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  <front>
    <journal-meta><journal-id journal-id-type="publisher">CP</journal-id><journal-title-group>
    <journal-title>Climate of the Past</journal-title>
    <abbrev-journal-title abbrev-type="publisher">CP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Clim. Past</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1814-9332</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/cp-17-1065-2021</article-id><title-group><article-title>The PMIP4 Last Glacial Maximum experiments: preliminary results and
comparison with the PMIP3 simulations</article-title><alt-title>The PMIP4 Last Glacial Maximum experiments</alt-title>
      </title-group><?xmltex \runningtitle{The PMIP4 Last Glacial Maximum experiments}?><?xmltex \runningauthor{M.~Kageyama et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Kageyama</surname><given-names>Masa</given-names></name>
          <email>masa.kageyama@lsce.ipsl.fr</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Harrison</surname><given-names>Sandy P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5687-1903</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kapsch</surname><given-names>Marie-L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9551-5370</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Lofverstrom</surname><given-names>Marcus</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Lora</surname><given-names>Juan M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9925-1050</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Mikolajewicz</surname><given-names>Uwe</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Sherriff-Tadano</surname><given-names>Sam</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4378-9166</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Vadsaria</surname><given-names>Tristan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6535-0576</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Abe-Ouchi</surname><given-names>Ayako</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1745-5952</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bouttes</surname><given-names>Nathaelle</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Chandan</surname><given-names>Deepak</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0756-754X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Gregoire</surname><given-names>Lauren J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0258-7282</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Ivanovic</surname><given-names>Ruza F.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7805-6018</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Izumi</surname><given-names>Kenji</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9651-6420</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff10">
          <name><surname>LeGrande</surname><given-names>Allegra N.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lhardy</surname><given-names>Fanny</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11">
          <name><surname>Lohmann</surname><given-names>Gerrit</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2089-733X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff12">
          <name><surname>Morozova</surname><given-names>Polina A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5959-7452</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Ohgaito</surname><given-names>Rumi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5717-1594</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff14">
          <name><surname>Paul</surname><given-names>André</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1961-139X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Peltier</surname><given-names>W. Richard</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5555-7661</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff15">
          <name><surname>Poulsen</surname><given-names>Christopher J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5104-4271</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Quiquet</surname><given-names>Aurélien</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6207-3043</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff16">
          <name><surname>Roche</surname><given-names>Didier M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6272-9428</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff10">
          <name><surname>Shi</surname><given-names>Xiaoxu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Tierney</surname><given-names>Jessica E.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9080-9289</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Valdes</surname><given-names>Paul J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1902-3283</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff17">
          <name><surname>Volodin</surname><given-names>Evgeny</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff18">
          <name><surname>Zhu</surname><given-names>Jiang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0908-5130</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Laboratoire des Sciences du Climat et de l'Environnement/Institut
Pierre-Simon Laplace, UMR CEA-CNRS-UVSQ, Université Paris-Saclay, 91191
Gif-sur-Yvette, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Archaeology, Geography and Environmental Science (SAGES),
University of Reading, Reading, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Max Planck Institute for Meteorology, 20146 Hamburg, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>University of Arizona, Tucson, AZ 85721, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Yale University, New Haven, CT 06520, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Atmospheric and Ocean Research Institute, The University of Tokyo,
Kashiwa, Japan</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Department of Physics, University of Toronto, 60 St. George Street,
Toronto, Ontario M5S1A7, Canada</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>School of Earth and Environment, University of Leeds, Woodhouse Lane, Leeds, LS2 9JT, UK</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>School of Geographical Sciences, University of Bristol, University
Road, Bristol, BS8 1SS, UK</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>NASA Goddard Institute for Space Studies, 2880 Broadway, New York, NY 10025, USA</institution>
        </aff>
        <aff id="aff11"><label>11</label><institution>Alfred Wegener Institute, Bremerhaven, Germany</institution>
        </aff>
        <aff id="aff12"><label>12</label><institution>Institute of Geography, Russian Academy of Science, Moscow, Russia</institution>
        </aff>
        <aff id="aff13"><label>13</label><institution>Japan Agency for Marine-Earth Science and Technology, Yokohama, Japan</institution>
        </aff>
        <aff id="aff14"><label>14</label><institution>MARUM – Center for Marine Environmental Sciences and Department of
Geosciences, <?xmltex \hack{\break}?>University of Bremen, Bremen, Germany</institution>
        </aff>
        <aff id="aff15"><label>15</label><institution>Department of Earth and Environmental Sciences, University of
Michigan, Ann Arbor, MI 48109, USA</institution>
        </aff>
        <aff id="aff16"><label>16</label><institution>Vrije Universiteit Amsterdam, Faculty of Science, Cluster Earth and
Climate, de Boelelaan 1085,  <?xmltex \hack{\break}?>Amsterdam, the Netherlands</institution>
        </aff>
        <aff id="aff17"><label>17</label><institution>Institute of Numerical Mathematics, Russian Academy of Sciences,
Moscow, Russia</institution>
        </aff>
        <aff id="aff18"><label>18</label><institution>Climate and Global Dynamics Laboratory, National Center for
Atmospheric Research, Boulder, CO 80305, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Masa Kageyama (masa.kageyama@lsce.ipsl.fr)</corresp></author-notes><pub-date><day>20</day><month>May</month><year>2021</year></pub-date>
      
