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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">GMD</journal-id><journal-title-group>
    <journal-title>Geoscientific Model Development</journal-title>
    <abbrev-journal-title abbrev-type="publisher">GMD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Geosci. Model Dev.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1991-9603</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/gmd-14-1253-2021</article-id><title-group><article-title>Using the anomaly forcing Community Land Model (CLM 4.5)<?xmltex \hack{\break}?> for crop yield
projections</article-title><alt-title>Anomaly forcing CLM</alt-title>
      </title-group><?xmltex \runningtitle{Anomaly forcing CLM}?><?xmltex \runningauthor{Y. Lu and X. Yang}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Lu</surname><given-names>Yaqiong</given-names></name>
          <email>yaqiong@imde.ac.cn</email>
        <ext-link>https://orcid.org/0000-0002-3791-1727</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Yang</surname><given-names>Xianyu</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Institute of Mountain Hazards and Environment, Chinese Academy
of Sciences, Chengdu 610040, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>National Center for Atmospheric Research, Boulder, CO 80305, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Chengdu University of Information Technology, Chengdu 610225, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yaqiong Lu (yaqiong@imde.ac.cn)</corresp></author-notes><pub-date><day>8</day><month>March</month><year>2021</year></pub-date>
      
      <volume>14</volume>
      <issue>3</issue>
      <fpage>1253</fpage><lpage>1265</lpage>
      <history>
        <date date-type="received"><day>6</day><month>June</month><year>2020</year></date>
           <date date-type="rev-request"><day>24</day><month>August</month><year>2020</year></date>
           <date date-type="rev-recd"><day>20</day><month>January</month><year>2021</year></date>
           <date date-type="accepted"><day>21</day><month>January</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Yaqiong Lu</copyright-statement>
        <copyright-year>2021</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://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021.html">This article is available from https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021.html</self-uri><self-uri xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021.pdf">The full text article is available as a PDF file from https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e104">Crop growth in land surface models normally requires high-temporal-resolution climate data (3-hourly or 6-hourly), but such high-temporal-resolution climate data are not provided by many climate model simulations
due to expensive storage, which limits modeling choices if there is an
interest in a particular climate simulation that only saved monthly outputs.
The Community Land Surface Model (CLM) has proposed an alternative approach
for utilizing monthly climate outputs as forcing data since version 4.5, and
it is called the anomaly forcing CLM. However, such an approach has never
been validated for crop yield projections. In our work, we created anomaly
forcing datasets for three climate scenarios (1.5 <inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, 2.0 <inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, and RCP4.5) and validated crop yields against the
standard CLM forcing with the same climate scenarios using 3-hourly data. We
found that the anomaly forcing CLM could not produce crop yields identical
to the standard CLM due to the different submonthly variations, crop
yields were underestimated by 5 %–8 % across the three scenarios (1.5, 2.0 <inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and RCP4.5) for the global average, and
28 %–41 % of cropland showed significantly different yields. However, the
anomaly forcing CLM effectively captured the relative changes between
scenarios and over time, as well as regional crop yield variations. We
recommend that such an approach be used for qualitative analysis of crop
yields when only monthly outputs are available. Our approach can be adopted
by other land surface models to expand their capabilities for utilizing
monthly climate data.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e143">Increasing numbers of future climate scenarios exhibit large uncertainties
for crop yield projections. Crop yields may increase or decrease depending
on which climate projection is used  (Lobell et al., 2008; Rosenzweig et
al., 2014; Urban et al., 2012). Ensemble future climate projections, such as
CMIP5, showed a large range of future climate projections, even for one
emission scenario  (Knutti and Sedlacek, 2013). Using all future
climate projections is not realistic not only because of the computational
expense but also because many of these future climate projections only save
monthly climate outputs that are not suitable for crop models that require
high-temporal-resolution forcing data. Some standalone process-based crop
models run in daily time steps, and some crop models embedded in land
surface models need at least 6 h of climate data as the forcing data to
represent diurnal cycles. Only a small portion of the CMIP5 (Coupled Model
Intercomparison Project 5) simulations (<inline-formula><mml:math id="M4" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 25 %) can be used as the
forcing data for crop models, leaving little room for crop modelers to
choose a particular climate model projection that is of interest.</p>
      <p id="d1e153">The Community Land Model (CLM)  (Oleson et al., 2013) is a
state-of-the-art land surface model that simulates biogeophysical (radiation
transfer, vegetation-soil-hydrology, surface energy fluxes, etc.) and
biogeochemical (soil carbon and nitrogen cycle, vegetation photosynthesis,
dynamic vegetation growth, etc.) processes. CLM is the default land model in
the Community Earth System Model (CESM)  (Hurrell et al., 2013), and it
can be run either online coupled with the rest of CESM (atmosphere and
ocean) or offline (the land<?pagebreak page1254?> model only, forced with climate datasets) for
multiple spatial extents (site, regional, and global) and at different
resolutions. The crop model derived from AgroIBIS  (Kucharik, 2003)
was introduced to CLM4.0 by Levis et al. (2012), and it is
responsible for crop growth phenology (temperature determined), carbon
allocation algorithms, and crop management (e.g., irrigation). The crop
model in CLM runs when the soil biogeochemical component is active, and it
was tested with the CLM-CN in version 4.0 and tested with CLM-BGC in version
4.5, where CLM-CN and CLM-BGC are officially supported soil biogeochemical
components in CLM4.0 and CLM4.5 respectively. Since their introduction, crop
models in the CLM have been developed to represent more crop types and
processes, such as soybean nitrogen fixation (Drewniak et al.,
2013), ozone impacts on yields    (Lombardozzi et al., 2015),
winter wheat growth responses to cold hazards  (Lu et al.,
2017), and maize growth responses to heat stress  (Peng et al., 2018). CLM
simulates nine crop types, accounting for 54 % of global total crop
production (other production is represented by the most similar crop type):
maize, soybean, spring wheat, winter wheat, cotton, rice, sugarcane,
tropical maize, and tropical soybean. In this study, we used CLM version 4.5
(Oleson et al., 2013).</p>
      <p id="d1e156">Since version 4.5, CLM offers a built-in function that indirectly uses
monthly climate outputs as the forcing data and is called the anomaly
forcing CLM  (Lawrence et al., 2015). Anomaly forcing CLM reconstructs new
subdaily forcing data by applying the precalculated future monthly anomaly
signals to user-defined historical subdaily forcing data, referred to as the
reference data. The future monthly anomaly signals are calculated by the
future monthly climate outputs and by use of historical monthly outputs. The
choice of reference data is arbitrary. Any existing subdaily forcing data
(e.g., CRUNCEP, Viovy, 2018, QIAN, Qian et al., 2006) for CLM
