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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-26-9207-2026</article-id><title-group><article-title>El Niño meets elevated Tibetan Plateau snow cover: independent and synergistic effects on the winter PM<sub>2.5</sub> dipole pattern in China</article-title><alt-title>El Niño meets elevated Tibetan Plateau snow cover</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3 aff4">
          <name><surname>Zhang</surname><given-names>Xiaorui</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7323-1630</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Han</surname><given-names>Yuyang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Chen</surname><given-names>Siyu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>An</surname><given-names>Xiadong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8992-0406</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Sheng</surname><given-names>Chen</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Duan</surname><given-names>Wansuo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Chen</surname><given-names>Xi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9952-9048</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>You</surname><given-names>Qinglong</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hao</surname><given-names>Xingyue</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Qiu</surname><given-names>Ziqi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Zhihan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhuang</surname><given-names>Zicheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff3 aff4">
          <name><surname>Gao</surname><given-names>Meng</given-names></name>
          <email>mmgao2@hkbu.edu.hk</email>
        <ext-link>https://orcid.org/0000-0002-8657-3541</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Key Laboratory for Geographical Process Analysis and Simulation of Hubei Province, College of Urban and Environmental Sciences, Central China Normal University, Wuhan, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Key Laboratory of Urban Meteorology, China Meteorological Administration, Beijing, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Geography, Hong Kong Baptist University, Hong Kong SAR, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute for Research and Continuing Education, Hong Kong Baptist University, Shenzhen, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Key Laboratory for Semi-Arid Climate Change of the Ministry of Education, Lanzhou University, Lanzhou, China</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of Atmospheric Sciences, Yunnan University, Kunming, China</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Laboratory of Atmospheric and Oceanic Dynamics, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing, China</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>State Key Laboratory of Earth System Numerical Modeling and Applications (LabESM), Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing, China</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Key Laboratory of Polar Atmosphere-ocean-ice System for Weather and Climate, Ministry of Education &amp; Department of Atmospheric and Oceanic Sciences, Fudan University, Shanghai, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Meng Gao (mmgao2@hkbu.edu.hk)</corresp></author-notes><pub-date><day>30</day><month>June</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>12</issue>
      <fpage>9207</fpage><lpage>9219</lpage>
      <history>
        <date date-type="received"><day>2</day><month>March</month><year>2026</year></date>
           <date date-type="rev-request"><day>7</day><month>April</month><year>2026</year></date>
           <date date-type="rev-recd"><day>26</day><month>May</month><year>2026</year></date>
           <date date-type="accepted"><day>19</day><month>June</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Xiaorui Zhang 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/26/9207/2026/acp-26-9207-2026.html">This article is available from https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e262">Snow cover over the Tibetan Plateau (TP) plays a vital role in shaping regional and large-scale atmospheric circulation through snow-albedo feedbacks. However, its influence on fine particulate matter (PM<sub>2.5</sub>) pollution in China remains unclear. This study reveals that winter PM<sub>2.5</sub> variability in China is controlled by both anthropogenic emissions and large-scale atmospheric circulation. Large-scale circulation creates a north-south dipole pattern over eastern China, which is mainly contributed by El Niño and snow cover over the northern TP. Observational data and model simulations confirm that El Niño mainly impacts PM<sub>2.5</sub> in southern China by enhancing moisture transport and wet scavenging, while increased snow cover over the northern TP independently promotes accumulation and hygroscopic growth of aerosols in northern China. Moreover, El Niño and TP snow cover interact synergistically, particularly during their positive phases, intensifying circulation anomalies linked to the PM<sub>2.5</sub> dipole. These findings emphasize the importance of cryospheric and oceanic variability in influencing winter air quality and offer valuable insights for improving seasonal prediction of air pollution in China.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42322902</award-id>
</award-group>
<award-group id="gs2">
<funding-source>China Meteorological Administration</funding-source>
<award-id>LUM-2025-12</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Research Grants Council, University Grants Committee</funding-source>
<award-id>C2002-22Y</award-id>
<award-id>HKBU12201023</award-id>
<award-id>HKBU12202824</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="d2e310">Over the past two decades, rapid industrialization, urbanization, and the resulting rise in energy consumption have caused frequent and severe fine particulate matter (PM<sub>2.5</sub>) pollution in China (Huang et al., 2014; Wu et al., 2024; Friedlingstein et al., 2022; Gao et al., 2020). Although stringent clean air regulations introduced since 2013 have resulted in a marked nationwide decline in PM<sub>2.5</sub> concentrations, heavy pollution episodes still commonly occur in major urban clusters, particularly during the winter months (Wang et al., 2020). Chronic exposure to elevated PM<sub>2.5</sub> levels significantly raises the risks of lung cancer as well as respiratory and cardiovascular diseases (Apte et al., 2015; Lin et al., 2018; Xiao et al., 2023). Beyond health impacts, severe haze events degrade visibility and adversely affect human well-being, tourism, transportation safety, and regional economic activities (Berman et al., 2019; Zhou et al., 2018).</p>
