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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Research article}?>
  <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-19-1777-2022</article-id><title-group><article-title>A convolutional neural network for spatial downscaling of satellite-based solar-induced chlorophyll fluorescence (SIFnet)</article-title><alt-title>SIFnet downscaling</alt-title>
      </title-group><?xmltex \runningtitle{SIFnet downscaling}?><?xmltex \runningauthor{J. Gensheimer et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Gensheimer</surname><given-names>Johannes</given-names></name>
          <email>johannes.gensheimer@bgc-jena.mpg.de</email>
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff3">
          <name><surname>Turner</surname><given-names>Alexander J.</given-names></name>
          <email>turneraj@uw.edu</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Köhler</surname><given-names>Philipp</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7820-1318</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Frankenberg</surname><given-names>Christian</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0546-5857</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Chen</surname><given-names>Jia</given-names></name>
          <email>jia.chen@tum.de</email>
        <ext-link>https://orcid.org/0000-0002-6350-6610</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Environmental Sensing and Modeling, Technical University of Munich (TUM), Munich, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Biogeochemical Integration, Max Planck Institute for Biogeochemistry, 07745 Jena, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Atmospheric Sciences, University of Washington, Seattle, WA, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Johannes Gensheimer (johannes.gensheimer@bgc-jena.mpg.de), Jia Chen (jia.chen@tum.de), and Alexander J. Turner (turneraj@uw.edu)</corresp></author-notes><pub-date><day>31</day><month>March</month><year>2022</year></pub-date>
      
