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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-18-7535-2026</article-id><title-group><article-title>Tracking recent extremes and interannual variability of global fire emissions using a near-real-time extension to the Global Fire Emissions Database</article-title><alt-title>Recent extremes and variability in GFED fire emissions</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Chen</surname><given-names>Yang</given-names></name>
          <email>yang.chen@uci.edu</email>
        <ext-link>https://orcid.org/0000-0002-0993-7081</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>van der Werf</surname><given-names>Guido R.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9042-8630</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mu</surname><given-names>Mingquan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>van Wees</surname><given-names>Dave</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5565-7155</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Hall</surname><given-names>Joanne V.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Giglio</surname><given-names>Louis</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Vernooij</surname><given-names>Roland</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Morton</surname><given-names>Douglas C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Xu</surname><given-names>Li</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Liu</surname><given-names>Tianjia</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3129-0154</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Scholten</surname><given-names>Rebecca C.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0144-0572</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Coffield</surname><given-names>Shane R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Follette-Cook</surname><given-names>Melanie B.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Ott</surname><given-names>Lesley</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Randerson</surname><given-names>James T.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth System Science, University of California, Irvine, 92612, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Meteorology and Air Quality Group, Wageningen University &amp; Research, Wageningen, the Netherlands</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>BeZero Carbon, London, UK</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Geographical Sciences, University of Maryland, College Park, MD, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Biospheric Sciences Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of Geography, University of British Columbia, Vancouver, BC, Canada</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Earth System Science Interdisciplinary Center, University of Maryland, College Park, MD, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yang Chen (yang.chen@uci.edu)</corresp></author-notes><pub-date><day>15</day><month>October</month><year>2026</year></pub-date>
      
      <volume>18</volume>
      <issue>10</issue>
      <fpage>7535</fpage><lpage>7555</lpage>
      <history>
        <date date-type="received"><day>25</day><month>February</month><year>2026</year></date>
           <date date-type="rev-request"><day>31</day><month>March</month><year>2026</year></date>
           <date date-type="rev-recd"><day>24</day><month>September</month><year>2026</year></date>
           <date date-type="accepted"><day>25</day><month>September</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Yang 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/18/7535/2026/essd-18-7535-2026.html">This article is available from https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e250">The Global Fire Emissions Database (GFED) is widely used to quantify spatiotemporal variability and long-term trends in burned area and fire emissions, supporting assessments of fire impacts on ecosystems and atmospheric composition. GFED has historically relied on observations from the Moderate Resolution Imaging Spectroradiometer (MODIS), but orbital drift and planned sensor decommissioning pose challenges for maintaining record continuity and near-real-time (NRT) monitoring. Here we present the GFED5 near-real-time extension (GFED5NRT), a global fire emissions dataset that enables daily NRT analyses using active fire observations from the Visible Infrared Imaging Radiometer Suite (VIIRS). GFED5NRT uses biome- and region-specific lookup tables of effective fire area and fuel consumption, derived from VIIRS observations and standard GFED5 datasets, to estimate burned area and emissions from VIIRS active fire counts in a manner consistent with the GFED5 time series. Comparisons with GFED5 and independent datasets show strong agreement in spatial patterns, seasonal cycles, and interannual variability of fire activity. GFED5NRT captures recent major fire extremes and provides daily global NRT estimates of burned area and emissions for multiple trace gases and aerosols. Together, GFED5 and GFED5NRT provide a coherent framework for long-term analyses and NRT monitoring of evolving fire regimes in a changing climate. The GFED5NRT dataset is publicly available at <ext-link xlink:href="https://doi.org/10.5281/zenodo.18702700" ext-link-type="DOI">10.5281/zenodo.18702700</ext-link> (Chen et al., 2026).</p>
  </abstract>
    
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<award-group id="gs1">
<funding-source>National Aeronautics and Space Administration</funding-source>
<award-id>80NSSC21K1362</award-id>
<award-id>80NSSC26K0278</award-id>
<award-id>80NSSC24K1823</award-id>
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<award-id>80NSSC24K0301</award-id>
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<funding-source>National Science Foundation</funding-source>
<award-id>RISE-2425932</award-id>
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<award-group id="gs3">
<funding-source>U.S. Department of Energy</funding-source>
<award-id>NA</award-id>
</award-group>
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<funding-source>Eric and Wendy Schmidt</funding-source>
<award-id>NA</award-id>
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  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Overview</title>
      <p id="d2e265">Recent studies have documented substantial shifts in the frequency and intensity of global wildfires, driven primarily by climate change and land-use dynamics (Jones et al., 2022). Although total global burned area has declined over recent decades (approximately <inline-formula><mml:math id="M1" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.2 % yr<sup>−1</sup>), largely due to reduced fire activity in African savannas (Andela et al., 2017) and croplands worldwide (Hall et al., 2024), fire risk has intensified in many other regions. Prolonged droughts and rising temperatures have increased the occurrence of extreme fire weather (Jain et al., 2022), weakened the nocturnal barrier to fire spread (Balch et al., 2022), and contributed to more severe fire events in boreal and temperate biomes (Cunningham et al., 2024; Jones et al., 2024). As fires increasingly extend into regions with high fuel loads, global fire emissions have remained relatively stable despite the overall decline in burned area (van der Werf et al., 2025). Meanwhile, expanding human settlement near wildlands (Schug et al., 2023) has increased the extent of the wildland-urban interface (WUI) (Chen et al., 2024; Guo et al., 2024; Tang et al., 2024), thereby increasing human exposure to wildfires (Teymoor Seydi et al., 2025) and wildfire smoke–related premature mortality (Zhao et al., 2025). Assessing these evolving fire regimes and their societal and environmental impacts requires long-term, internally consistent global fire emissions datasets.</p>
      <p id="d2e287">Near-real-time (NRT) fire emissions products are critical for the timely assessment of fire impacts on atmospheric chemistry and air quality, rapid response to evolving fire disasters, and the placement of such events in the context of the historical record. Several widely used operational NRT systems rely primarily on fire radiative power (FRP) observations from geostationary (GEO) and low Earth orbit (LEO) satellites. For example, the Copernicus Atmosphere Monitoring Service (CAMS) Global Fire Assimilation System (GFAS) (Kaiser et al., 2012) and NASA's Quick Fire Emissions Dataset (QFED) (Darmenov and da Silva, 2015) estimate emissions based on active fire detections from the Moderate Resolution Imaging Spectroradiometer (MODIS) sensors, with calibrations tied to external inventories or constrained by atmospheric observations. The Fire INventory from NCAR (FINN) (Wiedinmyer et al., 2011, 2023) provides fire emissions estimates derived from land cover data and active fires, supporting regional air quality applications. Similarly, NOAA's Hazard Mapping System (HMS) (Schroeder et al., 2008), the Blended Global Biomass Burning Emissions Product (GBBEPx) (Zhang et al., 2012; Li et al., 2022) and the HRRR-Smoke model (Ahmadov et al., 2017) integrate observations from multiple satellite sensors to improve detection and emissions quantification. These systems provide indispensable datasets for NRT monitoring and forecasting, but further efforts are needed to ensure consistency with long-term historical records.</p>
      <p id="d2e290">The Global Fire Emissions Database (GFED) is a suite of gridded datasets that provide global estimates of burned area and associated emissions of gases and aerosols from landscape fires. Burned area estimates in GFED are primarily derived from satellite observations of surface reflectance change and the delineation of fire-affected areas. GFED emissions calculations follow the Seiler and Crutzen (1980) framework, combining burned area with fuel consumption estimates from a biogeochemical model and emission factors derived from laboratory and field measurements. GFED has undergone several iterations, resulting in multiple versions that progressively refine burned area and emissions (Chen et al., 2023; Giglio et al., 2006, 2010; Randerson et al., 2012; van der Werf et al., 2006, 2010, 2017). The most recent release, GFED version 5 (GFED5) (van der Werf et al., 2025), improves burned area estimates by accounting for small fires undetected by moderate-resolution sensors (Chen et al., 2023) and by incorporating higher-resolution imagery and a cropland-specific methodology to better represent agricultural burning (Hall et al., 2024). The full GFED5 product covers the 1997–2022 period. The core emissions model uses multiple 500 m MODIS products to track the temporal evolution of aboveground and surface fuels across ecosystems, with explicit treatment of deforestation and peat fires (van Wees et al., 2022). Emission factors draw upon an extensive compilation of field and laboratory measurements, including aircraft observations from recent field campaigns (Binte Shahid et al., 2024). Interannual variability over 1997–2022 is substantial in this record (Table S1 in the Supplement), with global burned area from GFED5 ranging from 620 to 920 million hectares per year (Mha yr<sup>−1</sup>) and fire emissions ranging from 2.9 to 4.4 petagrams of carbon per year (Pg C yr<sup>−1</sup>). Across GFED versions, mean global annual burned area over this period ranges from 340 to 780 Mha yr<sup>−1</sup>, while mean annual fire emissions range from 2.0 to 3.4 Pg C yr<sup>−1</sup>, reflecting differences in input datasets and methodological choices.</p>
      <p id="d2e341">While GFED has provided essential retrospective data for understanding fire impacts on the Earth system, reducing data latency to support NRT applications remains a priority. However, the MODIS instruments aboard NASA's Terra and Aqua satellites, which provide core data for many global burned area and emissions datasets, are aging and have experienced orbital drift that has substantially altered their local overpass times (Loeb et al., 2024; Parkinson, 2022). The GFED5 dataset ends in 2022, when orbital drift-induced changes surpassed the thresholds defined for high-quality science products. The Visible Infrared Imaging Radiometer Suite (VIIRS) instruments on multiple NASA and NOAA satellites offer many of the same capabilities as MODIS and are widely considered a viable continuity data source for MODIS-based land products (Román et al., 2024; Giglio et al., 2025). Here, we present a system for generating GFED5-compatible NRT global burned area and emissions datasets for the post-MODIS era using 375 m VIIRS active fire detections (Fig. 1). We are motivated by the urgent need to quantify recent fire extremes and place their magnitudes in the context of the GFED5 global record. This work represents a first step toward developing global fire records that merge VIIRS and MODIS observations, prior to a more comprehensive fusion of science-quality burn area time series from the two sensors, which remains a key priority but requires further investment. Our approach (Fig. 2) uses a two-step scaling framework. First, daily VIIRS active fire counts are converted to burned area using region- and biome-specific effective fire areas (burned area per active fire) derived from GFED5. Second, burned area is converted into emissions using fuel consumption lookup tables constructed from GFED5 burned area and emissions as a function of fire type and continental-scale region. This framework features several novel aspects: (1) joint estimation of burned area and emissions through a unified scaling approach; (2) classification of fires into 16 broad ecosystem types to support biome-specific analyses; and (3) contextualization of recent fire activity within a long-term, internally consistent global fire record.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e347">Timelines of GFED5NRT products and primary input datasets. Layers shown include VIIRS active fire counts, burned area, and fire emissions. The dashed lines for GFED5 denote the pre-MODIS period, when data were reported at coarser spatial resolution. Dotted lines for GFED5NRT denote the periods used for data calibration and for deriving scaling coefficients.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f01.png"/>

