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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-17-721-2021</article-id><title-group><article-title>Technical note: Considerations on using uncertain proxies in the
analogue method for spatiotemporal reconstructions of millennial-scale
climate</article-title><alt-title>Analogue reconstructions on millennial timescales</alt-title>
      </title-group><?xmltex \runningtitle{Analogue reconstructions on millennial timescales}?><?xmltex \runningauthor{O. Bothe and E. Zorita}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Bothe</surname><given-names>Oliver</given-names></name>
          <email>ol.bothe@gmail.com</email>
        <ext-link>https://orcid.org/0000-0002-6257-8786</ext-link></contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Zorita</surname><given-names>Eduardo</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7264-5743</ext-link></contrib>
        <aff id="aff1"><institution>Institute of Coastal Systems – Analysis and Modeling, Helmholtz Zentrum Geesthacht, 21502 Geesthacht, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Oliver Bothe (ol.bothe@gmail.com)</corresp></author-notes><pub-date><day>29</day><month>March</month><year>2021</year></pub-date>
      
      <volume>17</volume>
      <issue>2</issue>
      <fpage>721</fpage><lpage>751</lpage>
      <history>
        <date date-type="received"><day>30</day><month>December</month><year>2019</year></date>
           <date date-type="rev-request"><day>16</day><month>January</month><year>2020</year></date>
           <date date-type="rev-recd"><day>11</day><month>January</month><year>2021</year></date>
           <date date-type="accepted"><day>18</day><month>February</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Oliver Bothe</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/17/721/2021/cp-17-721-2021.html">This article is available from https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021.html</self-uri><self-uri xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021.pdf">The full text article is available as a PDF file from https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e87">Inferences about climate states and climate variability of the Holocene
and the deglaciation rely on sparse paleo-observational proxy data.
Combining these proxies with output from climate simulations is a means
for increasing the understanding of the climate throughout the last tens
of thousands of years. The analogue method is one approach to do this.
The method takes a number of sparse proxy records and then searches
within a pool of more complete information (e.g., model simulations) for
analogues according to a similarity criterion. The analogue method is
non-linear and allows considering the spatial covariance among proxy
records.</p>
    <p id="d1e90">Beyond the last two millennia, we have to rely on proxies that are not
only sparse in space but also irregular in time and with considerably
uncertain dating. This poses additional challenges for the analogue
method, which have seldom been addressed previously. The method has to
address the uncertainty of the proxy-inferred variables as well as the
uncertain dating. It has to cope with the irregular and non-synchronous
sampling of different proxies.</p>
    <p id="d1e93">Here, we describe an implementation of the analogue method including a
specific way of addressing these obstacles. We include the uncertainty
in our proxy estimates by using “ellipses of tolerance” for tuples
of individual proxy values and dates. These ellipses are central to our
approach. They describe a region in the plane spanned by proxy dimension
and time dimension for which a model analogue is considered to be
acceptable. They allow us to consider the dating as well as the data
uncertainty. They therefore form the basic criterion for selecting valid
analogues.</p>
    <p id="d1e96">We discuss the benefits and limitations of this approach. The results
highlight the potential of the analogue method to reconstruct the
climate from the deglaciation up to the late Holocene. However, in the
present case, the reconstructions show little variability of their
central estimates but large uncertainty ranges. The reconstruction by
analogue provides not only a regional average record but also allows
assessing the spatial climate field compliant with the used proxy
predictors. These fields reveal that uncertainties are also locally
large. Our results emphasize the ambiguity of reconstructions from
spatially sparse and temporally uncertain, irregularly sampled proxies.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e108">It is a pervasive idea in environmental and climate sciences that past
states provide us with information about the future
<xref ref-type="bibr" rid="bib1.bibx84 bib1.bibx54" id="paren.1"/>. Therefore, paleoclimatology aims to
understand past spatial and temporal climate variability, preferentially
using a dynamical understanding of the climate processes. To achieve
this, we need spatial and temporal information about past climate states
and past climate evolutions. Our understanding of the past, however,
relies on spatially and temporally sparse paleo-information. Data
assimilation methods and data-science approaches are ways to provide
estimates for the gaps in time and space. One simple approach is the
analogue method or so-called proxy surrogate reconstructions
<xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx48" id="paren.2"/>. This method is similar to k-nearest-neighbor classification algorithms in machine learning applications.
The present paper discusses an implementation of the analogue
method for<?pagebreak page722?> reconstructing surface temperature over timescales including
the Holocene and the last deglaciation.</p>
      <p id="d1e117">If we want to use the analogue method beyond approximately the last two
millennia, we have to tackle additional challenges, which usually can be
evaded for the Common Era. For example, our proxy records are not only
spatially sparse but they also have a coarse temporal resolution on
these timescales. Furthermore, the sampling generally is irregular for
each individual proxy. Indeed, sample dates differ between proxies on
these timescales, and these dates are also uncertain. Recently,
<xref ref-type="bibr" rid="bib1.bibx48" id="text.3"/> used the approach to reconstruct the climate at
Marine Isotope Stage 3 (MIS3; 24 000 to 59 000 years before present;
24–59 kyr BP) addressing such challenges. Including part of a deglacial
period, as we do here, further complicates applications as we consider a
climate trajectory with strong trends.</p>
      <p id="d1e123">The basic idea of the analogue method is simple. An analogy tries to
explain an item based on the item's resemblance or equivalence to
something else. In the analogue method, one uses a set of sparse
proxies, i.e., predictors, and searches for analogues for them in a pool
of candidates that are spatially more complete. In paleoclimatology, the
predictors can be local proxy records and the candidate analogues can be
fields from climate model simulations. One assesses the similarity of
the simulation output and the proxy records at the proxy locations to
find valid analogues. The reconstructed field is then the complete field
given by the analogue.</p>
      <p id="d1e126">It is important to note that comparable approaches suffer from a
trade-off between accuracy and reliability of reconstructions, as shown
by <xref ref-type="bibr" rid="bib1.bibx2" id="text.4"/> for a particle filter method. This depends on
quality and quantity of the available proxy records. This drawback also
affects the analogue method, as shown by <xref ref-type="bibr" rid="bib1.bibx36" id="text.5"/> and
<xref ref-type="bibr" rid="bib1.bibx41" id="text.6"/>, who find that the skill
accumulates at the predictor locations. Similarly, <xref ref-type="bibr" rid="bib1.bibx93" id="text.7"/>
highlight that the analogue method may perform badly in regions with
little proxy coverage.</p>
      <p id="d1e142">Most paleoclimate applications of the analogue method focused on the
Common Era of the last 2000 years
<xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx103 bib1.bibx41 bib1.bibx42 bib1.bibx93 bib1.bibx72" id="paren.8"><named-content content-type="pre">e.g.,</named-content></xref>.
In this context, <xref ref-type="bibr" rid="bib1.bibx43" id="text.9"/> call the results of the
analogue method a “proxy surrogate reconstruction”.
<xref ref-type="bibr" rid="bib1.bibx42" id="text.10"/> provide a comparison of the analogue approach
to more complex common data assimilation techniques. Applications often
only consider the single best analogue, which may not necessarily be
appropriate especially for predictors affected by uncertainty.
Paleo-applications of the analogue method generally try to upscale the
local proxy information but the analogue method was also applied for
downscaling of large-scale information
<xref ref-type="bibr" rid="bib1.bibx110" id="paren.11"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p id="d1e161">Here, we describe another approach to obtain reconstructions by analogue
over millennial timescales based on spatially and temporally sparse and
uncertain proxies. It differs in some aspects from the approach so far
applied to shorter and more recent periods. Our approach tries to
explicitly consider not only age uncertainties
<xref ref-type="bibr" rid="bib1.bibx48" id="paren.12"><named-content content-type="pre">compare with</named-content></xref> but also the uncertainties of the
proxy values or, similarly, of the temperature reconstructions inferred
from these proxies. We make specific assumptions on the uncertainty of
the data and the dates of the proxy predictors. We further account for
the temporal irregularity of the sampling of different predictors. As
explained in more detail later, our approach considers an analogue
candidate simulation field as a valid analogue if it complies with our
assumptions on the uncertainty of the proxy predictors. We apply the
method over time periods encompassing parts of the last deglaciation
until the late 20th century of the Common Era (CE). That is, we try to
apply the analogue method over a period when the climate cannot validly
be described as stationary at local, regional, and global spatial
scales.</p>
      <p id="d1e169">Beyond the mentioned challenges for analogue reconstructions on
millennial timescales, the method is also constrained by the pool of
available analogue fields. <xref ref-type="bibr" rid="bib1.bibx104" id="text.13"/> considers how likely
it is to observe two atmospheric flows over the Northern Hemisphere that
resemble each other within the observational uncertainty. The study
finds that a pool would have to include a nonillion, i.e., <inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">30</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>,
potential analogues to achieve this. Obviously, we aim for less
accuracy in paleoclimatology due to larger uncertainties. However, there
are still only few climate simulations for relevant timescales, and
these simulations also cover only parts of the time periods of interest.
Furthermore, these simulations stem from different climate models whose
reliability on these timescales may not have been shown yet
<xref ref-type="bibr" rid="bib1.bibx108 bib1.bibx54" id="paren.14"/>.</p>
      <p id="d1e189">The next section first summarizes again the main characteristics of
analogue searches for paleo-reconstructions. Afterwards, we present our
way of dealing with uncertain tuples of data and date, that is,
describing ranges of tolerance for which we choose analogues. Simulation
fields are considered analogues if they fall within these tolerance
ranges at all considered proxy locations. We also describe how we
consider the fact that different proxies are sampled at different times.
The section also presents our selection of a simulation pool. We present
results for a multimillennial period for a pseudo-proxy setup
<xref ref-type="bibr" rid="bib1.bibx88" id="paren.15"><named-content content-type="pre">compare</named-content></xref> and a realistic setup for the
European–North Atlantic sector. We also shortly describe results for
alternative proxy setups. Finally, we discuss our assumptions and
results. We aim to emphasize the opportunities of the analogue method
while also highlighting its challenges.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Analogue method, assumptions, and data</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>General method</title>
      <p id="d1e212">In an analogue search, one tries to complement incomplete information
from one dataset by data from other more<?pagebreak page723?> complete datasets. One ranks
the more complete data by their similarity to the available information in
the first dataset. In paleoclimatology, this usually means that one uses
a set of spatially sparse proxy records and wants to find fields from
simulations or reanalyses that are most analogous to the proxy records
at their locations. The pool of candidate fields depends on the
available simulations and reanalyses.</p>
      <p id="d1e215">If, for example, one uses proxies for temperature, such a ranking may
simply provide the simulated temperature field that has the smallest
Euclidean distance to the sparse proxy information at their locations.
Alternatively, one can consider not just one but a small number of good
analogues with small distances
<xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx41 bib1.bibx42 bib1.bibx93" id="paren.16"/>.
However, it is also possible to define a range of tolerable deviations
from the proxy predictor values and consider all analogue candidates
that are within this range as valid analogues
<xref ref-type="bibr" rid="bib1.bibx6" id="paren.17"><named-content content-type="pre">compare</named-content></xref>. <xref ref-type="bibr" rid="bib1.bibx68" id="text.18"/> discuss the effect of
the choice of similarity measures for a different application.</p>
      <p id="d1e229">An important aspect of a paleoclimate reconstructions is the uncertainty
of the reconstructed data. To our knowledge, only <xref ref-type="bibr" rid="bib1.bibx48" id="text.19"/> and
<xref ref-type="bibr" rid="bib1.bibx72" id="text.20"/> consider the uncertainty of the final reconstruction
among earlier paleo-applications of the analogue method, and only
<xref ref-type="bibr" rid="bib1.bibx48" id="text.21"/> use proxies with prominent age uncertainties in
their work on MIS3. They perform multiple reconstructions to obtain
reconstruction uncertainties by shifting the dates of their proxies
within the stated age uncertainties. Uncertainty information is
particularly relevant for applications like the one of
<xref ref-type="bibr" rid="bib1.bibx48" id="text.22"/>, where one has to deal with predictors that are
sparse, irregular, and uncertainly dated.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Present application of the analogue method</title>
      <p id="d1e252">We use spatially and temporally sparse proxies, affected by
uncertainties in their values and their dating for analogue searches on
millennial timescales. Next, we detail our simplifying assumptions about
what the data represent, their uncertainties, and the dating
uncertainties. We also describe how we choose the dates for which we
perform the climate reconstruction.</p>
<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Variable of interest</title>
      <p id="d1e262">Our interest is in temperature. Specifically, we concentrate on means of
seasonal or annual temperature at the surface. We consider proxies for
which the literature previously reports a sensitivity to temperature in
the form of a calibration relation. We search for analogues within fields of
simulated surface temperature. To do the comparison, we consider the
model variable “surface temperature” over the European–North Atlantic
domain shown in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. The reconstruction also uses these
fields.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e269">Map of the reconstruction domain and the proxy
predictors: for the pseudo-proxy setup (blue), experiment P01, and for
the main proxy setup (red), experiment E01. Please note the small
offset between the proxy locations and their pseudo-proxy counterparts on
the discrete model grid.</p></caption>
            <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f01.png"/>