      <volume>17</volume>
      <issue>3</issue>
      <fpage>1065</fpage><lpage>1089</lpage>
      <history>
        <date date-type="received"><day>31</day><month>December</month><year>2019</year></date>
           <date date-type="rev-request"><day>23</day><month>January</month><year>2020</year></date>
           <date date-type="rev-recd"><day>21</day><month>December</month><year>2020</year></date>
           <date date-type="accepted"><day>31</day><month>January</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Masa Kageyama et al.</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://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021.html">This article is available from https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021.html</self-uri><self-uri xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e461">The Last Glacial Maximum (LGM, <inline-formula><mml:math id="M1" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 21 000 years ago)
has been a major focus for evaluating how well state-of-the-art climate
models simulate climate changes as large as those expected in the future
using paleoclimate reconstructions. A new generation of climate models has
been used to generate LGM simulations as part of the Paleoclimate Modelling
Intercomparison Project (PMIP) contribution to the Coupled Model
Intercomparison Project (CMIP). Here, we provide a preliminary analysis and
evaluation of the results of these LGM experiments (PMIP4, most of which are PMIP4-CMIP6) and compare them with the previous generation of simulations
(PMIP3, most of which are PMIP3-CMIP5). We show that the global averages of the
PMIP4 simulations span a larger range in terms of mean annual surface air
temperature and mean annual precipitation compared to the PMIP3-CMIP5
simulations, with some PMIP4<?pagebreak page1066?> simulations reaching a globally colder and
drier state. However, the multi-model global cooling average is similar for
the PMIP4 and PMIP3 ensembles, while the multi-model PMIP4 mean annual
precipitation average is drier than the PMIP3 one. There are important
differences in both atmospheric and oceanic circulations between the two
sets of experiments, with the northern and southern jet streams being more
poleward and the changes in the Atlantic Meridional Overturning Circulation
being less pronounced in the PMIP4-CMIP6 simulations than in the PMIP3-CMIP5
simulations. Changes in simulated precipitation patterns are influenced by
both temperature and circulation changes. Differences in simulated climate
between individual models remain large. Therefore, although there are
differences in the average behaviour across the two ensembles, the new
simulation results are not fundamentally different from the PMIP3-CMIP5
results. Evaluation of large-scale climate features, such as land–sea
contrast and polar amplification, confirms that the models capture these
well and within the uncertainty of the paleoclimate reconstructions.
Nevertheless, regional climate changes are less well simulated: the models
underestimate extratropical cooling, particularly in winter, and
precipitation changes. These results point to the utility of using
paleoclimate simulations to understand the mechanisms of climate change and
evaluate model performance.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e480">The climate of the Last Glacial Maximum (LGM; <inline-formula><mml:math id="M2" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 21 000 years
ago) has been a focus of the Paleoclimate Modelling Intercomparison Project
(PMIP) since its inception. It is the most recent global cold extreme and
as such has been widely documented and used for benchmarking
state-of-the-art climate models (Braconnot et al., 2012; Harrison et al.,
2014, 2015). The increase in global temperature from the LGM until now
(<inline-formula><mml:math id="M3" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 4 to 6 <inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C; Annan and Hargreaves, 2015;
Friedrich et al., 2016) has been the same order of magnitude as the increase
projected by 2100 CE under moderate-to-high emission scenarios. The LGM
world was very different from the present one, with large ice sheets
covering northern North America and Fennoscandia, in addition to the
Greenland and Antarctic ice sheets still present today. These additional ice
sheets resulted in a lowering of the global sea level by <inline-formula><mml:math id="M5" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 120 m,
which induced changes in the land–sea distribution. The closure of the
Bering Strait and the exposure of the Sunda and Sahul shelves between
southeast Asia and the Maritime Continent are the most prominent of these
changes in land–sea geography. Atmospheric greenhouse gas (GHG)
concentrations were lower than pre-industrial (PI) values, leading to
cooling in addition to that induced by the large ice sheets. The cooling is
more pronounced in the high latitudes than in the tropics and greater over
land than ocean. The polar amplification and the land–sea contrast signals
simulated by the previous generation of paleoclimate simulations
(PMIP3 – Coupled Model Intercomparison Project; PMIP3-CMIP5)
are similar in magnitude (although opposite in sign) to the
signals seen in future projections and have been shown to be consistent with
climate observations for the historic period and reconstructions for the LGM
(Braconnot et al., 2012; Izumi et al., 2013; Harrison et al., 2014, 2015).
However, while the models are able to represent the thermodynamic behaviour
that gives rise to these large-scale temperature gradients, they
underestimate cooling on land, especially winter cooling, and overestimate
tropical cooling over the oceans (Harrison et al., 2014). Thus, one question
to be addressed with the new PMIP4-CMIP6 simulations is whether there is any
improvement in capturing regional temperature changes. The large temperature
changes during the LGM compared to the pre-industrial period make this interval a natural focus for efforts to
constrain climate sensitivity but attempts to do this using the PMIP3-CMIP5
simulations were inconclusive (Schmidt et al., 2014; Harrison et al., 2014),
in part because of the limited number of LGM simulations available and in
part because of the limited range of climate sensitivity sampled by these
models. Changes in model configuration have resulted in several of the
PMIP4-CMIP6 models having substantially higher climate sensitivity than the
PMIP3-CMIP5 versions of the same models, and thus the range of climate
sensitivity sampled by the PMIP4-CMIP6 models is much wider. This provides
an opportunity to re-examine whether the LGM could provide a strong
constraint on climate sensitivity (Renoult et al., 2020; Zhu et al., 2021).</p>
      <p id="d1e513">The atmospheric general circulation was strongly modified from its modern-day conditions by changes in coastlines at low latitudes (DiNezio and
Tierney, 2013) and by the presence of the Laurentide and Fennoscandian ice
sheets (e.g. Laîné et al., 2009; Löfverström et al., 2014, 2016;
Ullman et al., 2014; Beghin et al., 2015; Liakka and Löfverström, 2018).
These changes in circulation had an impact on precipitation, which was
reduced globally (Bartlein et al., 2011) but increased locally, for example,
in southwestern North American and in the Mediterranean region (e.g. Kirby
et al., 2013; Beghin et al., 2016; Goldsmith et al., 2017; Lora et al.,
2017; Lora, 2018; Löfverström and Lora, 2017; Löfverström and Liakka, 2016;
Löfverström, 2020; Rehfeld et al., 2020). The interplay between
temperature-driven and circulation-driven changes in regional precipitation
during the LGM represents a test of the ability of state-of-the-art models to
simulate precipitation changes under future scenarios, where both
thermodynamic (e.g. related to the Clausius–Clapeyron relationship) and
dynamic (e.g. related to changes in the position of the storm tracks and
extent of the subtropical anticyclones) effects contribute to changes in the
amount and location of precipitation (e.g. Boos, 2012; Scheff and Freirson,
2012; Lora, 2018). Evaluation of the PMIP3-CMIP5 simulations showed that
models underestimate the LGM reduction in mean annual precipitation over
land (Harrison et al., 2014), reflecting the underestimation of temperature
changes in the simulations (Li et al., 2013).<?pagebreak page1067?> This resulted in an
underestimation of the observed aridity (precipitation minus
evapotranspiration). While the models reproduced circulation-induced changes
in precipitation in western North America, they showed no increase in
precipitation south of the North American ice sheet and only limited impact
on the precipitation of the circum-Mediterranean region (Harrison et al.,
2014; Lora, 2018; Morrill et al., 2018). Thus, one question to be addressed
with the new PMIP4-CMIP6 simulations is whether there is any improvement in
capturing regional precipitation changes. One complication here is that most
of the reconstructions used to evaluate the PMIP3-CMIP5 simulations were
pollen based and relied on statistical approaches that do not account for
the direct impact of low CO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on water-use efficiency (Prentice and
Harrison, 2009; Gerhardt and Ward, 2010; Bragg et al., 2013; Scheff et al.,
2017) and could therefore be dry biased. However, new methods have been
developed that account for this effect (Prentice et al., 2017), and thus it
is possible to determine whether accounting for the effect of low CO<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
resolves model–data mismatches in regional precipitation at the LGM.</p>
      <p id="d1e534">The LGM boundary conditions also had a strong impact on ocean circulation,
as documented via multiple tracers (e.g. Lynch-Stieglitz et al., 2007;
Jaccard and Galbraith, 2011; Böhm et al., 2015), which suggest a
shallower North Atlantic Deep Water (NADW) cell and expanded Antarctic Bottom Water
(AABW). In addition, Gebbie (2014) used a combination of synthesis of multiple
tracers measured in sediment cores for the LGM and a global tracer transport
model to show that these tracers are compatible with a vertical distribution
of NADW and AABW similar to today but that the core of the NADW water mass
shoals by 1000 m. None of these proposed reconstructions of glacial
circulation are consistent with the PMIP3-CMIP5 model results (Muglia and
Schmittner, 2015), which all show a deepening of the Atlantic Meridional
Overturning Circulation (AMOC), with NADW reaching the ocean floor in the
northern North Atlantic for some models. Previous studies show that this
increase in AMOC is related to changes in northern extratropical wind stress
due to the presence of the high ice sheets (Oka et al., 2012; Muglia and
Schmittner, 2015; Klockmann et al., 2016; Sherriff-Tadano et al., 2018;
Galbraith and de Lavergne, 2019). Thus, the simulation of the AMOC, and ocean
circulation in general, during the LGM could be highly sensitive to the ice-sheet reconstructions used as boundary conditions (see, e.g. Ullman et al.,
2014; Beghin et al., 2016). There is still some uncertainty about the height
and shape (although not the extent) of the LGM ice sheets, so the protocol
for the LGM PMIP4-CMIP6 experiment takes this uncertainty into account by
allowing for alternative ice-sheet configurations (Kageyama et al., 2017) in
order to test the sensitivity of LGM climate and ocean circulation to ice-sheet configuration. The PMIP4-CMIP6 LGM experimental protocol also includes
changes in other forcings, including vegetation changes and changes in
atmospheric dust loadings and their uncertainties. Thus, the new PMIP4-CMIP6
simulations provide opportunities to examine the response of the climate
system to multiple forcings, to calculate the impact of individual forcings
through sensitivity experiments and to investigate how these forcings
combine to produce circulation and climate changes in the marine and
terrestrial realms.</p>
      <p id="d1e537">In this paper, we present preliminary results from the PMIP4-CMIP6 LGM
simulations, compare them to the PMIP3-CMIP5 results (Sect. 3) and
evaluate their realism against a range of climatic reconstructions (Sect. 4).
We focus on temperature and precipitation, extratropical circulation,
energy transport and the AMOC.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Material and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>PMIP3-CMIP5 and PMIP4-CMIP6 protocols for the LGM simulations</title>
      <p id="d1e555">The protocol of the LGM experiments changed between the PMIP3-CMIP5 and
PMIP4-CMIP6 phases (Kageyama et al., 2017), partly to accommodate new
information about boundary conditions and partly to capitalise on new
features of the climate models. The main difference between the PMIP3-CMIP5
and PMIP4-CMIP6 simulations is the specification of the ice sheets. The
PMIP3-CMIP5 simulations all used the same ice sheet, which was created as a
composite of three separate ice-sheet reconstructions (Abe-Ouchi et al.,
2015); the PMIP4-CMIP6 protocol allows modelling groups to use one of three
separate ice-sheet reconstructions: the original PMIP3-CMIP5 ice sheet to
facilitate comparison with the earlier simulations, ICE-6G_C
(Argus et al., 2014; Peltier et al., 2015) and GLAC-1D (Lev Tarasov, personal
communication, 2016; Ivanovic et al., 2016). All three reconstructions have similar
ice-sheet extent, but the heights of the Laurentide, Fennoscandian and West
Antarctica ice sheets differ significantly, by several hundred metres in
some places. Comparisons of the simulations made with alternative ice-sheet
reconstructions will ultimately allow an assessment of the impact of forcing
