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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-26-14229-2026</article-id><title-group><article-title>Light absorption properties and composition of water-soluble brown carbon in North China Plain: implication for an enhancing role of  nitrogenous organic compounds</article-title><alt-title>Light absorption properties of water-soluble brown carbon in North China Plain</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Wu</surname><given-names>Can</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Huijun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sun</surname><given-names>Kehan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Li</surname><given-names>Rongjie</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Yan</surname><given-names>Ziting</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Chen</surname><given-names>Yubao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Li</surname><given-names>Zheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Xiao</surname><given-names>Binyu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Ren</surname><given-names>Yanqin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Wang</surname><given-names>Gehui</given-names></name>
          <email>ghwang@geo.ecnu.edu.cn</email>
        <ext-link>https://orcid.org/0000-0002-0181-4685</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Key Lab of Geographic Information Science of the Ministry of Education, School of Geographic Sciences, East China Normal University, Shanghai 210062, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute of Eco-Chongming, East China Normal University, 3663 North Zhongshan Road, Shanghai 200062, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>State Key Laboratory of Environmental Criteria and Risk Assessment, Chinese Research Academy of Environmental Sciences, Beijing 100012, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Gehui Wang (ghwang@geo.ecnu.edu.cn)</corresp></author-notes><pub-date><day>9</day><month>October</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>19</issue>
      <fpage>14229</fpage><lpage>14243</lpage>
      <history>
        <date date-type="received"><day>16</day><month>December</month><year>2025</year></date>
           <date date-type="rev-request"><day>12</day><month>January</month><year>2026</year></date>
           <date date-type="rev-recd"><day>18</day><month>August</month><year>2026</year></date>
           <date date-type="accepted"><day>14</day><month>September</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Can Wu 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/26/14229/2026/acp-26-14229-2026.html">This article is available from https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e181">Brown carbon (BrC), an efficiently light-absorbing carbonaceous aerosol, exerts significant impacts on the global energy budget and regional climate, attracting growing scientific attention. To advance understanding of the spatial variability of atmospheric BrC and its dominant formation pathways in the North China Plain (NCP), light absorption properties, chemical composition and formation process of the water-soluble BrC in 2023 winter were investigated by conducting simultaneous measurements at five sites across the NCP, namely, Beijing, Tianjin, Luancheng (rural site), Handan and Jinan. Our results showed that the average light absorption coefficient at 365 nm (abs<sub>365</sub>) in Luancheng was approximately 1.1–3.5 times higher than those in urban ones. However, mass absorption efficiency displayed a distinctly different spatial pattern, with the strongest light-absorptivity (1.40 <inline-formula><mml:math id="M2" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 m<sup>2</sup> g<sup>−1</sup>) recorded in Jinan. Notably, average abs<sub>365</sub> in four urban sites exhibited a decline of <inline-formula><mml:math id="M6" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45 % from 2018 to 2023 compared to those previous observations. Furthermore, the light-absorptivity of water-soluble BrC was enhanced from clean to haze period at the most sampling sites along with the increasing <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio, indicating that nitrogenous organic compounds (NOCs) were important chromophores of water-soluble BrC in the NCP. Additionally, These NOCs were found to be closely associated with aqueous reactions, in which ammonia played an important role. These results elucidate the substantial contribution of NOCs to atmospheric BrC in the NCP, and further suggest a potentially important role of NH<sub>3</sub> emission control in alleviating wintertime haze and BrC pollution under moist conditions in this region.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42130704</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42477097</award-id>
</award-group>
<award-group id="gs3">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2023YFC3707401</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="d2e268">Light-absorbing organic aerosol, optically defined as brown carbon (BrC), is prevalent in the troposphere and efficiently absorbs solar radiation, thereby perturbing the global energy budget and influencing regional climate (Liu et al., 2020; Laskin et al., 2015; Samset et al., 2018). Recent modeling studies demonstrates that BrC is responsible for <inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> % of the direct radiative effect (DRE) caused by carbonaceous aerosols (Zeng et al., 2020; Feng et al., 2013; Zhang et al., 2017; Liu et al., 2015a). Most significantly, BrC even dominates the DRE in certain regions of the Earth, e.g., in the remote tropical upper troposphere (Zhang et al., 2020). However, these reported BrC DRE have large uncertainty, partly stemming from the poor understanding of optical properties and atmospheric evolution of BrC. Unlike black carbon (BC), BrC is characterized by a pronounced dependence of light-absorption on wavelength, with absorbance increasing steeply near UV wavelengths (Andreae and Gelencsér, 2006). Consequently, abundant BrC can also reduce the amount of ultraviolet sunlight reaching surface, subsequently altering tropospheric photochemistry. Indeed, growing evidence reveal a nonnegligible reduction in photolysis rates of the ozone and radicals with enhanced BrC load (Hammer et al., 2016; Gligorovski et al., 2015; Jo et al., 2016; He and Carmichael, 1999). Beyond the climatic and atmospheric effects, multiple BrC chromophores (e.g, polycyclic aromatic and nitro-heterocyclic compounds) also pose adverse health effects because of their strong oxidative potential (Fang et al., 2019; Daellenbach et al., 2020).</p>
      <p id="d2e281">Diverse sources of atmospheric BrC have been identified, including the various primary emissions and complex secondary formation. Primary BrC is known to be directly emitted from the incomplete combustion of biomass and other fuels (Washenfelder et al., 2015; Lack et al., 2012; Chen et al., 2017; Yan et al., 2017), of which optical properties are inherently related to combustion conditions and fuel types (Ni et al., 2021; Xie et al., 2017; Stockwell et al., 2015). And field measurements and laboratory studies indicated that the aromatics, conjugated systems, and highly functionalized species with high light-absorptivity can be secondarily formed via <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</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:mrow></mml:math></inline-formula> photooxidation of various precursors (Hems and Abbatt, 2018; Jiang et al., 2019; Finewax et al., 2018), or reactions initiated by ammonia/amines with atmospherically relevant carbonyls (Updyke et al., 2012; Powelson et al., 2014; Grace et al., 2020). These processes would generate abundant N-containing compounds (NOCs), which have been recognized as significant components of BrC (Lin et al., 2015; Yang et al., 2022; Wang et al., 2025a). Notably, the latest modeling study suggested that the NOCs dominate the global organic aerosol absorption, accounting for 18 % of global DRE induced by carbonaceous aerosols (Li et al., 2025). These absorptive NOCs are probably responsible for an enhanced light absorption of BrC in the upper boundary layer, as a result of their efficient formation in the lifting air masses (Wu et al., 2024a; Wu et al., 2024b). Moreover, the further aging processes would chemically modify the BrC composition, subsequently leading to either an increase (photodarkening) or decrease (photobleaching) in light-absorptivity of BrC chromophores (Wong et al., 2017; Jiang et al., 2022; Hems et al., 2021). These dynamic natures of BrC drive pronounced spatiotemporal heterogeneity in its chemical components and optical properties, propagating significant uncertainties in climate models that limit the reliable projection and mitigation of the climate effects caused by diverse BrC.</p>
      <p id="d2e310">Over the past decade, stringent emission control measures, such as shifting residential coal to natural gas/electricity, eliminating small coal-fired industrial boilers, and banning straw burning, etc., have been implemented in the North China Plain (NCP) (Chen et al., 2024b; Zheng et al., 2018). Given the substantial contribution of primary emissions to atmospheric BrC, BrC level in this region was expected to drastically decrease. Nevertheless, high loads of strongly light-absorbing BrC were still detected frequently in this region (Wang et al., 2025c; Chen et al., 2024a; Gong et al., 2023; Sun et al., 2026). Therefore, the sources and formation mechanism remain elusive in the NCP. Moreover, the atmospheric environment in this region also undergone significant changes, characterized particularly by enhanced atmospheric oxidation capacity driven by reduced NO<sub><italic>x</italic></sub> emissions and elevated O<sub>3</sub> levels, as well as persistently high NH<sub>3</sub> loadings due to insufficient controls on agricultural emissions (Li et al., 2019; Zheng et al., 2018; Zhu et al., 2023). Our recent studies demonstrate that such an ammonia-rich environment plays a key role in enhancing BrC absorption, primarily by reducing aerosol acidity and facilitating the formation of light-absorbing NOCs (Liu et al., 2023; Zhang et al., 2024). These findings imply that the primary drivers of BrC formation may have changed relative to those in the past. Motivated by this, atmospheric BrC in the NCP were collected during the 2023 winter and analyzed for the characteristics of water-soluble BrC. We investigated the spatial difference of chemical composition and light-absorption of water-soluble BrC, and discussed the role of NOCs in the BrC light absorption and their formation pathways.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Materials and Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Sampling</title>
      <p id="d2e355">The multi-site observations were synchronously conducted on the North China Plain from 15 November to 31 December 2023 (Fig. S1). Four of the sampling sites are located in urban areas, namely Beijing (BJ), Tianjin (TJ), Handan (HD) and Jinan (JN), which are surrounded by the traffic arteries and dense residential and commercial buildings. And the remaining one, adjacent to Luancheng (LC), serves as a rural station free from significant industrial influences. At each site, the PM<sub>2.5</sub> samples with a 12 h interval were collected onto prebaked (at 450 °C for 6 h) quartz filters using high- (1.13 m<sup>3</sup> min<sup>−1</sup>) or medium-volume (100 L min<sup>−1</sup>) air samplers; All the samplers located on the rooftops approximately 15–20 m above ground level. After sampling, the filter samples were wrapped in prebaked aluminum foils and stored in a freezer (at <inline-formula><mml:math id="M18" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18 °C) prior to analysis.</p>
      <p id="d2e407">Hourly concentrations of PM<sub>2.5</sub> and associated pollutants (e.g., NO<sub>2</sub>, O<sub>3</sub>, CO) at the sampling sites were obtained from the National Urban Air Quality Real-time Release Platform of China (<uri>https://air.cnemc.cn:18007/</uri>, last access: 6 April 2025), of which monitoring sites are adjacent to ours with a distance of <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> km. The meteorological data including ambient temperature (<inline-formula><mml:math id="M23" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>) and relative humidity (RH) were downloaded from National Climatic Data Center (<uri>https://www.ncei.noaa.gov/</uri>, last access: 6 April 2025).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Chemical analysis</title>
      <p id="d2e469">A piece of each filter was extracted with 40 mL ultrapure Milli-Q water (18.2 M<inline-formula><mml:math id="M24" display="inline"><mml:mi mathvariant="normal">Ω</mml:mi></mml:math></inline-formula>) under ultrasonication for 30 min. A part of the extract was used for the detection of water-soluble ions (SO<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M26" 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>, Cl<sup>−</sup>, Na<sup>+</sup>, NH<inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, K<sup>+</sup>, Mg<sup>2+</sup> and Ca<sup>2+</sup>) by using an ion chromatography; The remaining part was detected for the water-soluble organic carbon (WSOC) and water-soluble total nitrogen (WSTN) via a total organic carbon (TOC) analyzer (Model TOC-L CPH, Shimadzu, Japan). And the water-soluble organic nitrogen (WSON) can be quantified by deducting the water-soluble inorganic nitrogen (WSIN) from WSTN (i.e., WSON <inline-formula><mml:math id="M33" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> WSTN <inline-formula><mml:math id="M34" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> WSIN), thereby revealing variations in the <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratios of water-soluble components across different sampling sites (Fig. S2). A DRI-model 2001 thermal–optical carbon analyzer following the IMPROVE-A protocol was applied here to measure organic carbon (OC) and element carbon (EC) of PM<sub>2.5</sub>.</p>
      <p id="d2e606">The molecular compositions in PM<sub>2.5</sub> samples, including nitro-aromatic compounds (NACs, Table S1), polycyclic aromatic hydrocarbons (PAHs) and others organic tracers, were extracted with a mixture of dichloromethane and methanol (<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>/</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula>); Subsequently, the extracts were derivatized via derivatization reagent (a mixture of 50 <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>L of N,O-bis-(trimethylsilyl)trifluoroacetamide (BSTFA) and 1 % trimethylsilyl chloride and 10 <inline-formula><mml:math id="M41" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>L of pyridine) prior to GC-MS analyses. More details of the extraction, derivatization and the GC-MS analyses can refer to elsewhere (Wang et al., 2006; Wu et al., 2025a).</p>
      <p id="d2e658">Additionally, the aerodyne high-resolution time-of-flight aerosol mass spectrometer (HR-AMS) was applied here to characterize the imidazole-related fragments (e.g., C<sub>3</sub>H<sub>3</sub>N<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and C<sub>3</sub>H<sub>4</sub>N<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in a typical humid haze event (12 to 31 December of 2023, Fig. S3), following the method reported by Ge et al. (2024). It should be pointed out that above fragments may stem from other nitrogen-containing precursors, which inevitably introduces uncertainties into the quantification. Accordingly, the concentrations derived from these fragment ions cannot represent the actual abundances of the real molecules. Even so, the fragment ion levels can still indicate the variation trends of imidazole N-heterocycles. Because imidazole concentrations measured by orbitrap mass spectrometry in our previous field campaign showed a significant positive correlation with offline-AMS signals of C<sub>3</sub>H<sub>3</sub>N<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and C<sub>3</sub>H<sub>4</sub>N<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (Fig. S4).</p>
      <p id="d2e783">The details of the extraction and derivatization can be found elsewhere (Wu et al., 2024a). Briefly, a part of the PM<sub>2.5</sub> filter was extracted following the procedure similar to that of other water-soluble components; then the extracts were atomized using argon as the carrier gas, dehydrated by a diffusion drier, and ultimately quantified by HR-AMS. Each sample was continuously monitored by HR-AMS for <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> min to obtain stable signal, and above procedure was also applied to the blank samples to account for any potential contamination or background signals. A deep post-processing was conducted for the V-mode data in this study using the Igor-based Aerosol Mass Spectrometer Analysis Toolkit. The mass concentration of imidazole-related fragments was calculated as the follow:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M56" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">IMs</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">IMs</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi mathvariant="normal">WSOM</mml:mi></mml:mrow></mml:math></disp-formula>

