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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-26-6283-2026</article-id><title-group><article-title>Continental and marine source regions contributing to the outflow of the Asian summer monsoon anticyclone during the PHILEAS campaign in summer 2023</article-title><alt-title>PHILEAS</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Vogel</surname><given-names>Bärbel</given-names></name>
          <email>b.vogel@fz-juelich.de</email>
        <ext-link>https://orcid.org/0000-0001-9763-3055</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Lauther</surname><given-names>Valentin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Köllner</surname><given-names>Franziska</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4967-5514</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4 aff5">
          <name><surname>Ekinci</surname><given-names>Fatih</given-names></name>
          
        <ext-link>https://orcid.org/0009-0001-5979-0778</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Rolf</surname><given-names>Christian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5329-0054</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Strobel</surname><given-names>Johannes</given-names></name>
          
        <ext-link>https://orcid.org/0009-0007-3457-6672</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>van Luijt</surname><given-names>Ronja</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Volk</surname><given-names>C. Michael</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff4">
          <name><surname>Borrmann</surname><given-names>Stephan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4774-9380</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Dragoneas</surname><given-names>Antonis</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2827-7733</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Eppers</surname><given-names>Oliver</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9487-4603</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Molleker</surname><given-names>Sergej</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2980-0330</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hoor</surname><given-names>Peter</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6582-6864</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Ort</surname><given-names>Linda</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Weyland</surname><given-names>Franziska</given-names></name>
          
        <ext-link>https://orcid.org/0009-0004-3067-3879</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Zahn</surname><given-names>Andreas</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Clemens</surname><given-names>Jan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2422-9454</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Günther</surname><given-names>Gebhard</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4111-6221</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kachula</surname><given-names>Oleh</given-names></name>
          
        <ext-link>https://orcid.org/0009-0006-4506-3605</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Müller</surname><given-names>Rolf</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5024-9977</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Ploeger</surname><given-names>Felix</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Riese</surname><given-names>Martin</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Climate and Energy Systems (ICE-4), Forschungszentrum Jülich, Jülich, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute for Atmospheric and Environmental Research, University of Wuppertal, Wuppertal, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Johannes Gutenberg University of Mainz, Institute for Atmospheric Physics, Mainz, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Max Planck Institute for Chemistry, Mainz, Germany</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Institute for Applied Geosciences (Environmental Mineralogy), Technical University of Darmstadt, Darmstadt, Germany</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Bärbel Vogel (b.vogel@fz-juelich.de)</corresp></author-notes><pub-date><day>11</day><month>May</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>9</issue>
      <fpage>6283</fpage><lpage>6319</lpage>
      <history>
        <date date-type="received"><day>19</day><month>November</month><year>2025</year></date>
           <date date-type="rev-request"><day>5</day><month>December</month><year>2025</year></date>
           <date date-type="rev-recd"><day>20</day><month>April</month><year>2026</year></date>
           <date date-type="accepted"><day>21</day><month>April</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Bärbel Vogel et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026.html">This article is available from https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e308">During the PHILEAS aircraft campaign, which probed the export of air from the Asian summer monsoon anticyclone (ASMA), observations were carried out from Germany and Alaska during August and September 2023. The flights from Germany sampled the western part of the ASMA and its westward outflow. The flights from Alaska probed filaments that had separated from the ASMA at its eastern flank and were transported across the Pacific. This work integrates PHILEAS aircraft in situ measurements with results from Lagrangian transport simulations. Our results show that air masses within the ASMA and its outflow are characterised by a mixture of different continental and marine sources. In the western part of the ASMA and its westward outflow, enhanced pollutants and greenhouse gases such as <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, aerosols, <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> were detected, indicating sources in South Asia. Additional marine air masses from the western Pacific, characterised by enhanced <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and low <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, were found in filaments separated at the ASMA's eastern flank. Thus, air masses from two different surface regions and with different chemical compositions are mixed in filaments separated at the ASMA's eastern flank. Our findings show that the chemical composition of the ASMA's outflow is highly variable and depends on altitude, surface emissions, mixing of air masses from different source regions, and the interplay between the ASMA and tropical cyclones. Overall, the results provide strong support for the Asian summer monsoon is an important pathway for transporting short-lived ozone-depleting and radiatively active substances into the stratosphere.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Deutsche Forschungsgemeinschaft</funding-source>
<award-id>VO 1276_7-1</award-id>
<award-id>HO-4225/17-1</award-id>
<award-id>HO-4225/19-1</award-id>
<award-id>KO 6470/1- 1</award-id>
<award-id>VO 1276/6-1</award-id>
<award-id>BO 1829/12-1</award-id>
<award-id>TRR 301 TPChange project Project-ID 428312742</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="d2e387">During boreal summer, the Asian summer monsoon forms a seasonally persistent, zonally confined circulation system that efficiently transports climate-relevant emissions (e.g. greenhouse gases, ozone-depleting substances, aerosol particles, and their gas-phase precursors) from near-surface levels to higher altitudes, specifically into the upper troposphere and lower stratosphere (UTLS) <xref ref-type="bibr" rid="bib1.bibx63 bib1.bibx84 bib1.bibx77 bib1.bibx108" id="paren.1"><named-content content-type="pre">e.g.</named-content></xref>. Between June and September, deep convection over South Asia, particularly over the northern Indian subcontinent and China, is associated with the formation of the Asian summer monsoon anticyclone (ASMA), which extends from northeastern Africa to the western Pacific at UTLS levels <xref ref-type="bibr" rid="bib1.bibx77 bib1.bibx107" id="paren.2"><named-content content-type="pre">e.g.</named-content></xref>. The strong anticyclonic circulation at the edge of the ASMA acts as an effective transport barrier <xref ref-type="bibr" rid="bib1.bibx79 bib1.bibx44" id="paren.3"><named-content content-type="pre">e.g.</named-content></xref>, leading to the confinement of tropospheric trace gases and aerosols within the anticyclone <xref ref-type="bibr" rid="bib1.bibx89 bib1.bibx61 bib1.bibx101 bib1.bibx12 bib1.bibx91" id="paren.4"><named-content content-type="pre">e.g.</named-content></xref>. However, filaments and sometimes smaller anticyclonic systems (eddies) are frequently shed from the ASMA during boreal summer – particularly at its northeastern flank (e.g. over northeastern China, Korea, and Japan). These structures are transported eastward along the subtropical jet stream towards North America (e.g. Alaska), and subsequently can reach the Atlantic Ocean and Europe <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx27 bib1.bibx100 bib1.bibx96 bib1.bibx14" id="paren.5"><named-content content-type="pre">e.g.</named-content></xref>. Likewise, air masses can be transported from the ASMA at its western flank (e.g. over northern Africa and the Mediterranean region) westward into the tropical tropopause layer. Finally, these young air masses from the ASMA can potentially be transported into the extratropical lower stratosphere and irreversibly mixed with the surrounding stratospheric air <xref ref-type="bibr" rid="bib1.bibx106" id="paren.6"/>.</p>
      <p id="d2e419">This process affects the chemical composition and radiative balance of the northern extratropical UTLS <xref ref-type="bibr" rid="bib1.bibx86 bib1.bibx1" id="paren.7"/>. Consequently, during the Asian summer monsoon season, the northern extratropical lower stratosphere is flooded by isentropic transport – sometimes referred to as “flushing” <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx10" id="paren.8"/> – with moist, polluted air originating from South Asia, which is among the most polluted and densely populated regions of the world. This results in enhanced concentrations of greenhouse gases (e.g. <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SF</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), pollutants (e.g. CO, PAN, aerosols), and short-lived ozone-depleting substances (e.g. <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CHCl</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), particularly those of anthropogenic origin in the northern extratropical UTLS <xref ref-type="bibr" rid="bib1.bibx78 bib1.bibx104 bib1.bibx106 bib1.bibx88 bib1.bibx111 bib1.bibx55 bib1.bibx25 bib1.bibx32 bib1.bibx87" id="paren.9"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d2e496">In the northwestern Pacific region, tropical cyclones (including typhoons) occur throughout the year, with peak activity from July to October <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx64" id="paren.10"/>, coinciding with the peak phase of the ASMA. The interplay between the spatial position of the ASMA and tropical cyclones plays a key role in controlling horizontal transport in the UTLS of marine air uplifted in the western Pacific, in particular if tropical cyclones occur at the edge of the ASMA. Measurements show that ozone- and aerosol-poor marine air, uplifted by tropical cyclones, can be injected into the anticyclonic flow of the ASMA <xref ref-type="bibr" rid="bib1.bibx104 bib1.bibx56 bib1.bibx58 bib1.bibx59 bib1.bibx33 bib1.bibx16 bib1.bibx5" id="paren.11"><named-content content-type="pre">e.g.</named-content></xref>. This process can lead to reduced ozone in the UTLS over South Asia <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx60" id="paren.12"/>. Further, wet marine air can be uplifted into the UTLS by typhoons and enhance water vapour in this region, however dehydration processes can also decrease water vapour in air masses uplifted by typhoons <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx60" id="paren.13"/>. Similarly, ice crystals can be injected into the lower stratosphere by tropical cyclones, leading to hydration. The resulting moist plumes can subsequently be affected by the flow of the ASMA <xref ref-type="bibr" rid="bib1.bibx75" id="paren.14"/>. Hence, the rapid uplift by tropical cyclones generally transports air of marine origin to altitudes of the ASMA, but upward transport of polluted air masses during landfall of tropical cyclones also occurs <xref ref-type="bibr" rid="bib1.bibx56" id="paren.15"><named-content content-type="pre">e.g.</named-content></xref>. Further, subsequent filaments separated from the ASMA can transport boundary layer air from the western Pacific into the northern extratropical UTLS (e.g. towards North America and Europe) <xref ref-type="bibr" rid="bib1.bibx104" id="paren.16"/>.</p>
      <p id="d2e525">Several balloon campaigns have been conducted over the past decades across the Indian subcontinent and China, aiming to measure trace gases – particularly ozone and water vapour – as well as aerosol backscatter within the ASMA <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx11 bib1.bibx102 bib1.bibx24" id="paren.17"><named-content content-type="pre">e.g.</named-content></xref>. As part of the StratoClim project, an aircraft campaign was carried out in Kathmandu (Nepal) during summer 2017, providing observations up to 20 <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> altitude and probing the top of the ASMA <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx1 bib1.bibx109" id="paren.18"><named-content content-type="pre">e.g.</named-content></xref>. Despite these unique measurements, further comprehensive in-situ data sets within the ASMA in other years remain lacking.</p>
      <p id="d2e547">Air masses from the eastward outflow of the ASMA, transported along the subtropical jet toward North America and further downstream, were observed during two aircraft campaigns over Europe and the North Atlantic: the “Transport and Composition in the Upper Troposphere and Lowermost Stratosphere” (TACTS) campaign, conducted jointly with the “Earth System Model Validation” (ESMVal) experiment in August and September 2012 <xref ref-type="bibr" rid="bib1.bibx104 bib1.bibx106 bib1.bibx70 bib1.bibx31 bib1.bibx88" id="paren.19"><named-content content-type="pre">e.g.</named-content></xref>, and the “Wave-driven ISentropic Exchange” (WISE) campaign in autumn 2017 <xref ref-type="bibr" rid="bib1.bibx111 bib1.bibx90 bib1.bibx55" id="paren.20"><named-content content-type="pre">e.g.</named-content></xref>. More recently, scientific efforts have focused on the eastern edge of the ASMA and its outflow towards the northern Pacific, including the “Asian Summer Monsoon Chemical and CLimate Impact” project (ACCLIP), conducted from South Korea in July and August 2022 <xref ref-type="bibr" rid="bib1.bibx73 bib1.bibx74 bib1.bibx97" id="paren.21"/>.</p>
      <p id="d2e563">The recent aircraft campaign “Probing High Latitude Export of Air from the Asian Summer Monsoon” (PHILEAS) <xref ref-type="bibr" rid="bib1.bibx87 bib1.bibx43 bib1.bibx47" id="paren.22"/> provided the first in situ observations in the northeastern Pacific region, where mixing of air from the ASMA into the extratropical lower stratosphere occurs <xref ref-type="bibr" rid="bib1.bibx106" id="paren.23"><named-content content-type="pre">e.g.</named-content></xref>. The PHILEAS campaign was conducted from Oberpfaffenhofen, Germany, and Anchorage, Alaska, USA, during summer and early autumn 2023 and provides a valuable dual-flank perspective, sampling both the western part of the ASMA and its westward outflow (via flights from Germany to the Mediterranean region, Israel and Jordan) as well as its eastward outflow (via flights from Alaska to the northeastern Pacific region). More details are given in the campaign overview paper <xref ref-type="bibr" rid="bib1.bibx87" id="paren.24"/>.</p>
      <p id="d2e581">Here, we combine PHILEAS aircraft measurements with global three-dimensional simulations using the Chemical Lagrangian Model of the Stratosphere (CLaMS) <xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx105 bib1.bibx81" id="paren.25"><named-content content-type="post">and references therein</named-content></xref>, which includes model tracers of surface origin, as well as CLaMS back-trajectory calculations initiated along all aircraft flight tracks. With CLaMS, we identify the origin of air masses and their transport pathways and transport times to the location of the measurements. In addition, trace gas measurements and the chemical composition of particles are used to link the PHILEAS measurements to specific source regions such as marine (e.g. <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, marine-influenced particles) and continental sources (e.g. <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, nitrate-containing particles) as well as monsoon-influenced air (e.g. <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). This allows a better source attribution combining model and measurement results.</p>
      <p id="d2e632">We will show that in general the PHILEAS measurements are influenced by air masses from South Asia and the Western Pacific, with the respective contributions strongly depending on the interplay between the ASMA circulation and tropical cyclones. Further, we demonstrate that the chemical composition of monsoon-influenced air measured during PHILEAS varies strongly and depends on the geographic source region at the Earth's surface. We discuss three research flights (F02, F06, and F08) as case studies because, on the one hand, they sampled very different dynamical and geographic situations: the western part of the anticyclone (F02), typhoon-influenced air within the westward outflow of the anticyclone (F06), and the eastward outflow of the anticyclone (F08). On the other hand, all three flights were influenced by marine air uplifted by tropical cyclones in the western Pacific, which contributes to the chemical composition of the air at the edge of the ASMA and its outflow. This results in mixing of polluted air from the Asian monsoon region with marine air from tropical cyclones, particularly within eddies or filaments separated at the eastern flank of the anticyclone.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e637">Regional map showing all HALO aircraft flight tracks over the Northern Hemisphere during the PHILEAS campaign 2023 (top). A total of 18 scientific flights (F02–F20; excluding the electromagnetic compatibility and turbulence calibration flights F01 and F03, and counting the double flights F07a/b and F10a/b as one flight each) were conducted between 6 August and 27 September 2023, departing from Oberpfaffenhofen, Germany, and Anchorage, Alaska, USA. Maximum altitudes up to <inline-formula><mml:math id="M15" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14.5 <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M17" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 410 <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature) were reached. Research flights from Alaska were conducted during local daytime, which corresponds to nighttime in Coordinated Universal Time (UTC), and therefore often crossed the International Date Line, marked as 1 <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula> (Alaska local time <inline-formula><mml:math id="M20" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> UTC <inline-formula><mml:math id="M21" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 7 <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>, Germany local time <inline-formula><mml:math id="M23" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> UTC <inline-formula><mml:math id="M24" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 2 <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> considering summer time).</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f01.png"/>