          </fig>

      <p id="d1e278">Theoretically, the variable or variables to be reconstructed can be
different from the variable or multiple variables represented by the
paleo-observational predictors. Indeed, we here assume that it is
possible to reconstruct annual temperatures from proxy records with
diverse seasonal attributions.</p>
      <p id="d1e282">Using temperature in a multi-proxy comparison requires a number of
assumptions. First, we assume that the proxy recorders indeed were
temperature sensitive. More importantly, here, we assume that all the
different recorders, aquatic or otherwise, represent temperature at the
surface. This is an assumption of convenience in view of potential
habitat biases of the proxy records
<xref ref-type="bibr" rid="bib1.bibx95 bib1.bibx99 bib1.bibx51 bib1.bibx52 bib1.bibx76 bib1.bibx100 bib1.bibx26 bib1.bibx77 bib1.bibx59 bib1.bibx60 bib1.bibx65 bib1.bibx101" id="paren.23"/>.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <label>2.2.2</label><title>Data handling and use of model simulation pool</title>
      <p id="d1e296">Section <xref ref-type="sec" rid="Ch1.S2.SS3.SSS1"/> gives details on our selected proxies. In short,
we choose 17 proxies at locations in the European–North Atlantic sector
(Fig. <xref ref-type="fig" rid="Ch1.F1"/>) from the compilation of <xref ref-type="bibr" rid="bib1.bibx67" id="text.24"/>.
These are from a variety of different proxy systems. We take these as
published by either <xref ref-type="bibr" rid="bib1.bibx67" id="text.25"/> or the original publications.
Therefore, calibrations and uncertainty estimates have diverse origins.
Considering the proxy ages and their uncertainties, we adopt those as
published.</p>
      <p id="d1e309">Optimally, one would aim for maximal consistency in the comparison.
Consistency among parameters and calibration ensures a relation among
the proxy predictors, which, one can assume, increases the chance that
the proxy records lead to a selection of physically meaningful
analogues. In this case, the proxies can effectively anchor the analogue
selection. We here assume that all chosen proxy types reliably<?pagebreak page724?> represent
the target of interest and a multi-proxy approach is viable.</p>
      <p id="d1e312">The analogue method allows searching for analogues at dates when there
is information. One can pool the predictor dates into consistent
intervals of, for example, 500 years, and search for analogues for these
500-year pools. One can follow the example of <xref ref-type="bibr" rid="bib1.bibx48" id="text.26"/> and
interpolate the proxy records to consistent time steps using the age
models for the individual records. We choose here a different approach;
we identify all the years for which at least one of the chosen proxy
records includes a dated value. We perform analogue searches for these
dates according to our considerations on uncertainty, which we describe
in the following (Sect. <xref ref-type="sec" rid="Ch1.S2.SS2.SSS3"/>).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e324">Information about the considered
proxy records: IDs, geographical location, seasonal attribution according to
<xref ref-type="bibr" rid="bib1.bibx67" id="text.27"/>, proxy type, seasonal attribution used here, and analogue
search setups that use the record. All proxy data are from the Supplement of
<xref ref-type="bibr" rid="bib1.bibx67" id="text.28"/>. Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/> provides references to original
publications and datasets. Proxy setups refer to those analogue search tests
where this proxy is included (compare also Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="7">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Proxy ID</oasis:entry>
         <oasis:entry colname="col2">Lat</oasis:entry>
         <oasis:entry colname="col3">Long</oasis:entry>
         <oasis:entry colname="col4">Season in</oasis:entry>
         <oasis:entry colname="col5">Proxy type</oasis:entry>
         <oasis:entry colname="col6">Season</oasis:entry>
         <oasis:entry colname="col7">Proxy</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">
                      <xref ref-type="bibr" rid="bib1.bibx67" id="text.29"/>
                    </oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">used</oasis:entry>
         <oasis:entry colname="col7">setups</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2043</oasis:entry>
         <oasis:entry colname="col2">36.1</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M2" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>2.6</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M3" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–3, 4–6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">M39-008</oasis:entry>
         <oasis:entry colname="col2">36.4</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M4" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.1</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–2, 4–7, 9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2011</oasis:entry>
         <oasis:entry colname="col2">67</oasis:entry>
         <oasis:entry colname="col3">7.6</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M6" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1–4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ODP984</oasis:entry>
         <oasis:entry colname="col2">61.4</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M7" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>24.1</oasis:entry>
         <oasis:entry colname="col4">Winter</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M8" 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> (<italic>N. pachyderma d.</italic>)</oasis:entry>
         <oasis:entry colname="col6">Winter</oasis:entry>
         <oasis:entry colname="col7">1, 7–9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GeoB 7702-3</oasis:entry>
         <oasis:entry colname="col2">31.7</oasis:entry>
         <oasis:entry colname="col3">34.1</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5">TEX86</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 5–9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IOW225517</oasis:entry>
         <oasis:entry colname="col2">57.7</oasis:entry>
         <oasis:entry colname="col3">7.1</oasis:entry>
         <oasis:entry colname="col4">Spring to winter</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–4, 6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IOW225514</oasis:entry>
         <oasis:entry colname="col2">57.8</oasis:entry>
         <oasis:entry colname="col3">8.7</oasis:entry>
         <oasis:entry colname="col4">Spring to winter</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">M25/4-KL11</oasis:entry>
         <oasis:entry colname="col2">36.7</oasis:entry>
         <oasis:entry colname="col3">17.7</oasis:entry>
         <oasis:entry colname="col4">Spring to winter</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–7</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">AD91-17</oasis:entry>
         <oasis:entry colname="col2">40.9</oasis:entry>
         <oasis:entry colname="col3">18.6</oasis:entry>
         <oasis:entry colname="col4">Annual (seasonal bias likely)</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–6</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake 850</oasis:entry>
         <oasis:entry colname="col2">68.4</oasis:entry>
         <oasis:entry colname="col3">19.2</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5">Chironomid transfer function</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 7–8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake Nujulla</oasis:entry>
         <oasis:entry colname="col2">68.4</oasis:entry>
         <oasis:entry colname="col3">18.7</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5">Chironomid transfer function</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 7–8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2015</oasis:entry>
         <oasis:entry colname="col2">58.8</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M13" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>26</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1–4</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">D13882</oasis:entry>
         <oasis:entry colname="col2">38.6</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M15" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>9.5</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1–6, 8</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GIK23258-2</oasis:entry>
         <oasis:entry colname="col2">75</oasis:entry>
         <oasis:entry colname="col3">14</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5">Foram transfer function</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 4–9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake Flarken</oasis:entry>
         <oasis:entry colname="col2">58.6</oasis:entry>
         <oasis:entry colname="col3">13.7</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5">Pollen MAT</oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">1, 7–9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake Tsuolbmajavri</oasis:entry>
         <oasis:entry colname="col2">68.7</oasis:entry>
         <oasis:entry colname="col3">22.1</oasis:entry>
         <oasis:entry colname="col4">Summer</oasis:entry>
         <oasis:entry colname="col5">Pollen MAT</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 5–9</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">RAPID-12-1K</oasis:entry>
         <oasis:entry colname="col2">62.1</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M17" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>17.8</oasis:entry>
         <oasis:entry colname="col4">Late spring to early summer</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M18" 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> (<italic>G. bulloides</italic>)</oasis:entry>
         <oasis:entry colname="col6">Summer</oasis:entry>
         <oasis:entry colname="col7">1, 6–9</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GeoB 5901-2</oasis:entry>
         <oasis:entry colname="col2">36.4</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M19" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>7.1</oasis:entry>
         <oasis:entry colname="col4">Annual</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6">Annual</oasis:entry>
         <oasis:entry colname="col7">3</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e1085">Each data point of a proxy series potentially represents a time interval
of a specific length, and the comparison should consider this temporal
resolution. That is, if one data point represents a 50-year accumulation
and another data point represents a 500-year accumulation, the procedure
ideally accounts for these differences. We decide to use typical
resolutions instead of individual resolution estimates to simplify the
procedure and allow a computationally more efficient analogue search for
data- and time-uncertain proxies. Indeed, it is not necessarily the case
that a proxy-record publication includes the information to estimate the
pointwise temporal resolution. Considering information provided by
<xref ref-type="bibr" rid="bib1.bibx67" id="text.30"/> on their proxies, we conclude for our chosen subset
of these (compare Table <xref ref-type="table" rid="Ch1.T1"/>) that the proxies have at best
centennial average resolutions. While there are proxies with higher and
lower resolutions, a reasonable estimate for the overall average
resolution is centennial.</p>
      <p id="d1e1093">Therefore, we decide to compare the proxy estimates to 101-year averages
of the model simulation output. That is, we compare them to 101-year
mean values, which we obtain by using a 101-year moving mean on the
simulation output time series that is closest to the proxy location.</p>
      <p id="d1e1096">In one test case, we do not preprocess the simulation output but use the
annually resolved values of the output for the comparison. For this
specific test, we also include the simulation data from the
FAMOUS-HadCM3 simulations for the Quantifying and Understanding the Earth System (QUEST) project
<xref ref-type="bibr" rid="bib1.bibx89" id="paren.31"><named-content content-type="pre">compare</named-content><named-content content-type="post">and Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS2"/></named-content></xref> for which output
data are only representative of decadal forcing conditions. We refer to
these as QUEST FAMOUS simulations. We do two more tests with differing
resolutions that use 51- and 501-year averages, respectively.</p>
      <p id="d1e1107">We test the whole approach by using pseudo-proxies. We construct the
pseudo-proxies following the ensemble approach of <xref ref-type="bibr" rid="bib1.bibx7" id="text.32"/>.
Their approach takes simulated grid-point data and transforms them in
multiple steps into a pseudo-proxy record. The steps follow the framework
of a proxy system model including a sensor model, an archive model, and
an observation model <xref ref-type="bibr" rid="bib1.bibx35" id="paren.33"><named-content content-type="pre">see</named-content></xref>. <xref ref-type="bibr" rid="bib1.bibx7" id="text.34"/>
first add a noise estimate for environmental non-temperature influences
at the sensor stage. This stage also includes adding a bias term due to
changing insolation. Next, the archive stage primarily represents a
smoothing of this record, which is meant to reflect effects of, e.g.,
bioturbation. The measurement stage adds another noise term. After
sampling this record at a specific number of dates, the procedure,
finally, also adds an error term for the proxy data reflecting effective
dating uncertainties. We set this term to zero in the script of
<xref ref-type="bibr" rid="bib1.bibx7" id="text.35"/> because we do not aim to transfer dating
uncertainty to the data uncertainty. Pseudo-proxy locations are
simulation data grid points close to the real proxy locations. Figure <xref ref-type="fig" rid="Ch1.F1"/> shows the 17 pseudo-proxy and proxy locations and allows us to
identify their slight offsets due to the discrete character of the
simulation data. The pseudo-proxy generation smooths each record to mimic
the temporal filtering effects of the real environmental archive. The
smoothing length is randomly chosen but temporally uniform for each
record. The search for analogues again uses 101-year mean estimates from
the simulation pool (compare the paragraph above).</p>
      <p id="d1e1126">Simulations potentially differ in their modern-day climate mean
<xref ref-type="bibr" rid="bib1.bibx109" id="paren.36"><named-content content-type="pre">compare, e.g.,</named-content></xref>. Using anomalies can
circumvent this issue. However, there is not a clear path in our
application towards computing them equivalently in simulations and proxy
data. If such a path exists, one can consider simulation output as
anomalies to the climatology over the 20th century or over the full
simulation period or over the longest period common to all simulations.
For example, <xref ref-type="bibr" rid="bib1.bibx48" id="text.37"/> construct the anomaly record for a data
series by subtracting the temporal mean calculated over the full period
of the record of interest. Their period of interest backs this decision.
The proxy records of <xref ref-type="bibr" rid="bib1.bibx48" id="text.38"/> suggest an overall rather stable
climate in the North Atlantic during Marine Isotope Stage 3, although a
number of Dansgaard–Oeschger (DO) events occurred during this period. We
presume that using anomalies allows us to include a wider range of
simulations and analogue candidates for each date.</p>
      <p id="d1e1141">However, in the present case, the period of interest includes mainly the
last 15 kyr. Thus, it spans part of the deglaciation from the Last
Glacial Maximum to the Holocene optimum. Our selection of simulations
can only piecewise cover that period of interest, which complicates the
construction of a surface temperature candidate pool. Indeed, the most
recent dates differ among the proxy records, and thus there is no
simple procedure to provide anomalies relative to a consistent modern
climate. Additionally, using anomalies may introduce climatic
inconsistencies if we are interested in climate variables other than
temperature. For these reasons, we decide that we cannot reasonably use
anomalies. Instead, we try to find analogues for the local proxy
reconstructions in their absolute temperature units without subtracting
any climatology.</p>
</sec>
<?pagebreak page725?><sec id="Ch1.S2.SS2.SSS3">
  <label>2.2.3</label><title>Proxy uncertainty</title>
      <p id="d1e1152">We are interested in millennial timescales from the last deglaciation
until the recent past. On these timescales, uncertainty affects our
proxy predictors in two ways. First, we have to consider the age or
dating uncertainty. Second, the measured proxy data and the temperatures
inferred from them are affected by various sources of uncertainty
<xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx77 bib1.bibx48" id="paren.39"><named-content content-type="pre">compare, e.g.,</named-content><named-content content-type="post">and their
references</named-content></xref>.</p>
      <p id="d1e1162">Previous applications of the analogue method usually did not consider
proxies with considerable age uncertainties except for
<xref ref-type="bibr" rid="bib1.bibx48" id="text.40"/>. <xref ref-type="bibr" rid="bib1.bibx48" id="text.41"/> consider the age uncertainty
by shifting the date of each proxy by <inline-formula><mml:math id="M21" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>500 years. Thereby, they
obtain an ensemble of <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">2</mml:mn><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> reconstructions from which they
calculate confidence intervals for their final reconstruction. They do
not separately consider the uncertainty of the proxy/reconstruction
value. For details, see <xref ref-type="bibr" rid="bib1.bibx48" id="text.42"/>.</p>
      <p id="d1e1192">Uncertainty of proxies in time and date is commonly expressed as central
value and a given uncertainty range. These ranges may be given as plus
and minus standard deviations around the central value, e.g.,
<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.64</mml:mn></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.58</mml:mn></mml:mrow></mml:math></inline-formula> standard deviation ranges, or as
percentage confidence intervals, e.g., 90 % or 99 % intervals. Such
usage of a percentage view can be extended to pairwise expressions of
the uncertainty. This is central to our approach.</p>
      <p id="d1e1219">That is, we choose a different approach (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) compared
to, e.g., <xref ref-type="bibr" rid="bib1.bibx48" id="text.43"/>. We interpret each data point in a proxy
series together with its dating as a data point in the two dimensional
space spanned by temperature and time. Each proxy data point is located
on this two-dimensional temperature–time plane and each point is
surrounded by uncertainty ranges along both dimensions. We can utilize
the uncertainty ranges in the two dimensions as our
“area of tolerance”, in which the analogue candidate simulation
fields should be located to be considered as good analogues. That is, the
area of tolerance defines our criterion for selection of good and valid
analogues. If a candidate field is within the tolerance areas at all
considered proxy locations, it is thought to be a valid analogue. We can
define tolerance ranges for different levels of pairwise proxy–time
uncertainty. In equivalence to common expressions of uncertainty or
confidence intervals, these can be formulated as pairwise 90 % or 99 %
intervals. These choices of intervals yield increasingly larger areas of
tolerance. For the real proxies, the data uncertainties that enter the
computation of the tolerance area follow our simplifying assumptions
detailed in Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS1"/>, while the dating uncertainties are taken from
the compilation published by <xref ref-type="bibr" rid="bib1.bibx67" id="text.44"/>. For the pseudo-proxy
setup, the pseudo-proxy algorithm of <xref ref-type="bibr" rid="bib1.bibx7" id="text.45"/> provides
estimates for data and dating uncertainty.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1238">Considerations on uncertainty and constructing tolerance envelopes: <bold>(a)</bold> example proxy data (line) and assumed data uncertainty at all dates when we reconstruct values. The number of dates is all dates when any of the proxies included has a dated data point. <bold>(b)</bold> Proxy data at three example dates and tolerance ellipses for these dates using data uncertainty and age/date uncertainty.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f02.png"/>

