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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-25-12811-2025</article-id><title-group><article-title>Divergent changes in aerosol optical hygroscopicity and new particle formation during a heatwave of summer 2022</article-title><alt-title>Divergent changes in aerosol optical hygroscopicity and new particle formation</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" equal-contrib="yes" corresp="no" rid="aff1">
          <name><surname>Hao</surname><given-names>Yuhang</given-names></name>
          
        <ext-link>https://orcid.org/0009-0003-9411-7962</ext-link></contrib>
        <contrib contrib-type="author" equal-contrib="yes" corresp="no" rid="aff1">
          <name><surname>Li</surname><given-names>Peizhao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Gou</surname><given-names>Yafeng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wang</surname><given-names>Zhenshuai</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Tian</surname><given-names>Mi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Chen</surname><given-names>Yang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7269-7933</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kuang</surname><given-names>Ye</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4813-9784</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Xu</surname><given-names>Hanbing</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wan</surname><given-names>Fenglian</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Luo</surname><given-names>Yuqian</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Huang</surname><given-names>Wei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff6">
          <name><surname>Chen</surname><given-names>Jing</given-names></name>
          <email>chen.jing@cqu.edu.cn</email>
        <ext-link>https://orcid.org/0000-0002-8994-4694</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>College of Environment and Ecology, Chongqing University, Chongqing 400045, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Center for the Atmospheric Environment Research, Chongqing Institute of Green and Intelligent Technology, Chinese Academy of Sciences, Chongqing 400714, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute for Environmental and Climate Research, Jinan University, Guangzhou 511443, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Experimental Teaching Center, Sun Yat-sen University, Guangzhou 510275, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>National Meteorological Center, China Meteorological Administration, Beijing 100081, China</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Key Laboratory of Three Gorges Reservoir Region's Eco-Environment, Ministry of Education, Chongqing University, Chongqing 400045, China</institution>
        </aff><author-comment content-type="econtrib"><p>These authors contributed equally to this work.</p></author-comment>
      </contrib-group>
      <author-notes><corresp id="corr1">Jing Chen (chen.jing@cqu.edu.cn)</corresp></author-notes><pub-date><day>15</day><month>October</month><year>2025</year></pub-date>
      
      <volume>25</volume>
      <issue>20</issue>
      <fpage>12811</fpage><lpage>12830</lpage>
      <history>
        <date date-type="received"><day>17</day><month>October</month><year>2024</year></date>
           <date date-type="rev-request"><day>15</day><month>November</month><year>2024</year></date>
           <date date-type="rev-recd"><day>4</day><month>August</month><year>2025</year></date>
           <date date-type="accepted"><day>8</day><month>August</month><year>2025</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2025 Yuhang Hao et al.</copyright-statement>
        <copyright-year>2025</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025.html">This article is available from https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e222">As a crucial climate-forcing driver, the aerosol optical enhancement factor (<inline-formula><mml:math id="M1" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)) is significantly modulated by chemical compositions and the evolution of particle number size distribution (PNSD), e.g., during new particle formation (NPF). However, mechanisms regulating aerosol optical hygroscopicity during different NPF days, particularly those under heatwaves due to global warming, remain poorly understood. In the hot summer of 2022 in urban Chongqing of southwest China, simultaneous measurements of aerosol optical and hygroscopic properties, PNSD, and bulk chemical compositions were conducted. Two distinct types of NPFs were identified: NPFs with relatively polluted periods (NPF<sub>polluted</sub>) and  clean cases during heatwave-dominated periods (NPF<sub>clean, HW</sub>). Compared to the NPF<sub>polluted</sub> events, NPF<sub>clean, HW</sub> occurred approximately 1 h earlier, and the subsequent growth was prolonged, accompanied by a smaller aerosol effective radius (<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and lower formation/growth rate during heatwaves. This agreed with the concurrently increased aerosol hemispheric backscattering fraction and scattering Ångström exponent. A generally higher <inline-formula><mml:math id="M7" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) was observed on NPF days than in non-event cases, partly attributable to distinct changes in PNSD patterns during NPF days. Moreover, heatwave-induced stronger photooxidation may intensify the formation of more hygroscopic secondary components and prolong the atmospheric aging/subsequent growth of both pre-existing and newly formed particles, largely contributing to the enhanced <inline-formula><mml:math id="M8" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), especially during NPF<sub>clean, HW</sub> days. The higher <inline-formula><mml:math id="M10" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and lowered <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> could synergistically elevate the aerosol direct radiative forcing, specifically under persistent heatwave conditions. Further in-depth exploration of molecular-level characterizations and the aerosol radiative impacts of both direct and indirect interactions under heatwaves in a warming climate is recommended.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42105075</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Venture and Innovation Support Program for Chongqing Overseas Returnees</funding-source>
<award-id>cx2021021</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="d2e348">Weather extremes (e.g., heatwaves) have become more and more frequent and intense, largely due to global climate change, and  heatwave-driven environmental, climatic, and health effects have garnered widespread attention (Hauser et al., 2016; Sun et al., 2016). The China Climate Bulletin 2022 confirmed that the national average temperature had reached an unprecedented high level since 2012 (China Meteorological Administration, 2022), and the risk of heatwaves in China will persist and potentially intensify in the future (Guo et al., 2016; Li et al., 2017). Extreme-heatwave events could pose significant threats to human health, the survival of organisms, agriculture, and socio-economic activities (e.g., power supply restrictions) (Brooke Anderson and Bell, 2011; Ma et al., 2021; Su, 2021). Moreover, heatwaves can trigger natural disasters such as droughts and wildfires, affecting social stability (Sharma and Mujumdar, 2017).</p>
      <p id="d2e351">Heatwaves can also affect atmospheric physical and chemical processes by modulating ambient meteorological conditions. Specifically, extremely high temperature weather is typically characterized by a combination of intensified solar radiation with elevated temperature and low humidity levels. This could significantly affect the formation and evolution of secondary aerosols in the atmosphere (Bousiotis et al., 2021; Hamed et al., 2011; Kurtén et al., 2007), given that  air temperature is crucial for chemical reactions (Xu et al., 2011). New particle formation (NPF) serves as a crucial source of atmospheric particulate matter and plays a significant role in the secondary transformation processes in the atmosphere (Zhu et al., 2021). Generally, NPF involves the initial formation of thermodynamically stable clusters from condensable vapors (e.g., ammonia, sulfuric acid, and organic precursor gases) and subsequent growth of the formed clusters, eventually reaching detectable sizes or even larger dimensions (Kerminen et al., 2018; Kulmala, 2003; Kulmala et al., 2012). Over time, these newly formed particles have the potential to serve as cloud condensation nuclei (CCN), thereby impacting the global climate (Salma et al., 2016). NPF events normally introduce a sharp increase in the number concentration of nucleation mode particles within a short time, altering the particle number size distribution (PNSD). These variations in PNSD likely influence the intrinsic physicochemical properties of aerosols, such as the optical hygroscopicity (Chen et al., 2014; Titos et al., 2016; Zhao et al., 2019).</p>
      <p id="d2e354">Aerosol hygroscopicity plays a critical role in the atmospheric environment and climate change, given the complex interaction between aerosol particles and water vapor (Zhao et al., 2019; Zieger et al., 2011). Water uptake by aerosols not only alters the particle size and composition (e.g., as reflected in the aerosol refractive index) but also impacts aerosol scattering efficiency, which further contributes to the uncertainty in aerosol radiative forcing estimation (Titos et al., 2016, 2021). The aerosol optical hygroscopicity parameter, <inline-formula><mml:math id="M12" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), defined as the ratio of the scattering coefficient at a certain RH to that of the dry condition, has been widely used to describe the aerosol scattering enhancement through water uptake (Covert et al., 1972; Titos et al., 2016; Zhao et al., 2019). Numerous studies have demonstrated that <inline-formula><mml:math id="M13" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) is influenced by  size distribution, in addition to particle chemical composition (Chen et al., 2014; Kuang et al., 2017; Petters and Kreidenweis, 2007; Quinn et al., 2005). There is currently limited research on the variations in aerosol optical hygroscopicity during NPF days despite significant changes in aerosol size distributions and chemical compositions, partly due to the fact that newly formed particles insignificantly affect the optical properties of aerosols (Kuang et al., 2018). However, previous studies have observed an enhancement in aerosol hygroscopicity (Cheung et al., 2020; Wu et al., 2015, 2016) and extinction coefficients (Shen et al., 2011; Sun et al., 2024) during the subsequent growth of NPF. It is suggested that the influence of NPF on aerosol hygroscopicity was likely due to changes in aerosol chemical composition at different stages of NPF events (Cheung et al., 2020), whereas the subsequent particle growth associated with NPF events can significantly affect particle hygroscopicity as well (Wu et al., 2016). Although previous studies have shown the dependences of aerosol hygroscopicity on chemical composition (Petters and Kreidenweis, 2007; Titos et al., 2016; Zhao et al., 2019) (e.g., variations in the composition of precursor species during NPF events), it is important to acknowledge that the utilized chemical compositions of NPF were either from PM<sub>2.5</sub> or from PM<sub>1</sub> bulk data. This may differ from the corresponding composition of newly formed ultrafine particles, primarily in the nucleation and Aitken modes, further introducing bias in exploring the impacts of NPF and subsequent growth on aerosol optical hygroscopicity. Hence, more comprehensive investigations on the mechanisms influencing  aerosol optical hygroscopicity from different perspectives are required, e.g., for the aspects of the evolution of particle size distribution in modulating aerosol optical and hygroscopic properties (Tang et al., 2019; Zhao et al., 2019). Additionally, field observations on <inline-formula><mml:math id="M16" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) under extreme-weather conditions (e.g., heatwaves) are rather scarce, largely hindering our understanding of how weather extremes (e.g., extremely high temperature) influence the optical hygroscopic properties of aerosols. This knowledge gap further impedes a comprehensive understanding of the aerosol water uptake property and resulting effects on air quality and the climate under varied synoptic conditions.</p>
      <p id="d2e396">During the summer of 2022, a rare heatwave event raged throughout China, especially in the Sichuan–Chongqing region of southwest China (Chen et al., 2024; Wang et al., 2024), with the daily maximum temperature exceeding 40° and lasting for 29 d, as observed at the Beibei meteorological station in Chongqing (Hao et al., 2023). This persistent heatwave not only impacted residents' daily lives significantly, but also affected  aerosol optical and hygroscopic properties, likely through changed aerosol physicochemical characteristics and relevant atmospheric processing during this period. In this study, a field observation was conducted by using a combination of a home-built humidified nephelometer system and a scanning mobility particle sizer (SMPS), along with total suspended particle (TSP) filter sampling. A main goal of this study is to investigate the influence of heatwaves on both aerosol optical hygroscopicity and the NPF with subsequent growth events, along with the related discrepancies. Furthermore, we aimed to explore the mechanisms behind the variability in <inline-formula><mml:math id="M17" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) under different meteorological conditions and diverse NPF events. This study will further enrich insights into the potential environmental impacts due to variations in aerosol optical hygroscopicity and size distribution, specifically under heatwaves in a changing climate.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Field observation</title>
      <p id="d2e421">A continuous field observation on aerosol optical, hygroscopic, and chemical properties was carried out from 29 July to 19 August  2022. A detailed description of the observation site is available in Supplement S1. During the observation period, urban Chongqing suffered a rare heatwave (Fig. S1; Chen et al., 2024; Wang et al., 2024), which significantly affected local transportation and industrial activities (Hao et al., 2023). The China Meteorological Administration (CMA) defines heatwaves as 3 or more consecutive days with daily maximum temperature (<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) above 35 °C (<uri>http://www.cmastd.cn/standardView.jspx?id=2103</uri> (last access: 7 October 2025); Guo et al., 2016; Sun et al., 2014; Tan et al., 2007). Since there is no unified definition of heatwaves worldwide, the whole study period was categorized into two stages according to CMA's criteria for daily <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> records and the excess heat factor (EHF) metric proposed by Nairn and Fawcett (2014) (Fig. S2a): (1) the normally hot period from 29 July to 6 August (marked as P1) and (2) the heatwave-dominated period from 7–19 August  (marked as P2), characterized by the consistent occurrence of <inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">max</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> exceeding 38 °C (approximately the lowest 25th percentile of temperature records for the whole observation period; Fig. S2b).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Instrumentation and methods</title>
<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Measurements of aerosol optical hygroscopicity</title>
      <p id="d2e475">The humidified nephelometer system, consisting of two three-wavelength (i.e., 450, 525, and 635 nm) nephelometers (Aurora 3000, Ecotech Inc.) and a humidification unit, was used to determine the aerosol light scattering enhancement factor, <inline-formula><mml:math id="M21" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH). Ambient air was first dried through a Nafion dryer (MD-700, Perma Pure LLC) to ensure RH <inline-formula><mml:math id="M22" display="inline"><mml:mspace width="0.125em" linebreak="nobreak"/></mml:math></inline-formula>&lt;<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> %, then split into two streams for both dry and humidified nephelometers operated in parallel. The flow rate for each nephelometer was 2.6 LPM. The aerosol scattering (<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and backscattering coefficients (<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">bsca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) were detected in a dry state (RH <inline-formula><mml:math id="M26" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 35 %) and at a controlled RH level of 85 <inline-formula><mml:math id="M27" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 %, respectively, with the humidification efficiency regulated automatically by a temperature-controlled water bath. More details on the home-built humidified nephelometer system are available in Kuang et al. (2017, 2020) and Xue et al. (2022).</p>
      <p id="d2e549">Hence, <inline-formula><mml:math id="M28" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) could be calculated as the ratio of the aerosol scattering coefficient at a predefined RH (<inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">RH</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) to the dry (<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">dry</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) state; i.e., <inline-formula><mml:math id="M31" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="1em"/><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">RH</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">dry</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (Covert et al., 1972). In this study, the <inline-formula><mml:math id="M33" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) discussed is mainly targeted at the 525 nm wavelength, unless otherwise specified. More information about the measurements of the humidified nephelometer system is illustrated in Sect. S2 of the Supplement.</p>
      <p id="d2e641">In addition to <inline-formula><mml:math id="M34" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), aerosol optical parameters, such as the scattering Ångström exponent (SAE; Schuster et al., 2006) and hemispheric backscattering fraction (HBF; Collaud Coen et al., 2007), were calculated as below:

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M35" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">SAE</mml:mi><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mi>ln⁡</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">HBF</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="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">bsca</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">bsca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> represent the aerosol scattering and backscattering coefficients at a specific wavelength <inline-formula><mml:math id="M38" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (e.g., <inline-formula><mml:math id="M39" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>1, <inline-formula><mml:math id="M40" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula>2), respectively.</p>
      <p id="d2e828">Both HBF and SAE reflect crucial optical properties of aerosols, e.g., an elevated HBF (or SAE) generally signifies a higher concentration (or a smaller particle size) of fine particles within the aerosol population (Jefferson et al., 2017; Kuang et al., 2017; Luoma et al., 2019). The HBF and SAE discussed in this study are targeted at the dry condition, unless otherwise specified. Based on the measurements with the humidified nephelometer system, the equivalent aerosol liquid water content (ALWC) and the corresponding fraction of ALWC (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) can also be obtained (Kuang et al, 2018; see Sect. S2 of the Supplement).</p>
      <p id="d2e843">The SMPS-measured concurrent particle number size distributions were further utilized to calculate the aerosol effective radius (<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and parameters representative of NPF events, e.g., the formation rate (FR) and growth rate (GR) of new particles, condensation sink (CS), and coagulation sink (CoagS) (Dal Maso et al., 2005; Kulmala et al., 2012). More details are provided in the Supplement (Sect. S5).</p>
      <p id="d2e857">Results of the offline chemical analysis with TSP filter samples are provided in Sect. S3 and Fig. S3. It should be noted that certain secondary organics and crustal elements (e.g., Ca<sup>2+</sup>, Mg<sup>2+</sup>) that could exhibit a broader size distribution may contribute to the observed discrepancy in the total mass concentration between the 24 h TSP samples and daily mean PM<sub>2.5</sub> (of similar temporal variations; Fig. S3) (Duan et al., 2024; Kim et al., 2020; Xu et al., 2021). Nonetheless, previous studies have reported that key components such as SNA (i.e., SO<inline-formula><mml:math id="M46" 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="M47" 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="M48" 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 primary organics of PM<sub>2.5</sub> (or PM<sub>10</sub>) were predominantly concentrated within the submicron size range (An et al., 2024; Bae et al., 2019; Chen et al., 2019; Duan et al., 2024; Kim et al., 2020; Xu et al., 2024). While the use of TSP samples contains some uncertainties, the bulk chemical information remains reasonable for characterizing the optical and hygroscopic properties of PM<sub>2.5</sub>. Descriptions of simultaneously collected meteorological and air quality data can be found in Sect. S4, and the 48 h/72 h backward trajectory analysis is given in Sect. S5 of the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <label>2.2.2</label><title>Determination of the aerosol direct radiative forcing (ADRF) enhancement factor</title>
      <p id="d2e968">Given the high sensitivity of aerosol optical properties (e.g., <inline-formula><mml:math id="M52" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)) to the changes in RH under real atmospheric conditions, the influence of RH, or rather the aerosol hygroscopicity, on ADRF can be quantitatively estimated with the radiative transfer model using the following equation (Chylek and Wong, 1995; Kotchenruther et al., 1999; L. Zhang et al., 2015):

