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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/essd-15-4519-2023</article-id><title-group><article-title>An integrated and homogenized global surface solar radiation dataset and its
reconstruction based on <?xmltex \hack{\break}?>a convolutional neural network approach</article-title><alt-title>An global surface solar radiation dataset  based on
a CNN approach</alt-title>
      </title-group><?xmltex \runningtitle{An global surface solar radiation dataset  based on
a CNN approach}?><?xmltex \runningauthor{B. Jiao et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff5">
          <name><surname>Jiao</surname><given-names>Boyang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Su</surname><given-names>Yucheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff5">
          <name><surname>Li</surname><given-names>Qingxiang</given-names></name>
          <email>liqingx5@mail.sysu.edu.cn</email>
        <ext-link>https://orcid.org/0000-0002-1424-4108</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Manara</surname><given-names>Veronica</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Wild</surname><given-names>Martin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3619-7568</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>School of Atmospheric Sciences, Sun Yat-sen University, and Key
Laboratory of Tropical Atmosphere–Ocean System, Ministry of Education,
Zhuhai 519082, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Public Meteorological Service Center, Meteorological Bureau of Zhuhai, Zhuhai 519082, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Environmental Science and Policy, Università degli
Studi di Milano,<?xmltex \hack{\break}?> via Celoria 10, 20133, Milan, Italy</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute for Atmospheric and Climate Science, ETH Zurich, Zurich,
Switzerland</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Southern Laboratory of Ocean Science and Engineering (Guangdong
Zhuhai), Zhuhai 519082, China </institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Qingxiang Li (liqingx5@mail.sysu.edu.cn)</corresp></author-notes><pub-date><day>6</day><month>October</month><year>2023</year></pub-date>
      
