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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</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/essd-18-2749-2026</article-id><title-group><article-title>Deriving regional and point source nitrogen oxides emissions in China from TROPOMI using the directional derivative approach with nonlinear chemical lifetime fitting</article-title><alt-title>Deriving regional and point source nitrogen oxides emissions in China from TROPOMI</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3 aff4">
          <name><surname>Chen</surname><given-names>Ling</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6014-2225</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Cai</surname><given-names>Zhaonan</given-names></name>
          <email>caizhaonan@mail.iap.ac.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Sun</surname><given-names>Kang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9930-7509</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff3">
          <name><surname>Liu</surname><given-names>Yi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9305-5358</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Yang</surname><given-names>Dongxu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Li</surname><given-names>Mingming</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Zhu</surname><given-names>Lingyun</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>State Key laboratory of Atmospheric Environment and Extreme Meteorology, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>State Key Laboratory of Infrared Physics, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai, 200083, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>University of Chinese Academy of Sciences, Beijing 100049, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Shanxi Center of Technology Innovation for Environmental Meteorology Forecast and Evaluation, Shanxi Institute of Meteorological Science, Taiyuan 030002, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Civil, Structural and Environmental Engineering, University at Buffalo, Buffalo, NY, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Research and Education in Energy, Environment and Water Institute, University at Buffalo, Buffalo, NY, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Laboratory of Middle Atmosphere and Global Environment Observation, Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Zhaonan Cai (caizhaonan@mail.iap.ac.cn)</corresp></author-notes><pub-date><day>21</day><month>April</month><year>2026</year></pub-date>
      
