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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-25-10625-2025</article-id><title-group><article-title>On the presence of high nitrite (NO<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in coarse particles at Mt. Qomolangma</article-title><alt-title>On the presence of NO<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in coarse particles at Mt. Qomolangma</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Zhang</surname><given-names>Zhongyi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6530-5997</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Ye</surname><given-names>Chunxiang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5417-2671</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wu</surname><given-names>Yichao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Zhou</surname><given-names>Tao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff5">
          <name><surname>Chen</surname><given-names>Pengfei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff5">
          <name><surname>Kang</surname><given-names>Shichang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zhang</surname><given-names>Chong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3852-3056</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Jiang</surname><given-names>Zhuang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5692-8308</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff3 aff6">
          <name><surname>Geng</surname><given-names>Lei</given-names></name>
          <email>genglei@ustc.edu.cn</email>
        <ext-link>https://orcid.org/0000-0003-2175-2538</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>National Key Laboratory of Deep Space Exploration/School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026, Anhui, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>SKL-ESPC &amp; SEPKL-AERM, College of Environmental Sciences and Engineering, and Center for Environment and Science, Peking University, Beijing 100871, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Deep Space Exploration Laboratory, Hefei, 230088, Anhui, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Key Laboratory of Cryospheric Science and Frozen Soil Engineering, Northwest Institute of Eco-Environment and Resources, Chinese Academy of Sciences, Lanzhou, 730000, Gansu, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>University of Chinese Academy of Sciences, Beijing, 100049, China</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>CAS Center for Excellence in Comparative Planetology, University of Science and Technology of China, Hefei 230026, Anhui, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Lei Geng (genglei@ustc.edu.cn)</corresp></author-notes><pub-date><day>17</day><month>September</month><year>2025</year></pub-date>
      
      <volume>25</volume>
      <issue>18</issue>
      <fpage>10625</fpage><lpage>10641</lpage>
      <history>
        <date date-type="received"><day>27</day><month>December</month><year>2024</year></date>
           <date date-type="rev-request"><day>16</day><month>January</month><year>2025</year></date>
           <date date-type="rev-recd"><day>30</day><month>July</month><year>2025</year></date>
           <date date-type="accepted"><day>31</day><month>July</month><year>2025</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2025 Zhongyi Zhang 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/25/10625/2025/acp-25-10625-2025.html">This article is available from https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e217">Atmospheric reactive nitrogen cycling, with nitrous acid (HONO) and particulate nitrite (NO<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) as important intermediates, is crucial for maintaining the atmospheric oxidation capacity of background atmosphere on the Tibetan Plateau. During an 11 d field campaign at the Base Camp of Mt. Qomolangma in spring of 2022, we observed significant enrichments of NO<inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in total suspended particulate (TSP) with a mean concentration of <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mn mathvariant="normal">375</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">386</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>, while NO<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was absent in fine particles (PM<sub>2.5</sub>). The comparison revealed that NO<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> predominately exists in coarse particles. Local surface soil at the sampling site also exhibited high levels of NO<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, with <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N value similar to NO<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP. This isotopic similarity suggests that wind-blown soil is probably the primary source of NO<inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP, accounting for the background levels. While concentration changes of water-soluble inorganic ions in TSP and PM<sub>2.5</sub> in response to shifts in air mass back-trajectories imply that atmospheric pollutants transported from South Asia may further elevate the NO<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, the specific mechanisms of long-range transport resulting in NO<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> accumulation in TSP rather than PM<sub>2.5</sub> remain unknown and need to be investigated. The elevated levels of TSP NO<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> may readily participate in atmospheric reactive nitrogen cycling through gas-particle partitioning or photolysis, leading to the production of HONO, OH and NO and thereby influencing oxidation chemistry. Further efforts on the sources and atmospheric chemistry of particulate nitrite are warranted, particularly in the pristine Tibetan Plateau, where even small inputs of NO<sub><italic>x</italic></sub> or HONO can disproportionately affect oxidant budgets and reactive nitrogen cycling.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>41822605</award-id>
<award-id>41871051</award-id>
<award-id>42273001</award-id>
<award-id>42371151</award-id>
<award-id>42494851</award-id>
<award-id>W2411030</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2022YFC3700701</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Anhui Provincial Key Research and Development Plan</funding-source>
<award-id>2022l07020032</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="d2e422">The Tibetan Plateau (TP), known as the “Third Pole”, represents one of the most climate-sensitive regions on Earth (Yao et al., 2012). Over recent decades, the TP has experienced significant and rapid climate warming, primarily driven by increasing aerosol loadings and greenhouse gas concentrations due to its geographic proximity to East Asia and South Asia with intensive anthropogenic emissions (Kang et al., 2019; Lau et al., 2010; Lüthi et al., 2015). Atmospheric oxidation capacity (AOC) regulates secondary aerosol formation and trace gases removal, including CH<sub>4</sub> (Wang et al., 2023; Ye et al., 2023, 2016; Andersen et al., 2023), therefore acting as a critical link between atmospheric pollution and regional climate warming. Previous studies have suggested that strong solar radiation, high ozone (O<sub>3</sub>) and relatively high water vapor dominate the relatively strong AOC over the TP (Lin et al., 2008). Recent field campaign further highlighted the rapid reactive nitrogen cycling, with N(III) species (i.e., HONO) as the intermediate, also plays an important role in maintaining the strong AOC in TP (Wang et al., 2023). For example, Wang et al. (2023) reported high-than-expected HONO (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula> pptv) in the Namco station, a representative background site in the central TP, with identified HONO sources including NO<sub>2</sub> heterogenous conversion, soil emission and particulate nitrate photolysis (Wang et al., 2023). Incorporating the observed HONO into model simulations approximately doubled the estimated OH abundance compared to simulations without HONO constraints. However, a detailed HONO budget analysis indicated these three dominant sources could not account for the observed high daytime HONO levels at the background site, implying the existence of additional, yet unidentified, HONO sources.</p>
      <p id="d2e466">Particulate nitrite (NO<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) likely represents a potential source of HONO through thermodynamic partitioning processes under favorable atmospheric conditions, provided particulate nitrite is present in significant amounts (VandenBoer et al., 2014a; Chen et al., 2019; Li, 2012). Interestingly, relatively high levels of nitrite in total suspended particulate (TSP) have also been reported from remote sites of TP, i.e., in a forest site in the Southeast Tibet (<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">140</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>) and at the Qomolangma monitoring station (QOMS, <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>) (Bhattarai et al., 2019, 2023). Such high levels of particulate nitrite may also contribute to the strong AOC in TP, either via directly photolysis to produce NO<sub><italic>x</italic></sub> (Jacobi et al., 2014) or indirectly serve as an important source of HONO through gas-particle partitioning (Reaction R1). However, the sources and formation mechanisms for the relatively high level of atmospheric NO<inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> observed in the TP remain unclear. 

          <disp-formula id="Ch1.R1" content-type="numbered reaction"><label>R1</label><mml:math id="M31" display="block"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow><mml:mo>↔</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HONO</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub></mml:mrow><mml:mo>↔</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">H</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">aq</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:mrow></mml:math></disp-formula>