      <volume>15</volume>
      <issue>10</issue>
      <fpage>4519</fpage><lpage>4535</lpage>
      <history>
        <date date-type="received"><day>8</day><month>May</month><year>2023</year></date>
           <date date-type="rev-request"><day>22</day><month>May</month><year>2023</year></date>
           <date date-type="rev-recd"><day>30</day><month>August</month><year>2023</year></date>
           <date date-type="accepted"><day>3</day><month>September</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2023 Boyang Jiao et al.</copyright-statement>
        <copyright-year>2023</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023.html">This article is available from https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e148">Surface solar radiation (SSR) is an essential factor in the flow of surface
energy, enabling accurate capturing of long-term climate change and
understanding of the energy balance of Earth's atmosphere system. However, the
long-term trend estimation of SSR is subject to significant uncertainties
due to the temporal inhomogeneity and the uneven spatial distribution of in situ observations. This paper develops an observational integrated and
homogenized global terrestrial (except for Antarctica) station SSR dataset (SSRIH<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">station</mml:mi></mml:msub></mml:math></inline-formula>) by integrating all available SSR observations,
including the existing homogenized SSR results. The series is then
interpolated in order to obtain a 5<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M3" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>
resolution gridded dataset (SSRIH<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>). On this basis, we further
reconstruct a long-term (1955–2018) global land (except for Antarctica) SSR
anomaly dataset with a 5<inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M7" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution
(SSRIH<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>) by training improved partial convolutional neural network
deep-learning methods based on 20th Century Reanalysis version 3 (20CRv3). Based on this, we
analysed the global land- (except for Antarctica) and regional-scale SSR trends
and spatiotemporal variations. The reconstruction results reflect the
distribution of SSR anomalies and have high reliability in filling and
reconstructing the missing values. At the global land (except for
Antarctica) scale, the decreasing trend of the SSRIH<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M11" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.276 <inline-formula><mml:math id="M12" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.205 W m<inline-formula><mml:math id="M13" 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> per decade) is smaller than the trend of the SSRIH<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M15" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.776 <inline-formula><mml:math id="M16" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.230 W m<inline-formula><mml:math id="M17" 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> per decade) from 1955 to
1991. The trend of the SSRIH<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (0.697 <inline-formula><mml:math id="M19" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.359 W m<inline-formula><mml:math id="M20" 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> per decade)
from 1991 to 2018 is also marginally lower than that of the SSRIH<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>
(0.851 <inline-formula><mml:math id="M22" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.410 W m<inline-formula><mml:math id="M23" 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> per decade). At the regional scale, the
difference between the SSRIH<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and SSRIH<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> is more significant
in years and areas with insufficient coverage. Asia, Africa, Europe and
North America cause the global dimming of the SSRIH<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, while Europe
and North America drive the global brightening of the SSRIH<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>.
Spatial sampling inadequacies have largely contributed to a bias in the
long-term variation of global and regional SSR. This paper's homogenized
gridded dataset and the Artificial Intelligence reconstruction gridded
dataset  (Jiao and Li, 2023) are both available at <ext-link xlink:href="https://doi.org/10.6084/m9.figshare.21625079.v1" ext-link-type="DOI">10.6084/m9.figshare.21625079.v1</ext-link>.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>41975105</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2018YFC1507705</award-id>
<award-id>2017YFC1502301</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung</funding-source>
<award-id>200020 188601</award-id>
</award-group>
<award-group id="gs4">
<funding-source>Ministero dell'Università e della Ricerca</funding-source>
<award-id>FSE – REACT EU, DM 10/08/2021 n. 1062</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<?pagebreak page4520?><sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e424">Energy flows at the Earth's surface play an essential role in climate change
and human activity and link to physical processes such as global warming,
glacier retreating, the hydrological cycle and the carbon budget  (Hoskins and
Valdes, 1990; Peixoto et al., 1992; Trenberth and Fasullo, 2013; Wild,
2012). As a critical factor characterizing surface energy flows, surface
solar radiation (SSR) largely determines the climatic conditions and
ecological environment in which we live. Therefore, a more accurate and
comprehensive analysis of the SSR fluxes will help better understand the
Earth's atmospheric system. In situ observations provide the most accurate baseline
data for measuring SSR. They allow for the first time the detection of
decadal changes in SSR known as “dimming and brightening”  (Wild et
al., 2005), especially considering that they cover a longer period
concerning another type of data, e.g. satellite data (Pfeifroth et al., 2018). Even observational data often have uneven
distribution and missing data with respect to the satellite data, especially
in areas with complex orography   (Manara et al., 2020).</p>
      <p id="d1e427">The sources of in situ SSR observations are mainly collected from the Global Energy
Balance Archive (GEBA)  (Wild et al., 2017) and the World Radiation
Data Centre (WRDC)  (Tsvetkov et al., 1995). Furthermore, other SSR
station series are obtained from the high-quality Baseline Surface Radiation
Network (BSRN)  (Driemel et al., 2018) and the data centres of
individual national hydrometeorological services. However, two issues still
need to be addressed: (1) the inhomogeneity of station data resulting from
station relocations and instrumentation changes severely impacting the climate
change assessment. For the regions with a relatively high density of
stations, like Europe  (Manara et al., 2019, 2016;
Sanchez-Lorenzo et al., 2013a, b, 2015), Japan (Ma et al., 2022) and China  (Ju et al., 2006;
Wang, 2014; Wang et al., 2015; Wang and Wild, 2016; S. Yang et al., 2018; You
et al., 2013), much previous work has redefined the degree and timing of
dimming and brightening by addressing the inhomogeneity of the SSR data series. For example, in Spain, the average annual homogenized SSR series has
a significant increasing trend (<inline-formula><mml:math id="M28" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula>3.9 W m<inline-formula><mml:math id="M29" 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> per decade) during the
1985–2010 period  (Sanchez-Lorenzo et al., 2013a). The period of
dimming observed in Italy's homogenized SSR series is not apparent in the
1960s and early 1970s, when the raw series (non-homogenized) are taken into
account (Manara et al., 2016). The direct measurements of SSR show a
level trend from 1961 to 2014 over Japan, while their homogenization series
display a decreasing trend (0.8–1.6 W m<inline-formula><mml:math id="M30" 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> per decade) (Ma et al.,
2022). In China, homogenization largely eliminated the dramatic non-climatic
rise of the early 1990s and also reduced the increasing trend from 1990 to
2016  (S. Yang et al., 2018). However, most of the research was still
limited to regional scales. (2) There is the issue of limited spatial sampling of long
observational stations and their uneven distribution, especially over areas
with complex orography. Considerable efforts have been devoted to filling in or interpolating the missing values in climate datasets (“spatial analysis”)
(Collins, 1996; Erxleben et al., 2002; Scudiero et al., 2016). The
traditional spatial interpolation methods commonly used include inverse
distance weighting (Fisher et al., 1993; Shepard, 1968), kriging (Krige, 1951) and thin-plate splines   (Bookstein, 1989). Since the 1980s, physical parametric interpolation  (Feng and Wang,
2021; Tang et al., 2019) and Bayesian fusion schemes  (Aguiar et
al., 2015) based on multi-source observational data have been widely used with the emergence of highly accurate and relatively precise satellite data.
However, the resulting fusion datasets cover too short a period to
investigate their decadal and multi-decadal variations and to study the
underlying causes. The spatial, temporal and spectral coverage of a single
satellite is limited, and multiple satellite data are therefore often used
in tandem with each other; however, such a discontinuity in time and space
can introduce inhomogeneity into a dataset  (Evan et al., 2007; Feng and
Wang, 2021; Shao et al., 2022). Reanalysis products are an important
complement containing long-term SSR data and therefore have been widely used in
climate studies  (Huang et al., 2018; Jiao et al., 2022; Urraca et al.,
2018; C. Zhou et al., 2018, 2017) due to the dynamically
consistent and spatiotemporally complete atmospheric fields with high
resolution and open access to data. However, existing studies have shown
that reanalysis products generally overestimate multi-year mean SSR values
compared to observations over land  (He et al., 2021). With the
continuous development of climate system simulations, model data from the
Coupled Model International Project (CMIP) have become an important resource
for conducting climate change research  (Gates et al., 1999; Zhou et al.,
2019). Previous studies have shown that the models used in CMIP6
overestimate the global mean SSR  (He et al., 2023; Jiao et al., 2022;
Wild, 2020). The rise of deep-learning and big-data techniques has brought
about an explosion of artificial intelligence (AI). Machine learning is
increasingly being used in spatial interpolation, such as the spatial
reconstruction of surface temperature datasets  (Huang et al., 2022; Kadow
et al., 2020) or the spatial and temporal reconstruction of
turbulence resolution   (Fukami et al., 2021). Furthermore, it shows high accuracy and low uncertainty in reproducing and predicting SSR
(Leirvik and Yuan, 2021; Tang et al., 2016; L. Yang et al., 2018; Yuan et
al., 2021). However, long-term homogenized SSR datasets with global
terrestrial coverage have yet to be developed, resulting in significant
uncertainties in assessing global SSR variation (Jiao et al., 2022).</p>
      <p id="d1e461">Therefore, developing a more homogeneous and comprehensive global long-term
SSR climatic dataset that provides a better benchmark for observational
constraints on the global surface energy balance and budget remains a valuable
and challenging task. This paper first homogenizes and grids the most
extensive collection of available global SSR station observations. Then, the
missing grid boxes and years are<?pagebreak page4521?> spatially interpolated using a convolutional
neural network (CNN) approach to obtain a globally covered land surface SSR
anomaly dataset. Finally, the reconstructed datasets are initially
analysed and evaluated. Thus, the paper is divided into seven main sections.
The data resources are introduced in Sect. 2. Section 3 presents the data
homogenization and the CNN model reconstruction methods. The data
homogenization and verification are shown in Sect. 4. Section 5 gives the
AI reconstruction results. Section 6 is the availability of the datasets.
Conclusions are provided at the end of the paper.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data</title>
      <p id="d1e472">Nine SSR datasets are collected to derive the global SSR variable. In
particular, six datasets contain data from observational stations (Sect. 2.1): two global ground-based measurement datasets (GEBA, WRDC) and four
homogenized products at the regional and country levels (Europe, China, Japan
and Italy). Three of the adopted datasets are reanalysis data (Sect. 2.2.1): fifth-generation European Centre for Medium-Range Weather Forecasts
(ECMWF) reanalysis (ERA5), 20th Century Reanalysis version 3 (20CRv3)
data and the Coupled Model Intercomparison Project Phase 6
(CMIP6) historical simulation output (125). Specifically, the ERA5 data are
used to fill the data over oceans and Antarctica (Sect. 3.2.1), and 20CRv3
data and CMIP6 simulations are used for AI model training (Sect. 5.1) and reconstruction. All are listed in Table 1.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e478">List of information on the various types of data used in this paper.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <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="right"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Abbreviation</oasis:entry>
         <oasis:entry colname="col3">Resolution</oasis:entry>
         <oasis:entry colname="col4">Time</oasis:entry>
         <oasis:entry colname="col5">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">In situ – raw</oasis:entry>
         <oasis:entry colname="col2">GEBA (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1922–2020</oasis:entry>
         <oasis:entry colname="col5">Wild et al. (2017)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">WRDC (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1964–2017</oasis:entry>
         <oasis:entry colname="col5">Tsvetkov et al. (1995)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">In situ – homo</oasis:entry>
         <oasis:entry colname="col2">China (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1950–2016</oasis:entry>
         <oasis:entry colname="col5">S. Yang et al. (2018)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Japan (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1870–2015</oasis:entry>
         <oasis:entry colname="col5">Ma et al. (2022)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Europe (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1922–2012</oasis:entry>
         <oasis:entry colname="col5">Sanchez-Lorenzo et al. (2015)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Italy (station)</oasis:entry>
         <oasis:entry colname="col3">Monthly</oasis:entry>
         <oasis:entry colname="col4">1959–2016</oasis:entry>
         <oasis:entry colname="col5">Manara et al. (2016, 2019)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Reanalysis/model</oasis:entry>
         <oasis:entry colname="col2">ERA5 (grid)</oasis:entry>
         <oasis:entry colname="col3">Monthly/0.25<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M32" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">1950–2020</oasis:entry>
         <oasis:entry colname="col5">Hersbach et al. (2020)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">20CRv3 (grid)</oasis:entry>
         <oasis:entry colname="col3">Monthly/0.7<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M35" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.7<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">1940–2015</oasis:entry>
         <oasis:entry colname="col5">Slivinski et al. (2019)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">CMIP6 (grid)</oasis:entry>
         <oasis:entry colname="col3">Monthly/–</oasis:entry>
         <oasis:entry colname="col4">1940–2014</oasis:entry>
         <oasis:entry colname="col5">Eyring et al. (2016)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>In situ observational data</title>
<sec id="Ch1.S2.SS1.SSS1">
  <label>2.1.1</label><title>Global datasets</title>
      <p id="d1e739">There are two main sources of raw SSR data (see Table 1): the ETH Zurich
GEBA with monthly data from 2445 globally distributed stations, starting
from 1922 until 2020, and the WRDC dataset with monthly globally distributed
data from 1136 stations since 1964. The first one is available for download
at <uri>https://geba.ethz.ch</uri> (last access: 2 July 2022). The second
one published the first SSR radiation balance data in 1965, and its
publication has been issued four times a year since 1993 and is available
for download at <uri>http://wrdc.mgo.rssi.ru/</uri> (last access: July
2021).</p>
</sec>
<sec id="Ch1.S2.SS1.SSS2">
  <label>2.1.2</label><title>National (regional) homogenized station datasets</title>
</sec>
<sec id="Ch1.S2.SS1.SSSx1" specific-use="unnumbered">
  <title>(1) Chinese homogenized SSR dataset</title>
      <p id="d1e762">The China Meteorological Radiation Fundamental Elements Monthly Value Data
Set was downloaded from <uri>http://www.nmic.cn</uri>  (last access: September 2022). The homogenized
SSR dataset in China is released by the National Meteorological Information
Centre (NMIC) of the China Meteorological Administration (CMA)  (S. Yang et a., 2018).
The data are available for the period between January 1950 and December 2014, and the
follow-up data are extended with raw observations from the NMIC. They used the sunshine duration (SSD) data from nearby stations to construct an arguably
better reference to identify inhomogeneities in the SSR data. Then, a
combined metadata and maximum-penalty <inline-formula><mml:math id="M37" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test (PMT) method was used to
detect the change points. Finally, they were adjusted by a quantile-matching
(QM) algorithm  (Wang and Feng, 2013). The final homogenized SSR station
dataset was converted to gridded data using the first difference method (FDM,
Peterson et al., 1998) and is available for download at
<uri>http://www.nmic.cn</uri> (last access: September 2022).</p>
</sec>
<sec id="Ch1.S2.SS1.SSSx2" specific-use="unnumbered">
  <title>(2) Japanese homogenized SSR dataset</title>
      <p id="d1e784">Ma et al. (2022) released a Japanese SSR homogenized dataset
in 2022 spanning the period between 1870 and 2015. First, they homogenized
SSD based on PMF (penalized maximal <inline-formula><mml:math id="M38" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula> test) and QM algorithms. They then
used the homogenized SSD from the previous step as a reference series,
combined with metadata and PMT, to detect change points. Finally, they
adjusted the change points by the QM algorithm. For more details on data
descriptions, the adopted methodology and downloading data, see
<uri>https://data.tpdc.ac.cn/en/data/45d73756-3f5a-4d27-82a4-952e268c20e8/</uri>
(last access: March 2022).</p>
</sec>
<sec id="Ch1.S2.SS1.SSSx3" specific-use="unnumbered">
  <title>(3) European homogenized SSR data</title>
      <p id="d1e804">A homogenized dataset of European SSR stations was developed by
Sanchez-Lorenzo et al. (2015)
and is currently available for full public download at <ext-link xlink:href="https://doi.org/10.1002/2015JD023321" ext-link-type="DOI">10.1002/2015JD023321</ext-link>.
They selected the 56 longest central European SSR series available in the GEBA
dataset with data for the period between 1922 and 2012. They adjusted them to ensure temporal homogeneity, homogenizing the data with the standard normal homogeneity test (Alexandersson, 1986) and the Craddock test     (Craddock, 1979).</p>
</sec>
<sec id="Ch1.S2.SS1.SSSx4" specific-use="unnumbered">
  <title>(4) Italian homogenized SSR dataset</title>
      <?pagebreak page4522?><p id="d1e816">The Italian homogenized SSR datasets are those published by  Manara et
al. (2019, 2016). As candidate stations to use as reference
series, they selected the 10 series located in the same area of the series to be tested, and that series correlates well with the test one. In particular, they tested the change points with the Craddock test
(Manara et al., 2017), and when a break is identified by more than one reference series, the preceding portion of the series is corrected, leaving the most recent portion unchanged. In this way, the SSR stations
were homogenized, and then the missing values were interpolated.
<?xmltex \hack{\newpage}?></p>
</sec>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Other datasets</title>
<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Reanalysis</title>
      <p id="d1e837">ERA5 can be used to fill in SSR data from the oceans and Antarctica and
carry out the global reconstruction, taking into account its high spatial
resolution and the reliable performance of SSR  (Jiao et al., 2022; Liang
et al., 2022). After the reconstruction, we removed the data for the ocean
reanalysis and maintained the data only in the land area (except for
Antarctica). In addition, two SSR data products (20CRv3, CMIP6) are used to
train AI models. These are the following.
<list list-type="order"><list-item>
      <p id="d1e842">ERA5 (space-filling data). ERA5 is the fifth generation of the European
Centre for Medium-Range Forecasts reanalysis product, which currently
publishes data from 1950 to the present  (Hersbach et al., 2020). In
addition, ERA5 has an hourly output and an uncertainty estimate from the
ensemble. The data are based on the Integrated Forecasting Model Cy41r2 run
in 2016, which contains a 4D-Var assimilation scheme. In ERA5, SSR is
obtained from a rapid radiation transfer model (RRTM)   (Mlawer et al., 1997). The present study utilizes monthly SSR data for the period
1955–2018 from ERA5 with a resolution of 0.25<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M40" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. They can be downloaded at
<uri>https://cds.climate.copernicus.eu</uri>  (last access: July 2022).</p></list-item><list-item>
      <p id="d1e874">20CRv3 (data for AI model training). The 20CR project is an effort led by the NOAA's Physical Sciences Laboratory and CIRES at the University of Colorado,
supported by the Department of Energy, to produce reanalysis datasets
spanning the entire 20th century and much of the 19th century
(Slivinski et al., 2019). 20CR provides a comprehensive global
atmospheric circulation dataset from 1850 to 2015. Its chief motivation is
to provide an observational validation dataset, with quantified
uncertainties, for assessing climate model simulations of the 20th century.
20CR uses an ensemble filter data assimilation method which directly
estimates the most likely state of the global atmosphere every 3 h and estimates the uncertainty in that analysis. The most recent version of
this reanalysis, 20CRv3, provides 8-times daily estimates of global
tropospheric variability across 75 km grids, spanning 1836 to 2015 (with an
experimental extension from 1806 to 1835). The present study uses monthly
SSR data of 20CRv3 (NOAA/CIRES/DOE 20CR, 80 members) from 1955 to 2015. We
selected all 80 members of the 20CR as input (1 for evaluation and to test
reconstruction, the other 79 for training the CNN model). The SSR of 20CRv3
has a spatial resolution of 0.7<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M43" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.7<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The download is available at <uri>https://portal.nersc.gov/archive/home/projects/incite11/</uri>  (last
access: May 2022).</p></list-item></list></p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <label>2.2.2</label><title>CMIP6 model output</title>
      <p id="d1e913"><list list-type="custom">
              <list-item><label>3.</label>