          </fig>

      <p id="d1e1253">To define these areas of tolerance, we still have to define their shape.
Our interest is in finding analogues that agree<?pagebreak page726?> with the proxy data but
also account for these uncertainties. Then, we could take the
uncertainty estimates of temperature and time to construct a
two-dimensional uniform estimate in the form of a rectangle of tolerance.
Analogue candidates would be valid analogues if they fall locally within
these rectangles. If they fall outside of the rectangle, they would not
be considered valid analogues. Although the uncertainties in temperature
and time are commonly taken to be Gaussian, the rectangular approach is
the best one if we consider the uncertainties of date and temperature
isolated from each other. Then, our tolerance for the temperature data
has the same structure at the border of our temporal tolerance range as
it has at the central estimate for the date. However, in our
application, we do not see both tolerance ranges in isolation. We assume
that our tolerance range is a two-dimensional pairwise construct in time
and temperature. Then, our tolerance construct takes the shape of a
two-dimensional Gaussian. This implies that our tolerance areas are
ellipses. Such ellipses can be computed dependent on an assumed pairwise
confidence level or coverage or in our interpretation tolerance range.
We refer to these as percentage levels.</p>
      <p id="d1e1256">According to our view of tolerance ranges as tolerance ellipses, we
accept fewer analogues for dates far away from the median proxy age
estimate. For these dates, analogue candidates need to be numerically
very close to the proxy. In contrast, we accept more analogues close to
the central age estimate of the proxy and tolerate that they may more
strongly differ from the numerical central estimate of the proxy. We
acknowledge that it may seem counterintuitive that we reduce the range
in data uncertainty at dates far away from our central best estimate of
temperature and date. This originates from our assumption that the pair
of data and date stems from a two-dimensional distribution that is
centered on our best estimate. Thereby, the likelihood of a valid pair of
data and date reduces further away from our best estimate according to
the assumptions on the distribution.</p>
      <p id="d1e1259">As we have estimates of the uncertainties of the data point, we can
construct and visualize the ellipses of tolerance around each data point
under the assumption of two-dimensional Gaussian tolerance areas. We use
the R <xref ref-type="bibr" rid="bib1.bibx75" id="paren.46"/> package ellipse <xref ref-type="bibr" rid="bib1.bibx70" id="paren.47"/> whose default
ellipse function follows <xref ref-type="bibr" rid="bib1.bibx69" id="text.48"/> by implementing the ellipse
equation as
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M25" display="block"><mml:mtable class="split" columnspacing="1em" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mi>y</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mo>=</mml:mo><mml:mo mathsize="1.1em">(</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>+</mml:mo><mml:mi>d</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>-</mml:mo><mml:mi>d</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:mo mathsize="1.1em">)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>
            where <inline-formula><mml:math id="M26" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> is our time dimension and <inline-formula><mml:math id="M27" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> is our temperature
dimension. Furthermore, <inline-formula><mml:math id="M28" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is the tolerance level of interest
(i.e., the percentage levels mentioned above) transformed to a <inline-formula><mml:math id="M29" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test
statistic as implemented by <xref ref-type="bibr" rid="bib1.bibx70" id="text.49"/>, <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the 1 standard deviation levels of the uncertainties in the <inline-formula><mml:math id="M31" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M32" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> directions,
<inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the best estimates of the values in the <inline-formula><mml:math id="M34" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M35" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> directions,
i.e., date and data, and <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi mathvariant="italic">θ</mml:mi><mml:mo>∈</mml:mo><mml:mo>[</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula>. <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mi>cos⁡</mml:mi><mml:mo>(</mml:mo><mml:mi>d</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="italic">ρ</mml:mi></mml:mrow></mml:math></inline-formula> is the
correlation between temperature and time uncertainties. However, we do
not consider potential non-zero covariances between dating uncertainty
and proxy uncertainty. For simplicity, we also do not take account of
the likely correlations between subsequent tuples of data and date.</p>
      <p id="d1e1499">A two-dimensional tolerance ellipse represents tolerance levels for
two-dimensional normal distributed data. However, as in the simple case
of a tolerance rectangle, our interest is only in the ellipse as a
binary decision criterion to consider the data included in the ellipse
and to neglect the data outside of the ellipse. That is, we use the
ellipse as an area of tolerance to identify valid analogues from our
analogue candidate simulation field pool. The ellipses provide the
maximal acceptable distance for simulated data to be considered as an
analogue (Fig. <xref ref-type="fig" rid="Ch1.F2"/>b). That is, the ellipses are not meant to
represent the uncertainty ranges in the value of the proxies. They are
rather meant to define a limit beyond which an analogue candidate is not
considered anymore. Essentially, the ellipses define a weighting scheme
(although with binary weights) based on the proxy and dating
uncertainties.</p>
      <p id="d1e1504">The ellipses are defined from points in the proxy–time space (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>b). We construct ellipses for those data points for which a
published record provides ages. Our tolerance range for a specific date
as well as the tolerance envelope for the full proxy record follows from
the superposition of the tolerance ellipses from successive data points
(see panels of Fig. <xref ref-type="fig" rid="Ch1.F2"/> and later Figs. <xref ref-type="fig" rid="Ch1.F5"/> and
<xref ref-type="fig" rid="Ch1.F8"/>). This envelope<?pagebreak page727?> generally provides for each date upper and
lower limits of values that the analogue candidates need to fall
between. However, the envelope may also result in the impossibility to
define analogues for specific locations or even for all locations for
specific dates.</p>
      <p id="d1e1516">That is, the superposition of ellipses constructs a tolerance envelope
(Fig. <xref ref-type="fig" rid="Ch1.F2"/>a), which we use to identify valid analogues from
our candidate pool. The ellipses around the data points mark the limit
of their pointwise two-dimensional area of influence in our search for
spatially resolved analogues. Their superposition is essential for
identifying those simulated data to be considered as analogues. If the
tolerance ranges for multiple data points in a record overlap for a
given year, we simply take their maximal ranges. Simulated data that
fall outside the tolerance ranges are rejected. Thus, for a selected
date, candidate analogues have to fall within the tolerance range at all
considered locations to be valid analogues.</p>
      <p id="d1e1521">Because we provide reconstructions only for those years for which one of
the chosen proxy records includes a dated value, and because our
tolerance estimates are essentially pointwise, the envelope may not be
one continuous envelope over the full period of interest. Furthermore,
because we use the envelopes as a decision criterion, it can happen that
the method fails to find any valid analogues for given years.</p>
      <p id="d1e1524">Our pointwise estimates are compliant with the initial uncertainty of
the proxies, and our final reconstruction uncertainties are an expression
of this initial confidence in the local data. This is in contrast to
<xref ref-type="bibr" rid="bib1.bibx48" id="text.50"/>, who provide an ensemble of reconstructions. Their
uncertainty estimate measures the uncertainty of the initial
reconstruction relative to shifted ages. That is, the two different
applications of the analogue method consider different things in their
uncertainty estimates. The reconstruction uncertainty in our approach
originates from the selected analogues.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS4">
  <label>2.2.4</label><title>Analogue search</title>
      <p id="d1e1539">The ellipses of tolerance allow in theory to produce reconstructions for
each year included in the dating uncertainty. That is, if a proxy series
has a value dated to the year 500 BP with a dating uncertainty of
<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> years, and if we decide to consider dates within
<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula>, then we can search for analogues from 600 to 400 BP.
However, we decide to only reconstruct values at those dates at which at
least one proxy is dated. That is, if only this hypothetical proxy has a
dated value between 600 and 400 BP and it only has this one dated value,
we perform the reconstruction only for the year 500 BP. Our assumption
is that this maximizes the link between the reconstruction and the
underlying proxies. Thus, if we increase the width of the tolerance
envelope, we usually do not obtain reconstructed values at more dates
but only increase the probability to find a valid analogue at a given
date. As we show later, there are exceptions, when the wider tolerance
envelopes lead to the inclusion of more proxies at specific dates so
that the search becomes more constrained and finding an analogue becomes
less likely.</p>
      <p id="d1e1566">In other applications of the analogue method, the choice of a valid
analogue usually relies on a distance metric. This is commonly the
Euclidean distance
<xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx42 bib1.bibx93" id="paren.51"><named-content content-type="pre">compare</named-content></xref>, although
<xref ref-type="bibr" rid="bib1.bibx48" id="text.52"/> use an unweighted root mean square error (RMSE) as
distance metric between their proxies and the analogue candidates from
their simulation pool. Based on such a distance, one can select the best
fit, a small number of good fits, e.g., the 10 analogues with the
smallest distance, or a composite or interpolation of a small number of
good fits.</p>
      <p id="d1e1577">Here, we deviate from this and decide neither on a fixed number of
analogues nor a defined metric. Candidates in our pool are valid
analogues if they are within the tolerance range (compare Sect. <xref ref-type="sec" rid="Ch1.S2.SS2.SSS3"/>) at all considered locations for a selected date. That is,
as described above, we have an envelope of tolerance values for specific
years and each proxy record. For our standard approach, a candidate is a
valid analogue for a date if it falls within the ellipse of tolerance
for all proxies. We also mention tests where an analogue is valid if it
is outside the ellipses at one location, at two locations, or at 25 % of
the locations. We consider only a small set of potential ellipses. These
use 90 % and 99.9 % percentage levels for the pseudo-proxy approach and
either 99 % or 99.99 % percentage levels for the various proxy setups.</p>
      <p id="d1e1582">We additionally show one instance of a reconstruction using just one
best analogue. For this test, we choose the analogue with the smallest
Euclidean distance to our proxy values. As we deal with proxy records
that are irregularly spaced in time, we have to find a way to select
dates for which to do a single best analogue reconstruction and get the
proxy values for these dates. To do so, we consider the proxy values
valid at all dates within a given range around their dating. We identify
the range of these values and take the midpoint of that range as the
proxy value for this date. We consider values within a 90 % or
<inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.64</mml:mn></mml:mrow></mml:math></inline-formula> standard deviation dating uncertainty around the dating. We
compute these based on 1 standard deviation inferred from the
originally published dating uncertainty.</p>
      <p id="d1e1596">In short, our reconstruction is based on the following workflow. We have
a set of sparse proxy predictors and a pool of simulated fields. As our
proxies are not only sparse in space and uncertain in their values but
also irregular and uncertain in time, we have to decide (a) when to
compare them, (b) in which resolution to compare them, and (c) how to
consider the uncertainties in time and value. Therefore, we decide to
(i) compare the proxies and simulated data for all dates when one proxy
is dated, (ii) compare the proxies to 101 moving means of the
simulated data, and (iii) take the proxy data values as valid within
an ellipse of tolerance around the dated value in time and temperature
space. Then analogue candidate simulation fields are valid<?pagebreak page728?> analogues if
they are within these tolerance ranges around all proxy records included
in the search.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Data</title>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Proxies</title>
      <p id="d1e1615">We concentrate on a European–North Atlantic domain (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). There, we choose 17 locations with proxy-inferred
temperature records from the collection of <xref ref-type="bibr" rid="bib1.bibx67" id="text.53"><named-content content-type="post">see also
Tables <xref ref-type="table" rid="Ch1.T1"/> and <xref ref-type="table" rid="App1.Ch1.S1.T3"/></named-content></xref>. Nine of these
series use alkenone <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> but the set also includes
temperatures derived from foraminifera <inline-formula><mml:math id="M42" 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> (two records), pollen (two),
chironomids (two), TEX86 (one), and foraminiferal assemblages (one) (compare
Table <xref ref-type="table" rid="Ch1.T1"/> and Fig. <xref ref-type="fig" rid="Ch1.F3"/>). For the various proxy
types, see, e.g., <xref ref-type="bibr" rid="bib1.bibx80" id="text.54"><named-content content-type="post">and their
references</named-content></xref> or
<xref ref-type="bibr" rid="bib1.bibx100" id="text.55"><named-content content-type="post">and their references</named-content></xref> for <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>,
<xref ref-type="bibr" rid="bib1.bibx1" id="text.56"><named-content content-type="post">and their references</named-content></xref> or <xref ref-type="bibr" rid="bib1.bibx101" id="text.57"><named-content content-type="post">and their
references</named-content></xref> for foraminiferal <inline-formula><mml:math id="M44" 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>, <xref ref-type="bibr" rid="bib1.bibx57" id="text.58"><named-content content-type="post">and their
references</named-content></xref> or <xref ref-type="bibr" rid="bib1.bibx99" id="text.59"><named-content content-type="post">and their references</named-content></xref>
for TEX86, <xref ref-type="bibr" rid="bib1.bibx86" id="text.60"/> and <xref ref-type="bibr" rid="bib1.bibx87" id="text.61"/> for the specific
pollen records, <xref ref-type="bibr" rid="bib1.bibx61" id="text.62"/> for the specific chironomid
records, and <xref ref-type="bibr" rid="bib1.bibx81" id="text.63"/> for the specific record using
foraminiferal assemblages.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1737">Information about the different proxy setups:
matrix of proxy records against proxy setup (P01, indigo, and E01 to
E09, burgundy red). For more information, see Table <xref ref-type="table" rid="Ch1.T1"/>.
Whited-out areas indicate that the relevant proxy is not included in the
respective proxy setup. Note that the pseudo-proxy setup (P01) does not
distinguish between proxy types and uses only approximate locations due
to the discrete simulation output.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f03.png"/>

