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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</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/acp-22-15867-2022</article-id><title-group><article-title>An assessment of land energy balance over East Asia from multiple lines of evidence and the roles of the Tibet Plateau, aerosols, and clouds</article-title><alt-title>An assessment of land energy balance over East Asia from multiple lines of evidence​​​​​​​</alt-title>
      </title-group><?xmltex \runningtitle{An assessment of land energy balance over East Asia from multiple lines of evidence​​​​​​​}?><?xmltex \runningauthor{Q. Wang et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Wang</surname><given-names>Qiuyan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8425-4256</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Zhang</surname><given-names>Hua</given-names></name>
          <email>huazhang@cma.gov.cn</email>
        <ext-link>https://orcid.org/0000-0001-9165-8649</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Yang</surname><given-names>Su</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Chen</surname><given-names>Qi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zhou</surname><given-names>Xixun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Xie</surname><given-names>Bing</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wang</surname><given-names>Yuying</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9762-8563</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff6">
          <name><surname>Shi</surname><given-names>Guangyu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <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>Collaborative Innovation Center on Forecast and Evaluation of
Meteorological Disasters, Nanjing University of Information Science and Technology, Nanjing 210044, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>State Key Laboratory of Severe Weather, Chinese Academy of
Meteorological Sciences,<?xmltex \hack{\break}?> Beijing 100081, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute for Atmospheric and Climate Science, ETH Zurich, 8092
Zurich, Switzerland</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>National Meteorological Information Center, China Meteorological
Administration, Beijing 100081, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Laboratory for Climate Studies of China Meteorological
Administration,<?xmltex \hack{\break}?> National Climate Center, Beijing 100081, China</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>State Key Laboratory of Numerical Modeling for Atmospheric Sciences
and Geophysical Fluid Dynamics, Institute of Atmospheric Physics, Chinese
Academy of Sciences, Beijing 100029, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Hua Zhang (huazhang@cma.gov.cn)</corresp></author-notes><pub-date><day>19</day><month>December</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>24</issue>
      <fpage>15867</fpage><lpage>15886</lpage>
      <history>
        <date date-type="received"><day>24</day><month>June</month><year>2022</year></date>
           <date date-type="rev-request"><day>27</day><month>June</month><year>2022</year></date>
           <date date-type="rev-recd"><day>30</day><month>October</month><year>2022</year></date>
           <date date-type="accepted"><day>8</day><month>November</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e194">With high emissions of aerosols and the known world's “Third Pole” of the Tibet Plateau (TP) in East Asia, knowledge on the energy budget over this region has been widely concerned. This study first attempts to estimate the present-day land energy balance over East Asia by combining
surface and satellite observations as well as the atmospheric reanalysis and Coupled Model Intercomparison Project Phase 6 (CMIP6) simulations.
Compared to the global land budget, a substantially larger fraction of
atmospheric shortwave radiation of 5.2 % is reflected, highly associated with the higher aerosol loadings and more clouds over East Asian land. While a slightly smaller fraction of atmospheric shortwave absorption of 0.6 % is unexpectedly estimated, possibly related to the lower water vapor content effects due to the thinner air over the TP to overcompensate for the aerosol
and cloud effects over East Asian land. The weaker greenhouse effect and
fewer low clouds due to the TP are very likely the causes of the smaller fraction of East Asian land surface downward longwave radiation. Hence, high
aerosol loadings, clouds, and the TP over East Asia play vital roles in the
shortwave budgets, while the TP is responsible for the longwave budgets
during this regional energy budget assessment. The further obtained cloud
radiative effects suggest that the presence of clouds results in a larger
cooling effect on the climate system over East Asian land than that over the globe. This study provides a perspective to understand fully the roles of
potential factors in influencing the different energy budget assessments
over regions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e206">Current patterns of Earth's weather and climate are largely determined by
the spatiotemporal distributions of energy exchanges between the surface,
atmosphere, and space. Theoretically, the outgoing longwave radiation (OLR)
is balanced by the incoming and reflected solar radiation at the top of the
atmosphere (TOA) to produce an equilibrium climate. The incoming solar
radiation can be scattered by clouds and aerosols or absorbed by the
intermediary atmosphere, thereby contributing to the diverse energy
transformation at the surface (Trenberth et al., 2009; Wild et al., 2013a).
The Earth's surface energy balance is of particular significance because it
is the key driver of atmospheric and oceanic circulations, hydrological
cycles, and various surface processes (Wild et al., 2008; Mercado et al.,
2009; Wild et al., 2013a; L'Ecuyer et al., 2015). Anthropogenic influences
on climate change are driven by the uneven distribution of the TOA net
radiation caused by forcings perturbed by variations of the atmospheric
composition of greenhouse gases and aerosols as well as aerosol–cloud interactions (Trenberth et al., 2009; Stephens et al., 2012; Wild et al.,
2013a; Trenberth et al., 2014; L'Ecuyer et al., 2015; Wild et al., 2019; Z. Wang et al., 2021).</p>
      <p id="d1e209">Many efforts have been made to quantify the magnitudes of different
radiative components or energy budgets in the climate system over a range of
time–space scales, such as on global scales (Lin et al., 2008; Trenberth et al., 2009; Stephens et al., 2012; Wild et al., 2013b, 2015;
L'Ecuyer et al., 2015; Wild et al., 2019; Wild, 2020), over land and ocean
domains or the energy transport between them (Fasullo and Trenberth, 2008a,
b; Trenberth et al., 2009; Wild et al., 2015; L'Ecuyer et al., 2015), over
the Arctic (Previdi et al., 2015; Christensen et al., 2016), and over
individual continents and ocean basins (L'Ecuyer et al., 2015; Kim and Lee,
2018; Thomas et al., 2020). The energy balance at the TOA can be accurately
monitored by satellites from the most advanced Clouds and the Earth's
Radiant Energy System (CERES) Energy Balanced and Filled (EBAF) data product
(Loeb et al., 2018), while considerably larger uncertainties appear at the
surface fluxes owing to weaker observational constraints (Raschke et al.,
2016; Kato et al., 2018; Huang et al., 2019). These assessments mostly build
upon complementary approaches from a combination of space and surface
observations, climate models, and reanalyses. To date, the discrepancies of
independent global mean surface radiative fluxes have been estimated to be within a few W m<inline-formula><mml:math id="M1" 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> (Wild, 2017a, b), enabling the accurate quantification of
global surface budgets. Besides, the surface radiative components simulated by various climate models vary substantially in a range of around
10–20 W m<inline-formula><mml:math id="M2" 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> on global scales but exhibit greater inter-model discrepancies on regional scales (Li et al., 2013; Wild et al., 2013a; Boeke
and Taylor, 2016; Wild et al., 2015; Wild, 2017a, b, 2020). Existing
challenges in the surface energy estimates include considerable uncertainties from surface albedo and skin temperature as well as the partitioning of surface net radiation into sensible and latent heat (SH; LH)
(Wild, 2017a, b).</p>
      <p id="d1e236">Due to the large population and the largest emission source of aerosols and
their precursors, East Asia, especially China, has long been a hotpot in
climate change research. Aerosols can interact with radiation directly by
scattering and absorbing solar/thermal radiation (Ghan et al., 2012) and
indirectly by modifying cloud microphysical properties and lifetimes (Li et
al., 2011), thereby influencing Earth's radiation balance. As the world's
largest and highest plateau, the Tibet Plateau (TP) covers nearly one-fifth of the East Asian land area, significantly affecting the atmospheric
circulation, energy budget, and water cycles of the climate system through its orographic and thermal effects (Liu et al., 2007; Xu et al., 2008a, b; Wu et
al., 2015). Deeper insights into the energy budget differences over East
Asian and global land against the background of high aerosol emissions and the TP role in East Asia are meaningful and essential attempts. Moreover, clouds play a key role in modulating global and regional energy
budgets and hydrological cycles by increasing the reflected solar radiation and also the downward thermal radiation, leading to a cooling and
warming of the climate system (Stephens, 2005; Wild et al., 2013a; Li and Mao, 2015; H. Wang et al., 2021). Therefore, our emphasis in this study is on the
regional characterization of the East Asian energy balance under both
all-sky and clear-sky conditions based on a combination of surface
observations, satellite-derived products, reanalysis, and Coupled Model
Intercomparison Project Phase 6 (CMIP6) models. The cloud influence on the radiative energy budgets at the TOA, within the atmosphere, and at the
surface is further quantified over this region. Section 2 introduces the
different data sources used in this study, including surface and satellite
observations, climate models, and reanalyses. Sections 3 and 4 provide detailed analyses of the all-sky and clear-sky estimates of the energy
balance components. The inferred cloud radiative effects (CREs) at the TOA,
within the atmosphere, and at the surface are presented in Sect. 5.
A summary and conclusions are given in Sect. 6. The present day in this study represents the years of 2010–2014, which correspond to the last 5 years of the historical simulations in CMIP6 climate models. East Asian land
as considered in this study consists of five countries, i.e., China, Japan, South and North Korea, as well as Mongolia.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data sources</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Surface observations</title>
      <p id="d1e254">Considering the efforts to diminish the inhomogeneities in the measurement
of ground-based surface (downward) solar radiation (SSR) (Tang et al., 2011;
Wang, 2014; Wang et al., 2015; Wang and Wild, 2016; He et al., 2018; Yang et
al., 2018, 2019) and the large number of observational stations over China, the homogenized monthly all-sky and clear-sky SSR datasets from the China
Meteorological Administration (CMA) National Meteorological Information
Center (NMIC) are used in this study (<uri>http://data.cma.cn/enl</uri>, last access: 10 February 2022) (Yang et al.,
2018, 2019). In this dataset, the clear-sky condition at observational sites
is defined based on the measured cloud fraction per day of no more than
15 % (Yang et al., 2018). Taking clear-sky data (with relatively complex
missing months compared to the all-sky dataset) as an example, sites with
more than 1 year of <inline-formula><mml:math id="M3" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 2 missing months were deleted to ensure <inline-formula><mml:math id="M4" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4 years of available data during the period 2010–2014, and then the
spline interpolation was performed on the missing months of the selected
sites. As a consequence, 99 and 76 sites are available for the all-sky and
clear-sky studies, respectively. Besides, to further explore the anthropogenic influence on SSR, 84 (62) urban and 15 (14) rural stations for all-sky (clear-sky) conditions are defined according to the administrative
divisions of China (Wang et al., 2017).</p>
      <p id="d1e274">For the remaining East Asian sites, we use the monthly Global Energy Balance
Archive (GEBA) dataset (<uri>http://www.geba.ethz.ch</uri>, last access: 25 February 2022) (Wild et al., 2017), which
contains a worldwide widespread distribution of monthly data from many
sources, e.g., from the World Radiation Data Center (WRDC) or the Baseline Surface Radiation Network (BSRN). Among these data sources, the BSRN
dataset has a much higher precision and temporal resolution (up to 1 min)
compared to the GEBA, but its site number is very limited over East Asia
(only a few sites located in Japan and one site in Xianghe, China, but with
no data available during this study period). Moreover, the relative random
error of the monthly SSR from the GEBA data evaluated by Gilgen et al. (1998) is 5 %.</p>
      <p id="d1e280">In order to retain as many sites as possible during the study period, we
widen the selection criterion of the GEBA data, i.e., sites with data <inline-formula><mml:math id="M5" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 4 years and missing months <inline-formula><mml:math id="M6" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 3. Eventually, 8, 2, 4, and 14 sites are
selected from the GEBA in China, Mongolia, South and North Korea, and Japan, respectively. In particular, among the 14 sites in Japan, five pairs of the duplicate sites are obtained from the WRDC and BSRN sources, respectively,
and the remaining 4 sites are only from the WRDC (9 sites available). For China, only 1 site from Hong Kong out of 8 GEBA sites is not repetitive from the abovementioned CMA sites (1 site available). Therefore, 16 out of 28 GEBA sites are available under all-sky conditions (including 15 sites over
regions outside China and 1 site over Hong Kong, China) by taking the average of these duplicate sites in Japan instead, while the clear-sky reference
sites are obtained from the interpolated CERES EBAF clear-sky estimates at
the GEBA sites (also 16 sites) due to the limited numbers of observational
sites over these regions. Additionally, we regard four island sites in Japan
as rural stations (not shown in the figures), while the sites in Mongolia as
well as South and North Korea are all urban sites.</p>
      <p id="d1e297">As shown in Fig. S1 in the Supplement, there are 99 (rural/total: 15/99) and 16 (rural/total: 4/16) sites from the CMA and GEBA available under all-sky conditions, respectively, whereas 76 (rural/total: 14/99) and 16 (from the
CERES-interpolated data at the 16 GEBA sites) sites are considered for
clear-sky conditions, respectively. More detailed station information is
given in Table S1.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Satellite observation</title>
      <p id="d1e308">Owing to the excellent temporal and spatial coverage of satellite
instruments, CERES data products are widely used to track variations of
Earth's energy budgets. The newly released CERES EBAF Edition 4.1 with a
monthly 1<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M8" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude–longitude resolution is used in this study (<uri>https://ceres.larc.nasa.gov/data/</uri>, last access: 20 March 2022). In this dataset,
the TOA radiation components are adjusted within their uncertainty ranges
based on the independent observational ocean estimates of the global heating rate (Loeb et al., 2018). Unlike the directly measured TOA energy budget,
the EBAF surface energy fluxes are calculated by the cloud and aerosol properties from satellite-derived products as well as the atmospheric
profiles from reanalysis, with a lower accuracy than their TOA counterparts
(Kato et al., 2018). The uncertainty ranges in 1<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M11" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> regional monthly all-sky and clear-sky longwave (LW) and shortwave (SW) radiation fluxes at the TOA are also documented by Loeb et al. (2018).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Climate models and reanalysis</title>
      <p id="d1e373">Data from 40 CMIP6 climate models are used for the analyses in this study, with their model abbreviations, modeling groups, and resolutions in Table S2. A detailed description of the modeling groups participating in CMIP6 is
provided at <uri>https://pcmdi.llnl.gov/CMIP6/</uri> (last access: 14 April 2022). The CMIP6 model-calculated
radiation fluxes under investigation for this study include energy budgets
under both all-sky and clear-sky conditions from “historical all forcings”
experiments covering the period 2010–2014. In these historical simulations,
both natural (e.g., solar variability and volcanic aerosols) and
anthropogenic (e.g., greenhouse gases, aerosols, and land use) forcings are
considered to reproduce the climate change and evolution since preindustrial
times as accurately as possible (Eyring et al., 2016). Only the first
ensemble member of each model is selected for the analysis, and the model numbers vary slightly among different available energy components.</p>
      <p id="d1e379">In the long history of the European Centre for Medium-Range Weather Forecasts (ECMWF), ERA5 is the fifth-generation product. It is a comprehensive reanalysis from 1959 to near real time, which assimilates as many
observations as possible in the upper air and near surface
(<uri>https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5</uri>, last access: 22 May 2022).
Monthly means of the radiative components from ERA5 are used in this study
with a resolution of 0.25<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M14" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.25<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (regridded
to 1<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M17" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). Compared to previous reanalyses
(such as ERA-Interim), a major strength of ERA5 is the much higher temporal
and spatial resolutions as well as a higher vertical resolution with 137 levels (Hersbach et al., 2020). Several independent studies have evaluated
the performance of ERA5 since its release. For example, excellent closure of
the Arctic energy budget based on ERA5 atmospheric data has been assessed by
Mayer et al. (2019). The representation of the surface irradiance of ERA5 has been compared with other reanalyses and with ground and satellite
observations (Trolliet et al., 2018; Urraca et al., 2018). Specifically,
Trolliet et al. (2018) found that the surface solar irradiance over the
tropical Atlantic Ocean from ERA5 exhibits fewer biases than the second
version of the Modern-Era Retrospective Analysis for Research and
Applications (MERRA-2). Urraca et al. (2018) reported that ERA5 can be a
valid alternative for satellite-derived products in terms of surface
irradiance in most inland stations compared to ERA-Interim or MERRA-2.
Furthermore, based on BSRN station data, Tang et al. (2021) pointed out that
the accuracy of ERA5 over land in terms of surface downward longwave radiation is higher than the CERES-derived product on average at both hourly and monthly timescales.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Assessment of land energy balance budgets under all-sky conditions</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Shortwave components</title>
      <p id="d1e452">Under all-sky conditions, the present-day annual land mean anomalies of TOA incident solar radiation as well as the SW net radiation at the TOA, within the atmosphere, and at the surface regarding their respective multi-model means as simulated by various CMIP6 models over East Asia are shown in Fig. 1a. A summary of the CMIP6 model statistics (such as the available model number, the model spread, and the standard deviation – SD) along with the corresponding multi-model mean as well as ERA5- and CERES-derived estimates of different energy balance components is listed in Table 1. As shown in Fig. 1a, with the exception of the BCC-CSM2-MR and BCC-CESM1 models, all models give an
estimate around 334 W m<inline-formula><mml:math id="M19" 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 TOA incoming solar radiation with a very
small SD of 0.2, closely matching the multi-model mean as well as the CERES
and ERA5 estimates (Table 1). The multi-model means of solar absorption at
the TOA, within the atmosphere, and at the surface are 217, 73, and 144 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>, respectively, all within 2 W m<inline-formula><mml:math id="M21" 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> of the biases against the CERES-derived estimates, while they are 3–4 W m<inline-formula><mml:math id="M22" 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> larger for those
from ERA5 at the TOA and within the atmosphere, yielding 1 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> of
bias against the CERES-based estimate at the surface (Table 1). However, the
individual models vary significantly in their simulated annual East Asian
land mean solar absorption, both at the TOA and the surface (Fig. 1a), with SDs of around 6 W m<inline-formula><mml:math id="M24" 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 inter-model spreads of more than 20 W m<inline-formula><mml:math id="M25" 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> (Table 1). Considering the smaller absolute amount of atmospheric and
surface solar absorption compared to the TOA counterpart (73 and 144 vs. 217 W m<inline-formula><mml:math id="M26" 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>; Table 1), the relative (percentage) differences relative to
their respective multi-model means <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">relative</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mo>(</mml:mo><mml:mi mathvariant="normal">percentage</mml:mi><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">difference</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mi mathvariant="normal">range</mml:mi><mml:mtext>multi-model mean</mml:mtext></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> indicate that the uncertainties within the atmosphere and
at the surface are larger than that at the TOA (i.e., TOA: <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">22</mml:mn><mml:mn mathvariant="normal">217</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula>; atmosphere: <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">19</mml:mn><mml:mn mathvariant="normal">73</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">26</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula>; surface: <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">23</mml:mn><mml:mn mathvariant="normal">144</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">16</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula>).</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="d1e669">Annual land mean anomalies of <bold>(a, b)</bold> shortwave (SW) and  <bold>(c, d)</bold> longwave (LW) budgets (unit: W m<inline-formula><mml:math id="M31" 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 regard to their respective multi-model means for the present-day climate under  <bold>(a, c)</bold> all-sky and  <bold>(b, d)</bold> clear-sky conditions over East Asia as simulated by various CMIP6 models.
The black, red, blue, and green lines represent the TOA incoming solar
radiation as well as the net SW/LW radiation at the TOA, within the atmosphere, and at the surface, respectively.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f01.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e705">Annual land mean estimates (unit: W m<inline-formula><mml:math id="M32" 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>) of the magnitudes of various energy balance components and cloud radiative effects (CREs) over East Asia under all-sky and clear-sky conditions at the TOA, within the atmosphere, and at the surface, respectively. The CMIP6 model
statistics (e.g., available model number, spread, standard deviation – SD) as well as the corresponding multi-model mean, ERA5-derived, and CERES-derived estimates are also given in the table.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Component</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col5" align="center">CMIP6 </oasis:entry>
         <oasis:entry colname="col6">ERA5</oasis:entry>
         <oasis:entry colname="col7">CERES</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">(W m<inline-formula><mml:math id="M33" 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>)</oasis:entry>
         <oasis:entry colname="col2">Models</oasis:entry>
         <oasis:entry colname="col3">Spread</oasis:entry>
         <oasis:entry colname="col4">SD</oasis:entry>
         <oasis:entry colname="col5">Mean</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col7">TOA </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Solar down</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">4</oasis:entry>
         <oasis:entry colname="col4">0.2</oasis:entry>
         <oasis:entry colname="col5">334</oasis:entry>
         <oasis:entry colname="col6">334</oasis:entry>
         <oasis:entry colname="col7">334</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Solar up all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">23</oasis:entry>
         <oasis:entry colname="col4">6</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M34" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>117</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M35" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>115</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M36" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>118</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Solar net all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">22</oasis:entry>
         <oasis:entry colname="col4">6.1</oasis:entry>
         <oasis:entry colname="col5">217</oasis:entry>
         <oasis:entry colname="col6">219</oasis:entry>
         <oasis:entry colname="col7">216</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Solar up clear-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">24</oasis:entry>
         <oasis:entry colname="col4">7</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M37" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>76</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M38" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>78</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M39" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>72</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Solar net clear-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">24</oasis:entry>
         <oasis:entry colname="col4">6.9</oasis:entry>
         <oasis:entry colname="col5">258</oasis:entry>
         <oasis:entry colname="col6">256</oasis:entry>
         <oasis:entry colname="col7">262</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW CRE</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">26</oasis:entry>
         <oasis:entry colname="col4">6.5</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M40" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>41</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M41" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>37</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M42" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Thermal up all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">12</oasis:entry>
         <oasis:entry colname="col4">3.5</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M43" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>224</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M44" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>225</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M45" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>226</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Thermal up clear-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">15</oasis:entry>
         <oasis:entry colname="col4">3.2</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M46" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>247</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M47" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>246</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M48" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>250</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW CRE</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">12</oasis:entry>
         <oasis:entry colname="col4">2.4</oasis:entry>
         <oasis:entry colname="col5">23</oasis:entry>
         <oasis:entry colname="col6">21</oasis:entry>
         <oasis:entry colname="col7">24</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Net CRE</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">24</oasis:entry>
         <oasis:entry colname="col4">5.8</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M49" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M50" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>16</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M51" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col7">Atmosphere </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW absorption all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">19</oasis:entry>
         <oasis:entry colname="col4">3.8</oasis:entry>
         <oasis:entry colname="col5">73</oasis:entry>
         <oasis:entry colname="col6">78</oasis:entry>
         <oasis:entry colname="col7">74</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW absorption clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">19</oasis:entry>
         <oasis:entry colname="col4">3.8</oasis:entry>
         <oasis:entry colname="col5">69</oasis:entry>
         <oasis:entry colname="col6">77</oasis:entry>
         <oasis:entry colname="col7">71</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW CRE</oasis:entry>
         <oasis:entry colname="col2">32</oasis:entry>
         <oasis:entry colname="col3">33</oasis:entry>
         <oasis:entry colname="col4">6.9</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW net all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">22</oasis:entry>
         <oasis:entry colname="col4">5.1</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M52" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>152</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M53" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>150</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M54" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>157</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW net clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">16</oasis:entry>
         <oasis:entry colname="col4">3.6</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M55" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>151</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M56" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>151</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M57" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>154</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW CRE</oasis:entry>
         <oasis:entry colname="col2">32</oasis:entry>
         <oasis:entry colname="col3">14</oasis:entry>
         <oasis:entry colname="col4">3.3</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M58" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2</oasis:entry>
         <oasis:entry colname="col6">1</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M59" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Net CRE</oasis:entry>
         <oasis:entry colname="col2">32</oasis:entry>
         <oasis:entry colname="col3">35</oasis:entry>
         <oasis:entry colname="col4">7.8</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">0</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col7">Surface </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW down all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">33</oasis:entry>
         <oasis:entry colname="col4">7.6</oasis:entry>
         <oasis:entry colname="col5">186</oasis:entry>
         <oasis:entry colname="col6">191</oasis:entry>
         <oasis:entry colname="col7">178</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW up all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">24</oasis:entry>
         <oasis:entry colname="col4">6.5</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M60" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>43</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M61" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>50</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M62" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>36</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW absorbed all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">23</oasis:entry>
         <oasis:entry colname="col4">6.1</oasis:entry>
         <oasis:entry colname="col5">144</oasis:entry>
         <oasis:entry colname="col6">141</oasis:entry>
         <oasis:entry colname="col7">142</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW down clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">25</oasis:entry>
         <oasis:entry colname="col4">4.6</oasis:entry>
         <oasis:entry colname="col5">242</oasis:entry>
         <oasis:entry colname="col6">238</oasis:entry>
         <oasis:entry colname="col7">236</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW up clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">27</oasis:entry>
         <oasis:entry colname="col4">6.8</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M63" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>53</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M64" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>59</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M65" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW absorbed clear-sky</oasis:entry>
         <oasis:entry colname="col2">32</oasis:entry>
         <oasis:entry colname="col3">36</oasis:entry>
         <oasis:entry colname="col4">7.8</oasis:entry>
         <oasis:entry colname="col5">189</oasis:entry>
         <oasis:entry colname="col6">179</oasis:entry>
         <oasis:entry colname="col7">191</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW CRE</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">28</oasis:entry>
         <oasis:entry colname="col4">6.6</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M66" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M67" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M68" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>49</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW down all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">27</oasis:entry>
         <oasis:entry colname="col4">7.9</oasis:entry>
         <oasis:entry colname="col5">280</oasis:entry>
         <oasis:entry colname="col6">273</oasis:entry>
         <oasis:entry colname="col7">285</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW up all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">23</oasis:entry>
         <oasis:entry colname="col4">7.1</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M69" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>352</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M70" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M71" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>354</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW net all-sky</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">23</oasis:entry>
         <oasis:entry colname="col4">5.7</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M72" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>71</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M73" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>74</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M74" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>69</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW down clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">26</oasis:entry>
         <oasis:entry colname="col4">6.8</oasis:entry>
         <oasis:entry colname="col5">256</oasis:entry>
         <oasis:entry colname="col6">253</oasis:entry>
         <oasis:entry colname="col7">256</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW up clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">23</oasis:entry>
         <oasis:entry colname="col4">7.1</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M75" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>351</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M76" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M77" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>353</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW net clear-sky</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">18</oasis:entry>
         <oasis:entry colname="col4">4.1</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M78" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>95</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M79" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>94</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M80" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>97</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW CRE</oasis:entry>
         <oasis:entry colname="col2">35</oasis:entry>
         <oasis:entry colname="col3">12</oasis:entry>
         <oasis:entry colname="col4">3.5</oasis:entry>
         <oasis:entry colname="col5">24</oasis:entry>
         <oasis:entry colname="col6">20</oasis:entry>
         <oasis:entry colname="col7">27</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Net CRE</oasis:entry>
         <oasis:entry colname="col2">32</oasis:entry>
         <oasis:entry colname="col3">31</oasis:entry>
         <oasis:entry colname="col4">6</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M81" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>21</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M82" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>18</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M83" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Net radiation</oasis:entry>
         <oasis:entry colname="col2">39</oasis:entry>
         <oasis:entry colname="col3">20</oasis:entry>
         <oasis:entry colname="col4">5.3</oasis:entry>
         <oasis:entry colname="col5">72</oasis:entry>
         <oasis:entry colname="col6">67</oasis:entry>
         <oasis:entry colname="col7">73</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LH</oasis:entry>
         <oasis:entry colname="col2">40</oasis:entry>
         <oasis:entry colname="col3">26</oasis:entry>
         <oasis:entry colname="col4">4.7</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M84" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>43</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M85" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>38</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SH</oasis:entry>
         <oasis:entry colname="col2">40</oasis:entry>
         <oasis:entry colname="col3">21</oasis:entry>
         <oasis:entry colname="col4">5.2</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M86" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>31</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M87" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>29</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e2022">Annual land mean surface downward <bold>(a)</bold> SW and <bold>(b)</bold> LW radiation (unit: W m<inline-formula><mml:math id="M88" 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>) under both all-sky (orange bars) and clear-sky (green bars) conditions over East Asia as calculated by various CMIP6 models.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f02.png"/>

