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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-26-14051-2026</article-id><title-group><article-title>Constraints on <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission in Thailand using GEMS satellite data</article-title><alt-title>Constraints on <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission in Thailand using GEMS satellite data</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff3">
          <name><surname>Thongsame</surname><given-names>Worapop</given-names></name>
          <email>t.worapop@gmail.com</email>
        <ext-link>https://orcid.org/0009-0009-1706-627X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Henze</surname><given-names>Daven K.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Pfister</surname><given-names>Gabriele</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9177-1315</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Kumar</surname><given-names>Rajesh</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3135-9556</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Barth</surname><given-names>Mary</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Paul M. Rady Mechanical Engineering, University of Colorado Boulder, Boulder, CO 80309, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>National Science Foundation, National Center for Atmospheric Research, Boulder, CO 80301, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Center for Atmospheric Science Research, National Astronomical Research Institute of Thailand, Chiang Mai 50180, Thailand</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Worapop Thongsame (t.worapop@gmail.com)</corresp></author-notes><pub-date><day>7</day><month>October</month><year>2026</year></pub-date>
      
      <volume>26</volume>
      <issue>19</issue>
      <fpage>14051</fpage><lpage>14072</lpage>
      <history>
        <date date-type="received"><day>22</day><month>April</month><year>2026</year></date>
           <date date-type="rev-request"><day>20</day><month>May</month><year>2026</year></date>
           <date date-type="rev-recd"><day>13</day><month>August</month><year>2026</year></date>
           <date date-type="accepted"><day>3</day><month>September</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Worapop Thongsame et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026.html">This article is available from https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e157">Nitrogen oxides (<inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:math></inline-formula>) are key pollutants that contribute to ozone and secondary aerosol formation, posing environmental and health risks. Accurate simulation and forecasting of <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> pollution is essential for developing mitigation strategies. Local inventories in Thailand are infrequently updated, leading researchers to use global inventories such as CAMS-GLOB-ANT for simulation. Global inventories carry uncertainties due to assumptions in emission factors, outdated activity data, and coarse temporal resolution. To address these limitations, this study applies a top-down approach to update <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Thailand using the iterative finite difference mass balance (IFDMB) method. Tropospheric <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column densities (VCDs) from GEMS version 3 are integrated with the WRF-Chem to refine CAMS-GLOB-ANT emissions for September 2023. The simulations with posterior emissions are evaluated against TROPOMI <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs and surface <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentration. Results show that the baseline simulation overestimates <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs across Thailand compared with GEMS, except in North Thailand. GEMS reports substantially higher <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> than TROPOMI – particularly over Lampang – reflecting retrieval uncertainty associated with the a priori profiles used in version 3. Consequently, IFDMB reduces <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions across most regions but increases in the North. The increase is attributed primarily to a retrieval artifact rather than to a genuine emission underestimate. Baseline <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Thailand are 35 852 Mg per month with North Thailand and 30 699 Mg per month without North. Our posterior emissions over three IFDMB schemes are 25 994, 34 808, and 36 870 Mg per month with North, and 15 376, 26 523, and 27 087 Mg per month without North. These adjustments improve model bias and error relative to GEMS. However, when evaluated against TROPOMI, we find an increase in the bias for North Thailand, likely due to discrepancies between GEMS and TROPOMI retrievals. These discrepancies highlight the importance of future retrieval algorithm improvement and calibration across satellite products. Comparisons to surface observations indicate that IFDMB shifts the <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> peak to later than observations. This is because observations are strongly influenced by local transportation sources, which are hard to observe and retrieved by GEMS and the model, respectively.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Aeronautics and Space Administration</funding-source>
<award-id>80NSSC22K1047</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Center for Atmospheric Research</funding-source>
<award-id>1852977</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e307">Nitrogen oxides (<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>) are significant air pollutants that impact both the environment and human health. In the atmosphere, the suite of <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> chemical reactions can lead to the formation of aerosol nitrate and ozone, worsening air quality (Adams et al., 2001; Philip et al., 2014; Thompson, 1992). The atmospheric deposition of <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> products and its potential for oxidation contribute to the acidification of soil (Zhang et al., 2012). For human health impacts, long-term exposure to <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is associated with increased mortality rates due to respiratory issues and cardiovascular diseases (Eum et al., 2022; Ji et al., 2015). In Thailand, 10 % of adult mortality in 2009 is attributable to <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> exposure (Pinichka et al., 2017). The primary sources of <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are anthropogenic, mainly from the combustion of fossil fuels in automobiles, power plants, and industrial activities (Cooper et al., 2017; Delmas et al., 1997). In urban areas of Thailand, such as Bangkok, vehicle emissions are the primary contributors to <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> levels (Uttamang et al., 2018). Conversely, in suburban areas like Rayong, the main sources of <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions are industrial activities (Poboon et al., 2012; Thawonkaew, 2016).</p>
      <p id="d2e415">Ground-based monitoring stations provide highly accurate measurements of hourly <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios; however, their spatial coverage is limited (Jeong and Hong, 2021). Moreover, <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> highly depends on localized sources (Crippa et al., 2023; Miyazaki et al., 2017) and has a short atmospheric lifetime (Horner et al., 2024), leading to sharp spatial gradients and strong heterogeneity in ambient concentrations (Li et al., 2023a). As a result, chemical transport models (CTMs) have become a widely adopted approach for studying <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and its impact on ozone as well as aerosol (Chen et al., 2013; Kim et al., 2024; Opio et al., 2022). Accurate simulation and forecasting of <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations require accurate anthropogenic emission inventories (Miyazaki et al., 2017). Traditionally, anthropogenic emissions are developed from a bottom-up method, i.e., using emission factors and activity data to generate emissions (Cooper et al., 2017; Crippa et al., 2023; Ding et al., 2017). However, this approach often introduces significant uncertainties due to assumptions made regarding emission factors and activity data (Martin et al., 2003). Furthermore, bottom-up inventories take time to collect, prepare, and process, making them potentially outdated in rapidly changing regions (Ding et al., 2017; Lamsal et al., 2011; Liu et al., 2016). Alternatively, top-down methods, which leverage satellite data, provide potentially more accurate and near-real-time emissions (Lin et al., 2010; Yang et al., 2021).</p>
      <p id="d2e462">Over the past two decades, various inverse methods using satellite observation to provide top-down emissions have emerged, such as Kalman filters, 4D-VAR, and mass balance (Cooper et al., 2017; Miyazaki et al., 2017; Napelenok et al., 2008; Qu et al., 2019). Among these, the mass balance method requires lower computational intensity for top-down emission constraining (Cooper et al., 2017; De Foy et al., 2014). This method is particularly effective for near-real-time updating of emissions using satellite observations (Lamsal et al., 2011). For constraining <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions, the mass balance method assumes a linear relationship between observed <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column density (VCD) and top-down <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions within a model grid cell, an assumption based on negligible horizontal transport when the lifetime of <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is short relative to the average transport time across a single grid cell of the model (Martin et al., 2003). However, <inline-formula><mml:math id="M30" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can still disperse to adjacent grid cells, especially given the higher resolution of more contemporary air quality models, leading to a smearing error (Cooper et al., 2017). This error results in underestimations of emission changes at the source and can erroneously overestimate changes in downwind regions (Turner et al., 2012). An iterative approach has been proposed to address this issue by progressively shifting the adjustment from neighboring grid cells toward actual sources through repeated updates (Ghude et al., 2013). Additionally, the relationship between <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission and <inline-formula><mml:math id="M32" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs is non-linear due to non-linear chemistry (Jena et al., 2015). The finite difference mass balance method has been developed to account for the non-linearity between emissions and <inline-formula><mml:math id="M33" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs (Cooper et al., 2017; Li et al., 2019). This improves accuracy by accounting for the sensitivity of changes in <inline-formula><mml:math id="M34" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs to emissions, thus providing a refined tool to tackle the challenges associated with the smearing problem (Lamsal et al., 2011).</p>
      <p id="d2e565">For the past few decades, <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> monitoring has relied on sun-synchronous Low Earth Orbit (LEO) satellites (e.g., GOME, SCIAMACHY, OMI, and TROPOMI) that provide a global map of tropospheric <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Boersma et al., 2008; Martin et al., 2003; Tang et al., 2013). With oversampling techniques, these instruments can resolve spatial features finer than 1 km (Jin et al., 2025). However, LEO satellites have limited temporal sampling, which can miss rapid changes or diurnal patterns of <inline-formula><mml:math id="M37" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Kim et al., 2023). To address the challenges in data availability, Geostationary Earth Orbit (GEO) satellites, which have higher temporal resolution than the LEO satellite, have been launched (Choi, 2018; Seo et al., 2025; Yang et al., 2024). The Geostationary Environment Monitoring Spectrometer (GEMS) is a GEO satellite for air quality monitoring from space, providing unprecedented temporal resolution and continuous observational capabilities that are not feasible with LEO satellites (Kim et al., 2023). This satellite is designed to measure air pollutants, including <inline-formula><mml:math id="M38" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, sulfur dioxide (<inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), formaldehyde (HCHO), and aerosols, over Asia (Kim et al., 2020). The hourly <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data from GEMS can provide improvement for anthropogenic emissions (Park et al., 2023) and information about <inline-formula><mml:math id="M41" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> diurnal variability (Park et al., 2024).</p>
      <p id="d2e647">In this study, we explore the potential of GEMS satellite data for updating anthropogenic <inline-formula><mml:math id="M42" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions over Thailand. Given the significant health impacts associated with <inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> exposure, accurate simulations are essential for developing effective mitigation policies. However, the lack of a local emission inventory poses a major limitation. Hence, our objective is to improve the accuracy of <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions used in air quality models and to assess diurnal variations in emissions. We employ a series of mass balance methods for adjusting anthropogenic <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions and utilize WRF-Chem to simulate <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations in Thailand. The analysis focuses on September 2023 – a period characterized by minimal biomass burning – allowing a clearer evaluation of anthropogenic emission contributions.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methodology</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>WRF-Chem</title>
      <p id="d2e720">We use the Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) version 4.2.2 (Fast et al., 2006; Grell et al., 2005) to simulate <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations over Thailand. The model domain and configuration, including grid nudging, largely follow Thongsame et al. (2024). The MOZART-MOSAIC with aqueous phase chemistry (Emmons et al., 2010; Knote et al., 2014; Zaveri et al., 2008) scheme is used for chemical and aerosol schemes. This scheme includes interactions of the aerosols with radiation and clouds. The online MEGAN version 2.04 (Guenther et al., 2006) and offline FINN versions 2.5 (Wiedinmyer et al., 2023) are used to represent biogenic and biomass burning emissions, respectively. Anthropogenic emissions are taken from the CAMS-GLOB-ANT v5.3 inventory (Granier et al., 2019), and the initial and boundary conditions come from the Whole Atmosphere Community Climate Model (WACCM; Granier et al., 2019). Figure 1 shows the distribution of <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions from CAMS-GLOB-ANT.</p>

