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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Measurement report}?>
  <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-23-9229-2023</article-id><title-group><article-title>Measurement report: Assessment of Asian emissions of ethane and propane with a chemistry transport model based on observations from the island of Hateruma</article-title><alt-title>Assessment of Asian emissions of ethane and propane</alt-title>
      </title-group><?xmltex \runningtitle{Assessment of Asian emissions of ethane and propane}?><?xmltex \runningauthor{A. R. Adedeji et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Adedeji</surname><given-names>Adedayo R.</given-names></name>
          <email>adedayo.adedeji@york.ac.uk</email><email>rasaqdayo@gmail.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Andrews</surname><given-names>Stephen J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Rowlinson</surname><given-names>Matthew J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5236-6536</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Evans</surname><given-names>Mathew J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4775-032X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Lewis</surname><given-names>Alastair C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hashimoto</surname><given-names>Shigeru</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Mukai</surname><given-names>Hitoshi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Tanimoto</surname><given-names>Hiroshi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5424-9923</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Tohjima</surname><given-names>Yasunori</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Saito</surname><given-names>Takuya</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Wolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, York, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>National Centre for Atmospheric Science, Department of Chemistry, University of York, York, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>National Institute for Environmental Studies, 16-2 Onogawa, Tsukuba, Ibaraki 305-8506, Japan</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Adedayo R. Adedeji (adedayo.adedeji@york.ac.uk, rasaqdayo@gmail.com)</corresp></author-notes><pub-date><day>22</day><month>August</month><year>2023</year></pub-date>
      
      <volume>23</volume>
      <issue>16</issue>
      <fpage>9229</fpage><lpage>9244</lpage>
      <history>
        <date date-type="received"><day>3</day><month>October</month><year>2022</year></date>
           <date date-type="rev-request"><day>15</day><month>November</month><year>2022</year></date>
           <date date-type="rev-recd"><day>23</day><month>June</month><year>2023</year></date>
           <date date-type="accepted"><day>12</day><month>July</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2023 </copyright-statement>
        <copyright-year>2023</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/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e178">The island of Hateruma is the southernmost inhabited island of Japan. Here we interpret observations of ethane (C<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>) and propane (C<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>) together with carbon monoxide (CO),  nitrogen oxides (NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>) and ozone (O<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) carried out in the island in 2018 with the GEOS-Chem atmospheric chemistry transport model. We simulated the mixing ratios of these species within a nested grid centred over the site, with a model resolution of 0.5<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M9" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. We use the Community Emissions Data System (CEDS) dataset for anthropogenic emissions and add a geological source of C<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>. The model captured the seasonality of primary pollutants (CO, C<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, C<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>) at the site – high mixing ratios in the winter months when oxidation rates are low and flow is from the north and low mixing ratios in the summer months when oxidation rates are higher and flow is from the south. It also simulates many of the synoptic-scale events with Pearson's correlation coefficients (<inline-formula><mml:math id="M19" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) of 0.74, 0.88 and 0.89 for CO, C<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, respectively. Mixing ratios of CO are simulated well by the model (slope of the linear fit between model results and measurements is 0.91), but simulated mixing ratios of C<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> are significantly lower than the observations (slopes of the linear fit between model results and measurements are 0.57 and 0.41, respectively), most noticeably in the winter months. Simulated NO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios were underestimated, but NO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> appears to be overestimated. The mixing ratio of O<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is moderately well simulated (slope of the linear fit between model results and observations is 0.76, with an <inline-formula><mml:math id="M31" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> of 0.87), but there is a tendency to underestimate mixing ratios in the winter months.
By switching off the model's biomass burning emissions we show that during winter, biomass burning has limited influence on the mixing ratios of compounds but can represent a more sizeable fraction in the summer.  We also show that increasing the anthropogenic emissions of C<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> within the domain by factors of 2.22 and 3.17 increases the model's ability to simulate these species in the winter months, consistent with previous studies.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>UK Research and Innovation</funding-source>
<award-id>NE/S012273/1</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Japan Society for the Promotion of Science</funding-source>
<award-id>JSPSJRP20181708</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<?pagebreak page9230?><sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e504">Transboundary flow of pollutants in the atmosphere is a major global issue <xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx38 bib1.bibx31" id="paren.1"/>. This is very concerning in some parts such as East Asia where highly polluting regions can significantly impact the atmospheric composition at large distances downwind due to the transport of long-lived atmospheric pollutants. As well as the transport of primary pollutants, secondary, en route production of pollutants such as ozone (O<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) and particulate matter (PM) can impact the concentration of these pollutants at long distances from their sources <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx20 bib1.bibx22" id="paren.2"/>.</p>
      <p id="d1e522">Ozone in the troposphere is produced from the oxidation of primary emitted compounds such as volatile organic compounds (VOCs), carbon monoxide (CO) and methane (CH<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>) in the presence of oxides of nitrogen (NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>). Thus increases in the emissions of these compounds can be expected to lead to increases in the concentration of O<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> downwind of the emission sites. The rapid industrialization in East Asia has led to increased emissions of these primary compounds, and this in turn has led to increases in the concentration of O<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx12" id="paren.3"/>.  Over the coming decades, there are predictions for this trend to continue <xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx24" id="paren.4"/>. It is therefore important to measure the regional concentrations of atmospheric pollutants such as O<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and its precursors (VOCs, NO<inline-formula><mml:math id="M42" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, CO, etc.) in East Asian source regions and downwind over the coming years.</p>
      <p id="d1e586">Finding suitable sites for making these long-term downwind measurements is, however, difficult. Sites need to be remote from local influences, yet sufficiently accessible for staff to visit for instrument maintenance and upgrades and for data to be transmitted back for processing, etc. Hateruma Island is a small island (12.7 km<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>) located off the coasts of both Taiwan and Japan's main islands and so is subject to East Asian outflow (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a and b).  It is the southernmost inhabited island (24.05<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 123.80<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) in the Japanese archipelago, 500 km south-west of Japan's Okinawa Island, and is 250 km off the coast of Taiwan  in the Pacific Ocean <xref ref-type="bibr" rid="bib1.bibx56" id="paren.5"/>.  As a part of its global monitoring effort, the Japanese National Institute for Environmental Studies' (NIES) Centre for Global Environmental Research (CGER) operates an atmospheric observatory on the island to carry out atmospheric measurements. CGER has made measurements of atmospheric constituents at the site over a number of years. During the winter the site is characterized by northerly winds and elevated pollution influenced by emissions from East Asian countries, whereas in the summer the air comes from the south and is typically cleaner <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx48" id="paren.6"/>. Observations of atmospheric composition at Hateruma Island have been used to analyse different problems.  For example, <xref ref-type="bibr" rid="bib1.bibx55" id="text.7"/> and <xref ref-type="bibr" rid="bib1.bibx41" id="text.8"/> used observations from Hateruma to assess national emissions of hydrofluorocarbons (HFCs) and hydrochlorofluorocarbons (HCFCs) from China, Korea and Japan. <xref ref-type="bibr" rid="bib1.bibx35" id="text.9"/> continuously measured the atmospheric mixing ratios of perfluorocarbons (PFCs) at Hateruma Island and Cape Ochi-ishi since 2006, to infer their global and regional emissions.  <xref ref-type="bibr" rid="bib1.bibx49" id="text.10"/> used observation of carbon monoxide (CO), carbon dioxide (CO<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and methane (CH<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>) to assess changing emissions from China and then went on to use a similar technique to assess the drop in CO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions from China due to COVID-19 regulations <xref ref-type="bibr" rid="bib1.bibx50" id="paren.11"/>.</p>
      <p id="d1e668">A wider range of observations are made at the site than have been previously published. These include measurements of CO, ethane (C<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>), propane (C<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>), nitrogen oxides (NO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>) and O<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. Although these observations themselves are useful, the use of a chemical transport model allows observations to be put into the context of our wider understanding of atmospheric emissions – deposition, transport and chemistry allowing.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e738"><bold>(a)</bold> The region of the high-resolution modelling domain spans from 14 to 42<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 100 to 145<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, indicated by the green box; <bold>(b)</bold> zoomed-in image to show the location of the island of Hateruma: 24.05<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 123.80<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, inside the red square.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f01.png"/>

