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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-26-8695-2026</article-id><title-group><article-title>Wintertime photochemistry of acyl peroxynitrates and ozone in South Korea during the ASIA-AQ campaign</article-title><alt-title>Wintertime PANs and ozone photochemistry in South Korea</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lee</surname><given-names>Young Ro</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Arterburn</surname><given-names>Linda</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Takeuchi</surname><given-names>Masayuki</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9327-6748</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Tanner</surname><given-names>David J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Roberts</surname><given-names>James M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Roozitalab</surname><given-names>Behrooz</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6987-2171</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff24 aff25">
          <name><surname>Jeong</surname><given-names>Daun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hills</surname><given-names>Alan J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hornbrook</surname><given-names>Rebecca S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6304-6554</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Apel</surname><given-names>Eric C.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9421-818X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Meinardi</surname><given-names>Simone</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Barletta</surname><given-names>Barbara</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Blake</surname><given-names>Nicola J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Blake</surname><given-names>Donald R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Kim</surname><given-names>Saewung</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4847-3272</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7 aff8">
          <name><surname>Wojnowski</surname><given-names>Wojciech</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Piel</surname><given-names>Felix</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7 aff9">
          <name><surname>Wisthaler</surname><given-names>Armin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5050-3018</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff10">
          <name><surname>Ball</surname><given-names>Katherine</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11">
          <name><surname>Crounse</surname><given-names>John D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5443-729X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11 aff12">
          <name><surname>Wennberg</surname><given-names>Paul O.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6126-3854</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13 aff14">
          <name><surname>Miech</surname><given-names>Jason</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0356-5088</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13 aff15">
          <name><surname>Choi</surname><given-names>Yonghoon</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6529-4722</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>DiGangi</surname><given-names>Joshua P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6764-8624</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Diskin</surname><given-names>Glenn S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3617-0269</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff16">
          <name><surname>Sebol</surname><given-names>Abby</given-names></name>
          
        <ext-link>https://orcid.org/0009-0006-7055-4764</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff17 aff23">
          <name><surname>Delaria</surname><given-names>Erin R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff18 aff19">
          <name><surname>Hannun</surname><given-names>Reem A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5195-5307</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff17 aff20">
          <name><surname>St. Clair</surname><given-names>Jason M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9367-5749</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff17">
          <name><surname>Wolfe</surname><given-names>Glenn M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6586-4043</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Cho</surname><given-names>Changmin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5977-2705</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Owen</surname><given-names>Courtney</given-names></name>
          