      <fig id="F1"><label>Figure 1</label><caption><p id="d2e747">Spatial distribution of <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions from CAMS-GLOB-ANT in September 2023. BMR is the Bangkok Metropolitan Region.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f01.png"/>

        </fig>

      <p id="d2e767">The simulation employs 42 vertical layers extending to approximately 63 hPa, with a horizontal resolution of <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mn mathvariant="normal">9</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">9</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>. The model tropopause is located at approximately 100 hPa. To compare with GEMS, WRF-Chem <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations are interpolated to GEMS vertical pressure levels. Tropospheric <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD from WRF-Chem is then calculated by integrating <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the surface to the GEMS-defined tropopause at 230 hPa. The GEMS averaging kernel is applied to the model-simulated <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles to account for the satellite's retrieval sensitivity, following previous approaches (Cooper et al., 2020; Park et al., 2024). The averaging kernel accounts for the sensitivity of the satellite and is applied to the model to mitigate uncertainties in the retrieval algorithm. Further details regarding the averaging kernels and the applied equations are provided in Sect. S6 in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>GEMS</title>
      <p id="d2e842">GEMS is an ultraviolet-visible instrument that measures back-scattered solar spectra in the 300–500 nm wavelength range (Kim et al., 2020). It is a geostationary orbit satellite, which was launched in February 2020, with a resolution of <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.5</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">8</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (Kim et al., 2023). The GEMS data span from November 2022 to the present, covering a geographical domain from 75 to 145° E and 5° S to 45° N (Park et al., 2024). Tropospheric <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs are retrieved using a Differential Optical Absorption Spectroscopy (DOAS) algorithm, applied over the 432–450 nm spectral window (Kim et al., 2023). Several studies have demonstrated strong correlations between GEMS <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and ground-based measurements in regions such as China and South Korea (Kim et al., 2023; Li et al., 2023b; Seo et al., 2025).</p>
      <p id="d2e886">For this research, we utilize version 3 of the GEMS Level 2 tropospheric <inline-formula><mml:math id="M58" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD (<uri>https://nesc.nier.go.kr/en/html/index.do</uri>, last access: 27 December 2024) in September 2023 for the Thailand area. For September 2023, the dataset provides up to 10 consecutive hourly snapshots of tropospheric <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD during daylight, from 00:45 to 07:45 UTC, with additional observations at 22:45 and 23:45 UTC.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e916"><bold>(a)</bold> Monthly average tropospheric <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD in September 2023 from GEMS with arrows indicating striping artifacts. The number of GEMS data per grid cell <bold>(b)</bold> and <bold>(c)</bold> the monthly average error, <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, after removing striping artifacts.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f02.png"/>

        </fig>

      <p id="d2e956">For this analysis, we select data between 00:45–04:45 and 06:45–07:45 UTC (07:45–11:45 and 13:45–14:45 LT), which collectively cover over 50 % of Thailand. As the GEMS scan at 05:45 UTC does not extend to Thailand, the 05:45 UTC data are linearly interpolated from adjacent hours (04:45 and 06:45 UTC) for updating the emission with the mass balance method. To ensure data quality, we retain only pixels with a cloud fraction below 0.3 (Park et al., 2024). We also filter data based on the final algorithm quality flag, a metric representing the reliability of each pixel's retrieval. Although a flag of 0 indicates an ideal measurement from the perspective of algorithmic issues, a systematic surface reflectance issue in GEMS version 3 prevents most pixels from achieving this score. Consequently, we use pixels with a quality flag of 0 or 1, ensuring sufficient data coverage while excluding severely degraded retrievals. Additionally, we have found striping artifacts present in the GEMS data (Fig. 2a). To ensure data quality and improve the reliability of the emission adjustment process, we manually remove these from our analysis. The data coverage in North Thailand is limited, and retrieval errors are relatively high in both North Thailand and the Bangkok Metropolitan Region (Fig. 2b and c). In GEMS version 3, the tropopause pressure level is assumed to be fixed at 230 hPa across all pixels. As GEMS does not publicly release full a priori model profiles required to change the tropopause in the algorithm, we are constrained to adopt the 230 hPa definition to ensure consistency between the satellite retrieval and our WRF-Chem model. Our sensitivity test using WRF-Chem reveals that a fixed tropopause at 230 hPa and the model's varying tropopause have a negligible impact during the daytime. This is because the <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Thailand during September is overwhelmingly dominated by near-surface emissions, and the <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> beyond 230 hPa is almost zero everywhere in Thailand.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>TROPOMI</title>
      <p id="d2e989">TROPOMI (TROPOspheric Monitoring Instrument) is a nadir-viewing UV–Visible spectrometer aboard Sentinel-5P that measures solar radiation backscattered from the Earth to retrieve atmospheric trace gases such as <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, HCHO, <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and CO (Judd et al., 2020; Veefkind et al., 2012). In this study, we use the Level 2 tropospheric <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD product from TROPOMI version 2, which represents the <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> amount between the surface and tropopause. The TROPOMI tropospheric <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrieval uses a DOAS technique in the 405–465 nm spectral window, and its horizontal resolution is approximately <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.5</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">5.5</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (Judd et al., 2020; Zhao et al., 2020).</p>
      <p id="d2e1089">For comparison with WRF-Chem simulations, we filter the TROPOMI data to retain only retrievals with a quality assurance value (qa_value) greater than 0.5, thereby excluding pixels affected by clouds, snow/ice, or retrieval artifacts. To ensure consistency in vertical sensitivity between the satellite and model data, we apply the TROPOMI-provided averaging kernels to the model-simulated <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> profiles. The TROPOMI satellite provides data around 10:30 am–01:30 pm LT for Thailand. The model outputs at the closest time to TROPOMI are used for comparison.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Ground-based monitoring data</title>
      <p id="d2e1111">For ground-based monitoring data, we use the data from the Pollution Control Department (PCD) of Thailand air quality stations (<uri>http://air4thai.pcd.go.th/webV3/</uri>, last access: 20 December 2024) to evaluate surface <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations from WRF-Chem. The PCD stations' measurements are based on the chemiluminescence technique, which detects <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  species (Pollution Control Department, 2022; Zhang et al., 2009). Hence, we compare WRF-Chem <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  (which includes <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>X</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  and its oxidation products) with <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from PCD. The PCD stations (20) are classified into roadside (14) and non-roadside stations (6) as shown in Fig. S14 in the Supplement. On average, the simulated <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  concentrations from WRF-Chem is higher than <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> by 5 % at the roadside stations and 6 % at the non-roadside stations.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Mass balance method</title>
<sec id="Ch1.S2.SS5.SSS1">
  <label>2.5.1</label><title>Finite difference mass balance</title>
      <p id="d2e1211">The mass balance method assumes a linear relationship between posterior <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions (<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and observed <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns (<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) (Martin et al., 2003). This approach directly utilizes the information from the observed and simulated <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns, but does not account for the uncertainties associated with emissions or satellite retrievals (Cooper et al., 2017). The finite difference mass balance (FDMB) method, which integrates information from prior emissions, observations, and their uncertainties through a Bayesian inversion, is more robust and physically reasonable (Drinkwater et al., 2023; Watanabe et al., 2023). This method formulates a cost function, <inline-formula><mml:math id="M85" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>, that penalizes deviations from observations and from prior emissions, and seeks the emissions that minimize <inline-formula><mml:math id="M86" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>. The total cost function is defined as the sum of a prediction error term (model–observation mismatch) and an emission error term (departure from the prior emissions):

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M87" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>J</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mo mathsize="1.1em">(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo mathsize="1.1em">)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mo mathsize="1.1em">(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo mathsize="1.1em">)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            where <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> is the squared difference between observed and modeled <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD, weighted by the uncertainty of the observation. The second term, <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, penalizes large adjustments to the emissions from the prior, by squaring the difference between the optimized emissions <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and prior <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, weighted by the prior uncertainty. <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the observation and emissions errors, respectively. In this study, we assume a 50 % relative uncertainty for the prior emissions based on previous studies (Jung et al., 2022; Park et al., 2024; Souri et al., 2020). The observation error is derived from the root mean square error (RMSE) in GEMS data, which is calculated from the spectral fitting residuals resulting from the DOAS (Differential Optical Absorption Spectroscopy) method in the spectral window between 432 and 450 nm. All of the terms in the above equation pertain to values in a single grid cell. The approach is applied independently across all grid cells in Thailand.</p>
      <p id="d2e1505">As <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is often quite low (on the order of 10 % or less of <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), the cost function in Eq. (2) can become overly sensitive to the prediction error term, potentially leading to overfitting. To prevent this, we introduce a regularization term <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to inflate the denominator of the first term. In contrast, <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is significantly small in background areas, where emissions are close to zero. This leads Eq. (2) to become sensitive to the parameter error term and results in underfitting. Consequently, we add another regularization term <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the second term. These regularization parameters effectively limit the influence of the prediction/parameter error term, thereby balancing the relative weights of the model–observation mismatch and the prior deviation terms. The low value of <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> leads to overfitting the solution to observations, while the high value of <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> leads to overfitting the solution to the prior, and vice versa for <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. As <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> only quantify relative errors, the <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> terms can also be interpreted as absolute contributions to the total observation and emissions errors, respectively, such as a detection limit for the former. In this study, we treat these regularization parameters as known (or estimated) fixed statistical values rather than tuning variables. For the <inline-formula><mml:math id="M107" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> values, we use <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">molec</mml:mi><mml:mo>.</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and 10 <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>  for <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. These numbers are based on the GEMS detection limit and background <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission near the Bangkok area. However, we also explore two more regularization parameters: <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">molec</mml:mi><mml:mo>.</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, representing the background tropospheric column in urban areas near Bangkok, and <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, representing emissions in rural areas. The sensitivity test of four combinations is performed to understand the impact of regularized parameters on the IFDMB. The short information is presented in Sect. 3.2, and full information is in Sect. S1.</p>
      <p id="d2e1825">In this study, we use the analytic solution for the mass balance method from Cooper et al. (2017) for the FDMB method. To solve for posterior emission (<inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>t</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), we minimize the cost function in Eq. (3), and the updated emission as:

              <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M119" display="block"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>t</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>E</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>g</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math id="M120" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> is the gain factor that describes the sensitivity of the inversion to the observations (<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) given the relative weighting of the uncertainties in emissions (<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and in tropospheric <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD (<inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>):

              <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M125" display="block"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>h</mml:mi><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msup><mml:mi>h</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo mathsize="1.1em">(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo mathsize="1.1em">)</mml:mo><mml:mo>+</mml:mo><mml:mo mathsize="1.1em">(</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo mathsize="1.1em">)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math id="M126" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> is from Cooper et al. (2017):

              <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M127" display="block"><mml:mrow><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:msub><mml:mi>E</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

            In the above, <inline-formula><mml:math id="M128" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula> is a factor accounting for the sensitivity of the modeled <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD change due to changes in emissions. <inline-formula><mml:math id="M130" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> quantifies the sensitivity of the fractional change in the tropospheric <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD to <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions (Lamsal et al., 2011),

              <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M133" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>E</mml:mi></mml:mrow><mml:mi>E</mml:mi></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mi mathvariant="normal">Ω</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:math></disp-formula>

            where <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>E</mml:mi></mml:mrow></mml:math></inline-formula> is the difference between baseline and perturbed <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions, and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:math></inline-formula> is the difference between the <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD of WRF-Chem from baseline and perturbed <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions. As noted in Cooper et al. (2017), the magnitude of the emissions perturbation used for <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>E</mml:mi></mml:mrow></mml:math></inline-formula> impacts the value of <inline-formula><mml:math id="M140" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>. For stability, we apply a 10 % perturbation to determine <inline-formula><mml:math id="M141" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, and we constrain <inline-formula><mml:math id="M142" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> to be in the range of 0.1–10.</p>
      <p id="d2e2196">The form of <inline-formula><mml:math id="M143" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> in Eq. (4) shows that if the prior uncertainty (<inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>a</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) is large relative to the observational uncertainty (<inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), the gain factor <inline-formula><mml:math id="M146" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> approaches 1, meaning the observations strongly influence the posterior emissions. Conversely, if the observations are very uncertain or the model is insensitive (small <inline-formula><mml:math id="M147" display="inline"><mml:mi>h</mml:mi></mml:math></inline-formula>), <inline-formula><mml:math id="M148" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> becomes small, and the solution remains closer to the prior emissions (<inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi>E</mml:mi><mml:mi>a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). This Bayesian formulation thus provides a balanced update to emissions, taking into account both the reliability of the observations and the confidence in prior emission estimates.</p>
</sec>
<sec id="Ch1.S2.SS5.SSS2">
  <label>2.5.2</label><title>Iteration</title>
      <p id="d2e2283">An iterative approach is applied to the finite difference mass balance methods. In this study, <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions are updated iteratively until the <inline-formula><mml:math id="M151" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> is minimized. The sensitivity factor (<inline-formula><mml:math id="M152" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>) is recalculated after each iteration to reflect changes in the <inline-formula><mml:math id="M153" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> response to updated emissions. By continuously updating <inline-formula><mml:math id="M154" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, the method aims to better capture the prevailing <inline-formula><mml:math id="M155" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  chemical regime under the observed <inline-formula><mml:math id="M156" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> column concentrations, rather than relying solely on sensitivities derived from the prior model state.</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e2355">Summary of emission update configurations and corresponding mass balance methods.</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">Update scheme</oasis:entry>
         <oasis:entry colname="col2">Update Scope</oasis:entry>
         <oasis:entry colname="col3">Diurnal Handling</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Baseline simulation</oasis:entry>
         <oasis:entry colname="col2">No update</oasis:entry>
         <oasis:entry colname="col3">Thongsame et al. (2024)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Fixed diurnal</oasis:entry>
         <oasis:entry colname="col2">Full-day update</oasis:entry>
         <oasis:entry colname="col3">Thongsame et al. (2024)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Daylight diurnal</oasis:entry>
         <oasis:entry colname="col2">Daylight hours only</oasis:entry>
         <oasis:entry colname="col3">Updated daylight diurnal</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Temporal average</oasis:entry>
         <oasis:entry colname="col2">Daylight hours only</oasis:entry>
         <oasis:entry colname="col3">3 h temporal average for updated daylight diurnal</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Experimental Design</title>
      <p id="d2e2444">Although IFDMB assumes negligible horizontal transport due to the short atmospheric lifetime of <inline-formula><mml:math id="M157" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, our high-resolution simulations (<inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mn mathvariant="normal">9</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">9</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) violate this assumption, as there may be significant horizontal transport of <inline-formula><mml:math id="M159" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to surrounding grid cells. To mitigate the smearing error, we regrid both GEMS and WRF-Chem <inline-formula><mml:math id="M160" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs to a coarser <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mn mathvariant="normal">45</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">45</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> resolution by spatially averaging over surrounding grid cells. To update <inline-formula><mml:math id="M162" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions, we apply IFDMB in three different configurations: Fixed diurnal, Daylight diurnal, and Temporal average (Table 1). Each approach is described below. For each method, we use some form of a monthly average of the GEMS data to update emissions. This helps reduce the impact of noise and missing data in satellite observations. Additionally, the smearing error is minimized when considering monthly average <inline-formula><mml:math id="M163" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs.</p>
<sec id="Ch1.S2.SS6.SSS1">
  <label>2.6.1</label><title>Fixed diurnal</title>
      <p id="d2e2548">For the fixed diurnal approach, we update monthly emissions without changing their diurnal variability. We calculate monthly averages of tropospheric <inline-formula><mml:math id="M164" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns from both GEMS and WRF-Chem (at the satellite overpass times) during September 2023 (Fig. 3a). These monthly averages are then used to compute a uniform scaling factor via each mass balance method (scaling factor<sub><italic>t</italic>=all</sub>). This scaling factor<sub><italic>t</italic>=all</sub> is applied consistently to <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions at all time steps, including both daytime and nighttime hours. As GEMS provides data during daylight only, we assume the relative differences between GEMS and WRF-Chem are similar at all times.</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e2603">Schematic diagram explaining emission update configurations and corresponding mass balance methods: <bold>(a)</bold> Fixed diurnal, <bold>(b)</bold> Daylight diurnal, and <bold>(c)</bold> Temporal average updates.</p></caption>
            <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f03.png"/>