      </fig>

      <fig id="F2"><label>Figure 2</label><caption><p id="d2e358">Schematic of the two-step scaling approach used to generate the GFED5NRT global burned area (BA) and fire emissions (EM) datasets from VIIRS active fire counts. Two biome-specific scaling factors – effective fire area (EFA; burned area per fire count) and fuel consumption (FC; carbon emissions per unit burned area) – were derived for each region by linking VIIRS active fire detections to the GFED5 data during the 2012–2022 overlapping period.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f02.png"/>

      </fig>

      <p id="d2e367">We applied the scaling algorithm to daily VIIRS active fire detections from the NOAA/NASA Suomi-NPP (SNPP) and NOAA-20 satellites, generating two independent time series of burned area and emissions estimates with minimal latency. To reduce biases associated with oblique viewing geometry and data gaps caused by intermittent instrument outages, we merged these streams to produce the combined GFED5 near-real-time extension (GFED5NRT). GFED5NRT extends the temporal coverage of GFED5, providing characterization of fire activity, burned area, and associated emissions during the post-MODIS era, as well as more timely documentation of recent extreme wildfire events. We developed a Python-based processing system that automatically retrieves VIIRS NRT active fire data from NASA's Fire Information for Resource Management System (FIRMS), applies corrections for viewing geometry and data gaps, and uses pre-calculated region- and biome-specific scaling coefficients to estimate daily burned area and emissions operationally. By combining contemporary satellite observations with a consistent scaling framework, GFED5NRT provides temporally consistent and reliable estimates of burned area and emissions across fire types, supporting both retrospective analyses of fire variability and NRT monitoring of ongoing fire activity.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and Method</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>GFED5 burned area and emissions</title>
      <p id="d2e385">The GFED5 burned area dataset was developed by integrating multiple remote sensing data streams (Chen et al., 2023). It builds primarily on the MODIS burned area time series (Giglio et al., 2018; Justice et al., 2002). To address both commission and omission errors associated with the coarse spatial resolution of MODIS (500 m), burned area estimates were calibrated using higher-resolution (20–30 m) observations from Landsat and Sentinel-2 alongside MODIS active fire data. Specifically, commission errors caused by unburned patches within burned MODIS pixels were corrected by scaling MODIS burned area using coefficients derived from high-resolution observations, while omission errors were corrected by relating MODIS active fire counts to high-resolution burned area sampled outside MODIS burned pixels. Agricultural burned area was further updated using the global cropland-focused burned area product GloCAB (Hall et al., 2024). GFED5 provides global monthly burned area estimates at 0.25° spatial resolution, with attribution by ecosystem and fire type.</p>
      <p id="d2e388">In van der Werf et al. (2025), a slightly modified version of the methodology described in Chen et al. (2023) was implemented to estimate GFED5 burned area (version 5.1) through 2022. GFED5 emissions were calculated using this burned area dataset within the classical framework of Seiler and Crutzen  (1980). For each 0.25° grid cell, emissions of individual species were estimated as the product of burned area, fuel consumption (defined as fuel load multiplied by combustion completeness), and species-specific emission factors that convert dry matter burned to chemical species emitted. Fuel consumption was derived using the Carnegie-Ames-Stanford Approach (CASA) biogeochemical model (Potter et al., 1993) and further constrained by multiple observational datasets at 500 m resolution (van Wees et al., 2022). Monthly emissions were temporally disaggregated to daily and hourly scales using active fire detections from a combination of polar-orbiting and geostationary satellites to capture sub-monthly variability in fire activity (Mu et al., 2011). The GFED5 burned area and emissions datasets (version 5.1) are publicly available at <uri>https://www.globalfiredata.org</uri>, last access: 1 October 2026.</p>
      <p id="d2e394">The gridded, fire-type-specific GFED5 data cover the core MODIS era from 2002 to 2022. As described in Chen et al. (2023) and van der Werf et al. (2025), GFED5 was also extended to the pre-MODIS period (1997–2001) using active fire detections from the Visible and Infrared Scanner (VIRS) aboard the Tropical Rainfall Measuring Mission (TRMM) and the Along Track Scanning Radiometers (ATSR) flown on multiple platforms. For this earlier period, the dataset was produced at a coarser 1° spatial resolution and does not distinguish among land cover types.</p>
      <p id="d2e397">Throughout this paper, GFED5 refers to the updated version 5.1 burned area and emissions datasets described in van der Werf et al. (2025), including the pre-MODIS period (Fig. 1). These standard products are used during the overlap period with VIIRS (2012–2022) to derive scaling coefficients that convert VIIRS active fire counts to burned area and emissions for the near-real-time product (Fig. 2).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>VIIRS active fire data</title>
      <p id="d2e408">VIIRS is a multi-band imaging instrument that collects imagery and radiometric measurements across visible and infrared wavelengths, enabling the detection of thermal anomalies associated with landscape fires and other heat sources. Compared with MODIS (1 km), the finer spatial resolution of VIIRS (375 m) provides more accurate fire location information and higher detection efficiency, thereby improving fire mapping, fire behavior characterization, and applications in disaster response and land management (Schroeder et al., 2025). Unlike MODIS, however, VIIRS lacks a 10:30 local time overpass, which may lead to underdetection of fires with diurnal cycles that peak in the late morning.</p>
      <p id="d2e411">The NASA VIIRS 375 m thermal anomalies and active fire products are distributed as both science-quality data (Schroeder et al., 2025) and NRT data. The science-quality datasets are quality-controlled and internally consistent, with a primary objective of supporting long-term climate research, but data latency is typically several months. In contrast, the NRT data stream is available within hours of observation, making it better suited for operational decision support and early warning applications.</p>
      <p id="d2e414">In this study, we obtained the science-quality VIIRS 375 m fire location products (VNP14IMGML and VJ114IMGML, Collection 2 version 4) from the University of Maryland Fuoco SFTP server (<uri>ftp://fuoco.geog.umd.edu</uri>, last access: 6 October 2026). These data from 2012 to 2022 were used to train the scaling model that converts active fire counts to burned area and fire emissions. To generate the GFED5NRT product, we used VIIRS NRT active fire data available through NASA LANCE FIRMS. As discussed below (Sect. 2.3.3), we selected the NRT fire image products (VNP14IMG_NRT and VJ114IMG_NRT), rather than the NRT fire location products (VNP14IMGDL_NRT and VJ114IMGDL_NRT), because the image products retain the full 2D swath raster fire mask. This geometric context is required to perform viewing-angle corrections, including calculating pixel size variations away from nadir.</p>
      <p id="d2e420">VIIRS instruments are currently carried on three satellites in the Joint Polar Satellite System (JPSS): SNPP, NOAA-20, and NOAA-21. Their orbital configuration allows each satellite to observe a given location at approximately the same local solar time, but from different viewing angles. Merging VIIRS observations across platforms has been shown to reduce artificial day-to-day variability and biases associated with changing viewing geometry (Giglio et al., 2025). In this study, we integrated VIIRS active fire observations from the SNPP and NOAA-20 to balance the need for a consistent historical record with continuity for future extensions of the GFED5NRT product. To further reduce biases arising from day-to-day variations in sensor viewing geometry, we additionally generated a GFED5NRT data layer that combines observations from both satellites, taking advantage of their deliberate orbital phasing.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Active fire recording and adjustments</title>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Active fire counts</title>
      <p id="d2e438">To ensure consistency with the fire-type classification and grid structure of standard GFED5, VIIRS active fire detections were aggregated by land cover class by overlaying fire centroids onto 500 m land cover maps. An annual land cover type was assigned to each 500 m MODIS sinusoidal grid cell (van Wees et al., 2022) using an integrated dataset combining the MODIS MCD12Q1 Collection 6.1 land cover product (Friedl and Sulla-Menashe, 2022), a tropical peatland map (Gumbricht et al., 2017), and a fire-persistence-based deforestation mask (Chen et al., 2023). A total of 16 land cover classes were defined, including 13 standard biome types and three special burning types: deforestation, peatland, and agricultural burning. In each 0.25° grid cell, active fire detections were aggregated across these classes, ensuring consistency with the burned area and emissions stratification applied in GFED5 (Table 2 of van der Werf et al., 2025). To minimize the effects of VIIRS sampling biases and retrieval uncertainties, additional corrections were applied prior to estimating burned area and emissions, as described in the following sections.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><title>Static hotspot filtering</title>
      <p id="d2e449">The VIIRS science-quality active fire products classify detected thermal anomalies into several categories, including vegetation fires, active volcanoes, offshore detections, and other static land heat sources. In contrast, the VIIRS NRT active fire products do not explicitly separate vegetation fires from persistent non-vegetation thermal sources. To address this limitation, we developed a static hotspot mask that combines two complementary sources of information. This mask has a spatial resolution of 0.01° <inline-formula><mml:math id="M7" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.01°.</p>
      <p id="d2e459">First, a hotspot-based static mask was constructed using historical SNPP VIIRS observations from 2012–2022 to identify 0.01° grid cells with more than five detections classified as non-vegetation fires (type <inline-formula><mml:math id="M8" display="inline"><mml:mo>≠</mml:mo></mml:math></inline-formula> 0). Second, a report-based static mask was compiled from documented locations of persistent thermal sources, including gas flares, landfills, volcanoes, solar power facilities, power plants, and refineries (see Sect. S1). These two components were combined to produce a comprehensive static hotspot mask that removes presumed non-vegetation thermal anomalies from the VIIRS NRT data, thereby improving the accuracy of fire detection and subsequent burned area and emissions estimates in GFED5NRT.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>VIIRS viewing geometry adjustment</title>
      <p id="d2e477">Each VIIRS active fire detection is associated with a specific scan angle, identified by the sample number in the science-quality VIIRS active fire location files. Detection efficiency varies with scan angle due to factors such as pixel size, canopy height, illumination geometry, atmospheric attenuation, and filtering by the retrieval algorithm. While these effects largely average out over monthly timescales, they can introduce significant biases in daily burned area and emission estimates (Giglio et al., 2025).</p>
      <p id="d2e480">To correct for this, we developed scan-angle-specific lookup tables using the full set of standard VIIRS active fire detections from SNPP during 2019–2021. Fire counts were stratified by cross-track sample number (0–6399), day/night status, month, and dominant land cover type within 0.25° grid cells (see Sect. S2). Weighting factors were derived for each sample bin based on total fire counts, removing scan angle dependence while conserving the total fire radiative power across all sample numbers (Fig. S1). This ensures that total emissions estimates remained unchanged. The resulting weighting factors were applied to individual VIIRS detections, and the corrected fire counts were aggregated by land cover type within each 0.25° grid cell.</p>
      <p id="d2e483">Scan angle information is available only in the science-quality product (VNP14IMGML and VJ114IMGML) and is absent in the NRT fire location products (VNP14IMGDL_NRT, VJ114IMGDL_NRT). To address this limitation, we used upstream two-dimensional NRT imagery products (VNP14IMG_NRT, VJ114IMG_NRT) to generate daily fire location files in a VNP14IMGDL_NRT-like format that incorporates both sample number and key fire attributes. These additional files were then used to perform viewing geometry correction and normalize fire counts.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS4">
  <label>2.3.4</label><title>Adjustment of fire counts in deforestation areas</title>