      <volume>18</volume>
      <issue>4</issue>
      <fpage>2749</fpage><lpage>2767</lpage>
      <history>
        <date date-type="received"><day>10</day><month>August</month><year>2025</year></date>
           <date date-type="rev-request"><day>3</day><month>November</month><year>2025</year></date>
           <date date-type="rev-recd"><day>22</day><month>March</month><year>2026</year></date>
           <date date-type="accepted"><day>5</day><month>April</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Ling Chen 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://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026.html">This article is available from https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e184">An appropriate representation of the NO<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and NO<sub><italic>x</italic></sub> lifetime is essential for estimating NO<sub><italic>x</italic></sub> emissions from satellite NO<sub>2</sub> observations. We introduce a satellite-based, data-driven approach that applies variable NO<inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and derives the nonlinear chemical lifetime using a piecewise fitting method based on the directional derivative approach (DDA). This method enables the estimation of both regional and point-source NO<sub><italic>x</italic></sub> emissions across China, representing the first application of a lightweight, satellite-driven method to directly capture nonlinear NO<sub><italic>x</italic></sub> lifetime for emission estimation over large, topographically complex region. The incorporation of a variable NO<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio enhances the accuracy of source divergence and emission estimates and the improved fitting scheme captures the nonlinear behavior of NO<sub><italic>x</italic></sub> chemistry. Anthropogenic contributions are isolated by subtracting natural sources from satellite-derived total emissions, with natural NO<sub><italic>x</italic></sub> identified using a seasonal criterion and further constrained by Nighttime Light (NTL) data. Estimated anthropogenic NO<sub><italic>x</italic></sub> emissions in China from 2019 to 2024 are 20.2, 18.5, 19.4, 18.9, 20.7 and 18.8 Tg, respectively, with annual uncertainties of 27 %–30 %. These values show good agreement with both bottom-up inventories and top-down inversions, with national scale discrepancies ranging from <inline-formula><mml:math id="M12" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11.8 % to 0.8 %. The DDA captures key spatial and temporal emission patterns, including consistent decline in NO<sub><italic>x</italic></sub> emissions in megacities and provincial disparities linked to urbanization and economic development. The DDA estimates are consistent with previous studies on power plant emissions, and emissions from 124 plants vary between 0.02–2.13 kg s<sup>−1</sup> for 2019–2024, with uncertainties spanning 4 %–78 %, averaging 16 %. This satellite-based, lightweight method enables low-latency, long-term monitoring of NO<sub><italic>x</italic></sub> emissions and offers a promising alternative to bottom-up inventories and resource-intensive top-down models. The data are publicly available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.18923337" ext-link-type="DOI">10.5281/zenodo.18923337</ext-link> (Chen et al., 2026).</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2022YFB3904802</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Shanghai Institute of Technical Physics, Chinese Academy of Sciences</funding-source>
<award-id>-</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="d2e361">Nitrogen oxides (NO<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> NO <inline-formula><mml:math id="M17" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<sub>2</sub>) are key reactive trace gases and major air pollutants in the troposphere, influencing ozone photochemistry, particulate matter and acid rain formation (Galloway et al., 2004). Accurate and near-real-time estimation of NO<sub><italic>x</italic></sub> emissions is crucial for air pollution control and provides a practical approach for estimating co-emitted CO<sub>2</sub> (Reuter et al., 2014, 2019; Miyazaki and Bowman, 2023; Li and Zheng, 2024).</p>
      <p id="d2e410">NO<sub>2</sub> tropospheric vertical column densities (TVCDs) retrieved from new generation satellite instruments at unprecedented high spatiotemporal resolution and accuracy (Verhoelst et al., 2021; van Geffen et al., 2022) have accelerated the development of lightweight, mass conservation-based inversion approaches for top-down NO<sub><italic>x</italic></sub> emission estimation. Methods such as the cross-sectional flux (CSF) (Reuter et al., 2019; Santaren et al., 2025), integrated mass enhancement (IME) (Santaren et al., 2025) and flux divergence approach (FDA) (Beirle et al., 2019, 2021, 2023) have advanced rapidly due to their low computational cost and minimal latency. These methods rely on NO<sub>2</sub> data and approximate meteorological transport velocities to estimate emissions. The CSF and IME methods first identify sources and then integrate emissions within plume contours based on enhancements above background. They are highly sensitive to wind speed and best suited for strong, distinct point sources with synchronous wind observations (Frankenberg et al., 2016; Koene et al., 2024; Krings et al., 2011; Varon et al., 2018). In contrast, the FDA generates a regional emission map and identifies sources by calculating the divergence of the horizontal flux. It is especially effective for detecting point sources without additional a priori knowledge (Ayazpour et al., 2025; Beirle et al., 2019, 2021, 2023; Koene et al., 2024).</p>
      <p id="d2e440">Since its proposal by Beirle et al. (2019), the FDA has been widely applied and refined for NO<sub><italic>x</italic></sub> emissions estimation, primarily driven by TROPOspheric Monitoring Instrument (TROPOMI) NO<sub>2</sub> data (Beirle et al., 2021, 2023; De Foy and Schauer, 2022; Koene et al., 2024). It has also been extended to long-lived gases like CH<sub>4</sub> (Veefkind et al., 2023) and CO<sub>2</sub> (Santaren et al., 2025). The FDA theory recommends explicit background subtraction (Koene et al., 2024), even for short-lived species like NO<sub>2</sub> (Cifuentes et al., 2025). However, a well-defined NO<sub>2</sub> background field may not exist (Koene et al., 2024). In practice, the NO<sub>2</sub> background is either empirically removed (Beirle et al., 2019; De Foy and Schauer, 2022; Rey-Pommier et al., 2022, 2023) or the entire column is treated as the enhanced field (Beirle et al., 2021, 2023). An alternative to the FDA is the directional derivative approach (DDA) as proposed by Sun (2022), which replaces the flux divergence term by a directional derivative, i.e., the inner product between horizontal wind and gradient of column amounts. Both the FDA and DDA establish the link between satellite-observed column amounts and emissions by vertically integrating the three-dimensional continuity equation, incorporating reasonable assumptions and approximations (Ayazpour et al., 2025; Koene et al., 2024). The primary difference between the FDA and DDA is the upper limit of vertical column integration (Ayazpour et al., 2025; Lonsdale and Sun, 2023). Integration in DDA is performed from surface to an intermediate altitude that does not need to be explicitly defined. As demonstrated in Ayazpour et al. (2025), the different upper limit used in the DDA ultimately leads to the directional derivative term and a topography term, which in combination replace the flux divergence term in the FDA. By spatially differentiating the column amounts, the DDA implicitly removes the background field that is invariant at the spatial scale of single grid cells. Another resultant benefit of the DDA is that the adopted horizontal wind does not have to approximate the full wind profile but only the lower levels, which leads to higher accuracy and error tolerance.</p>
      <p id="d2e507">Two key challenges remain for NO<sub><italic>x</italic></sub> emission estimation using the FDA and DDA, including the NO<inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and the nonlinear NO<sub><italic>x</italic></sub> lifetime. When emitted, NO<sub><italic>x</italic></sub> is dominated by NO, which is rapidly oxidized by ozone (O<sub>3</sub>) to form NO<sub>2</sub>. As the plume mixes with ambient air, the balance between NO and NO<sub>2</sub> is determined by the availability of oxidants that oxidizes NO to NO<sub>2</sub> and radiations that photolyze NO<sub>2</sub> to NO. The dominant sink of NO<sub><italic>x</italic></sub> is the reaction between NO<sub>2</sub> and OH, which is modulated by the complex interplay between NO<sub><italic>x</italic></sub>, O<sub>3</sub>, and volatile organic compounds (VOCs) (Laughner and Cohen, 2019). This nonlinear photochemical evolution causes significant variations in the NO<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and NO<sub><italic>x</italic></sub> lifetime, both over time and distance from the emission source (Krol et al., 2024; Meier et al., 2024). Constrained by the availability of observational data and the rationale for maintaining algorithmic efficiency, both existing FDA and DDA applications have necessarily involved substantial simplifications. Previous studies have accounted for the variability of NO<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratios across different pixels using auxiliary data (Beirle et al., 2021, 2023; Ayazpour et al., 2025; Cifuentes et al., 2025; Meier et al., 2024), rather than assuming a constant value (Beirle et al., 2019; De Foy and Schauer, 2022; Lonsdale and Sun, 2023; Sun, 2022). Efforts have also been made to consider factors such as NO<sub><italic>x</italic></sub> concentration, latitude, season (Beirle et al., 2023; Lange et al., 2022) and distance from the emission source (Krol et al., 2024; Meier et al., 2024) to account for the variability of NO<sub><italic>x</italic></sub> lifetime. However, capturing these nonlinear variations (Laughner and Cohen, 2019) remains difficult. Meanwhile, due to the challenges above, most existing studies focus on point sources rather than emissions from large regions.</p>
      <p id="d2e700">In this work, we augment the DDA by applying a variable NO<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio from a global high-resolution chemical transport model and deriving a more realistic nonlinear NO<sub><italic>x</italic></sub> lifetime using an improved satellite data-driven piecewise fitting approach. Based on the augmented DDA, we estimate NO<sub><italic>x</italic></sub> emissions in China from 2019 to 2024. We evaluate the estimated emissions by comparing regional and point-source emissions with bottom-up inventories and top-down datasets. The paper is structured as follows: Sect. 2 describes the input datasets. Section 3 outlines the methods with a focus on NO<sub><italic>x</italic></sub> lifetime fitting, the isolating anthropogenic NO<sub><italic>x</italic></sub> from total emissions, and uncertainties. Section 4 presents the validation, along with the distribution and variations of emissions. Section 5 discusses limitations, followed by the conclusions (Sect. 7).</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>TROPOMI NO<sub>2</sub></title>
      <p id="d2e780">The operational offline TROPOMI NO<sub>2</sub> TVCD product (S5P_L2__NO2___HiR2) (van Geffen et al., 2024) from NASA GES DISC (<uri>https://daac.gsfc.nasa.gov/datasets/</uri>, last access: 17 April 2026) for 2019–2024 is used in this study. TROPOMI is on board of ESA's Sentinel-5 Precursor (S5P) early-afternoon LEO satellite with a high signal-to-noise ratio (Veefkind et al., 2012). It provides global daily coverage with a spatial resolution of 7.0 km <inline-formula><mml:math id="M56" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.5 km before 6 August 2019 and updated to 5.5 km <inline-formula><mml:math id="M57" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.5 km thereafter. The data are filtered according to the following criteria: qa <inline-formula><mml:math id="M58" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.75 and cloud fraction (CF) <inline-formula><mml:math id="M59" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3 to remove very cloudy scenes, ice-snow cover scenes and erroneous retrievals (van Geffen et al., 2022; Verhoelst et al., 2021); solar zenith angle (SZA) <inline-formula><mml:math id="M60" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 65° to exclude observations with low solar elevation, and viewing zenith angles (VZA) <inline-formula><mml:math id="M61" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 56° to minimize unfavorable viewing conditions at the edges of the swath, following Beirle et al. (2023).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Wind fields data</title>
      <p id="d2e846">Wind fields are provided by the European Centre for Medium-Range Weather Forecasts (ECMWF) ERA5 reanalysis data (<uri>https://cds.climate.copernicus.eu/datasets/</uri>, last access: 17 April 2026). The 500 m wind fields are interpolated from hourly data on pressure levels, while the 10 m wind fields are directly obtained from hourly data on single levels. Both datasets have a spatial resolution of 0.25° <inline-formula><mml:math id="M62" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25°. Details on the selection of wind heights and data processing are provided in Sect. 3.1.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Chemical data</title>
      <p id="d2e867">The chemical data for NO and NO<sub>2</sub> are sourced from the Goddard Earth Observing System composition forecast (GEOS-CF) system (<uri>https://gmao.gsfc.nasa.gov/gmao-products/geos-cf/</uri>, last access: 16 April 2026) to derive the NO<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio. GEOS-CF integrates the offline GEOS-Chem chemistry module into the GEOS weather and aerosol modeling system, enabling global near real-time estimates (hindcasts) and 5 d forecasts of atmospheric constituents at a high spatial resolution of 25 km <inline-formula><mml:math id="M65" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 25 km (Keller et al., 2021; Knowland et al., 2022). The NO<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratios are highest near emission sources because freshly emitted NO rapidly consumes local ozone and is subsequently oxidized to NO<sub>2</sub> as the plume mixes with background air (Meier et al., 2024). Following Beirle et al. (2021, 2023), NO<sub>2</sub> columns are converted to NO<sub><italic>x</italic></sub> using the near-surface photostationary state, with the NO<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio from the near-surface model layer with a 1-hour temporal resolution (chm_tavg_1hr_g1440x721_v1) used in this study to better represent near-source conditions and the resulting NO<sub><italic>x</italic></sub> gradients (Ayazpour et al., 2025; Sun, 2022).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Inventories</title>
      <p id="d2e985">Two inventories for natural and anthropogenic sources are used. Soil NO<sub><italic>x</italic></sub> emissions are obtained from the CAMS global emission inventory (<uri>https://ads.atmosphere.copernicus.eu/datasets/cams-global-emission-inventories/</uri>, last access: 17 April 2026), which provides monthly estimates from fertilizer/manure application and atmospheric deposition at a 0.5° resolution (Hoesly et al., 2018; Simpson et al., 2014; Yienger and Levy II, 1995). Since the inventory is updated only until 2018 and soil NO<sub><italic>x</italic></sub> variability is relatively small compared to total emissions, the 2018 data serve as a proxy for 2019–2024.</p>
      <p id="d2e1009">Biomass burning and vegetation fires NO<sub><italic>x</italic></sub> emissions are derived from the CAMS global biomass burning emissions (GFAS) (<uri>https://ads.atmosphere.copernicus.eu/datasets/cams-global-fire-emissions-gfas/</uri>, last access: 17 April 2026). GFAS v1.2 provides near-real-time daily averaged fire NO<sub><italic>x</italic></sub> fluxes using satellite observations of fire radiative power (FRP) on a global 0.1° <inline-formula><mml:math id="M76" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.1° grid (Kaiser et al., 2012). The data covers 2019–2024.</p>
      <p id="d2e1040">Anthropogenic NO<sub><italic>x</italic></sub> emissions for validation are sourced from the Multi-resolution Emission Inventory model for Climate and air pollution research (MEIC, v1.4, 2019–2020, <uri>http://meicmodel.org.cn</uri>, last access: 17 April 2026) and the Emissions Database for Global Atmospheric Research (EDGAR, v8.1, 2019–2022, <uri>https://edgar.jrc.ec.europa.eu</uri>, last access: 17 April 2026). MEIC provides high-resolution, multi-scale databases of anthropogenic emissions for China at a 0.25° <inline-formula><mml:math id="M78" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25° resolution (Geng et al., 2024; Li et al., 2017). EDGAR delivers global coverage at 0.1° <inline-formula><mml:math id="M79" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.1° resolution, with emissions derived through statistical downscaling of national inventories using high-resolution spatial proxies (Crippa et al., 2024; Solazzo et al., 2021).</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Point source data</title>
      <p id="d2e1081">The point source emissions derived from DDA are evaluated against the point source catalog provided by Beirle et al. (2023). For point source detection, their catalog uses coal, gas, and oil power plants with capacities <inline-formula><mml:math id="M80" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 100 MW from the Global Power Plant Database (Byers et al., 2019), identifying over 1100 NO<sub><italic>x</italic></sub> point sources worldwide. Their validation shows good agreement in Germany and the United States, demonstrating the catalog's reliability.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Nighttime light data</title>
      <p id="d2e1108">NASA's Black Marble nighttime lights (NTL) product suite, derived from the Visible Infrared Imaging Radiometer Suite (VIIRS) Day/Night Band (DNB) onboard the Suomi National Polar-orbiting Partnership (SNPP), serves as a constraint on anthropogenic emissions (Román et al., 2018; Wang et al., 2021). The Lunar BRDF-Adjusted Nighttime Lights Yearly L3 Global 15 arcsec Linear Lat/Lon Grid product (VNP46A4) provides high spatial resolution at 500 m and is available from January 2012 onward (<uri>https://viirsland.gsfc.nasa.gov/Products/NASA/BlackMarble.html</uri>, last access: 17 April 2026). This study uses data from 2019 to 2023. Due to the current unavailability of VNP46A4 data for 2024, the 2023 dataset is applied as a substitute.</p>
</sec>
<sec id="Ch1.S2.SS7">
  <label>2.7</label><title>National accounts data</title>
      <p id="d2e1122">National accounts data of annual Gross Domestic Product (GDP) and provincial Gross Regional Product (GRP) are from National Bureau of Statistics of China (<uri>https://data.stats.gov.cn</uri>, last access: 17 April 2026).</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Framework of the directional derivative approach</title>
      <p id="d2e1144">The mathematical framework of the DDA is detailed in Sun (2022) and further developed by Ayazpour et al. (2025). Based on satellite-observed NO<sub>2</sub> TVCDs, NO<sub><italic>x</italic></sub> emissions <inline-formula><mml:math id="M84" display="inline"><mml:mi>E</mml:mi></mml:math></inline-formula> can be estimated as:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M85" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi>E</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mo>(</mml:mo><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mi>X</mml:mi><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mi mathvariant="italic">τ</mml:mi></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          where <inline-formula><mml:math id="M86" display="inline"><mml:mi mathvariant="normal">∇</mml:mi></mml:math></inline-formula> denotes the two-dimensional horizontal vector differential operator in Cartesian coordinates, i.e., <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. No terrain-following coordinate system is used in this formulation. <inline-formula><mml:math id="M90" display="inline"><mml:mi mathvariant="normal">Ω</mml:mi></mml:math></inline-formula> is NO<sub>2</sub> TVCD, <inline-formula><mml:math id="M92" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> is the NO<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio, <inline-formula><mml:math id="M94" display="inline"><mml:mi mathvariant="bold-italic">u</mml:mi></mml:math></inline-formula> is the profile-weighted horizontal wind from surface to a conceptual altitude (<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) which is not explicitly needed and defined, <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is surface wind, and <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is surface altitude. <inline-formula><mml:math id="M98" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M99" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> are fitting parameters representing the inverse of scale height and NO<sub><italic>x</italic></sub> lifetime, respectively. The tendency term (<inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mo>∂</mml:mo><mml:mo>(</mml:mo><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:math></inline-formula>) becomes negligible when averaging over a month or longer or under the steady-state approximation. It should be noted that this approximation may not hold for a single satellite overpass, potentially leading to significant errors (Koene et al., 2024). Assuming <inline-formula><mml:math id="M102" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M103" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> stay constant over the averaging period, the spatiotemporal averaged emissions <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mi>E</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> for a given time period and horizontal resolution can be expressed as:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M105" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mi>E</mml:mi></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mfenced open="〈" close="〉"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mfenced open="〈" close="〉"><mml:mrow><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mi>X</mml:mi><mml:mfenced close="〉" open="〈"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced></mml:mrow><mml:mi mathvariant="italic">τ</mml:mi></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          Here, the operator <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:mo>〉</mml:mo></mml:mrow></mml:math></inline-formula> denotes spatiotemporal averaging. The first and second terms of Eq. (2) are referred as the DDf estimator (Ayazpour et al., 2025), reflecting the contributions of advection transport to local NO<sub><italic>x</italic></sub> emissions. The third component is the topography correction as emphasized by Ayazpour et al. (2025), it is directly derived from the continuity equation rather than serving merely as an empirical adjustment (Koene et al., 2024). The sum of the first three terms is referred to as DDf_topo estimator. The last term describes the NO<sub><italic>x</italic></sub> chemistry approximated by first-order loss.</p>
      <p id="d2e1593">Integration in DDA is performed from <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to an intermediate altitude <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. While the ideal approach would involve winds at all vertical levels, the full wind profile is typically unavailable. Instead, a single-layer wind, known as the effective wind field, is used to approximate the average state of the full profile. Ayazpour et al. (2025) utilized the effective wind field height using WRF-CMAQ simulations and found that the 500 m wind is most suitable, which aligns with Beirle et al. (2023). Consequently, the horizontal wind <inline-formula><mml:math id="M111" display="inline"><mml:mi mathvariant="bold-italic">u</mml:mi></mml:math></inline-formula> is interpolated to 500 m above the surface, while <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> directly obtained as the 10 m wind from ERA5.</p>
      <p id="d2e1636">To apply Eq. (2), the physics-based oversampling approach (Sun et al., 2018) is used to resample the level 2 pixels into 0.025° <inline-formula><mml:math id="M113" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.025° grid cells with appropriate weighting, then coarsened to 0.05° <inline-formula><mml:math id="M114" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05°. Winds in ERA5, the NO<inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio (<inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in GEOS-CF data are resampled to match this spatial resolution and temporally aligned with satellite overpasses, allowing for the calculation of all bracketed terms in Eq. (2). Yearly NTL data from SNPP/VIIRS are also resampled at the same spatial resolution. The spatial differentiation in gradient calculation is conducted on 0.05° <inline-formula><mml:math id="M117" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05° grid cells with second order central difference. All bracketed terms are averaged at a monthly scale before <inline-formula><mml:math id="M118" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M119" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> are fitted (see in Sect. 3.2) to derive emissions <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mfenced close="〉" open="〈"><mml:mi>E</mml:mi></mml:mfenced></mml:mrow></mml:math></inline-formula> in mol m<sup>−2</sup> s<sup>−1</sup>, and the conversion to mass assumes NO<sub><italic>x</italic></sub> as NO<sub>2</sub>.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Nonlinear NO<sub><italic>x</italic></sub> lifetime fitting</title>
      <p id="d2e1772">To avoid additional assumptions and external computations (Beirle et al., 2021, 2023), DDA performs a data-driven fitting approach based on monthly fluxes to determine <inline-formula><mml:math id="M126" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M127" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> across grids with negligible emissions (<inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mfenced open="〈" close="〉"><mml:mi>E</mml:mi></mml:mfenced><mml:mo>≈</mml:mo></mml:mrow></mml:math></inline-formula> 0) (Ayazpour et al., 2025; Lonsdale and Sun, 2023; Sun, 2022), where Eq. (2) can be rewritten as:

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M129" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mfenced open="〈" close="〉"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mfenced open="〈" close="〉"><mml:mrow><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mfenced open="〈" close="〉"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mfenced close="〉" open="〈"><mml:mrow><mml:mi>f</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced><mml:mo>+</mml:mo><mml:mi mathvariant="italic">ε</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          Here,  <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is an estimate of <inline-formula><mml:math id="M131" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is an estimate of the inverse of <inline-formula><mml:math id="M133" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M135" display="inline"><mml:mi mathvariant="italic">ε</mml:mi></mml:math></inline-formula> represent the offset and random error in the predicted variable, which cannot be accounted for by any linear combinations of predictors.</p>
      <p id="d2e1961">Both the FDA and DDA methods in prior studies have exhibited substantial negative emissions and/or underestimation of total emissions (Ayazpour et al., 2025; Beirle et al., 2019, 2021, 2023; De Foy and Schauer, 2022; Lonsdale and Sun, 2023; Sun, 2022). A single <inline-formula><mml:math id="M136" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> fitted in relatively clean region tends to overestimate the chemistry lifetime, then the NO<sub><italic>x</italic></sub> flux is underestimated. Therefore, a more realistic representation of NO<sub><italic>x</italic></sub> lifetime is critical for accurate emission estimation (Beirle et al., 2023; Krol et al., 2024; Laughner and Cohen, 2019; Meier et al., 2024). The photochemical reactions of NO<sub><italic>x</italic></sub>–O<sub>3</sub>–VOCs depends on the concentrations of NO<sub><italic>x</italic></sub>, O<sub>3</sub>, and VOCs, as well as on photolysis and meteorological conditions (Pusede et al., 2015; Sillman et al., 1990; Souri et al., 2023). Even under identical NO<sub><italic>x</italic></sub> concentrations and at the same latitude (Beirle et al., 2023; Lange et al., 2022), the lifetime still vary considerably due to the complex interplay of NO<sub><italic>x</italic></sub> and VOC chemistry (Laughner and Cohen, 2019).</p>
      <p id="d2e2044">To derive more realistic lifetime, we fit <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> across stratified column amount intervals <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:mo>〈</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:mo>〉</mml:mo></mml:mrow></mml:math></inline-formula> within subregions instead of fitting a single lifetime across the domain to account for the NO<sub><italic>x</italic></sub> reactivity nonlinearity. We partition the study domain into four subregions by employing NO<sub><italic>x</italic></sub> concentration as the primary criterion due to its dominant control over chemical lifetime (Pusede et al., 2015) with additional consideration of latitude and terrain effects. Figure 1a shows the four subregions. The east (E) and west (W) sections are divided by the Hu line (HL) that extends from Heihe (127.54° E, 50.25° N) to Tengchong (98.50° E, 25.03° N). The E and W sections are further subdivided into north (N) and south (S) subregions by latitudes 35° N for the west and 30° N for the east. The resultant four subregions are denoted as WN, WS, EN, ES thereafter. The HL is a well-known natural geographical boundary that divides China into two contrasting regions in terms of terrain, climate, population density, and economic activity. The eastern part, encompassing most of China's plains and rivers (Fig. 1b), is dominated by the East Asian monsoon, supports 96 % of the population, contributes the majority of national productivity, and faces severe air pollution. In contrast, the western region is characterized by elevated terrain, a westerly climate, and sparse population (Hu, 1935; Zhang et al., 2022). So, the above factors implicitly account for variations in O<sub>3</sub> and its precursors influenced by human activities (Jin et al., 2020; Martin et al., 2004; Souri et al., 2023), differences in natural VOCs emissions from vegetation under varying climatic and geographical conditions (Guenther et al., 1995; Sprengnether et al., 2002; Palmer et al., 2006), and meteorological influences on transport and photochemistry (Duncan et al., 2010; Li et al., 2020; Pusede et al., 2015).</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e2100">Four subregions divided by the Hu line and <bold>(a)</bold> average NO<sub>2</sub> TVCDs of 2019 as an example; <bold>(b)</bold> altitude.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f01.png"/>