          </fig>

</sec>
<sec id="Ch1.S2.SS6.SSS2">
  <label>2.6.2</label><title>Daylight diurnal</title>
      <p id="d2e2629">Instead of monthly averaging, we compute the mean GEMS and WRF-Chem <inline-formula><mml:math id="M168" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs for each GEMS scanning hour (Park et al., 2024). Specifically, the mean GEMS VCD at hour 08:00 LT comes from averaging GEMS data at 08:00 am LT every day in September 2023 (Fig. 3b). Hourly scaling factors are derived from these means and applied to emissions at the corresponding hour (scaling factor<sub><italic>t</italic>=8</sub> at Fig. 3b). The emissions at the same hour are updated with the scaling factors of the same hour. This method captures the monthly diurnal variability of GEMS <inline-formula><mml:math id="M170" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and propagates it to the emission inventory. Since GEMS retrievals are only available during the daylight, emissions during nighttime hours remain unchanged. This update scheme takes advantage of the fact that the lifetime of <inline-formula><mml:math id="M171" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> being generally relatively short. The <inline-formula><mml:math id="M172" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD at any given hour is impacted by emissions from that exact same hour. For example, <inline-formula><mml:math id="M173" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD at 08:00 LT is the result of emissions at 08:00 LT, under the assumption that emissions from 06:00 LT or 07:00 LT have no residual impact on the <inline-formula><mml:math id="M174" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD at 08:00 LT. We acknowledge this is a simplification; in reality, emissions take time to undergo chemical conversion (e.g., 08:00 LT emission peaking in <inline-formula><mml:math id="M175" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD around 08:15–08:30 LT), and the emissions before 08:00 LT have impacts on <inline-formula><mml:math id="M176" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD at 08:00 LT due to the multiple hour lifetime of <inline-formula><mml:math id="M177" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S2.SS6.SSS3">
  <label>2.6.3</label><title>Temporal averaging</title>
      <p id="d2e2754">This method accounts for the persistence of <inline-formula><mml:math id="M178" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the atmosphere, acknowledging that observed <inline-formula><mml:math id="M179" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs at a given hour reflect not only current emissions but also emissions from prior hours (Park et al., 2024). Although <inline-formula><mml:math id="M180" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> has a relatively short lifetime, it still spans several hours. To address this, we assume that emissions affect <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs for up to two subsequent hours. For instance, <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emitted from a point source at 08:00 LT is assumed to contribute to the <inline-formula><mml:math id="M183" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs measured at 08:00, 09:00, and 10:00 LT. Therefore, the scaling factor for each hour is calculated from the average of <inline-formula><mml:math id="M184" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD at that hour and the following two hours every day in September 2023 (Fig. 3c). For example, the scaling factor for hour 08:00 LT is based on the mean <inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD observed at 08:00, 09:00, and 10:00 LT every day in September 2023 (scaling factor<sub><italic>t</italic>=8</sub> at Fig. 3c). In the inverse method configuration, the average of <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs at 08:00, 09:00, and 10:00 LT is used rather than the 06:00 and 07:00 LT because the emissions have not emitted yet. This temporal smoothing better represents the time-integrated nature of <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> accumulation. For hours near the end of the GEMS window, such as 14:00 and 15:00 LT, only two and one data points are used for the average, respectively. This is because there is only one subsequent data point from 14:00 LT and no subsequent data for 15:00 LT. As the hourly scaling factors are calculated from monthly moving averages of data in each hour, the emissions at the same hour are updated with the same factors.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS7">
  <label>2.7</label><title>Evaluation method</title>
      <p id="d2e2891">Three metrics, namely, normalized mean bias (NMB), normalized root mean square error (NRMSE), and correlation coefficient (<inline-formula><mml:math id="M189" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>), are used to evaluate the performance of the IFDMB solution in comparison to our simulation using the prior emissions. The observation error (<inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) provided by GEMS and TROPOMI data is used to normalize mean bias (MB) and root mean square error (RMSE). We compare our results with tropospheric <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD from GEMS and TROPOMI, and with in situ <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> measurements from PCD stations. For GEMS and TROPOMI, the monthly average tropospheric <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the Thailand grid cells are compared with the monthly average WRF-Chem results. This is because only emissions in Thailand are updated, while emissions outside Thailand remain the same. For the satellite data, our metrics are normalized with the observation error. However, for PCD stations, we evaluate our results with non-normalized MB, non-normalized RMSE, and <inline-formula><mml:math id="M194" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>. This is because the PCD stations have not reported the observation error. Additionally, we compare the monthly average diurnal <inline-formula><mml:math id="M195" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> profile with PCD data.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2966">Monthly average tropospheric <inline-formula><mml:math id="M196" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD in September 2023 from GEMS (left) and the baseline simulation (right). High <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs are observed over urban areas such as Chiang Mai, Lampang, and the Bangkok Metropolitan Region (BMR), as well as over the Mae Moh power plant and industrial zones in Saraburi and Rayong.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f04.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Comparison between baseline simulation and GEMS</title>
      <p id="d2e3013">This section shows the performance of the WRF-Chem simulation using the prior emissions (the CAMS-GLOB-ANT inventory), aka the baseline simulation, compared to GEMS <inline-formula><mml:math id="M198" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs before applying any mass balance methods. Overall, the baseline simulation significantly overestimates the monthly average <inline-formula><mml:math id="M199" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the Bangkok Metropolitan Region and East Thailand (Fig. 4). The baseline simulation shows that the <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD is dominated by large point sources from many sectors. In North Thailand, the prior emissions identify the Mae Moh coal power plant (energy sector) as the main source of <inline-formula><mml:math id="M201" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, with a signal that significantly overwhelms the urban emissions from Chiang Mai and Lampang (Fig. 1). In the Bangkok Metropolitan Region, the model suggests a mixed contribution from the dense residential and transportation sectors of the urban area. Additionally, industrial estates in Saraburi and Rayong produce high <inline-formula><mml:math id="M202" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> – as strong as urban emissions in Bangkok. GEMS presents a contrasting picture that emphasizes the role of urban sources. In North Thailand, GEMS has the highest <inline-formula><mml:math id="M203" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs centered over the urban areas of Chiang Mai and Lampang, which are dominated by residential and transportation emissions. The Mae Moh power plant appears as only a moderate signal in the GEMS observations. This pattern holds in the Bangkok Metropolitan Region, where GEMS again highlights the urban area, while the signals from major industrial estates in Rayong and Saraburi are notably weaker than the urban emissions. Additionally, the GEMS <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in North Thailand are as large as in the Bangkok Metropolitan Region, while the baseline simulation shows significantly larger <inline-formula><mml:math id="M205" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the Bangkok Metropolitan Region. This direct contradiction between the baseline simulation and GEMS highlights that the CAMS-GLOB-ANT is likely to overestimate energy and industrial emissions relative to the residential and transportation emissions in Thailand. The baseline simulation shows high NMB and NRMSE in most regions, with comparatively better performance in North and West Thailand (Figs. 5 and S15). However, GEMS data availability is high in Central Thailand and the Bangkok Metropolitan Region, moderate in the North and East, and very limited in West Thailand (Fig. 2). When averaged across all grid cells in Thailand, the baseline simulation yields an NMB of 83.52 and an NRMSE of 151.94 relative to GEMS. These metrics quantitatively support the widespread overestimation of modeled <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, though the correlation coefficient across the domain remains moderate (<inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.65</mml:mn></mml:mrow></mml:math></inline-formula>). In the Bangkok Metropolitan Region, the baseline simulation shows an even more pronounced overestimation, with an NMB of 278.67 and an NRMSE of 336.69. Despite these high biases, the correlation coefficient in this area is exceptionally strong (<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.96</mml:mn></mml:mrow></mml:math></inline-formula>). This suggests that while the baseline <inline-formula><mml:math id="M209" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> spatial distribution strongly agrees with the satellite, the absolute VCDs of the prior emissions in this region are severely overestimated.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3154">Spatial distribution of Normalized Mean Bias (NMB) of <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD between WRF-Chem and GEMS of IFDMB for September 2023 using <bold>(a)</bold> prior emissions, and emissions updated by <bold>(b)</bold> fixed diurnal, <bold>(c)</bold> daylight diurnal, and <bold>(d)</bold> temporal average update schemes. Monthly statistical evaluations averaged across all grid cells in Thailand are provided for each simulation.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f05.png"/>

        </fig>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3188">Evolution of the total cost function <inline-formula><mml:math id="M211" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> <bold>(a)</bold>, <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <bold>(b)</bold>, and <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <bold>(c)</bold> over five iterations of IFDMB with three update schemes: fixed diurnal (orange), daylight diurnal (blue), and temporal average (purple). The optimal iteration for each scheme is marked with a filled circle.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Evolution and optimization of mass balance methods</title>
      <p id="d2e3244">To determine the optimal number of iterations for the IFDMB inversion, we calculate the total cost function <inline-formula><mml:math id="M214" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> based on comparisons between <inline-formula><mml:math id="M217" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from WRF-Chem and GEMS at each iteration (Fig. 6). Our results show that <inline-formula><mml:math id="M218" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> decreases substantially during iterations 1 and 2 across all update schemes, but it begins to increase beyond iteration 3 (Fig. 6a). This increase in the total cost function is primarily driven by a rise in <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 6c). The <inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> term slightly decreases after iteration 2. However, <inline-formula><mml:math id="M221" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> does not decrease monotonically due to overadjustment; it may increase in some iterations before decreasing again in subsequent steps (Fig. 6b). There are several reasons supporting the rapid convergence within 2–4 iterations. The iteration in IFDMB accounts for horizontal transport and the nonlinear chemistry of <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Regarding transport, we reduce the smearing error by regridding both GEMS and WRF-Chem <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs to a coarser resolution. We also use monthly averages of GEMS and WRF-Chem, which reduce the impact of noise and missing data in the satellite observations and further minimize the smearing error. Together, these steps largely confine <inline-formula><mml:math id="M224" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> transported out of a source grid cell to the same coarse grid cell. The transport effect that iterations would otherwise need to resolve is therefore absorbed before the inversion begins, which is why only few iterations are required. Additionally, the GEMS observation error is on the order of <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (Fig. 2c), whereas the GEMS <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD data is on the order of <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (Fig. 2a). This large difference in magnitude results in a dominant <inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>prediction</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> term in Eq. (1), which drives a substantial emission adjustment during the very first iteration, followed by much smaller adjustments in subsequent iterations. Furthermore, our regularization parameters prevent over-adjustment and avoid oscillatory fluctuations during convergence. In this study, we assume a 50 % relative uncertainty for the prior emissions error. However, the true uncertainty for specific sectors like power plants and industry may be lower due to direct emissions reporting. This large assumed emission uncertainty yields a relatively small <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mtext>parameter</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> penalty term, giving the IFDMB algorithm the flexibility to make large initial emission adjustments to reconcile the model with the GEMS observations. Our analysis shows that the daylight diurnal scheme exhibits significant overadjustment because it assumes an immediate response of <inline-formula><mml:math id="M230" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs to emission changes. For the fixed diurnal and daylight diurnal update schemes, iteration 2 provides the lowest <inline-formula><mml:math id="M231" display="inline"><mml:mi>J</mml:mi></mml:math></inline-formula> and is thus selected as optimal. For the temporal average update scheme, iteration 4 yields the optimal performance.</p>
      <p id="d2e3436">Additionally, we performed a sensitivity analysis of the regularization parameters in the IFDMB framework, using a fixed diurnal update, to evaluate the impacts of <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. We found that varying these parameters alters the results significantly – yielding differences of <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % to 60 % – with the model showing particular sensitivity to <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Table S1 in the Supplement). Increasing <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M239" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">molec</mml:mi><mml:mo>.</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> limits the influence of satellite constraints, resulting in higher NMB and NRMSE values, particularly in Central and East Thailand (Figs. S1 and S2). A low value for <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> permits large emission adjustments across all of Thailand, including regions with high GEMS retrieval errors, such as North Thailand (Fig. S3). Conversely, a higher <inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> value restricts these adjustments. In North Thailand, where retrieval uncertainty is high, increasing <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> benefits the IFDMB by preventing the model from overfitting to highly uncertain GEMS data. However, this same increase has a detrimental impact on the Bangkok Metropolitan Region. Because uncertainty is comparatively low here, a high <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> limits emission improvements. Regarding <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, increasing its value from 1 to 10 <inline-formula><mml:math id="M245" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>  has minimal impact when <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is low.</p>
      <p id="d2e3636">This is because a low <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> permits aggressive emission adjustments nationwide; variations in <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> become negligible. The impact of <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is much more pronounced when <inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is high. <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> primarily governs adjustments for smaller emission sources in rural areas. Consequently, a high <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> allows for greater adjustments in these low-emission zones, which leads to overfitting to the GEMS data in the rural North. A low <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> leads to underfitting in Central Thailand and the Bangkok Metropolitan Region. Overall, the adjustable parameters in the IFDMB offer valuable flexibility to manage the mismatch between GEMS and TROPOMI by moderating emission updates in high-error regions and balancing prior and posterior estimates. In this study, we applied fixed regularization parameters across the entirety of Thailand. However, our findings indicate that a large <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> benefits high-uncertainty areas like North Thailand, whereas a low <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> benefits the Bangkok Metropolitan Region and Central Thailand. This highlights the potential of using spatially varying parameters based on regional uncertainty rather than fixed domain-wide values. Nevertheless, because we aim to treat these parameters as fixed statistical values rather than tuned parameters, an exhaustive fine-tuning exploration is beyond the scope of this paper.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Comparison with GEMS</title>
      <p id="d2e3747">This section presents the results from WRF-Chem simulations using the IFDMB method evaluated with GEMS. The IFDMB with all three update schemes reduces both NMB and NRMSE in GEMS compared to the baseline simulation (Fig. 5). The IFDMB with fixed diurnal update demonstrates the highest improvement among the three update schemes. The NMB and NRMSE reduce by about 60 % for the fixed diurnal update averaged across all grid cells in Thailand. Reductions are most pronounced in Central Thailand and the Bangkok Metropolitan Region (Figs. 5 and S15). In Bangkok Metropolitan Region, the IFDMB with fixed diurnal update reduces NMB to 29.46 and NRMSE to 51.93. The correlation coefficient remains the same as 0.96. Overestimated <inline-formula><mml:math id="M256" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from transportation and residential sectors are substantially corrected. However, improvements in North and West Thailand are more modest. The improvement in those areas is limited due to the low data density and high errors in those areas. The correlation coefficient (<inline-formula><mml:math id="M257" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) improves from 0.65 (baseline simulation) to 0.84.</p>
      <p id="d2e3768">The IFDMB with daylight diurnal and temporal average updates produces similar results. Both methods improve the performance in urban areas, particularly in Bangkok and big cities in North Thailand, but are less effective in other areas (Figs. 5 and S15). The NMB is reduced by 14 % for the IFDMB with daylight diurnal update and 9 % for the temporal average update averaged across all grid cells in Thailand. However, within the Bangkok Metropolitan Region, these two schemes show lower performance. Specifically in the Bangkok Metropolitan Region, the NMB decreases to 160.26 under the daylight diurnal update and to 110.52 under the temporal average update. Similarly, the NRMSE in this region drops to 214.43 and 158.45 for the daylight diurnal and temporal average updates, respectively. Despite these remaining absolute biases, the correlation coefficient R remains exceptionally strong at approximately 0.96 for both methods. Notably, both updates exhibit small improvements during early morning hours (e.g., 08:00–09:00 am LT) compared to the IFDMB with fixed diurnal update (Fig. S16). Since these methods only update emissions during the daylight, uncorrected nighttime emissions likely contribute to the error of <inline-formula><mml:math id="M258" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD in the early morning. In contrast, the fixed diurnal update, which adjusted emissions at all time steps, shows lower NMB and NRMSE throughout the day. The NRMSE reduction for these two methods is around 20 % and correlation coefficients improve to 0.74 for the daylight diurnal update and 0.78 for the temporal average update.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e3784">The change in monthly average <inline-formula><mml:math id="M259" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions for the IFDMB compared to prior emissions: <bold>(a)</bold> prior emissions, <bold>(b)</bold> IFDMB with fixed diurnal update, <bold>(c)</bold> IFDMB with daylight diurnal update, and <bold>(d)</bold> IFDMB with temporal average update.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f07.png"/>