      </fig>

</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Measurements during PHILEAS 2023</title>
      <p id="d2e737">As part of the PHILEAS project, a measurement campaign using the German HALO (High Altitude and Long Range) research aircraft was conducted from Oberpfaffenhofen, Germany, and Anchorage, Alaska, USA, during summer 2023 (Fig. <xref ref-type="fig" rid="F1"/>) to investigate trace gas and aerosol characteristics of air affected by the Asian summer monsoon <xref ref-type="bibr" rid="bib1.bibx87" id="paren.26"/>. Maximum flight altitudes of up to <inline-formula><mml:math id="M26" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14.5 <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>, corresponding to potential temperatures up to <inline-formula><mml:math id="M28" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 410 <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, were reached. Flights from Oberpfaffenhofen (F02–F06, F20) targeted the western part of the ASMA over the Eastern Mediterranean, Israel, and Jordan, as well as the region north of Oberpfaffenhofen up to Spitsbergen to sample the lower northern extratropical background stratosphere. Flights from Anchorage (F08–F18) focused on investigating the outflow at the eastern flank of the ASMA. Transfer flights between Oberpfaffenhofen and Anchorage (F07a, F07b, F19) can be used to infer the background state of the northern extratropical UTLS <xref ref-type="bibr" rid="bib1.bibx19" id="paren.27"><named-content content-type="pre">e.g.</named-content></xref>. The PHILEAS measurements provide a valuable data set to characterise key processes governing the transport of particles and trace gases from South Asia – one of the most polluted regions of the world – into the northern UTLS. Measurements from the following in situ instruments on board the HALO aircraft are used in our study: <list list-type="bullet"><list-item>
      <p id="d2e783">The chemical composition of aerosol particles (larger than <inline-formula><mml:math id="M30" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 100 <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>) was detected by the ERICA (ERC Instrument for the Chemical composition of Aerosols) Aerosol Mass Spectrometer (ERICA-AMS). It is based on thermal desorption with subsequent electron-impact ionisation, providing in-situ real-time mass concentrations of particulate nitrate, sulfate, and ammonium <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx42" id="paren.28"/>. The conversion of the measured ERICA-AMS raw signal into mass concentrations involves several steps <xref ref-type="bibr" rid="bib1.bibx22" id="paren.29"><named-content content-type="pre">for more details, see</named-content></xref>. The detection limit was determined for each measurement point by analysing the noise of the background measurement when a shutter in front of the ERICA-AMS ionisation region was closed (blocking ambient air and aerosol). Further, a de-trending method was applied <xref ref-type="bibr" rid="bib1.bibx4" id="paren.30"><named-content content-type="pre">for more details, see</named-content></xref>. In addition, single-particle mass spectra were obtained from the ERICA-LAMS part, which uses laser ablation and ionisation mass spectrometry. With ERICA-LAMS, particle fractions of certain particle types were analysed that are typically associated with marine-influenced air masses. Particle types were classified into three main categories based on characteristic ion marker peaks. Sodium chloride (Na/Cl) was identified by peaks at <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula>23, <inline-formula><mml:math id="M33" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35, and <inline-formula><mml:math id="M34" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>37 (<inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Na</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>). Methanesulfonic acid (MSA) was identified by a peak at <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M38" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>95 (<inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>), and trimethylamine (TMA) by peaks at <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula>58 and <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">59</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M42" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn><mml:msup><mml:mi mathvariant="normal">N</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">9</mml:mn><mml:msup><mml:mi mathvariant="normal">N</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx85 bib1.bibx34 bib1.bibx46 bib1.bibx112" id="paren.31"/>. These tracers are typically associated with marine-influenced air masses. However, TMA can also originate from anthropogenic sources such as animal husbandry and biomass burning <xref ref-type="bibr" rid="bib1.bibx28" id="paren.32"/>.</p></list-item><list-item>
      <p id="d2e972">Ozone (<inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) was measured with FAIRO, a lightweight (14.5 <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">kg</mml:mi></mml:mrow></mml:math></inline-formula>) instrument with high accuracy (2 %) and high time resolution (10 <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Hz</mml:mi></mml:mrow></mml:math></inline-formula>) developed for the HALO aircraft. FAIRO combines a dual-beam UV photometer with a UV-LED as a light source and a dry chemiluminescence detector <xref ref-type="bibr" rid="bib1.bibx114" id="paren.33"/>. In our study, ozone-poor air is used as indicator for tropospheric marine air and ozone-rich air for stratospheric air <xref ref-type="bibr" rid="bib1.bibx57 bib1.bibx59" id="paren.34"><named-content content-type="pre">e.g.</named-content></xref>.</p></list-item><list-item>
      <p id="d2e1011">Water vapour (<inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>) measurements were obtained from the Fast In situ Stratospheric Hygrometer (FISH), which is based on the Lyman-<inline-formula><mml:math id="M48" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> photofragment fluorescence technique <xref ref-type="bibr" rid="bib1.bibx116" id="paren.35"/>. The FISH inlet was mounted facing forward to measure total water which is the sum of gas-phase water and water in ice particles. A correction procedure is applied to calculate gas-phase water from FISH measurements in clouds <xref ref-type="bibr" rid="bib1.bibx68" id="paren.36"><named-content content-type="pre">for more details, see e.g.</named-content></xref>. The uncertainty for the water measurements by FISH during PHILEAS is 5 % plus an offset of 0.8 <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppmv</mml:mi></mml:mrow></mml:math></inline-formula>. The FISH instrument is calibrated every second flight and an instrument drift <inline-formula><mml:math id="M50" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 1 % is estimated based on these regular calibrations for the PHILEAS campaign, which is included in the accuracy estimate. The relative humidity with respect to ice (<inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) – a measure for potential cloud formation – is derived from <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal">gas</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> using <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M54" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 100 <inline-formula><mml:math id="M55" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal">gas</mml:mi></mml:msub></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">ice</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">ice</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the ice saturation mixing ratio as a function of temperature <xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx51" id="paren.37"/>. Here, <inline-formula><mml:math id="M58" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> is used to analyse the impact of the ASMA and of tropical cyclones <xref ref-type="bibr" rid="bib1.bibx104 bib1.bibx88" id="paren.38"><named-content content-type="pre">e.g.</named-content></xref>.</p></list-item><list-item>
      <p id="d2e1191">Dichloromethane (<inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and dibromomethane (<inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) were measured by HAGAR-V on board of HALO. HAGAR-V comprises a two-channel gas chromatograph (GC) with electron capture detection (ECD) as well as a non-dispersive infrared absorption module for the detection of <inline-formula><mml:math id="M61" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. In addition, a mass spectrometer (MS) coupled to two GC channels by a two-position valve to alternately use the detector and thereby double the time resolution of the wide range of measured species is integrated <xref ref-type="bibr" rid="bib1.bibx55" id="paren.39"/>. HAGAR-V uses two different in-flight calibration gases for a calibration measurement every fifth sample. The used gases were calibrated at the University of Frankfurt based on AGAGE-derived calibrations according to the SIO-14 (<inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and the NOAA-03 (<inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) scales. During PHILEAS the average measurement precision of <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was 1.3 % and 2.3 %, respectively. In our study, <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are used as markers for anthropogenic sources – in particular from South Asia – and for natural oceanic sources – in particular for the western Pacific –, respectively <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx1" id="paren.40"><named-content content-type="pre">e.g.</named-content></xref>.</p></list-item><list-item>
      <p id="d2e1343">Methane (<inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) measurements are used from UMAQS, the University of Mainz Airborne Quantum Cascade Laser (QCL) Spectrometer <xref ref-type="bibr" rid="bib1.bibx69 bib1.bibx52" id="paren.41"><named-content content-type="pre">e.g.</named-content></xref>. Direct absorption of an infrared QCL laser at 2989 <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">cm</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> for <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at a constant cell pressure of 40 <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Torr</mml:mi></mml:mrow></mml:math></inline-formula> is used to determine its concentration, which is converted to mixing ratio using measured cell pressure and temperature. The instrument does in-flight calibrations against secondary gas standards of compressed dried ambient air, which are compared to standards from NOAA prior and after the campaign. With this setup, a total uncertainty (1 sigma) for the 1 <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Hz</mml:mi></mml:mrow></mml:math></inline-formula> data set of 0.7 <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula> for <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> under in-flight conditions on straight legs was achieved. Here, <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios are used as an indicator of air influenced by the Asian summer monsoon <xref ref-type="bibr" rid="bib1.bibx98" id="paren.42"><named-content content-type="pre">e.g.</named-content></xref>.</p></list-item></list></p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Lagrangian transport simulations</title>
      <p id="d2e1448">The Chemical Lagrangian Model of the Stratosphere (CLaMS) <xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx65 bib1.bibx83" id="paren.43"><named-content content-type="post">and references therein</named-content></xref> was developed to study transport and chemical processes throughout the upper troposphere and stratosphere. In this study, CLaMS is driven by high-resolution ERA5 reanalysis data <xref ref-type="bibr" rid="bib1.bibx36" id="paren.44"/> provided by the European Centre for Medium-Range Weather Forecasts (ECMWF). We used ERA5 data on native model levels, including 137 vertical levels up to 0.01 <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:math></inline-formula>, with a horizontal resolution of 0.3° <inline-formula><mml:math id="M77" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3° (<inline-formula><mml:math id="M78" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 31 <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>; according to a spectral trunction of <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mtext>L</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> 639) and an hourly time resolution. The high-resolution ERA5 reanalysis has already been used for pure CLaMS trajectory calculations <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx108 bib1.bibx109 bib1.bibx16 bib1.bibx15" id="paren.45"/> and is used here for the first time for global three-dimensional CLaMS simulations (in addition to <xref ref-type="bibr" rid="bib1.bibx113" id="altparen.46"/>). Technical improvements were implemented to accelerate the reading of ERA5 reanalysis data (here used in netCDF format). Furthermore, the storage of the ERA5 reanalysis data was changed from distributed memory to shared memory using the Message Passing Interface (MPI).</p>
      <p id="d2e1508">In CLaMS, the diabatic approach is used to calculate vertical velocities at these atmospheric altitudes. Specifically, potential temperature is used as the vertical coordinate at pressures below approximately 300 <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:math></inline-formula>, i.e. in the upper troposphere and stratosphere. At higher pressures (for <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>p</mml:mi><mml:mtext>surface</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M83" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.3), a pressure-based, orography-following hybrid coordinate (expressed in units of <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) is applied <xref ref-type="bibr" rid="bib1.bibx83" id="paren.47"/>. At lower pressure levels, vertical velocity is determined solely by the total diabatic heating rate from ERA5 reanalysis <xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx81" id="paren.48"/>. Total diabatic heating rates include clear-sky radiative heating, cloud radiation, latent heat release, as well as turbulent and diffusive heat transport for the upper troposphere and stratosphere.</p>
      <p id="d2e1556">The upward transport and convection in CLaMS (in both trajectory calculations and three-dimensional simulations) depend on the underlying reanalysis data <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx16 bib1.bibx109" id="paren.49"/>. For the use of high-resolution ERA5 data, no additional parametrisation for convection is applied in our simulations. Although an additional parametrisation for convection in CLaMS has been developed <xref ref-type="bibr" rid="bib1.bibx49 bib1.bibx50" id="paren.50"/>, it is in its present form designed for use with down-sampled ERA5 data (with a 1° <inline-formula><mml:math id="M85" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1° horizontal resolution and a 6-hourly temporal resolution). This approach is a computing-time-saving alternative that is well suited for global, multi-annual CLaMS simulations. The representation of convection and tropical cyclones (e.g., typhoons) in ERA5 has substantially improved compared to its predecessor, ERA-Interim <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx58 bib1.bibx62 bib1.bibx16 bib1.bibx109" id="paren.51"><named-content content-type="pre">e.g.,</named-content></xref>, and represents the best data currently provided by ECMWF. However, unresolved small-scale convection in ERA5 represents a potential limitation of our simulations. Furthermore, vertical transport in the lower stratosphere in ERA5 has been found to be somewhat too slow <xref ref-type="bibr" rid="bib1.bibx81 bib1.bibx109" id="paren.52"/>, which may affect air masses transported upward into the stratosphere and subsequently advected isentropically to higher latitudes.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1583">Geographical map showing the global distribution of surface–origin tracers implemented in CLaMS (top). The South Asia tracer is defined as the sum of several surface–origin tracers in the Asian summer monsoon region (TIB <inline-formula><mml:math id="M86" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> IND <inline-formula><mml:math id="M87" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NIN <inline-formula><mml:math id="M88" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> ECH <inline-formula><mml:math id="M89" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> BoB <inline-formula><mml:math id="M90" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NIO <inline-formula><mml:math id="M91" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Neast <inline-formula><mml:math id="M92" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NAF), and serves as a good proxy for the ASMA (bottom, grey background). The Western Pacific tracer (SEA <inline-formula><mml:math id="M93" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Wpool <inline-formula><mml:math id="M94" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TWP <inline-formula><mml:math id="M95" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NWP) is a good indicator of air uplifted into the UTLS by tropical cyclones in the western Pacific and, more generally, of air masses with marine origin (bottom, yellow background).</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f02.png"/>

