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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-26-12715-2026</article-id><title-group><article-title>Chlorine enhances nocturnal heterogeneous uptake of NO<sub>2</sub> in coastal atmosphere under sea-land breeze circulation</article-title><alt-title>Chlorine enhances nocturnal heterogeneous uptake of NO<sub>2</sub></alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Lin</surname><given-names>Ziyi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff4">
          <name><surname>Yong</surname><given-names>Xiuwen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff4">
          <name><surname>Li</surname><given-names>Lingjun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Chen</surname><given-names>Yuping</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Xu</surname><given-names>Lingling</given-names></name>
          <email>Linglingxu@iue.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Ji</surname><given-names>Xiaoting</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Yang</surname><given-names>Chen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Zhang</surname><given-names>Keran</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Zhang</surname><given-names>Feng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Chen</surname><given-names>Ziying</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Chen</surname><given-names>Gaojie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Fan</surname><given-names>Xiaolong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Li</surname><given-names>Mengren</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Chen</surname><given-names>Jinsheng</given-names></name>
          <email>jschen@iue.ac.cn</email>
        <ext-link>https://orcid.org/0000-0002-0285-6094</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>State Key Laboratory of Advanced Environmental Technology, Institute of Urban Environment,  Chinese Academy of Sciences, Xiamen 361021, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Fujian Key Laboratory of Atmospheric Ozone Pollution Prevention, Institute of Urban Environment,  Chinese Academy of Sciences, Xiamen 361021, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>University of Chinese Academy of Sciences, Beijing 100049, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Fujian Agriculture and Forestry University, Fuzhou, 350002, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Lingling Xu (Linglingxu@iue.ac.cn) and Jinsheng Chen (jschen@iue.ac.cn)</corresp></author-notes><pub-date><day>8</day><month>September</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>17</issue>
      <fpage>12715</fpage><lpage>12728</lpage>
      <history>
        <date date-type="received"><day>10</day><month>June</month><year>2026</year></date>
           <date date-type="rev-request"><day>1</day><month>July</month><year>2026</year></date>
           <date date-type="rev-recd"><day>29</day><month>August</month><year>2026</year></date>
           <date date-type="accepted"><day>31</day><month>August</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Ziyi Lin et al.</copyright-statement>
        <copyright-year>2026</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/26/12715/2026/acp-26-12715-2026.html">This article is available from https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e243">Heterogeneous uptake of NO<sub>2</sub> serves as a significant source for reactive nitrogen species, playing an important role in atmospheric chemistry. Laboratory studies have demonstrated that chlorine can promote the heterogeneous NO<sub>2</sub> uptake, yet this effect under real ambient conditions remains poorly elucidated. Based on comprehensive field observations, a machine learning technique, and a multiphase chemical box model in the coastal city of Xiamen, China, this study reveals the enhancement effect of chlorine (Cl) on NO<sub>2</sub> uptake and quantifies the impact of this enhanced uptake on reactive nitrogen species during nocturnal sea-land breeze (SLB) periods. Compared with non-SLB days, nocturnal concentrations of nitrous acid (HONO) and particulate nitrate (NO<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) increased significantly during SLB days, with high mean value of NO<sub>2</sub> uptake rate constant (kNO<sub>2</sub>) reaching 9.70 <inline-formula><mml:math id="M9" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>. Machine learning revealed that chlorine was the most important influencing factor for the enhanced kNO<sub>2</sub>. Incorporating this kNO<sub>2</sub> into the chemical box model substantially resolved the underestimation of HONO concentration and NO<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production under SLB conditions. Notably, nocturnal NO<sub>2</sub> uptake dominated HONO formation (83.9 %), while making a substantial contribution (46.4 %) to nitrate formation. This study highlights the critical role of chlorine-enhanced NO<sub>2</sub> uptake in atmospheric reactive nitrogen cycling and provides valuable insights for nocturnal chemistry in complex coastal environments.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42677128</award-id>
<award-id>U22A20578</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2022YFC3700304</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Chinese Academy of Sciences</funding-source>
<award-id>2023T3013</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="d2e393">Nitrous acid (HONO) and nitrate (NO<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) are key reactive nitrogen species in the atmosphere. HONO, a major source of OH radicals, significantly contributes to the formation of O<sub>3</sub> and secondary aerosols by influencing radical budget (Acker et al., 2006; Alicke et al., 2003). NO<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is an important chemical component of particulate matter (PM), contributing to PM pollution and acid rain (Cao et al., 2022; Qu and Han, 2021). As a crucial source of both HONO and NO<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, the heterogeneous uptake of NO<sub>2</sub> has attracted considerable attention (Xuan et al., 2025; Carter et al., 1982).</p>
      <p id="d2e450">Traditionally, the uptake of NO<sub>2</sub> in bulk solution was considered extremely slow, and thus this process was often negligible (Lee and Schwartz, 1981). However, numerous field observations have indicated that NO<sub>2</sub> uptake plays a significant role in the formation of HONO and NO<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. Previous studies have revealed a strong correlation between NO<sub>2</sub> and HONO after excluding homogeneous formation and primary emissions, suggesting efficient heterogeneous conversion of NO<sub>2</sub> to HONO (Su et al., 2008; Zhang et al., 2024). Studies have also found that incorporating NO<sub>2</sub> uptake mechanisms into models can substantially improve the HONO simulation, especially at night (Zhang et al., 2023, 2024; Xuan et al., 2024; Shi et al., 2020). Using an aerosol-fog sampling system and a box model, Xu et al (2024), found that NO<sub>2</sub> uptake was the primary driver of the rapid increase in NO<inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> during fog events. Currently, the reported reaction rate constant for NO<sub>2</sub> uptake vary widely across different types of surfaces, spanning several orders of magnitude from 10<sup>−7</sup> s<sup>−1</sup> to 10<sup>−5</sup> s<sup>−1</sup> (Zhang et al., 2025b). Multiple factors have been demonstrated to affect the NO<sub>2</sub> uptake rate constant (kNO<sub>2</sub>) in laboratories, including NO<sub>2</sub> concentrations, aerosol particle size, ionic strength, pH, NH<sub>3</sub>, and liquid water content (Liu and Abbatt, 2021; Gen et al., 2024; Zhang et al., 2025a). In the real atmosphere, research during haze events showed that parameterization schemes of kNO<sub>2</sub> considering relative humidity (RH) and NH<sub>3</sub> influences significantly improved the simulation results of heterogeneous HONO formation (Zhang et al., 2023). Long-term observations revealed that changes in aerosol chemical composition could alter aerosol pH, consequently affecting the uptake kinetics of NO<sub>2</sub> to HONO (Zhang et al., 2025b).</p>