              <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M53" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">FR</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:mfenced close="]" open="["><mml:mrow><mml:msubsup><mml:mi>T</mml:mi><mml:mi mathvariant="normal">a</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>×</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>×</mml:mo><mml:mo mathsize="2.5em">[</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>×</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo mathsize="2.5em">]</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is the solar constant, <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the atmosphere transmittance, <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the fractional cloud amount, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the albedo of the underlying surface, <inline-formula><mml:math id="M58" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>(RH) is the upscattering fraction at a defined RH, and <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the optical thicknesses of the aerosol layer due to light scattering and light absorption, respectively, which can be expressed as follows (Kotchenruther et al., 1999):

              <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M61" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>M</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>M</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math id="M62" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> is the column burden of aerosol (unit: g m<sup>−2</sup>), <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass scattering efficiency (MSE), and <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mass absorption efficiency (MAE). The direct radiative forcing is usually calculated with the assumption that the absorption enhancement is negligible in comparison to the aerosol scattering enhancement (Xia et al., 2023).</p>
      <p id="d2e1280">Hence, the dependence of ADRF on RH (i.e., <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH)) can be estimated by Eq. (5) (Chylek and Wong, 1995; Kotchenruther et al., 1999; L. Zhang et al., 2015):

              <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M67" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">dry</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>×</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">RH</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>R</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>×</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">β</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">dry</mml:mi><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">dry</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

            where the constant parameters used are <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.15</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> m<sup>2</sup> g<sup>−1</sup> (Hand and Malm, 2007; Fierz-Schmidhauser et al., 2010). It should be noted that the assumed constant <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> might introduce some uncertainty in the calculated <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH), given the fact that the contribution of absorption by brown carbon was unknown, although the mass fraction of BC in TSP remained almost constant (i.e., 4.6 % <inline-formula><mml:math id="M74" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.1 %, Fig. S3) during the observation period. The parameter <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was calculated by dividing <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> in the dry condition by the mass concentration of PM<sub>2.5</sub> (i.e., <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> PM<sub>2.5</sub>). <inline-formula><mml:math id="M80" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> could be calculated empirically from the measured HBF: <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.0817</mml:mn><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1.8495</mml:mn><mml:mo>×</mml:mo><mml:mi mathvariant="normal">HBF</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.9682</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mi mathvariant="normal">HBF</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (Delene and Ogren, 2002).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Overview of the aerosol optical hygroscopicity and PNSD measurements</title>
      <p id="d2e1696">Figure 1 displays the time series of the measured aerosol scattering coefficients, <inline-formula><mml:math id="M82" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), PNSD, and the corresponding meteorological conditions and air pollutants during the study period. A sharp decrease in aerosol scattering coefficients and PM<sub>2.5</sub>, accompanied by  continuous excellent visibility over 20 km, was observed after 6 August, indicating a markedly cleaner environment during P2 in comparison to P1 in the summer of 2022 of Chongqing. This can largely be attributed to the reduction in anthropogenic emissions (e.g., NO<sub>2</sub> and CO but not SO<sub>2</sub>) from limited outdoor activities influenced by the heatwaves in P2, as well as from the partial suspension of industries and transportation to alleviate the power shortage issue (Chen et al., 2024). Notably, the increased wind speed and enhanced mixing layer height (MLH) also enabled a more favorable atmospheric diffusion condition in P2, facilitating the dilution of surface air pollutants (Zhang et al., 2008). However, a higher mass concentration of SO<sub>2</sub> was observed in the P2 period, likely due to a surge in electricity demand and resulting higher emissions from power plants operating  at almost full capacity during the heatwave (Su, 2021; Teng et al., 2022). Moreover, significant discrepancies in aerosol optical and hygroscopic properties were observed under different synoptic conditions (Table S2). Both HBF and SAE were higher during the P2 period, aligning with the smaller <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Table S2). <inline-formula><mml:math id="M88" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) was found to be relatively higher (<inline-formula><mml:math id="M89" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 0.05) on heatwave days, with  mean values of 1.61 <inline-formula><mml:math id="M91" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.12 and 1.71 <inline-formula><mml:math id="M92" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.15 during the P1 and P2 periods, respectively. In contrast, ALWC was more abundant during the normally hot P1 period than the heatwave-dominated P2 period. This is likely due to the fact that the derivation algorithm of ALWC utilized in this study (Kuang et al., 2018) is partly dependent on (e.g., positively correlated to) the dry aerosol scattering coefficient or, rather, the aerosol volume concentration in the dry condition (refer to Sect. S3 and Fig. S11 of the Supplement). The mean <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for P2 was about 46.8 % of that for the P1 period, and the corresponding mean level of ALWC was approximately 55.8 % of that for P1. This partly agrees with the stronger aerosol optical hygroscopicity, with a marginally higher <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> during the P2 period, highlighting a complex interaction between the optical enhancement and aerosol physicochemical properties.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e1820">Time series of the measured aerosol scattering coefficients, <inline-formula><mml:math id="M95" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), meteorological conditions, air pollutants, and particle number size distribution during the study period.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f01.png"/>

        </fig>

      <p id="d2e1836">The particle number size distribution data suggested that NPF events occurred on about half of the observation days (Fig. 1i), with an overall occurrence frequency of 52.4 % (Fig. S4a). This indicates that summer NPF events are rather frequent in Chongqing, being notably more common than those observed in other regions of the world, e.g., Beijing (16.7 %, Deng et al., 2020; <inline-formula><mml:math id="M96" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 %, Wang et al., 2013), Dongguan (4 %, Tao et al., 2023), Hyytiälä (<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> %, Dada et al., 2017), and LiLLE (<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi mathvariant="italic">&lt;</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> %, Crumeyrolle et al., 2023). Moreover, the frequent NPF events during heatwaves formed substantially ultrafine particles that contributed less to aerosol optical properties in comparison to large particles (Fig. S13), partially explaining the significantly lower levels of total scattering coefficients observed during the P2 period. It should be noted that the hourly <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> values during the P2 period were exclusively below 100 Mm<sup>−1</sup> (approximately the lowest 10th percentile of <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> data, regarded as the threshold value of relatively polluted cases; Fig. S2c), suggesting a much cleaner environment compared to the relatively polluted P1 period. Correspondingly, NPF events occurring during the relatively polluted P1 period (as detailed in Sect. 3.2) are defined as NPF<sub>polluted</sub>, while cases during the cleaner and heatwave-dominated P2 period are classified as NPF<sub>clean, HW</sub>.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Characteristics of NPF events in different periods</title>
      <p id="d2e1945">Aside from gaseous precursors (e.g., SO<sub>2</sub>, volatile organic compounds), meteorological conditions also play a key role in the occurrence of NPF events. In brief, NPF events are more likely to appear under sunny and clean conditions (Bousiotis et al., 2021; Crumeyrolle et al., 2023; Deng et al., 2021; Wang et al., 2017). The backward trajectory analysis revealed that a southerly breeze was predominant during the study period (Fig. S4b). Although the surface wind vector slightly varied between the P1 and P2 periods, this consistency in air mass origins suggests that some other factors (e.g., changes in environmental conditions and emissions of gaseous precursors under heatwaves) could have played a crucial role in modulating NPF events. To further explore the characteristics of NPF events in different periods, the time-averaged diurnal variations in meteorological parameters and air pollutant concentrations during both NPF events and non-event days are presented in Fig. 2.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1959">Diurnal variations in temperature <bold>(a)</bold>, PM<sub>2.5</sub> mass loading <bold>(b)</bold>, RH <bold>(c)</bold>, SO<sub>2</sub>
<bold>(d)</bold>, UVB <bold>(e)</bold>, H<sub>2</sub>SO<sub>4</sub> <bold>(f)</bold>, O<inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> O<sub><italic>X</italic></sub> <bold>(g)</bold>, O<sub>3</sub> <bold>(h)</bold>, WS <bold>(i)</bold>, NO<sub>2</sub> <bold>(j)</bold>, MLH <bold>(k)</bold>, and CO <bold>(l)</bold> during P1 (red) and P2 (blue) NPF days (solid line), as well as the corresponding non-event days (dashed line).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f02.png"/>