      </fig>

<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Lagrangian three-dimensional simulations including surface–origin tracer</title>
      <p id="d2e1670">Three-dimensional CLaMS simulations that include irreversible mixing (applied here every 24 <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx48" id="paren.53"><named-content content-type="pre">e.g.</named-content></xref> provide a very good representation of observed tracer gradients in the UTLS, particularly near the tropopause and at the edge of the ASMA <xref ref-type="bibr" rid="bib1.bibx105 bib1.bibx107 bib1.bibx80 bib1.bibx82" id="paren.54"><named-content content-type="pre">e.g.</named-content></xref>. Here, we use CLaMS simulations with 32 different regional model tracers of surface origin (hereafter referred to as “surface–origin tracers”) that together cover the entire Earth's surface (Fig. <xref ref-type="fig" rid="F2"/>). The simulation starts on 1 May 2023, during the pre-monsoon period, and covers the entire Asian summer monsoon season of 2023.</p>
      <p id="d2e1694">These surface–origin tracers are released into the model boundary layer (approximately 2–3 <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> above the surface, accounting for orography) every 24 <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> and are subsequently transported – by advection and mixing – into the free atmosphere over the course of the simulation. Surface–origin tracers serve as a valuable diagnostic tool for identifying the surface source regions of air masses. In addition, a surface–origin tracer representing the global model boundary layer (MBL), corresponding to the sum of all regional surface–origin tracers shown in Fig. <xref ref-type="fig" rid="F2"/>, is included. The global MBL tracer provides an estimate of the age of the air: low MBL fractions indicate a large fraction of aged air masses (i.e. air older than 1 May 2023), such as stratospheric background air.</p>
      <p id="d2e1715">Previous model studies using CLaMS surface–origin tracers (albeit with a slightly different definition of tracer regions) indicate that young air masses originating from South Asia are largely confined within the ASMA. In contrast, air masses from adjacent regions – particularly from Southeast Asia and the western Pacific – tend to be located near the edge of the ASMA <xref ref-type="bibr" rid="bib1.bibx105 bib1.bibx107 bib1.bibx7" id="paren.55"><named-content content-type="pre">e.g.</named-content></xref>. Our simulations show that the following surface–origin tracers contribute in general to the composition of the ASMA: Northern Indian Subcontinent (NIN), Indian Subcontinent (IND), Tibetan Plateau (TIB), Eastern China (ECH), Bay of Bengal (BoB), Northern Indian Ocean (NIO), as well as the Near East (Neast) and Northern Africa (NAF), with the latter two contributing only in small fractions to the composition of the ASMA. In the following, we use the sum of these surface–origin tracers as a marker for air originating from the ASMA and refer to it as the South Asia tracer (although some of these regions are not part of South Asia in the classical geographical sense, the term “South Asia” is used here in an extended sense).</p>
      <p id="d2e1723">Air masses from the western Pacific, that is the sum of the surface–origin tracers of Southeast Asia (SEA), Warm Pool (Wpool), Tropical Western Pacific (TWP) and Northern Western Pacific (NWP) (Fig. <xref ref-type="fig" rid="F2"/>) also play a role in the chemical composition of the ASMA <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx60 bib1.bibx33 bib1.bibx108 bib1.bibx16" id="paren.56"><named-content content-type="pre">e.g.</named-content></xref> and are frequently observed at its edge <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx107" id="paren.57"><named-content content-type="pre">e.g.</named-content></xref>, partly due to uplift associated with tropical cyclones.</p>
      <p id="d2e1739">In general, the Asian summer monsoon is divided into the Indian (South Asian), East Asian, and Western North Pacific summer monsoon regions <xref ref-type="bibr" rid="bib1.bibx110" id="paren.58"/>. The role of the East Asian monsoon on the chemical composition of the ASMA was studied based on measurements taken during the ACCLIP campaign from South Korea in July and August 2022 <xref ref-type="bibr" rid="bib1.bibx97 bib1.bibx73 bib1.bibx74" id="paren.59"><named-content content-type="pre">e.g.</named-content></xref>. Compared to that, the StratoClim measurements sampled the core region of the Indian summer monsoon <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx1 bib1.bibx109" id="paren.60"><named-content content-type="pre">e.g.</named-content></xref>. The CLaMS regional surface-origin tracers can be used to link the PHILEAS measurements to sub-regions reflecting the influence of the Indian (South Asian) (surface-origin tracers: IND, NIN) and the East Asian (surface-origin tracer: ECH) as well as to the western North Pacific (surface-origin tracer: NWP) summer monsoon.</p>
      <p id="d2e1755">These surface–origin tracers – especially the South Asia tracer (excluding contributions from the Near East and Northern Africa) – were used for flight planning during the PHILEAS campaign <xref ref-type="bibr" rid="bib1.bibx87" id="paren.61"/> to identify the ASMA, as well as filaments and anticyclonic structures (eddies) detached from it, where simulations with ECMWF forecast and analysis products were used for flight planning. We demonstrate that the South Asia tracer serves as a reliable proxy for polluted air originating from the Asian summer monsoon region. Additionally, the Western Pacific tracer is a useful indicator of air uplifted into the UTLS by tropical cyclones in the western Pacific, and more generally, it serves as a marker for air masses of marine origin.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Back-trajectory calculations and dehydration analysis</title>
      <p id="d2e1769">CLaMS trajectory calculations consider only advective transport, neglecting mixing processes entirely. However, back-trajectory calculations are well suited to analyse the detailed transport pathway, transport time, and surface origin of air parcels and therefore provide added value compared to three-dimensional CLaMS simulations including irreversible mixing <xref ref-type="bibr" rid="bib1.bibx107 bib1.bibx55 bib1.bibx108 bib1.bibx109" id="paren.62"><named-content content-type="pre">as has been shown in previous publications, e.g.</named-content></xref>. CLaMS diabatic back-trajectories were initiated along the entire flight paths (every 1 <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">s</mml:mi></mml:mrow></mml:math></inline-formula>) of all 18 research flights conducted during the PHILEAS campaign. On average, the research flights lasted 6 to 8 <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>, resulting in approximately 23 000 to 33 000 trajectories calculated per flight, depending on flight duration. Trajectories are considered to terminate in the model boundary layer when they first descend to below approximately 2–3 <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> above the Earth's surface, accounting for orography (i.e., when the vertical hybrid pressure-potential-temperature coordinate, <inline-formula><mml:math id="M102" display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula>, satisfies <inline-formula><mml:math id="M103" display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M104" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 120 <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx108 bib1.bibx109" id="paren.63"><named-content content-type="pre">see details in, e.g.,</named-content></xref>. The transport time of each air parcel is defined as the time difference between the start and end points of its back-trajectory in the model boundary layer. Trajectories not ending in the model boundary layer were calculated back to 1 May 2023; representing older air found in the UTLS region. Thus, the length of these trajectories span the same time period as the global three-dimensional CLaMS simulations that include surface–origin tracers (i.e., a quasi-forward calculation including irreversible mixing) and cover both the pre-monsoon and monsoon period. Along the CLaMS back-trajectories as well as along the flight tracks of all scientific PHILEAS flights the local tropopause heights (first and second) were calculated from ERA5 reanalysis data based on the WMO definition according to <xref ref-type="bibr" rid="bib1.bibx37" id="text.64"/>.</p>
      <p id="d2e1839">In addition, the temperature evolution along the back-trajectories is used to check if dehydration can possibly occur along the trajectories. That is in particular important at the convective outflow of tropical cyclones <xref ref-type="bibr" rid="bib1.bibx58" id="paren.65"><named-content content-type="pre">e.g.</named-content></xref>, but also tropical convection can impact hydration and dehydration in the UTLS <xref ref-type="bibr" rid="bib1.bibx93 bib1.bibx99" id="paren.66"><named-content content-type="pre">e.g.</named-content></xref>. To estimate dehydration, the minimum of the water vapour saturation mixing ratio with respect to ice (<inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">ice</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) along the back-trajectories is calculated based on ERA5 temperatures and pressures. Dehydration is only relevant in a first approximation for air masses that are transported from the troposphere into the lower stratosphere. Therefore, tropopause heights along the trajectories are used to check whether the trajectories originate in the troposphere before reaching <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">ice</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and remain in the stratosphere afterwards.</p>
      <p id="d2e1906">Trajectories originating in the stratosphere and being transported into the troposphere, but with only a very short residence time just below the tropopause, are filtered out. Air parcels along the flight track are marked as dehydrated when the following criteria are fulfilled: trajectory (at least 80 % of the time) is below the tropopause before reaching <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">ice</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and above afterwards, in addition FISH <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> measurements (total water) should be greater equal <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mi mathvariant="normal">sat</mml:mi><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">ice</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and to exclude measurements inside of clouds, FISH <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has to be lower than 90 %. We determined a value of 80 % as threshold because the time periods of dehydration using thresholds of 70 %, 80 %, and 90 % along the flight tracks remain nearly the same.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Air mass origin and impact of tropical cyclones</title>
      <p id="d2e2003">In this study, we focus on the UTLS, and therefore only consider back-trajectories of aircraft measurements taken above 340 <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature. To determine the origin of the air masses sampled during the PHILEAS aircraft campaign, it is crucial to identify the location where the back-trajectories intersect the model boundary layer. Figure <xref ref-type="fig" rid="F3"/> (top) shows the frequency distribution of locations where air parcels were traced back to the model boundary layer for all CLaMS back-trajectories initiated above 340 <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> across all 18 research flights (F02–F20).</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e2026">Frequency distribution of locations where air parcels along the flight tracks of all PHILEAS research flights (F02–F20) were traced back to the model boundary layer using CLaMS back-trajectory calculations. Frequency distributions are shown for measurements above 340 <inline-formula><mml:math id="M114" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> in a global view (top) as well as zoomed in on South Asia and the western Pacific (middle). To highlight sources in Asia reaching altitudes of the ASMA an additional frequency distribution for measurements between 360 and 420 <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> is shown (bottom).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f03.png"/>

        </fig>

      <p id="d2e2051">Above 340 <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, most back-trajectories originate from two main regions (Fig. <xref ref-type="fig" rid="F3"/>, middle): (1) South Asia – particularly the Indian Subcontinent, the Arabian Sea, the Bay of Bengal, the Tibetan Plateau, China, and Mainland Southeast Asia – and (2) the Western Pacific, including the eastern coast of China and the regions around Taiwan and the Philippines. The frequency distribution of locations where air parcels were traced back to the model boundary layer motivated our definition of the South Asia tracer and Western Pacific tracer introduced in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>.</p>
      <p id="d2e2067">When focusing on measurements above the maximum level of convective outflow (i.e. 360 <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) up to the maximum flight altitude (420 <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>), corresponding to the vertical extent of the ASMA <xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx29" id="paren.67"/> (Fig. <xref ref-type="fig" rid="F3"/>, bottom), distinct source regions emerge. The highest frequencies of air mass origins are found over the Arabian Sea, the Bay of Bengal, the northeastern part of the Indian subcontinent, and the western Pacific.</p>
      <p id="d2e2091">Particularly in the western Pacific, frequent occurrence of strong tropical cyclones is found impacting the PHILEAS measurements. Figure <xref ref-type="fig" rid="F4"/> shows the frequency distribution of locations where CLaMS back-trajectories are traced back to the model boundary layer, zoomed to the western Pacific and overlaid with all cyclone tracks that occurred in the western Pacific between 6 June and 8 September 2023 and may have impacted the PHILEAS measurements (provided by the Japan Meteorological Agency; (<uri>https://www.jma.go.jp/jma/jma-eng/jma-center/rsmc-hp-pub-eg/besttrack.html</uri>, last access: 9 October 2024). The cyclone category is indicated along each cyclone track: tropical depression, tropical storm, severe tropical storm, typhoon and extra-tropical cyclone.</p>