      <p id="d2e654">Investigations in coastal areas reported higher NO<sub>2</sub> uptake rates in marine air masses compared to continental ones (Zha et al., 2014; Yang et al., 2021), overall surpassing those measured at continental urban, suburban, and rural sites (Wentzell et al., 2010; Kleffmann et al., 2003; Zhang et al., 2020; Hao et al., 2020; Cui et al., 2018). These findings suggest that heterogeneous NO<sub>2</sub> uptake plays a particularly critical role in the coastal troposphere. Within the marine boundary layer, chloride ions are abundant due to sea spray. Chloride ions exhibit special surface propensity, making them tend to distribute at the air-water interface (Knipping et al., 2000; Piatkowski et al., 2014; Jungwirth and Tobias, 2006). Laboratory studies demonstrated that chloride ions can establish a surface-directed electric field, which attracts atmospheric NO<sub>2</sub> molecules and promotes their further uptake at air-water interface (Wang et al., 2025a; Zhang et al., 2025a). Nevertheless, the influence of chlorine on NO<sub>2</sub> uptake in realistic coastal atmosphere and the consequent impacts on reactive nitrogen cycling remain to be fully elucidated.</p>
      <p id="d2e693">Sea-land breeze (SLB) events occur frequently in coastal urban areas (Chen et al., 2023; Liu et al., 2025; Xie et al., 2023). During SLB periods, the coastal boundary layer experiences intensive interactions between marine and continental air masses, providing a natural laboratory to investigate the effect of sea-salt chloride on NO<sub>2</sub> uptake. In this study, a multi-parameter field observation was conducted in Xiamen, a typical coastal city in China, during the autumn and winter seasons characterized by frequent SLB events (Chen et al., 2023). Based on observations, the characteristics of SLB days were revealed and kNO<sub>2</sub> under both SLB and non-SLB conditions were quantified. Using machine learning method, the significant promoting effect of chlorine on NO<sub>2</sub> uptake during nocturnal SLB periods was demonstrated. Furthermore, the obtained kNO<sub>2</sub> was incorporated into an advanced multiphase box model to evaluate the impact of chlorine-enhanced NO<sub>2</sub> uptake on atmospheric reactive nitrogen cycling. This study highlights the role of previously overlooked chlorine on NO<sub>2</sub> uptake for nocturnal chemistry in coastal atmosphere.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Field measurements and sea-land breeze identification</title>
      <p id="d2e766">Our observations were conducted at the Atmospheric Observation Supersite (24.61° N, 118.06° E) of the Institute of Urban Environment (IUE), Chinese Academy of Sciences in Xiamen, from 18 November 2023 to 6 January 2024. Xiamen is a coastal city in southeastern China. The observation site is located approximately 5 km from the shore and is surrounded by residential, commercial areas and major traffic arteries. Instruments were deployed on the roof of the IUE building at approximately 70 m above ground level. Virtually no high buildings obstructed the path between the site and the coast, making it a typical coastal urban site.</p>
      <p id="d2e769">A suite of atmospheric parameters was observed simultaneously. Ambient HONO was measured online by a water-based long-path absorption photometer (Zhichen Beijing, China) (Xuan et al., 2024). Sulfuric acid (H<sub>2</sub>SO<sub>4</sub>) and HCl were measured using a long time-of-flight chemical ionization mass spectrometer, equipped with a nitrate reagent ion source (Aerodyne Research Inc., USA) (Yang et al., 2023). The chemical composition of PM<sub>2.5</sub> was analyzed using both a MARGA ADI 2080 (Metrohm Applikon, Switzerland) and an ACSM (Aerodyne Research Inc., USA) (Liu et al., 2022; Chen et al., 2022). Particle number size distribution (PNSD) in the range of 2–300 nm was measured by two scanning mobility particle sizers (TSI inc., USA) equipped with a long-DMA (2.5–62 nm) and a nano-DMA (7–300 nm), respectively (Li et al., 2025). Additionally, a range of commercial instruments were employed to monitor trace gases (NO, NO<sub>2</sub>, SO<sub>2</sub>, O<sub>3</sub>, and VOCs), meteorological parameters (ambient temperature, RH, wind-speed, wind-direction and ultraviolet radiation), and photolysis rates (<inline-formula><mml:math id="M58" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>O<sup>1</sup>D, <inline-formula><mml:math id="M60" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>NO<sub>2</sub>, <inline-formula><mml:math id="M62" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>HONO, <inline-formula><mml:math id="M63" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>NO<sub>3</sub>, <inline-formula><mml:math id="M65" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>HCHO and <inline-formula><mml:math id="M66" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>H<sub>2</sub>O<sub>2</sub>) (Liu et al., 2022). Detailed descriptions of instrument operation, species identification, and calibration are provided in Sect. S1 in the Supplement. Hourly BLH data were obtained from the ERA5 reanalysis dataset (Hersbach et al., 2020).</p>
      <p id="d2e915">Sea-land breeze days were identified based on observed wind-speed and wind-direction according to the criteria established in our previous work (Chen et al., 2023). Briefly, the coastline in Xiamen is characterized by a northeast-southwest trend, the sea breeze is blowing from the east-south, and the land breeze is blowing from the west-north-northeast. According to observed wind direction, a natural day could be divided into four periods. Specifically, 01:00–08:00 LT (land breeze period), 13:00–20:00 LT (sea breeze period), and 09:00–12:00 LT and 21:00–24:00 LT (mixed sea-land breeze period). A day was classified as an SLB day if the following three conditions were met: (1) the 24 h mean wind speed was <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> m s<sup>−1</sup>; (2) during the land breeze period, the land breeze persisted for <inline-formula><mml:math id="M71" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4 h and the sea breeze lasted <inline-formula><mml:math id="M72" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 2 h; and (3) during the sea breeze period, sea breeze persisted for <inline-formula><mml:math id="M73" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4 h and the land breeze lasted <inline-formula><mml:math id="M74" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 2 h. As shown in Fig. S1 (light blue areas), a total of 23 SLB days were identified during the observation period. The remaining days were classified as non-SLB days. Figure S2 illustrates that the wind patterns on SLB days differed from those on non-SLB days, characterized by a higher prevalence of southeasterly sea breezes.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Calculation of HONO from heterogeneous formation processes and NO<sub>2</sub> uptake rate</title>