        </fig>

      <p id="d2e2124">Given the small interannual variability and limited impact on reactive species emission estimation (Ayazpour et al., 2025), <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is fitted using the same climatological months, whereas <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is fitted for each individual month using NO<sub>2</sub> TVCD percentile bins constructed independently for that month and subsequently averaged over the same months for each subregion during 2019–2024. First, <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is fitted in grid cells with rough terrain (0.001 m s<inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>&lt;</mml:mo><mml:mfenced close="〉" open="〈"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>&lt;</mml:mo></mml:mrow></mml:math></inline-formula> 0.1 m s<sup>−1</sup>), where emissions are negligible (DDf <inline-formula><mml:math id="M157" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 5 <inline-formula><mml:math id="M158" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>−9</sup> mol m<sup>−2</sup> s<sup>−1</sup>). Then, <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is fitted in flat terrain (where <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mfenced open="〈" close="〉"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:msub><mml:mi>z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfenced><mml:mo>&lt;</mml:mo></mml:mrow></mml:math></inline-formula> 0.001 m s<sup>−1</sup>) without strong NO<sub><italic>x</italic></sub> emission sources (DDf_topo <inline-formula><mml:math id="M166" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 10<sup>−10</sup> mol m<sup>−2</sup> s<sup>−1</sup>). The fitting is performed across piecewise bins defined by NO<sub>2</sub> TVCD percentiles. TVCD percentiles are binned at 10 % intervals for each month in WN and EN, while in WS and ES, due to narrower lower percentile ranges, bin widths are expanded to 20 % below the 80th percentile and remain 10 % above it to ensure robust fitting performance. For month-bins where fitting fails (<inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), appropriate adjustments are made by merging neighboring bins or revising percentile thresholds. A total of 1393 month-bins are successfully fitted across the four subregions. The number of grid cells per bin ranges from 3 to 9388 (10th percentile: 17; median: 91; mean: 199), indicating that most bins contain sufficient data for robust lifetime fitting, while bins with very small sample sizes are rare and have negligible influence on the overall regression. For each subregion, average TVCD and <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> per month-bin are calculated from successfully fitted bins. TVCDs can be grouped into intervals as described above, the mean TVCD of each interval is matched to the nearest month-bin and the corresponding <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is used to calculate flux.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Anthropogenic NO<sub><italic>x</italic></sub> emissions separation</title>
      <p id="d2e2447">The DDA quantifies total NO<sub><italic>x</italic></sub> emissions, from which anthropogenic contributions to the total emission rates over a certain area need to be isolated by subtracting natural sources. Globally, anthropogenic emissions dominant, while natural sources, such as soil emissions, biomass burning, and lightning, account for approximately 30 %–40 % (Jaeglé et al., 2005; Müller and Stavrakou, 2005). Regional variation of natural sources contributions is substantial, with around 14 % in East Asia (Zhao and Wang, 2009), and 8 % in eastern China (Lin, 2012). Nevertheless, these estimates involve significant uncertainties (Ding et al., 2017; Rey-Pommier et al., 2022), including potential underestimation (Song et al., 2021). Previous studies typically designated regions dominated by anthropogenic emissions as mean NO<sub>2</sub> TVCDs higher than 1.0 <inline-formula><mml:math id="M178" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>15</sup> molec. cm<sup>−2</sup> (Li and Zheng, 2024; Liu et al., 2016a). However, due to the presence of unexpectedly high or poorly understood natural NO<sub><italic>x</italic></sub> emissions over this threshold (Kong et al., 2023; Song et al., 2021), it is not applied to filter natural sources in this study. Since natural NO<sub><italic>x</italic></sub> is primarily emitted during the summer and remains low in winter (Liu et al., 2016a; van der A et al., 2006), while anthropogenic NO<sub><italic>x</italic></sub> emissions typically peak in winter (Lonsdale and Sun, 2023), we identify natural-source grid cells based on seasonal criterion and further constrain them using NTL data. Grid cells with either the highest averaged NO<sub>2</sub> TVCDs in summer or the lowest values in winter comparing to other seasons, and with NTL <inline-formula><mml:math id="M185" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.01 nW cm<sup>−2</sup> sr<sup>−1</sup>, are classified as natural NO<sub><italic>x</italic></sub> sources and excluded from the areal integration to get anthropogenic NO<sub><italic>x</italic></sub> emission rates. For the remaining grid cells, we subtract soil and biomass burning emissions (from CAMS data) from the satellite-derived emissions to isolate anthropogenic contributions.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Uncertainty analysis</title>
      <p id="d2e2591">To quantify uncertainties, DDf is calculated as the mean directional derivative along the zonal/meridional (<inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="bold-italic">y</mml:mi></mml:mrow></mml:math></inline-formula>) and diagonal directions (<inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">r</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="bold-italic">s</mml:mi></mml:mrow></mml:math></inline-formula>) (Li et al., 2026) on a 0.05° <inline-formula><mml:math id="M192" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05° grid: 

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M193" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="normal">DDf</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>/</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced><mml:mrow><mml:mi>x</mml:mi><mml:mo>/</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfenced><mml:mrow><mml:mi>x</mml:mi><mml:mo>/</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="normal">DDf</mml:mi><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow></mml:mfenced><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">∇</mml:mi><mml:mi>f</mml:mi></mml:mrow></mml:mfenced><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>r</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>r</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>r</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>r</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Ω</mml:mi><mml:msub><mml:mi>u</mml:mi><mml:mi>s</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>f</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          Standard deviation of the difference between DDf<sub><italic>x</italic>∕<italic>y</italic></sub> and DDf<sub><italic>r</italic>∕<italic>s</italic></sub> is used to estimate random error <inline-formula><mml:math id="M196" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> of DDf:

            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M197" display="block"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">SD</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">DDf</mml:mi><mml:mrow><mml:mi>x</mml:mi><mml:mo>/</mml:mo><mml:mi>y</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">DDf</mml:mi><mml:mrow><mml:mi>r</mml:mi><mml:mo>/</mml:mo><mml:mi>s</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          The random errors at daily, monthly, and annual scales for 2019–2024 consistently decrease as the mean satellite data coverage (<inline-formula><mml:math id="M198" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>) increases (Fig. 2). This observed scaling follows the theoretical relationship <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:msqrt><mml:mi>N</mml:mi></mml:msqrt></mml:mrow></mml:math></inline-formula> (black line in Fig. 2), in agreement with the central limit theorem for independent random errors. Here, <inline-formula><mml:math id="M200" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reflects the precision of a single satellite overpass, calculated at the monthly scale as:

            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M201" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">exp</mml:mi><mml:mo>(</mml:mo><mml:mo>〈</mml:mo><mml:mi mathvariant="normal">log</mml:mi><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>⋅</mml:mo><mml:mo>〈</mml:mo><mml:mi mathvariant="normal">log</mml:mi><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>〉</mml:mo><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> denote the random error and mean satellite coverage for month <inline-formula><mml:math id="M204" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, respectively. The results further demonstrate that temporal averaging effectively reduces random errors in emission quantification.</p>