      <fig id="F4"><label>Figure 4</label><caption><p id="d2e2101">Frequency distribution of locations where air parcels were traced back to the model boundary layer using CLaMS back-trajectory calculations (for aircraft measurements taken above potential temperature levels of 360 <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>), overlaid with cyclone tracks in the western Pacific. Cyclone categories are indicated as follows: Tropical Depression (TD), Tropical Storm (TS), Severe Tropical Storm (STS), Typhoon (TY), Extra-tropical Cyclone (ETC). The following cyclones are included: (A) Guchol (6–16 June 2023), (B) Talim (13–18 July 2023), (C) Doksuri (20–30 July 2023), (D) Khanun (26 July–11 August 2023), (E) Lan (7–18 August 2023), (F) Dora (12–22 August 2023), (G) Saola (22 August–3 September 2023), (H) Damrey (23–30 August 2023), (I) Haikui (27 August–6 September 2023) (J) Kirogi (29 August–6 September 2023) and (K) Yun-Yeung (4–8 September 2023). The end of each cyclone track is marked by the corresponding capital letter.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f04.png"/>

        </fig>

      <p id="d2e2118">A strong local coincidence between the frequency distribution of air mass origins and cyclone tracks is found for tropical cyclones (B) Talim, (C) Doksuri, (G) Saola and (I) Haikui north of the Philippines; the latter three were all categorised as a typhoon in this region (Fig. <xref ref-type="fig" rid="F4"/>). Furthermore, a strong spatial overlap is observed for tropical cyclones (D) Khanun during its transition from a typhoon to a severe tropical storm off the eastern coast of China, and later during its landfall in the region of Japan, Korea, and the Chinese coast. For each PHILEAS flight (F02–F20), a local coincidence is found between the frequency distribution of air mass origins (for measurements above 360 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature) at least with one of the tropical cyclones shown in Fig. <xref ref-type="fig" rid="F4"/>. Further details are discussed for selected PHILEAS flights in Sect. <xref ref-type="sec" rid="Ch1.S4.SS3"/>.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title><inline-formula><mml:math id="M121" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations indicating pollution sources in South Asia</title>
      <p id="d2e2170">Tracer–tracer relations of different measured trace gases are commonly used to diagnose mixing between air masses of different origin, such as between tropospheric and stratospheric air masses <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx35 bib1.bibx72" id="paren.68"><named-content content-type="pre">e.g.</named-content></xref>. In this study, tracer–tracer relations, namely <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations, based on in situ measurements are combined with surface–origin tracers from three–dimensional global CLaMS simulations <xref ref-type="bibr" rid="bib1.bibx103 bib1.bibx55" id="paren.69"><named-content content-type="pre">e.g.</named-content></xref>. The CLaMS surface–origin tracers are interpolated in space and time along the flight paths of all PHILEAS research flights (F02–F20). Only flight segments above 340 <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> are considered here in tracer–tracer relations to remove the impact of the lower troposphere. Using <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations in combination with CLaMS surface-origin tracers, the variability of the chemical composition of monsoon-influenced air depending on the air mass origin – thus the variability of <inline-formula><mml:math id="M128" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources in Asia – will be analysed. Further, we will demonstrate that air masses originating from South Asia exhibit a different chemical composition compared to those from the western Pacific.</p>
      <p id="d2e2262">South Asia is a substantial source of methane (<inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) – an important greenhouse gas, primarily due to elevated emissions from rice paddies <xref ref-type="bibr" rid="bib1.bibx76 bib1.bibx94 bib1.bibx98" id="paren.70"><named-content content-type="pre">e.g.</named-content></xref>. These emissions lead to a statistically significant increase in <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the ASMA and subsequently in the northern extratropical UTLS during summer and autumn <xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx88 bib1.bibx115" id="paren.71"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d2e2297">The PHILEAS campaign overview paper by <xref ref-type="bibr" rid="bib1.bibx87" id="text.72"/> proposed an identification of monsoon-influence based on <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios exceeding a threshold of 1850 <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula> (referring to <xref ref-type="bibr" rid="bib1.bibx88" id="altparen.73"/>). In our study, no specific <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> threshold is applied, because in the outflow of the ASMA, mixing of monsoon air with surrounding air masses occurs, reducing the enhanced <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios associated with the ASMA. Because only flight segments above 340 <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> are considered here, enhanced <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measured in the lower troposphere over Europe and North America and in particular measured during take-off and landing of the research aircraft are not taken into account in our analysis.</p>
      <p id="d2e2368">Dichloromethane (<inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), a chlorine-containing very short-lived halogenated substance (VSLS), originates mainly from anthropogenic sources – in particular from China and India <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx92" id="paren.74"/>. An average annual increase of 13 % in emissions of the industrially produced <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was reported for the time period between 2011 and 2019 – primarily from eastern China <xref ref-type="bibr" rid="bib1.bibx2" id="paren.75"/>. Recent studies highlight the increasing influence of chlorine-containing VSLS such as <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that is not regulated by the Montreal Protocol on the stratospheric chlorine budget and therefore their possible role in ozone depletion <xref ref-type="bibr" rid="bib1.bibx41 bib1.bibx13 bib1.bibx18" id="paren.76"><named-content content-type="pre">e.g.</named-content></xref>. The coincidence of strong <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources in Asia, in particular in eastern China, and the Asian summer monsoon that transport surface emissions from Asia very fast into the northern lower stratosphere, makes <inline-formula><mml:math id="M141" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements in the ASMA and in its outflow very important. Previous aircraft measurements already confirm that <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is enhanced over Asia. Over the Indian subcontinent <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios up to <inline-formula><mml:math id="M144" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 140 <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> were measured during the StratoClim aircraft campaign in 2017, a factor of more than two more than reported previously at the tropical tropopause (<inline-formula><mml:math id="M146" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx1" id="paren.77"/>. During the ACCLIP aircraft campaign in 2022 record-breaking mixing ratios up to <inline-formula><mml:math id="M148" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 600 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> were measured at tropopause altitudes at the eastern edge of the ASMA (over Korea and Japan) <xref ref-type="bibr" rid="bib1.bibx73" id="paren.78"/>. Export of air from the ASMA to the northern extratropical UTLS leads to enhanced <inline-formula><mml:math id="M151" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios over the Atlantic Ocean and Northern Europe <xref ref-type="bibr" rid="bib1.bibx55" id="paren.79"/> as well as in the Arctic <xref ref-type="bibr" rid="bib1.bibx54" id="paren.80"/>.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e2588"><inline-formula><mml:math id="M152" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M153" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations for all scientific PHILEAS flights F02–F20, colour-coded by entire <bold>(a)</bold> model boundary layer (MBL) and <bold>(b)</bold> potential temperature for measurements above 340 <inline-formula><mml:math id="M154" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>. The MBL tracer serves as an indicator for young air (younger than 1 May 2023). The <bold>(c)</bold> South Asia (TIB <inline-formula><mml:math id="M155" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> IND <inline-formula><mml:math id="M156" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NIN <inline-formula><mml:math id="M157" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> ECH <inline-formula><mml:math id="M158" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> BoB <inline-formula><mml:math id="M159" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NIO <inline-formula><mml:math id="M160" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Neast <inline-formula><mml:math id="M161" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NAF) and <bold>(d)</bold> Western Pacific (SEA <inline-formula><mml:math id="M162" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Wpool <inline-formula><mml:math id="M163" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TWP <inline-formula><mml:math id="M164" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NWP) tracers indicate different origins of air in different parts of the <inline-formula><mml:math id="M165" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M166" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relation.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f05.png"/>

        </fig>

      <p id="d2e2743">In this study, we use <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M168" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations as an indicator of monsoon-influenced air. The variability of <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over Asia helps to identify local source regions within the continent. The <inline-formula><mml:math id="M170" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M171" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relation over all scientific PHILEAS flights (F02–F20) is shown in Figure <xref ref-type="fig" rid="F5"/>. It demonstrates that the <inline-formula><mml:math id="M172" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M173" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relation is split into three distinct branches (clearly distinguishable by visual inspection) with varying <inline-formula><mml:math id="M174" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios at high <inline-formula><mml:math id="M175" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels (greater than 2000 <inline-formula><mml:math id="M176" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>): up to 300 <inline-formula><mml:math id="M177" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M178" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (branch 1 in Fig. <xref ref-type="fig" rid="F5"/>), around 150 <inline-formula><mml:math id="M179" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> (branch 2 in Fig. <xref ref-type="fig" rid="F5"/>), and nearly 100 <inline-formula><mml:math id="M180" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> (branch 3 in Fig. <xref ref-type="fig" rid="F5"/>). All three branches are associated with contributions of the global model boundary layer (MBL; released since 1 May 2023) tracer exceeding 60 % (Fig. <xref ref-type="fig" rid="F5"/>a), indicating young air masses and reflecting the short atmospheric lifetime of <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M182" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 6 months). Branches 1 and 2 correspond to measurements around 350 <inline-formula><mml:math id="M183" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature, while branch 3 was observed at higher altitudes, around 370 <inline-formula><mml:math id="M184" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F5"/>b). Thus only branch 3 constitutes measurements at altitudes of the ASMA.</p>
      <p id="d2e2973">Analysis of the South Asia and Western Pacific surface-origin tracers in Fig. <xref ref-type="fig" rid="F5"/>c–d reveals that branches 1 and 2 have intermediate contributions from South Asia (reddish colours; fractions greater than 45 % ) mixed with lower fractions from the Western Pacific (<inline-formula><mml:math id="M185" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 25 %–35 %), except in the part of the relation in Fig. <xref ref-type="fig" rid="F5"/>d denoted by 1b, where also substantial fractions from the Western Pacific (<inline-formula><mml:math id="M186" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 40 %–50 %) were found. The surface-origin tracers for more specific regions, which contribute to the South Asia and Western Pacific tracer (Appendix <xref ref-type="sec" rid="App1.Ch1.S1.SS1"/>; Fig. <xref ref-type="fig" rid="FA1"/>), show that branch 1 is related to air mass origin in eastern China (ECH) and the Northern Western Pacific (NWP; in particular in region 1b) and branch 2 is related to eastern China (ECH), Northern Indian Subcontinent (NIN) and the Tropical Western Pacific (TWP). Thus our findings confirm that enhanced <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the UTLS can be attributed to sources in China <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx2 bib1.bibx73 bib1.bibx43" id="paren.81"/>.</p>
      <p id="d2e3018">In contrast, in branch 3 the fractions from South Asia are up to 70 %, with minor contributions from the Western Pacific (tracer lower than 10 %). Here the Indian Subcontinent (IND) and Bay of Bengal (BoB) are the main surface-origin tracers that contribute (Appendix <xref ref-type="sec" rid="App1.Ch1.S1.SS1"/>; Fig. <xref ref-type="fig" rid="FA1"/>). <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios in a similar range (up to about 140 <inline-formula><mml:math id="M189" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) were also measured during the StratoClim aircraft campaign over the Indian subcontinent, near the tropopause <xref ref-type="bibr" rid="bib1.bibx1" id="paren.82"/>.</p>
      <p id="d2e3053">Large fractions of the Western Pacific tracer (up to 70 %) are found for <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios of <inline-formula><mml:math id="M191" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1950 <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios of <inline-formula><mml:math id="M194" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50–60 <inline-formula><mml:math id="M195" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> denoted as region 4 in Fig. <xref ref-type="fig" rid="F5"/>d. These low <inline-formula><mml:math id="M196" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios correspond to the northern hemispheric background from ground-based <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements during summer performed outside of Asia (<uri>https://www-air.larc.nasa.gov/missions/agage/static/figures/monthly/pdf/CH2Cl2_mm.pdf</uri>, last access: 5 May 2026; <uri>https://gml.noaa.gov/hats/gases/CH2Cl2.html</uri>, last access: 27 January 2026). Thus, air masses in region 4 are most likely marine air from the western Pacific, because both <inline-formula><mml:math id="M198" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M199" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> have only minor marine sources, and a large fraction – up to 70 % – of the Western Pacific tracer is found.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3184">Research flight F02 on 6 August 2023 conducted from Oberpfaffenhofen, Germany, to the Mediterranean area intruding into the western part of the ASMA (South Asia surface–origin tracer at 370 <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 12:00 UTC, left). The entire anticyclone (top) as well as a zoom to the flight area (bottom) are shown. A belt of air from the western Pacific is found around the outer edge of the ASMA (Western Pacific surface–origin tracer at 370 <inline-formula><mml:math id="M201" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 12:00 UTC, right). The surface–origin tracer distributions are based on a CLaMS simulation driven by ERA5. To align the flight tracks with the synoptic CLaMS model output at 12:00 UTC, the actual flight positions (white line) were extrapolated to 12:00 UTC positions using forward and backward CLaMS trajectories to calculate the synoptic HALO flight track (black line). To indicate the edge of the ASMA (indigo line), the boundary of the ASMA is calculated using the Montgomery streamfunction. An optimised Montgomery streamfunction value gives the ASMA boundary (MSF <inline-formula><mml:math id="M202" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 357.3 <inline-formula><mml:math id="M203" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>3</sup> <inline-formula><mml:math id="M205" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) for 6 August 2023 at 12:00 UTC and 370 <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> using ERA5 reanalysis data based on the method by <xref ref-type="bibr" rid="bib1.bibx44" id="text.83"/>. The climatological isentropic transport barrier (PV <inline-formula><mml:math id="M207" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.4 <inline-formula><mml:math id="M208" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">PVU</mml:mi></mml:mrow></mml:math></inline-formula>) derived by <xref ref-type="bibr" rid="bib1.bibx53" id="text.84"/> for the Northern Hemisphere at 370 <inline-formula><mml:math id="M209" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> during summer indicates the barrier between the tropical tropopause layer and the extra-tropical lower stratosphere (olive line). Further, horizontal winds from ERA5 are indicated by white arrows. Time intervals 1–3 shown in Fig. <xref ref-type="fig" rid="F8"/> are marked in magenta.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f06.png"/>