can be used as the reference data. The historical monthly outputs are
recommended to be averaged over multiple years to represent the historical means and
avoid affecting the monthly anomaly signal by rare, extreme events in a
particular year. Such an arbitrary choice is because the goal of the
original anomaly forcing CLM is not to reconstruct future forcing that is
identical to the actual future forcing when the high-temporal-resolution
data were saved. Rather, the original goal of the anomaly forcing CLM is to
understand the influences due to the anomaly signal by comparing the
simulation with the anomaly forcing CLM to the simulation run with the
reference data. The differences between the two simulations are due to the
anomaly signals.</p>
      <p id="d1e159">In our study, we modified the anomaly forcing CLM to fit our goals to
understand whether we could simply use the anomaly forcing CLM for crop
yield projections when only monthly climate data were available. We
carefully chose the historical monthly data and the reference data so that
the reconstructed future anomaly forcing had nearly identical monthly means
to the desired subdaily future forcing, but we used different submonthly
variations. We created anomaly forcing datasets for three future scenarios
(1.5 <inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, 2.0 <inline-formula><mml:math id="M6" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, and RCP4.5) for
2006–2075 for which both the subdaily and monthly climate outputs were
available from three CESM simulations. With the three paired CLM
simulations, we validated the anomaly forcing CLM by comparing it to the
standard CLM.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
      <p id="d1e188">The original anomaly forcing CLM has been available since CLM4.5. This
approach reconstructs the subdaily (3-hourly or 6-hourly) forcing data by
applying the monthly anomaly signal to user-selected subdaily reference
data; therefore, it indirectly uses the monthly atmospheric outputs as the
forcing data for CLM. This approach does not change any of the scientific
code in CLM; it only adds code that reads the monthly anomaly signals and
automatically applies these to the reference data while the CLM is running.
There were two monthly anomaly signals for RCP4.5 and RCP8.5 that were
generated using the CESM future projections and were ready for use. It is
the user's choice to select which subdaily reference (e.g., CRUNCEP or
CLMQIAN) and which years to use. By simply modifying the user_nl_cpl name list and adding data streams of the anomaly
forcing variables (see the appendix for the detailed usage), the anomaly
forcing CLM will automatically read the monthly anomaly signal and apply the
signal to each time step of the reference data within a month. When the
reference data period is shorter than the anomaly signal period, the anomaly
forcing CLM will cycle the same reference data until the simulation is
complete. Because the different selections of reference data can generate
different forcings, even with the same monthly anomaly signals, one should
not use the simulation from the anomaly forcing CLM to represent the actual
simulation. Rather, the original goal of the anomaly forcing CLM is to
compare the simulation with the anomaly forcing and simulation with the
reference forcing data to understand the effects of the monthly anomaly
signals on land surface variables.</p>
      <p id="d1e191">The goal of this work is to test how well crop yield projections from the
anomaly forcing CLM compare to the projections from the standard forcing
CLM, given that anomaly forcing has the same monthly average as standard
forcing. We selected three future scenarios for CESM simulations that saved
both monthly outputs and 3-hourly outputs, where the 3-hourly outputs were
directly used in the standard forcing CLM, and the monthly outputs were
indirectly used in the anomaly forcing CLM. We calculated the anomaly
forcing signals using the monthly CESM outputs and the monthly average of
reference data, so that when applying the anomaly signals to the reference
data, it is expected to generate identical monthly means as does regular
forcing. However, due to a limit in calculations of precipitation anomalies
(precipitation anomaly ratio less than 5) and how the CLM treats snow
and rainfall, the anomaly forcing CLM did not show<?pagebreak page1255?> identical snow and
rainfall monthly averages and introduced bias in the crop yield simulations
(see the results section).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e197">A summary of the original anomaly forcing CLM and the modifications
in this work.</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="justify" colwidth="5cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="8cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Original anomaly forcing CLM</oasis:entry>
         <oasis:entry colname="col3">Modifications in this work</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">3 h/6 h reference data</oasis:entry>
         <oasis:entry colname="col2">User choice</oasis:entry>
         <oasis:entry colname="col3">6 h Community Atmosphere Model outputs from one historical low-warming ensemble simulation 1996–2005</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Monthly anomaly signals</oasis:entry>
         <oasis:entry colname="col2">Existing for RCP4.5 and RCP8.5</oasis:entry>
         <oasis:entry colname="col3">Anomalies between future scenarios and monthly means of reference data <?xmltex \hack{\hfill\break}?>Three future scenarios: 1.5, 2.0 <inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and RCP4.5 <?xmltex \hack{\hfill\break}?>Each scenario had monthly outputs and 3 h outputs</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Goals</oasis:entry>
         <oasis:entry colname="col2">Climate impact due to anomaly signals when comparing the anomaly run with the reference run</oasis:entry>
         <oasis:entry colname="col3">Given that anomaly forcing has the same monthly mean as the standard CLM forcing, can we use it for crop yield projections?</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e278">We randomly chose the 6-hourly reference data (1996–2005) from one of the 11
historical low-warming ensemble CESM simulations. Additionally, we selected
three CESM future simulations for the 1.5 <inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, 2.0 <inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, and RCP4.5 scenarios, where all the three simulations
saved both the monthly outputs and the 3-hourly outputs. We then calculated
the monthly anomaly signal at each grid cell for each scenario (1.5, 2.0,
and RCP45) from 2006–2075. The monthly anomaly signals are differences for
temperature, specific humidity, wind, and air pressure and are ratios for
solar radiation and precipitation between the monthly outputs of each
scenario and the 1996–2005 averaged monthly values of the reference data.
The anomaly forcing signal has both spatial and monthly variations. When
running the anomaly forcing simulation for 2006–2070, CLM repeatedly uses
the 10-year reference period and applies the anomaly signal of a month to
all subdaily reference forcing in this month. For example, an anomaly
forcing simulation for 2006 January uses the 1996 January reference data
plus or multiplied by (if the anomaly signal is a ratio) the 2006 January
anomaly signal. If the 2006 January temperature anomaly is 1 K for a grid
cell, then all 1996 January reference data will be increased by 1 K for the
grid cell.</p>
      <p id="d1e299">The monthly anomaly signal is calculated at each grid cell (<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi></mml:mrow></mml:math></inline-formula>). For
temperature, pressure, wind, and humidity, the anomaly signal is the
difference between the future monthly data and the historical monthly
average (Eq. 1). For solar radiation, longwave radiation, and
precipitation, the anomaly signal is the ratio between the future monthly
data and the historical monthly average (Eq. 2). We set the maximum
ratio for precipitation to 5 to avoid unrealistic extreme precipitation,
which also introduced biases in precipitation (discussed in the discussion
section).