      <p id="d1e918">CMIP6 model output (data for AI model training). The Coupled Model
Intercomparison Project, driven by the World Climate Research Program, is
now in its sixth phase. Specifically, CMIP6 is considered the current state-of-the-art way of producing future climate simulations, including predicting
future SSR based on different climate scenarios (W. Zhou et al., 2018).
It provides an important resource for studying current and future climate
change (Eyring et al., 2016). The historical simulations of CMIP6 are
designed to reproduce observed climate and climate change constrained by
radiative forcing. CMIP6 historical simulation spans between 1850 and 2014. In
this study, we selected 125 members out of a total of 507 members from
several CMIP6 large-ensemble models (with more than 10 realizations and runs)
with high correlation coefficients with observations as input to train and
validate the CNN model (1 for evaluation and to test reconstruction, the
other 124 for training the CNN model). We selected the monthly downward
shortwave radiation from 1955 to 2014 (see Table S1 in the Supplement).  The data can be downloaded at <uri>https://esgf-node.llnl.gov/search/cmip6</uri> (last access: July 2022).</p>
              </list-item>
            </list></p>
</sec>
</sec>
</sec>
<?pagebreak page4523?><sec id="Ch1.S3">
  <label>3</label><title>Methods</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Data quality control (QC) and homogenization</title>
      <p id="d1e943">The SSR data homogenization method is only applied to the two non-homogenized
in situ observation datasets (GEBA and WRDC). The QC and homogenization flowchart (Fig. 1) is divided into three steps: (1) QC; (2) homogenization; and (3) integration and consolidation.</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="d1e948">Flowchart of quality control (QC) (first step), homogenization
(second step) and integration (third step).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f01.png"/>