        </fig>

      <p id="d2e3293">To demonstrate that other parts of the world, besides South Asia and the Western Pacific, have only a minor impact on the PHILEAS measurements, the <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M211" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relation is shown for surface–origin tracers representing the northern background (only relevant for local <inline-formula><mml:math id="M212" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions observed during take-off and landing of the HALO aircraft) that contributes with a fraction of <inline-formula><mml:math id="M213" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 % and the residual surface (mainly parts of the Southern Hemisphere) that has a negligibly impact (<inline-formula><mml:math id="M214" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 0 %) on the PHILEAS flights in Appendix <xref ref-type="sec" rid="App1.Ch1.S1.SS1"/> (Fig. <xref ref-type="fig" rid="FA2"/>).</p>
      <p id="d2e3353">In the following, we discuss three research flights (F02, F06, and F08) as case studies, focusing on potential temperature levels of the ASMA (greater than 360 <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>), to analyse the impact of the origin of the air masses on the chemical composition of the ASMA and its outflow, as well as the influence of tropical cyclones at these potential temperature levels. The presented analysis of the <inline-formula><mml:math id="M216" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M217" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relationship for all PHILEAS flights helps to place the measured <inline-formula><mml:math id="M218" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M219" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios of the selected case studies within the variability observed across all PHILEAS flights.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e3420">Surface–origin tracers for the model boundary layer, South Asia and the Western Pacific interpolated in space and time along the flight track of research flight F02 on 6 August 2023. In addition, individual surface-origin tracers with fractions greater than 10 % are shown as a stacked plot (TIB, IND, NIN, BoB, NIO, and SEA).</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Case studies of selected flights</title>
<sec id="Ch1.S4.SS3.SSS1">
  <label>4.3.1</label><title>Research flight F02 (6 August 2023): The western part of the anticyclone</title>
      <p id="d2e3444">Research flight F02 on 6 August 2023 was conducted from Oberpfaffenhofen, Germany, to the Mediterranean area and intruded into the western part of the ASMA located over the eastern Mediterranean region (Fig. <xref ref-type="fig" rid="F6"/>, left). To indicate the edge of the ASMA, its horizontal boundary is calculated on selected isentropes using an optimised Montgomery streamfunction value based on the recently published method by <xref ref-type="bibr" rid="bib1.bibx44" id="text.85"/>. An advantage of this method is that it can be applied at any time scale, allowing the selection of individual days or specific hours. In Fig. <xref ref-type="fig" rid="F6"/>, the optimised Montgomery streamfunction value is calculated on 370 <inline-formula><mml:math id="M220" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature for 6 August 2026 at noon using ERA5 reanalysis data. A belt of air from the western Pacific is found at the outer edge of the ASMA that was crossed by the HALO aircraft twice (Fig. <xref ref-type="fig" rid="F6"/>, right). Further, at the turning point of the flight track above the Arabian Peninsula, a filament of air from the western Pacific was reached caused by a meandering subtropical jet.</p>
      <p id="d2e3464">Air masses measured in the western part of the ASMA and in its westward outflow (air outside the ASMA) mainly originate from the Indian subcontinent (IND, NIN, BoB, TIB, NIO); the main contributions from the western Pacific are from Southeast Asia (SEA) (Fig. <xref ref-type="fig" rid="F7"/>). Between approximately 09:15 and 13:30 UTC,  the ASMA (Fig. <xref ref-type="fig" rid="F6"/>, bottom panel, interval 2) and the belt of air from the western Pacific (Fig. <xref ref-type="fig" rid="F6"/>, bottom panel, intervals 1 and 3), were crossed by the research plane. Qualitatively Fig. <xref ref-type="fig" rid="F7"/> shows that within this flight segment (intervals 1–3) the South Asia tracer and the Western Pacific tracer along the flight track exhibit opposite variations indicating that here the two different air masses are separated and not well mixed. This separation is caused by the transport barrier at the edge of the ASMA. Before and after this flight segment (intervals 1–3), fractions of the South Asia tracer are in general small <inline-formula><mml:math id="M221" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 % (except at 13:50 UTC where a small monsoon-influenced filament (outflow) was crossed).</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e3484">Surface–origin tracers interpolated along the flight track of research flight F02 on 6 August 2023, potential temperature along the flight track, potential temperature at the tropopause as well as measurements of different chemical trace gases such as <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M224" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M225" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, relative humidity with respect to ice <inline-formula><mml:math id="M227" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as well as nitrate mass concentration and TMA fractions from aerosol particles. Only regional surface–origin tracers with fractions greater than 20 % are shown for better visibility. In intervals 1 and 3 (see Fig. <xref ref-type="fig" rid="F6"/>) enhanced fraction of the Western Pacific and in interval 2 of the South Asia tracer are found. Note that <inline-formula><mml:math id="M228" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M229" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and nitrate are smoothed over 10 <inline-formula><mml:math id="M230" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">s</mml:mi></mml:mrow></mml:math></inline-formula>.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f08.png"/>

          </fig>

      <p id="d2e3607">Main parts of research flight F02 in particular intervals 1–3 are below the local tropopause (Fig. <xref ref-type="fig" rid="F8"/>), thus characterise tropospheric air masses. In contrast to the end of the flight outside the ASMA over Europe, stratospheric air was measured. The time series of the surface–origin tracers interpolated along the flight track of research flight F02 are qualitatively compared with measurements of different chemical trace gases namely <inline-formula><mml:math id="M231" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M232" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M233" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M235" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> including <inline-formula><mml:math id="M236" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as well as particulate nitrate and the number fraction of particulate TMA (Fig. <xref ref-type="fig" rid="F8"/>). The number fraction refers to the number of particles containing TMA divided by the total number of particles measured within the 10 <inline-formula><mml:math id="M237" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:math></inline-formula> time interval.</p>
      <p id="d2e3701">Particulate nitrate is used as indicator for air from the Asian tropopause aerosol layer (ATAL) <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx4 bib1.bibx47" id="paren.86"><named-content content-type="pre">e.g.</named-content></xref>; mass concentrations of up to 0.8 <inline-formula><mml:math id="M238" 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> were found in time interval 2. During the StratoClim aircraft campaign over the Indian subcontinent in summer 2017, nitrate mass concentrations of up to 1 <inline-formula><mml:math id="M239" 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> were measured within the ASMA and the ATAL <xref ref-type="bibr" rid="bib1.bibx4" id="paren.87"/>. Further, PHILEAS measurements show that outside the ASMA (and the ATAL), nitrate mass concentrations in UTLS aerosol are generally very low, often close to zero. Further, in time interval 2 enhanced fractions of the South Asia tracer (up to 70 %) are found simultaneously with enhanced mixing ratios of pollutants and greenhouse gases such as <inline-formula><mml:math id="M240" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (up to 120 <inline-formula><mml:math id="M241" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M242" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M243" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 2000 <inline-formula><mml:math id="M244" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>) and enhanced fraction of TMA-containing particles (up to 6 %).</p>
      <p id="d2e3801">Interval 2 (Fig. <xref ref-type="fig" rid="F8"/>) is flanked by interval 1 and 3 – crossing the belt of air from the western Pacific at the edge of the ASMA – here fractions of the Western Pacific tracer of up to 35 % are simulated. Within these flight segments mixing ratios of pollutants and greenhouse gases such as <inline-formula><mml:math id="M245" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M246" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as well as mass concentrations of particulate nitrate are low or are decreasing (e.g. in interval 3). Marine sources are indicated by low ozone mixing ratios (<inline-formula><mml:math id="M247" display="inline"><mml:mo lspace="0mm">≲</mml:mo></mml:math></inline-formula> 100 <inline-formula><mml:math id="M248" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>) or enhanced dibromomethane <inline-formula><mml:math id="M249" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M250" display="inline"><mml:mo lspace="0mm">≳</mml:mo></mml:math></inline-formula> 0.7–0.8 <inline-formula><mml:math id="M251" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx1" id="paren.88"/> that has mostly natural oceanic sources in contrast to chlorinated VSLS such as <inline-formula><mml:math id="M252" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that has mainly anthropogenic sources. In all three intervals 1–3, ozone mixing ratios are low and <inline-formula><mml:math id="M253" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios are enhanced indicating marine sources, however there is no strong difference between interval 2 compared to interval 1 and 3.</p>
      <p id="d2e3915">An increased fraction of TMA-containing particles during intervals 2 and 3 (Fig. <xref ref-type="fig" rid="F8"/>, bottom) was observed. Gaseous TMA originates from both natural and anthropogenic sources, including emissions from marine biota, biomass burning, and animal husbandry <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx23 bib1.bibx28" id="paren.89"/>. Once released into the atmosphere, TMA can participate in aerosol chemistry through gas-to-particle conversion and dissolution in cloud droplets. ERICA-LAMS single-particle spectra further indicate that TMA was internally mixed with nitrate, ammonium, and sulfate (see Fig. <xref ref-type="fig" rid="FB1"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/>). These observations suggest, first, that TMA may contribute to particle formation and growth within the ASMA, alongside ammonium, nitrate, and sulfate. Second, they point to South Asia and the Western Pacific as potential source regions, and/or to shared emission sources – such as agricultural activities in northern India – for TMA and other compounds like ammonia.</p>
      <p id="d2e3927">In general, the Asian summer monsoon is a source of water vapour in the UTLS caused by the relatively high cold point tropopause in the ASMA <xref ref-type="bibr" rid="bib1.bibx89 bib1.bibx78 bib1.bibx88" id="paren.90"/>. Also during flight F02 the tropopause is at higher potential temperature during flight segments within the ASMA (corresponding to enhanced fractions of the South Asia tracer in interval 2; Fig. <xref ref-type="fig" rid="F8"/>). Research flight F02 is the only flight probing air from inside the western part of the ASMA, therefore relatively high water vapour mixing ratios (up to <inline-formula><mml:math id="M254" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 <inline-formula><mml:math id="M255" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppmv</mml:mi></mml:mrow></mml:math></inline-formula>) in interval 2 (Fig. <xref ref-type="fig" rid="F8"/>) are measured above 360 <inline-formula><mml:math id="M256" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature (for more details to <inline-formula><mml:math id="M257" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> mixing ratios during PHILEAS see Fig.  <xref ref-type="fig" rid="FA3"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S1.SS2"/>). In general, <inline-formula><mml:math id="M258" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> is decreasing with increasing potential temperature, however, there is also a lot of additional variability of FISH total water mixing ratios along the flight path of research flight F02. Low fractions of the relative humidity with respect to ice (<inline-formula><mml:math id="M259" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) (<inline-formula><mml:math id="M260" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 20 %) indicate that cloud formation did not occur during the measurements in intervals 1–3, thus FISH total water mixing ratios correspond here to gas-phase <inline-formula><mml:math id="M261" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> mixing ratios. FISH <inline-formula><mml:math id="M262" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> in intervals 1 and 3, are different compared to water vapour in interval 2 at adjacent levels of potential temperature below the local tropopause. These findings suggest that air masses in intervals 1 and 3 or parts of them have different origins and transport pathways compared to air masses measured in interval 2.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e4039">Frequency distribution of the locations where air parcels were traced back from the flight track of research Flight F02 on 6 August 2023 to the model BL  <bold>(a, c, e, g)</bold> and mean transport time <bold>(b, d, f, h)</bold> for the entire flight (above 340 <inline-formula><mml:math id="M263" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) <bold>(a, b)</bold> and time intervals 1–3 <bold>(c–h)</bold> (see Fig. <xref ref-type="fig" rid="F6"/>). Reddish colours indicate mean transport times of a few days found for air from Bay of Bengal in time interval 2 <bold>(f)</bold> and from Southeast Asia in time interval 1 <bold>(d)</bold> and 3 <bold>(h)</bold>. Short transport times found in time interval 1 and 3 from the Western Pacific have a coincidence with the storm track of tropical cyclone Doksuri (C) (20–30 July 2023, for more details to cyclone category see Fig. <xref ref-type="fig" rid="F4"/>).</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f09.jpg"/>