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M11" 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:msub><mml:mi mathvariant="normal">af</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">fut</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">hist</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub></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:msub><mml:mi mathvariant="normal">af</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">fut</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">hist</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          Here <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">af</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is anomaly forcing signal at a location <inline-formula><mml:math id="M13" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M14" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> in a
month <inline-formula><mml:math id="M15" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">fut</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the averaged future value, and <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">hist</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mi>m</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>
is the averaged historical value at a location <inline-formula><mml:math id="M18" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M19" display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula> in a month <inline-formula><mml:math id="M20" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>.</p>
      <p id="d1e529">We set up global CLM crop simulations (compset CLM45BGCCROP) at 1.9<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> by 2.5<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude by longitude, respectively, using the anomaly forcing CLM and
the regular forcing CLM for the 1.5 <inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, 2.0 <inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
warming, and RCP4.5 scenarios. All simulations used the default nitrogen
fertilization rates and a constant CO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> level of 359.8 ppm. For each
scenario, we validate the crop yield in the anomaly forcing CLM to the
regular forcing CLM to determine if we can use the anomaly forcing CLM for
future crop yield projections. We also studied whether the anomaly forcing
CLM has a similar crop growth response to transient CO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and nitrogen
fertilization. The transient CO<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and nitrogen fertilization did not add
extra computational cost compared to the constant CO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and nitrogen
fertilization simulation. However, due to our limited computational
resources we could not afford more experiments, and we only tested such responses
for the RCP4.5 scenario. The transient CO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> levels in the RCP45 scenario
gradually increased from 379 ppm in 2006 to 530 ppm in 2070. To test the
nitrogen fertilization effects, we simply added a zero nitrogen
fertilization simulation here. For the crop yield analysis, we aggregated
the individual crop yield into an integrated crop yield by area weighted
mean based on the crop area map MAPSMAP (<uri>https://www.mapspam.info/</uri>, last access: 1 March 2021) 2005
crop area. The regional crop yield was simply the regional averaged crop
yield at nine regions defined in Ren et al. (2018).</p>
      <p id="d1e617">We adopted the two-sample Kolmogorov–Smirnov test (KS test) to test the
statistical significance of differences between the anomaly forcing CLM and
the standard CLM for atmospheric forcing data and yield. We used the KS test
because some variables at some grid cells did not necessarily follow normal
distributions. The KS test is a nonparametric test that detects differences
in the empirical probability distributions between two samples, and the two
samples do not need to have normal distributions  (Justel et al., 1997;
Marozzi, 2013). When repeated using the 10-year reference data, we expected
that the 10-year-averaged monthly anomaly forcing would show no significant
differences from the regular forcing. Thus, for the atmospheric forcing
data, we tested probability distribution differences between anomaly forcing
and regular forcing for every 10-year averaged monthly dataset (sample size
was <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mn mathvariant="normal">7</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">12</mml:mn><mml:mo>=</mml:mo><mml:mn mathvariant="normal">84</mml:mn></mml:mrow></mml:math></inline-formula>). For crop yields, we used the every 10-year averaged annual
yields (sample size was 7). We used a linear regression coefficient (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>),
bias (Eq. 3), and percentage differences (Eq. 4) in our evaluations.

              <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M32" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtext>bias</mml:mtext><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="normal">CLM</mml:mi><mml:mtext>anomaly forcing</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">CLM</mml:mi><mml:mtext>standard</mml:mtext></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">%</mml:mi><mml:mtext>differences</mml:mtext><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mo>⋅</mml:mo><mml:mfenced close=")" open="("><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="normal">CLM</mml:mi><mml:mtext>anomaly
forcing</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="normal">CLM</mml:mi><mml:mi mathvariant="normal">standard</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e720">We aimed to generate an anomaly forcing that produced identical monthly
averages as its counterpart regular forcing (the desirable 3-hourly forcing
data for CLM) but with different submonthly variations. All atmospheric
forcing variables achieved this goal except for precipitation and its liquid
and ice components, rain and snow. The linear regression coefficients
(<inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) between anomaly forcing and standard forcing for the monthly means
of incoming solar radiation, bottom layer atmosphere temperatures (sigma
vertical coordinate, <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>.9925), pressures, humidities, and winds
all showed <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values above 0.99, and there were also no significant
differences for these variables for all grid cells. However, for rain and
snow, the <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values were 0.63–0.87 and 0.88–0.96<?pagebreak page1256?> across the three
scenarios, respectively (Fig. 1a). Statistically significant differences
were also found for rain and snow in many regions in the Northern Hemisphere
(Fig. 2). We used monthly variances as a measure of the submonthly
variations. We calculated the variation for 12 months in each decade, so
we have 7 decades and 12 months of variance, and the sample size is 84 when
setting up the regression. <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> for variances of forcing were low for
most variables except for incoming solar radiation (Fig. 1b). Such lower
<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> values indicated that anomaly forcing could not represent the
submonthly variations as well as the regular forcing.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e793">Linear regression coefficients (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>) between <bold>(a)</bold> decade-averaged monthly mean (sample size <inline-formula><mml:math id="M40" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 12 months <inline-formula><mml:math id="M41" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 7 decades <inline-formula><mml:math id="M42" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 84)
between anomaly forcing and regular forcing and <bold>(b)</bold> every 10-year-averaged
monthly variance between anomaly forcing and regular forcing.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f01.png"/>

      </fig>

      <p id="d1e841">There were two error sources for precipitation. First, there was overall
average lower precipitation in the anomaly forcing by 0.02, 0.03, and 0.2 mm/d in the 1.5, 2.0 <inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and
RCP45 scenarios, respectively. Such a slightly lower precipitation was because
we set the maximum precipitation anomaly ratio to 5 to avoid unrealistically
extreme precipitation levels. A ratio of 5 was suggested by NCAR scientists David
Lawrence and Sean Swenson, who are core developers of CLM and wrote the
initial anomaly forcing code in CLM. Most of the unrealistic extreme
precipitation ratios are actually due to the nearly zero historical
precipitation (the denominator of Eq. 2). The cap for the precipitation
anomaly ratio is used to avoid such situation. Second, the CLM used the
temperature in each time step to determine if the given precipitation was
rain or snow. Precipitation was rain when temperature was above 273.15 K,
otherwise it was snow. Therefore, the different submonthly variations in
temperature resulted in different submonthly variations for snow and rain.
Due to this problem, the lower precipitation did not evenly distribute to
the rain and snow bias, for which rain was underestimated by 0.08–0.3 mm/d, and snow was overestimated by 0.06–0.11 mm/d across the three
scenarios. The significantly different regions were mainly in the Northern
Hemisphere and the Antarctic, and most regions in the Southern Hemisphere
did not show significant differences in rain or snow. How the rain and snow
biases affected yield projections will be discussed.</p>
      <p id="d1e854">When compared to crop yield simulations in the standard CLM, the anomaly
forcing CLM underestimated crop yields by 5 %–8 % across the three scenarios
for the global average, and 28 %–41 % of cropland showed statistically
significant differences in yields. The rainfed crop yield differences across
the three scenarios showed largely similar spatial distributions:
overestimation in the northern US and Europe and underestimation in the
Southern Hemisphere and in East Asia (Fig. 3d–f). The overestimated
rainfed crop yield (mainly for maize and wheat) in the anomaly forcing CLM
is due to higher water availability in these regions, which is a result of
higher snow in the anomaly forcing CLM. For irrigated crops, such
overestimations in the northern US and Europe disappear (Fig. 3g–i)
because sufficient irrigation was added to the irrigated soil column in the
standard CLM, which removed the plant water stress that was seen for rainfed
crops. However, the underestimations in the Southern Hemisphere and East
Asia were persistent, because water availability does not cause yield
differences for irrigated crops; we suspect such underestimations were
caused by the other error in forcing data: the different submonthly
variations in the forcing data.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e859">70-year averaged differences between anomaly forcing and regular
forcing for rain <bold>(a–c)</bold> and snow <bold>(d–f)</bold> for the 1.5, 2.0 <inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and
RCP4.5 scenarios. All differences shown here are statistically significant
differences tested using the Kolmogorov–Smirnov test with a sample size of 84.
The gray areas are regions that did not show significant differences.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f02.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e885">The percentage differences of 70-year integrated yields between
the anomaly forcing CLM and the standard CLM for all crops <bold>(a–c)</bold>, rainfed
crops <bold>(d–f)</bold>, and irrigated crops <bold>(g–i)</bold> for the 1.5, 2.0 <inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and RCP45 scenarios. The white regions are where no crops
grow based on the historical crop map in 2005 (MAPSPAM 2005;
<uri>https://www.mapspam.info/</uri>, last access: 1 March 2021). For plots <bold>(a)</bold>–<bold>(c)</bold>, we showed only the significant
differences as determined using the Kolmogorov–Smirnov test with a sample
size of 7. The regions with insignificant differences are masked as gray in
<bold>(a)</bold>–<bold>(c)</bold>. For plots <bold>(d)</bold>–<bold>(i)</bold>, we did not mask the insignificant differences to show an
overall bias.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f03.png"/>

