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  <front>
    <journal-meta><journal-id journal-id-type="publisher">BG</journal-id><journal-title-group>
    <journal-title>Biogeosciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">BG</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Biogeosciences</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1726-4189</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/bg-23-5593-2026</article-id><title-group><article-title>Uncertainty in Land Carbon Fluxes Simulated by CMIP6 Models from Treatments of Crop Distributions and Photosynthetic Pathways</article-title><alt-title>Uncertainty in Land Carbon Fluxes Simulated by CMIP6 Models</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Ovwemuvwose</surname><given-names>Joseph</given-names></name>
          <email>j.ovwemuvwose22@imperial.ac.uk</email><email>josovw@gmail.com</email>
        <ext-link>https://orcid.org/0000-0002-6724-059X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Prentice</surname><given-names>Ian Colin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1296-6764</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Graven</surname><given-names>Heather</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Physics, Imperial College London, London, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Georgina Mace Centre for the Living Planet, Department of Life Sciences, Imperial College London, London, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Earth System Science, Tsinghua University, Beijing, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Joseph Ovwemuvwose (j.ovwemuvwose22@imperial.ac.uk, josovw@gmail.com)</corresp></author-notes><pub-date><day>13</day><month>August</month><year>2026</year></pub-date>
      
      <volume>23</volume>
      <issue>15</issue>
      <fpage>5593</fpage><lpage>5605</lpage>
      <history>
        <date date-type="received"><day>4</day><month>August</month><year>2025</year></date>
           <date date-type="rev-request"><day>18</day><month>August</month><year>2025</year></date>
           <date date-type="rev-recd"><day>4</day><month>June</month><year>2026</year></date>
           <date date-type="accepted"><day>22</day><month>June</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Joseph Ovwemuvwose 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://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026.html">This article is available from https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026.html</self-uri><self-uri xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e118">A reliable representation of the diversity of vegetation in terrestrial ecosystems is needed for the accurate simulation of present and future biogeochemical cycling and global climate, particularly as climate change affects different vegetation types differently. We compare the distributions of crops and of C<sub>3</sub> vs. C<sub>4</sub> photosynthetic pathways in both natural vegetation and crops across Earth System Models in the 6th Coupled Model Intercomparison Project (CMIP6). We find a large range in C<sub>3</sub> and C<sub>4</sub> crops, natural and total vegetation for area and gross primary production (GPP) across the models. Even though 10 of the 11 models used Land Use Harmonisation (LUH2) crop areas as input data, modelled total crop area ranges from <inline-formula><mml:math id="M5" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 28 % to <inline-formula><mml:math id="M6" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 10 % of a satellite-based estimate. The C<sub>3</sub> and C<sub>4</sub> crop areas were <inline-formula><mml:math id="M9" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 56 % to <inline-formula><mml:math id="M10" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 15 % and <inline-formula><mml:math id="M11" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 100 % to <inline-formula><mml:math id="M12" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 38 % of LUH2 for 2014, respectively. The C<sub>4</sub> fraction of total vegetation area in the models is 9 %–25 %, compared to 20 % <inline-formula><mml:math id="M14" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % in observation-based estimates for the year 2014. Total global GPP varies by a factor of two across the models, and the C<sub>4</sub> fraction of GPP ranges from 12 % to 27 %. Simulated trends in the fraction of GPP by C<sub>3</sub> vs. C<sub>4</sub> vegetation type (<inline-formula><mml:math id="M18" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula> 20 % to <inline-formula><mml:math id="M19" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 29 %) would have changed global stable carbon isotopic discrimination by <inline-formula><mml:math id="M20" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 0.35 ‰ to <inline-formula><mml:math id="M21" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 0.11 ‰ over 1975–2005, not including changes in discrimination over time within C<sub>3</sub> and C<sub>4</sub> vegetation, indicating that modeled changes in the fraction of GPP by C<sub>3</sub> and C<sub>4</sub> vegetation do not account for the <inline-formula><mml:math id="M26" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 0.7 ‰ increase indicated by atmospheric data. Disparity in vegetation with these photosynthetic pathways in models contributes to uncertainty in land carbon flux simulations, and further constraints and improvements in models are needed.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Schmidt Futures</funding-source>
<award-id>G-21-61881</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e344">The terrestrial biosphere captures <inline-formula><mml:math id="M27" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 % of anthropogenically emitted CO<sub>2</sub> annually (Friedlingstein et al., 2025) reducing CO<sub>2</sub> accumulation in the atmosphere and the accompanying global warming. However, this CO<sub>2</sub> uptake may be sensitive to future climate change (Arora et al., 2020). Understanding the mechanisms contributing to the CO<sub>2</sub> uptake, including the role of different types of vegetation and land use, is essential to understanding potential carbon-climate feedback and future changes to the terrestrial carbon cycle.</p>
      <p id="d2e390">The implementation of land use and land cover change (LUCC) and its impact on vegetation cover and dynamics are important components of terrestrial biosphere model development (Hu et al., 2021; Lam et al., 2021; Hurtt et al., 2020; Wang et al., 2022). LUCC is mainly driven by agriculture. The fraction of global land area used for agriculture increased from 14 % in 1850 to about 37 % in 2015 (Hurtt et al., 2020), and LUCC emitted about 118 PgC between 1850 and 2020 (Houghton and Castanho, 2023). In addition to CO<sub>2</sub> emissions, the biophysical effects of land conversion also drive global temperature rise due to changes in surface albedo (Arora and Boer, 2010; Houghton et al., 2012). The alteration of the land surface will continue to be significant in the future as, for example, it has been projected that 14 % of vegetation and 5 % of soil carbon stocks will be lost to cropland expansion globally over 2010–2050 in a “middle-of-the-road” scenario (Molotoks et al., 2018).</p>