      <p id="d2e340">PM<sub>2.5</sub> originates from both direct emissions and secondary formation from gaseous precursors (Huang et al., 2014). In China, anthropogenic emissions largely drive the long-term trends in PM<sub>2.5</sub> (Xiao et al., 2021; Zhang and Gao, 2026), and reductions in emissions have been crucial to recent improvements in air quality (Gao et al., 2020). Nevertheless, meteorological factors strongly influence PM<sub>2.5</sub> variability on daily, seasonal, and interannual timescales by affecting pollutant emissions, transport, dispersion, removal, and chemical production (Xiao et al., 2021; Zhai et al., 2019; Chen et al., 2020). For instance, enhanced wind speeds during winter associated with cold air outbreaks from Siberia can lower PM<sub>2.5</sub> concentrations by as much as 28 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup> for every 1 m s<sup>−1</sup> increase in wind speed (Zhang et al., 2022; Huang et al., 2021). Additionally, high relative humidity favors aerosol hygroscopic growth and secondary formation, particularly in northern China, where PM<sub>2.5</sub> exhibits greater hygroscopicity when concentrations exceed 90 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup> in winter (Cheng et al., 2015; Huang et al., 2014).</p>
      <p id="d2e441">Emerging evidence suggests that meteorological conditions conducive to severe air pollution are closely linked to large-scale climate patterns (Zhang et al., 2025; Gao et al., 2023). El Niño-Southern Oscillation (ENSO), the primary ocean-atmosphere coupled climate signal near the equator, has been extensively shown to influence winter PM<sub>2.5</sub> pollution in China (An et al., 2023; Xie et al., 2022). Previous studies have shown that ENSO can significantly intensify early winter PM<sub>2.5</sub> levels over the Beijing-Tianjin-Hebei (BTH) region by inducing atmospheric teleconnections that generate anticyclonic circulation anomalies over Northeast Asia, which suppress ventilation and favor pollutant accumulation (Zhao et al., 2022). Consistently, El Niño years are associated with increased winter PM<sub>2.5</sub> concentrations over BTH and decreased levels over the Pearl River Delta (PRD) (Xie et al., 2022; An et al., 2022). In addition, PM<sub>2.5</sub> variability in China has also been connected to other major climate modes, including Arctic sea ice fluctuations and the Pacific Decadal Oscillation (An et al., 2023; Zhang et al., 2025; Yin et al., 2021).</p>
      <p id="d2e480">The Tibetan Plateau (TP) is a distinctive high-altitude region notable for its extensive and persistent snow cover (Li et al., 2018; Yao et al., 2012). Owing to its high albedo, emissivity, and low thermal conductivity, the snow cover significantly influences surface energy balance and atmospheric heating across the TP (Barnett et al., 1988; Yao et al., 2015). Changes in snow cover on the TP can markedly affect thermal state of the plateau and influence regional and broader atmospheric circulation patterns through snow-albedo feedbacks (Li et al., 2018; You et al., 2020). Previous studies have documented the impacts of TP snow cover on the East Asian monsoon, precipitation in South and East Asia, and the frequency of landfalling typhoons in China (Jia et al., 2021; Chen et al., 2021; You et al., 2020; Xie et al., 2005; Yao et al., 2019). However, the influence of TP snow cover on PM<sub>2.5</sub> pollution over China remains largely unexplored.</p>
      <p id="d2e493">In this study, we demonstrate that, alongside ENSO, snow cover over the northern Tibetan Plateau independently influences winter PM<sub>2.5</sub> variability in China. Using a combination of empirical orthogonal function (EOF) analysis, statistical methods, and sensitivity simulations, we illustrate the physical mechanisms underlying the associations with both El Niño and TP snow cover. Additionally, synergistic diagnostic and composite analyses are used to examine how El Niño and TP snow cover jointly influence circulation patterns associated with PM<sub>2.5</sub> in China. These findings provide new insights into the roles of cryospheric and oceanic variability in shaping winter air quality in China and carry important implications for enhancing seasonal predictions of PM<sub>2.5</sub> pollution.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data</title>
      <p id="d2e538">Snow cover data were obtained from the National Oceanic and Atmospheric Administration (NOAA) Climate Data Record (Robinson et al., 2012), provided by the Rutgers University Global Snow Lab. This original weekly snow dataset, with a horizontal resolution of 25 km, spans from October 1966 to the present. In this study, the snow data were averaged into monthly means and regridded to <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">°</mml:mi><mml:mo>×</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">°</mml:mi></mml:mrow></mml:math></inline-formula> grids.</p>
      <p id="d2e557">Satellite-derived daily ground-level PM<sub>2.5</sub> concentrations over China were obtained from the Long-term Gap-free High-resolution Air Pollutants concentration dataset (LGHAP) version 2 (Bai et al., 2024). The LGHAP PM<sub>2.5</sub> data, covering 2005–2021, have a spatial resolution of 1 km and were developed by integrating satellite retrievals, ground-based observations, and numerical simulations through machine learning methods. Validation against observations from the China National Environmental Monitoring Center (CNEMC) indicates strong reliability, with a high correlation coefficient of 0.95 and a root mean square error (RMSE) of 12.03 <inline-formula><mml:math id="M30" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, supporting its suitability for long-term spatiotemporal analysis (Bai et al., 2024).</p>
      <p id="d2e598">Meteorological variables including sea surface temperature (SST), geopotential height, zonal and meridional winds at 200 hPa, 500 hPa and the surface, relative humidity, precipitation, planetary boundary layer height, surface sensible heat flux, surface latent heat flux, surface net long-wave radiation flux, surface net short-wave radiation flux, top net long-wave radiation flux, top net short-wave radiation flux, and snow albedo at a spatial resolution of <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.25</mml:mn><mml:mi mathvariant="italic">°</mml:mi><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn><mml:mi mathvariant="italic">°</mml:mi></mml:mrow></mml:math></inline-formula> were obtained from the European Centre for Medium-Range Weather Forecasts (ECMWF) ERA5 dataset (Zhang et al., 2022; You et al., 2020; Hersbach et al., 2020). The monthly sea ice concentration data, with a horizontal resolution of <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.0</mml:mn><mml:mi mathvariant="italic">°</mml:mi><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1.0</mml:mn><mml:mi mathvariant="italic">°</mml:mi></mml:mrow></mml:math></inline-formula> was provided by Met Office Hadley Centre. The winter El Niño indices during 2005–2021 were retrieved from NOAA.</p>
      <p id="d2e633">To examine the atmospheric response to snow cover anomalies, the total atmospheric column heat source (<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), was calculated as, following by Zhao and Chen (2001),