          </fig>

      <p id="d1e1748">We do not include all records from <xref ref-type="bibr" rid="bib1.bibx67" id="text.64"/> within the chosen
domain. We do not consider additional seasonal attributions for the
foraminifera assemblage data of <xref ref-type="bibr" rid="bib1.bibx81" id="text.65"><named-content content-type="post">compare also
<xref ref-type="bibr" rid="bib1.bibx67 bib1.bibx82" id="altparen.66"/></named-content></xref>. We further
excluded the alkenone unsaturation ratios of <xref ref-type="bibr" rid="bib1.bibx4" id="text.67"><named-content content-type="post">see also
<xref ref-type="bibr" rid="bib1.bibx67" id="altparen.68"/></named-content></xref> as well after initial tests due to
concerns about the potential influence of sea ice in simulations.
Indeed, we find (not shown) that including this record puts very strong
constraints on the analogue candidates and can reduce the chance of
finding valid analogues. We exclude two more records because they are
co-located with other proxies. That is, we do not use the stacked
radiolarian assemblage records of <xref ref-type="bibr" rid="bib1.bibx27" id="text.69"><named-content content-type="post">see also
<xref ref-type="bibr" rid="bib1.bibx67" id="altparen.70"/></named-content></xref> because the upper part of the record
is from the same upper core as the <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> data of
<xref ref-type="bibr" rid="bib1.bibx14" id="text.71"><named-content content-type="post">see also
<xref ref-type="bibr" rid="bib1.bibx67" id="altparen.72"/></named-content></xref>. Similarly,  we decide ad hoc  to use
the <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> data of
<xref ref-type="bibr" rid="bib1.bibx12" id="text.73"><named-content content-type="post">see also <xref ref-type="bibr" rid="bib1.bibx67" id="altparen.74"/></named-content></xref> instead of that of
<xref ref-type="bibr" rid="bib1.bibx55" id="text.75"><named-content content-type="post">see also <xref ref-type="bibr" rid="bib1.bibx67" id="altparen.76"/></named-content></xref>, which are basically
co-located. We use the data of <xref ref-type="bibr" rid="bib1.bibx55" id="text.77"/> in one alternative proxy
setup. Table <xref ref-type="table" rid="Ch1.T1"/> and Fig. <xref ref-type="fig" rid="Ch1.F3"/> provide details on
our different proxy setups. All in all, we consider nine different
setups of proxy networks, which we name E01 to E09. In a
pseudo-proxy setup, we use a network of locations equivalent to E01 and
therefore name this pseudo-proxy setup P01.</p>
      <p id="d1e1840">We consider the seasonal attributions of individual proxy records in our
search for analogues. We generally take the attributions and the
calibrations for the records as published by <xref ref-type="bibr" rid="bib1.bibx67" id="text.78"/> but
also check the references provided by them. Seasonal attributions are
diverse for the various proxy records. The majority is either for summer
season (seven) or annual (eight) according to <xref ref-type="bibr" rid="bib1.bibx67" id="text.79"/>. We compare
the proxies to the simulation output season that is close to the
seasonal attribution as given by <xref ref-type="bibr" rid="bib1.bibx67" id="text.80"/> or the original
publication. For simplicity's sake, we only consider the modern
meteorological seasons DJF (December to February), MAM (March to May),
JJA (June to August), and SON (September to November) as well as the
calendar annual simulation means (compare Table <xref ref-type="table" rid="Ch1.T1"/>). We do
ignore possible calendar effects <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx54" id="paren.81"><named-content content-type="pre">e.g.,</named-content></xref>.</p>
      <p id="d1e1859">Regarding proxy uncertainty, we decided to assume an uncertainty of
<inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mi mathvariant="italic">σ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> K for all proxies as we were not able to infer full
uncertainties for every temperature reconstruction either from
<xref ref-type="bibr" rid="bib1.bibx67" id="text.82"/> or from the original publications. This reduces the
uncertainty for some records and potentially increases the uncertainty
for others. We regard this to be a reasonable simplification.</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="d1e1879">Information about the number of available
proxies for the dates to be reconstructed: <bold>(a)</bold> the pseudo-proxy
setup, <bold>(b–j)</bold> the various proxy setups according
to Fig. <xref ref-type="fig" rid="Ch1.F3"/> and Table <xref ref-type="table" rid="Ch1.T1"/>. In panels <bold>(b)</bold> to
<bold>(j)</bold>, we show results for two different assumptions on the
uncertainties: a 99 % envelope and a 99.99 % envelope (compare Sect. <xref ref-type="sec" rid="Ch1.S2.SS2.SSS3"/>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f04.png"/>

          </fig>

      <p id="d1e1907">We performed reconstruction exercises for various proxy setups. We
concentrate on the full set of proxies mentioned above (see Fig. <xref ref-type="fig" rid="Ch1.F1"/> and first 17 lines of Table <xref ref-type="table" rid="Ch1.T1"/>). Figure <xref ref-type="fig" rid="Ch1.F4"/>b visualizes how many of these 17 proxies are available for
the dates for which we aim to reconstruct temperature. The figure shows
this for two different assumptions on uncertainty (red and grey lines;
see Sect. <xref ref-type="sec" rid="Ch1.S2.SS2.SSS3"/>).</p>
      <p id="d1e1918">Figure <xref ref-type="fig" rid="Ch1.F3"/> and Table <xref ref-type="table" rid="Ch1.T1"/> give a first impression of
setups for additional reconstructions. We shortly describe the results
for these alternative setups in our results section below. Most notably,
among these alternative tests are setups that use only <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>
proxies (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). The difference between the two
<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> setups is that E03 uses the GeoB 5901-2 record instead of the
M39-008 record  (compare Table <xref ref-type="table" rid="Ch1.T1"/> and Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p>
</sec>
<?pagebreak page729?><sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><title>Pseudo-proxies</title>
      <p id="d1e1974">We use pseudo-proxies calculated following <xref ref-type="bibr" rid="bib1.bibx7" id="text.83"/> to test
our approach. <xref ref-type="bibr" rid="bib1.bibx7" id="text.84"/> provide pseudo-proxies based on
simulated annual mean temperature and for a global selection of grid
points from the TraCE-21ka simulation <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx64" id="paren.85"/>. Here, we
calculate the pseudo-proxies for annual average data and for the chosen
European–North Atlantic domain only. The approach also provides randomly
chosen pseudo-age uncertainties. Following <xref ref-type="bibr" rid="bib1.bibx7" id="text.86"/> and
their repository <xref ref-type="bibr" rid="bib1.bibx8" id="paren.87"/>, these are based on assumptions on the
smoothing of the pseudo-proxies and a Gaussian term.</p>
      <?pagebreak page730?><p id="d1e1992">Here, the pseudo-proxy computation uses QUEST FAMOUS simulation data
<xref ref-type="bibr" rid="bib1.bibx89" id="paren.88"/>. Specifically, we use the simulation ALL-5G (see
Tables <xref ref-type="table" rid="App1.Ch1.S1.T4"/> and <xref ref-type="table" rid="App1.Ch1.S1.T5"/>). For details on this and
the other QUEST FAMOUS simulations, please see <xref ref-type="bibr" rid="bib1.bibx89" id="text.89"/>. The
FAMOUS-HadCM3 simulations for QUEST use accelerated forcings
<xref ref-type="bibr" rid="bib1.bibx89" id="paren.90"><named-content content-type="pre">compare</named-content></xref>. That is, the last glacial cycle of
approximately 120 000 years of climate forcing was simulated in
approximately 12 000 simulation years. Thus, the annual simulation data
are only representative of 10 years of climate evolution. The data are
available in monthly resolution for the full simulation period for air
temperature at 1.5 m height and as snapshots every 10 simulation
years for surface temperature. We use the simulation year annual means
of the air temperature data for the construction of the pseudo-proxies.
The FAMOUS-HadCM3 simulations use a very-low-resolution atmospheric
model with a 5<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude by 7.5<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude grid. Therefore,
we use the Climate Data Operators (CDO) application from the Max Planck Institute for Meteorology
(<uri>https://code.mpimet.mpg.de/projects/cdo/</uri>, last access: 18 August 2020)
to remap the data to a 0.5 by 0.5<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid and use this for the
pseudo-proxy calculations. In these remapped data, we follow
<xref ref-type="bibr" rid="bib1.bibx7" id="text.91"/> and use grid-point data close to proxy locations
used in the realistic setup.</p>
      <p id="d1e2044">We modify the pseudo-proxy script of <xref ref-type="bibr" rid="bib1.bibx7" id="text.92"/> to account
for the reduced temporal resolution of the available QUEST FAMOUS data.
This primarily means considering the default parameter settings that are
given in time units. It also includes ad hoc scaling of the randomly chosen
dating uncertainty to approximate the distribution of the observed
dating uncertainties. The latter modification also avoids
individual data points extending their influence too far along the time
dimension.</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="d1e2053">Pseudo-proxy data and assumed uncertainties for the 17 locations in our pseudo-proxy application.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f05.png"/>

          </fig>

      <p id="d1e2062">The 17 pseudo-proxy locations are close to the realistic proxy locations
(compare Fig. <xref ref-type="fig" rid="Ch1.F1"/>). Figure <xref ref-type="fig" rid="Ch1.F4"/>a visualizes the
number of pseudo-proxy locations with data against the dates at which we
try to reconstruct values. The pseudo-proxy records are shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/>. The figure also visualizes our assumptions on the
uncertainty of the pseudo-proxies in terms of the tolerance envelope
(compare Sect. <xref ref-type="sec" rid="Ch1.S2.SS2.SSS3"/>).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e2076">Information about the pool of
simulation data: model name, the project for which the simulations were
performed, the simulated periods from this model output, the number of total
years. All simulation data are remapped to 0.5 by 0.5<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grids. References
and data locations are provided in Appendix Table <xref ref-type="table" rid="App1.Ch1.S1.T4"/>. The
Appendix also lists all individual simulations used in Table <xref ref-type="table" rid="App1.Ch1.S1.T5"/>. Note FAMOUS-HadCM3 uses accelerated forcings.
We thus chose to exclude this simulation for most
cases.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">Project</oasis:entry>
         <oasis:entry colname="col3">Periods</oasis:entry>
         <oasis:entry colname="col4">Total years</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM, mid-Holocene</oasis:entry>
         <oasis:entry colname="col4">400</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">COSMOS-ASO</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM</oasis:entry>
         <oasis:entry colname="col4">600</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO-Mk3L-1-2</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM</oasis:entry>
         <oasis:entry colname="col4">500</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM, mid-Holocene, past 1000 years</oasis:entry>
         <oasis:entry colname="col4">9309</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadCM3</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">Past 1000 years</oasis:entry>
         <oasis:entry colname="col4">1001</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-CC</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
         <oasis:entry colname="col4">35</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-ES</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
         <oasis:entry colname="col4">102</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM, mid-Holocene, past 1000 years</oasis:entry>
         <oasis:entry colname="col4">1701</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">PMIP3</oasis:entry>
         <oasis:entry colname="col3">LGM, mid-Holocene, past 1000 years</oasis:entry>
         <oasis:entry colname="col4">1400</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">Last millennium ensemble</oasis:entry>
         <oasis:entry colname="col3">Past 1000 years, pre-industrial control, industrial</oasis:entry>
         <oasis:entry colname="col4">33 156</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CCSM3</oasis:entry>
         <oasis:entry colname="col2">TraCE-21ka</oasis:entry>
         <oasis:entry colname="col3">LGM to present</oasis:entry>
         <oasis:entry colname="col4">22 040</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">Millennium COSMOS</oasis:entry>
         <oasis:entry colname="col3">Past 1000 years, pre-industrial control, industrial, projection</oasis:entry>
         <oasis:entry colname="col4">5909</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3</oasis:entry>
         <oasis:entry colname="col2">Quaternary QUEST</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
         <oasis:entry colname="col4">6014</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>Simulations</title>
      <p id="d1e2332">Table <xref ref-type="table" rid="Ch1.T2"/> provides a general overview of the various
simulations in our pool of candidates. Tables <xref ref-type="table" rid="App1.Ch1.S1.T4"/> to <xref ref-type="table" rid="App1.Ch1.S1.T5"/> give additional information. We
only consider previously published simulations. These stem from a
variety of projects and were performed with a variety of models. The
projects are TraCE-21ka (“Simulation of Transient Climate Evolution over
the last 21 000 years”) <xref ref-type="bibr" rid="bib1.bibx64" id="paren.93"/>, the Paleoclimate Modelling
Intercomparison Project phase III
<xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx10" id="paren.94"><named-content content-type="pre">PMIP3;</named-content></xref>, the CESM Last Millennium
Ensemble Project <xref ref-type="bibr" rid="bib1.bibx73" id="paren.95"/>, the Max Planck Institute
Community Simulations of the last millennium <xref ref-type="bibr" rid="bib1.bibx53" id="paren.96"/>, and
Quaternary QUEST <xref ref-type="bibr" rid="bib1.bibx89" id="paren.97"><named-content content-type="pre">e.g.,</named-content></xref>. We include the QUEST FAMOUS
simulations only for a test case and exclude them for the main
discussions due to their specific characteristics (compare Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS2"/>).</p>
      <p id="d1e2363">We use simulations for various different time periods to increase the
candidate pool. We assume that simulation climatologies can differ over
a relatively wide range <xref ref-type="bibr" rid="bib1.bibx109" id="paren.98"><named-content content-type="pre">e.g.,</named-content></xref>.
Simulations from the TraCE-21ka and the QUEST projects are transient
over periods covering approximately the last 22 kyr and the last glacial
cycle, respectively. Otherwise, the simulations are transient over the
last millennium or time slices for the mid-Holocene and the Last
Glacial Maximum. Additionally we also include pre-industrial control
simulations. Such a multi-model and multi-time-period candidate pool
effectively follows suggestions of <xref ref-type="bibr" rid="bib1.bibx90" id="text.99"/>. We note that
considering simulations for the last millennium as candidate for the
Last Glacial Maximum can introduce climatological inconsistencies if the
method identifies these fields as analogues.</p>
      <p id="d1e2374">We remap all simulation output to a 0.5 by 0.5<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> grid for the
construction of pseudo-proxies and for the search for analogues. The
motivation is that thereby fewer proxies are close to the same grid
point. However, resulting differences between grid points are likely
small. We use the original resolution for the final regional average
reconstructions and the evaluation of field data. Local grid-point
evaluations are done against the remapped files.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Pseudo-proxy application</title>
      <p id="d1e2403">The pseudo-proxy application allows highlighting the possibilities of our
implementation of the analogue method. It further already provides a
glimpse at potential problems.</p>
      <p id="d1e2406">We recapture our approach briefly. Our analogue method searches for
analogues within the full pool of simulation fields but excludes the
FAMOUS-HadCM3 output from the QUEST project. Pseudo-proxies are derived
from this latter simulation. We compare the pseudo-proxy predictors to
101-year moving averages of the simulation output. We concentrate on
90 % tolerance ellipses in the pseudo-proxy application of the analogue
search but also include results for 99.9 % tolerance ellipses. Valid
analogues are those simulation fields that are within the resultant
tolerance envelopes for all pseudo-proxy locations available for a date.</p>
      <p id="d1e2409">Temperatures are reconstructed for the full domain of the
European–North Atlantic sector including the Arctic (Fig. <xref ref-type="fig" rid="Ch1.F1"/>) and over a multimillennial period leading up to the late
20th century CE. Figure <xref ref-type="fig" rid="Ch1.F4"/>a highlights that most
pseudo-proxies are defined at all dates. That is, the chosen sample dates
of the pseudo-proxies are close to each other, and thereby the generated
dating uncertainties result in relatively large overlaps. Figure <xref ref-type="fig" rid="Ch1.F5"/> presents the pseudo-proxies including their tolerance
envelopes.</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="d1e2421">Reconstruction results for the pseudo-proxy
application of the analogue method: <bold>(a)</bold> regional averages for
101-year moving averages for two different tolerance envelope levels
(90 %, reds, 99.9 %, grey). Lines show the 101-year moving average
regional target in the TraCE-21ka simulation (blue), the median of all
analogues (90 %, red, 99.9 %, black), and the range of all analogues for the respective tolerance ranges (colored shading). Panel <bold>(b)</bold> shows the number of analogues found for each of the dates considered for both setups (90 %, red, 99.9 %, black). Panel <bold>(c)</bold> adds 101-year moving averages of local pseudo-proxy data (grey), local target data (blue), the range of all local analogue values (light red), and the local median of
the analogues (red) for two locations (warmer case: 36.25<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 2.75<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W; colder case: 57.75<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 8.75<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) and for the 90 % tolerance envelopes only.
Panels <bold>(d)</bold> and <bold>(e)</bold> provide expansions of regional <bold>(d)</bold> and local <bold>(e)</bold> 101-year moving average analogues into 101-year long
time series for the 90 % tolerance envelopes only. The panels show the
median (red), the range (light red), and two valid analogue examples of
the expansions. Due to the coarse resolution for the QUEST FAMOUS data,
panels <bold>(c)</bold> and <bold>(e)</bold> use the remapped data of the
simulation.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f06.png"/>