      <p id="d2e987">Due to the absence of agricultural fields near the sampling site and its proximity to major traffic arteries, the primary emission of HONO was attributed to vehicles. Only nighttime data were used in our study, the uncertainties associated with photochemical process, such as NO<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> photolysis were excluded. Therefore, the nighttime corrected HONO (HONO<sub>corr</sub>) is calculated as follows:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M78" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mrow><mml:mi mathvariant="normal">corr</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi mathvariant="normal">vehicle</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></disp-formula>

          where HONO<sub><italic>t</italic></sub> is the observed HONO concentration, <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi mathvariant="normal">vehicle</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the HONO emission from vehicles, and <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the HONO production from homogeneous reactions. <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mrow><mml:mi mathvariant="normal">vehicle</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is calculated as the NO<inline-formula><mml:math id="M83" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> concentration multiplied by the emission factor 0.005 (Zhang et al., 2025b). <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is calculated as follows:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M85" display="block"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>,</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:msub><mml:mo>×</mml:mo><mml:mo>[</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>]</mml:mo><mml:mo>×</mml:mo><mml:mo>[</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>]</mml:mo><mml:mo>×</mml:mo><mml:mn mathvariant="normal">3600</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">s</mml:mi></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (cm<sup>3</sup> molec.<sup>−1</sup> s<sup>−1</sup>) is calculated in the Master Chemical Mechanism 3.3.1 (MCM v3.3.1 <uri>https://mcm.york.ac.uk/MCM/</uri>, last access: 4 September 2026), 3600 s represents the 1 h integration interval, and the concentration of OH radicals is estimated based on the steady-state balance of H<sub>2</sub>SO<sub>4</sub> (Nie et al., 2022). Because H<sub>2</sub>SO<sub>4</sub> is primarily produced by the reaction of SO<sub>2</sub> and OH and is mainly lost via condensation sink (CS) onto particle surfaces, the OH concentration can be estimated as below:

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M95" display="block"><mml:mrow><mml:mo>[</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><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">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>]</mml:mo><mml:mo>×</mml:mo><mml:mi mathvariant="normal">CS</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>×</mml:mo><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is 5 <inline-formula><mml:math id="M97" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−13</sup> cm<sup>3</sup> s<sup>−1</sup> (Seinfeld et al., 1998), and CS (s<sup>−1</sup>) is calculated as follows (Kulmala et al., 2012):

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M102" display="block"><mml:mrow><mml:mi mathvariant="normal">CS</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mi>D</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:msubsup><mml:mo>∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mrow><mml:mi mathvariant="normal">p</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">max</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:msubsup><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi>v</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the diffusion coefficient of H<sub>2</sub>SO<sub>4</sub>, <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the particle diameter derived from the measured PNSD, <inline-formula><mml:math id="M107" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> is the transitional correction factor, and <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the particle number concentration of diameter <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e1575">In line with previous studies (Zhang et al., 2025b, 2020, 2024), the heterogeneous conversion of NO<sub>2</sub> to form HONO<sub>corr</sub> at night is considered a pseudo-first-order reaction. The reaction rate constant (<inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, s<sup>−1</sup>) is calculated based on the conversion of NO<sub>2</sub> during a given period (from <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) as follows:

            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M117" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">kNO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mrow><mml:mi mathvariant="normal">corr</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mrow><mml:mi mathvariant="normal">corr</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M118" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> is the mean concentration of NO<sub>2</sub> between <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e1771">To evaluate the sensitivity of the results to the assumed emission factor, the calculation of HONO<sub>corr</sub> and <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. S3) were calculated using emission factors of 0.005, 0.008 and 0.012 (Xu et al., 2015), while the observational inputs, analysis periods and calculation procedures held constant.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Machine learning technique</title>
      <p id="d2e1806">Random Forest (RF) algorithm, a machine learning technique extensively applied in atmospheric (Yang et al., 2024; Lin et al., 2026b; Zhang et al., 2025b), was employed to elucidate the primary drivers of kNO<sub>2</sub>. The model was built using the “scikit-learn” library (<uri>https://github.com/scikit-learn/scikit-learn/blob/fe2edb3cd/sklearn/ensemble/</uri>, last access: 10 June 2026) in a python environment. Drawing upon previously identified factors influencing kNO<sub>2</sub> (e.g., pH, RH, NH<sub>3</sub>) (Liu and Abbatt, 2021; Gen et al., 2024; Zhang et al., 2025a, 2023) alongside the specific characteristics of the coastal urban environment, we incorporated meteorological parameters (RH and <inline-formula><mml:math id="M127" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>), atmospheric reactive species (proxy of effective particle-phase chloride (Cl<sub>total</sub>), NH<sub>3</sub>, and NO<sub>2</sub>), and heterogeneous-related parameters (pH, SA, and ground surfaces areas) as input variables for the RF model. Cl<sub>total</sub> was defined as the sum of particulate Cl<sup>−</sup> and gaseous HCl. It was used as a depletion-corrected proxy for the particulate Cl<sup>−</sup> burden before acid displacement. During NO<sub>2</sub> uptake, the generated H<sup>+</sup> can protonate particulate Cl<sup>−</sup> and release HCl to the gas phase. Consequently, measured particulate Cl<sup><sup>−</sup></sup> represents the residual fraction after depletion, whereas HCl retains information about part of the chloride transferred from the particle phase. Their sum therefore represents, to some extent, the chloride burden before depletion. To evaluate the suitability of Cl<sub>total</sub> as a proxy for the depletion-corrected Cl<sup>−</sup> burden, two additional RF models were constructed by replacing Cl<sub>total</sub> with either Cl<sup>−</sup> or gaseous HCl. Variance inflation factors (VIFs) were calculated for the predictor set of each RF model. A VIF below 10 was used to indicate the absence of severe multicollinearity. Only nighttime data were used to train the model to eliminate the effects of photochemical processes on kNO<sub>2</sub> quantification, thereby enabling a more precise identification of key drivers. Detailed RF hyperparameter configurations and model evaluation are provided in Sect. S2. In this study, the dominant factors were identified based on RF factor importance, which quantifies the percentage contribution of each variable to kNO<sub>2</sub> (Breiman, 2001; Gregorutti et al., 2017). Furthermore, one-dimensional partial dependence plots (PDPs) were employed to delineate the main effects of individual variables, while bivariate PDPs were utilized to visualize and access the interaction effects between pairs of factors on kNO<sub>2</sub> (Goldstein et al., 2015).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Multiphase chemical box model</title>