      <volume>19</volume>
      <issue>6</issue>
      <fpage>1777</fpage><lpage>1793</lpage>
      <history>
        <date date-type="received"><day>20</day><month>December</month><year>2021</year></date>
           <date date-type="rev-request"><day>22</day><month>December</month><year>2021</year></date>
           <date date-type="rev-recd"><day>1</day><month>March</month><year>2022</year></date>
           <date date-type="accepted"><day>1</day><month>March</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 Johannes Gensheimer et al.</copyright-statement>
        <copyright-year>2022</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/19/1777/2022/bg-19-1777-2022.html">This article is available from https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022.html</self-uri><self-uri xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e143">Gross primary productivity (GPP) is the sum of leaf photosynthesis and represents a crucial component of the global carbon cycle. Space-borne estimates of GPP typically rely on observable quantities that co-vary with GPP such as vegetation indices using reflectance measurements (e.g., normalized difference vegetation index, NDVI, near-infrared reflectance of terrestrial vegetation, NIR<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>, and kernel normalized difference vegetation index, kNDVI). Recent work has also utilized measurements of solar-induced chlorophyll fluorescence (SIF) as a proxy for GPP.  However, these SIF measurements are typically coarse resolution, while many processes influencing GPP occur at fine spatial scales. Here, we develop a convolutional neural network (CNN), named SIFnet, that increases the resolution of SIF from the TROPOspheric Monitoring Instrument (TROPOMI) on board of the satellite Sentinel-5P by a factor of 10 to a spatial resolution of 500 m. SIFnet utilizes coarse SIF observations together with high-resolution auxiliary data.  The auxiliary data used here may carry information related to GPP and SIF. We use training data from non-US regions between April 2018 until March 2021 and evaluate our CNN over the conterminous United States (CONUS). We show that SIFnet is able to increase the resolution of TROPOMI SIF by a factor of 10 with a <inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and RMSE metrics of 0.92 and 0.17 mW m<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> sr<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> nm<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, respectively. We further compare SIFnet against a recently developed downscaling approach and evaluate both methods against independent SIF measurements from Orbiting Carbon Observatory 2 and 3 (together OCO-2/3). SIFnet performs systematically better than the downscaling approach (<inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.78</mml:mn></mml:mrow></mml:math></inline-formula> for SIFnet, <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.72</mml:mn></mml:mrow></mml:math></inline-formula> for downscaling), indicating that it is picking up on key features related to SIF and GPP. Examination of the feature importance in the neural network indicates a few key parameters and the spatial regions in which these parameters matter.  Namely, the CNN finds low-resolution SIF data to be the most significant parameter with the NIR<inline-formula><mml:math id="M8" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> vegetation index as the second most important parameter.  NIR<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> consistently outperforms the recently proposed kNDVI vegetation index.  Advantages and limitations of SIFnet are investigated and presented through a series of case studies across the United States. SIFnet represents a robust method to infer continuous, high-spatial-resolution SIF data.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e254">Photosynthesis represents the single largest CO<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> flux between the atmosphere and the biosphere.  At the canopy level, the sum of all leaf photosynthesis is termed gross primary productivity (GPP), and accurate characterization of GPP represents a major uncertainty in the carbon cycle <xref ref-type="bibr" rid="bib1.bibx18" id="paren.1"/>. Directly measuring GPP from remote sensing systems (e.g., satellites) is not presently possible. Instead, previous work has utilized stationary measurements of net ecosystem exchange (NEE) from flux towers that can be decomposed into GPP and respiration <xref ref-type="bibr" rid="bib1.bibx43" id="paren.2"><named-content content-type="pre">e.g.,</named-content></xref>. Observable quantities from satellites (e.g., vegetation indices computed from reflectance data) are then related to GPP inferred from flux towers <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx31 bib1.bibx50 bib1.bibx58" id="paren.3"><named-content content-type="pre">e.g.,</named-content></xref> in light use efficiency (LUE) <xref ref-type="bibr" rid="bib1.bibx37" id="paren.4"/> or machine learning models <xref ref-type="bibr" rid="bib1.bibx31" id="paren.5"/> to derive global estimates of GPP.</p>
      <p id="d1e286">Vegetation indices such as the normalized difference vegetation index  (NDVI) and near-infrared reflectance of terrestrial vegetation (NIR<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>) combine two (or more) spectral bands with different absorption characteristics <xref ref-type="bibr" rid="bib1.bibx25" id="paren.6"/> to infer quantities related to plant physiology and canopy structure.  The MODIS instrument was launched on the Terra and Aqua satellites in 1999 and 2002, respectively.  This instrument has proved particularly useful due, in part, to the long operational lifetime, and vegetation indices can be derived from the individual reflectance bands of MODIS. More recently launched satellites, like Sentinel-5P, carry instruments with the necessary signal-to-noise ratio and spectral resolution to retrieve solar-induced chlorophyll fluorescence (SIF).  The electromagnetic signal SIF is emitted by chlorophylls during photosynthesis. SIF is emitted in the red–far-red wavelengths of 650–850 nm <xref ref-type="bibr" rid="bib1.bibx36" id="paren.7"/>. It is a way, besides photochemistry and nonphotochemical quenching, for de-excitement of the chlorophylls <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx32" id="paren.8"/>. Even though the link between chlorophyll fluorescence and photosynthesis is nonlinear at leaf and canopy scale, that does not hold for satellite scales, in which a linear relationship of SIF to GPP is frequently reported <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx36 bib1.bibx17 bib1.bibx29" id="paren.9"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p id="d1e312">Vegetation indices (also termed greenness) can be regarded as a measure of photosynthetic capacity <xref ref-type="bibr" rid="bib1.bibx46" id="paren.10"/>, whereas SIF indicates photosynthetic activity. SIF has been shown to be a powerful proxy for estimating GPP <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx54" id="paren.11"/>, to capture the impact of drought on photosynthetic activities across different vegetation types <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx9" id="paren.12"/>, and to assess the regional source of carbon emissions <xref ref-type="bibr" rid="bib1.bibx48" id="paren.13"/>.</p>
      <p id="d1e327"><xref ref-type="bibr" rid="bib1.bibx32" id="text.14"/> described the first retrievals of SIF from the TROPOspheric Monitoring Instrument (TROPOMI), the sole instrument on the Sentinel-5P satellite.  The TROPOMI instrument has an equatorial crossing time of 13:30 local solar time and a 16 d orbit cycle. TROPOMI has a wide swath (2600 km across track) that allows for near-daily temporal resolution and a spatial resolution of 5.5 <inline-formula><mml:math id="M12" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 3.5 km. This was a substantial improvement to previous satellite instruments measuring SIF that were limited to 40 <inline-formula><mml:math id="M13" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 40 km spatial resolution <xref ref-type="bibr" rid="bib1.bibx30" id="paren.15"/>.  Despite the higher spatial resolution of TROPOMI, there have been efforts to estimate SIF at finer spatial scales <xref ref-type="bibr" rid="bib1.bibx53" id="paren.16"><named-content content-type="pre">e.g.,</named-content></xref>. This is motivated by the importance of fine-scale phenomena in the carbon cycle such as ecosystem fragmentation <xref ref-type="bibr" rid="bib1.bibx24" id="paren.17"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p id="d1e360">Globally, 20 % and 70 % of the remaining forests are within a distance of 100 m and 1 km, respectively, from the forest edges, meaning that most of the forests are fragmented <xref ref-type="bibr" rid="bib1.bibx24" id="paren.18"/>. <xref ref-type="bibr" rid="bib1.bibx44" id="text.19"/> show that the carbon uptake and storage of trees near the forest edge increase up to 13 <inline-formula><mml:math id="M14" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % and 10 <inline-formula><mml:math id="M15" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1 %, respectively. On the other hand most of our understanding about forest carbon fluxes comes from intact ecosystems, resulting in a mismatch between the ecosystems we are trying to quantify and the data we are using to do so <xref ref-type="bibr" rid="bib1.bibx51" id="paren.20"/>. Higher-resolution estimates of photosynthetic activity might enable us to include fragmentation effects of ecosystems to global carbon cycle estimates or biosphere models like <xref ref-type="bibr" rid="bib1.bibx31" id="text.21"/>, <xref ref-type="bibr" rid="bib1.bibx56" id="text.22"/>, and <xref ref-type="bibr" rid="bib1.bibx54" id="text.23"/>. Additionally, recent work has shown the importance of fine-scale variations in the urban biosphere on the overall carbon flux for a city <xref ref-type="bibr" rid="bib1.bibx38" id="paren.24"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p id="d1e401">There has been some recent work with the goal of increasing the resolution of existing global SIF estimates through downscaling methods (i.e., physics-based methods). For example, <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx54" id="text.25"/> used NIR<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> to partition SIF within a particular TROPOMI scene and oversampled it using a 16 d window afterwards, resulting in a daily 500 m SIF estimate over the conterminous United States (CONUS). <xref ref-type="bibr" rid="bib1.bibx14" id="text.26"/> downscaled GOME-2 satellite SIF from 0.5 to 0.05<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> using a parameterization with a term for the fraction of absorbed photosynthetically active radiation (fAPAR), one for water stress, and one for heat stress based on MODIS data. <xref ref-type="bibr" rid="bib1.bibx49" id="text.27"/> used airborne data to downscale far-red SIF from canopy to leaf level.</p>
      <p id="d1e431">Machine learning has also been used to create global, high-resolution SIF data sets. <xref ref-type="bibr" rid="bib1.bibx33" id="text.28"/>, <xref ref-type="bibr" rid="bib1.bibx57" id="text.29"/>, and <xref ref-type="bibr" rid="bib1.bibx59" id="text.30"/> used spectral bands from MODIS as input to neural networks that were trained with Orbiting Carbon Observatory 2 (OCO-2) SIF data to build global continuous SIF products at 0.05<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution. OCO-2 has a narrow swath, and, therefore, the networks are trained only in the regions where OCO-2 SIF is available by using MODIS data as input. After training, the global MODIS data are used as input to estimate SIF on a global scale. <xref ref-type="bibr" rid="bib1.bibx20" id="text.31"/> use MODIS reflectance data as input and predict GOME-2 normalized by clear-sky irradiance. Multiplying that with a MODIS-derived photosynthetic active radiation product results in a MODIS only estimated SIF, termed RSIF. <xref ref-type="bibr" rid="bib1.bibx60" id="text.32"/> trained a convolutional neural network (CNN) with MODIS data on the artificial GOSIF data set <xref ref-type="bibr" rid="bib1.bibx33" id="paren.33"/> at a resolution of 0.05<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and used the trained network and MODIS data at a resolution of 0.008<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> to estimate SIF at 0.008<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The physics-based downscaling approach from <xref ref-type="bibr" rid="bib1.bibx53" id="text.34"/> can only consider one variable for weighting the SIF signal, while the machine-learning-based approaches in the literature can consider more than one variable – but many do not use SIF data as an input to their model, meaning that they estimate SIF based on reflectance data.</p>
      <p id="d1e492">Here we build a convolutional neural network to obtain high-resolution SIF, named SIFnet.  SIFnet increases the spatial resolution of TROPOMI SIF by considering coarse-resolution SIF with high-resolution auxiliary data as input. These auxiliary data consist of either proxies of SIF or photosynthetic drivers. SIFnet is trained using data with near-global coverage.  Different model parameters (structure, input features, and scaling factors) are compared and evaluated. After training the model, the resolution of TROPOMI SIF is refined by a factor of 10 to a spatial resolution of 0.005<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. This product is then compared against a recent downscaling method from the literature <xref ref-type="bibr" rid="bib1.bibx53" id="paren.35"/>. Both high-resolution estimates are validated over CONUS against the independent SIF measurements of the OCO-2 and OCO-3 instruments (together OCO-2/3) <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx41" id="paren.36"/>.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data sets</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data sources</title>
      <p id="d1e525">The input data to the neural network are listed in Table <xref ref-type="table" rid="Ch1.T1"/>. These diverse global data products are expected to capture a broad range of photosynthetic drivers. The table divides the data into time-varying or time-invariant and training or validation data. The native spatial resolution is shown in the last column of Table <xref ref-type="table" rid="Ch1.T1"/>. In a first step, all data sets are aggregated to 0.05<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial resolution and 16 d time steps. In the case of a higher native spatial resolution, the data are regridded by computing the mean value that falls into the coarse-resolution grid cell. In the case of coarser resolutions than 0.05<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, it is resampled to the common grid.  Quality control flags and cloud filtering are applied when necessary.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e553">Data sets used in this work. ENF: evergreen needleleaf forest;
EBF: evergreen broadleaf forest; DNF: deciduous needleleaf forest; DBF: deciduous broadleaf forest; MF: mixed forest; UF: unknown forest.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="center"/>
     <oasis:colspec colnum="6" colname="col6" align="center"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col3">Data </oasis:entry>
         <oasis:entry colname="col4">Time</oasis:entry>
         <oasis:entry colname="col5">Training</oasis:entry>
         <oasis:entry colname="col6">Validation</oasis:entry>
         <oasis:entry colname="col7">Spatial</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">invariant</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">resolution</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">Sentinel-5P TROPOMI<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">SIF at 740 nm</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M36" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">0.05<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MODIS</oasis:entry>
         <oasis:entry colname="col2">MODIS bands</oasis:entry>
         <oasis:entry colname="col3">NIR, red, blue,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M38" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">500 m</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MCD43A4.v006</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">green, SWIR1,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">(v06)<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col2"/>
         <oasis:entry rowsep="1" colname="col3">SWIR2, SWIR3</oasis:entry>
         <oasis:entry rowsep="1" colname="col4"/>
         <oasis:entry rowsep="1" colname="col5"/>
         <oasis:entry rowsep="1" colname="col6"/>
         <oasis:entry rowsep="1" colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Vegetation indices</oasis:entry>
         <oasis:entry colname="col3">NIRv, kNDVI,  NDVI,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M40" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">500 m</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">EVI</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ERA5-Land</oasis:entry>
         <oasis:entry colname="col2">Temperature</oasis:entry>
         <oasis:entry colname="col3">Mean air temperature,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M41" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">0.1<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Hourly – ECMWF</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">mean air temperature</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Climate Reanalysis<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col2"/>
         <oasis:entry rowsep="1" colname="col3">with 16 d delay</oasis:entry>
         <oasis:entry rowsep="1" colname="col4"/>
         <oasis:entry rowsep="1" colname="col5"/>
         <oasis:entry rowsep="1" colname="col6"/>
         <oasis:entry rowsep="1" colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Precipitation</oasis:entry>
         <oasis:entry colname="col3">Total precipitation,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M44" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">0.1<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">total precipitation</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">with 16 d delay</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">NASA USDA Enhanced SMAP </oasis:entry>
         <oasis:entry colname="col3">Surface soil moisture,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M46" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">10 km</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">Soil Moisture<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">subsurface soil moisture</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">Solar zenith angle<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">Cosine of the  solar zenith</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M49" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">Computed</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">angle</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">USDA GMTED2010: </oasis:entry>
         <oasis:entry colname="col3">Elevation</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M50" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M51" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">7.5 arcsec</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">Global Multi-resolution </oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">Terrain Elevation Data 2010<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">Copernicus Corine global land cover </oasis:entry>
         <oasis:entry colname="col3">Non-vegetated, ENF,  EBF,</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M53" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M54" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">100 m</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">classification (CLC2018)<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">DNF, DBF, MF,  UF, shrubs,</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">grassland, crops, wetland</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">Forest  fragmentation<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col3">Forest share</oasis:entry>
         <oasis:entry rowsep="1" colname="col4"><inline-formula><mml:math id="M57" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col5"><inline-formula><mml:math id="M58" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry rowsep="1" colname="col6"/>
         <oasis:entry rowsep="1" colname="col7">30 m</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">Edge share</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M59" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M60" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">30 m</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">OCO-2<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">SIF at 740 nm</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M62" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">2.25 <inline-formula><mml:math id="M63" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.29 km</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">OCO-3<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">SIF at 740 nm</oasis:entry>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M65" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">2.25 <inline-formula><mml:math id="M66" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.29 km</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e556">References: <inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx32" id="text.37"/>; <inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx45" id="text.38"/>; <inline-formula><mml:math id="M27" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx11" id="text.39"/>; <inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx15" id="text.40"/>; <inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx42" id="text.41"/>; <inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx12" id="text.42"/>; <inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx7" id="text.43"/>; <inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx39" id="text.44"/>; <inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx40" id="text.45"/>; <inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx41" id="text.46"/>.</p></table-wrap-foot></table-wrap>