        </fig>

<sec id="Ch1.S3.SS1.SSS1">
  <label>3.1.1</label><title>QC</title>
      <p id="d1e964">The QC of SSR data includes the following steps.
<list list-type="order"><list-item>
      <p id="d1e969">Simple integration is integration of the GEBA (2445) and WRDC (1136)
datasets, removing stations with no data and leaving 2681 stations.</p></list-item><list-item>
      <p id="d1e973">Removing duplicate stations. (a) For stations with similar latitude and
longitude, we consider two stations with totally identical latitude and
longitude to be the same station. (b) For stations less than 10 km apart, we
averaged the duplicate stations in these a and b cases. (c) For special duplicate
stations, we stitched together data of the duplicate stations based on
metadata from the CMA.</p></list-item><list-item>
      <p id="d1e977">Remove stations, years or months for which a climatic analysis cannot be
established: we remove stations with records of less than 10 years and
values more than 3 times (3<inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> criterion, Olanow and Koller, 1998) the standard deviation of the SSR anomalies.</p></list-item><list-item>
      <p id="d1e988">Candidate stations (487) with a record length greater than 15 years in
the period 1971–2000 are selected. We added stations (715) with more than 10 years of SSR records to increase the number of available stations for a
better homogenization of the candidate stations (Fig. 2).</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e993">Spatial distribution of candidate stations (“*”) and added
stations (“<inline-formula><mml:math id="M46" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>”). The different colour bars represent the length of the
station record in months.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f02.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <label>3.1.2</label><title>Station series homogenization</title>
      <p id="d1e1018">This paper uses the RHtestV4 software package to test and adjust the SSR
station data for homogeneity (<uri>http://etccdi.pacificclimate.org/software.shtml</uri>m last access: July 2021)  (Wang and Feng, 2013).
The package is based on the empirical penalty functions PMF  (Wang,
2008a) and PMT (Wang, 2008b; Wang et al., 2007) for the
homogenization test. It takes into account the lag-1 autocorrelation of the
time series. It embeds a multiple linear regression algorithm to
significantly reduce the problem of an unbalanced distribution of
pseudo-identification rates and test efficacy. Also, RHtestV4 uses the QM
algorithm  (Vincent et al., 2012; Wang et al., 2010) and mean adjustments to adjust the identified change points.</p>
      <p id="d1e1024">The specific steps are as follows.
<list list-type="custom"><list-item><label>1.</label>
      <p id="d1e1029">Building the reference series
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e1034">We processed the data from all station series (715) into the annual
first difference (FD) series <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Eq. 1)    (Peterson et al., 1998).</p></list-item><list-item><label>b.</label>
      <p id="d1e1049">We calculated the correlation of the annual FD series between the series
from the potential reference pool and the candidate stations.</p></list-item><list-item><label>c.</label>
      <p id="d1e1053">We calculated the distance between the potential reference pool stations
and candidate stations.</p></list-item><list-item><label>d.</label>
      <p id="d1e1057">We selected potential stations according to the correlation coefficient
(CC <inline-formula><mml:math id="M48" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M49" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.6) between the series from potential reference pool
and candidate stations. The potential stations also satisfy the limits
in distances (<inline-formula><mml:math id="M50" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M51" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 500 km) between the potential pool stations and
candidate stations.</p></list-item><list-item><label>e.</label>
      <p id="d1e1089">We obtain the reference FD series (Re) based on the <inline-formula><mml:math id="M52" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> potential reference
series (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Pe</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and the CCs (<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) between the
potential reference series (<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Pe</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and candidate
station series (Eq. 2).</p></list-item><list-item><label>f.</label>
      <p id="d1e1133">The synthesized reference FD series (Re) (Eq. 2), plus the average of
all potential reference series (<inline-formula><mml:math id="M56" display="inline"><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula>), yields the final annual reference series (<inline-formula><mml:math id="M57" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) (Eq. 3).</p>
      <p id="d1e1153"><disp-formula specific-use="gather" content-type="numbered"><mml:math id="M58" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">Pe</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msub><mml:mspace width="1em" linebreak="nobreak"/><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></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 class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">Re</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>m</mml:mi></mml:msubsup><mml:msub><mml:mi mathvariant="normal">Pe</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:msubsup><mml:mi>c</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mo>∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>m</mml:mi></mml:msubsup><mml:msubsup><mml:mi>c</mml:mi><mml:mi>i</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle></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 class="stylechange" displaystyle="true"/><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Re</mml:mi><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>R</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula><inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the raw observational station SSR in the year <inline-formula><mml:math id="M60" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>,
Re is the final reference series, Pe<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mi>i</mml:mi></mml:msub></mml:math></inline-formula> is the potential reference series, and <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the CC between the potential reference series and the candidate station series.</p></list-item></list></p></list-item><list-item><label>2.</label>
      <p id="d1e1334">Testing and adjusting the candidate series</p>
      <p id="d1e1337">The homogenization test algorithm used in this paper is the PMT. This method
is a reference series-dependent test for a normalized candidate series. It
assumes that the linear trend of the time series is zero and uses the degree
of mean deviation at different points in the series to find change points.
Furthermore, it eliminates the effect of different sample lengths on the
test results. At the same time, the method introduces an empirical penalty
factor, which effectively improves detection. We used the PMT to test the
homogeneity of the candidate series based on the reference series
established in (1). We then adjusted the statistically
significant (<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) change points obtained using the mean
adjustment method (<inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>). We homogenized the monthly series for 66 stations (see Fig. S1 in the Supplement).</p></list-item></list></p>
</sec>
<?pagebreak page4524?><sec id="Ch1.S3.SS1.SSS3">
  <label>3.1.3</label><title>Integration and consolidation</title>
      <p id="d1e1372">As can be seen from Fig. 1, the candidate stations (487) are relatively
sparse. To better adapt deep-learning methods for the dataset reconstruction
later, we adjusted, added and integrated station series based on the results
of homogenized data from other scholars. (1) We added stations with more than
10-year overall (1955–2018) records but no more than 15 years during the 1971–2000
period and removed those stations that were clearly inhomogeneous (25) and
some years of station (3). (2) We subsequently integrated monthly SSR series for 116 stations based on the results of homogenization from other
scholars: China (56), Japan (8), Europe (2) and Italy (50). After the above
steps, we ended up with a homogenized dataset containing 944 stations (Fig. 3). The details of the processing and classification are shown in Table S2
(see the Supplement).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1377">Spatial distribution of stations after homogenization (unit
months). Different colours represent the length of the station records in months.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f03.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>CNN model reconstruction methods</title>
      <p id="d1e1395">The CNN deep-learning model network architecture uses a U-shaped structure
similar to U-Net (Ronneberger et al., 2015). The advantage of using this model is that (1) both high- and low-frequency information of the picture can be<?pagebreak page4525?> retained, and when reconstructing the SSR data, not only will the grid point information close to the missing measurement point be considered, but information from more distant locations will be too (which may be remotely correlated with that missing measurement point). (2) This makes the
model convergence faster and more economical in terms of computational
resources. The upper part of the U-shaped structure, which has no downsamples or a low number of downsamples, represents the high-frequency information of the graph. These sections contain much of the detail in the
graph, and the relationships between similar grid points are conveyed by this
section. The lower half of the U-shaped structure is downsampled more often
and represents the lower-frequency information of the graph. The global
radiation of a wide range of undulations is transmitted by it, and then the
information at the various levels of the U-shaped structure is connected and
transmitted through the skip connection, allowing the whole network to
remember all the information of the picture very well. The model uses
nearest-neighbour upsampling in the decoding phase, and the skip links will
concatenate two feature maps and two masks as the feature and mask inputs
for the next part of the convolution layer. The input to the last part of
the convolution layer will contain the original input image concatenated
with the holes and the original mask, allowing the model to replicate the
gap-free pixels. The complex and variable nature of the sea–land boundary
then has a significant impact on the reconstruction when we reconstruct the
global land SSR data. Therefore, we use partial convolution at the image
boundaries with a suitable image padding, ensuring that the padding content
at the image boundaries is not affected by values outside the image. The
deep-learning models' convolutional layers and loss functions are described in the Supplement.</p>
      <p id="d1e1398">We further reconstruct a long-term (1955–2018) global SSR anomaly dataset
(SSRIH<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>) by using improved partial CNN deep-learning methods based
on a “perfect” dataset. A CNN consists of three parts: a convolutional layer
to reduce the number of weights by extracting local features, a pooling
layer to reduce peacekeeping and prevent overfitting, and a fully connected
layer to output the desired result. In this paper, a modified CNN is used to model the reconstruction of the SSR data, with the convolutional
layer replaced by a partial convolution method and mask update. This method
is the latest in image restoration effects and can restore irregular holes,
an advantage over other image restoration methods that can only restore
rectangular holes. Therefore, this paper uses the modified CNN model
(Kadow et al., 2020) to recover the missing part of the global
terrestrial SSR (except Antarctica). The specific reconstruction steps and
processes are as in Fig. 4.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1415">Flowchart of AI reconstruction.</p></caption>
          <?xmltex \igopts{width=441.017717pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f04.png"/>