      <p id="d2e2012">The multiphase chemical box model was established based on the Framework for 0-D Atmospheric Modeling (F0AM) (Wolfe et al., 2016). As shown in Tables S1 and S2, comprehensive HONO and NO<inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> budgets were incorporated into the F0AM model to simulate the variations of HONO and NO<inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. The ISORROPIA II model (Seinfeld et al., 1998) was integrated into the model to determine aerosol pH, aerosol liquid water content and the partitioning ratio of HNO<sub>3</sub> and NO<inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. Six simulation scenarios were conducted: simulations without heterogeneous NO<sub>2</sub> uptake for (1) SLB and (2) non-SLB days; simulations with NO<sub>2</sub> uptake for (3) SLB and (4) non-SLB days, using the mean kNO<sub>2</sub> derived from SLB days for the SLB simulation and that derived from non-SLB days for the non-SLB simulation, respectively; and two additional sensitivity simulations for SLB days using the (5) 25th and (6) 75th percentiles of the kNO<sub>2</sub> distribution derived from SLB days. The ability of the model to reproduce real atmospheric processes was evaluated by comparing the simulated HONO and NO<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> with observations. Due to the underestimation of total particulate nitrate concentrations measured by instruments, the performance of NO<inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> simulations was evaluated by comparing the trends of the simulated NO<inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production rate with the observed NO<inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentration. In contrast, as HONO predominantly exists in the gas phase, the simulated HONO was evaluated directly against the observed HONO concentrations.</p>
      <p id="d2e2146">As for the model simulation, each simulation was preceded by a 3 d spin-up to allow intermediate species concentrations to stabilize. The mean diurnal pattern of trace gas concentrations, meteorological parameters, and the results from the ISORROPIA II model during SLB days and non-SLB days were used as input data to constrain the box model. Notably, the concentrations of HONO and NO<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> were not constrained by observed values. More details about the model incorporating mechanisms, modules, and simulation settings are provided in Sect. S3 and our previous study (Lin et al., 2026a).</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>Characteristics of atmospheric species during SLB days</title>
      <p id="d2e2178">Figure S1 shows the time series of the observed parameters. Based on the identification criteria detailed in the Methods section, 23 d were classified as SLB days, accounting for 48 % of entire observation period. The diurnal patterns of major observed parameters are summarized in Fig. S4, revealing that the primary differences between the two types of days predominantly emerged at night. Compared to non-SLB days, SLB days exhibited rapid nighttime accumulation of HONO and NO<inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, accompanied by elevated chlorine levels, NO<inline-formula><mml:math id="M159" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> concentrations, and aerosol surface area (SA) concentrations. Additionally, consistent with our previous study, SLB days were characterized by higher temperature and RH at night (Chen et al., 2022). Figure 1 and Table S3 further summarizes the nighttime observational results on SLB and non-SLB days. By definition, SLB days are influenced by persistent sea breezes, which likely enhances the impact of sea-salt aerosols. As shown in Fig. 1a, the Cl<sup>−</sup> concentrations were comparatively higher on SLB days (0.154 <inline-formula><mml:math id="M161" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup>) than on non-SLB days (0.139 <inline-formula><mml:math id="M163" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup>). Specifically, this overall increase (Fig. S5) was primarily driven by elevated levels during the sea breeze (18:00–20:00 LT) and mixed sea-land breeze (21:00–00:00 LT) periods, while concentrations declined during the land breeze (01:00–06:00 LT) period. The elevation pattern of Cl<sup>−</sup> indicates that the more abundant Cl<sup>−</sup> transported by stronger sea breezes on SLB days can persist into the subsequent mixed sea-land breeze periods. Additionally, Fig. S6 shows a moderate positive correlation between Na<sup>+</sup> and Cl<sup>−</sup> on SLB days (<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.67</mml:mn></mml:mrow></mml:math></inline-formula>), compared with a weaker relationship on non-SLB days (<inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.28</mml:mn></mml:mrow></mml:math></inline-formula>). Because sodium chloride (NaCl) is a major component of sea salt, this contrast is consistent with a greater sea-salt influence on Cl<sup>−</sup> on SLB days. As for gaseous chlorine, Fig. 1b shows that the concentration of HCl was significantly higher on SLB days (96.2 ppt) than on non-SLB days (67.5 ppt). This further confirms that, under the influence of sea-salt aerosols on SLB days, chlorine levels are distinctly elevated in the nighttime coastal troposphere.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e2326">Box plots of key observed parameters during nocturnal SLB and non-SLB periods. <bold>(a)</bold> Cl<sup>−</sup>, <bold>(b)</bold> HCl, <bold>(c)</bold> NO<sub>2</sub>, <bold>(d)</bold> HONO, <bold>(e)</bold> NO<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, <bold>(f)</bold> RH, <bold>(g)</bold> SA, and <bold>(h)</bold> ambient temperature (<inline-formula><mml:math id="M175" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>). The box shows the 25th–75th percentiles with whiskers representing <inline-formula><mml:math id="M176" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 standard deviation. The black dot and black line within the box represent the mean and the median. Differences between SLB and non-SLB days were tested using a two-sample <inline-formula><mml:math id="M177" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test. Statistical significances are denoted as <sup>∗</sup>(<inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>), <sup>∗∗</sup>(<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>) and <sup>∗∗∗</sup>(<inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>). For all panels except <bold>(h)</bold>, the number adjacent to the significance symbol denotes the ratio of the mean value on SLB days to that on non-SLB days; in panel <bold>(h)</bold>, it denotes the absolute difference between the means.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026-f01.png"/>

        </fig>