uncertainties on simulated climates.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e561">PMIP3 and PMIP4 models analysed in the present study. The spin-up
duration is only given for the new PMIP4-CMIP6 models.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.80}[.80]?><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="78pt"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="55pt"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="90pt"/>
     <oasis:colspec colnum="4" colname="col4" align="justify" colwidth="48pt"/>
     <oasis:colspec colnum="5" colname="col5" align="justify" colwidth="48pt"/>
     <oasis:colspec colnum="6" colname="col6" align="justify" colwidth="68pt"/>
     <oasis:colspec colnum="7" colname="col7" align="justify" colwidth="136pt"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">Climate</oasis:entry>
         <oasis:entry colname="col3">Reference</oasis:entry>
         <oasis:entry colname="col4">Ice</oasis:entry>
         <oasis:entry colname="col5">Spin-up</oasis:entry>
         <oasis:entry colname="col6">PMIP/CMIP</oasis:entry>
         <oasis:entry colname="col7">Additional comments</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">sensitivity</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">duration</oasis:entry>
         <oasis:entry colname="col5">phase and</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">(<inline-formula><mml:math id="M8" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi></mml:mrow><mml:msup><mml:mi>T</mml:mi><mml:mtext>eq</mml:mtext></mml:msup></mml:mrow></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">(years)</oasis:entry>
         <oasis:entry colname="col5">rip (<inline-formula><mml:math id="M9" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CCSM4</oasis:entry>
         <oasis:entry colname="col2">2.9</oasis:entry>
         <oasis:entry colname="col3">Brady et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">3.3</oasis:entry>
         <oasis:entry colname="col3">Voldoire et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5  r1i1p1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">COSMOS-ASO</oasis:entry>
         <oasis:entry colname="col2">4.1</oasis:entry>
         <oasis:entry colname="col3">Raddatz et al. (2007); <?xmltex \hack{\hfill\break}?>Budich et al. (2010), <?xmltex \hack{\hfill\break}?>Wetzel et al. (2010)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3  <?xmltex \hack{\hfill\break}?>r1i1p1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">FGOALS-g2</oasis:entry>
         <oasis:entry colname="col2">4.4</oasis:entry>
         <oasis:entry colname="col3">Zheng and Yu (2013)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">2.1</oasis:entry>
         <oasis:entry colname="col3">Ullman et al. (2014)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p150</oasis:entry>
         <oasis:entry colname="col7">PMIP3 ice sheet</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">2.1</oasis:entry>
         <oasis:entry colname="col3">Ullman et al. (2014)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 <?xmltex \hack{\hfill\break}?>r1i1p151</oasis:entry>
         <oasis:entry colname="col7">ICE-5G ice extent but lower Laurentide Ice Sheet altitude</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">4.1</oasis:entry>
         <oasis:entry colname="col3">Dufresne et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MIROC-ESM</oasis:entry>
         <oasis:entry colname="col2">4.7</oasis:entry>
         <oasis:entry colname="col3">Sueyoshi et al. (2013)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p1</oasis:entry>
         <oasis:entry colname="col7">Initial ocean state was taken from PMIP2 MIROC4m</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">3.5</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p1</oasis:entry>
         <oasis:entry colname="col7">AO, initial state for spin-up from PMIP2 simulation</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">3.5</oasis:entry>
         <oasis:entry colname="col3">Adloff et al. (2018)</oasis:entry>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p2</oasis:entry>
         <oasis:entry colname="col7">AOV</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MRI-CGCM3</oasis:entry>
         <oasis:entry colname="col2">2.6</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">PMIP3</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">PMIP3-CMIP5 r1i1p1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">AWI-ESM1-1-LR (short name: <?xmltex \hack{\hfill\break}?>AWIESM1)</oasis:entry>
         <oasis:entry colname="col2">3.6</oasis:entry>
         <oasis:entry colname="col3">Sidorenko et al. (2015), <?xmltex \hack{\hfill\break}?>Lohmann et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">1300</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">AWI-ESM-2-1-LR (short name <?xmltex \hack{\hfill\break}?>AWIESM2)</oasis:entry>
         <oasis:entry colname="col2">3.6</oasis:entry>
         <oasis:entry colname="col3">Sidorenko et al. (2019)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">600</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">CESM1.2</oasis:entry>
         <oasis:entry colname="col2">3.6</oasis:entry>
         <oasis:entry colname="col3">Tierney et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">ICE-6GC</oasis:entry>
         <oasis:entry colname="col5">1800</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">UoT-CCSM4</oasis:entry>
         <oasis:entry colname="col2">3.2</oasis:entry>
         <oasis:entry colname="col3">Peltier and Vettoretti <?xmltex \hack{\hfill\break}?>(2014),  Chandan and <?xmltex \hack{\hfill\break}?>Peltier (2018), Chandan and  Peltier (2017)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">2900 years</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">HadCM3B-M2.1aD</oasis:entry>
         <oasis:entry colname="col2">2.7</oasis:entry>
         <oasis:entry colname="col3">Valdes et al. (2017)</oasis:entry>
         <oasis:entry colname="col4">GLAC-1D <?xmltex \hack{\hfill\break}?>ICE-6G_C <?xmltex \hack{\hfill\break}?>PMIP3</oasis:entry>
         <oasis:entry colname="col5">400 <?xmltex \hack{\hfill\break}?>400 <?xmltex \hack{\hfill\break}?>2900</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7">All simulations were initialised from a long (<inline-formula><mml:math id="M10" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 5000-year) LGM run that used the same model configuration but ICE5G boundary conditions (ice mask, global orography, bathymetry, land–sea mask) and PMIP3 trace gases. The climatologies were calculated from the 100 years following the spin-up period.</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">iLOVECLIM1.1.4</oasis:entry>
         <oasis:entry colname="col2">3.2 <?xmltex \hack{\hfill\break}?>(after 2500 <?xmltex \hack{\hfill\break}?>years)</oasis:entry>
         <oasis:entry colname="col3">Lhardy et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">GLAC-1D <?xmltex \hack{\hfill\break}?>ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">5000</oasis:entry>
         <oasis:entry colname="col6">PMIP4</oasis:entry>
         <oasis:entry colname="col7">5000 years from a PI restart; EMIC</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">iLOVECLIM1.1.4</oasis:entry>
         <oasis:entry colname="col2">3.2 <?xmltex \hack{\hfill\break}?>(after 2500 <?xmltex \hack{\hfill\break}?>years)</oasis:entry>
         <oasis:entry colname="col3">Lhardy et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">5000</oasis:entry>
         <oasis:entry colname="col6">PMIP4</oasis:entry>
         <oasis:entry colname="col7">5000 years from a PI restart; EMIC</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">INM-CM4-8</oasis:entry>
         <oasis:entry colname="col2">2.1</oasis:entry>
         <oasis:entry colname="col3">Volodin et al. (2018)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">50</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6 r1i1p1f1</oasis:entry>
         <oasis:entry colname="col7"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">IPSLCM5A2</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">Sepulchre et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">1200</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6</oasis:entry>
         <oasis:entry colname="col7">Spin-up from <italic>piControl</italic></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MIROC-ES2L</oasis:entry>
         <oasis:entry colname="col2">2.7</oasis:entry>
         <oasis:entry colname="col3">Ohgaito et al. (2021) <?xmltex \hack{\hfill\break}?>Hajima et al. (2020)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_C</oasis:entry>
         <oasis:entry colname="col5">8960</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6 r1i1p1f2</oasis:entry>
         <oasis:entry colname="col7">First 6760 years integrated using the MIROC-ES2L physical core; following 2200 years integrated using MIROC-ES2L</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM1.2</oasis:entry>
         <oasis:entry colname="col2">2.77</oasis:entry>
         <oasis:entry colname="col3">Mauritsen et al. (2019)</oasis:entry>
         <oasis:entry colname="col4">ICE-6G_c</oasis:entry>
         <oasis:entry colname="col5">3850</oasis:entry>
         <oasis:entry colname="col6">PMIP4-CMIP6 r1i1p1f1</oasis:entry>
         <oasis:entry colname="col7">3850 years after restart from a previous <italic>lgm</italic> simulation.</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>PMIP3, PMIP3-CMIP5, PMIP4 and PMIP4-CMIP6 models</title>
      <?pagebreak page1069?><p id="d1e1264">The LGM model output analysed here are from the PMIP4-CMIP6 and PMIP3-CMIP5
<italic>lgm</italic> experiments. We use the corresponding <italic>piControl</italic> experiments as a reference, which are
termed “PI” throughout the paper. Some of the models, although
following the PMIP3-CMIP5 or PMIP4-CMIP6 protocols, did not formally take
part in CMIP (i.e. have not performed the DECK experiments for CMIP6 or
have not performed other experiments than PMIP experiments for CMIP5). These
are referred to as “PMIP3” and “PMIP4” models in Table 1. We will refer
to the full ensemble of PMIP3-CMIP5 and PMIP3-non-CMIP5 experiments as the
PMIP3 ensemble and similarly for the PMIP4 ensemble. A total of 13 PMIP4 LGM
simulations are currently available and slightly more than the 11 LGM
simulations in PMIP3 (Table 1). The PMIP3 ensemble includes one model that
ran an additional sensitivity test to ice-sheet height (GISS-E2R; Ullman et
al., 2014) and one model that ran simulations with and without dynamic
vegetation (MPI-ESM-P; Adloff et al., 2018). The PMIP4-CMIP6 ensemble
includes three simulations made with updated versions of the models that
contributed to PMIP3-CMIP5, specifically IPSLCM, MIROC and MPI-ESM (Table 1).
However, the IPSL simulation for PMIP4 does not use the latest IPSLCM6
version specifically developed for CMIP6 due to the impossibility to run the
<italic>lgm</italic> experiment with this version. Most of the models that have run the
PMIP4-CMIP6 LGM simulations are general circulation models (GCMs) but
iLOVECLIM is an Earth system model of intermediate complexity, which is
considerably faster than the GCMs. The iLOVECLIM and the HadCM3B-M2.1aD GCMs are
the only models in the ensemble to have run simulations using different ice-sheet reconstructions (both models ran with ICE-6G_C and
GLAC-1D, and HadCM3B-M2.1aD also ran with the PMIP3 ice sheet). The LGM
simulations were either initialised from a previous LGM simulation or were
spun up from the pre-industrial state. The length of the spin-up therefore
varies (Table 1), as does the length of the equilibrium LGM simulation in
these preliminary analyses. The INM-CM4-8 results are from the beginning of
an <italic>lgm</italic> simulation and the model is not yet fully equilibrated. All other models
have run for several millennia. Our preliminary analyses are based on
variables available by 14 December 2020. Although several of the
PMIP4-CMIP6 models have higher climate sensitivity than the equivalent models in
PMIP3-CMIP5, this is not reflected in the ensemble analysed here. In fact,
the PMIP4-CMIP6 ensemble, as of December 2020, has lower climate
sensitivities than the PMIP3-CMIP5 models (Table 1): equilibrium
sensitivities to a CO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> doubling from pre-industrial values range from
2.1 to 3.6 <inline-formula><mml:math id="M12" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, (mean: 3.0 <inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) in the current PMIP4-CMIP6
ensemble, while the range is from 2.1 to 4.7 <inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (mean:
3.4 <inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) in the PMIP3-CMIP5 ensemble.</p>
      <p id="d1e1325">All in all, only a minority of models present in the PMIP3 ensemble ran the
PMIP4 simulation, so that the PMIP4 ensemble differs from the PMIP3 one
because of the update of these models but mostly because it gathers new
models compared to PMIP3. This adds up to the change in protocol from PMIP3
to PMIP4 to explain differences in model results between these two phases of
PMIP.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Sources of information on LGM climate</title>
      <p id="d1e1336">The PMIP3-CMIP5 model simulations were evaluated against two benchmark
datasets: pollen-based reconstructions of seasonal temperature (mean annual
temperature – MAT, mean temperature of the coldest month – MTCO, mean
temperature of the warmest month – MTWA, growing season temperature
indexed by growing degree days above a baseline of 0 <inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), mean