          </fig>

      <p id="d2e4082">Analysing the back-trajectories from Flight F02, main source regions are the Bay of Bengal, the Northern Indian Subcontinent and the Western Pacific (Fig. <xref ref-type="fig" rid="F9"/>a) in accordance with CLaMS simulations using surface–origin tracers (Fig. <xref ref-type="fig" rid="F8"/>). Interval 2 is dominated by air from the Bay of Bengal and the Northern Indian Subcontinent (Fig. <xref ref-type="fig" rid="F9"/>e and f), whereby air masses in interval 1 (Fig. <xref ref-type="fig" rid="F9"/>c and d) and 3 (Fig. <xref ref-type="fig" rid="F9"/>g and h) were mainly traced back to the Western Pacific. The trajectory endpoints in the model boundary layer have a strong coincidence with the track of tropical cyclone Doksuri in particular with the location where it is classified as a typhoon. Thus, our findings show that air masses from the western Pacific found in interval 1 and 3 are uplifted by tropical cyclone Doksuri.</p>
      <p id="d2e4095">The temporal evolution of the South Asia tracer at 370 <inline-formula><mml:math id="M264" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature (Fig. <xref ref-type="fig" rid="FC1"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) shows, that large fraction of the South Asia tracer were uplifted in the Bay of Bengal and adjoining continental regions to the UTLS between 1 and 3 August 2023 and subsequently were transported westward with the anticyclonic flow of the ASMA to the Mediterranean area. The temporal evolution of the Western Pacific tracer at 370 <inline-formula><mml:math id="M265" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature (Fig. <xref ref-type="fig" rid="FC2"/> and <xref ref-type="fig" rid="FC3"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) shows the impact of tropical cyclone Doksuri uplifting large fractions of the Western Pacific tracer up to 370 <inline-formula><mml:math id="M266" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, thus to potential temperature levels of the UTLS. Subsequently, enhanced fractions of the Western Pacific tracer uplifted by tropical cyclone Doksuri (from 23 to 27 July) were transported anticyclonically around the ASMA's southern edge. Thereafter, at the western flank of the ASMA over the Atlantic Ocean these air masses were captured by the subtropical jet and were transported eastwards. Thus, a belt of air with enhanced fractions of the Western Pacific tracer is forming between the northern edge of the ASMA and the subtropical jet that was measured during research flight F02 (Fig. <xref ref-type="fig" rid="F6"/>).</p>
      <p id="d2e4135">Thus, simulations with CLaMS indicate that air masses at the edge of the ASMA have a different origin compared to air masses inside the anticyclone which is in agreement with signatures found in measurements of different chemical trace gases and in the occurrence of particles formed within the ATAL (here indicated by nitrate mass concentrations).</p>
      <p id="d2e4138">Further, TMA-containing particles found in interval 2 indicate the influence from marine sources and/or sources in regions within rural areas with livestock farming and biomass burning such as in regions around the Bay of Bengal (West Bengal or Bangladesh). High mixing ratios of <inline-formula><mml:math id="M267" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> up to <inline-formula><mml:math id="M268" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.9 <inline-formula><mml:math id="M269" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> supports the hypothesis that natural oceanic sources or at least coastal regions contribute to air masses in interval 2. Interval 3 represents a mixture of air from South Asia and the Western Pacific; thus, both agricultural activities around the Bay of Bengal and marine sources in the Western Pacific are potential sources of TMA and <inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e4191">As in Fig. <xref ref-type="fig" rid="F6"/> but for research flight F06 on 16 August 2023 conducted from Oberpfaffenhofen, Germany, to the Mediterranean region (towards southern Italy). Research flight F06 reaches the outer edge of the ASMA (South Asia surface–origin tracer at 370 <inline-formula><mml:math id="M271" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 12:00 UTC, left), which is dominated by air from the western Pacific (Western Pacific surface–origin tracer at 370 <inline-formula><mml:math id="M272" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 12:00 UTC, right). The ASMA boundary (indigo line) is given by MSF <inline-formula><mml:math id="M273" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 356.6 <inline-formula><mml:math id="M274" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>3</sup> <inline-formula><mml:math id="M276" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for 16 August 2023 at 12:00 UTC and 370 <inline-formula><mml:math id="M277" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>. Time interval 1 shown in Fig. <xref ref-type="fig" rid="F11"/> is marked in magenta (bottom).</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f10.jpg"/>

          </fig>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e4274">Surface–origin tracers interpolated along the flight track of research flight F06 on 16 August 2023, potential temperature along the flight track, potential temperature at the tropopause as well as measurements of different chemical trace gases such as <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M280" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M281" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M282" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, relative humidity with respect to ice <inline-formula><mml:math id="M283" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as well as nitrate mass concentration from aerosol particles. Regional surface–origin tracers with fractions greater than 5 % are shown. In interval 1 enhanced fraction of the South Asia and Western Pacific tracer are found; the dominant regional source region is the Northern Western Pacific (NWP, purple in Fig. <xref ref-type="fig" rid="F11"/>a). Note that <inline-formula><mml:math id="M284" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and nitrate are smoothed over 10 <inline-formula><mml:math id="M286" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">s</mml:mi></mml:mrow></mml:math></inline-formula>. Along the <inline-formula><mml:math id="M287" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> time series, flight segments are colour-coded in light-blue, when along the CLaMS back-trajectories possible dehydration is indicated.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f11.png"/>

          </fig>

</sec>
<sec id="Ch1.S4.SS3.SSS2">
  <label>4.3.2</label><title>Research flight F06 (16 August 2023): Typhoon air within the westward outflow of the anticyclone </title>
      <p id="d2e4417">Research flight F06 on 16 August 2023 conducted from Oberpfaffenhofen, Germany, to the Mediterranean area (in direction of South Italy) reached the westward outflow of the ASMA which is mixed with air from the Western Pacific (Fig. <xref ref-type="fig" rid="F10"/>). At the southern turning point of research flight F06, a filament (interval 1) with large fractions of the Western Pacific tracer is reached. In this filament, the fractions from the Western Pacific tracer (up to 40 %) are higher than from the South Asia tracer (about 20 %); the main source region is here the Northern Western Pacific (Fig. <xref ref-type="fig" rid="F11"/>a). Within interval 1 also the tropopause is enhanced or a second tropopause exists (indicating Rossby wave breaking along the subtropical jet <xref ref-type="bibr" rid="bib1.bibx106" id="paren.91"/>) compared to other flight segments (Fig. <xref ref-type="fig" rid="F8"/>b). Therefore within interval 1 the flight track was below the tropopause or between the first and second tropopause.</p>
      <p id="d2e4429">A comparison with chemical trace gases shows that in interval 1 the mixing ratios of <inline-formula><mml:math id="M288" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (up to 80 <inline-formula><mml:math id="M289" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M290" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (up to 1950 <inline-formula><mml:math id="M291" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>) are lower than in the western part of the ASMA during research flight F02 (interval 2 in Fig. <xref ref-type="fig" rid="F8"/> with up to 120 <inline-formula><mml:math id="M292" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M293" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M294" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M295" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2000 <inline-formula><mml:math id="M296" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>), but still higher than in the stratospheric background at these altitudes (<inline-formula><mml:math id="M297" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M298" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math id="M299" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M300" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M301" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 1900 <inline-formula><mml:math id="M302" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>). Low amounts of <inline-formula><mml:math id="M303" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (below 100 <inline-formula><mml:math id="M304" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>) and enhanced amounts of <inline-formula><mml:math id="M305" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (higher than 0.8 <inline-formula><mml:math id="M306" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) indicate the influence from marine sources in interval 1 (Fig. <xref ref-type="fig" rid="F11"/>).</p>
      <p id="d2e4632">Dehydration occurs mostly in flight segments after interval 1 and sometimes also before interval 1 indicating that the air parcels have passed the cold point tropopause. During interval 1 no dehydration was found even in the flight segment above the 1st tropopause (but below the second tropopause) indicating moistening of the lower stratosphere in flight segments with enhanced fractions of the Western Pacific. This indicates another origin and transport pathway of air masses in interval 1 compared to the adjacent flight segments.</p>
      <p id="d2e4635">The South Asia tracer has small fractions of about 20 % in interval 1 indicating some westward outflow of the ASMA. However, during research flight F06, the low nitrate concentrations including interval 1 indicate that the flight was outside the ATAL and that the air masses likely did not originate from the ATAL. Further, no enhanced levels of sodium chloride-, TMA-, or MSA-containing particles were detected during Interval 1 (not shown), suggesting that marine-sourced particles may have been removed during transport, possibly through washout processes.</p>

      <fig id="F12" specific-use="star"><label>Figure 12</label><caption><p id="d2e4641">Frequency distribution of the locations where air parcels were traced back from the flight track of research Flight F06 on 16 August 2023 to the model BL (left) and mean transport time (right) for the entire flight (above 340 <inline-formula><mml:math id="M307" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) <bold>(a, b)</bold> and time intervals 1 <bold>(c, d)</bold>. Reddish colours indicate mean transport times of a few days found for air from the Northern Western Pacific during time interval 1 <bold>(d)</bold>. Short transport time in time interval 1 coincidence with the storm track of tropical cyclone (D) Khanun (26 July–11 August 2023, for more details to cyclone category see Fig. <xref ref-type="fig" rid="F4"/>).</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f12.jpg"/>

          </fig>

      <p id="d2e4669">The origin of the back-trajectories in interval 1 coincide with the storm track of tropical cyclone Khanun (26 July–11 August 2023) (Fig. <xref ref-type="fig" rid="F12"/>c and d). The temporal evolution of the Western Pacific tracer at 370 <inline-formula><mml:math id="M308" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature (Fig. <xref ref-type="fig" rid="FC3"/> in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) shows the impact of tropical cyclone Khanun in particular on 1 and 2 August 2023. Subsequently, enhanced fractions of the western Pacific tracer uplifted by tropical cyclone Khanun were transported anticyclonically around the ASMA's southern edge. These air masses were measured during research flight F06 in interval 1 (Fig. <xref ref-type="fig" rid="F10"/>).</p>
      <p id="d2e4688">Research flight F06 on 16 August 2023 demonstrates the impact of tropical cyclones in the western Pacific on the UTLS over South Europe, transporting a relatively large amount of <inline-formula><mml:math id="M309" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and low <inline-formula><mml:math id="M310" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to the UTLS over South Europe and most likely further into the lower extra-tropical stratosphere within double tropopauses.</p>

      <fig id="F13" specific-use="star"><label>Figure 13</label><caption><p id="d2e4720">As in Fig. <xref ref-type="fig" rid="F6"/> but for research flight F08 on 26–27 August 2023 conducted from Anchorage probing a filament over Alaska separated from the ASMA (South Asia surface–origin tracer at 370 and at 390 <inline-formula><mml:math id="M311" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 00:00 UTC, left), which is mixed with air from the western Pacific (Western Pacific surface–origin tracer at 370 and 390 <inline-formula><mml:math id="M312" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, 00:00 UTC, right). The calculated synoptic HALO flight track position at 27 August 2023 is shown at 00:00 UTC (black line). The ASMA boundaries (indigo line) are given by MSF <inline-formula><mml:math id="M313" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 357.0 <inline-formula><mml:math id="M314" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>3</sup> <inline-formula><mml:math id="M316" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at 370 <inline-formula><mml:math id="M317" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> and MSF <inline-formula><mml:math id="M318" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 367.6 <inline-formula><mml:math id="M319" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>3</sup> <inline-formula><mml:math id="M321" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at 390 <inline-formula><mml:math id="M322" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> for 27 August 2023 at 00:00 UTC. Climatological isentropic transport barriers (olive line) at 370 <inline-formula><mml:math id="M323" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> (PV <inline-formula><mml:math id="M324" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.4 <inline-formula><mml:math id="M325" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">PVU</mml:mi></mml:mrow></mml:math></inline-formula>) and at 390 <inline-formula><mml:math id="M326" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> (8.6 <inline-formula><mml:math id="M327" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">PVU</mml:mi></mml:mrow></mml:math></inline-formula>) are given. Time intervals 1–3 shown in Fig. <xref ref-type="fig" rid="F15"/> are marked in magenta in the zoomed plots. The zoomed plots indicate that the shape and location of the monsoon-influenced filament are different at 370 <inline-formula><mml:math id="M328" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> compared to 390 <inline-formula><mml:math id="M329" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f13.jpg"/>

          </fig>

</sec>
<sec id="Ch1.S4.SS3.SSS3">
  <label>4.3.3</label><title>Research flight F08 (26/27 August 2023): The eastward outflow of the anticyclone</title>
      <p id="d2e4917">Research flight F08 on 26/27 August 2023, conducted from Anchorage, measured the eastward outflow of the ASMA in a filament over Alaska. This filament, separated from the main ASMA, is well mixed with air from the Western Pacific (Fig. <xref ref-type="fig" rid="F13"/>). This monsoon-influenced filament is separated from the northern extratropical UTLS by the subtropical jet that constitutes a transport barrier on an isentropic level. Subsequent mixing of this monsoon-influenced air into the northern extratropical UTLS can occur <xref ref-type="bibr" rid="bib1.bibx106" id="paren.92"/>.</p>

      <fig id="F14" specific-use="star"><label>Figure 14</label><caption><p id="d2e4927">Surface–origin tracers for the model boundary layer, South Asia and the Western Pacific interpolated in space and time along the flight track of research flight F08 on 26 August 2023. In addition individual surface–origin tracers with fractions greater than 5 % are shown as a stacked plot. The main contributions are from China and the western Pacific (ECH, NWP, TWP).</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f14.png"/>

          </fig>

      <fig id="F15" specific-use="star"><label>Figure 15</label><caption><p id="d2e4938">As Fig. <xref ref-type="fig" rid="F11"/> but for research flight F08 on 26–27 August 2023. Regional surface–origin tracers with fractions greater than 10 % are shown. Three time intervals (1–3) high-lighting enhanced nitrate mass concentrations in aerosol particles as an indicator of air from the ATAL as well as enhanced fraction of the South Asia tracer (indicating ASMA air) and the Western Pacific tracer are marked in grey.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f15.png"/>