      <p id="d1e1473">MODIS measures the reflected radiance from the earth surface in seven different spectral bands covering the visible and infrared spectral region. Vegetation indices are computed by combining the near-infrared (where chlorophyll is non-absorbing) and the red band (where chlorophyll is highly absorbing) <xref ref-type="bibr" rid="bib1.bibx25" id="paren.47"/>. Specifically, the normalized difference vegetation index (NDVI) <xref ref-type="bibr" rid="bib1.bibx52" id="paren.48"/>,  near-infrared vegetation index (NIR<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx2" id="paren.49"/>, the kernel NDVI (kNDVI) <xref ref-type="bibr" rid="bib1.bibx8" id="paren.50"/>, and the enhanced vegetation index (EVI) <xref ref-type="bibr" rid="bib1.bibx26" id="paren.51"/> are computed as follows:

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M68" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">NDVI</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">NIR</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">NDVI</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">kNDVI</mml:mi><mml:mo>=</mml:mo><mml:mi>tanh⁡</mml:mi><mml:mo>(</mml:mo><mml:msup><mml:mi mathvariant="normal">NDVI</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">EVI</mml:mi><mml:mo>=</mml:mo><mml:mi>G</mml:mi><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">BLUE</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>L</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

            EVI coefficients for MODIS are as follows: <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi>L</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">7.5</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mi>G</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx26" id="paren.52"/>. <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the near infrared band, <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the red band, and <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">BLUE</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the blue band from the MODIS satellites.</p>
      <p id="d1e1759">Temperature and precipitation are taken from ERA5-Land data at the time step of interest and with a delay of one time step. Soil moisture has been shown to be a strong driver of global photosynthesis  due, in part, to its impact on vapor-pressure deficit <xref ref-type="bibr" rid="bib1.bibx28" id="paren.53"/>. Here we use the coarse-resolution NASA USDA Soil Moisture Active Passive (SMAP) soil moisture <xref ref-type="bibr" rid="bib1.bibx15" id="paren.54"/> as a model input and explore its correlation with TROPOMI SIF.  The cosine of the solar zenith angle (SZA) is a proxy for photosynthetically active radiation (PAR) under cloud-free conditions <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx54" id="paren.55"/>.</p>
      <p id="d1e1771">Time-invariant data sets consist of elevation data, fractional land cover classification, and forest fragmentation data. The land cover classification <xref ref-type="bibr" rid="bib1.bibx7" id="paren.56"/> is resampled to 11 fractional classes. The forest fragmentation data consist of two bands and have a native resolution of 30 m. One band describes the share of forest within the grid cell (forest share) and the other how much of that forest is edge forest (defined as a maximum distance to an edge or other land cover type of 30 m).  OCO-2 and OCO-3 have high spatial resolution (2.25 <inline-formula><mml:math id="M76" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.29 km) but small swaths (10 km) and a 16 d revisit time.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Covariation of input data sets with SIF</title>
      <p id="d1e1792">We are interested in understanding what these different data sets are telling us about SIF and also how they co-vary with each other. We compare all collected time variant data against TROPOMI SIF in the spatial and temporal domain. As a quantitative measure, we compute the Pearson correlation coefficient (<inline-formula><mml:math id="M77" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) <xref ref-type="bibr" rid="bib1.bibx3" id="paren.57"/>. Figure <xref ref-type="fig" rid="Ch1.F1"/> shows a scatter comparison of SIF against the auxiliary data at the lowest resolution of the two corresponding sets. Negative SIF values (on the <inline-formula><mml:math id="M78" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis in Fig. <xref ref-type="fig" rid="Ch1.F1"/>) are due to relatively high retrieval errors which scale with radiance levels <xref ref-type="bibr" rid="bib1.bibx32" id="paren.58"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1822">Scatter comparison of SIF to timely changing auxiliary data. The time span of measurements is from April 2018 to March 2021 at 16 d resolution. Longitude and latitude borders are from <inline-formula><mml:math id="M79" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>180 to 180<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math id="M81" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60 to 70<inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, respectively. The comparison resolution corresponds to the lowest resolution of the two corresponding products. For all MODIS data the resolution is 0.05<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and for precipitation, air temperature, surface soil moisture (ssm), and subsurface soil moisture (susm) 0.1<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. To quantify the goodness of fit we compute the Pearson correlation coefficient (<inline-formula><mml:math id="M85" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>) for each subplot <xref ref-type="bibr" rid="bib1.bibx3" id="paren.59"/>.</p></caption>
          <?xmltex \igopts{width=401.183858pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f01.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1894">Pearson correlation coefficient of NIR<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> and kNDVI to TROPOMI SIF. Data are compared at 0.05<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial resolution and in 16 d time steps starting in April 2018 until March 2021. The value per grid cell in <bold>(a)</bold> and <bold>(b)</bold> represents the Pearson correlation coefficient of the vegetation index to SIF in time. Panel <bold>(c)</bold> represents the difference in correlation of the vegetation indices to SIF.</p></caption>
          <?xmltex \igopts{width=495.077953pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f02.png"/>