        </fig>

      <p id="d2e2082">As stated in Sect. 3.1, NPF events during the P1 period tended to occur in relatively polluted environments compared to those of P2 NPF<sub>clean, HW</sub> events, as evidenced by the frequent occurrence of <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> Mm<sup>−1</sup>, increased air pollutant concentrations, and lower visibility levels during P1 (Table S2, Fig. 1). Additionally, the mean CS of the NPF<sub>polluted</sub> events was above 0.015 s<sup>−1</sup> (Table S2), which could be considered  “polluted” NPF cases (Shang et al., 2023). On P2 NPF<sub>clean, HW</sub> days, the overall mean <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> was <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mn mathvariant="normal">33.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">11.7</mml:mn></mml:mrow></mml:math></inline-formula> Mm<sup>−1</sup>, decreased by 68.0 % (39.3 %) in comparison to that for P1 NPF<sub>polluted</sub> days (P2 non-event days). In addition, the mean PM<sub>2.5</sub> concentration was even lower than 10.0 <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<sup>−3</sup>, and the corresponding visibility level was almost maintained at 30 km (Fig. 1e). All the above implies that the P2 NPF<sub>clean, HW</sub> events were generally accompanied by a much cleaner environment. It is notable that the increase in SO<sub>2</sub> concentration after 09:00 LT (Fig. 2d), along with the significant decrease in PM<sub>2.5</sub> mass loadings after 08:00 LT during P1 NPF<sub>polluted</sub> events (Fig. 2b), likely favored the occurrence of NPF events. The higher gas-phase sulfuric acid (i.e., H<sub>2</sub>SO<sub>4</sub>, as estimated with the UVB and SO<sub>2</sub> concentration; Lu et al., 2019; Sect. S4) on the same NPF days (Fig. 2f) further suggests that sulfuric acid concentration was a critical factor for the occurrence of P1 NPF<sub>polluted</sub> events.</p>
      <p id="d2e2330">The diurnal evolutions of meteorological conditions (e.g., <inline-formula><mml:math id="M134" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, RH, MLH) for NPF events were distinct between the P1 and P2 periods, although relatively insignificant differences were observed for both NPF days and non-event days within the same period (Fig. 2). This likely suggests that meteorological factors might not be the predominant determining factor of NPF occurrence during the heatwaves of the summer of 2022  in urban Chongqing, while NPF could be accompanied by quite different meteorological conditions depending on gaseous precursors and pre-existing condensation sinks. For instance, the NPF<sub>clean, HW</sub> events were typically clean-type NPF, characterized by lower background aerosol loading, higher temperature, and favorable atmospheric dispersion capacity with the higher MLH. However, it is reported that excessive heat can increase the evaporation rate of critical acid-base clusters during the nucleation process and reduce the stability of initial molecular clusters (Bousiotis et al., 2021; Kurtén et al., 2007; Zhang et al., 2012), in line with a recent study reporting that NPF events were weaker during heatwaves in a Siberian boreal forest due to the unstable clusters (Garmash et al., 2024). On the other hand, the emission rate of biogenic VOCs (BVOC<sub>S</sub>, e.g., isoprene, monoterpene) from nearby plants and trees would decrease when temperature exceeded around 40 °C (Guenther et al., 1991; Pierce and Waldruff, 1991), despite the fact that BVOCs play a key role in the nucleation mechanism of NPF (Wang et al., 2017; Zhang et al., 2004). Hence, the even higher temperature (e.g., <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula>°) likely suppressed the nucleation processes and the subsequent growth of nucleation mode particles on P2 non-event days (Fig. S6b2), in spite of higher concentrations of SO<sub>2</sub> and H<sub>2</sub>SO<sub>4</sub>.</p>
      <p id="d2e2404">To further investigate the effect of heatwaves on NPF events, the diurnal variations in PNSD, <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and particle mode diameter (<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) are shown in Fig. S6. Aerosol number and volume concentrations, as well as <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, for different modes are illustrated in Figs. S7–S8, and the relationship between temperature and the duration of NPF events is displayed in Fig. S9. Distinct particle size distributions were observed for different NPF event days. While the number concentrations of Aitken mode particles (<inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">Ait</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) were comparable during NPF days of both periods, the corresponding number concentration of nucleation mode particles (<inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">Nuc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) was significantly higher on P1 NPF<sub>polluted</sub> days (1880.8 <inline-formula><mml:math id="M147" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2261.5 cm<sup>−3</sup>) than on P2 NPF days (1132.0 <inline-formula><mml:math id="M149" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1333.5 cm<sup>−3</sup>) (Figs. 1i, S7). Different from that of the P1 NPF<sub>polluted</sub> cases, the P2 NPF<sub>clean, HW</sub> event did not start from the minimum size, and the reduced <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">Nuc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> during the P2 period is likely attributable to the influence of transport on the local nucleation and growth processes (Fig. S4; Cai et al., 2018; Lee et al., 2019). Namely, some nucleation mode particles transported from upwind regions or from the mixing layer downwards had undergone atmospheric aging and thereby a certain degree of growth upon arrival (Cai et al., 2018; Lai et al., 2022; Platis et al., 2016), resulting in relatively lower concentrations of smaller-sized particles than in the case of locally formed particles. However, the local formation of sub-25 nm particles and the continuous growth process were still distinctly observed under heatwaves (Figs. 1i, S6, S15). The NPF events under heatwaves usually initiated earlier (Fig. S9), with  <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:mi mathvariant="normal">Nuc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> in P2 NPF<sub>clean, HW</sub> cases peaking about an hour earlier in comparison to NPF<sub>polluted</sub> days (Fig. S8a). <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on P2 NPF<sub>clean, HW</sub> days also reached its minimum earlier than on P1 NPF<sub>polluted</sub> days (Fig. S6). Since the sunrise and sunset times did not significantly vary within the study period (i.e., less than a half-hour discrepancy), heatwaves likely provided more favorable conditions (e.g., enhanced volatile gaseous emissions, low RH; Bousiotis et al., 2021; Hamed et al., 2007; Wang et al., 2024) for the occurrence of NPF events in urban Chongqing. This is supported by the earlier start time of NPF<sub>clean, HW</sub>, corresponding to higher temperature ranges (Fig. S9). Furthermore, the end time of subsequent particle growth during the P2 period was even later (i.e., <inline-formula><mml:math id="M161" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 21:00 LT) than that of P1 cases (Fig. S9). Given that the growth rates of new particles were generally lower during P2 NPF<sub>clean, HW</sub> events (Table S2), these explosively formed new particles could persist longer in the warmer atmosphere and probably underwent aging processes with a relatively higher oxidation degree. This is supported by the commonly higher ratios of secondary organic carbon (SOC) to organic carbon (OC) (i.e., SOC <inline-formula><mml:math id="M163" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> OC <inline-formula><mml:math id="M164" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 0.5) during the NPF<sub>clean, HW</sub> days (Fig. S3b). In addition, aerosol <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was significantly smaller on the NPF<sub>clean, HW</sub> days under heatwave conditions. <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> were maintained at nearly the same level below/approaching 50 nm during the subsequent growth on the P2 NPF<sub>clean, HW</sub> days, while <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was generally above 50 nm and larger than <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for both P1 NPF<sub>polluted</sub> cases and non-event days (Fig. S6). The diurnal patterns of aerosol volume concentrations for different size modes were similar to those of aerosol number concentrations during NPF events (Fig. S8b1–b3). However, <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of both Aitken mode particles (<inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">Ait</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and accumulation mode particles (<inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">Acc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) was smaller during P2 NPF<sub>clean, HW</sub> events than during P1 NPF<sub>polluted</sub> events (Fig. S8c2–c3), which may further influence size-dependent aerosol optical and hygroscopic properties (e.g., <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, HBF, SAE, <inline-formula><mml:math id="M180" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)). The decrease in <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">Ait</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">Acc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> during heatwaves can be attributed to three factors: (1) evaporation of the outer layer of particles and unstable clusters due to heatwaves (Bousiotis et al., 2021; Cusack et al., 2013; Deng et al., 2020; Garmash et al., 2024; Li et al., 2019), (2) lower FR and GR of particles under cleaner-environment conditions (Table S2), and (3) reduced emissions of larger primary particles during the P2 period.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Characteristics of the aerosol optical and hygroscopic properties on different types of NPF days</title>
      <p id="d2e2916">Diurnal variations in the aerosol optical and hygroscopic parameters during different NPF days are shown in Fig. 3, and the corresponding results for non-event days are shown in Fig. S10. Generally, <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> possessed a similar bimodal diurnal pattern to that of the accumulation mode aerosol volume concentration (<inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mrow><mml:mi mathvariant="normal">Acc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) (Fig. S8b3), as supported by the positive correlation between <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and SMPS-measured aerosol volume concentration (Fig. S12). This is also consistent with Mie theory, with a stronger increase in the scattering efficiency for accumulation mode particles (Titos et al., 2021). The diurnal pattern of <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> also varied distinctly between different NPF days. Specifically, a minor peak in <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> around 12:00 LT (Fig. 3a) was influenced by the newly formed particles during P2 NPF<sub>clean, HW</sub> events, which contributed more significantly to the aerosol number and volume concentrations within 100 nm size ranges in markedly clean environments (Fig. S5c1, c2). Instead of a noontime peak, <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> was observed with an early peak around the morning rush hours, and a maximum value similarly occurred at nighttime on P1 NPF<sub>polluted</sub> days.</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e3045">Diurnal variations in <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>
<bold>(a)</bold>, <inline-formula><mml:math id="M192" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) <bold>(b)</bold>, HBF<sub>525</sub> <bold>(c)</bold>, ALWC <bold>(d)</bold>, SAE<sub>635∕450</sub> <bold>(e)</bold>, and <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <bold>(f)</bold> on NPF days during P1 (red line) and P2 (blue line) periods. The shaded areas represent the corresponding <inline-formula><mml:math id="M196" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1<inline-formula><mml:math id="M197" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> standard deviations.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f03.png"/>