      </fig>

      <p id="d1e788">Here we use a chemical transport model (GEOS-Chem) together with observations of the key atmospheric gases (CO, C<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, C<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, NO, NO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) measured at the observatory in Hateruma in 2018 to evaluate the model's ability to simulate the long-range transport of key species to the island of Hateruma and our understanding of emissions in the region. We start with a description of the observations made at the site (Sect. <xref ref-type="sec" rid="Ch1.S2"/>) and provide a meteorological context for the observations using back trajectories. We then describe the GEOS-Chem model configuration in Sect. <xref ref-type="sec" rid="Ch1.S3"/> and show an evaluation of the model performance in Sect. <xref ref-type="sec" rid="Ch1.S4"/>. Based on this evaluation we assess the sensitivity of the model to biomass burning emissions in Sect. <xref ref-type="sec" rid="Ch1.S5"/>, and in Sect. <xref ref-type="sec" rid="Ch1.S6"/> we explore scaling anthropogenic Asian C<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M69" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> emissions to better reflect the observations at the site. We draw conclusions in Sect. 7.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Observations and meteorological context</title>
      <p id="d1e910">In this section, we describe the observations made at the site used for this study and the meteorological context of the air arriving at the site.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Observations</title>
      <p id="d1e920">The observatory is located on the eastern corner of the island, with a disused airport and the populated area (with electricity generation from diesel engines and wind power) located to the west. We expect limited local anthropogenic emissions on the island because of its small size and population. The location of the population and power generation to the west of the observations also limits potential contamination at the site from most wind directions. A number of different observations are made at the site, but we are only concerned with a subset of the observations in this study. Table <xref ref-type="table" rid="Ch1.T1"/> gives the observations used in the study and the method used to make them. Observations are available hourly for most of 2018 with some missing periods.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e928">Physical and chemical variables measured hourly at Hateruma between 1 January to 31 December 2018 (see references for QA/QC information). Data capture indicates the number of hours when observations are available out of the 8760 h for the year.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Variables</oasis:entry>
         <oasis:entry colname="col2">Method</oasis:entry>
         <oasis:entry colname="col3">Data captured</oasis:entry>
         <oasis:entry colname="col4">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Temperature</oasis:entry>
         <oasis:entry colname="col2">Pt100 (YOKOGAWA E734)</oasis:entry>
         <oasis:entry colname="col3">8751/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Wind speed</oasis:entry>
         <oasis:entry colname="col2">Wind speed and direction transmitter (YOKOGAWA WA7601)</oasis:entry>
         <oasis:entry colname="col3">8751/8760</oasis:entry>
         <oasis:entry colname="col4">
                    <xref ref-type="bibr" rid="bib1.bibx41" id="text.12"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Wind direction</oasis:entry>
         <oasis:entry colname="col2">Wind speed and direction transmitter (YOKOGAWA WA7601)</oasis:entry>
         <oasis:entry colname="col3">8751/8760</oasis:entry>
         <oasis:entry colname="col4">
                    <xref ref-type="bibr" rid="bib1.bibx41" id="text.13"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Relative humidity</oasis:entry>
         <oasis:entry colname="col2">Capacitance hygrometer (VISALA HUMICAP HMP155)</oasis:entry>
         <oasis:entry colname="col3">8751/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Carbon monoxide (CO)</oasis:entry>
         <oasis:entry colname="col2">GC/RGD (Peak Performer 2, Peak Laboratories)</oasis:entry>
         <oasis:entry colname="col3">8604/8760</oasis:entry>
         <oasis:entry colname="col4">
                    <xref ref-type="bibr" rid="bib1.bibx49" id="text.14"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ethane (C<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">Preconcentration/GC/MS</oasis:entry>
         <oasis:entry colname="col3">5600/8760</oasis:entry>
         <oasis:entry colname="col4">
                    <xref ref-type="bibr" rid="bib1.bibx35" id="text.15"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Propane (C<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">Preconcentration/GC/MS</oasis:entry>
         <oasis:entry colname="col3">5600/8760</oasis:entry>
         <oasis:entry colname="col4">
                    <xref ref-type="bibr" rid="bib1.bibx35" id="text.16"/>
                  </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Nitrogen oxide (NO)</oasis:entry>
         <oasis:entry colname="col2">NO/NO<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/NO<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> analyser (HSS-100, Sonoma Technology Inc.)</oasis:entry>
         <oasis:entry colname="col3">432/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Nitrogen dioxide (NO<inline-formula><mml:math id="M77" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">NO/NO<inline-formula><mml:math id="M78" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/NO<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> analyser (HSS-100, Sonoma Technology Inc.)</oasis:entry>
         <oasis:entry colname="col3">8088/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Nitrogen dioxide (NO<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">NO/NO<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>/NO<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> analyser (HSS-100, Sonoma Technology Inc.)</oasis:entry>
         <oasis:entry colname="col3">8088/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ozone (O<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">UV absorption O<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> analyser (Model 1100, Dylec Inc.)</oasis:entry>
         <oasis:entry colname="col3">8600/8760</oasis:entry>
         <oasis:entry colname="col4">–</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

      <?pagebreak page9231?><p id="d1e1273">Measurements of CO, ethane and propane were made with outside air drawn from a main tower (sampling inlet: 36.5 m above ground and 46.5 m above sea level). CO was measured with a gas chromatograph–reduction gas detector (GC/RGD; Peak Performer 2, Peak Laboratories) <xref ref-type="bibr" rid="bib1.bibx49" id="paren.17"/>. Ethane and propane were measured with an automated preconcentration–gas-chromatography–mass-spectrometry (GC/MS) instrument (7890B/5977B, Agilent Technologies) designed for hourly measurements of natural and anthropogenic halocarbons <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx35" id="paren.18"/>. Ethane and propane measurements were calibrated using a gravimetrically prepared standard gas (Taiyo Nippon Sanso Co. Ltd.).</p>
      <p id="d1e1283">Air for <inline-formula><mml:math id="M85" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mtext mathvariant="italic">y</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and O<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> measurements was drawn from a sub-tower (sampling inlet: 14.8 m above ground and 24.8 m above sea level). Measurements of NO, NO<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> were made by HSS-100 (Sonoma Technology Inc. (STI)) with a blue light converter for NO<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (NO<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> converter) and a molybdenum converter for NO<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> (NO<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> converter) <xref ref-type="bibr" rid="bib1.bibx11" id="paren.19"/>. The conversion efficiencies of the converters were monitored daily with NO<inline-formula><mml:math id="M93" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gas (<inline-formula><mml:math id="M94" display="inline"><mml:mo lspace="0mm">≈</mml:mo></mml:math></inline-formula> 5 ppb) generated by a gas dilution system with gas phase titration (NO<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>: <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mn mathvariant="normal">79</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> %, NO<inline-formula><mml:math id="M97" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>: <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mn mathvariant="normal">98</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> %). The detection limit of the NO measurement was about 2 ppt for 1 min acquisition. Ozone concentration was measured by UV absorption (Dylec 1100, Dylec Co., Ltd), which was calibrated with Standard Reference Photometer No. 35 (National Institute for Standard and Technology) located at NIES.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Meteorological context</title>
      <p id="d1e1442">Over the course of 1 year, the observatory is exposed to air masses from a wide range of locations. We calculate 10 d back trajectories for the site every hour from January to December in 2018 (52 weeks duration) using meteorological data from NCEP Global Forecast System <xref ref-type="bibr" rid="bib1.bibx30" id="paren.20"/> and the FLEXible PARTicle dispersion model (FLEXPART)  <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx44" id="paren.21"/>.</p>
      <?pagebreak page9232?><p id="d1e1451">Figure <xref ref-type="fig" rid="Ch1.F2"/>b shows the ratio of the time that these 10 d trajectories spent over the different regions shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>a. Over the year, most of the air is oceanic in origin from either the North or South Pacific (43 % and 34 %). However, the air masses can also spend a significant fraction of time over inland China (3.6 %), Russia (4.6 %), Korea (1.7 %), Japan (3.9 %), South-East Asia (3.1 %),  the Philippines (1.2 %) and the three east China city regions (Beijing, Shanghai, Hong Kong) (3.7 %).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1460">Trajectory analysis of air arriving at Hateruma: <bold>(a)</bold> location of the regions analysed; <bold>(b)</bold> weekly average percentage of time air masses spent over these regions.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f02.png"/>