        </fig>

      <p id="d1e1931">Figure <xref ref-type="fig" rid="Ch1.F2"/> shows spatial patterns of the Pearson correlation coefficients between both NIR<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> and kNDVI to SIF. In both our spatial (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) and temporal (Fig. <xref ref-type="fig" rid="Ch1.F1"/>) analyses, we find NIR<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is a better predictor for SIF than kNDVI, which contradicts the recent findings from <xref ref-type="bibr" rid="bib1.bibx8" id="text.60"/>. However, <xref ref-type="bibr" rid="bib1.bibx8" id="text.61"/> used GOME-2 SIF instead of TROPOMI SIF.</p>
      <p id="d1e1965">The vegetation index NIR<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> outperforms kNDVI in nearly all vegetated regions. Only central Asia, the Sahara, and very high latitudes show a better correlation of kNDVI with SIF. At the same time, these regions generally show a weaker correlation of vegetation indices with SIF.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Development and optimization of SIFnet</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Training and optimization of the neural network</title>
      <p id="d1e1993">Convolutional neural networks (CNNs) are supervised machine learning methods that need matching feature and ground truth data pairs to compute the loss that is back propagated <xref ref-type="bibr" rid="bib1.bibx4" id="paren.62"/>. As such, we begin by coarsening SIF data to 0.5<inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and use it with auxiliary data at 0.05<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> as input to SIFnet, allowing us to estimate SIF at 0.05<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The model output is compared against the measured TROPOMI SIF at 0.05<inline-formula><mml:math id="M94" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. After optimizing the model it can resolve a scaling factor of 10 between coarse-resolution input SIF and model output SIF. Figure <xref ref-type="fig" rid="Ch1.F3"/> visualizes this method. In the following step of estimating high-resolution SIF, the feature SIF data have a resolution of 0.05<inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and auxiliary data of 0.005<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, resulting in a model output of SIF at 0.005<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2067">CNN model structure and training and estimation method. Yellow and red blocks are convolutional and ReLU layers, respectively. Notation of convolutional layers: <inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>X</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>X</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>: kernel sizes are <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mi>X</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>; ch<inline-formula><mml:math id="M100" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>: number of channels is <inline-formula><mml:math id="M101" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>. For training, the data are upscaled. We input auxiliary data at the target resolution and SIF data at a factor of 10 coarser.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f03.png"/>

