rev-recd"><day>7</day><month>June</month><year>2025</year></date>
           <date date-type="accepted"><day>22</day><month>June</month><year>2025</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2025 Can Ye et al.</copyright-statement>
        <copyright-year>2025</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025.html">This article is available from https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e229">Hydrogen peroxide (H<sub>2</sub>O<sub>2</sub>) is a key atmospheric oxidant, crucial for oxidation capacity and sulfate production. However, its chemistry remains understudied compared to ozone (O<sub>3</sub>), limiting our understanding of photochemical pollution. In summer 2016, atmospheric peroxides and trace gases were measured at a rural site in the North China Plain. H<sub>2</sub>O<sub>2</sub> was the dominant peroxide (0.62 <inline-formula><mml:math id="M10" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.80 ppb), constituting 69 % of total peroxides. It exhibited diurnal variation similar to peroxyacetyl nitrate (PAN) and O<sub>3</sub>, indicating photochemical production. The <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio was higher on high-particle days, suggesting that H<sub>2</sub>O<sub>2</sub> uptake by particles reduces its concentration. A box model with default gas-phase chemistry overestimated H<sub>2</sub>O<sub>2</sub> by a factor of 2.7, and including particle uptake of H<sub>2</sub>O<sub>2</sub> (uptake coefficient of 6 <inline-formula><mml:math id="M19" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup>) improved agreement with observations, although we note that this value carries some uncertainty related to the assumed HO<sub>2</sub> uptake coefficient.</p>