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M35" display="block"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">SH</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">LP</mml:mi></mml:mrow></mml:math></disp-formula>

          where SH denotes surface sensible heat flux, <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> represents net atmospheric column radiation, and LP is latent heat released through condensation.</p>
      <p id="d2e685">Anthropogenic emissions of sulfur dioxide (SO<sub>2</sub>) and nitrogen oxides (NO<sub><italic>x</italic></sub>) for the period 2005–2021 were obtained from the Multi-resolution Emission Inventory for China (MEIC) (Wu et al., 2024).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Statistical methods</title>
      <p id="d2e714">The interannual spatiotemporal variability of winter PM<sub>2.5</sub> concentrations over China during 2005–2021 was analyzed using EOF decomposition. The first two EOF modes were emphasized, as they were well separated from higher-order modes based on the North test (North et al., 1982).</p>
      <p id="d2e726">To diagnose the propagation characteristics of atmospheric Rossby waves, the horizontal wave activity flux (WAF) was computed using the formulation based on the conservation of wave-activity momentum (Takaya and Nakamura, 2001):

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M40" display="block"><mml:mrow><mml:mi>W</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mfenced open="|" close="|"><mml:mover accent="true"><mml:mi mathvariant="bold-italic">U</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close="]" open="["><mml:mtable class="array" columnalign="center"><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msup><mml:msubsup><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>x</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Ψ</mml:mi><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Ψ</mml:mi><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Ψ</mml:mi><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>v</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:msup><mml:msubsup><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mi>y</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Ψ</mml:mi><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:msub><mml:mi mathvariant="normal">Ψ</mml:mi><mml:mrow><mml:mi>y</mml:mi><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M41" display="inline"><mml:mi mathvariant="italic">ψ</mml:mi></mml:math></inline-formula> denotes the geostrophic stream function, and subscripts represent partial derivatives. <inline-formula><mml:math id="M42" display="inline"><mml:mi mathvariant="bold-italic">U</mml:mi></mml:math></inline-formula> corresponds to the horizontal wind vector, whereas <inline-formula><mml:math id="M43" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M44" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> indicate its zonal and meridional components, respectively. <inline-formula><mml:math id="M45" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> represents the two-dimensional Rossby wave activity flux.</p>
      <p id="d2e974">To assess whether a synergistic effect exists between the influences of Niño 1<inline-formula><mml:math id="M46" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index and Tibetan Plateau snow cover (TPSC) on winter PM<sub>2.5</sub> variability, the statistical diagnostic method proposed by Li et al. (2019) was applied. The Niño 1<inline-formula><mml:math id="M48" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC indices were classified into positive (<inline-formula><mml:math id="M49" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula>), neutral (0), and negative (<inline-formula><mml:math id="M50" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>) phases based on <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> standard deviations. The combinations of Niño 1<inline-formula><mml:math id="M52" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC phases are summarized in Table 1.</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e1036">The combinations of different phases of the winter Niño 1<inline-formula><mml:math id="M53" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC during 1979–2021.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="center"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Niño 1<inline-formula><mml:math id="M54" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2  (<inline-formula><mml:math id="M55" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col3">Niño 1<inline-formula><mml:math id="M56" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2  (0)</oasis:entry>
         <oasis:entry colname="col4">Niño 1<inline-formula><mml:math id="M57" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2  (<inline-formula><mml:math id="M58" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col5">Total</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">TPSC  (<inline-formula><mml:math id="M59" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">1983, 2007, 2019</oasis:entry>
         <oasis:entry colname="col3">1982, 1986, 2014, 2020</oasis:entry>
         <oasis:entry colname="col4">1981, 1989, 1997, 2000</oasis:entry>
         <oasis:entry colname="col5">11</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TPSC  (0)</oasis:entry>
         <oasis:entry colname="col2">1995, 1998, 2016, 2017</oasis:entry>
         <oasis:entry colname="col3">1979, 1980, 1990, 1993, 1999, 2003, 2011, 2015</oasis:entry>
         <oasis:entry colname="col4">1996, 2002, 2008</oasis:entry>
         <oasis:entry colname="col5">15</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TPSC  (<inline-formula><mml:math id="M60" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">1987, 1992</oasis:entry>
         <oasis:entry colname="col3">1984, 1988, 1991, 1994, 2004, 2005, 2006,</oasis:entry>
         <oasis:entry colname="col4">1985, 2001, 2018</oasis:entry>
         <oasis:entry colname="col5">17</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">2009, 2010, 2012, 2013, 2021</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Total</oasis:entry>
         <oasis:entry colname="col2">9</oasis:entry>
         <oasis:entry colname="col3">24</oasis:entry>
         <oasis:entry colname="col4">11</oasis:entry>
         <oasis:entry colname="col5">43</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>CESM model experiments</title>