        The stable nitrogen and oxygen isotopic compositions (<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O; where <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">sample</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">reference</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> ‰ and with <inline-formula><mml:math id="M36" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> denoting the <inline-formula><mml:math id="M37" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi><mml:msup><mml:mo>/</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M38" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi><mml:msup><mml:mo>/</mml:mo><mml:mn mathvariant="normal">16</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi><mml:msup><mml:mo>/</mml:mo><mml:mn mathvariant="normal">16</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> ratios; <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.52</mml:mn><mml:mo>×</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>) may provide diagnostic information regarding the sources and formation pathways of atmospheric nitrite. Similar isotopic approaches have been widely used to explore the nitrate (NO<inline-formula><mml:math id="M41" 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>) sources (Morin et al., 2008; Zong et al., 2020; Geng et al., 2014; Fang et al., 2011; Hastings et al., 2003; Zhang et al., 2022, 2021b; Liu et al., 2018; Felix and Elliott, 2014; Miller et al., 2018). Considering that atmospheric NO<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> may share similar sources and formation pathways with NO<inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, the specific NO<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> formation pathways are expected to be characterized by distinct oxygen or nitrogen isotopic endmembers, despite reports on the atmospheric NO<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> isotopic compositions are rare. For instance, NO<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> produced from the photolysis of particulate 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> may possess very negative <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values compared to NO<inline-formula><mml:math id="M49" 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>, analogous to the pronounced nitrogen isotope fractionation effects associated with snow nitrate photolysis (Erbland et al., 2013; Frey et al., 2009), while the <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of NO<inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is expected to closely resemble that of NO<inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> as the oxygen atom in NO<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is imparted from NO<inline-formula><mml:math id="M54" 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>, unless significant oxygen atom exchange between NO<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and aerosol water occurs. The <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of NO<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (and HONO) from primary emission sources is expected to be negligible, while that generated from heterogeneous reactions of NO<sub>2</sub> on the aerosol surface would be characterized by positive <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values depending on the degree of NO<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and aerosol water oxygen isotope exchange. These unique isotopic fingerprints may be utilized in distinguishing the sources and formation pathways of atmospheric NO<inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e1030">To gain insight into the sources and/or formation mechanisms of atmospheric NO<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in the pristine environment of TP, we collected the TSP and fine particulate matter (PM<sub>2.5</sub>) synchronously at the Base Camp, the north slope of the Mt. Qomolangma during the campaign of “Earth Summit Mission-2022” scientific expedition from 24 April to 6 May 2022, with additional surface soil samples collected in May 2023. The NO<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentration and multi-isotopic signatures (<inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) in aerosol and surface soil were then determined in order to evaluate the potential sources of atmospheric NO<inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. Additionally, the potential environmental implication of atmospheric nitrite was explored in the term of atmospheric oxidation capacity at this pristine environment.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Material and Method</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Site description</title>
      <p id="d2e1127">The Base Camp is located in the middle of the Rongbuk valley (86.85° E, 28.14° N), situated <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5200</mml:mn></mml:mrow></mml:math></inline-formula> m above sea level (m a.s.l.) on the north slope of the Mt. Qomolangma (Zou et al., 2008; Zhu et al., 2006). The surrounding surface consists of loosed soil, gravel, broken rocks of various sizes, with sparse vegetation due to the semi-arid status (Ming et al., 2007; Zou et al., 2008). Rongbuk valley is characterized by a depth of <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m and a floor width of <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> m, with elevations of the surrounding mountains exceeding 6000 m on both sides (Zou et al., 2008). Attributed to the unique topography, the local air circulation is dominated by mountain and valley breezes. The predominant wind regime is the katabatic flow of southerly and southeasterly, which is typically persists from noon to midnight (Zhu et al., 2006; Zou et al., 2008; Zhou et al., 2011). The nearest accessible area for residents and visitors is at least 2 km north of the Base Camp. During the campaign, electricity and natural gases were routinely used for cooking and hot water production. There were intermittent vehicle exhaust emissions around the station during daytime for the daily necessaries supporting, i.e., water and food. To minimize the influence of local anthropogenic activities on sampling, the instruments were set in the southeast (upwind direction, Fig. S1 in the Supplement) and approximately 100 m away from the living space of the Base Camp. The anthropogenic influence on the sampling is expected to be minimal.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Field campaign and sample collection</title>
      <p id="d2e1168">From 26 April to 6 May 2022, TSP samples were collected simultaneously with NO<sub>2</sub> using a homemade denuder-filter system (Zhou et al., 2022). A similar system has been widely used to separately collect atmospheric particulate matter and N-containing gases for isotopic analysis (Chai et al., 2019, 2021), suggesting the mutual interference between the particulate and gaseous phases to be minimal. A polytetrafluoroethylene (PTFE) sleeve is used to assemble the homemade denuder with the filter pack, flowmeter, and pump. The filter pack was placed in the front of the denuder. All connections between the various parts of the sampling apparatus are made using <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>/</mml:mo><mml:msup><mml:mn mathvariant="normal">8</mml:mn><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> Teflon tubing. A detailed description of the sampling apparatus can be found in our previous report (Zhou et al., 2022). Whatman quartz filter (circles, diam. 47 mm, pre-heated at 400 °C for 3 h before use) was placed into the filter pack to collect TSP sample. In the present study, the collected bulk aerosol can be regarded as TSP since no size-selective inlet was employed. The flow rate was controlled at 30 L min<sup>−1</sup> using a flowmeter. Previous reports have indicated that the flow rate has negligible effect on the concentrations of sulphate, nitrate, and ammonium when using quartz filter for sampling (Keck and Wittmaack, 2005). To minimize the potential influence of the loose ground surface on the TSP collection, a mountain tent was used to separate the pump (out the tent) with the denuder-filter system (in the other side of tent), and the inlet Teflon tube was stretched out of the tent for <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> m height straight.</p>
      <p id="d2e1220">From 24 April to 6 May 2022, PM<sub>2.5</sub> were sampled using a high-volume aerosol sampler (TH-1000F; Wuhan Tianhong Instruments Co. Ltd., China) equipped with PM<sub>2.5</sub> inlet and Whatman quartz-fiber filters (sheets, 203 mm <inline-formula><mml:math id="M78" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 254 mm) at a flow rate of 1.5 m<sup>3</sup> min<sup>−1</sup>. All the quartz filters were pre-heated at 400 °C for 3 h before use. In general, TSP and PM<sub>2.5</sub> samples were collected with diurnal resolution during this campaign, with daytime samples from approximately 09:00–20:00 and nighttime samples from 21:00–08:00 (local time), respectively. From 2 to 4 May, we collected the daytime TSP and PM<sub>2.5</sub> samples in the morning (09:00–14:00) and afternoon (14:00–20:00), respectively. A total of 24 TSP samples (including 2 blanks) and 29 PM<sub>2.5</sub> (including 3 blanks) were collected during this campaign. After each sampling period, quartz filters were removed from the filter pack/PM<sub>2.5</sub> inlet and immediately wrapped in pre-baked aluminum foil and then stored in frozen until analysis to minimize potential loss of nitrite. During the campaign, snowfall events occurred on the night of 29 April and during the daytime of 30 April.</p>
      <p id="d2e1306">Surface soil samples (0–5 cm depth, <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula>) were collected in May 2023 from the east slope, west slope and south sides of the Rongbuk valley. A polytetrafluoroethylene (PTFE) shovel was used to collect soil. The collected soil was immediately transferred to clean plastic bags, sealed and kept frozen. Soil samples were transported into laboratory using a cold chain. Upon arrival at our laboratory, the soil samples were passed through a 60-mesh screen (<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn></mml:mrow></mml:math></inline-formula> mm) to remove larger particles and thoroughly homogenized prior to chemical and isotopic analysis.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Ionic concentration analysis and uncertainty estimation</title>
      <p id="d2e1339">Water-soluble inorganic ions (WSIs, including Na<sup>+</sup>, NH<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, K<sup>+</sup>, Mg<sup>2+</sup>, Ca<sup>2+</sup>, Cl<sup>−</sup>, NO<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M94" 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 SO<inline-formula><mml:math id="M95" 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>) in TSP (entire filter, <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">16.6</mml:mn></mml:mrow></mml:math></inline-formula> cm<sup>2</sup>) and PM<sub>2.5</sub> (<inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:math></inline-formula> section, <inline-formula><mml:math id="M100" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 13.0 cm<sup>2</sup>) were extracted using 20 mL Milli-Q ultrapure water (18.2 <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">cm</mml:mi></mml:mrow></mml:math></inline-formula>) in an ultrasonic bath at room temperature for 30 min. Note the TSP filters were cut to fit the filter holder from the standard Whatman quartz-fiber filters which were also used as the PM<sub>2.5</sub> filters. After filtration through a 0.22 <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> pore size syringe filter which was pre-cleaned with ultrapure water, the filtrate was subjected to inorganic species analysis using ion chromatography (Dionex Aquion) (Zhang et al., 2020). Blank filters were pretreated and measured the same as real samples, and the limits of detection (LOD) was calculated as 3 times of standard deviations of blanks (Fang et al., 2015a). In general, Na<sup>+</sup> in the blank filters is comparable to samples, a well-known issue for the Whatman quartz filter which is high in Na<sup>+</sup> blank. Therefore, in this study, we discarded the Na<sup>+</sup> data. The volatile components (i.e., NH<inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M110" 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 K<sup>+</sup> in blank are low but several times higher than the detection limits; SO<inline-formula><mml:math id="M112" 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>, Mg<sup>2+</sup> and Ca<sup>2+</sup> in blank are significantly higher than the respective LOD but lower than samples by at least five times (the lower end). All reported concentrations of each ion were blank corrected as follows: 