      <p id="d2e402">HO<sub>2</sub> recombination contributed 91 % of H<sub>2</sub>O<sub>2</sub> production, with a peak rate of 1 ppb h<sup>−1</sup>. Major removal pathways included particle uptake (69 %), dry deposition (25 %), OH reaction (4 %), and photolysis (2 %). Relative incremental reactivity (RIR) analysis showed that reducing NO<sub><italic>x</italic></sub>, PM<sub>2.5</sub>, and alkanes increased H<sub>2</sub>O<sub>2</sub>, while reducing alkenes, aromatics, CO, and HONO decreased it, with alkenes having the strongest effect. <inline-formula><mml:math id="M30" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula> in 82 % of cases) indicated that O<sub>3</sub> formation was in a transition and NO<sub><italic>x</italic></sub>-sensitive regime, emphasizing the need for further volatile organic compound (VOC) and NO<sub><italic>x</italic></sub> reductions to mitigate both H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> pollution. These findings improve our understanding of H<sub>2</sub>O<sub>2</sub> chemistry and provide insights into the mitigation of photochemical pollution in rural North China.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42305099</award-id>
<award-id>42275111</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e599">The atmospheric oxidation capacity is a critical determinant of atmospheric self-cleaning, influencing the residence time and persistence of pollutant gases. Quantifying this capacity is essential for elucidating the lifetimes of pollutants, the formation of aerosols, and their subsequent radiative forcing effects. Hydrogen peroxide (H<sub>2</sub>O<sub>2</sub>) serves as a significant atmospheric oxidant, primarily generated through the recombination of hydroperoxyl radicals (HO<sub>2</sub>), which are themselves derived from reactions involving hydroxyl radicals (OH), volatile organic compounds (VOCs), and carbon monoxide (CO). Consequently, the formation of H<sub>2</sub>O<sub>2</sub> is intrinsically linked to atmospheric oxidation capacity, with its concentration serving as a direct indicator of the intensity of this capacity. Furthermore, as H<sub>2</sub>O<sub>2</sub> represents a terminal product in the ozone (O<sub>3</sub>) formation chain reaction, its concentration can be utilized to assess the sensitivity of O<sub>3</sub> production to precursors (Sillman, 1995; Reeves and Penkett, 2003; Nunnermacker et al., 2008; He et al., 2010). Owing to its strong oxidative potential and high Henry's law constant, H<sub>2</sub>O<sub>2</sub> readily dissolves in cloud droplets, where it oxidizes sulfur dioxide (SO<sub>2</sub>) to form sulfuric acid (H<sub>2</sub>SO<sub>4</sub>), thereby contributing to sulfate aerosol formation and acid rain deposition (Calvert et al., 1985). Research indicated that H<sub>2</sub>O<sub>2</sub>-mediated oxidation of SO<sub>2</sub> in cloud water accounts for 60 %–80 % of global SO<sub>2</sub> oxidation (Penkett et al., 1979; Calvert et al., 1985; Sofen et al., 2011). Additionally, recent studies have highlighted the significant role of particle-phase H<sub>2</sub>O<sub>2</sub> oxidation in sulfate formation during winter (Ye et al., 2018, 2021b; Gao et al., 2024). Given its potent oxidative properties, H<sub>2</sub>O<sub>2</sub> also poses substantial risks to human health and vegetation (Chen et al., 2010). Thus, a precise understanding of H<sub>2</sub>O<sub>2</sub> chemistry is imperative to advance the knowledge of atmospheric oxidation processes and to diagnose underlying secondary pollution formation mechanisms.</p>
      <p id="d2e822">Atmospheric H<sub>2</sub>O<sub>2</sub> concentrations are currently reported to range from 0.1 to 13 ppb (Balasubramanian and Husain, 1997; Walker et al., 2006; Ren et al., 2009; Guo et al., 2014; He et al., 2010; Qin et al., 2018; Fischer et al., 2015, 2019; Ye et al., 2022; Allen et al., 2022; Zhang et al., 2018), with their spatial and temporal variability governed by a balance between production sources and removal pathways. H<sub>2</sub>O<sub>2</sub> is generated through both primary and secondary sources. Primary sources of H<sub>2</sub>O<sub>2</sub> include biomass burning, which can contribute substantially under specific conditions. For instance, Ye et al. (2022) reported elevated H<sub>2</sub>O<sub>2</sub> concentrations during biomass combustion events, which promote secondary sulfate formation and thereby increase fine particulate matter (PM<sub>2.5</sub>) concentrations. The dominant secondary source is the recombination of HO<sub>2</sub> radicals, a process enhanced during summer months due to increased solar radiation, which elevates HO<sub>2</sub> concentrations and consequently leads to higher H<sub>2</sub>O<sub>2</sub> levels. However, under elevated nitrogen oxide (NO<sub><italic>x</italic></sub>) conditions, nitric oxide (NO) reacts competitively with HO<sub>2</sub>, suppressing H<sub>2</sub>O<sub>2</sub> formation and resulting in reduced atmospheric concentrations. Another secondary source involves the ozonolysis of alkenes, which produces Criegee intermediates that can decompose to form H<sub>2</sub>O<sub>2</sub> (Becker et al., 1990). This pathway is particularly relevant during nighttime and potentially in winter, when photochemical activity is diminished (Lee et al., 2008b). For example, alkene ozonolysis was found to dominate wintertime H<sub>2</sub>O<sub>2</sub> levels (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> %) (Qin et al., 2018), although the yields are generally low, often below 10 %. Additionally, the release of H<sub>2</sub>O<sub>2</sub> from the particle phase has been proposed as a potential source, although its contribution is considered negligible compared to gas-phase production. Recent studies, however, have highlighted that under polluted conditions, high concentrations of humic-like substances and transition metals can facilitate particle-phase H<sub>2</sub>O<sub>2</sub> formation, which subsequently partitions into the gas phase, significantly enhancing gas-phase H<sub>2</sub>O<sub>2</sub> levels (Ye et al., 2021b; Liu et al., 2021).</p>
      <p id="d2e1082">H<sub>2</sub>O<sub>2</sub> can be removed by photolysis, which not only depletes H<sub>2</sub>O<sub>2</sub> but also serves as a source of hydroperoxyl radicals (HO<sub><italic>x</italic></sub>). However, due to lower photolysis frequency, the contribution of H<sub>2</sub>O<sub>2</sub> photolysis to atmospheric HO<sub><italic>x</italic></sub> production is generally much smaller compared to the photolysis of O<sub>3</sub>, nitrous acid (HONO), and formaldehyde (HCHO). Notably, particle-phase H<sub>2</sub>O<sub>2</sub> photolysis has been identified as a critical source of free radicals within aerosols, accelerating aerosol aging and promoting the formation of secondary pollutants. Rao et al. (2023) further emphasized a significantly accelerated rate for the air–water interface H<sub>2</sub>O<sub>2</sub> photolysis, underscoring its importance as a source of particle-phase OH. Dry deposition is another key removal mechanism, leading to a vertical gradient in H<sub>2</sub>O<sub>2</sub> concentrations, with peak levels observed at approximately 2 km above the surface (Watanabe et al., 2016; Klippel et al., 2011). Due to its high solubility, wet deposition through rainwater scavenging also effectively removes H<sub>2</sub>O<sub>2</sub> from the atmosphere. Moreover, laboratory and field studies have demonstrated that heterogeneous uptake by particles can significantly contribute to H<sub>2</sub>O<sub>2</sub> removal under polluted conditions. Qin et al. (2022) reported a maximum uptake coefficient of 2.49 <inline-formula><mml:math id="M111" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−3</sup> for H<sub>2</sub>O<sub>2</sub> by ambient particles, with the uptake coefficient influenced by the concentration of transition metals within the particles.</p>
      <p id="d2e1296">In addition to H<sub>2</sub>O<sub>2</sub>, the atmosphere contains a variety of organic peroxides, such as methyl hydroperoxide (CH<sub>3</sub>OOH), formed through reactions between HO<sub>2</sub> and organic peroxy (RO<sub>2</sub>) radicals. While H<sub>2</sub>O<sub>2</sub> is the most abundant peroxide in the atmosphere, organic peroxides are recognized as a significant component of secondary organic aerosol (SOA), contributing to aerosol composition and properties. However, due to analytical challenges associated with measuring organic peroxides, most studies on atmospheric peroxides have only focused on H<sub>2</sub>O<sub>2</sub> (Zhang et al., 2012).</p>
      <p id="d2e1382">Photochemical pollution has emerged as a critical air quality issue in China, impacting both urban and rural regions. H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> are key products of photochemical pollution, and elucidating their chemical behavior is essential for developing effective strategies to mitigate photochemical pollution. However, compared to the extensive research on O<sub>3</sub>, studies on H<sub>2</sub>O<sub>2</sub> remain limited due to the technical challenges and complexities associated with its measurement. In recent years, O<sub>3</sub> concentrations in the North China Plain have exhibited a significant upward trend (Li et al., 2019; Wang et al., 2020; Lu et al., 2020), yet the characteristics of H<sub>2</sub>O<sub>2</sub> in this region remain poorly understood. Furthermore, the implementation of national emission reduction policies has led to a substantial decline in NO<sub><italic>x</italic></sub>, while VOCs persist at elevated levels (Liu et al., 2023). This shift toward low-NO<sub><italic>x</italic></sub> and high-VOC conditions is more conducive to H<sub>2</sub>O<sub>2</sub> formation. Although photochemical pollution is traditionally considered an urban phenomenon, recent studies have highlighted its increasing prevalence in rural areas, where pollution levels are gradually approaching those observed in urban areas (Ma et al., 2016). Rural regions typically exhibit lower NO<sub><italic>x</italic></sub> concentrations than urban areas, creating conditions more favorable for H<sub>2</sub>O<sub>2</sub> production. Despite this, research on H<sub>2</sub>O<sub>2</sub> in rural areas of the heavily polluted North China Plain remains scarce. Consequently, there is an urgent need to investigate H<sub>2</sub>O<sub>2</sub> chemistry in rural environments to inform targeted control strategies for photochemical pollution.</p>
      <p id="d2e1568">This study is based on a field campaign conducted in a rural area of the North China Plain, during which a comprehensive suite of gaseous (including H<sub>2</sub>O<sub>2</sub>), particulate matter, and meteorological parameters were measured. Here we investigate the temporal variations in H<sub>2</sub>O<sub>2</sub> and its relationships with other oxidants (e.g., O<sub>3</sub> and peroxyacetyl nitrate, PAN) and preliminarily estimate organic peroxide concentrations. A zero-dimensional box model was employed to examine the influence of particles on the H<sub>2</sub>O<sub>2</sub> budget and the sensitivity of H<sub>2</sub>O<sub>2</sub> production to various chemical species. Finally, we explore the potential of H<sub>2</sub>O<sub>2</sub> as an indicator for determining O<sub>3</sub> sensitivity and discuss the control strategy for alleviating photochemical pollution.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Experiments</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Measurement site</title>
      <p id="d2e1696">The observational experiment was conducted at the Station of Rural Environment, Research Center for Eco-Environmental Sciences (SRE-RCEES; 38°42<sup>′</sup> N, 115°15<sup>′</sup> E), located in Dongbaituo village, Wangdu county, Hebei province. Situated approximately 180 km southwest of Beijing, the station is surrounded primarily by farmland with no nearby industrial facilities, making it an ideal site for studying typical rural atmospheric conditions. This location has historically served as a key site for numerous large-scale observational campaigns (Tan et al., 2017; Peng et al., 2021). The experiment took place from 6 July to 12 August 2016, with the primary objective of investigating the underlying causes of photochemical pollution in the rural North China Plain.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>H<sub>2</sub>O<sub>2</sub> measurements</title>
      <p id="d2e1744">H<sub>2</sub>O<sub>2</sub> concentrations were measured using the AL-2021 H<sub>2</sub>O<sub>2</sub> monitor (Aero-Laser) (Lazrus et al., 1986). The instrument operates on the following principle: gas-phase peroxides in ambient air are collected by the buffered solution in a glass stripping coil. The trapped peroxides then react with p-hydroxyphenyl acetic acid (POPHA) under the catalysis of peroxidase, producing a fluorescent dimer. This dimer exhibits maximal light absorption at a characteristic wavelength of 320 nm and emits fluorescence with a central wavelength of 400 nm. By continuously monitoring the intensity of this fluorescence signal, the instrument enables online quantitative detection of atmospheric peroxides. To differentiate between H<sub>2</sub>O<sub>2</sub> and organic peroxides, a dual-channel measurement approach was employed. Channel A measures the total peroxide content, while channel B incorporates catalase into the absorbent solution to selectively decompose H<sub>2</sub>O<sub>2</sub>, thereby measuring only organic peroxides. The H<sub>2</sub>O<sub>2</sub> concentration is determined by the difference in signals between the two channels. Although channel B provides an approximation of organic peroxides, it is important to note that the percentage of organic peroxides reported in this study represents a lower limit, as the collection efficiency of the stripping coil technique varies significantly among different organic peroxide species. While H<sub>2</sub>O<sub>2</sub> is efficiently trapped due to its high solubility (Henry's law constant of <inline-formula><mml:math id="M172" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10<sup>5</sup> M atm<sup>−1</sup>), many organic peroxides such as methyl hydroperoxide (MHP) have substantially lower solubilities (Henry's law constant of 3 <inline-formula><mml:math id="M175" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>2</sup> M atm<sup>−1</sup>), resulting in lower collection efficiencies. Additionally, the catalase used to differentiate between H<sub>2</sub>O<sub>2</sub> and organic peroxides may not completely discriminate between certain hydroperoxide species, further contributing to uncertainty in organic peroxide quantification. The detection limit of the H<sub>2</sub>O<sub>2</sub> measurement instrument is 50 ppt, with an uncertainty of 10 %. To ensure the stability of the instrument's operation, regular calibrations are performed at fixed intervals. In several previous field experiments (Ye et al., 2018, 2021b, a; Liu et al., 2021), this instrument has been successfully utilized to measure atmospheric H<sub>2</sub>O<sub>2</sub>, demonstrating high reliability and consistent operational stability.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Other species</title>
      <p id="d2e1977">NO<sub><italic>x</italic></sub>, O<sub>3</sub>, SO<sub>2</sub>, PM<sub>2.5</sub>, CO, and total reactive nitrogen (NO<sub><italic>y</italic></sub>) were measured using commercial instruments from Thermo Electron. Volatile organic compounds (VOCs) were quantified by gas chromatography with a flame ionization detector (GC-FID), while nitrous acid (HONO) was measured using a long-path absorption photometer (LOPAP) from QUMA. The aerosol surface area density was calculated by combining data from a scanning mobility particle sizer (SMPS) and an aerodynamic particle sizer (APS). PAN was analyzed using gas chromatography with electron capture detection (GC-ECD). Gas-phase meteorological data were collected using a portable meteorological station (Model WXT520, Vaisala, Finland). The photolysis rate constant of NO<sub>2</sub> (<inline-formula><mml:math id="M190" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(NO<sub>2</sub>)) was measured directly, and other photolysis rate constants were derived using the tropospheric ultraviolet and visible (TUV) radiation model, scaled based on <inline-formula><mml:math id="M192" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(NO<sub>2</sub>) measurements. Detailed information on the experimental instruments is provided in Table S1 in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Box model descriptions</title>
      <p id="d2e2076">A zero-dimensional box model based on the RACM2-LIM1 mechanism was employed to investigate the sources and removal mechanisms of H<sub>2</sub>O<sub>2</sub>. This model is widely recognized for its ability to accurately model HO<sub><italic>x</italic></sub> radicals (Tan et al., 2017; Ma et al., 2022). Given that the HO<sub>2</sub> is a critical precursor for H<sub>2</sub>O<sub>2</sub> formation, the model's strong performance in simulating free radicals provides confidence in its ability to reliably simulate H<sub>2</sub>O<sub>2</sub> concentrations. The model was constrained using input parameters including photolysis rate constants (<inline-formula><mml:math id="M202" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(NO<sub>2</sub>), <inline-formula><mml:math id="M204" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(O<sup>1</sup>D), <inline-formula><mml:math id="M206" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(HONO), <inline-formula><mml:math id="M207" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(H<sub>2</sub>O<sub>2</sub>), <inline-formula><mml:math id="M210" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>(HCHO)), VOCs, NO, NO<sub>2</sub>, O<sub>3</sub>, HONO, methane (CH<sub>4</sub>), CO, and meteorological data (temperature, relative humidity, and pressure). VOCs were categorized into different reactivity-based groups according to their reaction rates with OH, as detailed in Table S2. The dry deposition rate constant for H<sub>2</sub>O<sub>2</sub> was set to 3 <inline-formula><mml:math id="M216" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−5</sup> s<sup>−1</sup>, and boundary layer heights were derived from the hybrid single-particle Lagrangian integrated trajectory (HYSPLIT) model.</p>
      <p id="d2e2302">The simulation focused on the period from 24 July to 3 August, selected for its stable meteorological conditions that were characterized by low wind speeds and predominantly static weather. During this period, the observed trends in H<sub>2</sub>O<sub>2</sub> concentrations exhibited consistent patterns, suggesting that local photochemical processes were the primary source of H<sub>2</sub>O<sub>2</sub>. This makes the selected time frame ideal for exploring H<sub>2</sub>O<sub>2</sub> sources using the box model. Additionally, elevated PM<sub>2.5</sub> concentrations during this period provided an opportunity to investigate the potential influence of particle uptake on H<sub>2</sub>O<sub>2</sub> removal. The rate coefficient of H<sub>2</sub>O<sub>2</sub> uptake by particles was parameterized as Eq. (1):