annual precipitation (MAP) and an index of soil moisture (Bartlein et al.,
2011); and a compilation of sea-surface temperature (SST) reconstructions
(MARGO Project Members, 2009).</p>
      <p id="d1e1348">In the Bartlein et al. (2011) dataset, reconstructions at individual pollen
sites were averaged to produce an estimate for a <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> grid;
reconstruction uncertainties are estimated as a pooled estimate of the
standard errors of the original reconstructions for all sites in each grid
cell. Although the Bartlein et al. (2011) dataset has good coverage for some
regions, coverage was sparse in the tropics, and there were no
reconstructions of LGM climate for Australia. Furthermore, not all of the
six climate variables were reconstructed at every site, so statistical
comparisons were more robust for some variables than others. The majority of
the reconstructions included in the Bartlein et al. (2011) dataset used
various sorts of statistical calibrations based on modern-day conditions and
therefore do not account for the impact that changes in CO<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> have on
water-use efficiency and hence plant distribution. Although Bartlein
et al. (2011) were unable to demonstrate a statistically significant difference
between statistical reconstructions and model-based inversions (which, in
principle, account for the CO<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> effect on plant distribution), their
analysis focused on the mid-Holocene where the CO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> effect is small.
There is therefore some concern that the dataset may overestimate aridity
at the LGM. Reconstructions which incorporate the effect of CO<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> are now
available for Australia (Prentice et al., 2017). Cleator et al. (2020) have
used 3-D variational data assimilation techniques with a prior derived from
the PMIP3-CMIP5 LGM simulations and the Bartlein et al. (2011) and Prentice
et al. (2017) pollen-based reconstructions, and incorporating the Prentice
et al. (2017) CO<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> correction, to produce a new global reconstruction
of terrestrial climate at the LGM. In addition to accounting for potential
effects of low CO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on moisture variables at the LGM, this
reconstruction produces coherent estimates of seasonal climate variables at
many more points than the original pollen-based reconstructions and also
extends the geographic coverage.</p>
      <p id="d1e1422">Tierney et al. (2020) provide a new synthesis of geochemical SST data
(<inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>,
TEX<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">86</mml:mn></mml:msub></mml:math></inline-formula>, <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Mg</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ca</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O) from the
LGM (defined as the period from 19 000 to 23 000 years ago) and the late
Holocene (defined as the period from 4000 years ago to the present) time
periods. This compilation builds upon the MARGO Project Members (2009) collection of
<inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Mg</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Ca</mml:mi></mml:mrow></mml:math></inline-formula> data by including new studies published
since MARGO was released, as well as expanding the collection to include
TEX<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">86</mml:mn></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O of foraminifera. The Tierney et al. (2020)
synthesis excludes microfossil-based SST estimates, on the basis that these (1) include no-analogue assemblages (Mix et al., 1999); (2) imply
warmer-than-present subtropical gyres, an inference that has been questioned
(Crowley, 2000; Telford et al., 2013); and (3) lack Bayesian proxy-system
models that were required for the data assimilation technique used by
Tierney et al. (2020).<?pagebreak page1070?> Tierney et al. (2020) use the data along with a model
prior from the isotope-enabled Community Earth System Model 1.2 (CESM1.2; Brady
et al., 2019) to produce a full-field data assimilation product. Here, we use
both the data synthesis and the data assimilation products, labelled
“Tierney2020” and “Tierney2020DA”, respectively. Data from the LGM and late
Holocene, respectively, were calibrated using Bayesian models that fully
propagate uncertainties (Tierney and Tingley, 2015; Tierney et al., 2018, 2019;
Malevich et al., 2019), yielding a 1000-member
posterior distribution of SSTs. These data were sorted from low to high
along the ensemble dimension, and then random error representative of
site-level downcore uncertainty following the Gaussian distribution <inline-formula><mml:math id="M32" display="inline"><mml:mi mathvariant="script">N</mml:mi></mml:math></inline-formula>(0, 0.5 <inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) was added back to the
matrix. This procedure effectively partitions the error variance; i.e. it
assumes that at any given site, absolute uncertainty in SST cancels out in
the anomaly calculation, while “relative” uncertainty associated with
downcore measurement and non-linearities in the calibration model is
preserved. The data were then averaged within a <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">5</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">5</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>
grid and differenced. The standard deviation associated with each grid point
is calculated from the differenced ensemble dimension.</p>
      <p id="d1e1558">In the present work, we also use other available reconstructions, all based
on at least part of the initial MARGO Project Members (2009) reconstructions at the core
sites: all are global reconstructions, obtained from this dataset via
different methods, as summarised by Paul et al. (2021). These datasets are
from
<list list-type="bullet"><list-item>
      <p id="d1e1563">Annan and Hargreaves (2013), who use the MARGO Project Members (2009) dataset, the
Bartlein et al. (2019) reconstructions on the continents, as well as the
PMIP2 model output to generate a reconstruction of the sea-surface
temperatures using multiple linear regression;</p></list-item><list-item>
      <p id="d1e1567">Kurahashi-Nakamura et al. (2017), who use the MARGO Project Members (2009) data, benthic
<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>O and <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">13</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>C data as well as the MIT General Circulation Model (MITgcm) in
combination with the method of Lagrange multipliers/adjoint method to
generate a global reconstruction;</p></list-item><list-item>
      <p id="d1e1593">Paul et al. (2021), who produced the GLOMAP2020 dataset based on the
floral and faunal assemblage data, as well as various sea-ice
reconstructions from MARGO Project Members (2009), together with an optimal gridding method
called DIVA to produce monthly global reconstructions. A caveat given in
Paul et al. (2021) about this reconstruction is that it may be too warm by
0.5 to 1.0 <inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C due to impacts of changes in seasonality and in the
thermal structure of the ocean that are not taken into account in their
reconstructions, as well as the impact due to heterogeneous spatial
sampling.</p></list-item></list>
These datasets reflect different approaches and choices of initial datasets
(only geochemical data for the Tierney et al. (2020) reconstructions, for
which the sites are often close to the coasts or only floral and faunal
assemblages for GLOMAP2020), which yields a range a results with illustrate
the uncertainty of the SST reconstructions. A crucial difference between the
Tierney et al. (2020) synthesis and the other datasets used here is that
the former implies more extensive tropical cooling during the LGM
(<inline-formula><mml:math id="M38" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>2.5 <inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C vs. <inline-formula><mml:math id="M40" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.5 <inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for MARGO, <inline-formula><mml:math id="M42" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.2 <inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for
GLOMAP2020, <inline-formula><mml:math id="M44" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.6 <inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for Annan and Hargreaves, 2013,
<inline-formula><mml:math id="M46" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1.7 <inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for Kurahashi-Nakamura et al., 2017). This can be
attributed to the exclusion of the microfossil data as well as recalibration
of the <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> proxy with the BAYSPLINE model (Tierney and
Tingley, 2018), which corrects for an observed reduced sensitivity of
<inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> to SST above approximately 24 <inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The
data-assimilated product from Tierney et al. (2020) is even cooler, which
might be related to the choice of the global model for the assimilation. A
further comparison is presented in Paul et al. (2021).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Data–model comparisons</title>
      <p id="d1e1739">We compare the model simulations to paleoclimate data, focusing on
large-scale features and regional changes. In these comparisons, the
reconstructions are expressed as mean values and the uncertainty by the
standard error of the reconstructions. Model outputs were extracted only for
the grid cells where there are observations. Model uncertainty is
represented by the standard deviation of 10 000 averages over 50 years
randomly picked in the <inline-formula><mml:math id="M51" display="inline"><mml:mo>≥</mml:mo></mml:math></inline-formula> 100-year-long time series of model
outputs. Thus, model uncertainty is not, strictly speaking, equivalent to
reconstruction uncertainty but merely provides some measure of the
variability engendered by sampling the simulated climate.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e1751">Mean annual surface air temperatures LGM–PI anomalies in <inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. <bold>(a)</bold> Zonal means,
PMIP3 model results shown as dashed lines,
PMIP4 model results shown as thick solid lines; <bold>(b)</bold> global means, PMIP3 model
results shown by crosses, PMIP4 models shown by filled circles; averages
over <bold>(c)</bold> the southern extratropics (90 to 30<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S),
<bold>(d)</bold> the tropics (30<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 30<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) and <bold>(e)</bold> the northern
extratropics (30 to 90<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N).</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f01.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Model results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Temperature</title>
      <p id="d1e1837">The global and annual mean temperature in the PMIP4 LGM simulations is
between 3.3 and 7.2 <inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C cooler than the PI simulations (Fig. 1,
Table S1). The largest changes in temperature between the LGM and PI
simulations (Fig. 2) are found over the Laurentide and Fennoscandian ice
sheets, reflecting the significant changes in surface height and albedo
caused by the ice sheets. Colder conditions are registered in the northern
midlatitudes and high latitudes, partly reflecting the advection of the cold
temperature anomalies downwind of the ice sheets. The cooling in the
tropics, which results from both the lower atmospheric GHG concentrations
and the remote influence of the northern ice sheets, is more muted. As
expected, the simulations show larger changes over the land than over ocean.
The ratio between the LGM–PI mean surface air temperature anomaly over
land and the anomaly over the ocean ranges from 1.0 to 1.6 over the tropics
(30<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 30<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) and from 1.90 to 5.5 for globally
averaged temperatures. Zonally averaged temperatures (Fig. 1a) confirm<?pagebreak page1071?> that
the PMIP4 ensemble also shows the expected polar amplification of
temperature changes in both the Northern Hemisphere and Southern Hemisphere.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1869">LGM mean annual temperature (in <inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) simulated by the
ensemble of PMIP4 models <bold>(a)</bold>, LGM–PI mean annual temperature anomaly
(in <inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) simulated by the same models (middle, where stippling
shows where models do not agree on the sign of changes), difference between
the PMIP4 and PMIP3 ensembles (in <inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, <bold>b</bold>). The PMIP4 average
is based on models listed in Table 1, except for iLOVECLIM simulations,
which are at lower resolution. The PMIP3 average is based on all PMIP3
models, except the GISS-E2-p151 simulation, which did not use the PMIP3 ice
sheet for its boundary conditions.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f02.png"/>