      <p id="d2e494">VIIRS active fire detections were aggregated by land cover type within each 0.25° grid cell, with individual detections assigned to land cover classes at 500 m resolution. In near-real-time applications, instantaneous land cover data are often unavailable, so the most recent available year of land cover information from the MODIS MCD12Q1 product is therefore used. However, in regions undergoing rapid deforestation, this temporal mismatch can lead to substantial misclassification: fires associated with recent forest loss may be missed, while unrelated fires may be incorrectly attributed to deforestation, resulting in biased emissions estimates.</p>
      <p id="d2e497">To mitigate this issue, VIIRS active fire counts were adjusted by assuming temporal stability in the monthly fraction of deforestation-related burning within 0.25° tropical deforestation grid cells. Climatological monthly fractions of deforestation-related fire counts, averaged over 2013–2022, were first calculated for each grid cell. These fractions were then applied to the total VIIRS active fire counts to derive adjusted estimates of deforestation-related fire activity. Fire counts associated with other land cover types were scaled proportionally to conserve the total number of detections.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Estimating burned area and emissions from active fire counts</title>
      <p id="d2e509">We applied a two-step scaling approach (Fig. 2) to convert VIIRS active fire counts, stratified into 16 land cover types at 0.25° resolution, into global burned area and fire emissions estimates.</p>
      <p id="d2e512">In the first step, biome-specific scaling factors, termed effective fire area (EFA) scalars, were derived for multiple geographical regions by relating science-quality VIIRS active fire detections to GFED5 burned area data during the MODIS-VIIRS overlap period (2012–2022). We used the same 14 continental-scale regions (hereafter GFED regions) defined in the standard GFED5 product (Fig. 2 in van der Werf et al., 2025). Only detections classified as vegetation fires (fire type code <inline-formula><mml:math id="M9" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0) were used in deriving EFA. EFA represents the mean burned area (km<sup>2</sup>) per active fire detection for each region and land cover type.</p>
      <p id="d2e531">We evaluated a suite of aggregation schemes for EFA estimation (Sect. S3; Table S2) that varied in spatial scale (0.25° grid cell, GFED region, or global), temporal resolution (annual or monthly), and treatment of land cover (lumped or type-specific). Based on overall performance across statistical metrics, including bias, correlation coefficient, and normalized root mean square error (Table S3), as well as aggregation efficiency (Table S2), we selected region- and land cover-specific EFA scalars associated with the Regftp scheme. In this scheme, active fires are aggregated within each GFED region by land cover or burning type (Table S2). These scalars were used to generate GFED5NRT. In principle, the Regftp scheme could yield up to 224 EFA scalars globally, from the product of 14 continental regions and 16 burning types; in practice, however, not all burning types occur in every region.</p>
      <p id="d2e534">The optimized EFA scalars were subsequently applied to VIIRS active fire counts to generate the GFED5NRT burned area product for years following the GFED5 record (1997–2022). Beginning in 2023, daily VIIRS active fire counts by land cover type were multiplied by corresponding EFA scalars to estimate burned area at 0.25° resolution.</p>
      <p id="d2e538">In the second step, we constructed a fuel consumption (FC) look-up table based on historical GFED5 burned area and emissions data. Using the same aggregation strategy as for EFA, we derived region- and biome-specific FC scalars, which were then applied to convert GFED5NRT burned area into emissions for each burning and/or land cover type. Several major land cover types exhibited pronounced long-term trends in FC during 2002–2022. To partially account for these trends, mean FC values from the more recent 2013–2022 period were used to estimate GFED5NRT emissions beyond 2022. Emissions of trace gases and aerosols were derived using the same emission factors as in the core GFED5 data, and for spatiotemporally variable savanna emission factors of CO<sub>2</sub>, CO, CH<sub>4</sub>, and N<sub>2</sub>O (Vernooij et al., 2023) we used a gridded (0.25°) daily climatology based on the 2002–2022 time series.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Generating the GFED5NRT products</title>
      <p id="d2e577">To support the operational, near-real-time production of daily GFED5NRT datasets, we developed a fully automated, standalone software system that implements the complete processing workflow (Fig. S2). The system is built primarily in Python and is distributed with all required ancillary inputs, including precomputed lookup tables and configuration files, allowing the pipeline to run independently without manual preparation. The workflow comprises sequential modules for automated acquisition of VIIRS active fire data, screening and filtering of detections, conversion of fire counts to burned area, and generation of corresponding emissions estimates. Execution of the workflow is managed by a master shell script that runs daily via a cron job. Upon execution, the script retrieves the latest VIIRS data from the FIRMS server, verifies global data completeness, and initiates GFED5NRT production only when sufficient coverage is available, thereby enabling robust and timely updates with minimal user intervention.</p>
      <p id="d2e580">Using this automated framework, daily GFED5NRT products are routinely generated with latencies of only a few hours. Three NRT product variants are produced: one based exclusively on SNPP VIIRS observations, one based on NOAA-20 VIIRS observations, and a combined product. In the combined product, burned area and emissions within each grid cell are calculated as the arithmetic mean of the SNPP- and NOAA-20-based estimates when both instruments are operating nominally. If observations from one satellite are unavailable, the combined product defaults to the remaining instrument. On days when active fire data are missing from both satellites, GFED5NRT production is suspended for that date. The pipeline is also adaptable to active fire detections from VIIRS sensors on other platforms such as NOAA-21, pending systematic evaluations of data quality and consistency. Each daily product is distributed in two compact NetCDF files: species files, which report emissions of individual trace gas and aerosol species, and ecosystem files, which describe the allocation of burned area and carbon emissions across the 16 land cover and burning classes. File structure, variable naming, and metadata conventions are fully consistent with those of the standard GFED5 products.</p>
      <p id="d2e583">When science-quality VIIRS active fire location data become available from the Fuoco server, the system will rerun the scaling procedure using these higher-quality inputs. During reprocessing, non-vegetation thermal anomalies are excluded directly using the fire type flag (type <inline-formula><mml:math id="M14" display="inline"><mml:mo>≠</mml:mo></mml:math></inline-formula> 0) provided in the science-quality data, and viewing geometry corrections are applied based on the sample column information in the same files. Dates with missing observations for individual VIIRS instruments, as documented on the FIRMS missing-dates webpage and summarized in Table S4, are filled using temporal interpolation. As science-quality data become available on an irregular schedule, the reprocessed GFED5NRT datasets are updated episodically for the SNPP-only, NOAA-20-only, and combined products. The daily datasets are subsequently aggregated to monthly products to facilitate analysis. Unless otherwise noted, all results presented in this study are based on the reprocessed, science-quality GFED5NRT combined product. For evaluation purposes, additional science-quality-based GFED5NRT burned area estimates derived solely from SNPP observations were generated for the 2012–2022 period.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Data for GFED5NRT evaluation</title>
      <p id="d2e601">We assessed the performance of the GFED5NRT burned area and fire emissions products using a diverse set of independent global and regional reference datasets.</p>
      <p id="d2e604">Evaluation of burned area focused on retrospective comparisons in Canada, South America, the United States (US), Europe, and Australia, where high-quality regional products are available. For South America, we used the INPE AQ1km burned area dataset (<uri>https://terrabrasilis.dpi.inpe.br/queimadas/aq1km/</uri>, last access: 10 January 2025), which is derived from MODIS 1 km imagery in combination with active fire detections from multiple satellite platforms (Libonati et al., 2015), as well as the MapBiomas Fire product (Collection 4; <uri>https://brasil.mapbiomas.org/en/mapbiomas-fogo/</uri>, last access: 21 May 2025), which is based on 30 m Landsat imagery and a machine-learning classification framework (Alencar et al., 2022). For Canada, we employed the Canadian National Fire Database (CNFDB; <uri>https://cwfis.cfs.nrcan.gc.ca/ha/nfdb</uri>, last access: 1 February 2025), which compiles fire perimeter records reported by provincial and territorial fire management agencies, and the National Burned Area Composite (NBAC; <uri>https://cwfis.cfs.nrcan.gc.ca/datamart/metadata/nbac</uri>, last access: 1 February 2025), a Landsat-based burned area product generated using change-detection techniques. In addition, two independent estimates of total burned area in Canada for 2023 were used for benchmarking purposes: NRCan_2023, derived from Natural Resources Canada Fire M3 hotspot-based fire perimeters, and TIIC_2023, produced using the Tracking Intra- and Inter-year Change (TIIC) algorithm (Pelletier et al., 2024). For the US, we utilized the Monitoring Trends in Burn Severity (MTBS; <uri>https://www.mtbs.gov/</uri>, last access: 9 March 2025) dataset, which uses Landsat imagery to provide comprehensive satellite-derived burned area data for large fire events exceeding specific regional size thresholds, alongside the Fire Program Analysis fire-occurrence database (FPA_FOD; Short, 2022), which compiles official federal, state, and local government fire reports to offer a detailed spatial inventory of wildfire activity. For Europe, we evaluated performance against the European Forest Fire Information System (EFFIS; <uri>https://forest-fire.emergency.copernicus.eu/</uri>, last access: 15 March 2026), which aggregates harmonized monthly burned area statistics reported by member countries and satellite-derived burned area mapping. Finally, for Australia, we relied on the regional data compiled within the ONFIRE database (Gincheva et al., 2024), which harmonizes fire perimeters and statistical data merged from individual state and territory fire management agencies into a common 1<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mi mathvariant="italic">°</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>×</mml:mo></mml:mrow></mml:math></inline-formula> 1° monthly gridded burned area product.</p>
      <p id="d2e637">To evaluate fire emissions, daily GFED5NRT emissions of carbon monoxide (CO), nitrogen oxides (NO<sub><italic>x</italic></sub>), and particulate matter (PM<sub>2.5</sub>) for 2023 were compared against three widely used global fire emissions inventories: the Fire Inventory from NCAR (FINN, version 2.5; Wiedinmyer et al., 2023), the Blended Global Biomass Burning Emissions Product (GBBEPx, version 3; Li et al., 2022), and the CAMS Global Fire Assimilation System (GFAS, version 1.2; Kaiser et al., 2012).</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e661">Mean EFA and FC by GFED region and aggregated land cover type. These scaling coefficients were derived from VIIRS active fire counts, and GFED5 burned area and emission data for 2012–2022. Land cover classes based on GFED5 burned area classifications (Table 2 in van der Werf et al., 2025) were consolidated into nine groups: BoreFor (“Boreal forest”, “Sparse boreal forest”, and “Tundra”); TempFor (“Temperate forest”); TropFor (“Tropical forest”); Defo (“Deforestation”); Peat (“Peatland”); Shrub (“Temperate shrubland”, “Temperate mosaic”, “Tropical shrubland”, and “Woody savanna”); Grass (“Temperate grassland”, “Tropical grassland”, and “Open savanna”); Crop (“Cropland”); and Other (all remaining burning types). The Peat category refers only to tropical peatland burning and excludes boreal peatlands. White grid cells indicate region–land-cover combinations with insufficient or no fire activity over 2012–2022 to compute robust scaling statistics.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f03.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Effective fire area and fuel consumption</title>
      <p id="d2e686">The GFED5NRT burned area (BA) and fire emissions (EM) products were derived from VIIRS active fire counts using two primary scaling coefficients: EFA and FC. Aggregated over the calibration period (2012–2022), EFA was calculated as the ratio of BA to the number of active fire detections, representing the mean burned area associated with a single VIIRS active fire detection, while FC was calculated as the ratio of EM to BA, reflecting the mean carbon emissions per unit burned area.</p>