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M230" display="block"><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn><mml:mo>×</mml:mo><mml:mi>c</mml:mi><mml:mo>×</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Here <inline-formula><mml:math id="M231" display="inline"><mml:mi>c</mml:mi></mml:math></inline-formula> is mean molecular speed of H<sub>2</sub>O<sub>2</sub>, <inline-formula><mml:math id="M234" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula> is the H<sub>2</sub>O<sub>2</sub> uptake coefficient, and <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is aerosol surface area density.</p>
      <p id="d2e2497">To assess the contributions of different precursors to H<sub>2</sub>O<sub>2</sub> production, a relative incremental reactivity (RIR) analysis was conducted. RIR was calculated using the following equation:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M240" display="block"><mml:mrow><mml:mi mathvariant="normal">RIR</mml:mi><mml:mfenced open="(" close=")"><mml:mi>X</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mfenced open="(" close=")"><mml:mi>X</mml:mi></mml:mfenced></mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>C</mml:mi><mml:mfenced close=")" open="("><mml:mi>X</mml:mi></mml:mfenced></mml:mrow><mml:mrow><mml:mi>C</mml:mi><mml:mfenced close=")" open="("><mml:mi>X</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          In Eq. (2), <inline-formula><mml:math id="M241" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> represents the primary pollutants that may influence H<sub>2</sub>O<sub>2</sub> concentrations. H<sub>2</sub>O<sub>2</sub> represents modeled H<sub>2</sub>O<sub>2</sub> in the base case. <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>C</mml:mi><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi>C</mml:mi><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> represents the relative change in primary pollutants. <inline-formula><mml:math id="M249" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>H<sub>2</sub>O<inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula>H<sub>2</sub>O<sub>2</sub> represents the relative change in modeled H<sub>2</sub>O<sub>2</sub> concentrations induced by the reduction in <inline-formula><mml:math id="M256" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>. Considering the variations in simulated radical concentrations and the deviations in the RIR, a 20 % reduction scenario was selected for further analysis. This approach allowed for the quantification of the sensitivity of H<sub>2</sub>O<sub>2</sub> production to variations in precursor concentrations, providing insights into the key drivers of H<sub>2</sub>O<sub>2</sub> formation in the rural North China Plain.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Time series overview</title>
      <p id="d2e2800">Figure 1 depicts H<sub>2</sub>O<sub>2</sub>, other related chemical species, and meteorological parameters during the observation period. Throughout the observation period, meteorological conditions were characterized by high temperature and relative humidity. High temperature generally increased the rate constants of photochemical reactions, while abundant water vapor enhanced the recombination rate of HO<sub>2</sub> and the reaction rate between O(<sup>1</sup>D) and water vapor (H<sub>2</sub>O). The maximum O<sub>3</sub> concentration reached 120 ppb, with the maximum daily 8 h average (MDA8) frequently exceeding the National Ambient Air Quality Standard (NAAQS) class-II standard of 82 ppb (25°, 1013 kPa). High-O<sub>3</sub>-pollution events often coincided with elevated H<sub>2</sub>O<sub>2</sub> concentrations (<inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> ppb), suggesting that O<sub>3</sub> production at this site may be sensitive to NO<sub><italic>x</italic></sub>. This hypothesis will be further investigated using the <inline-formula><mml:math id="M273" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M274" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios in Sect. 3.6 on O<sub>3</sub> sensitivity. NO<sub><italic>x</italic></sub> concentrations peaked in the morning, driven by factors such as traffic emissions and lower boundary layer height. Daytime NO concentrations were generally below 1 ppb, while daily peak H<sub>2</sub>O<sub>2</sub> concentrations exhibited significant day-to-day variability, ranging from approximately 0.2 ppb to 4 ppb. Higher H<sub>2</sub>O<sub>2</sub> concentrations were observed during periods of intense solar radiation, indicating that local photochemical reactions play a significant role in H<sub>2</sub>O<sub>2</sub> production. Notably, elevated H<sub>2</sub>O<sub>2</sub> levels were only observed when NO concentrations were low, consistent with the known mechanism of H<sub>2</sub>O<sub>2</sub> formation under low-NO<sub><italic>x</italic></sub> conditions.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e3080">Measurements of H<sub>2</sub>O<sub>2</sub>, other related chemical species, and meteorological parameters at the SRE-RCEES site during the observation period.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f01.png"/>