      </fig>

      <?pagebreak page1257?><p id="d1e934">The global 70-year averaged yields <inline-formula><mml:math id="M46" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> standard deviation in the
standard CLM (Ren et al., 2018) and in the anomaly forcing CLM are
4.38 <inline-formula><mml:math id="M47" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.09 and 4.03 <inline-formula><mml:math id="M48" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.16 t/ha, respectively, in the 1.5 <inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C scenario; 4.36 <inline-formula><mml:math id="M50" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.11 and 4.01 <inline-formula><mml:math id="M51" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.14 t/ha,
respectively, in the 2.0 <inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C scenario; and 3.95 <inline-formula><mml:math id="M53" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.13 and 3.72 <inline-formula><mml:math id="M54" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.14, respectively, in the RCP45 scenario (Fig. 4). The anomaly
forcing CLM captured the regional yield variations. Latin America (LAC)
showed the highest yield while India (IND) showed the lowest yields for both
the anomaly forcing CLM and the standard CLM across the three scenarios.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1008">Regional comparisons of the 70-year integrated mean yields and
yield standard deviations between the anomaly forcing CLM and the standard
CLM. The error bars indicate 70-year yield standard deviations. CHN: China;
EU: European Union; IND: India; LAC: Latin America; ODC: other developing
countries; OIC: other industrialized countries; SSA: sub-Saharan Africa; TC:
transition countries; USA: United States.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f04.png"/>

      </fig>

      <p id="d1e1017">Although the crop yields were underestimated, the anomaly forcing CLM could
qualitatively represent the spatial yield differences between two climate
scenarios. Comparing 2.0 to 1.5 <inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, there was a
4 %–8 % yield increase in the northern US and a 0 %–4 % yield decrease (Fig. 5a) in the southeastern US. When comparing the RCP45 to the 1.5 <inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C scenario, crop yields in the US were largely reduced (up to
50 %). The anomaly forcing CLM clearly captured these yield differences
(Fig. 5b and d).</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="d1e1040">The percentage of 70-year integrated yield differences between 2.0
and 1.5 <inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C <bold>(a, b)</bold> and between RCP45 and 1.5 <bold>(c, d)</bold>
in the standard CLM and the anomaly forcing CLM.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f05.png"/>

      </fig>

      <p id="d1e1064">The anomaly forcing CLM also captured yield changes over time for each
climate scenario. The three scenarios showed some similarities in yield
changes from 2006–2015<?pagebreak page1258?> to 2066–2075. For example, crop yields increased in
southeastern China and decreased in sub-Saharan Africa. There were also yield
changes that were unique to each scenario that were also found in the
anomaly forcing CLM. For example, crop yields increased in Europe for the
1.5 <inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C scenario (Fig. 6a–b) while they decreased in Europe for
the 2.0 <inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and RCP45 scenarios (Fig. 6c–f), and crop yields
declined in the US for the RCP45 scenario (Fig. 6e–f) while they
increased for the 1.5 and 2.0 <inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C scenarios (Fig. 6a–d).</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="d1e1096">The percentage yield difference from 2006–2015 to 2066–2075 in the
standard CLM and anomaly forcing CLM across the three scenarios.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f06.png"/>