        </fig>

      <p id="d1e1476">There is, however, significant seasonal variation in air mass origin. The fraction that is oceanic (North and South Pacific) is lowest in the winter at around 60 % and is more prevalent in the summer at around 80 %.  There is a shift in origin from the North Pacific region in the winter to the South Pacific region in the summer. This pattern can be attributed to the annual meteorological cycle of this region characterized by the East Asian monsoon seasons <xref ref-type="bibr" rid="bib1.bibx41 bib1.bibx55 bib1.bibx56 bib1.bibx57" id="paren.22"/>. For the remaining 20 %–40 % of the time, flow from China, Japan, Korea and Russia dominates in the winter, spring and autumn. During the summer months (April to August), the air originates from a southerly direction (Philippines, South-East Asia, Borneo).</p>
      <p id="d1e1482">The site is therefore mainly subject to relatively clean oceanic air with occasional exposure to air from Russia, Korea and China in the winter and the Philippines, South-East Asia and Borneo in the summer.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Chemical transport model configuration</title>
      <p id="d1e1494">We use a chemical transport model, GEOS-Chem  version 12.7.1 (<ext-link xlink:href="https://doi.org/10.5281/zenodo.3676008" ext-link-type="DOI">10.5281/zenodo.3676008</ext-link>, <xref ref-type="bibr" rid="bib1.bibx45" id="altparen.23"/>) to help analyse the measurements made at Hateruma. The model was first described by <xref ref-type="bibr" rid="bib1.bibx4" id="text.24"/> but has had substantial improvements since then (<uri>https://geoschem.github.io/</uri>, last access: 11 August 2023). We use a regional simulation with a spatial resolution of 0.5<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M100" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> over the domain shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>a. The model includes a detailed HO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–VOC-ozone–halogen–aerosol tropospheric chemistry as described by <xref ref-type="bibr" rid="bib1.bibx40" id="text.25"/> and is driven by offline meteorology from the NASA Global Modelling and Assimilation Office (<uri>http://gmao.gsfc.nasa.gov</uri>, last access: 5 September 2021) forward-processing product (GEOS-FP).</p>
      <p id="d1e1562">To generate restart files and boundary conditions, the model was run in a  global configuration at a 4<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M105" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M106" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal resolution for 2 years (1 January 2017–1 January 2019) with the first year regarded as spin-up. We then run the model in its regional configuration using the boundary conditions derived from the global simulation and output the result every hour. Figures <xref ref-type="fig" rid="App1.Ch1.S1.F12"/>–<xref ref-type="fig" rid="App1.Ch1.S1.F15"/> in the Appendix show a comparison between the model simulations run at the native meteorological resolution of 0.25<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M108" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M109" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and the simulation run at 0.5<inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M111" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M112" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The differences between the two models are minimal, so we adopt the coarser 0.5<inline-formula><mml:math id="M113" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M114" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution version as it is substantially faster to run with only a small degradation in performance.</p>
      <p id="d1e1671">We run the model in a slightly different emission configuration than its default. We use the  Community Emissions Data System (CEDS) emissions with applied monthly and diurnal variability as described in <xref ref-type="bibr" rid="bib1.bibx18" id="text.26"/> for all anthropogenic emissions other than for those from aircraft where we use the Aviation Emissions Inventory Code (AEIC) <xref ref-type="bibr" rid="bib1.bibx42" id="paren.27"/>. This contrasts with the model default configuration which uses <xref ref-type="bibr" rid="bib1.bibx51" id="text.28"/> and <xref ref-type="bibr" rid="bib1.bibx54" id="text.29"/> for anthropogenic ethane and propane emissions but does makes our simulation consistent with recent Coupled Model Intercomparison Project (CMIP) model evaluations <xref ref-type="bibr" rid="bib1.bibx15" id="paren.30"/>. The CEDS emissions were available at 0.1<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution and the Harmonized Emissions Component (HEMCO) module <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx25" id="paren.31"/>) interpolates all emissions to the grid resolution (0.5<inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M118" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) of the model.</p>
      <p id="d1e1727">We also include geological emissions of ethane and propane that may represent a normally missing source <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx7" id="paren.32"/>. We assume a global total of 3.0 Tg yr<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> of ethane and 1.7 Tg yr<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> of propane <xref ref-type="bibr" rid="bib1.bibx7" id="paren.33"/>. We spatially distribute these emissions using a geological methane emission dataset <xref ref-type="bibr" rid="bib1.bibx8" id="paren.34"/>. This source represents only 10 %–20 % of the global emissions of both ethane and propane, and we do not believe that these geological emissions are of specific importance for this region.</p>
      <p id="d1e1764">Other emissions include offline soil NO<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx53" id="paren.35"/> and online lightning NO<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions <xref ref-type="bibr" rid="bib1.bibx28" id="paren.36"/>. The PARANOX ship plume model by <xref ref-type="bibr" rid="bib1.bibx19" id="text.37"/>, which calculates the ageing of emissions in ship exhaust plumes for NO<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, HNO<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> was applied to the CEDS shipping emissions  <xref ref-type="bibr" rid="bib1.bibx18" id="paren.38"/>.  Biomass burning emissions use the Global Fire Emissions Database GFED 4.1 <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx2 bib1.bibx13 bib1.bibx32 bib1.bibx52" id="paren.39"/>. Biogenic emissions follow the estimation from the Model of Emissions of Gases and Aerosols from Nature (MEGAN) 2.1 <xref ref-type="bibr" rid="bib1.bibx16" id="paren.40"/>. The natural emissions of acetaldehyde follow the calculation from <xref ref-type="bibr" rid="bib1.bibx26" id="text.41"/>. Natural sources of NH<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>  are adapted from the Global Emission InitiAtive (GEIA) as described by <xref ref-type="bibr" rid="bib1.bibx5" id="text.42"/>, with the inclusion of the Arctic seabird emissions <xref ref-type="bibr" rid="bib1.bibx34" id="paren.43"/>.</p>
      <p id="d1e1850">Table <xref ref-type="table" rid="Ch1.T2"/> gives the list of simulations performed and the sections in which these simulations are discussed.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1858">Summary of GEOS-Chem model simulations and reference sections.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model simulation</oasis:entry>
         <oasis:entry colname="col2">Type</oasis:entry>
         <oasis:entry colname="col3">Section</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1st</oasis:entry>
         <oasis:entry colname="col2">Base simulation</oasis:entry>
         <oasis:entry colname="col3">3 and 5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2nd</oasis:entry>
         <oasis:entry colname="col2">No-shipping emission simulation</oasis:entry>
         <oasis:entry colname="col3">3.7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">3rd</oasis:entry>
         <oasis:entry colname="col2">North Asian biomass burning emission turned off</oasis:entry>
         <oasis:entry colname="col3">4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">4th</oasis:entry>
         <oasis:entry colname="col2">South Asian biomass burning emission turned off</oasis:entry>
         <oasis:entry colname="col3">4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5th</oasis:entry>
         <oasis:entry colname="col2">Scaled anthropogenic emission simulation 1</oasis:entry>
         <oasis:entry colname="col3">5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">6th</oasis:entry>
         <oasis:entry colname="col2">Scaled anthropogenic emission simulation 2</oasis:entry>
         <oasis:entry colname="col3">5</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{2}?></table-wrap>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Model results and performance</title>
      <p id="d1e1971">In order to assess the veracity of the GEOS-Chem model simulation we compare its performance: first against the meteorological observations made at the site and then against measurements of atmospheric chemical constituents. Since the model and observation data are available  hourly and observation data capture is high in most cases, instances of missing data were dropped for both the observation and the model before comparison. The observation data were adjusted from Japan standard time (JST) to model default time (UTC). We compare hourly values from the observations and from the<?pagebreak page9233?> model for the physical and chemical variables except for NO, NO<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>, where we compare local daylight averages due to high variability.</p>
      <p id="d1e1992">We use a number of standard metrics for describing the measurements and model (mean, median, standard deviation, 25th and 75th percentiles). When assessing the model performance we assess this in terms of the root mean square error (RMSE), mean bias and Pearson's correlation coefficient (<inline-formula><mml:math id="M130" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>). We also calculate the slope of the best-fit lines using orthogonal distance regression (ODR).</p>
      <p id="d1e2002">In the case of wind direction, which is circular and not linear, the methodology for the estimation of RMSE and bias follows <xref ref-type="bibr" rid="bib1.bibx10" id="text.44"/> and <xref ref-type="bibr" rid="bib1.bibx6" id="text.45"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2014">Observed and modelled <bold>(a)</bold> wind direction, <bold>(b)</bold> wind speed , <bold>(c)</bold> temperature and <bold>(d)</bold> relative humidity at Hateruma.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f03.png"/>