          </fig>

      <p id="d2e4950">Air masses measured in this monsoon-influenced filament of the ASMA (intervals 1–3 in Fig. <xref ref-type="fig" rid="F13"/>) originate mainly from East China (ECH) and the Western Pacific (NWP and TWP) (Figs. <xref ref-type="fig" rid="F14"/> and <xref ref-type="fig" rid="F15"/>a), in contrast to the western part of the ASMA measured during research flight F02, where air originates mainly from the Indian subcontinent (IND, NIN, BoB; Figs. <xref ref-type="fig" rid="F7"/> and <xref ref-type="fig" rid="F8"/>a). Within the monsoon-influenced filament measured on 26/27 August, somewhat higher fractions (by approximately a factor of two) of the South Asia tracer are generally found compared to the Western Pacific tracer (Fig. <xref ref-type="fig" rid="F14"/>), in contrast to air in the western part of the ASMA (flight F02), where fractions of the South Asia tracer are higher by about a factor of 7 (Fig. <xref ref-type="fig" rid="F7"/>). During research flight F08, both tracers are positively correlated, in contrast to flight F02, where the two tracers are negatively correlated. This indicates that during the separation of the filament from the ASMA, air from inside the ASMA (high amounts of the South Asia tracer) was mixed with air located at its outer edge (high amounts of the Western Pacific tracer). The temporal evolution of the South Asia and the Western Pacific tracer at 370 <inline-formula><mml:math id="M330" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature from 19 to 27 August 2023 is shown in Fig. <xref ref-type="fig" rid="FC4"/> (Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) demonstrating the mixing of these two air masses.</p>
      <p id="d2e4980">The time series of the surface–origin tracers interpolated along the flight track of research flight F08 are also qualitatively compared with measurements of several chemical trace gases (Fig. <xref ref-type="fig" rid="F15"/>). In our study, we focus on measurements above 340 <inline-formula><mml:math id="M331" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature (thus to UTLS levels) in contrast to other recent studies that include measurements from research flight F08 below this level (conducted during the first hours of the flight, which are not shown in Fig. <xref ref-type="fig" rid="F15"/>). These studies link enhanced <inline-formula><mml:math id="M332" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios (up to 300 <inline-formula><mml:math id="M333" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) measured in this flight segment to sources in eastern China <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx87" id="paren.93"/>, which is consistent with our CLaMS simulations but which is not discussed further here.</p>
      <p id="d2e5023">In the following, we will focus on the flight track measured after <inline-formula><mml:math id="M334" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 22:00 UTC crossing the monsoon-influenced filament. After <inline-formula><mml:math id="M335" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 22:00 UTC, the South Asia and the Western Pacific tracer are positively correlated (Fig. <xref ref-type="fig" rid="F15"/>a). Both surface-origin tracers are further positively correlated with <inline-formula><mml:math id="M336" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (with values up to 110 <inline-formula><mml:math id="M337" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>), a marker for anthropogenic sources in Asia, <inline-formula><mml:math id="M338" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (with values up to 1980 <inline-formula><mml:math id="M339" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula>), a marker for monsoon-influenced air and <inline-formula><mml:math id="M340" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (with values up to 0.9 <inline-formula><mml:math id="M341" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>), a marker for natural oceanic sources. <inline-formula><mml:math id="M342" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, a tracer of marine tropospheric (low values) and stratospheric air (high values), shows more complex behaviour in detail but is generally negatively correlated with both the South Asia and the Western Pacific tracers, indicating the impact of ozone-poor marine air. However, <inline-formula><mml:math id="M343" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increases with potential temperature (interval 2), consistent with the increasing influence of stratospheric air.</p>
      <p id="d2e5132">The three intervals 1–3 (shown in Fig. <xref ref-type="fig" rid="F13"/>) are at different levels of potential temperature and are selected to highlight enhanced nitrate mass concentrations in aerosol particles as an indicator of air from the ATAL (ASMA) (Fig. <xref ref-type="fig" rid="F15"/>f, the small peak at 21:40 UTC is not considered here, but yield similar results as for interval 1, however with a lower amount of air parcels). Similar as for F06 also here in F08, no enhanced levels of sodium chloride-, TMA-, or MSA-containing particles were detected during interval 1–3 (not shown), suggesting that marine-sourced particles may have been removed during transport to potential temperature levels above 360 <inline-formula><mml:math id="M344" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, possibly through washout processes.</p>
      <p id="d2e5147">In contrast to research flight F02 inside the western part of the ASMA, the flight segments of research flight F08 above <inline-formula><mml:math id="M345" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 360 <inline-formula><mml:math id="M346" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> were also above the local 1st tropopause, thus in the lower stratosphere (Fig. <xref ref-type="fig" rid="F15"/>b). In intervals 1, 2 and 3 (all three intervals are above the tropopause) also water vapour is enhanced compared to adjacent flight segments at the same potential temperature level. Here, in intervals 1–3, cloud formation processes along the flight track can be excluded (<inline-formula><mml:math id="M347" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RH</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M348" display="inline"><mml:mo>≲</mml:mo></mml:math></inline-formula> 10 %). Findings from back-trajectory calculations show that in intervals 1, 2 and 3 dehydration (flight segments that are shown in light–blue in Fig. <xref ref-type="fig" rid="F15"/>e) does not occur (only for a minor number of trajectories), thus enhanced <inline-formula><mml:math id="M349" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> is found within the filament separated from the ASMA. In particular in intervals 2 and 3, hydration is evident above 380 <inline-formula><mml:math id="M350" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature.</p>
      <p id="d2e5209">This demonstrates that both polluted air from South Asia as well as marine air contribute to the chemical composition of the monsoon-influenced filament separated from the ASMA. Caused by the mixing of two air masses with different tropospheric origin, the chemical composition of the filaments separated at the eastern edge of the anticyclone is different from the chemical composition of the ASMA's air itself measured during research flight F02.</p>

      <fig id="F16" specific-use="star"><label>Figure 16</label><caption><p id="d2e5215">Frequency distribution of the locations where air parcels were traced back from the flight track of research Flight F08 on 26–27 August 2023, to the model BL (left) and mean transport time (right) for the entire flight (above 340 <inline-formula><mml:math id="M351" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) <bold>(a, b)</bold> and time intervals 1–3 <bold>(c–h)</bold>. An accumulation of trajectory endpoints is found in South Asia as well as in the western Pacific. The time intervals are on different levels of potential temperatures whereby the potential temperature is increasing from interval 1 to 3. The origin of the back-trajectories in the selected interval coincide with the storm track of tropical cyclones (B) Talim (13–18 July 2023), (C) Doksuri (20–30 July 2023), (D) Khanun (26 July–11 August 2023), however for the highest potential temperature level in interval 3, only Talim and Doksuri play a role (for more details to cyclone category see Fig. <xref ref-type="fig" rid="F4"/>).</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f16.jpg"/>

          </fig>

      <p id="d2e5240">The back-trajectory analysis shows that an accumulation of trajectory endpoints is found in South Asia as well as in the western Pacific in agreement with simulations using surface–origin tracers (Fig. <xref ref-type="fig" rid="F16"/>). The origin of the back-trajectories in intervals 1, 2 and 3 coincide with the storm track of several tropical cyclones (Fig. <xref ref-type="fig" rid="F16"/>c–h). The time intervals are on different levels of potential temperatures whereby the potential temperature is increasing from interval 1 to 3 (Fig. <xref ref-type="fig" rid="F15"/>b). The origin of the back-trajectories in the selected intervals coincide with the storm track of tropical cyclones (B) Talim (13–18 July 2023), (C) Doksuri (20–30 July 2023), (D) Khanun (26 July–11 August 2023), however for the highest potential temperature level at <inline-formula><mml:math id="M352" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 400 <inline-formula><mml:math id="M353" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> in interval 3, only Talim and Doksuri play a role. Longer transport times (<inline-formula><mml:math id="M354" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 40–60 <inline-formula><mml:math id="M355" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">d</mml:mi></mml:mrow></mml:math></inline-formula>) are found from storm tracks of tropical cyclones at the model boundary layer to flight segments at 400 <inline-formula><mml:math id="M356" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature compared to flight segments at lower potential temperature.</p>
      <p id="d2e5288">Filaments separated at the eastern flank of the ASMA transport a mixture of polluted air from South Asia and marine air from the western Pacific towards the lower extratropical UTLS. Thus, regarding the eastward outflow of the ASMA by the separation of filaments or eddy shedding, our findings demonstrate that within these filaments contributions of air from the western Pacific also have to be taken into account.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d2e5302">We combined PHILEAS HALO aircraft measurements with global three-dimensional CLaMS simulations, including model tracers of surface origin and with pure CLaMS back-trajectory calculations started along all aircraft flight tracks. Both three-dimensional simulations and back-trajectory calculations are driven by the high-resolution ERA5 reanalysis. Boundary source regions and transport times of air masses measured during the PHILEAS campaign were identified. Main source regions in South Asia and in the western Pacific (impacted by tropical cyclones) were found. Caused by the high-resolution of the ERA5 reanalysis data and the Lagrangian transport including irreversible mixing in CLaMS, a remarkable agreement between fine-scale structures found in measured chemical tracers and in simulated surface–origin tracers along the flight tracks are identified.</p>
      <p id="d2e5305">Our findings show that for the PHILEAS campaign, the South Asia tracer serves as a reliable proxy for polluted air originating from the Asian summer monsoon region. Additionally, the Western Pacific tracer is a useful marker for air masses of marine origin, and more specifically, an indicator of air uplifted into the UTLS by tropical cyclones in the western Pacific. Regional surface–origin tracers, sub-regions of the South Asia or the Western Pacific tracer such as Northern Indian Subcontinent (NIN), Indian Subcontinent (IND), Tibetan Plateau (TIB), Eastern China (ECH), Bay of Bengal (BoB), Indian Ocean (IND) or Northern Western Pacific (NWP) narrow the air mass origin of the PHILEAS measurements to smaller source regions.</p>
      <p id="d2e5308">Measured mixing ratios of <inline-formula><mml:math id="M357" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the HAGAR-V instrument depend strongly on the specific source region in Asia and 3 different branches with enhanced <inline-formula><mml:math id="M358" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (higher than the background value at tropopause heights of <inline-formula><mml:math id="M359" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50 <inline-formula><mml:math id="M360" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx1" id="paren.94"><named-content content-type="pre">e.g.</named-content></xref>) and <inline-formula><mml:math id="M361" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> larger than 1920 <inline-formula><mml:math id="M362" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppbv</mml:mi></mml:mrow></mml:math></inline-formula> (as an indicator for monsoon-influenced air) are found. The highest <inline-formula><mml:math id="M363" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios (200–300 <inline-formula><mml:math id="M364" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>) are found in air masses influenced by sources in China and mixed with air from the Northern Western Pacific, particularly at altitudes below the ASMA (<inline-formula><mml:math id="M365" display="inline"><mml:mo lspace="0mm">≤</mml:mo></mml:math></inline-formula> 360 <inline-formula><mml:math id="M366" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>), driven by both convection and strong <inline-formula><mml:math id="M367" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources in eastern China. Further, CLaMS simulations indicate that <inline-formula><mml:math id="M368" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios of <inline-formula><mml:math id="M369" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 150 <inline-formula><mml:math id="M370" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula> are a mixture of air from eastern China, Northern Indian Subcontinent and the Tropical Western Pacific; this is also valid for potential temperature levels below 360 <inline-formula><mml:math id="M371" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>. <inline-formula><mml:math id="M372" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios of <inline-formula><mml:math id="M373" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 100 <inline-formula><mml:math id="M374" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">ppt</mml:mi></mml:mrow></mml:math></inline-formula>, at potential temperature levels of the ASMA (<inline-formula><mml:math id="M375" display="inline"><mml:mo lspace="0mm">≥</mml:mo></mml:math></inline-formula> 360 <inline-formula><mml:math id="M376" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>) are associated with air masses mainly from the Indian Subcontinent and Bay of Bengal where <inline-formula><mml:math id="M377" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sources can be assumed to be much lower than in China. In general, transport above the maximum convective outflow level (<inline-formula><mml:math id="M378" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 360,K) is much slower; thus, mixing with <inline-formula><mml:math id="M379" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-poor air within the ASMA becomes more important compared to air masses observed in the upper troposphere that are directly influenced by fast uplift of air from the main <inline-formula><mml:math id="M380" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> source regions in Asia. The short chemical lifetime of <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M382" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 6 months) plays only a minor role in the spatial distribution of <inline-formula><mml:math id="M383" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> within the ASMA and its outflow compared to the time scales of mixing (dilution; <inline-formula><mml:math id="M384" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> hours to several weeks).</p>
      <p id="d2e5627">The presented case studies of three single research flights (F02, F06, and F08) are focused on the western part of the ASMA – the eastern part of the main anticyclone was not reached during the PHILEAS flights – and likewise on its westward and eastward outflow at potential temperature levels <inline-formula><mml:math id="M385" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 360 <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>. Measurements of pollutants and greenhouse gases such as <inline-formula><mml:math id="M387" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M388" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and water vapour as well as enhanced nitrate mass concentrations (a sign for particles from the ATAL) indicate sources in South Asia in agreement with CLaMS South Asia surface–origin tracer finding sources in the region of the ASMA. Further, enhanced TMA was found in the western part of the ASMA during research flight F02, with an enhanced influence from northern India, in particular from West Bengal, Bangladesh, and the Bay of Bengal. Potentially large agricultural sources of TMA, as well as natural oceanic sources, may be associated with the measurements.</p>
      <p id="d2e5673">Our findings show that the PHILEAS measurements are in general impacted by tropical cyclones in the western Pacific. The model simulations demonstrate that the outer edge of the ASMA in 2023 is impacted by marine air from the western Pacific uplifted by tropical cyclones. The contribution of the surface-origin tracers in the ASMA and at its edge are highly inhomogeneous and depend on the interplay of tropical cyclones and the ASMA in agreement with trace gas and particle measurements from research flights F02, F06, and F08. Subsequent mixing of polluted air from inside the ASMA and marine air (including enhanced natural <inline-formula><mml:math id="M389" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) at its edge occurs at the eastern flank of the anticyclone when filaments are separated from the main anticyclone. Therefore, the chemical composition of air in the eastward outflow of the anticyclone differs from the western part of the ASMA. Furthermore, air masses measured in the eastward outflow of the ASMA are mainly from East China and the Western Pacific (from the region of East Asian and Western North Pacific summer monsoons) in contrast to the western part that originates mainly from the Indian subcontinent (from the region of the Indian summer monsoon). Our findings are schematically summarised in Fig. <xref ref-type="fig" rid="F17"/> for potential temperature levels of the ASMA; however, the interplay between the ASMA and tropical cyclones is highly variable and can differ in individual cases.</p>