        </fig>

      <p id="d1e1911">Although the broad-scale patterns of temperature changes are similar, there
are differences between the PMIP4 and PMIP3 ensembles. The PMIP4 ensemble
average is warmer than the PMIP3 ensemble average (Fig. 2 bottom) over North
America, south of the ice sheet, over the Labrador and Nordic Seas and the
Tibetan Plateau. On the other hand, the PMIP4 average is colder than the
PMIP3 one in regions close to West Antarctica, over some areas of the
Laurentide Ice Sheet, over the marine part of the Fennoscandian Ice Sheet
and in the North Atlantic and the northern part of the North Pacific. The
largest difference between the PMIP3 and PMIP4 averages is over the northern
North Atlantic and Nordic Seas, probably reflecting differences in sea-ice
cover in these areas. Zonally averaged temperatures (Fig. 1a) show that the
PMIP4 global mean annual temperature LGM–PI anomalies spread over a
larger range than the PMIP3 ensemble, with a few PMIP4 models (in particular
the three HadCM3 simulations and CESM1.2) showing larger cooling than the
coldest PMIP3 models. Nonetheless, the multi-model average of the global
mean annual temperature LGM–PI anomalies are similar for both ensembles
(<inline-formula><mml:math id="M63" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>4.71 <inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the PMIP3 ensemble, <inline-formula><mml:math id="M65" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.77 <inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the PMIP4
ensemble; see Supplement Table S1).</p>
      <?pagebreak page1072?><p id="d1e1947">The northern extratropics are slightly colder in the PMIP3 simulations
(multi-model LGM–PI MAT anomaly of <inline-formula><mml:math id="M67" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.5 <inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) than in the PMIP4
simulations (multi-model average of <inline-formula><mml:math id="M69" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.8 <inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). The minimum cooling and
maximum cooling over the PMIP3 and PMIP4 ensembles are also very similar.
The PMIP3 and PMIP4 simulations yield similar cooling in the tropics
(multi-model average of <inline-formula><mml:math id="M71" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.8 <inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the PMIP3 ensemble and of
<inline-formula><mml:math id="M73" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.7 <inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the PMIP4 ensemble, with similar minima and maxima;
see Table S1). However, the cooling of the southern extratropics is more
variable in the PMIP4 simulations (<inline-formula><mml:math id="M75" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>1.2 to approximately <inline-formula><mml:math id="M76" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>8.15 <inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) than in
the PMIP3 simulations (<inline-formula><mml:math id="M78" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>2.4 to approximately <inline-formula><mml:math id="M79" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.8 <inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), and its multi-model
average is larger for the PMIP4 ensemble (<inline-formula><mml:math id="M81" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>4.8 <inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, compared to
<inline-formula><mml:math id="M83" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.8 <inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the PMIP3 ensemble). Therefore, most of the difference
in the global average cooling, which ranges from <inline-formula><mml:math id="M85" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.3 to <inline-formula><mml:math id="M86" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.2 <inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
in the PMIP4 simulations and between <inline-formula><mml:math id="M88" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.7 and <inline-formula><mml:math id="M89" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.7 <inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in the PMIP3
simulations, stems from differences in the simulated temperatures over the
Southern Hemisphere. It is difficult to assign these differences between the
PMIP3 and PMIP4 ensembles to a single reason, since both models and
protocols have changed between these two phases. Sensitivity experiments and
in-depth study of the experiments carried out with the PMIP3 and PMIP4
protocols but with the same models will be necessary to disentangle the
reasons for the differences between the PMIP3 and PMIP4 results. It is in
fact rather intriguing that the average cooling over the North American ice
sheet is larger in the PMIP4 ensemble, given that both the ICE-6G_C
and the GLAC-1D reconstructions yield significantly lower altitudes than the
PMIP3 ice-sheet reconstruction, used in all the PMIP3 experiments.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e2144">Same as Fig. 2 but for the 250 hPa zonal wind. The PMIP4 average
is based on all models listed in Table 1. The PMIP3 average is based on all
PMIP3 models in Table 1, except the GISS-E2-p151 simulation, which did not
use the PMIP3 ice sheet for its boundary conditions.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Atmospheric and oceanic circulation</title>
      <p id="d1e2161">The PMIP4-CMIP6 models simulate large changes in the Northern Hemisphere
upper tropospheric atmospheric circulation (Fig. 3), in response to LGM
boundary conditions, in particular over North America and the North
Atlantic. The North Atlantic jet stream is narrower and stronger compared to
the PI, as shown by an increase reaching more than 10 m s<inline-formula><mml:math id="M91" 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 250 hPa
zonal wind south of the<?pagebreak page1073?> Laurentide Ice Sheet and extending into the North
Atlantic, and a decrease in zonal wind to the northwest and southeast of
these regions. The strengthening and narrowing of the North Atlantic jet
stream was also a characteristic of the PMIP3-CMIP5 simulations (Beghin et
al., 2016). However, in the PMIP4-CMIP6 simulations, the jet stream extends
further north than in the PMIP3 simulations (Fig. 3, bottom), most
prominently near the Laurentide Ice Sheet. This could be because the
Laurentide Ice Sheet is lower in the ICE-6G reconstruction than the ice
sheet used in the PMIP3-CMIP5 simulations (see, e.g. Ullman et al., 2014;
Beghin et al., 2015; Lofverstom et al., 2016) but may also reflect changes
in the representation of the zonal winds between the two sets of
simulations. This is supported by the fact that there are differences
between the PMIP3-CMIP5 and PMIP4 simulations away from the Laurentide Ice
Sheet, in particular over the Southern Ocean, where the jet stream is also
located more poleward in the PMIP4 than the PMIP3 simulations. Sensitivity
experiments using the PMIP3-CMIP5 ice sheets with PMIP4 models, as planned
in the PMIP4 LGM experiment protocol (Kageyama et al., 2017), should help
resolve the question of whether differences in model treatment or boundary
conditions are responsible for the differences in atmospheric circulation
between the two ensembles.</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="d1e2178">Mean Atlantic Meridional Overturning Circulation (mean meridional
stream function for the Atlantic Ocean at 30<inline-formula><mml:math id="M92" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) simulated by the
PMIP3 and PMIP4 models for PI and LGM. Numbers in Sv indicate the LGM–PI
anomaly in terms of maximum Atlantic meridional overturning streamfunction.
Numbers in metres indicate the LGM–PI anomaly in terms of NADW vertical
extension, the NADW vertical extent being defined here as the depths over
which the mean meridional stream function for the Atlantic Ocean at
30<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N is positive.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f04.png"/>

        </fig>

      <p id="d1e2205">The extent of the NADW cell (identified in Fig. 4
by the depths for which the Atlantic meridional overturning
streamfunction at 30<inline-formula><mml:math id="M94" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N is positive) simulated by PMIP4 models is
very similar for LGM and PI, except for iLOVECLIM and IPSLCM5A2, which show
a very large deepening of the NADW cell for LGM (Fig. 4). Two of the
PMIP4-CMIP6 models (INM-CM4-8 and MIROC-ES2L) show a deep NADW cell reaching
the ocean floor in the North Atlantic, whereas five of the PMIP4-CMIP6
models (MPI-ESM1.2, UoT-CCSM4, AWIESM2, CESM1.2, HadCM3) simulate a clear
AABW in the North Atlantic. UoT-CCSM4 and CESM1.2
even shows a shallowing of the NADW cell for LGM. The intrusion of AABW cell
(defined by negative values in the Atlantic meridional overturning
streamfunction at 30<inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) into the North Atlantic was shown by some
of the PMIP3-CMIP5 simulations (CCSM4, MPI-ESM-1.0P) but not as much as the
PMIP4 simulations (AWIESM2, CESM1.2, MPI-ESM-1.2, UoT-CCSM4 and the three
HadCM3 simulations, Fig. 4 and Muglia and Schmittner, 2015). Five of the PMIP3-CMIP5
models produced a NADW cell reaching the ocean floor in the North Atlantic
and only two had extensive AABW. The maximum strength of the NADW cell
itself strengthens in all of the PMIP4 simulations by as much as 11 Sv for
IPSLCM5A2. This strengthening is consistent with PMIP3-CMIP5 results and is
likely to be associated with the vigorous surface wind over the northern
North Atlantic (Muglia and Schmittner, 2015; Sherriff-Tadano and Abe-Ouchi, 2020)
and the closure of the Bering Strait (Hu et al., 2015). The strength
of the AMOC reduces south of 30<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N in UoT-CCSM4 (see Supplement
Fig. S2). iLOVECLIM performed simulations of LGM with two different ice-sheet reconstructions (ICE6G, GLAC1D) and shows a weaker NADW cell in GLAC-1D
than that produced by ICE-6G_C (Fig. 4). This weakening is
likely to be associated with a lower topography of the ice sheet of GLAC1D
(e.g. Zhang et al., 2014). On the other hand, HadCM3 was used with the PMIP3,
ICE-6G_C and GLAC-1D ice sheets, and the results in terms of
AMOC are very similar for the ICE-6G_C and GLAC-1D ice
sheets, for which the AMOC slightly strengthens compared to PI, while the
AMOC is similar to the PI one for the simulation using the PMIP3 ice sheet.</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="d1e2238">Meridional energy transport for the PI reference state (left-hand side) and
LGM–PI anomaly (right-hand side). <bold>(a, b)</bold> Total energy transport, <bold>(c, d)</bold> atmospheric
energy transport, <bold>(e, f)</bold> oceanic energy transport.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f05.png"/>

        </fig>

      <p id="d1e2256">These circulation changes in the Atlantic Ocean are reflected in the total
ocean heat transport (Fig. 5, bottom, the PMIP4 results available for this
analysis are from all simulations but the HadCM3 simulations). MPI-ESM1.2
simulates an increase in northward ocean heat transport at all latitudes for
the LGM compared to PI, while MIROC-ES2L simulates an increase in this
transport from 15<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 60<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. UoT-CCSM4 and CESM1.2 are
the only models simulating a decrease in northward heat transport over a
significant range of latitudes, from 50<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 70<inline-formula><mml:math id="M100" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, in
the <italic>lgm</italic> run compared to the <italic>piControl</italic> one. INCM4-CM4-8 simulates  increased ocean
transport south of 20<inline-formula><mml:math id="M101" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. IPSLCM5A2's ocean transport decreases
south of 30<inline-formula><mml:math id="M102" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S and between the Equator and 30<inline-formula><mml:math id="M103" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N but
significantly increases in the southern tropics. All PMIP4 models simulate
an increase in northward atmospheric heat transport, in the tropics and up
to 50<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, in the <italic>lgm</italic> simulation compared to <italic>piControl</italic>. MIROC-ES2L simulates an
increase up to 70<inline-formula><mml:math id="M105" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N (Fig. 5, middle). In summary, all models
simulate an increase, in their <italic>lgm</italic> run compared to <italic>piControl</italic>, in northward heat transport
(Fig. 5, top) in the tropics and northern midlatitudes, although in the
UoT-CCSM4 and CESM1.2 models the increase is confined between
<inline-formula><mml:math id="M106" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 and 50<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. This increase in northward heat
transport in the tropics and northern midlatitudes during the LGM as
compared to PI was also simulated by most PMIP3-CMIP5 models. Given that the
magnitude of the heat transport increase is similar in the PMIP4 and
PMIP3-CMIP6 simulations, the warmer temperatures at high northern latitudes
in the PMIP4-CMIP6 simulations cannot be due to differences in northward
ocean heat transport.</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="d1e2378"><bold>(a, b)</bold> PMIP4-CMIP6 multi-model LGM mean annual precipitation in mm d<inline-formula><mml:math id="M108" 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>. <bold>(c)</bold> PMIP4-CMIP6 multi-model LGM–PI mean annual
precipitation anomaly (mm d<inline-formula><mml:math id="M109" 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>) with stippling showing areas where less than
nine models agree on the sign of change. <bold>(b)</bold> Difference between the
PMIP4-CMIP6 and the PMIP3 multi-model means of the LGM mean annual
precipitation (mm d<inline-formula><mml:math id="M110" 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>). <bold>(d)</bold> Difference between the PMIP4-CMIP6 and
the PMIP3 multi-model means of the PI mean annual precipitation (mm d<inline-formula><mml:math id="M111" 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=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Hydrological cycle</title>
      <p id="d1e2455">The large-scale gradients in precipitation are similar in the multi-model
average of the PMIP4 LGM and PI simulations (Fig. 6, top left), with maximum
precipitation in the tropics (Intertropical Convergence Zone (ITCZ) and monsoon
regions) and secondary maxima in the midlatitudes, corresponding to the
position of the North Pacific, North Atlantic and Southern Ocean
storm tracks. The PMIP4 models show a decrease in precipitation between the
LGM and PI in all these high-precipitation areas (Fig. 6, bottom left and
Fig. 7, top left). There are some regions where precipitation increases<?pagebreak page1074?> during
the LGM compared to the PI: at least nine PMIP4 models (as shown by the areas
which are not stippled) show more precipitation over the subtropical Pacific
Ocean and to the south of the Laurentide Ice Sheet, over southern Africa and
over the Iberian Peninsula, and some simulate an increase in precipitation
over the northern and southern subtropical zones in the Pacific and over the
southern subtropical zone in the Atlantic. However, the areas with decreased
precipitation are much more extensive than areas with increased
precipitation, so zonal averages for the southern extratropics, tropics and
northern extratropics (Fig. 7) all show a decrease in precipitation.</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="d1e2460">Same as Fig. 1 for mean annual precipitation in mm yr<inline-formula><mml:math id="M112" 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=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f07.png"/>

