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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/essd-12-2971-2020</article-id><title-group><article-title>A Last Glacial Maximum forcing dataset <?xmltex \hack{\break}?>for ocean modelling</article-title><alt-title>A Last Glacial Maximum forcing dataset for ocean modelling</alt-title>
      </title-group><?xmltex \runningtitle{A Last Glacial Maximum forcing dataset for ocean modelling}?><?xmltex \runningauthor{A. L. Mor\'{e}e and J. Schwinger}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Morée</surname><given-names>Anne L.</given-names></name>
          <email>anne.moree@uib.no</email>
        <ext-link>https://orcid.org/0000-0002-0283-5947</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Schwinger</surname><given-names>Jörg</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7525-6882</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Geophysical Institute, University of Bergen and Bjerknes Centre for
Climate Research, 5007 Bergen, Norway</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>NORCE Climate, Bjerknes Centre for Climate Research, 5007 Bergen,
Norway</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Anne L. Morée (anne.moree@uib.no)</corresp></author-notes><pub-date><day>20</day><month>November</month><year>2020</year></pub-date>
      
      <volume>12</volume>
      <issue>4</issue>
      <fpage>2971</fpage><lpage>2985</lpage>
      <history>
        <date date-type="received"><day>16</day><month>May</month><year>2019</year></date>
           <date date-type="rev-request"><day>1</day><month>July</month><year>2019</year></date>
           <date date-type="rev-recd"><day>30</day><month>September</month><year>2020</year></date>
           <date date-type="accepted"><day>10</day><month>October</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 Anne L. Morée</copyright-statement>
        <copyright-year>2020</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020.html">This article is available from https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e97">Model simulations of the Last Glacial Maximum (LGM;
<inline-formula><mml:math id="M1" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 21 000 years before present) can aid the interpretation of
proxy records, can help to gain an improved mechanistic understanding of the LGM
climate system, and are valuable for the evaluation of model performance in
a different climate state. Ocean-ice only model configurations forced by
prescribed atmospheric data (referred to as “forced ocean models”)
drastically reduce the computational cost of palaeoclimate modelling
compared to fully coupled model frameworks. While feedbacks between the
atmosphere and ocean and sea-ice compartments of the Earth system are not
present in such model configurations, many scientific questions can be
addressed with models of this type. Our dataset supports simulations of the
LGM in a forced ocean model set-up while still taking advantage of the
complexity of fully coupled model set-ups. The data presented here are
derived from fully coupled palaeoclimate simulations of the Palaeoclimate
Modelling Intercomparison Project phase 3 (PMIP3). The data are publicly
accessible at the National Infrastructure for Research Data (NIRD) Research Data Archive at
<ext-link xlink:href="https://doi.org/10.11582/2020.00052" ext-link-type="DOI">10.11582/2020.00052</ext-link> (Morée and Schwinger, 2020). They
consist of 2-D anomaly forcing fields suitable for use in ocean models that
employ a bulk forcing approach and are optimized for use with CORE forcing
fields. The data include specific humidity, downwelling long-wave and
short-wave radiation, precipitation, wind (<inline-formula><mml:math id="M2" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M3" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> components), temperature,
and sea surface salinity (SSS). All fields are provided as climatological
mean anomalies between LGM and pre-industrial (PI) simulations. These anomaly
data can therefore be added to any pre-industrial ocean forcing dataset in
order to obtain forcing fields representative of LGM conditions as simulated
by PMIP3 models. Furthermore, the dataset can be easily updated to reflect
results from upcoming and future palaeo-model intercomparison activities.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e133">The Last Glacial Maximum (LGM; <inline-formula><mml:math id="M4" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 21 ka) is of interest to the climate research
community because of the relative abundance of proxy data and because it is
the most recent profoundly different climatic state of our planet. For these
reasons, the LGM is extensively studied in modelling frameworks (e.g.
Menviel et al., 2017; Brady et al., 2012; Otto-Bliesner et al., 2007;
Bouttes et al., 2011; Buchanan et al., 2016; Lynch-Stieglitz et al., 2016;
Kageyama et al., 2017). Model simulations of the past ocean can not only
provide a method to gain a mechanistic understanding of marine proxy
records, but they can also inform us about model performance in a different
climatic state of the Earth system (Braconnot et al., 2012). Typical
state-of-the-art tools to simulate the (past) Earth system are climate or
Earth system models as used, for example, in the Coupled Model
Intercomparison Project phase 5 (CMIP5; Taylor et al., 2011). Besides
simulating our present climate, these CMIP5 models are also used to simulate
past climate states (such as the LGM) in the Palaeoclimate Modelling
Intercomparison Project phase 3 (PMIP3). However, the computational costs and
runtime of such fully coupled model frameworks are a major obstacle for
their application to palaeoclimate modelling.<?pagebreak page2972?> Palaeoclimate modelling
optimally requires long simulations (thousands to tens of thousands of years) in
order to provide the necessary time for relevant processes to emerge (e.g.