        </fig>

      <p id="d1e2495">In this setting, the analogue search tries to identify analogues for
1830 dates. Our implementation finds between 1 and 7919 analogues on
531 dates (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b); it fails to find analogues for dates
during the deglaciation and the glacial maximum. Analogues stem mainly
from the Trace-21ka simulation. Occasionally, output from the PMIP3
past1000 simulation with IPSL-CM5A-LR is also classified as valid
analogues.</p>
      <p id="d1e2500">Results change if we consider a wider tolerance envelope. For an 99.9 %
tolerance envelope instead of a 90 % one, we are able to find between 1
and 16 944 valid analogues at 1438 of 1830 dates (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b). Analogues stem from four additional simulations
compared to the smaller tolerance envelope. These are the PMIP3
midHolocene and lgm setups of IPSL-CM5A-LR, the COSMOS-ASO lgm setup,
and the GISS-E2-R past1000 ensemble member r1i1p122.</p>
      <?pagebreak page731?><p id="d1e2505"><?xmltex \hack{\newpage}?>Figures <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F7"/> provide information on which
types of reconstructions we obtain from our analogue method. Figure <xref ref-type="fig" rid="Ch1.F6"/>a indicates the area mean reconstructions for two
different tolerance envelopes. It shows the resulting reconstruction
medians in black and red for 99.9 % and 90 % tolerance assumptions,
respectively. The blue line in the panel is the 101-year moving average
regional temperature from the simulation, i.e., the reconstruction
target. Shading in the panel shows the full range of potential
analogues.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2517">Temperature field reconstructions in <inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the
pseudo-proxy approach: example of a 101-year mean annual temperature
analogue reconstruction for the European–North Atlantic sector in <inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
centered in the year 8000 before 1950. <bold>(a)</bold> One example
analogue, <bold>(b)</bold> local median of all analogues, <bold>(c)</bold> local
minimum of all analogues, and <bold>(d)</bold> local maximum of all
analogues. Panels <bold>(c)</bold> and <bold>(d)</bold> show differences to the
median in <inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f07.png"/>

        </fig>

      <p id="d1e2573">The results are encouraging but problems are obvious. We are able to
find valid analogues for both tolerance ranges.</p>
      <p id="d1e2576">Analogues are regularly relatively close to the target for the narrow
tolerance range. However, their number is often small and there are
periods without any valid analogues. The range does seldom include the
target. Further, the reconstruction with a narrow tolerance assumption
does not provide valid analogues earlier than approximately 13 500 BP.</p>
      <p id="d1e2579">On the other hand, the range of potential analogues is only weakly
constrained for the wider tolerance range. For example, the analogue
search may regard more than 17 000 records of the TraCE-21ka simulation
as valid analogues around the year 10 000 BP (compare Fig. <xref ref-type="fig" rid="Ch1.F6"/>b). This wide range often includes the target. However, the
target is mostly<?pagebreak page732?> above the median estimate. The reconstruction gives a
rather constant estimate from a small number of analogues for the period
earlier than 16 000 years before present.</p>
      <p id="d1e2584">The pseudo-proxies, together with their uncertainties, are a weak
constraint during most of the period of interest if we assume a wider
tolerance but they fail to capture the target if we assume a stronger
knowledge about their value. In addition, the reconstruction envelopes
and medians show rather little variability and often give nearly
constant values over long periods. That is, the set of valid analogues
has a notable overlap for these periods. The lacking variability among
analogues together with the potentially wide range of analogues is
reflected in the small variability in the reconstruction median.</p>
      <p id="d1e2587">Besides the regional average, the results allow us to extract the local
representations. Figure <xref ref-type="fig" rid="Ch1.F6"/>c shows two examples for the narrow
90 % tolerance assumption. These are for the pseudo-proxies at
36.25<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 2.75<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, and 57.75<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 8.75<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. We refer to those as the warmer southern
and colder northern locations, respectively. The panel plots again the
target simulation output in blue, the full analogue range in light red,
and the analogue median in red. We also add the pseudo-proxy in grey.</p>
      <p id="d1e2628">At both locations, the range is very small for the narrow tolerance
range. At the southern location, the reconstruction median is generally
below the target, and the range is hardly identifiable and does not
include the target. This is comparable to the northern location, where,
however, the median is generally above the target. Even for the wide
tolerance range, the target is more often outside than within the full
analogue range at the southern location, while at the northern location
the range includes the target regularly (not shown). Thus, the range of
potential analogue cases is still relatively narrow at the southern
location but can be already quite wide at the northern location. Also
locally, analogue range and median show little variability. In the
northern case, the analogue medians fail for both tolerance assumptions
to capture the average characteristics of the pseudo-proxy except for
approximately the most recent 3 kyr.</p>
      <p id="d1e2632">The pseudo-reconstruction results suggest that the approach can provide
local information in addition to the regional average. Relatively wide
tolerance appears to be necessary to capture the local characteristics
at the two chosen locations. This is more successful for some periods
but success always varies regionally.</p>
      <p id="d1e2635">Since we search analogues among temporal moving window averages, the
analogue search provides one more result of interest. Any analogue state
represents a temporal average. Since we also know the period that has
been averaged, we can provide the climatic time-varying sequence. This
informs us about the time variations underlying the analogue average
climate state. That is, we obtain climate evolutions that comply with
our proxy constraints. This, for example, allows us to get an impression of
how temperature changed on subcentennial, e.g., interannual, timescales
or to obtain an estimate of the interannual variability. Figure <xref ref-type="fig" rid="Ch1.F6"/>d and e provide such expansions of 101-year average
states into 101-year time series. They do so for a narrow tolerance
assumption. The panels show the range and the median of 101-year series
for all found analogues for one specific year. They also add two
examples of 101-year time series. Panel (d) is for the regional average
and panel (e) for the grid point at 36.25<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 2.75<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W. Both show 101-year
expansions around the average centered at the year 8000 BP.</p>
      <p id="d1e2658">Although we consider a narrow tolerance range, which results in very
narrow ranges around the mean analogue state, the expanded range of
potential analogues is still notably wide. The two examples of valid
analogues highlight how<?pagebreak page733?> much two climates may differ over the period,
although both are valid analogues considering the proxy uncertainty.
Wider tolerance ranges give larger ranges of reconstructions and result
in larger differences between the 101-year time series.</p>
      <p id="d1e2661">Finally, our reconstruction approach allows considering the spatial
fields of valid analogues. Figure <xref ref-type="fig" rid="Ch1.F7"/> adds an example for
101-year mean annual temperature. It shows one valid analogue field in
panel (a) and the local median, minimum, and maximum values of all
analogues in panels (b) to (d), respectively. The chosen date is the year
8000 BP for the narrow tolerance range. Panel (a) also adds the values
for the pseudo-proxies that enter the analogue search. The example
analogue and the pseudo-proxies agree to some extent but disagreement is
notable south of Iceland. There are more than 1000 analogues for this
year. Their local range at no point exceeds 4 <inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for the
narrow tolerance setup. Local positive deviations from the median may
differ most strongly over Greenland and in Scandinavia. In the latter
region, proxies should constrain our search for analogues. Local
negative deviations may become largest over comparable domains. We do
not show the equivalent figure for the wide tolerance assumption but
note that in this case the local range of results may exceed 20 <inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and that largest positive excursions occur southwest of
Svalbard, where a proxy constrains our search. The largest negative
excursions are located at the eastern border of our domain in the
Barents Sea, where our search is effectively unconstrained.</p>
      <?pagebreak page734?><p id="d1e2684">The pseudo-proxy application of our implementation of an analogue search
shows the viability of such approaches for reconstructing past climates
from spatially sparse proxies with temporally sparse, irregular, and
uncertain ages. The pseudo-proxy tests also show that the results depend
on our assumptions on how tolerant we are with respect to our confidence
in the proxy input. Overall, the pseudo-proxies are only weak constraints
on the potential climate.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Application to real proxies</title>
      <p id="d1e2695">Already the pseudo-proxy test highlights the potential but also the
associated problems in using the analogue method for the type of proxies
we are interested in, together with a limited pool of candidate fields.
The analogue reconstruction is able to capture the target data but the
search may provide either a very wide or a too-narrow uncertainty range
relative to the target. Wide ranges occur mostly due to the large number
of valid analogues, while narrow ranges signal that there are only few
analogues fitting the proxy data under the made assumptions on the
fidelity of the proxies. The method may overall fail to provide valid
analogues.</p>
      <p id="d1e2698">Our focus here is on a multi-archive and multi-proxy reconstruction
using 17 proxies (compare Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS1"/>) for the European–North
Atlantic sector for approximately the last 15 kyr. Preliminary tests
showed that using a 90 % tolerance level leads to ranges that are too
narrow to find any suitable analogues (not shown). We only show the
results for using 99 % and 99.99 % tolerance levels in the estimation of
our tolerance envelopes around proxy records. For the meaning of these
levels, see the descriptions for Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>).</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="d1e2707">Proxy data and assumed uncertainties for all proxy-record locations in our analogue search under two different tolerance envelopes.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f08.png"/>

        </fig>

      <p id="d1e2717">Figure <xref ref-type="fig" rid="Ch1.F8"/> shows the proxies and their constructed tolerance
envelopes for the locations in Fig. <xref ref-type="fig" rid="Ch1.F1"/>. The panels
highlight that the real proxy values are less equally distributed
through time, are generally smoother, and differ more in their lengths
compared to the pseudo-proxy setup. Figure <xref ref-type="fig" rid="Ch1.F4"/>b already showed
how the number of available proxies increases from 11 to 17 but then
again decreases until only five proxies are available for the earliest
dates. Below we compare the full 17-proxy setup to different sets of
proxies. Table <xref ref-type="table" rid="Ch1.T1"/> and Figs. <xref ref-type="fig" rid="Ch1.F3"/> to <xref ref-type="fig" rid="Ch1.F4"/>
give details for the different sets.</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="d1e2735">Reconstruction results for the analogue method
under two different tolerance assumptions: panel <bold>(a)</bold> shows median and range of all analogues of regional averages for 101-year moving averages
for an assumed 99 % tolerance envelope (red) and a 99.99 % envelope
(blue). Panel <bold>(b)</bold> provides the number of analogues found for each of
the dates considered; red: 99 % envelope, blue: 99.99 % envelope.
Panel <bold>(c)</bold> adds  the proxy
data (grey) for the location of the MD95-2043  record, and the range and median of all local analogue values for a
99 % envelope (red) and a 99.99 % envelope (blue). Panels <bold>(d)</bold> and <bold>(e)</bold> give
expansions of regional <bold>(d)</bold> and local (36.1<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 2.6<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W; MD95-2043) <bold>(e)</bold> 101-year moving averages in 101-year series ranges. They give the median (red), the range (light red), and two valid analogue examples of the expansions. Both panels only show results for the 99 % tolerance envelope.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f09.png"/>

        </fig>

      <p id="d1e2784">In the case of the main set of 17 proxies, our implementation tries to
find analogues for 1781 dates. There are between 1 and 900 analogues
for 141 dates for 99 % tolerance envelopes (see Fig. <xref ref-type="fig" rid="Ch1.F9"/>b).
Analogues come from two different simulations. It is obvious that the
method often fails to provide a valid analogue.</p>
      <p id="d1e2789">For the 99.99 % envelope, these basic results change. The method
identifies 1 to 31 304 analogues at 1288 dates (see Fig. <xref ref-type="fig" rid="Ch1.F9"/>b). These come from 42 different simulations. There are no
valid analogues between <inline-formula><mml:math id="M72" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 10 and <inline-formula><mml:math id="M73" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14 kyr BP. Otherwise, there are extended periods with many analogues and
other periods with few analogues.</p>
      <p id="d1e2808">For the narrower tolerance assumption, the method finds valid analogues
only for the recent past millennia (Fig. <xref ref-type="fig" rid="Ch1.F9"/>). Even then, it
is only successful for few periods (Fig. <xref ref-type="fig" rid="Ch1.F9"/>b). In this
case, the range of the area average reconstruction (Fig. <xref ref-type="fig" rid="Ch1.F9"/>a) and at the local proxy location (Fig. <xref ref-type="fig" rid="Ch1.F9"/>c)
is very narrow. There is very little regional or local temporal
variability in the analogues. However, the reconstruction may reflect
well the average state of the local proxy series (Fig. <xref ref-type="fig" rid="Ch1.F9"/>c). As for the pseudo-proxy test, we can expand the
analogues, i.e., the 101-year moving means, to show the underlying
time variations (Fig. <xref ref-type="fig" rid="Ch1.F9"/>d and e). These again provide an
impression of interannual variability that is compliant with our proxy
constraints on the centennial average. These panels emphasize the very
narrow range of potential analogues for the regional average but also
for the local series. For the chosen year, there is only a small number
of analogues, which form a sequence of consecutive simulated years from
one simulation. Therefore, the two examples in panels (d) and (e) are
simply time-shifted sequences.</p>
      <p id="d1e2825">For the wider tolerance envelope, the method identifies valid analogues
for more dates (Fig. <xref ref-type="fig" rid="Ch1.F9"/>) and, generally, there are more
valid analogues for these dates (Fig. <xref ref-type="fig" rid="Ch1.F9"/>b). However, there
are more proxies available for some dates (compare Fig. <xref ref-type="fig" rid="Ch1.F4"/>)
and this increases the number of constraints on the analogue candidates
for these dates. Thus, there are dates when the range of the regional
average reconstruction for a 99.99 % tolerance envelope does not
necessarily include the 99 % envelope data.</p>
      <?pagebreak page735?><p id="d1e2834">The range of the reconstruction may be regionally or locally wide for
the 99.99 % envelope, but this does not ensure that it locally includes
the proxy values (Fig. <xref ref-type="fig" rid="Ch1.F9"/>c). There is little temporal
variability in the reconstructed data. This is mainly because of the
large number of analogues and the relatively low temporal variation in
the set of valid analogues (Fig. <xref ref-type="fig" rid="Ch1.F9"/>b). Further, the
reconstruction is rather constant.</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="d1e2843">Field information for the analogue search: two
examples of 101-year mean annual temperature analogue reconstructions
for the European–North Atlantic sector in <inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. <bold>(a, e)</bold> One example analogue, <bold>(b, f)</bold> local median of all analogues, <bold>(c, g)</bold> difference of local minimum to local median of all analogues, and <bold>(d, h)</bold> difference of local maximum to local median of all
analogues. Panels <bold>(a)</bold> to <bold>(d)</bold> are for the 99 % tolerance
envelope and the year 2429 BP; panels <bold>(e)</bold> to <bold>(h)</bold> are for the
99.99 % tolerance envelope and the year 14 105 BP.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f10.png"/>