        </fig>

<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Data pre-processing</title>
      <p id="d1e1432">The homogenized station data are converted to grid box anomalies using the
climate anomalies method (CAM) (Jones et al., 2001). CAM is a commonly
used method for converting station anomaly data to gridded data. We divide
all global areas into a 5<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M67" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid, after
which we calculate the SSR anomalies (relative to 1923–2020) within the grid
box by averaging the anomalies of all the stations (at least one station in it).
If more than one site exists in the same grid box, the record length of this grid box is the total length of all sites in that grid box.
Finally, we removed the values that were more than 3 times the standard
deviation of the SSR anomaly time series after gridding. SSRs are all
processed as daily average anomalies, i.e. monthly anomalies divided by 30
(each month is approximated as 30 d). We multiply all the values by 30 again when the reconstruction is complete. The global land (except for
Antarctica) distribution and coverage of SSRs after gridding are shown in
Fig. 5a, b.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1462"><bold>(a)</bold> Spatial distribution of 5<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M70" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid boxes
(SSRIH<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>) obtained by interpolating the homogenized global land (except
for Antarctica) SSR series. The different colours represent the length (the
sum of all the records) of the station record in unit years. <bold>(b)</bold> Grid box
coverage for the homogenized global land (except for Antarctica) SSR
(SSRIH<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>) except for Antarctica.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f05.png"/>

          </fig>

      <p id="d1e1520">As seen in Fig. 5a, the SSR is spatially sparsely distributed across South
America and Africa. As shown in Fig. 5b, SSR coverage increased yearly
from 1950 until the mid-1970s, when it slowly decreased. In 2013, the
coverage rate decreased sharply due to untimely data submission. Considering
the SSR coverage above, we only kept the years (1955–2018) with data
coverage of more than 8 % of global land (except for Antarctica) areas.</p>
      <?pagebreak page4526?><p id="d1e1524">Comparisons show that ERA5 has a high spatial resolution and relatively
reliable performance in the temporal variations and long-term trends
(Liang et al., 2022; Jiao et al., 2022). To obtain a higher data
coverage and ensure that the AI model runs well, we used the ERA5 to fill
the SSR of the homogenized global gridded SSR in the Antarctic and ocean areas.
However, if we use the SSR of ERA5 to directly fill the SSR of the homogenized
global gridded SSR (SSRIH<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>) in the Antarctic and in the ocean areas,
then the relatively weaker ocean SSR variations (variabilities, decadal
changes, trends) from ERA5 will inevitably introduce certain
systematic biases in land SSR reconstruction due to the SSRs having the lower
coverage on the land. Therefore, we designed an algorithm to avoid excessive
diffusion of SSR system bias in terrestrial areas: we first calculated the
ratios <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> between the SSR from ERA5 and from SSRIH<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>
on the land in all <inline-formula><mml:math id="M77" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> years. For a single grid box, the <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> have
small changes and are regarded as a constant <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Eq. 4),
and the <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> vary by latitude and longitude in both the marine
and land areas. We then extrapolated the <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for all the
grid boxes along the land and sea boundaries. If there is no observation
there, then the adjacent ocean ERA5 SSR is used to take its place after it
is adjusted according to the differences between the SSR variations
(represented by the linear trends) for the different underlying surfaces (Eq. 5):<?xmltex \hack{\newpage}?>