          Where <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">IMs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denotes to the concentration of the imidazole-related fragments. <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">IMs</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is mass contribution of the imidazole-related fragments to the total fragments measured by HR-AMS; WSOM refers to atmospheric concentration of water-soluble organic matter (<inline-formula><mml:math id="M59" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>)</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Optical Absorption of BrC</title>
      <p id="d2e878">The light-absorbing chromophores (i.e., BrC) were also extracted with 10 mL ultrapure Milli-Q water, following the procedure for water-soluble ions. A UV–vis spectrometer was applied here to record the absorption spectra of all the extracts, which were finally converted into absorption coefficient (abs<sub><italic>λ</italic></sub>, M m<sup>−1</sup>) at a given wavelength (<inline-formula><mml:math id="M63" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>) using the following equation:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M64" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">abs</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mn mathvariant="normal">700</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi>L</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>l</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mi>ln⁡</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>

          Where <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the absorbance at wavelength <inline-formula><mml:math id="M66" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (nm), <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>v</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> refer to the volume of the extractant and air through corresponding to filter punches, respectively. The optical path length is 1 cm (i.e, <inline-formula><mml:math id="M69" display="inline"><mml:mi>l</mml:mi></mml:math></inline-formula>). From abs<sub><italic>λ</italic></sub>, the mass absorption coefficient (MAE<sub><italic>λ</italic></sub>, m<sup>2</sup> g<sup>−1</sup>) can be characterized as:

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M74" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">MAE</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">abs</mml:mi><mml:mi mathvariant="italic">λ</mml:mi></mml:msub></mml:mrow><mml:mi>C</mml:mi></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          Where <inline-formula><mml:math id="M75" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is the mass concentration of water-soluble organic carbon.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Random forest analysis for water-soluble organic nitrogen</title>
      <p id="d2e1093">Random forest (RF), as a powerful tool for regression and prediction (Hu et al., 2017; Vu et al., 2019), was employed here to elucidate the relationships between secondary WSON (WSONsec) and potential factors (NH<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<sub>2</sub>, O<sub>3</sub>, ALWC, pH and meteorological factors). The importance of each factor to WSONsec can be determined by a SHAP method originally proposed by Lundberg and Lee (2017). Rooted in cooperative game theory, SHAP framework as a model-agnostic additive feature attribution method enables an in-depth exploration of interaction effects and effectively alleviates poor interpretability of machine learning models. In the RF model design, 70 % of the dataset including all the samples from the five monitoring sites was randomly divided into a training subset to construct the RF model, and the remaining 30 % (i.e., test set) was used to assess the model performance. Following systematic hyperparameter optimization, the decision tree (<inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>n</mml:mi><mml:mi mathvariant="normal">tree</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) was set to 300 to balance model performance and computational efficiency; and number of variables split at each node (<inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>n</mml:mi><mml:mi mathvariant="normal">mtry</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) was limited to 12 to avoid overfitting. Additionally, a 10-fold cross-validation strategy was adopted here to optimize model parameters and estimate model performance. The RF model was constructed using the “randomForest” R package, of which performance was evaluated by coefficient of determination (<inline-formula><mml:math id="M81" 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>), mean square error (MSE) or root-mean-square error (RMSE) and mean absolute error (MAE). As summarized in Table S2, the simulated WSONsec corrected strongly with observed ones, and the error metric remained at low levels; Thess indicated that the model could reconstruct commendably the variations of WSONsec in this study.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Theoretical estimation of particulate fraction of NACs (<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>)</title>
      <p id="d2e1181">Since gas-phase nitro-aromatic compounds (NACs) were not detected in this study, the particulate-phase fraction (<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of NACs was calculated based on absorption equilibrium theory (Pankow et al., 2001; Zuend and Seinfeld, 2012), and the specific calculation method referred to that reported by Chen et al. (2025). As shown in the following equations:

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M84" 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 class="stylechange" displaystyle="true"/><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi mathvariant="normal">PM</mml:mi></mml:mrow><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi mathvariant="normal">PM</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></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:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi mathvariant="normal">PM</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">760</mml:mn><mml:mo>×</mml:mo><mml:mi>f</mml:mi><mml:mo>×</mml:mo><mml:mi>R</mml:mi><mml:mo>×</mml:mo><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup><mml:mo>×</mml:mo><mml:msub><mml:mi>P</mml:mi><mml:mi>V</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>M</mml:mi><mml:mo>×</mml:mo><mml:mi mathvariant="italic">ξ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          Herein, <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the mass concentrations of the organic molecule in gas and particle phase, respectively. <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> refers to gas–particle partitioning coefficient, and is determine by many factors in Eq. (5). Specifically, <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi>V</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the saturation pressure (Pa), which is 0.00378 torr for 4-nitrophenol (at 298 K).  <inline-formula><mml:math id="M89" display="inline"><mml:mi mathvariant="italic">ξ</mml:mi></mml:math></inline-formula> is the activity coefficient of the species, adopting from the values reported by Wang et al. (2019). <inline-formula><mml:math id="M90" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> refers to the molecular weight of NAC species (g mol<sup>−1</sup>). Additionally, <inline-formula><mml:math id="M92" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> is the gas constant (8.314 J (mol K)<sup>−1</sup>), <inline-formula><mml:math id="M94" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> is the temperature (K), <inline-formula><mml:math id="M95" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> denotes the fraction of organic matter in particle, and PM is the mass concentration of PM<sub>2.5</sub>.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Result and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Spatial variation of PM<sub>2.5</sub> Chemical Composition</title>
      <p id="d2e1476">As shown in Table 1 and Fig. S3, the PM<sub>2.5</sub> concentration across the North China Plain (NCP) exhibited significant spatial heterogeneity, ranging from 4.0 to 223.7 <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>. Specifically, the highest average PM<sub>2.5</sub> load was recorded in JN (94.1 <inline-formula><mml:math id="M102" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 37.8 <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>), partially attributed to unfavorable topographic conditions and intensive anthropogenic emissions. The average PM<sub>2.5</sub> level at remaining sampling sites decreased gradually from south to north. Notably, the PM<sub>2.5</sub> concentration in Beijing during the campaign was only a quarter of that recorded a decade ago (158 <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>), indicating a notable air quality improvement in BJ over recent years. Even so, multi-day haze episodes (PM<sub>2.5</sub> <inline-formula><mml:math id="M110" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 75 <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) still occurred frequently in BJ (Fig. S3), of which hourly peak concentration even reached up to 203 <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, about 3-fold of National Air Quality Standard grade-II (75 <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>). Additionally, these events were also observed simultaneously at other sites, suggesting that regional PM<sub>2.5</sub> pollution remains a persistent challenge during winter across the NCP, particularly in its southern region.</p>
      <p id="d2e1670">The spatiotemporal differences in chemical compositions, sources of organic matter (OM) in PM<sub>2.5</sub> among sampling sites are illustrated in Fig. 1. As the major component of PM<sub>2.5</sub>, water soluble ions (WSIs) accounted for approximately 30 %–53 % of PM<sub>2.5</sub>; Similar to the spatial pattern of PM<sub>2.5</sub>, WSIs also exhibited high loads in JN (40.4 <inline-formula><mml:math id="M122" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 23.2 <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) and HD (44.1 <inline-formula><mml:math id="M125" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 34.3 <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>), which were <inline-formula><mml:math id="M128" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.2–4 fold of those measured in other sites. From Fig. 1, nitrate was the most abundant ion across the NCP, accounting for 14 %–27 % of PM<sub>2.5</sub>, followed by sulfate (5 %–9 %) and ammonium (4 %–11 %), respectively. Compared to those in urban sites, relative abundance of SNA (SO<inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M131" 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 NH<inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in rural site (LC) moderately enhanced by 10 %–23 %, indicating a significant influence of secondary aerosol formation in the rural area. Furthermore, a relatively high concentration of chloride was detected among the sampling sites, even with a molarity being <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula>-fold of that of sulfate (Fig. S5a). A strong correlation between chloride and levoglucosan+Benzo[k]fluoranthene (BkF) across the sampling sites (<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.97</mml:mn></mml:mrow></mml:math></inline-formula>) implied that combustion emissions were the primary source for the abundant chloride in the NCP (Fig. S5b). These abundant chlorides could promote heterogeneous formation of sulfate as evidenced by a robust relationship chloride and SOR (<inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) (Fig. S5c). This finding was consistent with the results of our laboratory experiments (Wang et al., 2025b, 2016), which demonstrated that the abundant chloride could significantly enhance the uptake of NO<sub>2</sub> by interfacial electrostatic attraction, subsequently accelerating sulfate formation.</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e1897">Optical properties of BrC, mass concentrations of chemical composition in PM<sub>2.5</sub>, and meteorological parameters at sampling sites.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Beijing</oasis:entry>
         <oasis:entry colname="col3">Tianjin</oasis:entry>
         <oasis:entry colname="col4">Luancheng</oasis:entry>
         <oasis:entry colname="col5">Handan</oasis:entry>
         <oasis:entry colname="col6">Jinan</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6">(i) Meteorological parameters and gaseous pollutants </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M138" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula> (°C)</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M139" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.1 <inline-formula><mml:math id="M140" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.6</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M141" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.2 <inline-formula><mml:math id="M142" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.9</oasis:entry>
         <oasis:entry colname="col4">1.2 <inline-formula><mml:math id="M143" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6.3</oasis:entry>
         <oasis:entry colname="col5">1.7 <inline-formula><mml:math id="M144" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6.6</oasis:entry>
         <oasis:entry colname="col6">3.1 <inline-formula><mml:math id="M145" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RH (%)</oasis:entry>
         <oasis:entry colname="col2">49 <inline-formula><mml:math id="M146" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21</oasis:entry>
         <oasis:entry colname="col3">50 <inline-formula><mml:math id="M147" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 19</oasis:entry>
         <oasis:entry colname="col4">54 <inline-formula><mml:math id="M148" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 22</oasis:entry>
         <oasis:entry colname="col5">59 <inline-formula><mml:math id="M149" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21</oasis:entry>
         <oasis:entry colname="col6">54 <inline-formula><mml:math id="M150" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 23</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">O<sub>3</sub>(<inline-formula><mml:math id="M152" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>)</oasis:entry>
         <oasis:entry colname="col2">29 <inline-formula><mml:math id="M154" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20</oasis:entry>
         <oasis:entry colname="col3">31 <inline-formula><mml:math id="M155" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18</oasis:entry>
         <oasis:entry colname="col4">31 <inline-formula><mml:math id="M156" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18</oasis:entry>
         <oasis:entry colname="col5">28 <inline-formula><mml:math id="M157" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 17</oasis:entry>
         <oasis:entry colname="col6">35 <inline-formula><mml:math id="M158" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 26</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<sub>2</sub>(<inline-formula><mml:math id="M160" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>)</oasis:entry>
         <oasis:entry colname="col2">41 <inline-formula><mml:math id="M162" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 26</oasis:entry>
         <oasis:entry colname="col3">48 <inline-formula><mml:math id="M163" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 31</oasis:entry>
         <oasis:entry colname="col4">44 <inline-formula><mml:math id="M164" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 23</oasis:entry>
         <oasis:entry colname="col5">46 <inline-formula><mml:math id="M165" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18</oasis:entry>
         <oasis:entry colname="col6">48 <inline-formula><mml:math id="M166" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 60</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">SO<sub>2</sub>(<inline-formula><mml:math id="M168" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>)</oasis:entry>
         <oasis:entry colname="col2">4 <inline-formula><mml:math id="M170" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5</oasis:entry>
         <oasis:entry colname="col3">4.7 <inline-formula><mml:math id="M171" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.4</oasis:entry>