            <disp-formula id="Ch1.E2" content-type="numbered"><label>1</label><mml:math id="M115" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">sample</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">blank</mml:mi></mml:msub><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">water</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">air</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> representing the ambient concentrations of specie <inline-formula><mml:math id="M117" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> in air (ng m<sup>−3</sup> or <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">sample</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">blank</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the concentrations determined by the ion chromatography (ng mL<sup>−1</sup>), <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">water</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the volume of ultrapure water used for extraction (20 mL), <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi>V</mml:mi><mml:mi mathvariant="normal">air</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the volume of air sampled for each PM<sub>2.5</sub> or TSP filter, <inline-formula><mml:math id="M126" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> is the ratio of particulate matter collection area for PM<sub>2.5</sub> or TSP filters to the filter area used for extraction.</p>
      <p id="d2e1828">The overall uncertainty in ion concentration was estimated according to the law of error propagation, accounting for the sampling air volume (3 % for PM<sub>2.5</sub> samples and 1 % for TSP samples as provided by the manufactures), the extraction of water volume (<inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula> % for pipetting from the manufacture Eppendorf), the blanks, and the analytical uncertainty from ion chromatography and calibration, assuming that these factors are independent. The analytical uncertainty for water-soluble ions concentration determination using ionic chromatography has been extensively assessed in our laboratory, with values typically <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % for all inorganic species at concentration of 500 ng mL<sup>−1</sup>. The combined uncertainty about the ionic concentrations in PM<sub>2.5</sub> and TSP are shown in Table S1 in the Supplement. In general, TSP samples are associated with relatively high overall uncertainty compared to PM<sub>2.5</sub> samples, perhaps due to the relatively high blank variability from the low mass loadings in TSP.</p>
      <p id="d2e1891">For soil ionic concentration analysis, 4.0 g sieved soil was extracted using 20 mL Milli-Q ultrapure water, shaken for 30 min at room temperature. After centrifugation, the extract was passed through 0.45 mm filters before ions analysis. The concentration determination of water-soluble inorganic ions in soil extract was similar to that of aerosol samples. Detailed procedure for the extraction of soil inorganic ions, especially the NO<inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> has been descried in previous report (Homyak et al., 2015).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Isotopic analysis</title>
      <p id="d2e1914">After concentration measurements, isotopic analyses (<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) of NO<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP were conducted using the azide method (Casciotti et al., 2007). The azide method can reduce nitrite ion in solution into N<sub>2</sub>O in a single step, while nitrate ion remains unchanged, ensuring no interference on the nitrite isotopic analysis. The azide reagent is prepared by mixing 2 M sodium azide with 40 % acetic acid at a <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> ratio by volume in our laboratory. NO<inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> standards and samples were pretreated under identical conditions concerning the total volume, nitrite amount, water isotope, and matrix. The <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, and <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of N<sub>2</sub>O reduced from NO<inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in the TSP samples and standards were determined using a Finnigan<sup>®</sup> MAT253 plus isotope ratio mass spectrometer (IRMS) equipped with a GasBench II and preconcentration system. The data calibration followed the procedures described in Albertin et al. (2021), using three international KNO<sub>2</sub> salt standards (RSIL-N10219, RSIL-N7373, and RSIL-N23 with respective <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N and <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values of 2.8 ‰/88.5 ‰, <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">79.6</mml:mn></mml:mrow></mml:math></inline-formula> ‰/4.2 ‰, and 3.7 ‰/11.4 ‰). The <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values of the three international references have not been certified. To address this, a series laboratory experiments was conducted to determine the true values of three international references in our laboratory (Zhang et al., 2025). In brief, each nitrite international reference was oxidized into NO<inline-formula><mml:math id="M152" 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> by O<sub>3</sub> produced from commercial ozone generator. A parallel flow of O<sub>3</sub> was also used to convert a normal KNO<sub>2</sub> salt (<inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) into NO<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to quantify the <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O transfer during O<sub>3</sub> oxidation, following the approach of (Vicars and Savarino, 2014). Based on these experiments, the <inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of RSIL-N7373 and RSIL-N23 are determined to be negligible, consistent with previous findings (Albertin et al., 2021), while the <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of RSIL-N10219 is determined to be (<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula>) ‰ in our laboratory. The <sup>17</sup>O-excess in samples is then calculated as <inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.52</mml:mn><mml:mo>×</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>. The standard deviations for <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of reference materials (<inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula>) were determined to be less than 0.1 ‰, 0.6 ‰, and 0.4 ‰, respectively.</p>
      <p id="d2e2326">For soil NO<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> isotopic analysis, <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30.0</mml:mn></mml:mrow></mml:math></inline-formula> g sieved soil was extracted using 150 mL Milli-Q ultra-pure water. The soil extract was then preconcentrated into 10 mL using ion-exchange resin before isotopic analysis. The preconcentration approach was widely used for nitrate isotopic analysis in snow and ice samples, and the detailed procedures and the performance have been provided in Erbland et al. (2013) and evaluated in our laboratory (Sect. S1 in the Supplement). The concentrated soil extracts (50 nmol NO<inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) was then subjected to soil NO<inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> isotopic analysis by converting into N<sub>2</sub>O via the azide method. For soil NO<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> isotopic analysis, <inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5.0</mml:mn></mml:mrow></mml:math></inline-formula> g sieved soil was extracted with 15 mL of 2 M KCl solution (Fang et al., 2015b). The remaining procedures of soil NO<inline-formula><mml:math id="M176" 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 NO<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> analysis were same as those for TSP samples, as aforementioned.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Complementary analyses of air mass backward trajectory</title>
      <p id="d2e2440">To evaluate the possible impact of biomass burning emissions or other pollution sources from South Asia, the Hybrid Single-Particle Lagrangian Integrated Trajectory (HYSPLIT) model (performed using TrajStat plugin of the MeteoInfo software) and archived Global Data Assimilation System (GDAS) of meteorological data were used to model the air mass back trajectories (Wang, 2014). In this study, 3 d air mass backward trajectories with arriving height of 1000 m above ground level were simulated to identify the most likely pathway and potential source regions of the air masses at the Base Camp (Bhattarai et al., 2023; Lin et al., 2021). Moreover, the Fire Information and Resource Management System (FIRMS) developed by Moderate Resolution Imaging Spectrometer (MODIS) (<uri>https://worldview.earthdata.nasa.gov</uri>, last access: 7 September 2024) was employed to identify the distribution of active fire spots during the sampling period.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e2448">The chemical compositions and time series of mass concentrations of water-soluble inorganic species (NO<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, SO<inline-formula><mml:math id="M179" 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="M180" 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>, Ca<sup>2+</sup>, etc.), as well as the corresponding mass fractions in respective TSP <bold>(a, b)</bold> and PM<sub>2.5</sub> <bold>(c, d)</bold> samples collected at Base Camp of Mt. Qomolangma in spring 2022.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025-f01.png"/>

        </fig>


</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Mass concentrations of water-soluble inorganic ions in TSP and PM<sub>2.5</sub></title>
      <p id="d2e2551">Figure 1 displays the chemical compositions of water-soluble inorganic ions, their corresponding time series and fractional contributions in TSP and PM<sub>2.5</sub>. Throughout the campaign, substantial variations of total WSIs in PM<sub>2.5</sub> and TSP were observed. For PM<sub>2.5</sub> samples, the mass concentrations of total WSIs before 30 April were higher than that from 1 to 6 May (<inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> versus <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M189" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>). The cut-off date of 30 April was selected based on observed shifts in concentrations of water-soluble ions and air mass origins (described in Sect. 4.2). This decline of total WSIs after 30 April was predominately driven by significant reductions in secondary inorganic species, i.e., SO<inline-formula><mml:math id="M191" 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="M192" 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="M193" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, with the magnitude by more than 60 %. In particular, NH<inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in PM<sub>2.5</sub> was on average (<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:mn mathvariant="normal">322</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">243</mml:mn></mml:mrow></mml:math></inline-formula>) ng m<sup>−3</sup> before 30 April whereas NH<inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in PM<sub>2.5</sub> collected during daytime and nighttime of 1 May were 1 and 3 ng m<sup>−3</sup>, respectively, and NH<inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in PM<sub>2.5</sub> extractions from 2 to 6 May was below the detection limit. Therefore, the fractional contribution of secondary inorganic species in PM<sub>2.5</sub> also decreased (Fig. 1d). Similarly, K<sup>+</sup> in PM<sub>2.5</sub>, a good tracer of biomass burning (Ma et al., 2003), also declined significantly after 30 April (<inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:mn mathvariant="normal">269</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">432</mml:mn></mml:mrow></mml:math></inline-formula> versus <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mn mathvariant="normal">22</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>; <inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>). The elevated concentrations of WSIs before 30 April (<inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M211" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) are comparable to previous reports at QOMS station (<inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.2</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M213" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) in the spring (Lin et al., 2021). In comparison, concentrations of Ca<sup>2+</sup> and Mg<sup>2+</sup>, tracers of wind-blown dust (Wang et al., 2002), decreased by less than 20 % after 30 April. In general, SO<inline-formula><mml:math id="M216" 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="M217" 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 Ca<sup>2+</sup> are the most abundant species in PM<sub>2.5</sub>, accounting for the majority of the mass of total WSIs. In addition, no clear diurnal variation of water-soluble inorganic ions in PM<sub>2.5</sub> was observed in this study (Fig. S2).</p>
      <p id="d2e2998">Some water-soluble inorganic ions (e.g., SO<inline-formula><mml:math id="M221" 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="M222" 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="M223" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in TSP showed similar variation trends with that in PM<sub>2.5</sub> throughout the campaign, while others, such as K<sup>+</sup>, exhibited divergent behavior (Fig. 1). For example, after 30 April, the secondary inorganic species in TSP declined considerably by over 50 % (i.e., NH<inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP declined by more than tenfold), while Ca<sup>2+</sup> in TSP decreased with a smaller degree (<inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> %) and Mg<sup>2+</sup> remained stable. In contrast, TSP K<sup>+</sup> (from both crustal and biomass burning sources) (Hsu et al., 2009) drastically surged on 3 and 4 May. Note that other species in TSP, i.e., SO<inline-formula><mml:math id="M231" 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> and NO<inline-formula><mml:math id="M232" 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> also increased to some extent on 3 May. The time series of water-soluble inorganic ions in the coarse-mode particulate, calculated as the differences between TSP and PM<sub>2.5</sub>, are presented in Fig. 2. Due to the overall analytical uncertainties, the air concentrations of SO<inline-formula><mml:math id="M234" 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> in PM<sub>2.5</sub> samples occasionally exceeded that in corresponding TSP samples on some days.</p>

      <fig id="F2"><label>Figure 2</label><caption><p id="d2e3177">The estimated chemical compositions and time series of mass concentrations of chemical species (NO<inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, SO<inline-formula><mml:math id="M237" 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="M238" 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>, Ca<sup>2+</sup>, etc.) in coarse-mode particulate during the springtime campaign (calculated as the difference between TSP and PM<sub>2.5</sub>). Discontinuities in the time series were observed for certain species (e.g., SO<inline-formula><mml:math id="M241" 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>), likely resulting from relatively lower concentrations in the TSP samples compared to those in the corresponding PM<sub>2.5</sub> samples. This discrepancy is likely attributed to the propagated uncertainties involved in the concentration analysis, sampling approach and blank corrections.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025-f02.png"/>

