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What can Palaeoclimate Modelling do for you?

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In modern environmental and climate science it is necessary to assimilate observational datasets collected over decades with outputs from numerical models, to enable a full understanding of natural systems and their sensitivities. During the twentieth and twenty-first centuries, numerical modelling became central to many areas of science from the Bohr model of the atom to the Lorenz model of the atmosphere. In modern science, a great deal of time and effort is devoted to developing, evaluating, comparing and modifying numerical models that help us synthesise our understanding of complex natural systems. Here we provide an assessment of the contribution of past (palaeo) climate modelling to multidisciplinary science and to society by answering the following question: What can palaeoclimate modelling do for you? We provide an assessment of how palaeoclimate modelling can develop in the future to further enhance multidisciplinary research that aims to understand Earth’s evolution, and what this may tell us about the resilience of natural and social systems as we enter the Anthropocene.
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Earth Systems and Environment
https://doi.org/10.1007/s41748-019-00093-1
ORIGINAL ARTICLE
What can Palaeoclimate Modelling doforyou?
A.M.Haywood1 · P.J.Valdes2· T.Aze1· N.Barlow1· A.Burke3· A.M.Dolan1· A.S.vonderHeydt4· D.J.Hill1·
S.S.R.Jamieson5· B.L.Otto‑Bliesner6· U.Salzmann7· E.Saupe8· J.Voss9
Received: 19 March 2019 / Accepted: 13 April 2019
© The Author(s) 2019
Abstract
In modern environmental and climate science it is necessary to assimilate observational datasets collected over decades with
outputs from numerical models, to enable a full understanding of natural systems and their sensitivities. During the twentieth
and twenty-first centuries, numerical modelling became central to many areas of science from the Bohr model of the atom
to the Lorenz model of the atmosphere. In modern science, a great deal of time and effort is devoted to developing, evalu-
ating, comparing and modifying numerical models that help us synthesise our understanding of complex natural systems.
Here we provide an assessment of the contribution of past (palaeo) climate modelling to multidisciplinary science and to
society by answering the following question: What can palaeoclimate modelling do for you? We provide an assessment of
how palaeoclimate modelling can develop in the future to further enhance multidisciplinary research that aims to understand
Earth’s evolution, and what this may tell us about the resilience of natural and social systems as we enter the Anthropocene.
Keywords Climate· Model· Palaeoclimate· Global change· Environmental change· Earth history
1 Introduction
Complex climate models, and latterly Earth System Models
(ESMs), are in the vanguard of attempts to assess the effects,
risks and potential impacts associated with the anthropo-
genic emission of greenhouse gases (GHG: IPCC 2013).
Climate predictions underpin scientific assessments of miti-
gation and societal adaptation pathways (IPCC 2013).
The use of models to understand the evolution of our
planet’s climate, environment and life (Fig.1), collectively
known as past (palaeo) climate modelling, has matured in
its capacity and capability since the first simulations using
a General Circulation Model (GCM) were published in the
1970s for the Last Glacial Maximum (e.g., Gates 1976).
Since then it has become apparent that to fully appreciate the
complex interactions between climate and the environment,
and to use this knowledge to address societal challenges, it
is necessary to adopt multidisciplinary scientific approaches
capable of robustly testing long-standing hypotheses that
describe the sensitivity/resilience of our planet and the life
forms that inhabit it. Multidisciplinary studies have provided
unique ways of evaluating the efficacy of climate and ESM
predictions in reproducing large-scale climate changes that
occurred in the past (Haywood etal. 2013), and this has
* A. M. Haywood
earamh@leeds.ac.uk
1 School ofEarth andEnvironment, University ofLeeds,
Woodhouse Lane, LeedsLS29JT, UK
2 School ofGeographical Sciences, University ofBristol,
University Road, BristolBS81SS, UK
3 Laboratoire d’Ecomorphologie et de Paleoanthropologie,
Universite de Montreal, Departement d’Anthropologie,
C.P. 6128, Centre-Ville, Montreal, QCH3C3J7, Canada
4 Department ofPhysics, Centre forComplex Systems Science,
Utrecht University, Princetonplein 5, 3584CCUtrecht,
TheNetherlands
5 Department ofGeography, Durham University, South Road,
DurhamDH13LE, UK
6 Climate andGlobal Dynamics Laboratory, National Center
forAtmospheric Research, 1850 Table Mesa Drive, Boulder,
CO80305, USA
7 Department ofGeography andEnvironmental Sciences,
Northumbria University, Newcastle City Campus, 2 Ellison
Place, NewcastleuponTyneNE18ST, UK
8 Department ofEarth Sciences, University ofOxford, South
Parks Road, OxfordOX13AN, UK
9 School ofMathematics, University ofLeeds, Woodhouse
Lane, LeedsLS29JT, UK
A.M.Haywood et al.