        </fig>

      <p id="d1e2049">The simulated SSR, however, shows the largest spread of more than 30 W m<inline-formula><mml:math id="M89" 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> (ranging from 172 to 205 W m<inline-formula><mml:math id="M90" 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>) among all the substantially differing all-sky surface radiation components, with a large SD of 7.6 W m<inline-formula><mml:math id="M91" 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> (Fig. 2a; Table 1). The multi-model mean SSR is estimated to be 186 W m<inline-formula><mml:math id="M92" 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>, suggesting positive and negative deviations of 8 and 5 W m<inline-formula><mml:math id="M93" 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> from the CERES- and ERA5-derived estimates, respectively (Table 1). Interestingly, although the discrepancy between them is very large (8 or 5 W m<inline-formula><mml:math id="M94" 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>), both the resulting surface solar absorption differences are very small (within 3 W m<inline-formula><mml:math id="M95" 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>), indicating that a higher SSR goes together
with a higher surface albedo (Table 1), which agrees well with that on a
global mean level (Wild et al., 2015).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Best estimates for the surface downward SW radiation</title>
      <p id="d1e2145">As a major component of Earth's energy balance, the solar radiation reaching
the Earth's surface governs a wide range of surface physical and chemical
processes. The spatial distributions of the site-based annual mean SSR from the CMA and GEBA (Sect. 2.1) over East Asia under all-sky conditions are presented in Fig. 3a together with the classified rural and urban sites. In short, the high values are mainly located at the high-elevation stations
over western China and a few island sites in Japan (e.g., Minamitorishima,
Japan; not shown in the figure), especially over the TP, with the largest
value reaching 263 W m<inline-formula><mml:math id="M96" 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> (Geer, Tibet), which is associated with the
high atmospheric transparency over these regions. However, the low annual mean values are primarily over southwestern China, with the smallest value of 103 W m<inline-formula><mml:math id="M97" 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> (Shapingba, Chongqing), which is possibly caused by the
higher aerosol loadings (Liao et al., 2015; de Leeuw et al., 2018) and more
clouds (Li et al., 2017; You et al., 2019; Lei et al., 2020; Zhang et al.,
2020) over these regions. This distribution pattern is highly consistent
with that over China documented by Q. Wang et al. (2021).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2174">Spatial distributions of annual mean surface downward solar radiation (SSR) (unit: W m<inline-formula><mml:math id="M98" 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>) under <bold>(a)</bold> all-sky and <bold>(b)</bold> clear-sky conditions over East Asia. The all-sky sites are available from 99 CMA and 16 GEBA stations, while there are 76 CMA and 16
CERES-interpolated sites for clear-sky conditions. The cross and circle
symbols indicate rural (19 vs. 18 for all-sky and clear-sky conditions) and
urban stations (96 vs. 74), respectively.</p></caption>
          <?xmltex \igopts{width=469.470472pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e2203">Spatial distributions of annual mean SSR biases (unit: W m<inline-formula><mml:math id="M99" 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>) derived from <bold>(a)</bold> CERES-EBAF, <bold>(c)</bold> the CMIP6 multi-model mean, and <bold>(e)</bold> ERA5 reanalysis at a combination of the CMA and GEBA sites under all-sky conditions over East Asia. The
corresponding comparisons of their respective annual means at the surface
sites with their observed counterparts are displayed in panels <bold>(b)</bold>,
<bold>(d)</bold>, and <bold>(f)</bold>, respectively. The cross and circle symbols
in panels <bold>(a)</bold>, <bold>(c)</bold>, and <bold>(e)</bold> as well as the orange and green stars in panels <bold>(b)</bold>, <bold>(d)</bold>, and <bold>(f)</bold> indicate rural and urban stations, respectively.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f04.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e2266">Annual station mean SSR biases (unit: W m<inline-formula><mml:math id="M100" 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>) derived from CERES-EBAF, the CMIP6 multi-model mean, and ERA5 compared to the surface observational sites under all-sky and clear-sky conditions during 2010–2014
over East Asian land together with the separate station averages of biases at urban and rural sites. The values in parentheses represent the
percentages of SSR biases relative to their respective station mean averages, with the largest percentages around 10 % and 4 % for all-sky and
clear-sky conditions.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right" colsep="1"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Station mean SSR biases</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col4" align="center" colsep="1">All-sky </oasis:entry>
         <oasis:entry rowsep="1" namest="col5" nameend="col7" align="center">Clear-sky </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">(unit: W m<inline-formula><mml:math id="M101" 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>)</oasis:entry>
         <oasis:entry colname="col2">All</oasis:entry>
         <oasis:entry colname="col3">Urban</oasis:entry>
         <oasis:entry colname="col4">Rural</oasis:entry>
         <oasis:entry colname="col5">All</oasis:entry>
         <oasis:entry colname="col6">Urban</oasis:entry>
         <oasis:entry colname="col7">Rural</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CERES-EBAF</oasis:entry>
         <oasis:entry colname="col2">3.8 (2.3 %)</oasis:entry>
         <oasis:entry colname="col3">4.2 (2.6 %)</oasis:entry>
         <oasis:entry colname="col4">1.7 (0.9 %)</oasis:entry>
         <oasis:entry colname="col5">0.4 (0.2 %)</oasis:entry>
         <oasis:entry colname="col6">0.5 (0.2 %)</oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M102" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3 (<inline-formula><mml:math id="M103" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.1 %)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CMIP6</oasis:entry>
         <oasis:entry colname="col2">13.8 (8.3 %)</oasis:entry>
         <oasis:entry colname="col3">15 (9.2 %)</oasis:entry>
         <oasis:entry colname="col4">7.4 (4.1 %)</oasis:entry>
         <oasis:entry colname="col5">9.1 (4 %)</oasis:entry>
         <oasis:entry colname="col6">9.7 (4.3 %)</oasis:entry>
         <oasis:entry colname="col7">6.4 (2.8 %)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ERA5</oasis:entry>
         <oasis:entry colname="col2">16.5 (10 %)</oasis:entry>
         <oasis:entry colname="col3">17.2 (10.5 %)</oasis:entry>
         <oasis:entry colname="col4">12.7 (7 %)</oasis:entry>
         <oasis:entry colname="col5">5.7 (2.5 %)</oasis:entry>
         <oasis:entry colname="col6">6.2 (2.7 %)</oasis:entry>
         <oasis:entry colname="col7">3.6 (1.5 %)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e2447">Annual land mean area-weighted average SSR (unit: W m<inline-formula><mml:math id="M104" 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>) from a combination of the CMA and GEBA (CERES-interpolated) site observations under all-sky (clear-sky) conditions during the period 2010–2014 over East Asia together with the corresponding estimates from the CERES-EBAF, CMIP6 multi-model means, and ERA5, respectively.</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="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Average annual mean SSR</oasis:entry>
         <oasis:entry colname="col2">Surface</oasis:entry>
         <oasis:entry colname="col3">CERES-EBAF</oasis:entry>
         <oasis:entry colname="col4">CMIP6</oasis:entry>
         <oasis:entry colname="col5">ERA5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">during 2010–2014 over</oasis:entry>
         <oasis:entry colname="col2">observations</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">East Asia (unit: W m<inline-formula><mml:math id="M105" 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>)</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">All-sky</oasis:entry>
         <oasis:entry colname="col2">174</oasis:entry>
         <oasis:entry colname="col3">178</oasis:entry>
         <oasis:entry colname="col4">186</oasis:entry>
         <oasis:entry colname="col5">191</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Clear-sky</oasis:entry>
         <oasis:entry colname="col2">230</oasis:entry>
         <oasis:entry colname="col3">236</oasis:entry>
         <oasis:entry colname="col4">242</oasis:entry>
         <oasis:entry colname="col5">238</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e2579">Figure 4 shows the distributions of annual mean SSR biases derived from CERES, the CMIP6 multi-model mean, and ERA5 against the surface observations, as well as the comparisons of their respective annual land means at the surface
sites with their observed counterparts. The corresponding quantifications of
the magnitudes of station mean biases are also given in Table 2. According to the comparisons, they all correlate well with the ground-based
observations, with their respective high correlation coefficients of 0.93,
0.87, and 0.89, indicative of the highest accuracy in the CERES-derived estimate (Fig. 4b, d, and f). To quantify their SSR mean biases against the corresponding observed counterparts, the CERES-based bias at all the sites is the smallest, with a station mean bias of 3.8 W m<inline-formula><mml:math id="M106" 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>, followed by the CMIP6 multi-model mean and the ERA5 reanalysis (with respective station mean
biases of 13.8 and 16.5 W m<inline-formula><mml:math id="M107" 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>) (Table 2). Additionally, among all the
aforementioned SSR estimates, the East Asian urban sites are in general more
significantly overestimated than the rural sites on average compared to the
surface observations (Fig. 4b, d, and f; Table 2). This further supports
the argument that rural stations might be more representative for larger-scale comparisons (e.g., the general circulation model grid scales) than the
urban stations (which are vulnerable to local pollution) (Wang et al.,
2018). The overestimations are mainly located in the high-latitude regions
over East Asia for CERES-derived estimates (among them the underestimations
mostly from rural sites), while the underestimates are primarily located in
lower-latitude and eastern coastal regions (Fig. 4a and b). The CMIP6
multi-model mean and ERA5-derived SSR generally greatly overestimate the
surface-based observations at both urban and rural sites, except for the regions over northern and northeastern Inner Mongolia, northwestern
Heilongjiang (located in northeastern China), and some individual sites over southwestern China (Fig. 4c–f). The annual land mean area-weighted average SSR over East Asia derived from CERES is estimated to be 178 W m<inline-formula><mml:math id="M108" 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>, which is closest to the surface observational estimate of 174 W m<inline-formula><mml:math id="M109" 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> compared to the much higher overestimations of both the CMIP6
multi-model mean and ERA5 (186 and 191 W m<inline-formula><mml:math id="M110" 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>) against the surface
observations (Table 3), which shows a high consistency with their bias
distributions and the collocated quantifications (Fig. 4; Table 2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e2644">Annual land mean SSR (unit: W m<inline-formula><mml:math id="M111" 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>) of various CMIP6 models as well as their respective model biases relative to an average over surface sites (99 CMA and 16 GEBA for all-sky, 76 CMA and 16 CERES-interpolated sites for clear-sky) under <bold>(a)</bold> all-sky and
<bold>(b)</bold> clear-sky conditions during 2010–2014 over East Asia. Green
stars represent various CMIP6 models. The best estimate here (orange circle) can be inferred from the intersection between the linear regression line (green
solid lines) and the zero-bias line (blue dotted lines). Furthermore, the
corresponding estimates from CERES-EBAF and ERA5 are also given by the red triangle and blue square, respectively.</p></caption>
          <?xmltex \igopts{width=449.553543pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f05.png"/>