        </fig>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e3274">Ion balance for PM<sub>2.5</sub> (<bold>a</bold>, blue circles) and TSP samples (<bold>b</bold>, blue hollow triangles: samples collected after 30 April; blue solid triangles: samples collected before 30 April). Concentrations are expressed in nanogram-equivalent weight per cubic meter (neq m<sup>−3</sup>).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025-f03.png"/>

        </fig>

      <p id="d2e3310">Figure 3 presents the ion balance of measured water-soluble ions in PM<sub>2.5</sub> throughout the campaign as well as in TSP collected before and after 30 April, respectively, to highlight the significant decline in TSP NO<inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. There is a strong correlation between cation and anion equivalents in PM<sub>2.5</sub> samples (<inline-formula><mml:math id="M248" 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">0.70</mml:mn></mml:mrow></mml:math></inline-formula>), whereas the correlations decreased in TSP samples (<inline-formula><mml:math id="M249" 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">0.46</mml:mn></mml:mrow></mml:math></inline-formula> before 30 April and 0.49 after that, respectively). The nanogram-equivalent weights of cation were significantly higher than that of anions for all samples, with ratio of cation to anion equivalent of <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> for PM<sub>2.5</sub>, <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.9</mml:mn></mml:mrow></mml:math></inline-formula> for TSP collected before 30 April, <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4.2</mml:mn></mml:mrow></mml:math></inline-formula> for TSP collected after 1 May. Clearly, the declines in TSP NO<inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> after 30 April resulted in relatively higher cation/anion equivalent ratio. The slopes of the correlation lines exceeded unity for PM<sub>2.5</sub> and TSP samples, indicating the alkaline nature of aerosol. The observed deficiency of anion can be attributed to the presence of carbonates (i.e., CaCO<sub>3</sub>), which can dissolve in water during extraction to release CO<inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</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> and/or HCO<inline-formula><mml:math id="M258" 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> despite the relatively low solubility (Zhang et al., 2021a).</p>
      <p id="d2e3471">The most distinct feature of chemical compositions in TSP was the elevated level and significant variation of NO<inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, ranging from 0.2 to 1291 ng m<sup>−3</sup> in air and with an average of <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:mn mathvariant="normal">375</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">386</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>. In comparison, NO<inline-formula><mml:math id="M263" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> consistently remained below the detection limit in PM<sub>2.5</sub> samples. Note during the laboratory measurements of ionic concentrations, TSP and PM<sub>2.5</sub> filters were extracted with ultrapure water and it was the extraction analyzed by ion chromatography. To ensure fair comparisons, similar areas of filters were extracted with same volume of ultrapure water, so that the extractions from the PM<sub>2.5</sub> filters should be more concentrated in atmospheric particulate species compared to that from the TSP filters, since PM<sub>2.5</sub> samples were collected at a much faster sampling speed (1.5 m<sup>3</sup> min<sup>−1</sup> vs. 30 L min<sup>−1</sup>) over the same sampling duration. Nevertheless, NO<inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was detectable only in the extractions of TSP filter. The determined NO<inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations in TSP in this study (<inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:mn mathvariant="normal">375</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">386</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>) were higher than previous reports conducted in various remote sites, such as at QOMS station (<inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> for TSP) (Bhattarai et al., 2023), at a forest site in the Southeast Tibet Plateau (<inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">140</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> for TSP) (Bhattarai et al., 2019), in the middle hills of the central Himalayas (<inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">210</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> for TSP) (Tripathee et al., 2021).</p>
      <p id="d2e3720">In particular, there was a dramatic decrease in TSP NO<inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> after 30 April, from a mean of (<inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mn mathvariant="normal">625</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">457</mml:mn></mml:mrow></mml:math></inline-formula>) to (<inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:mn mathvariant="normal">147</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">145</mml:mn></mml:mrow></mml:math></inline-formula>) ng m<sup>−3</sup>, in line with the declines in other secondary inorganic species. Over the course of the campaign, NO<inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> comprised approximately 8 % of the total WSIs mass in TSP, while its contribution reached maximum of <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> % on 27 and 28 April, being one of the most abundant components on the 2 d. In addition, there was a strong correlation between NO<inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and NO<inline-formula><mml:math id="M288" 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> throughout the campaign (<inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.75</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>, Fig. S3). Meanwhile, the mean mass ratio of NO<inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to NO<inline-formula><mml:math id="M292" 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> was <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % throughout the campaign, but on several days (i.e., night of 27 April) NO<inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations significantly exceeded that of NO<inline-formula><mml:math id="M295" 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> (802 vs. 663 ng m<sup>−3</sup>). Previous study also reported comparable NO<inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and NO<inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations in at a forest site in the Southeast Tibet (summer: 100 vs. 110 ng m<sup>−3</sup>; winter: 180 vs. 270 ng m<sup>−3</sup>) (Bhattarai et al., 2019).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3964">Time series of multiple isotopic signatures of NO<inline-formula><mml:math id="M301" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M302" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M303" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M305" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) as well as corresponding concentrations in TSP samples during “Earth Summit Mission” scientific expedition in spring 2022. The gray shaded area denotes local nighttime.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Isotopic signatures of nitrite in TSP</title>
      <p id="d2e4037">Figure 4 presents the times series of <inline-formula><mml:math id="M306" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N, <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M308" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of NO<inline-formula><mml:math id="M309" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP, along with the NO<inline-formula><mml:math id="M310" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations. Similar to the variation trend of NO<inline-formula><mml:math id="M311" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations, NO<inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> isotopes varied in a wider range before 30 April, but became more stable afterward. For example, <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) ranged from <inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.9</mml:mn></mml:mrow></mml:math></inline-formula> ‰ to 0.8 ‰, with a relatively large standard deviation before 30 April compared to that after 30 April ((<inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">4.3</mml:mn></mml:mrow></mml:math></inline-formula>) ‰ vs. (<inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula>) ‰). The large variability in <inline-formula><mml:math id="M318" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) before 1 May is predominately attributed to the two high values observed in daytime of 27 April and night of 28 April. Note that the two high <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) samples were also associated with relatively high NO<inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> mass concentrations. In contrast to the declining trend of NO<inline-formula><mml:math id="M323" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations, the mean <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M325" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) values were comparable before and after 30 April. Relatively large variability was observed in TSP <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M327" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>), ranging from <inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9.0</mml:mn></mml:mrow></mml:math></inline-formula> ‰ to 3.9 ‰ and with an average of (<inline-formula><mml:math id="M329" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3.8</mml:mn></mml:mrow></mml:math></inline-formula>) ‰. TSP <inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M331" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) varied within a narrow range from <inline-formula><mml:math id="M332" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> ‰ to <inline-formula><mml:math id="M333" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> ‰ and with a mean of (<inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>) ‰. During the campaign, no significant correlations were observed between <inline-formula><mml:math id="M335" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M336" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) and the NO<inline-formula><mml:math id="M337" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations; while <inline-formula><mml:math id="M338" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M339" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) appeared to be moderately correlated with the NO<inline-formula><mml:math id="M340" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations (Fig. S5).</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e4455">The measured nitrite (and nitrate) concentration and isotopic signatures in surface soil collected in the Rongbuk Valley.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Soil sample ID</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col5" align="center" colsep="1">NO<inline-formula><mml:math id="M341" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" namest="col6" nameend="col9" align="center">NO<inline-formula><mml:math id="M342" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Conc.</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M344" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M345" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry colname="col6">Conc.</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M346" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N</oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">(ng g<sup>−1</sup>)</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">(ng g<sup>−1</sup>)</oasis:entry>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">East-1</oasis:entry>
         <oasis:entry colname="col2">67.7</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M351" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12.0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">6.1</oasis:entry>
         <oasis:entry colname="col5">3.3</oasis:entry>
         <oasis:entry colname="col6">1127.3</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.7</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">23.4</oasis:entry>
         <oasis:entry colname="col9">5.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">East-2</oasis:entry>
         <oasis:entry colname="col2">76.1</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M353" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11.9</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">2.7</oasis:entry>
         <oasis:entry colname="col5">2.2</oasis:entry>
         <oasis:entry colname="col6">1098.3</oasis:entry>
         <oasis:entry colname="col7">1.3</oasis:entry>
         <oasis:entry colname="col8">18.1</oasis:entry>
         <oasis:entry colname="col9">3.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">East-3</oasis:entry>
         <oasis:entry colname="col2">82.3</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">14.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">6.0</oasis:entry>
         <oasis:entry colname="col5">3.3</oasis:entry>
         <oasis:entry colname="col6">2978.1</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">25.4</oasis:entry>
         <oasis:entry colname="col9">6.6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">West-1</oasis:entry>
         <oasis:entry colname="col2">88.6</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M356" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.1</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">8.9</oasis:entry>
         <oasis:entry colname="col5">1.6</oasis:entry>
         <oasis:entry colname="col6">3176.5</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M357" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.1</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">44.5</oasis:entry>
         <oasis:entry colname="col9">13.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">West-2</oasis:entry>
         <oasis:entry colname="col2">106.2</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M358" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7.0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">11.4</oasis:entry>
         <oasis:entry colname="col5">1.5</oasis:entry>
         <oasis:entry colname="col6">2880.3</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M359" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">22.1</oasis:entry>
         <oasis:entry colname="col9">6.2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">West-3</oasis:entry>
         <oasis:entry colname="col2">179.3</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M360" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">12.7</oasis:entry>
         <oasis:entry colname="col5">1.4</oasis:entry>
         <oasis:entry colname="col6">7686.9</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">35.8</oasis:entry>
         <oasis:entry colname="col9">11.4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">South-1</oasis:entry>
         <oasis:entry colname="col2">53.8</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M362" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">12.7</oasis:entry>
         <oasis:entry colname="col5">6.7</oasis:entry>
         <oasis:entry colname="col6">3651.2</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M363" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">32.6</oasis:entry>
         <oasis:entry colname="col9">10.1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">South-2</oasis:entry>
         <oasis:entry colname="col2">42.3</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M364" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9.0</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">18.1</oasis:entry>
         <oasis:entry colname="col5">7.3</oasis:entry>
         <oasis:entry colname="col6">1683.2</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M365" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">49.3</oasis:entry>
         <oasis:entry colname="col9">14.8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">South-3</oasis:entry>
         <oasis:entry colname="col2">48.9</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M366" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">12.4</oasis:entry>
         <oasis:entry colname="col5">6.7</oasis:entry>
         <oasis:entry colname="col6">385.5</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M367" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8">45.7</oasis:entry>
         <oasis:entry colname="col9">14.9</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Surface soil nitrite concentration and isotopic signature</title>
      <p id="d2e5085">The concentration of soil NO<inline-formula><mml:math id="M368" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (and NO<inline-formula><mml:math id="M369" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) as well as the corresponding isotopic signatures are displayed in Table 1. The soil NO<inline-formula><mml:math id="M370" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> content on the west slope of Rongbuk Valley (on average 124.7 ng g<sup>−1</sup>) was higher than that observed on the east and south sides (75.3 and 48.3 ng g<sup>−1</sup>, respectively). The mean surface soil NO<inline-formula><mml:math id="M373" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and NO<inline-formula><mml:math id="M374" 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> in the Rongbuk Valley were 82.8 and 2740.8 ng g<sup>−1</sup>, respectively. The soil NO<inline-formula><mml:math id="M376" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations were significantly higher than the NO<inline-formula><mml:math id="M377" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> by a factor of <inline-formula><mml:math id="M378" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula>–40. In general, the measured soil NO<inline-formula><mml:math id="M379" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations at the Rongbuk valley were significantly lower than other remote regions of TP (i.e., 23.1 <inline-formula><mml:math id="M380" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">g</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at Naqu, 8.4 <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">g</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at Yangbajing), while soil NO<inline-formula><mml:math id="M382" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations were comparable to these reports (i.e., 90.3 ng g<sup>−1</sup> at Naqu, 131.2 ng g<sup>−1</sup> at Yangbajing) (Wang et al., 2019). Soil <inline-formula><mml:math id="M385" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) values ranged from <inline-formula><mml:math id="M387" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13.2</mml:mn></mml:mrow></mml:math></inline-formula> ‰ to <inline-formula><mml:math id="M388" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.2</mml:mn></mml:mrow></mml:math></inline-formula> ‰ (on average <inline-formula><mml:math id="M389" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.4</mml:mn></mml:mrow></mml:math></inline-formula> ‰), which are comparable to TSP <inline-formula><mml:math id="M390" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M391" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) (<inline-formula><mml:math id="M392" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">7.3</mml:mn></mml:mrow></mml:math></inline-formula> ‰). In comparison, we observed positive soil <inline-formula><mml:math id="M393" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M394" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M395" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>), ranging from 2.7 ‰ to 18.1 ‰ (on average 10.5 ‰) and 1.4 ‰ to 7.3 ‰ (on average 3.8 ‰), respectively, in contrast to the negative <inline-formula><mml:math id="M397" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M398" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) and near-zero <inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) observed in TSP samples. The determined soil <inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M402" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) is comparable to that in laboratory incubated soil (11.8 ‰–12.5 ‰) (Lewicka-Szczebak et al., 2021).</p>