        </fig>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e3819">Hourly <inline-formula><mml:math id="M260" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions averaged across nine grid cells in <bold>(a)</bold> Bangkok and <bold>(b)</bold> North Thailand comparing IFDMB with different update schemes: prior emission (gray), IFDMB with fixed diurnal update (orange), IFDMB with daylight diurnal update (blue), and IFDMB with temporal average update (purple). The pink line represents the GEMS window for Thailand.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Emissions updates</title>
      <p id="d2e3853">The use of GEMS satellite data to update <inline-formula><mml:math id="M261" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions with the IFDMB method provides an increase in emissions in the North and West Thailand, while emission reductions are obtained in other areas (Fig. 7). The fixed diurnal update produces the largest emission adjustments, as it applies the scaling factor uniformly across all time steps, including periods with and without GEMS observations (Fig. 8). In this case, daily <inline-formula><mml:math id="M262" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions increase approximately 20 <inline-formula><mml:math id="M263" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mole</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in North and West Thailand, while they decrease by about 30 <inline-formula><mml:math id="M264" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mole</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in other regions (Fig. 7). The IFDMB with daylight diurnal update, which only modifies emissions during hours with available GEMS data, results in the smallest overall changes. Increases and decreases are generally below 20 <inline-formula><mml:math id="M265" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mole</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> across all regions (Fig. 7). The IFDMB with temporal average update produces similar results to the daylight diurnal update. However, the emission reduction in the Bangkok Metropolitan Region is stronger than the daylight diurnal update, with the reduction of about 30 <inline-formula><mml:math id="M266" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mole</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. A notable feature across all update schemes is the significant amplification of <inline-formula><mml:math id="M267" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Lampang. This enhancement arises because the CAMS-GLOB-ANT inventory lacks representation of large point sources in that area, whereas GEMS indicates elevated <inline-formula><mml:math id="M268" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. Consequently, the IFDMB compensates for the discrepancy between simulated and observed <inline-formula><mml:math id="M269" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> by intensifying the small prior emissions in Lampang.</p>
      <p id="d2e4016">For the diurnal variability, prior emissions follow almost the same diurnal profile across all regions in Thailand, depending on the dominant sectors. However, GEMS-informed updates reveal differences in diurnal variability across Thailand (Fig. 8). In Bangkok and North Thailand, the prior profile has a sharp morning peak between 08:00–09:00 LT, followed by a flat midday period extending to 16:00 LT. In contrast, both the IFDMB daylight diurnal and temporal average updates exhibit more dynamic variability, with pronounced peaks between 09:00–11:00 LT and a subsequent decline throughout the GEMS observation window in Bangkok. In North Thailand, the IFDMB daylight diurnal update peaks around 12:00–14:00 LT, while the temporal average update peaks earlier, around 09:00–11:00 LT. Our study reveals that the diurnal variability from Thongsame et al. (2024), which shows peaks aligned with morning and evening rush hours, is different from the GEMS diurnal variability. GEMS provides the potential to refine the diurnal variability during the daylight in Thailand. However, GEMS tends to underestimate <inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the early morning and late afternoon, due to unfavorable viewing geometries during those times (Park et al., 2024). Future research is required to analyze this uncertainty and its impacts on diurnal variability.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e4032">Monthly average tropospheric <inline-formula><mml:math id="M271" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD in September 2023 from: GEMS sampled at all available data <bold>(a)</bold>, the baseline simulation applying GEMS averaging kernel sampled at GEMS scanning times <bold>(b)</bold>, GEMS sampled at the TROPOMI overpass time <bold>(c)</bold>, the baseline simulation applying the GEMS averaging kernel sampled at the TROPOMI overpass time <bold>(d)</bold>, TROPOMI <bold>(e)</bold>, and the baseline simulation applying the TROPOMI averaging kernel sampled at TROPOMI overpass time <bold>(f)</bold>.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f09.png"/>

        </fig>


</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Comparison with TROPOMI</title>
      <p id="d2e4082">In this section, we compare tropospheric <inline-formula><mml:math id="M272" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from the WRF-Chem simulations and GEMS with those from TROPOMI (Fig. 9). Because GEMS and TROPOMI differ in their averaging kernels and overpass times, a direct comparison is not feasible. Therefore, we focus on assessing the relative spatial distributions of <inline-formula><mml:math id="M273" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. To compare the <inline-formula><mml:math id="M274" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD between GEMS and TROPOMI, WRF-Chem is used as the intercomparison platform, following the methodology of Zhang et al. (2010). This approach applies the AKs from each satellite to the same WRF-Chem outputs to assess how the distinct vertical sensitivities of the instruments differ relative to the model (Fig. 9b, d, and f). To ensure consistency, the GEMS and WRF-Chem VCDs closest to the TROPOMI overpass time are selected for comparison (Fig. 9c and d). The differences between the GEMS and TROPOMI overpass times are about 15 min. The monthly average GEMS <inline-formula><mml:math id="M275" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs at the TROPOMI overpass times are slightly higher than the monthly average <inline-formula><mml:math id="M276" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> derived from all GEMS observations (Fig. 9a and c). Moreover, they exhibit increased noise, particularly over rural areas. Overall, both satellites show similar spatial patterns of <inline-formula><mml:math id="M277" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, except in North Thailand. High <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is consistently observed in the Bangkok Metropolitan Region, Saraburi, and Rayong from both GEMS and TROPOMI. In North Thailand, both satellites detect high <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> associated with the Mae Moh power plant; however, GEMS shows anomalously high <inline-formula><mml:math id="M280" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over Lampang that is not observed by TROPOMI (Fig. 9c and e). The <inline-formula><mml:math id="M281" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels in Lampang from GEMS exceed those in Bangkok, whereas TROPOMI indicates the highest <inline-formula><mml:math id="M282" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over the Bangkok Metropolitan Region. Additionally, TROPOMI generally has higher background <inline-formula><mml:math id="M283" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> levels compared to source regions. To further examine the magnitude differences, we apply the respective averaging kernels of GEMS and TROPOMI to the baseline simulation. The results indicate that TROPOMI retrieves higher <inline-formula><mml:math id="M284" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs than GEMS across most regions, except in Lampang, where GEMS values remain substantially larger (Fig. 9d and f).</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e4232">NMB of <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD between WRF-Chem and TROPOMI of IFDMB for September 2023 using <bold>(a)</bold> prior emissions, and emissions updated by <bold>(b)</bold> fixed diurnal, <bold>(c)</bold> daylight diurnal, and <bold>(d)</bold> temporal average update schemes. Monthly statistical evaluations averaged across all grid cells in Thailand are provided for each simulation.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f10.png"/>