      <fig id="F2"><label>Figure 2</label><caption><p id="d2e3167">The relationship between the random error (<inline-formula><mml:math id="M205" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) and mean satellite data coverage (<inline-formula><mml:math id="M206" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>) at different time scales.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f02.png"/>

        </fig>

      <p id="d2e3190">Since the topography correction and chemical loss terms in Eq. (2) are determined through fitting, only the overall Root Mean Square Error (RMSE) can be evaluated, rather than grid-level precision. Therefore, the random error of DDf is employed to characterize the uncertainties in DDA emission estimation, encompassing both satellite retrieval noise and the random error arising from the DDf estimator.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Results</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Effects of NO<inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio correction and lifetime fitting</title>
      <p id="d2e3228">To illustrate the developments in this study, Fig. 3 compares three DDA-based results before and after applying the NO<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio correction and improved fitting scheme: (1) a constant NO<inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio of 1.32 and monthly single-lifetime fitting (fixed_<inline-formula><mml:math id="M210" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> and single_<inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, corresponding to the original DDA framework by Sun (2022); (2) the variable NO<inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and monthly single-lifetime fitting (variable_<inline-formula><mml:math id="M213" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> and single_<inline-formula><mml:math id="M214" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>), based on the modification by Ayazpour et al. (2025) and marking the first application of GEOS-CF chemical data in satellite-based emission estimation; (3) a combination of the variable NO<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and piecewise fitting with nonlinear NO<sub><italic>x</italic></sub> lifetime for each month (variable_<inline-formula><mml:math id="M217" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> and nonlinear_<inline-formula><mml:math id="M218" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>), while the latter represents the major improvement in this study. Using a variable NO<inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio better captures strong NO<sub><italic>x</italic></sub> gradients near point sources, improving the accuracy of point source emission estimates. However, this approach still leads to notable underestimation of regional emissions. The nonlinear lifetime fitting more effectively accounts for the balance among local emissions, horizontal transport, and chemical loss, reducing negative emission grids and increasing regional emission estimates. Consequently, the improved fitting scheme minimizes artifacts in mountainous and remote regions compared to earlier results (Ayazpour et al., 2025; Beirle et al., 2023; Lonsdale and Sun, 2023; Sun, 2022).</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>NO<sub><italic>x</italic></sub> lifetime</title>
      <p id="d2e3399">The lifetime of NO<sub><italic>x</italic></sub> is known as a complicated function of NO<sub><italic>x</italic></sub> chemistry regimes (Laughner and Cohen, 2019). At very low NO<sub><italic>x</italic></sub> concentration, NO<sub><italic>x</italic></sub> lifetime increases with NO<sub><italic>x</italic></sub> concentration. As NO<sub><italic>x</italic></sub> concentration rises, the lifetime decreases because increased NO enhances the chain reactions involving organic compounds (RH) and HO<sub><italic>x</italic></sub> (HO<inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> OH <inline-formula><mml:math id="M230" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HO<inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> RO<sub>2</sub>), accelerating RH oxidation to produce O<sub>3</sub> (“NO<sub><italic>x</italic></sub>-limited” regime) and further oxidizing NO. At high NO<sub><italic>x</italic></sub> concentration, as NO<sub><italic>x</italic></sub> reaches saturation, the reaction between OH and NO<sub>2</sub> becomes much faster than the reaction between OH and RH, dominating the fate of HO<sub><italic>x</italic></sub> and slowing O<sub>3</sub> production (“NO<sub><italic>x</italic></sub>-suppressed” regime), resulting in the opposite trend in NO<sub><italic>x</italic></sub> lifetime (Laughner and Cohen, 2019; Pusede et al., 2015).</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e3591">Comparison of three DDA-based results, including <bold>(a)</bold> anthropogenic NO<sub><italic>x</italic></sub> emissions estimates in China for 2019 and <bold>(b)</bold> spatial distribution in Shanxi province for 2019, shown as an example of complex topography.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f03.png"/>

        </fig>

      <p id="d2e3615">Figure 4 shows the monthly climatology of NO<sub><italic>x</italic></sub> lifetimes from the improved fitting scheme described in Sect. 3.2. For each subregion and each climatological month, the fitted lifetime is shown as bubbles corresponding to bins of NO<sub>2</sub> TVCD. The size of bubbles scales with the mean NO<sub>2</sub> TVCD for the bin. The results clearly demonstrate the nonlinear variability of NO<sub><italic>x</italic></sub> lifetime as a function of TVCDs and show significant discrepancies between subregions. The results closely match the theoretical calculated NO<sub><italic>x</italic></sub> lifetime versus NO<sub><italic>x</italic></sub> concentrations under different VOC reactivities by Laughner and Cohen (2019), capturing the turning points marked by an increase in lifetime at low NO<sub><italic>x</italic></sub> concentrations (region I), the subsequent decrease with rising NO<sub><italic>x</italic></sub> (region II), and the eventual increase under NO<sub><italic>x</italic></sub>-saturated conditions (region III). The range of lifetimes vary from 0.71–26.47 h, and the average values across the subregions range from 3.17–7.85 h. Due to fitting failures in July–August, the number of bins in WN is substantially reduced, requiring broad bin merging and resulting in lifetimes that are likely overestimated and unrepresentative. The results are consistent with the 2–8 h range reported by Lange et al. (2022) as well as the 2 h (low NO<sub>2</sub>) to over 7 h (high NO<sub>2</sub>) given by Laughner and Cohen (2019).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e3721">Monthly NO<sub><italic>x</italic></sub> lifetimes for <bold>(a)</bold> WN, <bold>(b)</bold> WS, <bold>(c)</bold> EN, and <bold>(d)</bold> ES. The bubble size indicates monthly mean NO<sub>2</sub> TVCD (<inline-formula><mml:math id="M256" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi></mml:mrow></mml:math></inline-formula> m<sup>−2</sup>) per bin. The <inline-formula><mml:math id="M258" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> <bold>(h)</bold>, <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> (coefficient of determination), and RMSE (root mean square error, nmol m<sup>−2</sup> s<sup>−1</sup>) for each subregion represent the month-bin averages. <inline-formula><mml:math id="M262" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> denotes the count of fitting grids across all months.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f04.png"/>