         <oasis:entry colname="col4">8.8 <inline-formula><mml:math id="M172" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.5</oasis:entry>
         <oasis:entry colname="col5">5.9 <inline-formula><mml:math id="M173" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.8</oasis:entry>
         <oasis:entry colname="col6">10.0 <inline-formula><mml:math id="M174" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11.0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6">(ii) Mass concentrations of PM<sub>2.5</sub> and its chemical composition (<inline-formula><mml:math id="M176" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">PM<sub>2.5</sub></oasis:entry>
         <oasis:entry colname="col2">38 <inline-formula><mml:math id="M179" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 36</oasis:entry>
         <oasis:entry colname="col3">52 <inline-formula><mml:math id="M180" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 50</oasis:entry>
         <oasis:entry colname="col4">74 <inline-formula><mml:math id="M181" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 46</oasis:entry>
         <oasis:entry colname="col5">80 <inline-formula><mml:math id="M182" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 49</oasis:entry>
         <oasis:entry colname="col6">94 <inline-formula><mml:math id="M183" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 38</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<inline-formula><mml:math id="M184" 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></oasis:entry>
         <oasis:entry colname="col2">5.4 <inline-formula><mml:math id="M185" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 7.3</oasis:entry>
         <oasis:entry colname="col3">13.0 <inline-formula><mml:math id="M186" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 14.6</oasis:entry>
         <oasis:entry colname="col4">19.0 <inline-formula><mml:math id="M187" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18.2</oasis:entry>
         <oasis:entry colname="col5">22.7 <inline-formula><mml:math id="M188" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20.8</oasis:entry>
         <oasis:entry colname="col6">17.3 <inline-formula><mml:math id="M189" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 13.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SO<inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.8 <inline-formula><mml:math id="M191" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.0</oasis:entry>
         <oasis:entry colname="col3">4.6 <inline-formula><mml:math id="M192" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.0</oasis:entry>
         <oasis:entry colname="col4">6.7 <inline-formula><mml:math id="M193" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 7.0</oasis:entry>
         <oasis:entry colname="col5">7.0 <inline-formula><mml:math id="M194" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.8</oasis:entry>
         <oasis:entry colname="col6">7.5 <inline-formula><mml:math id="M195" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NH<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.6 <inline-formula><mml:math id="M197" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.2</oasis:entry>
         <oasis:entry colname="col3">5.7 <inline-formula><mml:math id="M198" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.9</oasis:entry>
         <oasis:entry colname="col4">8.2 <inline-formula><mml:math id="M199" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 8.6</oasis:entry>
         <oasis:entry colname="col5">9.1 <inline-formula><mml:math id="M200" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 8.0</oasis:entry>
         <oasis:entry colname="col6">7.3 <inline-formula><mml:math id="M201" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Cl<sup>−</sup></oasis:entry>
         <oasis:entry colname="col2">1.0 <inline-formula><mml:math id="M203" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.7</oasis:entry>
         <oasis:entry colname="col3">3.2 <inline-formula><mml:math id="M204" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.7</oasis:entry>
         <oasis:entry colname="col4">2.8 <inline-formula><mml:math id="M205" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.7</oasis:entry>
         <oasis:entry colname="col5">2.9 <inline-formula><mml:math id="M206" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.9</oasis:entry>
         <oasis:entry colname="col6">2.3 <inline-formula><mml:math id="M207" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">OM</oasis:entry>
         <oasis:entry colname="col2">9.1 <inline-formula><mml:math id="M208" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.2</oasis:entry>
         <oasis:entry colname="col3">7.9 <inline-formula><mml:math id="M209" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.7</oasis:entry>
         <oasis:entry colname="col4">18.5 <inline-formula><mml:math id="M210" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11</oasis:entry>
         <oasis:entry colname="col5">18.7 <inline-formula><mml:math id="M211" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10.7</oasis:entry>
         <oasis:entry colname="col6">16.3 <inline-formula><mml:math id="M212" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 7.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">EC</oasis:entry>
         <oasis:entry colname="col2">2.7 <inline-formula><mml:math id="M213" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.4</oasis:entry>
         <oasis:entry colname="col3">2.8 <inline-formula><mml:math id="M214" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.7</oasis:entry>
         <oasis:entry colname="col4">4.4 <inline-formula><mml:math id="M215" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.5</oasis:entry>
         <oasis:entry colname="col5">3.1 <inline-formula><mml:math id="M216" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.9</oasis:entry>
         <oasis:entry colname="col6">4.2 <inline-formula><mml:math id="M217" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">WSOC</oasis:entry>
         <oasis:entry colname="col2">3.2 <inline-formula><mml:math id="M218" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.8</oasis:entry>
         <oasis:entry colname="col3">4.9 <inline-formula><mml:math id="M219" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.1</oasis:entry>
         <oasis:entry colname="col4">7.3 <inline-formula><mml:math id="M220" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.0</oasis:entry>
         <oasis:entry colname="col5">7.5 <inline-formula><mml:math id="M221" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.1</oasis:entry>
         <oasis:entry colname="col6">4.8 <inline-formula><mml:math id="M222" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.7</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">WSON</oasis:entry>
         <oasis:entry colname="col2">0.65 <inline-formula><mml:math id="M223" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.64</oasis:entry>
         <oasis:entry colname="col3">1.2 <inline-formula><mml:math id="M224" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.1</oasis:entry>
         <oasis:entry colname="col4">2.5 <inline-formula><mml:math id="M225" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.6</oasis:entry>
         <oasis:entry colname="col5">2.3 <inline-formula><mml:math id="M226" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.6</oasis:entry>
         <oasis:entry colname="col6">1.3 <inline-formula><mml:math id="M227" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.8</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6">(iii) Optical properties of BrC, ALWC and acidity of PM<sub>2.5</sub></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">abs<sub>365</sub> (Mm<sup>−1</sup>)</oasis:entry>
         <oasis:entry colname="col2">2.3 <inline-formula><mml:math id="M231" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.9</oasis:entry>
         <oasis:entry colname="col3">5.7 <inline-formula><mml:math id="M232" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.8</oasis:entry>
         <oasis:entry colname="col4">8.0 <inline-formula><mml:math id="M233" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.7</oasis:entry>
         <oasis:entry colname="col5">8.2 <inline-formula><mml:math id="M234" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.0</oasis:entry>
         <oasis:entry colname="col6">6.9 <inline-formula><mml:math id="M235" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MAE (m<sup>2</sup> g<sup>−1</sup>)</oasis:entry>
         <oasis:entry colname="col2">0.71 <inline-formula><mml:math id="M238" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.5</oasis:entry>
         <oasis:entry colname="col3">1.12 <inline-formula><mml:math id="M239" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.05</oasis:entry>
         <oasis:entry colname="col4">1.10 <inline-formula><mml:math id="M240" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.04</oasis:entry>
         <oasis:entry colname="col5">1.05 <inline-formula><mml:math id="M241" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02</oasis:entry>
         <oasis:entry colname="col6">1.4 <inline-formula><mml:math id="M242" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">pH</oasis:entry>
         <oasis:entry colname="col2">5.6 <inline-formula><mml:math id="M243" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.1</oasis:entry>
         <oasis:entry colname="col3">3.8 <inline-formula><mml:math id="M244" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.8</oasis:entry>
         <oasis:entry colname="col4">3.3 <inline-formula><mml:math id="M245" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.4</oasis:entry>
         <oasis:entry colname="col5">4.1 <inline-formula><mml:math id="M246" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.2</oasis:entry>
         <oasis:entry colname="col6">4.0 <inline-formula><mml:math id="M247" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ALWC (<inline-formula><mml:math id="M248" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>)</oasis:entry>
         <oasis:entry colname="col2">9.7 <inline-formula><mml:math id="M250" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21.6</oasis:entry>
         <oasis:entry colname="col3">21.0 <inline-formula><mml:math id="M251" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 38</oasis:entry>
         <oasis:entry colname="col4">36 <inline-formula><mml:math id="M252" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 74</oasis:entry>
         <oasis:entry colname="col5">47 <inline-formula><mml:math id="M253" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 72</oasis:entry>
         <oasis:entry colname="col6">41 <inline-formula><mml:math id="M254" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 70</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d2e1909">ALWC: aerosol liquid water content; ALWC and pH were simulated by thermodynamic model (ISORROPIA-II), details can be found in Sect. S5.</p></table-wrap-foot></table-wrap>