        </fig>

      <p id="d2e4264">Our baseline simulation overestimates tropospheric <inline-formula><mml:math id="M286" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs across Thailand relative to TROPOMI satellite observations (Fig. 9e and f). The model predicts strong <inline-formula><mml:math id="M287" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD from energy, industry, transportation, and residential sectors almost everywhere, whereas TROPOMI detects high <inline-formula><mml:math id="M288" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> only in specific areas. In particular, TROPOMI shows high <inline-formula><mml:math id="M289" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> only over the Bangkok Metropolitan Region (attributed largely to residential emissions) and at certain major point sources (e.g., the Mae Moh power plant in the North and large industrial zones in Central Thailand). Most other areas, including city centers in North and Northeast Thailand, exhibit only moderate <inline-formula><mml:math id="M290" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the TROPOMI data. Additionally, TROPOMI shows moderate to low <inline-formula><mml:math id="M291" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> along the major roads in Thailand, whereas the baseline simulation shows clear <inline-formula><mml:math id="M292" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> enhancements. The monthly NMB from the baseline simulation is 0.8 (Figs. 10 and S17). This emphasizes the overestimation of TROPOMI <inline-formula><mml:math id="M293" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs with the baseline simulation. The monthly NRMSE is 1.21 (Fig. 10). We have found that the baseline simulation is moderately correlated with the monthly average TROPOMI (<inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.79</mml:mn></mml:mrow></mml:math></inline-formula>).</p>
      <p id="d2e4369">The IFDMB with fixed diurnal update significantly reduces NMB and NRMSE for TROPOMI, except in North Thailand. The NMB drops by roughly 25 % relative to the baseline simulation, and NRMSE also declines by about 29 % (Fig. 10). Because the baseline simulation overpredicts <inline-formula><mml:math id="M295" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in nearly all locations, the emission reductions from the IFDMB with fixed diurnal update lead to a closer match with TROPOMI across most of Thailand. For example, in the Bangkok Metropolitan Region and East Thailand, the IFDMB with fixed diurnal update significantly improves the NMB and NRMSE, while moderately reducing NMB and NRMSE in Central and Northeast Thailand (Figs. 10 and S17). In these areas, the <inline-formula><mml:math id="M296" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD from transportation and residential sectors is decreased, aligning better with the TROPOMI levels.</p>
      <p id="d2e4394">In contrast, the IFDMB with fixed diurnal update worsens the agreement with TROPOMI in North Thailand by increasing the NMB and NRMSE. This degradation is primarily due to the discrepancy between GEMS and TROPOMI <inline-formula><mml:math id="M297" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> observations (Fig. 9c and e). While TROPOMI shows relatively low <inline-formula><mml:math id="M298" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in North Thailand compared to the Bangkok Metropolitan Region, GEMS has high <inline-formula><mml:math id="M299" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the North. Moreover, the baseline simulation already overestimates <inline-formula><mml:math id="M300" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in North Thailand relative to TROPOMI (Fig. 10a). As a result, the IFDMB – driven by GEMS – further increases <inline-formula><mml:math id="M301" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in the North, exacerbating the overestimation when compared to TROPOMI (Fig. 10b). This leads to a noticeable decline in the overall WRF-Chem–TROPOMI correlation, dropping to <inline-formula><mml:math id="M302" display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.61</mml:mn></mml:mrow></mml:math></inline-formula> (Fig. 10b). However, in the Bangkok Metropolitan Region, the update slightly improves the agreement, with monthly correlation coefficients increasing from 0.90 to 0.93 (Table S4).</p>
      <p id="d2e4465">The daylight diurnal and temporal average updates exhibit spatial trends similar to the fixed diurnal update, with improvements in most regions but degradation in North Thailand (Figs. 10 and S17). Across all grid cells, these two schemes do not yield net improvements in overall NMB and NRMSE (Fig. 10). The daylight diurnal update slightly increases NMB by 5 % and reduces NRMSE by 2 % relative to the baseline simulation. In contrast, the temporal average update increases NMB and NRMSE by 31 % and 17 %, respectively. The apparent deterioration in national-scale performance primarily stems from the mismatch between GEMS and TROPOMI in North Thailand.</p>
      <p id="d2e4468">To isolate this effect, we evaluate model performance in the Bangkok Metropolitan Region, where GEMS and TROPOMI show strong consistency (Table S4). In this region, the daylight diurnal update reduces NMB and NRMSE by 54 % and 39 %, respectively, compared with the baseline simulation (Table S4). The temporal average update yields even larger improvements, reducing NMB by 81 % and NRMSE by 61 % (Table S4). However, this update scheme performs the poorest in North Thailand. The temporal average update shows stronger emission adjustment near TROPOMI overpass time (09:00–11:00 LT) compared to the daylight diurnal update. This leads to more impact on the model performance with TROPOMI.</p>
      <p id="d2e4471">Overall, the IFDMB with all three update schemes reduce the model bias and error in areas such as the Bangkok Metropolitan Region, Saraburi, and Rayong industrial estates. This is because TROPOMI's spatial pattern resembles GEMS, with high <inline-formula><mml:math id="M303" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over the Bangkok Metropolitan Region and moderate VCDs over the Saraburi and Rayong industrial estates. However, improving model performance in North Thailand remains a challenge because GEMS and TROPOMI exhibit substantial differences in <inline-formula><mml:math id="M304" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over this region. TROPOMI <inline-formula><mml:math id="M305" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in North Thailand align more closely with the baseline simulation, having a strong signal from the Mae Moh power plant that is higher than the surrounding urban areas. In contrast, GEMS presents the highest <inline-formula><mml:math id="M306" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over the Lampang urban area instead. The inconsistency between GEMS and TROPOMI in North Thailand is a crucial finding.</p>
      <p id="d2e4518">Our analysis indicates that the GEMS–TROPOMI discrepancy primarily arises from uncertainties in the prior model profile used by the GEMS retrieval algorithm. TROPOMI version 2 uses the TM5-MP global model with the MACCity emission inventory for its retrieval algorithm (Douros et al., 2023; Williams et al., 2017). GEMS version 3 employs the GEOS-Chem model with the ASIA-AQv3 emission inventory as its prior input for <inline-formula><mml:math id="M307" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals. Our analysis shows that the ASIA-AQv3 inventory reports anomalously high <inline-formula><mml:math id="M308" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in the Lampang region compared to other inventories (Fig. S6). This high <inline-formula><mml:math id="M309" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission likely causes GEMS to overestimate <inline-formula><mml:math id="M310" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over Lampang which is not observed by TROPOMI and the baseline simulation. The high <inline-formula><mml:math id="M311" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions from ASIA-AQv3 also result in significantly larger retrieval errors in the Lampang area (Fig. 2). Supporting this interpretation, GEMS <inline-formula><mml:math id="M312" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> using the Direct Vertical Column Fitting (DVCF) algorithm from Yang et al. (2024) yields much lower <inline-formula><mml:math id="M313" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over Lampang, in line with the TROPOMI observations. Notably, the GEMS version 3 data used in this study do agree well with TROPOMI over the Bangkok Metropolitan Region, Saraburi, and Rayong. Detailed comparisons are provided in Sects. S2 and S3.</p>
      <p id="d2e4600">These differences between satellite products highlight the importance of bias correction, calibration, and cross-validation for satellite-based <inline-formula><mml:math id="M314" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements. For example, Kim et al. (2023) also find that both GEMS and TROPOMI underestimate <inline-formula><mml:math id="M315" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs compared to Pandora measurements in Seosan, South Korea, with GEMS exhibiting a greater degree of underestimation than TROPOMI. The fact that GEMS and TROPOMI can yield markedly different <inline-formula><mml:math id="M316" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (as seen in Thailand) underscores the need to calibrate and validate these satellite retrievals using independent observations in Thailand. However, achieving robust calibration in Thailand is challenging due to the scarcity of ground-based measurements. In 2023, only a single Pandora spectrometer was operational in Bangkok. Data from this instrument exhibit substantial uncertainty during the Thai winter season (October–January) (Kanchanachat, 2026), and there is no cross-validation by other instruments. Furthermore, compared to Korea, China, and Japan, the Bangkok Pandora site reports significantly lower <inline-formula><mml:math id="M317" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs relative to GEMS (Jung et al., 2025). Consequently, we exclude its observations from our analysis. We recommend leveraging data from the ASIA-AQ field campaign to improve the accuracy and consistency of satellite <inline-formula><mml:math id="M318" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> assessments in Thailand. Even though this field campaign is limited to the Bangkok and Chiang Mai areas and spans only a short time period, it provides useful information to resolve the biases in the satellite products.</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e4660">The daytime diurnal variability of normalized <inline-formula><mml:math id="M319" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations from PCD stations (black) and WRF-Chem: the baseline simulation (gray), IFDMB with fixed diurnal update (orange), IFDMB with daylight diurnal update (blue), and IFDMB with temporal average update (purple). PCD stations are classified into roadside stations <bold>(a)</bold> and non-roadside stations <bold>(b)</bold>. The pink line is the GEMS scanning time in Thailand from 08:00–15:00 LT.</p></caption>
          <graphic xlink:href="https://acp.copernicus.org/articles/26/14051/2026/acp-26-14051-2026-f11.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Comparison with data from PCD stations</title>
      <p id="d2e4694">Hourly observations from PCD stations are used to evaluate how different emission update schemes affect the simulated diurnal variability of <inline-formula><mml:math id="M320" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. As the GEMS hourly scanning times occur between 08:00 and 15:00 Thailand local time, model–observation comparisons are limited to daylight hours. We restrict the comparison to 08:00–15:00 LT period to ensure a fair evaluation, as only the fixed diurnal scheme adjusts emissions outside this period, while the others revert to the prior emissions. The PCD stations are mostly located in Central and Northeast Thailand, and the Bangkok Metropolitan Region (Fig. S14). The baseline simulation systematically underestimates monthly average <inline-formula><mml:math id="M321" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios by 10–15 ppbv at 14 roadside PCD sites throughout the day and underestimates daytime <inline-formula><mml:math id="M322" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> by 3 ppbv or less at six non-roadside PCD sites (Fig. S18). The IFDMB with GEMS-based top-down emission adjustment exacerbates the underestimation of <inline-formula><mml:math id="M323" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios at roadside PCD stations (Fig. S18), although it provides the same magnitude of concentration for non-roadside PCD stations. All inversion schemes lead to an increase in bias and error at roadside stations. These discrepancies arise primarily from differences in spatial resolution between the GEMS (<inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3.5</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">8</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>), WRF-Chem (<inline-formula><mml:math id="M325" display="inline"><mml:mrow><mml:mn mathvariant="normal">9</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">9</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>), and PCD stations (point-scale), as well as strong local contributions of transportation emissions at the PCD sites. Moreover, both GEMS observations and WRF-Chem simulations are regridded to <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:mn mathvariant="normal">45</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">45</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> for the mass balance calculation in this study to reduce smearing errors associated with horizontal transport. However, this introduces resolution errors by averaging over spatially heterogeneous emission sources. This grid-averaged value is heavily influenced by regional <inline-formula><mml:math id="M327" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pollution and is therefore much lower than the <inline-formula><mml:math id="M328" display="inline"><mml:mrow class="chem"><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 from local hotspots, such as a busy roadway, that may occupy only a small fraction of that grid cell. Consequently, we do not focus on reproducing absolute <inline-formula><mml:math id="M329" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios in this study but instead assess changes and improvements in diurnal patterns as shown in <inline-formula><mml:math id="M330" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations normalized by their monthly average value (Fig. 11).</p>
      <p id="d2e4845">Observed <inline-formula><mml:math id="M331" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios typically peak near 08:00 LT, during the morning rush hour, whereas the baseline simulation and WRF-Chem simulations using posterior emissions have an earlier peak between 06:00 and 07:00 LT. Furthermore, the model has higher <inline-formula><mml:math id="M332" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>  levels at night, while observations have high <inline-formula><mml:math id="M333" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> during the day. This discrepancy indicates that the diurnal profile from Thongsame et al. (2024) used in the baseline simulation does not fully capture the real-world traffic patterns for <inline-formula><mml:math id="M334" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. In particular, the default diurnal profile fails to reproduce the morning traffic peak and instead shows a high level of <inline-formula><mml:math id="M335" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> during nighttime. The fixed diurnal update scheme does not improve the temporal correlation between modeled and observed <inline-formula><mml:math id="M336" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios at roadside or non-roadside stations (Fig. 11). As this update scheme does not alter the shape of the diurnal profile, the simulated <inline-formula><mml:math id="M337" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> peak continues to occur at night, leaving the morning underestimation unresolved. The daylight diurnal and temporal average updates also show limited improvement in diurnal variability (Fig. 11). At roadside stations, both produce afternoon <inline-formula><mml:math id="M338" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> diurnal variability closer to that of the PCD data but fail to reproduce the morning peak. At non-roadside stations, both schemes capture similar morning diurnal variability yet diverge in the afternoon. The temporal average update yields a slight mid-day dip, whereas the daylight diurnal update produces a modest increase (Fig. 11). The PCD data exhibit a small increase around 14:00 LT and a drop by 15:00 LT, which is more consistent with the daylight diurnal update. Overall, the GEMS-based diurnal variability does not capture the observed morning rush-hour but slightly improves afternoon diurnal variability. However, using the GEMS satellite to only update the diurnal variability introduces an unrealistic diurnal profile in the model – an abrupt increase and drop in the <inline-formula><mml:math id="M339" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions profile (Fig. 8). We recommend implementing a smoothing technique in future work to mitigate such discontinuities. In this study, we applied a 5-point moving average to the posterior emissions from the IFDMB with the daylight diurnal update (Sect. S4). While this smoothing technique has a small impact on absolute <inline-formula><mml:math id="M340" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations, it yields a more physically realistic <inline-formula><mml:math id="M341" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentration profile by mitigating the abrupt changes in the transition zones bordering the GEMS observation window. In summary, while the fixed diurnal update does not improve model–observation agreement due to its unchanged emission profile, the daylight diurnal and temporal average updates offer some potential for spatially resolved diurnal refinements. However, the lack of satellite observations during critical rush-hour periods (early morning and evening) limits their effectiveness. Although GEMS-based updates alone do not substantially improve <inline-formula><mml:math id="M342" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> simulations at PCD stations due to resolution and timing mismatches, the satellite provides valuable information for refining regionally specific diurnal patterns, which could enhance WRF-Chem performance in future studies.</p>