      </fig>

<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Meteorological variables</title>
      <p id="d1e2042">Figure <xref ref-type="fig" rid="App1.Ch1.S2.F16"/> in Appendix B shows the wind rose representing observed and modelled wind speed and direction at the site. As the populated part of the island lies to the west of the site, this highlights that the local contamination is likely small. Figure <xref ref-type="fig" rid="Ch1.F3"/> shows a comparison between the hourly observed and modelled time series for wind speed, wind direction, temperature and relative humidity at the observatory.</p>
      <p id="d1e2049">The wind direction (10 m above surface) is plotted in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a as the incidence angle of the wind (north: 0  and 360<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). The observations are given with a resolution of 22.5<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> clockwise, which gives them a blocky appearance. Overall, the model captured the observed wind direction well throughout the year with few discrepancies. The modelled wind direction has a low RMSE (6.5<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) and a slightly positive bias (6.5<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). This could be attributed to a small error in meteorological fields used in our simulations or to potentially a small error in the measurements. The seasonal variability in wind direction is well represented in Fig. <xref ref-type="fig" rid="Ch1.F3"/>b, with the summer time characterized by winds coming from the south and the winter having winds from a more northerly direction.</p>
      <p id="d1e2093">The modelled wind speed has a correlation coefficient (<inline-formula><mml:math id="M135" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) of 0.90 and a RMSE of 2.17 m s<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F3"/>b). The wind speeds are lower in the model (mean of 6.43 <inline-formula><mml:math id="M137" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.12 (1<inline-formula><mml:math id="M138" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) m s<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) than in the observations (mean of 7.83 <inline-formula><mml:math id="M140" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.79 (1<inline-formula><mml:math id="M141" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) m s<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). This may reflect local reductions in wind speed over the island due to increased surface drag not being represented in the model due to its grid resolution.</p>
      <p id="d1e2170">Surface temperatures (2 m above surface) show a high degree of correlation (<inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.92</mml:mn></mml:mrow></mml:math></inline-formula>) and a  RMSE of 1.75 <inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, with the mean observed surface temperature (24.53 <inline-formula><mml:math id="M145" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4.27 (1<inline-formula><mml:math id="M146" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) <inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) close to that simulated (24.76 <inline-formula><mml:math id="M148" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3.67 (1<inline-formula><mml:math id="M149" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) <inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). There is, however, significant hourly variation not captured by the model (Fig. <xref ref-type="fig" rid="Ch1.F3"/>c). This again could be due to resolution impacts at different scales since the island is smaller than the model grid box at Hateruma. Local heating and cooling at the observatory and the island will not be represented in the model fields.</p>
      <?pagebreak page9234?><p id="d1e2244">The modelled surface relative humidity (RH at 2 m above the surface in Fig. <xref ref-type="fig" rid="Ch1.F3"/>d) is less well captured (<inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.77</mml:mn></mml:mrow></mml:math></inline-formula>; RMSE <inline-formula><mml:math id="M152" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 11.26 %), with the modelled mean (73.09 <inline-formula><mml:math id="M153" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 9.89 (1<inline-formula><mml:math id="M154" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) %) lower than the observed mean (82.00 <inline-formula><mml:math id="M155" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10.32 (1<inline-formula><mml:math id="M156" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) %). This difference could again be attributed to the sub-grid issues where the meteorology used in the model is on a fairly coarse scale compared to the observations.</p>
      <p id="d1e2297">In general, the model performance compared to the meteorological observations is relatively good, reflecting the observational data assimilated into the GEOS-FP meteorological fields. We can now assess the model performance in simulating the mixing ratio of the trace gases observed at the site.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Carbon monoxide</title>
      <p id="d1e2308">Figure <xref ref-type="fig" rid="Ch1.F4"/>a (left) shows the time series of CO measured and modelled at the site, with Fig. <xref ref-type="fig" rid="Ch1.F4"/>a (right) showing the correlation between the hourly modelled and measured values. Mixing ratios are highest in the winter months reflecting transport from north Asia (China, Korea, Japan) and the North Pacific (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and lower oxidation by OH in the winter months <xref ref-type="bibr" rid="bib1.bibx37" id="paren.46"/>. The mixing ratios are lower in the summer reflecting transport from southern regions (they are further away and typically have lower emissions) and increased oxidation due to enhanced OH concentrations in the summer <xref ref-type="bibr" rid="bib1.bibx37" id="paren.47"/>. <xref ref-type="bibr" rid="bib1.bibx23" id="text.48"/> measured CO in northern Japan and reported a similar seasonality in CO mixing ratios over the year.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2329">Modelled and measured hourly <bold>(a)</bold> CO, <bold>(b)</bold> C<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and <bold>(c)</bold> C<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios calculated for the Hateruma site.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f04.png"/>

        </fig>

      <p id="d1e2384">Over the year, the model simulates the CO mixing ratio well with a mean value of 146 <inline-formula><mml:math id="M161" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 77 (1<inline-formula><mml:math id="M162" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) ppbv compared to mean observations of 136 <inline-formula><mml:math id="M163" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 62 (1<inline-formula><mml:math id="M164" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) ppbv. The median CO mixing ratios calculated and measured are 127 and 122 ppbv, respectively. The 25th and 75th percentile modelled is 89 and 180 ppbv compared to 89 and 169 ppbv observed. There is a good degree of correlation (<inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.74</mml:mn></mml:mrow></mml:math></inline-formula>) between the model and measurements with a RMSE of 53 ppbv and the line of best fit having a slope of 0.91.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2430">Modelled and measured mean daytime <bold>(a)</bold> NO, <bold>(b)</bold> NO<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and <bold>(c)</bold> NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios calculated for Hateruma.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Ethane</title>
      <?pagebreak page9235?><p id="d1e2474">Similar to CO, the highest observed ethane (C<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>) mixing ratios occur in the winter, while the mixing ratios in the summer are substantially lower (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b – left). The model results underestimate the mean mixing ratio (972 <inline-formula><mml:math id="M170" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 541 (1<inline-formula><mml:math id="M171" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv) compared to the observations (1188 <inline-formula><mml:math id="M172" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 842 (1<inline-formula><mml:math id="M173" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv)) with a RMSE of 481 pptv. Also, a median mixing ratio is calculated to be 942 pptv, with a 25th to 75th percentile spread of 552–1386 ppbv, while the median from observation is 1134 pptv with a spread of 368–1825 pptv. This underestimate in modelled ethane results is most noticeable in the winter months. However, in the summer the model outputs can give overestimates. This leads to two populations in the model–measurement scatter plot (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b – right) with a strongly correlated but overestimated population at observed mixing ratios below 500 pptv (in the summer) and another population with underestimated mixing ratios above this (in winter). The correlation coefficient between model outputs and measurements is relatively high at 0.88, but the linear fit between model results and measurements is dominated by the wintertime underestimate to give a slope of 0.57.</p>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Propane</title>
      <p id="d1e2536">Figure <xref ref-type="fig" rid="Ch1.F4"/>c (left) shows the comparison between the measured and modelled time series for propane (C<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>). A similar pattern to C<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> is seen with high wintertime mixing ratios and much lower values in the summer. Unlike C<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> though, a summer time overestimate is not evident. The model captures much of the variability in the C<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios with a correlation coefficient of 0.89 (Fig. <xref ref-type="fig" rid="Ch1.F4"/>c – right). The mean mixing ratio of C<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> is 391 <inline-formula><mml:math id="M184" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 432 (1<inline-formula><mml:math id="M185" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv for the measurements and 210 <inline-formula><mml:math id="M186" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 198 (1<inline-formula><mml:math id="M187" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv for the model. The median C<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio calculated and measured is 156 pptv (25th and 75th percentiles of 69 and 335 pptv) and 221 pptv (25th and 75th percentiles of 62 and 611 pptv), respectively. The RMSE is 320 pptv, and the slope of the linear fit between calculated results and measurements is 0.41. Thus, similar to the situation with C<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, the model substantially underestimates C<inline-formula><mml:math id="M192" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios.</p>
</sec>
<sec id="Ch1.S4.SS5">
  <label>4.5</label><?xmltex \opttitle{$\mathrm{NO}_{x}$}?><title>
          <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
        </title>
      <p id="d1e2738">Here, we evaluate the model's performance in simulating NO and NO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (collectively known as NO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>). The short lifetime of NO and NO<inline-formula><mml:math id="M197" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (on the order of minutes to hours during the day) makes evaluation against model data difficult due to large and rapid variations. During the day NO mixing ratios are high due to the photolysis of NO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. During the night, away from recent emissions, its mixing ratios are effectively zero.  For this evaluation, we compare mean day values (06:00 to 18:00 local time) between the model results and observations. Figure <xref ref-type="fig" rid="Ch1.F5"/>a shows the comparison between the measured and modelled daytime mean for the NO mixing ratio. The mean observed value (7 <inline-formula><mml:math id="M199" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 28 (1<inline-formula><mml:math id="M200" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv) is substantially lower than the modelled value (21 <inline-formula><mml:math id="M201" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 41 (1<inline-formula><mml:math id="M202" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv). The model also shows very little skill in the day-to-day variability with an <inline-formula><mml:math id="M203" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> of 0.03 and a slope of 0.5 for the linear fit.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e2817">Modelled and measured hourly <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios calculated for the Hateruma site.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f06.png"/>