        <ext-link>https://orcid.org/0009-0003-4921-5678</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Lesko</surname><given-names>Kirk</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Franchin</surname><given-names>Alessandro</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Winstead</surname><given-names>Edward L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Ziemba</surname><given-names>Luke D.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Moore</surname><given-names>Richard</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2911-4469</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Wiggins</surname><given-names>Elizabeth B.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff21 aff22">
          <name><surname>Symonds</surname><given-names>Guy</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff21 aff22">
          <name><surname>Kim</surname><given-names>Dongwook</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2172-3588</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff21 aff22">
          <name><surname>Day</surname><given-names>Douglas A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3213-4233</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff21 aff22">
          <name><surname>Campuzano-Jost</surname><given-names>Pedro</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3930-010X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff21 aff22">
          <name><surname>Jimenez</surname><given-names>Jose L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6203-1847</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Ullmann</surname><given-names>Kirk</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hall</surname><given-names>Samuel R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Crawford</surname><given-names>James H.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Huey</surname><given-names>L. Gregory</given-names></name>
          <email>greg.huey@eas.gatech.edu</email>
        <ext-link>https://orcid.org/0000-0002-0518-7690</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Earth and Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Mechanical Engineering, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Chemical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Atmospheric Chemistry Observations &amp; Modeling Laboratory, NSF National Center for Atmospheric Research, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Chemistry, University of California, Irvine, CA, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of Earth System Science, University of California, Irvine, CA, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Department of Chemistry, University of Oslo, Oslo, Norway</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Department of Analytical Chemistry, Gdańsk University of Technology, Gdańsk, Poland</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Institute for Ion Physics and Applied Physics, University of Innsbruck, Innsbruck, Austria</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>Division of Chemistry and Chemical Engineering, California Institute of Technology, Pasadena, CA, USA</institution>
        </aff>
        <aff id="aff11"><label>11</label><institution>Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA</institution>
        </aff>
        <aff id="aff12"><label>12</label><institution>Division of Engineering and Applied Science, California Institute of Technology, Pasadena, CA, USA</institution>
        </aff>
        <aff id="aff13"><label>13</label><institution>NASA Langley Research Center, Hampton, VA, USA</institution>
        </aff>
        <aff id="aff14"><label>14</label><institution>Oak Ridge Associated Universities, Oak Ridge, TN, USA</institution>
        </aff>
        <aff id="aff15"><label>15</label><institution>Analytical Mechanics Associates, Hampton, VA, USA</institution>
        </aff>
        <aff id="aff16"><label>16</label><institution>Department of Atmospheric and Oceanic Science, University of Maryland, College Park, MD, USA</institution>
        </aff>
        <aff id="aff17"><label>17</label><institution>NASA Goddard Space Flight Center, Greenbelt, MD, USA</institution>
        </aff>
        <aff id="aff18"><label>18</label><institution>NASA Ames Research Center, Moffett Field, CA, USA</institution>
        </aff>
        <aff id="aff19"><label>19</label><institution>Department of Geology and Environmental Science, University of Pittsburgh, Pittsburgh, PA, USA</institution>
        </aff>
        <aff id="aff20"><label>20</label><institution>Goddard Earth Sciences Technology and Research II, University of Maryland, Baltimore, MD, USA</institution>
        </aff>
        <aff id="aff21"><label>21</label><institution>Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff22"><label>22</label><institution>Department of Chemistry, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff23"><label>23</label><institution>Earth System Science Interdisciplinary Center, University of Maryland, College Park, MD, USA</institution>
        </aff>
        <aff id="aff24"><label>a</label><institution>now at: Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff25"><label>b</label><institution>now at: Chemical Sciences Laboratory, National Oceanic and Atmospheric Administration, Boulder, CO, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">L. Gregory Huey (greg.huey@eas.gatech.edu)</corresp></author-notes><pub-date><day>22</day><month>June</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>12</issue>
      <fpage>8695</fpage><lpage>8715</lpage>
      <history>
        <date date-type="received"><day>15</day><month>December</month><year>2025</year></date>
           <date date-type="rev-request"><day>9</day><month>February</month><year>2026</year></date>
           <date date-type="rev-recd"><day>4</day><month>May</month><year>2026</year></date>
           <date date-type="accepted"><day>8</day><month>May</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Young Ro Lee 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/26/8695/2026/acp-26-8695-2026.html">This article is available from https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e674">Wintertime photochemical air pollution in East Asia remains poorly constrained despite its impact on regional air quality. Sources and formation pathways of acyl peroxynitrates (PANs) and ozone (O<sub>3</sub>), key photochemical products, are not well understood, hindering effective mitigation strategies. We investigate PANs and O<sub>3</sub> over South Korea using observations from the ASIA-AQ campaign (February–March 2024). PANs reached 5.5 ppbv, strongly correlating with formaldehyde and particulate matter, indicating active winter photochemistry. Median PANs were higher in the mid-southern peninsula (MS; 990 pptv) and Yellow Sea (1200 pptv) than the Seoul Metropolitan Area (840 pptv). Elevated homologue-to-acetyl peroxynitrate ratios over the MS, with enhanced acryloyl peroxynitrate, acrolein, and ethylene oxide, provided tracers for petrochemical emissions and their impacts. Acetaldehyde contributed 53 %–80 % of PAN production. Ethanol was a major precursor of acetaldehyde (<inline-formula><mml:math id="M3" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 50 %). Strong correlations (<inline-formula><mml:math id="M4" 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> <inline-formula><mml:math id="M5" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.8) of ethanol and halocarbons indicate industrial and solvent sources under-represented in inventories. Formaldehyde and C<sub>2+</sub> aldehydes contributed <inline-formula><mml:math id="M7" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 % to ozone production. Low ozone production efficiency (<inline-formula><mml:math id="M8" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 10) and radical termination dominated by nitric acid and PANs (<inline-formula><mml:math id="M9" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 80 %) indicate VOC-limited conditions. The fractional PANs contribution to NO<sub><italic>x</italic></sub> loss increased with decreasing OH reactivity ratio of NO<sub>2</sub> to aldehydes, suggesting spatial increases in ozone production following NO<sub><italic>x</italic></sub> reductions. These findings demonstrate that a comprehensive understanding of VOC oxidation, particularly oxygenates from industrial sources, is essential for representing winter photochemistry. PANs measurements provide critical constraints on oxidation processes and their implications for emission control.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Aeronautics and Space Administration</funding-source>
<award-id>80NSSC23K0826</award-id>
<award-id>80NSSC21K1704</award-id>
<award-id>80NSSC23K0818</award-id>
<award-id>80NSSC23K0819</award-id>
<award-id>80NSSC21K1704</award-id>
<award-id>80NSSC24K0005</award-id>
<award-id>80NSSC21K1451</award-id>
<award-id>80NSSC23K0828</award-id>
<award-id>80NSSC23K0825</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Science Foundation</funding-source>
<award-id>1852977</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="d2e791">Wintertime photochemical smog remains a persistent air quality challenge in East Asia. Despite reduced solar radiation and temperatures, observations indicate active oxidation of volatile organic compounds (VOCs) and nitrogen oxides (NO<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> NO <inline-formula><mml:math id="M14" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<sub>2</sub>) by atmospheric radicals, especially the hydroxy radical (OH) (Tan et al., 2018; Lu et al., 2019; An et al., 2019). The photooxidation of VOCs and NO<sub><italic>x</italic></sub> (hereafter VOC–NO<sub><italic>x</italic></sub> photochemistry) produces a suite of oxidized VOCs species when sufficient OH levels are sustained by photolysis of nitrous acid (HONO) and ozone (O<sub>3</sub>). Products include aldehydes (Apel et al., 2010), as well as NO<sub><italic>x</italic></sub> oxidation products (NO<sub><italic>z</italic></sub>) such as nitric acid (HNO<sub>3</sub>), acyl peroxynitrates (PANs; RC(O)OONO<sub>2</sub>), alkyl nitrates (ANs; RONO<sub>2</sub>) and particulate nitrate (pNO<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>) (Guo et al., 2014; Tan et al., 2018; Fu et al., 2020; Lee et al., 2021).</p>
      <p id="d2e908">Understanding the atmospheric impacts of VOC–NO<sub><italic>x</italic></sub> photochemistry requires an accurate representation of emissions and oxidation pathways (Bates et al., 2021; von Schneidemesser et al., 2023). A growing body of observations in East Asia points to high VOC levels influenced by complex emissions from combustion (e.g., vehicle exhaust and biomass burning) and non-combustion sources (e.g., volatile chemical products; VCPs), both of which are poorly constrained in inventories (McDonald et al., 2018; Li et al., 2019; Simpson et al., 2020; Travis et al., 2024). Uncertainties in emissions, and consequently in post-emission atmospheric processing, translate to uncertainties in the simulation of photochemical products, including major smog pollutants such as O<sub>3</sub> and fine particulate matter (PM<sub>2.5</sub>). Reducing these uncertainties is therefore critical for predicting the extent of air pollution and formulating mitigation strategies for present environmental issues such as decadal rise in average surface O<sub>3</sub> concentrations, increasing winter–spring O<sub>3</sub> levels, and severe winter haze events (Cooper et al., 2020; Li et al., 2020, 2021; Zhai et al., 2019).</p>
      <p id="d2e956">VOC emission reductions have been proposed to mitigate O<sub>3</sub> and particulate pollution (i.e., VOC-limited chemical regime) in winter–spring East Asia, but the complexity in VOC emissions and chemical evolution complicate identification of which VOCs contribute to photochemistry and pollutant formation (Li et al., 2021; Schroeder et al., 2020; Nault et al., 2018).</p>
      <p id="d2e968">An experimental approach is to examine observed secondary products of VOC oxidation (e.g., Ryerson et al., 2003). Among these, formed via VOC–NO<sub><italic>x</italic></sub> photochemistry, PANs are effective tracers of VOC oxidation and often a major component of NO<sub><italic>z</italic></sub> (Roberts, 2007). Recent field observations across East Asia, including China and South Korea, underscore the diagnostic utility of PANs as tracers of VOC–NO<sub><italic>x</italic></sub> photochemistry. For example, in China, wintertime acetyl peroxynitrate (PAN), the simplest and most abundant member of PANs, strongly correlates with PM<sub>2.5</sub>, often more so than with O<sub>3</sub>, partly due to titration of O<sub>3</sub> by elevated NO<sub><italic>x</italic></sub> (Qiu et al., 2019, 2020; Lu et al., 2019; Xu et al., 2021). Here, PAN serves as a more useful indicator of photochemistry than O<sub>3</sub> and provides observational evidence for the contribution of atmospheric chemistry to particulate pollution. Similarly, in the Seoul Metropolitan Area (SMA), home to 50 % of South Korea's population, springtime production of O<sub>3</sub> was found to be dominated by local oxidation of small (<inline-formula><mml:math id="M40" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> C<sub>5</sub>) anthropogenic alkenes and aromatics (<inline-formula><mml:math id="M42" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> C<sub>7</sub>) such as toluene and xylenes from traffic and solvent emissions. Organic aerosol (OA) production was driven by oxidation of aromatics and other VOCs with semi- and intermediate volatility (SVOCs and IVOCs) (Simpson et al., 2020; Schroeder et al., 2020; Nault et al., 2018). The dominant role of secondary formation is further demonstrated by the co-occurrence of OA and O<sub>3</sub> with short-lived photochemical tracers including formaldehyde (CH<sub>2</sub>O) and PAN (Schroeder et al., 2020; Nault et al., 2018).</p>
      <p id="d2e1105">More recently, an evaluation of Korea-United States Air Quality (KORUS-AQ) observations by Nault et al. (2024) showed that approximately half of the species comprising PANs predicted by near-explicit box model simulations were unmeasured despite their importance in O<sub>3</sub> and radical chemistry in the SMA. To reconcile the PANs budget, GEOS-Chem transport model simulations required increased VOC emissions from non-combustion sources, such as VCPs, and revised chemical mechanisms (Bey et al., 2001; Travis et al., 2024). Consistent with this, in New York City (NYC), PAN formation in WRF-Chem simulations was highly sensitive to oxygenated VCPs such as ethanol and isopropanol whose inclusion increased predicted PAN by 15 %–20 % (Grell et al., 2005; Coggon et al., 2021). These studies demonstrated difficulties in constraining both the magnitude and speciation of PANs, and their utility as VOC–NO<sub><italic>x</italic></sub> photochemical tracers in polluted urban environments with complex VOCs.</p>
      <p id="d2e1126">A large data set of PANs observations has been accumulated globally, spanning regions from remote hemispheric backgrounds to heavy pollution (Roberts, 2007; Fischer et al., 2014; Lee et al., 2025). However, such observations in East Asia, including South Korea, remain scarce. To address this gap, in situ airborne observations onboard the NASA DC-8 were conducted over South Korea in February and March 2024 as part of the Airborne Satellite Investigation of Asian Air Quality (ASIA-AQ) campaign. A key objective was to assess South Korean air quality in winter and build upon KORUS-AQ findings (Crawford et al., 2021). The ASIA-AQ instrument suite includes measurements of PANs, their oxygenated VOC (OVOC) precursors (e.g., aldehydes, alcohols, and esters), and aromatic oxidation products. To our knowledge, no prior studies have provided such a comprehensive measurement of those compounds. Therefore, the ASIA-AQ observations offer a unique opportunity to characterize wintertime photochemical processing in East Asia.</p>
      <p id="d2e1129">This work investigates wintertime photochemistry in South Korea, focusing on the chemistry and distribution of PANs. We report measurements of PANs, including rarely observed homologues such as acryloyl peroxynitrate (APAN) and benzoyl peroxynitrate (PBzN). Combining kinetic calculations and 0-D box modeling, highly constrained by observations, we examine key factors controlling PAN and O<sub>3</sub> production. For this examination, we focus on diagnosing instantaneous PAN and O<sub>3</sub> production using observed precursors across different regions in South Korea. To systematically represent spatial and pollution-dependent variations in photochemistry, we analyze the fractional contribution of NO<sub><italic>x</italic></sub> loss pathways to either PANs or HNO<sub>3</sub> formation as well as ozone production efficiency (OPE) as a function of the probability of OH reacting with NO<sub>2</sub> or aldehydes.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods and data analysis</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Brief overview of the ASIA-AQ campaign</title>
      <p id="d2e1192">The ASIA-AQ campaign was conducted over the Philippines, South Korea, Thailand, and Taiwan from 6 February to 27 March 2024. Airborne measurements were primarily obtained from the NASA DC-8 and G-III, complemented by satellite, ground-based, and additional aircraft observations from domestic collaborators (ASIA-AQ, 2023). This work focuses on five DC-8 research flights (RFs) over South Korea and the Yellow Sea from 17 February to 11 March, during cold conditions (median temperature of 4 °C at altitudes below 500 m).</p>
      <p id="d2e1195">During ASIA-AQ, DC-8 flights departed from Osan Air Base and followed consistent transects at altitudes ranging from <inline-formula><mml:math id="M53" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 200 m to 2.5 km. The near-constant flight paths were performed to obtain consistent and representative sampling of the South Korean atmosphere. Each RF included 4–6 low approaches at Seoul and Gimpo Airports to capture vertical distributions over urban areas, totaling 27 low approaches over the SMA during the campaign. To assess regional air pollution, the DC-8 flights included sampling over relatively remote regions such as the Yellow Sea and the mid- and southern regions of the peninsula. Measurement locations and conditions during the campaign are shown in Fig. S1 in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>TD-CIMS measurements</title>
      <p id="d2e1213">A comprehensive suite of chemical, optical, and meteorological measurements was obtained aboard the DC-8 aircraft during the ASIA-AQ campaign. Table S1 summarizes the measurements used in this study, including instrumental techniques, uncertainties, and references. Of the measured compounds, this study focuses primarily on PANs measured by the Georgia Tech Thermal Dissociation-Chemical Ionization Mass Spectrometer (GT TD-CIMS) with a Time-of-Flight (ToF) mass analyzer (TofWerk/Aerodyne). Building on established methods (Slusher et al., 2004; Zheng et al., 2011; Lee et al., 2020), this deployment incorporated several key modifications, as shown in Fig. S2. A major improvement was the replacement of the quadrupole mass filter with a ToF analyzer (resolving power <inline-formula><mml:math id="M54" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5000 m <inline-formula><mml:math id="M55" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M56" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> m), which enhanced mass resolution and thereby improved the selective measurement of PAN homologues. As in our prior DC-8 deployments, quantification of PANs was further supported by the continuous addition of isotopically labeled PAN (C<sup>13</sup>H<sub>3</sub>C<sup>13</sup>(O)OONO<sub>2</sub>) for calibrations and periodic NO addition to react away peroxyacyl radicals in the thermal dissociation (TD) region for background determination. In addition, post-campaign laboratory experiments were carried out to constrain sensitivities of PAN homologues relative to that of PAN, following the method described in Roberts et al. (2022).</p>
      <p id="d2e1274">An additional modification to the GT TD-CIMS was the use of an automated variable orifice upstream of the heated Teflon inlet (i.e., TD region), replacing the in-line pressure controller used in the KORUS-AQ and Atmospheric Tomography (ATom) campaigns (Fig. S2). The variable orifice, previously applied to regulate flow tube pressure across altitude ranges (Chen et al., 2016), maintained constant pressure in both the TD and Ion Molecule Reaction (IMR) regions during ASIA-AQ. This also reduced interactions with metal surfaces compared to the previous inlet system (Lee et al., 2020). While wall losses for most PANs are minimal, this configuration is expected to improve the measurements of PBzN for which potential loss on Teflon inlet wall has been reported (Zheng et al., 2011; Liu et al., 2019). It should be noted that such potential effects were further resolved by applying homologue-specific sensitivities during data analysis.</p>
      <p id="d2e1278">Finally, the CIMS instrument utilized a vacuum ultraviolet (VUV) lamp (Heraeus, PKS 106) as an ion source (Ji et al., 2020), eliminating the safety and regulatory constraints associated with polonium-210 sources (1.5–20 mCi) used in previous flight instruments (e.g., Lee et al., 2020, 2022). For a campaign such as ASIA-AQ, with the extended duration and multiple deployment sites, the VUV lamp reduces logistical demand in contrast to radioactive sources that require regulatory oversight (Lee et al., 2020).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>VOCs measurements and data analysis</title>
      <p id="d2e1289">This study includes kinetic calculations and 0-D box modeling, both highly constrained by observations, including an extensive suite of hydrocarbons and OVOC measurements, on the NASA DC-8. During ASIA-AQ, VOCs were measured by the NSF NCAR Trace Organic Gas Analyzer with a time-of-flight mass spectrometer (TOGA-TOF), the University of California, Irvine Whole Air Sampler (WAS), and the University of Oslo FUSION proton transfer-reaction time-of-flight mass spectrometer (PTR-ToF-MS; Reinecke et al., 2023). Among these, the TOGA-TOF, which utilizes fast in situ gas chromatography coupled with a high-resolution time-of-flight electron impact mass spectrometer served as the primary dataset (Apel et al., 2010; Hornbrook et al., 2016). Analyses incorporating VOC observations utilized data merged to the TOGA sampling interval (35 s of integrated sampling every 2 min). For analyses using only PANs data (Sect. 3.1), measurements were merged to a 1 s time base. All DC-8 measurement data are publicly available through the NASA data archive (<ext-link xlink:href="https://doi.org/10.5067/SUBORBITAL/ASIA-AQ/DATA001" ext-link-type="DOI">10.5067/SUBORBITAL/ASIA-AQ/DATA001</ext-link>).</p>
      <p id="d2e1295">To assess regional variability in atmospheric composition and photochemistry, the time-averaged data were categorized into three regions based on geographic boundaries: Seoul Metropolitan Area (SMA), Mid and South (MS), and Yellow Sea (YS) (Fig. S3a). In addition, we incorporated 1 km <inline-formula><mml:math id="M61" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1 km gridded data from the Statistical Geographic Information Service (SGIS) of the Korean government (<uri>https://sgis.kostat.go.kr</uri>, last access: 4 May 2026) to complement chemical observations with spatially resolved information relevant to anthropogenic activities. The statistical data includes industrial facilities, classified by sector (Fig. S3b–c), as well as population density. For this analysis, industrial sectors included manufacturing, power generation, and utilities/management. The population and industrial facility densities were averaged within a 5 km radius of each DC-8 measurement point, denoted as PD<sub>5 km</sub> and ID<sub>5 km</sub>, respectively, and used to support qualitative interpretation of pollutant distribution using chemical tracer measurements.</p>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Kinetic calculations of instantaneous rates and reactivity</title>
      <p id="d2e1333">A series of kinetic calculations were conducted to estimate instantaneous production rates of O<sub>3</sub> and reactive nitrogen (NO<sub><italic>y</italic></sub>), including nitric acid (HNO<sub>3</sub>) and PANs, based on observed concentrations, photolysis frequencies, and established kinetic parameters. These estimates were integrated with observations and box model simulations to investigate O<sub>3</sub> and NO<sub><italic>z</italic></sub> formation during the campaign.</p>
      <p id="d2e1381">As daytime oxidation of atmospheric species is primarily initiated by reaction with OH, instantaneous production rates, considered here, depend on OH reactivity. In this work, the OH reactivity of an individual compound <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) is defined as the product of its observed concentrations and its corresponding OH rate coefficients (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). The summed OH reactivity (<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi>X</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is then obtained by adding the individual contributions (Eq. 1).