CaCO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> compensation) (Braconnot et al., 2007). Complex fully coupled
models can not typically be run into full equilibrium (which requires
hundreds to thousands of years of integration) due to computational costs
(Eyring et al., 2016). Therefore, the PMIP3 models exhibit model drift
(especially in the deep ocean; e.g. Marzocchi and Jansen, 2017). Since
significant differences between a (drifting) non-equilibrated state and the
equilibrium model state can impede the comparison of model results with proxy
data, a well equilibrated model with minimal drift is desirable. The
third phase of the PMIP project (Braconnot et al., 2012) limits global
mean sea surface temperature drift to under 0.05 K per century and requires
the Atlantic Meridional Overturning Circulation to be stable (Kageyama et
al., 2018).</p>
      <p id="d1e152">We refer to a “forced ocean model” as a model of the
ocean–sea-ice–atmosphere system in which the atmosphere is represented by
prescribed 2-D forcing fields. Such model set-ups have been extensively used
in model intercomparison studies such as the Coordinated Ocean-ice Reference
Experiments (COREs; Griffies et al., 2009) and more recently in the CMIP6
Ocean Model Intercomparison Project (OMIP; Griffies et al. 2016). A forced
ocean model can be used whenever ocean–atmosphere feedbacks are of minor
importance, and it has the advantage of reducing the computational costs –
making longer or more numerous model runs feasible. The use of PMIP output in forced
ocean modelling is common practice (e.g. Muglia and Schmittner, 2015;
Khatiwala et al., 2019). Until now, however, there is no standardized dataset
available that can be used to easily derive a Last Glacial Maximum model
forcing. Therefore, we present 2-D (surface) anomaly fields of CMIP5/PMIP3
experiments of “lgm” (representing the Last Glacial Maximum state of the Earth
system) minus “piControl” (representing the pre-industrial, PI, state) calculated
from monthly climatological PMIP3 output. The PMIP3 output is the result of
global boundary conditions and forcings (such as insolation and ice sheet
cover) applied in the fully coupled PMIP3 models (Braconnot et al., 2012).
Our dataset (Morée and Schwinger, 2020) is a unique compilation of
existing data, which has been processed and reformatted such that it can be readily applied
in a forced ocean model framework that uses a bulk forcing approach similar
to Large and Yeager (2004). Since this approach has been popularized through
coordinated model intercomparison activities (Griffies et al., 2009), a
majority of forced ocean models today use this approach. The 2-D anomaly
fields presented here can be added to the pre-industrial forcing of a forced
ocean model in order to obtain an atmospheric forcing representative of the
LGM. The data are climatological mean anomalies, and as such they are suitable for
equilibrium LGM “time-slice” modelling of the ocean. In Sect. 2, a general
description of the dataset and data sources is provided alongside an
overview of the variables (Table 1). The description of the procedure
followed to make this dataset (Sect. 3) should support any extension of the
dataset with additional (PMIP-derived) variables if needed. The PMIP4
guidelines (Kageyama et al., 2017) can support users in designing a specific
model set-up, for example, regarding the land–sea mask, trace gas
concentrations, river run-off, or other conditions and forcings that one would want
to apply to a model. Limitations of the dataset are discussed in Sect. 4.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e158">Summary of the data showing variable description, units, format
(lat <inline-formula><mml:math id="M6" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> long, time), and NetCDF variable name(s). Formats follow CORE
conventions (Large and Yeager, 2004). The wind component variables are
provided in separate files (Morée and Schwinger, 2020). In each NetCDF
file (i.e. for each variable), the model spread is provided alongside the
anomaly field named “variablename_spread”.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Variable description</oasis:entry>
         <oasis:entry colname="col2">Units</oasis:entry>
         <oasis:entry colname="col3">Resolution (lat <inline-formula><mml:math id="M7" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> long), time</oasis:entry>
         <oasis:entry colname="col4">Variable name</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Specific humidity</oasis:entry>
         <oasis:entry colname="col2">kg kg<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">94 <inline-formula><mml:math id="M9" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 1460</oasis:entry>
         <oasis:entry colname="col4">huss</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Downwelling long-wave radiation</oasis:entry>
         <oasis:entry colname="col2">W m<inline-formula><mml:math id="M10" 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="col3">94 <inline-formula><mml:math id="M11" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 365</oasis:entry>
         <oasis:entry colname="col4">rlds</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Downwelling short-wave radiation</oasis:entry>
         <oasis:entry colname="col2">W m<inline-formula><mml:math id="M12" 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="col3">94 <inline-formula><mml:math id="M13" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 365</oasis:entry>
         <oasis:entry colname="col4">rsds</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Precipitation</oasis:entry>
         <oasis:entry colname="col2">mm d<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">94 <inline-formula><mml:math id="M15" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 12</oasis:entry>
         <oasis:entry colname="col4">pr</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Wind (<inline-formula><mml:math id="M16" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M17" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> components)</oasis:entry>
         <oasis:entry colname="col2">m s<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3">94 <inline-formula><mml:math id="M19" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 1460</oasis:entry>
         <oasis:entry colname="col4">uas and vas</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Temperature</oasis:entry>
         <oasis:entry colname="col2">K</oasis:entry>
         <oasis:entry colname="col3">94 <inline-formula><mml:math id="M20" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192, 1460</oasis:entry>
         <oasis:entry colname="col4">tas</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Sea surface salinity</oasis:entry>
         <oasis:entry colname="col2">psu</oasis:entry>
         <oasis:entry colname="col3">180 <inline-formula><mml:math id="M21" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 360, 12</oasis:entry>
         <oasis:entry colname="col4">sos</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2">
  <label>2</label><title>General description of the dataset</title>
      <p id="d1e442">The data presented in this article are 2-D anomaly fields of the LGM versus the
pre-industrial state based on PMIP3 (Braconnot et al., 2012). We note that
the PMIP3/CMIP5 pre-industrial state, which is the result of piControl
experiments, represents the year 1850 and is therefore strictly speaking
already influenced by anthropogenic forcing (e.g. Eyring et al., 2016). Our
anomaly fields can be used as atmospheric LGM forcing fields for ocean-only