      <p id="d2e3261">The average concentration of OM ranged from 7.9 <inline-formula><mml:math id="M255" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.7 to 18.7 <inline-formula><mml:math id="M256" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10.7 <inline-formula><mml:math id="M257" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, accounting for 17 %–25 % of PM<sub>2.5</sub>. Although OM was a predominant species in PM<sub>2.5</sub> at most sites, its spatial distribution differed slightly from that of PM<sub>2.5</sub>, with high loads in LC (18.5 <inline-formula><mml:math id="M262" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11 <inline-formula><mml:math id="M263" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) and HD (18.7 <inline-formula><mml:math id="M265" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10.7 <inline-formula><mml:math id="M266" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>). To determine the sources of the abundant OM, a PMF was applied here and identified three types OM sources (Fig. S6, Sect. S1). From Fig. 1, a significant fraction of OM (40 %–55 %) at urban sites was associated with secondary formation, comparable to that in northern regions of China (50 %) (Chen et al., 2024b). In contrast, combustion-derived primary OM accounted for less than 40 % of the total OM. This finding was consistent with the field observations,  which demonstrated a widespread decline in primary OM in NCP during 2013–2020 due to the significant reduction in residential fuel burning (Chen et al., 2024b). Notably, about 55 % of OM at rural site was derived from combustion, reflecting an urban-rural variation in sources.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e3383">Chemical composition of PM<sub>2.5</sub> and sources for organic matters (OM) at different sampling sites. The mass concentration data correspond to PM<sub>2.5</sub>. The maps are the reproductions from © Mapbox (<uri>https://account.mapbox.com/</uri>, last access: 3 December 2025).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Spatial variability in optical properties of BrC</title>
      <p id="d2e3421">Figure 2a displays the average absorption spectra of WSOC across the sampling sites, which exhibits the marked feature of BrC with the reduced light absorption from the ultraviolet to the visible ranges. As illustrated in Table 1 and Fig. 2, the light absorption coefficient at 365 nm (abs<sub>365</sub>) displayed a spatial pattern similar to that of organic matter (OM) across the five sampling sites. Specifically, the highest average abs<sub>365</sub>was observed at LC site, with average of (8.0 <inline-formula><mml:math id="M272" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.7 Mm<sup>−1</sup>), followed by HD (7.9  <inline-formula><mml:math id="M274" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5.0 Mm<sup>−1</sup>), JN (6.9 <inline-formula><mml:math id="M276" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.0 Mm<sup>−1</sup>), TJ (5.7 <inline-formula><mml:math id="M278" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.8 Mm<sup>−1</sup>) and BJ (2.3 <inline-formula><mml:math id="M280" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.9 Mm<sup>−1</sup>), respectively. Across the sampling sites, abs<sub>365</sub> correlated robustly (<inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.73</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M284" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) with levoglucosan being a known tracer for biomass burning (BB). This implied that water-soluble BrC in the NCP was significantly affected by fresh emissions from BB, which aligns with the prior observations in China (Li et al., 2022b; Desyaterik et al., 2013; Li et al., 2023). Additionally, the BB emission was more pronounced in rural areas, as indicated by a higher mass fraction of levoglucosan to OM (0.67 <inline-formula><mml:math id="M285" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.39 %), which was approximately 2.1 to 5 times higher than those in urban areas. These findings highlight the significant impact of anthropogenic combustion on air quality in the rural NCP. From Fig. 2b, the average light-absorption of urban BrC in the NCP exhibited a decline of <inline-formula><mml:math id="M286" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45 % from 10.7 <inline-formula><mml:math id="M287" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.0 Mm<sup>−1</sup> in 2018 to 5.8 <inline-formula><mml:math id="M289" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.2 Mm<sup>−1</sup> in 2023. Beijing exhibited a more substantial reduction, where the abs<sub>365</sub> was only 16 % of that recorded a decade ago (Fig. 2b). Even so, the averaged abs<sub>365</sub> in the NCP still remains higher than that in Nanjing, Guangzhou and urban areas in developed countries (Table S3).</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e3648">Optical properties of BrC at each sampling site. <bold>(a, c)</bold> Average absorption spectra and mass absorption coefficient of WSOC; <bold>(b, d)</bold> Comparison of abs<sub>365</sub> and MAE<sub>365</sub> in different cities of China (NJ, XA and GZ represent Nanjing, Xi'an and Guangzhou; Superscripts indicate the corresponding years, for instance, the superscript “11” refers to 2011. The datasets of <bold>(b)</bold> and <bold>(d)</bold> were derived from the literature, and given in Table S4).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f02.png"/>