              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M73" display="block"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi>X</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">where</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>[</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:math></disp-formula>

            The instantaneous production rate of ozone (<inline-formula><mml:math id="M74" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>)) can be approximated by the rate at which peroxy radicals (HO<sub>2</sub> and RO<sub>2</sub>) react with NO (Eq. 2) and was used to calculate modeled <inline-formula><mml:math id="M78" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>). Given the absence of peroxy radical measurements during ASIA-AQ, we estimate <inline-formula><mml:math id="M80" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) using Eq. (3), following Rosen et al. (2004) and Perring et al. (2013), which represent ozone production as a function of <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">VOC</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, OH concentration, speciated radical yields (<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and alkyl nitrate branching ratios (<inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), as summarized in Table S2. A constant OH concentration of 2 <inline-formula><mml:math id="M85" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup> was used for the base case to generalize the analysis and enable application across a broader observational dataset than model simulations that require fully synchronized inputs. Modeled OH concentrations were used when comparing kinetic calculations to model simulations.

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M88" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</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:mrow><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>≅</mml:mo><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:msub><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi>i</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:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mo movablelimits="false">∑</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mrow><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:mrow></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:mo>[</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>]</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>≅</mml:mo><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>[</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>]</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">VOC</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            Similarly, production rates of HNO<sub>3</sub> (<inline-formula><mml:math id="M90" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(HNO<sub>3</sub>)) and PANs (<inline-formula><mml:math id="M92" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs)) are estimated using Eqs. (4)–(5), respectively. In Eq. (5), <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">PAN</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents the fraction of acyl peroxy radicals (PAs) reacting with NO<sub>2</sub> relative to the total loss pathways, and <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mrow><mml:mi mathvariant="normal">Hydrogen</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">Abstraction</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the branching ratio for hydrogen abstraction of the corresponding aldehydes. The OH reactivity from aldehyde precursors of PANs (<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is calculated using observed mixing ratios of acetaldehyde, propanal, butanals, acrolein and benzaldehyde. The photolytic loss of OVOC, <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">OVOC</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>, is the product of measured photolysis frequencies and OVOCs concentrations (acetone, methyl ethyl ketone, and biacetyl), weighted by the photolytic yield of acetyl peroxy (PA) radical (<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">PA</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), generally unity except for biacetyl, which yields two PA radicals. Based on the rate estimates, ozone production efficiency (OPE) is approximated as the ratio of <inline-formula><mml:math id="M99" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) to the sum of HNO<sub>3</sub> and PANs production rates (Eq. 6).

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M102" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>P</mml:mi><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:mo>=</mml:mo><mml:mo>[</mml:mo><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>]</mml:mo><mml:msub><mml:mi>R</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:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</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 left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi>P</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">PAs</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>≅</mml:mo><mml:mi mathvariant="normal">PANs</mml:mi></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mo>∑</mml:mo><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mrow><mml:mi mathvariant="normal">Hydrogen</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">Abstraction</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mfenced close="]" open="["><mml:mi mathvariant="normal">OH</mml:mi></mml:mfenced><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">ALD</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">PA</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi>j</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">OVOC</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>]</mml:mo><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd><mml:mtext>6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">where</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">PAN</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">PA</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:mrow></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:mrow><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">PA</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:mrow></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:mo>+</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">PA</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:msub><mml:mo>[</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">OPE</mml:mi><mml:mo>=</mml:mo><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mfenced open="/" close=""><mml:mrow><mml:mi>P</mml:mi><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:mo>+</mml:mo><mml:mi>P</mml:mi><mml:mfenced close=")" open="("><mml:mi mathvariant="normal">PANs</mml:mi></mml:mfenced></mml:mrow></mml:mfenced></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.S2.SS3.SSS2">
  <label>2.3.2</label><title>Steady state 0-D box modeling</title>
      <p id="d2e2218">We used a zero-dimensional box model (F0AM; The Framework for 0-D Atmospheric Modeling; Wolfe et al., 2016) to simulate production rates of O<sub>3</sub> and NO<sub><italic>z</italic></sub>. The model was constrained using synchronous measurements of trace gases and meteorological parameters that were averaged to the TOGA sampling interval (TOGA-merge). A complete list of observational constraints is provided in Table S3. To interpret airborne measurements under rapidly changing spatial and temporal conditions, we used the flight steady-state method (Crawford et al., 1999). This approach is widely used in airborne studies and is particularly suited for estimating concentrations of short-lived species (e.g., radicals) and diagnosing instantaneous photochemistry (Olson et al., 2006; Schroeder et al., 2020). In this work, each model step is treated as an independent steady-state run incorporating the near-explicit chemical mechanism (the Master Chemical Mechanism (MCM) v3.3.1; Jenkin et al., 2015) to iterate through full diurnal cycles until unconstrained species (e.g., radicals) converged within 1 % (e.g., Nault et al., 2024). A similar approach has been previously applied to investigate radical chemistry, ozone production and reactive nitrogen processing for KORUS-AQ (Brune et al., 2022; Schroeder et al., 2020; Nault et al., 2024). To account for differences between observed and modeled <inline-formula><mml:math id="M105" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> values, we apply a scaling factor to all <inline-formula><mml:math id="M106" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> values based on the averaged ratio of measured to MCM-parameterized <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi>j</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> and <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. In addition, a first-order loss is applied to all species, equivalent to a 12 h lifetime, following Brune et al. (2022) and Nault et al. (2024). However, due to the short atmospheric lifetime of the species considered here and the use of highly constrained input for instantaneous rate calculations, this loss term has a minimal influence (<inline-formula><mml:math id="M109" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M110" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5 % variability for a factor of two change in loss rate) on the results in this study (Fig. S4).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Observations of PANs over the Korean Peninsula and the Yellow Sea</title>
      <p id="d2e2308">High PANs levels were observed across the Korean Peninsula (mean <inline-formula><mml:math id="M111" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M112" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>; 1.06 <inline-formula><mml:math id="M113" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.64 ppbv) and the YS (1.43 <inline-formula><mml:math id="M114" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.95 ppbv) during ASIA-AQ, with the maximum value (5.5 ppbv) measured in Gyeonggi Province within the SMA. These elevated PANs levels were accompanied by high levels of CH<sub>2</sub>O, odd oxygen (O<sub><italic>x</italic></sub>; approximated as O<inline-formula><mml:math id="M117" 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>NO<sub>2</sub>), OA and aerosol concentrations (number, volume, and surface area) with generally <inline-formula><mml:math id="M119" 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> <inline-formula><mml:math id="M120" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5 across the selected regions (Fig. S5), indicating a strong photochemical relevance.</p>
      <p id="d2e2397">Correlations of PANs with aerosols were particularly strong during ASIA-AQ, exceeding those with O<sub><italic>x</italic></sub>, similar to wintertime China (Qiu et al., 2019, 2020; Lu et al., 2019; Xu et al., 2021). During ASIA-AQ aerosol concentrations were measured by multiple instruments targeting different particle size ranges, providing additional constraints on these relationships. As shown in Fig. S5, aerosol concentrations (i.e., number, volume, and surface area) were highly correlated with PANs (<inline-formula><mml:math id="M122" 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> up to <inline-formula><mml:math id="M123" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.9) with the strongest relationships for fine particles (<inline-formula><mml:math id="M124" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 1 <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) measured by an Ultra-High Sensitivity Aerosol Spectrometer (UHSAS). These observations suggest that PANs broadly capture the impacts of active VOC–NO<sub><italic>x</italic></sub> photochemistry on both gaseous and particulate pollution under cold conditions in East Asia, consistent with previous observations of the region (Lu et al., 2019; Xu et al., 2021; Lee et al., 2021).</p>
      <p id="d2e2454">Significant heterogeneity in both concentration and speciation of PANs demonstrated the influence of complex emission sources and photochemical processing. For example, the observed PANs distribution reflected the regional extent of photochemical pollution, extending well beyond source regions, and impacting downwind areas. Despite spanning more remote areas, median mixing ratios of PANs in the MS (990 pptv) and YS (1200 pptv) were higher than those in the SMA (840 pptv). This contrasts with the much higher population and industrial densities (e.g., <inline-formula><mml:math id="M127" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 40 times greater median PD<sub>5 km</sub> and ID<sub>5 km</sub>) in the SMA as well as more abundant precursor emissions. Figure 1a shows the spatial distribution, with the DC-8 flight tracks colored by PANs mixing ratios overlaid on a population density map (top panel), and longitudinal PANs quartiles and median PD<sub>5 km</sub> in 0.02° bins (bottom panel). The longitudinal medians frequently exceeding 1 ppbv, including in remote areas, were particularly notable over the MS and YS. The longitudinal pattern of the MS showed increasing concentrations near the western and eastern boundaries, in close proximity to major industrial facilities including Banweol Industrial Complex (BIC), Daesan petrochemical complex (DPCC) and Gumi Industrial Complex (GIC), suggesting their potential contributions to pollutant distributions in the MS. In addition to South Korean sources, biomass burning plumes from China contributed to marked increases in PANs over the YS, as evidenced by concurrent enhancements of hydrogen cyanide (HCN) and acetonitrile (CH<sub>3</sub>CN) (Figs. S5 and S6). These observations are consistent with high PAN episodes in Seoul (<inline-formula><mml:math id="M132" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 3 ppbv in 2019) (Savic et al., 2024) and at Gosan Climate Observatory (up to 2.4 ppbv), located near the southern YS (Han et al., 2017), attributed to long-range transport of biomass burning emissions from China. Consequently, the observed PANs distribution during ASIA-AQ is impacted by diverse sources including urban, industrial, and biomass burning emissions.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e2511"><bold>(a)</bold> (Top) Map of South Korea DC-8 flight tracks colored by PANs mixing ratios, overlaid on a 1 km<sup>2</sup> population density map. (Bottom) Longitudinal dependence of median PANs over the Yellow Sea (YS, red), Seoul Metropolitan Area (SMA, orange) and Mid and South (MS, blue) in 0.02° bins. The dashed lines represent longitudinal 25th and 75th percentiles of PANs. The shaded areas indicate median PD<sub>5 km</sub> of the selected regions in 0.02° bins. <bold>(b)</bold> Scatter plots of median PAN homologues versus median PAN (i.e., homologue <inline-formula><mml:math id="M135" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios), binned in intervals of 500 pptv PAN, with error bars denoting the 25th and 75th percentiles of the homologues in each bin. The red, orange, and blue solid lines indicate linear regression slopes for the 1 s merged data obtained over the YS, SMA and MS, respectively, during ASIA-AQ. Recent observations from Southern California (beige), the Southeastern United States (green), Colorado Front Range (pink), Yellow River Delta in China (light brown), and SMA (gray) and petrochemical plumes (black) from KORUS-AQ are also shown as dashed lines and shaded sectors.</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f01.png"/>