      </fig>

      <p id="d1e1106">All simulations in the above evaluations adopted a constant CO<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> level
(359.8 ppm) and crop-type-dependent fixed nitrogen fertilization (25–500 kgN/ha), so whether the anomaly forcing CLM simulated a similar or different
crop growth response to CO<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or nitrogen fertilization is unknown. Due
to limited computational resources, we tested crop responses to transient
CO<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and nitrogen fertilization only for the RCP45 scenario and assumed
that the other scenarios would show the same differences as the RCP45
scenario. The transient CO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the RCP45 scenario gradually increased
from 379 ppm in 2006 to 530 ppm in 2075. To test the effects of nitrogen
fertilization, we simply added a zero nitrogen fertilization simulation.
Although all grid cells had the same amounts of CO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> increase in a given
year (no spatial<?pagebreak page1259?> variation), crop yields had spatial variations in response
to transient CO<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Most regions showed a 5 %–10 % yield increase, but
some regions showed much higher yield increases, such as northern India, the
southern edge of the Sahara, and Australia (Fig. 7a). Such crop yield
responses to transient CO<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> spatial patterns were also captured by the
anomaly forcing CLM (Fig. 7b). Similar for the crop yield responses to
nitrogen fertilization, the anomaly forcing CLM simulated crop yield
increase spatial patterns (Fig. 7c–d), in which the Southern Hemisphere
and Asia had greater yield increases in response to nitrogen fertilization.</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="d1e1175">70-year averaged integrated crop yield response to transient CO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and to no nitrogen fertilization in the anomaly forcing CLM <bold>(a, b)</bold> and in
the standard CLM <bold>(c, d)</bold> for the RCP45 scenario.</p></caption>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://gmd.copernicus.org/articles/14/1253/2021/gmd-14-1253-2021-f07.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e1207">In this work, we created anomaly forcing datasets for three future climate
scenarios, and we validated the crop yields in the anomaly forcing CLM by
comparison with the crop yields in the standard CLM. The differences between
the anomaly forcing CLM and standard CLM were due only to differences in
forcing data, for which the standard CLM used regular forcing (3-hourly
forcing) and the anomaly forcing CLM used anomaly forcing. We found that the
anomaly forcing CLM underestimated crop yields but identified the regional
yield variations, as well as yield differences between two climate scenarios
and yield changes over time. The anomaly forcing CLM could not generate the
exact same crop yields as the standard CLM due to errors in precipitation
and in the submonthly variations. However, it could be used for qualitative
analysis of relative crop yield changes among different scenarios and over
time.</p>
      <p id="d1e1210">The overall underestimation of crop yields may be due to differences in
phenology that resulted from different submonthly variations. Some of the
low yields in the anomaly forcing CLM may be explained by shorter grain fill
periods. For example, the lower rice yields in southeastern China are due to a
5–10 d shorter grain fill period in the anomaly forcing CLM (Fig. S1a–c in the Supplement); maize and soybean in the Southern Hemisphere also showed a 1–5 d
shorter grain fill period that may account for the lower yields (Fig. S1d–i). In addition to the low yields, the anomaly forcing CLM also simulated
lower GPP and LAI compared to the standard CLM (Fig. S2a1–b3), and the
spatial<?pagebreak page1260?> distributions of GPP and LAI differences were very similar to the
yield differences.</p>
      <p id="d1e1213">Some regions in the Northern Hemisphere showed higher rainfed crop yields in
the anomaly forcing CLM, which is due to higher soil moisture at planting
that resulted from higher snow levels in the Northern Hemisphere. Crop
growth in CLM is very sensitive to the soil moisture at planting, and higher
soil moisture (Fig. S2c1–c3) results in unstressed crop growth and hence
produces higher yields. When adequate irrigation is applied, both the
anomaly forcing and the standard CLM models have sufficient water for crop
growth, and the overestimations disappeared. Therefore, the anomaly forcing
may not be appropriate for estimating the actual future irrigation demands
but is able to distinguish the relative differences in irrigation demand
across different climate scenarios.</p>
      <p id="d1e1216">The energy fluxes in the anomaly forcing CLM and in the standard CLM were
different due to different crop growth rates and differences in forcing
data. The higher snow cover in the Northern Hemisphere creates higher albedo
and lower absorbed solar radiation and hence lower surface energy fluxes.
The higher LAI increased the summer latent heat flux up to 5 W/m<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>
(Fig. S3), while the annual latent heat flux showed values 5–10 W/m<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>
(Fig. S2d1–d3) lower in the anomaly forcing CLM due to the lower
net radiation. In the Southern Hemisphere, lower LAI (Fig. S2a1–a3)
resulted in lower latent heat fluxes (Fig. S2d1–d3) and higher sensible
heat fluxes (Fig. S2e1–e3).</p>
      <p id="d1e1238">The regional yield comparisons indicate that the anomaly forcing CLM
effectively captured regional yield variations but with slightly lower yield
biases. We want to point out that the very high crop yields in Latin America
and sub-Saharan Africa and the very low crop yields in India in both the
anomaly forcing CLM and the standard CLM approaches are not realistic when
compared to the UNFAO yields (<uri>http://www.fao.org/statistics/en/</uri>, last access: 1 March 2021). Such
biases in the CLM have been discussed by Levis et al. (2018),
and the low yields in India are due to incorrect crop phenology when crops
entered the grain fill during the dry season. The high yields in Latin
American and in sub-Saharan Africa were due to the nitrogen fertilization
amounts based on US levels, which are too high for these regions.</p>
      <p id="d1e1244">The crop model in the most recent version of CLM5.0 includes new features as
reported in Lombardozzi et al. (2020). For example CLM5.0 uses
time-varying spatial distributions of major crop types and has updated
fertilization and irrigation schemes. These updates of crop model in CLM5.0
may improve the crop yield simulations for both standard CLM and anomaly
forcing CLM compared to crop yield in reality. The anomaly forcing method in
CLM5.0 remains unchanged so we speculate that the bias due to anomaly forcing may
still exist in CLM5.0. For example, CLM5.0 uses the same threshold to differentiate rain and snow, so the bias due to higher snow cover in the Northern
Hemisphere may still exist in CLM5.0. However, how the magnitude of
the bias will change is unclear. We suggest that the anomaly forcing of CLM5.0
be tested if the research interest is in absolute yield or in qualitative
difference.</p>
      <?pagebreak page1261?><p id="d1e1247">Our approach can be adopted by other land surface models to expand their
capabilities for utilizing monthly climate data. The source code of the
anomaly forcing CLM is available at the repository website Zenodo
<ext-link xlink:href="https://doi.org/10.5281/zenodo.3900671" ext-link-type="DOI">10.5281/zenodo.3900671</ext-link> (Lu, 2020). The path is
post4.5crop_slevis/models/lnd/clm/src/cpl/lnd_import_ export.F90 when unzip post4.5crop_slevis_codeforGMD.tar.gz. The Fortran code could be
transplanted to other land surface models which use NetCDF format
atmospheric forcing.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e1262">The Community Land Surface model offers an alternative way to utilize the
monthly climate as the forcing data. Such an approach could expand user
choice of forcing data when high-temporal-resolution climate data are not
available. In this work, we created anomaly forcing data for three climate
scenarios (1.5 <inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, 2.0 <inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C warming, and RCP4.5)
and validated crop yield projections in the anomaly forcing CLM against the