model set-ups when added to pre-industrial forcing fields (as done by, for example, Muglia and Schmittner, 2015; Khatiwala et al., 2019) and are optimized for
use in combination with CORE forcing fields (Griffies et al., 2009). We note
that the CORE forcing is based on modern era (1948–2009) reanalysis and
observations and thus is not a pre-industrial forcing. However, the
anthropogenic climate signal contained in these data is relatively small,
particularly in comparison to the uncertainties of the LGM–PI anomalies (see
below). The basis of the anomaly data is monthly climatological PMIP3
output. Any variables presented at sub-monthly time resolutions are therefore
time-interpolated. We chose to time-interpolate the variables to their
respective time resolution in the CORE Normal Year Forcing format (CORE-NYF;
Large and Yeager, 2004). The anomalies are calculated as the mean of the
difference between monthly climatologies of the “lgm” and “piControl” PMIP3
model runs. In cases where modelling groups provided more than one ensemble
member, we included only the first member in our calculations. The data are
the mean anomaly of five PMIP3 models (CNRM-CM5, IPSL-CM5A-LR, GISS-E2-R,
MIROC-ESM, and MRI-CGCM3; Table 2) as only these models provide output for
all variables. A discussion on the limitations of our dataset is provided in
Sect. 4.</p>
      <p id="d1e445">The variables are (i) near-surface specific humidity, (ii) downwelling
long-wave radiation, (iii) downwelling short-wave radiation, (iv) precipitation,
(v) wind (<inline-formula><mml:math id="M22" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M23" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> components), (vi) near-surface temperature, and (vii) sea
surface salinity (SSS) (Table 1). The SSS anomaly field can be used to
adjust SSS restoring in LGM simulations.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e465">PMIP3 models used in this study.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="6cm"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="4.6cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model name</oasis:entry>
         <oasis:entry colname="col2">Modelling group</oasis:entry>
         <oasis:entry colname="col3">Reference</oasis:entry>
         <oasis:entry colname="col4">Source data reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">CNRM-CERFACS (France)</oasis:entry>
         <oasis:entry colname="col3">Voldoire et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">piControl: Sénési et al. (2014a) <?xmltex \hack{\hfill\break}?>lgm: Sénési et al. (2014b)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">IPSL (Institut Pierre Simon Laplace, France)</oasis:entry>
         <oasis:entry colname="col3">Dufresne et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">piControl: Caubel et al. (2016) <?xmltex \hack{\hfill\break}?>lgm: Kageyama et al. (2016)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MIROC-ESM</oasis:entry>
         <oasis:entry colname="col2">MIROC (JAMSTEC and NIES, Japan)</oasis:entry>
         <oasis:entry colname="col3">Sueyoshi et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">piControl: JAMSTEC et al. (2015a) <?xmltex \hack{\hfill\break}?>lgm: JAMSTEC et al. (2015b)</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MRI-CGCM3</oasis:entry>
         <oasis:entry colname="col2">MRI (Meteorological Research Institute, Japan)</oasis:entry>
         <oasis:entry colname="col3">Yukimoto et al. (2012)</oasis:entry>
         <oasis:entry colname="col4">piControl: Yukimoto et al. (2015a) <?xmltex \hack{\hfill\break}?>lgm: Yukimoto et al. (2015b)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">NASA/GISS (Goddard Institute for Space Studies, USA)</oasis:entry>
         <oasis:entry colname="col3">Schmidt et al. (2014)</oasis:entry>
         <oasis:entry colname="col4">piControl: NASA-GISS (2014a) <?xmltex \hack{\hfill\break}?>lgm: NASA-GISS (2014b)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?pagebreak page2973?><p id="d1e589">All variables (Sects. 3.1–7) of the monthly climatological PMIP3 output have
been regridded (Table 3, #1), averaged (Table 3, #2), and differenced
(Table 3, #3) to calculate the anomaly fields. Additional procedures for
each variable are provided in the respective part of Sect. 3, together with
a figure of each variable's annual mean anomaly and model spread. Alongside
the lgm–piControl anomaly for each variable, the model spread across all
five models has been made available. The individual model anomalies for each of
the variables are presented in Fig. A1. In order to give the reader the
opportunity to compare the anomaly data with typical pre-industrial values
for each of the variables, we provide the multi-model annual mean for the
piControl experiment in Fig. A2.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e595">Package commands applied in this study. Detailed information on
these commands can be found in the respective netCDF Operator (NCO) and Climate Data Operator (CDO) documentation
online. All operations were performed with either CDO version 1.9.3
(Schulzweida, 2019) or NCO version 4.6.9. The complete list of commands is
available in the NetCDF files under global attribute “history”.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">#</oasis:entry>
         <oasis:entry colname="col2">CDO or NCO command</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">1</oasis:entry>
         <oasis:entry colname="col2">cdo remapbil,t62grid</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">2</oasis:entry>
         <oasis:entry colname="col2">cdo ensmean</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">3</oasis:entry>
         <oasis:entry colname="col2">cdo sub</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">4</oasis:entry>
         <oasis:entry colname="col2">cdo setmisstodis</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">5</oasis:entry>
         <oasis:entry colname="col2">ncap2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">6</oasis:entry>
         <oasis:entry colname="col2">cdo inttime</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?pagebreak page2974?><p id="d1e677">The inter-model disagreement is described for each variable in Sect. 3 and
could, for example, be used to guide adjustments to the amplitude of the
forcing anomaly for model tuning purposes. Additionally, proxy-based
reconstructions are available for some of the variables, which can constrain
potential adjustments to the forcing anomaly fields. We note, however, that
for none of our variables does a purely proxy-based global reconstruction exist
– underlining the value of model-based reconstructions. A combination of
model and proxy data makes it feasible to create global coverage for air
temperatures (e.g. Annan and Hargreaves, 2013), but we are not aware of
similar efforts for any of our other variables. Regional proxy-based
reconstructions, although mostly quantitative and only over the continents,
exist for humidity (e.g. Alexandre et al., 2018), precipitation (e.g.
Mendes et al., 2019), and wind direction and strength (e.g. Markewich
et al., 2015). Regarding ocean proxies, salinity reconstructions are highly
uncertain (Rohling, 2000) but could also provide some constraint to the
model data. We leave the decision to the individual modelling groups whether
to adjust their forcing fields for their specific application.
<?xmltex \hack{\newpage}?>
All operations were performed with NetCDF toolkits Climate Data Operator (CDO) version 1.9.3
(Schulzweida, 2019) or netCDF Operator (NCO) version 4.6.9. The main functions used are
documented in Table 3 and referred to in the text at the first occurrence.