      </fig>

      <p id="d2e2550">The speciation of PANs during ASIA-AQ exhibited heterogeneity as well. As shown in Fig. 1b, the relative abundance of PAN and its homologues (i.e., homologue <inline-formula><mml:math id="M136" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios), derived from linear regression slopes, was at the upper end of previous reported values. These ratios exceeded those from recent US observations from biogenic (Toma et al., 2019), industrial (Lindaas et al., 2019) and urban (Southern California during Fire Influence on Regional to Global Environments Experiment – Air Quality, FIREX-AQ 2019) regions, as well as during KORUS-AQ, and were most comparable to our measurements at a polluted remote site in China (Lee et al., 2021). Efficient thermal decomposition favors higher homologue <inline-formula><mml:math id="M137" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios due to the <inline-formula><mml:math id="M138" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15 %–25 % faster thermolysis of PAN than its homologues (Kabir et al., 2014; Gomez et al., 2025). Consequently, the colder ASIA-AQ conditions in South Korea relative to the US studies are unlikely to explain the higher ratios. Although not well constrained by experiments, potential slower OH oxidation of PAN compared to most larger homologues does not account for the observed homologue ratios and likely has a minor impact. However, it certainly contributes to a shorter lifetime of APAN (a few hours with <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow><mml:mi mathvariant="normal">APAN</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M140" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1 to 2 <inline-formula><mml:math id="M141" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−11</sup> cm<sup>3</sup> molec.<sup>−1</sup> s<sup>−1</sup> and [OH] <inline-formula><mml:math id="M146" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M147" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup>) which depresses APAN <inline-formula><mml:math id="M150" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios in cold environments (Orlando and Tyndall, 2002). Instead, the elevated ratios point to a significant degree of photochemical pollution driven by photooxidation of complicated VOC mixtures, rarely observed outside East Asia in recent years.</p>
      <p id="d2e2693">In addition, the variance in data points and the homologue ratios in Fig. 1b also point toward varying source contributions, with greater variability associated with homologues from more specific sources. Propionyl peroxynitrate (PPN) and the sum of iso- and n-butyl peroxynitrate (PBN), formed from a broad range of anthropogenic alkanes and alkenes, showed relatively consistent ratios, whereas APAN and PBzN, formed from more reactive and source-specific alkenes and their product aldehydes (e.g., 1,3-butadiene and acrolein for APAN, and styrene and benzaldehyde for PBzN), showed considerable variability. For example, PBzN/PAN ratios were lower over the YS compared to over the peninsula, consistent with significantly reduced aromatic concentrations (Fig. S6a). In contrast, this pattern is not observed for APAN <inline-formula><mml:math id="M151" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios, despite the short lifetime of APAN due to removal by OH, because biomass burning is also a major source of APAN (Fig. S6b; Roberts et al., 2022).</p>
      <p id="d2e2703">Among all regions, the MS exhibited the highest homologue <inline-formula><mml:math id="M152" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios, with the most pronounced enhancements for the ratios of APAN and PBzN. A consistent increase in the ratios for APAN and PBzN was observed in the MS with their concentrations reaching hundreds of pptv and the strongest regional correlation (<inline-formula><mml:math id="M153" 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> <inline-formula><mml:math id="M154" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.5) between the two species. Based on our previous field measurements in various environments, such elevated levels and ratios have only been observed in regions with dominant contributions of petrochemical and biomass burning emissions. While PANs observations are widely used to assess VOC–NO<sub><italic>x</italic></sub> photochemistry over the past decades, their application to APAN and PBzN remain scarce, particularly in East Asia. Given their clear enhancements, limited precursor sources and low background concentrations, APAN and PBzN can provide valuable insights into complex photochemical processes. Therefore, in the following section, we present a case study using these tracers to investigate regional-scale pollution in the MS.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Investigation of MS pollution using APAN and PBzN</title>
      <p id="d2e2747">Although significant pollution over the MS was observed during ASIA-AQ, this region is understudied. For this purpose, we utilize APAN as a primary tracer, complemented by PBzN as an additional proxy for anthropogenic aromatic sources. APAN is particularly useful due to its short atmospheric lifetime and substantial enhancements over low background levels observed in this region. Figure 2 presents spatial distributions of APAN and APAN <inline-formula><mml:math id="M156" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios, along with wind rose plots in 0.5° longitudinal bins and back trajectories (HYSPLIT; Stein et al., 2015) initiated at the 10 largest APAN <inline-formula><mml:math id="M157" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN values. Elevated APAN concentrations and APAN <inline-formula><mml:math id="M158" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios up to 343 pptv and 0.2, respectively, were consistently associated with west and northwesterly winds (270°–315°), indicating transport from west coast industrial sources. Although median APAN levels were low (24 pptv), upper-end values were elevated and spatially extensive. Longitudinal profiles in Fig. 3a show APAN increasing near the eastern and western boundaries, consistent with the PANs distribution in Fig. 1a. In addition to the major influence of industrial sources from the northwest, the southeastern enhancements may also reflect secondary contribution from sources to the south and east, including the Gumi Industrial Complex, associated with variable winds.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e2773">APAN and APAN <inline-formula><mml:math id="M159" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios over the MS illustrated as marker color and size, respectively, overlaid on a 1 km<sup>2</sup> industrial facility density map, with wind rose plots for three 0.5° longitudinal bins colored by APAN mixing ratios. The black lines with solid circles indicate back trajectories initiated at the 10 largest APAN <inline-formula><mml:math id="M161" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN values. The cyan, yellow, and magenta triangles indicate the locations of Banweol Industrial, Daesan Petrochemical, and Gumi Industrial Complexes, respectively.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f02.png"/>

        </fig>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e2807"><bold>(a)</bold> APAN, acrolein (ACR) and EtO (ethylene oxide) as a function of longitude over the MS. The solid red line and shaded area indicate longitudinal 50th, 25th, and 75th percentiles, respectively, of APAN in 0.02° bins, and the dashed red lines are the longitudinal 1st and 99th percentiles. The orange and blue markers represent ACR and EtO mixing ratios. The inset shows correlation of ACR with APAN (red markers with black linear fit line) and with EtO (yellow markers with beige linear fit line). <bold>(b)</bold> Scatter plots of PBzN <inline-formula><mml:math id="M162" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> benzaldehyde (BENZAL) versus APAN <inline-formula><mml:math id="M163" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> ACR over the MS. The markers are colored and sized by OH exposure, defined as the product of OH concentration and time over the photochemical age of an air amass, and O<sub>3</sub> mixing ratios, respectively.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f03.png"/>