        </fig>

      <p id="d1e2886">Figure <xref ref-type="fig" rid="Ch1.F10"/> plots examples of a field and of the local minima,
median, and maxima of potential analogues for the two different
tolerance envelopes. The upper row uses the 99 % envelope reconstruction
for the year 2429 BP and the lower row uses the 99.9 % envelope
reconstruction for the year 14 105 BP. For both dates, all valid
analogues are from only one simulation each. The examples in Fig. <xref ref-type="fig" rid="Ch1.F10"/>a and e also include as dots the proxy values
available for the respective dates. These highlight that, for the late
Holocene date, the found analogues capture the proxies rather well
though with exceptions over Scandinavia. However, the analogues for
<inline-formula><mml:math id="M75" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 14 kyr BP strongly disagree with the one proxy at high
northern latitudes. The range of analogues is very narrow for the late
Holocene example from the narrow tolerance case. Differences become
largest over Greenland and along the sea-ice edge. For the deglacial
example and the wider tolerance case, differences become largest east
and west of Iceland.</p>
<?pagebreak page736?><sec id="Ch1.S3.SS2.SSSx1" specific-use="unnumbered">
  <title>Results for different proxy setups</title>
      <p id="d1e2905">Table <xref ref-type="table" rid="Ch1.T1"/> introduces a number of additional proxy setups (E02
to E09). These use different subselections of proxies from our initial
selection. Further, most of them test sparser sets of locations around
central Europe (compare Table <xref ref-type="table" rid="Ch1.T1"/>). Figure <xref ref-type="fig" rid="Ch1.F3"/>
provides additional information about which records are included in the
different setups and their proxy types. Here, we shortly present the
results.</p>
      <p id="d1e2914">Experiment E01 is our main setup. It was described in the previous
section. It uses the 17 chosen proxy locations, which we also use for
the pseudo-proxy setup. Setups E02 and E03 are based only on alkenone
<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> records and E03 replaces M39-008 by GeoB 5901-2, as both
are co-located. E04 to E09 include different numbers of other proxy
types instead of <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the
availability of proxies for the different setups. Figure <xref ref-type="fig" rid="Ch1.F8"/>
presents the proxy data and assumed uncertainties including the GeoB
5901-2  record. For more information, see Table <xref ref-type="table" rid="Ch1.T1"/> and Fig. <xref ref-type="fig" rid="Ch1.F3"/>.</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="d1e2962">Visualizing the reconstructions for the various
proxy setups: <bold>(a)</bold> E01, <bold>(b)</bold> E02, <bold>(c)</bold> E03,
<bold>(d)</bold> E04, <bold>(e)</bold> E05, <bold>(f)</bold> E06, <bold>(g)</bold> E07,
<bold>(h)</bold> E08, <bold>(i)</bold> E09. All panels include the median and
the full range for the reconstructions under a 99 % tolerance envelope
(red) and a 99.99 % envelope (blue). Panel <bold>(a)</bold> additionally
includes a setup in black where we do not consider 101-year moving
averages of simulation data but all simulation output as provided
including the FAMOUS-HadCM3 simulations for QUEST. Orange points in
panel <bold>(a)</bold> are for a test considering only the single best
analogues for each date.</p></caption>
            <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f11.png"/>

          </fig>

      <p id="d1e3005">Figure <xref ref-type="fig" rid="Ch1.F11"/> shows the reconstruction results for the proxy
setups E01 to E09. All panels plot the reconstructions using the 99 %
and the 99.99 % tolerance envelopes. Panel (a) adds for our main setup a
reconstruction where we consider interannual data for the simulations
and include the QUEST FAMOUS-HadCM3 simulations. The panel also includes
the results of testing an analogue approach where only the single best
analogue is considered at each date.</p>
      <p id="d1e3011">The panels of Fig. <xref ref-type="fig" rid="Ch1.F11"/> highlight that loosening the
tolerance constraint and thereby widening the tolerance envelope leads
to valid analogues for notably more dates as well as a wider range of
valid analogues. We also obtain analogues at more dates if we keep the
tolerance envelope at the lower level but do not preprocess the
simulation output to 101-year moving means (Fig. <xref ref-type="fig" rid="Ch1.F11"/>a, black
lines). This inclusion of interannual data increases the number of
analogues throughout the reconstruction period. This variation of the
experiment also uses more simulation data by including the QUEST FAMOUS
data, but this only affects the reconstruction success in the 15th
millennium BP in this setup. We performed further tests with different
averaging periods of 51 and 501 years, respectively, while keeping the
narrow tolerance envelope (not shown). Increasing the averaging period
to 501 years reduces the number of valid analogues and the<?pagebreak page737?> number of
dates with any valid analogues. Reducing the averaging period to 51 years allows us to find a few valid analogues in the 15th and 16th
millennia BP. In this setting, the approach also finds more valid
analogues in recent millennia.</p>
      <p id="d1e3018">Generally, the method appears to provide more complete reconstructions
among our proxy setups for those that only include <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>
records (Fig. <xref ref-type="fig" rid="Ch1.F11"/>b, c). That is, such consistent sets of
proxies provide a more continuous reconstruction for both local
tolerance assumptions. Nevertheless, we fail to obtain valid analogues,
i.e., reconstructed values at the end of the deglaciation. While results
are quite similar over much of the period between both reconstruction
attempts (E02 and E03), the second setup allows a wider and potentially
colder range in the period before <inline-formula><mml:math id="M79" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12 kyr BP.</p>
      <p id="d1e3047">Further panels of Fig. <xref ref-type="fig" rid="Ch1.F11"/> add different setups. Panel (d)
complements the <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> proxies by one foraminiferal assemblage
record. Panels (e) and (f) also test different setups dominated by
<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> but including other proxies. Panels (g) to (i) use
different small setups of proxies around the European area.</p>
      <p id="d1e3086">Multi-archive setups with fewer proxies give generally wider ranges of
possible analogues. Otherwise, all setups tend to be in a comparable
range regarding their median and their range considering the last 10
millennia. Differences between all setups are largest in the 14th
millennium BP due to a larger range for some reconstructions.</p>
      <p id="d1e3089">Both multi-proxy setups in panels (e) and (f) fail to provide analogues
before the deglaciation for the narrower tolerance assumption. The
setups in panels (g) and (i) are notably warmer in the 14th millennium
BP compared to results in panel (h) but also compared to other setups.
This holds for both tolerance envelopes. A common difference is the
inclusion of M39-008 while excluding the <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msubsup><mml:mi>U</mml:mi><mml:mn mathvariant="normal">37</mml:mn><mml:mrow><mml:msup><mml:mi>K</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>  D13882 record
(compare Table <xref ref-type="table" rid="Ch1.T1"/> and Fig. <xref ref-type="fig" rid="Ch1.F3"/>). The latter
record is thought to represent summer temperatures off the west coast of
Portugal, while the former is meant to represent annual temperatures in
the Gulf of Cádiz. We note that panels (e) and (f) also are warmer
compared to other setups in the 14th millennium BP for the wider
tolerance range. These also include M39-008 and exclude D13882. Please
note that the Supplement of <xref ref-type="bibr" rid="bib1.bibx67" id="text.100"/> refers to D13882 as D13822.</p>
      <p id="d1e3116">Generally, we find that the reconstructions from different setups differ
in their ability to reconstruct climate for specific periods. Indeed,
different setups may provide notably different climates, particularly
for the early part of the time period of interest. Particular proxies
appear to shift the results for the earlier part of our reconstruction
between a warmer and a colder deglacial estimate. It is beyond the scope
of this paper to disentangle the reasons for this. All setups provide
rather constant reconstruction ranges.</p>
      <p id="d1e3120">As noted, Fig. <xref ref-type="fig" rid="Ch1.F11"/>a adds a single best analogue
reconstruction, where the reconstructed value for a given date is the
analogue candidate with the smallest Euclidean distance to the proxy
values for that date. During the past approximately four millennia, as
well as during the period from 8000 to 10 000 years BP, the single
best estimate is included in the ranges of our other reconstruction
efforts. Indeed it is close to the test with interannual data throughout
the Common Era of the last 2000 years.</p>
      <?pagebreak page738?><p id="d1e3125">In the period between 4000 and 8000 years BP, when other
approaches give very narrow ranges due to few valid analogues, there are
cases when the result from the single best analogue setup differs
notably from the other efforts. However, it is still within the range of
results from the other experiments for earlier and later periods. Such
deviations from the tolerance area approach are reasonable since our
construction of the proxy values for the single best analogue search can
provide a notably different proxy state compared to the tolerance
envelopes constructed for our standard approach. Another potential
explanation is that the analogue that minimizes the overall distance may
be outside of one or even multiple tolerance ranges. Finally, we already
mentioned that changing a tolerance level may change the number of proxy
locations included in a search. For example, widening a tolerance level
may result in inclusion of more proxy locations for specific dates. The
construction of the proxy values for the single best search similarly
changes the underlying multi-dimensional proxy vector. Indeed, an
inspection of the data indicates that, in our test case, the found
analogue does fall outside the tolerance ranges at least at one
location.</p>
      <p id="d1e3128">We also note that the single best analogue approach allows us to obtain
estimates when the other approaches fail between 10 000 to 14 000 years BP. Comparably to our other reconstruction attempts, the single best
analogue reconstruction shows only little variability. Noteworthy are
the reconstructed values in the 15th millennium BP where the single best
analogue represents a Holocene-level warm climate and not a deglacial
climate.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e3133">Visualizing alternative reconstructions:
<bold>(a)</bold> E01 with rectangular tolerance range, <bold>(b)</bold> E01 with
relaxed criteria for analogue selection. Panel <bold>(a)</bold> includes the
median and the full range for the reconstructions under a 99 % tolerance
envelope (red) and a 99.99 % envelope (blue). Panel <bold>(b)</bold> shows
range and median for setups where the analogue candidates are valid even
if they fail at one (red) or two (blue) locations or at 25 % of all
locations (black).</p></caption>
            <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://cp.copernicus.org/articles/17/721/2021/cp-17-721-2021-f12.png"/>