      <fig id="F4a" specific-use="star"><label>Figure 4</label><caption><p id="d2e691"> </p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f04-part01.png"/>

        </fig>

      <fig id="F4b" specific-use="star"><label>Figure 4</label><caption><p id="d2e702">Monthly time series of regionally summed <bold>(a)</bold> burned area (Mha per month) and <bold>(b)</bold> fire emissions (Tg C per month) from GFED5 (2002–2022; black lines) and GFED5NRT (derived from SNPP and NOAA-20 combined, 2023–2024; orange lines). For comparison, the time series of GFED5NRT derived using SNPP only (GFED5NRT_VNP, 2012–2024; green lines) is also shown.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f04-part02.png"/>

        </fig>

      <p id="d2e718">As shown in Fig. 3, both EFA and FC exhibit substantial variability across land cover types and geographic regions. On average, EFA values are higher in grasslands and shrublands than in forests, reflecting differences in fire behavior and detection efficiency. The contrast arises from slower fire spread and more persistent burning within forests, combined with under-detection of fast-moving fires in grasslands and shrublands. Exceptionally low EFA values occur in tropical peatlands and deforested regions, where high fuel loads and prolonged smoldering combustion result in repeated active fire detections over relatively small areas. In contrast, croplands exhibit the highest EFA values among all land cover types, suggesting that agricultural burning is frequently under-detected, due to short fire duration, small fire size, low fire intensity, or burning that occurs between VIIRS overpasses (Hall et al., 2016, 2024).</p>
      <p id="d2e721">Fuel consumption varies systematically by land cover type, consistent with differences in average fuel availability and biomass density. FC generally decreases from forests to shrublands, grasslands, and croplands, reflecting the declining gradient in ecosystem biomass. Across most GFED regions, FC values are relatively consistent, with notable exceptions including elevated FC for peatland fires in Equatorial Asia (EQAS) and deforestation fires in southern-hemisphere South America (SHSA).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Evaluation of GFED5NRT</title>
      <p id="d2e732">We first evaluated the GFED5NRT burned area and emissions products by comparing them with the standard GFED5 dataset over their overlapping period (2012–2022). Monthly time series of burned area and emissions from GFED5NRT closely match those from GFED5 across all GFED regions, capturing both seasonal cycles and interannual variability (Fig. 4). Agreement is generally strong, though moderate spatial variations emerge among individual regions (Fig. 5; Table 1). Comparisons of gridded burned area and emissions at 0.25° resolution further confirm strong spatial consistency between the two datasets (Fig. S3; Table 1). To further assess consistency, we compared monthly latitudinal zonal anomalies of burned area and emissions – normalized as <inline-formula><mml:math id="M18" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-scores – between GFED5 and GFED5NRT using Hovmöller diagrams (Fig. 6). The close correspondence of anomaly structures, together with the smooth transition from the GFED5 period (2012–2022) to the GFED5NRT period (2023–2024), indicates strong internal consistency between the two datasets at large spatial scales. Direct comparisons during extreme fire events further show that GFED5NRT closely reproduces the magnitude and spatial patterns of the corresponding GFED5 anomalies (Fig. S4). Overall, these results demonstrate that GFED5NRT provides a reliable near-real-time extension of GFED5, maintaining strong temporal and spatial consistency with the standard product.</p>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e744">Global maps of the Spearman correlation between GFED5 and GFED5NRT <bold>(a)</bold> burned area and <bold>(b)</bold> carbon emissions during 2012–2022. The global mean correlation coefficients weighted by the spatial pattern of mean annual burned area or emissions are also shown in the figure.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f05.png"/>