        </fig>

      <p id="d2e2845">The inset of Fig. 3a shows acrolein (ACR), a primary aldehyde precursor of APAN, correlated most strongly (<inline-formula><mml:math id="M165" 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> <inline-formula><mml:math id="M166" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.6) with APAN and ethylene oxide (EtO) among all ASIA-AQ measurements. It is noted that concurrent airborne measurements of these species were conducted for the first time in East Asia. Given the short lifetimes of APAN and acrolein, the enhancements are indicative of recent emissions from local to regional sources. The source of APAN and acrolein being dominated by biomass burning in the MS is unlikely due to a lack of correlation with HCN and CH<sub>3</sub>CN (Holzinger et al., 1999). The positive relationship between acrolein and benzene (<inline-formula><mml:math id="M168" 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> <inline-formula><mml:math id="M169" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.6) measured by TOGA in the SMA, but not in the MS, suggests that urban emissions do not explain the observations over the MS. Instead, the results point to industrial sources, particularly petrochemical facilities along the west coast, as the origin of both acrolein and APAN, supported by strong correlations with EtO, a tracer almost exclusively emitted from petrochemical activity (Robinson et al., 2024).</p>
      <p id="d2e2893">Recently, Robinson et al. (2024) reported EtO levels reaching hundreds of pptv in southeastern Louisiana's petrochemical corridor, exceeding EPA estimates (median difference of 21 pptv) and highlighting both the scarcity of ambient EtO data and potential negative health risks. Further evidence for a similar source attribution in South Korea is provided by back trajectories in Fig. 2, which intersects the BIC, a major industrial complex hosting roughly 13 000 metal manufacturing and 1400 petrochemical facilities, including synthetic rubber production (Chae et al., 2024). Although the back trajectories of the selected points did not directly intersect the DPCC, observations during KORUS-AQ demonstrated that its emissions influence the YS and southern Chungcheong regions adjacent to the MS. For example, our previous work showed efficient production of APAN and acrolein from 1,3-butadiene oxidation in plumes near DPCC and over the YS (Lee et al., 2022). In addition, the highest acrolein level observed during ASIA-AQ over the YS (600 pptv) coincided with the maximum 1,3-butadiene mixing ratio (1447 pptv) and elevated APAN (90 pptv), indicating the continued impact of petrochemical emissions in South Korea and their potential contribution to observations over the MS. Given the rapid formation of acrolein from 1,3-butadiene oxidation, direct source attribution is challenging. However, the strong positive relationship of APAN with EtO supports a dominant contribution from petrochemical emissions and suggest elevated exposure to highly toxic pollutants in the MS.</p>
      <p id="d2e2896">Previous model simulations by Lee et al. (2022) predict PBzN formation from styrene oxidation in the DPCC plumes. Our PBzN measurements during ASIA-AQ showed consistent enhancements alongside APAN, in agreement with the simulations. Figure 3b shows both APAN <inline-formula><mml:math id="M170" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> acrolein and PBzN <inline-formula><mml:math id="M171" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> benzaldehyde ratios increase generally with OH exposure, which provides an observation-based proxy for the extent of photochemical processing by OH radical, consistent with secondary formation from aldehyde precursors. The OH exposure, derived using Eq. (S1) based on observed isopropyl nitrate to propane ratios (see Sect. S5.1) captured the expected decay in the NO<sub><italic>x</italic></sub> contribution to NO<sub><italic>y</italic></sub> (approximated as NO<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> PANs <inline-formula><mml:math id="M175" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M176" 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> pNO<inline-formula><mml:math id="M177" 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 the increase in PANs to aldehyde ratios with increasing OH exposure (Fig. S7). Both APAN <inline-formula><mml:math id="M178" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> acrolein and PBzN <inline-formula><mml:math id="M179" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> benzaldehyde ratios increased with O<sub>3</sub> as well, further implicating photochemical oxidation of petrochemical VOCs in O<sub>3</sub> production, consistent with markedly significant O<sub>3</sub> levels up to 250 ppbv in petrochemical plumes during KORUS-AQ (Fried et al., 2020; Cho et al., 2021; Lee et al., 2022). Together, observations over the MS provide strong observational evidence of regional-scale photochemical pollution influenced by petrochemical emissions, with APAN, PBzN and their precursors as effective tracers of this impact.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Observation-based kinetic calculations and box modeling for diagnosis of VOC–NO<sub><italic>x</italic></sub> photochemistry</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Instantaneous production of PANs</title>
      <p id="d2e3043">To interpret the observed distributions of PANs, we use a combined analysis based on kinetic calculations and model simulations to estimate instantaneous production rates of PANs and their precursor contributions. For this purpose, we investigate the influence of precursor oxidation on PANs formation by focusing on the relative abundances of speciated PANs, which are less sensitive to atmospheric mixing and dilution than absolute concentrations. These processes are difficult to constrain in model simulations, particularly in regions with complex and uncertain emissions. Figure 4a compares observed fractional contributions with modeled instantaneous production rates (<inline-formula><mml:math id="M184" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs)), where <inline-formula><mml:math id="M185" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) denotes the combined production of PANs and corresponding peroxyacyl (PAs) radicals as a chemical family. The agreement between observations and <inline-formula><mml:math id="M186" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) suggests that local photooxidation is consistent with the chemical evolution responsible for the observed PANs distribution. This agreement was strongest over inland regions, where the influence of local emissions and recent photochemistry is expected to be more pronounced.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3069"><bold>(a)</bold> Averaged fractional contributions of observed PANs compounds (bright colored bars) and those of modeled instantaneous production rates of PANs, <inline-formula><mml:math id="M187" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs), (colored bars with patterns) over the SMA, MS, and YS. The split <inline-formula><mml:math id="M188" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>-axis is used to improve visibility of the homologue contributions. <bold>(b)</bold> Averaged <inline-formula><mml:math id="M189" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) over the SMA, MS, and YS along with precursor contributions. The left three bars correspond to <inline-formula><mml:math id="M190" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN) and other bars corresponds to <inline-formula><mml:math id="M191" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN homologues).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f04.png"/>

        </fig>

      <p id="d2e3119">Regional differences in <inline-formula><mml:math id="M192" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) and precursor contributions are illustrated in Fig. 4b. <inline-formula><mml:math id="M193" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) was higher over the MS and YS, consistent with elevated PANs mixing ratios and indicative of abundant precursors and active local formation. In contrast to regions with simpler VOC composition, in which acetaldehyde often dominates PAN production, our analysis illustrates non-acetaldehyde sources including methyl ethyl ketone (MEK), biacetyl (BIACET) and methyl glyoxal (MGLYOX), accounted for up to 47 % of PAN formation on average. While MEK and BIACET were measured, MGLYOX from model simulations was used for <inline-formula><mml:math id="M194" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs) calculations. The findings in this work suggest that less common precursors are critical for PAN chemistry over South Korea, which has been hypothesized in previous studies from KORUS-AQ (Nault et al., 2024) and from other polluted environments (Liu et al., 2010).</p>
      <p id="d2e3144">As the structure of PANs becomes more complex, the range of possible precursors narrows (Roberts, 2007). Consistent with this general tendency, contributions of unconventional precursors on PAN homologue formation was limited. Although PPN had a non-negligible contribution from ethyl glyoxal, analogous with MGLYOX contribution for PAN formation, propanal dominated its production. Larger homologues including APAN, PBN and PBzN were produced almost exclusively from their respective aldehyde precursors. Though present at much lower levels than PAN, the simpler formation pathways of the larger PAN compounds make them useful photochemical tracers for their precursor sources.</p>
      <p id="d2e3147">Constraining PAN formation from non-acetaldehyde precursors, hereafter <inline-formula><mml:math id="M195" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub>, has been a focus of research, particularly in environments impacted by isoprene and aromatics (Roberts et al., 2006; Liu et al., 2010; Nault et al., 2024; Travis et al., 2024). Major PAN precursors identified in the previous section such as MEK, BIACET, and MGLYOX can originate from both biogenic and anthropogenic sources (Fischer et al., 2014), complicating source attribution in East Asia, including South Korea, where both sources are prominent (Simpson et al., 2020). With limited isoprene during wintertime ASIA-AQ conditions, PAN formation is expected to be dominated by anthropogenic sources, providing a testbed to assess their impacts on PAN precursors.</p>
      <p id="d2e3179">Given that MGLYOX is expected to contribute significantly to <inline-formula><mml:math id="M197" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> and is a known product of aromatic oxidation (e.g., Fu et al., 2008; Nishino et al., 2010), we investigate the fractional contribution of PAN precursors as a function of aromatic contribution to OH reactivity (Fig. 5a–c). The modeled <inline-formula><mml:math id="M199" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN) exhibited decreasing relative contribution from acetaldehyde with increasing aromatic contribution to OH reactivity. This is most prominent over the SMA, where aromatic contributions are the highest (Fig. 5a). Over the SMA, the acetaldehyde contribution decreased to <inline-formula><mml:math id="M200" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 %, with substantial contributions from MEK, BIACET, and MGLYOX, consistent with regional mean <inline-formula><mml:math id="M201" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN) shown in Fig. 4. The contribution of MEK was also higher in regions with greater aromatic influence, while the impacts of BIACET are relatively constant.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3234"><bold>(a–c)</bold> Modeled fractional contributions from PAN production channels as a function of aromatic contribution to OH reactivity from VOCs, <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">Aromatics</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M203" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VOCs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, over the SMA, MS, and YS. Inferred <inline-formula><mml:math id="M205" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> as a function of <bold>(d)</bold> <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">Aromatics</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M208" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VOCs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <bold>(e)</bold> mixing ratios of aromatic oxidation products. The solid fit lines in <bold>(d)</bold> and <bold>(e)</bold> are provided as a visual aid. <bold>(f)</bold> Inferred <inline-formula><mml:math id="M210" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> based on kinetic calculations compared to modeled <inline-formula><mml:math id="M212" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub>. The bold dashed line is the <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> line. Inferred and modeled <inline-formula><mml:math id="M215" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> are in units of molec. cm<sup>−3</sup> s<sup>−1</sup>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f05.png"/>