        </fig>

      <p id="d2e3107">The average H<sub>2</sub>O<sub>2</sub> concentration during the whole observation period was 0.62 <inline-formula><mml:math id="M292" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.80 ppb, significantly higher than wintertime concentrations (0.19 ppb) at the same site (Ye et al., 2021b), as summer conditions with high solar radiation intensity and relative humidity are more conducive to H<sub>2</sub>O<sub>2</sub> production. This average concentration also exceeded summer H<sub>2</sub>O<sub>2</sub> levels reported in urban areas such as Beijing (0.27 ppb) (Qin et al., 2018) and Hong Kong (0.32 ppb) (Guo et al., 2014), likely due to lower NO<sub><italic>x</italic></sub> levels at the rural site, which favor H<sub>2</sub>O<sub>2</sub> formation. Compared to the H<sub>2</sub>O<sub>2</sub> concentrations reported at rural sites in other countries, the levels observed in this study were lower than those in Kinterbish (Watkins et al., 1995) and Whiteface Mountain (1.61 ppb) (Balasubramanian and Husain, 1997). It is worth mentioning that an average H<sub>2</sub>O<sub>2</sub> concentration of 0.51 <inline-formula><mml:math id="M304" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.90 ppb was reported at the same site in summer 2014 (Wang et al., 2016), lower than the current study's findings, reflecting a potential increasing trend in H<sub>2</sub>O<sub>2</sub> concentrations over time. In addition, multiyear measurements at the summit of Mount Tai revealed an increasing trend in H<sub>2</sub>O<sub>2</sub> concentrations in cloud water from 2014 to 2018 (Li et al., 2020), indirectly indicating rising gas-phase H<sub>2</sub>O<sub>2</sub> levels in the North China Plain. The significant reduction in NO<sub><italic>x</italic></sub> emissions in the North China Plain over recent years, while VOC levels remained relatively high or decreased less sharply, has likely shifted the atmospheric chemistry towards conditions more favorable for HO<sub>2</sub> recombination, potentially contributing to the observed increasing trend in H<sub>2</sub>O<sub>2</sub> concentrations. This aligns with the known sensitivity of H<sub>2</sub>O<sub>2</sub> formation to NO<sub><italic>x</italic></sub> levels.</p>
      <p id="d2e3363">Elevated H<sub>2</sub>O<sub>2</sub> concentrations and high relative humidity in rural areas facilitate the oxidation of SO<sub>2</sub> by H<sub>2</sub>O<sub>2</sub> in both aerosol water and cloud water, contributing to sulfate formation and increased PM<sub>2.5</sub> levels. During the observation period, the average PM<sub>2.5</sub> concentration reached 57 <inline-formula><mml:math id="M325" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, and the co-occurrence of PM<sub>2.5</sub> and O<sub>3</sub> pollution was frequently observed. This dual pollution phenomenon suggests that high concentrations of oxidants may play a significant role in driving secondary aerosol formation. PAN, another key secondary oxidant measured in this study, reached a maximum concentration of 2.9 ppb. Similar to H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub>, PAN is a product of photochemical pollution, and its temporal trends closely mirrored those of H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub>. These trends will be analyzed in detail in Sect. 3.2. As strong oxidizing agents, H<sub>2</sub>O<sub>2</sub>, O<sub>3</sub>, and PAN are proven to be damaging to vegetation and human health. Given the high concentrations of these oxidants observed in this study, photochemical pollution in rural areas poses serious risks to agricultural productivity and human health.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Diurnal patterns of three photochemical oxidants</title>
      <p id="d2e3559">The average diurnal trends in H<sub>2</sub>O<sub>2</sub>, PAN, and O<sub>3</sub> exhibited pronounced daily variations, with concentrations peaking during the daytime and declining at night (Fig. 2). These trends closely followed solar radiation patterns, highlighting the significant contribution of photochemical reactions to their formation. In addition, the pronounced daily variations also indicated the presence of abundant precursors in the region facilitating the production of H<sub>2</sub>O<sub>2</sub>, PAN, and O<sub>3</sub>. In the early morning, as solar radiation intensified, the photolysis of HONO initiated daytime photochemical reactions (Reaction R1), generating peroxyl radicals (Reaction R2). These radicals reacted with NO to produce O<sub>3</sub> (Reactions R3–R6), HO<sub>2</sub> recombination underwent bimolecular recombination to produce H<sub>2</sub>O<sub>2</sub> (Reaction R7), and peroxyacetyl radicals (PA) reacted with NO<sub>2</sub> to form PAN (Reaction R8). These processes led to a rapid increase in the concentrations of all three oxidants, with peak concentrations reaching 1.8, 1.2, and 84 ppb for H<sub>2</sub>O<sub>2</sub>, PAN, and O<sub>3</sub>, respectively.</p>

      <fig id="F2"><label>Figure 2</label><caption><p id="d2e3692">Average diurnal cycles of H<sub>2</sub>O<sub>2</sub>, PAN, and O<sub>3</sub> observed throughout the entire campaign period at the SRE-RCEES site.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f02.png"/>

        </fig>

      <p id="d2e3728">Despite sharing similar photochemical formation pathways, the peak times of the three oxidants differed due to variations in their production and removal rates. PAN concentrations peaked around 12:00 LT (all subsequent times are in local time, LT), approximately 2–3 h earlier than H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub>, a phenomenon also observed in previous studies (Lee et al., 2008a). This earlier peak in PAN can be attributed to its higher thermal decomposition rate at midday. In contrast, the peaks for H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> both occurred around 16:00. Notably, in urban areas, H<sub>2</sub>O<sub>2</sub> peaks often lag behind O<sub>3</sub> peaks. For example, observations at the urban Tai'an site in the North China Plain revealed that H<sub>2</sub>O<sub>2</sub> peaks occurred approximately 2 h after O<sub>3</sub> peaks (Ye et al., 2021a). This delay can be explained by HO<sub>2</sub> chemistry under varying NO<sub><italic>x</italic></sub> conditions. Under high-NO<sub><italic>x</italic></sub> conditions, HO<sub>2</sub> primarily reacts with NO (reaction rate constant of 8.9 <inline-formula><mml:math id="M371" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−12</sup> cm<sup>3</sup> molecule<sup>−1</sup> s<sup>−1</sup> at 298 K), whereas under low-NO<sub><italic>x</italic></sub> conditions, HO<sub>2</sub> undergoes bimolecular recombination to form H<sub>2</sub>O<sub>2</sub> (reaction rate constant of 1.5 <inline-formula><mml:math id="M380" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−12</sup> cm<sup>3</sup> molecule<sup>−1</sup> s<sup>−1</sup> at 298 K). In urban settings, H<sub>2</sub>O<sub>2</sub> peaks only occur when NO concentrations drop to around 100 ppt, allowing HO<sub>2</sub> recombination to dominate, thus delaying the H<sub>2</sub>O<sub>2</sub> peak relative to O<sub>3</sub>. However, at this rural site, daytime NO concentrations were consistently low, resulting in simultaneous peaks for O<sub>3</sub> and H<sub>2</sub>O<sub>2</sub>. 