The atmospheric anomaly data are on a Gaussian grid with 94 <inline-formula><mml:math id="M24" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 192
(lat <inline-formula><mml:math id="M25" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> long) grid points. The SSS fields are on a regular
180 <inline-formula><mml:math id="M26" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 360 (lat <inline-formula><mml:math id="M27" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> long) grid. Regridding any of the files to a
different model grid should be straightforward (e.g. Table 3, #1) as it
was ensured that all files contain the information needed for re-gridding.
The variables, grid, and time resolution are chosen to be compatible with the
CORE forcing fields (Large and Yeager, 2004), which have been extensively
used in the ocean modelling community as they are the standard in ocean
model comparisons (Griffies et al., 2009, 2016). We anticipate that the
variables selected here should be useful in different model set-ups as well.
We intend to provide a dataset that is flexible with respect to the use of
different land–ocean masks in different models. Therefore, we account for
changes in sea level (i.e. a larger land area in the LGM) which can affect
variables in coastline areas by applying the following masking procedure:
(i) masking the multi-model mean anomaly with the maximum lgm land mask
across all models, then (ii) extrapolating the variable over land using a
distance-weighted average (Table 3, #4), and (iii) finally masking the
data with a present-day land mask (based on the World Ocean Atlas 2013
1<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> resolution land mask) but with the ocean extended in a 1.5<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> radius over land. Therefore, our anomaly forcing dataset can likely
be used with any pre-industrial land–sea mask. By following this
procedure, the grid points affected by land–sea mask changes are thus filled
with the extrapolated model mean anomaly from the LGM coastal ocean. In the
case of NorESM-OC (Schwinger et al., 2016), the atmospheric anomaly fields
were added to its CORE-NYF fields (Large and Yeager, 2004) to obtain an LGM
normal-year forcing under the assumption of unchanged spatial and temporal
variability for the respective variable. Note that the addition of the
anomaly fields to the user's own model forcing could lead to physically
unrealistic and/or non-meaningful results for some variables (such as negative
precipitation or radiation). This must be corrected for by capping off
sub-zero values (Table 3, #5) after the addition of the anomaly.</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>The variables</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Specific humidity anomaly</title>
      <p id="d1e744">The mean anomaly of near-surface specific humidity over the five models was
time interpolated (Table 3, #6) to a 6-hour time resolution from the
monthly climatological PMIP3 output. The annual mean lgm–piControl anomaly
field (Fig. 1a) shows a global decrease in specific humidity, as would be expected
from decreased air temperatures (Sect. 3.6). The anomaly is most pronounced
around the Equator where we see a decrease of 2–3 <inline-formula><mml:math id="M30" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> kg kg<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, while the anomaly is nearly zero towards both poles. The model
spread of the anomaly shows a disagreement between the PMIP3 models
generally in the order of 1–2 <inline-formula><mml:math id="M33" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> kg kg<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, but it is
larger (up to 4 <inline-formula><mml:math id="M36" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> kg kg<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in the Northern Hemisphere's
western boundary current regions and close to the Arctic ice edge (Fig. 1b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e843">Annual mean specific humidity lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in kg kg<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Downwelling long-wave radiation anomaly</title>
      <p id="d1e878">The anomaly for surface downwelling long-wave radiation is time-interpolated
(Table 3, #6) to a daily time resolution. The annual mean anomaly field
(Fig. 2a) shows globally decreased downwelling long-wave radiation in the
lgm experiment compared to the piControl experiment in the order of
10–30 W m<inline-formula><mml:math id="M40" 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 most of the ocean due to a generally cooler atmosphere
(Sect. 3.6). The largest anomalies lie close to the northern ice sheets
with up to <inline-formula><mml:math id="M41" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>90 W m<inline-formula><mml:math id="M42" 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 radiation in the lgm experiment than in
the piControl experiment. Ice is likely also the main contributor to the
high (60–90 W m<inline-formula><mml:math id="M43" 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>) inter-model spread in the North Atlantic and Southern
oceans (Fig. A3). The remainder of the ocean exhibits a better agreement
with inter-model spreads generally below 20 W m<inline-formula><mml:math id="M44" 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. 2b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e938">Annual mean downwelling long-wave radiation lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in W m<inline-formula><mml:math id="M45" 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>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Downwelling short-wave radiation anomaly</title>
      <p id="d1e973">The surface downwelling short-wave radiation anomaly field is
time-interpolated (Table 3, #6) to daily fields as was done for downwelling
long-wave radiation. The annual mean anomaly is especially pronounced around
the Laurentide and Scandinavian ice sheets, where strong positive anomalies
of over <inline-formula><mml:math id="M46" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30 W m<inline-formula><mml:math id="M47" 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> exist (Fig. 3a). Globally, the annual
mean downwelling short-wave radiation anomaly generally falls in a range of
<inline-formula><mml:math id="M48" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>15 to <inline-formula><mml:math id="M49" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>15 W m<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> over the ocean. The anomaly field shows negative
anomalies and positive ones in an alternating spatial pattern
approximately symmetrical around the Equator in the Pacific basin. The
inter-model spread is largest in the North Atlantic region and along the
Equator (Fig. 3b). Due to the large model disagreement of up to 50 W m<inline-formula><mml:math id="M51" 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 this variable (Fig. 3), the inter-model spread and mean anomaly are of
similar magnitude, although a consistent pattern is present in the anomaly
field.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e1036">Annual mean downwelling short-wave radiation lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in W m<inline-formula><mml:math id="M52" 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>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Precipitation anomaly and river run-off</title>
      <p id="d1e1071">The anomaly precipitation presented here is the lgm–piControl anomaly at the
air–sea interface and includes both the liquid and solid phases from all
types of clouds (both large-scale and convective). The units were converted
to millimetres per day (mm d<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) to comply with the CORE forcing format (causing a deviation
from the Climate and Forecast Convention 1.6). The resulting annual mean anomaly generally
falls in the range of <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> to 2 mm d<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> and is most pronounced along
the Equator (Fig. 4a). The models show a mean increase in precipitation
directly south of the Equator<?pagebreak page2975?> in the Pacific basin, as well as in the
Pacific subtropics off the western North American coast. The North Atlantic
also receives a mean positive precipitation anomaly, offsetting part of the
positive salinity anomaly there, which is potentially relevant for the
simulation of deepwater formation in this region (Sect. 3.7). Negative mean
precipitation anomalies are most pronounced directly north of the Equator
and north of <inline-formula><mml:math id="M56" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 40<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in the Pacific basin, as well as
in the Atlantic Arctic. The inter-model spread is up to <inline-formula><mml:math id="M58" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5 mm d<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> around the Equator, likely due to the model disagreement about