        </fig>

      <p id="d2e3473">To complement our model analysis, we use kinetic calculations to infer <inline-formula><mml:math id="M219" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN) from non-acetaldehyde sources (inferred <inline-formula><mml:math id="M220" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub>), using Eqs. (S2)–(S3) in Sect. S2.2. This analysis provides an additional constraint on <inline-formula><mml:math id="M222" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> to our model analysis because direct experimental quantification remains challenging due in part to significant interferences in even state-of-the-art mass spectrometric and optical techniques for MGLYOX measurements (Koss et al., 2018). Briefly, the method leverages extensive measurements of PANs and their precursors and is based on two assumptions: (1) observed PAN-to-homologue ratios are representative of the ratios of their instantaneous production rates; and (2) PAN homologues are dominantly formed from their corresponding aldehydes. These assumptions were assessed in the previous section using model simulations and found reasonable.</p>
      <p id="d2e3542">The inferred <inline-formula><mml:math id="M224" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> was illustrated as a function of aromatic contribution to OH reactivity (Fig. 5d) as well as the summed concentrations of observed aromatic oxidation products including benzaldehyde, cresol, phenol, nitrocresol, and nitrophenol (Fig. 5e). The inferred <inline-formula><mml:math id="M226" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub> increased with these proxies for aromatic oxidation, consistent with the modeled contribution of MGLYOX in this work and previous model studies in East Asia (Liu et al., 2010; Fischer et al., 2014). Notably, the values based on PAN <inline-formula><mml:math id="M228" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PPN ratios were generally lower than those from other homologues, consistent with minor contributions to PPN from non-propanal precursors (8 %–18 %) and almost exclusive contribution of the respective aldehydes to larger PAN homologues. When compared to the model-derived <inline-formula><mml:math id="M229" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PAN)<sub>w∕o CH<sub>3</sub>CHO</sub>, the kinetic estimates were in reasonable accord, supporting the validity of the estimations from two different methods (Fig. 5f). Overall, our observation-based diagnostic, combining model simulations and kinetic calculations, provides strong evidence for the contribution of non-acetaldehyde sources to PAN formation in South Korea. This contribution is particularly important in the SMA where aromatics are more abundant.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Contribution of ethanol and other precursors to secondary acetaldehyde production</title>
      <p id="d2e3648">Despite the important contributions of non-acetaldehyde sources to PAN production, acetaldehyde remains the most important precursor of PAN on average. In urban environments, acetaldehyde is often dominated by secondary production from oxidation of hydrocarbons from anthropogenic emissions, although acetaldehyde can originate from primary emissions from various anthropogenic and biogenic sources (e.g., Grosjean et al., 2002; Millet et al., 2010; de Gouw et al., 2018). Here, we investigate the source of acetaldehyde as it is of particular importance for PAN as well as O<sub>3</sub> formation (e.g., Sect. 3.2.3) in South Korea.</p>
      <p id="d2e3660">The pie chart in Fig. 6a shows fractional contribution of direct precursors of modeled acetaldehyde production, <inline-formula><mml:math id="M232" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO), with a mean value of 51 <inline-formula><mml:math id="M234" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 46 (1<inline-formula><mml:math id="M235" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv h<sup>−1</sup> over South Korea. The bar charts illustrate how <inline-formula><mml:math id="M237" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO) and its direct precursors change upon removal of the selected major precursors in model simulations for South Korea. The most significant reduction of <inline-formula><mml:math id="M239" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO) was found when ethanol was set to zero. Compared to the base case simulation, <inline-formula><mml:math id="M241" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO) decreased by nearly a half. This result from a simple diagnostic box modeling is consistent with a 50 % reduction in acetaldehyde without including ethanol in GEOS-Chem transport model simulations for the SMA during KORUS-AQ (Travis et al., 2024). To a lesser extent, oxidation of more common hydrocarbon precursors (e.g., ethane and propene) and carbonyls (e.g., propanal and ethyl acetate) also contributed to <inline-formula><mml:math id="M243" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3773"><bold>(a)</bold> Pie chart illustrating the fractional contributions to direct acetaldehyde production, <inline-formula><mml:math id="M245" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO), from individual pathways in the base-case model simulation (mean <inline-formula><mml:math id="M247" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO) <inline-formula><mml:math id="M249" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 51 ppt h<sup>−1</sup>). C<sub>2</sub>H<sub>5</sub>OH <inline-formula><mml:math id="M253" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH represent ethanol oxidation by OH. C<sub>2</sub>H<sub>5</sub>O and C<sub>3</sub>H<sub>7</sub>O<sub>2</sub> denote alkoxy and hydroxy alkoxy radicals, respectively, which decompose to form acetaldehyde. ETHACET <inline-formula><mml:math id="M259" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH indicates OH oxidation of ethyl acetate. Others include minor pathways such as OH oxidation of MEK and PPN, and ozonolysis of propene and butene isomers. The bar charts illustrate changes of <inline-formula><mml:math id="M260" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO) in response to removal of the selected major precursors of acetaldehyde in model simulations. <bold>(b)</bold> Scatter plot showing median industrial facility density (ID<sub>5 km</sub>) as a function of population density (PD<sub>5 km</sub>), binned in intervals of 1000, with shaded areas indicating the 25th and 75th percentiles in each bin. <bold>(c)</bold> Scatter plots of CHBrCl<sub>2</sub>, HCFC-142b and HFC-134a versus ethanol, with colored and gray markers indicating measurements during low approaches and normal operations, respectively.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f06.png"/>

        </fig>

      <p id="d2e3965">The substantial contribution of ethanol to <inline-formula><mml:math id="M265" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(CH<sub>3</sub>CHO), particularly due to its high abundance at low altitudes (median <inline-formula><mml:math id="M267" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 ppbv, maximum <inline-formula><mml:math id="M268" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 13 ppbv at altitudes <inline-formula><mml:math id="M269" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 500 m), underscores its importance for PAN and motivate further investigation on its local sources in South Korea. Recent model analyses based on KORUS-AQ data have identified ethanol as a key precursor to acetaldehyde and PAN, consistent with findings in this work, using estimated ethanol levels from ethanol <inline-formula><mml:math id="M270" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> methanol ratios of 0.4 obtained from previous ground-based campaign (the Megacity Air Pollution Studies-Seoul; MAPS-Seoul) (Nault et al., 2024; Travis et al., 2024). The ASIA-AQ observations over South Korea showed a moderately correlated relationship between ethanol and methanol (<inline-formula><mml:math id="M271" 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:mrow></mml:math></inline-formula> 0.44) and an ethanol <inline-formula><mml:math id="M272" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> methanol ratio of 0.48, derived from the slope of a linear regression, supporting these estimates. In addition, Travis et al. (2024) demonstrated that increasing ethanol emission factors by a factor of 40 over those in current emission inventory (KORUS-AQ v5) was necessary to reduce model bias in PAN over the SMA from <inline-formula><mml:math id="M273" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50 % to <inline-formula><mml:math id="M274" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>23 %, while the significant increase in ethanol was attributed to VCPs.</p>
      <p id="d2e4047">Consistent with this source attribution, Beaudry et al. (2025) reported that reproducing ethanol levels during KORUS-AQ and MAPS-Seoul campaigns required per capita VCP emissions in South Korea to be 2.4 times higher than in the US. In contrast to the implementation of population-based emissions of ethanol from VCPs, no significant relationship was found between ethanol and PD<sub>5 km</sub>, suggesting ethanol is from a source unrelated to local population density or is distributed over large areas. In addition, Fig. 6b illustrates co-location of industrial facilities and populated areas using scatter plot of ID<sub>5 km</sub> over PD<sub>5 km</sub>. This spatial overlap of the sources may partially explain improved model performance implementing population-based emissions when ethanol emissions from industrial sources contribute to the observed distribution. This indicated that a comprehensive source attribution including VCP emissions from industrial and consumer products, as well as other possible sources (e.g., fuel combustion), is critical for accurately assessing atmospheric impacts of ethanol. Supporting this interpretation, Fig. 6c shows that ethanol correlated most strongly with halocarbons, including bromodichloromethane (CHBrCl<sub>2</sub>), HCFC-142b, and HFC-134a with <inline-formula><mml:math id="M279" 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> <inline-formula><mml:math id="M280" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.8. The strong positive relationships were particularly noticeable during low approaches near major urban airports (i.e., Seoul and Gimpo), suggesting surface emissions from industrial (e.g., chemical production, refrigerants and blowing agents) and solvent-related sources (ATSDR, 2005, 2020, and references therein). Beyond air quality implications, investigation of ethanol and halocarbon emissions over South Korea has the potential to improve understanding of the sources and distributions of short-lived (O<sub>3</sub>) and longer-lived (HCFCs, HFCs) climate forcers, given increasing background levels of such halocarbons with unidentified sources in East Asia (Choi et al., 2024).</p>
      <p id="d2e4114">In summary, ethanol and other species were significant sources of acetaldehyde. Previous studies have attributed ethanol emissions to VCPs based on findings from US cities. However, our results indicate that such attribution requires a more detailed understanding of local sources, including industrial activities near populated areas. The heterogenous distribution of VOCs and PANs observed in this work support this conclusion.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Instantaneous production rates, efficiency, and chemical regimes of O<sub>3</sub></title>
      <p id="d2e4134">Ozone formation is evaluated based on instantaneous ozone production rates, <inline-formula><mml:math id="M283" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>), and efficiency, OPE. For this evaluation we use a combined analysis incorporating kinetic calculations and model simulations. This analysis enables a detailed diagnostic of ozone production by integrating observation-based estimates using experimental parameters with near-explicit chemical modeling that includes precursors not directly measured such as radicals. Figure 7a shows <inline-formula><mml:math id="M285" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) from kinetic calculations using Eq. (3) and an OH concentration of 2 <inline-formula><mml:math id="M287" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup> as a function of NO<sub><italic>x</italic></sub> on a logarithmic scale, with OH exposure shown in the upper panel. The general increase in <inline-formula><mml:math id="M291" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) is due to increasing OH reactivity with NO<sub><italic>x</italic></sub>, as the calculation does not account for suppression of OH at high NO<sub><italic>x</italic></sub> levels.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e4244"><bold>(a)</bold> Median ozone production, <inline-formula><mml:math id="M295" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>), from kinetic calculations using [OH] <inline-formula><mml:math id="M297" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M298" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup> for the SMA (orange line with circles), MS (blue line with triangles) and YS (red line with squares) in 0.5-logarithmic NO<sub><italic>x</italic></sub> bins. Vertical and horizontal lines represent 25th and 75th percentiles on the respective axes. The OH exposure (lines with markers) for each region is shown in the upper panel. Pie charts indicate the fractional contribution of each of the VOC classes (defined in the legend) to <inline-formula><mml:math id="M302" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>). <bold>(b–d)</bold> Comparisons of <inline-formula><mml:math id="M304" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) from kinetic calculations using modeled [OH] (black lines with shaded areas representing precursor contributions) and model simulations based on the sum of reactions of peroxy radicals with NO over the selected regions (red dashed lines). Sequential model step on the <inline-formula><mml:math id="M306" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>-axis represents sequential indices of model output, used to illustrate the comparison between kinetic calculations and model simulations. <bold>(e)</bold> Box and whisker plot of instantaneous ozone production efficiency (OPE), along with regional averages (red markers).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f07.png"/>

        </fig>

      <p id="d2e4362"><inline-formula><mml:math id="M307" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) from kinetic calculations is more effective for evaluating relative precursor contributions independent of OH. The pie charts in Fig. 7a show substantial contributions of oxygenates, especially C<sub>2+</sub> aldehydes to <inline-formula><mml:math id="M310" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>), second in importance to CO. Other important oxygenated contributors include formaldehyde as well as ketones and alcohols such as MEK, methanol, ethanol, and isopropanol, which together account for <inline-formula><mml:math id="M312" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 95 % of this category. Less significantly, primary hydrocarbons including methane (CH<sub>4</sub>), alkanes, alkenes, and aromatics over South Korea showed similar contributions, while aromatic impacts were minimal in the YS. Less-reactive species such as CO and CH<sub>4</sub> were more important over the YS, likely due to sampling of air masses with biomass burning influence and with longer time since emissions.</p>
      <p id="d2e4435">When modeled OH was used in the kinetic calculations, instead of using a constant value for generalization, <inline-formula><mml:math id="M315" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) from kinetic calculations was in excellent agreement with model simulations based on Eq. (2) (Fig. 7b–d). This indicates that the modeled oxidative chemistry driving ozone production and radical cycling can be explained by the current understanding of observed VOC photooxidation. Consistent with the averaged impacts shown in Fig. 7a, oxygenates including C<sub>2+</sub> aldehydes and formaldehyde showed significant and persistent contribution in all regions. In addition, peak ozone production over the YS occurred during episodic enhancements of alkenes that dominated <inline-formula><mml:math id="M318" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>), which was attributed to sampling of relatively fresh petrochemical plumes, also described in Sect. 3.1. Another important measure for ozone production is OPE. Figure 7e shows modeled OPE using box plots, with red markers indicating regional averages. OPE generally decreased with increasing NO<sub><italic>x</italic></sub>, resulting in the lowest and highest values in the SMA and YS, respectively. Higher OPE indicates more efficient radical propagation relative to termination by NO<sub><italic>x</italic></sub>. The interquartile ranges of OPE for the SMA (3.3–5.3) and MS (4–7.8) were comparable to the previous reported values in East Asia (<inline-formula><mml:math id="M322" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M323" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10) in winter–spring, though only limited values are available for winter (Lin et al., 2011; Lee et al., 2021; Kim et al., 2020; Oak et al., 2019).</p>
      <p id="d2e4515">A key factor determining OPE and the prevailing chemical regime is the balance of radical (RO<inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> OH <inline-formula><mml:math id="M325" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HO<inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> RO<sub>2</sub>) termination pathways, including self-reactions of peroxy radicals and reactions with NO<sub><italic>x</italic></sub>, which removes radicals and NO<sub><italic>x</italic></sub> from ozone producing photochemical cycles. The modeled instantaneous radical loss indicates that radical loss by reaction with NO<sub><italic>x</italic></sub> dominates over the SMA (88 %) and MS (80 %), with nitric acid (HNO<sub>3</sub>) and PANs as the major products and smaller contributions from alkyl nitrates and nitroaromatic compounds (Fig. 8). It should be noted that the chemistry of nitroaromatics in the MCM mechanism may be uncertain and needs further investigation (Bates et al., 2021; MacFarlane et al., 2025). The dominant contributions of HNO<sub>3</sub> and PANs to radical loss are consistent with wintertime observations in Beijing based on direct radical measurements (Tan et al., 2018; Lu et al., 2019). Other minor radical termination pathways include formation of peroxides, HONO, and pernitric acid (HO<sub>2</sub>NO<sub>2</sub>).</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e4624">Averaged fractional contributions of modeled instantaneous radical loss pathways over the SMA, MS, and YS (pie charts), along with markers colored by instantaneous fraction of radical loss by NO<sub><italic>x</italic></sub> in total loss (Ln <inline-formula><mml:math id="M336" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M337" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula>).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f08.png"/>