                <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M394" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R3"><mml:mtd><mml:mtext>R1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">HONO</mml:mi><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R4"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">VOCs</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R5"><mml:mtd><mml:mtext>R3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OVOC</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R6"><mml:mtd><mml:mtext>R4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R7"><mml:mtd><mml:mtext>R5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>→</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">O</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R8"><mml:mtd><mml:mtext>R6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">O</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mi mathvariant="normal">P</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R9"><mml:mtd><mml:mtext>R7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>M</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mo>+</mml:mo><mml:mi>M</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R10"><mml:mtd><mml:mtext>R8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="normal">O</mml:mi></mml:mfenced><mml:mi mathvariant="normal">OO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>M</mml:mi><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="normal">O</mml:mi></mml:mfenced><mml:msub><mml:mi mathvariant="normal">OONO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mfenced close=")" open="("><mml:mi mathvariant="normal">PAN</mml:mi></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mspace width="1em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mo>+</mml:mo><mml:mi>M</mml:mi></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          Following their peaks, the concentrations of all three oxidants declined rapidly. For H<sub>2</sub>O<sub>2</sub>, this decrease was primarily driven by dry deposition and, in the evening, enhanced uptake by liquid aerosols formed as relative humidity increased. O<sub>3</sub> concentrations dropped due to a combination of dry deposition and NO titration, while PAN levels decreased mainly through thermal decomposition. At night, the absence of photochemical reactions caused all three oxidants to maintain low concentrations.</p>
      <p id="d2e4442">Figure 3 illustrates the average diurnal trends in ROOH and H<sub>2</sub>O<sub>2</sub>. The trends in total peroxides closely align with those of H<sub>2</sub>O<sub>2</sub>, indicating similar production and removal mechanisms. H<sub>2</sub>O<sub>2</sub> accounts for 69 % of the total peroxides on average, while ROOH (0.28 ppb) constitutes 31 %. This demonstrates that peroxides in rural areas are predominantly dominated by H<sub>2</sub>O<sub>2</sub>, consistent with the findings of Wang et al. (2016) at this site. However, it is important to note that the percentage of ROOH reported in this study represents a lower limit, as not all ROOH is fully captured by the measurement technique. In contrast, Liang et al. (2013) reported that ROOH accounted for 80 % of total peroxides in urban areas such as Beijing. The difference in organic peroxide proportions between Beijing and Wangdu can likely be attributed to variations in chemical conditions, such as differences in VOC compositions, which influence the types and abundances of the peroxyl radicals formed.</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e4520">Average diurnal cycles of H<sub>2</sub>O<sub>2</sub> and organic peroxides (ROOH) observed throughout the entire campaign period at the SRE-RCEES site.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f03.png"/>

        </fig>

      <p id="d2e4547">The diurnal variation in the relative contributions of H<sub>2</sub>O<sub>2</sub> and ROOH to total peroxides reflects their distinct production and loss mechanisms. H<sub>2</sub>O<sub>2</sub> dominates (over 90 %) around 19:00 due to strong photochemical production via HO<sub>2</sub> recombination during the day, while its contribution drops to <inline-formula><mml:math id="M413" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 % by 05:00 due to nighttime losses (e.g., heterogeneous uptake and dry deposition) without replenishment. In contrast, ROOH contributes more significantly in the early morning, likely due to slower loss rates compared to H<sub>2</sub>O<sub>2</sub>. ROOH molecules such as CH<sub>3</sub>OOH (methyl hydroperoxide) have much lower dry-deposition rates – approximately 30 times lower than that of H<sub>2</sub>O<sub>2</sub> – leading to less nighttime loss and a higher relative contribution to total peroxides during early-morning hours. The minimum in ROOH concentration observed around 19:00 represents a transitional point. By this time, daytime photochemical production has largely ceased due to diminishing solar radiation, leading to a decline from its afternoon peak as the removal processes continue. The subsequent increase in ROOH concentration after 19:00, which makes 19:00 a local minimum, may be attributed to nighttime chemical production primarily through (a) the ozonolysis of alkenes (O<inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> alkenes <inline-formula><mml:math id="M420" display="inline"><mml:mrow><mml:mo>→</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>→</mml:mo></mml:mrow></mml:math></inline-formula> RO<sub>2</sub> <inline-formula><mml:math id="M422" display="inline"><mml:mo>→</mml:mo></mml:math></inline-formula> ROOH) and (b) NO<sub>3</sub> radical-initiated oxidation of VOCs (NO<sub>2</sub> <inline-formula><mml:math id="M425" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> O<sub>3</sub> <inline-formula><mml:math id="M427" display="inline"><mml:mo>→</mml:mo></mml:math></inline-formula> NO<sub>3</sub>; NO<sub>3</sub> <inline-formula><mml:math id="M430" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> VOCs <inline-formula><mml:math id="M431" display="inline"><mml:mrow><mml:mo>→</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>→</mml:mo></mml:mrow></mml:math></inline-formula> RO<sub>2</sub> <inline-formula><mml:math id="M433" display="inline"><mml:mo>→</mml:mo></mml:math></inline-formula> ROOH). These processes become major sources of RO<sub>2</sub> (and subsequently ROOH) during the night. In contrast, H<sub>2</sub>O<sub>2</sub> typically continues to decrease throughout the night. Although ozonolysis can also be a source of H<sub>2</sub>O<sub>2</sub>, H<sub>2</sub>O<sub>2</sub> generally has a higher dry-deposition velocity than many ROOH species, leading to more efficient net removal overnight. These differences highlight the distinct photochemical dynamics and loss mechanisms of H<sub>2</sub>O<sub>2</sub> compared to ROOH, influenced by diurnal variations in radiation, precursor concentrations, and meteorological conditions.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Correlations between different atmospheric oxidants</title>
      <p id="d2e4875">The formation of H<sub>2</sub>O<sub>2</sub>, O<sub>3</sub>, and PAN is closely linked to VOCs, NO<sub><italic>x</italic></sub>, and solar radiation. Consequently, their concentrations are typically elevated and well-correlated during photochemical pollution episodes. Here, we investigate the relationships among these oxidants. Figure 4 illustrates the correlations between the daily maximum concentrations of H<sub>2</sub>O<sub>2</sub>, O<sub>3</sub>, and PAN. A good correlation (<inline-formula><mml:math id="M450" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.55</mml:mn></mml:mrow></mml:math></inline-formula>) was observed between PAN and O<sub>3</sub>, consistent with previous studies (Lee et al., 2008a; Zhang et al., 2014; Xu et al., 2021; Sun et al., 2020). In contrast, the correlation between H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> was weak (<inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.19</mml:mn></mml:mrow></mml:math></inline-formula>). Prior research has shown positive correlations between H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> during photochemical pollution due to their shared dependence on VOC and NO<sub><italic>x</italic></sub> photochemistry (Hua et al., 2008; Takami et al., 2003; Ye et al., 2021a; Guo et al., 2022), while negative correlations have been reported in the clean marine boundary layer where O<sub>3</sub> photolysis dominates radical production (Ayers et al., 1992). The lack of a positive correlation between O<sub>3</sub> and H<sub>2</sub>O<sub>2</sub> in this rural polluted environment may indicate additional factors influencing H<sub>2</sub>O<sub>2</sub> concentrations. Notably, heterogeneous uptake by particles has been shown to affect H<sub>2</sub>O<sub>2</sub> levels (de Reus et al., 2005; Qin et al., 2018), and given the relatively high PM<sub>2.5</sub> concentrations during the observation period, we hypothesize that heterogeneous loss reduces gas-phase H<sub>2</sub>O<sub>2</sub>, weakening its correlation with O<sub>3</sub>. Additionally, aqueous-phase reactions in aerosol water or cloud droplets, facilitated by high relative humidity during the campaign, could further reduce gas-phase H<sub>2</sub>O<sub>2</sub> without affecting O<sub>3</sub>, contributing to the decoupling of their peak values. While the focus on daytime maxima limits the direct relevance of nighttime chemistry, processes such as alkene ozonolysis or nocturnal deposition could influence background H<sub>2</sub>O<sub>2</sub> levels, indirectly affecting daytime peaks.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e5203">Correlations of the O<sub>3</sub> daily maximum with H<sub>2</sub>O<sub>2</sub> and the PAN daily maximum.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f04.png"/>