        </fig>

      <p id="d1e2671">However, the ground-based observations are spatially limited with sparse stations in some remote regions and are thus inadequate for many applications, as they may be not representative for real situations. To
better constrain the large spread in the model-based SSR outlined above, we
combine the ground-based observations to obtain the best estimate referring
to the approach introduced in Wild et al. (2013a). Figure 5a gives various
CMIP6 model biases of all-sky SSR at all the surface sites and their
respective East Asian land means. The higher overestimations relative to
surface observations generally correspond to higher model-based East Asian
land means, with a much higher correlation coefficient of 0.96 than that of
0.88 on the global scale (Wild et al., 2015). Thus, the best estimate of the
annual East Asian land mean SSR is deduced to be 174.2 <inline-formula><mml:math id="M112" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.3 W m<inline-formula><mml:math id="M113" 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<inline-formula><mml:math id="M114" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> uncertainty) in light of the linear regression analysis. The corresponding estimates from CERES and ERA5 are also labeled in the figure,
at 178 and 191 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>, respectively, implying a slight and substantial
overestimation for CERES and ERA5 estimates. There is an overall tendency
that most models overestimate the surface downward SW fluxes (36 out of 39
sites) compared to the ground-based observations, with a multi-model mean
overestimation relative to site observations of 13.8 W m<inline-formula><mml:math id="M116" 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>, which is
also a longstanding issue in climate modeling (Wild et al., 1995, 2015).</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Longwave components</title>
      <p id="d1e2732">Similarly to the all-sky SW counterparts, obvious discrepancies can still be noted in the annual land mean LW radiation over East Asia among models, especially for those within the atmosphere and at the surface (Fig. 1c).
Correspondingly, the simulated TOA OLR varies in a range of 12 W m<inline-formula><mml:math id="M117" 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>,
which is almost 10 W m<inline-formula><mml:math id="M118" 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> lower than that within the atmosphere (22 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>) and at the surface (23 W m<inline-formula><mml:math id="M120" 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>) (Table 1). The estimated annual East Asian land-mean TOA OLR from the CMIP6 multi-model mean is <inline-formula><mml:math id="M121" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>224 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>, within 2 W m<inline-formula><mml:math id="M123" 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> of the deviations from the CERES- and ERA5-inferred estimates. The model spread of the simulated annual land-mean net LW radiation becomes larger from the TOA to the surface, with SDs of 3.5, 5.1, and 5.7 W m<inline-formula><mml:math id="M124" 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>, respectively, which shows the same tendency as
the relative (percentages) differences with respect to their multi-model
means (5.4 %, 14.5 %, and 32.4 %).</p>
      <p id="d1e2827">These large discrepancies in surface net LW radiation between models are
particularly evident in the surface downward LW radiation (Fig. 2b; Table 1), with a range of up to 27 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> (from 267 to 294 W m<inline-formula><mml:math id="M126" 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 a SD of 7.9 W m<inline-formula><mml:math id="M127" 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>, which is also the largest deviation among all the components under all-sky conditions. Compared to the CERES estimates, the slightly
lower surface upward LW radiation (<inline-formula><mml:math id="M128" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>352 vs. <inline-formula><mml:math id="M129" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>354 W m<inline-formula><mml:math id="M130" 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 much lower surface downward LW radiation (280 vs. 285 W m<inline-formula><mml:math id="M131" 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>) from the multi-model means are the major reason for the small deviation (within 2 W m<inline-formula><mml:math id="M132" 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>) of the surface net LW radiation between them (Table 1). It is interesting to note that the annual East Asian land mean surface upward LW radiation estimated from ERA5 is the lowest among all these estimates, at <inline-formula><mml:math id="M133" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347 W m<inline-formula><mml:math id="M134" 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>, suggesting the lowest surface skin temperature of the ERA5 product
according to the Stefan–Boltzmann law, followed by the estimates from the multi-model mean and CERES (Table 1). Besides, the annual land mean surface downward LW radiation estimated by ERA5 is 273 W m<inline-formula><mml:math id="M135" 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>,
approximately 7 and 12 W m<inline-formula><mml:math id="M136" 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> lower than the estimates by the CMIP6
multi-model mean and CERES, respectively (Table 1). Therefore, both the
lower surface upward and downward LW radiation fluxes result in the small
deviation in the estimated surface net LW radiation from ERA5 compared to
those from the multi-model mean and CERES (Table 1). Since the reanalysis
products take as many observed atmospheric parameters with global coverage
as possible into consideration during the radiative transfer calculations,
they are widely used to obtain more accurate surface LW radiation (Simmons
et al., 2004; Wild et al., 2015). We also examined the corresponding surface
LW fluxes from another reanalysis, namely MERRA-2, and found much lower
annual land means than those from ERA5, in particular for the surface
downward LW radiation (not shown), which arrives at similar conclusions to those documented by Urraca et al. (2018). Thus, considering the limited
observational surface LW radiation data over East Asia, ERA5 might be the
best reference for the estimates of the annual land mean surface upward and downward LW radiation, at <inline-formula><mml:math id="M137" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347 and 273 W m<inline-formula><mml:math id="M138" 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>, respectively (Table 1).</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Discussion of land energy balance over East Asia under all-sky conditions</title>
<sec id="Ch1.S3.SS4.SSS1">
  <label>3.4.1</label><title>Radiative components</title>
      <p id="d1e2995">Figure 6a displays the schematic diagram of the all-sky land mean energy balance over East Asia, including the abovementioned SW and LW radiation budgets and other radiative components discussed in the following. The
estimated annual East Asian land mean incoming, reflected, and net SW radiation as well as the OLR at the TOA are therefore 334, <inline-formula><mml:math id="M139" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>118, 216, and <inline-formula><mml:math id="M140" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>226 W m<inline-formula><mml:math id="M141" 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> (Table 1), respectively, based on the CERES EBAF dataset.
The corresponding uncertainties are obtained from the uncertainty of 2.5
(1<inline-formula><mml:math id="M142" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> uncertainty) W m<inline-formula><mml:math id="M143" 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 both SW and LW fluxes given by Loeb et al. (2018). The annual East Asian land-mean TOA OLR in CERES-EBAF is estimated to be 10 W m<inline-formula><mml:math id="M144" 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> larger than the TOA-absorbed SW radiation, implying an energy loss of 10 W m<inline-formula><mml:math id="M145" 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> at the TOA under all-sky
conditions, which should be compensated by the LH and SH transported from
regions outside East Asia (Fig. 6a).</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="d1e3070">Diagrams of the annual land mean energy balance (unit: 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>) over East Asia under <bold>(a)</bold> all-sky and <bold>(b)</bold> clear-sky conditions for the present-day climate. The uncertainty ranges are also given in parentheses.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f06.png"/>

          </fig>

      <p id="d1e3097">For the SSR, the annual East Asian land mean best estimate based on the CMIP6 multi-model simulations and surface observations is 174.2 W m<inline-formula><mml:math id="M147" 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> (Figs. 5a and 6a). Considering the abnormally high overestimation by
ERA5 compared to surface observation, the high value of the uncertainty
range is given by the estimate from CERES EBAF (178 W m<inline-formula><mml:math id="M148" 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>), while its
low value is from the lowest model estimate (172 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>; Fig. 2a) (Fig. 6a). The all-sky surface albedo information is derived from the ratio
between the CERES-derived surface upward and downward solar radiation, with
a radiation-weighted average of around 0.2 (36.4/178.3) over East Asian land. However, the corresponding surface albedos estimated by the CMIP6
multi-model mean and ERA5 are substantially higher than that from CERES, with respective averages of around 0.23 (42.7/186.4) and 0.26 (49.6/191).
Considering the large spatial coverage of remote sensing measurement to map
albedo globally, the CERES-derived annual East Asian land mean surface albedo is adopted as the best estimate in this study. Therefore, considering the rounded best SSR estimate of 174 W m<inline-formula><mml:math id="M150" 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 calculated surface-reflected and surface-absorbed SW radiation fluxes are around <inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 and 139 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>, respectively. As shown in Table 1, the uncertainty range of the surface-absorbed SW radiation is 132–144 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> according to the lowest value of CMIP6 models and the highest estimate among the aforementioned estimates, which gives rise to an uncertainty range of the surface-reflected solar radiation of 34–40 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>. Together with the annual East Asian
land mean SW absorption at the TOA and surface of 216 and 139 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>, the best estimate for the atmospheric SW absorption is therefore 77 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>, which is within 4 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> of the differences between those estimated from the CMIP6 multi-model mean and CERES, and closes to the ERA5-derived estimate of 78 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> (Table 1). The uncertainty range of the atmospheric SW absorption is also determined by the estimates from
different data sources as shown in Fig. 6a.</p>
      <p id="d1e3242">The downward LW radiation emitted by the atmosphere is mainly sensitive to
the near-surface temperature, water vapor, and cloud properties, while the
surface emission is in proportion to the skin temperature according to the
Stefan–Boltzmann law. As analyzed in Sect. 3.3, the best estimates of the East Asian annual land mean surface upward and downward LW radiation amount to <inline-formula><mml:math id="M159" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347 and 273 W m<inline-formula><mml:math id="M160" 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>, respectively, with uncertainty ranges also coming from the above-discussed different data sources (Fig. 6a). The surface
net LW radiation is then estimated to be <inline-formula><mml:math id="M161" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>74 W m<inline-formula><mml:math id="M162" 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> based on the surface upward and downward LW radiation outlined above. Combined with the TOA outgoing thermal radiation of <inline-formula><mml:math id="M163" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>226 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>, the estimated atmospheric net LW radiation is <inline-formula><mml:math id="M165" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>152 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>, which is close to the collocated estimates from the multi-model mean (<inline-formula><mml:math id="M167" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>152 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>) and ERA5 (<inline-formula><mml:math id="M169" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>150 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</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) but
deviates substantially from the CERES-derived estimate of <inline-formula><mml:math id="M171" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>157 W m<inline-formula><mml:math id="M172" 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>
(Table 1). Considering the surface-absorbed SW radiation of 139 W m<inline-formula><mml:math id="M173" 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 best estimate for surface net radiation is 65 W m<inline-formula><mml:math id="M174" 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>, suggesting that
around 65 W m<inline-formula><mml:math id="M175" 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> of energy is available for the non-radiative SH and LH. Besides, the ERA5 estimate of 67 W m<inline-formula><mml:math id="M176" 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> is very close to the best estimate of 65 W m<inline-formula><mml:math id="M177" 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>, while much higher estimates of 72 and 73 W m<inline-formula><mml:math id="M178" 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 obtained from the multi-model mean and CERES (Table 1),
respectively.</p>
</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <label>3.4.2</label><title>Non-radiative components</title>
      <p id="d1e3461">The surface net radiation is mainly balanced by the non-radiative components
of SH and LH in addition to a very small proportion of ground heat flux and
melt (less than 1 %) (Ohmura, 2004). However, due to the lack of
constraints from in situ and space observations, this partitioning of the surface net radiation into SH and LH is still subject to considerable
uncertainties. As shown in Fig. S2, the simulated annual East Asian
land-mean LH and SH vary greatly between different models, with a range of 26 and 21 W m<inline-formula><mml:math id="M179" 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>, respectively, as well as the relative discrepancies relative to their respective multi-model means of 60 %
<inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mfenced close=")" open="("><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">26</mml:mn><mml:mn mathvariant="normal">43</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and 68 %
<inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mfenced close=")" open="("><mml:mrow><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mn mathvariant="normal">21</mml:mn><mml:mn mathvariant="normal">31</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula>, respectively,
showing larger discrepancies between models with larger uncertainties in SH
(Table 1). The best SH estimate can therefore be obtained from the residual
of the LH. To obtain a more accurate surface LH from available datasets of
the multi-model mean and ERA5, we take an average of them as the best
estimate, namely <inline-formula><mml:math id="M182" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 W m<inline-formula><mml:math id="M183" 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 uncertainty ranges of which are also
given according to these estimates (Fig. 6a). Note that all the values in
this study are calculated on the basis of one decimal point, which may
result in 1 W m<inline-formula><mml:math id="M184" 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> of bias during the rounding process. Combined with
the surface net radiation and LH of 65 and <inline-formula><mml:math id="M185" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 W m<inline-formula><mml:math id="M186" 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>, respectively, the surface SH is estimated to be <inline-formula><mml:math id="M187" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>25 W m<inline-formula><mml:math id="M188" 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 uncertainty range of which
is also given by the existing estimates from various CMIP6 models and ERA5
(Fig. 6a). Besides, although the annual land mean SH estimated from MERRA-2 is much higher than the estimates from the multi-model mean and ERA5 (not shown), the estimated LH is around <inline-formula><mml:math id="M189" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>39 W m<inline-formula><mml:math id="M190" 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> (not shown), very
close to the best estimate of <inline-formula><mml:math id="M191" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>40 W m<inline-formula><mml:math id="M192" 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>, which increases our confidence
in the estimation of this quantity.</p>
</sec>
<sec id="Ch1.S3.SS4.SSS3">
  <label>3.4.3</label><title>Comparisons with global land mean estimates</title>
      <p id="d1e3635">Notable discrepancies exist in the global land mean energy budgets reported by Wild et al. (2015) and the regional ones over East Asia in this study (Fig. S3; Table 4). For the SW budgets, the estimated annual land-mean TOA incident solar radiation over East Asia is 9 W m<inline-formula><mml:math id="M193" 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> higher than that over global land (334 vs. 325 W m<inline-formula><mml:math id="M194" 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>), implying a slightly lower land mean solar zenith angle over East Asia. Comparisons also show a slightly higher relative percentage of TOA-reflected solar radiation of 0.8 % despite the much lower surface-reflected SW radiation of 4.3 % over East Asian land compared to global land with respect to their respective TOA incident solar radiation (thereafter called “relative
percentage” for short). This suggests a much more relative atmospheric SW reflection of 5.2 % over East Asian land, which agrees fairly well with
more aerosols (Wei et al., 2019) and more clouds (King et al., 2013; Fan et
al., 2018; also see Fig. S4) over this region compared to global land.
However, the annual land mean solar radiation reaching the East Asian surface is around 10 W m<inline-formula><mml:math id="M195" 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> lower than that over global land (174 vs. 184 W m<inline-formula><mml:math id="M196" 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>), approximately accounting for 52.1 % and 56.6 % of their respective incident solar radiation at the TOA, respectively, indicating a lower fraction of solar energy arriving at the East Asian surface compared to global land. Together with the lower annual land mean surface albedo over East Asian land compared to global land (20 % vs. 26 %), this leads to
the similar relative percentages of surface absorptions (41.6 % vs.
41.9 %). Although the magnitudes of the atmospheric SW absorptions over East Asian and global land are nearly the same (both around 77 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 corresponding relative percentage over East Asian land is a little bit
lower than that over global land (around 0.6 %). This is somewhat
unexpected due to the existence of more clouds and aerosol loadings over East Asian land, which is possibly offset by the lower water vapor contents
caused by the higher altitudes and thinner air over the TP.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T4" specific-use="star"><?xmltex \currentcnt{4}?><label>Table 4</label><caption><p id="d1e3701">Comparisons of the annual mean SW/LW energy balance components (unit: W m<inline-formula><mml:math id="M198" 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 East Asian land (this study) and global land (Wild et al., 2015) as well as the corresponding relative percentages with regard to their respective TOA incident solar radiation/surface LW
emissions and the relative percentage differences between them.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right" colsep="1"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Component</oasis:entry>
         <oasis:entry rowsep="1" namest="col2" nameend="col3" align="center" colsep="1">East Asian land </oasis:entry>
         <oasis:entry rowsep="1" namest="col4" nameend="col5" align="center">Global land </oasis:entry>
         <oasis:entry colname="col6">Percentage</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Annual</oasis:entry>
         <oasis:entry colname="col3">Relative</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5">Relative</oasis:entry>
         <oasis:entry colname="col6">difference</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">mean</oasis:entry>
         <oasis:entry colname="col3">percentage</oasis:entry>
         <oasis:entry colname="col4">mean</oasis:entry>
         <oasis:entry colname="col5">percentage</oasis:entry>
         <oasis:entry colname="col6"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6">SW budget </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TOA solar down</oasis:entry>
         <oasis:entry colname="col2">334</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4">325</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TOA solar up</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M199" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>118</oasis:entry>
         <oasis:entry colname="col3">35.3 %</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M200" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>112</oasis:entry>
         <oasis:entry colname="col5">34.5 %</oasis:entry>
         <oasis:entry colname="col6">0.8 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Atmospheric SW absorption</oasis:entry>
         <oasis:entry colname="col2">77</oasis:entry>
         <oasis:entry colname="col3">23.1 %</oasis:entry>
         <oasis:entry colname="col4">77</oasis:entry>
         <oasis:entry colname="col5">23.7 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M201" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.6 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Atmospheric SW reflection</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M202" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>83</oasis:entry>
         <oasis:entry colname="col3">24.9 %</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M203" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>64</oasis:entry>
         <oasis:entry colname="col5">19.7 %</oasis:entry>
         <oasis:entry colname="col6">5.2 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Surface solar down</oasis:entry>
         <oasis:entry colname="col2">174</oasis:entry>
         <oasis:entry colname="col3">52.1 %</oasis:entry>
         <oasis:entry colname="col4">184</oasis:entry>
         <oasis:entry colname="col5">56.6 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M204" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.5 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Surface solar up</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M205" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35</oasis:entry>
         <oasis:entry colname="col3">10.5 %</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M206" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>48</oasis:entry>
         <oasis:entry colname="col5">14.8 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M207" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.3 %</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Surface solar absorption</oasis:entry>
         <oasis:entry colname="col2">139</oasis:entry>
         <oasis:entry colname="col3">41.6 %</oasis:entry>
         <oasis:entry colname="col4">136</oasis:entry>
         <oasis:entry colname="col5">41.9 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M208" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.3 %</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6">LW budget </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TOA LW up</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M209" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>226</oasis:entry>
         <oasis:entry colname="col3">65.1 %</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M210" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>232</oasis:entry>
         <oasis:entry colname="col5">62.4 %</oasis:entry>
         <oasis:entry colname="col6">2.7 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Atmospheric LW absorption</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M211" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>152</oasis:entry>
         <oasis:entry colname="col3">43.8 %</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M212" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>166</oasis:entry>
         <oasis:entry colname="col5">44.6 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M213" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.8 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Surface LW down</oasis:entry>
         <oasis:entry colname="col2">273</oasis:entry>
         <oasis:entry colname="col3">78.7 %</oasis:entry>
         <oasis:entry colname="col4">306</oasis:entry>
         <oasis:entry colname="col5">82.3 %</oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M214" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.6 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Surface LW up</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M215" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>347</oasis:entry>
         <oasis:entry colname="col3">1</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M216" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>372</oasis:entry>
         <oasis:entry colname="col5">1</oasis:entry>
         <oasis:entry colname="col6">–</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e4160">For the LW budgets, the regional surface LW emission over East Asia is
estimated to be much lower than the global land mean estimates in Wild et al. (2015) (Fig. S3), which mainly results from the lower temperature over the TP induced by high altitudes. The relative percentage of land mean surface downward LW radiation with respect to the surface emission over East Asia is about 78.7 %, which is lower than the global estimate of
82.3 %, corresponding well to a reduction in the greenhouse effect and fewer low clouds due to the TP (Fig. S4) considering its coverage over East Asian
land. Ultimately, a higher percentage of LW radiation is emitted into space over East Asian land compared to global land (65.1 % vs. 62.4 %). Our
estimates also indicate approximately similar amounts of LH (40 vs. 38 W m<inline-formula><mml:math id="M217" 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 much lower SH (25 vs. 32 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>) over East Asia compared to the global land mean estimates (Fig. S3), which is possibly related to the lower East Asian land surface temperature.</p>
      <p id="d1e4188">In general, as can be concluded from Table 4, although much less surface SW
radiation (4.3 %) is reflected over East Asian land compared to global land, a slightly higher SW reflection of 0.8 % is estimated at the TOA,
indicating a much larger atmospheric SW reflection of 5.2 % due to the stronger scattering from aerosols and clouds over East Asian land than
global land. However, the SW absorption within the atmosphere over East
Asian land is 0.6 % lower than that over global land despite the higher absorption from clouds and aerosols, which is possibly offset by the lower
water vapor contents caused by the thinner air over the TP. The lower
surface temperature, weaker greenhouse effect, and fewer low clouds due to the high altitudes and the thinner air over the TP in East Asian land are
the major reasons for the relatively lower surface LW emission, fewer and more fractions of surface downward LW radiation of 3.6 % and the OLR of 2.7 % over East Asian land compared to global land, respectively.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Assessment of land energy balance budgets under clear-sky conditions</title>
      <p id="d1e4201">The clear-sky land energy balance budgets over East Asia are similarly
evaluated as all-sky conditions. Detailed analyses are given in the Supplement if the reader is interested. The annual land mean SW clear-sky absorptions at the TOA and the surface over East Asia show larger variations among different models
than those under all-sky conditions (Fig. 1a and b; Table 1), which is consistent with those reported by Wild et al. (2019) but is amazingly in contrast to the recognition that the representation of clouds is the largest
uncertainty in climate models (Dolinar et al., 2015). In particular, the surface SW clear-sky absorptions simulated by various models still exhibit a
larger uncertainty than the TOA counterparts despite the lower absolute values (Fig. 1b; Table 1). In contrast to the all-sky counterparts, the simulated clear-sky SSR among different models shows a notably smaller
inter-model spread and SD than the surface SW absorptions (Table 1), with a much smaller model discrepancy compared to the all-sky conditions (Fig. 2a;
Table 1).</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="d1e4206">Spatial distributions of annual mean SSR biases derived from <bold>(a)</bold> CERES-EBAF, <bold>(b)</bold> the CMIP6 multi-model mean, and <bold>(c)</bold> ERA5 reanalysis against surface observations from a combination
of the CMA and CERES-interpolated sites under clear-sky conditions over East
Asia. The corresponding comparisons of their respective annual land means at
the surface sites with their observed counterparts are displayed in
panels <bold>(b)</bold>, <bold>(d)</bold>, and <bold>(f)</bold>, respectively. The cross and circle symbols in panels <bold>(a)</bold>, <bold>(c)</bold>, and <bold>(e)</bold> as well as the orange and green stars in panels <bold>(b)</bold>, <bold>(d)</bold>, and <bold>(f)</bold> indicate rural and urban stations, respectively.</p></caption>
        <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f07.png"/>