        </fig>

      <p id="d1e2837">Figure <xref ref-type="fig" rid="Ch1.F5"/>b (left) compares the time series of daily average <inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> between the measured and modelled, with Fig. <xref ref-type="fig" rid="Ch1.F5"/>b (right) showing the relationship as a scatter plot and best-fit line. The model simulates <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> better than <inline-formula><mml:math id="M207" display="inline"><mml:mi mathvariant="normal">NO</mml:mi></mml:math></inline-formula>. The mean <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratio measured is 260 <inline-formula><mml:math id="M209" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 185 (1<inline-formula><mml:math id="M210" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv, while the modelled <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mean mixing ratio is 182 <inline-formula><mml:math id="M212" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 323 (1<inline-formula><mml:math id="M213" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv. The median <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratio observed is 198 pptv with a 25th and 75th percentile range of 127 and 335 pptv, whereas the calculated ratio is 121 pptv, with a 25th to 75th percentile range of 97 and 152 pptv. The correlation coefficient between observation and measurement is, however, low (0.36) with a RMSE of 322 pptv, and the slope of the linear fit is 0.65.</p>
      <?pagebreak page9236?><p id="d1e2937">Generally, the model performance for the NO<inline-formula><mml:math id="M215" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> species is poorer than  for other species. This likely reflects a number of problems. It is difficult to make observations at these low concentrations <xref ref-type="bibr" rid="bib1.bibx33" id="paren.49"/>, and for many days the NO observations are below the detection limit. It also likely reflects the short lifetime of NO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> making it susceptible to local chemical and emissions processes which the model cannot resolve. Summer NO and NO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> observed at Hateruma is higher than model estimates, which is similar to the observations by <xref ref-type="bibr" rid="bib1.bibx17" id="text.50"/> over Mongolia where thermally decomposed peroxyacetyl nitrate (PAN) during the warmer season contributes to higher NO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels in remote regions. However, in general the modelled NO<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> at Hateruma (dominated by NO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) underestimates the observed values.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e3004">Mean and standard deviations in mixing ratios of measured and modelled species over different seasons between 1 January 2018–31 December 2018.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right" colsep="1"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry namest="col2" nameend="col3" align="center" colsep="1">Spring </oasis:entry>
         <oasis:entry namest="col4" nameend="col5" align="center" colsep="1">Summer </oasis:entry>
         <oasis:entry namest="col6" nameend="col7" align="center" colsep="1">Autumn </oasis:entry>
         <oasis:entry namest="col8" nameend="col9" align="center">Winter </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Measured</oasis:entry>
         <oasis:entry colname="col3">Modelled</oasis:entry>
         <oasis:entry colname="col4">Measured</oasis:entry>
         <oasis:entry colname="col5">Modelled</oasis:entry>
         <oasis:entry colname="col6">Measured</oasis:entry>
         <oasis:entry colname="col7">Modelled</oasis:entry>
         <oasis:entry colname="col8">Measured</oasis:entry>
         <oasis:entry colname="col9">Modelled</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CO (ppbv)</oasis:entry>
         <oasis:entry colname="col2">177 <inline-formula><mml:math id="M221" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 56</oasis:entry>
         <oasis:entry colname="col3">178 <inline-formula><mml:math id="M222" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 73</oasis:entry>
         <oasis:entry colname="col4">99 <inline-formula><mml:math id="M223" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 49</oasis:entry>
         <oasis:entry colname="col5">100 <inline-formula><mml:math id="M224" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 54</oasis:entry>
         <oasis:entry colname="col6">110 <inline-formula><mml:math id="M225" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 45</oasis:entry>
         <oasis:entry colname="col7">120 <inline-formula><mml:math id="M226" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 51</oasis:entry>
         <oasis:entry colname="col8">160 <inline-formula><mml:math id="M227" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 61</oasis:entry>
         <oasis:entry colname="col9">187 <inline-formula><mml:math id="M228" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>  85</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">C<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> (pptv)</oasis:entry>
         <oasis:entry colname="col2">1854 <inline-formula><mml:math id="M231" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 611</oasis:entry>
         <oasis:entry colname="col3">1382 <inline-formula><mml:math id="M232" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 441</oasis:entry>
         <oasis:entry colname="col4">458 <inline-formula><mml:math id="M233" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 415</oasis:entry>
         <oasis:entry colname="col5">554 <inline-formula><mml:math id="M234" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 366</oasis:entry>
         <oasis:entry colname="col6">579 <inline-formula><mml:math id="M235" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 476</oasis:entry>
         <oasis:entry colname="col7">698 <inline-formula><mml:math id="M236" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 359</oasis:entry>
         <oasis:entry colname="col8">1638 <inline-formula><mml:math id="M237" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 691</oasis:entry>
         <oasis:entry colname="col9">1249 <inline-formula><mml:math id="M238" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 468</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">C<inline-formula><mml:math id="M239" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M240" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> (pptv)</oasis:entry>
         <oasis:entry colname="col2">588 <inline-formula><mml:math id="M241" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 416</oasis:entry>
         <oasis:entry colname="col3">314 <inline-formula><mml:math id="M242" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 195</oasis:entry>
         <oasis:entry colname="col4">105 <inline-formula><mml:math id="M243" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 187</oasis:entry>
         <oasis:entry colname="col5">79 <inline-formula><mml:math id="M244" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 86</oasis:entry>
         <oasis:entry colname="col6">154 <inline-formula><mml:math id="M245" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 242</oasis:entry>
         <oasis:entry colname="col7">118 <inline-formula><mml:math id="M246" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 117</oasis:entry>
         <oasis:entry colname="col8">646 <inline-formula><mml:math id="M247" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 473</oasis:entry>
         <oasis:entry colname="col9">332 <inline-formula><mml:math id="M248" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>  212</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO (pptv)</oasis:entry>
         <oasis:entry colname="col2">3 <inline-formula><mml:math id="M249" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 9</oasis:entry>
         <oasis:entry colname="col3">20 <inline-formula><mml:math id="M250" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 28</oasis:entry>
         <oasis:entry colname="col4">16 <inline-formula><mml:math id="M251" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 49</oasis:entry>
         <oasis:entry colname="col5">19 <inline-formula><mml:math id="M252" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6</oasis:entry>
         <oasis:entry colname="col6">6 <inline-formula><mml:math id="M253" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18</oasis:entry>
         <oasis:entry colname="col7">17 <inline-formula><mml:math id="M254" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 16</oasis:entry>
         <oasis:entry colname="col8">6 <inline-formula><mml:math id="M255" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 17</oasis:entry>
         <oasis:entry colname="col9">30 <inline-formula><mml:math id="M256" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 74</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (pptv)</oasis:entry>
         <oasis:entry colname="col2">276 <inline-formula><mml:math id="M258" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 160</oasis:entry>
         <oasis:entry colname="col3">169 <inline-formula><mml:math id="M259" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 166</oasis:entry>
         <oasis:entry colname="col4">222 <inline-formula><mml:math id="M260" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 178</oasis:entry>
         <oasis:entry colname="col5">132 <inline-formula><mml:math id="M261" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 42</oasis:entry>
         <oasis:entry colname="col6">229 <inline-formula><mml:math id="M262" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 190</oasis:entry>
         <oasis:entry colname="col7">123 <inline-formula><mml:math id="M263" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 74</oasis:entry>
         <oasis:entry colname="col8">316 <inline-formula><mml:math id="M264" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 193</oasis:entry>
         <oasis:entry colname="col9">296 <inline-formula><mml:math id="M265" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>  602</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<inline-formula><mml:math id="M266" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> (pptv)</oasis:entry>
         <oasis:entry colname="col2">1183 <inline-formula><mml:math id="M267" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 882</oasis:entry>
         <oasis:entry colname="col3">1497 <inline-formula><mml:math id="M268" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1296</oasis:entry>
         <oasis:entry colname="col4">383 <inline-formula><mml:math id="M269" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 518</oasis:entry>
         <oasis:entry colname="col5">839 <inline-formula><mml:math id="M270" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1078</oasis:entry>
         <oasis:entry colname="col6">440 <inline-formula><mml:math id="M271" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 432</oasis:entry>
         <oasis:entry colname="col7">890 <inline-formula><mml:math id="M272" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1080</oasis:entry>
         <oasis:entry colname="col8">751 <inline-formula><mml:math id="M273" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 572</oasis:entry>
         <oasis:entry colname="col9">1467 <inline-formula><mml:math id="M274" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1678</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">O<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>   (ppbv)</oasis:entry>
         <oasis:entry colname="col2">47 <inline-formula><mml:math id="M276" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 13</oasis:entry>
         <oasis:entry colname="col3">46 <inline-formula><mml:math id="M277" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 14</oasis:entry>
         <oasis:entry colname="col4">28 <inline-formula><mml:math id="M278" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 18</oasis:entry>
         <oasis:entry colname="col5">27 <inline-formula><mml:math id="M279" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>  12</oasis:entry>
         <oasis:entry colname="col6">33 <inline-formula><mml:math id="M280" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 16</oasis:entry>
         <oasis:entry colname="col7">29 <inline-formula><mml:math id="M281" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11</oasis:entry>
         <oasis:entry colname="col8">43 <inline-formula><mml:math id="M282" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 7</oasis:entry>
         <oasis:entry colname="col9">40 <inline-formula><mml:math id="M283" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 9</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{3}?></table-wrap>