      <p id="d2e1228">The Community Earth System Model version 2.1.3 (CESM v2.1.3) was employed to investigate how circulation patterns and PM<sub>2.5</sub> concentrations respond to SST and snow cover anomalies. The model was configured with a horizontal resolution of <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.94</mml:mn><mml:mi mathvariant="italic">°</mml:mi><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1.25</mml:mn><mml:mi mathvariant="italic">°</mml:mi></mml:mrow></mml:math></inline-formula> and 70 vertical layers (Gent et al., 2011), using the FWHIST component. The atmospheric processes were simulated using the Community Atmosphere Model version 6, while chemical and land processes were represented by the Whole Atmosphere Community Climate Model version 6 (Gettelman et al., 2019). The aerosol microphysical and chemical processes in CESM have been extensively developed and validated in previous studies (Gettelman et al., 2019; Danabasoglu et al., 2020; Liu et al., 2021). We assessed CESM's ability to reproduce observed surface air temperature, relative humidity, and PM<sub>2.5</sub> concentrations in the control simulation (CESM<sub>ctrl</sub>), as shown in Fig. S1 in the Supplement. The results demonstrate that CESM<sub>ctrl</sub> generally captures the spatial patterns and interannual variability of these variables. Quantitatively, the mean fractional biases (MFBs) and mean fractional errors (MFEs) for PM<sub>2.5</sub> fall within the widely adopted model performance criteria of <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">60</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula> for MFB and below <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">75</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula> for MFE (Boylan and Russell, 2006), indicating acceptable simulation skill. CESM reproduces meteorological variables better than aerosol concentrations, which are subject to larger uncertainties arising from emission inputs, chemical processing, and aerosol-cloud interactions (Liu et al., 2021; Danabasoglu et al., 2020).</p>
      <p id="d2e1319">SST was prescribed to isolate the effects of SST forcing. CESM<sub>ctrl</sub> was forced with monthly varying climatological SSTs. Two additional sensitivity experiments were conducted: (1) CESM<sub>ElNiño</sub>, in which composite winter SST anomalies associated with Niño 1<inline-formula><mml:math id="M71" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 were imposed; and (2) CESM<sub>TPSC</sub>, in which surface albedo over the northern Tibetan Plateau (86–94° E, 35–40° N) was set to a minimum of 0.8 to represent enhanced snow cover conditions (Cohen and Rind, 1991), following Wang et al. (2021). Specifically, when the model-simulated albedo falls below 0.8, it is reset to 0.8 to represent increased snow cover over the northern Tibetan Plateau. Grid points where albedo already exceeds this threshold retain their original values. All simulations covered the period from November 2010 to February 2011, during which both Niño 1<inline-formula><mml:math id="M73" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC were in neutral phases (Table 1). Surface PM<sub>2.5</sub> concentrations were derived from the model output by extracting the lowest vertical level of the simulated three-dimensional PM<sub>2.5</sub> field. Given the uncertainties in CESM-simulated PM<sub>2.5</sub> concentrations, model outputs are interpreted in terms of the direction and spatial pattern of PM<sub>2.5</sub> changes rather than their absolute magnitudes. Statistical significance was evaluated using daily model output during the winter simulation period.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e1407">Spatial patterns of <bold>(a)</bold> EOF1, and <bold>(b)</bold> EOF2. Interannual variations of standardized <bold>(c)</bold> PC1 and <bold>(d)</bold> PC2 during winter from 2005 to 2021.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f01.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Major modes of winter PM<sub>2.5</sub> concentrations over China</title>
      <p id="d2e1454">Figure 1 presents the leading two EOF modes of winter PM<sub>2.5</sub> concentrations over China. Both modes are distinctly separated according to the North test, indicating their statistical robustness. The dominant mode (EOF1), accounting for 56.2 % of the total variance, exhibits a spatially coherent pattern characterized by uniformly elevated PM<sub>2.5</sub> concentrations across eastern China. The corresponding normalized principal component (PC1) shows a pronounced increase from 2005 to 2013, followed by a marked decline after 2014. This temporal evolution closely mirrors trends in anthropogenic emissions, with rapid growth in energy consumption and emissions during 2005–2013 while the introduction of stringent clean air policies since 2013. Quantitatively, PC1 is almost perfectly correlated with regional mean PM<sub>2.5</sub> concentrations (<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.99</mml:mn></mml:mrow></mml:math></inline-formula>) and also shows strong correlations with anthropogenic NO<sub><italic>x</italic></sub> and SO<sub>2</sub> emissions (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.70</mml:mn></mml:mrow></mml:math></inline-formula> and 0.71, respectively). These relationships indicate that EOF1 primarily represents the influence of anthropogenic emission variability on winter PM<sub>2.5</sub> over eastern China.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1538">Anomalies of <bold>(a)</bold> geopotential height (m, shading) and wind fields (m s<sup>−1</sup>, vector) at 500 hPa, <bold>(b)</bold> relative humidity at 1000 hPa (%), <bold>(c)</bold> total precipitation (mm per month), <bold>(d)</bold> surface wind speed (m s<sup>−1</sup>), and <bold>(e)</bold> planetary boundary layer height (m) during winter over 2005–2021 obtained by regression upon normalized PC2. Dotted areas represent statistical significance with 95 % confidence according to Student's <inline-formula><mml:math id="M89" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f02.png"/>

        </fig>

      <p id="d2e1594">EOF2, accounting for 13.2 % of the total variance, reveals a pronounced north-south dipole pattern in winter PM<sub>2.5</sub> concentrations over eastern China, characterized by positive anomalies in northern China and negative anomalies in southern China. PC2 displays strong interannual variability, with predominantly negative values before 2012 and mainly positive values during 2013–2020. We examined the correlations between PC2 and anthropogenic SO<sub>2</sub> and NO<sub><italic>x</italic></sub> emissions across eastern, northern, and southern China. The correlation coefficients between PC2 and SO<sub>2</sub> (NO<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> emissions are <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.31</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.37</mml:mn></mml:mrow></mml:math></inline-formula> (0.07), and <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.33</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.11</mml:mn></mml:mrow></mml:math></inline-formula>) in eastern, northern, and southern China, respectively. None of these correlations are statistically significant, and critically, they exhibit no north-south dipole structure that could mirror the EOF2 pattern. This confirms that the spatially heterogeneous emission controls do not drive the EOF2 dipole structure. To elucidate the meteorological conditions underlying the EOF2 dipole structure, regression maps of atmospheric circulation and meteorological fields onto the normalized PC2 are shown in Fig. 2. At the 500 