        </fig>

      <p id="d1e2481">The broad-scale patterns of change in precipitation in the PMIP4 simulations
are similar to those found in the PMIP3-CMIP5 simulations (Fig. 7, top
left). However, the PMIP4 multi-model average is drier than the PMIP3-CMIP5
one (Fig. 6) at the global scale as well as for the southern extratropics
and for the tropics. It is similar for both ensembles for the northern
extratropics. The geographic patterning in the precipitation changes between
the PMIP4 and PMIP3-CMIP5 ensembles (Fig. 6, top right) are complex,
particularly in the tropical where the wetter–drier–wetter pattern in the
meridional direction suggests differences in ITCZ representation between the
two generations of models. This is confirmed by the same figure drawn for
the PI (Fig. 6, bottom right), which shows very similar patterns in the
PMIP3 vs. PMIP4 anomalies. Both ensembles show a consistent decrease in
zonally averaged precipitation in the southern and northern extratropics
(Fig. 7). As for the mean annual temperature, the simulated range of
precipitation changes is larger for PMIP4 ensemble compared to the PMIP3
one, except for the northern extratropics for which both ensembles show a
similar range (Figs. 7 and 2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2487">Same as Fig. 2 for mean annual evaporation (left-hand side) and mean annual
net precipitation (precipitation–evaporation, right-hand side). All values are in
mm d<inline-formula><mml:math id="M113" 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>. Stippling shows areas where less than nine models agree on the sign of
change.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f08.png"/>

        </fig>

      <p id="d1e2508">Evapotranspiration patterns in the PMIP4 LGM and PI simulations are
characterised by maximum values in the subtropics and decrease towards high
latitudes. The models simulate a global decrease in LGM evapotranspiration
relative to the PI that strongly peaks over and around the Northern
Hemisphere ice sheets (Fig. 8, left). These results are in agreement with
the broad patterns of the PMIP3-CMIP5 ensemble, except for a stronger
decrease in evaporation in the northern North Atlantic, which corresponds to
the larger average cooling in these regions in the PMIP4 ensemble compared
to the PMIP3 ensemble. As a result, net precipitation (precipitation minus
evapotranspiration) in the PMIP4 ensemble is higher during the LGM than the PI
in the extratropics – particularly over the midlatitude eastern Pacific<?pagebreak page1076?> in
both hemispheres and over most of North America – with the exception of the
North Atlantic, where evaporation decreases are more localised and do not
compensate for the reductions in precipitation (Fig. 8, right). This,
together with colder temperatures, could help explain why the PMIP4 models
simulate a stronger AMOC at the LGM. Substantial reductions in continental
net precipitation only occur over tropical South America and high-latitude
regions, over the Labrador Sea and its surrounding ice sheets, while Africa,
Australia and the midlatitude regions of Eurasia and the Americas see
little change or even increased net precipitation.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Data–model comparisons</title>
      <p id="d1e2520">The evaluation of the PMIP3-CMIP5 LGM simulations showed that large-scale
climate features, such as the ratio of changes in land–sea temperature,
high-latitude temperature amplification and precipitation scaling with
temperature, were broadly consistent with modern observations (Braconnot et
al., 2012; Izumi et al., 2013; Harrison et al., 2014, 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e2525">Comparison of terrestrial climate variables from the combined
Bartlein et al. (2011) and Prentice et al. (2017) dataset and from the
Cleator et al. (2020) reconstruction using data assimilation, averaged over
20<inline-formula><mml:math id="M114" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitudinal bands. The variables are mean annual temperature
(MAT), mean temperature of the coldest month (MTCO), mean temperature of the
warmest month (MTWA) and mean annual precipitation (MAP). The orange
boxplots show the results from the Bartlein et al. (2011) and Prentice
et al. (2017) combined dataset, the dark blue boxplots for the reconstructions
by Cleator et al. (2020) at sites for which there are reconstructions in the
combined dataset, and the green boxplots show the results for the full
reconstructions from Cleator et al. (2020).</p></caption>
        <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f09.png"/>

      </fig>

      <p id="d1e2543">All PMIP3 and PMIP4 models simulate larger cooling over land than over
oceans, on average for the tropics and for the globe. Figure 10 shows averages
of model output sampled at sites for which there are reconstructions
compared to the averages of the reconstructed values. Since the different
reconstructions do not cover the same sites, the averages of the model
values at reconstruction sites differ slightly for each dataset. However,
for all datasets, the multi-model relationship between the average cooling
over land and that over the ocean is approximately linear. Figure 10 allows a
comparison between model output and reconstructions averaged over land and
over oceans, as well as a comparison of the ratio of the land cooling over
the ocean cooling. Although the Cleator et al. (2020) dataset has a larger
spatial coverage than the Bartlein et al. (2011) dataset, there is no
significant difference between the two datasets for most of the temperature
variables across common grid cells (Fig. 9). However, the new reconstructions
have a reduced range at the warm end, especially between 0 and 40<inline-formula><mml:math id="M115" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
so that for the averages over the tropics, most simulations are recorded
as within or warmer than the land-based reconstructions, while they are
within or colder than the Bartlein et al. (2011) reconstructions (Fig. 10,
left-hand side). The results for the global averages are fairly consistent for both
land-based reconstructions (Fig. 10, right-hand side) but the uncertainty is smaller
for the Cleator et al. (2020) dataset. All in all, there are as many
simulations within the range of globally averaged reconstructed temperatures
of Cleator et al. (2020) as that of Bartlein et al. (2011) but the models
outside this range tend to be on the warm side for the Cleator et al. (2020)
dataset and both on the warm and cold sides for the Bartlein et al. (2011)
dataset.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e2558">LGM–PI mean annual temperature anomaly over land vs. LGM–PI
mean annual temperature anomaly over oceans, averaged over the tropics
(30<inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–30<inline-formula><mml:math id="M117" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, left-hand side) and over the globe (right-hand side). The
model output considered for the averages is taken only on grid points for
which there are reconstructions. The top plots are based on the
reconstructions used to evaluate the PMIP3-CMIP5 models: the Bartlein et al. (2020)
database and the MARGO (2009) SST reconstructions. The bottom plots
are based on the most recent reconstructions: Cleator et al. (2020) for
terrestrial data and Tierney et al. (2020) for the SSTs.</p></caption>
        <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f10.png"/>

      </fig>

      <p id="d1e2585">The reconstructions of the LGM–Late Holocene SST anomalies provided by
Tierney et al. (2020) are colder than the MARGO reconstructions in the
tropics, and although this removes the apparent cold-bias shown by some
simulations, this results in some simulations falling outside the window of
reconstructed SSTs at the warm end. This is even more the case if we compare
the results to the data-assimilated product from Tierney et al. (2020),
which has a global coverage (Fig. 10, left-hand side, bottom line). The results from
this latter dataset contrast the results from other global products,
as shown in Supplement Fig. S3. These other global datasets (Annan and
Hargreaves, 2013; Kurahashi-Nakamura et al.,<?pagebreak page1077?> 2017; GLOMAP2020 from Paul et al.,
2021) are all derived, at least in part, from the MARGO Project Members (2009) dataset,
which might explain their overall consistency with the averages estimated by
MARGO Project Members (2009). We have added the warmest estimate (GLOMAP2020) which includes
uncertainties in Fig. 10 to obtain a more complete view of the available
reconstructions as of 2020, keeping in mind that the authors of the
GLOMAP2020 reconstruction estimate that it could be biased by 0.5 to
1.0 <inline-formula><mml:math id="M118" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in the tropics. The simulated mean annual surface air
temperature decreases over the tropical oceans stand between these two
extremes. This illustrates that model-related uncertainties are comparable
with the uncertainties raising from the multiple approaches taken to
reconstruct both the continental and oceanic temperatures.</p>
      <p id="d1e2597">The ratio for the land–sea difference in changes in mean annual temperature
in the tropics in the PMIP4 simulations is compatible with the ratio
reconstructed from the Bartlein et al. (2011) and MARGO Project Members (2009) datasets.
This is also the case if we consider the more recent reconstructions by
Cleator et al. (2020) and Tierney et al. (2020), although the multi-model
land–sea ratio appears to be smaller than that suggested by the
reconstructions. This is the case for both the tropical and global averages.
However, it would not be compatible with a land–sea contrast based on the
Cleator et al. (2020) dataset and the GLOMAP2020 dataset, even if the warm
bias pointed by its authors is taken into account. We are therefore left
with large uncertainties on the topic of LGM cooling over land and oceans,
from the reconstructions as well as from the models. The uncertainties based
on the ensemble of model results and<?pagebreak page1078?> on the ensemble of continental and
marine reconstructions are actually very similar.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e2602">LGM–PI mean annual temperature anomaly over the northern
extratropics (30–90<inline-formula><mml:math id="M119" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) vs. over the northern tropics
(0–30<inline-formula><mml:math id="M120" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N). The model output considered for the averages is taken
only on grid points for which there are reconstructions. The four panels are
based on the data syntheses of Bartlein et al. (2011) <bold>(a)</bold>, MARGO Project Members
(2009) <bold>(b)</bold>, Cleator et al. (2020) <bold>(c)</bold> and Tierney et al. (2020) <bold>(d–e)</bold>.</p></caption>
        <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f11.png"/>