the sign and location of changes in the inter-tropical convergence zone
(Fig. 4b). Related to precipitation fluxes, river run-off fluxes also changed
between the lgm and piControl model experiments. As land–sea masks and river
routing are very model specific, we can not provide a gridded river run-off
anomaly. Instead, we provide mean absolute and relative large-scale river
run-off changes integrated over ocean basins (North/South Atlantic,
North/South Pacific, Indian Ocean; Table 4). These anomalies can be used by
modelling groups to scale pre-industrial river run-off. Note that evaporation
simulated by a forced ocean model will generally not equal the sum of the
prescribed precipitation and river run-off. For long integrations, it is
therefore necessary to adjust one (or both) of these forcings to close the
freshwater balance and avoid salinity drift. We assume that modelling groups
employing our anomaly forcing will have such a mechanism suitable for their
model in place.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T4" orientation="landscape"><?xmltex \currentcnt{4}?><label>Table 4</label><caption><p id="d1e1147">River run-off simulated by the PMIP3 models. Note that only
four of the models (CNRM-CM5, IPSL-CM5A-LR, MIROC-ESM, and MRI-CGCM3)
provide the necessary output. Arctic is defined as the region north of
65<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and the eastern boundaries of the Southern Ocean sectors of
the Pacific, Atlantic, and Indian oceans are at 70<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, 20<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E,
and 148<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, respectively.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.9}[.9]?><oasis:tgroup cols="8">
     <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:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Global</oasis:entry>
         <oasis:entry colname="col3">Arctic</oasis:entry>
         <oasis:entry colname="col4">North Atlantic</oasis:entry>
         <oasis:entry colname="col5">South Atlantic</oasis:entry>
         <oasis:entry colname="col6">North Pacific</oasis:entry>
         <oasis:entry colname="col7">South Pacific</oasis:entry>
         <oasis:entry colname="col8">Indian</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">PI, in 10<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula> kg s<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (mean<inline-formula><mml:math id="M66" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>max<inline-formula><mml:math id="M67" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>min)</oasis:entry>
         <oasis:entry colname="col2">1.20 <inline-formula><mml:math id="M68" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 1.41 <inline-formula><mml:math id="M69" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 1.07</oasis:entry>
         <oasis:entry colname="col3">0.12 <inline-formula><mml:math id="M70" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.16 <inline-formula><mml:math id="M71" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.07</oasis:entry>
         <oasis:entry colname="col4">0.38 <inline-formula><mml:math id="M72" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.49 <inline-formula><mml:math id="M73" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.32</oasis:entry>
         <oasis:entry colname="col5">0.14 <inline-formula><mml:math id="M74" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.17 <inline-formula><mml:math id="M75" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.13</oasis:entry>
         <oasis:entry colname="col6">0.29 <inline-formula><mml:math id="M76" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.33 <inline-formula><mml:math id="M77" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.25</oasis:entry>
         <oasis:entry colname="col7">0.15 <inline-formula><mml:math id="M78" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.21 <inline-formula><mml:math id="M79" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.09</oasis:entry>
         <oasis:entry colname="col8">0.12 <inline-formula><mml:math id="M80" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.16 <inline-formula><mml:math id="M81" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.08</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">LGM, in 10<inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula> kg s<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (mean<inline-formula><mml:math id="M84" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>max<inline-formula><mml:math id="M85" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>min)</oasis:entry>
         <oasis:entry colname="col2">1.23 <inline-formula><mml:math id="M86" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 1.41 <inline-formula><mml:math id="M87" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.93</oasis:entry>
         <oasis:entry colname="col3">0.04 <inline-formula><mml:math id="M88" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.08 <inline-formula><mml:math id="M89" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.004</oasis:entry>
         <oasis:entry colname="col4">0.38 <inline-formula><mml:math id="M90" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.48 <inline-formula><mml:math id="M91" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.20</oasis:entry>
         <oasis:entry colname="col5">0.15 <inline-formula><mml:math id="M92" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.17 <inline-formula><mml:math id="M93" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.12</oasis:entry>
         <oasis:entry colname="col6">0.31 <inline-formula><mml:math id="M94" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.38 <inline-formula><mml:math id="M95" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.24</oasis:entry>
         <oasis:entry colname="col7">0.18 <inline-formula><mml:math id="M96" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.23 <inline-formula><mml:math id="M97" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.14</oasis:entry>
         <oasis:entry colname="col8">0.17 <inline-formula><mml:math id="M98" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.25 <inline-formula><mml:math id="M99" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 0.12</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Relative change, in % (mean<inline-formula><mml:math id="M100" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>max<inline-formula><mml:math id="M101" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>min)</oasis:entry>
         <oasis:entry colname="col2">1.8 <inline-formula><mml:math id="M102" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 16.3 <inline-formula><mml:math id="M103" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M104" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>13.2</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M105" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>70.4 <inline-formula><mml:math id="M106" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M107" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45.2 <inline-formula><mml:math id="M108" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M109" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>93.9</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M110" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.7 <inline-formula><mml:math id="M111" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 20.5 <inline-formula><mml:math id="M112" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M113" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35.7</oasis:entry>
         <oasis:entry colname="col5">4.4 <inline-formula><mml:math id="M114" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 37.7 <inline-formula><mml:math id="M115" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M116" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>14.2</oasis:entry>
         <oasis:entry colname="col6">6.9 <inline-formula><mml:math id="M117" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 20.6 <inline-formula><mml:math id="M118" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M119" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10.2</oasis:entry>
         <oasis:entry colname="col7">29.6 <inline-formula><mml:math id="M120" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 59.8 <inline-formula><mml:math id="M121" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 5.6</oasis:entry>
         <oasis:entry colname="col8">43.4 <inline-formula><mml:math id="M122" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 94.5 <inline-formula><mml:math id="M123" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 2.6</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e1759">Annual mean precipitation lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in mm d<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><?xmltex \opttitle{Wind anomalies: $u$ and $v$ components}?><title>Wind anomalies: <inline-formula><mml:math id="M125" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M126" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> components</title>