        </fig>

      <p id="d2e5239">To test this hypothesis, we analyzed the <inline-formula><mml:math id="M480" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio on polluted (daily average PM<sub>2.5</sub> <inline-formula><mml:math id="M482" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 50 <inline-formula><mml:math id="M483" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) and clean days (daily average PM<sub>2.5</sub> <inline-formula><mml:math id="M486" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math id="M487" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>). While O<sub>3</sub> and H<sub>2</sub>O<sub>2</sub> share similar photochemical formation pathways, O<sub>3</sub> is less affected by particle uptake. O<sub>3</sub> lifetime was estimated to be 13 d with respect to heterogeneous uptake for dust mass concentrations of 1000 <inline-formula><mml:math id="M494" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, highlighting the minor role of particle uptake on O<sub>3</sub> removal (Tang et al., 2017). If the <inline-formula><mml:math id="M497" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio remains stable across polluted and clean conditions, heterogeneous uptake likely has minimal impact on H<sub>2</sub>O<sub>2</sub>. However, if the ratio is higher during polluted periods, it is possible that PM<sub>2.5</sub> may scavenge H<sub>2</sub>O<sub>2</sub> by heterogeneous uptake. As shown in Fig. 5, the <inline-formula><mml:math id="M503" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio during peak photochemical hours (09:00–18:00) was markedly higher on polluted days compared to clean days, supporting the hypothesis that heterogeneous uptake by PM<sub>2.5</sub> significantly reduces H<sub>2</sub>O<sub>2</sub> concentrations. It is important to note that this method provides only a preliminary assessment, as uncertainties exist due to differences in the dependence of H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> on peroxyl radical concentrations and their respective responses to radiation intensity. In addition, differences in photochemical regimes, potentially driven by varying <inline-formula><mml:math id="M510" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">VOC</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios between clean and polluted days, could also influence the <inline-formula><mml:math id="M511" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relationship independently of particle uptake effects. In the following section, we further examine the impact of PM<sub>2.5</sub> on H<sub>2</sub>O<sub>2</sub> budget using a box model.</p>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e5639">Average <inline-formula><mml:math id="M515" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from 09:00 to 18:00 on clean (daily average PM<sub>2.5</sub> <inline-formula><mml:math id="M517" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 50 <inline-formula><mml:math id="M518" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) and polluted days (daily average PM<sub>2.5</sub> <inline-formula><mml:math id="M521" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math id="M522" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Investigation of the H<sub>2</sub>O<sub>2</sub> budget</title>
      <p id="d2e5773">To better understand the sources and removal mechanisms of H<sub>2</sub>O<sub>2</sub>, we employed a box model to simulate its concentrations. As shown in Fig. 6, base simulations using the model's default H<sub>2</sub>O<sub>2</sub> source and removal mechanisms overestimated H<sub>2</sub>O<sub>2</sub> concentrations compared to observations, with a simulated-to-measured ratio of 2.7. This discrepancy suggests an unaccounted removal pathway, consistent with our earlier hypothesis of H<sub>2</sub>O<sub>2</sub> removal by particle uptake. When a parameterized uptake mechanism with an uptake coefficient of 6 <inline-formula><mml:math id="M534" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup> was incorporated into the box model, the simulated H<sub>2</sub>O<sub>2</sub> concentrations and trends aligned well with observed values (Fig. 6), confirming the significant role of particle uptake in H<sub>2</sub>O<sub>2</sub> removal in rural areas. This uptake coefficient is comparable with the value (5 <inline-formula><mml:math id="M540" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup>) estimated during a dense Saharan dust event (de Reus et al., 2005) and lower than the value of 1 <inline-formula><mml:math id="M542" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−3</sup> reported by Wang et al. (2016), which may be likely due to differences in particulate matter composition. Sensitivity tests indicated that an uptake coefficient of 1 <inline-formula><mml:math id="M544" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−3</sup> resulted in underestimation (Fig. S1), supporting 6 <inline-formula><mml:math id="M546" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup> as the optimal value for our study. This coefficient falls within the range (10<sup>−4</sup>–10<sup>−3</sup>) determined in laboratory studies for H<sub>2</sub>O<sub>2</sub> uptake on ambient particles collected on filters or artificial particles (Pradhan et al., 2010; Romanias et al., 2012; Qin et al., 2022). We believe that this value represents a reasonable estimate for the conditions at our sampling site, although we acknowledge that a more dynamic treatment of heterogeneous processes that accounts for variations in aerosol composition, phase state, and ambient RH would be valuable in future studies.</p>

      <fig id="F6"><label>Figure 6</label><caption><p id="d2e6027">Observed and modeled H<sub>2</sub>O<sub>2</sub> concentrations from 24 July to 3 August.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f06.png"/>

        </fig>

      <p id="d2e6054">It should be mentioned that previous studies have demonstrated that considering HO<sub>2</sub> uptake by particles can partially explain the discrepancy between observed and modeled HO<sub>2</sub> concentrations under low-NO<sub><italic>x</italic></sub> conditions (Kanaya et al., 2007a, b; Whalley et al., 2010; Ma et al., 2022), as well as the phenomenon of increasing O<sub>3</sub> concentrations with decreasing particulate matter levels (Li et al., 2019). Since HO<sub>2</sub> is a precursor to H<sub>2</sub>O<sub>2</sub>, its uptake by particles naturally reduces H<sub>2</sub>O<sub>2</sub> concentrations. However, laboratory-measured HO<sub>2</sub> uptake coefficients exhibit significant variability, ranging from 10<sup>−5</sup> to 0.82, and are strongly influenced by the composition of the particulate matter (Thornton et al., 2008; Taketani et al., 2012; George et al., 2013; Lakey et al., 2015). Through analysis of the measured radical budget and related parameters, Tan et al. (2020) showed that the HO<sub>2</sub> uptake was not important in the North China Plain in 2014, with an uptake coefficient of 0.08. Given that our observational experiments were conducted at the same site with a similar particulate matter composition, we also assumed an HO<sub>2</sub> uptake coefficient of 0.08 to investigate its impact on the H<sub>2</sub>O<sub>2</sub> budget. Under this assumption, we found that an H<sub>2</sub>O<sub>2</sub> uptake coefficient of 4.5 <inline-formula><mml:math id="M571" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup> resulted in good agreement between modeled and observed H<sub>2</sub>O<sub>2</sub> concentrations (Fig. S1). The results indicate that considering HO<sub>2</sub> uptake reduces the H<sub>2</sub>O<sub>2</sub> uptake coefficient by 25 %. Therefore, uncertainties in the HO<sub>2</sub> uptake coefficient significantly affect the accurate simulation of H<sub>2</sub>O<sub>2</sub> concentrations and the estimation of the H<sub>2</sub>O<sub>2</sub> uptake coefficient. A more precise parameterization scheme for HO<sub>2</sub> uptake is critical for models to accurately assess the global distribution of H<sub>2</sub>O<sub>2</sub> concentrations and their environmental impacts.</p>
      <p id="d2e6355">Figure 7 depicts the H<sub>2</sub>O<sub>2</sub> production rates and removal rates by different pathways. The percentage contribution of different pathways is shown in Fig. S2. HO<sub>2</sub> bimolecular recombination was identified as the dominant H<sub>2</sub>O<sub>2</sub> production pathway, contributing 91 % of the H<sub>2</sub>O<sub>2</sub> production, with a maximum yield of 1.0 ppb h<sup>−1</sup> at noon. This highlighted rapid photochemical production as the primary driver of H<sub>2</sub>O<sub>2</sub> pollution at the rural site. In contrast, the reaction of O<sub>3</sub> with alkenes accounted for 9 % of H<sub>2</sub>O<sub>2</sub> production (Fig. S2), with a maximum yield of 0.07 ppb h<sup>−1</sup>, primarily from O<inline-formula><mml:math id="M600" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/></mml:mrow></mml:math></inline-formula>OLI reactions. This mechanism was found to be significant during winter pollution due to high alkene and NO concentrations inhibiting HO<sub>2</sub> recombination (Qin et al., 2018). Heterogeneous uptake dominated H<sub>2</sub>O<sub>2</sub> removal, accounting for 69 %, with a maximum removal rate of 0.7 ppb h<sup>−1</sup>, underscoring its importance during summer pollution periods. Dry deposition, photolysis, and reaction with OH radicals contributed 25 %, 2 %, and 4 % H<sub>2</sub>O<sub>2</sub> losses, respectively. These findings provide a comprehensive understanding of H<sub>2</sub>O<sub>2</sub> sources and sinks in rural environments, emphasizing the critical role of particle uptake in the H<sub>2</sub>O<sub>2</sub> budget.</p>