        </fig>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e762">Performance statistics for GFED5NRT burned area and fire emissions relative to the standard GFED5 product during 2012–2022 for the 14 GFED regions and the globe. Spatial statistics are calculated from the multi-year mean values at each 0.25° grid cell within a region, whereas temporal statistics are calculated from the monthly time series of regional totals over the 132-month overlap period. <inline-formula><mml:math id="M19" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>, Pearson correlation coefficient; <inline-formula><mml:math id="M20" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>, slope of a reduced major axis regression; nRMSE, root-mean-square error normalized by the mean value, expressed as a percentage; TSS, Taylor Skill Score, combining correlation and normalized standard deviation into a single skill metric ranging from 0 to 1, with 1 indicating perfect agreement with observations.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="17">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right" colsep="1"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right" colsep="1"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right"/>
     <oasis:colspec colnum="12" colname="col12" align="right"/>
     <oasis:colspec colnum="13" colname="col13" align="right" colsep="1"/>
     <oasis:colspec colnum="14" colname="col14" align="right"/>
     <oasis:colspec colnum="15" colname="col15" align="right"/>
     <oasis:colspec colnum="16" colname="col16" align="right"/>
     <oasis:colspec colnum="17" colname="col17" align="right"/>
     <oasis:thead>
       <oasis:row>

         <oasis:entry rowsep="1" colname="col1" morerows="2">Region</oasis:entry>

         <oasis:entry rowsep="1" namest="col2" nameend="col9" align="center" colsep="1">Burned Area </oasis:entry>

         <oasis:entry rowsep="1" namest="col10" nameend="col17" align="center">Fire Emissions </oasis:entry>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry namest="col2" nameend="col5" align="center" colsep="1">Spatial Corr. </oasis:entry>

         <oasis:entry namest="col6" nameend="col9" align="center" colsep="1">Temporal Corr. </oasis:entry>

         <oasis:entry namest="col10" nameend="col13" align="center" colsep="1">Spatial Corr. </oasis:entry>

         <oasis:entry namest="col14" nameend="col17" align="center">Temporal Corr. </oasis:entry>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry colname="col2"><inline-formula><mml:math id="M21" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col3"><inline-formula><mml:math id="M22" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col4">nRMSE</oasis:entry>

         <oasis:entry colname="col5">TSS</oasis:entry>

         <oasis:entry colname="col6"><inline-formula><mml:math id="M23" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col7"><inline-formula><mml:math id="M24" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col8">nRMSE</oasis:entry>

         <oasis:entry colname="col9">TSS</oasis:entry>

         <oasis:entry colname="col10"><inline-formula><mml:math id="M25" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col11"><inline-formula><mml:math id="M26" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col12">nRMSE</oasis:entry>

         <oasis:entry colname="col13">TSS</oasis:entry>

         <oasis:entry colname="col14"><inline-formula><mml:math id="M27" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col15"><inline-formula><mml:math id="M28" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula></oasis:entry>

         <oasis:entry colname="col16">nRMSE</oasis:entry>

         <oasis:entry colname="col17">TSS</oasis:entry>

       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>

         <oasis:entry colname="col1">BONA</oasis:entry>

         <oasis:entry colname="col2">0.86</oasis:entry>

         <oasis:entry colname="col3">1.09</oasis:entry>

         <oasis:entry colname="col4">98</oasis:entry>

         <oasis:entry colname="col5">0.74</oasis:entry>

         <oasis:entry colname="col6">0.93</oasis:entry>

         <oasis:entry colname="col7">1.18</oasis:entry>

         <oasis:entry colname="col8">60</oasis:entry>

         <oasis:entry colname="col9">0.85</oasis:entry>

         <oasis:entry colname="col10">0.80</oasis:entry>

         <oasis:entry colname="col11">1.01</oasis:entry>

         <oasis:entry colname="col12">127</oasis:entry>

         <oasis:entry colname="col13">0.66</oasis:entry>

         <oasis:entry colname="col14">0.94</oasis:entry>

         <oasis:entry colname="col15">1.05</oasis:entry>

         <oasis:entry colname="col16">77</oasis:entry>

         <oasis:entry colname="col17">0.88</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">TENA</oasis:entry>

         <oasis:entry colname="col2">0.78</oasis:entry>

         <oasis:entry colname="col3">0.99</oasis:entry>

         <oasis:entry colname="col4">106</oasis:entry>

         <oasis:entry colname="col5">0.62</oasis:entry>

         <oasis:entry colname="col6">0.79</oasis:entry>

         <oasis:entry colname="col7">1.16</oasis:entry>

         <oasis:entry colname="col8">39</oasis:entry>

         <oasis:entry colname="col9">0.62</oasis:entry>

         <oasis:entry colname="col10">0.80</oasis:entry>

         <oasis:entry colname="col11">0.97</oasis:entry>

         <oasis:entry colname="col12">124</oasis:entry>

         <oasis:entry colname="col13">0.66</oasis:entry>

         <oasis:entry colname="col14">0.97</oasis:entry>

         <oasis:entry colname="col15">0.86</oasis:entry>

         <oasis:entry colname="col16">33</oasis:entry>

         <oasis:entry colname="col17">0.92</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">CEAM</oasis:entry>

         <oasis:entry colname="col2">0.92</oasis:entry>

         <oasis:entry colname="col3">0.97</oasis:entry>

         <oasis:entry colname="col4">49</oasis:entry>

         <oasis:entry colname="col5">0.85</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">1.07</oasis:entry>

         <oasis:entry colname="col8">18</oasis:entry>

         <oasis:entry colname="col9">0.98</oasis:entry>

         <oasis:entry colname="col10">0.89</oasis:entry>

         <oasis:entry colname="col11">0.99</oasis:entry>

         <oasis:entry colname="col12">70</oasis:entry>

         <oasis:entry colname="col13">0.79</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">1.03</oasis:entry>

         <oasis:entry colname="col16">22</oasis:entry>

         <oasis:entry colname="col17">0.98</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">NHSA</oasis:entry>

         <oasis:entry colname="col2">0.93</oasis:entry>

         <oasis:entry colname="col3">0.96</oasis:entry>

         <oasis:entry colname="col4">55</oasis:entry>

         <oasis:entry colname="col5">0.87</oasis:entry>

         <oasis:entry colname="col6">0.98</oasis:entry>

         <oasis:entry colname="col7">1.08</oasis:entry>

         <oasis:entry colname="col8">22</oasis:entry>

         <oasis:entry colname="col9">0.96</oasis:entry>

         <oasis:entry colname="col10">0.92</oasis:entry>

         <oasis:entry colname="col11">1.04</oasis:entry>

         <oasis:entry colname="col12">55</oasis:entry>

         <oasis:entry colname="col13">0.84</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">0.92</oasis:entry>

         <oasis:entry colname="col16">24</oasis:entry>

         <oasis:entry colname="col17">0.97</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">SHSA</oasis:entry>

         <oasis:entry colname="col2">0.94</oasis:entry>

         <oasis:entry colname="col3">1.00</oasis:entry>

         <oasis:entry colname="col4">47</oasis:entry>

         <oasis:entry colname="col5">0.88</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">1.12</oasis:entry>

         <oasis:entry colname="col8">17</oasis:entry>

         <oasis:entry colname="col9">0.97</oasis:entry>

         <oasis:entry colname="col10">0.90</oasis:entry>

         <oasis:entry colname="col11">1.00</oasis:entry>

         <oasis:entry colname="col12">72</oasis:entry>

         <oasis:entry colname="col13">0.82</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">1.10</oasis:entry>

         <oasis:entry colname="col16">22</oasis:entry>

         <oasis:entry colname="col17">0.97</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">EURO</oasis:entry>

         <oasis:entry colname="col2">0.91</oasis:entry>

         <oasis:entry colname="col3">1.00</oasis:entry>

         <oasis:entry colname="col4">90</oasis:entry>

         <oasis:entry colname="col5">0.83</oasis:entry>

         <oasis:entry colname="col6">0.95</oasis:entry>

         <oasis:entry colname="col7">1.00</oasis:entry>

         <oasis:entry colname="col8">31</oasis:entry>

         <oasis:entry colname="col9">0.90</oasis:entry>

         <oasis:entry colname="col10">0.84</oasis:entry>

         <oasis:entry colname="col11">1.08</oasis:entry>

         <oasis:entry colname="col12">122</oasis:entry>

         <oasis:entry colname="col13">0.72</oasis:entry>

         <oasis:entry colname="col14">0.90</oasis:entry>

         <oasis:entry colname="col15">0.89</oasis:entry>

         <oasis:entry colname="col16">52</oasis:entry>

         <oasis:entry colname="col17">0.80</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">MIDE</oasis:entry>

         <oasis:entry colname="col2">0.88</oasis:entry>

         <oasis:entry colname="col3">0.99</oasis:entry>

         <oasis:entry colname="col4">146</oasis:entry>

         <oasis:entry colname="col5">0.78</oasis:entry>

         <oasis:entry colname="col6">0.96</oasis:entry>

         <oasis:entry colname="col7">0.97</oasis:entry>

         <oasis:entry colname="col8">24</oasis:entry>

         <oasis:entry colname="col9">0.91</oasis:entry>

         <oasis:entry colname="col10">0.89</oasis:entry>

         <oasis:entry colname="col11">0.93</oasis:entry>

         <oasis:entry colname="col12">170</oasis:entry>

         <oasis:entry colname="col13">0.74</oasis:entry>

         <oasis:entry colname="col14">0.96</oasis:entry>

         <oasis:entry colname="col15">0.89</oasis:entry>

         <oasis:entry colname="col16">26</oasis:entry>

         <oasis:entry colname="col17">0.92</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">NHAF</oasis:entry>

         <oasis:entry colname="col2">0.97</oasis:entry>

         <oasis:entry colname="col3">0.97</oasis:entry>

         <oasis:entry colname="col4">31</oasis:entry>

         <oasis:entry colname="col5">0.95</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">0.98</oasis:entry>