        </fig>

      <p id="d1e2128">Figure <xref ref-type="fig" rid="Ch1.F3"/> shows our chosen CNN model structure for SIFnet. The model consists of convolutional and rectified linear unit (ReLU) layers that are arranged in a sequence. After the first convolutional block there is a residual connection that skips one ReLU and two convolutional layers. Convolutional kernel sizes are either (3,3) or (1,1). This structure is adapted from the literature findings from, for example, <xref ref-type="bibr" rid="bib1.bibx34" id="text.63"/>. Further, several model structures (Sect. S4.3 in the Supplement) with a different amount of layers, channels, or residual blocks are compared. The chosen model structure represents the best trade-off between complexity and performance. The input feature collinearity and principal component analysis (PCA) presented in Sect. S3 show that some input features have high correlations with each other. A total of 9 out of the 19 PCs in the time variant and 13 out of the 15 PCs in the time-invariant data carry above 99 % of the variance. This suggests that fewer channels should be used in the CNN layers than the feature dimension (because some variables are similar). Therefore the number of channels in the first layer of SIFnet reduces the complexity from 34 to 16 channels (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). More complex model structures did not result in a notably improved loss metrics (Sect. S4.3).</p>
      <p id="d1e2139">For training SIFnet we use 3 years of data (April 2018–March 2021) in 16 d time steps. The study regions are shown in  Sect. S2. There are five folds used as training data: two folds over Asia, one over Europe, one over the  southern part of Africa, and one over South America.  Our validation region is North America (Fig. S4). The hyperparameter tuning is done by training the model on the five folds and computing the loss of the validation data. The parameters are optimized to minimize the loss of the validation data set. Due to computational reasons and the size of the data set, we do not apply a cross validation in the optimization process. The final product consists of high-resolution SIF at 0.005<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> and is validated against independent SIF measurements of the instruments OCO-2 and OCO-3.</p>
      <p id="d1e2151">We center and scale each feature individually by subtracting the mean and normalizing by the standard deviation. For data augmentation of the training data, we use random crops and random flips. Each day of one fold has a matrix size of 1200 <inline-formula><mml:math id="M103" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 900 pixels. We analyze 69 d in 16 d steps over 3 years. For each input during the training process we randomly crop a matrix with a size of 100 <inline-formula><mml:math id="M104" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 100 pixels. As some areas have a large fraction of missing values (e.g., due to water or clouds), we only use cropped matrices that consist of <inline-formula><mml:math id="M105" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 80 % valid pixels in the SIF product. Further, we randomly flip vertically and horizontally, both with a probability of 0.5. These data augmentation methods provide us with a huge database that should avoid overfitting the network parameters. During training, all missing values in the data are set to zero. That mainly affects water regions as the share of missing values in the SIF data used is 91.2 % caused by water. In case there is a missing value in the SIF training sample, all feature values of this pixel are also set to zero to ensure the network does not learn false relationships between the predictors and the target variable (that also applies to vegetated regions). For the MODIS bands we applied the quality index value 0 (best quality only). This filtering also removes pixels that include clouds. To ensure a high coverage we interpolated in time for MODIS. Further, training and test folds are selected based on coverage; i.e., the regions near the Equator (between <inline-formula><mml:math id="M106" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>22.5<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) are not included in the data cubes as MODIS reflectance is sensitive to clouds which appear frequently in these regions (compare Figs.  S2 and S4). All static variables have full coverage on land. ERA5 data has full spatial and temporal coverage. We did not apply any further quality filtering on SMAP soil moisture data. The data are provided as a level 3 product on Google Earth Engine.</p>
      <p id="d1e2191">Our individual loss function is comprised of two loss terms. We use the mean squared error (MSE) loss in combination with the structural dissimilarity index (DSSIM). The DSSIM is the countermeasure of the structural similarity index (SSIM): DSSIM <inline-formula><mml:math id="M108" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 1 <inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> SSIM​​​​​​​ <xref ref-type="bibr" rid="bib1.bibx6" id="paren.64"/>. Therefore, we are not only optimizing the overall deviation of the estimated SIF to the measured SIF but also the structural patterns. Section S4.4 shows the benefit of including both MSE and SSIM terms in the loss function.  Equation (<xref ref-type="disp-formula" rid="Ch1.E5"/>) shows our loss function:
            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M110" display="block"><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="script">L</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi>a</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">MSE</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">DSSIM</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi>a</mml:mi><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>n</mml:mi></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:munderover><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>Y</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:msub><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>Y</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="italic">μ</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>Y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>⋅</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p><?xmltex \hack{\newpage}?>
      <p id="d1e2421"><?xmltex \hack{\noindent}?>where <inline-formula><mml:math id="M111" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number of data points, <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the data point <inline-formula><mml:math id="M113" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> in measured (target variable) SIF, <inline-formula><mml:math id="M114" display="inline"><mml:mover accent="true"><mml:mrow><mml:msub><mml:mi>y</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:math></inline-formula> is the data point <inline-formula><mml:math id="M115" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> in estimated SIF, <inline-formula><mml:math id="M116" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> values are all data points of measured (target variable) SIF, <inline-formula><mml:math id="M117" display="inline"><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula> values are all data points of estimated SIF, <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>Y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the mean of <inline-formula><mml:math id="M119" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:msub></mml:mrow></mml:math></inline-formula> is the mean of <inline-formula><mml:math id="M121" display="inline"><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:math></inline-formula>, <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>Y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the variance of <inline-formula><mml:math id="M123" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:msub></mml:mrow></mml:math></inline-formula> is the variance of <inline-formula><mml:math id="M125" display="inline"><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:math></inline-formula>, <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>Y</mml:mi><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo mathvariant="normal" stretchy="true">̃</mml:mo></mml:mover></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the covariance of <inline-formula><mml:math id="M127" display="inline"><mml:mi>Y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M128" display="inline"><mml:mover accent="true"><mml:mi>Y</mml:mi><mml:mo stretchy="true" mathvariant="normal">̃</mml:mo></mml:mover></mml:math></inline-formula>, and <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>L</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and  <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi>L</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> are variables for stabilization with <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:mi>L</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 2 bit px<inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.03</mml:mn></mml:mrow></mml:math></inline-formula>. The parameters <inline-formula><mml:math id="M135" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M136" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> define the weights of the overall loss of the two individual losses. The overall model performance did not show a notable sensitivity to different <inline-formula><mml:math id="M137" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M138" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> values. To approximately keep the individual losses in the same order of magnitude, we set <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula>. DSSIM is in the range of 0 to 1, with 0 meaning structurally similar and 1 structurally dissimilar.</p>
      <p id="d1e2774">We use the optuna library for the hyperparameter tuning of the learning rate, weight decay, and epoch of the CNN <xref ref-type="bibr" rid="bib1.bibx1" id="paren.65"/>.  Here, a tree-structured Parzen estimator sampler suggests the parameters of the next trial which is based on a Gaussian mixture model. Section S4.1 provides more details on this hyperparameter tuning.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Results of model optimization</title>
      <p id="d1e2788">Figure <xref ref-type="fig" rid="Ch1.F4"/> summarizes the results of the optimized model. We observe an overall <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.92, SSIM of 0.87, and RMSE of 0.17 mW m<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> sr<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> nm<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> between the estimated SIF from SIFnet and retrieved SIF from TROPOMI at 0.05<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F4"/>e). SSIM is calculated by comparing the average SIF signal of the 3 years under investigation. Figure <xref ref-type="fig" rid="Ch1.F4"/>e shows the three metrics for each month of the year.  We observe the lowest <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values in January, February, and March.  These are associated with low SIF values and, consequently, lower signal-to-noise ratios which drive the decreased performance. SSIM also indicates reduced performance during this time period. RMSE values are correlated with overall productivity with the lowest RMSE in winter; this is expected as this metric depends on the magnitude of the signal.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2867">Test set results of CNN training at 0.05<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. Panel <bold>(a)</bold> shows low-resolution SIF that is used as model input, <bold>(b)</bold> shows the estimated SIF at 0.05<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> by SIFnet, <bold>(c)</bold> shows the measured TROPOMI SIF at 0.05<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> from <xref ref-type="bibr" rid="bib1.bibx32" id="text.66"/>, <bold>(d)</bold> shows the scatter comparison between TROPOMI SIF and the SIFnet estimate at 0.05<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, and <bold>(e)</bold> shows for each investigated month the metrics <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, SSIM, and RMSE. Metrics are calculated at 16 d resolution and averaged to monthly values afterwards.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Which features drive SIFnet?</title>
      <p id="d1e2950">We are particularly interested in understanding which features drive our neural net.  Here we evaluate the feature importance using the permutation feature importance method <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx16 bib1.bibx22 bib1.bibx23" id="paren.67"/> with our North American validation data at a target resolution of 0.05<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The method first computes the RMSE including all input features (RMSE<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">orig</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:math></inline-formula>). We then apply the following three steps.
<list list-type="order"><list-item>
      <p id="d1e2979">Shuffle all pixels of one input feature randomly in time and space.</p></list-item><list-item>
      <p id="d1e2983">Compute the new RMSE of the estimation (RMSE<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">F</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">shuf</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:math></inline-formula>).</p></list-item><list-item>
      <p id="d1e3003">Compare the shuffled RMSE to the original: <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mrow><mml:mi mathvariant="normal">F</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">shuf</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">RMSE</mml:mi><mml:mrow><mml:mi mathvariant="normal">F</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">shuf</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">RMSE</mml:mi><mml:mrow><mml:mi mathvariant="normal">orig</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula></p></list-item></list></p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e3049">Feature importance. Panel <bold>(a)</bold> shows the total RMSE of the permuted feature divided by the RMSE without feature permutation, and <bold>(b)</bold> shows the RMSE of each pixel with permuted features divided by the RMSE without feature permutation. Some input variables are clustered, and all variables of that class are permuted at the same time. <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">MODIS</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>: all seven MODIS bands; LULC: all 11 land cover classes;  other VIs: kNDVI, NDVI, and EVI; Mereor.: temperature, precipitation, temperature with 16 d delay, and precipitation with 16 d delay; SM: surface soil moisture and subsurface soil moisture.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f05.png"/>