      </fig>

      <p id="d1e2642">The amplification of temperature changes at high northern latitudes compared
to the tropics is apparent over both the land and the ocean domains,
although the amplification appears to be smaller in the new data syntheses
(Fig. 11), except of the Tierney et al. (2020) data-assimilated product. For
the ocean domain, this could reflect the influence of seasonal production on
the extratropical sites, with indicators being more sensitive to summer
changes or to changes in the seasonal production cycle. Comparisons of the
amplification over land areas with the Bartlein et al. (2011) dataset
suggest that the simulated tropical cooling is too large in the PMIP3-CMIP5
simulations, whereas the extratropical cooling was both larger and smaller
than that suggested by the reconstructions in both ensembles. Simulated tropical
temperatures are more consistent with or warmer than the Cleator et al. (2020)
reconstructions, suggesting that the apparent overestimation of
tropical cooling in the PMIP3-CMIP5 simulations over land may reflect the
paucity of tropical data points in Bartlein et al. (2011). However, the
discrepancies between the simulated and reconstructed extratropical land
temperatures are still present: there are several PMIP3 and PMIP4
simulations that are much colder than the reconstructions and many which
are warmer than the reconstructions. Although polar amplification is more
muted over the ocean domain, the comparisons show a similar picture to the
land-based comparisons. Simulated tropical ocean temperatures are more
compatible with the Tierney et al. (2020) than the MARGO Project Members (2009) synthesis.
Simulated extratropical temperature changes in the PMIP3-CMIP5 ensemble mean are
considerably colder than those shown by either of these syntheses, but most tend
to be on the warm side of the Tierney et al. (2020) data-assimilated
product.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e2648">Data–model comparisons for North America (20–50<inline-formula><mml:math id="M121" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
140–60<inline-formula><mml:math id="M122" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), the North Atlantic Ocean (30–50<inline-formula><mml:math id="M123" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
60–10<inline-formula><mml:math id="M124" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), western Europe (35–70<inline-formula><mml:math id="M125" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N,
10<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–30<inline-formula><mml:math id="M127" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), extratropical Asia (35–75<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N),
tropical Americas (30<inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–30<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 120–60<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W),
Africa (35<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–35<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 10<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W–50<inline-formula><mml:math id="M135" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)
and tropical oceans (30<inline-formula><mml:math id="M136" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S–30<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N). MTCO: mean
temperature of the coldest month, MTWA: mean temperature of the warmest
month, MAT: mean annual temperature, MAP: mean annual precipitation,
MATocean: mean annual temperature over the oceans. The error bars for the
reconstructions are based on the standard error given at each site: the
average and associated standard deviation over the specific area are
obtained by computing 10 000 times the average of randomly drawn values in
the Gaussian distributions defined at each site by the reconstruction mean
and standard error, taken as the standard deviation of the Gaussian.
Uncertainty for the model results has been computed based on the 10 000
randomly picked groups of 50 years which were averaged to obtain 10 000
estimates of the 50-year average for a specific region and variable. These
were so small that they do not appear on the plots.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f12.png"/>

      </fig>

      <p id="d1e2812">The LGM climate is characterised by an increase in temperature seasonality
in extratropical regions, with larger changes in winter than in summer
(Izumi et al., 2013). This is confirmed by the Cleator et al. (2020)
reconstructions. In general, this change in seasonality is reproduced by the
models, although the ranges of PMIP4 results for winter are less distinct
from their summer counterparts than for the PMIP3 models. The multi-model
average seasonality is, however, increased for both ensembles. The simulated
cooling in winter temperature is smaller than that indicated by the Bartlein et al. (2011)
reconstructions (Fig. 12, top line). This is not the case
compared to the Cleator et al. (2020) reconstructions, with which more
models are in agreement, except for western Europe, which remains a region of
model–data discrepancy. The magnitude of the summer cooling is more
consistent between the PMIP4 simulations and the Cleator et al. (2020)
reconstructions than between the PMIP3 simulations and the Bartlein et al. (2011)
reconstructions in North America,<?pagebreak page1079?> Europe and extratropical Eurasia.
Finally, the North Atlantic mean annual cooling simulated by the PMIP4
models spans a larger range that of the PMIP3 ensemble. While the PMIP3 ensemble mean
showed temperatures within or above the reconstructed ranges from all
oceanic datasets, the PMIP4 ensemble average stands within the range of the
reconstructions, with six individual models being within this range, four above and three below. It is therefore quite difficult to determine the cause of the
discrepancy in western Europe winter temperatures, which was previously
assigned to an underestimation of the North Atlantic cooling. Some of the
PMIP4 simulations are in fact much colder over both the North Atlantic and
western Europe, and could be studied to further disentangle this model–data
disagreement.</p>
      <p id="d1e2815">Regional changes in the tropics (Fig. 12, bottom line) are more muted than
those in the northern extratropics, and seasonality differences are small.
We therefore base our comparisons on the mean annual temperature and mean
annual precipitation. Both PMIP3 and PMIP4 multi-model averages
underestimate MAT cooling over tropical America, which is consistent for
both reconstructions. More PMIP4 results stand within the reconstructed
range over tropical America. Over tropical Africa, the PMIP3 models were
broadly consistent with the Barltein et al. (2011) reconstructed MAP anomaly
but underestimate this cooling if we refer to the more recent Cleator et
al. (2020) reconstructions. This is also the case for the PMIP4 models, but four
simulations (IPSLCM5A2 and the three HadCM3 simulations) are now within the
reconstructed range. This is probably related to the simulated tropical SSTs
being colder in these simulations. The reconstructed changes in tropical
precipitation over America are larger in the Cleator et al. (2020) dataset
than in Bartlein et al. (2011), and both PMIP3 and PMIP4 models underestimate
the reconstructed drying (Fig. 12). The PMIP4 models, however, all simulate
the correct negative sign of the reconstructed precipitation change. There
is a large difference between the estimates of precipitation change given by
the Bartlein et al. (2011) and the Cleator et al. (2019) datasets for
tropical Africa, with the Cleator et al. (2020) reconstructions reducing the
drying reconstructed by Bartlein et al. (2011). The ranges of PMIP3 and
PMIP4 results are broadly similar over this region, and there are the same
number of models (four) within the reconstructed range of Cleator et al. (2020),
while no model result was compatible with the Bartlein et al. (2011)
reconstructions. All other models underestimate the change or even simulate
an increase in precipitation. All in all, the simulated changes in
precipitation are therefore more consistent with the newer dataset. Thus,
there is no systematic improvement in the<?pagebreak page1080?> simulation of tropical climates
between the PMIP4 and PMIP3 ensembles.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e2820">Relationships between global mean temperature changes (<inline-formula><mml:math id="M138" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis,
average computed on all model points) and global mean temperature changes
for grid points where there are reconstructions (<inline-formula><mml:math id="M139" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis, one plot per
dataset). For each plot/dataset, the models whose average falls in the range of
the average of the reconstructions are marked by vertical dotted lines down
to the <inline-formula><mml:math id="M140" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis.</p></caption>
        <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/1065/2021/cp-17-1065-2021-f13.png"/>

      </fig>

      <p id="d1e2850">The six data syntheses can be used to try and constrain the global MAT
change from LGM to PI. There is a good correlation between the change in
global average MAT over the reconstruction grid points and computed taking
all the model grid points into account (Fig. 13). The idea here is therefore
to take advantage of this relationship to obtain a range in the global MAT
anomaly from the reconstructions. There are models with results below, within
and above<?pagebreak page1081?> the average of all of the reconstructions, except MARGO Project Members (2009) and
GLOMAP2020, for which no model simulates MAT LGM–PI anomalies above the
reconstructed range of values. Retaining only the models which produce
changes in MAT consistent with the reconstructions (and reconstruction
uncertainty), the globally averaged change in MAT is between <inline-formula><mml:math id="M141" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>5.7 and
<inline-formula><mml:math id="M142" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7 <inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C using the Bartlein et al. (2011), between <inline-formula><mml:math id="M144" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.7 and
<inline-formula><mml:math id="M145" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.6 <inline-formula><mml:math id="M146" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C using the Cleator et al. (2020) datasets, between <inline-formula><mml:math id="M147" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.7
and <inline-formula><mml:math id="M148" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.3 <inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the Tierney et al. (2020) dataset and above
<inline-formula><mml:math id="M150" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.9 and <inline-formula><mml:math id="M151" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.4 <inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the MARGO Project Members (2009) and GLOMAP2020
datasets, respectively. Taken altogether, these estimates span a larger range than previous estimates, which indicate changes in MAT of between 4 and
6 <inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Annan and Hargreaves, 2015; Friedrich et al., 2016).</p>
</sec>
<?pagebreak page1082?><sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions and perspectives</title>
      <p id="d1e2965">The results from the PMIP4 models differ from those of the PMIP3 ensemble in
several ways. The multi-model global cooling is similar in both ensembles
but the PMIP4 ensemble range is larger, with four simulations showing colder
results than the coldest PMIP3 model. This feature mainly arises from the
Southern Hemisphere extratropics, and it is currently difficult to
disentangle whether it is due to the PMIP4 model ensemble being largely
different from the PMIP3 ensemble or  the changes in protocol from PMIP3
to PMIP4 (see also Zhu et al., 2021). The change in the ice sheets appears
to have an impact on atmospheric circulation over North America and the
North Atlantic. The AMOC increases less in the PMIP4 than in the PMIP3
simulations, and the depth of the NADW cell remains more stable, except for
two models, in contrast with more than half the models of the PMIP3-CMIP5
ensemble, which simulated a large deepening of this cell. This could be due
to the changes in atmospheric circulation over the North Atlantic, as well
as changes in the North Atlantic freshwater balance. Changes<?pagebreak page1083?> in
precipitation are generally similar for the PMIP3 and PMIP4 ensembles and
characterised by less precipitation overall. Reduced evaporation due to
colder temperatures partially compensates for the reduction in
precipitation, so that areas of negative and significant LGM–PI anomalies
in net precipitation (i.e. precipitation minus evaporation) are larger than
areas with positive LGM–PI precipitation anomalies. However, both
precipitation and net precipitation changes show large spatial
heterogeneity and different regional-scale patterns of change between the
PMIP4 and PMIP3 ensembles, which appears to be related to the performance of
the model ensemble for PI. Additional sensitivity experiments are needed to
separate the effects of changes in model configuration and sensitivity on
general circulation features, such as the position of the jet streams, from
the effects of differences in boundary conditions, such as the improved
realism of the ice-sheet configuration.</p>
      <p id="d1e2968">The PMIP4-CMIP6 ensemble confirms that the models simulate large-scale
thermodynamic behaviour common to historical and future simulations, such as
land–sea contrast and polar amplification. The results from PMIP3 and
PMIP4 align on the same relationships for these large-scale characteristics
of climate change. The new reconstructions of Tierney et al. (2020) and
Cleator et al. (2020) are in<?pagebreak page1084?> better agreement than with the reconstructions
from Bartlein et al. (2011) and MARGO Project Members (2009) used to evaluate these features
previously (Braconnot et al., 2012; Izumi et al., 2013; Harrison et al.,
2014, 2015) for the tropical and global averages. However, global
reconstructions of the surface ocean temperatures, such as the Tierney et al. (2020)
data-assimilated product, the GLOMAP2020 data by Paul et al. (2021) and the reconstructions by Annan and Hargreaves (2013) and
Kurahashi-Nakamura et al. (2017), show a wide range of results in terms of
tropical temperatures (from <inline-formula><mml:math id="M154" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1 to <inline-formula><mml:math id="M155" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4 <inline-formula><mml:math id="M156" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C), which prevents firm
conclusions on the model–data comparisons based on such global
reconstructions. Interestingly, evaluating the uncertainty on tropical
cooling from the PMIP model ensemble on the one hand and from the
ensemble of continental and marine reconstructions on the other yields very
similar results.</p>
      <p id="d1e2994">The simulated global change in MAT averaged over all the grid cells where
reconstructions are available is well correlated with the global average on
all model grid points, providing a constraint on the value of the global LGM
cooling compared to PI. Using the terrestrial datasets as a constraint
indicates a global cooling between <inline-formula><mml:math id="M157" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6.7 and <inline-formula><mml:math id="M158" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.7 <inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, while using
Tierney et al. (2020) as a constraint indicates a global cooling of <inline-formula><mml:math id="M160" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.9 to
<inline-formula><mml:math id="M161" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.2 <inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and using the MARGO Project Members (2009) and GLOMAP2020 datasets
constrains the global average to be above <inline-formula><mml:math id="M163" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.9 and
<inline-formula><mml:math id="M164" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>4.4 <inline-formula><mml:math id="M165" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, respectively. The constrained range (<inline-formula><mml:math id="M166" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>6.7 to
<inline-formula><mml:math id="M167" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>3.2 <inline-formula><mml:math id="M168" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) is larger than previous estimates (<inline-formula><mml:math id="M169" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>4 to <inline-formula><mml:math id="M170" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>6 <inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C).</p>
      <p id="d1e3114">There is no obvious improvement in model performance at a regional scale
between the PMIP3 and PMIP4 ensembles. In some cases (e.g. summer temperature
over western Europe and extratropical Asia), the PMIP4 ensemble demonstrates
a better ability to capture the changes depicted by the reconstructions; in
some others (e.g. winter temperatures over Europe, mean annual precipitation
over tropical America), the PMIP4 ensemble is still far from the
reconstructed values.</p>
      <p id="d1e3118">Our analyses present a first picture of the PMIP4 LGM experiments. Results
from CMIP6 models with high climate sensitivity have only recently become
available (Zhu et al., 2021) and will need to be considered in a full
assessment of the PMIP4-CMIP6 simulations. Sensitivity experiments, for
example, to different ice-sheet configurations, are needed to disentangle the
impact of model improvements from those related to using more realistic
boundary conditions. Additional planned simulations will also help to
disentangle the impacts of changes in vegetation and aerosol loading on the
LGM climate. A more systematic evaluation of the simulated climates, using a
wider range of paleoenvironmental data, will be helpful in understanding
why there are persistent mismatches between the simulations and
reconstructions at a regional scale. Nevertheless, this preliminary analysis
demonstrates the utility of the PMIP4-CMIP6 simulations in addressing
questions about the response of climate to large changes in forcing and
illustrates the need to investigate the causes of inter-model differences in
these responses.</p>
</sec>