standard CLM. The anomaly forcing CLM underestimated crop yields by 5 %–8 %,
which was largely due to the differences in phenology and photosynthesis
that resulted from the different submonthly variations. How CLM treated
precipitation as rain or snow also introduced biases in crop yields and in
the energy flux simulations. Although the anomaly forcing CLM could not
generate crop yields identical to the standard CLM, it could be used for
qualitative analysis of crop yield changes across various scenarios over
time.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<?pagebreak page1262?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title> A user guide for using anomaly forcing CLM</title>
      <p id="d1e1295">Running the anomaly forcing CLM is similar to the standard CLM but with
several additional steps. First, the monthly anomaly data are prepared as
described in the method section. Then, the user needs to modify
user_nl_cpl and user_nl_datm to specify which forcing variables to add to the
anomaly signals. There are seven anomaly forcing variables (Table A2), and
the user can specify one, or two, or all variables in the two name lists
(user_nl_cpl and user_nl_datm). The final step is to add the corresponding anomaly
forcing data streams depending on which anomaly forcing variables were
specified in user_nl_cpl and
user_nl_datm.</p>
<sec id="App1.Ch1.S1.SS1">
  <label>A1</label><?xmltex \opttitle{Modify user\_nl\_cpl and user\_nl\_datm}?><title>Modify user_nl_cpl and user_nl_datm</title>
      <p id="d1e1306">The user may add part or all of the following text to user_nl_ cpl.<?xmltex \hack{\newline}?></p>
      <p id="d1e1310"><?xmltex \hack{\noindent}?>cplflds_custom <inline-formula><mml:math id="M73" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 'Sa_prec_af-<inline-formula><mml:math id="M74" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1328"><?xmltex \hack{\noindent}?>'Sa_prec_af-<inline-formula><mml:math id="M75" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_tbot_af-<inline-formula><mml:math id="M76" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1347"><?xmltex \hack{\noindent}?>'Sa_tbot_af-<inline-formula><mml:math id="M77" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_pbot_af-<inline-formula><mml:math id="M78" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1365"><?xmltex \hack{\noindent}?>'Sa_pbot_af-<inline-formula><mml:math id="M79" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_shum_af-<inline-formula><mml:math id="M80" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1383"><?xmltex \hack{\noindent}?>'Sa_shum_af-<inline-formula><mml:math id="M81" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_u_af-<inline-formula><mml:math id="M82" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1401"><?xmltex \hack{\noindent}?>'Sa_u_af-<inline-formula><mml:math id="M83" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_v_af-<inline-formula><mml:math id="M84" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1419"><?xmltex \hack{\noindent}?>'Sa_v_af-<inline-formula><mml:math id="M85" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> x2l','Sa_swdn_af-<inline-formula><mml:math id="M86" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x',</p>
      <p id="d1e1437"><?xmltex \hack{\noindent}?>'Sa_swdn_af-<inline-formula><mml:math id="M87" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l','Sa_lwdn_af-<inline-formula><mml:math id="M88" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> a2x',</p>
      <p id="d1e1456"><?xmltex \hack{\noindent}?>'Sa_lwdn_af-<inline-formula><mml:math id="M89" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l'<?xmltex \hack{\newline}?></p>
      <p id="d1e1468"><?xmltex \hack{\noindent}?>Add part or all of the following text into user_nl_datm.<?xmltex \hack{\newline}?></p>
      <p id="d1e1473"><?xmltex \hack{\noindent}?>anomaly_forcing<inline-formula><mml:math id="M90" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula>
'Anomaly.Forcing.Precip',</p>
      <p id="d1e1484"><?xmltex \hack{\noindent}?>'Anomaly.Forcing.Temperature', 'Anomaly.Forcing.Pressure', 'Anomaly.Forcing.Humidity',</p>
      <p id="d1e1488"><?xmltex \hack{\noindent}?>'Anomaly.Forcing.Uwind', 'Anomaly.Forcing.Vwind',</p>
      <p id="d1e1492"><?xmltex \hack{\noindent}?>'Anomaly.Forcing.Shortwave', 'Anomaly.Forcing.Longwave'<?xmltex \hack{\newline}?><?xmltex \hack{\newpage}?><?xmltex \hack{\noindent}?>Also attach the anomaly forcing data streams in user_nl_datm.<?xmltex \hack{\newline}?><?xmltex \bgroup\small?><?xmltex \hack{\noindent}?>streams <inline-formula><mml:math id="M91" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> “datm.streams.txt.CLMCRUNCEP.Solar 1996 1996 2005”, “datm.streams.txt.CLMCRUNCEP.Precip 1996 1996 2005”,<?xmltex \egroup?></p>
      <p id="d1e1513"><?xmltex \bgroup\small?>“datm.streams.txt.CLMCRUNCEP.TPQW 1996 1996 2005”,<?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?> “datm.streams.txt.presaero.clim_2000 1 1 1”,<?xmltex \egroup?></p>
      <p id="d1e1521"><?xmltex \bgroup\small?>“datm.streams.txt.Anomaly.Forcing.Precip 2006 2006 2075”,<?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?> “datm.streams.txt.Anomaly.Forcing.Temperature 2006 2006 2075”,<?xmltex \egroup?></p>
      <p id="d1e1529"><?xmltex \bgroup\small?>“datm.streams.txt.Anomaly.Forcing.Pressure 2006 2006 2075”,<?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?> “datm.streams.txt.Anomaly.Forcing.Humidity 2006 2006 2075”,<?xmltex \egroup?></p>
      <p id="d1e1537"><?xmltex \bgroup\small?>“datm.streams.txt.Anomaly.Forcing.Uwind 2006 2006 2075”,<?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?> “datm.streams.txt.Anomaly.Forcing.Vwind 2006 2006 2075”,<?xmltex \egroup?></p>
      <p id="d1e1545"><?xmltex \bgroup\small?>“datm.streams.txt.Anomaly.Forcing.Shortwave 2006 2006 2075”,<?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?> “datm.streams.txt.Anomaly.Forcing.Longwave 2006 2006 2075”,<?xmltex \egroup?></p>
      <p id="d1e1553"><?xmltex \bgroup\small?>“/glade/p/work/yaqiong/inputdata/atm/datm7/co2.1pt5degC. streams.txt 1901 1901 2075”<?xmltex \egroup?></p><?xmltex \hack{\small}?>
      <p id="d1e1560"><?xmltex \hack{\noindent}?><?xmltex \bgroup\small?>mapalgo <inline-formula><mml:math id="M92" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 'bilinear', 'bilinear', 'bilinear', 'bilinear', 'bilinear', 'bilinear', 'bilinear', 'bilinear', 'bilinear',<?xmltex \egroup?></p>
      <p id="d1e1573"><?xmltex \bgroup\small?>'bilinear', 'bilinear', 'bilinear','nn'<?xmltex \egroup?></p>
      <p id="d1e1578"><?xmltex \hack{\noindent}?><?xmltex \bgroup\small?>tintalgo <inline-formula><mml:math id="M93" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 'coszen', 'nearest', 'linear', 'linear', 'nearest', 'nearest', 'nearest', 'nearest', 'nearest', 'nearest',<?xmltex \egroup?></p>
      <p id="d1e1591"><?xmltex \bgroup\small?>'nearest', 'nearest','linear'<?xmltex \hack{\newline}?><?xmltex \egroup?></p>
      <p id="d1e1597"><?xmltex \bgroup\small?>Any combination or subset of anomaly forcing variables can be used. For example,<?xmltex \egroup?></p>
      <p id="d1e1602"><?xmltex \hack{\noindent}?><?xmltex \bgroup\small?>cplflds_custom <inline-formula><mml:math id="M94" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 'Sa_prec_af-<inline-formula><mml:math id="M95" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>a2x', 'Sa_ prec_af-<inline-formula><mml:math id="M96" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula>x2l' (in user_nl_cpl)<?xmltex \egroup?></p>
      <p id="d1e1630"><?xmltex \hack{\noindent}?><?xmltex \bgroup\small?>anomaly_forcing<inline-formula><mml:math id="M97" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula>'Anomaly.Forcing.Precip' (in user_nl_datm)<?xmltex \egroup?></p>
      <?pagebreak page1263?><p id="d1e1643"><?xmltex \bgroup\small?>will only adjust precipitation. The reference data and period are defined in env_run.xml. <?xmltex \hack{\clearpage}?><?xmltex \egroup?></p>
</sec>
<sec id="App1.Ch1.S1.SS2">
  <label>A2</label><title>Add the anomaly forcing data stream</title>
      <p id="d1e1657">The anomaly forcing data stream is where the data path of the
monthly anomaly forcing signal can be specified and the code can be told which variable to
retrieve. A list of all anomaly forcing data stream file names and the
variables in the anomaly forcing data and the code are given in Table A1. An
example of the content in user_datm.streams.txt.Anomaly.Forcing.Humidity is also attached. The user only
needs to add the corresponding variable data streams that are defined in
user_nl_cpl.</p>