      </fig>

      <p id="d1e4253">To further constrain the outlined inter-model discrepancy of the simulated
clear-sky SSR, surface observations from the CMA and CERES-interpolated
estimates at the GEBA sites are utilized in this study. The high values of
the station-based clear-sky SSR are mainly located in the TP but with an abnormally high value located in southern China (Fig. 3b). All the East
Asian land mean clear-sky SSR estimates from CERES, the CMIP6 multi-model mean, and ERA5 agree reasonably well with the surface observations but with smaller correlation coefficients ranging from 0.78 to 0.82 compared to the
all-sky conditions (Fig. 7b, d, and f). The CERES-derived clear-sky SSR is
mainly overestimated in central and western China but with slight underestimations mainly located in northeastern, eastern, and southern China
(Fig. 7a). Similar bias patterns can also be found in the clear-sky SSR from
the CMIP6 multi-model mean and ERA5 compared to the surface observations,
except for some individual sites over northeastern Inner Mongolia, eastern
China, western Mongolia, and Japan (Fig. 7c and e) but with relatively smaller overestimations than the all-sky counterparts (Fig. 4c and e; Table 2). Specifically, the smallest station mean bias in the CERES-derived SSR
compared to the multi-model mean and ERA5 (Table 2) can be attributed to its
evenly distributed surface sites of overestimations and underestimations (Fig. 7b, d, f). Again, among all the aforementioned clear-sky SSR biases,
more overestimations exist in urban stations than rural stations (Figs. 4b, d, f and 7b, d, f; Table 2). Consequently, all East Asian land mean area-weighted averages of clear-sky SSR from CERES, the CMIP6 multi-model mean, and ERA5 show higher overestimations of around 6, 12, and 8 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>, respectively, compared to the surface observed counterpart of 230 W m<inline-formula><mml:math id="M220" 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>
(Table 3). Based on the similar method introduced in Wild et al. (2015), the
best estimate for the East Asian land mean clear-sky SSR is determined to be 234 <inline-formula><mml:math id="M221" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 1.1 W m<inline-formula><mml:math id="M222" 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<inline-formula><mml:math id="M223" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> uncertainty), with a slightly smaller correlation coefficient of 0.94 and smaller deviations from the CERES and
ERA5 estimates compared to the all-sky counterparts (Fig. 5b; Table 3).
Besides, the overestimations still exist in the observed land mean clear-sky SSR for most climate models over East Asia, with a smaller multi-model mean overestimation of 9.1 W m<inline-formula><mml:math id="M224" 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> than the all-sky counterparts.</p>
      <p id="d1e4320">This clear-sky energy budget only represents the removal of cloud but
maintains the same atmospheric conditions as the all-sky conditions, which
is not balanced because it is not the equilibrium state the Earth would
achieve when no clouds could form. Ultimately, the clear-sky East Asian
land mean energy budget is not closed and has no quantifications of SH and LH as displayed in Fig. 6b. In addition to the analyses above, the clear-sky TOA energy budgets are derived from the CERES-derived product, with uncertainty ranges referring to Loeb et al. (2018), while the surface LW budgets are
again from ERA5 reanalysis. Also, an additional clear-sky radiation-weighted surface albedo of 0.19 from CERES is obtained to estimate the surface-reflected and absorbed SW radiation. Apart from the TOA budget, all the remaining uncertainty ranges are given by different data sources from various CMIP6
models as well as the multi-model mean, CERES-derived, and ERA5-derived estimates.</p>
      <p id="d1e4323">We double-check the energy balance components evaluated in this study by referring to the uncertainty ranges from the CERES-derived product given by Kato et al. (2018) (Table 5), which indicates that all estimated energy
components fall within these uncertainty ranges, except for the all-sky
surface downward LW radiation, with about 3 W m<inline-formula><mml:math id="M225" 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> lower than the
corresponding lowest CERES range. This is in line with its much higher
CERES-derived estimate compared to that of ERA5 (285 vs. 273 W m<inline-formula><mml:math id="M226" 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>) (Table 1).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T5"><?xmltex \currentcnt{5}?><label>Table 5</label><caption><p id="d1e4353">Uncertainties (unit: 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>) in 1<inline-formula><mml:math id="M228" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M229" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M230" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> regional monthly surface SW, LW, and net (SW <inline-formula><mml:math id="M231" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> LW) fluxes under all-sky and clear-sky conditions for the CERES-EBAF Edition 4.1 product (referring to Kato et al., 2018) as well as its corresponding estimates of various surface fluxes.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Uncertainties (1<inline-formula><mml:math id="M232" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col2">All-sky</oasis:entry>
         <oasis:entry colname="col3">Clear-sky</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">SW down</oasis:entry>
         <oasis:entry colname="col2">178 <inline-formula><mml:math id="M233" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 14</oasis:entry>
         <oasis:entry colname="col3">236 <inline-formula><mml:math id="M234" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW up</oasis:entry>
         <oasis:entry colname="col2">36 <inline-formula><mml:math id="M235" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11</oasis:entry>
         <oasis:entry colname="col3">45 <inline-formula><mml:math id="M236" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW net</oasis:entry>
         <oasis:entry colname="col2">142 <inline-formula><mml:math id="M237" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 13</oasis:entry>
         <oasis:entry colname="col3">191 <inline-formula><mml:math id="M238" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 13</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW down</oasis:entry>
         <oasis:entry colname="col2">285 <inline-formula><mml:math id="M239" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 9</oasis:entry>
         <oasis:entry colname="col3">256 <inline-formula><mml:math id="M240" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW up</oasis:entry>
         <oasis:entry colname="col2">354 <inline-formula><mml:math id="M241" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 15</oasis:entry>
         <oasis:entry colname="col3">353 <inline-formula><mml:math id="M242" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 15</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LW net</oasis:entry>
         <oasis:entry colname="col2">69 <inline-formula><mml:math id="M243" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 17</oasis:entry>
         <oasis:entry colname="col3">97 <inline-formula><mml:math id="M244" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 17</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SW <inline-formula><mml:math id="M245" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> LW net</oasis:entry>
         <oasis:entry colname="col2">73 <inline-formula><mml:math id="M246" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20</oasis:entry>
         <oasis:entry colname="col3">95 <inline-formula><mml:math id="M247" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e4626">Overall, around 21.6 % and 56.9 % of the TOA incoming solar radiation
are absorbed by the atmosphere and surface, respectively, for clear-sky
conditions, while these absorptions are 23.1 % and 41.6 % for all-sky
conditions. This implies that the existence of clouds results in more
atmospheric SW absorption of around 1.5 % and much less surface solar
absorption of around 15.3 % with respect to the TOA incoming solar
radiation.</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>The cloud radiative effects (CREs)</title>
      <p id="d1e4638">According to the annual land mean best estimates of radiative components over East Asia under all-sky and clear-sky conditions obtained in the previous sections, the present-day CREs can be inferred quantitatively over this region. The calculated SW, LW, and net CREs at the TOA, within the atmosphere, and at the surface are therefore presented in Fig. 8. Moreover, the corresponding calculation formulas are also given as follows.

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M248" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">outgoing</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">SW</mml:mi><mml:mtext>all-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">outgoing</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">SW</mml:mi><mml:mtext>clear-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></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:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">outgoing</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">LW</mml:mi><mml:mtext>all-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">outgoing</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">LW</mml:mi><mml:mtext>clear-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></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 mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable rowspacing="0.2ex" class="split" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="normal">SW</mml:mi><mml:mtext>all-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi mathvariant="normal">SW</mml:mi><mml:mtext>clear-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi mathvariant="normal">LW</mml:mi><mml:mtext>all-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:msub><mml:mi mathvariant="normal">LW</mml:mi><mml:mtext>clear-sky</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd><mml:mtext>6</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:mi mathvariant="normal">Surface</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">total</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>+</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Atmospheric</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">SW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mi mathvariant="normal">Atmospheric</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mi mathvariant="normal">TOA</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="normal">surface</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">net</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">LW</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">CRE</mml:mi></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e5044">Diagram of the annual land mean SW, LW, and net (SW <inline-formula><mml:math id="M249" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> LW) cloud radiative effects (CREs) (unit: W m<inline-formula><mml:math id="M250" 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>) at the TOA, within the atmosphere, and at the surface over East Asia, calculated by the differences
between all-sky and clear-sky radiation budgets as given in Fig. 7.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f08.png"/>

      </fig>

      <p id="d1e5072">The best estimates for the annual East Asian land mean reflected solar radiation at the TOA under all-sky and clear-sky conditions are <inline-formula><mml:math id="M251" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>118 and <inline-formula><mml:math id="M252" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>72 W m<inline-formula><mml:math id="M253" 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>, respectively, differing by <inline-formula><mml:math id="M254" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46 W m<inline-formula><mml:math id="M255" 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>, indicating that the clouds give rise to an extra 46 W m<inline-formula><mml:math id="M256" 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> solar reflection at the TOA, thus
cooling the Earth–atmosphere system. Similarly, the TOA LW CRE, obtained as the difference between the TOA thermal radiation under all-sky and clear-sky
conditions, is 24 W m<inline-formula><mml:math id="M257" 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>, suggesting a warming effect of clouds on the
system. Thus, the estimated TOA net CRE is <inline-formula><mml:math id="M258" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22 W m<inline-formula><mml:math id="M259" 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>, pointing out that the overall effects of clouds result in an energy loss and net cooling to the system, not only in the global mean, but also over East Asian land.</p>
      <p id="d1e5165">At the Earth's surface, the shading effects of clouds are estimated to
reduce the surface solar radiation by 60 W m<inline-formula><mml:math id="M260" 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>, from 234 to 174 W m<inline-formula><mml:math id="M261" 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>, while the surface solar absorption differs by 51 W m<inline-formula><mml:math id="M262" 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>, from 190 to 139 W m<inline-formula><mml:math id="M263" 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>; that is, the surface net SW CRE is <inline-formula><mml:math id="M264" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>51 W m<inline-formula><mml:math id="M265" 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 cloudy skies, the estimated surface downward LW radiation increases from 253
to 273 W m<inline-formula><mml:math id="M266" 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 an increase of 20 W m<inline-formula><mml:math id="M267" 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>, illustrating that the surface net LW CRE is 20 W m<inline-formula><mml:math id="M268" 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 therefore leads to a surface
warming. Thus, the surface net CRE, i.e., the sum of the surface net SW and LW CRE, is then <inline-formula><mml:math id="M269" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>31 W m<inline-formula><mml:math id="M270" 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>, indicating that clouds contribute more to the SW energy budgets. Eventually, the clouds lead to enhancements of the
SW and LW absorptions within the atmosphere of around 5 and 4 W m<inline-formula><mml:math id="M271" 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>, respectively, thus resulting in an atmospheric net CRE of 9 W m<inline-formula><mml:math id="M272" 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
East Asian land.</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="d1e5318">Annual land mean anomalies of <bold>(a)</bold> SW, <bold>(b)</bold> LW, and <bold>(c)</bold> net (SW+LW) CREs (unit: W m<inline-formula><mml:math id="M273" 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>) at the TOA (red line), within the atmosphere (blue line), and at the surface (green line) with regard to their respective multi-model means over East
Asia, respectively, as represented by various CMIP6 models. The numbers in
the parentheses indicate the available CMIP6 climate models for the
corresponding radiation components.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/15867/2022/acp-22-15867-2022-f09.png"/>