        </fig>

      <p id="d2e3146">Both HBF and SAE on P2 NPF<sub>clean, HW</sub> days were significantly higher than during P1 NPF<sub>polluted</sub> cases (Fig. 3c, e), largely due to the smaller <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> observed during the heatwave-dominated period (Table S2). Moreover, the correlation between HBF (or SAE) and particle size in each mode was weaker on NPF days than on non-event days, especially for NPF<sub>clean, HW</sub> days (Fig. S14). The strongest negative correlation was found between HBF and <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of the accumulation mode in comparison to other modes, highlighting that HBF is more sensitive to the size distribution of accumulation mode particles (Collaud Coen et al., 2007). Given that NPF would largely enhance the abundance of both nucleation and Aitken mode aerosols (Fig. S7), no significant variation in HBF was observed during the daytime due to the weakened correlation between HBF and <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">Acc</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> of NPF events. SAE is commonly used as an indicator of particle size distribution, almost decreasing monotonously with the increase in aerosol size within 1 <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>m (Kuang et al., 2017, 2018; Luoma et al., 2019). Accordingly, SAE decreased over the morning and evening rush hours, when coarse particles (e.g., aged particles, road dust, automobile exhaust) generated during anthropogenic activities were present, accompanied by an increase in CO, which is taken as a proxy for primary emissions (Fig. 2l) (Yarragunta et al., 2021). In contrast, the abundant ultrafine particles formed during NPF events led to a continuous increase in SAE during the day.</p>
      <p id="d2e3234"><inline-formula><mml:math id="M205" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) exhibited a similar diurnal pattern on  P1 and P2 NPF days (Fig. 3b). During the daytime, <inline-formula><mml:math id="M206" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) remained relatively stable and gradually increased until peaking around 16:00–18:00 LT, with a generally higher <inline-formula><mml:math id="M207" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) particularly after 15:00 LT during P2 NPF<sub>clean, HW</sub> days than during P1 cases. The insignificant fluctuations in relatively lower <inline-formula><mml:math id="M209" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) levels before  noon could be attributed to the continuous development of the mixing layer (Fig. 2k), leading to  efficient mixing of particles in the nocturnal residual layer with anthropogenic emissions near the ground. Additionally, photochemical reactions in the afternoon facilitated the formation of more hygroscopic secondary aerosols with a higher oxidation level (Liu et al., 2014; R. Zhang et al., 2015). The diurnal patterns of O<sub>3</sub> and the O<inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> O<sub><italic>X</italic></sub> ratio (i.e., an indicator of atmospheric oxidation capacity, where O<inline-formula><mml:math id="M213" 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> O<inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO<sub>2</sub>, Tian et al., 2021) also showed similar trends (Fig. 2g, h). The presence of black carbon (BC) mixed with organic compounds (e.g., from traffic emissions and residential cooking activities) explained the rapid decrease in <inline-formula><mml:math id="M216" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) during the evening rush hours (Liu et al., 2011). Furthermore, the daily mean <inline-formula><mml:math id="M217" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) for NPF days was higher than that of non-event days (Table S2), particularly after the end of NPF events around 12:00 LT. Given that newly formed particles were too small to significantly impact the total light scattering (Fig. S11a), this indicates that the atmospheric conditions conducive to the occurrence of NPF may promote further growth (e.g., via intensified/prolonged photooxidation or atmospheric aging processes) of pre-existing particles and newly formed ones, partly contributing to enhanced aerosol optical hygroscopicity, as indicated by the concurrent variations in ALWC and <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in urban Chongqing during the hot summer (Asmi et al., 2010; Wang et al., 2019; Wu et al., 2016). The diurnal pattern of ALWC closely mirrored the variation in <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, while <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> followed a similar evolution to <inline-formula><mml:math id="M221" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH). This suggests that ALWC was more sensitive to changes in the aerosol volume concentration, as determined by the corresponding retrieval algorithm (Kuang et al., 2018). <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> levels were slightly higher during NPF days in comparison to those on non-event days (Table S2). This difference was more pronounced in the afternoon of NPF days (e.g., even exceeding 50 %; Fig. 3f), verifying the enhancement of aerosol hygroscopicity during the subsequent growth and atmospheric aging of both pre-existing and newly formed particles.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Heatwave-induced divergent changes in aerosol optical hygroscopicity</title>
      <p id="d2e3423">To further explore the impacts of heatwaves on <inline-formula><mml:math id="M223" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) during diverse NPF events, data mainly within the time window of 08:00–22:00 LT (i.e., typically covering the complete process of NPF and subsequent growth, while excluding higher-RH conditions at night) were utilized for the following discussion.</p>
      <p id="d2e3433">Although ultrafine particles exhibited higher number concentrations during the study period, accumulation mode particles dominated the aerosol volume concentration and contributed predominantly to the total light scattering (Figs. S7, S13). A positive correlation between <inline-formula><mml:math id="M224" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and the volume fraction of accumulation mode particles (VF<sub>Acc.</sub>) was found on non-event days (Fig. 4c–d), when the aerosol size distribution was undisturbed by newly formed ultrafine particles and the corresponding VF<sub>Acc.</sub> was maintained at a high level of approximately 0.95 (Fig. 4a–b). The notably positive correlation between <inline-formula><mml:math id="M228" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> could be linked to the secondary formation of hygroscopic particles within the accumulation mode, primarily via photochemical reactions, and further intensified by heatwaves during the non-event day, particularly in the P2 period (Gu et al., 2023; Liu et al., 2014; R. Zhang et al., 2015; Zhang et al., 2024). Consequently, <inline-formula><mml:math id="M230" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) at a specific <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was generally higher during the P2 period in comparison to that of P1 (Fig. 4c–d), also with high <inline-formula><mml:math id="M232" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) levels observed for smaller-size cases of <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M234" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 110 nm under some extremely high temperature conditions (<inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mi mathvariant="italic">&gt;</mml:mi><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula>°, as highlighted by the dashed red circle in Fig. 4d). The higher SOC <inline-formula><mml:math id="M236" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> OC on P2 non-event days further demonstrated the stronger secondary aerosol formation in comparison to P1 non-event days (Fig. S3b).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3562">Diurnal variations in <bold>(a)</bold> the number fraction (NF<sub>Acc.</sub>) and <bold>(b)</bold> volume fraction of accumulation mode particles (VF<sub>Acc.</sub>) on P1 (red) and P2 (blue) NPF days (solid line) and non-event days (dashed line). The time window of 08:00–22:00 LT is shaded in red. The relationship of <inline-formula><mml:math id="M239" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) with <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and VF<sub>Acc.</sub> (as indicated by the colored dots) on P1 <bold>(c)</bold> and P2 non-event days <bold>(d)</bold> and on P1 <bold>(e)</bold> and P2 <bold>(f)</bold> NPF days during the 08:00–22:00 LT time window.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f04.png"/>