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

      <p id="d1e3125">The data shown in this paper can be found on the IPSL repository (<ext-link xlink:href="https://doi.org/10.14768/de241ea7-4c3d-4b56-8140-5de6940903be" ext-link-type="DOI">10.14768/de241ea7-4c3d-4b56-8140-5de6940903be</ext-link>, Kageyama, 2021.). The results from the PMIP3-CMIP5 and PMIP4-CMIP6
models can be found on the ESGF (Earth System Grid Federation) website. In particular, the CMIP6 <italic>lgm</italic> runs have the associated DOIs:
AWI-ESM-1-1-LR: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.9330" ext-link-type="DOI">10.22033/ESGF/CMIP6.9330</ext-link> (last access: February 2020, Shi et al., 2020);
INM-CM4-8: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.5075" ext-link-type="DOI">10.22033/ESGF/CMIP6.5075</ext-link>  (last access: August 2019, Volodin et al., 2019a);
MIROC-ES2L: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.5644" ext-link-type="DOI">10.22033/ESGF/CMIP6.5644</ext-link> (last access: June 2019, Ohgaito et al., 2019);
MPI-ESM1-2-LR: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.6642" ext-link-type="DOI">10.22033/ESGF/CMIP6.6642</ext-link> (last access: July 2019, Jungclaus et al., 2019).
The associated <italic>piControl</italic> simulations have the following DOIs:
AWI-ESM-1-1-LR: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.9335" ext-link-type="DOI">10.22033/ESGF/CMIP6.9335</ext-link>  (last access: February 2020, Danek et al., 2020);
INM-CM4-8: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.5080" ext-link-type="DOI">10.22033/ESGF/CMIP6.5080</ext-link> (last access: June 2019, Volodin et al., 2019b);
MIROC-ES2L: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.5710" ext-link-type="DOI">10.22033/ESGF/CMIP6.5710</ext-link> (last access: August 2019, Hajima et al., 2019);
MPI-ESM1-2-LR: <ext-link xlink:href="https://doi.org/10.22033/ESGF/CMIP6.6675" ext-link-type="DOI">10.22033/ESGF/CMIP6.6675</ext-link>  (last access: July 2019, Wieners et al., 2019).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3162">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/cp-17-1065-2021-supplement" xlink:title="pdf">https://doi.org/10.5194/cp-17-1065-2021-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3171">MK, MLK, UM, SST, TV, AAO, NB, DC, LJG, RFI, KI, ALG, FL, GL, PAM, RO, WRP,
CJP, AQ, DMR, XS, PJV, EV and JZ provided the model output presented in this
paper. SPH, AP and JET provided new climatic reconstructions. MK, SPH,
MLK, ML, JML, SST, TV and AP prepared the figures and wrote the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3177">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e3183">This article is part of the special issue “Paleoclimate Modelling
Intercomparison Project phase 4 (PMIP4) (CP/GMD inter-journal SI)”. It is not
associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3189">The authors would like to thank all the modelling groups who provided the
PMIP3 and PMIP4 output for this analysis, WCRP, CMIP panel, PCMDI, ESGF
infrastructures for sharing data, WCRP and CLIVAR for supporting the PMIP
project. Masa Kageyama acknowledges the use of the IPSL (ESPRI – Ensemble de
Services Pour la Recherche l'IPSL – computing and data centre
(<uri>https://mesocentre.ipsl.fr/</uri>, last access: April 2021) which is supported by CNRS, Sorbonne
Université, Ecole Polytechnique, CNES and through national and
international grants) and LSCE storage and computing facilities for the
analyses presented in this paper. The IPSL model was run on the
Très Grande Infrastructure de Calcul (TGCC) at Commissariat à
l'Energie Atomique (gen2212 project). Xiaoxu Shi and Gerrit Lohmann acknowledge<?pagebreak page1085?> the German
Climate Computing Center (DKRZ) for the AWI-ESM simulations. We thank the
two reviewers and editor for their helpful comments on the first version of
the manuscript.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3197">Masa Kageyama is funded by CNRS. Sandy P. Harrison acknowledges funding from the ERC-funded
project GC2.0 (Global Change 2.0: Unlocking the past for a clearer future;
grant no. 694481). The MPI-M contribution was supported by the German
Federal Ministry of Education and Research (BMBF) as a Research for
Sustainability initiative (FONA) through the project PalMod (FKZ:
grant no. 01LP1504C). Jessica E. Tierney acknowledges funding from the US National Science Foundation
(grant no. AGS-1602301) and the Heising-Simons Foundation (grant no. 2016-015). Ruza F. Ivanovic
acknowledges partial support from the UK Natural Environment Research
Council (grant no. NE/K008536/1) and additionally from UK Research and Innovation
(grant no. MR/S016961/1), who also support Lauren J. Gregoire. Christopher J. Poulsen acknowledges funding from the
US National Science Foundation (AGS-2002397) and the Heising-Simons
Foundation (grant no. 2016-012). Xiaoxu Shi and Gerrit Lohmann acknowledge the support of the PACMEDY
and PALMOD2 projects. Ayako Abe-Ouchi acknowledges the financial support
from JSPS KAKENHI (grant no. 17H06104) and MEXT KAKENHI (grant no. 17H06323).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3203">This paper was edited by Julien Emile-Geay and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>The PMIP4 Last Glacial Maximum experiments: preliminary results and comparison with the PMIP3 simulations</article-title-html>
<abstract-html><p>The Last Glacial Maximum (LGM,  ∼ &thinsp;21&thinsp;000 years ago)
has been a major focus for evaluating how well state-of-the-art climate
models simulate climate changes as large as those expected in the future
using paleoclimate reconstructions. A new generation of climate models has
been used to generate LGM simulations as part of the Paleoclimate Modelling
Intercomparison Project (PMIP) contribution to the Coupled Model
Intercomparison Project (CMIP). Here, we provide a preliminary analysis and
evaluation of the results of these LGM experiments (PMIP4, most of which are PMIP4-CMIP6) and compare them with the previous generation of simulations
(PMIP3, most of which are PMIP3-CMIP5). We show that the global averages of the
PMIP4 simulations span a larger range in terms of mean annual surface air
temperature and mean annual precipitation compared to the PMIP3-CMIP5
simulations, with some PMIP4 simulations reaching a globally colder and
drier state. However, the multi-model global cooling average is similar for
the PMIP4 and PMIP3 ensembles, while the multi-model PMIP4 mean annual
precipitation average is drier than the PMIP3 one. There are important
differences in both atmospheric and oceanic circulations between the two
sets of experiments, with the northern and southern jet streams being more
poleward and the changes in the Atlantic Meridional Overturning Circulation
being less pronounced in the PMIP4-CMIP6 simulations than in the PMIP3-CMIP5
simulations. Changes in simulated precipitation patterns are influenced by
both temperature and circulation changes. Differences in simulated climate
between individual models remain large. Therefore, although there are
differences in the average behaviour across the two ensembles, the new
simulation results are not fundamentally different from the PMIP3-CMIP5
results. Evaluation of large-scale climate features, such as land–sea
contrast and polar amplification, confirms that the models capture these
well and within the uncertainty of the paleoclimate reconstructions.
Nevertheless, regional climate changes are less well simulated: the models
underestimate extratropical cooling, particularly in winter, and
precipitation changes. These results point to the utility of using
paleoclimate simulations to understand the mechanisms of climate change and
evaluate model performance.</p></abstract-html>
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