      </fig>

      <p id="d1e5348">The above CRE best estimates are compared with the corresponding estimates
from different data sources (Fig. 9; Table 1). Generally, compared to the LW
CREs (Fig. 9b), the simulated SW CREs show larger spreads and SDs amongst the models (Fig. 9a; Table 1). For the SW CREs at the TOA, within the
atmosphere, and at the surface, the CERES-derived estimates match perfectly
with the best estimates mentioned above, within 2 W m<inline-formula><mml:math id="M274" 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> of the biases,
followed by the estimates from the multi-model means and ERA5 (Table 1). For
the LW CREs, the calculated TOA LW CREs from the CMIP6 multi-model mean and
CERES differ by no more than 1 W m<inline-formula><mml:math id="M275" 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> compared to the best estimate,
while large differences are noted at the surface LW CREs, thereby leading to
their opposite signs in the atmospheric LW CREs (Fig. 9b; Table 1).
Specifically, since the ERA5-based TOA LW CRE deviates by no more than 3 W m<inline-formula><mml:math id="M276" 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 best estimate of 24 W m<inline-formula><mml:math id="M277" 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 nearly the same
surface LW CRE, the estimated atmospheric LW CRE is therefore the closest to
the best estimate (Table 1). This is owing to the fact that we make use of
the ERA5 data as the reference to estimate the surface LW radiation. Thus,
the major reason for the large discrepancies in the atmospheric and surface
LW CREs estimated from different data sources with respect to the best
estimates in this study is the determination of the surface downward and
upward LW radiation, which is also the reason for the large deviations in
their net CREs (Fig. 9c).</p>
      <p id="d1e5399">A better comparison with the global annual mean best estimates of CREs by Wild et al. (2019) is given in Fig. S5. At the TOA, slightly lower and much lower East Asian land-mean SW and LW CREs of 1 and 4 W m<inline-formula><mml:math id="M278" 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> result in 3 W m<inline-formula><mml:math id="M279" 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> more energy loss at the TOA compared to the
globe. At the surface, much lower annual East Asian land-mean SW and LW CREs of 3 and 8 W m<inline-formula><mml:math id="M280" 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 estimated compared to the values over the globe, leading to a net CRE deviation of 5 W m<inline-formula><mml:math id="M281" 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> indicative of 5 W m<inline-formula><mml:math id="M282" 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> more energy loss at the surface. However, lower and higher
annual East Asian land-mean SW and LW CREs of 2 and 4 W m<inline-formula><mml:math id="M283" 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> within the atmosphere contribute to the nearly close net CRE with a deviation of no more than 2 W m<inline-formula><mml:math id="M284" 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> compared to the global mean estimates. On the
whole, lower annual East Asian land-mean best estimates in the absolute values of surface SW and LW CREs as well as the TOA LW CRE compared to their global mean counterparts give rise to the CRE differences between them.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Summary and conclusions</title>
      <p id="d1e5495">This study aims to explore how the energy budgets are interrupted by the
complex orographic and thermal effects of the TP as well as the high anthropogenic aerosol emissions over East Asian land compared to global
land, based on complementary data sources from space and surface
observations as well as the CMIP6 climate models and ERA5 reanalysis. A further quantitative investigation of CREs at the TOA, within the
atmosphere, and at the surface is also conducted.</p>
      <p id="d1e5498">Comparisons between all-sky and clear-sky energy budgets indicate that the
overall effects of clouds greatly reduce the surface solar absorption by
about 15.3 % and enhance that within the atmosphere by 1.5 %. Compared
to the global land energy budget estimates from Wild et al. (2015), for the
SW budgets, a notably more atmospheric SW reflection of 5.2 % but with a slightly less atmospheric SW absorption of 0.6 % with respect to their respective TOA incident solar radiation is estimated over East Asian land, possibly indicating that the lower water vapor content effects due to the TP overcompensate for the aerosol and cloud effects over East Asian land. For
the LW budgets, a substantially lower surface LW emission of around 25 W m<inline-formula><mml:math id="M285" 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 a smaller relative surface downward LW radiation of around 3.6 % with respect to their respective surface emissions can be noticed
over East Asian land compared to global land, which possibly result from the lower regional surface skin temperature as well as the weaker greenhouse effect and fewer low clouds mainly induced by the high altitude and thinner
air over the TP, thus leading to a higher percentage of regional OLR of 2.7 %.</p>
      <p id="d1e5513">The CREs over East Asian land are inferred through the energy budget
differences between all-sky and clear-sky conditions. The clouds reduce the
solar absorption at the TOA by 46 W m<inline-formula><mml:math id="M286" 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 enhance the TOA thermal
radiation by 24 W m<inline-formula><mml:math id="M287" 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>, respectively, leading to a TOA net CRE of <inline-formula><mml:math id="M288" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>22 W m<inline-formula><mml:math id="M289" 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>, a more cooling effect on the regional climate system than that over the globe (<inline-formula><mml:math id="M290" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>19 W m<inline-formula><mml:math id="M291" 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>). At the surface, the net CRE is estimated to be <inline-formula><mml:math id="M292" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>31 W m<inline-formula><mml:math id="M293" 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> according to less solar absorption of 51 W m<inline-formula><mml:math id="M294" 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 more
downward thermal radiation of 20 W m<inline-formula><mml:math id="M295" 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>, indicative of larger cloud
impacts on SW radiation. Within the atmosphere, the estimated net CRE is 9 W m<inline-formula><mml:math id="M296" 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> due to the increases in solar absorption and net thermal radiation of 5 and 4 W m<inline-formula><mml:math id="M297" 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>, respectively. Compared to the global
mean best estimates of CREs as introduced by Wild et al. (2019), relatively
lower East Asian land mean best estimates of surface SW and LW CREs as well as the TOA LW CRE contribute to the CRE differences between them.</p>
      <p id="d1e5647">On the whole, all the estimated land mean energy balance components over East Asia in this study fall within the uncertainty ranges of the CERES-derived assessments, except for the all-sky surface downward LW
radiation. More accurate and reliable datasets should be utilized to reduce
the substantial uncertainties in the regional energy balance estimates,
particularly in the surface budgets, and more widespread temporal and
spatial representations of energy budget research are recommended for more
comprehensive comparisons in future. For example, newly published surface
radiation products with high resolutions based on satellite datasets (e.g.,
Letu et al., 2022; Xu et al., 2022) are expected to make sense in improving
the accuracy of the regional/global surface radiation budget studies.</p>
</sec>