hPa level, a pronounced anticyclonic circulation anomaly is observed over northeastern China and Japan, accompanied by a weaker cyclonic anomaly over the southern Tibetan Plateau. This configuration induces anomalous southerly flow across eastern China. In southern China, these southerly winds transport humid air from the South China Sea, enhancing precipitation by approximately 0.2 mm per month  and promoting wet removal of PM<sub>2.5</sub>. In contrast, over northern China, the southerly anomalies weaken atmospheric ventilation, as reflected by reduced surface wind speeds (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula> m s<sup>−1</sup>) and a suppressed planetary boundary layer height (<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> m), favoring pollutant accumulation and increasing PM<sub>2.5</sub> levels. As a result, anomalous southerly flow exerts opposite influences on winter PM<sub>2.5</sub> concentrations in northern and southern China, which is consistent with previous findings (Zhang et al., 2022; An et al., 2022). These results confirm that EOF2 dipole pattern primarily reflects large-scale meteorological forcing rather than anthropogenic emission variability.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e1759">Correlation and partial correlation patterns of PC2 with <bold>(a, c)</bold> winter SST and <bold>(b, d)</bold> Tibetan Plateau snow cover, with the influence of Niño 1<inline-formula><mml:math id="M106" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 removed. Dotted areas represent statistical significance with 95 % confidence according to Student's <inline-formula><mml:math id="M107" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f03.png"/>

        </fig>

      <p id="d2e1788">To further elucidate the large-scale climate drivers underlying the EOF2 mode, correlation analyses were performed between PC2 and winter SST anomalies (Fig. 3). Strong correlations are found over the central and eastern equatorial Pacific, indicating a close linkage with ENSO, consistent with its well-documented influence on East Asian climate (Zhao et al., 2022; Xie et al., 2022). The correlation coefficients between PC2 and the Niño 1<inline-formula><mml:math id="M108" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2, Niño 3, and Niño 3.4 indices are 0.53, 0.51, and 0.51, respectively (all significant at the 95 % confidence level). Significant correlations are also identified between PC2 and SST anomalies in the Southern Hemisphere, resembling the pattern associated with the Antarctic Oscillation (AAO). The correlation coefficient between PC2 and the AAO index reaches <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.48</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M110" 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>). To isolate the ENSO contribution, partial correlation analysis was performed by removing the ENSO signal with Niño 1<inline-formula><mml:math id="M111" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index, which exhibits the strongest correlation with PC2. After excluding the ENSO signal, the SST-PC2 relationship over the Northern Hemisphere becomes statistically insignificant (Fig. 3c). Consistently, the partial correlation between PC2 and the AAO index decreases to <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.22</mml:mn></mml:mrow></mml:math></inline-formula> and is no longer significant (<inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula>), attributed to the strong coupling between ENSO and the AAO (Han et al., 2017). Although Arctic sea ice has been reported to influence PM<sub>2.5</sub> pollution in China (An et al., 2023; Yin et al., 2021; Zhang et al., 2025), no significant correlation is detected between Arctic sea ice and PC2 (Fig. S2). In contrast, snow cover over the northern Tibetan Plateau becomes significantly correlated with PC2 after the ENSO signal is removed (Fig. 3d), suggesting that Tibetan Plateau snow anomalies exert an additional and independent modulation of the north-south dipole pattern of winter PM<sub>2.5</sub> over eastern China.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e1870">Anomalies of <bold>(a)</bold> geopotential height (m, shading) and wind fields (m s<sup>−1</sup>, vector) at 500 hPa, <bold>(b)</bold> relative humidity at 1000 hPa (%), <bold>(c)</bold> total precipitation (mm per month), <bold>(d)</bold> surface wind speed (m s<sup>−1</sup>), and <bold>(e)</bold> planetary boundary layer height (m) during winter over 1979–2021 obtained by regression upon normalized Niño 1<inline-formula><mml:math id="M118" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index. Dotted areas represent statistical significance with 95 % confidence according to Student's <inline-formula><mml:math id="M119" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f04.png"/>

        </fig>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e1935">CESM simulated responses of horizontal distribution of near-surface PM<sub>2.5</sub> concentration (<inline-formula><mml:math id="M121" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) over eastern China during winter to <bold>(a)</bold> Niño 1<inline-formula><mml:math id="M122" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2, and <bold>(b)</bold> higher albedo forcing over the northern TP. Dotted areas indicate responses that are significant at the 95 % confidence level based on a two-tailed Student's <inline-formula><mml:math id="M123" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test applied to daily simulated anomalies during the winter period.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Impacts of El Niño on winter PM<sub>2.5</sub> over China</title>
      <p id="d2e2011">As noted above, PC2 exhibits the strongest correlation with the Niño 1<inline-formula><mml:math id="M125" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index and also shows statistically significant correlations with other Niño indices. El Niño-related warming of the tropical Pacific can trigger a Rossby wave propagating into East Asia. This induces a strong negative and weak positive geopotential anomaly over South and North of China, respectively, which closely resembles the wave train regressed by PC2 (Fig. S3). Figure 4 illustrates the regression patterns of meteorological conditions onto the normalized Niño 1<inline-formula><mml:math id="M126" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index. During strong El Niño winters, positive geopotential height anomalies emerge over the western Pacific (Fig. 4a), favoring southwesterly flow over southern China and southeasterly flow over northern China. As a result, moisture transport from adjacent oceans into southern China is enhanced, leading to a significant increase in relative humidity exceeding 2 % over the PRD (Fig. 4b) and increased precipitation of approximately 0.4 mm per month (Fig. 4c). The more humid conditions promote wet scavenging of aerosols, thereby reducing PM<sub>2.5</sub> concentrations in southern China. In contrast, over northern China, the anomalous southeasterly winds, which are opposite to the prevailing northwesterly flow, partly weaken near-surface wind speeds (Fig. 4d). Similar meteorological conditions are also found for Niño 3.4 index (Fig. S4). This meteorological contrast induced by El Niño supports the observed north-south dipole pattern of winter PM<sub>2.5</sub> over eastern China identified in EOF2.</p>