        </fig>

      <p id="d1e3075">Figure <xref ref-type="fig" rid="Ch1.F5"/> shows the feature importance of clustered input classes and individual features to the overall estimation. Multiple applications of the feature permutation yielded negligible differences in feature importance. Figure <xref ref-type="fig" rid="Ch1.F5"/>a shows the RMSE share of shuffled data to the RMSE of unshuffled data. SIFnet finds low-resolution SIF (SIF<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LR</mml:mi></mml:msub></mml:math></inline-formula>) to be the most important input variable, followed by the vegetation index NIR<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> and the cosine of the solar zenith angle (<inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>). All other variables do not contribute notably to the model output. This result strengthens our findings from Figs. <xref ref-type="fig" rid="Ch1.F1"/> and <xref ref-type="fig" rid="Ch1.F2"/> that NIR<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is better correlated with SIF from TROPOMI than kNDVI. Further, our feature importance is in line with <xref ref-type="bibr" rid="bib1.bibx13" id="text.68"/> in which they find a high correlation of SIF with NIR<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> multiplied with photosynthetic active radiation (PAR), of which the <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> can be used as a proxy. The CNN is a data-driven method and is not restricted by LUE terms. Although SM and meteorology (air temperature and precipitation) play a key role for photosynthesis, we find that they are not important to our model output. This does not necessarily imply that SIF is not linked to these parameters. This can be explained by the following. (1) The variables SM and those from ERA-5 are at coarser resolution than the actual model output of the training phase which is at 0.05<inline-formula><mml:math id="M163" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (10 000 and 11 132 m for SM and ERA-5, respectively). Therefore each pixel at the resolution of 0.05<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> does not have its unique value for SM or ERA-5, but multiple cells can be within one SM or ERA-5 pixel. (2) Not only do the auxiliary data of the model estimate higher-resolution SIF, but they are computed together with coarse-resolution SIF. Therefore, events like heat stress that impact a bigger area than the actual model output might be represented in the coarse-resolution SIF. (3) We have aggregated the data used to 16 d time steps. LUE parameters influencing SIF might have a bigger impact on the estimation at higher temporal resolutions.</p>
      <p id="d1e3174">Figure <xref ref-type="fig" rid="Ch1.F5"/>b shows the spatial feature importance over the validation set in North America for the four most important features. We observe that SIF<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LR</mml:mi></mml:msub></mml:math></inline-formula> has the biggest impact in the eastern US, which corresponds strongly to the high vs. low productivity regions in the US. NIR<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is a strong predictor in the southeastern US and in shrub regions in the western US. The contribution of <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is highest at high latitudes and weakens at lower latitudes. NIR<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is found to be less predictive of SIF at high latitudes.  The land mask is the fourth most important input feature and contributes most in shrub regions. These four features consistently stand out as the strongest predictors.  Other inputs such as fragmentation and soil moisture were not found to be strong predictors here. In Sect. S4.6 we test higher scaling factors between low- and high-resolution SIF. Even with scaling factors of 20 and 50 low-resolution SIF stays the most and second most important input feature, respectively.</p>
      <p id="d1e3220">We also examined different combinations of inputs such as directly including the MODIS bands as opposed to vegetation indices derived from MODIS bands (see Fig. S11). Low-resolution SIF remains the most important feature, followed by the NIR band <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The land cover products increase in relevance.  Interestingly, when low-resolution SIF is omitted as input for the model, we observe contrasting results to Fig. <xref ref-type="fig" rid="Ch1.F5"/> in which NIR<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is no longer a leading predictor. We find that <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, kNDVI, and NDVI are the four most important features in this case (see Fig. S12).  This may result from the collinearity between input features or suggests that another combination of <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">NIR</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ρ</mml:mi><mml:mi mathvariant="normal">RED</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is better correlated to SIF than, for example, NIR<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> or kNDVI. This finding was robust to multiple optimizations and permutations.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Comparison of SIFnet to downscaled SIF</title>
      <p id="d1e3310">Figure <xref ref-type="fig" rid="Ch1.F6"/> shows the 0.005<inline-formula><mml:math id="M176" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> SIF estimated by SIFnet and downscaled SIF from <xref ref-type="bibr" rid="bib1.bibx53" id="text.69"/>.  The difference between the two SIF estimates can be seen in Fig. <xref ref-type="fig" rid="Ch1.F6"/>c. SIFnet predicts lower SIF in the western US drylands and higher SIF over forested regions in the eastern US.  This prediction of lower SIF in drylands is interesting because <xref ref-type="bibr" rid="bib1.bibx53" id="text.70"/> resorted to an ad hoc bias correction in these regions due to a low signal-to-noise ratio. Recent work from <xref ref-type="bibr" rid="bib1.bibx55" id="text.71"/> concluded that SIF and NIR<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> capture complementary events in western US drylands as a proxy for GPP and that the linear correlation of SIF to GPP was substantially lower in these regions compared to other vegetation types.  We also observe systematic differences in the predicted SIF in urban areas. These regions are further evaluated in Fig. S17. Notably, the SIFnet estimate is systematically lower than the downscaling estimate in most urban regions examined here, Seattle being a notable exception. Both SIFnet and the downscaling approach allocate SIF to large urban parks and green spaces, but SIFnet predicts little-to-no SIF over the rest of the urban area.  In particular, SIFnet estimates nearly zero SIF in the urban core of Los Angeles and San Francisco. SIFnet and the downscaling method predict comparable SIF as we move away from the urban core. Fine-scale features in the urban region are visible in both SIF estimates such as the Schiller Woods in Chicago  (42.0<inline-formula><mml:math id="M178" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 87.8<inline-formula><mml:math id="M179" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e3365">SIFnet estimated SIF at 0.005<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> for CONUS and its comparison to downscaled SIF. Panel <bold>(a)</bold> shows the SIFnet estimated SIF at 0.005<inline-formula><mml:math id="M181" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, <bold>(b)</bold> shows the downscaled SIF from <xref ref-type="bibr" rid="bib1.bibx53" id="text.72"/>, and <bold>(c)</bold> shows the difference between SIFnet and downscaled SIF. Negative values imply a higher SIFnet SIF and positive values a higher downscaled SIF value.</p></caption>
          <?xmltex \igopts{width=469.470472pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f06.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Validation against OCO-2/3 SIF</title>
      <p id="d1e3414">The differences in SIF predicted from SIFnet and the downscaled SIF beg the question: which is correct?  Here we evaluate both SIF products against independent SIF observations from OCO-2 and OCO-3 <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx41" id="paren.73"/>. These instruments have higher spatial resolution than TROPOMI and, as such, can be used to evaluate the high-resolution patterns predicted by both SIFnet and the downscaling approach.  Specifically, OCO-2 and OCO-3 have nadir footprint sizes of 2.25 <inline-formula><mml:math id="M182" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.29 km.  However, OCO-2 and OCO-3 do not provide full spatial coverage.  They observe narrow swaths that are <inline-formula><mml:math id="M183" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 km across-track. OCO-3 also provides a scanning mode to observe urban areas. Here, we use quality-checked OCO-2 data from April 2018 until March 2021 and OCO-3 data from July 2019 until March 2021. To compare the ungridded OCO-2 and OCO-3 data against the SIF estimated from TROPOMI, we compute the weighted average of all 0.005<inline-formula><mml:math id="M184" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid cells that fall within the bounds of an OCO footprint. Here, the TROPOMI estimates are subsampled to 0.0005<inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (approx. 50 m at Equator), and the mean value is computed for all values which fall into the OCO footprint. For a quantitative comparison between OCO-2/3 and the SIFnet and downscaled estimate, the metrics <inline-formula><mml:math id="M186" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>, and RMSE are computed.</p>
      <p id="d1e3471">The high-resolution SIF estimates from SIFnet, the downscaling, and OCO are instantaneous SIF measurements taken at a specific time of the day, while the time of TROPOMI observations can differ substantially. Here, we compute the daily average SIF by scaling with the cosine of the SZA <xref ref-type="bibr" rid="bib1.bibx17" id="paren.74"/>:
          <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M188" display="block"><mml:mrow><?xmltex \hack{\hbox\bgroup\fontsize{9.5}{9.5}\selectfont$\displaystyle}?><mml:mi mathvariant="normal">Daily</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SIF</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="normal">SIF</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mo>∫</mml:mo><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:msubsup><mml:mi>cos⁡</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>,</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>[</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><?xmltex \hack{$\egroup}?><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mi mathvariant="normal">Daily</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SIF</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the daily integrated SIF estimate, <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi mathvariant="normal">SIF</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the instantaneous SIF at the individual measurement time, SZA is the solar zenith angle, <inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">s</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the time of the satellite measurement, <inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">o</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the time of sunrise, and <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the time of sunset. This implicitly assumes that both PAR and SIF scale with <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">SZA</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> under cloud-free conditions, and we neglect Rayleigh scattering, as well as gas absorption. Although this approach neglects several water or light conditions, it provides our best estimate of daily SIF and enables comparison between multiple SIF products with different measurement times <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx32 bib1.bibx17" id="paren.75"/>. The method is equivalent to the daily correction scheme for OCO-2, OCO-3, and TROPOMI <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx41 bib1.bibx17" id="paren.76"/>. Additionally, we performed a sensitivity study in which we trained SIFnet using daily corrected SIF and found the results to be generally insensitive to the use of instantaneous vs. daily corrected SIF (see Fig. S18). Following this, we chose to apply the daily correction after deriving the high-resolution SIF.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e3699">Validation of SIFnet and downscaled SIF to OCO-2 and OCO-3 SIF over CONUS. Comparison from April 2018 until March 2021 in 16 d time steps. Daily OCO-2 and OCO-3 data are assigned to the closest 16 d time step. Panel <bold>(a)</bold> shows the gridded correlation of the two products against the combined data of OCO-2 and OCO-3. We first compute the SIF data from SIFnet and downscaling estimate that falls into the OCO footprint. Then we assign every OCO footprint to the closest grid point on the 1<inline-formula><mml:math id="M195" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid dependent on the center location of that footprint and compute the Pearson correlation coefficient. Panel <bold>(b)</bold> shows the scatter comparison of the weighted average of all grid cells on the 0.005<inline-formula><mml:math id="M196" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> estimated SIFnet SIF (ours) and downscaled SIF <xref ref-type="bibr" rid="bib1.bibx53" id="paren.77"/> that fall into the OCO-2 or OCO-3 footprint.</p></caption>
        <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f07.png"/>