          </fig>

      <p id="d1e3154">We consider two more modifications of our approach. Figure <xref ref-type="fig" rid="Ch1.F12"/>
shows, first, results using a rectangular tolerance region, and,
secondly, reconstructions for tests where an analogue candidate is valid
although it falls outside the tolerance region at one, two, or 25 % of
the locations. The rectangular setup has minimal influence on the
reconstruction but gives more homogeneous ranges of valid analogues and
succeeds on slightly more dates in finding valid analogues. Relaxing the
tolerance criteria results in very wide ranges in the early part of the
study period. Due to few available proxies in that period, the criterion
to fit 75 % of locations is stricter than the criterion that allows the analogue search to
fail at two locations. The resulting reconstructions still have<?pagebreak page739?> little
variability. They also either give a wide and nearly constant range of
potential values or a very narrow range.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e3169">Our implementation of an analogue search method for reconstructing
surface temperature over multimillennial timescales relies on a number
of decisions, which are uncommon compared to other paleo-reconstruction
efforts on multimillennial timescales. Central to our assumptions is
that taking account of the uncertainty in our underlying data is
indispensable in analogue approaches for paleoclimatology and,
particularly, if one uses spatially and temporally sparse as well as
data- and age-uncertain proxies. There is one prime motivation behind our
specific handling of uncertainty in terms of tolerance ranges and our
selection of reconstruction dates: the analogue search for a chosen date
should use as much information about this date as possible, including
the uncertainty of other data points whose age uncertainties include the
currently given date of interest.</p>
      <p id="d1e3172">This leads to the use of tolerance ellipses. Assumptions here are that,
firstly, data and date are inseparable; secondly, this assumption
also holds for the tuple and its two-dimensional uncertainty; and,
thirdly, a reconstruction exercise has to consider both parts of
the uncertainty to sufficiently estimate the range of reconstructed
values. Admittedly, our procedure is a simplified approach to
incorporating these assumptions. More correctly, one would calculate the
multivariate joint distribution and use a measure of likelihood to
select the analogues. As a side note, the highly dimensional space for
all proxies also follows a multivariate distribution, which one could
then employ in more sophisticated data-science approaches.</p>
      <p id="d1e3175">We trust that considering both parts of the uncertainty enables better
and more reliable reconstruction estimates. We concede that this
procedure may exaggerate the range of potential climates and thereby may
reduce the precision of the reconstruction
<xref ref-type="bibr" rid="bib1.bibx2" id="paren.101"><named-content content-type="pre">compare also</named-content></xref>. We postulate that this, however, is
only partly due to the assumptions on uncertainty, which may transfer
uncertainty to too many records. We think it is also because the
simulation pool is not fully consistent with all the proxies
simultaneously. It is beyond the scope of the present study to
investigate whether this, in turn, is because of unreliable simulations,
lacking overlap between reconstructed and simulated climates, or lacking
reliability of the proxy records, that is, their errors.</p>
      <p id="d1e3183">With respect to the lacking precision of the reconstructions,
<xref ref-type="bibr" rid="bib1.bibx2" id="text.102"/> already identified a similar issue in their particle
filter data assimilation approach. <xref ref-type="bibr" rid="bib1.bibx2" id="text.103"/> note that in a
setup where one has only few and highly uncertain proxy predictors the
reconstruction tends to lack accuracy. We think that for the analogue
method one could remedy this by weighing the valid analogues by a
distance measure relative to the pattern of proxy predictors or by their
agreement with each individual predictor. We note that the analogue
method in the present setting may represent the recent climate worse
than simply taking the average over the period of instrumental
observations.</p>
      <p id="d1e3193">Our handling of uncertainty in terms of tolerance results in
difficulties in implementing a distance measure like the Euclidean. A
more formal definition of similarity should take into account the
multivariate and correlated nature of uncertainty: in time and across
proxies.</p>
      <p id="d1e3196">Our choice of elliptic tolerance regions may seem counterintuitive.
Mainly, two related arguments are imaginable. First, the idea can be
proposed that time and data are independent and a uniform rectangular
selection criteria could be suggested. We address this already in the
description of the method. Here, we concentrate on another argument.
Following this second argument, our uncertainty about the value should
not shrink at the border of our temporal uncertainty range but should
become wider there, as we are less confident that the data value even is
valid there. This also assumes an independence of dating and data and
their uncertainties. However, our argument for the ellipse is the
following. We regard our time-data point as sampled from a
two-dimensional distribution. If we regard this to be a uniform
distribution, we would also use a rectangular tolerance area. However,
we regard the distribution as a two-dimensional Gaussian, which can be
visualized as an ellipse in the two-dimensional plain. Thereby, the
probability density for a<?pagebreak page740?> valid point is reduced further away from the best
estimate. If our analogue pool would well sample the climate space, we
could weigh our time-data points by their likelihood within the
two-dimensional Gaussian plain. Then values that are far off in either
or both dimensions would be given less weight. However, as we have only
a rather small candidate pool, we resort to a binary criterion of
inclusion and exclusion.</p>
      <p id="d1e3199">Related to our handling of uncertainty is our approach of reconstructing
data for those years when at least one proxy predictor is dated. This
also may contribute to the wide range of the reconstructions by
neglecting information in between these dates. Alternatively, one could
pool the proxy dates into constant intervals of, for example, 100 years.
The underlying assumptions here are as strong as those in our procedure. We
note that <xref ref-type="bibr" rid="bib1.bibx48" id="text.104"/> use the published age models to interpolate
their proxy records to consistent time steps. They compare their proxies
to 10-year averages of the simulation pool. Incorporating, presumably
Bayesian, age models maximizes the available prior information used.
Nevertheless, we decide against interpolation procedures, even based on
Bayesian age models, assuming that this may result in overconfident
reconstructions. For example, interpolation could suggest more certainty
in reconstructed values where and when we have little or no proxy
information (see, e.g., Fig. <xref ref-type="fig" rid="Ch1.F8"/>i between approximately 9
and 11 kyr BP).</p>
      <p id="d1e3207">Additional assumptions relate to characteristics of the considered proxy
predictors. This includes our decision to generally compare the proxy
predictors to centennial averages of the simulation output. Thereby, we
do not allow for the fact that the proxy sensor might record
extreme-like events. Similarly, we also do not consider the differing
resolutions for each date and each location. Further, we compare the
proxy predictors and the simulation pool in terms of temperatures
instead of using surrogate proxies in proxy units from the simulation
pool. Finally, the use of temperature for the surface and for an
attributed and calibrated season does not account for the sensor-specific habitats and seasonal sensitivities or their changes
<xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx60" id="paren.105"><named-content content-type="pre">compare</named-content></xref>. That is, while we make
assumptions about, e.g., seasonality, these do not account for the
possibility that the recorder changes its seasonality adaptively
relative to environmental conditions. Our comparison is thus based on
the assumption that the proxy-inferred climate property and the proxy
record relate reasonably well to the parameter of interest (annual
surface temperature) and that, in turn, comparisons to the equivalent
simulated output are valid. In doing that, we rely on the previously
published information about the considered proxy record. Similarly, our
expansion of the temporal average reconstructions into 101-year
time series relies on the quality of the proxy data and on appropriate
assumptions on the temporal representativeness of the data. The
possibility for such a temporal downscaling is a unique feature of
analogue search reconstructions from temporal averages and of comparable
data assimilation techniques.</p>
      <p id="d1e3215">Possible improvements of the method would respect more explicitly the
irregular resolution of the proxy records and the different resolutions
between the records. Similarly, applications benefit if we can
discriminate whether a proxy sensor records mean climatic conditions or
extreme-like events. Including the proxy specific habitat and growth
season also leads to a more appropriate comparison, as does employing
proxy forward models to make the comparison in proxy units.</p>
      <p id="d1e3218">Better understanding of the proxy systems and availability of the full
simulation output data would allow for analogue searches that are more
specific for each proxy series. It further would enable the use of
locally calibrated process-based forward integrations by proxy system
models. The advent of proxy system forward models in principle allows
the production of proxy parameter representations in the virtual environment of
the simulations
<xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx102 bib1.bibx96 bib1.bibx35 bib1.bibx20 bib1.bibx22 bib1.bibx21 bib1.bibx23 bib1.bibx50 bib1.bibx26" id="paren.106"/>
but there are still gaps in the understanding of how the sensor
recording of the biological, physical, chemical, or geological process
reacts to the environment. Additionally, records may lack necessary
information. While such applications are quickly developing
<xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx50 bib1.bibx26 bib1.bibx58" id="paren.107"><named-content content-type="pre">see</named-content></xref>, data
assimilation of this kind of information is still not operational even
for the Common Era with its potentially high resolution and potentially
high-quality proxies <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx94 bib1.bibx34" id="paren.108"/>.</p>
      <p id="d1e3233">It is generally advisable to use consistent proxy parameters, a
consistent recalibration, and a consistent calibration target. This
should increase the probability of the proxy predictors constraining the
pool of potential analogues (compare the results in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>). Often such consistency is an implicit or explicit
assumption <xref ref-type="bibr" rid="bib1.bibx77" id="paren.109"><named-content content-type="pre">compare, e.g.,</named-content></xref>. On the other hand, the analogue approach, in
theory, should allow using different parameters and calibrations if the
comparison is to the same target. Indeed, ideally, it should also
compensate even a comparison of different parameters. This, however,
depends on how much proxy records indeed constrain the ultimate target
property for the reconstruction.</p>
      <p id="d1e3243">Our reconstruction is only for the approximate domain of the proxy
predictors. However, it may be possible that a set of proxy predictors
from, for example, Europe also provides information on larger-scale
climate variables. Further, we deal only with temperature
reconstructions. However, climate is more than simply temperature.
Indeed, if there is evidence that the proxy predictors are relevant
constraints on other climate fields beyond, in this example,
temperature, the pool of analogues can provide information on other
climate variables.</p>
      <p id="d1e3246">However, reconstructing other variables for hydrology or climate
dynamics depends on a sufficient number of proxy records that reliably
represent these. That is, there are two<?pagebreak page741?> conditions on the proxy records:
they have to represent the variable and there has to be enough of them.
In addition, we have to be confident that the simulation pool reliably
represents the climate variable and its spatial distribution.
Considering the number of available reliable proxies for, e.g.,
precipitation and the quality of simulations' representation of it, we
would expect that reconstruction success using the analogue method may
be worse for these other variables than for temperature
<xref ref-type="bibr" rid="bib1.bibx40" id="paren.110"><named-content content-type="pre">compare also</named-content></xref>.</p>
      <p id="d1e3254">Regarding the temporal resolution, a test of our method suggests that,
for a given assumed tolerance level, the analogue search is more
successful in finding valid analogues if we consider higher-resolution
data and less successful if we reduce the resolution of the data. That
is, the method performs slightly better in finding valid analogues when
we use 51-year averaged simulation data than when we use 101-year
averaged data, and it is even more successful in finding valid analogues
using interannual data. While such an interannual analogue search may
misinterpret what the proxy data represent, it may be a more truthful
comparison considering the potential level of environmental noise in the
proxy data relative to the targeted temperature signal.</p>
      <p id="d1e3257">Similarly, we find more valid analogues if we use less stringent
criteria in our search for valid analogues. A single best analogue
reconstruction also gives a more continuous reconstruction.</p>
      <p id="d1e3260">However, all approaches have in common that reconstruction medians as
well as reconstruction ranges are relatively constant over time. The
reconstructions show little variability and are lacking clear
differences in climate between the late and early Holocene.</p>
      <p id="d1e3264">A likely reason for the small variability in central estimates and the
generally rather constant character of our reconstructions could be that
the space of valid analogues is too unconstrained and the method labels
too many candidates as valid analogues. However, also the single best
approach shows such a behavior. That is, while the reconstruction is
undoubtedly only weakly constrained, even the best analogues differ
little between subsequent dates. Part of this may be due to our choice
to consider a rather large temporal range of influence of individual
dated records. Our ellipses of tolerance may result in a strong
influence of an unlikely value at a specific date. This could
potentially be solved by considering explicitly the likelihood of a
value at a date instead of simply taking a binary criterion. A less
complex solution could be obtained by pooling proxy values in temporal
windows, weighting them within these windows, and then performing a
reconstruction considering specific ranges of tolerance.</p>
      <p id="d1e3267">Our aim here is to use the local proxy uncertainty to select analogues.
There is a trade-off between considering the uncertainty of the proxies
and constraining the number of analogues. That is, if we want to
consider the uncertainty in the way we do, then we allow for weakly
constrained analogue ranges. If we allow different levels of proxy
uncertainty, we can choose only the best <inline-formula><mml:math id="M83" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> analogues. We, in turn,
can limit the number of analogues or weigh them by particular criteria,
e.g., based on their distance to individual proxies or their overall
Euclidean distance.</p>
      <p id="d1e3277">Beyond these methodological aspects, the size and character of the pool
of analogue candidates influence the quality of the results. Indeed,
the lacking sensitivity to differences in climate and the lacking
variability in our results may be a sign of an insufficient pool size or
an insufficient overlap between simulated climate and the environmental
conditions described by the proxy records.</p>
      <p id="d1e3280">Our results suggest that a pool including the mid-Holocene, Last Glacial
Maximum, and transient deglacial simulations does not ensure finding
valid analogues for the time period of the deglaciation and the
Holocene. An insufficient large pool of candidate analogues requires
more tolerant assumptions on uncertainty to obtain valid analogues.
Thereby, the analogues remain unconstrained. A small pool also allows
for non-uniqueness of analogues. Additionally, climatological
inconsistencies become more likely if the range of simulated periods in
the model pool is wide.</p>
      <p id="d1e3283">We do not use anomalies. If there was a large ensemble of simulations
over our period of interest, the use of anomalies would be advisable.
Similarly, if all proxy records had common modern age data, there might
be a valid anomaly building process. However, we include simulations for
time slices with notable different climatologies, and proxy records
begin at various modern dates. One solution could be a sliding
climatology for the proxies, which is added again for the final
reconstruction. We note that, if we want to apply proxy forward models
based on the calibration between measured property and temperature, we do
not use anomalies either because calibration relations frequently need
temperature on either the Celsius or Kelvin scales.</p>
      <p id="d1e3286">This section outlined a number of potential improvements of the
approach. Some of these would increase the number of necessary
computations. While the increase in costs is not prohibitive, we decided
against including such procedures here. However, it appears particularly
worthwhile to try to implement a workflow that combines feasible data-science methods, some version of simple data assimilation, and a proxy
system model framework like PRYSM
<xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx22 bib1.bibx23 bib1.bibx50" id="paren.111"/> in future attempts of
spatiotemporally resolved reconstructions if the interest is in a
dynamical understanding of the climate variability over multimillennial
timescales.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Summary and concluding remarks</title>
      <p id="d1e3301">The analogue method is a computationally cheap data assimilation
approach. Here, we discuss a specific application for time-uncertain,
sparse, and irregularly sampled proxies. We focus on the North Atlantic
sector and the time period from approximately 15 kyr BP to the late 20th
century.</p>
      <?pagebreak page742?><p id="d1e3304">The approach succeeds in providing reconstructions in a pseudo-proxy
setup for some past dates. Already, this setup highlights two potential
problems. The method may either fail to find valid analogues or provide
a wide range of potential analogues which do not necessarily include a
target climate. These problems relate to assumptions on the uncertainty
in the proxy input data.</p>
      <p id="d1e3307">The approach performs comparably for realistic proxy setups. However,
then, the analogue search often fails to find valid analogues as none of
our candidate fields comply with our criteria for a valid analogue. That
is, the method fails to provide a climate reconstruction because of a
lack of valid analogues. In the present case, this particularly occurs
over the late deglaciation and early Holocene.</p>
      <p id="d1e3310"><?xmltex \hack{\newpage}?>Furthermore, our reconstructions by analogue are generally rather
imprecise for the used proxies and a limited pool of simulation data.
The range of potential analogue values can become very wide for a given
date. Regional average reconstruction medians show little variation over
time.</p>
      <p id="d1e3315">The analogue method is non-linear and considers the spatial covariances
between the proxy records. While it lacks precision in our setup, it
nevertheless provides us with spatial field estimates of past climate
states that are consistent with the regional inter-relations as
presented by the proxy predictors.</p><?xmltex \hack{\clearpage}?>
</sec>

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

<?pagebreak page743?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Additional information on the chosen proxies and the simulation pool</title>
<sec id="App1.Ch1.S1.SS1">
  <label>A1</label><title>References for the chosen proxy records</title>

<?xmltex \floatpos{hb!}?><table-wrap id="App1.Ch1.S1.T3"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A1}?><label>Table A1</label><caption><p id="d1e3341">Additional information for the used proxy records: proxy ID, main reference, and reference for the datasets. For additional information, see Table <xref ref-type="table" rid="Ch1.T1"/>.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.88}[.88]?><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Proxy ID</oasis:entry>
         <oasis:entry colname="col2">Original publication</oasis:entry>
         <oasis:entry colname="col3">Data references</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2043</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx12" id="text.112"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx13" id="text.113"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">M39-008</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx12" id="text.114"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx13" id="text.115"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2011</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx14" id="text.116"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx44" id="text.117"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">ODP 984</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx15" id="text.118"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx16" id="text.119"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GeoB 7702-3</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx17" id="text.120"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx18" id="text.121"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IOW225517</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx32" id="text.122"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx33" id="text.123"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IOW225514</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx32" id="text.124"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx33" id="text.125"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">M25/4-KL11</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx31" id="text.126"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx30" id="text.127"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">AD91-17</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx39" id="text.128"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx38" id="text.129"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake 850</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx61" id="text.130"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx62" id="text.131"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Lake Nujulla</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx61" id="text.132"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx62" id="text.133"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MD95-2015</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx66" id="text.134"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx45" id="text.135"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">D13882</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx78" id="text.136"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx79" id="text.137"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GIK23258-2</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx81" id="text.138"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx82" id="text.139"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Flarken Lake</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx87" id="text.140"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx91" id="text.141"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Tsuolbmajavri Lake</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx86" id="text.142"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx91" id="text.143"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RAPID-12-1K</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx97" id="text.144"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx98" id="text.145"/></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GeoB 5901-2</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx55" id="text.146"/></oasis:entry>
         <oasis:entry colname="col3"><xref ref-type="bibr" rid="bib1.bibx56" id="text.147"/></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <p id="d1e3630">Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/> provides references to the original publications
for the individual proxy records. The table further adds references to
the datasets directly and thereby the repositories where the records are
available.</p>
</sec>
<sec id="App1.Ch1.S1.SS2">
  <label>A2</label><title>Additional information on the simulation pool</title>
      <p id="d1e3643">Table <xref ref-type="table" rid="App1.Ch1.S1.T4"/> provides references for the various models from
which we include simulations in the candidate pool. The table further
gives links to the repositories where interested researchers can obtain
the simulation data.</p>