1 3
provided valuable out-of-sample tests for the tools used to
predict future climate and environmental change.
The march towards multidisciplinary assessment of past
climate and environmental states has accelerated through the
construction of models that have more complete representa-
tions of the Earth system at higher spatial resolution. From
relatively simple three-dimensional representations of the
atmosphere, models have developed to include representa-
tions of the oceans and land cover, and incorporate the inter-
actions between atmosphere, oceans, and the land and ice
sheets. They have developed to enable dynamic simulation
of the distribution of past vegetation cover, ice sheet distri-
bution and variability, and ocean/terrestrial biogeochemical
cycles (Prinn 2013). Each development has brought with
it opportunities to form new research collaborations with
observational-based scientists to test hypotheses for Earth
evolution in novel and exciting ways, and to relate this
knowledge towards addressing societal challenges.
Whilst some of the contributions made by palaeoclimate
modelling to wider research efforts are obvious, the util-
ity of, and access to, model simulations has grown to such
a degree that many of the connections between palaeocli-
mate modelling and other disciplines are not appreciated.
Unsurprisingly, the way in which palaeoclimate modelling
addresses societal needs, as generally expressed through
UN SDGs and scientific grand challenges, is not fully
appreciated either. Here we address this issue through the
exploration of palaeoclimate modelling’ s (using complex
numerical models) contribution to the better understanding
of climate sensitivity, data-model comparison and geological
proxy interpretation, life and its resiliency, glacial and sea-
level history, hydrology, anthropology and natural resource
exploration as well as energy-based research. We also dis-
cuss potential avenues for the future that have the capability
to enhance the contribution of palaeoclimate modelling to
other disciplines and to better address societal needs.
2 The Climate Sensitivity Grand Challenge
Studies of climate sensitivity quantify changes in global
mean temperature in response to variations in atmospheric
CO2 concentration. The concept of equilibrium climate
states has been crucial in this respect. Equilibrium Climate
Sensitivity (ECS) is the temperature difference in response
to a doubling of CO2, where the climate is assumed to be
in equilibrium before and after the CO2 perturbation (e.g.,
Von der Heydt etal. 2016). An important aim of quantifying
Fig. 1 Global annual mean temperature variation of the Earth through
time (last 400 million years) predicted by the Hadley Centre Coupled
Climate Model version 3 (HadCM3), compared with geologically
derived estimates of temperature variability over the same period [the
Royer etal. 2004 temperature record, the Zachos etal. 2008; Lisiecki
and Raymo 2005 benthic oxygen isotope stack, as well as the EPICA
and NGRIP ice core records; Jouzel et al. 2007 and NGRIP Mem-
bers 2004. Geological epochs include the Devonian (D), Carbon-
iferous (C) Permian (P), Triassic (Tr), Jurassic (J) Cretaceous (K),
Eocene (Eoc), Oligocene (Oli.), Miocene (Mio), Pliocene and Pleis-
tocene (Pleist.)] Future predictions of temperature change are based
on HadCM3 simulations using different Representative Concentration
Pathways (RCPs). Horizontal blue lines represent geological evidence
for ice sheets in the northern (NH) and southern (SH) hemispheres.
Major evolutionary characteristics and events over the last 400 mil-
lion years represented by cartoon silhouettes
What can Palaeoclimate Modelling doforyou?
1 3
ECS has always been to predict future climate change, where
ECS plays a role in quantifying the expected warming in
the year 2100. Moreover, in view of recent plans to limit
future global warming to between 1.5 and 2°C (Paris Agree-
ment), establishing ECS is crucial to determining how to
cap greenhouse gas emissions to limit warming to within
this range and contribute to objectives described under the
climate action SDG.
In addition to the direct radiative effect caused by a
change in CO2 concentration, surface temperature responds
to feedbacks operating in the climate system. These feed-
backs can act on different timescales and amplify (or
dampen) the initial temperature change as a result of CO2
forcing. Certain fast(er) feedback processes, such as surface
albedo-temperature feedbacks, tend to lead to an amplified
climate response to CO2-induced radiative forcing. ECS esti-
mates have mostly been derived using climate models that
represent fast(er) feedbacks, where fast means fast enough
to approach an equilibrium climate state within a century.