<table-wrap id="T2" specific-use="star"><label>Table 2</label><caption><p id="d2e5513">Particulate nitrite concentration and formation pathways/sources compiled in the literature.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="2.5cm"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="3cm"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Site</oasis:entry>
         <oasis:entry colname="col2">Period</oasis:entry>
         <oasis:entry colname="col3" align="right">NO<inline-formula><mml:math id="M403" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> Conc. (Mean, ng m<sup>−3</sup>)</oasis:entry>
         <oasis:entry colname="col4" align="left">Formation pathways/Sources</oasis:entry>
         <oasis:entry colname="col5">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">QOMS station</oasis:entry>
         <oasis:entry colname="col2">Apr 2017</oasis:entry>
         <oasis:entry colname="col3" align="right">60</oasis:entry>
         <oasis:entry colname="col4" align="left">Biomass burning emission transported from South Asia</oasis:entry>
         <oasis:entry colname="col5">Bhattarai et al. (2023)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Bakersfield, California</oasis:entry>
         <oasis:entry colname="col2">May–Jul 2010</oasis:entry>
         <oasis:entry colname="col3" align="right">150</oasis:entry>
         <oasis:entry colname="col4" align="left">HONO uptake on lofted alkaline soil particles.</oasis:entry>
         <oasis:entry colname="col5">VandenBoer et al. (2014a)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Jinan, China</oasis:entry>
         <oasis:entry colname="col2">Nov 2013–Jan 2014</oasis:entry>
         <oasis:entry colname="col3" align="right">2080</oasis:entry>
         <oasis:entry colname="col4" align="left">Heterogeneous reactions of NO<sub>2</sub></oasis:entry>
         <oasis:entry colname="col5">Wang et al. (2015)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Seoul, Korea</oasis:entry>
         <oasis:entry colname="col2">May–Jul 2005</oasis:entry>
         <oasis:entry colname="col3" align="right">1410</oasis:entry>
         <oasis:entry colname="col4" align="left">Heterogeneous reactions of NO<sub>2</sub></oasis:entry>
         <oasis:entry colname="col5">Song et al. (2009)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Shanghai, China</oasis:entry>
         <oasis:entry colname="col2">Jun 2020</oasis:entry>
         <oasis:entry colname="col3" align="right">210</oasis:entry>
         <oasis:entry colname="col4" align="left">Heterogeneous reactions of NO<sub>2</sub>, reduction of NO<sub>2</sub> by S(IV)</oasis:entry>
         <oasis:entry colname="col5">Shang et al. (2021)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Mt. Heng, China</oasis:entry>
         <oasis:entry colname="col2">Apr 2009</oasis:entry>
         <oasis:entry colname="col3" align="right">2500</oasis:entry>
         <oasis:entry colname="col4" align="left">Surface TiO<sub>2</sub> photocatalysis of NO<sub>2</sub></oasis:entry>
         <oasis:entry colname="col5">Nie et al. (2012)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d2e5749">The significant contrast in NO<inline-formula><mml:math id="M411" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations between TSP and PM<sub>2.5</sub> samples, as shown in Fig. 1, suggests that at the sampling site atmospheric NO<inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> overwhelmingly exists in coarse particles. This observation is consistent with previous studies across the TP, which also reported the absence of NO<inline-formula><mml:math id="M414" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in fine mode particles (PM<sub>2.5</sub> and PM<sub>1.0</sub>) using either online real-time instrument or offline filter sampling (Decesari et al., 2010; Xu et al., 2020, 2024; Zhao et al., 2020), while relatively high levels of TSP NO<inline-formula><mml:math id="M417" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> have been reported (Bhattarai et al., 2019, 2023; Tripathee et al., 2017). In general, the chemical sources of particle NO<inline-formula><mml:math id="M418" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in the atmosphere encompass the uptake of HONO, particulate nitrate photolysis, and the NO<sub>2</sub>-related reactions (i.e., photo-enhanced uptake of NO<sub>2</sub> on mineral dust, heterogeneous reaction of NO<sub>2</sub> on the surface of aerosol) (Nie et al., 2012; VandenBoer et al., 2014a; Chen et al., 2019; Shang et al., 2021), as summarized in Table 2. In addition to these in-situ atmospheric processes, growing evidence has revealed that long-range transport of atmospheric pollutants from South Asia also contributes considerably to aerosol loadings in TP in the spring (Kang et al., 2019; Bhattarai et al., 2023; Zhao et al., 2020), which may also bring nitrite along with other pollutants. Moreover, the lifting of surface dust can also contribute to the atmospheric coarse particles and significantly influence the chemical composition of TSP (Zhang et al., 2021a; Pokharel et al., 2019), and therefore soil nitrite could also be a potential source for TSP NO<inline-formula><mml:math id="M422" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. In the following discussion, we examine the potential importance of the abovementioned processes to the observed high NO<inline-formula><mml:math id="M423" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> content in coarse particle and discern the most likely ones.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>The potential effects of atmospheric chemistry on NO<inline-formula><mml:math id="M424" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP</title>
      <p id="d2e5912">Increasing evidence supports particulate nitrate photolysis as an important source of atmospheric HONO especially in pristine atmosphere, with NO<inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> serving as the intermediate in the subsequent gas-particle partition process (Andersen et al., 2023; Ye et al., 2016). In theory, particulate NO<inline-formula><mml:math id="M426" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (and HONO) produced from particulate nitrate photolysis might be associated with extremely negative <inline-formula><mml:math id="M427" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values, due to the significant nitrogen isotopic fractionation effect during nitrate photolysis (Erbland et al., 2013; Frey et al., 2009). For example, NO<inline-formula><mml:math id="M428" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>  in water of hypersaline ponds and soil of McMurdo Dry Valleys, Antarctica, produced from the NO<inline-formula><mml:math id="M429" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> photolysis, were characterized by significantly negative <inline-formula><mml:math id="M430" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values (<inline-formula><mml:math id="M431" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M432" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> ‰) (Peters et al., 2014). However, <inline-formula><mml:math id="M433" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M434" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in this study was only <inline-formula><mml:math id="M435" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 ‰ lower than the <inline-formula><mml:math id="M436" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M437" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in TSP samples collected during this campaign (on average (<inline-formula><mml:math id="M438" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3.3</mml:mn></mml:mrow></mml:math></inline-formula>) ‰, Sect. S1) and that at the QOMS stations (annual average of (<inline-formula><mml:math id="M439" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.3</mml:mn></mml:mrow></mml:math></inline-formula>) ‰) (Wang et al., 2020). The similarity in <inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N isotopes between NO<inline-formula><mml:math id="M441" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and NO<inline-formula><mml:math id="M442" 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> suggests particulate nitrate photolysis is unlikely to be the primary source of the TSP NO<inline-formula><mml:math id="M443" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e6133">In addition to nitrate photolysis, the absorption of HONO on alkaline aerosols (i.e., lofted dust and road salt particles) can also result in accumulation of NO<inline-formula><mml:math id="M444" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> into the particle phase (VandenBoer et al., 2014a; Chen et al., 2019). For example, VandenBoer et al. (2014a) observed a synchronous enhancement of fine particle NO<inline-formula><mml:math id="M445" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (as high as 730 ng m<sup>−3</sup>) alongside the buildup of HONO (up to 1.37 ppbv) after sunset in an agricultural site (VandenBoer et al., 2014a). However, the levels of HONO in terrestrial background environments, typically on the order of dozens of pptv (Ye et al., 2023), are obviously too low to support the observed unexpectedly high levels of particulate NO<inline-formula><mml:math id="M447" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (up to 1300 ng m<sup>−3</sup>). What is more, previous studies indicated the HONO uptake predominately occurs on fine particles (Wang et al., 2015; Chen et al., 2019; Shang et al., 2021), while our observations indicated NO<inline-formula><mml:math id="M449" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> only exists in coarse particles.</p>
      <p id="d2e6209">The uptake of NO<sub>2</sub> on mineral dust has also been identified as a significant route for the formation of particulate NO<inline-formula><mml:math id="M451" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> or gas-phase HONO (Nie et al., 2012; Ndour et al., 2008). For example, Nie et al. (2012) found a significantly enhanced NO<inline-formula><mml:math id="M452" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in coarse particle during daytime in a dust storm event in Mt. Heng (up to 4.5 <inline-formula><mml:math id="M453" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) (Nie et al., 2012). The proposed mechanism is initiated by photo-enhanced conversion of NO<sub>2</sub> to NO<inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> via photo-produced electrons on surface of dust. Nevertheless, given the relatively small NO<sub>2</sub> uptake coefficients on mineral dust or salt surface (generally lower than <inline-formula><mml:math id="M457" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) (Yu et al., 2021; Bao et al., 2022; Xuan et al., 2025) and the low concentration of NO<sub>2</sub> in pristine environment of TP (e.g., <inline-formula><mml:math id="M459" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">140</mml:mn></mml:mrow></mml:math></inline-formula> pptv at Namco (Wang et al., 2023), and would be even lower at Mt. Qomolangma), such high levels of particulate NO<inline-formula><mml:math id="M460" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> are beyond the capacity of NO<sub>2</sub> heterogeneous reactions.</p>
      <p id="d2e6355">Other than the above-mentioned rationales, the atmospheric physicochemical processes leading to NO<inline-formula><mml:math id="M462" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production would influence both fine and coarse-mode particles, and some of the processes (e.g., HONO uptake) preferentially interact with fine-mode particles. However, the observation indicated NO<inline-formula><mml:math id="M463" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> only exists in TSP but not PM<sub>2.5</sub>, suggesting atmospheric physicochemical processes are unlikely to account for the elevated levels of NO<inline-formula><mml:math id="M465" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in TSP.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Potential effect of atmospheric pollutants in South Asia via long-range transport</title>
      <p id="d2e6411">There is a growing body of compelling evidence indicating that the elevated aerosol loadings and some chemical species in TP during spring, i.e., black carbon (Cong et al., 2015; Kang et al., 2019) and soluble components (Dasari et al., 2023; Bhattarai et al., 2023; Lin et al., 2021; Wang et al., 2020; Zhao et al., 2020) are significantly linked to biomass burning emissions from South Asia, which can penetrate into TP via long range transport. Recently, Bhattarai et al. (2023) observed synchronously elevated water-soluble nitrogen compounds (i.e., NO<inline-formula><mml:math id="M466" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NH<inline-formula><mml:math id="M467" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M468" 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>), levoglucosan (a molecule marker for biomass burning) and bulk <inline-formula><mml:math id="M469" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N signatures in TSP at QOMS station, once upon the arrival of biomass burning plumes from South Asia (Bhattarai et al., 2023). Specially, they found that TSP NO<inline-formula><mml:math id="M470" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> averaged 60 ng m<sup>−3</sup> during the spring biomass burning influenced episodes, while NO<inline-formula><mml:math id="M472" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was always below the detection limit in other seasons (Bhattarai et al., 2023). This suggests that biomass burning events in South Asia and the subsequent long-range transport could contribute to the accumulation of NO<inline-formula><mml:math id="M473" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in aerosols in Tibet.</p>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e6512">The modelled air-mass back trajectories during “Earth Summit Mission” scientific expedition in spring 2022 (<bold>a</bold>: from 1 to 6 May; <bold>b</bold>: 26 to 30 April). The active fire spots captured by MODIS (<uri>https://worldview.earthdata.nasa.gov</uri>, last access: 7 September 2024), the red dots in the figure) are also presented.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/25/10625/2025/acp-25-10625-2025-f05.jpg"/>