        </fig>

      <p id="d2e3688">As a metric for characterizing the light absorptivity of BrC, the MAE at 365 nm (MAE<sub>365</sub>) was quantified by the linear regression slope of abs<sub>365</sub> against WSOC. As illustrated in Fig. 2c, MAE<sub>365</sub> exhibits a distinctly different spatial pattern relative to abs<sub>365</sub>. A strikingly high MAE<sub>365</sub> value was measured in JN (1.4 <inline-formula><mml:math id="M300" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.04 m<sup>2</sup> g<sup>−1</sup>), on par with those found in severely polluted regions like Xingtai, Xi'an and Delhi, India (1.2–1.6 m<sup>2</sup> g<sup>−1</sup>, in the cold season) (Li et al., 2023; Wu et al., 2020; Kirillova et al., 2014); And the MAE<sub>365</sub> value also falls within the range for documented BrC emitted from residential coal combustion (e.g., 1.20–1.59 m<sup>2</sup> g<sup>−1</sup> for bituminous coal) (Ni et al., 2021), suggesting that coal combustion is one of the potential sources of atmospheric BrC in JN. Additionally, TJ, LC and HD shared a comparable MAE<sub>365</sub> value of approximately 1.1 m<sup>2</sup> g<sup>−1</sup>, which closely matches the values associated with biomass burning-derived BrC (1.2 <inline-formula><mml:math id="M311" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.3 m<sup>2</sup> g<sup>−1</sup>) (Cao et al., 2021). This finding further indicated a significant effect of biomass burning on the wintertime BrC in the NCP, which can be corroborated by the concentration-weighted trajectory (CWT) analysis. As shown in Fig. 3, high CWT loadings for abs<sub>365</sub> were predominantly associated with regions characterized by concentrated fire hotspots, especially in LC, HD and their adjacent areas. Of note, the MAE<sub>365</sub> of the BrC in BJ was the lowest (0.71 <inline-formula><mml:math id="M316" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 m<sup>2</sup> g<sup>−1</sup>), only half that of JN. This relatively weak light absorptivity of BrC in BJ may be attributable to substantial vehicle emissions, as BrC from this source typically exhibits relatively low MAE values, ranging from approximately 0.35 to 0.71 m<sup>2</sup> g<sup>−1</sup> (Tang et al., 2020; Huang et al., 2022). Another possibility is that the aerosol in BJ was more age, because BrC light-absorption would decay in the aerosol aging process as revealed by observational and experimental findings (Hems et al., 2021; Qiu et al., 2024). This can be confirmed by the <inline-formula><mml:math id="M321" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Benzo</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="normal">e</mml:mi><mml:mo>]</mml:mo><mml:mi mathvariant="normal">pyrene</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Benzo</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="normal">a</mml:mi><mml:mo>]</mml:mo><mml:mi mathvariant="normal">pyrene</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Benzo</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="normal">e</mml:mi><mml:mo>]</mml:mo><mml:mi mathvariant="normal">pyrene</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> ratio (<inline-formula><mml:math id="M322" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">BaP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>). Since BaP is easily degraded via atmospheric oxidation while BeP is chemically stable, a higher <inline-formula><mml:math id="M323" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">BaP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> value indicates more aged atmospheric aerosols. As shown in Fig. S7a, the <inline-formula><mml:math id="M324" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">BaP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> ratio in BJ was relatively higher than those at other sampling sites. Moreover, a negative correlation between <inline-formula><mml:math id="M325" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">BaP</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">BeP</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and MAE<sub>365</sub>further supported this hypothesis (Fig. S7b). In Fig. 2d, we can note that unlike the temporal evolution of abs<sub>365</sub>, the MAE<sub>365</sub> of the water-soluble BrC at most sampling sites undergone indistinctive variations in response to the reduction in anthropogenic emission.</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e4100">The CWT analysis of BrC at sampling sites along with fire hotspot. Fire hotspot data from Fire Information for Resource Management System (FIRMS) were applied to evaluate open biomass burning intensity during the campaign. The data were acquired from the Visible Infrared Imaging Radiometer Suite (VIIRS) sensor and processed using a fire detection algorithm to identify active fire hotspots.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f03.png"/>

        </fig>

      <p id="d2e4109">As depicted in Fig. 4a, the optical properties of water-soluble BrC in different periods are plotted in the AAE-MAE<sub>405</sub> (log scale) space, with reference to the optically defined BrC classes proposed by Saleh (2020). On average, the water-soluble BrC across the sampling sites exhibits optical characteristics consistent with biomass-burning and coal-combustion sources, falling into the “weakly” absorbing BrC class. This observation reinforced remarkable impacts of combustion sources on BrC in the NCP. Of particular note, the BrC light-absorptivity was enhanced from clean (PM<inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&lt;</mml:mo></mml:mrow></mml:math></inline-formula> 75 <inline-formula><mml:math id="M331" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) to haze (PM<sub>2.5</sub> <inline-formula><mml:math id="M334" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 75 <inline-formula><mml:math id="M335" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>) periods at most sampling sites, coinciding with the increasing <inline-formula><mml:math id="M337" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio (Fig. 4a). And a positive correlation between <inline-formula><mml:math id="M338" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio and abs<sub>365</sub> was also found across the NCP (Fig. 4b), indicating that NOCs likely serve as the potential chromophores modulating BrC optical properties in this region (Figue S8). Accordingly, the high <inline-formula><mml:math id="M340" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio was also associated with an elevated WSOC/OC ratio (Fig. 4b), implying that the secondary formation was likely the predominant source of the N-containing chromophores in the NCP.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e4238">Graphical representation of optical-based BrC classes in log<sub>10</sub>(MAE<sub>405</sub>)-AAE space <bold>(a)</bold>. The shaded regions represent very weakly light-absorbing BrC (VW-BrC), weakly light-absorbing BrC (W-BrC), moderately light-absorbing BrC (M-BrC), strongly light-absorbing BrC (S-BrC), and absorbing BC, respectively. Panel <bold>(b)</bold> shows the linear fit regressions for abs<sub>365</sub> with <inline-formula><mml:math id="M344" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio (Diamonds indicate the averaged abs<sub>365</sub> and <inline-formula><mml:math id="M346" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio of all sites in each binned <inline-formula><mml:math id="M347" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> interval, with bars representing standard deviations).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Secondary formation N-containing compounds in the NCP</title>
      <p id="d2e4334">To obtain the contribution of secondary formation to the water-soluble organic nitrogen, a tracer method analogous to that used for estimating secondary organic carbon (SOC) with EC as a tracer was adopted here (Sect. S2 in the Supplement). This approach assumes that combustion-related primary WSON (WSONpri) share the common sources with EC and can be approximated using a representative primary <inline-formula><mml:math id="M348" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">WSON</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> ratio. Based on the sensitivity tests (Table S4), the primary <inline-formula><mml:math id="M349" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">WSON</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> ratios used here can capture temporal variations of the WSONpri, which positively correlated with CO at all sampling sites. Even so, the secondary WSON (WSONsec) may still be overestimated because a fraction of WSONpri may arise from non-combustion sources. Therefore, the derived secondary fractions here should be interpreted as semi-quantitative estimates rather than precise source apportionments. From the results illustrated in Fig. 5a, a dominant role of secondary formation in WSON accumulation was observed across five sites. Specifically, secondary WSON in BJ explained more than approximately 64 <inline-formula><mml:math id="M350" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21 % of the total WSON, which was comparable to those at other urban sites but was approximately 1.2-fold of that in LC. Such spatial pattern was attribute to the enhanced primary emission (e.g., biomass burning) in rural site. Additionally, the fractional contribution of WSONsec increased with the rising PM<sub>2.5</sub> levels (Fig. S8) across sampling sites, particularly in BJ. Above findings further highlighted the critical role of secondary formation in regulating the abundance of strongly light-absorbing N-containing chromophores during haze periods.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e4379">Aqueous formation of N-containing compounds in the NCP.  Fractional contribution of primary water-soluble organic nitrogen (WSONpri) and secondary WSON (WSONsec) to the total <bold>(a)</bold>; SHAP feature importance assessment for the key factors affecting WSONsec <bold>(b)</bold>; Linear correlation between IMs-related fragments and NH<inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> with different PM<sub>2.5</sub> loads (the fragment signals do not represent absolute molecular abundances) <bold>(c)</bold>; panel <bold>(d)</bold> shows the linear fit regressions for WSONsec <inline-formula><mml:math id="M354" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> WSON with pH value across the NCP. (Circles in <bold>c</bold> and <bold>d</bold> show grouped mean statistics over all sampling site).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f05.png"/>