      </fig>

      <p id="d1e3736">Figure <xref ref-type="fig" rid="Ch1.F7"/> shows a comparison of both SIFnet and the downscaled SIF to OCO-2 and OCO-3. Specifically, Fig. <xref ref-type="fig" rid="Ch1.F7"/>a shows the correlation of SIFnet and the downscaled estimate with OCO-2/3 for every 1<inline-formula><mml:math id="M197" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> pixel over CONUS. Both SIFnet and the downscaled SIF generally show good agreement with <inline-formula><mml:math id="M198" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> in excess of 0.7 for most of the high-productivity regions.  We observe weaker correlations in the western drylands due, in part, to a lower signal-to-noise ratio.  Overall, we find SIFnet to perform systematically better than the downscaled SIF, as shown in the difference plot. Figure <xref ref-type="fig" rid="Ch1.F7"/>b summarizes these spatial patterns in a scatterplot comparison. SIFnet again shows better performance than the downscaled SIF against OCO-2, OCO-3, and OCO-2/3. The Pearson correlation coefficient <inline-formula><mml:math id="M199" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> is 0.78 and 0.72 for the SIFnet and downscaled estimate, respectively, when comparing to all OCO data (right column in Fig. <xref ref-type="fig" rid="Ch1.F7"/>b). The generally high RMSE indicates different scales and variability in the data sets.</p>
      <p id="d1e3771">Deviations between TROPOMI and OCO-2/3 also appear at a grid of 0.05<inline-formula><mml:math id="M200" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (Fig. S19). The <inline-formula><mml:math id="M201" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> coefficient is 0.61 and 0.62 between TROPOMI and OCO-2 and OCO-3 SIF, respectively. Indeed, one might expect better correlations here as both present SIF at 740 nm. However, as pointed out in <xref ref-type="bibr" rid="bib1.bibx32" id="text.78"/>, the uncertainty of both TROPOMI and OCO-2 SIF is expected to lead to a certain spread between the data sets. In addition, we do not account for differences in acquisition times and viewing–illumination geometry, which can lead to additional uncertainties in this comparison. For reference, when comparing single footprints of TROPOMI SIF to aggregated OCO-2 SIF for June 2018 globally, <xref ref-type="bibr" rid="bib1.bibx32" id="text.79"/> found a <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.67; only additional aggregation leads to a <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.88. The mean deviation of TROPOMI SIF to OCO-2 SIF is close to the average standard deviation of TROPOMI SIF (0.4 mW m<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> sr<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> nm<inline-formula><mml:math id="M206" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). In our analysis, from the 16 d product from TROPOMI SIF for April 2018 until March 2021 at 0.05<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, we observe an average error in the TROPOMI SIF of 0.43 mW m<inline-formula><mml:math id="M208" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> sr<inline-formula><mml:math id="M209" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> nm<inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for the CONUS. That error is close to the RMSE between instantaneous TROPOMI SIF and instantaneous OCO-2 SIF (0.37 mW m<inline-formula><mml:math id="M211" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> sr<inline-formula><mml:math id="M212" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> nm<inline-formula><mml:math id="M213" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). To compare TROPOMI and OCO-2/3 SIF we aggregate the OCO-2/3 footprints to the same grid as our TROPOMI data (0.05<inline-formula><mml:math id="M214" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). As we aggregate multiple OCO-2 or OCO-3 footprints to match one TROPOMI grid cell at 0.05<inline-formula><mml:math id="M215" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, the certainty of the OCO measurements increases, and therefore the RMSE between TROPOMI and OCO SIF decreases.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e3962">SIFnet and downscaled SIF, the difference between these, and the difference in correlation to OCO-2 and OCO-3 for four urban regions. The first column shows the SIFnet estimate, the second the downscaled SIF from <xref ref-type="bibr" rid="bib1.bibx53" id="text.80"/>, the third the difference between SIFnet and downscaled SIF, and the last the difference in correlation of the high-resolution SIF estimates to combined OCO-2 and OCO-3 data on a 0.02<inline-formula><mml:math id="M216" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid multiplied with the <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="script">L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> norm between the SIFnet and downscaled estimate.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f08.png"/>

      </fig>

      <p id="d1e3994">Figure <xref ref-type="fig" rid="Ch1.F8"/> presents a detailed comparison of SIFnet and the downscaled SIF in four US cities. The first column shows the SIFnet estimate, the second the downscaled SIF from <xref ref-type="bibr" rid="bib1.bibx53" id="text.81"/>, the third the difference between SIFnet and downscaled SIF, and the last column the difference in correlation of the high-resolution SIF estimates to combined OCO-2 and OCO-3 data on a 0.02<inline-formula><mml:math id="M218" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid multiplied by the <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="script">L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> norm between the SIFnet and the downscaled SIF. The column on the right highlights both regions where the differences in predicted SIF are large and which product is performing better. As such, the right column will show white in areas where the difference in predicted SIF is small or the correlation with OCO is similar. While we observe large differences in predicted SIF for the urban areas (column 3), we do not find one product to perform systematically better in urban areas. This likely indicates the complexity in the SIF signal arising from urban areas.  Additionally, urban areas make up a small fraction of the overall land mass and, as such, do not represent a large share of the training data in SIFnet. These factors likely contribute to the heterogeneous performance observed in the right column of Fig. <xref ref-type="fig" rid="Ch1.F8"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e4026">SIFnet SIF, downscaled SIF, MODIS NIR<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>, and a Google Earth cut-out for a part of Chicago. Left panel shows the SIFnet estimate, second panel shows the downscaled estimate from <xref ref-type="bibr" rid="bib1.bibx53" id="text.82"/>, third panel shows MODIS NIR<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> for Chicago, and last panel shows the Google Earth cut-out <xref ref-type="bibr" rid="bib1.bibx21" id="paren.83"/>. For panels 1–3 the average data for April 2018 until March 2021 is shown.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://bg.copernicus.org/articles/19/1777/2022/bg-19-1777-2022-f09.png"/>