      <p id="d2e402">To represent plant diversity and function, most model developers use plant functional types (PFTs) that group vegetation by similar features such as growth form, ecological requirements, and photosynthetic pathways. This helps to account for the variation in adaptive mechanisms and ecological distribution of different plants (Haxeltine and Prentice, 1996; Hurtt et al., 2020; Wullschleger et al., 2014). One important characteristic of plants is their use of either the C<sub>3</sub> or C<sub>4</sub> photosynthetic pathways. In C<sub>3</sub> plants, the first product of the photosynthetic pathway is a three-carbon molecule called 3-phosphoglycerate (3-PGA), whereas in C<sub>4</sub> plants, it is a four-carbon molecule called oxaloacetate. C<sub>3</sub> and C<sub>4</sub> types also differ in their response to changes in soil moisture content, temperature, CO<sub>2</sub>, and light (Luo et al., 2024). For more information about the anatomical/structural and physiological differences between vegetations with these photosynthetic pathways, which drive their distinct climate and CO<sub>2</sub> concentration responses, see Luo et al. (2024), Cortés et al. (2021), Smith and Boers (2023), Polley et al. (1994), Farquhar et al. (1989), Still et al. (2003), Ehleringer and Björkman (1977).</p>
      <p id="d2e478">Under increasing temperatures, especially those above the thermal optimum threshold, productivity in C<sub>3</sub> vegetation is limited by increased photorespiration (Hermida-Carrera et al., 2016), which reduces photosynthetic efficiency in C<sub>3</sub> plants. In contrast, C<sub>4</sub> species overcome photorespiration through their CO<sub>2</sub> concentrating mechanism that increases the amount of CO<sub>2</sub> at the site of carboxylation (da Silva et al., 2020), leading to an abundance of C<sub>4</sub> species (natural grasses and crops such as maize) in hot areas in the tropics and sub-tropics (Luo et al., 2024). While rising temperature generally favours C<sub>4</sub> plants, rising atmospheric CO<sub>2</sub> concentration confers a physiological advantage upon C<sub>3</sub> species (Polley et al., 1994) due to a reduction in photorespiration and an increase in water use efficiency. This CO<sub>2</sub> fertilisation effect is responsible for the increasing presence of C<sub>3</sub> woody species in previously C<sub>4</sub> dominated grasslands (Luo et al., 2024). Shifts in C<sub>3</sub> and C<sub>4</sub> species composition and carbon fluxes across different regions are projected to continue in future due to changing temperature, water availability and increasing CO<sub>2</sub> concentration in the atmosphere (Cortés et al., 2021; Smith and Boers, 2023; Winslow et al., 2003).</p>
      <p id="d2e619">A change in the relative contributions of C<sub>3</sub> and C<sub>4</sub> vegetation to global productivity may contribute to a global trend in stable photosynthetic carbon isotope discrimination (<inline-formula><mml:math id="M58" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>) because C<sub>3</sub> plants discriminate against carbon-13 more strongly than C<sub>4</sub> plants (Farquhar et al., 1989). Since atmospheric studies have indicated that <inline-formula><mml:math id="M61" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula> increased by 0.7 ‰ over 1975–2005 globally (Keeling et al., 2017), and by 0.4 ‰ over 2000–2011 in the Northern Hemisphere (Peters et al., 2018), understanding the effect of changes in vegetation type on discrimination would help to quantify the environmental and physiological factors influencing plant function and resulting discrimination, including soil moisture content, vapour pressure deficit and stomatal conductance (Cornwell et al., 2018; Griffis et al., 2010; Francey and Farquhar, 1982).</p>
      <p id="d2e673">Currently, the relative contribution and its change over time of C<sub>3</sub> vs. C<sub>4</sub> vegetation to global terrestrial biosphere productivity, and their ecological roles in climate change mitigation, are not well known. Using remote sensing products, physiological modelling, and crop data, Still et al. (2003) found that C<sub>3</sub> and C<sub>4</sub> area abundances are 87.4 and 18.8 million km<sup>2</sup> (17.7 % as C<sub>4</sub>), and C<sub>3</sub> and C<sub>4</sub> gross primary production were 114.7 and 35.3 PgC yr<sup>−1</sup> (23 % as C<sub>4</sub>), respectively, on average for the 1980s and 1990s. More recently, Luo et al. (2024) used global observations of plant photosynthetic pathways, satellite remote sensing, and photosynthetic optimality theory to estimate a similar level of C<sub>4</sub> area coverage (17.5 %), but a lower fraction of gross primary productivity (19.4 %), compared to Still et al. (2003). Luo et al. (2024) showed that C<sub>4</sub> vegetation coverage decreased from 17.7 % to 17.1 % over 2001 to 2019 as natural C<sub>4</sub> grass cover declined in favour of C<sub>3</sub> vegetation, especially C<sub>3</sub> trees in tropical grasslands and savannas. In comparison, across the TRENDY ensemble of dynamic global vegetation models, there were large ranges of 7 %–23 % of vegetation area and 2 %–40 % of productivity from C<sub>4</sub> vegetation (Luo et al., 2024), showing a need for better constraints and understanding of C<sub>3</sub> <inline-formula><mml:math id="M79" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> C<sub>4</sub> vegetation competition and change over time.</p>
      <p id="d2e851">Here we investigate the contribution of vegetation diversity representation to uncertainty in carbon flux simulation in Earth System Models. We evaluate the representation of C<sub>3</sub> and C<sub>4</sub> vegetation over 1850–2014 in 11 Earth System Models used in the 6th Coupled Model Intercomparison project (CMIP6). We assess the distribution, productivity and carbon content of C<sub>3</sub> and C<sub>4</sub> vegetation and compare with observation/satellite-based estimates where possible. We also explore the potential trend in global carbon isotope discrimination <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">Δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C due to C<sub>3</sub> and C<sub>4</sub> vegetation changes simulated in the models.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Materials and Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>CMIP6 Models Outputs and the LUH v2 Data</title>
      <p id="d2e935">To analyze the CMIP6 models, we obtained the output for the following variables from the CMIP6-ESGF repository (<uri>https://esgf-node.ipsl.upmc.fr/search/cmip6-ipsl/</uri>, last access: 28 July 2026): fractions of C<sub>3</sub> and C<sub>4</sub> vegetation coverage (c3PftFrac and c4PftFrac), C<sub>3</sub> and C<sub>4</sub> crop fraction (cropFracC3 and cropFracC4), total crop fraction (cropFrac), gross primary production (gpp), grid cell area (areacella), and percentage of each grid cell covered by land (sftlf). The necessary output was available from 11 models (Table 1). Brief descriptions of the implementation of vegetation abundance in each of the 11 models are provided in the Supplement (section “Materials and Methods S1”).</p>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e980">Summary of each model's definition of crop cover and our calculation of C<sub>3</sub> and C<sub>4</sub> crop cover. More detail is given in SM Materials and Methods.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Earth System</oasis:entry>