         <oasis:entry colname="col8">15</oasis:entry>

         <oasis:entry colname="col9">0.98</oasis:entry>

         <oasis:entry colname="col10">0.94</oasis:entry>

         <oasis:entry colname="col11">1.01</oasis:entry>

         <oasis:entry colname="col12">46</oasis:entry>

         <oasis:entry colname="col13">0.89</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">1.02</oasis:entry>

         <oasis:entry colname="col16">12</oasis:entry>

         <oasis:entry colname="col17">0.99</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">SHAF</oasis:entry>

         <oasis:entry colname="col2">0.96</oasis:entry>

         <oasis:entry colname="col3">0.98</oasis:entry>

         <oasis:entry colname="col4">29</oasis:entry>

         <oasis:entry colname="col5">0.92</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">1.00</oasis:entry>

         <oasis:entry colname="col8">17</oasis:entry>

         <oasis:entry colname="col9">0.97</oasis:entry>

         <oasis:entry colname="col10">0.94</oasis:entry>

         <oasis:entry colname="col11">1.02</oasis:entry>

         <oasis:entry colname="col12">39</oasis:entry>

         <oasis:entry colname="col13">0.88</oasis:entry>

         <oasis:entry colname="col14">1.00</oasis:entry>

         <oasis:entry colname="col15">1.01</oasis:entry>

         <oasis:entry colname="col16">9</oasis:entry>

         <oasis:entry colname="col17">0.99</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">BOAS</oasis:entry>

         <oasis:entry colname="col2">0.86</oasis:entry>

         <oasis:entry colname="col3">1.05</oasis:entry>

         <oasis:entry colname="col4">103</oasis:entry>

         <oasis:entry colname="col5">0.75</oasis:entry>

         <oasis:entry colname="col6">0.94</oasis:entry>

         <oasis:entry colname="col7">1.00</oasis:entry>

         <oasis:entry colname="col8">45</oasis:entry>

         <oasis:entry colname="col9">0.88</oasis:entry>

         <oasis:entry colname="col10">0.85</oasis:entry>

         <oasis:entry colname="col11">1.04</oasis:entry>

         <oasis:entry colname="col12">91</oasis:entry>

         <oasis:entry colname="col13">0.73</oasis:entry>

         <oasis:entry colname="col14">0.97</oasis:entry>

         <oasis:entry colname="col15">1.00</oasis:entry>

         <oasis:entry colname="col16">39</oasis:entry>

         <oasis:entry colname="col17">0.94</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">CEAS</oasis:entry>

         <oasis:entry colname="col2">0.83</oasis:entry>

         <oasis:entry colname="col3">0.97</oasis:entry>

         <oasis:entry colname="col4">77</oasis:entry>

         <oasis:entry colname="col5">0.69</oasis:entry>

         <oasis:entry colname="col6">0.97</oasis:entry>

         <oasis:entry colname="col7">0.91</oasis:entry>

         <oasis:entry colname="col8">20</oasis:entry>

         <oasis:entry colname="col9">0.94</oasis:entry>

         <oasis:entry colname="col10">0.79</oasis:entry>

         <oasis:entry colname="col11">1.00</oasis:entry>

         <oasis:entry colname="col12">81</oasis:entry>

         <oasis:entry colname="col13">0.64</oasis:entry>

         <oasis:entry colname="col14">0.97</oasis:entry>

         <oasis:entry colname="col15">0.97</oasis:entry>

         <oasis:entry colname="col16">17</oasis:entry>

         <oasis:entry colname="col17">0.95</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">SEAS</oasis:entry>

         <oasis:entry colname="col2">0.94</oasis:entry>

         <oasis:entry colname="col3">0.97</oasis:entry>

         <oasis:entry colname="col4">48</oasis:entry>

         <oasis:entry colname="col5">0.89</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">1.06</oasis:entry>

         <oasis:entry colname="col8">20</oasis:entry>

         <oasis:entry colname="col9">0.98</oasis:entry>

         <oasis:entry colname="col10">0.90</oasis:entry>

         <oasis:entry colname="col11">1.00</oasis:entry>

         <oasis:entry colname="col12">80</oasis:entry>

         <oasis:entry colname="col13">0.81</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">1.01</oasis:entry>

         <oasis:entry colname="col16">19</oasis:entry>

         <oasis:entry colname="col17">0.99</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">EQAS</oasis:entry>

         <oasis:entry colname="col2">0.90</oasis:entry>

         <oasis:entry colname="col3">1.02</oasis:entry>

         <oasis:entry colname="col4">71</oasis:entry>

         <oasis:entry colname="col5">0.81</oasis:entry>

         <oasis:entry colname="col6">0.99</oasis:entry>

         <oasis:entry colname="col7">1.09</oasis:entry>

         <oasis:entry colname="col8">29</oasis:entry>

         <oasis:entry colname="col9">0.97</oasis:entry>

         <oasis:entry colname="col10">0.92</oasis:entry>

         <oasis:entry colname="col11">0.93</oasis:entry>

         <oasis:entry colname="col12">92</oasis:entry>

         <oasis:entry colname="col13">0.85</oasis:entry>

         <oasis:entry colname="col14">0.99</oasis:entry>

         <oasis:entry colname="col15">1.03</oasis:entry>

         <oasis:entry colname="col16">35</oasis:entry>

         <oasis:entry colname="col17">0.98</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">AUST</oasis:entry>

         <oasis:entry colname="col2">0.96</oasis:entry>

         <oasis:entry colname="col3">0.98</oasis:entry>

         <oasis:entry colname="col4">50</oasis:entry>

         <oasis:entry colname="col5">0.92</oasis:entry>

         <oasis:entry colname="col6">0.95</oasis:entry>

         <oasis:entry colname="col7">1.05</oasis:entry>

         <oasis:entry colname="col8">22</oasis:entry>

         <oasis:entry colname="col9">0.91</oasis:entry>

         <oasis:entry colname="col10">0.94</oasis:entry>

         <oasis:entry colname="col11">1.00</oasis:entry>

         <oasis:entry colname="col12">57</oasis:entry>

         <oasis:entry colname="col13">0.89</oasis:entry>

         <oasis:entry colname="col14">0.97</oasis:entry>

         <oasis:entry colname="col15">1.03</oasis:entry>

         <oasis:entry colname="col16">21</oasis:entry>

         <oasis:entry colname="col17">0.94</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Global</oasis:entry>

         <oasis:entry colname="col2">0.97</oasis:entry>

         <oasis:entry colname="col3">1.00</oasis:entry>

         <oasis:entry colname="col4">61</oasis:entry>

         <oasis:entry colname="col5">0.94</oasis:entry>

         <oasis:entry colname="col6">0.94</oasis:entry>

         <oasis:entry colname="col7">1.07</oasis:entry>

         <oasis:entry colname="col8">8</oasis:entry>

         <oasis:entry colname="col9">0.88</oasis:entry>

         <oasis:entry colname="col10">0.94</oasis:entry>

         <oasis:entry colname="col11">1.04</oasis:entry>

         <oasis:entry colname="col12">77</oasis:entry>

         <oasis:entry colname="col13">0.88</oasis:entry>

         <oasis:entry colname="col14">0.98</oasis:entry>

         <oasis:entry colname="col15">1.04</oasis:entry>

         <oasis:entry colname="col16">7</oasis:entry>

         <oasis:entry colname="col17">0.97</oasis:entry>

       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e1792">Monthly <inline-formula><mml:math id="M29" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-score of burned area (BA) and fire emissions (EM) in each 0.25° latitudinal band. <bold>(a)</bold> GFED5 (2012–2022) and GFED5NRT (SNPP and NOAA-20 combined version; 2023–2024). Red dashed vertical lines denote the start of the GFED5NRT record in 2023. <bold>(b)</bold> GFED5NRT derived using SNPP only (GFED5NRT_VNP) for 2012–2024. The unitless <inline-formula><mml:math id="M30" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-score, or the normalized anomaly, is defined as <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mi>v</mml:mi><mml:mo>-</mml:mo><mml:mi>m</mml:mi><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mi mathvariant="normal">SD</mml:mi></mml:mrow></mml:math></inline-formula>, where <italic>v </italic> is the monthly burned area or emissions, <inline-formula><mml:math id="M32" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is the climatological monthly mean, and SD is the standard deviation of interannual variability. The same climatological means and standard deviations from GFED5 (2012–2022) were used for the calculations of <inline-formula><mml:math id="M33" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-scores in all three datasets.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f06.png"/>