<?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S1.T2"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A1}?><label>Table A1</label><caption><p id="d1e1664">A list of the anomaly forcing data streams and the corresponding
variables in the anomaly forcing data and the code.</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="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Data stream file names</oasis:entry>
         <oasis:entry colname="col2">Variables in data</oasis:entry>
         <oasis:entry colname="col3">Variables in code</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Humidity<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">huss</oasis:entry>
         <oasis:entry colname="col3">shum_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Precip</oasis:entry>
         <oasis:entry colname="col2">pr</oasis:entry>
         <oasis:entry colname="col3">prec_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Pressure</oasis:entry>
         <oasis:entry colname="col2">ps</oasis:entry>
         <oasis:entry colname="col3">pbot_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Shortwave</oasis:entry>
         <oasis:entry colname="col2">rsds</oasis:entry>
         <oasis:entry colname="col3">swdn_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Temperature</oasis:entry>
         <oasis:entry colname="col2">tas</oasis:entry>
         <oasis:entry colname="col3">tbot_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Uwind</oasis:entry>
         <oasis:entry colname="col2">uas</oasis:entry>
         <oasis:entry colname="col3">u_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Vwind</oasis:entry>
         <oasis:entry colname="col2">vas</oasis:entry>
         <oasis:entry colname="col3">v_af</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">user_datm.streams.txt.Anomaly.Forcing.Longwave</oasis:entry>
         <oasis:entry colname="col2">rlds</oasis:entry>
         <oasis:entry colname="col3">lwdn_af</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e1667">
<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>*</mml:mo></mml:msup></mml:math></inline-formula> An example of the content in the data stream is given below.<?xmltex \hack{\\}?><inline-formula><mml:math id="M99" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> dataSource<inline-formula><mml:math id="M100" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?>GENERIC<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{2mm}}?><inline-formula><mml:math id="M101" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /dataSource<inline-formula><mml:math id="M102" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{2mm}}?><inline-formula><mml:math id="M103" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> domainInfo<inline-formula><mml:math id="M104" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M105" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> variableNames<inline-formula><mml:math id="M106" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>time<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>xc  lon<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>yc  lat<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>area<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>mask<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M107" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /variableNames<inline-formula><mml:math id="M108" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M109" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> filePath<inline-formula><mml:math id="M110" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>/glade/p/cesmdata/cseg/inputdata/share/domains<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M111" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /filePath<inline-formula><mml:math id="M112" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M113" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> fileNames<inline-formula><mml:math id="M114" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>domain.lnd.fv0.9x1.25_gx1v6.090309.nc<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M115" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /fileNames<inline-formula><mml:math id="M116" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{2mm}}?><inline-formula><mml:math id="M117" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /domainInfo<inline-formula><mml:math id="M118" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{2mm}}?><inline-formula><mml:math id="M119" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> fieldInfo<inline-formula><mml:math id="M120" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M121" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> variableNames<inline-formula><mml:math id="M122" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>huss shum_af<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M123" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /variableNames<inline-formula><mml:math id="M124" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M125" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> filePath<inline-formula><mml:math id="M126" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>THE ANOMALY FORCING SIGNAL DATA PATH<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M127" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /filePath<inline-formula><mml:math id="M128" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M129" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> fileNames<inline-formula><mml:math id="M130" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>THE ANOMALY FORCING SIGNAL DATA NAME<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M131" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /fileNames<inline-formula><mml:math id="M132" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M133" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> offset<inline-formula><mml:math id="M134" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{6mm}}?>0<?xmltex \hack{\\}?><?xmltex \hack{\hspace*{4mm}}?><inline-formula><mml:math id="M135" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /offset<inline-formula><mml:math id="M136" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula><?xmltex \hack{\\}?><?xmltex \hack{\hspace*{2mm}}?><inline-formula><mml:math id="M137" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> /fieldInfo<inline-formula><mml:math id="M138" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula></p></table-wrap-foot></table-wrap>