</sec>
<sec id="Ch1.S4.SS6">
  <label>4.6</label><?xmltex \opttitle{NO${}_{y}$}?><title>NO<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula></title>
      <p id="d1e3776">Figure <xref ref-type="fig" rid="Ch1.F5"/>c (left) shows the daily average measured and modelled time series for gas phase reactive nitrogen species (NO<inline-formula><mml:math id="M285" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>). We define here NO<inline-formula><mml:math id="M286" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> for the model as NO <inline-formula><mml:math id="M287" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M288" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M289" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula>N<inline-formula><mml:math id="M291" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M292" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M293" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M295" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M297" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> PAN (which will tend to marginally underestimate the true modelled NO<inline-formula><mml:math id="M298" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> as it misses halogen nitrates and some other minor constituents such as NO<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and some organic nitrates). We assumed that none of the particulate nitrate is measured. Figure <xref ref-type="fig" rid="Ch1.F5"/>c (right) shows the scatter plot with the line of best fit between measurements and calculations. The mean observed NO<inline-formula><mml:math id="M300" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratio is 683 <inline-formula><mml:math id="M301" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 698 (1<inline-formula><mml:math id="M302" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv, while the mean modelled NO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratio is 1173 <inline-formula><mml:math id="M304" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1340 (1<inline-formula><mml:math id="M305" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv. The correlation coefficient between observation and model calculations is 0.79 with a RMSE of 1035 pptv. The slope of the best-fit line is 1.55.  Thus, the model appears to overestimate NO<inline-formula><mml:math id="M306" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios by roughly 50 % despite not including some of the NO<inline-formula><mml:math id="M307" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> species and the potential for some particulate NO<inline-formula><mml:math id="M308" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> being sampled by the observations.
The model performance is better than for NO<inline-formula><mml:math id="M309" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>.  However, whereas the NO<inline-formula><mml:math id="M310" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> appears to be underestimated in the model, the NO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> is overestimated. HNO<inline-formula><mml:math id="M312" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and PAN are dominant in the model-estimated NO<inline-formula><mml:math id="M313" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> levels at Hateruma. Thus, the NO<inline-formula><mml:math id="M314" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> overestimate and the NO<inline-formula><mml:math id="M315" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> underestimate could be related to NO<inline-formula><mml:math id="M316" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> formation and loss pathways <xref ref-type="bibr" rid="bib1.bibx17" id="paren.51"/>.</p>
      <p id="d1e4062">A simulation without shipping emissions within the high-resolution domain reduces NO<inline-formula><mml:math id="M317" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios by 25 %. Thus, even switching off these emissions entirely does not compensate fully for the model overestimate and makes the model underestimation of NO<inline-formula><mml:math id="M318" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> worse. It is therefore unclear why the model overestimates the NO<inline-formula><mml:math id="M319" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios. This could indicate excessive emissions in the region, too long a modelled NO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> lifetime or some difficulty in the model chemistry. Further work will be necessary to understand NO<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> in the region.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e4122">Percentage change in <bold>(a)</bold> C<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M324" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, <bold>(b)</bold> C<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, <bold>(c)</bold> CO, <bold>(d)</bold> O<inline-formula><mml:math id="M327" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, <bold>(e)</bold> NO<inline-formula><mml:math id="M328" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> and <bold>(f)</bold> NO<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios between standard and simulations without north Asian or south Asian biomass burning.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e4217">C<inline-formula><mml:math id="M330" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M333" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> modelled plotted against measurements in the base simulation (<bold>a</bold> and <bold>d</bold>) and scaled anthropogenic emission simulations with initial correction factor (<bold>b</bold> and <bold>e</bold>) and optimized correction factor (<bold>c</bold> and <bold>f</bold>). Data are split into a southern-flow period (July–September) in blue and a northern-flow period (October–June) in red. <inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M335" display="inline"><mml:mrow><mml:msub><mml:mi>S</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> give the slope of the line of best fit for the time series in southern- and northern-flow periods, respectively.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS7">
  <label>4.7</label><title>Ozone</title>
      <p id="d1e4312">Figure <xref ref-type="fig" rid="Ch1.F6"/> (left) shows the measured and modelled time series for O<inline-formula><mml:math id="M336" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. In general, the model performs well (RMSE of 8 ppbv; mean measured O<inline-formula><mml:math id="M337" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> of 38 <inline-formula><mml:math id="M338" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 16 (1<inline-formula><mml:math id="M339" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) ppbv; mean model O<inline-formula><mml:math id="M340" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> of 36 <inline-formula><mml:math id="M341" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 14 (1<inline-formula><mml:math id="M342" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) ppbv) and simulates much of the variability with a correlation coefficient (<inline-formula><mml:math id="M343" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) of 0.87. However, the line of best fit between observations and model results is low, with a slope of 0.76 (Fig. <xref ref-type="fig" rid="Ch1.F6"/> – right).  The median O<inline-formula><mml:math id="M344" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio calculated is 35 ppbv (25th and 75th percentiles of 22 and 46 ppbv), whereas the corresponding measurement is 40 ppbv (25th and 75th percentiles of 24 and 49 ppbv).</p>
      <p id="d1e4391">During the summer, there are periods of low O<inline-formula><mml:math id="M345" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, reaching 6.5 ppbv. The model fails to capture these low mixing ratios and simulated a minimum of 10 ppbv. Conversely, in the winter months, the model reproduces much of the variability but has a tendency to underestimate the observed mixing ratios. Overall, this leads to overestimates for low mixing ratios and underestimates for high mixing ratios. Thus, there is a reduced slope of the linear fit in the scatter plot (Fig. <xref ref-type="fig" rid="Ch1.F6"/>).</p>
</sec>
<sec id="Ch1.S4.SS8">
  <label>4.8</label><title>Summary</title>
      <p id="d1e4413">In general the model has some skill at picking out the variations in meteorological history of the air masses arriving at the site, reflected in the generally high correlation coefficients between the model and the measurements. This mainly reflects the quality of the data assimilation used in the NASA-generated meteorological fields. The success in simulating the absolute mixing ratios is more varied. Table <xref ref-type="table" rid="Ch1.T3"/> summarizes the mean calculated and measured mixing ratios for spring (February–April), summer (May–July), autumn (August–October) and winter (November–January).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e4420">Time series of hourly <inline-formula><mml:math id="M346" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <bold>(a)</bold> and  <inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <bold>(b)</bold> observed and modelled mixing ratios (scaled anthropogenic emission simulation 2).</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f09.png"/>

        </fig>

      <p id="d1e4467">There is a clear seasonality in the observations at Hateruma, and this is similar to other oceanic sites in East Asia. Such a seasonality is reported at Cape Ochi-ishi (43<inline-formula><mml:math id="M348" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>10′ N, 145<inline-formula><mml:math id="M349" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>30′ E)  and the Oki Islands (36<inline-formula><mml:math id="M350" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>17′ N, 133<inline-formula><mml:math id="M351" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>11′ E), where Asian outflows amplifies the winter concentrations of hydrocarbons <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx39" id="paren.52"/>. While NO<inline-formula><mml:math id="M352" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> has a very short atmospheric lifetime and its formation and loss are related to NO<inline-formula><mml:math id="M353" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> species such as HNO<inline-formula><mml:math id="M354" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and PAN, it is reported to have different seasonality in polluted and remote regions <xref ref-type="bibr" rid="bib1.bibx17" id="paren.53"/>.</p>
      <p id="d1e4541">As shown in Table <xref ref-type="table" rid="Ch1.T3"/>, carbon monoxide mixing ratios are relatively well simulated in all seasons with a small bias toward high values in the autumn and winter. Ethane is underestimated in the spring and winter but overestimated in the summer and autumn. Propane mixing ratios are underestimated in all seasons. NO<inline-formula><mml:math id="M355" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> observations are overestimated by the model, whereas NO and NO<inline-formula><mml:math id="M356" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios are underestimated.</p>
      <p id="d1e4564">Although the largest divergences in the model results compared to observations are found for NO<inline-formula><mml:math id="M357" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M358" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> species, there is uncertainty about the accuracy of these measurements at such low mixing ratios. Thus, we focus on the hydrocarbons in which we have more confidence. The model underestimates  C<inline-formula><mml:math id="M359" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M360" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M361" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M362" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios especially in the spring and winter. We therefore conduct a number of model experiments to investigate these observations. We first run simulations to assess the role of biomass burning in controlling the mixing ratios of these species at the site, we then assess how much the Asian anthropogenic source of these compounds would have to increase by in order to give agreement between the model and the measurements in the winter months.</p>
</sec>
</sec>
<?pagebreak page9237?><sec id="Ch1.S5">
  <label>5</label><title>Biomass burning sources</title>
      <p id="d1e4632">In order to understand the impact of biomass burning on the composition of the air arriving at the site, we conduct an additional simulation, switching off the biomass burning emissions from north Asia and South Asia separately as shown in Fig. <xref ref-type="fig" rid="App1.Ch1.S2.F17"/>. Two global simulations were run switching off the northern or southern Asian biomass burning to generate new boundary conditions, and then these were used for the two regional simulations which again switched off the biomass burning in either the north or south of Asia.</p>
      <p id="d1e4637">Figure <xref ref-type="fig" rid="Ch1.F7"/>a–f show the time series of the percentage change in modelled mixing ratios of C<inline-formula><mml:math id="M363" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M364" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, C<inline-formula><mml:math id="M365" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M366" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, CO, O<inline-formula><mml:math id="M367" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M368" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M369" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> at the site when biomass burning emissions in either the northern or southern domain are switched off. Given the short lifetime of NO<inline-formula><mml:math id="M370" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M371" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, the site is less sensitive to biomass burning NO<inline-formula><mml:math id="M372" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> than CO, C<inline-formula><mml:math id="M373" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M374" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M375" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M376" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, and Fig. <xref ref-type="fig" rid="Ch1.F7"/>d and f show the correlation between O<inline-formula><mml:math id="M377" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M378" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> when less ozone is formed due to switching off emissions, more NO<inline-formula><mml:math id="M379" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is accumulated.</p>
      <p id="d1e4800">During the winter months the contributions from north and South Asia are relatively small; however, in the summer, both sources can contribute significantly (20 %–35 %) to the modelled C<inline-formula><mml:math id="M380" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M381" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, C<inline-formula><mml:math id="M382" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M383" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> and CO. The contributions are smaller for O<inline-formula><mml:math id="M384" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> reaching a maximum at 10 % during events in the summer. There is a sharp dip around 10 August where CO, C<inline-formula><mml:math id="M385" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M386" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M387" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M388" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula> levels drop by around 40 %–50 % due to switching off north Asian biomass burning emissions. After this sharp dip, the next decline from 16 August was more sustained and due to South Asian biomass burning emission. These sharp dips correspond to the passing of typhoons in the area, which can rapidly draw air from different direction for short period of time. Figure <xref ref-type="fig" rid="App1.Ch1.S2.F18"/> shows the back-trajectory analysis for this period when the wind direction rapidly changed. There<?pagebreak page9238?> is also a tendency for increased Asian fire activity in the summer which explains why the strong and rapidly changing wind would bring in more emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e4890">Scatter plot showing hourly <bold>(a)</bold> <inline-formula><mml:math id="M389" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <bold>(b)</bold> <inline-formula><mml:math id="M390" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios between observation mixing ratios and  model calculations with scaling (scaled anthropogenic emission simulation 2). Red dashed line shows best-fit line before scaling.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f10.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e4939">Percentage changes in average July mixing ratios of <bold>(a)</bold> OH and <bold>(b)</bold> O<inline-formula><mml:math id="M391" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> after increasing Asian ethane and propane anthropogenic emissions.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f11.png"/>