         <oasis:entry colname="col2">Resolution:</oasis:entry>
         <oasis:entry colname="col3">Land</oasis:entry>
         <oasis:entry colname="col4">C<sub>3</sub> Crop</oasis:entry>
         <oasis:entry colname="col5">C<sub>4</sub> Crop</oasis:entry>
         <oasis:entry colname="col6">Definition of</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">Lat, Long (°)</oasis:entry>
         <oasis:entry colname="col3">Model</oasis:entry>
         <oasis:entry colname="col4">Fraction</oasis:entry>
         <oasis:entry colname="col5">Fraction</oasis:entry>
         <oasis:entry colname="col6">crop cover</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">ACCESS-ESM1.5</oasis:entry>
         <oasis:entry colname="col2">1.25, 1.875</oasis:entry>
         <oasis:entry colname="col3">CABLE</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">Zero everywhere</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CanESM5</oasis:entry>
         <oasis:entry colname="col2">2.813, 2.813</oasis:entry>
         <oasis:entry colname="col3">CLASS-CTEM</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">cropFracC4</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM2</oasis:entry>
         <oasis:entry colname="col2">0.938, 1.25</oasis:entry>
         <oasis:entry colname="col3">CLM5.0</oasis:entry>
         <oasis:entry colname="col4">cropFrac <inline-formula><mml:math id="M96" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c3PftFrac</oasis:entry>
         <oasis:entry colname="col5">cropFrac <inline-formula><mml:math id="M97" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c4PftFrac</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM2-WACCM</oasis:entry>
         <oasis:entry colname="col2">0.938, 1.25</oasis:entry>
         <oasis:entry colname="col3">CLM5.0</oasis:entry>
         <oasis:entry colname="col4">cropFrac <inline-formula><mml:math id="M98" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c3PftFrac</oasis:entry>
         <oasis:entry colname="col5">cropFrac <inline-formula><mml:math id="M99" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c4PftFrac</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-CM2-SR5</oasis:entry>
         <oasis:entry colname="col2">0.938, 1.25</oasis:entry>
         <oasis:entry colname="col3">CLM4.5</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">Zero everywhere</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMCC-ESM2</oasis:entry>
         <oasis:entry colname="col2">0.938, 1.25</oasis:entry>
         <oasis:entry colname="col3">CLM4.5</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">Zero everywhere</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM6.1</oasis:entry>
         <oasis:entry colname="col2">1.406, 1.406</oasis:entry>
         <oasis:entry colname="col3">ISBA-CTRIP</oasis:entry>
         <oasis:entry colname="col4">cropFrac <inline-formula><mml:math id="M100" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c3PftFrac</oasis:entry>
         <oasis:entry colname="col5">cropFrac <inline-formula><mml:math id="M101" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c4PftFrac</oasis:entry>
         <oasis:entry colname="col6">ECOCLIMAP-II fixed</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-ESM2.1</oasis:entry>
         <oasis:entry colname="col2">1.406, 1.406</oasis:entry>
         <oasis:entry colname="col3">ISBA-CTRIP</oasis:entry>
         <oasis:entry colname="col4">cropFrac <inline-formula><mml:math id="M102" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c3PftFrac</oasis:entry>
         <oasis:entry colname="col5">cropFrac <inline-formula><mml:math id="M103" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c4PftFrac</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-1-2-HAM</oasis:entry>
         <oasis:entry colname="col2">1.875, 1.875</oasis:entry>
         <oasis:entry colname="col3">JSBACH</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">cropFracC4</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM1-2-LR</oasis:entry>
         <oasis:entry colname="col2">1.875, 1.875</oasis:entry>
         <oasis:entry colname="col3">JSBACH</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">cropFracC4</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">UKESM1</oasis:entry>
         <oasis:entry colname="col2">1.25, 1.875</oasis:entry>
         <oasis:entry colname="col3">JULES-TRIFFID</oasis:entry>
         <oasis:entry colname="col4">cropFracC3</oasis:entry>
         <oasis:entry colname="col5">cropFracC4</oasis:entry>
         <oasis:entry colname="col6">LUH2 mapped onto PFTs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">with C<sub>3</sub> <inline-formula><mml:math id="M105" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> C<sub>4</sub> competition</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">from TRIFFID</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d2e1446">To specify crop cover, ten of the eleven CMIP6 models use the Land Use Harmonisation version 2 (LUH2) dataset (Hurtt et al., 2020, Table 1), so we also analyse the LUH2 data directly here. LUH2 estimates the fractional area and transition of use of 12 categories at an annual and 0.25° by 0.25° spatiotemporal resolution, starting from the year 850 (Hurtt et al., 2020). Five of these categories are C<sub>3</sub> annual crops, C<sub>3</sub> perennial crops, C<sub>3</sub> nitrogen-fixing crops, C<sub>4</sub> annual crops and C<sub>4</sub> perennial crops. We group these categories into C<sub>3</sub> crops and C<sub>4</sub> crops, and their sum as total crops.</p>
      <p id="d2e1514">The UKESM1 model uses the LUH2 crop cover data with some modifications, including simulation of competition between C<sub>3</sub> and C<sub>4</sub> vegetation using the dynamic vegetation model TRIFFID (Top-down Representation of Interactive Foliage and Floral Including Dynamics, Sellar et al., 2019, Clark et al., 2011). Other models use the LUH2 data more directly, but differences can result from mapping the LUH2 data onto the model's PFTs, land cover and grid maps.</p>
      <p id="d2e1535">In CNRM-CM6.1, the crop cover is based on the ECOCLIMAP-II database (Voldoire et al., 2019). CNRM-CM6.1 adopts a vegetation cover map that is fixed to its present-day distribution, so that temporal changes in crop area are not included. The reasoning for using a fixed distribution is that the carbon cycle is not fully resolved in the model and there is uncertainty in the impacts of land use and land cover change on carbon flux (Faroux et al., 2013; Voldoire et al., 2019; Gasser et al., 2020).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Global Land Vegetation Cover and Productivity</title>
      <p id="d2e1546">We analysed changes in the vegetation cover (C<sub>3</sub>, C<sub>4</sub> cropland and natural vegetation) for the 11 CMIP6 models by calculating the gridded annual area fraction for C<sub>3</sub> and C<sub>4</sub> vegetation for each year 1850–2014, which we also separated into crops, natural and total vegetation. We also calculated gridded annual gross primary production (GPP) for C<sub>3</sub> and C<sub>4</sub> vegetation in crops, natural and total vegetation in each model. We combined gridded estimates into global totals.</p>