        </fig>

      <p id="d2e3836">The consistent lifetime patterns highlight the dominant role of NO<sub><italic>x</italic></sub> concentration in determining <inline-formula><mml:math id="M264" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>. However, even at comparable NO<sub><italic>x</italic></sub> levels and over the same periods, <inline-formula><mml:math id="M266" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> exhibits subregional variations driven by distinct ambient conditions (e.g., O<sub>3</sub> and VOCs concentrations, meteorological parameters) and differences in NO<sub><italic>x</italic></sub> emission sources. WN is located in the northern China, sees increased NO<sub><italic>x</italic></sub> emissions during the colder half of the year due to heating demand. WS is situated on the sparsely populated Tibetan Plateau, has primarily natural NO<sub><italic>x</italic></sub> sources, including unexpectedly high NO emissions from lakes (Kong et al., 2023). EN exhibits distinct anthropogenic emissions, with higher NO<sub><italic>x</italic></sub> and longer <inline-formula><mml:math id="M272" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> in winter due to heating, and lower NO<sub><italic>x</italic></sub> in summer, where intense photochemical reactions result in a shorter <inline-formula><mml:math id="M274" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>. ES is located in southern China with smaller annual temperature variations, shows less pronounced seasonal discrepancies in <inline-formula><mml:math id="M275" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>. Additionally, high natural VOCs emissions during the growing season of vegetables (Cao et al., 2022) in ES contribute to a longer <inline-formula><mml:math id="M276" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> (Laughner and Cohen, 2019).</p>
      <p id="d2e3955">We provide detailed comparisons of the lifetime fitting parameters for the three DDA-based approaches in Table S1 in the Supplement. The variable NO<inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio correction improves the accuracy of source divergence and emission estimates, while the piecewise fitting approach captures nonlinear NO<sub><italic>x</italic></sub> chemistry and yields a shorter overall lifetime with lower fitting RMSE. Across the four subregions, NO<sub><italic>x</italic></sub> lifetimes without ratio correction and fitting scheme improvement are approximately 2 to 3 times those derived in this study, specifically 1.7 times in ES, 2.8–2.9 times in EN and WN, and 3.3 times in WS (figure omitted), although the values primarily represent the mean state associated with the nonlinear characterization of lifetime. These results highlight the great importance of accounting for the variable NO<inline-formula><mml:math id="M280" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and nonlinear NO<sub><italic>x</italic></sub> lifetime, particularly in clean and heavily polluted regions, while the influence is comparatively less pronounced in moderately polluted areas.</p>
      <p id="d2e4019">In addition, the scale height (<inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi>X</mml:mi></mml:mrow></mml:math></inline-formula>) fitting results for each subregion are presented in Fig. S1. Scale height shows clear seasonal and regional variability, generally higher in the cleaner and more remote regions (WN and WS) than in the more polluted regions (EN and ES). Its variability is primarily controlled by boundary layer mixing, as <inline-formula><mml:math id="M283" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> links surface concentration to column density, reflecting the effective vertical mixing depth (Lonsdale and Sun, 2023; Sun, 2022).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Regional NO<sub><italic>x</italic></sub> emissions</title>
<sec id="Ch1.S4.SS3.SSS1">
  <label>4.3.1</label><title>Comparison with inventories</title>
      <p id="d2e4066">The spatial distribution of national anthropogenic NO<sub><italic>x</italic></sub> emissions based on DDA in China for 2019 is shown in Fig. 5a, with the corresponding total emissions provided in Fig. S2. The identified hotspots align closely with areas of intensive human activity, covering both urban and rural regions as well as transportation routes. Traces of faint anthropogenic emissions remain clearly visible even in the remote, sparsely populated Northwest China (Fig. S3).</p>
      <p id="d2e4078">The derived anthropogenic emissions of China from 2019 to 2024 are compared with: (1) two bottom-up emission inventories (MEIC and EDGAR), and (2) two top-down datasets, the Inversed Emission Inventory for Chinese Air Quality (CAQIEI) (Kong et al., 2024) and results from Li and Zheng (2024). CAQIEI assimilates surface observations using an ensemble Kalman filter (EnKF) and the Nested Air Quality Prediction Modeling System, while the results provided by Li and Zheng (2024) are based on TROPOMI NO<sub>2</sub> combined with GEOS-Chem. Note that these datasets are only available in limited years, while DDA covers all years. National scale comparisons show that DDA agrees well with other inventories and produces slightly lower estimates (Fig. 5b). Based on DDA calculations, the anthropogenic NO<sub><italic>x</italic></sub> emissions of China are estimated to be 20.2, 18.5, 19.4, 18.9, 20.7 and 18.8 Tg from 2019 to 2024, with uncertainties of 27 %–30 %. The corresponding total emissions are 29.8, 28.8, 28.7, 28.2, 28.7 and 27.4 Tg, respectively, with uncertainties of 29 %–32 %. These results indicate fluctuating trends in anthropogenic NO<sub><italic>x</italic></sub> emissions: a sharp decline in 2020 due to the COVID-19 lockdowns (Lonsdale and Sun, 2023; Miyazaki et al., 2021; Cooper et al., 2022), a modest rebound in 2021–2022, a peak in 2023 (surpassing 2019 levels despite total NO<sub><italic>x</italic></sub> remaining lower), and a subsequent drop in 2024 to 7.1 % below 2019 levels. The differences between DDA and EDGAR, MEIC, CAQIEI and Li and Zheng are <inline-formula><mml:math id="M290" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.7 % to 0.8 %, <inline-formula><mml:math id="M291" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.3 % to <inline-formula><mml:math id="M292" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.4 %, <inline-formula><mml:math id="M293" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.2 % to <inline-formula><mml:math id="M294" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.5 %, and <inline-formula><mml:math id="M295" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11.8 % to <inline-formula><mml:math id="M296" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.8 %, respectively. Notably, the DDA approach provides long-term emission estimates with low latency, demonstrating a key advantage of this satellite-based lightweight estimation method over conventional bottom-up inventories and computationally intensive top-down data assimilation systems.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e4169">National anthropogenic NO<sub><italic>x</italic></sub> emissions of China for <bold>(a)</bold> spatial distribution at 0.05° <inline-formula><mml:math id="M298" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05°, with 2019 as an example, and <bold>(b)</bold> comparisons with previous inventories from 2019–2024.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f05.png"/>

          </fig>

      <p id="d2e4201">The primary cause of the lower estimates is the systematic low bias in TROPOMI NO<sub>2</sub> column amounts (Beirle et al., 2023; Liu et al., 2024), most likely due to a priori assumptions and a tropospheric negative bias of approximately 30 % from ground-based validation (van Geffen et al., 2022). Meanwhile, we attribute a larger proportion of total emissions to natural sources compared to the latter two top-down methods, varying between 28.1 %–35.6 %, with an average of 32.1 % (Fig. S4). CAQIEI assigned soil and biomass burning NO<sub><italic>x</italic></sub> from CAMS and GFAS as natural sources (approximately 2.0 Tg) and subtracts them from the total NO<sub><italic>x</italic></sub> estimates (23.8 Tg in 2019 and 21.4 Tg in 2020, relative to 29.8 and 28.8 Tg in DDA). While Li and Zheng (2024) designated regions dominated by natural emissions as grids with mean NO<sub>2</sub> TVCDs less than 1.0 <inline-formula><mml:math id="M303" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<sup>15</sup> molec. cm<sup>−2</sup>, this threshold is not applied in this study, as described in Sect. 3.3. Based on satellite observations, Kong et al. (2023) found unexpectedly high NO emissions from remote lakes on the Tibetan Plateau, with per-unit-area emissions exceeding those from crop fields in summer. Lin et al. (2024) highlighted a severe underestimation of soil NO<sub><italic>x</italic></sub> in the current CAMS inventory, while Opacka et al. (2025) also identified underestimated soil and lightning NO<sub><italic>x</italic></sub>. Using natural nitrogen isotopes in precipitation to trace atmospheric NO<sub><italic>x</italic></sub> sources, Song et al. (2021) showed that the relative contributions of natural NO<sub><italic>x</italic></sub> average 57 <inline-formula><mml:math id="M310" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 13 % in East Asia, a value that had long been underestimated. In this work, we identify natural sources based on seasonal emission patterns and constrain them with NTL data. From 2019 to 2023, the number of grid cells indicative of human activity increased by 48.6 % (Fig. S5). As a result, anthropogenic NO<sub><italic>x</italic></sub> emissions in 2023 are 0.5 Tg higher than in 2019, despite total NO<sub><italic>x</italic></sub> in 2023 being 1.1 Tg lower.</p>
      <p id="d2e4331">Table S2 shows NO<sub><italic>x</italic></sub> emissions from sensitivity tests of the anthropogenic NO<sub><italic>x</italic></sub> filter threshold, and Fig. S6 presents the probability density function (PDF) of NTL to support the selection of the NTL threshold. The results indicate that without applying the NTL constraint, anthropogenic NO<sub><italic>x</italic></sub> emissions would be underestimated. The differences among results obtained with different NTL thresholds are relatively small (<inline-formula><mml:math id="M316" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>4.9 % to 3.6 %). Under the selected threshold of 0.01 nW cm<sup>−2</sup> sr<sup>−1</sup>, more than 90 % of NTL grids are identified as anthropogenic sources, and this threshold also helps minimize the resampling effect from 500 m to 0.05° in dark regions. Overall, the small differences among different thresholds and the good agreement with other datasets demonstrate the robustness of the anthropogenic NO<sub><italic>x</italic></sub> source filtering approach used in this study. Although separating anthropogenic and natural sources in dimly lit grids remains challenging, it is clear that natural emissions in China are indeed underestimated, as noted by Song et al. (2021) and isolating these contributions from total emissions continues to require further work.</p>
      <p id="d2e4402">For subnational scale (Fig. 6a, b), DDA shows excellent agreement with inventories in the Central, North, and Southwest regions; slightly higher values in the Northeast and Northwest; somewhat lower values in the South; and significantly lower values in East China during 2019–2020. The results also demonstrate a stronger consistency between DDA and MEIC (The Pearson correlation coefficient (<inline-formula><mml:math id="M320" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) ranges from 0.86–0.87) compared to EDGAR (<inline-formula><mml:math id="M321" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> 0.76–0.79). MEIC uses high-resolution localized data, while EDGAR relies on coarser global datasets, resulting in discrepancies in spatial allocation accuracy for China (Crippa et al., 2024; Liu et al., 2016b). Given the good agreement of DDA with inventories in 2019–2021 (Fig. 5b), the discrepancy with EDGAR in 2022 does not undermine the reliability of the estimates in this work, despite the current lack of inventories for comparison.</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e4421">Comparisons of anthropogenic NO<sub><italic>x</italic></sub> emissions between DDA, MEIC and EDGAR for <bold>(a)</bold> national and subnational scales in 2019, and <bold>(b)</bold> same as <bold>(a)</bold> but in 2020, <bold>(c)</bold> provincial scale in 2019.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f06.png"/>