      </fig>

      <p id="d1e4963">The periods of model overestimate in summer ethane, notably in August (Fig. <xref ref-type="fig" rid="Ch1.F4"/>b), correspond to periods with a high fraction of modelled ethane biomass burning (<inline-formula><mml:math id="M392" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 30 %). However, the model overestimate (see Fig. <xref ref-type="fig" rid="Ch1.F4"/>b) is much large than this (<inline-formula><mml:math id="M393" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 100 %). Thus, even if the biomass burning is switched off all together, the model overestimate during the summer would still remain. This suggests that the model overestimate of C<inline-formula><mml:math id="M394" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M395" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> in the summer is not primarily related to the modelled representation of biomass burning but likely results in uncertainties in the anthropogenic emissions of ethane south of Hateruma.</p>
      <p id="d1e5003">During the wintertime the model underestimates the observed ethane and propane. This is a period when the contribution from biomass burning is relatively low (<inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> %). Thus<?pagebreak page9239?> the potential for the underestimate in wintertime ethane and propane to be related to errors in the biomass burning appears to be small. Instead, we now evaluate how much the Asian anthropogenic source of ethane and propane would have to be increased by in order to fit the observed mixing ratios.</p>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Anthropogenic emissions</title>
      <p id="d1e5024">The period between October to June (Figs. <xref ref-type="fig" rid="Ch1.F4"/>–<xref ref-type="fig" rid="Ch1.F6"/>) is characterized by elevated levels of pollution at the site due to flow from Russia, China, Korea and Japan (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). It is also a period when the model substantially underestimates the mixing ratios of ethane and propane. In this section we explore what scaling factor would have to be applied to the Asian anthropogenic emissions of ethane and propane within the high-resolution domain to better fit those observations.</p>
      <p id="d1e5033">Figure <xref ref-type="fig" rid="Ch1.F8"/>a and d show modelled ethane and propane plotted against observations in our base model. We separate the plot into two periods here as southern flow (blue, July–September) and northern flow (red, October–June). It is obvious from the comparison that during the northern-flow period, the model-measured slope is lower than expected (0.62 for ethane and 0.41 propane), whereas in the southern-flow period it is substantially overestimated for ethane (3.97) and to a smaller extent also for propane (1.51).</p>
      <p id="d1e5038">Given the site's largest exposure to relatively recent north Asian emissions in the northern-flow period, we focus on this. We multiply the Asian anthropogenic emission of ethane and propane within the high-resolution domain by a first rough estimate of a correction factor “A” (1.75 for ethane and 2.58 for propane, which are roughly the reciprocal of the model– measurement slopes show in Fig. <xref ref-type="fig" rid="Ch1.F8"/>, i.e. 1<inline-formula><mml:math id="M397" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>0.62 and 1<inline-formula><mml:math id="M398" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>0.41) aimed at making the slope of the linear fit in the northern-flow period become 1. This would represent a correction factor if all of the ethane and propane observed at the site were from within the high-resolution simulation domain and the oxidation lifetimes were correct.</p>
      <p id="d1e5057">The annual simulation was re-run with the anthropogenic emissions of ethane and propane increased by the A factor within the “Asian” high-resolution domain (Fig. <xref ref-type="fig" rid="Ch1.F8"/>b and e). Assuming a linear response, these two simulations allow the mixing ratios of ethane and propane in the base simulation to be represented as <inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">Asian</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mrow><mml:mi mathvariant="normal">Rest</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">the</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">world</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and the mixing ratios in the simulation with increased emissions to be represented as  <inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.75</mml:mn><mml:mo>×</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">Asian</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mrow><mml:mi mathvariant="normal">Rest</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">the</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">world</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for ethane and <inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:mo>]</mml:mo><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.58</mml:mn><mml:mo>×</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mi mathvariant="normal">Asian</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mi>X</mml:mi><mml:msub><mml:mo>]</mml:mo><mml:mrow><mml:mi mathvariant="normal">Rest</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">the</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">world</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for propane. The base mixing ratios at each time point can then be decomposed to give an Asian component (although this is only the component within the higher-resolution domain) and a “Rest of the world” component. A scaling can then be applied, which optimizes the fit between the measurement and the model by finding an optimized multiplier for the Asian emission: <inline-formula><mml:math id="M402" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">optimized</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e5216">The value of <inline-formula><mml:math id="M403" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">optimized</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is found to be 2.22 and 3.17 for ethane and propane, respectively, if the best-fit line is optimized (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). This is consistent with the value found by optimizing the ratio of mean mixing ratios in the period when the wind flow is northerly (calculated as 2.24 and 3.14, for ethane and propane, respectively). Re-running the model with these increases in the ethane and propane emissions within the domain gives a scatter plot of ethane and propane measurements versus model values in Fig. <xref ref-type="fig" rid="Ch1.F8"/>c and f, a time series shown in Fig. <xref ref-type="fig" rid="Ch1.F9"/>, and a correlation between the whole dataset in Fig. <xref ref-type="fig" rid="Ch1.F10"/>. The  correlation coefficient (<inline-formula><mml:math id="M404" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) is slightly reduced after the scaling (0.88 to 0.84 and 0.89 to 0.86 for <inline-formula><mml:math id="M405" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and  <inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, respectively).</p>
      <?pagebreak page9240?><p id="d1e5278">For the northern-flow period (October to June), when the air is predominantly off north Asia, the modelled ethane now has a mean of 1443 <inline-formula><mml:math id="M407" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 737 (1<inline-formula><mml:math id="M408" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv compared to an observed mean of 1449 <inline-formula><mml:math id="M409" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 725 (1<inline-formula><mml:math id="M410" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv. The propane simulation has a mean of 493 <inline-formula><mml:math id="M411" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 418 (1<inline-formula><mml:math id="M412" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv compared to an observed mean of  494 <inline-formula><mml:math id="M413" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 407 (1<inline-formula><mml:math id="M414" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv. During the southern-flow period (July–September), the model now significantly overestimates the ethane (mean simulated <inline-formula><mml:math id="M415" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 587 <inline-formula><mml:math id="M416" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 352 (1<inline-formula><mml:math id="M417" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv; mean observed <inline-formula><mml:math id="M418" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 308 <inline-formula><mml:math id="M419" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 99 (1<inline-formula><mml:math id="M420" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv) and propane (mean simulated <inline-formula><mml:math id="M421" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 105 <inline-formula><mml:math id="M422" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 88 (1<inline-formula><mml:math id="M423" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv; mean observed <inline-formula><mml:math id="M424" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 60 <inline-formula><mml:math id="M425" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 37 (1<inline-formula><mml:math id="M426" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) pptv).</p>
      <p id="d1e5424">The improvement in model performance during the northern flow and the degradation in performance during the southern flow point towards a non-uniformity in the correction factor. This could indicate a  difference in the seasonality of the emissions compared to those used in <xref ref-type="bibr" rid="bib1.bibx18" id="text.54"/> with a significant reduction in the summer time emissions compared to the winter, or it could indicate a different reason for the increase in north Asia compared to south Asia, which is primarily sampled in the summer.</p>
      <p id="d1e5430">The comparison of ethane and propane observations with model results shows that a large increase in the prescribed emissions of these tracers is necessary, in agreement with previous studies. <xref ref-type="bibr" rid="bib1.bibx7" id="text.55"/> found it necessary to increase CEDS anthropogenic ethane emissions by a factor of roughly 2 and CEDS propane emission by a factor of nearly 3 to get agreement between their model and observations. These are very similar to the ratios found here.   <xref ref-type="bibr" rid="bib1.bibx51" id="text.56"/> found it necessary to substantially increase anthropogenic ethane sources to fit observations. <xref ref-type="bibr" rid="bib1.bibx27" id="text.57"/> measured vertical profiles of VOCs (including C<inline-formula><mml:math id="M427" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M428" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> and C<inline-formula><mml:math id="M429" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M430" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>) and reported that emission fluxes were up to 3 times larger than in the Multi-resolution Emission Inventory for China (MEIC) inventory estimates. It seems likely that current estimates of north Asian emissions of ethane and propane are currently underestimated.</p>
      <p id="d1e5479">Figure <xref ref-type="fig" rid="Ch1.F11"/>a and b show the impact of the increase (with the optimized factors) in Asian ethane and propane anthropogenic emissions on the mixing ratios of average hydroxyl radical and ozone in the region in July, respectively. This is the period of the highest ozone mixing ratios over China. The effect on the OH mixing ratios in July was small and patchy with up to a 2 % reduction in some places. On the other hand, O<inline-formula><mml:math id="M431" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios increased slightly, reaching a maximum over Beijing, where that amounts to a 2 % (around 1 ppbv) increase.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d1e5501">Measurements were made of a number of compounds in the air over the island of Hateruma (CO, C<inline-formula><mml:math id="M432" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M433" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>, C<inline-formula><mml:math id="M434" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M435" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:math></inline-formula>, NO, NO<inline-formula><mml:math id="M436" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M437" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M438" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>).  We show that the site is mainly subject to clean Pacific air throughout the year. If the site is subject to polluted air masses, these are more likely to have originated from north Asia (Russia, China, Japan, Korea, etc.) in the winter months and from south Asia (Philippines, Borneo and other regions in South-East Asia including Vietnam, Indonesia, peninsular Malaysia and Thailand) in the summer months. This gives the site a significant seasonal cycle in the mixing ratios of pollutants considered in this study except NO<inline-formula><mml:math id="M439" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>.</p>
      <p id="d1e5577"><?xmltex \hack{\newpage}?>We have compared these observations to the output of the GEOS-Chem model, run in a regional configuration. We find that CO and O<inline-formula><mml:math id="M440" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> are well simulated; the model overestimates NO<inline-formula><mml:math id="M441" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> observations but tends to  underestimates NO, NO<inline-formula><mml:math id="M442" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, ethane and propane.</p>
      <p id="d1e5608">The underestimates in ethane and propane during the wintry months are unlikely to be reconciled by increases in biomass burning emissions but could be reconciled by substantial (factors of 2–3) increases in the Asian anthropogenic source of these compounds (consistent with previous studies). These large increases in emissions have negligible influence on the hydroxyl radical mixing ratios and very little impact on the ozone in the region's  cities such as Beijing, where there is up to 1 ppbv change in ozone mixing ratios in July.</p>
      <p id="d1e5611">We do not believe the overestimates of NO<inline-formula><mml:math id="M443" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula> can be attributed to problems with the simulation of shipping NO<inline-formula><mml:math id="M444" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, as even switching off the shipping NO<inline-formula><mml:math id="M445" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions does not remove the overestimate. Also, biomass burning emissions can only contribute up to 10 % of NO<inline-formula><mml:math id="M446" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> levels estimated at the site; therefore, the overestimates likely lies in the emissions of NO<inline-formula><mml:math id="M447" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> from industrial regions close by, in issues with the chemistry or in the observations.</p>
      <p id="d1e5660">The site's location is unusual and is subject to air masses from a large number of sites and so can be used to understand emissions of compounds from a number of location. Future plans to enhance the measurement capability at the site with a gas-chromatography–mass-spectrometry system (GC-MS) should allow an evaluation of a large number of different organic compounds, further enhancing the capacity to understand sources of pollution in the region.</p>
</sec>