      <p id="d2e1604">We calculated annual maps of the area fraction of C<sub>3</sub> crops (cropFracC3) and C<sub>4</sub> crops (cropFracC4). Most models included the cropFracC3 and cropFracC4 variables that could be used directly (Table 1). Some models had to be treated differently due to the output provided. ACCESS-ESM1.5, CMCC-CM2-SR5, and CMCC-ESM2 did not provide cropFracC4, and their cropFracC3 was equal to the total crop fraction (cropFrac), so we specified the fraction of C<sub>4</sub> crops to be zero everywhere. The CESM2 models did not provide cropFracC3 and cropFracC4 variables, but they did provide c3PftFrac or c4PftFrac (the fractions for total vegetation), so cropFracC3 and cropFracC4 were calculated by multiplying cropFrac by c3PftFrac or c4PftFrac. In CNRM-CM6-1 and CNRM-ESM2.1, the cropFracC3 and cropFracC4 variables were identical to the c3PftFrac and c4PftFrac variables, which appears to be an error in the output. So, in CNRM-CM6-1 and CNRM-ESM2.1, cropFracC3 and cropFracC4 were calculated by multiplying cropFrac by c3PftFrac or c4PftFrac.We also compared the total cropland area in all the models and the LUH2 dataset to a satellite-based estimate from Potapov et al. (2022).</p>
      <p id="d2e1634">To calculate the fractions of natural C<sub>3</sub> and C<sub>4</sub> vegetation, we subtracted cropFracC3 and cropFracC4 from c3PftFrac or c4PftFrac (the total C<sub>3</sub> and C<sub>4</sub> vegetation fractions). Therefore, for each grid cell, we had the fractional area of C<sub>3</sub> and C<sub>4</sub> crops and of C<sub>3</sub> and C<sub>4</sub> natural vegetation.</p>
      <p id="d2e1710">The GPP from C<sub>3</sub> or C<sub>4</sub> vegetation was not provided, so we estimated these by multiplying the total GPP by the area fractions. In Luo et al. (2024), it was found that the per-unit-area photosynthetic rate of C<sub>4</sub> grass was generally higher than that of C<sub>3</sub> vegetation, indicating that these calculations may overestimate the proportion assigned to C<sub>3</sub> vegetation. Therefore, we conducted a reliability analysis to determine the similarity between the values and distribution of C<sub>3</sub> and C<sub>4</sub> crops obtained from cropFrac <inline-formula><mml:math id="M140" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c3PftFrac and cropFrac <inline-formula><mml:math id="M141" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> c4PftFrac in the models (CESM2, CESM2-WACCM, CNRM-ESM2-1 and CNRM-CM6.1) and LUH2 values and distribution using kernel density estimate (KDE) (Silverman, 1986; Chen, 2017) and constructed spatial probability distribution plots using all land pixels for C<sub>3</sub>, C<sub>4</sub> and total crops for the year 2014 (Chiang et al., 2021). We also visually compared the spatial distribution of these values to LUH2 and to UKESM1 and MPI-ESM-1-2-HAM, two models that provided their C<sub>3</sub> and C<sub>4</sub> crops.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Global Stable Carbon Isotopic Discrimination</title>
      <p id="d2e1836">To estimate how the simulated changes in C<sub>3</sub> and C<sub>4</sub> fractions of GPP influenced the global stable carbon isotopic discrimination, we estimated discrimination assuming fixed values for stable carbon isotope discrimination by C<sub>3</sub> and C<sub>4</sub> vegetation. This neglects any environmental or physiological effects on discrimination that may be simulated by the models to isolate the potential effect from changes in C<sub>3</sub> and C<sub>4</sub> fractions of GPP alone. The total annual global stable carbon isotopic discrimination (<inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) was calculated by the following weighted average with GPP:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M153" display="block"><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">GPP</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>+</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">GPP</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">GPP</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>+</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">GPP</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

          Here, GPP<sub>C<sub>3</sub></sub> and GPP<sub>C<sub>4</sub></sub> are the integrated GPP for all C<sub>3</sub> and C<sub>4</sub> vegetation each year, and <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are the fixed stable carbon isotope discrimination for C<sub>3</sub> and C<sub>4</sub>, respectively. We also calculated the global natural stable carbon isotopic discrimination (<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) using the natural C<sub>3</sub> and C<sub>4</sub> GPP for all the models using the same weighted average approach. To calculate the effect of crops on the global annual stable carbon isotope discrimination (<inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">crop</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), we subtracted <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e2161"><inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> were specified as the means of C<sub>3</sub> and C<sub>4</sub> plant leaf stable carbon isotope discrimination observations from the database of 3987 species published by Cornwell et al. (2018), which are 20.7 ‰ for <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and 6.3 ‰ for <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 1). The two peaks in the histogram are assumed to correspond to the highest count for the species with either the C<sub>3</sub> and C<sub>4</sub> photosynthetic pathways. A breakpoint of 12.5 ‰ was chosen for C<sub>3</sub> and C<sub>4</sub> based on the midpoint between the two peaks, such that discrimination values lower than 12.5 ‰ in Fig. 1 are taken to correspond to vegetation with the C<sub>4</sub> photosynthetic pathway while values higher than 12.5 ‰ correspond to stable carbon isotope discrimination in vegetation with the C<sub>3</sub> photosynthetic pathway. The means of these two distributions were calculated and used to specify the fixed C<sub>3</sub> and C<sub>4</sub> discrimination: 20.7 ‰ for <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and 6.3 ‰ for <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

      <fig id="F1"><label>Figure 1</label><caption><p id="d2e2347">Stable carbon isotope discrimination in leaves from the database published by Cornwell et al. (2018).</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f01.png"/>

        </fig>


</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Result</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Crops Spatial Distribution and its Change between 1970 and 2014</title>
      <p id="d2e2374">Based on the LUH2 dataset averaged over 1970–2014, the highest C<sub>3</sub> crop abundance is in agricultural regions in central North America, southwest Europe, southeast and south Asia, Sub-Saharan Africa, southeast South America and southern Australia (Figs. 2 and 3) (Hurtt et al., 2020). The fractional crop area is between 60 % and 100 % in these regions. For C<sub>4</sub> crops, the highest abundance is in the Great Plains in North America, Sub-Saharan Africa, Southwest Asia and Southeast Asia (Fig. 2).</p>