      <p id="d2e2046">To further verify the role of El Niño-like SST anomalies, sensitivity simulations were conducted by imposing warm SST anomalies associated with the Niño 1<inline-formula><mml:math id="M129" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index (Fig. S5). Figure 5a shows the differences between the CESM<sub>ElNiño</sub> and CESM<sub>ctrl</sub> experiments, which isolate the atmospheric and PM<sub>2.5</sub> response to El Niño forcing. Consistent with the statistical analysis, the imposed El Niño-like SST pattern strengthens the western Pacific subtropical high, induces anomalous southerly winds over eastern China, and enhances moisture transport into southern China (Fig. S6a, b). Consequently, surface PM<sub>2.5</sub> concentrations decrease markedly in southern China, with reductions of approximately 12 <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup> over the Sichuan Basin and 6 <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup> over the Yangtze River Delta (Fig. 5a). In contrast, PM<sub>2.5</sub> concentrations increase slightly over northeastern China by about 3 <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, further confirming the El Niño-driven north-south dipole structure captured by EOF2.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e2170">Anomalies for <bold>(a)</bold> snow albedo (dimensionless, multiplied by 100), <bold>(b)</bold> top net short-wave radiation flux (W m<sup>−2</sup>), <bold>(c)</bold> top net long-wave radiation flux (W m<sup>−2</sup>), <bold>(d)</bold> surface sensible heat flux (W m<sup>−2</sup>), <bold>(e)</bold> surface latent heat flux (W m<sup>−2</sup>), <bold>(f)</bold> total atmospheric column heat source (W m<sup>−2</sup>) during winter over 1979–2021 obtained by regression upon normalized TPSC index. Dotted areas represent statistical significance with 95 % confidence according to Student's <inline-formula><mml:math id="M146" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Impacts of TP snow anomalies on winter PM<sub>2.5</sub> over China</title>
      <p id="d2e2284">After excluding the ENSO signal, PC2 remains significantly correlated with snow cover over the northern TP (Fig. 3d), indicating that interannual variability in winter PM<sub>2.5</sub> over China is also modulated by TP snow anomalies. To quantify this relationship, we define a Tibetan Plateau Snow Cover (TPSC) index as the wintertime area-averaged snow cover over the northern TP (86–94° E, 35–40° N), described by the blue box in Fig. 3d. The TPSC index associated snow albedo exhibits pronounced interannual variability throughout 1979–2021, with notably elevated values in recent years (Fig. S7). The correlation coefficient between the Niño 1<inline-formula><mml:math id="M149" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 index and the TPSC index is <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.28</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.24</mml:mn></mml:mrow></mml:math></inline-formula>), indicating that the linear dependence between the two predictors is weak and statistically insignificant. To formally evaluate the degree of multicollinearity among PC2, Niño 1<inline-formula><mml:math id="M152" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2, and TPSC, we computed the Variance Inflation Factor (VIF) for each variable. The resulting VIF values are 1.87, 1.90, and 1.47, respectively, all well below the commonly adopted threshold of 5 (O'Brien, 2007), confirming that multicollinearity does not pose a meaningful threat to the robustness of the partial correlation results. Partial correlation analysis reveals a significant positive correlation between the TPSC index and PC2 (<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.49</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M154" 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>). In contrast, no statistically significant relationship emerges when a domain-wide TP snow cover index is employed, suggesting that the dynamically relevant snow signal is regionally confined to the northern TP rather than reflecting a plateau-wide forcing.</p>
      <p id="d2e2357">Figure 6 illustrates anomalies in surface heat fluxes and the total atmospheric column heat source regressed onto the TPSC index. Enhanced snow cover over the northern TP increases snow albedo by approximately 0.02, leading to an increase in upward shortwave radiation exceeding 4 W m<sup>−2</sup> through the snow-albedo feedback. Meanwhile, a reduction of about 3 W m<sup>−2</sup> in upward longwave radiation is observed over the northern TP, driven by lower surface temperatures associated with reduced short-wave radiation absorption by the surface. In contrast, anomalies in sensible and latent heat fluxes remain weak (<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> W m<sup>−2</sup>). As a consequence, a pronounced cooling effect on the atmospheric column is found over the northern TP, exceeding 5 W m<sup>−2</sup>.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e2420">Anomalies for <bold>(a)</bold> pressure-longitude cross sections averaged over 80–100° E of temperature (K), <bold>(b)</bold> zonal wind speeds at 200 hPa (m s<inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <bold>(c)</bold> geopotential height (m, shading) and wind fields (m s<sup>−1</sup>, vector) at 500 hPa, <bold>(d)</bold> relative humidity at 1000 hPa (%), <bold>(e)</bold> surface wind speed (m s<sup>−1</sup>), and <bold>(f)</bold> planetary boundary layer height (m) during winter over 1979–2021 obtained by regression upon normalized TPSC index. Dotted areas represent statistical significance with 95 % confidence according to Student's <inline-formula><mml:math id="M163" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> test.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f07.png"/>

        </fig>

      <p id="d2e2495">The cooling effect over TP modulates the meridional temperature gradient and weakens the subtropical westerly jet north of the Plateau (Fig. 7a). Associated with enhanced snow cover, 200 hPa zonal wind speeds are reduced by up to 15 m s<sup>−1</sup>, inducing an anomalous anticyclonic circulation over northern China (Fig. 7b, c). Under the influence of positive geopotential height anomalies, near-surface wind speeds decrease by more than 0.1 m s<sup>−1</sup>, and the planetary boundary layer height is reduced by approximately 15 m. These stagnant conditions favor pollutant accumulation, while concurrently elevated surface relative humidity enhances aerosol hygroscopic growth (Fig. 7d), together contributing to increased PM<sub>2.5</sub> concentrations over northern China.</p>