      <p id="d2e4982">Our findings also underscore the tradeoffs in the application of mass balance methods. The IFDMB approach, when applied at the <inline-formula><mml:math id="M343" display="inline"><mml:mrow><mml:mn mathvariant="normal">45</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">45</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> resolution, offers computational efficiency and is well-suited for adjusting regional-scale emissions over long temporal periods. However, its coarse spatial resolution limits its ability to capture fine-scale urban variability and accurately constrain emissions from local sources such as traffic. Moreover, reducing or removing the aggregation for IFDMB provides no significant difference in roadside stations (Sect. S5). For non-roadside stations, the <inline-formula><mml:math id="M344" display="inline"><mml:mrow><mml:mn mathvariant="normal">45</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">45</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> resolution performs better than <inline-formula><mml:math id="M345" display="inline"><mml:mrow><mml:mn mathvariant="normal">27</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">27</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> resolution and <inline-formula><mml:math id="M346" display="inline"><mml:mrow><mml:mn mathvariant="normal">9</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">9</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> resolution (Fig. S11). In contrast, other inversion techniques – such as 4D-Var or ensemble Kalman filter (EnKF) methods – coupled with high-resolution models, would be more effective for resolving local emissions. However, these approaches are computationally expensive and may not be feasible for long-term simulation. Therefore, the IFDMB with GEMS data provides practical and efficient adjustments to regional <inline-formula><mml:math id="M347" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Thailand.</p>
</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><title>Inversion approaches</title>
      <p id="d2e5080">This section provides an evaluation of the performance and inherent trade-offs of the different update schemes used in our study. The IFDMB method is a practical advancement of the mass balance approach for emission adjustment by integrating satellite and prior information. In our study, regularization parameters <inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are introduced to balance constraints between the prior emissions and GEMS. These parameters control the trade-off between overfitting and underfitting to the satellite data. For example, the discrepancy between GEMS and TROPOMI in North Thailand indicates high uncertainty in the satellite observations. In this region, a higher <inline-formula><mml:math id="M350" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> value, which affects the prediction error term, allows IFDMB to place less weight on the GEMS data, reducing the risk of over-adjustment in areas with more uncertain observations. Although our study does not fully evaluate the sensitivity of IFDMB to <inline-formula><mml:math id="M351" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, preliminary tests with varying parameter values are presented in Sect. S1.</p>
      <p id="d2e5138">We find that with <inline-formula><mml:math id="M353" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, IFDMB can partially accommodate the uncertainty in the GEMS data due to ASIA-AQv3 inventory used for the GEMS retrieval. Our IFDMB still leads to increased bias and error for WRF-Chem in North Thailand when compared with TROPOMI, particularly for the daylight diurnal and temporal average update schemes. These schemes are more uncertain than the fixed diurnal update because of fewer available data points in each update. The <inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> parameter, which affects the emissions error term, helps prevent IFDMB from excessively adjusting small emissions, but our results indicate that <inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> has a stronger influence on IFDMB performance than <inline-formula><mml:math id="M356" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The overall performance of IFDMB also depends on the relative uncertainties from GEMS and the prior emissions. In this study, we apply a fixed uncertainty of 50 % to the prior emissions, which may not reflect the true variability in real-world conditions. Additionally, the GEMS error is lower than the error reported in TROPOMI. Therefore, future work should focus on developing more accurate, region-specific estimates of both satellite and prior emission uncertainties to further improve IFDMB performance and reliability.</p>
      <p id="d2e5196">For the update schemes, all three schemes for IFDMB offer improvements over the prior simulation when evaluated against GEMS data. However, each scheme involves trade-offs in how it treats diurnal variability, and these trade-offs determine which scheme is best suited to a given application. For applications focused on monthly-average <inline-formula><mml:math id="M357" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> improvement or on updating emissions at the national or regional scale where the diurnal cycle matters less than spatial accuracy, we recommend the fixed diurnal update. This scheme applies a uniform monthly-averaged correction factor to emissions at all hours and produces the most substantial improvements against GEMS observations. However, this method could not correct the diurnal variability of emissions. The ground-based PCD data clearly show that the baseline simulation misrepresents the diurnal cycle, with the model peaking at night instead of during morning and evening rush hours. The high <inline-formula><mml:math id="M358" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentration during the nighttime from the model is likely due to the low planetary boundary layer at that time (Thongsame et al., 2024). The fixed diurnal update simply scales down the incorrect diurnal profile, without improving the diurnal variability. We find that it lowers the correlation at 08:00 LT from 0.70 to 0.60 at roadside stations and from 0.70 to 0.66 at non-roadside stations. Even so, the fixed diurnal update remains a simple and effective method, as it is the only scheme able to update emissions during both daytime and nighttime using monthly-average data; because GEMS only provides information during daylight hours, the other two schemes must leave nighttime emissions unchanged from the prior.</p>
      <p id="d2e5221">The daylight diurnal and temporal average updates are designed to address diurnal issues by incorporating hourly GEMS data. These schemes only adjust emissions during daylight hours, resulting in more modest improvements in GEMS agreement. Their key weakness, however, is the introduction of an unrealistic diurnal profile. Because the algorithms have no observational constraints outside the GEMS timing window, they revert to the prior profile at night. This is due to the limitations of our update schemes. For studies focused on daytime hourly <inline-formula><mml:math id="M359" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> concentrations and diurnal variability, we recommend the daylight diurnal update scheme. Because the daylight diurnal and temporal average schemes yield no significant difference in performance, we favor the daylight diurnal update for its simpler implementation. It improves the correlation at 08:00 LT from 0.70 to 0.75 at non-roadside PCD stations, while the correlation at roadside stations remains unchanged at 0.70. By applying the smoothing technique, the impact of the unrealistic diurnal profile would be reduced. Unlike the fixed diurnal update, it can adjust the diurnal profile region by region rather than applying a single uniform profile across the domain, though this benefit remains limited by GEMS's spatial resolution. The challenge of this scheme is how to refine emissions outside the GEMS coverage period, as no UV/Vis satellite observations are available at night. Future research should consider integrating additional datasets – such as from the recent ASIA-AQ field campaign data, Pandora spectrometer measurements, and PCD stations – with satellite observations to develop accurate diurnal profiles. Nevertheless, GEMS provides valuable information for constraining daylight diurnal variability across different regions of Thailand.</p>
</sec>
<sec id="Ch1.S3.SS8">
  <label>3.8</label><title>Comparison with previous studies</title>
      <p id="d2e5243">We compare our results with another study using GEMS to adjust regional emissions. Our baseline simulation shows consistent results with Park et al. (2024) when comparing monthly average <inline-formula><mml:math id="M360" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs with GEMS data. Specifically, in our September 2023 simulation, the baseline simulation overestimates <inline-formula><mml:math id="M361" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs across most of Thailand, except in the North. Similarly, using the CMAQ model for March–April 2022, Park et al. (2024) report an overestimation of <inline-formula><mml:math id="M362" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD compared to GEMS across all regions of Thailand, including the North. The key difference in the North is due to the dominant emission sources during the two study periods. In Park et al. (2024), the simulation period is during the haze season, when biomass burning emissions mainly contribute to <inline-formula><mml:math id="M363" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in North Thailand during March–April (Lalitaporn, 2017; Oo et al., 2021). In contrast, our study period in September 2023 corresponds to the non-haze season, when biomass burning activity is minimal. Therefore, the underestimation in North Thailand, in our case, is likely attributable to anthropogenic emission inventories rather than biomass burning. Additionally, Park et al. (2024) use GEMS version 2 for emission adjustment, while our study utilizes GEMS version 3, which may also contribute to differences.</p>
      <p id="d2e5290">Regarding top-down emission updates, our IFDMB produces similar regional trends to Park et al. (2024) across all update schemes. In both studies, posterior <inline-formula><mml:math id="M364" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions decrease in the Bangkok Metropolitan Region, Central, and Northeast Thailand. However, our study shows an increase in posterior <inline-formula><mml:math id="M365" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in North Thailand, while Park et al. (2024) report a decrease in this region. This contrast again likely reflects seasonal differences in emission sources – anthropogenic in our case, biomass burning in theirs.</p>
      <p id="d2e5315">Our analysis also shows that the daylight diurnal and temporal average update schemes produce higher simulation errors in the morning hours when evaluated against GEMS, compared to midday periods. This pattern arises because these update schemes modify emissions only during daylight hours while leaving nighttime emissions unchanged. Although <inline-formula><mml:math id="M366" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is a short-lived species, it still can have a multi-hour lifetime, meaning that emissions from previous hours influence concentrations at any given time. Consequently, unchanged nighttime emissions can impact early morning <inline-formula><mml:math id="M367" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations. Furthermore, as noted in recent work (Lange et al., 2024; Park et al., 2024), GEMS observations in the early morning and late afternoon are subject to greater uncertainty due to unfavorable viewing geometries, often leading to underestimation of <inline-formula><mml:math id="M368" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> columns. This observational bias further complicates the evaluation of morning model performance when using GEMS data alone. In the future, we plan to integrate other observations, which provide nighttime data, for these update schemes. As our study is one of the first applications of GEMS geostationary data to update local emissions specifically focused on Thailand, we have not yet applied other instruments to infer nighttime anthropogenic activities such as thermal infrared (TIR) instruments or VIIRS night light products.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusion</title>
      <p id="d2e5360">This study applies high-temporal-resolution GEMS satellite data to update anthropogenic <inline-formula><mml:math id="M369" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions over Thailand during September 2023 to improve the air quality modeling and assess diurnal variability of emissions. We compare WRF-Chem simulations using posterior emissions with observations from both the satellite and surface PCD stations to highlight the strengths and limitations of the IFDMB method using GEMS. We find that the baseline simulation from CAMS-GLOB-ANT v5.3 significantly overestimates tropospheric <inline-formula><mml:math id="M370" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs across Thailand in comparison to both GEMS and TROPOMI, except in North Thailand where GEMS indicates this inventory is an underestimation. We attribute this underestimation primarily to retrieval uncertainty associated with the a priori in GEMS version 3 rather than to a genuine emission deficit. By applying the IFDMB inversion technique, the fixed diurnal update increases <inline-formula><mml:math id="M371" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission by about 20 <inline-formula><mml:math id="M372" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>  in North and West Thailand while decreasing them by about 30 <inline-formula><mml:math id="M373" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">mol</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> across most other regions. In contrast, the daylight diurnal and temporal average updates produce generally smaller adjustments. Including North Thailand, total <inline-formula><mml:math id="M374" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions are 35 852 Mg per month in baseline, compared with posterior totals of 25 994 Mg per month (fixed diurnal), 34 808 Mg per month (daylight diurnal), and 36 870 Mg per month (temporal average). Excluding North Thailand, the corresponding totals are 30 699 Mg per month (baseline), 15 376 Mg per month (fixed diurnal), 26 523 Mg per month (daylight diurnal), and 27 087 Mg per month (temporal average). Because North Thailand accounts for about 14 % of national <inline-formula><mml:math id="M375" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions, the GEMS retrieval uncertainty in this region propagates to a 10 %–20 % effect on the national posterior totals. WRF-Chem simulations using posterior emissions show improved agreement with TROPOMI in most regions, especially the Bangkok Metropolitan Region. In this area, the fixed diurnal and temporal average updates achieve NMB reductions of 83 % and 81 %, and NRMSE reductions of 76 % and 61 %, respectively. The daylight diurnal update reduces NMB by 54 % and NRMSE by 39 %. However, the improvement in North Thailand is limited due to the discrepancy between GEMS and TROPOMI data in this area. Further refinement of retrieval algorithms and cross-satellite calibration would be expected to improve IFDMB performance there. Evaluation against PCD stations shows that the baseline simulation underestimates <inline-formula><mml:math id="M376" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios by 10–15 ppbv at roadside site. WRF-Chem using posterior emissions further exacerbates this underestimation at roadside PCD stations. This is attributed to strong differences in spatial resolution combined with the short lifetime of <inline-formula><mml:math id="M377" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The roadside PCD stations are mainly influenced by local transportation emissions, whereas GEMS captures broader urban and industrial emissions. Despite this limitation, GEMS demonstrates the potential to constrain the area-specific daytime diurnal variability of <inline-formula><mml:math id="M378" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions, allowing diurnal emission profiles to be updated for each region rather than applying a uniform diurnal profile. This leads the model to be more accurate and reflects real-world emission patterns.</p>
      <p id="d2e5504">Our results are broadly consistent with previous study using GEMS data to constrain <inline-formula><mml:math id="M379" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions over Southeast Asia during the haze season (March–April 2022). Both simulations overestimate <inline-formula><mml:math id="M380" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs relative to GEMS across most regions which results in <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emission reductions across Thailand. However, our IFDMB approaches increase the <inline-formula><mml:math id="M382" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in North Thailand during September 2023 whereas previous study decreases the emissions. This key divergence is mainly due to the high biomass burning emission in haze season and the differences between GEMS versions. Moreover, our study highlights the limitations of mass balance method using GEMS observation for refining <inline-formula><mml:math id="M383" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Thailand. The coarsening of GEMS and WRF-Chem data to <inline-formula><mml:math id="M384" display="inline"><mml:mrow><mml:mn mathvariant="normal">45</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">45</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> for mass balance method reduces smearing errors, but introduces resolution errors that prevent accurate representation of local traffic emission. A further limitation is the discrepancy between GEMS and TROPOMI <inline-formula><mml:math id="M385" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in North Thailand, which is attributed to the a priori emission inventory used in the GEMS retrieval algorithm. This emphasizes the calibration and bias correction for satellite data in Thailand in the future.</p>
      <p id="d2e5593">In summary, this study demonstrates both the value and limitations of GEMS observations for refining <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions in Thailand. GEMS provides valuable insights into the spatial distribution and daylight diurnal variability of <inline-formula><mml:math id="M387" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> across the region. By integrating GEMS data with mass balance methods, we improve the performance of <inline-formula><mml:math id="M388" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> simulations using WRF-Chem, particularly in the Bangkok Metropolitan Region, which showed substantial improvement when compared to TROPOMI observations. These results underscore the benefits of geostationary satellites such as GEMS for near-real-time emission constraints. However, limitations related to satellite retrieval uncertainty, spatial resolution, and local emission representation remain challenges Thailand. For future work, we recommend combining GEMS observations with complementary datasets – such as PCD stations, LEO satellite, and data from the recent ASIA-AQ field campaign – to enhance data assimilation and reduce potential biases in GEMS retrievals.</p>
</sec>