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

      <p id="d1e5654">The surface observations of the CMA and GEBA used in this study are available at <uri>http://data.cma.cn/enl</uri>​​​​​​​ (application required, last access: 10 February 2022; CMA, 2022) and <uri>https://geba.ethz.ch/data-retrieval.html</uri> (login required, last access: 25 February 2022; GEBA, 2022), respectively. The satellite-derived product CERES EBAF Edition 4.1 is obtained at <uri>https://ceres.larc.nasa.gov/data/</uri> (last access: 20 March 2022; CERES, 2022). The CMIP6 climate models are from <uri>https://pcmdi.llnl.gov/CMIP6/</uri> (last access: 14 April 2022; CMIP6, 2022). The ERA5 reanalysis is acquired from <uri>https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5</uri>  (last access: 22 May 2022; ECMWF, 2022).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e5672">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-22-15867-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-22-15867-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e5681">HZ, MW, and QW proposed the main ideas of this study. QW designed and wrote the manuscript. SY provided the homogenized ground-based surface solar radiation data. QC, XZ, and GS contributed to the interpretation of the results. BX and YW assisted with the figures. All the co-authors participated in discussions and provided constructive suggestions.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e5687">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e5693">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="d1e5699">The Global Energy Balance
Archive (GEBA) is co-funded by the Federal Office of Meteorology and
Climatology, MeteoSwiss, within the framework of GCOS Switzerland.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e5704">This research has been supported by the National Key R&amp;D Program of China (grant no. 2017YFA0603502), the National Natural Science Foundation of China (grant no. 42275039), and the S&amp;T Development Fund of CAMS (grant nos. 2021KJ004 and 2022KJ019).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e5711">This paper was edited by Yafang Cheng and reviewed by two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><?label 1?><mixed-citation>Boeke, R. C. and Taylor, P. C.: Evaluation of the Arctic surface radiation budget in CMIP5 models, J. Geophys. Res.-Atmos., 121, 8525–8548, <ext-link xlink:href="https://doi.org/10.1002/2016JD025099" ext-link-type="DOI">10.1002/2016JD025099</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><?label 1?><mixed-citation>CERES: Data Products, National Aeronautics and Space Administration (NASA) [data set], <uri>https://ceres.larc.nasa.gov/data/</uri>, last access: 20 March 2022.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><?label 1?><mixed-citation>Christensen, M. W., Behrangi, A., L'Ecuyer, T. S., Wood, N. B., Lebsock, M.
D., and Stephens, G. L.: Arctic observation and reanalysis integrated
system: A new data product for validation and climate study, B. Am.
Meteorol. Soc., 97, 907–916, <ext-link xlink:href="https://doi.org/10.1175/BAMS-D-14-00273.1" ext-link-type="DOI">10.1175/BAMS-D-14-00273.1</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><?label 1?><mixed-citation>CMA: Surface observational radiation data, China Meteorological Administration National Meteorological Information Center [data set], <uri>http://data.cma.cn/enl</uri>, last access: 10 February 2022.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><?label 1?><mixed-citation>CMIP6: Climate models, The World Climate Research Programme [data set], <uri>https://pcmdi.llnl.gov/CMIP6/</uri>, last access: 14 April 2022.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><?label 1?><mixed-citation>de Leeuw, G., Sogacheva, L., Rodriguez, E., Kourtidis, K., Georgoulias, A. K., Alexandri, G., Amiridis, V., Proestakis, E., Marinou, E., Xue, Y., and van der A, R.: Two decades of satellite observations of AOD over mainland China using ATSR-2, AATSR and MODIS/Terra: data set evaluation and large-scale patterns, Atmos. Chem. Phys., 18, 1573–1592, <ext-link xlink:href="https://doi.org/10.5194/acp-18-1573-2018" ext-link-type="DOI">10.5194/acp-18-1573-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><?label 1?><mixed-citation>Dolinar, E. K., Dong, X., Xi, B., Jiang, J. H., and Su, H.: Evaluation of
CMIP5 simulated clouds and TOA radiation budgets using NASA satellite
observations, Clim. Dynam., 44, 2229–2247,
<ext-link xlink:href="https://doi.org/10.1007/s00382-014-2158-9" ext-link-type="DOI">10.1007/s00382-014-2158-9</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><?label 1?><mixed-citation>ECMWF: ERA5 Reanalysis, European Centre for Medium-Range Weather Forecasts [data set], <uri>https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5</uri>, last access: 22 May 2022.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><?label 1?><mixed-citation>Eyring, V., Bony, S., Meehl, G. A., Senior, C. A., Stevens, B., Stouffer, R. J., and Taylor, K. E.: Overview of the Coupled Model Intercomparison Project Phase 6 (CMIP6) experimental design and organization, Geosci. Model Dev., 9, 1937–1958, <ext-link xlink:href="https://doi.org/10.5194/gmd-9-1937-2016" ext-link-type="DOI">10.5194/gmd-9-1937-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><?label 1?><mixed-citation>Fan, T., Zhao, C., Dong, X., Liu, X., Yang, X., Zhang, F., Shi, C., Wang,
Y., and Wu, F.: Quantify contribution of aerosol errors to cloud fraction
biases in CMIP5 Atmospheric Model Intercomparison Project simulations, Int.
J. Climatol., 38, 3140–3156, <ext-link xlink:href="https://doi.org/10.1002/joc.5490" ext-link-type="DOI">10.1002/joc.5490</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><?label 1?><mixed-citation>Fasullo, J. T. and Trenberth, K. E.: The annual cycle of the energy budget.
Part I: Global mean and land-ocean exchanges, J. Climate, 21, 2297–2312,
<ext-link xlink:href="https://doi.org/10.1175/2007JCLI1935.1" ext-link-type="DOI">10.1175/2007JCLI1935.1</ext-link>, 2008a.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><?label 1?><mixed-citation>Fasullo, J. T. and Trenberth, K. E.: The annual cycle of the energy budget.
Part II: Meridional structures and poleward transports, J. Climate, 21,
2313–2325, <ext-link xlink:href="https://doi.org/10.1175/2007JCLI1936.1" ext-link-type="DOI">10.1175/2007JCLI1936.1</ext-link>, 2008b.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><?label 1?><mixed-citation>GEBA: Surface measured energy fluxes, ETH Zurich (Switzerland) [data set], <uri>https://geba.ethz.ch/data-retrieval.html</uri>, last access: 25 February 2022.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><?label 1?><mixed-citation>Ghan, S. J., Liu, X., Easter, R. C., Zaveri, R., Rasch, P. J., Yoon, J.-H,
and Eaton, B.: Toward a minimal representation of aerosols in climate
models: Comparative decomposition of aerosol direct, semidirect, and
indirect radiative forcing, J. Climate, 25, 6461–6476,
<ext-link xlink:href="https://doi.org/10.1175/JCLI-D-11-00650.1" ext-link-type="DOI">10.1175/JCLI-D-11-00650.1</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib15"><label>15</label><?label 1?><mixed-citation>Gilgen, H., Wild, M., and Ohmura, A.: Means and trends of shortwave
irradiance at the surface estimated from global energy balance archive data,
J. Climate, 11, 2042–2061,
<ext-link xlink:href="https://doi.org/10.1175/1520-0442(1998)011&lt;2042:MATOSI&gt;2.0.CO;2" ext-link-type="DOI">10.1175/1520-0442(1998)011&lt;2042:MATOSI&gt;2.0.CO;2</ext-link>, 1998.</mixed-citation></ref>
      <ref id="bib1.bib16"><label>16</label><?label 1?><mixed-citation>He, Y., Wang, K., Zhou, C., and Wild, M.: A revisit of global dimming and
brightening based on the sunshine duration, Geophys. Res. Lett., 45,
4281–4289, <ext-link xlink:href="https://doi.org/10.1029/2018GL077424" ext-link-type="DOI">10.1029/2018GL077424</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib17"><label>17</label><?label 1?><mixed-citation>Hersbach, H., Bell, B., Berrisford, P., Hirahara, S., Horányi, A.,
Muñoz-Sabater, J., Nicolas, J., Peubey, C., Radu, R., Schepers, D.,
Simmons, A., Soci, C., Abdalla, S., Abellan, X., Balsamo, G., Bechtold, P.,
Biavati, G., Bidlot, J., Bonavita, M., De Chiara, G., Dahlgren, P., Dee, D.,
Diamantakis, M., Dragani, R., Flemming, J., Forbes, R., Fuentes, M., Geer,
A., Haimberger, L., Healy, S., Hogan, R. J., Hólm, E., Janisková,
M., Keeley, S., Laloyaux, P., Lopez, P., Lupu, C., Radnoti, G., de Rosnay,
P., Rozum, I., Vamborg, F., Villaume, S., and Thépaut, J.: The ERA5
global reanalysis, Q. J. Roy. Meteor. Soc., 146, 1999–2049,
<ext-link xlink:href="https://doi.org/10.1002/qj.3803" ext-link-type="DOI">10.1002/qj.3803</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bib18"><label>18</label><?label 1?><mixed-citation>Huang, G., Li, Z., Li, X., Liang, S., Yang, K., Wang, D., and Zhang, Y.:
Estimating surface solar irradiance from satellites: Past, present, and
future perspectives, Remote Sens. Environ., 233, 111371,
<ext-link xlink:href="https://doi.org/10.1016/j.rse.2019.111371" ext-link-type="DOI">10.1016/j.rse.2019.111371</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib19"><label>19</label><?label 1?><mixed-citation>Kato, S., Rose, F. G., Rutan, D. A., Thorsen, T. J., Loeb, N. G., Doelling,
D. R., Huang, X., Smith, W. L., Su, W., and Ham, S.: Surface Irradiances of
Edition 4.0 Clouds and the Earth's Radiant Energy System (CERES) Energy
Balanced and Filled (EBAF) data product, J. Climate, 31, 4501–4527,
<ext-link xlink:href="https://doi.org/10.1175/JCLI-D-17-0523.1" ext-link-type="DOI">10.1175/JCLI-D-17-0523.1</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib20"><label>20</label><?label 1?><mixed-citation>Kim, B. and Lee, K.: Radiation component calculation and energy budget
snalysis for the Korean Peninsula region, Remote Sens., 10, 1147,
<ext-link xlink:href="https://doi.org/10.3390/rs10071147" ext-link-type="DOI">10.3390/rs10071147</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib21"><label>21</label><?label 1?><mixed-citation>King, M. D., Platnick, S., Menzel, W. P., Ackerman, S. A., and Hubanks, P.
A.: Spatial and temporal distribution of clouds observed by MODIS onboard
the Terra and Aqua satellites, IEEE T. Geosci. Remote Sens., 51, 3826–3852,
<ext-link xlink:href="https://doi.org/10.1109/TGRS.2012.2227333" ext-link-type="DOI">10.1109/TGRS.2012.2227333</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib22"><label>22</label><?label 1?><mixed-citation>L'Ecuyer, T. S., Beaudoing, H. K., Rodell, M., Olson, W., Lin, B., Kato, S.,
Clayson, C. A., Wood, E., Sheffield, J., Adler, R., Huffman, G., Bosilovich,
M., Gu, G., Robertson, F., Houser, P. R., Chambers, D., Famiglietti, J. S.,
Fetzer, E., Liu, W. T., Gao, X., Schlosser, C. A., Clark, E., Lettenmaier,
D. P., and Hilburn, K.: The observed state of the energy budget in the early
twenty-First century, J. Climate, 28, 8319–8346,
<ext-link xlink:href="https://doi.org/10.1175/JCLI-D-14-00556.1" ext-link-type="DOI">10.1175/JCLI-D-14-00556.1</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib23"><label>23</label><?label 1?><mixed-citation>Lei, Y., Letu, H., Shang, H., and Shi, J.: Cloud cover over the Tibetan
Plateau and eastern China: a comparison of ERA5 and ERA-Interim with
satellite observations, Clim. Dynam., 54, 2941–2957,
<ext-link xlink:href="https://doi.org/10.1007/s00382-020-05149-x" ext-link-type="DOI">10.1007/s00382-020-05149-x</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bib24"><label>24</label><?label 1?><mixed-citation>Letu, H., Nakajima, T. Y., Wang, T., Shang, H., Ma, R., Yang, K., Baran,
A. J., Riedi, J., Ishimoto, H., and Yoshida, M.: A new benchmark for surface
radiation products over the East Asia-Pacific region retrieved from the
Himawari-8/AHI next-generation geostationary satellite, B. Am. Meteorol.
Soc., 103, E873–E888, <ext-link xlink:href="https://doi.org/10.1175/BAMS-D-20-0148.1" ext-link-type="DOI">10.1175/BAMS-D-20-0148.1</ext-link>, 2022.</mixed-citation></ref>
      <ref id="bib1.bib25"><label>25</label><?label 1?><mixed-citation>Li, J. and Mao, J.: A preliminary evaluation of global and East Asian cloud
radiative effects in reanalyses, Atmos. Ocean. Sci. Lett., 8, 100–106,
<ext-link xlink:href="https://doi.org/10.3878/AOSL20140093" ext-link-type="DOI">10.3878/AOSL20140093</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib26"><label>26</label><?label 1?><mixed-citation>Li, J., Mao, J., and Wang, F.: Comparative study of five current reanalyses
in characterizing total cloud fraction and top-of-the-atmosphere cloud
radiative effects over the Asian monsoon region, Int. J. Climatol., 37,
5047–5067, <ext-link xlink:href="https://doi.org/10.1002/joc.5143" ext-link-type="DOI">10.1002/joc.5143</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib27"><label>27</label><?label 1?><mixed-citation>Li, J.-L. F., Waliser, D. E., Stephens, G., Lee, S., L'Ecuyer, T., Kato,
S., Loeb, N., and Ma, H.: Characterizing and understanding radiation budget
biases in CMIP3/CMIP5 GCMs, contemporary GCM, and reanalysis, J. Geophys.
Res.-Atmos., 118, 8166–8184, <ext-link xlink:href="https://doi.org/10.1002/jgrd.50378" ext-link-type="DOI">10.1002/jgrd.50378</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib28"><label>28</label><?label 1?><mixed-citation>Li, Z., Niu, F., Fan, J., Liu, Y., Rosenfeld, D., and Ding, Y.: Long-term
impacts of aerosols on the vertical development of clouds and precipitation,
Nat. Geosci., 4, 888–894, <ext-link xlink:href="https://doi.org/10.1038/ngeo1313" ext-link-type="DOI">10.1038/ngeo1313</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bib29"><label>29</label><?label 1?><mixed-citation>Liao, H., Chang, W., and Yang, Y.: Climatic effects of air pollutants over
china: A review, Adv. Atmos. Sci., 32, 115–139,
<ext-link xlink:href="https://doi.org/10.1007/s00376-014-0013-x" ext-link-type="DOI">10.1007/s00376-014-0013-x</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib30"><label>30</label><?label 1?><mixed-citation>Lin, B., Stackhouse Jr., P. W., Minnis, P., Wielicki, B. A., Hu, Y., Sun,
W., Fan, T., and Hinkelman, L. M.: Assessment of global annual atmospheric
energy balance from satellite observations, J. Geophys. Res.-Atmos., 113, D16114, <ext-link xlink:href="https://doi.org/10.1029/2008JD009869" ext-link-type="DOI">10.1029/2008JD009869</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib31"><label>31</label><?label 1?><mixed-citation>Liu, Y., Bao, Q., Duan, A., Qian, Z. A., and Wu, G.: Recent progress in the
impact of the Tibetan Plateau on climate in China, Adv. Atmos. Sci., 24,
1060–1076, <ext-link xlink:href="https://doi.org/10.1007/s00376-007-1060-3" ext-link-type="DOI">10.1007/s00376-007-1060-3</ext-link>, 2007.</mixed-citation></ref>
      <ref id="bib1.bib32"><label>32</label><?label 1?><mixed-citation>Loeb, N. G., Doelling, D. R., Wang, H., Su, W., Nguyen, C., Corbett, J. G.,
Liang, L., Mitrescu, C., Rose, F. G., and Kato, S.: Clouds and the Earth's
Radiant Energy System (CERES) Energy Balanced and Filled (EBAF)
Top-of-Atmosphere (TOA) Edition-4.0 data product, J. Climate, 31, 895–918,
<ext-link xlink:href="https://doi.org/10.1175/JCLI-D-17-0208.1" ext-link-type="DOI">10.1175/JCLI-D-17-0208.1</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib33"><label>33</label><?label 1?><mixed-citation>Mayer, M., Tietsche, S., Haimberger, L., Tsubouchi, T., Mayer, J., and Zuo,
H.: An improved estimate of the coupled Arctic energy budget, J. Climate,
32, 7915–7934, <ext-link xlink:href="https://doi.org/10.1175/JCLI-D-19-0233.1" ext-link-type="DOI">10.1175/JCLI-D-19-0233.1</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib34"><label>34</label><?label 1?><mixed-citation>Mercado, L. M., Bellouin, N., Sitch, S., Boucher, O., Huntingford, C., Wild,
M., and Cox, P. M.: Impact of changes in diffuse radiation on the global
land carbon sink, Nature, 458, 1014–1017, <ext-link xlink:href="https://doi.org/10.1038/nature07949" ext-link-type="DOI">10.1038/nature07949</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib35"><label>35</label><?label 1?><mixed-citation>Ohmura, A.: Cryosphere During the Twentieth Century, The state of the
planet: frontiers and challenges in geophysics, Geophys. Monogr. Ser., 150,
239–257, <ext-link xlink:href="https://doi.org/10.1029/150gm19" ext-link-type="DOI">10.1029/150gm19</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bib36"><label>36</label><?label 1?><mixed-citation>Previdi, M., Smith, K. L., and Polvani, L. M.: How well do the CMIP5 models
simulate the Antarctic atmospheric energy budget?, J. Climate, 28,
7933–7942, <ext-link xlink:href="https://doi.org/10.1175/JCLI-D-15-0027.1" ext-link-type="DOI">10.1175/JCLI-D-15-0027.1</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib37"><label>37</label><?label 1?><mixed-citation>Raschke, E., Kinne, S., Rossow, W. B., Stackhouse, P. W., and Wild, M.:
Comparison of radiative energy flows in observational datasets and climate
modeling, J. Appl. Meteorol. Clim., 55, 93–117,
<ext-link xlink:href="https://doi.org/10.1175/JAMC-D-14-0281.1" ext-link-type="DOI">10.1175/JAMC-D-14-0281.1</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib38"><label>38</label><?label 1?><mixed-citation>Simmons, A. J., Jones, P. D., Da Costa Bechtold, V., Beljaars, A. C. M.,
Kållberg, P. W., Saarinen, S., Uppala, S. M., Viterbo, P., and Wedi, N.:
Comparison of trends and low-frequency variability in CRU, ERA-40, and
NCEP/NCAR analyses of surface air temperature, J. Geophys. Res.-Atmos., 109, D24115, <ext-link xlink:href="https://doi.org/10.1029/2004JD005306" ext-link-type="DOI">10.1029/2004JD005306</ext-link>, 2004.</mixed-citation></ref>
      <ref id="bib1.bib39"><label>39</label><?label 1?><mixed-citation>Stephens, G. L.: Cloud feedbacks in the climate system: A critical review,
J. Climate, 18, 237–273, <ext-link xlink:href="https://doi.org/10.1175/JCLI-3243.1" ext-link-type="DOI">10.1175/JCLI-3243.1</ext-link>, 2005.</mixed-citation></ref>
      <ref id="bib1.bib40"><label>40</label><?label 1?><mixed-citation>Stephens, G. L., Li, J., Wild, M., Clayson, C. A., Loeb, N., Kato, S.,
L'Ecuyer, T., Stackhouse, P. W., Lebsock, M., and Andrews, T.: An update on
Earth's energy balance in light of the latest global observations, Nat.
Geosci., 5, 691–696, <ext-link xlink:href="https://doi.org/10.1038/ngeo1580" ext-link-type="DOI">10.1038/ngeo1580</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib41"><label>41</label><?label 1?><mixed-citation>Tang, W.-J., Yang, K., Qin, J., Cheng, C. C. K., and He, J.: Solar radiation trend across China in recent decades: a revisit with quality-controlled data, Atmos. Chem. Phys., 11, 393–406, <ext-link xlink:href="https://doi.org/10.5194/acp-11-393-2011" ext-link-type="DOI">10.5194/acp-11-393-2011</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bib42"><label>42</label><?label 1?><mixed-citation>Tang, W. J., Qin, J., Yang, K., Zhu, F., and Zhou, X.: Does ERA5 outperform
satellite products in estimating atmospheric downward longwave radiation at
the surface?, Atmos. Res., 252, 105453, <ext-link xlink:href="https://doi.org/10.1016/j.atmosres.2021.105453" ext-link-type="DOI">10.1016/j.atmosres.2021.105453</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bib43"><label>43</label><?label 1?><mixed-citation>Thomas, C. M., Dong, B., and Haines, K.: Inverse modeling of global and
regional energy and water cycle fluxes using earth observation data, J.
Climate, 33, 1707–1723, <ext-link xlink:href="https://doi.org/10.1175/JCLI-D-19-0343.1" ext-link-type="DOI">10.1175/JCLI-D-19-0343.1</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bib44"><label>44</label><?label 1?><mixed-citation>Trenberth, K. E., Fasullo, J. T., and Kiehl, J.: Earth's global energy
budget, B. Am. Meteorol. Soc., 90, 311–324, <ext-link xlink:href="https://doi.org/10.1175/2008BAMS2634.1" ext-link-type="DOI">10.1175/2008BAMS2634.1</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib45"><label>45</label><?label 1?><mixed-citation>Trenberth, K. E., Fasullo, J. T., and Balmaseda, M. A.: Earth's energy
imbalance, J. Climate, 27, 3129–3144, <ext-link xlink:href="https://doi.org/10.1175/JCLI-D-13-00294.1" ext-link-type="DOI">10.1175/JCLI-D-13-00294.1</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib46"><label>46</label><?label 1?><mixed-citation>Trolliet, M., Walawender, J. P., Bourlès, B., Boilley, A., Trentmann, J., Blanc, P., Lefèvre, M., and Wald, L.: Downwelling surface solar irradiance in the tropical Atlantic Ocean: a comparison of re-analyses and satellite-derived data sets to PIRATA measurements, Ocean Sci., 14, 1021–1056, <ext-link xlink:href="https://doi.org/10.5194/os-14-1021-2018" ext-link-type="DOI">10.5194/os-14-1021-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib47"><label>47</label><?label 1?><mixed-citation>Urraca, R., Huld, T., Gracia-Amillo, A., Martinez-de-Pison, F. J., Kaspar,
F., and Sanz-Garcia, A.: Evaluation of global horizontal irradiance
estimates from ERA5 and COSMO-REA6 reanalyses using ground and
satellite-based data, Sol. Energy, 164, 339–354,
<ext-link xlink:href="https://doi.org/10.1016/j.solener.2018.02.059" ext-link-type="DOI">10.1016/j.solener.2018.02.059</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib48"><label>48</label><?label 1?><mixed-citation>Wang, H., Zhang, H., Xie, B., Jing, X., He, J., and Liu, Y.: Evaluating the
Impacts of Cloud Microphysical and Overlap Parameters on Simulated Clouds in
Global Climate Models, Adv. Atmos. Sci., 39, 2172–2187, <ext-link xlink:href="https://doi.org/10.1007/s00376-021-0369-7" ext-link-type="DOI">10.1007/s00376-021-0369-7</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bib49"><label>49</label><?label 1?><mixed-citation>Wang, K.: Measurement biases explain discrepancies between the observed and
simulated decadal variability of surface incident solar radiation, Sci.
Rep., 4, 6144, <ext-link xlink:href="https://doi.org/10.1038/srep06144" ext-link-type="DOI">10.1038/srep06144</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib50"><label>50</label><?label 1?><mixed-citation>Wang, K., Ma, Q., Li, Z., and Wang, J.: Decadal variability of surface
incident solar radiation over China: Observations, satellite retrievals, and
reanalyses, J. Geophys. Res.-Atmos., 120, 6500–6514,
<ext-link xlink:href="https://doi.org/10.1002/2015JD023420" ext-link-type="DOI">10.1002/2015JD023420</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib51"><label>51</label><?label 1?><mixed-citation>Wang, Q., Zhang, H., Yang, S., Chen, Q., Zhou, X., Shi, G., Cheng, Y., and
Wild, M.: Potential driving factors on surface solar radiation trends over
China in recent years, Remote Sens., 13, 704, <ext-link xlink:href="https://doi.org/10.3390/rs13040704" ext-link-type="DOI">10.3390/rs13040704</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bib52"><label>52</label><?label 1?><mixed-citation>Wang, Y. and Wild, M.: A new look at solar dimming and brightening in
China, Geophys. Res. Lett., 43, 11777–11785​​​​​​​, <ext-link xlink:href="https://doi.org/10.1002/2016GL071009" ext-link-type="DOI">10.1002/2016GL071009</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bib53"><label>53</label><?label 1?><mixed-citation>Wang, Y., Trentmann, J., Yuan, W., and Wild, M.: Validation of CM SAF
CLARA-A2 and SARAH-E surface solar radiation datasets over China, Remote
Sens., 10, 1977, <ext-link xlink:href="https://doi.org/10.3390/rs10121977" ext-link-type="DOI">10.3390/rs10121977</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib54"><label>54</label><?label 1?><mixed-citation>Wang, Y., Wild, M., Sanchez-Lorenzo, A., and Manara, V.: Urbanization effect on trends in sunshine duration in China, Ann. Geophys., 35, 839–851, <ext-link xlink:href="https://doi.org/10.5194/angeo-35-839-2017" ext-link-type="DOI">10.5194/angeo-35-839-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib55"><label>55</label><?label 1?><mixed-citation>Wang, Z., Lin, L., Xu, Y., Che, H., Zhang, X., Zhang, H., Dong, W., Wang,
C., Gui, K., and Xie, B.: Incorrect Asian aerosols affecting the attribution
and projection of regional climate change in CMIP6 models, npj Clim. Atmos.
Sci., 4, 1–8, <ext-link xlink:href="https://doi.org/10.1038/s41612-020-00159-2" ext-link-type="DOI">10.1038/s41612-020-00159-2</ext-link>, 2021.</mixed-citation></ref>
      <ref id="bib1.bib56"><label>56</label><?label 1?><mixed-citation>Wei, J., Peng, Y., Guo, J., and Sun, L.: Performance of MODIS Collection 6.1
Level 3 aerosol products in spatial-temporal variations over land, Atmos.
Environ., 206, 30–44, <ext-link xlink:href="https://doi.org/10.1016/j.atmosenv.2019.03.001" ext-link-type="DOI">10.1016/j.atmosenv.2019.03.001</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib57"><label>57</label><?label 1?><mixed-citation>Wild, M.: Progress and challenges in the estimation of the global energy
balance, AIP Conf. Proc., 1810, 20004, <ext-link xlink:href="https://doi.org/10.1063/1.4975500" ext-link-type="DOI">10.1063/1.4975500</ext-link>, 2017a.</mixed-citation></ref>
      <ref id="bib1.bib58"><label>58</label><?label 1?><mixed-citation>Wild, M.: Towards global estimates of the surface energy budget, Curr. Clim.
Change Rep., 3, 87–97, <ext-link xlink:href="https://doi.org/10.1007/s40641-017-0058-x" ext-link-type="DOI">10.1007/s40641-017-0058-x</ext-link>, 2017b.</mixed-citation></ref>
      <ref id="bib1.bib59"><label>59</label><?label 1?><mixed-citation>Wild, M.: The global energy balance as represented in CMIP6 climate models,
Clim. Dynam., 55, 553–577, <ext-link xlink:href="https://doi.org/10.1007/s00382-020-05282-7" ext-link-type="DOI">10.1007/s00382-020-05282-7</ext-link>, 2020.</mixed-citation></ref>
      <ref id="bib1.bib60"><label>60</label><?label 1?><mixed-citation>Wild, M., Ohmura, A., Gilgen, H., and Roeckner, E.: Validation of general
circulation model radiative fluxes using surface observations, J. Climate,
8, 1309–1324, <ext-link xlink:href="https://doi.org/10.1175/1520-0442(1995)008&lt;1309:VOGCMR&gt;2.0.CO;2" ext-link-type="DOI">10.1175/1520-0442(1995)008&lt;1309:VOGCMR&gt;2.0.CO;2</ext-link>, 1995.</mixed-citation></ref>
      <ref id="bib1.bib61"><label>61</label><?label 1?><mixed-citation>Wild, M., Grieser, J., and Schär, C.: Combined surface solar brightening
and increasing greenhouse effect support recent intensification of the
global land-based hydrological cycle, Geophys. Res. Lett., 35, L17706,
<ext-link xlink:href="https://doi.org/10.1029/2008GL034842" ext-link-type="DOI">10.1029/2008GL034842</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib62"><label>62</label><?label 1?><mixed-citation>Wild, M., Folini, D., Schär, C., Loeb, N., Dutton, E. G., and
König-Langlo, G.: The global energy balance from a surface perspective,
Clim. Dynam., 40, 3107–3134, <ext-link xlink:href="https://doi.org/10.1007/s00382-012-1569-8" ext-link-type="DOI">10.1007/s00382-012-1569-8</ext-link>, 2013a.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bib63"><label>63</label><?label 1?><mixed-citation>Wild, M., Folini, D., Schär, C., Loeb, N., Dutton, E. G., and
König-Langlo, G.: A new diagram of the global energy balance, AIP
Conf. Proc., 1531, 628–631, <ext-link xlink:href="https://doi.org/10.1063/1.4804848" ext-link-type="DOI">10.1063/1.4804848</ext-link>, 2013b.</mixed-citation></ref>
      <ref id="bib1.bib64"><label>64</label><?label 1?><mixed-citation>Wild, M., Folini, D., Hakuba, M. Z., Schär, C., Seneviratne, S. I.,
Kato, S., Rutan, D., Ammann, C., Wood, E. F., and König-Langlo, G.: The
energy balance over land and oceans: an assessment based on direct
observations and CMIP5 climate models, Clim. Dynam., 44, 3393–3429,
<ext-link xlink:href="https://doi.org/10.1007/s00382-014-2430-z" ext-link-type="DOI">10.1007/s00382-014-2430-z</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib65"><label>65</label><?label 1?><mixed-citation>Wild, M., Hakuba, M. Z., Folini, D., Schär, C., and Long, C.: New
estimates of the Earth radiation budget under cloud-free conditions and
cloud radiative effects, AIP Conf. Proc., 1810, 90012, <ext-link xlink:href="https://doi.org/10.1063/1.4975552" ext-link-type="DOI">10.1063/1.4975552</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bib66"><label>66</label><?label 1?><mixed-citation>Wild, M., Hakuba, M. Z., Folini, D., Dörig-Ott, P., Schär, C., Kato,
S., and Long, C. N.: The cloud-free global energy balance and inferred cloud
radiative effects: an assessment based on direct observations and climate
models, Clim. Dynam., 52, 4787–4812, <ext-link xlink:href="https://doi.org/10.1007/s00382-018-4413-y" ext-link-type="DOI">10.1007/s00382-018-4413-y</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib67"><label>67</label><?label 1?><mixed-citation>Wu, G., Duan, A., Liu, Y., Mao, J., Ren, R., Bao, Q., He, B., Liu, B., and
Hu, W.: Tibetan Plateau climate dynamics: recent research progress and
outlook, Natl. Sci. Rev., 2, 100–116, <ext-link xlink:href="https://doi.org/10.1093/nsr/nwu045" ext-link-type="DOI">10.1093/nsr/nwu045</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bib68"><label>68</label><?label 1?><mixed-citation>Xu, J., Liang, S., and Jiang, B.: A global long-term (1981–2019) daily land surface radiation budget product from AVHRR satellite data using a residual convolutional neural network, Earth Syst. Sci. Data, 14, 2315–2341, <ext-link xlink:href="https://doi.org/10.5194/essd-14-2315-2022" ext-link-type="DOI">10.5194/essd-14-2315-2022</ext-link>, 2022.</mixed-citation></ref>
      <ref id="bib1.bib69"><label>69</label><?label 1?><mixed-citation>Xu, X., Lu, C., Shi, X., and Gao, S.: World water tower: An atmospheric
perspective, Geophys. Res. Lett., 35, L20815, <ext-link xlink:href="https://doi.org/10.1029/2008GL035867" ext-link-type="DOI">10.1029/2008GL035867</ext-link>,
2008a.</mixed-citation></ref>
      <ref id="bib1.bib70"><label>70</label><?label 1?><mixed-citation>
Xu, X., Zhang, R., Koike, T., Lu, C., Shi, X., Zhang, S., Bian, L., Cheng,
X., Li, P., and Ding, G.: A new integrated observational system over the
Tibetan Plateau, B. Am. Meteorol. Soc., 89, 1492–1496, 2008b.</mixed-citation></ref>
      <ref id="bib1.bib71"><label>71</label><?label 1?><mixed-citation>Yang, S., Wang, X. L., and Wild, M.: Homogenization and trend analysis of
the 1958–2016 in situ surface solar radiation records in China, J. Climate,
31, 4529–4541, <ext-link xlink:href="https://doi.org/10.1175/JCLI-D-17-0891.1" ext-link-type="DOI">10.1175/JCLI-D-17-0891.1</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bib72"><label>72</label><?label 1?><mixed-citation>Yang, S., Wang, X. L., and Wild, M.: Causes of dimming and brightening in
China inferred from homogenized daily clear-sky and all-sky in situ surface
solar radiation records (1958–2016), J. Climate, 32, 5901–5913,
<ext-link xlink:href="https://doi.org/10.1175/JCLI-D-18-0666.1" ext-link-type="DOI">10.1175/JCLI-D-18-0666.1</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib73"><label>73</label><?label 1?><mixed-citation>You, Q., Liu, J., and Pepin, N.: Changes of summer cloud water content in
China from ERA-Interim reanalysis, Global Planet. Change, 175, 201–210,
<ext-link xlink:href="https://doi.org/10.1016/j.gloplacha.2019.02.014" ext-link-type="DOI">10.1016/j.gloplacha.2019.02.014</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bib74"><label>74</label><?label 1?><mixed-citation>Zhang, H., Zhao, M., Chen, Q., Wang, Q., Zhao, S., Zhou, X., and Peng, J.:
Water and ice cloud optical thickness changes and radiative effects in East
Asia, J. Quant. Spectrosc. Radiat. Transf., 254, 107213,
<ext-link xlink:href="https://doi.org/10.1016/j.jqsrt.2020.107213" ext-link-type="DOI">10.1016/j.jqsrt.2020.107213</ext-link>, 2020.</mixed-citation></ref>