        </fig>

      <p id="d2e6530">In this study, the mass concentrations and compositions of water-soluble ions, including SO<inline-formula><mml:math id="M474" 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="M475" 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>, NH<inline-formula><mml:math id="M476" 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 TSP NO<inline-formula><mml:math id="M477" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, also varied substantially throughout the springtime campaign (Fig. 1). The potential effect of South Asian pollutants on our observations was explored by analyzing the air masses origins during the sampling period. As shown in Fig. 5, during the first-half of the campaign (i.e., before 30 April), air masses predominately originated from or passed through northern India and Nepal with intensive human activities and numerous fire hotspots (represented by the dense red dots in Fig. 5), indicating the potential impact of South Asia pollutants on aerosol loadings of TP. Correspondingly, elevated concentrations of secondary inorganic ions (i.e., NH<inline-formula><mml:math id="M478" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M479" 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 SO<inline-formula><mml:math id="M480" 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>) in TSP and PM<sub>2.5</sub> were observed before 30 April, which are comparable to the values of previous reports in QOMS station when arrived air masses experiencing severe biomass burning emissions (Bhattarai et al., 2023; Lin et al., 2021). Meanwhile, elevated levels of TSP NO<inline-formula><mml:math id="M482" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M483" display="inline"><mml:mrow><mml:mn mathvariant="normal">625</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">457</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>) was observed during this biomass burning-impacted period, and <inline-formula><mml:math id="M485" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M486" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) values exhibited substantial variability. TSP samples collected during daytime of 27 April and night of 28 April were associated with high NO<inline-formula><mml:math id="M487" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations and <inline-formula><mml:math id="M488" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M489" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) values. In comparison, TSP NO<inline-formula><mml:math id="M490" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in other samples were significantly <sup>15</sup>N-depleted. Assuming that biomass burning emission accounted for the two high <inline-formula><mml:math id="M492" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M493" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) samples (Bhattarai et al., 2023), the observed relatively low <inline-formula><mml:math id="M494" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M495" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) in other samples before 30 April likely indicated the potential contribution from additional emission sources.</p>
      <p id="d2e6797">From 1 to 6 May, air masses originated primarily from the inside of the TP or surroundings and none of the fire hotspot was detected at the whole TP and along the air mass trajectories (Fig. 5), potentially excluding the influence of biomass burning and anthropogenic emissions during this period. Accompanied by this significant shift in air mass origins, the concentrations of NH<inline-formula><mml:math id="M496" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, NO<inline-formula><mml:math id="M497" 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 SO<inline-formula><mml:math id="M498" 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> in both PM<sub>2.5</sub> and TSP, as well as the TSP NO<inline-formula><mml:math id="M500" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> apparently decreased. In particular, NH<inline-formula><mml:math id="M501" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in most PM<sub>2.5</sub> and TSP samples were below the detection limit during this period. Furthermore, K<sup>+</sup> in PM<sub>2.5</sub>, a common tracer for biomass burning, declined from <inline-formula><mml:math id="M505" display="inline"><mml:mrow><mml:mn mathvariant="normal">269</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">432</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> before 30 April to <inline-formula><mml:math id="M507" display="inline"><mml:mrow><mml:mn mathvariant="normal">22</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> after 30 April, with the difference being statistically significant (<inline-formula><mml:math id="M509" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>). Meanwhile, the average TSP NO<inline-formula><mml:math id="M510" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> also declined significantly from <inline-formula><mml:math id="M511" display="inline"><mml:mrow><mml:mn mathvariant="normal">625</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">457</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> before 30 April to <inline-formula><mml:math id="M513" display="inline"><mml:mrow><mml:mn mathvariant="normal">147</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">145</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup> after 30 April. Note substantially high levels of TSP NO<inline-formula><mml:math id="M515" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> were also observed on several days after 30 April, i.e., during daytime of 3 May (<inline-formula><mml:math id="M516" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>). Although the TSP NO<inline-formula><mml:math id="M518" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentrations varied in wide range after 30 April, the <inline-formula><mml:math id="M519" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M520" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) was relatively stable and comparable to that determined before 30 April (except for the two high <inline-formula><mml:math id="M521" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N(NO<inline-formula><mml:math id="M522" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) samples).</p>
      <p id="d2e7115">In short summary, these results likely suggest the significant impact of South Asia pollutants (i.e., biomass burning emissions) through long-range transport on the TSP NO<inline-formula><mml:math id="M523" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, especially for samples collected before 30 April. However, it is difficult for the long-range transport to explain why NO<inline-formula><mml:math id="M524" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is predominately present in coarse particles, as fine mode particle is typically easier to be transported in principle. While further studies need to be conducted to find out the exact reasons, one possibility is that the size partition of fine particle NO<inline-formula><mml:math id="M525" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> toward the coarse mode range during transport. Similar size shifts of NO<inline-formula><mml:math id="M526" 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> have been observed and used to explain the enrichment of NO<inline-formula><mml:math id="M527" 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> in coarse-mode aerosols in marine environment (Matsumoto et al., 2009). In addition, the coarse mode particles in this study contain more alkaline species (Fig. 2), which makes nitrite more stable in TSP during the transport or more stably exist in TSP after being uptake when the polluted air masses reaching TP. For the period after 30 April, since air masses originated from clean regions with little to no biomass burning sources, other sources of nitrite might be required.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>The potential effects of lofted dust</title>
      <p id="d2e7186">Previous reports have confirmed that wind-blown mineral dust contributed significantly to coarse mode aerosols in TP (Kang et al., 2016; Zhang et al., 2021a). Notably, surface soil collected from the Rongbuk valley is characterized with elevated NO<inline-formula><mml:math id="M528" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> concentration (up to 180 ng g<sup>−1</sup>, Table 1). The surface soil NO<inline-formula><mml:math id="M530" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is expected to mainly reside in the coarse mode after suspended in the atmosphere (Drakaki et al., 2022), consistent with our observations that particle NO<inline-formula><mml:math id="M531" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was predominately confined into coarse particle. The unique environment of Rongbuk valley, characterized by exposed surface soil and strong wind (reaching as high as 9 m s<sup>−1</sup> during this campaign) could facilitate the resuspension of soil components into the atmosphere. Furthermore, small localized tornadoes were frequently observed before 30 April, while the snow events occurred in 30 April would reduce the soil-derived dust emission by increasing the snow coverage and enriching the soil moisture. In fact, concentrations of Ca<sup>2+</sup> in TSP, which predominately originate from dust emission, also declined to some extent after 30 April.</p>
      <p id="d2e7262">In addition, the comparable <inline-formula><mml:math id="M534" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>N values of NO<inline-formula><mml:math id="M535" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> between TSP collected after 1 May (<inline-formula><mml:math id="M536" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">8.0</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> ‰) and the surface soil (<inline-formula><mml:math id="M537" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3.0</mml:mn></mml:mrow></mml:math></inline-formula> ‰) also supports that locally emitted surface soil is an important contributor to the observed high levels of TSP NO<inline-formula><mml:math id="M538" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. But one should note that the oxygen isotopes (<inline-formula><mml:math id="M539" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M540" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) of TSP NO<inline-formula><mml:math id="M541" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> were significantly lower compared to that in soil NO<inline-formula><mml:math id="M542" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, indicating that the original soil NO<inline-formula><mml:math id="M543" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> oxygen isotope may have been modified after resuspension. This discrepancy could be explained by the potential oxygen isotope exchanges between TSP NO<inline-formula><mml:math id="M544" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and aerosol liquid water (fractionation effect of <inline-formula><mml:math id="M545" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="italic">ε</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">16</mml:mn></mml:mrow></mml:math></inline-formula> ‰ at local temperature, <inline-formula><mml:math id="M546" display="inline"><mml:mrow><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">270</mml:mn></mml:mrow></mml:math></inline-formula> K, <inline-formula><mml:math id="M547" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mn mathvariant="normal">18</mml:mn></mml:msup><mml:msub><mml:mi mathvariant="italic">ε</mml:mi><mml:mi mathvariant="normal">eq</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.12</mml:mn><mml:mi>T</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">48.79</mml:mn></mml:mrow></mml:math></inline-formula> (Buchwald and Casciotti, 2013)), which tend to deplete both the initial <inline-formula><mml:math id="M548" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M549" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M550" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M551" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>).</p>
      <p id="d2e7505">We noted the oxygen isotope exchange process between NO<inline-formula><mml:math id="M552" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and H<sub>2</sub>O also occurs in surface soil. Previous study indicated that in high-altitude arid regions of TP (i.e., <inline-formula><mml:math id="M554" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5000</mml:mn></mml:mrow></mml:math></inline-formula> m), denitrification process dominated the surface soil NO<inline-formula><mml:math id="M555" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> production, accounting for <inline-formula><mml:math id="M556" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">75</mml:mn></mml:mrow></mml:math></inline-formula> % (Wang et al., 2019). Soil NO<inline-formula><mml:math id="M557" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> generated from denitrification process is expect to inherit the <inline-formula><mml:math id="M558" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O signatures of substrate NO<inline-formula><mml:math id="M559" 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>. In this study, the surface soil <inline-formula><mml:math id="M560" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M561" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) were positive with average values of 9.6 ‰ (Table 1). The positive soil <inline-formula><mml:math id="M562" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M563" 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>) have been observed on arid environments (Wang et al., 2016), such as desert soil, where the low water moisture favors the preservation of atmospherically derived NO<inline-formula><mml:math id="M564" 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>. One could estimate that soil <inline-formula><mml:math id="M565" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M566" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) derived from the denitrification would be 9.6 ‰, nitrite from other sources (e.g., nitrification) should possess zero <inline-formula><mml:math id="M567" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O, thus in total nitrite in soil should possess <inline-formula><mml:math id="M568" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of <inline-formula><mml:math id="M569" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7.2</mml:mn></mml:mrow></mml:math></inline-formula> ‰ (estimated as <inline-formula><mml:math id="M570" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.75</mml:mn><mml:mo>×</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>(</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>). However, the determined soil <inline-formula><mml:math id="M571" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M572" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) (3.8 ‰) is significantly lower compared to the estimated soil <inline-formula><mml:math id="M573" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M574" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>), indicating the occurrence of exchange process between soil water and NO<inline-formula><mml:math id="M575" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, which would reduce the soil <inline-formula><mml:math id="M576" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M577" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) to some extent. The exchange process between soil water and NO<inline-formula><mml:math id="M578" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is particularly evident in west slope of Rongbuk Valley, where soil <inline-formula><mml:math id="M579" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M580" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) is as low as 1.5 ‰ while soil <inline-formula><mml:math id="M581" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M582" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) is on average 10.3 ‰. Soil <inline-formula><mml:math id="M583" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M584" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) should be erased to near-zero if exchange process between soil water and NO<inline-formula><mml:math id="M585" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> was efficient. Therefore, the fact that the observed soil <inline-formula><mml:math id="M586" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M587" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) remain above 0 ‰ indicates unfavorable conditions for the oxygen isotope exchange process, likely due to the extremely low soil moisture content (<inline-formula><mml:math id="M588" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> %) in surface soil (Ma et al., 2023).</p>