      <p id="d2e2395">The models that do not use LUH2 data directly, UKESM1 (which used LUH2 indirectly) and CNRM-CM6-1, show differences with LUH2 (Figs. 2 and 3). UKESM1 underestimates C<sub>3</sub> crops in Sub-Saharan and central Africa and in Southeast Asia, particularly in India, which is likely due to decreased precipitation in UKESM1 in these areas since the vegetation cover is coupled to its simulated climate (Sellar et al., 2019) and UKESM1 underestimates precipitation in India. UKESM1 estimates more C<sub>4</sub> crop coverage than LUH2, particularly in Asia (Figs. 2 and 3 and Table S1 in the Supplement). Crop coverage in UKESM1 is about 10 % lower than LUH2 between the equator and 30° N (Fig. 3). CNRM-CM6-1 has less C<sub>4</sub> crop cover in Europe and Africa, but more in North and South America, compared to LUH2 (Figs. 2 and 3). For models using LUH2 directly, there was still disagreement between the models and the LUH2 crop coverage, which could be due to a number of reasons, such as preprocessing of the LUH2 vegetation classes into the plant functional types (PFTs) and remapping of the LUH2 data into the spatial resolution needed for each model (Table S1). For the models where we calculated C<sub>3</sub> and C<sub>4</sub> crop cover by multiplying cropFract by C3PftFrac and C4PftFrac, CESM2, CESM2-WACCM, CNRM-ESM2-1 and CNRM-CM6.1, we found that the kernel density estimate (KDE) and visual comparison of the values of C<sub>3</sub> and C<sub>4</sub> crops distribution show they are within the range of values for UKESM1, MPI-ESM-1-2-HAM and LUH2 in terms of magnitude, range and spatial distribution as shown by the spatial distribution, and the overlap area in the percentage cover vs. density plots. For example, the overlap area between LUH2 and CESM2 in C<sub>3</sub> and C<sub>4</sub> crop cover is 0.68 and 0.70, respectively, which is close enough to that between LUH2 and MPI-ESM-1-2-HAM, which is 0.74 and 0.50, respectively (Figs. 3, S7–S13).</p>
      <p id="d2e2480">The models incorporating LUH2 have similar patterns in C<sub>3</sub> and C<sub>4</sub> crop; however, the total area of crops in these models differed from LUH2 by <inline-formula><mml:math id="M197" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 19 % to <inline-formula><mml:math id="M198" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 3 % and from satellite-based estimate by <inline-formula><mml:math id="M199" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 28 % to <inline-formula><mml:math id="M200" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 10 % (Fig. 4, Table S1) from Potapov et al. (2022) study that analysed the change in global cropland area in the first two decades of the twenty-first century using satellite and sample data that estimate crop cover at <inline-formula><mml:math id="M201" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10.9 and <inline-formula><mml:math id="M202" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 11.42 million km<sup>2</sup> respectively between 2003 and 2006. CanESM5 was the most consistent with LUH2. Inconsistencies among the models that use the LUH2 dataset may be due to how the data were pre-processed before incorporation into the model, due to grid spacing or due to differences in the model PFTs compared to LUH2 categories, particularly as some models did not include C<sub>4</sub> crops. Also, because the variables cropFracC3 and cropFracC4 were not available for all models, our crop-fraction calculations may have contributed to the discrepancies. The magnitude of area abundance for C<sub>3</sub> and C<sub>4</sub> crop and natural vegetation for the years 1970 and 2014 are provided in the Supplement (Table S2).</p>
      <p id="d2e2581">Between 1970 and 2014, there were decreases in crop coverage in North America, Europe, Southern Africa, Chile, Japan and New Zealand, but increases in South and Southeast Asia, Africa and South America (Figs. 3b and S1). The largest increases of 10 % or more were concentrated around the eastern region of South America, especially in Brazil, the southern fringes of the Sahara Desert (sub-Saharan Africa) and southeast Africa. The largest decreases of more than 20 % were across the corn belt of the United States and in southwest and central Europe. Changes in crop area in UKESM1 were consistent with LUH2 except in the low latitudes of the Northern Hemisphere, where increases in C<sub>3</sub> crops in Africa and Asia were underestimated, compared to LUH2 (Figs. 3b and S1).</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e2596">Mean percentage of Earth surface covered by crops between 1970 and 2014 for C<sub>3</sub> and C<sub>4</sub> in LUH2, CNRM-CM6.1 and UKESM1-0-LL. Other models not shown use the LUH2 crop variables directly for their crop coverage and change.</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f02.png"/>

        </fig>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e2625">Mean and change in crop coverage averaged over latitude between 1970 and 2014. <bold>(a)</bold> Mean crop coverage <bold>(b)</bold> change in crop coverage.</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Global Temporal Trends in Vegetation Coverage</title>
      <p id="d2e2648">There is a strong positive trend in the area of croplands from 1850 until 2014 (Fig. 4a). Total crop area rose by 200 % in LUH2 and models using LUH2 data. Crop area in UKESM1 was lower than LUH2 but increased in a greater proportion, from 3 to 10 million m<sup>2</sup> (217 %). In CNRM-CM6, the total crop area was fixed at <inline-formula><mml:math id="M211" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14 million km<sup>2</sup>, similar to LUH2 in the 1990s.</p>
      <p id="d2e2676">While representing a smaller fraction of total crop area (10 %–45 %) (Fig. 4a and g), the area of C<sub>4</sub> crops increased in greater proportion (<inline-formula><mml:math id="M214" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 300 %) than C<sub>3</sub> crops (160 %) in the LUH2 data (Fig. 4). Historically, in the CESM2 models, C<sub>3</sub> crop area is lower and C<sub>4</sub> crop area is higher than in LUH2, despite the model using LUH2 data, although this may be affected by our calculation from the variables provided (Table 1). In UKESM1, the C<sub>3</sub> crop area was much smaller than LUH2, while its C<sub>4</sub> crop area was larger (Fig. 4). UKESM1 C<sub>3</sub> crop area peaked between the 1980s and 90s before declining slightly in the 2000s, in contrast to LUH2, where it continued to increase after 2010. UKESM1 C<sub>4</sub> crop area rose through 2014, when it was about 42 % higher than LUH2. CNRM-CM6-1 had a fixed C<sub>4</sub> crop fraction of 24 %, slightly higher than the C<sub>4</sub> crop fraction in LUH2 in the 1990s. ACCESS-ESM1-5, CMCC-ESM2 and CMCC-CM2-SR5 do not have C<sub>4</sub> crops, so their total crop area is equivalent to the C<sub>3</sub> crop area.</p>