        </fig>

      <p id="d2e4656">In addition to OPE, the ratio of radical loss by NO<sub><italic>x</italic></sub> (Ln) to total loss (<inline-formula><mml:math id="M339" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula>), Ln <inline-formula><mml:math id="M340" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M341" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> ratio, provides an additional diagnostic measure for ozone formation regimes, with Ln <inline-formula><mml:math id="M342" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M343" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M344" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5 indicating VOC-limited regimes and Ln <inline-formula><mml:math id="M345" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M346" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M347" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.5 indicating NO<sub><italic>x</italic></sub>-limited regimes (Kleinman et al., 2002). Figure 8a shows a median Ln <inline-formula><mml:math id="M349" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M350" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> values of 0.9 over South Korea, representative of VOC-limited regimes with major radical loss driven by HNO<sub>3</sub> and PANs formation in the region. Over the YS, radical-radical reactions producing peroxides become increasingly important, resulting in a lower median Ln <inline-formula><mml:math id="M352" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M353" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> of 0.4.</p>
      <p id="d2e4779">To investigate potential impacts of emission changes on chemical regimes, model sensitivity simulations were conducted by evaluating <inline-formula><mml:math id="M354" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(PANs), <inline-formula><mml:math id="M355" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>(O<sub>3</sub>) and OPE responses to perturbations of NO<sub><italic>x</italic></sub> and VOCs constraints (<inline-formula><mml:math id="M358" display="inline"><mml:mo lspace="0mm">±</mml:mo></mml:math></inline-formula>40 % of the base case). Figure S8a–b show the average relative changes of P(PANs) and P(O<sub>3</sub>) exhibit a strong positive response to VOCs across all regions, while NO<sub><italic>x</italic></sub> perturbation produces opposite responses in South Korea and a weaker effect in the YS. In contrast to this regional difference, OPE showed more uniform response across regions as it represents the average changes in the ratio between formation of radicals and NO<sub><italic>x</italic></sub> oxidation products (Fig. S8c). The model sensitivity results point out that PANs and ozone formation during ASIA-AQ occurred in VOC-limited conditions and suggest that VOC reductions, especially anthropogenic aldehydes, alkenes and aromatics, would be more effective than NO<sub><italic>x</italic></sub> controls for mitigation of photochemical pollution.</p>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Diagnostic kinetic and model analysis on NOx loss pathways</title>
      <p id="d2e4867">A defining feature of the ASIA-AQ observations was the substantial variability in pollutant distributions, reflecting a broad range of photochemical conditions and pollution intensities (e.g., NO<sub><italic>x</italic></sub> levels spanning orders of magnitude; Fig. 7a). While NO<sub><italic>x</italic></sub> removal was dominated by HNO<sub>3</sub> and PANs, which together accounted for <inline-formula><mml:math id="M366" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 90 % of modeled NO<sub><italic>x</italic></sub> loss over South Korea, their relative contributions varied largely during the campaign, in part due to this variability. Romer et al. (2020) evaluated observed relative contributions of HNO<sub>3</sub> and alkyl nitrates (RONO<sub>2</sub>) to NO<sub><italic>x</italic></sub> loss during the summer daytime across multiple campaigns in the US over 15 years, using kinetic calculations based on instantaneous production rates. They pointed out the relative contribution of HNO<sub>3</sub> decline with the OH reactivity ratio of NO<sub>2</sub> to the sum of VOCs (<inline-formula><mml:math id="M373" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M374" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M375" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VOCs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), suggesting increased importance of RONO<sub>2</sub> chemistry with decreases in NO<sub><italic>x</italic></sub> levels.</p>
      <p id="d2e5011">Using a similar kinetic approach to Romer et al. (2020), we investigate the fractional contribution of PANs to total NO<sub><italic>x</italic></sub> loss (<inline-formula><mml:math id="M379" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Here, observation-based <inline-formula><mml:math id="M380" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M381" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) is defined as the ratio of observed PANs to the sum of observed PANs, HNO<sub>3</sub>, and particulate inorganic nitrate (pNO<sub>3<sup>−</sup>inorganic</sub>). pNO<sub>3<sup>−</sup>inorganic</sub> was estimated by excluding organic nitrate contribution (<inline-formula><mml:math id="M385" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 10 % of pNO<inline-formula><mml:math id="M386" 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> over South Korea) from total nitrate measured by the University of Colorado Aerosol Mass Spectrometer (CU aircraft AMS), following the method of Day et al. (2022). This diagnostic analysis may be particularly relevant for wintertime East Asia, where cold conditions extend PANs lifetime (effective lifetime of <inline-formula><mml:math id="M387" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3 d) and enable efficient NO<sub><italic>x</italic></sub> sequestration (e.g., Fig. 8). The competition among HNO<sub>3</sub> and PANs formation is a critical factor that controls NO<sub><italic>x</italic></sub> lifetimes and the spatial extent of ozone pollution, as HNO<sub>3</sub> formation constitutes a permanent sink, whereas PANs serve as a reservoir and can facilitate NO<sub><italic>x</italic></sub> transport on local–regional scales.</p>
      <p id="d2e5173">During ASIA-AQ, <inline-formula><mml:math id="M393" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> varied substantially (0.2–0.94) and had an inverse relationship with the OH reactivity ratio of NO<sub>2</sub> to the sum of observed aldehyde precursors of PANs (<inline-formula><mml:math id="M395" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M396" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M397" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). The decrease in <inline-formula><mml:math id="M398" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M400" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> suggests the importance of competition between OH reacting with NO<sub>2</sub> to form HNO<sub>3</sub> versus with aldehydes to form PAs, which promotes PANs formation, in determining NO<sub><italic>x</italic></sub> loss pathways. It should be noted that <inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is more relevant than <inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">VOCs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> used in previous studies for the analysis herein and may provide a more consistent basis for future analyses, given that kinetic calculations are sensitive to the selection of VOCs and their associated kinetic parameters (e.g., alkyl nitrate branching ratios and yields).</p>
      <p id="d2e5334">The observed dependence of <inline-formula><mml:math id="M407" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math id="M408" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M409" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M410" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is consistent with kinetic expressions (Eqs. S4–S6) that define the ratio of instantaneous PANs production rates to the combined rates of PANs and HNO<sub>3</sub> production. These equations exhibit a negative relationship of <inline-formula><mml:math id="M412" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M414" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M415" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and NO <inline-formula><mml:math id="M416" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, reflecting a broader dependence of <inline-formula><mml:math id="M418" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on NO<sub><italic>x</italic></sub> to aldehydes ratios. For comparison with <inline-formula><mml:math id="M420" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, we include estimates from kinetic calculations assuming a constant [OH] <inline-formula><mml:math id="M421" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M422" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup> (<inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> based on kinetic calculations; <inline-formula><mml:math id="M426" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) from calculations using modeled [OH] (<inline-formula><mml:math id="M427" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">w</mml:mi><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal">model</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>), and from full model simulations (<inline-formula><mml:math id="M428" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">model</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) in Fig. 9a. As expected from the kinetic equations, all estimates exhibit a decreasing trend with increasing <inline-formula><mml:math id="M429" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M430" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M431" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, in reasonable accordance with the observations.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e5638"><bold>(a)</bold> Median observed fractional contribution of PANs to the total NO<sub><italic>x</italic></sub> loss based on observations (<inline-formula><mml:math id="M433" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>; black line with markers) along with median ratios of instantaneous PANs production rates to the combined rates of PANs and HNO<sub>3</sub> production from kinetic calculations using [OH] <inline-formula><mml:math id="M435" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M436" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup> (<inline-formula><mml:math id="M439" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>; red line with markers) and modeled [OH] (<inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">w</mml:mi><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal">model</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>; orange line with markers), and from model simulations (<inline-formula><mml:math id="M441" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">model</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>; blue line with markers) in 0.2-logarithmic <inline-formula><mml:math id="M442" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M443" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M444" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> bins. All data points used to calculate <inline-formula><mml:math id="M445" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are illustrated as gray markers. <bold>(b)</bold> Median modeled Ln <inline-formula><mml:math id="M446" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M447" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> (red line with markers) and OPE (OPE<sub>model</sub>; purple line with markers) and kinetic calculated OPE (OPE<sub>kc</sub>; green line with markers) in 0.2-logarithmic <inline-formula><mml:math id="M450" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M451" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M452" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> bins. The error bars in both figures indicate 25th and 75th percentiles in each bin.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/8695/2026/acp-26-8695-2026-f09.png"/>