      <p id="d2e2531">Because TP snow cover is itself influenced by local temperature, precipitation, and large-scale circulation variability, the statistical relationship may overestimate its impact on meteorological conditions and PM<sub>2.5</sub>. To assess the causal impact of TP snow cover, we performed a targeted CESM experiment (CESM<sub>TPSC</sub>) in which surface albedo over the northern TP (86–94° E, 35–40° N) was prescribed with a minimum value of 0.8. Surface albedo represents the reflectivity of the land surface, integrating contributions from all surface components including snow, soil, and vegetation. A minimum value of 0.8 was imposed to simulate persistent high snow cover conditions, consistent with the characteristically high reflectivity of snow-dominated surfaces (Cohen and Rind, 1991). The CESM results reproduce a coherent cooling response over the northern TP and a corresponding weakening of the subtropical westerly jet, which leads to increases in surface relative humidity and reductions in both planetary boundary layer height and near-surface wind speed over northern China (Fig. S6), supporting positive PM<sub>2.5</sub> anomalies over the BTH (Fig. 5b). These modeled responses are consistent with the observational regression analysis, reinforcing the physical credibility of the identified snow-forcing mechanism.</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e2563">Composite of the geopotential height (m, shading) and wind fields (m s<sup>−1</sup>, vector) at 500 hPa for <bold>(a)</bold> Niño 1<inline-formula><mml:math id="M171" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup>&amp;TPSC<sup>+</sup>, <bold>(b)</bold> Niño 1<inline-formula><mml:math id="M174" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>−</sup>&amp;TPSC<sup>−</sup>, <bold>(c)</bold> Niño 1<inline-formula><mml:math id="M177" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>+</sup>, <bold>(d)</bold> Niño 1<inline-formula><mml:math id="M180" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>−</sup>, <bold>(e)</bold> TPSC<inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>Niño 1<inline-formula><mml:math id="M184" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup>, and <bold>(f)</bold> TPSC<inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>Niño 1<inline-formula><mml:math id="M187" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>−</sup>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/9207/2026/acp-26-9207-2026-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Synergistic effects of El Niño and elevated TP snow cover on winter PM<sub>2.5</sub> in China</title>
      <p id="d2e2786">The individual impacts of El Niño and the TP snow cover on winter PM<sub>2.5</sub> in China have been confirmed, however, whether these two factors exert synergistic effects remains unclear. Following Li et al. (2019), we disentangle their respective and combined influences on circulation patterns associated with PM<sub>2.5</sub> pollution. We focus on atmospheric circulation rather than PM<sub>2.5</sub> concentrations directly, as meteorological variables are available over a longer period (1979–2021), whereas PM<sub>2.5</sub> observations are limited to 2005–2021.</p>
      <p id="d2e2825">Composite geopotential height anomalies for different combinations of Niño 1<inline-formula><mml:math id="M194" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC phases are shown in Fig. 8. Following Li et al. (2019), the symbol “&amp;” denotes years when two indices occur simultaneously in the specified phase (e.g., “Niño 1<inline-formula><mml:math id="M195" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup>&amp;TPSC<sup>+</sup>” indicates years when both Niño 1<inline-formula><mml:math id="M198" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC are positive), whereas the symbol “<inline-formula><mml:math id="M199" display="inline"><mml:mo>\</mml:mo></mml:math></inline-formula>” denotes years when only the first index is in the specified phase while the second index is not (e.g., “Niño 1<inline-formula><mml:math id="M200" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>+</sup>” indicates years when Niño 1<inline-formula><mml:math id="M203" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 is positive but TPSC is neutral or negative). During Niño 1<inline-formula><mml:math id="M204" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup>&amp;TPSC<sup>+</sup> (Niño 1<inline-formula><mml:math id="M207" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>−</sup>&amp;TPSC<inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> years, strong positive (negative) geopotential height anomalies develop over northern China and the western Pacific, accompanied by negative (positive) anomalies over the TP. This circulation configuration strongly favors the north-south dipole pattern of winter PM<sub>2.5</sub> over eastern China (Fig. 8a, b).</p>
      <p id="d2e2973">By contrast, during Niño 1<inline-formula><mml:math id="M211" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>+</sup> or TPSC<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>Niño 1<inline-formula><mml:math id="M215" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup> years, similar circulation structures emerge but with substantially weaker anomaly amplitudes (Fig. 8c, e). Notably, during Niño 1<inline-formula><mml:math id="M217" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>+</sup> years, El Niño also induces a negative geopotential height anomaly located over TP (Fig. 8c), similar to the impacts of TP snow (Fig. 7a). Previous studies confirmed that winter El Niño has positive impacts on TP snow by increasing storm activity and resultant snowfall (Shaman and Tziperman, 2005), which reinforce snow-albedo feedbacks and strengthen the associated circulation response. This process amplifies both the spatial extent and magnitude of circulation anomalies in Niño 1<inline-formula><mml:math id="M220" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>+</sup>&amp;TPSC<sup>+</sup>, indicating significant synergistic effects of El Niño and TP snow cover during their positive phases.</p>
      <p id="d2e3088">During Niño 1<inline-formula><mml:math id="M223" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>−</sup> years, positive geopotential height anomalies are observed over Northeast Asia (Fig. 8d), which appear inconsistent with the regression results (Fig. 4a). This discrepancy arises because the Niño 1<inline-formula><mml:math id="M226" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>TPSC<sup>−</sup> composite includes three years with neutral TPSC conditions and four years with positive TPSC anomalies (Table 1). As a result, the circulation pattern is partly influenced by positive TPSC signals and exhibits geopotential height features resembling those associated with TPSC<inline-formula><mml:math id="M229" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> years (Fig. 8e). This inconsistency reflects a methodological limitation related to the small sample size inherent in the phase-classification approach (Li et al., 2019). Although geopotential height anomalies during Niño 1<inline-formula><mml:math id="M230" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>−</sup>&amp;TPSC<sup>−</sup> years are stronger than those in &amp;TPSC<inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>\</mml:mo></mml:mrow></mml:math></inline-formula>Niño 1<inline-formula><mml:math id="M234" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2<sup>−</sup> years, suggesting that simultaneous negative phases of Niño 1<inline-formula><mml:math id="M236" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TPSC may also interact synergistically to enhance the circulation response, the synergistic effect is more robust and dynamically coherent during their positive phases. Therefore, we primarily conclude that Niño 1<inline-formula><mml:math id="M237" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>2 and TP snow cover interact synergistically when both are in their positive phases.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Discussion</title>