      <p id="d2e2796">The area of natural vegetation decreases in all models from 1850 until 1940–1970, when four models (CNRM-ESM2-1, UKESM1, MPI-ESM-1-2-HAM and MPI-ESM1-2-LR) start increasing while the others continue decreasing. Natural vegetation is similarly dominated by C<sub>3</sub>, with 9 %–23 % of natural vegetation as C<sub>4</sub> in 2014, and most of the decline in natural vegetation area is in C<sub>3</sub> vegetation. The trend in natural C<sub>4</sub> vegetation area is inconsistent across the models. In CanESM5 and ACCESS-ESM1-5, the natural C<sub>4</sub> vegetation area decreased over 1850–2014, while for MPI-ESM-1-2-HAM and MPI-ESM1-2-LR the natural C<sub>4</sub> vegetation area increased especially from 1990. For the CESM2, CMCC-ESM2 and CMCC-CM2-SR5 , the natural C<sub>4</sub> vegetation area was constant until the early 2000s before falling slightly. The UKESM1 estimate of the area of natural C<sub>4</sub> vegetation for 2000–2014 compares well with Luo et al. (2024)'s, while other models simulate up to 15 % larger and up to 63 % smaller areas (Fig. 4h).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2875">Global temporal trends in vegetation area from 1850 to 2014 in CMIP6 models. Trend of the area covered by <bold>(a)</bold> total crop, <bold>(b)</bold> total natural vegetation <bold>(c)</bold> total global vegetation, <bold>(d)</bold> C<sub>3</sub> crops, <bold>(e)</bold> C<sub>3</sub> natural vegetation, <bold>(f)</bold> total C<sub>3</sub> vegetation, <bold>(g)</bold> C<sub>4</sub> crop, <bold>(h)</bold> C<sub>4</sub> natural vegetation and <bold>(i)</bold> total C<sub>4</sub> vegetation. All models except CNRM-CM6-1 used LUH2 data to inform their crop coverage. ACCESS-ESM1-5, CMCC-ESM2 and CMCC-CM2-SR5 do not have C<sub>4</sub> crops.</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f04.png"/>

        </fig>

      <p id="d2e2976">For the total vegetation area, four models have distinct positive trends from the late 1960s through to 2014 (CNRM-ESM2.1, UKESM1, MPI-ESM-1-2-HAM and MPI-ESM1-2-LR) (Fig. 4c), driven mostly by an increase in C<sub>4</sub> natural vegetation (Fig. 4h). In the other models, the increase in crop area is balanced by the decrease in area covered by natural vegetation. The estimated total vegetated area from the European Space Agency Climate Change Initiative (ESA-CCI) for 2000–2014 is matched by the CMCC-ESM2 and CMCC-CM2-SR5, while the CESM2 models simulate larger vegetated areas and all other models simulate smaller vegetated areas. The ESA CCI data shows a small increase that may be caused by the replacement of bare ground by natural grasses (Fig. S2).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Global Trends in Gross Primary Production</title>
      <p id="d2e2996">While all the models simulate an increase in GPP, the magnitude and contribution by vegetation types (in this context: crop/natural and C<sub>3</sub> <inline-formula><mml:math id="M243" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> C<sub>4</sub>) differ (Fig. 5). The models disagree on the magnitude of total global GPP, ranging from 80 PgC yr<sup>−1</sup> in CNRM- ESM2.1 to 150 PgC yr<sup>−1</sup> in MPI-ESM-1-2-HAM and MPI-ESM1-2-LR (<inline-formula><mml:math id="M247" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula> 20 % to <inline-formula><mml:math id="M248" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 29 %) in 2014 (Gier et al., 2024; Arora et al., 2020) (Fig 5c). The total GPP for all the models increased steadily until the 1960s and then grew sharply for the rest of the historical period (Fig. 5c).</p>
      <p id="d2e3063">The increase in GPP in crops is linked to the cropland expansion, while the GPP change in natural vegetation is decoupled from the change in area (Figs. S5 and S6). In Fig. 4a, the total crop area increased by 200 % compared to Fig. 4b, in which natural vegetation decreased by 7 % on average. Comparing this change in area to the change in GPP in Fig. 5a and b, total crop GPP increased by 209 % on average. However, for CNRM-CM6.1 with a temporally fixed vegetation cover, the increase in total crop GPP is only 18 %. For natural vegetation, even though there is a mean 7 % decrease in total natural vegetation cover, there is an <inline-formula><mml:math id="M249" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 18 % increase in GPP on average. In CNRM-CM6-1 with a fixed vegetation cover, the trend of C<sub>3</sub>, C<sub>4</sub> and total crop GPP is not as strong compared to other models, especially before 1970 (Fig. 5a, d and g). They increased by 32 %, 27 %, and 18 % for C<sub>3</sub>, C<sub>4</sub> and total crop GPP, respectively, compared to the ensemble mean increase of 195 %, 251 % and 209 %, respectively (Fig. 5a, d and g).</p>
      <p id="d2e3109">For GPP in natural vegetation, there are large ranges of 63–107 PgC yr<sup>−1</sup> simulated for C<sub>3</sub> vegetation and 9–23 PgC yr<sup>−1</sup> simulated for C<sub>4</sub> vegetation across the models before 1970 (Fig. 5e and h). Despite the decrease in natural C<sub>3</sub> vegetation area before 1970, the C<sub>3</sub> GPP trend is generally either weakly negative or unchanging until 1970 (Fig. 5e). Then all models increase steadily over 1970–2014. In natural C<sub>4</sub> vegetation, there is generally an increase in GPP since 1850, but the increase is not at the same rate in all the models. It is weaker in ACCESS-ESM1-5, CanESM5 and UKESM1 (Fig. 5h). Natural C<sub>4</sub> GPP decreased and remained relatively constant in ACCESS-ESM1-5 and CESM2 models, respectively, over 2000–2014.</p>
      <p id="d2e3191">The proportion of total GPP by C<sub>4</sub> vegetation in the models is 12 %–27 % (Fig. 5i), compared to 23 % in Still et al. (2003) and 20 <inline-formula><mml:math id="M263" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % in Luo et al. (2024). Compared to other model simulations, the range was 2 %–40 % in TRENDY models (Luo et al., 2024), and 18 %–27 % in previous modelling studies (Farquhar and Lloyd, 1993; Fung et al., 1997).</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e3213">Temporal trend in gross primary production (GPP) between 1850 and 2014. Trend of GPP of <bold>(a)</bold> total crop, <bold>(b)</bold> total natural vegetation <bold>(c)</bold> total global vegetation, <bold>(d)</bold> C<sub>3</sub> crops, <bold>(e)</bold> C<sub>3</sub> natural vegetation, <bold>(f)</bold> total C<sub>3</sub> vegetation, <bold>(g)</bold> C<sub>4</sub> crop, <bold>(h)</bold> C<sub>4</sub> natural vegetation and <bold>(i)</bold> total C<sub>4</sub> vegetation.</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Global Trends in Stable Carbon Isotope Discrimination</title>
      <p id="d2e3313">The models disagree on the magnitude and trend of <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">crop</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Fig. 6), for our calculation of discrimination based only on the fraction of GPP from C<sub>3</sub> and C<sub>4</sub> vegetation, neglecting any physiological or environmental effects Eq. (1). As a result of the 12 %–27 % range in C<sub>4</sub> fraction of total GPP, the global total stable carbon discrimination ranges from 16.9 ‰ to 19.5 ‰ (Table S2) in 2014 across the models, compared to 16.5 ‰ in Still et al. (2003). Models simulate no change (CESM2 models), slightly increasing <inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (ACCESS-ESM1.5 and CNRM-CM6.1) or decreasing <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (all other models). The strongest decreases in <inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> were in MPI-ESM-1-2-HAM and MPI-ESM1-2-LR, which had the strongest increases in C<sub>4</sub> vegetation area (Fig. 6). Compared to the strong positive trend in the global stable carbon isotope discrimination trend derived by Keeling et al. (2017) from atmospheric <inline-formula><mml:math id="M280" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C data, the effect of vegetation change in the models was much smaller or had the opposite sign (Fig. 6).</p>