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M82" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="normal">median</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">OBS</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">land</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">ERA</mml:mi><mml:msub><mml:mn mathvariant="normal">5</mml:mn><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">land</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:msub><mml:mi mathvariant="normal">OBS</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="italic">&amp;</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mi mathvariant="normal">land</mml:mi></mml:mfenced></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">ERA</mml:mi><mml:msub><mml:mn mathvariant="normal">5</mml:mn><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="italic">&amp;</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:mi mathvariant="normal">ocean</mml:mi></mml:mfenced><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">O</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="1em"/><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi>n</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e1786"><inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">median</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the median value of the ratios of observation (OBS) and ERA5 land SSR series. OBS<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">land</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is the land SSR for the year <inline-formula><mml:math id="M85" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> from the SSRIH<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> in a single grid. ERA5<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">land</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is the land SSR for the year <inline-formula><mml:math id="M88" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> from ERA5 in a single
grid.
OBS<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="italic">&amp;</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>(land) is the land SSR along the sea–land boundary (land)
for the year <inline-formula><mml:math id="M90" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> from the SSRIH<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>.
ERA5<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi>i</mml:mi><mml:mi mathvariant="italic">_</mml:mi><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="italic">&amp;</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>(ocean) is the ocean SSR along the sea–land boundary for the year <inline-formula><mml:math id="M93" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> from ERA5.
<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">O</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the trend of the ERA5 SSR in ocean areas in all <inline-formula><mml:math id="M95" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> years, and
<inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the trend of the ERA5 SSR in areas in all <inline-formula><mml:math id="M97" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> years.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>AI model reconstruction</title>
      <p id="d1e1955">We use a server (configured with processor Intel (R) Core (TM) i7-8700 CPU @
3.20 GHz 3.19 GHz, RAM 32G, 64-bit OS, GPU model 516.94, NVIDIA GeForce 1080T
version, Python 3.9.12 64-bit, CUDA 10.1) for AI model training. The
specific training steps are as follows.
<list list-type="order"><list-item>
      <p id="d1e1960">A total of 768 missing-value masks (monthly masks between 1955 and 2018)
were prepared for training and validation using “1” for existing and “0” for
missing values.</p></list-item><list-item>
      <p id="d1e1964">The 20CRv3–CMIP6 training set (monthly values between 1955 and 2015/2014) and missing-value masks are fed into the 20CR-AI and CMIP6-AI model for
training.</p></list-item><list-item>
      <p id="d1e1968">We perform 1 500 000 training sessions with an interval of 10 000
sessions for the training output model.</p></list-item></list></p>
      <p id="d1e1971">Afterwards, the two AI models are validated against the root mean squared
error (RMSE) and CCs of the reconstructed SSRs (SSR<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula>SSR<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>).
The validation set SSRs, and the optimal number of training cycles is
1 100 000 (see Figs. S2,  S3 and S4 in the Supplement). The initial
hyperparameters of the model are set as follows: a learning rate of <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and
learning fine-tuning of <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. First, we set the batch size to 16 in the first
500 000 iterations and fine-tune it to 18 in the last 10 000 000 iterations,
for a total of<?pagebreak page4527?> 1 500 000 iterations, to suppress the overfitting phenomenon
generated during the training process. We validate the model every 10 000
times and with early stopping if the validation shows a decreasing trend, and the
final number of training times used is 1 100 000. Second, L2 (ridge regression) regularization is also added to regulate the loss function (see Eq. S9 in the Supplement).</p>
      <p id="d1e2037">The training result models generated by the different AI models are obtained
separately for the different training sets. The model is first used to
reconstruct a reanalysis validation set with the same missing-value mask as
the original observation dataset. This is followed by a validation of the
reconstruction against the original reanalysis dataset (calculation of CC
and RMSE) to understand the discrepancies in the model reconstruction.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Data homogenization and verification</title>
      <p id="d1e2050">We homogenized the original monthly station or gridded SSR time series
(SSRIH<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">station</mml:mi></mml:msub></mml:math></inline-formula> or SSRIH<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>) using the method in Sect. 3.1.2. We
selected six continental regions, excluding Antarctica and the Arctic, from
the eight continents of the world defined by Xu et al. (2018) (Asia, Africa, South America, Europe, North America, Australia,
Antarctica and the Arctic). The decreasing trend of the SSRIH<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> is
consistent with the original gridded SSR series (SSRI<inline-formula><mml:math id="M105" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>) during
1955–1991, while the increasing trend during 1991–2018 is weaker. At the
regional scale, the SSRIH<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> has a generally similar variation to the
SSRI<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>, and the SSRIH<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> is usually more representative of climate
change than the SSRI<inline-formula><mml:math id="M109" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> at individual stations.</p>
      <p id="d1e2126">Figure S5 (see the Supplement) illustrates the long-term variations of global
(Fig. S5a in the Supplement) and continental land SSR (Fig. S5b in the Supplement)
from the SSRI<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> and SSRIH<inline-formula><mml:math id="M111" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (except for Antarctica) during
1955–2018. The most prominent change revolves around the adjustment around
1992: the SSR anomalies were systematically adjusted upward from 1987 to
1992, while the SSR anomalies were systematically adjusted downward from
1993 onwards. Thus, there is a significant decreasing trend for both the global
land SSRI<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M113" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.995 <inline-formula><mml:math id="M114" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.251 W m<inline-formula><mml:math id="M115" 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> per decade) and global
land SSRIH<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M117" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.776 <inline-formula><mml:math id="M118" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.230 W m<inline-formula><mml:math id="M119" 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> per decade) (except for
Antarctica) from 1955 to 1991, while the increasing trend of the global land
SSRIH<inline-formula><mml:math id="M120" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> from 1991 to 2018 is 0.851 <inline-formula><mml:math id="M121" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.410 W m<inline-formula><mml:math id="M122" 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> per
decade, slightly smaller than the increasing trend of the SSRI<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>
(0.999 <inline-formula><mml:math id="M124" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.504 W m<inline-formula><mml:math id="M125" 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> per decade). It is worth noting that 1992
happened to be the second year of the eruption of Mount Pinatubo, and the
homogenized SSR data integrated in this paper may be affected by this event.
However, overall, the homogenization also has limited effects on the global SSR
variations from Fig. S5 (see the Supplement), which is consistent with the
influence of data homogenization on a wide range of surface air temperatures
(Brohan et al., 2006; Xu et al., 2013).</p>
      <p id="d1e2275">On the regional scale, the differences between the SSRIH<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> and
SSRI<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> are more pronounced in Asia and Europe (see Fig. S5b in the
Supplement). Asia's homogenized SSR shows that the regional average SSR has been
declining significantly over the period 1958–1990; this dimming trend mostly
diminished over the period 1991–2005 and was replaced by a brightening trend
in the recent decade. The SSRIH<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> in Asia is higher than the
SSRI<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> from 1985 to 1990 and lower than the SSRI<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> from 2012
to 2015. The SSRIH<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> shows a more moderate short-term increase in
Europe from 1960 to 1980. Note also that the Australian raw data prior to
1988 were artificially detrended because at the time the Australia Weather
Service was afraid that the instruments would drift. Therefore, they
detrended them and unfortunately did not store the raw data, and the SSR
evolution in Australia is artificial with no trend   (Wild et al.,
2005). In addition, the SSRI<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">station</mml:mi></mml:msub></mml:math></inline-formula> and SSRIH<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">station</mml:mi></mml:msub></mml:math></inline-formula> comparisons
for all 66 stations are shown in Fig. S1 (see the Supplement).</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>AI reconstruction and comparison</title>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Training of the AI model</title>
      <p id="d1e2367">We produce two (20CRv3 and CMIP6) separate training and validation sets: we
select the first member data of the reanalysis data and the model data,
respectively, as the validation set, and the remaining 79 (124) ensemble
members as the training sets, where each ensemble member included 732 (720)
months of SSR data. Each validation set included 732 (720) samples, while
the training sets contained 57 828 (89 280) ensemble members. All the above
data, including the in situ observations, are then resampled to monthly anomalies
of 5<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M135" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. We reconstruct the SSR of 20CRv3 and CMIP6 with missing values based on the 20CRv3 and CMIP6 datasets using the method in Sect. 3.2 and obtain two
reconstructions, SSR<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and SSR<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, respectively. The SSR of
20CRv3 and CMIP6 with missing values uses the SSRIH<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> mask between 1955
and 2015/2014. We compare the global land (except for Antarctica) or regional
annual anomaly variation of SSR<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> or SSR<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. The results show
that SSR<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is significantly more consistent with the validation set
than SSR<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>.</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="d1e2479">Reconstruction capabilities of the AI model.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f06.png"/>