Together with observations of the instrumental period,
ECS incorporating fast(er) feedbacks is estimated to range
between 1.5 and 4.5°C (Solomon 2007). This range has
changed little since the first estimates of ECS (Charney etal.
1979).
However, since 1979 our scientific understanding of the
stability of ECS, and how slow(er) feedbacks may alter
it, has grown substantially. This is in no small part due to
palaeoclimate modelling. The concept of longer term cli-
mate sensitivity, or Earth system sensitivity, emerged from
studying the way climate varied in response to variations
in atmospheric CO2 concentration (Hansen etal. 2008).
One of the most salient observations made by palaeocli-
matology is that the magnitude of reconstructed climate
change in the past can be hard to reconcile with the abso-
lute CO2 forcing at a given time, and from fast(er) climate
feedbacks alone. This draws attention to an important
limitation of a scientific focus that is restricted to mod-
ern and recent climate states, as it is incapable of provid-
ing the kind of broader perspective needed to determine
how climate responds to CO2 forcing in the longer term
(multi-centennial to millennial timescales). It has been
possible to reconcile the magnitude of past climate change
to direct CO2 forcing, in part by considering the contri-
bution to temperature change that can be derived from
slower responding components of the Earth system, such
as the response of ice sheets and vegetation cover (Hansen
etal. 2008; Lunt etal. 2010a; Rohling etal. 2012; Hay-
wood etal. 2013). In addition, palaeoclimate modelling
has highlighted that ECS itself may not be a constant. The
nature of the climate system, which can affect feedback
processes, may influence how the surface temperature
responds to CO2-based forcing. However, the degree to
which ECS variations according to base state are influ-
enced by the specific model chosen remains unknown. As
such, palaeoclimate modelling has made an important con-
tribution towards understanding the complexity of deriv-
ing ECS. More broadly, it is helping us to understand how
the sensitivity of global temperature to CO2 variation may
have changed in the past in response to the first order con-
trols of palaeogeography (see Fig.2).
Fig. 2 Global mean annual surface air temperature as a function of
atmospheric CO2 simulated by the Community Climate Model Ver-
sion 4 (CCSM4) at the National Center for Atmospheric Research.
Red dots show the simulated global temperature response to rising
CO2 concentration based when using modern geography, ice sheets
and vegetation in the model. Green dots show the simulated global
temperature response to rising CO2 concentration when using modern
geography, Pliocene ice sheets and vegetation in the model. Blue dots
show the simulated global temperature response to rising CO2 con-
centration when using Eocene or Cretaceous geography, no ice sheets
and prescribed palaeo vegetation (Bitz etal. 2012; Brady etal. 2013;
Baatsen etal. 2018; Tabor etal. 2016; Feng etal. 2017)
A.M.Haywood et al.
1 3
3 Model/Data Comparison: Veracities,
Uncertainties andSynergies
Proxy data-based environmental reconstructions play a
central role in evaluating the ability of climate models to
simulate past, present and future climate change. Over the
last few decades, several paleoclimate modelling intercom-
parison projects have provided compilations of terrestrial
and marine biological and geochemical data to facilitate
global data-model comparisons for different time intervals
in Earth history (e.g., Kageyama etal. 2018). For qualita-
tive and quantitative comparison, climate models are either
used in “forward mode” (i.e., models are capable of simulat-
ing proxy systems, such as biomes or isotopes) or “inverse
mode” where proxy data measurements are translated into
the same climatological values produced by climate mod-
els (temperature/precipitation, etc.). One of the greatest
strengths of palaeoclimate simulations is their ability to
provide process-based explanations for past environmental
change. Testing the importance of feedback mechanisms
through palaeoclimate modelling was a major step towards
identifying and understanding non-linear responses of
the environment to climate change. A prominent example
includes the analysis of vegetation, ocean and soil feed-
backs simulated in palaeoclimate models to understand
the strong response of the African monsoon and associated
rapid “greening” of the Sahara during the Holocene Afri-
can Humid Period (AHP). The AHP is recorded in mul-
tiple archaeological and geological records, but cannot be
explained by orbital forcing alone (Claussen etal. 1999;
Tjallingii etal. 2008; Tierney etal. 2017).