  </ref-list></back>
    <!--<article-title-html>An assessment of land energy balance over East Asia from multiple lines of evidence and the roles of the Tibet Plateau, aerosols, and clouds</article-title-html>
<abstract-html/>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Boeke, R. C. and Taylor, P. C.: Evaluation of the Arctic surface radiation budget in CMIP5 models, J. Geophys. Res.-Atmos., 121, 8525–8548, <a href="https://doi.org/10.1002/2016JD025099" target="_blank">https://doi.org/10.1002/2016JD025099</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>
CERES: Data Products, National Aeronautics and Space Administration (NASA) [data set], <a href="https://ceres.larc.nasa.gov/data/" target="_blank"/>, last access: 20 March 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>
Christensen, M. W., Behrangi, A., L'Ecuyer, T. S., Wood, N. B., Lebsock, M.
D., and Stephens, G. L.: Arctic observation and reanalysis integrated
system: A new data product for validation and climate study, B. Am.
Meteorol. Soc., 97, 907–916, <a href="https://doi.org/10.1175/BAMS-D-14-00273.1" target="_blank">https://doi.org/10.1175/BAMS-D-14-00273.1</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>
CMA: Surface observational radiation data, China Meteorological Administration National Meteorological Information Center [data set], <a href="http://data.cma.cn/enl" target="_blank"/>, last access: 10 February 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>
CMIP6: Climate models, The World Climate Research Programme [data set], <a href="https://pcmdi.llnl.gov/CMIP6/" target="_blank"/>, last access: 14 April 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>
de Leeuw, G., Sogacheva, L., Rodriguez, E., Kourtidis, K., Georgoulias, A. K., Alexandri, G., Amiridis, V., Proestakis, E., Marinou, E., Xue, Y., and van der A, R.: Two decades of satellite observations of AOD over mainland China using ATSR-2, AATSR and MODIS/Terra: data set evaluation and large-scale patterns, Atmos. Chem. Phys., 18, 1573–1592, <a href="https://doi.org/10.5194/acp-18-1573-2018" target="_blank">https://doi.org/10.5194/acp-18-1573-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>
Dolinar, E. K., Dong, X., Xi, B., Jiang, J. H., and Su, H.: Evaluation of
CMIP5 simulated clouds and TOA radiation budgets using NASA satellite
observations, Clim. Dynam., 44, 2229–2247,
<a href="https://doi.org/10.1007/s00382-014-2158-9" target="_blank">https://doi.org/10.1007/s00382-014-2158-9</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>
ECMWF: ERA5 Reanalysis, European Centre for Medium-Range Weather Forecasts [data set], <a href="https://www.ecmwf.int/en/forecasts/datasets/reanalysis-datasets/era5" target="_blank"/>, last access: 22 May 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>
Eyring, V., Bony, S., Meehl, G. A., Senior, C. A., Stevens, B., Stouffer, R. J., and Taylor, K. E.: Overview of the Coupled Model Intercomparison Project Phase 6 (CMIP6) experimental design and organization, Geosci. Model Dev., 9, 1937–1958, <a href="https://doi.org/10.5194/gmd-9-1937-2016" target="_blank">https://doi.org/10.5194/gmd-9-1937-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>
Fan, T., Zhao, C., Dong, X., Liu, X., Yang, X., Zhang, F., Shi, C., Wang,
Y., and Wu, F.: Quantify contribution of aerosol errors to cloud fraction
biases in CMIP5 Atmospheric Model Intercomparison Project simulations, Int.
J. Climatol., 38, 3140–3156, <a href="https://doi.org/10.1002/joc.5490" target="_blank">https://doi.org/10.1002/joc.5490</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>
Fasullo, J. T. and Trenberth, K. E.: The annual cycle of the energy budget.
Part I: Global mean and land-ocean exchanges, J. Climate, 21, 2297–2312,
<a href="https://doi.org/10.1175/2007JCLI1935.1" target="_blank">https://doi.org/10.1175/2007JCLI1935.1</a>, 2008a.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>
Fasullo, J. T. and Trenberth, K. E.: The annual cycle of the energy budget.
Part II: Meridional structures and poleward transports, J. Climate, 21,
2313–2325, <a href="https://doi.org/10.1175/2007JCLI1936.1" target="_blank">https://doi.org/10.1175/2007JCLI1936.1</a>, 2008b.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation>
GEBA: Surface measured energy fluxes, ETH Zurich (Switzerland) [data set], <a href="https://geba.ethz.ch/data-retrieval.html" target="_blank"/>, last access: 25 February 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Ghan, S. J., Liu, X., Easter, R. C., Zaveri, R., Rasch, P. J., Yoon, J.-H,
and Eaton, B.: Toward a minimal representation of aerosols in climate
models: Comparative decomposition of aerosol direct, semidirect, and
indirect radiative forcing, J. Climate, 25, 6461–6476,
<a href="https://doi.org/10.1175/JCLI-D-11-00650.1" target="_blank">https://doi.org/10.1175/JCLI-D-11-00650.1</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>15</label><mixed-citation>
Gilgen, H., Wild, M., and Ohmura, A.: Means and trends of shortwave
irradiance at the surface estimated from global energy balance archive data,
J. Climate, 11, 2042–2061,
<a href="https://doi.org/10.1175/1520-0442(1998)011&lt;2042:MATOSI&gt;2.0.CO;2" target="_blank">https://doi.org/10.1175/1520-0442(1998)011&lt;2042:MATOSI&gt;2.0.CO;2</a>, 1998.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>16</label><mixed-citation>
He, Y., Wang, K., Zhou, C., and Wild, M.: A revisit of global dimming and
brightening based on the sunshine duration, Geophys. Res. Lett., 45,
4281–4289, <a href="https://doi.org/10.1029/2018GL077424" target="_blank">https://doi.org/10.1029/2018GL077424</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>17</label><mixed-citation>
Hersbach, H., Bell, B., Berrisford, P., Hirahara, S., Horányi, A.,
Muñoz-Sabater, J., Nicolas, J., Peubey, C., Radu, R., Schepers, D.,
Simmons, A., Soci, C., Abdalla, S., Abellan, X., Balsamo, G., Bechtold, P.,
Biavati, G., Bidlot, J., Bonavita, M., De Chiara, G., Dahlgren, P., Dee, D.,
Diamantakis, M., Dragani, R., Flemming, J., Forbes, R., Fuentes, M., Geer,
A., Haimberger, L., Healy, S., Hogan, R. J., Hólm, E., Janisková,
M., Keeley, S., Laloyaux, P., Lopez, P., Lupu, C., Radnoti, G., de Rosnay,
P., Rozum, I., Vamborg, F., Villaume, S., and Thépaut, J.: The ERA5
global reanalysis, Q. J. Roy. Meteor. Soc., 146, 1999–2049,
<a href="https://doi.org/10.1002/qj.3803" target="_blank">https://doi.org/10.1002/qj.3803</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>18</label><mixed-citation>
Huang, G., Li, Z., Li, X., Liang, S., Yang, K., Wang, D., and Zhang, Y.:
Estimating surface solar irradiance from satellites: Past, present, and
future perspectives, Remote Sens. Environ., 233, 111371,
<a href="https://doi.org/10.1016/j.rse.2019.111371" target="_blank">https://doi.org/10.1016/j.rse.2019.111371</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>19</label><mixed-citation>
Kato, S., Rose, F. G., Rutan, D. A., Thorsen, T. J., Loeb, N. G., Doelling,
D. R., Huang, X., Smith, W. L., Su, W., and Ham, S.: Surface Irradiances of
Edition 4.0 Clouds and the Earth's Radiant Energy System (CERES) Energy
Balanced and Filled (EBAF) data product, J. Climate, 31, 4501–4527,
<a href="https://doi.org/10.1175/JCLI-D-17-0523.1" target="_blank">https://doi.org/10.1175/JCLI-D-17-0523.1</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>20</label><mixed-citation>
Kim, B. and Lee, K.: Radiation component calculation and energy budget
snalysis for the Korean Peninsula region, Remote Sens., 10, 1147,
<a href="https://doi.org/10.3390/rs10071147" target="_blank">https://doi.org/10.3390/rs10071147</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>21</label><mixed-citation>
King, M. D., Platnick, S., Menzel, W. P., Ackerman, S. A., and Hubanks, P.
A.: Spatial and temporal distribution of clouds observed by MODIS onboard
the Terra and Aqua satellites, IEEE T. Geosci. Remote Sens., 51, 3826–3852,
<a href="https://doi.org/10.1109/TGRS.2012.2227333" target="_blank">https://doi.org/10.1109/TGRS.2012.2227333</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>22</label><mixed-citation>
L'Ecuyer, T. S., Beaudoing, H. K., Rodell, M., Olson, W., Lin, B., Kato, S.,
Clayson, C. A., Wood, E., Sheffield, J., Adler, R., Huffman, G., Bosilovich,
M., Gu, G., Robertson, F., Houser, P. R., Chambers, D., Famiglietti, J. S.,
Fetzer, E., Liu, W. T., Gao, X., Schlosser, C. A., Clark, E., Lettenmaier,
D. P., and Hilburn, K.: The observed state of the energy budget in the early
twenty-First century, J. Climate, 28, 8319–8346,
<a href="https://doi.org/10.1175/JCLI-D-14-00556.1" target="_blank">https://doi.org/10.1175/JCLI-D-14-00556.1</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>23</label><mixed-citation>
Lei, Y., Letu, H., Shang, H., and Shi, J.: Cloud cover over the Tibetan
Plateau and eastern China: a comparison of ERA5 and ERA-Interim with
satellite observations, Clim. Dynam., 54, 2941–2957,
<a href="https://doi.org/10.1007/s00382-020-05149-x" target="_blank">https://doi.org/10.1007/s00382-020-05149-x</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>24</label><mixed-citation>
Letu, H., Nakajima, T. Y., Wang, T., Shang, H., Ma, R., Yang, K., Baran,
A. J., Riedi, J., Ishimoto, H., and Yoshida, M.: A new benchmark for surface
radiation products over the East Asia-Pacific region retrieved from the
Himawari-8/AHI next-generation geostationary satellite, B. Am. Meteorol.
Soc., 103, E873–E888, <a href="https://doi.org/10.1175/BAMS-D-20-0148.1" target="_blank">https://doi.org/10.1175/BAMS-D-20-0148.1</a>, 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>25</label><mixed-citation>
Li, J. and Mao, J.: A preliminary evaluation of global and East Asian cloud
radiative effects in reanalyses, Atmos. Ocean. Sci. Lett., 8, 100–106,
<a href="https://doi.org/10.3878/AOSL20140093" target="_blank">https://doi.org/10.3878/AOSL20140093</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>26</label><mixed-citation>
Li, J., Mao, J., and Wang, F.: Comparative study of five current reanalyses
in characterizing total cloud fraction and top-of-the-atmosphere cloud
radiative effects over the Asian monsoon region, Int. J. Climatol., 37,
5047–5067, <a href="https://doi.org/10.1002/joc.5143" target="_blank">https://doi.org/10.1002/joc.5143</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>27</label><mixed-citation>
Li, J.-L. F., Waliser, D. E., Stephens, G., Lee, S., L'Ecuyer, T., Kato,
S., Loeb, N., and Ma, H.: Characterizing and understanding radiation budget
biases in CMIP3/CMIP5 GCMs, contemporary GCM, and reanalysis, J. Geophys.
Res.-Atmos., 118, 8166–8184, <a href="https://doi.org/10.1002/jgrd.50378" target="_blank">https://doi.org/10.1002/jgrd.50378</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>28</label><mixed-citation>
Li, Z., Niu, F., Fan, J., Liu, Y., Rosenfeld, D., and Ding, Y.: Long-term
impacts of aerosols on the vertical development of clouds and precipitation,
Nat. Geosci., 4, 888–894, <a href="https://doi.org/10.1038/ngeo1313" target="_blank">https://doi.org/10.1038/ngeo1313</a>, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>29</label><mixed-citation>
Liao, H., Chang, W., and Yang, Y.: Climatic effects of air pollutants over
china: A review, Adv. Atmos. Sci., 32, 115–139,
<a href="https://doi.org/10.1007/s00376-014-0013-x" target="_blank">https://doi.org/10.1007/s00376-014-0013-x</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib30"><label>30</label><mixed-citation>
Lin, B., Stackhouse Jr., P. W., Minnis, P., Wielicki, B. A., Hu, Y., Sun,
W., Fan, T., and Hinkelman, L. M.: Assessment of global annual atmospheric
energy balance from satellite observations, J. Geophys. Res.-Atmos., 113, D16114, <a href="https://doi.org/10.1029/2008JD009869" target="_blank">https://doi.org/10.1029/2008JD009869</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib31"><label>31</label><mixed-citation>
Liu, Y., Bao, Q., Duan, A., Qian, Z. A., and Wu, G.: Recent progress in the
impact of the Tibetan Plateau on climate in China, Adv. Atmos. Sci., 24,
1060–1076, <a href="https://doi.org/10.1007/s00376-007-1060-3" target="_blank">https://doi.org/10.1007/s00376-007-1060-3</a>, 2007.
</mixed-citation></ref-html>
<ref-html id="bib1.bib32"><label>32</label><mixed-citation>
Loeb, N. G., Doelling, D. R., Wang, H., Su, W., Nguyen, C., Corbett, J. G.,
Liang, L., Mitrescu, C., Rose, F. G., and Kato, S.: Clouds and the Earth's
Radiant Energy System (CERES) Energy Balanced and Filled (EBAF)
Top-of-Atmosphere (TOA) Edition-4.0 data product, J. Climate, 31, 895–918,
<a href="https://doi.org/10.1175/JCLI-D-17-0208.1" target="_blank">https://doi.org/10.1175/JCLI-D-17-0208.1</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib33"><label>33</label><mixed-citation>
Mayer, M., Tietsche, S., Haimberger, L., Tsubouchi, T., Mayer, J., and Zuo,
H.: An improved estimate of the coupled Arctic energy budget, J. Climate,
32, 7915–7934, <a href="https://doi.org/10.1175/JCLI-D-19-0233.1" target="_blank">https://doi.org/10.1175/JCLI-D-19-0233.1</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib34"><label>34</label><mixed-citation>
Mercado, L. M., Bellouin, N., Sitch, S., Boucher, O., Huntingford, C., Wild,
M., and Cox, P. M.: Impact of changes in diffuse radiation on the global
land carbon sink, Nature, 458, 1014–1017, <a href="https://doi.org/10.1038/nature07949" target="_blank">https://doi.org/10.1038/nature07949</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib35"><label>35</label><mixed-citation>
Ohmura, A.: Cryosphere During the Twentieth Century, The state of the
planet: frontiers and challenges in geophysics, Geophys. Monogr. Ser., 150,
239–257, <a href="https://doi.org/10.1029/150gm19" target="_blank">https://doi.org/10.1029/150gm19</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib36"><label>36</label><mixed-citation>
Previdi, M., Smith, K. L., and Polvani, L. M.: How well do the CMIP5 models
simulate the Antarctic atmospheric energy budget?, J. Climate, 28,
7933–7942, <a href="https://doi.org/10.1175/JCLI-D-15-0027.1" target="_blank">https://doi.org/10.1175/JCLI-D-15-0027.1</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib37"><label>37</label><mixed-citation>
Raschke, E., Kinne, S., Rossow, W. B., Stackhouse, P. W., and Wild, M.:
Comparison of radiative energy flows in observational datasets and climate
modeling, J. Appl. Meteorol. Clim., 55, 93–117,
<a href="https://doi.org/10.1175/JAMC-D-14-0281.1" target="_blank">https://doi.org/10.1175/JAMC-D-14-0281.1</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib38"><label>38</label><mixed-citation>
Simmons, A. J., Jones, P. D., Da Costa Bechtold, V., Beljaars, A. C. M.,
Kållberg, P. W., Saarinen, S., Uppala, S. M., Viterbo, P., and Wedi, N.:
Comparison of trends and low-frequency variability in CRU, ERA-40, and
NCEP/NCAR analyses of surface air temperature, J. Geophys. Res.-Atmos., 109, D24115, <a href="https://doi.org/10.1029/2004JD005306" target="_blank">https://doi.org/10.1029/2004JD005306</a>, 2004.
</mixed-citation></ref-html>
<ref-html id="bib1.bib39"><label>39</label><mixed-citation>
Stephens, G. L.: Cloud feedbacks in the climate system: A critical review,
J. Climate, 18, 237–273, <a href="https://doi.org/10.1175/JCLI-3243.1" target="_blank">https://doi.org/10.1175/JCLI-3243.1</a>, 2005.
</mixed-citation></ref-html>
<ref-html id="bib1.bib40"><label>40</label><mixed-citation>
Stephens, G. L., Li, J., Wild, M., Clayson, C. A., Loeb, N., Kato, S.,
L'Ecuyer, T., Stackhouse, P. W., Lebsock, M., and Andrews, T.: An update on
Earth's energy balance in light of the latest global observations, Nat.
Geosci., 5, 691–696, <a href="https://doi.org/10.1038/ngeo1580" target="_blank">https://doi.org/10.1038/ngeo1580</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib41"><label>41</label><mixed-citation>
Tang, W.-J., Yang, K., Qin, J., Cheng, C. C. K., and He, J.: Solar radiation trend across China in recent decades: a revisit with quality-controlled data, Atmos. Chem. Phys., 11, 393–406, <a href="https://doi.org/10.5194/acp-11-393-2011" target="_blank">https://doi.org/10.5194/acp-11-393-2011</a>, 2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib42"><label>42</label><mixed-citation>
Tang, W. J., Qin, J., Yang, K., Zhu, F., and Zhou, X.: Does ERA5 outperform
satellite products in estimating atmospheric downward longwave radiation at
the surface?, Atmos. Res., 252, 105453, <a href="https://doi.org/10.1016/j.atmosres.2021.105453" target="_blank">https://doi.org/10.1016/j.atmosres.2021.105453</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib43"><label>43</label><mixed-citation>
Thomas, C. M., Dong, B., and Haines, K.: Inverse modeling of global and
regional energy and water cycle fluxes using earth observation data, J.
Climate, 33, 1707–1723, <a href="https://doi.org/10.1175/JCLI-D-19-0343.1" target="_blank">https://doi.org/10.1175/JCLI-D-19-0343.1</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib44"><label>44</label><mixed-citation>
Trenberth, K. E., Fasullo, J. T., and Kiehl, J.: Earth's global energy
budget, B. Am. Meteorol. Soc., 90, 311–324, <a href="https://doi.org/10.1175/2008BAMS2634.1" target="_blank">https://doi.org/10.1175/2008BAMS2634.1</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib45"><label>45</label><mixed-citation>
Trenberth, K. E., Fasullo, J. T., and Balmaseda, M. A.: Earth's energy
imbalance, J. Climate, 27, 3129–3144, <a href="https://doi.org/10.1175/JCLI-D-13-00294.1" target="_blank">https://doi.org/10.1175/JCLI-D-13-00294.1</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib46"><label>46</label><mixed-citation>
Trolliet, M., Walawender, J. P., Bourlès, B., Boilley, A., Trentmann, J., Blanc, P., Lefèvre, M., and Wald, L.: Downwelling surface solar irradiance in the tropical Atlantic Ocean: a comparison of re-analyses and satellite-derived data sets to PIRATA measurements, Ocean Sci., 14, 1021–1056, <a href="https://doi.org/10.5194/os-14-1021-2018" target="_blank">https://doi.org/10.5194/os-14-1021-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib47"><label>47</label><mixed-citation>
Urraca, R., Huld, T., Gracia-Amillo, A., Martinez-de-Pison, F. J., Kaspar,
F., and Sanz-Garcia, A.: Evaluation of global horizontal irradiance
estimates from ERA5 and COSMO-REA6 reanalyses using ground and
satellite-based data, Sol. Energy, 164, 339–354,
<a href="https://doi.org/10.1016/j.solener.2018.02.059" target="_blank">https://doi.org/10.1016/j.solener.2018.02.059</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib48"><label>48</label><mixed-citation>
Wang, H., Zhang, H., Xie, B., Jing, X., He, J., and Liu, Y.: Evaluating the
Impacts of Cloud Microphysical and Overlap Parameters on Simulated Clouds in
Global Climate Models, Adv. Atmos. Sci., 39, 2172–2187, <a href="https://doi.org/10.1007/s00376-021-0369-7" target="_blank">https://doi.org/10.1007/s00376-021-0369-7</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib49"><label>49</label><mixed-citation>
Wang, K.: Measurement biases explain discrepancies between the observed and
simulated decadal variability of surface incident solar radiation, Sci.
Rep., 4, 6144, <a href="https://doi.org/10.1038/srep06144" target="_blank">https://doi.org/10.1038/srep06144</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib50"><label>50</label><mixed-citation>
Wang, K., Ma, Q., Li, Z., and Wang, J.: Decadal variability of surface
incident solar radiation over China: Observations, satellite retrievals, and
reanalyses, J. Geophys. Res.-Atmos., 120, 6500–6514,
<a href="https://doi.org/10.1002/2015JD023420" target="_blank">https://doi.org/10.1002/2015JD023420</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib51"><label>51</label><mixed-citation>
Wang, Q., Zhang, H., Yang, S., Chen, Q., Zhou, X., Shi, G., Cheng, Y., and
Wild, M.: Potential driving factors on surface solar radiation trends over
China in recent years, Remote Sens., 13, 704, <a href="https://doi.org/10.3390/rs13040704" target="_blank">https://doi.org/10.3390/rs13040704</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib52"><label>52</label><mixed-citation>
Wang, Y. and Wild, M.: A new look at solar dimming and brightening in
China, Geophys. Res. Lett., 43, 11777–11785​​​​​​​, <a href="https://doi.org/10.1002/2016GL071009" target="_blank">https://doi.org/10.1002/2016GL071009</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib53"><label>53</label><mixed-citation>
Wang, Y., Trentmann, J., Yuan, W., and Wild, M.: Validation of CM SAF
CLARA-A2 and SARAH-E surface solar radiation datasets over China, Remote
Sens., 10, 1977, <a href="https://doi.org/10.3390/rs10121977" target="_blank">https://doi.org/10.3390/rs10121977</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib54"><label>54</label><mixed-citation>
Wang, Y., Wild, M., Sanchez-Lorenzo, A., and Manara, V.: Urbanization effect on trends in sunshine duration in China, Ann. Geophys., 35, 839–851, <a href="https://doi.org/10.5194/angeo-35-839-2017" target="_blank">https://doi.org/10.5194/angeo-35-839-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib55"><label>55</label><mixed-citation>
Wang, Z., Lin, L., Xu, Y., Che, H., Zhang, X., Zhang, H., Dong, W., Wang,
C., Gui, K., and Xie, B.: Incorrect Asian aerosols affecting the attribution
and projection of regional climate change in CMIP6 models, npj Clim. Atmos.
Sci., 4, 1–8, <a href="https://doi.org/10.1038/s41612-020-00159-2" target="_blank">https://doi.org/10.1038/s41612-020-00159-2</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib56"><label>56</label><mixed-citation>
Wei, J., Peng, Y., Guo, J., and Sun, L.: Performance of MODIS Collection 6.1
Level 3 aerosol products in spatial-temporal variations over land, Atmos.
Environ., 206, 30–44, <a href="https://doi.org/10.1016/j.atmosenv.2019.03.001" target="_blank">https://doi.org/10.1016/j.atmosenv.2019.03.001</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib57"><label>57</label><mixed-citation>
Wild, M.: Progress and challenges in the estimation of the global energy
balance, AIP Conf. Proc., 1810, 20004, <a href="https://doi.org/10.1063/1.4975500" target="_blank">https://doi.org/10.1063/1.4975500</a>, 2017a.
</mixed-citation></ref-html>
<ref-html id="bib1.bib58"><label>58</label><mixed-citation>
Wild, M.: Towards global estimates of the surface energy budget, Curr. Clim.
Change Rep., 3, 87–97, <a href="https://doi.org/10.1007/s40641-017-0058-x" target="_blank">https://doi.org/10.1007/s40641-017-0058-x</a>, 2017b.
</mixed-citation></ref-html>
<ref-html id="bib1.bib59"><label>59</label><mixed-citation>
Wild, M.: The global energy balance as represented in CMIP6 climate models,
Clim. Dynam., 55, 553–577, <a href="https://doi.org/10.1007/s00382-020-05282-7" target="_blank">https://doi.org/10.1007/s00382-020-05282-7</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib60"><label>60</label><mixed-citation>
Wild, M., Ohmura, A., Gilgen, H., and Roeckner, E.: Validation of general
circulation model radiative fluxes using surface observations, J. Climate,
8, 1309–1324, <a href="https://doi.org/10.1175/1520-0442(1995)008&lt;1309:VOGCMR&gt;2.0.CO;2" target="_blank">https://doi.org/10.1175/1520-0442(1995)008&lt;1309:VOGCMR&gt;2.0.CO;2</a>, 1995.
</mixed-citation></ref-html>
<ref-html id="bib1.bib61"><label>61</label><mixed-citation>
Wild, M., Grieser, J., and Schär, C.: Combined surface solar brightening
and increasing greenhouse effect support recent intensification of the
global land-based hydrological cycle, Geophys. Res. Lett., 35, L17706,
<a href="https://doi.org/10.1029/2008GL034842" target="_blank">https://doi.org/10.1029/2008GL034842</a>, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib62"><label>62</label><mixed-citation>
Wild, M., Folini, D., Schär, C., Loeb, N., Dutton, E. G., and
König-Langlo, G.: The global energy balance from a surface perspective,
Clim. Dynam., 40, 3107–3134, <a href="https://doi.org/10.1007/s00382-012-1569-8" target="_blank">https://doi.org/10.1007/s00382-012-1569-8</a>, 2013a.