        </fig>

      <p id="d2e5897">Because <inline-formula><mml:math id="M453" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represent a ratio of production rates, it is largely independent of OH concentrations, as indicated by the overlap between <inline-formula><mml:math id="M454" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">w</mml:mi><mml:mo>/</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal">model</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> in Fig. 9a. This suggests that the consistently higher <inline-formula><mml:math id="M456" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">model</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> values than both <inline-formula><mml:math id="M457" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M458" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">kc</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">w</mml:mi><mml:mo>/</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal">model</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are not driven by differences in OH but instead by other factors such as additional PANs sources in the model not accounted for by the kinetic calculations (detailed discussion in Sect. 3.2.1). Despite the similar dependence of observed and estimated <inline-formula><mml:math id="M459" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mi mathvariant="normal">PANs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on <inline-formula><mml:math id="M460" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M461" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M462" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the estimated values systematically underestimated <inline-formula><mml:math id="M463" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. This discrepancy likely reflects the cumulative nature of the observations, which integrate ambient processes such as total nitrate loss and unaccounted PANs contributions from chemical production, transport, and background sources.</p>
      <p id="d2e6074">The diagnostic ratio <inline-formula><mml:math id="M464" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M465" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M466" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> effectively characterizes the observed partitioning of NO<sub><italic>x</italic></sub> loss. To further assess its utility, we examine the sensitivity of Ln <inline-formula><mml:math id="M468" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M469" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> and OPE to changes in <inline-formula><mml:math id="M470" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M471" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M472" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. As shown in Fig. 9b, Ln <inline-formula><mml:math id="M473" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M474" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> from model simulations increase with <inline-formula><mml:math id="M475" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M476" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M477" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, indicating shift toward VOC-limited conditions at higher NO<sub><italic>x</italic></sub> to aldehyde ratios. Consistent with this, OPE decreases with increasing <inline-formula><mml:math id="M479" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M480" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M481" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in both kinetic calculations (using [OH] <inline-formula><mml:math id="M482" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M483" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>6</sup> molec. cm<sup>−3</sup>) and model simulations. These sensitivities likely represent that lower <inline-formula><mml:math id="M486" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M487" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M488" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> facilitates radical propagation and PANs formation, while higher values favor HNO<sub>3</sub> formation and thus radical termination. Although not explicitly stated in kinetic expressions, <inline-formula><mml:math id="M490" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M491" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M492" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> likely evolves with photochemical aging as NO<sub><italic>x</italic></sub> is converted to HNO<sub>3</sub> and PANs, and secondary aldehydes are produced downwind. Consistent with this interpretation, OH exposure generally decreases with <inline-formula><mml:math id="M495" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M496" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M497" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (not shown).</p>
      <p id="d2e6421">Overall, the dependence of <inline-formula><mml:math id="M498" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">obs</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> on <inline-formula><mml:math id="M499" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M500" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M501" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, consistent with kinetic theory, suggests continued NO<sub><italic>x</italic></sub> reduction, following the trends observed over the past decade over South Korea and other East Asian countries (Duncan et al., 2016), may decrease <inline-formula><mml:math id="M503" display="inline"><mml:mrow><mml:msub><mml:mi>R</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> <inline-formula><mml:math id="M504" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M505" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">ALD</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and shift NO<sub><italic>x</italic></sub> loss pathways more toward PANs formation than HNO<sub>3</sub> in winter. Supporting this postulation, <inline-formula><mml:math id="M508" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">χ</mml:mi><mml:mrow><mml:mi mathvariant="normal">PANs</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">model</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> increased by 22 % on average in sensitivity simulations with a 40 % reduction in NO<sub><italic>x</italic></sub> constraints. However, the predicted increase in PANs likely represents an upper limit, as observed aldehydes were constrained in the simulations, despite their yields from VOC oxidation often being NO<sub><italic>x</italic></sub>-dependent (e.g., Millet et al., 2010). The potential shift in NO<sub><italic>x</italic></sub> loss partitioning in response to NO<sub><italic>x</italic></sub> reductions may result in extended spatial impacts of NO<sub><italic>x</italic></sub> emissions and consequently ozone pollution, which may be further exacerbated by increase in OPE (Fig. S8 and Fig. 9).</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusion</title>
      <p id="d2e6606">This study provides a comprehensive characterization of wintertime acyl peroxynitrates (PANs) chemistry over South Korea during the Airborne and Satellite Investigation of Asian Air Quality (ASIA-AQ) campaign, combining novel measurements of rare acetyl peroxynitrate (PAN) homologues with integrated kinetic and modeling analysis. Our findings reveal active photochemical processing despite cold conditions and provide critical insights into volatile organic compounds (VOC) sources, oxidation pathways, and their implications for air quality management.</p>
      <p id="d2e6609">PANs levels were persistently elevated across South Korea and the Yellow Sea (YS) (frequently exceeding 1 ppbv, maximum 5.5 ppbv), with strong correlations to formaldehyde (CH<sub>2</sub>O), odd oxygen (O<sub><italic>x</italic></sub>; approximated as O<inline-formula><mml:math id="M516" 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> NO<sub>2</sub>) and secondary aerosols confirming active winter photochemistry. Regional pollution was extensive, with higher median PANs in remote areas (the mid- and southern region (MS): 990 pptv; YS: 1200 pptv) than in the Seoul Metropolitan Area (SMA: 840 pptv) despite lower emissions, demonstrating significant transport and regional impacts. Elevated homologue <inline-formula><mml:math id="M518" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> PAN ratios, particularly for acryloyl peroxynitrate (APAN) and benzoyl peroxynitrate (PBzN), indicate complex source influences. Notably, strong correlations between APAN, acrolein, and ethylene oxide provided strong evidence of petrochemical impacts and associated toxic exposures in the MS, with back trajectories indicating transport from west coast industrial complexes.</p>
      <p id="d2e6659">Mechanistic analysis demonstrated that while acetaldehyde dominates PAN production (53 %–80 %), other precursors including aromatics make significant contributions (up to 47 % in Seoul). Ethanol was demonstrated to be a critical precursor, as it contributes approximately 50 % to acetaldehyde formation. In addition, ethanol was very strongly correlated with industrial halocarbons (<inline-formula><mml:math id="M519" 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> <inline-formula><mml:math id="M520" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.8), including bromodichloromethane, HCFC-142b and HFC-134a, indicating important industrial and solvent sources beyond consumer products. This finding challenges previous attributions to volatile chemical products alone and highlights the need for better constraints on industrial VOC emissions in South Korea.</p>
      <p id="d2e6680">Ozone production analysis confirmed VOC-limited conditions across South Korea, with aldehydes (formaldehyde and C<sub>2+</sub> aldehydes) contributing approximately 20 %–30 % of instantaneous ozone production. Radical loss was dominated (<inline-formula><mml:math id="M522" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 80 %) by formation of nitric acid and PANs, with median Ln <inline-formula><mml:math id="M523" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M524" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> ratios of 0.9 indicating strong VOC limitation. Ozone production efficiency values (<inline-formula><mml:math id="M525" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 10) were consistent with wintertime observations elsewhere in East Asia.</p>
      <p id="d2e6724">A finding with important policy implications is that continued NO<sub><italic>x</italic></sub> reductions may paradoxically expand the spatial extent of ozone pollution. Our diagnostic analysis shows that the fractional contribution of PANs to NO<sub><italic>x</italic></sub> loss increases systematically as the ratio of NO<sub>2</sub> to aldehyde reactivity decreases. Model simulations indicate that a 40 % NO<sub><italic>x</italic></sub> reduction could increase PANs' contribution to NO<sub><italic>x</italic></sub> loss by 22 %, shifting nitrogen oxide chemistry toward the longer-lived PANs reservoir rather than permanent removal as nitric acid. This shift, combined with increases in ozone production efficiency, may extend the spatial impacts of NO<sub><italic>x</italic></sub> emissions and exacerbate regional ozone pollution.</p>
      <p id="d2e6782">These findings have implications for air quality management in South Korea and East Asia. Effective control of wintertime photochemical pollution requires prioritizing reductions in aldehydes and their precursors – particularly ethanol and reactive alkenes from both industrial and consumer sources. Better characterization of industrial VOC emissions, including from petrochemical facilities, is essential. While concurrent NO<sub><italic>x</italic></sub> reductions remain important for long-term benefits and reducing fine particulate matter, policymakers should anticipate potential near-term increases in the spatial extent of ozone pollution as NO<sub><italic>x</italic></sub> levels decline. Together with prior springtime observations from KORUS-AQ, future studies of summertime PANs in South Korea would improve understanding of seasonable differences in their chemistry and inform broader control strategies for photochemical pollution. Finally, our integrated approach demonstrates the value of comprehensive PAN homologue measurements as diagnostic tools for understanding complex urban and regional photochemistry.</p>
</sec>

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

      <p id="d2e6807">All data used in this work is available at <uri>https://www-air.larc.nasa.gov/cgi-bin/ArcView/asiaaq</uri> (last access: 18 June 2026). The F0AM model (version 4.3.0.1) and setup file are available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.10069985" ext-link-type="DOI">10.5281/zenodo.10069985</ext-link> (Wolfe and Haskins, 2023).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e6816">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-8695-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-8695-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e6825">All of the authors reviewed and edited the document and participated in the investigation by data acquisition or flight planning. YRL conceived and performed the formal analysis and wrote the first draft of the document. LA was responsible for data curation. LGH was responsible for obtaining funding and aided in writing the first draft.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e6831">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="d2e6837">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="d2e6843">The authors thank the flight crew of the NASA-DC8.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e6848">YRL was supported by NASA (grant no. 80NSSC21K1704). LA, DT and LGH were supported by NASA (grant no. 80NSSC23K0826). AJH, RSH and ECA were supported in part by NASA (grant no. 80NSSC23K0818). SM, BB, NJB and DRB were supported by NASA (grant no. 80NSSC23K0819). PTR-ToF-MS measurements aboard the NASA DC-8 during ASIA-AQ were partially funded by the Austrian Federal Ministry for Climate Action, Environment, Energy, Mobility, Innovation, and Technology (BMK), represented by the Austrian Research Promotion Agency (FFG), through the Austrian Space Applications Programme (ASAP 2022, grant no. FO999900547). IONICON Analytik is acknowledged for supplying a FUSION PTR-ToF-MS analyzer and providing staff support. WW gratefully acknowledges the support from Gdańsk University of Technology through the DEC-4/1/2024/IDUB/II.1b/Am grant under the Americium International Career Development – “Excellence Initiative – Research University” program. JDC and POW were supported by NASA (grant no. 80NSSC21K1704). KB was supported by NASA FINESST (grant no. 80NSSC24K0005). GS, DK, DD, PCJ and JLJ were supported by NASA (grant no. 80NSSC21K1451 and grant no. 80NSSC23K0828). NASA (grant no. 80NSSC23K0825) funded the CAFS deployment and SH and KU. AS, ERD, RAH, JMSC, and GMW were supported by the NASA Tropospheric Composition Program. This material is based upon work supported by the NSF National Center for Atmospheric Research, which is a major facility sponsored by the US National Science Foundation under Cooperative Agreement grant no. 1852977.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e6854">This paper was edited by Eva Y. Pfannerstill and reviewed by two anonymous referees.</p>
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