      <p id="d2e3232">This study reveals that winter PM<sub>2.5</sub> variability across China is governed by a combination of anthropogenic emissions and large-scale climate variability. The leading EOF mode reflects the dominant role of emission changes, capturing the rapid increase in PM<sub>2.5</sub> before 2013 and a sharp decline due to stringent clean air policies. In contrast, the second mode highlights a circulation-driven north-south dipole pattern over eastern China, underscoring the critical role of atmospheric circulation in redistributing PM<sub>2.5</sub>.</p>
      <p id="d2e3262">Previous studies have established that ENSO can significantly modulate winter PM<sub>2.5</sub> over China through atmospheric teleconnections. For instance, higher (lower) winter PM<sub>2.5</sub> concentrations are observed over BTH (PRD) during El Niño years (Xie et al., 2022; An et al., 2022; Zhao et al., 2022). While these studies have identified a north-south dipole structure in PM<sub>2.5</sub> and emphasized the role of ENSO, the effect of ENSO on northern China PM<sub>2.5</sub> remains debated (Zhao et al., 2022), with its influence being more robustly established over southern China. Our results are broadly consistent with these findings and further clarify that El Niño primarily modulates winter PM<sub>2.5</sub> through large-scale circulation anomalies that enhance moisture transport and wet scavenging in southern China, while its effect on northern China ventilation is comparatively weaker and less definitive.</p>
      <p id="d2e3310">Beyond ENSO, we identify that elevated snow cover over the northern TP increases snow albedo and cools the atmospheric column via snow-albedo feedbacks, weakening the subtropical westerly jet and inducing anticyclonic anomalies over northern China. These circulation changes promote stagnant conditions and enhance aerosol hygroscopic growth, increasing PM<sub>2.5</sub> concentrations in northern China. This represents a previously underexplored pathway by which cryospheric anomalies influence surface air quality (Chen et al., 2021; You et al., 2020; Yao et al., 2019), thereby broadening current understanding of how climate modes regulate aerosol distributions. Importantly, El Niño and TP snow cover do not act independently. During their concurrent positive phases, circulation anomalies over East Asia are amplified, leading to a more pronounced north-south PM<sub>2.5</sub> dipole. Specifically, El Niño exerts a dominant control over PM<sub>2.5</sub> variability in southern China, whereas TP snow cover plays a more decisive role in northern China.</p>
      <p id="d2e3340">Several limitations of this study should be acknowledged.The relatively short PM<sub>2.5</sub> observational limits constrains the robustness of statistical relationships at longer timescales. In addition, the idealized albedo perturbation in the CESM<sub>TPSC</sub> experiment does not explicitly simulate snow depth, density, or melting processes, which may lead to an overestimation of snow forcing strength compared to realistic conditions. Moreover, the CESM sensitivity experiments are based on a single-winter simulation, preventing a rigorous assessment of statistical significance in the presence of internal atmospheric variability. The model results are therefore interpreted as qualitative sensitivity tests that support the directionality of the identified mechanisms rather than as quantitative estimates of forced responses. Nevertheless, the consistency between EOF analysis, regression diagnostics, and targeted model experiments increases confidence in our main conclusions. Our results suggest that, in addition to anthropogenic emissions, ENSO and TP snow cover are dominant climate factors, modulating winter PM<sub>2.5</sub> variability in China. These insights offer promising potential for enhancing seasonal prediction of winter air quality and informing PM<sub>2.5</sub> pollution management strategies.</p>
</sec>

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

      <p id="d2e3384">The meteorological Reanalysis are from ERA5 reanalysis data (<uri>https://cds.climate.copernicus.eu/datasets</uri>, last access: 25 June 2026). Snow cover data is obtained from <ext-link xlink:href="https://doi.org/10.7289/V5N014G9" ext-link-type="DOI">10.7289/V5N014G9</ext-link> (Robinson et al., 2012). MEIC anthropogenic emissions can be found from <uri>http://meicmodel.org.cn</uri> (last access: 25 June 2026). Satellite derived ground-level PM<sub>2.5</sub> data is from <ext-link xlink:href="https://doi.org/10.5281/zenodo.8313613" ext-link-type="DOI">10.5281/zenodo.8313613</ext-link> (Bai and Li, 2023).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e3408">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-9207-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-9207-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e3417">This study was conceived by MG and XZ. XZ, YH and SC conducted simulations. XA, CS, WD, XC and QY assisted with the discussion and commented on the paper. XH, ZQ, Z, Zhang and Z, Zhuang. assisted with data collections and statistical analysis. All authors contributed to the final interpretation and writing of the manuscript with major contributions by MG and XZ.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e3423">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="d2e3429">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><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e3435">This study was supported by the grants from the National Natural Science Foundation of China (Project No. 42322902 and 42375095), Key Laboratory of Urban Meteorology, China Meteorological Administration (Project No. LUM-2025-12), the Research Grants Council of the Hong Kong Special Administrative Region, China (Project Nos. C2002-22Y, HKBU12201023, and HKBU12202824), and National Key Research and Development Programs of China (No. 2022YFC3700103).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e3441">This paper was edited by Zhonghua Zheng and reviewed by two anonymous referees.</p>
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