      <p id="d2e7952">Upon resuspension into atmosphere, the soil-derived dust aerosols usually exhibited a certain degree of hygroscopicity (Tang et al., 2016; Chen et al., 2020), allowing the absorption of water molecule on dust aerosol. For example, the aerosol water was determined to account for <inline-formula><mml:math id="M589" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 % of the total PM<sub>10</sub> mass during Saharan dust plumes (Cardoso et al., 2018). Based on laboratory experiment, Tang et al. (2019) reported that Asian dust also exhibited substantial hygroscopic property and revealed that the water-soluble inorganic ions, such as Cl<sup>−</sup>, SO<inline-formula><mml:math id="M592" 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> and NO<inline-formula><mml:math id="M593" 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> played a critical role in the absorption of water molecules on dust aerosol (Tang et al., 2019). In the present study, the SO<inline-formula><mml:math id="M594" 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> and NO<inline-formula><mml:math id="M595" 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> account for <inline-formula><mml:math id="M596" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % of the total mass of water-soluble ions in TSP, implying the potential uptake of water vapor on aerosol surface. In addition to water-soluble ions, the hygroscopicity of mineral dust also depends on the surface areas, and wind-blown dust experiences a substantial increase in surface area after being lifted into the atmosphere, enhancing its capacity for water uptake (Chen et al., 2020; Seisel et al., 2004). The hygroscopicity of dust aerosol is expected to accelerate the oxygen isotope exchanges between NO<inline-formula><mml:math id="M597" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and aerosol liquid water. The atmospheric water vapor <inline-formula><mml:math id="M598" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O isotope in TP is determined to be significantly negative (approximately <inline-formula><mml:math id="M599" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> ‰ to <inline-formula><mml:math id="M600" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> ‰ at a remote site in TP with altitude of <inline-formula><mml:math id="M601" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4200</mml:mn></mml:mrow></mml:math></inline-formula> m) (Yu et al., 2015). Similarly, the oxygen isotope exchange between NO<inline-formula><mml:math id="M602" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and H<sub>2</sub>O would also homogenize and erase original soil <inline-formula><mml:math id="M604" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O(NO<inline-formula><mml:math id="M605" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) signals, because aerosol liquid water is characterized by negligible <inline-formula><mml:math id="M606" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O values (Luz and Barkan, 2005). Consequently, isotope exchange with aerosol water would further reduce both <inline-formula><mml:math id="M607" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M608" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of TSP NO<inline-formula><mml:math id="M609" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, effectively masking the original isotopic signature inherited from surface soil.</p>
      <p id="d2e8190">We also noted that NO<inline-formula><mml:math id="M610" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> in surface soil is significantly lower than NO<inline-formula><mml:math id="M611" 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>, by on average 35 times (Table 1), contrasting with the chemical compositions in TSP. It is important to note that during the complex dust generation and aerosolization processes, water-soluble ions exhibit significant chemical enrichment relative to that in parent soil (Wu et al., 2022; Gao et al., 2023). For example, Wu et al. (2022) reported that contents of nitrate in sand dust-derived PM<sub>10</sub> is higher than the original soil samples by <inline-formula><mml:math id="M613" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>–80 times, while sulphate can be up to 500 times higher than the original soil. Although the enrichment of nitrite has not been evaluated to the extent of our knowledge, we propose that the observed discrepancy of nitrate <inline-formula><mml:math id="M614" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> nitrite ratio between TSP and surface soil can be reconciled if the nitrite is enriched more efficiently than nitrate during dust aerosolization, i.e., by a factor of 30. To further assess the potential contribution of resuspended soil to elevated nitrite in TSP, we conducted a rough estimation based on laboratory investigations from Wu et al. (2022). First, the springtime TSP concentrations observed in the nearby QOMS station is used (<inline-formula><mml:math id="M615" display="inline"><mml:mrow><mml:mn mathvariant="normal">65.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">50.9</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M616" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; Liu et al., 2017), as TSP mass concentrations surrounding the Base camp were not available. Second, we assume the nitrite content in soil-derived coarse particles to be similar to that of nitrate (0.2 %) in laboratory-generated dust aerosol from natural sandy and gravel soils (Wu et al., 2022), which is comparable to the soil texture of the Rongbuk Valley. This assumption can also explain the comparable amounts of nitrite and nitrate observed in TSP samples in this study. Results shown that the concentrations of nitrite in TSP can be approximately <inline-formula><mml:math id="M617" display="inline"><mml:mrow><mml:mn mathvariant="normal">130</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">102</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>, on the same order with the observed nitrite concentration in TSP after 30 April (<inline-formula><mml:math id="M619" display="inline"><mml:mrow><mml:mn mathvariant="normal">147</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">145</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>) but substantially lower than that before 30 April (<inline-formula><mml:math id="M621" display="inline"><mml:mrow><mml:mn mathvariant="normal">625</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">457</mml:mn></mml:mrow></mml:math></inline-formula> ng m<sup>−3</sup>). Therefore, we speculate that the resuspension of surface soil may account for the observed TSP nitrite after 30 April, whereas the biomass burning and soil together co-contributed to the high TSP nitrite before 30 April. This is also consistent with the shift of air mass origins, which clearly indicated that airmasses before 30 April is significantly impacted by the biomass burning emissions, and after 30 April airmasses primarily originated from clean regions. While we acknowledge that this simplistic estimation is subject to substantial uncertainty, it provides a first-order assessment supporting the hypothesis that wind-blown soil dust contributes to coarse-mode particulate nitrite. Previously, wind-blown mineral dust has been verified as a potential source for aerosol water-soluble ions (Engelbrecht et al., 2016; Wu et al., 2022, 2012) and dust aerosol is also recognized as one of the important aerosol types over TP (Pokharel et al., 2019).</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusion and Implications</title>
      <p id="d2e8358">Unexpectedly high levels of NO<inline-formula><mml:math id="M623" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> associated with coarse-particle were observed in the pristine environment at Mt. Qomolangma in the spring, 2022. After examining the potential contributions of various NO<inline-formula><mml:math id="M624" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> sources with assistance from air mass back-trajectory and isotope analyses, we propose that both soil-derived nitrite and long-range transport of pollutants from South Asia may contribute to coarse-particle NO<inline-formula><mml:math id="M625" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> during spring at Mt. Qomolangma. This is also consistent with previous reports showing that dust and biomass burning emissions through long-range transport from South Asia are the predominant contributors to the springtime aerosol loadings over TP (Zhao et al., 2020; Pokharel et al., 2019). The nitrite concentrations and isotopes further indicated that soil-derived nitrite likely serves as a baseline source of atmospheric NO<inline-formula><mml:math id="M626" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, maintaining the background levels of TSP NO<inline-formula><mml:math id="M627" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> at this pristine site, reflected by the relatively stable isotopes when soil-derived nitrite predominated. In addition, air masses originating from South Asia would result in elevated levels of NO<inline-formula><mml:math id="M628" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> observed before 30 April by bringing additional biomass burning and anthropogenic pollutants, as evidenced by the more varied isotopes before 30 April compared to after that day when air mass origins shifted from South Asia to central and north Tibet. However, the detailed mechanisms of nitrite enriched on the coarse particle remain unknown and need further explorations.</p>
      <p id="d2e8434">In the atmosphere, photolysis of particle nitrite can produce OH radical and NO, the latter is essential for the formation of atmospheric oxidants and secondary aerosols. Moreover, the elevated levels of particle NO<inline-formula><mml:math id="M629" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> may serve as an important HONO source through the gas-to-particle partition process (VandenBoer et al., 2014a), and the thermodynamic equilibrium between particulate nitrite and HONO ([pN(III)] <inline-formula><mml:math id="M630" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [HONO] ratio) is primarily governed by the particle acidity and liquid water content (LWC) in theory (Fountoukis and Nenes, 2007; VandenBoer et al., 2014a; Chen et al., 2019). Based on the observed TSP NO<inline-formula><mml:math id="M631" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and estimated ratio of [pN(III)] <inline-formula><mml:math id="M632" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> [HONO] (from 4.8 to 10.6, Sect. S2 in the Supplement), we can estimate the potential level of atmospheric HONO if the partition ever occurs at this site (VandenBoer et al., 2014b), and result indicates HOHO would be at 8–15 pptv, on the same order with the observations at a central Tibetan site (<inline-formula><mml:math id="M633" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> pptv at Namco; Wang et al., 2023). Given that TSP concentrations usually reach maximum during spring over TP, i.e., <inline-formula><mml:math id="M634" display="inline"><mml:mrow><mml:mn mathvariant="normal">65</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">51</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M635" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at the nearby QOMS station (Liu et al., 2017), our findings suggest that the coarse-particle may serve as a potential source of atmospheric HONO and NO<sub><italic>x</italic></sub> assuming the TSP are associated with nitrite. Although the coarse-particle tend to deposit rapidly within hours, their potential to influence local atmospheric chemistry remains important to some extent, particularly considering the frequent dust events in TP (loose arid/semiarid surface, sparse vegetation, and strong winds; Long et al., 2025) and the ubiquity of long-range transport of biomass burning emissions from South Asia during this season. The impact of the TSP nitrite on the budget of NO<sub><italic>x</italic></sub>, HONO and OH radicals especially in the background atmosphere could be investigated using regional or global atmospheric transport model, once the detailed mechanism regarding the sources and chemistry of TSP nitrite been elucidated. In summary, our results highlight the need for further investigation into the sources, partitioning, and chemical reactivity of aerosol-phase nitrite, particularly in the pristine Tibetan Plateau, where even small inputs of NO<sub><italic>x</italic></sub> or HONO can disproportionately affect oxidant budgets and reactive nitrogen cycling.</p>
</sec>