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

<app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Comparison of simulation resolutions</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F12"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e5676">Modelled time series comparing <inline-formula><mml:math id="M448" display="inline"><mml:mi mathvariant="normal">CO</mml:mi></mml:math></inline-formula> simulation at 0.25<inline-formula><mml:math id="M449" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M450" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M451" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 0.5<inline-formula><mml:math id="M452" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M453" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M454" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution at the site.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f12.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F13"><?xmltex \currentcnt{A2}?><?xmltex \def\figurename{Figure}?><label>Figure A2</label><caption><p id="d1e5745">Modelled time series comparing <inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulation at 0.25<inline-formula><mml:math id="M456" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M457" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M458" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 0.5<inline-formula><mml:math id="M459" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M460" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M461" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution at the site.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f13.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F14"><?xmltex \currentcnt{A3}?><?xmltex \def\figurename{Figure}?><label>Figure A3</label><caption><p id="d1e5819">Modelled time series comparing <inline-formula><mml:math id="M462" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulation at 0.25<inline-formula><mml:math id="M463" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M464" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M465" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 0.5<inline-formula><mml:math id="M466" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M467" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M468" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution at the site.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f14.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F15"><?xmltex \currentcnt{A4}?><?xmltex \def\figurename{Figure}?><label>Figure A4</label><caption><p id="d1e5897">Modelled time series comparing <inline-formula><mml:math id="M469" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulation at 0.25<inline-formula><mml:math id="M470" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M471" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.3125<inline-formula><mml:math id="M472" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and 0.5<inline-formula><mml:math id="M473" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M474" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.625<inline-formula><mml:math id="M475" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution at the site.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f15.png"/>

      </fig>

<?xmltex \hack{\vspace*{122mm}}?><?xmltex \hack{\newpage}?>
</app>

<?pagebreak page9241?><app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><title>Other figures</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F16"><?xmltex \currentcnt{B1}?><?xmltex \def\figurename{Figure}?><label>Figure B1</label><caption><p id="d1e5986">Wind rose for <bold>(a)</bold> observed and <bold>(b)</bold> modelled wind speed (m s<inline-formula><mml:math id="M476" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and direction  at Hateruma.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f16.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F17"><?xmltex \currentcnt{B2}?><?xmltex \def\figurename{Figure}?><label>Figure B2</label><caption><p id="d1e6015">Annual mean biomass burning emission flux for C<inline-formula><mml:math id="M477" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M478" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula> in 2018 (GFED). Regions indicated are the north and South Asia region, which had biomass burning emissions switched off in the simulations. The Asia box extends from 46 to 180<inline-formula><mml:math id="M479" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E; north Asia box covers 82 to 24<inline-formula><mml:math id="M480" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, while South Asia spans <inline-formula><mml:math id="M481" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> to 24<inline-formula><mml:math id="M482" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f17.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F18"><?xmltex \currentcnt{B3}?><?xmltex \def\figurename{Figure}?><label>Figure B3</label><caption><p id="d1e6083">Back-trajectory analysis showing air masses arriving at Hateruma between <bold>(a)</bold> 10–11 August and <bold>(b)</bold> 16–17 August.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/9229/2023/acp-23-9229-2023-f18.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e6104">Hateruma observation data are available from the Global Environmental Database (GED)
<ext-link xlink:href="https://doi.org/10.17595/20230217.001" ext-link-type="DOI">10.17595/20230217.001</ext-link> <xref ref-type="bibr" rid="bib1.bibx36" id="paren.58"/>. GEOS-Chem model output is also available from GED
<ext-link xlink:href="https://doi.org/10.17595/20230707.001" ext-link-type="DOI">10.17595/20230707.001</ext-link> <xref ref-type="bibr" rid="bib1.bibx1" id="paren.59"/>. GEOS-Chem version 12.7.1 was used in this project <ext-link xlink:href="https://doi.org/10.5281/zenodo.3676008" ext-link-type="DOI">10.5281/zenodo.3676008</ext-link> <xref ref-type="bibr" rid="bib1.bibx45" id="paren.60"/>, and input data files for GEOS-Chem can be downloaded from <uri>http://geoschemdata.wustl.edu</uri> <xref ref-type="bibr" rid="bib1.bibx46" id="paren.61"/>.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e6135">AA ran the GEOS-Chem simulations and made the analysis and visualization of the model outputs. MR contributed the FLEXPART model outputs and visualization. ME, SA, AL and TS developed the project. ME assisted in the analysis and interpretation of all model outputs. TS provided the ethane and propane observations. YT contributed the CO data while SH, HM and HT provided the <inline-formula><mml:math id="M483" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi mathvariant="normal">y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and O<inline-formula><mml:math id="M484" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> observations used in model validation. The paper was written by AA and ME with contributions from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e6172">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e6178">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e6185">This project was undertaken on the Viking Cluster, which is a high-performance computing facility provided by the University of York. We are grateful for computational support from the University of York High Performance Computing service, Viking and the Research Computing team.
We thank staff members of the Global Environmental Forum Foundation (GEFF) for their help in running the instruments at Hateruma station.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e6190">This research has been supported by UK Research and Innovation (grant no. NE/S012273/1) and the Japan Society for the Promotion of Science (grant no. JSP-SJRP20181708).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e6196">This paper was edited by Andrea Pozzer and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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