      <p id="d2e3430">The models also disagree on the sign and magnitude of the trends in change in <inline-formula><mml:math id="M281" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M282" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula> 0.83 ‰ to 1.7 ‰) and <inline-formula><mml:math id="M283" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">crop</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M284" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula> 0.5 ‰ to 0.2 ‰ , Table S2). Among models with decreasing <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the trend is primarily driven by growth in the productivity of C<sub>4</sub> natural vegetation, affecting <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in MPI-ESM-1-2-HAM and MPI-ESM1-2-LR, but by growth in the productivity of C<sub>4</sub> Crops, affecting <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">crop</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the UKESM1 and CanESM5 models (Fig. 6).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e3523">Trend of global stable carbon isotope discrimination between 1850 and 2014. 10 year average stable carbon isotope discrimination of <bold>(a)</bold> total vegetation (<inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(b)</bold> difference in <inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">tot</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from 1850, <bold>(c)</bold> component of difference due to natural vegetation (<inline-formula><mml:math id="M292" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">nat</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and <bold>(d)</bold> due to crops (<inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">crop</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>).</p></caption>
          <graphic xlink:href="https://bg.copernicus.org/articles/23/5593/2026/bg-23-5593-2026-f06.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d2e3598">By examining the components of global vegetation area and GPP by vegetation types, we find that CMIP6 models span a large range for nearly all variables. Some models showed stronger gains in GPP in natural C<sub>3</sub> vegetation, while for others the strongest gains were in either crop or natural C<sub>4</sub> vegetation. Therefore, better quantification of vegetation types and more consistency in models would improve future carbon modelling. For example, total vegetated areas in some models that are much lower than the ESA-CCI estimate (Harper et al., 2023) and total C<sub>4</sub> vegetated areas in some models that are much lower than the Luo et al. (2024) estimate can probably be ruled out. Additionally, Zhao et al. (2025) show that the uncertainty in the terrestrial biosphere GPP simulation in models depends strongly on the area of each PFTs and this dependence enabled them to reduce the spread in land carbon estimates by <inline-formula><mml:math id="M297" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 75 %. They also found that changes in PFTs distribution is responsible for 56 % <inline-formula><mml:math id="M298" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21 % climate-induced variability in dynamic global vegetation models (DGVMs) GPP. This spread across models in many cases reflects the lack of observational constraints and may also be linked to the discrepancies in the natural vegetation composition in the context of our study.</p>
      <p id="d2e3642">Even though nearly all the models use LUH2 as input data, their crop areas and, in particular, their attribution to C<sub>3</sub> and C<sub>4</sub> vegetation are not consistent. While most models underestimated total crop area compared to LUH2 (Fig. 4a), another satellite-based cropland map (Potapov et al., 2022) estimates a lower crop area that overlaps some of the CMIP6 models' crop areas. Therefore, the spread in crop area across the models may reflect uncertainty in their input crop-area data. A limitation of some current models is that they do not include C<sub>4</sub> crops; thus, carbon fluxes associated with C<sub>4</sub> crops cannot be simulated in those models. In the future, the total crop area is likely to increase (Molotoks et al., 2018; O'Neill et al., 2016), so agriculture will exert an even stronger influence on carbon fluxes.</p>
      <p id="d2e3681">The range in global GPP was even larger than the range in vegetated area across the models, both for total (GPP: <inline-formula><mml:math id="M303" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 23 % to <inline-formula><mml:math id="M304" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 37 % vs. area: <inline-formula><mml:math id="M305" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 11 % to <inline-formula><mml:math id="M306" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 8 %, compared to the model mean) and for C<sub>3</sub> (GPP: <inline-formula><mml:math id="M308" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 24 % to <inline-formula><mml:math id="M309" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 32 % vs. area: <inline-formula><mml:math id="M310" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 19% to <inline-formula><mml:math id="M311" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 8 %) vegetation types. In C<sub>4</sub> natural vegetation, there was also disagreement over the sign of the GPP trend, with some models showing increases in GPP in grid cells dominated by C<sub>4</sub> (<inline-formula><mml:math id="M314" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 75 %; Fig. S3; a–d), and others showing decreases. These inconsistencies indicate that models' parametrisations, simulated climate and other factors (Campbell et al., 2017; Hou et al., 2022; Lavergne et al., 2022; Zscheischler et al., 2014) are at least as important as vegetation area for GPP simulation. Therefore, achieving consistency in the area for vegetation types is not sufficient, and an improved understanding and representation of C<sub>3</sub> and C<sub>4</sub> GPP in models are needed.</p>
      <p id="d2e3794">The range in total area fraction of C<sub>4</sub> vegetation of 10 %–26 % in the CMIP6 models spans the observation-based estimates of 17.1 %–17.7 % (Still et al., 2003; Luo et al., 2024) and has a similar range as the dynamic global vegetation models in the TRENDY project (7 %–23 %; Luo et al., 2024). Since the observation-based estimates are quite consistent, model simulations of carbon fluxes can likely be improved by detailed comparison and specification of C<sub>4</sub> vegetation cover in particular PFTs within models to better align them with observational estimates.</p>