        </fig>

      <p id="d2e1863">The NASA VIIRS VNP64A1 burned area product, recently introduced as a successor to the long-term MODIS record, uses a modified mapping algorithm to provide global fire data continuity from 2012 into the coming decade (Giglio et al., 2025). Here we compare the GFED5NRT burned area estimates with VNP64A1. Overall, GFED5NRT and VNP64A1 identify burning in broadly similar regions in 2023, but GFED5NRT detects substantially more burned area overall, including in areas where VNP64A1 shows little or no burning (Fig. S5), consistent with its greater sensitivity to small and low-intensity fires through the active fire-based scaling.</p>
      <p id="d2e1866">Compared with regional burned area datasets derived from high-resolution satellite observations and fire records, annual burned area estimates from GFED5 and GFED5NRT are generally of comparable magnitude, and exhibit similar interannual variability within and across regions (Fig. S6). These reference datasets differ substantially in mapping methodology and coverage: some exclude small burned patches, others omit cropland or non-forest burning, which likely explain the tendency for GFED5 and GFED5NRT to report higher annual burned area, most notably in Europe, where EFFIS includes only fires larger than 30 ha that are at least partially forested. In Canada, GFED5 and GFED5NRT estimates are slightly higher than NBAC during extreme fire years (e.g., 2023 and 2024), likely because NBAC explicitly delineates small unburned islands that may not be resolved at coarser spatial resolutions. In Brazil, GFED5 and GFED5NRT totals generally agree with the INPE AQ1km product, but are substantially higher than MapBiomas, reflecting well-documented methodological differences among these datasets. In the US, MTBS's minimum size threshold (202–405 ha) and FPA_FOD's exclusion of prescribed and controlled burns likely explain why GFED5 and GFED5NRT run consistently higher than these reference datasets. In Australia, GFED5 and GFED5NRT closely track ONFIRE in magnitude and timing of major fire years (e.g., the 2019–2020 “Black Summer”).</p>
      <p id="d2e1869">Finally, comparisons of daily CO, NO<sub><italic>x</italic></sub>, and PM<sub>2.5</sub> emissions in 2023 with three widely used global fire emissions inventories – FINN, GBBEPx, and GFAS – show that GFED5NRT captures similar day-to-day variability in global fire emissions (Figs. 7 and S7), although substantial regional differences remain in the absolute magnitude of emissions. These discrepancies underscore the importance of multi-dataset comparisons for uncertainty characterization, particularly when applying fire emissions products to air quality modeling, climate research, and carbon budget analyses.</p>

      <fig id="F7" specific-use="star"><label>Figure 7</label><caption><p id="d2e1892">Comparison of daily global and regional CO emission totals in 2023 from GFED5NRT with three existing daily fire emissions datasets: the Fire Inventory from NCAR (FINN, v2.5), the Blended Global Biomass Burning Emissions Product (GBBEPx, v3), and the CAMS Global Fire Assimilation System (GFAS, v1.2). Light-colored lines show the original daily time series, and the dark-colored lines show the 5 d smoothed time series.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Fire burned area and emissions in 2023 and 2024</title>
      <p id="d2e1909">Based on GFED5NRT, global fire emissions are substantially elevated in both 2023 and 2024 relative to the GFED5 long-term mean for 2002–2022 (Figs. 8 and 9; Table S5). In 2023, the global total fire emissions (3.89 Pg C yr<sup>−1</sup>) were anomalously high, driven by record-breaking emissions in boreal North America and positive anomalies in Central America, southern Africa, and Australia. In 2024, global fire emissions were even higher (4.03 Pg C yr<sup>−1</sup>), reflecting a second consecutive year of extreme emissions in boreal North America, combined with pronounced positive anomalies in South America and southern Africa. Given that global fire emissions were relatively low in 2021 and 2022, the large positive wildfire emissions anomalies observed in subsequent years likely contributed substantially to the anomalously high atmospheric CO<sub>2</sub> growth rate observed during the 2023–2024 ENSO event (Friedlingstein et al., 2025).</p>

      <fig id="F8a" specific-use="star"><label>Figure 8</label><caption><p id="d2e1947"> </p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f08-part01.png"/>

        </fig>

      <fig id="F8b" specific-use="star"><label>Figure 8</label><caption><p id="d2e1958">Annual time series of regionally summed <bold>(a)</bold> burned area (Mha yr<sup>−1</sup>) and <bold>(b)</bold> fire emissions (Tg C yr<sup>−1</sup>),  merging three GFED5 products: the core period (2002–2022, orange), the pre-MODIS period (1997–2001, gray), and the GFED5NRT product (2023–2024, red).</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f08-part02.png"/>

        </fig>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e2000">Global maps of <inline-formula><mml:math id="M41" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-scores (standardized anomalies) for GFED5NRT burned area and fire emissions in 2023 and 2024. Red and blue colors indicate positive and negative anomalies, respectively. Numbers show the mean <inline-formula><mml:math id="M42" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-scores (normalized using the GFED5 data during 2002–2022) for each of the 14 GFED regions.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f09.png"/>

        </fig>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e2025">Global maps of <bold>(a)</bold> standardized anomalies and <bold>(b)</bold> annual mean fire emissions from GFED5NRT averaged over 2023–2024. Red polygons indicate identified regional fire events during 2023–2024.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f10.png"/>