      <p id="d1e1810">Both for the <inline-formula><mml:math id="M127" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M128" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> component of the wind speed, the lgm–piControl anomaly
is time-interpolated to 6-hourly fields. The annual mean meridional wind
velocity (<inline-formula><mml:math id="M129" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula>, southerly winds) anomaly shows a pronounced increase
(<inline-formula><mml:math id="M130" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 3–5 m s<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in southerly winds around the north-western edge of
the Laurentide Ice Sheet, as well as over the north-western edge of the Scandinavian Ice
Sheet (Fig. 5a). Alongside that, a pronounced decrease (<inline-formula><mml:math id="M132" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 3–5 m s<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in southerly winds is simulated along the eastern North American
coast and the Canadian Archipelago. The open ocean anomalies are generally
small (at most <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). The inter-model spread has no
pronounced pattern but is sizable with <inline-formula><mml:math id="M136" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1–5 m s<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
disagreement between the PMIP3 models (Fig. 5b). The mean zonal wind velocity (<inline-formula><mml:math id="M138" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>,
westerly winds) anomaly shows alternating negative and positive anomaly
bands with an approximate <inline-formula><mml:math id="M139" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>2 m s<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> range (Fig. 6a). This pattern
is stronger in the Northern Hemisphere north of <inline-formula><mml:math id="M141" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. The inter-model spread (<inline-formula><mml:math id="M143" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1–3 m s<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) has
little structure except for the <inline-formula><mml:math id="M145" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 4–5 m s<inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> disagreement
in the Southern Ocean south of <inline-formula><mml:math id="M147" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 40<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and the
<inline-formula><mml:math id="M149" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3–5 m s<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> disagreement in the North Atlantic (Fig. 6b).
In the Southern Ocean, the band of large<?pagebreak page2976?> disagreement in westerly wind speeds
reflects the large uncertainty in the simulated position of the Southern
Hemisphere's jet stream, both in pre-industrial times and the LGM. This
disagreement is reinforced by the fact that shifts in the jet position
between pre-industrial times and the LGM also depend on the simulated expansion of
sea ice (Sime et al. 2016; Fig. A3).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2034"> Annual mean meridional wind velocity lgm–piControl anomaly  <bold>(a)</bold> and
model spread <bold>(b)</bold> (in m s<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f05.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Temperature anomaly</title>
      <p id="d1e2069">The near-surface atmospheric temperature is time-interpolated to calculate
the 6-hourly mean anomaly for temperature. The annual mean anomaly is most
pronounced in the North Atlantic, where open ocean anomalies exceed <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> K.
Elsewhere, the annual mean temperature anomaly is <inline-formula><mml:math id="M153" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> K (Fig. 7a).
There is a clear pattern in the model spread: the models show a large spread
(<inline-formula><mml:math id="M155" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 10 K) north of <inline-formula><mml:math id="M156" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 45<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, as well as
south of <inline-formula><mml:math id="M158" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S (5–10 K), likely due to the
disagreement about ice cover (Fig. A3). At lower latitudes, the model spread
is generally smaller (0–3 K) (Fig. 7b).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2141">Annual mean zonal wind velocity lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in m s<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e2170">Annual mean temperature lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in K).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><title>Sea surface salinity anomaly</title>
      <p id="d1e2193">Global mean salinity is initialized in PMIP3 models with a 1 psu higher
salinity to account for the concentrating effect of the decrease in sea
level (Kageyama et al., 2017). Sea surface salinity, however, shows a more
variable annual mean lgm–piControl change due to changes in the global
hydrological cycle (Fig. 8). The sea surface salinity anomaly is presented
on a regular <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> grid for ease of use. The resulting annual mean SSS anomaly
(Fig. 8a) shows an increase in sea surface salinity (<inline-formula><mml:math id="M162" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 psu)
over the Southern Ocean south of <inline-formula><mml:math id="M163" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 55<inline-formula><mml:math id="M164" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, as well as
in the Arctic (<inline-formula><mml:math id="M165" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 3 psu) and the northern Indian Ocean
(<inline-formula><mml:math id="M166" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 1 psu). A <inline-formula><mml:math id="M167" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2 psu anomaly is simulated in the
Canadian Archipelago, the Labrador Sea, and across the North Atlantic between
what is now Canada and Europe (Fig. 8a). Freshening is simulated close to
some continents and is especially pronounced around Scandinavia (about <inline-formula><mml:math id="M168" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3 psu). Simulated ocean circulation can be very sensitive to fresh water
forcing and thus SSS, especially in the North Atlantic (e.g. Rahmstorf,
1996; Spence et al., 2008). Applications of SSS restoring using the SSS
anomaly field should therefore be done with caution and attention to its
effects on the meridional overturning circulation. The tuning of the salinity
anomaly in important deepwater formation regions of up to about <inline-formula><mml:math id="M169" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 psu, such as done by, for example, Winguth et al. (1999), may be required to
obtain a satisfactory circulation field in reasonable agreement with proxy
data. Such adjustments fall well within the PMIP3 model spread (Fig. 8b) and
show the current limitations of fully coupled PMIP3 models in simulating an
LGM hydrological cycle consistent with proxy records of ocean circulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e2269">Annual mean sea surface salinity lgm–piControl anomaly <bold>(a)</bold> and
model spread <bold>(b)</bold> (in psu).</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f08.png"/>

        </fig>

</sec>
</sec>
<?pagebreak page2977?><sec id="Ch1.S4">
  <label>4</label><title>Limitations of the dataset</title>
      <p id="d1e2293">The anomaly fields presented here are a model-based “best estimate” of the
LGM anomaly relative to the pre-industrial state. There are some important
limitations to these data related to the temporal resolution, the use of
model means, and the fact that we rely on modelling results only.</p>
      <p id="d1e2296">Proxy data with global coverage are unavailable for most of the variables
needed to force stand-alone ocean models. We do not attempt to constrain the
anomaly fields using the spatially limited information from available proxy
data. Consequently, where PMIP3 models are in disagreement with proxy data,
our dataset will be so, too. The limitations (or uncertainty) of the PMIP3
simulations can be seen through the large inter-model spread which is
provided with the anomaly data. This does not preclude the possibility that
PMIP3 models collectively (i.e. such that the model spread is small)
disagree with available proxy data. Nevertheless, PMIP3 is the state of the
art for the modelling of past climates at present (Braconnot et al., 2012;
Braconnot and Kageyama, 2015).</p>
      <p id="d1e2299">By adding multi-model mean anomalies to forcing fields, dynamical
inconsistencies (e.g. between wind and temperature fields) will be created.