      <p id="d2e3816">The trends in C<sub>3</sub> vs. C<sub>4</sub> contributions to GPP simulated by CMIP6 models produced differing trends in stable carbon isotopic discrimination when only C<sub>3</sub> and C<sub>4</sub> fractions of GPP are used to calculate discrimination trends Eq. (1) (Fig. 6). The simulated changes in C<sub>3</sub> and C<sub>4</sub> fractions of GPP did not produce strong increasing trends as found by analysis of atmospheric <inline-formula><mml:math id="M325" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C data (Keeling et al., 2017; Peters et al., 2018). Since the effect of changing C<sub>3</sub> and C<sub>4</sub> fractions of GPP on stable carbon isotopic discrimination varied widely across the CMIP6 models, it is still uncertain how much they could add to or oppose changes in stable carbon isotopic discrimination caused by environmental or physiological effects. Nevertheless, Lavergne et al. (2026) found that accounting for the changes in C<sub>3</sub> and C<sub>4</sub> vegetation abundance improves the modelled trends in atmospheric carbon isotope composition compared to the data. In particular, since the GPP trend in the models (11 % to 18 %, Fig. S4) is weaker than the CO<sub>2</sub> fertilisation effect over the 20th century based on carbonyl sulphide data (<inline-formula><mml:math id="M331" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula> 30 %; Campbell et al., 2017), there may have been a more positive C<sub>3</sub> vegetation-driven trend in stable carbon isotopic discrimination in reality than in the models. Since the CMIP6 models did not provide output for GPP for C<sub>3</sub> and C<sub>4</sub> vegetation or for crops and natural vegetation, we had to scale total GPP by the area fractions of each vegetation type for grid cells with mixed vegetation. This calculation may not represent the models' actual attribution precisely, since C<sub>4</sub> vegetation can have higher GPP relative to area (Luo et al., 2024) in grid cells with a mosaic of C<sub>3</sub> and C<sub>4</sub>. However, the extra resources needed in the C<sub>4</sub> photosynthetic pathway (Ehleringer, 1978) to concentrate CO<sub>2</sub> may make the difference between C<sub>3</sub> and C<sub>4</sub> CO<sub>2</sub> uptake minimal, especially if they co-occur relatively equally in such grid cells. Incorporating more detailed vegetation information from the models would improve the accuracy of the calculations, and analysis based on TRENDY models could be a good place to start.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d2e4048">We analysed changes in vegetation with C<sub>3</sub> and C<sub>4</sub> photosynthetic pathways for natural vegetation and crops in 11 CMIP6 models over the historical period of 1850 to 2014. Except for one model that used a fixed vegetation distribution, the models include the expansion of agriculture using LUH2 data. Still, there is a significant variation in the fraction of area and GPP allocated to crops in these models, and the UKESM1 model strongly underestimated crops in Asia and Africa, likely due to biases in simulated climate. The C<sub>4</sub> fraction of vegetated area has remained relatively constant in the models, though there is a large range in simulated C<sub>4</sub> area fraction of 10 % to 26 % in 2014, while observation-based estimates are quite consistent at 17.1 %–17.7 % from the 1980s to 1990s and between 2001 and 2019 (Luo et al., 2024; Still et al., 2003). Overall, the total vegetation area in most models is not changing, but the global vegetation composition is changing in favour of crops. Whereas all the models agree that C<sub>3</sub> vegetation GPP and total global GPP are increasing, the magnitude of the increase spans a wide range. In C<sub>4</sub> vegetation, the models disagree on the magnitude of GPP and the sign of its trend, especially in natural vegetation, implying that our understanding of and model parametrisations for the simulation of C<sub>4</sub> GPP need improvement. The strong positive trends in UKESM1 C<sub>4</sub> crop and MPI-ESM-1-2-HAM and MPI-ESM1-2-LR C<sub>4</sub> natural vegetation area clearly drive the decline in their global stable carbon isotopic discrimination trend, an effect that is not as pronounced in other models' vegetation categories. However, due to the large uncertainty in vegetation area abundance and GPP, it will be difficult to determine if this effect of change in vegetation area abundance and GPP on the global stable carbon isotopic discrimination trend is consistent across all the models. We have shown in this study that carbon flux simulations in current ESMs include uncertainties in the C<sub>3</sub> and C<sub>4</sub> photosynthetic pathways in crops and natural vegetation; reducing these uncertainties will require stronger observational constraints and more robust and realistic model parameterisations.</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d2e4155">The code (Jupyter notebooks) used for the analysis of the CMIP6 models data and for the data visualization can be found in the following Github repository: <uri>https://github.com/jovwemuvwose/CMIP6_Model_Analysis_Project_2025_version2</uri> (last access: 28 July 2026) and Zenodo at <ext-link xlink:href="https://doi.org/10.5281/zenodo.16883407" ext-link-type="DOI">10.5281/zenodo.16883407</ext-link> (Ovwemuvwose, 2025).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e4167">The CMIP6 models data used in the are available at the World Climate Research Programme (WCRP) Coupled Model Intercomparison Project (Phase 6) website: <uri>https://esgf-node.ipsl.upmc.fr/projects/cmip6-ipsl/</uri> (last access: 28 July 2026). The leaf carbon isotope data by Cornwell et al. (2018) are available at <ext-link xlink:href="https://doi.org/10.1111/geb.12764" ext-link-type="DOI">10.1111/geb.12764</ext-link>. For the ESA CCI, LUH2, Still, Potapov and Luo data used in Fig. 4, see <ext-link xlink:href="https://doi.org/10.5194/ESSD-15-1465-2023" ext-link-type="DOI">10.5194/ESSD-15-1465-2023</ext-link> (Harper et al., 2023), <ext-link xlink:href="https://doi.org/10.5194/gmd-13-5425-2020" ext-link-type="DOI">10.5194/gmd-13-5425-2020</ext-link> (Hurtt et al., 2020), <ext-link xlink:href="https://doi.org/10.1029/2001GB001807" ext-link-type="DOI">10.1029/2001GB001807</ext-link> (Still et al., 2003), <ext-link xlink:href="https://doi.org/10.1038/s43016-021-00429-z" ext-link-type="DOI">10.1038/s43016-021-00429-z</ext-link> (Potapov et al., 2022) and <ext-link xlink:href="https://doi.org/10.1038/s41467-024-45606-3" ext-link-type="DOI">10.1038/s41467-024-45606-3</ext-link> (Luo et al., 2024) respectively. For the Keeling_vsCO2, Keeling_vstime used in Fig. 7 see <ext-link xlink:href="https://doi.org/10.1073/pnas.1619240114" ext-link-type="DOI">10.1073/pnas.1619240114</ext-link> (Keeling et al., 2017). The processed data used for the figures can be made available by the authors on request.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e4195">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/bg-23-5593-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/bg-23-5593-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e4204">JO and HG conceptualize the overarching research and CIP contributed to broadening it; JO prepared and created the published work, specifically data analysis and visualization and writing of the initial draft of the manuscript. HG and CIP reviewed and edited the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e4210">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="d2e4216">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e4222">This project is supported by Schmidt Sciences, LLC.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e4227">This research has been supported by the Schmidt Futures (grant no. G-21-61881).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e4233">This paper was edited by Benjamin Stocker and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

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