          </fig>

      <p id="d2e4451">At the provincial scale (Fig. 6c), NO<sub><italic>x</italic></sub> emissions derived from DDA align well with bottom-up inventories, with about 80 % of provinces falling within <inline-formula><mml:math id="M324" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>60 % of MEIC and EDGAR. DDA shows consistently lower emissions in economically developed provinces (mostly in East and South China) and higher in less developed western provinces. The significant difference in Xizang's emissions arises from DDA identifying substantially more human activity than reported in inventories.</p>
</sec>
<sec id="Ch1.S4.SS3.SSS2">
  <label>4.3.2</label><title>Differentiated patterns in provincial NO<sub><italic>x</italic></sub> emissions changes</title>
      <p id="d2e4488">The anthropogenic NO<sub><italic>x</italic></sub> emissions map reveals a significant decline in urban areas, particularly in heavily pollutant regions, from 2019 to 2024 (Fig. 7a). However, certain localized areas or point sources, particularly those in the Northeast, Northwest, and South, exhibit noticeable increases. At provincial scale (Fig. 7b), NO<sub><italic>x</italic></sub> emissions increase by less than 10 % in Gansu, Hunan, and Inner Mongolia; by 10 %–30 % in Chongqing, Guangxi, Qinghai, Yunnan, and Xinjiang; and by more than 50 % in Xizang. At the subnational scale (Fig. 7c), which aggregates total emissions from provincial groups, NO<sub><italic>x</italic></sub> emissions decline by more than 10 % in the North and East, and by less than 10 % in the Northeast, Central, and South, while slight increases under 10 % are observed in the Southwest and Northwest. Year-on-year changes in anthropogenic emissions from 2020 to 2024 are shown in Fig. S7. In other words, NO<sub><italic>x</italic></sub> emissions at the provincial scale display a differentiated temporal pattern, with declines in the central and eastern regions but increases in the west.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e4529">Changes in anthropogenic NO<sub><italic>x</italic></sub> emissions from 2019 to 2024, <bold>(a)</bold> grid scale at 0.05° <inline-formula><mml:math id="M331" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.05°, <bold>(b)</bold> provincial scale, and <bold>(c)</bold> subnational scale.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f07.png"/>

          </fig>

      <p id="d2e4563">Air pollutant emissions evolve in response to urbanization and macroeconomic development, which influence policy regulations and industrial restructuring, forming a feedback loop that further shapes economic growth at both national and city scales (Miyazaki and Bowman, 2023; Wang et al., 2019). Anthropogenic NO<sub><italic>x</italic></sub> emissions constrained by nighttime lights reflect the extent of human activity, and their share of total NO<sub><italic>x</italic></sub> emissions can serve as a useful indicator of regional urbanization (Wang et al., 2021). Figure 8 presents the relationships among provincial NO<sub><italic>x</italic></sub> emission changes, their contributions to total NO<sub><italic>x</italic></sub> and GRP. Provincial positive changes in anthropogenic NO<sub><italic>x</italic></sub> emissions often coincide with increases in their share of total NO<sub><italic>x</italic></sub> (Fig. 8a), particularly in economically less developed regions with relatively low GRP, where anthropogenic sources constitute a small to moderate portion of total NO<sub><italic>x</italic></sub> (Fig. 8b) and NO<sub>2</sub> TVCDs are generally low (Fig. S8). In the early stages of economic development, a resource-intensive model driven by fuel consumption dominates, with GRP growth accompanied by rising NO<sub><italic>x</italic></sub> emissions at the expense of environmental quality. As the economy progresses, shifts in industry sectors and air quality mitigation measures contribute to a decline in NO<sub><italic>x</italic></sub> emissions, with regional economic levels potentially playing a key role in driving these changes (Miyazaki and Bowman, 2023; Wang et al., 2019). The disparities in industrial structure and economic development levels across regions may account for the current differentiated patterns in provincial NO<sub><italic>x</italic></sub> emissions.</p>

      <fig id="F8" specific-use="star"><label>Figure 8</label><caption><p id="d2e4669"><bold>(a)</bold> Provincial changes in anthropogenic NO<sub><italic>x</italic></sub> emissions from 2019 to 2024 (<inline-formula><mml:math id="M344" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<sub><italic>x</italic></sub>) and their contributions to total NO<sub><italic>x</italic></sub> in 2024 (<inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>), with bubble color indicating changes in the <inline-formula><mml:math id="M348" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> proportion (<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>A</mml:mi><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>), provinces with positive <inline-formula><mml:math id="M350" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<sub><italic>x</italic></sub> are labeled;<bold> (b)</bold> Same as <bold>(a)</bold>, but showing the relationship between <inline-formula><mml:math id="M352" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>/</mml:mo><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> and GRP in 2024, with bubble color indicating <inline-formula><mml:math id="M353" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<sub><italic>x</italic></sub>.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f08.png"/>

          </fig>

</sec>
<sec id="Ch1.S4.SS3.SSS3">
  <label>4.3.3</label><title>Consistent downward trend in NO<sub><italic>x</italic></sub> emissions across megacities</title>
      <p id="d2e4822">Six megacities of China with GDP rankings in the top ten and populations exceeding ten million are selected to present the time series of monthly NO<sub><italic>x</italic></sub> emissions and changes (Fig. 9). Values in the bottom right corner represent the percentage of months with negative relative changes. The results are in good agreement with the decreased NO<sub><italic>x</italic></sub> during the strict COVID-19 lockdowns (e.g., February–May 2020 in Wuhan, February–May 2022 in Shanghai) (Miyazaki et al., 2021; Cooper et al., 2022), and the increase during major holidays (e.g., Spring Festival in January–February, summer holiday in July–August, National Day holiday in October). Seasonal variability of NO<sub><italic>x</italic></sub> emissions in megacities is influenced by meteorological conditions. Heating demand leads to markedly higher emissions in autumn and winter than in spring and summer (Miyazaki et al., 2021), with more pronounced variability in northern cities such as Beijing. In contrast, emission fluctuations associated with rising electricity demand during hot seasons (Lange et al., 2022) are more pronounced in the five southern cities. Meanwhile, as China's clean air actions progress, megacities exhibit a consistent downward trend in NO<sub><italic>x</italic></sub> emissions, with the proportion of negative changes higher than positive. Shanghai and Beijing have relatively high emissions, but they show a greater share of months with declines from 2020–2024 compared to 2019, reflecting stronger efforts in emission reduction.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e4863">Monthly NO<sub><italic>x</italic></sub> emissions for 2020–2024 and relative changes from 2019 in China's megacities, with Beijing, Shanghai, Wuhan, Hangzhou, Shenzhen and Chengdu as examples.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f09.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S4.SS4">
  <label>4.4</label><title>Point source emissions</title>
      <p id="d2e4890">Point source emissions in DDA (from power plants in this study) are quantified by integrating over a 15 km radius, following the approach and locations of 124 power plants reported by Beirle et al. (2023). Figure 10a presents the estimated NO<sub><italic>x</italic></sub> emissions from these plants in China for 2019. From 2019 to 2024, emissions from the 124 plants range from 0.02–2.13 kg s<sup>−1</sup>, with uncertainties between 4 %–78 %, averaging 16 %. Overall, the plants show an average emission decline of 23 % over this period.</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e4916">Comparisons of NO<sub><italic>x</italic></sub> point source emissions between the DDA and Beirle et al. (2023) data.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2749/2026/essd-18-2749-2026-f10.png"/>