      <p id="d2e2490">Figure 1c indicates that the concentration of NO<sub>2</sub> on SLB days (mean: 28.3 ppb) was significantly higher than that on non-SLB days (23.2 ppb). Within our study area, ship emissions, cross-sea bridge traffic, and road traffic contribute substantial NO<inline-formula><mml:math id="M185" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, and the enhanced local circulation on SLB days can promote NO<sub>2</sub> accumulation (Chen et al., 2023). The mean concentrations of HONO and NO<inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on SLB day were 0.836 ppb and 3.61 <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup>, respectively, which were significantly higher than the corresponding values of 0.497 ppb and 3.13 <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup> on non-SLB days (Fig. 1d, e). To better understand the elevated HONO levels, HONO<sub>corr</sub> concentrations, defined as the observed HONO concentration subtracts contributions from primary emissions and gas-phase production, were calculated to represent the nocturnal HONO produced from heterogeneous conversion. The ratio of HONO<sub>corr</sub> <inline-formula><mml:math id="M194" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<sub>2</sub> was notably higher on SLB days (0.030) than on non-SLB days (0.021), indicating more active heterogeneous conversion of NO<sub>2</sub>to HONO on SLB days. Multiple studies have confirmed that NO<sub>2</sub> uptake is a primary source of nocturnal heterogeneous HONO formation (Zhang et al., 2023, 2022). Here, the higher SA concentrations on SLB days were also conducive to heterogeneous reactions (Fig. 1g). Furthermore, Fig. 2a–b indicate a moderate positive correlation between HONO<sub>corr</sub> and NO<inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, with the correlation coefficient (<inline-formula><mml:math id="M200" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) increasing from 0.56 on non-SLB days to 0.76 on SLB days. The HONO<sub>corr</sub> concentrations under the two conditions overlapped mainly below 1.5 ppb. Within this overlapping range, the correlation on SLB days remained significant (<inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.63</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. S7a) but was close to that on non-SLB days (<inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.56</mml:mn></mml:mrow></mml:math></inline-formula>), indicating that the wider concentration range partly contributed to the higher full-range correlation on SLB days, while the positive relationship between HONO<sub>corr</sub> and NO<inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> persisted within the overlapping range. As shown in Reaction (R1), NO<sub>2</sub> uptake via disproportionation simultaneously produces HONO and HNO<sub>3</sub>, the latter of which is further converted to NO<inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> via gas-particle partitioning. Thus, nocturnal NO<sub>2</sub> uptake is also likely an important contributor to the formations of NO<inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on SLB days. Figure 2c, d show that the full-range correlation between HONO<sub>corr</sub> and gaseous HCl was stronger on SLB days than on non-SLB days (<inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.58</mml:mn></mml:mrow></mml:math></inline-formula> versus 0.16). Within the overlapping HONO<sub>corr</sub> range below 1.5 ppb, the correlation on SLB days decreased to (<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.47</mml:mn></mml:mrow></mml:math></inline-formula>) but remained significant (<inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. S7b) and appreciably higher than that on non-SLB days. This result indicates that the stronger HCl-HONO<sub>corr</sub> relationship during SLB periods cannot be explained solely by the wider HONO<sub>corr</sub> range. The H<sup>+</sup> generated by NO<sub>2</sub> uptake can combine with Cl<sup>−</sup> (Reactions R2–R3). Simultaneously, the aerosol pH in the coastal region of southeastern China was relatively low (approximately 1.92 <inline-formula><mml:math id="M222" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.34 during nocturnal SLB periods), chloride depletion could easily occur, leading to the observed positive correlation between HONO<sub>corr</sub> and HCl. The enhanced chloride depletion can also explain our observations of a significant increase in gaseous HCl but not in Cl<sup>−</sup>concentrations on SLB days. Similarly, the rapid decline in Cl<sup>−</sup> concentration during land breeze periods (Fig. S4) could also be explained by chloride depletion. 

                <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M226" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R6"><mml:mtd><mml:mtext>R1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><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 mathvariant="normal">ad</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="normal">aerosol</mml:mi><mml:mo>/</mml:mo><mml:mtext>ground surface</mml:mtext></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R7"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">NaCl</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:msup><mml:mi mathvariant="normal">Na</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R8"><mml:mtd><mml:mtext>R3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:mi mathvariant="normal">HCl</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><mml:mo>⇋</mml:mo><mml:mi mathvariant="normal">HCl</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e3073">Relationship between HONO<sub>corr</sub> and the important products of heterogeneous chemical processes during nocturnal SLB and non-SLB periods. HONO<sub>corr</sub> denotes the corrected HONO concentration from secondary conversion. The products include <bold>(a, b)</bold> NO<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and <bold>(c, d)</bold> HCl. Blue and red dots represent observations during SLB days and non-SLB days, respectively. Each panel displays the linear regression fits and Pearson correlation coefficients (<inline-formula><mml:math id="M230" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) for the corresponding periods.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Enhanced rate of NO<sub>2</sub> uptake and its influencing factors</title>
      <p id="d2e3144">The values of kNO<sub>2</sub> on SLB days and non-SLB days were derived as Fig. S8. Overall, the average kNO<sub>2</sub> values on SLB days (9.70 <inline-formula><mml:math id="M234" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>) were significantly higher than those on non-SLB days (6.72 <inline-formula><mml:math id="M237" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>), by a factor of approximately 1.44. Across the tested emission factors, the mean HONO<sub>corr</sub> decreased from 0.58 to 0.51 ppb on SLB days, whereas kNO<sub>2</sub> varied by no more than 6.2 %, indicating limited sensitivity of the derived rate constant to the assumed emission factor (Fig. S3). As presented in Table S4, a prolonged increase in the HONO<sub>corr</sub> <inline-formula><mml:math id="M243" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<sub>2</sub> ratio was also observed during 17 of the 23 SLB days (see an example in Fig. S9). In contrast, this phenomenon was virtually absent on non-SLB days, indicating a sustained nocturnal enhancement of kNO<sub>2</sub> during SLB periods. Compared with existing field observations, the kNO<sub>2</sub> on SLB days was broadly consistent with the levels reported under the sea-case scenario in coastal cities of China such as Qingdao (1.25 <inline-formula><mml:math id="M247" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−5</sup> s<sup>−1</sup>) and Hong Kong (8.81 <inline-formula><mml:math id="M250" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>) (Yang et al., 2021; Zha et al., 2014), while it was markedly higher than those values observed in major non-coastal cities including Beijing (7.78 <inline-formula><mml:math id="M253" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−7</sup>–5.75 <inline-formula><mml:math id="M255" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>) (Wang et al., 2017b; Zhang et al., 2020, 2022; Xuan et al., 2023; Jia et al., 2020), Nanjing (1.19 <inline-formula><mml:math id="M258" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> – 2.22 <inline-formula><mml:math id="M260" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>) (Zheng et al., 2020; Liu et al., 2019), and Guangzhou (4.44 <inline-formula><mml:math id="M263" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup>–6.67 <inline-formula><mml:math id="M265" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−6</sup> s<sup>−1</sup>) (Su et al., 2008; Li et al., 2012; Qin et al., 2009). The consistently higher kNO<sub>2</sub> in coastal areas implies that coastal atmospheric environments are likely more conducive to NO<sub>2</sub> uptake.