<?xmltex \hack{\clearpage}?>
</sec>
</app>
  </app-group><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e2165">The CLM source code used in our study is available at repository website
Zenodo: <ext-link xlink:href="https://doi.org/10.5281/zenodo.3900671" ext-link-type="DOI">10.5281/zenodo.3900671</ext-link> (Lu, 2020).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e2174">Our research data are available at the repository website Zenodo at <ext-link xlink:href="https://doi.org/10.5281/zenodo.4571653" ext-link-type="DOI">10.5281/zenodo.4571653</ext-link> (Lu, 2021).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e2180">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/gmd-14-1253-2021-supplement" xlink:title="pdf">https://doi.org/10.5194/gmd-14-1253-2021-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2189">YL designed and performed the simulations. YL and XY analyzed the results and wrote the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2195">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2201">We thank the topical editor Christoph Müller and two anonymous
reviewers for their great comments that largely improved our paper. We
also thank NCAR scientists Sean Swenson and David Lawrence for the
instruction of using the anomaly forcing approach, and Peter Lawrence for
providing the crop area maps. This work was supported by the National
Science Foundation under grant number AGS-1243095 and the National Natural
Science Foundation of China (no. 41975135). We would like to acknowledge
high-performance computing support from Yellowstone (ark:/85065/d7wd3xhc),
provided by NCAR's Computational and Information Systems Laboratory,
sponsored by the National Science Foundation.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2206">This research has been supported by the National Science Foundation (grant no. AGS-1243095) and the National Natural Science Foundation of China (grant no. 41975135).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2212">This paper was edited by Christoph Müller and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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  </ref-list></back>
    <!--<article-title-html>Using the anomaly forcing Community Land Model (CLM 4.5) for crop yield projections</article-title-html>
<abstract-html><p>Crop growth in land surface models normally requires high-temporal-resolution climate data (3-hourly or 6-hourly), but such high-temporal-resolution climate data are not provided by many climate model simulations
due to expensive storage, which limits modeling choices if there is an
interest in a particular climate simulation that only saved monthly outputs.
The Community Land Surface Model (CLM) has proposed an alternative approach
for utilizing monthly climate outputs as forcing data since version 4.5, and
it is called the anomaly forcing CLM. However, such an approach has never
been validated for crop yield projections. In our work, we created anomaly
forcing datasets for three climate scenarios (1.5&thinsp;°C warming, 2.0&thinsp;°C warming, and RCP4.5) and validated crop yields against the
standard CLM forcing with the same climate scenarios using 3-hourly data. We
found that the anomaly forcing CLM could not produce crop yields identical
to the standard CLM due to the different submonthly variations, crop
yields were underestimated by 5&thinsp;%–8&thinsp;% across the three scenarios (1.5, 2.0&thinsp;°C, and RCP4.5) for the global average, and
28&thinsp;%–41&thinsp;% of cropland showed significantly different yields. However, the
anomaly forcing CLM effectively captured the relative changes between
scenarios and over time, as well as regional crop yield variations. We
recommend that such an approach be used for qualitative analysis of crop
yields when only monthly outputs are available. Our approach can be adopted
by other land surface models to expand their capabilities for utilizing
monthly climate data.</p></abstract-html>
<ref-html id="bib1.bib1"><label>1</label><mixed-citation>
Drewniak, B., Song, J., Prell, J., Kotamarthi, V. R., and Jacob, R.: Modeling agriculture in the Community Land Model, Geosci. Model Dev., 6, 495–515, <a href="https://doi.org/10.5194/gmd-6-495-2013" target="_blank">https://doi.org/10.5194/gmd-6-495-2013</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>2</label><mixed-citation>Hurrell, J. W., Holland, M. M., Gent, P. R., Ghan, S., Kay, J. E., Kushner, P. J., Lamarque, J. F., Large, W. G., Lawrence, D., Lindsay, K., Lipscomb, W. H., Long, M. C., Mahowald, N., Marsh, D. R., Neale, R. B., Rasch, P., Vavrus, S., Vertenstein, M., Bader, D., Collins, W. D., Hack, J. J., Kiehl, J., and Marshall, S.: The Community Earth System Model A Framework for Collaborative Research, B. Am. Meteorol. Soc., 94, 1339–1360, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>3</label><mixed-citation>Justel, A., Pena, D., and Zamar, R.: A multivariate Kolmogorov-Smirnov test of goodness of fit, Stat. Probabil. Lett., 35, 251–259, 1997.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>4</label><mixed-citation>Knutti, R. and Sedlacek, J.: Robustness and uncertainties in the new CMIP5 climate model projections, Nat. Clim. Change, 3, 369–373, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>5</label><mixed-citation>Kucharik, C. J.: Evaluation of a Process-Based Agro-Ecosystem Model (Agro-IBIS) across the US Corn Belt: Simulations of the Interannual
Variability in Maize Yield, in: Earth Interact, 7, 14, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>6</label><mixed-citation>Lawrence, D. M., Koven, C. D., Swenson, S. C., Riley, W. J., and Slater, A. G.: Permafrost thaw and resulting soil moisture changes regulate projected high-latitude CO<sub>2</sub> and CH<sub>4</sub> emissions, Environ. Res. Lett., 10,  094011, <a href="https://doi.org/10.1088/1748-9326/10/9/094011" target="_blank">https://doi.org/10.1088/1748-9326/10/9/094011</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>7</label><mixed-citation>Levis, S., Badger, A., Drewniak, B., Nevison, C., and Ren, X. L.: CLMcrop yields and water requirements: avoided impacts by choosing RCP 4.5 over 8.5, Climatic Change, 146, 501–515, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>8</label><mixed-citation>Levis, S., Bonan, G. B., Kluzek, E., Thornton, P. E., Jones, A., Sacks, W. J., and Kucharik, C. J.: Interactive Crop Management in the Community Earth System Model (CESM1): Seasonal Influences on Land-Atmosphere Fluxes, J. Climate, 25, 4839–4859, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>9</label><mixed-citation>Lobell, D. B., Burke, M. B., Tebaldi, C., Mastrandrea, M. D., Falcon, W. P., and Naylor, R. L.: Prioritizing climate change adaptation needs for food security in 2030, Science, 319, 607–610, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>10</label><mixed-citation>Lombardozzi, D., Levis, S., Bonan, G., Hess, P. G., and Sparks, J. P.: The Influence of Chronic Ozone Exposure on Global Carbon and Water Cycles, J. Climate, 28, 292–305, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>11</label><mixed-citation>Lombardozzi, D. L., Lu, Y. Q., Lawrence, P. J., Lawrence, D. M., Swenson, S., Oleson, K. W., Wieder, W. R., and Ainsworth, E. A.: Simulating Agriculture in the Community Land Model Version 5, J. Geophys. Res.-Biogeo., 125, e2019JG005529, <a href="https://doi.org/10.1029/2019JG005529" target="_blank">https://doi.org/10.1029/2019JG005529</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>12</label><mixed-citation>Lu, Y., Williams, I. N., Bagley, J. E., Torn, M. S., and Kueppers, L. M.: Representing winter wheat in the Community Land Model (version 4.5), Geosci. Model Dev., 10, 1873–1888, <a href="https://doi.org/10.5194/gmd-10-1873-2017" target="_blank">https://doi.org/10.5194/gmd-10-1873-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>13</label><mixed-citation> Lu, Y.: Source code for Using the anomaly forcing Community Land Model (CLM) for crop yield projections, Zenodo, <a href="https://doi.org/10.5281/zenodo.3900671" target="_blank">https://doi.org/10.5281/zenodo.3900671</a>, 2020.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>14</label><mixed-citation>
Lu, Y.: Crop yield data of Using the anomaly forcing Community Land Model (CLM 4.5) for crop yield projections, Zenodo, <a href="https://doi.org/10.5281/zenodo.4571653" target="_blank">https://doi.org/10.5281/zenodo.4571653</a>, 2021.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>15</label><mixed-citation>Marozzi, M.: Nonparametric Simultaneous Tests for Location and Scale Testing: A Comparison of Several Methods, Commun. Stat.-Simul. C, 42, 1298–1317, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>16</label><mixed-citation>Oleson, K., Lawrence, D., Bonan, G., Drewniak, B., Huang, M., Koven, C., Levis, S., Li, F., Riley, W., Subin, Z., Swenson, S., and Thornton, P.: Technical Description of version 4.5 of the Community Land Model (CLM), National Center for Atmospheric Rsearch, Boulder, CO, NCAR/TN-503+STR, 434 pp., 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>17</label><mixed-citation>Peng, B., Guan, K. Y., Chen, M., Lawrence, D. M., Pokhrel, Y., Suyker, A., Arkebauer, T., and Lu, Y. Q.: Improving maize growth processes in the community land model: Implementation and evaluation, Agr. Forest. Meteorol., 250, 64–89, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>18</label><mixed-citation>Qian, T., Dai, A., Ternberth, K. E., and Olseon, K. W.: Simulation of Global Land Surface Conditions from 1948 to 2004. Part I: Forcing Data and Evaluations, J. Hydrometeorol., 7, 953–975, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>19</label><mixed-citation>Ren, X., Lu, Y., O'Neill, B. C., and Weitzel, M.: Economic and biophysical impacts on agriculture under 1.5&thinsp;°C and 2&thinsp;°C warming, Environ. Res. Lett., 13, 115006, <a href="https://doi.org/10.1088/1748-9326/aae6a9" target="_blank">https://doi.org/10.1088/1748-9326/aae6a9</a>,  2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>20</label><mixed-citation>Rosenzweig, C., Elliott, J., Deryng, D., Ruane, A. C., Muller, C., Arneth, A., Boote, K. J., Folberth, C., Glotter, M., Khabarov, N., Neumann, K., Piontek, F., Pugh, T. A. M., Schmid, E., Stehfest, E., Yang, H., and Jones, J. W.: Assessing agricultural risks of climate change in the 21st century in a global gridded crop model intercomparison, P. Natl. Acad. Sci. USA, 111, 3268–3273, 2014.

</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>21</label><mixed-citation>Urban, D., Roberts, M. J., Schlenker, W., and Lobell, D. B.: Projected temperature changes indicate significant increase in interannual variability of U.S. maize yields, Climatic Change, 112, 525–533, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>22</label><mixed-citation>Viovy, N.: CRUNCEP Version 7 – Atmospheric Forcing Data for the Community Land Model, Research Data Archive at the National Center for Atmospheric Research, Computational and Information Systems Laboratory, <a href="https://doi.org/10.5065/PZ8F-F017" target="_blank">https://doi.org/10.5065/PZ8F-F017</a>, 2018.
</mixed-citation></ref-html>--></article>