        </fig>

      <p id="d2e4934">The resulting estimates are validated against Beirle et al. (2023) for 2019–2021, as shown in Fig. 10b. The two datasets show good agreement, with an <inline-formula><mml:math id="M364" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.81, both indicating a decline in NO<sub><italic>x</italic></sub> emissions from 2019 to 2021. Generally, NO<sub><italic>x</italic></sub> emissions from the DDA are slightly lower than those from Beirle et al. (2023), with a slope of 0.83. For comparison, results from DDA test without ratio correction and fitting scheme improvement (fixed_<inline-formula><mml:math id="M367" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> and single_<inline-formula><mml:math id="M368" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>) are also shown in Fig. S9, further illustrating the improvement in point source quantification achieved in this study. It should be noted that point source emissions include all fossil fuel emission sources within the defined radius, leading to a positive bias (Beirle et al., 2023).</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Discussion</title>
      <p id="d2e4990">We estimate NO<sub><italic>x</italic></sub> emissions using the DDA by applying a variable NO<inline-formula><mml:math id="M370" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and deriving a more realistic nonlinear NO<sub><italic>x</italic></sub> lifetime through a piecewise fitting approach in each subregion. This scheme combines multiple linear fits based on NO<sub>2</sub> TVCD levels, providing a simple and robust way to represent nonlinear NO<sub><italic>x</italic></sub> chemistry in the DDA framework.</p>
      <p id="d2e5046">Region partitioning mainly depends on NO<sub><italic>x</italic></sub> concentration, latitude, and terrain. By using HL as the east-west dividing line, the results implicitly consider variations in O<sub>3</sub> and its precursors driven by human activities, differences in natural VOCs emissions from vegetation across different climates and geographies, and meteorological effects on transport and photochemistry. It is worth noting that HL is used as a boundary for partitioning because it provides a suitable division, where regional divisions improve fitting performance but have a limited impact compared to grading NO<sub><italic>x</italic></sub> concentration levels.</p>
      <p id="d2e5076">The random error of DDf in Eq. (2) described in Sect. 3.4 is used to characterize the uncertainties in DDA emission estimation. Annual anthropogenic emissions uncertainties range from 27 %–30 % at the national scale and 15 %–40 % at the subnational scale. At provincial scale, uncertainties vary more widely, from 8 %–59 %. The average uncertainty for point sources is 16 %. Note that the error does not include the fitting uncertainties related to the topographic correction and chemical loss terms in Eq. (2), indicating that the reported uncertainty is likely underestimated.</p>
      <p id="d2e5079">Additionally, the anthropogenic NO<sub><italic>x</italic></sub> emissions are derived by subtracting natural sources from total emissions, a step that may introduce unknown uncertainties. For point sources, spatial integration that includes all fossil fuel sources within the defined radius may lead to a positive bias.</p>
      <p id="d2e5092">The DDA adopts a data-driven fitting approach to derive parameters independently, eliminating the need for additional assumptions or external calculations. However, this method requires regions with sufficient terrain diversity (including both rough and flat areas) and an adequate number of observations that satisfy the fitting criteria. The fitted scale heights and chemical lifetimes represent effective subregional parameters derived from grid cells in clean regions, which may lead to overestimation of scale heights in heavily polluted areas and do not fully reflect the sensitivity of NO<sub><italic>x</italic></sub> lifetimes to environmental conditions, although the regional averages still capture nonlinear NO<sub><italic>x</italic></sub> chemistry. As these are fitting parameters, their physical interpretation should be treated cautiously to avoid over-interpretation (Lonsdale and Sun, 2023). Future observations with higher spatial resolution could improve the representation of scale height and chemical lifetime across heterogeneous regions, while future studies could focus on developing appropriate thresholds for automated global partitioning.</p>
      <p id="d2e5113">Since satellite-based inversion quantifies total NO<sub><italic>x</italic></sub> emissions, isolating natural sources is crucial for accurately estimating anthropogenic emissions. However, the current understanding of natural sources remains limited, with substantial discrepancies and uncertainties across previous studies  (Jaeglé et al., 2005; Kong et al., 2023; Li and Zheng, 2024; Lin, 2012; Lin et al., 2024; Müller and Stavrakou, 2005; Song et al., 2021; Zhao and Wang, 2009). We attribute 28.1 %–35.6 % of China's total NO<sub><italic>x</italic></sub> emissions to natural sources, indicating that natural emissions in China have been underestimated, as noted by Song et al. (2021).</p>
      <p id="d2e5134">This work primarily aims to propose a practical and insightful perspective for addressing nonlinear NO<sub><italic>x</italic></sub> chemistry in satellite-based emission estimation, rather than focusing on improvements in data quality itself (e.g., air mass factor correction in satellite NO<sub>2</sub> retrievals).</p>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Code and data availability</title>
      <p id="d2e5163">Code relevant to this paper can be found in Sun (2022) at <ext-link xlink:href="https://doi.org/10.5281/zenodo.7987812" ext-link-type="DOI">10.5281/zenodo.7987812</ext-link> (Sun, 2023). The data can be found at <ext-link xlink:href="https://doi.org/10.5281/zenodo.18923337" ext-link-type="DOI">10.5281/zenodo.18923337</ext-link> (Chen et al., 2026), Table S3 provides a description of the dataset.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d2e5180">We present an improved satellite-based framework for estimating NO<sub><italic>x</italic></sub> emissions across China, leveraging the directional derivative approach (DDA) alongside TROPOMI NO<sub>2</sub> observations, ERA5 wind fields, and variable NO<inline-formula><mml:math id="M386" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratios derived from GEOS-CF. The DDA addresses several challenges in satellite-based emission quantification. It corrects divergence artifacts induced by terrain-driven flows, reduces biases from using single-level wind fields, and suppresses background signal contamination implicitly.</p>
      <p id="d2e5218">In this work, by incorporating a spatially variable NO<inline-formula><mml:math id="M387" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio and implementing a data-driven, piecewise fitting strategy, we account for nonlinear NO<sub><italic>x</italic></sub> chemistry and improve the estimation of NO<sub><italic>x</italic></sub> lifetimes across diverse emission regimes. The NO<inline-formula><mml:math id="M390" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio correction improves the accuracy of source divergence and emission estimates, with the major advancement being the piecewise fitting approach, which captures the nonlinear NO<sub><italic>x</italic></sub> chemistry. The fitting scheme clusters NO<sub>2</sub> concentration levels within localized regions, reduces fitting errors, mitigates artifacts in mountainous and remote areas, and improves the overall reliability of the estimates. It enables the estimation of both point-source and regional NO<sub><italic>x</italic></sub> emissions across China, representing the first application of a lightweight, satellite-driven NO<sub><italic>x</italic></sub> emissions estimator in such a large and topographically complex region.</p>
      <p id="d2e5310">NO<sub><italic>x</italic></sub> lifetimes vary from 0.71–26.47 h with NO<sub><italic>x</italic></sub> concentrations, and average values across the four subregions range from 3.17–7.85 h, reflecting the nonlinear variability of lifetime as a function of NO<sub>2</sub> TVCDs. Significant discrepancies in regional ambient conditions, such as O<sub>3</sub> and VOCs concentrations, meteorological parameters, and differences in NO<sub><italic>x</italic></sub> emission sources, also contribute to this variability. Without ratio correction and fitting improvements, lifetimes across the four subregions are about 2 to 3 times those found in this study, reaching 1.7 times in ES, 2.8–2.9 times in EN and WN, and 3.3 times in WS, highlighting the critical need to consider variable NO<inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratios and nonlinear lifetimes, particularly in clean and heavily polluted regions.</p>
      <p id="d2e5376">Anthropogenic contributions are isolated by subtracting natural sources from satellite-derived total emissions, with natural NO<sub><italic>x</italic></sub> identified using a seasonal criterion and further constrained by NTL data. Estimated anthropogenic NO<sub><italic>x</italic></sub> emissions in China are 20.2, 18.5, 19.4, 18.9, 20.7 and 18.8 Tg from 2019 to 2024, with annual uncertainties of 27 %–30 %. The corresponding total emissions are 29.8, 28.8, 28.7, 28.2, 28.7 and 27.4 Tg, respectively, and natural sources account for 28.1 %–35.6 % of the totals in this study.</p>
      <p id="d2e5398">Spatial and temporal trends show consistent NO<sub><italic>x</italic></sub> reductions in megacities, while provincial-level patterns reflect regional differences in urbanization and economic development.</p>
      <p id="d2e5410">From 2019 to 2024, emissions from the 124 power plants range from 0.02–2.13 kg s<sup>−1</sup>, with uncertainties between 4 %–78 %, averaging 16 %. Overall, the plants show an average emission decline of 23 % over this period.</p>
      <p id="d2e5425">Validation against established inventories, including MEIC, EDGAR, and other top-down inversions, demonstrates strong agreement with national level discrepancies ranging from <inline-formula><mml:math id="M405" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11.8 % to 0.8 %. At the provincial scale, the DDA shows consistently lower emissions in economically advanced regions and higher in less developed Northeast and western areas. For point sources, our estimates closely match those from previous study, with an <inline-formula><mml:math id="M406" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.81 and a slope of 0.83.</p>
      <p id="d2e5446">Looking forward, this framework holds promise for global-scale application and for separating natural and anthropogenic NO<sub><italic>x</italic></sub> sources. Its low-latency, data-driven nature offers critical value for air quality management, CO<sub>2</sub> co-emission estimation, and international efforts such as the Global Stocktake.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d2e5466">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-18-2749-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/essd-18-2749-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e5477">ZNC, LC, and KS designed this study. KS constructed the algorithm codebase and LC executed optimizations. LC performed the analysis and wrote the paper with ZNC, KS and YL. MML and LYZ provided comments. YL supervised the study.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e5483">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="d2e5489">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="d2e5495">We thank ESA and NASA for the TROPOMI, GEOS-CF, and VNP46 datasets; ECMWF for providing the ERA5 and CAMS datasets; and Tsinghua University and the EDGAR team for MEIC and EDGAR bottom-up emissions inventories.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e5500">This research was supported by the National Key R&amp;D Program of China (grant no. 2022YFB3904802), the Open Fund of State Key Laboratory of Infrared Physics, Shanghai Institute of Technical Physics, Chinese Academy of Sciences.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e5507">This paper was edited by Graciela Raga and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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