      <fig id="F7"><label>Figure 7</label><caption><p id="d2e6603">Modeled H<sub>2</sub>O<sub>2</sub> sources and sinks.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Precursor control to mitigate H<sub>2</sub>O<sub>2</sub> pollution</title>
      <p id="d2e6658">It is evident that photochemical pollution in rural areas is associated with elevated concentrations of H<sub>2</sub>O<sub>2</sub>, necessitating urgent measures to mitigate H<sub>2</sub>O<sub>2</sub> pollution by regulating its precursor compounds. Given the diversity of precursors involved in H<sub>2</sub>O<sub>2</sub> formation, a critical objective is to quantify the relative contribution of each precursor of H<sub>2</sub>O<sub>2</sub> pollution to establish prioritized control strategies. In this study, the RIR method was employed to identify the most effective pollutants for H<sub>2</sub>O<sub>2</sub> control (Fig. 8). Here it should be noted that the RIR analysis was performed using the adjusted model with an H<sub>2</sub>O<sub>2</sub> uptake coefficient of 6 <inline-formula><mml:math id="M627" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup> that showed good agreement with observations. The results demonstrate that reducing NO concentrations leads to an increase in H<sub>2</sub>O<sub>2</sub> levels, as the reaction between NO and HO<sub>2</sub> inhibits H<sub>2</sub>O<sub>2</sub> production. However, under realistic conditions, a decrease in NO also results in reduced NO<sub>2</sub> levels. Since the NO<sub>2</sub> heterogeneous reaction is a significant source of HONO, which serves as a key precursor for OH that influences H<sub>2</sub>O<sub>2</sub> formation, a decline in NO<sub>2</sub> consequently reduces H<sub>2</sub>O<sub>2</sub> concentrations. To validate this hypothesis, RIR values for NO<sub><italic>x</italic></sub> were calculated. Although the absolute RIR values for NO<sub><italic>x</italic></sub> remained negative (<inline-formula><mml:math id="M643" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.06), they were significantly lower than those for NO (<inline-formula><mml:math id="M644" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.9), indicating that the reduction in H<sub>2</sub>O<sub>2</sub> due to decreased NO<sub>2</sub> partially offsets the increase in H<sub>2</sub>O<sub>2</sub> caused by reduced NO.</p>

      <fig id="F8"><label>Figure 8</label><caption><p id="d2e6980">Sensitivity of H<sub>2</sub>O<sub>2</sub> production to different chemical species.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f08.png"/>

        </fig>

      <p id="d2e7007">Furthermore, the negative RIR value for alkanes (<inline-formula><mml:math id="M652" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.06) suggests that lowering alkane concentrations enhances H<sub>2</sub>O<sub>2</sub> production, likely due to their lower photochemical reactivities with OH. When alkane levels are reduced, OH radicals preferentially react with more reactive alkenes and aromatics, leading to increased HO<sub>2</sub> and hence more H<sub>2</sub>O<sub>2</sub> formation. The RIR values for alkenes (0.51), aromatics (0.15), and CO (0.26) were consistently positive, indicating that reducing these pollutants is effective in reducing H<sub>2</sub>O<sub>2</sub> concentrations, with alkenes exhibiting the most pronounced effect. Consequently, controlling alkene concentrations within anthropogenic VOCs should be prioritized, aligning with findings from previous studies (Wang et al., 2016; Ye et al., 2021a). Coal combustion and gasoline exhaust were identified as the primary sources of alkenes in the region, underscoring the importance of regulating these emissions to mitigate H<sub>2</sub>O<sub>2</sub> pollution. Additionally, the RIR value for HONO was 0.12, indicating that reducing HONO concentrations can further diminish H<sub>2</sub>O<sub>2</sub> levels by limiting the primary radical source. Elevated HONO concentrations have been observed across various sites in China, contributing over 40 % of the primary radical production. Thus, reducing HONO emissions represents a potential mitigating strategy for H<sub>2</sub>O<sub>2</sub>. Ye et al. (2022) reported that HONO emissions due to fertilizer use significantly increase H<sub>2</sub>O<sub>2</sub> levels in rural areas, suggesting that reducing excessive fertilizer use could mitigate H<sub>2</sub>O<sub>2</sub> pollution. Moreover, NO<sub>2</sub> heterogeneous reactions at various interfaces and nitrate photolysis are additional sources of HONO (Xue et al., 2020; Xue et al., 2022), highlighting the potential to reduce H<sub>2</sub>O<sub>2</sub> by decreasing NO<sub>2</sub> concentrations and subsequently limiting HONO production.</p>
      <p id="d2e7210">The RIR value for PM<sub>2.5</sub> (<inline-formula><mml:math id="M675" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.6) was found to be negative, as reducing PM<sub>2.5</sub> decreases the uptake of H<sub>2</sub>O<sub>2</sub>, thereby increasing its gas-phase concentration. Recent studies have extensively examined the impact of PM<sub>2.5</sub> reduction on O<sub>3</sub> concentrations, attributing this phenomenon to diminished HO<sub>2</sub> radical uptake and enhanced photolysis rates, both of which elevate O<sub>3</sub> levels (Wang et al., 2019; Song et al., 2022). These mechanisms similarly contribute to increased H<sub>2</sub>O<sub>2</sub> concentrations, yet the effect of particulate matter reduction on H<sub>2</sub>O<sub>2</sub> has been largely overlooked. This study demonstrates that PM<sub>2.5</sub> reduction also decreases H<sub>2</sub>O<sub>2</sub> uptake, further exacerbating its gas-phase concentration. This increase in H<sub>2</sub>O<sub>2</sub> could enhance sulfate formation efficiency and pose greater threats to human health and ecosystems. Given the critical role of H<sub>2</sub>O<sub>2</sub> in an atmospheric oxidation capacity, in global sulfate aerosol formation, and on human health, further research is warranted to investigate H<sub>2</sub>O<sub>2</sub> trends, environmental impacts, and mitigation strategies.</p>
</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Implications for O<sub>3</sub> formation</title>
      <p id="d2e7430">H<sub>2</sub>O<sub>2</sub> measurements serve as a valuable indicator of O<sub>3</sub> production sensitivity. Under NO<sub><italic>x</italic></sub>-poor conditions, the HO<sub>2</sub> recombination to form H<sub>2</sub>O<sub>2</sub> represents the primary radical termination pathway. Conversely, under NO<sub><italic>x</italic></sub>-sufficient conditions, the reaction between NO<sub>2</sub> and OH to form nitric acid (HNO<sub>3</sub>) constitutes the dominant termination mechanism. Sillman (1995) identified the <inline-formula><mml:math id="M707" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio as a robust indicator of O<sub>3</sub> sensitivity, with model simulations revealing that a ratio between 0.2 and 0.3 corresponds to a transitional regime, while values exceeding 0.3 indicate NO<sub><italic>x</italic></sub>-limited conditions and values below 0.2 suggest VOC-limited conditions. In the absence of direct gaseous HNO<sub>3</sub> measurements, alternative metrics such as the <inline-formula><mml:math id="M711" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M712" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios can be employed to assess O<sub>3</sub> sensitivity (Sillman et al., 1998), where NO<sub><italic>z</italic></sub> encompasses HNO<sub>3</sub>, PAN, HONO, and alkyl nitrates, and NO<sub><italic>y</italic></sub> is defined as NO<sub><italic>z</italic></sub> <inline-formula><mml:math id="M718" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<sub><italic>x</italic></sub>.</p>

      <fig id="F9"><label>Figure 9</label><caption><p id="d2e7691">O<sub>3</sub> concentrations values from 1 to 11 August. The red points represent measurements where <inline-formula><mml:math id="M721" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is greater than 0.15, while the blue points correspond to measurements where <inline-formula><mml:math id="M722" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is less than or equal to 0.15.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f09.png"/>

        </fig>

      <p id="d2e7759">In this study, simultaneous measurements of H<sub>2</sub>O<sub>2</sub> and NO<sub><italic>z</italic></sub> enabled the determination of O<sub>3</sub> sensitivity using the <inline-formula><mml:math id="M727" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratio, with a transitional range identified at 0.15–0.20 (Sillman et al., 1998). The analysis focused on the period of intense photochemical activity between 10:00 and 17:00. As illustrated in Fig. 9, over 82 % of measured <inline-formula><mml:math id="M728" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values exceeded 0.15, indicating that the rural study area predominantly exhibited NO<sub><italic>x</italic></sub>-limited or transitional conditions during most of the observed period. It is important to note that this metric can be influenced by additional factors. For instance, significant uptake of H<sub>2</sub>O<sub>2</sub> by particles was observed in this study, suggesting that the actual photochemical production of H<sub>2</sub>O<sub>2</sub> is higher than the measured concentrations. Consequently, the theoretical <inline-formula><mml:math id="M734" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratio is likely greater than the observed values, implying that O<sub>3</sub> production is more strongly aligned with NO<sub><italic>x</italic></sub>-limited or transitional regimes.</p>