      
      </body>
    <back><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d2e5634">The source code for WRF-Chem version 4.2.2 (Skamarock et al., 2019) is available at <uri>https://github.com/wrf-model/WRF</uri> (last access: 15 January 2023). The model configuration follows Thongsame et al. (2024), incorporating biomass burning emissions from FINN2.5 (Wiedinmyer et al., 2023) and anthropogenic emissions from CAMS-GLOB-ANT v5.3 (<ext-link xlink:href="https://doi.org/10.24380/D0BN-KX16" ext-link-type="DOI">10.24380/D0BN-KX16</ext-link>, Granier et al., 2019).</p>

      <p id="d2e5643">Observation data from PCD stations can be accessed at <uri>http://air4thai.pcd.go.th/webV3/</uri> (last access: 20 December 2024). The GEMS data are available at <uri>https://nesc.nier.go.kr/en/html/index.do</uri> (last access: 27 December 2024). The information of TROPOMI data can be found at <uri>https://www.tropomi.eu/</uri> (last access: 25 April 2025).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e5655">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-26-14051-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-26-14051-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5664">WT and DKH designed the experiments, and WT carried them out. RK, MB, and GP provide resources and supervision. All authors edited the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5670">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="d2e5676">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e5682">WT is supported by the Development and Promotion of Science and Technology Talents Project (DPST) fellowship. WT and DKH recognize support from NASA. RK, MB, and GP are supported by the NSF National Center for Atmospheric Research (NCAR), which is a major facility sponsored by the U.S. National Science Foundation.</p><p id="d2e5684">We acknowledge use of the WRF-Chem preprocessor tools {mozbc, fire_emiss, etc.} provided by the Atmospheric Chemistry Observations and Modeling Lab (ACOM) of National Center for Atmospheric Research (NCAR). We would like to acknowledge high-performance computing support from Derecho (<ext-link xlink:href="https://doi.org/10.5065/qx9a-pg09" ext-link-type="DOI">10.5065/qx9a-pg09</ext-link>) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5692">This research has been supported by the NASA (grant no. 80NSSC22K1047), the U.S. National Science Foundation (cooperative agreement no. 1852977), and the Development and Promotion of Science and Technology Talents Project (DPST), Royal Thai Government.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5698">This paper was edited by James Lee and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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