      </fig>

      <p id="d1e4060">However, there are some notable successes of SIFnet in urban areas that can be mapped directly to features in the urban area.  Figure <xref ref-type="fig" rid="Ch1.F9"/> shows both SIFnet and the downscaled SIF along with NIR<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> from MODIS and a true color image of Chicago. A feature clearly stands out in both the downscaled SIF and NIR<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> image.  This is a region with missing NIR<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> and effectively no downscaled SIF. However, SIFnet does not show a strong gradient here.  This region corresponds to the Chicago airport. In the MODIS NIR<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> image it is visible that there are no valid data available for that region for the 3 investigated years. The downscaling method from <xref ref-type="bibr" rid="bib1.bibx53" id="text.84"/> relies only on NIR<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> in the weighting function. If there are no data available for the region, they are interpolated in space and time. Here, it shows that the method seems to fail in urban regions where no MODIS NIR<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> signal is available. SIFnet handles this region better and seems to rely on other auxiliary data if there is no MODIS NIR<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> available. In Fig. <xref ref-type="fig" rid="Ch1.F8"/> it is also visible that the SIFnet estimate correlates better with the OCO-X data than the downscaled SIF for the region of the Chicago airport.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e4143">Here, we develop a convolutional neural network (CNN) model named SIFnet to increase the resolution of TROPOMI SIF by a factor of 10. The novelty of our method consists of using coarse-resolution SIF measurements together with high-resolution auxiliary data as model input to estimate high-resolution SIF. After optimization and hyperparameter tuning of SIFnet, the estimated SIF at 500 m resolution yields an <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msup><mml:mi>r</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and RMSE of 0.92 and 0.17, respectively, when compared against validation data (Fig. <xref ref-type="fig" rid="Ch1.F4"/>). We further compare the output of SIFnet against a recently developed downscaling method to estimate high-resolution SIF <xref ref-type="bibr" rid="bib1.bibx53" id="paren.85"/> and evaluate both methods against independent observations from the Orbiting Carbon Observatory 2 and 3 (OCO-2/3).  SIFnet is found to perform systematically better than the downscaling approach when compared against independent measurements.  Through interpretable machine learning methods, we identify the key features that SIFnet utilizes to accurately predict high-resolution spatial patterns of SIF.  We find that SIFnet relies heavily on the low-resolution SIF feature (SIF<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LR</mml:mi></mml:msub></mml:math></inline-formula>) and the vegetation index NIR<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="Ch1.F5"/>).</p>
      <p id="d1e4183">SIFnet is a multi-layer CNN that increases the spatial resolution of the TROPOMI SIF by a factor of 10. Our model uses auxiliary data sets related to gross primary productivity and SIF as inputs and yields a high-resolution SIF estimate. The model is trained using three years of data from Asia, Europe, Africa, and South America.  North America is used as the validation data set.  Our loss function is comprised of two terms: the mean squared error and the structural dissimilarity index. The combination of these two terms improved the performance of our model.</p>
      <p id="d1e4186">SIFnet was further compared to the recent downscaled SIF product developed by <xref ref-type="bibr" rid="bib1.bibx53" id="text.86"/>. The two high-resolution estimates showed pronounced differences across the western US drylands. This difference is particularly interesting because these drylands tend to be low-productivity regions and traditionally have been difficult for SIF to accurately capture due to the low signal-to-noise ratio. Both high-resolution SIF estimates were compared to independent observations from OCO-2/3. SIFnet performed systematically better than the downscaled SIF (<inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.78</mml:mn></mml:mrow></mml:math></inline-formula> for SIFnet, <inline-formula><mml:math id="M233" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.72</mml:mn></mml:mrow></mml:math></inline-formula> for downscaling). SIFnet and the downscaling method also yielded differences in urban regions. However, there was substantial heterogeneity in the performance of SIFnet and downscaling in urban areas. One product did not perform systematically better than the other within urban areas. The mixed results in urban areas likely relates to both the complexity of the photosynthetic activity in urban areas, as well as the lack of training data, as urban areas represent a small fraction of the total landmass.</p>
      <p id="d1e4216">We adapted techniques from the area of interpretable machine learning to assess the key features driving SIFnet. Specifically, we conducted random permutations to input data sets and assessed the impact on the resulting RMSE.  From this, we found that SIFnet relies most heavily on the low-resolution SIF feature (SIF<inline-formula><mml:math id="M234" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">LR</mml:mi></mml:msub></mml:math></inline-formula>). The second most important factor is the MODIS vegetation index NIR<inline-formula><mml:math id="M235" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula>. NIR<inline-formula><mml:math id="M236" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> is also found to outperform the recently proposed kNDVI vegetation index, in contrast to <xref ref-type="bibr" rid="bib1.bibx8" id="text.87"/>. The interpretable machine learning approach also allowed us to identify spatial regions of importance for the different parameters. Interestingly, SIFnet relies more heavily on NIR<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">v</mml:mi></mml:msub></mml:math></inline-formula> in the western drylands where the SIF signal-to-noise ratio is low. This implies that SIFnet is picking up on key physics that lead to the improved performance relative to the downscaling method. Overall, SIFnet represents a robust method to infer continuous high-spatial-resolution information about processes related to gross primary productivity.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e4262">The high-resolution SIF for CONUS from April 2018 until March 2021 is available here: <ext-link xlink:href="https://doi.org/10.5281/zenodo.6321987" ext-link-type="DOI">10.5281/zenodo.6321987</ext-link> <xref ref-type="bibr" rid="bib1.bibx19" id="paren.88"/>. Further data can be requested from the authors.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e4271">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/bg-19-1777-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/bg-19-1777-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e4280">JG, AJT, and JC conceived the study. JG compiled data sets, conducted data analysis, and generated figures. JG wrote the manuscript. All authors edited the manuscript and provided feedback. JG did the literature research. PK and CF generated the TROPOMI SIF data. JC provided project guidance. All authors contributed to the discussion and interpretation of the results. All authors have read and agreed to the published version of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e4286">The contact author has declared that neither they nor their co-authors have any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e4292">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4298">We thank Xiaojing Tang, Luca Lloyd, and Lucy Hutyra from Boston University, USA, for providing us with their valuable global data about forest fragmentation.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e4303">This research has been supported by the Institute for Advanced Study, Technische Universität München (grant no. 291763), the Deutsche Forschungsgemeinschaft (grant no. 419317138), the NASA Early Career Faculty program (grant no. 80NSSC21K1808), and the NASA Carbon Cycle Science program (grant no. 80HQTR21T0101).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>This work was supported by the German Research<?xmltex \notforhtml{\newline}?> Foundation (DFG) and the Technical University of Munich <?xmltex \notforhtml{\newline}?>(TUM) in the framework of the Open Access Publishing Program.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e4316">This paper was edited by Martin De Kauwe and reviewed by two anonymous referees.</p>
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