      <fig id="F10"><label>Figure 10</label><caption><p id="d2e7941">Correlation between daily maxima of O<sub>3</sub> and NO<sub><italic>z</italic></sub>. The numbers adjacent to the solid dots represent the dates.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/6991/2025/acp-25-6991-2025-f10.png"/>

        </fig>

      <p id="d2e7968">To corroborate these findings, the <inline-formula><mml:math id="M739" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratio was also utilized to evaluate O<sub>3</sub> sensitivity (Fig. 10). The relationship between peak O<sub>3</sub> concentrations and peak NO<sub><italic>z</italic></sub> concentrations demonstrated a good positive correlation (<inline-formula><mml:math id="M743" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.71</mml:mn></mml:mrow></mml:math></inline-formula>), with a regression slope of 4.98. This slope is comparable with the value (3.3–7.6) reported in a mountainous area north of Beijing (Wang et al., 2006) but lower than those (6–11) observed in Houston (Daum et al., 2004). Notably, the positive correlation persisted up to NO<sub><italic>z</italic></sub> concentrations of 12 ppb, differing from observations at other sites where the slope typically decreased for NO<sub><italic>z</italic></sub> levels above 10 ppb (Trainer et al., 1993). This deviation can be attributed to reduced O<sub>3</sub> production efficiency under VOC-limited conditions. However, the sustained positive correlation across the entire study period suggests that the generation of NO<sub><italic>z</italic></sub> is consistently accompanied by O<sub>3</sub> production, further supporting the prevalence of NO<sub><italic>x</italic></sub>-sensitive or transitional regimes. These results align with those derived from the <inline-formula><mml:math id="M750" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratio, affirming the utility of <inline-formula><mml:math id="M751" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as a reliable indicator of O<sub>3</sub> sensitivity.</p>
      <p id="d2e8148">The findings underscore the importance of controlling NO<sub><italic>x</italic></sub> concentrations to mitigate photochemical pollution in rural areas. Tan et al. (2017) similarly reported that O<sub>3</sub> production in the rural North China Plain is primarily NO<sub><italic>x</italic></sub>-limited. As NO<sub><italic>x</italic></sub> emissions continue to decline due to regulatory efforts, an increasing number of regions may transition to NO<sub><italic>x</italic></sub>-limited or transitional regimes, highlighting the potential benefits of stringent NO<sub><italic>x</italic></sub> reduction strategies for future O<sub>3</sub> pollution control. However, given the need for synergistic management of H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub>, a dual approach targeting both NO<sub><italic>x</italic></sub> and VOC emissions remains essential. This integrated strategy will be critical to achieve effective and sustainable air quality improvements.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d2e8261">To investigate photochemical pollution in rural areas, measurements of H<sub>2</sub>O<sub>2</sub> and related parameters were conducted in the Wangdu region during the summer of 2016. H<sub>2</sub>O<sub>2</sub> exhibited a distinct diurnal pattern, with an average concentration of 0.62 <inline-formula><mml:math id="M768" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.80 ppb. Daily maximum concentrations of H<sub>2</sub>O<sub>2</sub> varied significantly, ranging from a minimum of 0.2 ppb to a maximum of 4 ppb. The diurnal cycles of H<sub>2</sub>O<sub>2</sub>, PAN, and O<sub>3</sub> all followed solar radiation trends, indicating that photochemical reactions predominantly control their production. A good correlation (<inline-formula><mml:math id="M774" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.55</mml:mn></mml:mrow></mml:math></inline-formula>) was observed between daily maximum concentrations of PAN and O<sub>3</sub>, whereas the correlation between maximum concentrations of H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> was weak, suggesting that unidentified processes influencing gas-phase H<sub>2</sub>O<sub>2</sub> concentrations may attenuate this relationship. Analysis of the <inline-formula><mml:math id="M781" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio revealed that this ratio was significantly higher on polluted days compared to clean days, implying that particle uptake likely reduces gas-phase H<sub>2</sub>O<sub>2</sub> concentrations.</p>
      <p id="d2e8467">To further elucidate the factors influencing H<sub>2</sub>O<sub>2</sub> concentrations, a box model was employed. The model simulations initially overestimated H<sub>2</sub>O<sub>2</sub> concentrations, with a modeled-to-observed ratio of 2.7. However, when an H<sub>2</sub>O<sub>2</sub> heterogeneous uptake mechanism was incorporated into the model scheme with an uptake coefficient of 6 <inline-formula><mml:math id="M790" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−4</sup>, the simulated H<sub>2</sub>O<sub>2</sub> concentrations aligned well with the observed data, underscoring the significant role of heterogeneous uptake in H<sub>2</sub>O<sub>2</sub> removal. The primary source of H<sub>2</sub>O<sub>2</sub> was identified as the bimolecular recombination of HO<sub>2</sub>, contributing 91 % of the total source strength, with a maximum production rate of 1 ppb h<sup>−1</sup>. The dominant removal pathways for H<sub>2</sub>O<sub>2</sub> included particle uptake (69 %), followed by dry deposition (25 %), reaction with OH (4 %), and photolysis (2 %).</p>
      <p id="d2e8639">Relative incremental reactivity (RIR) analysis demonstrated that reducing NO<sub><italic>x</italic></sub>, PM<sub>2.5</sub>, and alkanes exacerbated H<sub>2</sub>O<sub>2</sub> concentrations, whereas lowering alkenes, aromatics, CO, and HONO effectively reduced H<sub>2</sub>O<sub>2</sub> pollution, with alkenes exhibiting the most pronounced impact. The <inline-formula><mml:math id="M808" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratio and the positive correlation between daily peak O<sub>3</sub> and NO<sub><italic>z</italic></sub> concentrations indicated that O<sub>3</sub> production predominantly occurred in transitional and NO<sub><italic>x</italic></sub>-limited regimes. To concurrently mitigate H<sub>2</sub>O<sub>2</sub> and O<sub>3</sub> pollution, a dual strategy focusing on VOC control and stringent NO<sub><italic>x</italic></sub> reduction is essential. This approach will be critical to achieve synergistic control of photochemical pollutants in rural areas.</p>
      <p id="d2e8795">Future research should focus on long-term H<sub>2</sub>O<sub>2</sub> monitoring across different environments in the region, refining the parameterization of heterogeneous uptake processes (particularly for HO<sub>2</sub> and H<sub>2</sub>O<sub>2</sub> under varying aerosol compositions) and investigating the impacts of changing <inline-formula><mml:math id="M822" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">VOC</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios on H<sub>2</sub>O<sub>2</sub> chemistry. In addition, further research on the interactions between gas-phase oxidants and aerosol processes will be vital for understanding the complex feedback mechanisms that influence air quality in rural and urban environments.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e8883">The data used in this study are available from the corresponding author upon request (yjmu@rcees.ac.cn).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e8886">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-25-6991-2025-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-25-6991-2025-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e8895">YM designed the experiments. CY performed the H<sub>2</sub>O<sub>2</sub> measurements and analyzed the data. CY wrote the paper with input from PL and CX. All authors contributed to measurements, discussing results, and commenting on the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e8919">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e8925">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e8931">We thank the science teams of the summer campaign for their support.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e8936">This research has been supported by the National Natural Science Foundation of China (grant nos. 42305099 and 42275111).The article processing charges for this open-access  publication were covered by the Max Planck Society.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e8947">This paper was edited by Yugo Kanaya and reviewed by Matthew Johnson and one anonymous referee.</p>
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