This means that the resulting forcing fields do not strictly obey the
equations of state or motion. A forcing dataset would typically be dynamically
consistent if the forcing would be the outcome of an atmospheric model or an
advanced reanalysis. The advantage of using model mean fields is that large
anomalies of individual models will be smoothed out where models disagree.
We believe that currently a main challenge for palaeo-modelling activities is
to achieve integration times that are long enough. Therefore, using a single forcing
(as opposed to using multiple forcings from individual models) seems to be
preferable. Regarding the dynamical inconsistencies, it is important to note
that the CORE forcing itself (for which our dataset is optimized) is a
mixture of reanalysis and observational data products and as such not
dynamically consistent.</p>
      <p id="d1e2302">PMIP3 model output is publicly available only as monthly mean fields, which
also results in some limitations for the anomaly forcing dataset. First,
although we interpolate the monthly mean anomaly fields to a higher (e.g.
6-hourly) temporal resolution, we implicitly assume that any sub-monthly
variability (e.g. the diurnal cycle) is preserved from the pre-industrial
climate state to the LGM state. We can currently not quantify the
implications of this assumption, but future phases of PMIP (providing
simulation output with higher temporal resolution) might alleviate this
problem. Second, we are not able to accurately re-reference near-surface
temperature and humidity to a different reference height. The CORE bulk
forcing method of Large and Yeager (2004) requires near-surface specific
humidity and temperature at the same height as the wind forcing (at 10 m). Humidity and temperature are, however, provided at 2 m height
in PMIP3 (as in most atmospheric data products). A procedure to<?pagebreak page2978?> re-reference
humidity and temperature from 2 to 10 m (e.g. Large and Yeager, 2004)
requires input data at a higher (sub-daily) time resolution in order to
resolve different boundary layer stability regimes. However, for an anomaly
forcing, the re-referencing only has an effect if it leads to different
temperature and/or humidity increments under the PI and the LGM state. For the open
ocean, this is barely the case, and taking a climatological anomaly of
2 m quantities and applying it at 10 m height is unproblematic. Over
sea ice, however, there could be a larger effect of the re-referencing (due
to a significantly different atmospheric stability in the LGM state),
especially regarding the temperature. Our analysis indicates that this is
probably the case over the central Arctic Ocean (not shown). For all other
regions, we estimate that the error made in applying the re-referencing
approach on monthly climatological-resolved data does not justify its
application. In general, the error made by omitting the re-referencing is
much smaller than the uncertainties of the anomalies (i.e. the model
spread), particularly at high latitudes.</p>
      <p id="d1e2306">Regarding the robustness of the dataset, we observe that the inclusion of
additional model data only leads to minor changes in the anomalies. An
example of this is given by comparing version 1 (Morée and Schwinger,
2019) and the current version 3 (Morée and Schwinger, 2020) of this
dataset, as the latter also includes the GISS-E2-R model for the calculation
of the anomalies. Indeed, individual model anomalies (Fig. A1) show broad
agreement, although the magnitude of the anomaly is less agreed on (as
discussed in more detail for the individual variables in Sect. 3).</p>
      <p id="d1e2309">Despite the limitations described here, we believe that using the mean PMIP3
anomaly of coupled models as forcing is currently the best available option
for use in stand-alone ocean models. For this purpose, our dataset provides
lgm–piControl anomalies in standardized format for the most common variables
used in ocean forcing.</p>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Data availability</title>
      <p id="d1e2321">The data are publicly accessible at the NIRD Research Data Archive at
<ext-link xlink:href="https://doi.org/10.11582/2020.00052" ext-link-type="DOI">10.11582/2020.00052</ext-link> (Morée and Schwinger, 2020). The
.md5 files contain an md5 checksum, which can be used to check whether
changes have been made to the respective NetCDF files.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Summary and conclusions</title>
      <p id="d1e2335">The output of the fully coupled PMIP3 simulations of CNRM-CM5, IPSL-CM5A-LR,
MIROC-ESM, MRI-CGCM3 and GISS-E2-R is converted to anomaly datasets intended
for use in forced ocean modelling of the LGM. All anomalies are calculated
as the difference between the “lgm” and “piControl” PMIP3 experiments. In
addition, all data are formatted in a way that further conversions (of, for
example, units or the grid) can be applied in a straightforward way.<?pagebreak page2979?> The
variables are provided in NetCDF format in separate files and distributed
by the NIRD Research Data Archive (Morée and Schwinger, 2020). A
climatological LGM forcing dataset can be created for any forced ocean
model by the addition of the presented 2-D anomaly fields to the model's
pre-industrial forcing. This approach enables the scientific community to
simulate the LGM ocean state in a forced ocean model set-up. We expect that
if additional forcing is needed for a specific model, the same approach as
described above can be followed. This process is simplified by providing all
main CDO and NCO commands used in creating the dataset (Table 3). All data
represent a climatological year, i.e. one annual cycle per variable. The
application of the data is thus suitable for “time-slice” equilibrium
simulations of the LGM and optimized for use with the CORE forcing format
(Large and Yeager, 2004).</p>
      <p id="d1e2338">The uncertainty of our anomaly forcing (approximated by the model spread of
the PMIP3 models) is generally of similar magnitude as the multi-model
annual mean. The complete attribution of the model spread to specific
processes is beyond the scope of this article, but our results show that
there is considerable uncertainty involved in the magnitude of the anomaly
for all variables presented here. Nevertheless, all mean anomalies show a
distinct spatial pattern that we expect to be indicative of the LGM–PI
changes. Finally, there is currently no other way to reconstruct most of
these variables than model simulations with state-of-the-art Earth system
models such as those applied in the PMIP3 experiments. For modelling
purposes, the inter-model disagreement of PMIP3 provides the user with leeway
to adjust the amplitude of the forcing (guided by the size of the model
spread, which is therefore provided alongside the variables in the dataset).