</mixed-citation></ref-html>
<ref-html id="bib1.bib63"><label>63</label><mixed-citation>
Wild, M., Folini, D., Schär, C., Loeb, N., Dutton, E. G., and
König-Langlo, G.: A new diagram of the global energy balance, AIP
Conf. Proc., 1531, 628–631, <a href="https://doi.org/10.1063/1.4804848" target="_blank">https://doi.org/10.1063/1.4804848</a>, 2013b.
</mixed-citation></ref-html>
<ref-html id="bib1.bib64"><label>64</label><mixed-citation>
Wild, M., Folini, D., Hakuba, M. Z., Schär, C., Seneviratne, S. I.,
Kato, S., Rutan, D., Ammann, C., Wood, E. F., and König-Langlo, G.: The
energy balance over land and oceans: an assessment based on direct
observations and CMIP5 climate models, Clim. Dynam., 44, 3393–3429,
<a href="https://doi.org/10.1007/s00382-014-2430-z" target="_blank">https://doi.org/10.1007/s00382-014-2430-z</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib65"><label>65</label><mixed-citation>
Wild, M., Hakuba, M. Z., Folini, D., Schär, C., and Long, C.: New
estimates of the Earth radiation budget under cloud-free conditions and
cloud radiative effects, AIP Conf. Proc., 1810, 90012, <a href="https://doi.org/10.1063/1.4975552" target="_blank">https://doi.org/10.1063/1.4975552</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib66"><label>66</label><mixed-citation>
Wild, M., Hakuba, M. Z., Folini, D., Dörig-Ott, P., Schär, C., Kato,
S., and Long, C. N.: The cloud-free global energy balance and inferred cloud
radiative effects: an assessment based on direct observations and climate
models, Clim. Dynam., 52, 4787–4812, <a href="https://doi.org/10.1007/s00382-018-4413-y" target="_blank">https://doi.org/10.1007/s00382-018-4413-y</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib67"><label>67</label><mixed-citation>
Wu, G., Duan, A., Liu, Y., Mao, J., Ren, R., Bao, Q., He, B., Liu, B., and
Hu, W.: Tibetan Plateau climate dynamics: recent research progress and
outlook, Natl. Sci. Rev., 2, 100–116, <a href="https://doi.org/10.1093/nsr/nwu045" target="_blank">https://doi.org/10.1093/nsr/nwu045</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib68"><label>68</label><mixed-citation>
Xu, J., Liang, S., and Jiang, B.: A global long-term (1981–2019) daily land surface radiation budget product from AVHRR satellite data using a residual convolutional neural network, Earth Syst. Sci. Data, 14, 2315–2341, <a href="https://doi.org/10.5194/essd-14-2315-2022" target="_blank">https://doi.org/10.5194/essd-14-2315-2022</a>, 2022.
</mixed-citation></ref-html>
<ref-html id="bib1.bib69"><label>69</label><mixed-citation>
Xu, X., Lu, C., Shi, X., and Gao, S.: World water tower: An atmospheric
perspective, Geophys. Res. Lett., 35, L20815, <a href="https://doi.org/10.1029/2008GL035867" target="_blank">https://doi.org/10.1029/2008GL035867</a>,
2008a.
</mixed-citation></ref-html>
<ref-html id="bib1.bib70"><label>70</label><mixed-citation>
Xu, X., Zhang, R., Koike, T., Lu, C., Shi, X., Zhang, S., Bian, L., Cheng,
X., Li, P., and Ding, G.: A new integrated observational system over the
Tibetan Plateau, B. Am. Meteorol. Soc., 89, 1492–1496, 2008b.
</mixed-citation></ref-html>
<ref-html id="bib1.bib71"><label>71</label><mixed-citation>
Yang, S., Wang, X. L., and Wild, M.: Homogenization and trend analysis of
the 1958–2016 in situ surface solar radiation records in China, J. Climate,
31, 4529–4541, <a href="https://doi.org/10.1175/JCLI-D-17-0891.1" target="_blank">https://doi.org/10.1175/JCLI-D-17-0891.1</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib72"><label>72</label><mixed-citation>
Yang, S., Wang, X. L., and Wild, M.: Causes of dimming and brightening in
China inferred from homogenized daily clear-sky and all-sky in situ surface
solar radiation records (1958–2016), J. Climate, 32, 5901–5913,
<a href="https://doi.org/10.1175/JCLI-D-18-0666.1" target="_blank">https://doi.org/10.1175/JCLI-D-18-0666.1</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib73"><label>73</label><mixed-citation>
You, Q., Liu, J., and Pepin, N.: Changes of summer cloud water content in
China from ERA-Interim reanalysis, Global Planet. Change, 175, 201–210,
<a href="https://doi.org/10.1016/j.gloplacha.2019.02.014" target="_blank">https://doi.org/10.1016/j.gloplacha.2019.02.014</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib74"><label>74</label><mixed-citation>
Zhang, H., Zhao, M., Chen, Q., Wang, Q., Zhao, S., Zhou, X., and Peng, J.:
Water and ice cloud optical thickness changes and radiative effects in East
Asia, J. Quant. Spectrosc. Radiat. Transf., 254, 107213,
<a href="https://doi.org/10.1016/j.jqsrt.2020.107213" target="_blank">https://doi.org/10.1016/j.jqsrt.2020.107213</a>, 2020.
</mixed-citation></ref-html>--></article>