        </fig>

      <p id="d1e2488">Figure 6a shows that the RMSE and CC of the SSR<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (0.247 W m<inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula>0.970 W m<inline-formula><mml:math id="M146" 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>) are smaller or larger than those of the SSR<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (0.518 W m<inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>/</mml:mo></mml:mrow></mml:math></inline-formula>0.937 W m<inline-formula><mml:math id="M149" 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>) with the original 20CR and CMIP6 dataset. The 20CR-AI model has a better reconstruction ability for SSR on the global land (except for Antarctica) scale. The RMSEs of the SSR<inline-formula><mml:math id="M150" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (SSR<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>)
are 1.460 (2.413) W m<inline-formula><mml:math id="M152" 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>, 1.109 (1.829) W m<inline-formula><mml:math id="M153" 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>, 2.219 (2.596) W m<inline-formula><mml:math id="M154" 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> and 1.286 (2.235) W m<inline-formula><mml:math id="M155" 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> in North America, Europe, Asia and the Northern Hemisphere, whereas these values are 1.116 (1.766) W m<inline-formula><mml:math id="M156" 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>, 0.622
(1.602) W m<inline-formula><mml:math id="M157" 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>, 1.877 (1.839) W m<inline-formula><mml:math id="M158" 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> and 0.772 (1.679) W m<inline-formula><mml:math id="M159" 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> in
South America, Africa, Australia and the Southern Hemisphere, respectively, concerning the
original 20CR and CMIP6 dataset. In other words, the RMSEs of the
SSR<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> are smaller than those of the SSR<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> for the original 20CR and CMIP6 dataset except for Australia. In addition, the CCs of the
SSR<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (SSR<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>) are 0.958 (0.830) W m<inline-formula><mml:math id="M164" 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>, 0.958 (0.987) W m<inline-formula><mml:math id="M165" 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>, 0.886 (0.669) W m<inline-formula><mml:math id="M166" 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>, 0.930 (0.965) W m<inline-formula><mml:math id="M167" 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>, 0.938 (0.930) W m<inline-formula><mml:math id="M168" 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>, 0.943 (0.916) W m<inline-formula><mml:math id="M169" 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>, 0.936 (0.875) W m<inline-formula><mml:math id="M170" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2<?pagebreak page4528?></mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and 0.903
(0.822) W m<inline-formula><mml:math id="M171" 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> in North America, Europe, Asia, the Northern Hemisphere, South
America, Africa, Australia and the Southern Hemisphere, respectively, with respect to the
original 20CR and CMIP6 dataset. That is, the CCs of the
SSR<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> are larger than those of the SSR<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> with the original 20CR and CMIP6 dataset except for Europe.</p>
      <?pagebreak page4529?><p id="d1e2863">Based on the above comparison, the higher uncertainty for CMIP6 model output
possibly biases the CMIP6-AI method. Thus, the accuracy of the SSR<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
is higher than that of the SSR<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mi mathvariant="normal">CMIP</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> at both global land (except for
Antarctica) and regional scales. Therefore, we choose the reconstruction
results of the 20CR-AI model as the final AI reconstruction dataset, and
subsequent analysis in the following sections is only based on this dataset.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Comparison of the spatial and temporal variation characteristics</title>
      <p id="d1e2898">We investigate the long-term trends and spatial and temporal variation of
the SSRIH<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, compare the differences between the SSRIH<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and
SSRIH<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>, and suggest that the area and magnitude of the high and low
centres of the SSRIH<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> are the same as those of the SSRIH<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>. The results of the global land (except for Antarctica) reconstruction are
consistent with dimming and brightening; the global dimming is primarily
dominated by decreasing trends in Asia, Europe, Africa and North America,
whereas Europe and North America are contributors to the increasing trends.</p>
      <p id="d1e2955">Figure 7 shows the spatial distribution of the SSRIH<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> and
SSRIH<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> for the 3 months (July 1960, July 1980 and July 2000).
Figure S6 (see the Supplement) displays the spatial distribution of the annual
SSRIH<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> and SSRIH<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> from 1955 to 2018. Figure 7 also shows that the area and the magnitude of the high and low centres in the SSRIH<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> are
the same as in the SSRIH<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>. The SSRIH<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> has mainly positive
anomalies in Africa and the Eurasian continent in July 1960, especially in
India and the Middle East. Afterwards, India showed a continuous and steady
decline in SSR. This confirms the well-known phenomenon of global dimming
over India  (Wild et al., 2009; Soni et al., 2016, 2012;
Padma Kumari et al., 2007; Kambezidis et al., 2012). In Australia, the
SSRIH<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> is dominated by negative anomalies in July 1980 and positive
anomalies in July 1960 and July 2000. In Greenland, the SSRIH<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> shows
a large positive anomaly during 3 months. In northern Russia, there is a
high value in July 2000. The reconstruction can better reflect the anomaly
distribution of observation information, and the grid boxes with the missing
values are infilled and reconstructed, which has high reliability.</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="d1e3060">Spatial distribution of the SSRIH<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> <bold>(a1–3)</bold> and
SSRIH<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> <bold>(b1–3)</bold> in typical months: 1–3 are July 1960, July 1980, and
July 2000, respectively.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f07.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e3099">Global land (except for Antarctica) time series of the annual
anomaly variations' SSR (relative to 1971–2000) before and after reconstruction.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f08.png"/>

        </fig>

      <p id="d1e3108">Figure 8 illustrates the global land (except for Antarctica) annual anomaly
variation and long-term trend of the SSRIH<inline-formula><mml:math id="M192" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> for the periods of
1955–2018, 1955–1991 and 1991–2018. Table S3 in the Supplement demonstrates the
trends of global SSR change evaluation for various data sources on different
scales. Also, we compare the differences between the SSRIH<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and
SSRIH<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>. The minimum value of the SSRIH<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> occurred in 1991
(<inline-formula><mml:math id="M196" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>2.411 W m<inline-formula><mml:math id="M197" 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>). The decreasing trend of the SSRIH<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> from 1955 to
1991 (<inline-formula><mml:math id="M199" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.276 <inline-formula><mml:math id="M200" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.205 W m<inline-formula><mml:math id="M201" 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> per decade) is slightly lower than that
of the SSRIH<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M203" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.776 <inline-formula><mml:math id="M204" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.230 W m<inline-formula><mml:math id="M205" 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> per decade). After
that, the SSRIH<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> turns to an increasing trend of 0.697 <inline-formula><mml:math id="M207" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.359 W m<inline-formula><mml:math id="M208" 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> per decade from 1991 to 2018. This suggests that the difference
between the SSRIH<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and SSRIH<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> may be caused by the results
observed in limited data coverage (such as in Africa and North America)
(Fig. 9). After homogenization and reconstruction, the trend (<inline-formula><mml:math id="M211" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.276 W m<inline-formula><mml:math id="M212" 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> per decade) from 1955 to 1991 corresponds to an overall reduction
of <inline-formula><mml:math id="M213" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.6 W m<inline-formula><mml:math id="M214" 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> over the dimming period, while that (0.697 W m<inline-formula><mml:math id="M215" 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> per
decade) from 1991 to 2018 corresponds to an overall increase of 2 W m<inline-formula><mml:math id="M216" 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>
over the brightening period. This is in amazing agreement with the <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> W m<inline-formula><mml:math id="M218" 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> for the dimming period and the 2 W m<inline-formula><mml:math id="M219" 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> for the brightening
period based on an overall surface energy budget assessment (Wild,
2012; see their Fig. 1). Also, similar conclusions (incomplete coverage of
observational data leads to an underestimation of global warming trends) have
been confirmed in global warming research  (Gulev et al., 2021; Li et al.,
2021).</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="d1e3402">Same as Fig. 8 but for regional annual anomaly variations.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/15/4519/2023/essd-15-4519-2023-f09.png"/>