Such adjustments can improve model–proxy data agreements, such as those described
for salinity in Sect. 3.7.</p><?xmltex \hack{\clearpage}?>
</sec>

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

<?pagebreak page2980?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title/>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F9"><?xmltex \currentcnt{A1}?><label>Figure A1</label><caption><p id="d1e2354">Annual mean individual model anomalies for each of the variables
(see Table 1) and models in the dataset. Units are the same as in the remainder of this
paper.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f09.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="App1.Ch1.S1.F10" specific-use="star"><?xmltex \currentcnt{A2}?><label>Figure A2</label><caption><p id="d1e2367">Annual mean for each of the variables (see Table 1) for the
piControl CMIP5/PMIP3 experiment.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f10.png"/>

      </fig>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F11"><?xmltex \currentcnt{A3}?><label>Figure A3</label><caption><p id="d1e2381">Annual mean model spread of sea-ice fraction.</p></caption>
        <?xmltex \igopts{width=270.301181pt}?><graphic xlink:href="https://essd.copernicus.org/articles/12/2971/2020/essd-12-2971-2020-f11.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2396">ALM prepared, visualized, and analysed the data
and wrote the original draft of the paper. ALM and JS together
conceptualized the method and revised the paper. JS provided
supervision throughout the study.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2402">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2408">We acknowledge the World Climate Research
Programme's Working Group on Coupled Modelling, which is responsible for
CMIP, and we thank the climate modelling groups (Table 2) for producing and
making available their model output. For CMIP, the US Department of
Energy's Program for Climate Model Diagnosis and Intercomparison provides
coordinating support and led development of software infrastructure in
partnership with the Global Organization for Earth System Science Portals.
This is a contribution to the Bjerknes Centre for Climate Research (Bergen,
Norway). Storage resources were provided by UNINETT Sigma2 – the National
Infrastructure for High Performance Computing and Data Storage in Norway
(project number ns2980k). The authors thank four anonymous reviewers and Editor Kirsten Elger for their valuable feedback on our paper.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2413">This research has been supported by CRESCENDO (Coordinated Research in Earth Systems and Climate: Experiments, kNowledge, Dissemination and Outreach; European Commission's Horizon 2020 European Union Framework Programme for Research and Innovation, grant no. 641816) and the Research Council of Norway (project INES 270061). Anne L. Morée is grateful for PhD funding through the Faculty for Mathematics and Natural Sciences of the University of Bergen (UoB), as well as support by the Meltzer fund of UoB and Erasmus Mundus to stay at ETH Zürich for part of this work.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2419">This paper was edited by Kirsten Elger and reviewed by four anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>A Last Glacial Maximum forcing dataset for ocean modelling</article-title-html>
<abstract-html><p>Model simulations of the Last Glacial Maximum (LGM;
 ∼ &thinsp;21 000 years before present) can aid the interpretation of
proxy records, can help to gain an improved mechanistic understanding of the LGM
climate system, and are valuable for the evaluation of model performance in
a different climate state. Ocean-ice only model configurations forced by
prescribed atmospheric data (referred to as <q>forced ocean models</q>)
drastically reduce the computational cost of palaeoclimate modelling
compared to fully coupled model frameworks. While feedbacks between the
atmosphere and ocean and sea-ice compartments of the Earth system are not
present in such model configurations, many scientific questions can be
addressed with models of this type. Our dataset supports simulations of the
LGM in a forced ocean model set-up while still taking advantage of the
complexity of fully coupled model set-ups. The data presented here are
derived from fully coupled palaeoclimate simulations of the Palaeoclimate
Modelling Intercomparison Project phase 3 (PMIP3). The data are publicly
accessible at the National Infrastructure for Research Data (NIRD) Research Data Archive at
<a href="https://doi.org/10.11582/2020.00052" target="_blank">https://doi.org/10.11582/2020.00052</a> (Morée and Schwinger, 2020). They
consist of 2-D anomaly forcing fields suitable for use in ocean models that
employ a bulk forcing approach and are optimized for use with CORE forcing
fields. The data include specific humidity, downwelling long-wave and
short-wave radiation, precipitation, wind (<i>v</i> and <i>u</i> components), temperature,
and sea surface salinity (SSS). All fields are provided as climatological
mean anomalies between LGM and pre-industrial (PI) simulations. These anomaly
data can therefore be added to any pre-industrial ocean forcing dataset in
order to obtain forcing fields representative of LGM conditions as simulated
by PMIP3 models. Furthermore, the dataset can be easily updated to reflect
results from upcoming and future palaeo-model intercomparison activities.</p></abstract-html>
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