      <fig id="F17"><label>Figure 17</label><caption><p id="d2e5696">Schematic of the ASMA and its westward and eastward outflow (brownish arrows). Marine air from the western Pacific (blue) can be uplifted by tropical cyclones to altitudes of the ASMA and subsequently transported around the outer edge of the ASMA (blue arrows). Mixing of polluted air from inside the ASMA (brown) with marine air (blue) at its edge occurs at the eastern flank of the anticyclone when filaments are separated from the main anticyclone. Air masses measured in the eastward outflow of the ASMA are mainly from eastern China (purple) and the western Pacific (from the region of East Asian and Western North Pacific summer monsoons) in contrast to the western part that originates mainly from the Indian subcontinent (from the region of the Indian summer monsoon; red).</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f17.png"/>

      </fig>

      <p id="d2e5705">Measurements of ozone-poor and relatively enhanced <inline-formula><mml:math id="M390" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> air that has mostly natural oceanic sources indicate sources in the Western Pacific in agreement with CLaMS Western Pacific surface–origin tracer as well as back-trajectory calculations indicating possible impact of tropical cyclones (e.g., region 1 in Figs. <xref ref-type="fig" rid="F11"/> and <xref ref-type="fig" rid="F15"/>). The uplift of marine air by tropical cyclones and the subsequent transport impacted by the ASMA is a potential source of <inline-formula><mml:math id="M391" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, ozone-poor air and water vapour contributing to the chemical composition of the UTLS. Bromine from very short lived substances such as <inline-formula><mml:math id="M392" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Br</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, primarily from natural oceanic sources, contributes substantially to the stratospheric bromine loading and has a significant impact on modelled ozone and ozone trends in particular in the extratropical UTLS <xref ref-type="bibr" rid="bib1.bibx95" id="paren.95"/>. Despite research flights F02, F06, and F08 were influenced by tropical cyclones and have marine sources, no significant particle fractions from sea salt and MSA as marine tracers were found. We emphasise that the intensity and duration of tropical cyclones has been increasing in recent decades <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx67 bib1.bibx45 bib1.bibx8" id="paren.96"><named-content content-type="pre">e.g.</named-content></xref>. Therefore, direct injections of marine air by rapid uplift in tropical cyclones to the outer edge of the ASMA will likely increase in the future.</p>
</sec>

      
      </body>
    <back><app-group>

<app id="App1.Ch1.S1">
  <label>Appendix A</label><title>Additional tracer-tracer relations</title>
<sec id="App1.Ch1.S1.SS1">
  <label>A1</label><title><inline-formula><mml:math id="M393" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M394" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">Cl</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> relations</title>

      <fig id="FA1"><label>Figure A1</label><caption><p id="d2e5817">The same as Fig. <xref ref-type="fig" rid="F5"/>, but for surface–origin tracers contributing to the South Asia (IND, NIN, ECH, TIB, BoB, NIO, Neast, NAF) and Western Pacific tracer (Wpool, TWP, NWP, SEA).</p></caption>
          
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f18.png"/>

        </fig>

      <fig id="FA2" specific-use="star"><label>Figure A2</label><caption><p id="d2e5832">The same as Fig. <xref ref-type="fig" rid="F5"/>, but colour-coded by CLaMS surface–origin tracers representing the northern background (CAM <inline-formula><mml:math id="M395" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Casia <inline-formula><mml:math id="M396" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NAM <inline-formula><mml:math id="M397" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NAO <inline-formula><mml:math id="M398" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NEA <inline-formula><mml:math id="M399" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NEP <inline-formula><mml:math id="M400" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NPO <inline-formula><mml:math id="M401" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TEP) and the residual surface (AMZ <inline-formula><mml:math id="M402" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> AUS <inline-formula><mml:math id="M403" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NEZ <inline-formula><mml:math id="M404" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SAF <inline-formula><mml:math id="M405" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SAM <inline-formula><mml:math id="M406" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SAO <inline-formula><mml:math id="M407" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SEP <inline-formula><mml:math id="M408" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SIO <inline-formula><mml:math id="M409" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SPO <inline-formula><mml:math id="M410" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> SWP <inline-formula><mml:math id="M411" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TAO).</p></caption>
          
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f19.png"/>

        </fig>


</sec>
<sec id="App1.Ch1.S1.SS2">
  <label>A2</label><title><inline-formula><mml:math id="M412" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M413" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> relations indicating water vapour sources in South Asia and the western Pacific</title>

      <fig id="FA3"><label>Figure A3</label><caption><p id="d2e6003"><inline-formula><mml:math id="M414" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M415" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> relations for all scientific PHILEAS flights F02–F20 for measurements above 360 <inline-formula><mml:math id="M416" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, i.e. at altitudes of the ASMA colour-coded by the South Asia and Western Pacific tracer and potential temperature. In addition, also the scientific flights F02 (6 August 2023), F06 (16 August 2023) and F08 (26–27 August 2023) are shown.</p></caption>
          
          <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f20.png"/>

        </fig>


</sec>
</app>

<app id="App1.Ch1.S2">
  <label>Appendix B</label><title>Bipolar mean spectrum of the TMA-containing particle type</title>

      <fig id="FB1"><label>Figure B1</label><caption><p id="d2e6058">Bipolar mean spectrum of the TMA-containing particle type (average over 354 particles) measured with ERICA-LAMS during F02. The mean spectrum indicates that TMA in single particles is internally mixed with sulfate, nitrate, ammonium, potassium, chloride, MSA, and organic compounds. The signal intensity axis is limited to 300 <inline-formula><mml:math id="M417" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mV</mml:mi></mml:mrow></mml:math></inline-formula>, while the <inline-formula><mml:math id="M418" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M419" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>97 actually reaches up to 3000 <inline-formula><mml:math id="M420" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mV</mml:mi></mml:mrow></mml:math></inline-formula>.</p></caption>
        
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f21.png"/>

      </fig>

</app>

<app id="App1.Ch1.S3">
  <label>Appendix C</label><title>Temporal evolution of the South Asia and Western Pacific tracer</title>

      <fig id="FC1"><label>Figure C1</label><caption><p id="d2e6114">Temporal evolution of the South Asia tracer at 370 <inline-formula><mml:math id="M421" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature from 1 to 6 August 2023. On 6 August 2023 the calculated synoptic HALO flight track position at 12:00 UTC of research flight F02 is indicated (black line). The climatological isentropic transport barrier for the Northern (PV <inline-formula><mml:math id="M422" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 6.4 <inline-formula><mml:math id="M423" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">PVU</mml:mi></mml:mrow></mml:math></inline-formula>; solid olive line) and Southern (PV <inline-formula><mml:math id="M424" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M425" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.2 <inline-formula><mml:math id="M426" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">PVU</mml:mi></mml:mrow></mml:math></inline-formula>; dashed olive line) Hemisphere at 370 <inline-formula><mml:math id="M427" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> during summer derived by <xref ref-type="bibr" rid="bib1.bibx53" id="text.97"/> indicates the barrier between the tropical tropopause layer and the extra-tropical lower stratosphere.</p></caption>
        
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f22.jpg"/>

      </fig>

      <fig id="FC2" specific-use="star"><label>Figure C2</label><caption><p id="d2e6184">Temporal evolution of the Western Pacific tracer at 370 <inline-formula><mml:math id="M428" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature from 15 to 31 July 2023. The impact of several tropical cyclones on the Western Pacific tracer is evident (reddish colours): Talim (B) (14–16 July), Doksuri (C) (23–27 July) and Khanun (D) (29 July–2 August; see next figure for August). Subsequent enhanced fractions of the Western Pacific tracer uplifted by tropical cyclones were transported anticyclonically around the ASMA's southern edge. Thereafter, at the western flank of the ASMA over Africa or the Atlantic Ocean the air is transported eastwards by the subtropical jet and a belt of the Western Pacific tracer is developing between the northern edge of the ASMA and the subtropical jet. The climatological isentropic transport barriers (olive lines) are the same as in Fig. <xref ref-type="fig" rid="FC1"/>.</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f23.jpg"/>

      </fig>

      <fig id="FC3" specific-use="star"><label>Figure C3</label><caption><p id="d2e6206">Same as Fig. <xref ref-type="fig" rid="FC2"/>, but from 1 to 18 August 2023. On 6 and 16 August 2023 the calculated synoptic HALO flight track position at 12:00 UTC of research flight F02 and F06, respectively, are indicated (black line).</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f24.jpg"/>

      </fig>

      <fig id="FC4" specific-use="star"><label>Figure C4</label><caption><p id="d2e6219">Temporal evolution of the South Asia and the Western Pacific tracer at 370 <inline-formula><mml:math id="M429" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula> potential temperature from 19 to 27 August 2023. On 27 August 2023 (00:00 UTC; in contrast to all other panels that are shown on 12:00 UTC) the calculated synoptic HALO flight track position of research flight F08 is indicated (black line).</p></caption>
        <graphic xlink:href="https://acp.copernicus.org/articles/26/6283/2026/acp-26-6283-2026-f25.jpg"/>

      </fig>


</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d2e6242">Observational data from the PHILEAS HALO mission are available via the HALO database (<uri>https://halo-db.pa.op.dlr.de/</uri>, last access: 6 May 2026). The ERA5 data used here are available from the ECMWF (<uri>https://www.copernicus.eu/en</uri>, last access: 6 May 2026). The tropical cyclone tracks in the western Pacific are provided by the Japan Meteorological Agency and are available under <uri>https://www.jma.go.jp/jma/jma-eng/jma-center/rsmc-hp-pub-eg/besttrack.html</uri> (last access: 9 October 2024). The CLaMS code is available on a GitLab server at <uri>https://jugit.fz-juelich.de/clams/CLaMS</uri> (last access: 6 May 2026). Results of the CLaMS simulations presented in this work are available from the corresponding author upon request.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e6260">BV developed the concept for this study and performed the CLaMS simulations with contributions of JC. VL, JS, RvL, MCV, FE, FK, SB, AD, OE, SM, JS, PH, LO, FW, CR, and AZ conducted the HALO PHILEAS measurements and the subsequent data analysis of these observations. MR, PH and CR coordinated the PHILEAS campaign including the scientific flight planning. OK provided the ASMA boundaries. BV wrote the paper with contributions of all authors. The interpretation of the results was discussed with all coauthors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e6266">The authors have the following competing interests: At least one of the (co-)authors is a member of the editorial board of <italic>Atmospheric Chemistry and Physics</italic>.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e6275">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e6281">We are grateful to all colleagues that were involved in the PHILEAS project, in particular applying and coordinating the project, planning the research flights including the provision of forecast products as well as preparing and conducting measurements onboard HALO and the subsequent data analysis. In particular we would like to thank Florian Obersteiner (KIT, Karlsruhe, Germany) for the FAIRO data, Daniel Kunkel (University Mainz, Germany) and Johannes Schneider (MPI, Mainz, Germany) for further discussion of the manuscript. We thank the European Centre for Medium-Range Weather Forecasts (ECMWF) for providing the the ERA5 reanalyses and the Jülich Supercomputing Centre (JSC; Research Centre Jülich, Germany) for the computing time on the supercomputer JUWELS (project CLaMS-ESM) and for the storage resources. Finally, we acknowledge Matthias Riße and Nicole Thomas very much for their support on a variety of technical issues related to this work and Karlheinz Nogai for the creation of the summary figure. ChatGPT was used for assistance with language refinement and Python programming.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e6287">The presented work was partly funded by the German Science Foundation (Deutsche Forschungsgemeinschaft, DFG) as part of the HALO Priority Program SPP 1294 (VO 1276/7-1, HO-4225/17-1 HO-4225/19-1, KO 6470/1-1), the NSFC–DFG project ATALTrack (VO 1276/6-1 and BO 1829/12-1) and the TRR 301 TPChange project (Project-ID 428312742).The article processing charges for this open-access publication were covered by the Forschungszentrum Jülich.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e6298">This paper was edited by Jianzhong Ma and reviewed by five anonymous referees.</p>
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