<?xmltex \floatpos{hb!}?><table-wrap id="App1.Ch1.S1.T4"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A2}?><label>Table A2</label><caption><p id="d1e3652">Additional information about the pool of simulation data: model name, main reference, and link to the provider of the data. For additional information, see Table <xref ref-type="table" rid="Ch1.T2"/>.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.88}[.88]?><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">References</oasis:entry>
         <oasis:entry colname="col3">Link (last access for all links cited in this table: 22 March 2021)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx107" id="text.148"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">COSMOS-ASO</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx11" id="text.149"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO-Mk3L-1-2</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx74" id="text.150"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx85" id="text.151"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadCM3</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx19" id="text.152"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-CC</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx49" id="text.153"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-ES</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx49" id="text.154"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx28" id="text.155"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx37" id="text.156"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://esgf-data.dkrz.de/</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx73" id="text.157"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://www.earthsystemgrid.org/dataset/ucar.cgd.ccsm4.CESM_CAM5_LME.html</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CCSM3</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx64" id="text.158"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://www.earthsystemgrid.org/project/trace.html</uri></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx53" id="text.159"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://cera-www.dkrz.de/WDCC/ui/cerasearch/project?acronym=MILLENNIUM_COSMOS</uri></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3</oasis:entry>
         <oasis:entry colname="col2"><xref ref-type="bibr" rid="bib1.bibx89" id="text.160"/></oasis:entry>
         <oasis:entry colname="col3"><uri>https://catalogue.ceda.ac.uk/uuid/a43dcfaccfae4824ab9ab2b572703e72</uri></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?pagebreak page744?><p id="d1e3870"><?xmltex \hack{\clearpage}?>Table <xref ref-type="table" rid="App1.Ch1.S1.T5"/> complements Tables <xref ref-type="table" rid="Ch1.T2"/> and <xref ref-type="table" rid="App1.Ch1.S1.T4"/>. They give the simulation IDs that
allow finding the simulations more easily in the repositories.</p>

<?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S1.T5"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A3}?><label>Table A3</label><caption><p id="d1e3885">Information on individual simulations: model, simulation, and period.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">Simulation ID</oasis:entry>
         <oasis:entry colname="col3">Period</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CNRM-CM5</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">COSMOS-ASO</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CSIRO-Mk3L-1-2</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p150</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p151</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p121</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p122</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p1221</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p123</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p124</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p125</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p126</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p127</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">GISS-E2-R</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p128</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadCM3</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-CC</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HadGEM2-ES</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">IPSL-CM5A-LR</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">lgm_r1i1p2</oasis:entry>
         <oasis:entry colname="col3">Last Glacial Maximum</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">midHolocene_r1i1p2</oasis:entry>
         <oasis:entry colname="col3">Mid-Holocene</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-P</oasis:entry>
         <oasis:entry colname="col2">past1000_r1i1p1</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">0850cntl.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Pre-industrial control</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">002.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">004.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">005.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">006.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">007.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">008.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">009.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">010.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">011.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">012.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">013.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">850forcing.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">GHG.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">GHG.002.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">GHG.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">LULC_HurttPongratz.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">LULC_HurttPongratz.002.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">LULC_HurttPongratz.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S1.T6"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A3}?><label>Table A3</label><caption><p id="d1e4506">Continued.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Model</oasis:entry>
         <oasis:entry colname="col2">Simulation ID</oasis:entry>
         <oasis:entry colname="col3">Period</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">ORBITAL.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">ORBITAL.002.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">ORBITAL.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">OZONE_AER.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">1850–2005 CE</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">SSI_VSK_L.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">SSI_VSK_L.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">SSI_VSK_L.004.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">SSI_VSK_L.005.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">VOLC_GRA.001.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">VOLC_GRA.002.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">VOLC_GRA.003.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">VOLC_GRA.004.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CESM1</oasis:entry>
         <oasis:entry colname="col2">VOLC_GRA.005.cam.h0</oasis:entry>
         <oasis:entry colname="col3">Last millennium</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CCSM3</oasis:entry>
         <oasis:entry colname="col2">trace</oasis:entry>
         <oasis:entry colname="col3">LGM to present</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">mil0001</oasis:entry>
         <oasis:entry colname="col3">Pre-industrial control</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">mil0006</oasis:entry>
         <oasis:entry colname="col3">Last millennium up 2005 CE</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">mil0021</oasis:entry>
         <oasis:entry colname="col3">Last millennium to 2100 CE</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">mil0025</oasis:entry>
         <oasis:entry colname="col3">Last millennium to 2100 CE</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">MPI-ESM-Cosmos</oasis:entry>
         <oasis:entry colname="col2">mil0026</oasis:entry>
         <oasis:entry colname="col3">Last millennium to 2100 CE</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3 (accelerated)</oasis:entry>
         <oasis:entry colname="col2">ALL-5G</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3 (accelerated)</oasis:entry>
         <oasis:entry colname="col2">GHG</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3 (accelerated)</oasis:entry>
         <oasis:entry colname="col2">ORB</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3 (accelerated)</oasis:entry>
         <oasis:entry colname="col2">ALL-ZH</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">FAMOUS-HadCM3 (accelerated)</oasis:entry>
         <oasis:entry colname="col2">ICE</oasis:entry>
         <oasis:entry colname="col3">Last glacial cycle</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

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

      <p id="d1e4837">We provide lists of valid analogues per date and
experiment at <ext-link xlink:href="https://doi.org/10.17605/OSF.IO/PJ9EG" ext-link-type="DOI">10.17605/OSF.IO/PJ9EG</ext-link> <xref ref-type="bibr" rid="bib1.bibx5" id="paren.161"/>. This allows identifying valid
climate states for dates. We also provide files for area mean analogue
ranges and medians.</p>

      <p id="d1e4846">The proxy data we use are available from the Supplement of
<xref ref-type="bibr" rid="bib1.bibx67" id="text.162"/> at <ext-link xlink:href="https://doi.org/10.1126/science.1228026" ext-link-type="DOI">10.1126/science.1228026</ext-link>
(see also <uri>https://science.sciencemag.org/content/suppl/2013/03/07/339.6124.1198.DC1</uri>, last access: 30 December 2019). Primary data citations are from
Cacho et al. (<xref ref-type="bibr" rid="bib1.bibx13" id="year.163"/>, <uri>https://www.ncdc.noaa.gov/paleo-search/study/6374</uri>, last access:
13 January 2020), Grimalt and Calvo (<xref ref-type="bibr" rid="bib1.bibx44" id="year.164"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.438810" ext-link-type="DOI">10.1594/PANGAEA.438810</ext-link>), Came et al. (<xref ref-type="bibr" rid="bib1.bibx16" id="year.165"/>, <uri>https://www.ncdc.noaa.gov/paleo-search/study/5593</uri>, last access:
13 January 2020),
Castañeda et al. (<xref ref-type="bibr" rid="bib1.bibx18" id="year.166"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.736909" ext-link-type="DOI">10.1594/PANGAEA.736909</ext-link>),
Emeis et al. (<xref ref-type="bibr" rid="bib1.bibx33" id="year.167"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.738458" ext-link-type="DOI">10.1594/PANGAEA.738458</ext-link>),
Emeis et al. (<xref ref-type="bibr" rid="bib1.bibx30" id="year.168"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.735959" ext-link-type="DOI">10.1594/PANGAEA.735959</ext-link>),
Giunta and Emeis (<xref ref-type="bibr" rid="bib1.bibx38" id="year.169"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.438366" ext-link-type="DOI">10.1594/PANGAEA.438366</ext-link>),
Larocque and Hall (<xref ref-type="bibr" rid="bib1.bibx62" id="year.170"/>, <uri>https://www.ncdc.noaa.gov/paleo-search/study/6349</uri>, last access:
13 January 2020),
Grimalt and Marchal (<xref ref-type="bibr" rid="bib1.bibx45" id="year.171"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.438814" ext-link-type="DOI">10.1594/PANGAEA.438814</ext-link>),
Rodrigues et al. (<xref ref-type="bibr" rid="bib1.bibx79" id="year.172"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.761811" ext-link-type="DOI">10.1594/PANGAEA.761811</ext-link>),
Sarnthein et al. (<xref ref-type="bibr" rid="bib1.bibx82" id="year.173"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.114683" ext-link-type="DOI">10.1594/PANGAEA.114683</ext-link>),
Sundqvist et al. (<xref ref-type="bibr" rid="bib1.bibx91" id="year.174"/>, <uri>https://www.ncdc.noaa.gov/paleo-search/study/15444</uri>, last access:
13 January 2020),
Thornalley et al. (<xref ref-type="bibr" rid="bib1.bibx98" id="year.175"/>, <uri>https://www.ncdc.noaa.gov/paleo-search/study/8623</uri>, last access:
13 January 2020), and
Kim et al. (<xref ref-type="bibr" rid="bib1.bibx56" id="year.176"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.438384" ext-link-type="DOI">10.1594/PANGAEA.438384</ext-link>). Regarding
<xref ref-type="bibr" rid="bib1.bibx91" id="text.177"/>, please refer also to Digerfeldt (<xref ref-type="bibr" rid="bib1.bibx25" id="year.178"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.740343" ext-link-type="DOI">10.1594/PANGAEA.740343</ext-link>, <xref ref-type="bibr" rid="bib1.bibx24" id="year.179"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.711884" ext-link-type="DOI">10.1594/PANGAEA.711884</ext-link>) and Voeltzel (<xref ref-type="bibr" rid="bib1.bibx105" id="year.180"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.740821" ext-link-type="DOI">10.1594/PANGAEA.740821</ext-link>, <xref ref-type="bibr" rid="bib1.bibx106" id="year.181"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.739916" ext-link-type="DOI">10.1594/PANGAEA.739916</ext-link>). Please see also Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>.
Simulation data are available from a number of sources. Data from simulations for PMIP3 can be obtained from the Earth System Grid Federation, e.g., at the node <uri>https://esgf-data.dkrz.de/projects/esgf-dkrz/</uri> (last access: 22 March 2021, ESGF, 2021). Last millennium ensemble data and TraCE-21ka output are available at <uri>https://www.earthsystemgrid.org/</uri> (last access: 22 March 2021, NCAR, 2021). Millennium COSMOS simulation data are best accessed via <uri>https://cera-www.dkrz.de/WDCC/ui/cerasearch/project?acronym=MILLENNIUM_COSMOS</uri> (last access: 22 March 2021, <xref ref-type="bibr" rid="bib1.bibx53" id="altparen.182"/>, <ext-link xlink:href="https://doi.org/10.5194/cp-6-723-2010" ext-link-type="DOI">10.5194/cp-6-723-2010</ext-link>). Quaternary QUEST data may be obtained via <uri>https://catalogue.ceda.ac.uk/uuid/a43dcfaccfae4824ab9ab2b572703e72</uri> (last access: 30 December 2019, <xref ref-type="bibr" rid="bib1.bibx63" id="altparen.183"/>). Please see also Table <xref ref-type="table" rid="App1.Ch1.S1.T4"/>.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e5005">OB designed and conducted the study and was the main
author. Both authors discussed the methods, the results, and their
implications.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e5011">The authors declare that they have no conflict of
interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e5017">This article is part of the special issue “Paleoclimate data synthesis and analysis of associated uncertainty (BG/CP/ESSD inter-journal SI)”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e5023">Funding for this research is by the German Federal Ministry of Education
and Research (BMBF) within the Research for Sustainability initiative
(FONA; <uri>https://www.fona.de/</uri>, last access: 22 March 2021) through the first and second phases of the
PalMod project (FKZ: 01LP1509A, FKZ: 01LP1926B). Discussions with
Marlene Klockmann and Sebastian Wagner helped to improve the manuscript.
We thank the two reviewers and the editor for their valuable comments.
We acknowledge the World Climate Research Programme, which coordinated and promoted the Coupled Model Intercomparison Project (CMIP). We thank the climate modelling groups for producing and making available their model output, the Earth System Grid Federation (ESGF) for archiving the data and providing access, and the multiple funding agencies who support CMIP and ESGF.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e5031">This research has been supported by the Bundesministerium für Bildung und Forschung (grant nos. 01LP1509A and 01LP1926B).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>The article processing charges for this open-access <?xmltex \notforhtml{\newline}?> publication  were covered by a Research <?xmltex \notforhtml{\newline}?> Centre of the Helmholtz Association.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e5044">This paper was edited by Lukas Jonkers and reviewed by two anonymous referees.</p>
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    <!--<article-title-html>Technical note: Considerations on using uncertain proxies in the analogue method for spatiotemporal reconstructions of millennial-scale climate</article-title-html>
<abstract-html><p>Inferences about climate states and climate variability of the Holocene
and the deglaciation rely on sparse paleo-observational proxy data.
Combining these proxies with output from climate simulations is a means
for increasing the understanding of the climate throughout the last tens
of thousands of years. The analogue method is one approach to do this.
The method takes a number of sparse proxy records and then searches
within a pool of more complete information (e.g., model simulations) for
analogues according to a similarity criterion. The analogue method is
non-linear and allows considering the spatial covariance among proxy
records.</p><p>Beyond the last two millennia, we have to rely on proxies that are not
only sparse in space but also irregular in time and with considerably
uncertain dating. This poses additional challenges for the analogue
method, which have seldom been addressed previously. The method has to
address the uncertainty of the proxy-inferred variables as well as the
uncertain dating. It has to cope with the irregular and non-synchronous
sampling of different proxies.</p><p>Here, we describe an implementation of the analogue method including a
specific way of addressing these obstacles. We include the uncertainty
in our proxy estimates by using <q>ellipses of tolerance</q> for tuples
of individual proxy values and dates. These ellipses are central to our
approach. They describe a region in the plane spanned by proxy dimension
and time dimension for which a model analogue is considered to be
acceptable. They allow us to consider the dating as well as the data
uncertainty. They therefore form the basic criterion for selecting valid
analogues.</p><p>We discuss the benefits and limitations of this approach. The results
highlight the potential of the analogue method to reconstruct the
climate from the deglaciation up to the late Holocene. However, in the
present case, the reconstructions show little variability of their
central estimates but large uncertainty ranges. The reconstruction by
analogue provides not only a regional average record but also allows
assessing the spatial climate field compliant with the used proxy
predictors. These fields reveal that uncertainties are also locally
large. Our results emphasize the ambiguity of reconstructions from
spatially sparse and temporally uncertain, irregularly sampled proxies.</p></abstract-html>
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