        </fig>

      <p id="d1e3411">Figure 9 demonstrates the long-term annual anomaly variations of the
SSRIH<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> in different regions and its results compared to the
SSRIH<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>. Table S4 in the Supplement shows the evaluation in continental and
hemispheric SSRIH<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> change trends on different scales. The
SSRIH<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> shows a similar annual anomaly variation to the global land
(except for Antarctica) average trend in North America and Asia, reaches a
minimum in the late 1970s or early 1990s, and follows a moderate reversal.
In Europe, the SSRIH<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> shows a decrease (<inline-formula><mml:math id="M225" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>2.180 <inline-formula><mml:math id="M226" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.866 W m<inline-formula><mml:math id="M227" 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> per decade) between 1963 and 1978 before turning to brightening
(1.081 <inline-formula><mml:math id="M228" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.312 W m<inline-formula><mml:math id="M229" 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> per decade). In South America and Australia
(Southern Hemisphere), the SSRIH<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> shows no significant variation. In
Africa, the SSRIH<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> has a dimming trend (<inline-formula><mml:math id="M232" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.506 <inline-formula><mml:math id="M233" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.496 W m<inline-formula><mml:math id="M234" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> per decade) from the 1950s to the 1990s, after which it remains
levelled off (0.340 <inline-formula><mml:math id="M235" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.998 W m<inline-formula><mml:math id="M236" 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> per decade). The SSRIH<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>
shows a decreasing trend (<inline-formula><mml:math id="M238" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.457 <inline-formula><mml:math id="M239" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.246 W m<inline-formula><mml:math id="M240" 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> per decade) until
the 1990s in the Northern Hemisphere and a brightening (0.887 <inline-formula><mml:math id="M241" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.415 W m<inline-formula><mml:math id="M242" 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> per decade) afterwards. The annual average anomaly variations in
regions and globally show that Asia, Africa, Europe and North America are
the four contributors to the global dimming, while Europe and North America
are two major contributors to the brightening. This is in general agreement with the results obtained by previous machine learning  (Yuan
et al., 2021). In addition, the discrepancy between the SSRIH<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> and
SSRIH<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> is more significant in low-coverage areas (right) than in
high-coverage regions (left). It is particularly pronounced before 1980 and
in South America. This suggests that the limited surface observations are
not representative of the continental variation in SSR.</p>
      <p id="d1e3664">The sources of error in the observational dataset can be divided into three
types. (1) Station errors are the uncertainties of individual station anomalies, including measurement errors (which are not the focus of the considerations
in this paper) and errors due to homogenization. The errors due to
homogenization adjustment are always approximately normally<?pagebreak page4530?> distributed
(Jones et al., 2008; see their Fig. 5 and Fig. S9 in the Supplement) and therefore have limited impacts on the global average SSR change
(Fig. S5a, b). (2) Sampling errors are the uncertainties in a grid box mean
caused by estimating the mean from a small number of point values
(Jones et al., 1997). (3) Bias error generally refers to systematic errors such as urbanization, which has not been discussed here. However, even the sum of the above errors is much smaller
than the errors due to limited data coverage (Li et al., 2010; see their Fig. 5). So, the focus of this study is to eliminate this kind of
error through the CNN reconstruction.</p>
</sec>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Data availability</title>
      <?pagebreak page4531?><p id="d1e3676">Both the SSRIH<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula> (the homogenized monthly gridded SSR data over
1923–2020) and the SSRIH<inline-formula><mml:math id="M246" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> (the monthly 20CR-AI model reconstructed
SSR data for 1955–2018) are currently publicly available on the figshare
website at <ext-link xlink:href="https://doi.org/10.6084/m9.figshare.21625079.v1" ext-link-type="DOI">10.6084/m9.figshare.21625079.v1</ext-link>    (Jiao and Li, 2023). These datasets are also available at <uri>http://www.gwpu.net</uri> (last access: May 2023)
for free.
<?xmltex \hack{\newpage}?></p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Conclusions</title>
      <p id="d1e3715">In this study, we integrate global station observations based on the raw
observational SSRs from GEBA and WRDC, combined with existing homogenized
SSR datasets from other scholars. Also, we homogenize the globally
distributed station data using the RHtestV4 software package. An improved
CNN deep-learning algorithm is subsequently used to reconstruct the SSR
anomalies. Thus, a reconstructed SSR anomaly dataset, SSRIH<inline-formula><mml:math id="M247" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula>, is
obtained based on training sets (20CRv3) for the years 1955–2018, with a
resolution of 5<inline-formula><mml:math id="M248" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M249" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M250" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The main results are
as follows.
<list list-type="order"><list-item>
      <p id="d1e3757">The first integrated and homogenized global SSR monthly dataset is
developed, which contains 944 stations in total and covers the longest
periods (from the 1920s to recent years). A 5<inline-formula><mml:math id="M251" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M252" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5<inline-formula><mml:math id="M253" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid box version of the monthly SSR anomaly dataset is derived.</p></list-item><list-item>
      <p id="d1e3786">This paper develops 5<inline-formula><mml:math id="M254" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M255" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 2.5<inline-formula><mml:math id="M256" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> full-coverage
monthly land (except for Antarctica) SSR anomaly reconstructed datasets
based on the above observations, using 20CRv3 to train the AI model.
Comparative validations and evaluations show that the SSRIH<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn mathvariant="normal">20</mml:mn><mml:mi mathvariant="normal">CR</mml:mi></mml:mrow></mml:msub></mml:math></inline-formula> provides a
reliable benchmark for global SSR variations.</p></list-item><list-item>
      <p id="d1e3827">On average, the global annual SSR variations based on the SSRIH<inline-formula><mml:math id="M258" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">grid</mml:mi></mml:msub></mml:math></inline-formula>
are not significantly different, except that the increasing (brightening)
trend after 1991 is a little smaller for the latter. The short-term
brightening SSR in Europe from the 1970s to the 1980s disappears at the
regional scale. At the same time, the brightening SSR after the 1990s in
Asia slowed or was delayed.</p></list-item></list></p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p id="d1e3838">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/essd-15-4519-2023-supplement" xlink:title="zip">https://doi.org/10.5194/essd-15-4519-2023-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3849">BJ: software, data curation, writing – original draft preparation,
visualization, investigation. YS: software, data curation.
QL: methodology, supervision, conceptualization, validation, writing – review and editing.
VM: provision of the homogenized Italian dataset, writing – review and editing.
MW: writing – review and editing.</p>
  </notes><?xmltex \hack{\newpage}?><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3856">At least one of the (co-)authors is a member of the editorial board of
<italic>Earth System Science Data</italic>. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3865">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="d1e3871">This research has been supported by  the Natural Science Foundation of China (grant no. 41975105) and the National Key R&amp;D Program of China (grant nos. 2018YFC1507705 and
2017YFC1502301). The Global Energy Balance Archive (GEBA) is co-funded by the Federal Office of Meteorology and Climatology
(MeteoSwiss) within the framework of GCOS Switzerland. Global dimming and brightening research at ETH Zurich is supported by the Swiss National Science Foundation (grant no. 200020 188601). Veronica Manara was supported by the Ministero dell'Università e della Ricerca of Italy (grant FSE – REACT EU, DM 10/08/2021 n.
1062).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3877">This study is supported by the Natural Science Foundation of China (grant no.
41975105) and the National Key R&amp;D Program of China (grant nos.
2018YFC1507705 and 2017YFC1502301). The Global Energy Balance Archive (GEBA) is
co-funded by the Federal Office of Meteorology and Climatology (MeteoSwiss)
within the framework of GCOS Switzerland. Global dimming and brightening
research at ETH Zurich is supported by the Swiss National Science Foundation (grant no. 200020 188601). Veronica Manara was supported by the
Ministero dell'Università e della Ricerca of Italy (grant FSE – REACT EU, DM 10/08/2021 n. 1062).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3883">This paper was edited by Jing Wei and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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