        </fig>

      <p id="d2e3645">Nevertheless, <inline-formula><mml:math id="M242" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) was almost independent of the two parameters (i.e., <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and VF<sub>Acc.</sub>) during NPF events (Fig. 4e–f). This is mainly due to the explosive formation of ultrafine particles and their subsequent growth on NPF days, significantly altering aerosol size distributions and inducing large fluctuations in  NF<sub>Acc.</sub> and VF<sub>Acc.</sub> compared with non-event days, especially during the P2 period (as shaded in Fig. 4a–b). Therefore, characterizing <inline-formula><mml:math id="M247" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) by the corresponding <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of aerosol populations was no longer applicable. Alternatively, SAE was commonly used to estimate or parameterize <inline-formula><mml:math id="M249" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) (Titos et al., 2014; Xia et al., 2023; Xue et al., 2022), in line with the similar diurnal patterns of <inline-formula><mml:math id="M250" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE observed in this study. Figure 5 demonstrates a significantly positive correlation between <inline-formula><mml:math id="M251" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE during NPF days in comparison to non-event days, with a similar slope of approximately 0.65, suggesting the consistent variation in <inline-formula><mml:math id="M252" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) with SAE across both periods. As larger particles contributed more to  aerosol volume concentrations (Fig. S5), the decrease in SAE also corresponded to an increase in <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 5a3, b3). Given that larger <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> values typically indicate the condition of  higher aerosol loading, <inline-formula><mml:math id="M255" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) increased with SAE, whereas it decreased with <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> or rather, the pollution level, during NPF days. The cleaner environment of the P2 period may further favor the occurrence of NPF events. Both <inline-formula><mml:math id="M257" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE exhibited a higher level on P2 NPF<sub>clean, HW</sub> days (as shown by the dashed lines in Fig. 5), probably due to the following two aspects. One is related to the smaller aerosol <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (with a larger SAE) due to the lower FR and GR, likely influenced by the evaporation of newly formed unstable clusters and particle coatings under heatwaves (Bousiotis et al., 2021; Cusack et al., 2013; Deng et al., 2020) during the subsequent growth of aerosols. Secondly, the higher temperature was normally associated with stronger photochemical oxidation, which could intensify the formation of secondary aerosol components with a higher hygroscopicity (Asmi et al., 2010; Gu et al., 2023; Liu et al., 2014; Wu et al., 2016; R. Zhang et al., 2015; Zhang et al., 2024). This is further supported by the slightly higher levels of UVB (P1: 2.6 <inline-formula><mml:math id="M260" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.9 W m<sup>−2</sup> versus P2: 2.7 <inline-formula><mml:math id="M262" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 2.0 W m<sup>−2</sup>) and O<inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula> O<sub><italic>X</italic></sub> (P1: 0.81 <inline-formula><mml:math id="M266" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.17 versus P2: 0.82 <inline-formula><mml:math id="M267" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.17) during P2 heatwave days, also in line with a recent study which demonstrated that heatwaves affected secondary organic aerosol (SOA) formation and aging by accelerating photooxidation in Beijing (Zhang et al., 2024).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3918">The relationship between <inline-formula><mml:math id="M268" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE<sub>635∕450</sub>, as well as temperature (as indicated by the color of the dots; missing values are represented in gray), on P1 non-event days <bold>(a1)</bold> and NPF<sub>polluted</sub> days <bold>(a2)</bold> during the 08:00–22:00 LT time window. The vertical (horizontal) dashed line represents the median value of SAE<sub>635∕450</sub> (<inline-formula><mml:math id="M272" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)). <bold>(a3)</bold> The corresponding <inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> under different SAE<sub>635∕450</sub> levels on P1 NPF<sub>polluted</sub> days. <bold>(b1–b3)</bold> The same but for the P2 period.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f05.png"/>

        </fig>

      <p id="d2e4032">It is worth noting that <inline-formula><mml:math id="M276" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) did not show a consistently higher level after the NPF<sub>clean, HW</sub> occurrence during the P2 period, and it was slightly higher within the first few hours of NPF occurrence (i.e., <inline-formula><mml:math id="M278" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12:00–15:00 LT) on P1 NPF<sub>polluted</sub> days (Fig. 3b). In fact, aerosol optical hygroscopicity does not fully correspond to the bulk hygroscopicity, primarily determined by aerosol chemical components, and the variability in aerosol optical features also plays a key role in <inline-formula><mml:math id="M280" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH). Hence, the size dependency of aerosol optical properties should be considered. The size-resolved <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> distribution and size-resolved cumulative frequency distribution (CFD) of <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> over different NPF days were calculated using  Mie theory, with good agreement between the theoretically calculated and measured <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> values (<inline-formula><mml:math id="M284" 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">0.99</mml:mn></mml:mrow></mml:math></inline-formula>). As shown in Figs. S11a and S13, new particles must grow into the accumulation mode size at least before they can exert a significant influence on the total scattering coefficient. The critical sizes corresponding to the cumulative frequency of 50 % in <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> were 358.7 and 333.8 nm on P1 and P2 NPF days, respectively. This indicates that relatively smaller particles – including the newly formed and grown particles mixed with pre-existing and aged particles – contributed a slightly higher portion to <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> on P2 NPF<sub>clean, HW</sub> days, while  <inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> was mainly contributed by larger particles on P1 NPF<sub>polluted</sub> days. Nevertheless, Mie theory suggests that these smaller particles generally have a weaker enhancement in total scattering after hygroscopic growth in comparison to larger size particles (Collaud Coen et al., 2007, Fig. S11a). Consequently, the changes in aerosol optical and hygroscopic properties necessitate consideration of both aerosol optical and chemical characteristics during different NPF events. Newly formed ultrafine particles contributed less to aerosol optical properties, resulting in  lower <inline-formula><mml:math id="M290" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) during the initial hours of P2 NPF<sub>clean, HW</sub> events compared to  P1 NPF<sub>polluted</sub> events (Fig. 3b), as evidenced by smaller <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for P2 NPF<sub>clean, HW</sub> events (Fig. S6). In contrast, the growth of pre-existing and newly formed particles into larger sizes would subsequently affect bulk aerosol optical properties, which was evidenced by the enhancement in the aerosol extinction coefficient observed after NPF occurrence in a recent study (Sun et al., 2024). Specifically, particles could undergo a longer and more intensified photochemical aging process during NPF<sub>clean, HW</sub> days, as influenced by persistent heatwaves, which facilitated the secondary formation of hygroscopic aerosols and jointly contributed to  higher <inline-formula><mml:math id="M296" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) after 15:00 LT (Fig. 3b).</p>
</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title><inline-formula><mml:math id="M297" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)-induced changes in aerosol direct radiative forcing</title>
      <p id="d2e4319">The changes in <inline-formula><mml:math id="M298" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) have significant implications for aerosol direct radiative forcing. Despite considerably lower <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> results during heatwaves, the corresponding mean <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) levels, particularly for P2 NPF<sub>clean, HW</sub> days, were higher than those of the P1 cases (Fig. 6a). A robust positive correlation (<inline-formula><mml:math id="M302" 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">0.68</mml:mn></mml:mrow></mml:math></inline-formula>) was observed between <inline-formula><mml:math id="M303" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and the aerosol radiative forcing enhancement factor, <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) (Fig. 6b). This is likely due to the enhanced <inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) with the larger forward scattering ratio <inline-formula><mml:math id="M306" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, or rather higher HBF for smaller particle sizes, as supported by a generally negative correlation between <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Specifically, the highest <inline-formula><mml:math id="M309" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) value of 2.21 <inline-formula><mml:math id="M310" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.23 was observed on P2 NPF<sub>clean, HW</sub> days, characterized by the highest <inline-formula><mml:math id="M312" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and smallest <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (i.e., highest HBF) of the entire study period.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e4500"><bold>(a)</bold> The boxplot of <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) during P1 and P2 NPF event and non-event days. <bold>(b)</bold> The relationship between <inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M316" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), as colored by the corresponding <inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, during P1 and P2 NPF and non-event days (shown with different symbols). <bold>(c)</bold> Occurrence frequency of the HBF<sub>525, RH</sub> <inline-formula><mml:math id="M319" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios during P1 and P2 NPF and non-event days. <bold>(d)</bold> The mean <inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) under different <inline-formula><mml:math id="M322" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) levels (the error bars represent <inline-formula><mml:math id="M323" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 standard deviation corresponding to <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M325" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH)), along with the reported <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M327" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) data for other regions in the world.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/12811/2025/acp-25-12811-2025-f06.png"/>