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e3526">Main and interaction effects of influencing factors for <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. Factor importance determined by the random forest <bold>(a)</bold> SLB days and <bold>(b)</bold> non-SLB days. Partial dependence plots for the primary drivers on SLB days: <bold>(c)</bold> Cl<sub>total</sub>, <bold>(d)</bold> RH, and <bold>(e)</bold> SA. Interactions between key factors on SLB days: <bold>(f)</bold> Cl<sub>total</sub> and NO<sub>2</sub>, <bold>(g)</bold> RH and NO<sub>2</sub>, and <bold>(h)</bold> RH and Cl<sub>total</sub>. In panels <bold>(a, b)</bold>, <inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">ground</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denotes ground surface areas calculated by 1 <inline-formula><mml:math id="M277" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> BLH (boundary layer height). In panels <bold>(c–h)</bold>, partial dependence reflects the extent to which the influencing factors affect kNO<sub>2</sub>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026-f03.png"/>

        </fig>

      <p id="d2e3655">A machine learning technique was used to further identify key drivers of the enhanced kNO<sub>2</sub> on SLB days. The RF models using Cl<sub>total</sub> reproduced the calculated kNO<sub>2</sub> well during both SLB and non-SLB periods, with <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values of 0.91 and 0.87, respectively (Fig. S10c, d). Replacing Cl<sub>total</sub> with either Cl<sup>−</sup> or HCl resulted in the respective chlorine variable ranking third after RH and SA (Figs. S10–S11). Particulate Cl<sup>−</sup> represents the residual particle-phase fraction, whereas HCl contains information on the fraction transferred to the gas phase through chloride depletion. Their respective importance therefore suggests that the Cl<sub>total</sub> signal was not determined by either component alone, but reflected their complementary information on the Cl<sup>−</sup> burden before depletion. All VIFs were below 10, indicating no severe multicollinearity between the chlorine metrics and the other predictors (Table S5). Because all three metrics retain part of the chlorine-related information, the RF models showed similar <inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values (0.89–0.91); nevertheless, the Cl<sub>total</sub>-based model had the highest <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and provided a more physically representative description of the association between depletion-corrected particulate chloride and kNO<sub>2</sub>. Notably, the role of Cl<sub>total</sub> and RH diminished substantially on non-SLB days (Fig. 3b), underscoring the profound modulation of these two influencing factors by the SLB circulation. Figure 3c–e further elucidate the specific impacts of these primary drivers on nocturnal kNO<sub>2</sub> under SLB conditions. Specifically, Cl<sub>total</sub> exhibits a positive correlation with kNO<sub>2</sub> (Fig. 3c). This phenomenon is likely attributable to the preferential partitioning of chloride ions at the gas-aqueous interface of aerosols (Zhang et al., 2025a; Shen et al., 2025; Wang et al., 2025a). The surface-bound Cl<sup>−</sup> can attract gaseous NO<sub>2</sub> molecules (Reaction R4) to form interfacial intermediates [Cl-NO<sub>2</sub>]<sup>−</sup>, thereby facilitating the overall NO<sub>2</sub> uptake process. Subsequent interaction analysis was consistent with the mechanisms proposed in laboratory studies (Reactions R4–R5) and suggest that similar processes may operate in the coastal boundary layer. Figure 3f shows that at a fixed NO<sub>2</sub> concentration, elevated chloride levels amplify the positive effect of NO<sub>2</sub> molecules on kNO<sub>2</sub>. This indicates that chloride ions actively promote the heterogeneous uptake of NO<sub>2</sub>, consequently accelerating the kNO<sub>2</sub>. Similar halogen-promoted effect has also been revealed in NO<sub>2</sub>-initiated aqueous-phase oxidation of dissolved SO<sub>2</sub> at the air-aqueous interface and of nitrate photolysis at the aqueous-phase surface (Wang et al., 2025a; Shen et al., 2025). Figure 3d shows a significant positive relationship exists between RH and kNO<sub>2</sub>, suggesting that moist sea breezes effectively supply the water molecules essential for the heterogeneous NO<sub>2</sub> uptake. This finding aligns with previously reported field observations highlighting RH-driven NO<sub>2</sub> uptake (Xuan et al., 2024). Analogous to Cl<sub>total</sub>, the interaction between RH and NO<sub>2</sub> reveals that at a constant NO<sub>2</sub> level, the positive impact of NO<sub>2</sub> on kNO<sub>2</sub> is enhanced under elevated RH. It implies that RH could also facilitate NO<sub>2</sub> uptake by promoting the interaction between NO<sub>2</sub> molecules and heterogeneous interface. Furthermore, Fig. 3h shows a threshold-dependent joint enhancement: kNO<sub>2</sub> increased when RH exceeded approximately 80 % and Cl<sub>total</sub> exceeded approximately 0.5 <inline-formula><mml:math id="M320" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup>, whereas the response was limited when either variable remained below these levels. Elevated RH can increase aerosol liquid water and maintain an aqueous particle phase, while Cl<sup>−</sup> in wetted chloride-containing particles can be preferentially accessible at the air-aqueous interface and enhance NO<sub>2</sub> adsorption and uptake (Zhang et al., 2025a; Wang et al., 2025a). Therefore, the bivariate PDPs response is consistent with high RH providing a favorable aqueous interfacial environment for chloride-associated NO<sub>2</sub> uptake. This interaction may partly explain the higher importance of RH and Cl<sub>total</sub> on SLB days. As a primary factor on both SLB and non-SLB days, SA positively correlates with kNO<sub>2</sub> (Fig. 3e). This indicates that an increase in aerosol surface area concentrations provides effective reaction interfaces for NO<sub>2</sub> uptake process, consistent with most atmospheric heterogeneous processes (Wang et al., 2017a; Ma et al., 2026). Moreover, Fig. S12 shows that on SLB days, concentrations of the major NO<sub>2</sub> uptake products (HONO and NO<inline-formula><mml:math id="M329" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) increased with those key factors including Cl<sub>total</sub>, RH, and SA, providing additional support for the above driving factor analysis. In general, the reasons underlying the enhanced kNO<sub>2</sub> on SLB days help to explain the multi-fold higher kNO<sub>2</sub> observed in coastal areas compared to non-coastal urban areas, highlighting ambient chlorine levels and RH as non-negligible contributors.