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

      <p id="d2e8548">The data supporting the findings of this study are available in the archival repository at  <ext-link xlink:href="https://doi.org/10.6084/m9.figshare.28188320.v1" ext-link-type="DOI">10.6084/m9.figshare.28188320.v1</ext-link> (Zhang and Geng, 2025).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e8554">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-25-10625-2025-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-25-10625-2025-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e8563">LG designed the research, interpreted the data; LG and ZZ prepared the manuscript with contributions from all co-authors; ZZ, YW, CY, TZ, CZ, ZJ, and PC, conducted the field sampling and laboratory measurements; LG, ZZ, and PC, acquired funding; LG, SK, and CY reviewed and edited the manuscript. All authors have given approval to the final version of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e8569">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="d2e8575">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. Also, please note that this paper has not received English language copy-editing.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e8581">We thank Yunhong Zhou for the help in air mass back trajectory analysis. The authors thank all researchers involved in the “Earth Summit Mission-2022” scientific expedition from Peking University, Hefei Institutes of Physical Science Anhui Institute of Optics and Fine Mechanics of Chinese Academy of Sciences, Minzu University of China.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e8586">Z.Z. acknowledges financial support from the National Natural Science Foundation of China (awards 42273001 and 42494851) and the Key Research and Development Plan Project of Anhui Province (2022l07020032). L.G. acknowledges financial support from the National Natural Science Foundation of China (awards W2411030, 42371151, and 41871051), the National Key R&amp;D Program of China (2022YFC3700701), and the Innovation Program for Quantum Science and Technology (2021ZD0303101). P.C. acknowledges financial support from the National Natural Science Foundation of China (award: 42371151).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e8592">This paper was edited by Armin Sorooshian and reviewed by Junling Li and two anonymous referees.</p>
  </notes><ref-list>
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