        </fig>

      <p id="d2e4654">The definition of <inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) in Eq. (5) implies its dependence  on both <inline-formula><mml:math id="M329" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and HBF-derived <inline-formula><mml:math id="M330" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M331" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>(dry), or, more precisely, the ratio of HBF<sub>525, RH</sub> <inline-formula><mml:math id="M333" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub>. The mean HBF<sub>525, RH</sub> was generally larger than HBF<sub>525</sub> in this study, specifically with the HBF<sub>525, RH</sub> <inline-formula><mml:math id="M338" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios centered around 1.8, and even approached 2.5 on P2 NPF<sub>clean, HW</sub> days (Fig. 6c, Table S2). This could differ from classical Mie theory with its spherical-particle premise; i.e., the observed light backscattering was enhanced after hydration, likely as a result of the evolution in particle morphology that significantly influences its optical properties (Mishchenko, 2009). Additionally, the predominant organic components, when  heterogeneously mixed with diverse chemical compositions (e.g., inorganics and black carbon), likely introduced the heterogeneity in aerosol hygroscopicity (Yuan and Zhao, 2023), which may alter particle morphology and thereby optical properties upon water uptake (Giordano et al., 2015; Tan et al., 2020; Tritscher et al., 2011). The efficient evaporation of organic coatings under extremely hot conditions could also contribute to the change in particle morphology (e.g., non-spherical irregular shapes) upon humidification, as evidenced by a recent study that reported that high-temperature conditions could accelerate the evaporation rate of SOA (Li et al., 2019). Given that the backward scattering intensity of non-spherical particles is suggested to be much larger than that of their spherical counterparts at scattering angles between 90 and 150° (Mishchenko, 2009; Yang et al., 2007) and that the HBF-derived asymmetry parameter (<inline-formula><mml:math id="M341" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula>) normally correlates positively with the aerosol forward scattering (Andrews et al., 2006; Marshall et al., 1995), the generally smaller <inline-formula><mml:math id="M342" display="inline"><mml:mrow><mml:msub><mml:mi>g</mml:mi><mml:mi mathvariant="normal">RH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> results (in comparison to <inline-formula><mml:math id="M343" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula>) confirmed the decrease (increase) in  forward (backward) light scattering after water uptake (Fig. S11c), likely implying a change in the morphological structure of particles. This is particularly evident for P2 NPF<sub>clean, HW</sub> days, during which a much lower level of <inline-formula><mml:math id="M345" display="inline"><mml:mrow><mml:msub><mml:mi>g</mml:mi><mml:mi mathvariant="normal">RH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> was observed (Fig. S11c). Another possible reason is the distinct size dependences of both light scattering and backscattering efficiencies (Fig. S11a), with much more significant enhancements in the backscattering efficiency and thereby HBF, specifically of accumulation mode particles after hygroscopic growth (Fig. S11b). As reflected by the Mie model, although the abundant newly formed particles were generally optically insensitive (e.g., below 100 nm), their contributions to <inline-formula><mml:math id="M346" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and especially to <inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">bsca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> could be amplified upon humidification (Fig. S11b). Moreover, the shift of the size distribution towards larger accumulation mode particles could also result in a significant elevation in HBF<sub>525, RH</sub> <inline-formula><mml:math id="M349" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios, especially under the condition of a smaller-mode diameter and narrower distribution of ultrafine-mode particles (e.g., during NPF events) (Fig. S16a1–b2 for the theoretical sensitivity tests of Sect. S9 in the Supplement). Furthermore, the HBF<sub>525, RH</sub> <inline-formula><mml:math id="M352" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratio exhibited a significant positive correlation with the real part of the complex refractive index (<inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of bulk aerosols (Fig. S17), and <inline-formula><mml:math id="M355" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> tends to increase with the aging process of organic species (Moise et al., 2015; G. Zhao et al., 2021). In this sense, the evolution of both aerosol size distribution patterns and chemical compositions, combined with the heterogeneity in aerosol hygroscopicity, could potentially change particle morphology and optical properties (e.g., complex refractive index and elevated HBF<sub>525, RH</sub>), particularly during heatwave-influenced NPF<sub>clean, HW</sub> days, characterized by the smallest aerosol <inline-formula><mml:math id="M358" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (102.8 <inline-formula><mml:math id="M359" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 12.4 nm) (Fig. S6), lowest number concentration (1897.0 <inline-formula><mml:math id="M360" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 680.8 cm<sup>−3</sup>) and fraction (0.20 <inline-formula><mml:math id="M362" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.10) of accumulation mode particles, intensified photooxidation, and a higher SOC <inline-formula><mml:math id="M363" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> OC ratio. The higher HBF<sub>525, RH</sub> <inline-formula><mml:math id="M365" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios increased the HBF-derived <inline-formula><mml:math id="M367" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>(RH)<inline-formula><mml:math id="M368" display="inline"><mml:mrow><mml:mo>/</mml:mo><mml:mi mathvariant="italic">β</mml:mi></mml:mrow></mml:math></inline-formula>(dry) levels, in combination with the elevated <inline-formula><mml:math id="M369" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), further resulting in the highest <inline-formula><mml:math id="M370" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) observed during P2 NPF<sub>clean, HW</sub> events. Given that previously observed HBF<sub>525, RH</sub> was typically lower than HBF<sub>525</sub> (Titos et al., 2021; Xia et al., 2023; L. Zhang et al., 2015), the mean <inline-formula><mml:math id="M374" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) results of this study (<inline-formula><mml:math id="M375" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(85 %) <inline-formula><mml:math id="M376" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 2.05 <inline-formula><mml:math id="M377" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.24) were significantly higher than those observed in the Yangtze River Delta (<inline-formula><mml:math id="M378" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(85 %) <inline-formula><mml:math id="M379" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.5, L. Zhang et al., 2015), the North China Plain (<inline-formula><mml:math id="M380" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(80 %) <inline-formula><mml:math id="M381" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1.6 <inline-formula><mml:math id="M382" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.2, Xia et al., 2023), and some other regions in the world (Titos et al., 2021, Fig. 6d). It should be noted that the reported <inline-formula><mml:math id="M383" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) for the UGR site (Spain) was even higher, likely due to the higher <inline-formula><mml:math id="M384" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M385" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> used in the derivation of <inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) in that area (Titos et al., 2021).</p>
      <p id="d2e5273">A recent study has indicated that continuous reduction in PM<sub>2.5</sub> mass loadings can increase the net solar radiation, thereby promoting NPF events (S. Zhao et al., 2021). Given the complexity and dynamic evolution of the atmospheric environment, these can further alter the intrinsic properties of aerosol particles (e.g., <inline-formula><mml:math id="M388" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH), HBF, morphology), potentially feeding back into aerosol–radiation interactions. Our findings suggest that NPF days may possess a relatively higher aerosol optical hygroscopicity in rather hot environments, e.g., the basin area and tropical regions. Meanwhile, NPF serves as a crucial secondary transformation process in the atmosphere (Zhu et al., 2021). The favorable atmospheric diffusion capability ensured the mixing of newly formed particles into the upper boundary layer, where it is colder and more humid compared to near the surface during heatwaves (Jin et al., 2022). Hence, the enhancement of aerosol optical hygroscopicity during the subsequent growth and aging of both pre-existing and newly formed particles possibly exacerbates secondary pollution and even triggers haze events (Hao et al., 2024; Kulmala et al., 2021). On the other hand, a large number of studies have demonstrated that the new particles with higher hygroscopicity could contribute more to the activation of CCN (Ma et al., 2016; Ren et al., 2021; Rosati et al., 2022; Sun et al., 2024; Wu et al., 2015), thereby modulating aerosol–cloud interactions and further the global climate (Fan et al., 2016; Merikanto et al., 2009; Westervelt et al., 2013). Additionally, the simultaneous decrease in aerosol effective radius and possibly evaporation-induced non-spherical particle morphology further enhance the aerosol direct radiative forcing enhancement factor, potentially amplifying the cooling effect mainly caused by light scattering aerosols. This highlights the need for further in-depth exploration of aerosol radiative impacts under heatwaves with a changing climate, given the continuous reductions in anthropogenic emissions and more intense emissions of biogenic origins with global warming. Moreover, more detailed information on the evolution of particle morphology with the changing environment (e.g., varied temperature and RH) would enrich insights into aerosol radiative forcing.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions and implications</title>
      <p id="d2e5301">A rare heatwave event raged throughout urban Chongqing of southwest China in the summer of 2022, which significantly influenced aerosol physicochemical properties and atmospheric processes (e.g., NPF and subsequent growth). Concurrent measurements of aerosol optical and hygroscopic properties, PNSD, and bulk chemical compositions were conducted to explore the mechanisms behind the variations in aerosol optical hygroscopicity during different NPF days under diverse weather conditions.</p>
      <p id="d2e5304">Although the air masses and the occurrence frequencies of NPF events were similar during different periods, NPF events exhibited distinct characteristics during the normally hot (P1, relatively polluted) and heatwave-dominated (P2, quite clean) periods. NPF<sub>polluted</sub> within the P1 period was favored by the decrease in background aerosol loading and the higher abundance of H<sub>2</sub>SO<sub>4</sub>. NPF<sub>clean, HW</sub> events, which occurred during the heatwave P2 period, were observed with lower CS, CoagS, FR, and GR, as well as smaller <inline-formula><mml:math id="M393" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M394" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, compared to P1 NPF<sub>polluted</sub> cases. According to the measured PNSDs, P1 NPF<sub>polluted</sub> events were mainly driven by local growth, while NPF<sub>clean, HW</sub> events may be largely affected by transport under heatwaves. In comparison to  P1 NPF<sub>polluted</sub> events, NPF<sub>clean, HW</sub> occurred approximately 1 h earlier, and the subsequent growth was longer during P2, likely intensifying the photochemical oxidation and prolonging atmospheric aging processes under heatwaves, thereby modulating the evolution of aerosol size distributions and chemical characteristics differently. Furthermore, significant differences in aerosol optical and hygroscopic properties were observed between the normally hot and heatwave-dominated NPF days. The newly formed and grown particles mixed with pre-existing aerosols contributed a minor <inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> noontime peak that occurred on the much cleaner P2 NPF<sub>clean, HW</sub> days, while <inline-formula><mml:math id="M402" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> peaked earlier, around the morning rush hours on P1 NPF<sub>polluted</sub> days. HBF and SAE were significantly higher on P2 NPF<sub>clean, HW</sub> days, primarily due to the smaller <inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for heatwave-influenced NPF<sub>clean, HW</sub> cases. <inline-formula><mml:math id="M407" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) remained relatively stable during the daytime of NPF days and peaked around 16:00–18:00 LT. Specifically, aerosol optical hygroscopicity was observed to be higher during the subsequent growth and aging of both pre-existing particles and newly formed ones on P2 NPF<sub>clean, HW</sub> days than that for P1 NPF<sub>polluted</sub> days, which aligned with the higher <inline-formula><mml:math id="M410" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">W</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> levels.</p>
      <p id="d2e5572">Compared with non-event cases, the daily mean <inline-formula><mml:math id="M411" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) levels were generally higher on NPF days in the  hot summer of 2022 in urban Chongqing. A significantly positive (negative) correlation between <inline-formula><mml:math id="M412" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE (<inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, or rather the pollution level) was observed on NPF days for both periods, accompanied by higher <inline-formula><mml:math id="M414" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) and SAE values on NPF<sub>clean, HW</sub> days. This was likely due to the observed lower FR and GR caused by possible evaporation of both unstable clusters and particle coatings under heatwaves (Bousiotis et al., 2021; Cusack et al., 2013; Deng et al., 2020; Garmash et al., 2024), thereby reducing aerosol sizes (e.g., <inline-formula><mml:math id="M416" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) while increasing SAE. Moreover, heatwave-influenced stronger photooxidation enhanced the formation of more hygroscopic secondary components during the subsequent growth and aging processes of both pre-existing and newly formed particles on P2 NPF<sub>clean, HW</sub> days in comparison to P1 NPF<sub>polluted</sub> cases. The aerosol light scattering or volume concentration was mainly contributed by the larger accumulation mode particles, while more ultrafine particles dominated the size distribution, especially for the initial stage of heatwave-influenced NPF<sub>clean, HW</sub> events, further leading to a lower <inline-formula><mml:math id="M421" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) following NPF occurrence (i.e., <inline-formula><mml:math id="M422" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12:00–15:00 LT) in comparison to P1 NPF<sub>polluted</sub> days.</p>
      <p id="d2e5714">Changes in <inline-formula><mml:math id="M424" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) could potentially impact the aerosol direct radiative forcing. A robust positive (negative) correlation existed between <inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) and <inline-formula><mml:math id="M426" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) (<inline-formula><mml:math id="M427" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Despite lower <inline-formula><mml:math id="M428" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi mathvariant="normal">sca</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">525</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> during heatwaves, the corresponding mean <inline-formula><mml:math id="M429" display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mi mathvariant="normal">RF</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>(RH) was relatively higher, and the maximum value of 2.21 <inline-formula><mml:math id="M430" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.23 was observed on P2 NPF<sub>clean, HW</sub> days, associated with the highest <inline-formula><mml:math id="M432" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>(RH) (1.71 <inline-formula><mml:math id="M433" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.13), smallest <inline-formula><mml:math id="M434" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (102.8 <inline-formula><mml:math id="M435" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 12.4 nm), and highest HBF<sub>525, RH</sub> <inline-formula><mml:math id="M437" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios (1.78 <inline-formula><mml:math id="M439" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.29). The above highlights that heatwaves can influence the NPF characteristics (e.g., the evolution in the aerosol size distribution pattern and chemical composition) and atmospheric processing (although with  decreased aerosol <inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M441" display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">mode</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, likely due to evaporation-driven  non-spherical particle morphology under persistently high temperature conditions). Further, variations in the aerosol size distribution and optical hygroscopicity under heatwaves were accompanied by  elevated HBF<sub>525, RH</sub> <inline-formula><mml:math id="M443" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HBF<sub>525</sub> ratios, potentially reducing the net solar radiation directly, especially in hot summer conditions. This study revealed divergent changes in aerosol optical and hygroscopic properties on different NPF days, thereby modulating the aerosol radiative forcing distinctly during a heatwave in the summer of 2022. A comprehensive understanding of the formation mechanisms of different NPF events (e.g., local formation versus  horizontal or vertical transport) in  diverse environments is crucial for the future. Last but not least, further explorations of detailed molecular-scale characterizations (e.g., molecular structures and compositions of newly and secondarily formed particles, as well as particle morphology) and aerosol radiative impacts, including  aerosol–cloud interactions during heatwaves under a changing climate, are highly recommended.</p>
</sec>