                <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M333" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R9"><mml:mtd><mml:mtext>R4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><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:msub><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:mfenced><mml:mi mathvariant="normal">surface</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R10"><mml:mtd><mml:mtext>R5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mfenced close="]" open="["><mml:mrow><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:mfenced><mml:mi mathvariant="normal">surface</mml:mi></mml:msub><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: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 mathvariant="normal">ad</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mo>→</mml:mo><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="normal">HONO</mml:mi><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Enhanced NO<sub>2</sub> uptake promotes the atmospheric reactive nitrogen cycle</title>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e4319">Quantified results from the multiphase chemical box model during SLB periods. <bold>(a)</bold> Diurnal variations in observed and simulated HONO concentrations with and without NO<sub>2</sub> uptake. <bold>(b)</bold> Relationship between the simulated NO<inline-formula><mml:math id="M336" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production rate and observed concentration with and without NO<sub>2</sub> uptake. Diurnal variations of HONO <bold>(c)</bold> and NO<inline-formula><mml:math id="M338" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> budgets <bold>(d)</bold> during SLB days. Diurnal variations of source contributions to <bold>(e)</bold> HONO and <bold>(f)</bold> NO<inline-formula><mml:math id="M339" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. The grey shaded areas represent the nighttime period.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026-f04.png"/>

        </fig>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e4403">Schematic of the chlorine-enhanced heterogeneous uptake of NO<sub>2</sub> during sea-land breeze days in coastal areas. Red arrows, black solid circles, and blue solid circles represent the enhancement of the uptake process, halide ions and water molecular, respectively.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/12715/2026/acp-26-12715-2026-f05.png"/>

        </fig>

      <p id="d2e4422">The above correlations analysis suggests that NO<sub>2</sub> uptake could play an important role in the production of HONO and NO<inline-formula><mml:math id="M342" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on SLB days. Since the HONO and NO<inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation were influenced by multiple meteorological factors and many atmospheric reaction pathways, a multiphase chemical box model was employed to evaluate the role of enhanced NO<sub>2</sub> uptake. As described in Methods, six simulation scenarios were set up. Incorporating NO<sub>2</sub> uptake mechanism substantially improved the simulated diurnal HONO profile during SLB periods: <inline-formula><mml:math id="M346" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> increased from 0.57 to 0.94, while mean absolute error (MAE) and root mean square error (RMSE) decreased from 0.58 to 0.11 ppb and from 0.64 to 0.13 ppb, respectively (Fig. 4a). For NO<inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, incorporating NO<sub>2</sub> uptake increased the mean simulated net NO<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation rate by 2.14 <inline-formula><mml:math id="M350" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−3</sup> h<sup>−1</sup> and strengthened the temporal consistency between the simulated net formation rate and observed concentration, increasing <inline-formula><mml:math id="M353" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> from 0.04 (<inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) to 0.64 (<inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.001</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. 4b). This improvement indicates that the added mechanism better represented the observed temporal variability in NO<inline-formula><mml:math id="M356" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> during SLB periods. Additionally, the NO<sub>2</sub> uptake could robustly explain the enhancements in both atmospheric reactive nitrogen species on SLB days across various kNO<sub>2</sub> quantiles (Fig. S13). In contrast, including NO<sub>2</sub> uptake under non-SLB conditions produced only limited improvements in the simulated HONO concentrations and the temporal covariation between NO<inline-formula><mml:math id="M360" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production rates and observed NO<inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations (Fig. S14). This suggests that NO<sub>2</sub> uptake had less explanatory importance under non-SLB conditions than during SLB periods, consistent with the stronger observed HONO<sub>corr</sub>-NO<inline-formula><mml:math id="M364" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> relationship on SLB days. Moreover, unlike on SLB days (Fig. S9), HONO<sub>corr</sub> <inline-formula><mml:math id="M366" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<sub>2</sub> did not exhibit a sustained nocturnal increase on non-SLB days, which resulted in numerous negative estimates of kNO<sub>2</sub> estimated using Eq. (5). Excluding these negative values likely led to an overestimated mean kNO<sub>2</sub> and, consequently, to the overprediction of HONO and NO<inline-formula><mml:math id="M370" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> under non-SLB conditions.</p>
      <p id="d2e4734">Figure 4c, d illustrate the simulated HONO and NO<inline-formula><mml:math id="M371" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> budgets for the scenarios incorporating NO<sub>2</sub> uptake on SLB days. Despite potential overestimations of non-SLB kNO<sub>2</sub>, the mean NO<sub>2</sub> uptake rate remained significantly higher on SLB days than on non-SLB days, with an average rate of 1.03 ppb h<sup>−1</sup> (Fig. S15). During nighttime, NO<sub>2</sub> uptake accounted for 83.8 % of HONO formation (Fig. 4e). The predominance of NO<sub>2</sub> uptake in nocturnal HONO formation has also been observed during PM pollution episodes in urban areas (Xuan et al., 2024; Jia et al., 2020). However, unlike the chlorine-driven reason identified here, those prior cases were primarily attributed to favorable heterogeneous reaction conditions, such as larger SA concentrations, lower BLH, and higher RH. In addition to NO<sub>2</sub> uptake, primary emissions from vehicle exhaust, coal combustion, and biomass burning are also recognized as major contributors to nighttime HONO in urban areas (Wang et al., 2025b; Zhang et al., 2022). In this study, primary emissions contributed only 15.5 % to nocturnal HONO formation, substantially less than the contribution from NO<sub>2</sub> uptake. As for nighttime NO<inline-formula><mml:math id="M380" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation, many studies had indicated that N<sub>2</sub>O<sub>5</sub> uptake was the dominant pathway in urban areas (Chen et al., 2020; Wang et al., 2018). However, the situation changed under the impact of the enhanced NO<sub>2</sub> uptake. Figure 4f shows that NO<sub>2</sub> uptake contributed 46.4 % to nocturnal NO<inline-formula><mml:math id="M385" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation, which was almost comparable to that of N<sub>2</sub>O<sub>5</sub> uptake (51.6 %). These values were obtained using the BT09 parameterization of <inline-formula><mml:math id="M388" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>N<sub>2</sub>O<sub>5</sub> (Bertram and Thornton, 2009b). Additional simulations using the EJ05 and GRI09 schemes yielded contributions of 47.0 %–47.9 % for NO<sub>2</sub> uptake and 50.0 %–50.9 % for N<sub>2</sub>O<sub>5</sub> uptake (Fig. S16 and Table S6), indicating that their comparable importance was insensitive to the choice of <inline-formula><mml:math id="M394" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>N<sub>2</sub>O<sub>5</sub> parameterization (Evans and Jacob, 2005; Hallquist et al., 2003; Griffiths et al., 2009). While chlorine can also promote the uptake of N<sub>2</sub>O<sub>5</sub> (Bertram and Thornton, 2009a), the relative enhancement in the contribution of NO<sub>2</sub> uptake to nocturnal NO<inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation was more pronounced. This might be related to the suppression of N<sub>2</sub>O<sub>5</sub> uptake caused by increased NO<inline-formula><mml:math id="M403" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> generating directly from NO<sub>2</sub> uptake. The increase in NO<inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> component of aerosol can shift the equilibrium between N<sub>2</sub>O<sub>5</sub> and NO<inline-formula><mml:math id="M408" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> toward N<sub>2</sub>O<sub>5</sub>, thereby reducing the contribution of N<sub>2</sub>O<sub>5</sub> to NO<inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation (Bertram and Thornton, 2009a; Wagner et al., 2013). Additionally, the enhanced NO<sub>2</sub> uptake process also competed for NO<sub>2</sub>, an important precursor of N<sub>2</sub>O<sub>5</sub> formation, especially in the NO<sub>2</sub>-limited regime for N<sub>2</sub>O<sub>5</sub> formation (Lin et al., 2025), ultimately reducing the overall enhancement effect on N<sub>2</sub>O<sub>5</sub> generation. Moreover, this comparable contribution of NO<sub>2</sub> and N<sub>2</sub>O<sub>5</sub> uptake NO<inline-formula><mml:math id="M426" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation was also found during fog events (Xu et al., 2024). Although the observed phenomenon was similar, the dominant drivers differed between fog conditions and coastal SLB periods. The former was primarily attributed to favorable uptake conditions such as abundant aerosol water content and high surface area concentration, whereas the latter was more due to the enhancement effect of chlorine levels and RH on the NO<sub>2</sub> uptake process. Overall, these results reveal the high contribution of NO<sub>2</sub> uptake to HONO and NO<inline-formula><mml:math id="M429" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation during SLB circulation periods, demonstrating that enhanced NO<sub>2</sub> uptake can significantly influence the atmospheric reactive nitrogen cycle in coastal urban areas.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d2e5325">Overall, our observations show that nighttime sea-land breeze period in this coastal urban site were characterized by stronger sea-salt aerosol influence, higher relative humidity, and elevated HONO and nitrate concentrations. Nighttime conditions led to a significant enhancement in the NO<sub>2</sub> uptake rate constant, mainly driven by increased chlorine levels and relative humidity. Multiphase chemical box model simulations further confirmed that this enhanced NO<sub>2</sub> uptake promoted HONO and nitrate formation. Figure 5 illustrates a schematic diagram of chlorine-enhanced heterogeneous uptake of NO<sub>2</sub> during sea-land breeze days. Under the influence of strong sea-land breeze circulation, the continuous influx of sea-salt aerosols transported by moist sea breezes leads to high chlorine levels during the night. Meanwhile, emission from vehicles and ships contribute substantial NO<sub>2</sub>, which accumulates in the coastal atmospheric boundary layer (Wen et al., 2023; Sun et al., 2025). Under these conditions, abundant chloride can effectively increase kNO<sub>2</sub> and promote the NO<sub>2</sub> uptake process, thereby influencing the formation of key atmospheric reactive nitrogen species, HONO and NO<inline-formula><mml:math id="M437" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, as well as broader reactive nitrogen cycling. Notably, other sea-salt halides (Br<sup>−</sup>, I<sup>−</sup>) exhibit similar chemical properties to chlorine and may also contribute to the elevated kNO<sub>2</sub> (Zhang et al., 2025a).</p>
      <p id="d2e5422">Although the observations were limited to one coastal urban site in autumn and winter, chlorine-enhanced NO<sub>2</sub> uptake may also occur in other coastal environments where chloride-rich sea-salt aerosols, high RH, and sufficient NO<sub>2</sub> coexist. Its magnitude is expected to vary seasonally and regionally with sea-salt loading, aerosol water content, aerosol composition, and NO<sub>2</sub> abundance. Therefore, the quantitative contribution derived here should be considered site- and period-specific, and multi-season observations at other coastal sites are needed to assess its broader relevance. Additionally, our study focuses specifically on nocturnal NO<sub>2</sub> uptake to form HONO, given that daytime HONO formation involves more complex factors such as photo-enhanced heterogeneous reactions of NO<sub>2</sub> and nitrate photolysis (Stemmler et al., 2006; Han et al., 2016; Ye et al., 2017; Zhou et al., 2011). Future investigations are warranted to explicitly evaluate the impact of chlorine on daytime NO<sub>2</sub> uptake. Moreover, current air quality models often exhibit considerable biases in simulating secondary pollutants such as O<sub>3</sub> and PM<sub>2.5</sub> over coastal areas (Huang et al., 2025; Ma et al., 2025; Mao et al., 2022). One possible reason is that the influence of chlorine on chemical processes like NO<sub>2</sub> uptake has not yet been adequately considered. Given the dense traffic and substantial NO<sub>2</sub> emission in coastal cities of China, greater attention should be paid to the chlorine-enhanced NO<sub>2</sub> uptake process and its subsequent impact on nocturnal chemistry in coastal urban atmosphere.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d2e5530">Data analysis methods are available on request from Jinsheng Chen (jschen@iue.ac.cn). The dataset can be accessed at Zenodo: <ext-link xlink:href="https://doi.org/10.5281/zenodo.21037074" ext-link-type="DOI">10.5281/zenodo.21037074</ext-link> (Lin et al., 2026c).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5536">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-12715-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-12715-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5545">Z.L. contributed to the conceptualization, investigation, methodology, data curation, software, analysis and writing of the original draft. L.X. and J.C. contributed to the data curation, reviewing and editing the text, supervision, and funding acquisition. X.Y., L.L., C.Y., X.J., Y.C., K.Z., F.Z., Z.C., G.C., X.F., and M.L. provided useful advice and revised the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5551">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="d2e5557">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. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e5563">The authors acknowledge all members of the atmospheric chemistry team at the Institute of Urban Environment.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5568">This work was funded by the National Natural Science Foundation of China (grant nos. 42677128 and U22A20578), the guiding project of seizing the commanding heights of “self-purifying city” (grant no. IUE-CERAE-202402), the National Key Research and Development Program (grant no. 2022YFC3700304), STS Plan Supporting Project of the Chinese Academy of Sciences in Fujian Province (grant no. 2023T3013), and Xiamen Atmospheric Environment Observation and Research Station of Fujian Province.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5574">This paper was edited by Daniel Knopf and reviewed by three anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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