        </fig>

<sec id="Ch1.S3.SS3.SSS1">
  <label>3.3.1</label><title>Aerosol aqueous formation of light-absorbing NOCs</title>
      <p id="d2e4442">The secondary WSON formation can be affected by multiple factors, e.g., NH<inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<sub>2</sub>, O<sub>3</sub>, ALWC, pH, NACs and meteorological factors. To investigate the contributions of these factors to WSONsec, a random forest analysis was conducted here and demonstrated that atmospheric WSONsec in the NCP was largely affected by NH<inline-formula><mml:math id="M358" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M359" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 48 %) and ALWC (<inline-formula><mml:math id="M360" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 28 %). Given the limited capability of the RF model to capture interactive and nonlinear relationships between driving factors and WSONsec, a generalized additive model (GAM) was applied here, which is a nonparametric modeling framework (Sect. S3). As shown in Fig. S9, the GAM model can robustly rebuild the WSONsec variation, and consistently identified NH<inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and ALWC as the primary driving factors of WSONsec. These results only reflect the statistical relationships among above factors and may not fully capture the responses of the actual atmosphere. Accordingly, we also analyzed the ionic fragments of hydroxy methanesulfonic acid (MSA) predominantly formed via aqueous-phase reactions, which exhibited a significant positive correlation with WSONsec during humid haze episode (Fig. S10). All the above evidence indicated that WSONsec formation was closely linked to the aqueous processing in this region. Above phenomenon is presumably prevalent across China, as it has been observed in the rural site (Xianghe) in the NCP, Yangtze River Delta, the Guanzhong Plain, and even the upper boundary layer (Liu et al., 2023; Wu et al., 2024a; Xiao et al., 2025). Previously, aqueous-phase reactions via <inline-formula><mml:math id="M362" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-dicarbonyls (e..g, methylglyoxal and glyoxal) with NH<sub>3</sub> have been identified as an important formation pathway for N-heterocyclic species (e.g., imidazoles, IMs) (Yang et al., 2024; Aiona et al., 2017; Lin et al., 2015), of which yield can be regulated by the chemical forms of ammonium in aerosol. Specially, the uptake coefficient of methylglyoxal or glyoxal (the prevalent <inline-formula><mml:math id="M364" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-dicarbonyls in the atmosphere) on (NH<sub>4</sub>)<sub>2</sub>SO<sub>4</sub> seed was significantly higher than on NH<sub>4</sub>HSO<sub>4</sub> seed, thereby leading to an enhanced yield of N-heterocycles and their oligomers (Li et al., 2021b). Whereas it has been confirmed theoretically that the aerosol across five sites were characterized by abundant (NH<sub>4</sub>)<sub>2</sub>SO<sub>4</sub>and NH<sub>4</sub>NO<sub>3</sub> as shown in Fig. S11a and Sect. S4. These hygroscopic (NH<sub>4</sub>)<sub>2</sub>SO<sub>4</sub>particles would promote N-containing compounds formation via NH<sub>3</sub>-mediated aqueous-phase chemistry. To further validate above assumption, IMs-related fragments (e.g., C<sub>3</sub>H<sub>3</sub>N<inline-formula><mml:math id="M381" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and C<sub>3</sub>H<sub>4</sub>N<inline-formula><mml:math id="M384" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) were measured by offline AMS analysis during a humid haze episode across the NCP. Although this approach does not provide actual ambient concentrations of individual imidazole compounds, the fragment signals can serve as supportive indicators to characterize the evolution of imidazole-related species, because they exhibit strong linear correlations with the measured ambient concentrations of the corresponding compounds. (Fig. S4). During this event, the <inline-formula><mml:math id="M385" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">ALWC</mml:mi><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ALWC</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was approximately 1.5-fold of that observed in the remaining periods (Fig. S11b), indicating that aerosols were far more likely to be in the liquid phase during this period. In the atmosphere, IMs can be either directly emitted from biomass burning or secondarily produced via aqueous reactions (Gao et al., 2021). As illustrated in Figs. 5c and S12, IMs-related fragments weakly correlated with the levoglucosan+BkF (<inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.02</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M387" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) but strongly with ammonium (<inline-formula><mml:math id="M388" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.93</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M389" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>), suggesting that a major fraction of the IMs-like heterocyclic compounds was secondarily formed during the humid event. As the haze episode evolved, the <inline-formula><mml:math id="M390" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">IMs</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">WSON</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M391" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>) ratio increased dramatically across the NCP, further suggesting an important role of NH<sub>3</sub>-induced chemistry in NOCs formation under moist environments.</p>
      <p id="d2e4838">Additionally, aerosol acidity also modulated the WSON formation, with relative importance being <inline-formula><mml:math id="M393" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 8 % (Fig. 5b). Figure 5d clearly demonstrates a negative correlation between the mass fraction of WSONsec in the total WSON and aerosol pH, indicating that acidic condition likely favors NOCs formation. It is possible that ammonia would be more readily partitioned into acidic aerosol, thereby promoting the formation of NOCs. Consistent with this hypothesis, our estimation of the gas-to-particle partitioning coefficient for NH<sub>3</sub> (<inline-formula><mml:math id="M395" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) showed that <inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> at pH 3.0 was one order of magnitude higher than that at pH 5.0 (Sect. S4). And numerous experimental evidences have established that the reactions of <inline-formula><mml:math id="M397" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> with carbonyl are generally acid catalyzed (Liu et al., 2015b; Zhang et al., 2015). Furthermore, our recent findings confirmed that compared to the neutral aerosols, acidic aerosols are more conducive to the formation of high-molecular-weight NOCs through carbonyl-to-NH<sub>3</sub> reactions, which exhibit stronger light-absorptivity (Zhang et al., 2024).</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <label>3.3.2</label><title>Gas-phase formation of light-absorbing NOCs</title>
      <p id="d2e4926">It is worth noting that NO<sub>2</sub> and O<sub>3</sub> explained over 8 % and 6 % of the variances in the WSONsec (Fig. 5b), implying that partial WSONsec presumably formed by gas-phase photochemical oxidation under relatively high NO<sub><italic>x</italic></sub> loadings. To verify this, nine NACs herein were quantified, which typically derived from gas-phase reactions of polyphenols with <inline-formula><mml:math id="M402" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals, and followed by partitioning into the aerosol. As shown in Fig. 6a, 4-Nitrophenol (4NP) and 4-Nitrocatechol (4NC) were the dominant species among the detected NACs. On average, they accounted for 56.8 %–74.0 % and 10.3 %–20.7 % of the total NACs across the five sites, respectively. This finding is consistent with previous observations reported in Shanghai (Liu et al., 2023), Dezhou (Li et al., 2021a), and Xinglong (Sun et al., 2026).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e4973">Chemical composition and formation of NACs. Fractional mass contribution of individual NAC to the total <bold>(a)</bold>; Relative contributions of primary emissions (NACs<sub>[pri])</sub> and secondary formation (NACs<sub>[sec]</sub>) to the detected NACs <bold>(b)</bold>; Pearson coefficients between NACs<sub>[sec]</sub>and various influencing factors <bold>(c)</bold>; Linear regression analysis for particulate 4NP with its gas-to-particle-phase partitioning coefficient <bold>(d)</bold>. (Triangles in panel <bold>d</bold> correspond to the bin-averaged 4NP versus <inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> over all sampling sites, cross bars represent standard deviation.)</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/14229/2026/acp-26-14229-2026-f06.png"/>