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

      <p id="d2e5934">The data in this study are available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.16783914" ext-link-type="DOI">10.5281/zenodo.16783914</ext-link> (Hao, 2025).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5940">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-25-12811-2025-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-25-12811-2025-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5949">YH and PL: methodology, investigation, data analysis, formal analysis, visualization, validation, writing – original draft and editing. YG and ZW: methodology, investigation, formal analysis. MT, YC, HX, and WH: data curation, methodology. FW and YL: investigation. YK: methodology, data analysis, writing – review and editing. JC: conceptualization, methodology, funding acquisition, data curation, writing – review and editing, supervision.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5955">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="d2e5961">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. 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="d2e5967">This work was supported by the National Natural Science Foundation of China (grant no. 42105075) and the Venture and Innovation Support Program for Chongqing Overseas Returnees (grant no. cx2021021). We thank Biao Xue for the technical support on the utilization and maintenance of the humidified nephelometer system. We also thank Ziqian Wang for  TSP filter sample collection and Jiawei Zhou for the corresponding offline chemical analysis.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5972">This research has been supported by the National Natural Science Foundation of China (grant no. 42105075) and the Venture and Innovation Support Program for Chongqing Overseas Returnees (grant no. cx2021021).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5978">This paper was edited by Imre Salma and reviewed by Junying Sun and three anonymous referees.</p>
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