        </fig>

      <p id="d2e2040">At a global scale, the inclusion of two additional years of burned area observations from GFED5NRT weakens (but does not reverse) the long-term declining trend in burned area observed during the core GFED5 period (Table S5). This global decline is driven by sustained reductions in burned area across northern Africa and boreal and central Asia (Fig. 8a). In these regions, burning levels in 2023 and 2024 from GFED5NRT are comparable to those observed near the end of the GFED5 record (2020–2022).</p>
      <p id="d2e2043">For emissions, the new GFED5NRT observations for 2023 and 2024 do not change the storyline reported by van der Werf et al. (2025) that while there is considerable interannual variability, there is no significant long-term trend in global carbon emissions from fires. Across regions, declining emissions trends in equatorial Asia, northern hemisphere Africa and central Asia are balanced by upward trends in boreal and temperate North America and southern hemisphere Africa. Within individual regions, a shift in fire activity toward ecosystems with higher fuel densities resulted in more positive trends in emissions than in burned area trends (Table S5).</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Recent fire extremes</title>
      <p id="d2e2054">Fire activity exhibited significant spatial heterogeneity, even within individual GFED regions. GFED5NRT enables the timely identification of regional extreme fire hotspots and the characterization of fire behavior within these areas. Using <inline-formula><mml:math id="M43" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>-score-based thresholds combined with spatial aggregation techniques (Sect. S4), we identified 16 recent extreme fire events during 2023–2024 (Fig. 10) and quantified their emissions relative to the 2002–2022 climatology (Fig. S8). These events spanned multiple continents and were predominantly concentrated in tropical and boreal forests and shrublands. Collectively, the 16 events produced mean annual emissions of 1.9 Pg C during 2023–2024, which is about 0.8 Pg C (73 %) above the 2002–2022 climatological average over the same regions (Table S6), accounting for about half of global fire emissions during this biennial period.</p>
      <p id="d2e2064">Emissions from individual extreme regions ranged from 5 to 68 standard deviations above their respective climatological means. The highest relative anomalies, exceeding three times the climatological mean, occurred in eastern and western Canada, and Bolivia. Several regions, including western Canada, Central America, and southeastern Siberia, experienced persistent extreme fire activity in both years (Fig. S8). Aggregated emission anomalies from these extreme regions reached 807 Tg C yr<sup>−1</sup>, more than compensating for negative anomalies in other regions (<inline-formula><mml:math id="M45" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>213 Tg C yr<sup>−1</sup>), and resulting in a net positive global emissions anomaly of 594 Tg C yr<sup>−1</sup>, equivalent to 2.7 standard deviations above the climatological mean.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Global wildfire situation updated by the GFED5NRT</title>
      <p id="d2e2119">The GFED5NRT dataset enables daily-scale quantification of burned area and fire-related emissions, substantially enhancing our ability to monitor evolving fire activity and its impacts. By providing timely estimates of burned area and emissions, GFED5NRT supports applications such as fire danger assessment, simulation and forecasting of smoke-driven air quality impacts, and rapid response to both direct fire hazards and downstream environmental and public health risks.</p>
      <p id="d2e2122">Figure 11 illustrates an example operational update, showing daily and cumulative global and regional fire emissions through a selected date. Figures S9 and S10 further demonstrate the utility of the dataset by highlighting two extreme fire events – one in BONA (2023) and another in SHSA (2024) – and placing them in the context of historical variability captured by the GFED5NRT datasets.</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e2127">Example summary figures (updated through 12 October 2025) automatically generated by the GFED5NRT system. <bold>(a)</bold> Daily fire emission sums (Tg C d<sup>−1</sup>) globally and by GFED regions.  Red lines show GFED5NRT data for 2025. Black lines and gray areas indicate the historical mean and <inline-formula><mml:math id="M49" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 standard deviation based on 2002–2022. <bold>(b)</bold> Cumulative fire emissions up to the reference date. Red, dark orange, orange, and gray lines represent 2025, 2024, 2023, and individual years from 2002–2022, respectively.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/7535/2026/essd-18-7535-2026-f11.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Uncertainty</title>
      <p id="d2e2170">Uncertainty in GFED5NRT stems from two primary sources: baseline uncertainties inherited from the GFED5 framework, and methodological uncertainties introduced by the NRT scheme developed here. We distinguish these components because GFED5NRT is designed to provide a methodologically consistent temporal extension of the established GFED5 record.</p>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Uncertainty inherited from GFED5</title>
      <p id="d2e2181">GFED5 burned area and emissions are subject to uncertainties in satellite-derived burned area and active fire observations, as well as in the subsequent modeling of fuel consumption and emissions, including assumptions regarding combustion completeness and emission factors and the representation of specific fire types such as agricultural burning, peat fires, and deforestation fires. These uncertainties are inherited by GFED5NRT and are not re-estimated as part of the NRT extension.</p>
      <p id="d2e2184">The baseline uncertainty of the GFED5 product has been evaluated in our prior assessments against independent observational datasets (Chen et al., 2023; Hall et al., 2024; van der Werf et al., 2025). These evaluations provide an empirical basis for assessing the magnitude and implications of uncertainty in the underlying GFED5 estimates. In contrast, a comprehensive analytical, bottom-up propagation of GFED5 uncertainty is not currently feasible, because it would require well-constrained empirical probability distributions and full error covariance matrices for numerous interdependent satellite, ecological, and physical parameters. Accordingly, we rely on these prior evaluations rather than deriving a new formal uncertainty budget for the baseline GFED5 product.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Additional uncertainty introduced by GFED5NRT</title>
      <p id="d2e2196">The principal additional uncertainties in GFED5NRT arise from the use of static scaling factors and land-cover information to translate NRT VIIRS active fire observations into the GFED5 framework. Effective fire area, fuel consumption scalars, and land cover classifications are held fixed during the NRT extension, maintaining consistency with the historical GFED5 record but potentially limiting representation of changes in fire size, fuel availability, fuel moisture, and plant functional type. In addition, active fire observations provide instantaneous rather than cumulative measures of fire activity and are subject to limitations such as cloud and smoke obscuration and variations in detection conditions. These factors introduce uncertainty beyond that inherited from GFED5.</p>
      <p id="d2e2199">We quantified the additional uncertainty by comparing GFED5NRT with GFED5 over their 2012–2022 overlap period, using region-aggregated monthly time series and grid-cell-level spatial patterns of burned area and emissions (Table 1 and Fig. 5). We report the Pearson correlation coefficient (<inline-formula><mml:math id="M50" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>), reduced major axis regression slope (<inline-formula><mml:math id="M51" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>), normalized root-mean-square error (nRMSE), and Taylor Skill Score (TSS), which combines the correlation and the ratio of standard deviations into a single measure of agreement (Taylor, 2001). Spatial TSS ranged from 0.62 to 0.95 for burned area and from 0.64 to 0.89 for emissions across regions, with global values of 0.94 and 0.88, respectively. Temporal TSS ranged from 0.62 to 0.98 for burned area and from 0.80 to 0.99 for emissions, with global values of 0.88 and 0.97, respectively.</p>
      <p id="d2e2216">These metrics demonstrate that GFED5NRT reliably reproduces continental-scale spatial gradients, seasonal cycles, interannual variability, and major fire anomalies captured in GFED5. However, regional divergences highlight the limitations of uniform regional scaling factors across landscapes with pronounced sub-regional heterogeneity in fuel types and fire behavior. Consequently, GFED5NRT is more robust when aggregated over broad spatial domains and long timeframes, whereas fine-scale assessments (e.g., grid-cell, national or subnational) carry substantially higher uncertainty, particularly regarding quantitative trends in burned area and emissions. Importantly, these evaluation metrics quantify inter-product consistency and transfer errors rather than formal parametric confidence bounds.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Independent benchmarking of GFED5NRT</title>
      <p id="d2e2227">To contextualize GFED5NRT within the broader observational landscape, we conducted systematic multi-dataset benchmarking (Sect. 3.2). Monthly GFED5NRT burned area was evaluated against independent global satellite products, including VIIRS VNP64A1, as well as high-resolution regional inventories (e.g., INPE, MapBiomas, NBAC, MTBS, EFFIS, and ONFIRE). In parallel, daily emissions were compared against operational fire-emission inventories, including FINN, GFAS, and GBBEPx, confirming the spatial and temporal coherence of GFED5NRT relative to existing services.</p>
      <p id="d2e2230">Future versions of GFED5NRT will target these uncertainties through several methodological refinements, including improved dynamic estimates of effective fire area and fuel consumption, incorporation of updated land-cover information, and refinement of algorithms for constraining fire-emissions estimates using fire radiative power observations. An important next step is establishing an integrated atmospheric validation pipeline to provide objective top-down constraints on fire emissions. Following the architecture of the International Land Model Benchmarking system (ILAMB; Collier et al., 2018), a chemical transport model driven by fire emissions inventories could be used to evaluate simulated trace gas (CO, NO<sub>2</sub>) and aerosol fields (aerosol optical depth, surface particulate concentrations) against surface networks and satellite retrievals. Such a benchmarking framework would enable standardized, quantitative assessments of individual inventories and track performance across model iterations.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Data availability</title>
      <p id="d2e2252">The reprocessed 2023–2024 GFED5NRT datasets are publicly archived in the open-access Zenodo repository (<ext-link xlink:href="https://doi.org/10.5281/zenodo.18702700" ext-link-type="DOI">10.5281/zenodo.18702700</ext-link>; Chen et al., 2026). Routinely updated GFED5NRT products, including the reprocessed 2023–2024 data, are freely accessible at <uri>https://www.globalfiredata.org</uri>, last access: 28 September 2026. The Python-based framework used to generate these products is openly available at <uri>https://github.com/ychenzgithub/GFED5NRT</uri>, last access: 13 October 2026.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Conclusions</title>
      <p id="d2e2272">The accelerating orbital drift and imminent decommissioning of the Terra and Aqua satellites necessitate fusing fire records derived from these platforms with other higher-resolution, continuous data streams. The GFED5NRT dataset presented here represents a first step toward addressing this challenge by providing a temporally consistent, extended record of burned area and fire emissions derived from VIIRS active-fire observations. GFED5NRT advances the GFED framework by integrating VIIRS data through a two-step scaling approach that uses region- and biome-specific effective fire area and fuel consumption look-up tables. This design preserves continuity with the established GFED5 product while extending the record beyond 2022. By combining GFED5 and GFED5NRT, we construct a near-real-time fire dataset that enables a more robust assessment of recent fire variability at regional and global scales. The new fire observations from GFED5NRT reveal record-breaking carbon emissions in 2023 in boreal North America and in 2024 in South America. Our analysis also confirms a significant global decline in burned area since 2002, driven primarily by reduced burning in Northern Hemisphere Africa and boreal and central Asia. However, this downward trend is likely weaker than previously reported by Andela et al. (2017) and Chen et al. (2023) due to higher levels of burning in Southern Hemisphere Africa, Australia, and boreal North America in the last two years. Global fire emissions remain relatively stable (van der Werf et al., 2025), with recent increases in North and South America balanced by declines in Asia.</p>
      <p id="d2e2275">Currently, GFED5NRT is implemented at daily temporal resolution based on VIIRS active fire products. However, many fire-related applications, such as rapid response and smoke transport modeling, require sub-daily information and short-term forecasts. Previous studies have addressed this need by parameterizing diurnal fire cycles using fire radiative power observations from geostationary satellites (Andela et al., 2015; Xu et al., 2017), and the standard GFED5 framework incorporates climatological hourly cycles derived from GOES observations (van der Werf et al., 2025). More recent efforts have further advanced these approaches by fusing observations from multiple polar-orbiting and geostationary sensors (Li et al., 2022; Zhang et al., 2012; Zheng et al., 2021). Incorporating such multi-sensor strategies into future GFED developments would enable estimation of sub-daily fire variability, substantially enhancing the dataset's value for real-time air quality forecasting and fire behavior monitoring.</p>
      <p id="d2e2278">Another critical next step is the development of a global multi-decade fire reanalysis that harmonizes burned area time series from MODIS and VIIRS with higher-resolution observations from Sentinel-2 and Landsat. In parallel, harmonizing surface reflectance time series across MODIS, VIIRS, and Landsat would enable the development of a dynamic fuels model that explicitly accounts for evolving disturbance regimes, climate variability, and land-use change over decadal timescales. These needs underscore the importance of sustained investment in VIIRS science products within the United States. Incorporating complementary land cover datasets, such as those from the Tropical Moist Forest (Vancutsem et al., 2021) and MapBiomas (Souza et al., 2020; Alencar et al., 2022), also offers substantial potential to improve estimates of deforestation-related fire emissions. While such an approach would not replace GFED5NRT, which is designed for rapid assessment, it would likely yield a more temporally homogeneous dataset better suited for retrospective analyses of long-term trends. We plan to use this framework as the foundation for a future GFED6 assessment, with an emphasis on improving temporal consistency across the full satellite record.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d2e2280">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-18-7535-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/essd-18-7535-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e2291">YC led the project, conceptualized the study, developed the methodology, performed the main data analysis, curated the data, and wrote the original draft of the manuscript. YC, GRvdW, LG, DCM, and JTR contributed to conceptualization, methodology design, data curation (YC, GRvdW, and JTR), and overall project supervision. YC, MM, DvW, JVH, and RV participated in the formal analysis. All authors (YC, GRvdW, MM, DvW, JVH, LG, RV, DCM, LX, TL, RCS, SRC, MBFC, LO, and JTR) contributed to the review and editing of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e2297">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="d2e2303">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><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e2309">This research has been supported by the National Aeronautics and Space Administration (NASA), Fire Sense Technology Program (grant nos. 80NSSC24K1823 and 80NSSC26K0278), the NASA, Fire Sense Implementation Team (grant nos. 80NSSC24K1317 and 80NSSC26K0889), the NASA Modelling, Analysis and Prediction Program (grant no. 80NSSC21K1362),   Interdisciplinary Science (grant no. 80NSSC24K0301),  Carbon Monitoring System Program (grant no. 80NSSC25K7211), and Earth Information System – Fire, the U.S. National Science Foundation (grant no. RISE-2425932), the U.S. Department of Energy, Office of Science, RUBISCO Science Focus Area, and the CALIPSO (Carbon Loss In Plants, Soils and Oceans) project, funded through the generosity of Eric and Wendy Schmidt by recommendation of the Schmidt Science Program.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e2315">This paper was edited by Hanqin Tian and reviewed by Emilio Chuvieco and two anonymous referees.</p>
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