          </fig>

      <p id="d2e5053">Furthermore, secondary NACs were also quantified following the semi-quantitative method of WSONsec. As depicted in Fig. 6b, secondary formation played a dominant role in NACs accumulation, contributing approximately 46 %–64 % of total NACs across the five sites. Notably, secondary NACs (NACs<sub>[sec]</sub>) at all sites except TJ correlated strongly with NO<sub>2</sub> (<inline-formula><mml:math id="M409" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) but displayed no significant relationships with levoglucosan and BkF, suggesting a potentially important role of gas-phase oxidation in NACs formation. Previously, it is has been well established that nitrite is an important source of aerosol aqueous-phase NO<sub>2</sub> radical (Vione et al., 2004), which can react with aromatic compounds (e.g., phenol or catechol) to yield corresponding NACs. However, secondary NACs (NACs<sub>[sec]</sub>) exhibited weak correlations with NO<inline-formula><mml:math id="M412" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and ALWC (Fig. 6c) and no significant correlation with the ionic fragments of MSA (Fig. S10), a species formed predominantly through aqueous-phase processing. These patterns were consistent with an important contribution of gas-phase oxidation to NACs<sub>[sec]</sub> formation during the campaign.</p>
      <p id="d2e5142">Notably, the NACs<sub>[sec]</sub> exhibited a temperature-dependent pattern across all sampling sites (<inline-formula><mml:math id="M415" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. 6c). It is possible that ambient temperature largely affected gas-to-particle partitioning of the NACs, thereby moderating the abundance of particulate NACs. On this basis, we theoretically estimated the fraction of particulate 4NP (<inline-formula><mml:math id="M416" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) relative to the total based on the Pankow's absorption equilibrium theory, obtaining an average <inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of 0.3 <inline-formula><mml:math id="M418" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.1 across the NCP. This predicted value was within the range of field observations (0.2 in Hongkong to 0.75 on Mt. Tai) (Li et al., 2022a; Chen et al., 2025). As depicted in Fig. 6d, the <inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> correlated positively with the particulate 4NP, again suggesting that partial NOCs are formed by gas-phase photooxidation reactions, subsequently partitioning into the aerosol. In addition, temperature can also affect the abundance of NACs regulating the rates of numerous photochemical reactions. For instance, Lignell et al. (2014) found that low temperature substantially restrained the photolysis of 2, 4-Dinitrophenol in secondary organic aerosols, with its decay rate at 0 °C dropping by nearly one order of magnitude relative to 25 °C. Correspondingly, the low-temperature atmospheric environment likely inhibited the photolysis of NACs during the campaign, thereby facilitating their accumulation in the particle phase. This may be one of the reasons for the significant negative correlation between NACs and temperature.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusion and implications</title>
      <p id="d2e5222">Synchronous observations of the optical properties and chemical compositions of water-soluble BrC were conducted at five sites across the NCP during the winter of 2023. The OM was identified as the predominant component of PM<sub>2.5</sub> at all sampling sites, accounting for 40 %–55 % of the PM<sub>2.5</sub>. The water-soluble BrC in rural area exhibited a higher light-absorption, being approximately 1.1–3.5 folds of those recorded at urban sites. Compared with the previous observations, the average light absorption of urban BrC decreased substantially by roughly 45 % over the period 2018–2023, which was mainly due to significant anthropogenic emission controls in the NCP. The average MAE<sub>365</sub> ranged from 0.7 <inline-formula><mml:math id="M423" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.04 to 1.40 <inline-formula><mml:math id="M424" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 m<sup>2</sup> g<sup>−1</sup>, with a distinctly different spatial pattern. Specially, a strikingly high MAE<sub>365</sub> value (1.40 <inline-formula><mml:math id="M428" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 m<sup>2</sup> g<sup>−1</sup>) was measured in JN, falls within the range for BrC emitted from residential coal combustion. While, the MAE<sub>365</sub> values of BrC (<inline-formula><mml:math id="M432" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1.1 m<sup>2</sup> g<sup>−1</sup>) in TJ, LC and HD were closely matched the values associated with biomass burning-derived BrC. The MAE<sub>365</sub> value in BJ was the lowest among all the sampling sites, which was likely ascribed to enhanced photobleaching during aerosol aging.</p>
      <p id="d2e5372">During the haze periods, we found that the MAE<sub>365</sub> of water-soluble BrC at most sample sites was 1.5-fold of that in clean periods, indicating enhanced light-absorptivity of BrC as the haze developed. Of particular note, a parallel variation was also found for <inline-formula><mml:math id="M437" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">N</mml:mi><mml:mo>:</mml:mo><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> ratio. These findings indicated that N-containing compounds (NOCs), as crucial chromophores affecting water-soluble BrC optical properties in the NCP, were abundantly formed in the aerosol aging process. Additionally, these secondary NOCs were closely associated with the aerosol aqueous reactions, in which ammonia playing an important role. In the previous observation conducted on Mt. Hua (Wu et al., 2024a), we also revealed that ammonia-driven aerosol aqueous reactions can also significantly promote BrC formation during the air mass lifting process. Consequently, NH<sub>3</sub> is probably one of the important factors contributing to the high loading of strongly light-absorbing BrC within the boundary layer across China. This effect is likely to be particularly pronounced during moist winter haze episodes, when enhanced aerosol liquid water facilitates aqueous-phase reactions. Accordingly, targeted NH<sub>3</sub> emission control may be important for further mitigating haze and BrC pollution under such conditions in ammonia-rich regions.</p>
</sec>

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

      <p id="d2e5419">The primary data used in this study can be obtained from <ext-link xlink:href="https://doi.org/10.5281/zenodo.17947347" ext-link-type="DOI">10.5281/zenodo.17947347</ext-link>  (Wu, 2025b). Other data utilized in the present study are available from the corresponding author on request.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5425">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-14229-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-14229-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5434">G.W. designed research and contributed analytic tools. CW, ZL BX and RL collected the samples. CW and YC conducted the sample analysis. CW performed the data interpretation. CW and GW wrote the paper. All authors contributed to the paper with useful scientific discussions.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5440">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="d2e5446">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="d2e5452">This work acknowledge financial support from the National Key Research and Development Program of China and the National Natural Science Foundation of China.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5457">This research has been supported by the National Key Research and Development Program of China (grant no. 2023YFC3706302) and the National Natural Science Foundation of China (grant nos. 42130704 and 42477097).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5463">This paper was edited by Alex Lee and reviewed by two anonymous referees.</p>
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