The majority of data-model comparison studies have
focused on the most recent geological past (such as the
AHP), and their outcomes and benefits for the understand-
ing of Holocene and Pleistocene environments have been
discussed elsewhere (Braconnot etal. 2012; Harrison etal.
2016). However, palaeoclimate modelling has also improved
our understanding of warm climates in the deeper geological
past, which were primarily controlled by elevated green-
house gas concentrations, providing an additional framework
for understanding future climate change. Whilst pre-Qua-
ternary warm climates hold the key to understanding how
environments respond to CO2-induced warming in the long
term, the uncertainties in defining geological boundary con-
ditions and reconstructing past environments increase with
geological age. Furthermore, disagreements between climate
model simulations and available geological data in the polar
regions remain, with models underestimating the degree of
warming (e.g., Masson-Delmotte etal. 2006; Haywood etal.
2013; Huber and Caballero 2011; Dowsett 2013).
The analysis of congruence between proxy data and
model simulations is of mutual benefit in that it has the
potential to improve the assessment of model performance,
and the robustness of proxy data-based environmental
reconstructions. Data assimilation, which incorporates
observations into numerical modelling, have been shown
to be a promising new technique in pre-Quaternary global
biome mapping projects to regionally improve model sim-
ulations and to increase the spatial and temporal resolution
of data-based vegetation reconstructions (Salzmann etal.
2008; Pound etal. 2012). In addition, the resolution of
the so-called “cool tropics paradox” is a prominent exam-
ple where palaeoclimate model outputs challenged sea
surface temperature (SST) estimates (e.g., D’Hondt and
Arthur 1996). Early estimates of tropical SSTs for the Cre-
taceous were far cooler than climate model simulations.
However, newer exceptionally well-preserved Palaeogene
microfossils (Sexton etal. 2006) led to a revision to higher
estimated SSTs bringing greater agreement between the
data and model estimates of tropical SSTs (Pearson etal.
2001). Furthermore, a long-standing discrepancy between
model simulations of atmospheric CO2 (pCO2), ice sheet
extent and the geological record of ice sheet and sea-level
variability during the icehouse of the Palaeozoic (330Ma)
prompted the generation of new high-resolution proxy
records of pCO2 that reconcile the geological archives and
model outputs (Montanez etal. 2016).
The spatial and temporal resolution, and accuracy of deep
time, pre-Quaternary reconstructions, have significantly
improved as science has progressed. The outputs from vari-
ous new international pre-Quaternary model intercompari-
son initiatives, for example, PlioMIP (Haywood etal. 2016)
and DeepMIP (Lunt etal. 2017) and proxy data syntheses,
for example, PlioVar PAGES (McClymont etal. 2015) and
PRISM3 (Dowsett etal. 2016) now enable reconstructions
of terrestrial and marine environmental change over multiple
time intervals during the last 65 million years at a global
scale (see Fig.3). Coincidentally, an increasing number
of exceptionally dated, high-resolution deep-time geologi-
cal records spanning several millions of years are becom-
ing available (Brigham-Grette etal. 2013; Herbert etal.
2015; Panitz etal. 2018). These allow, for the first time,
combined model-data approaches to analyse the role and
importance of climate extremes, astronomical cycles, non-
linear responses and feedback mechanisms, and non-modern
analogue environments.
4 Palaeoclimate Modelling
andUnderstanding Life onEarth: Past,
Present andFuture
There is increasing concern over how Earth’s biota will
respond to the rapid climatic changes already underway
(Urban 2015; Thomas etal. 2004; Barnosky etal. 2011).
What can Palaeoclimate Modelling doforyou?
1 3
These concerns are highlighted in the UN Sustainability
Goals of preserving and protecting biodiversity for the
maintenance of ecosystem goods and services, both on land
and in the water. However, preservation and maintenance
of biodiversity rely on accurate understanding and predic-
tions of climate-life dynamics on both short and long time
scales (Finnegan etal. 2015; McKinney 1997; Dawson etal.
2011). Species’ interactions with climate on longer time
scales provide necessary insights into biotic responses to
differing rates of environmental change, non-analogue cli-
mate scenarios, and extreme warmth (Barnosky etal. 2011;
Finnegan etal. 2015; Williams and Jackson 2007), all of
which have relevance to changes that are occurring today
(Williams etal. 2007).
Predictive models of biotic responses to climate change
can be sourced from the integration of fossils and palaeocli-
mate data. Palaeoclimate models are essential to disentangle
biotic responses to climate change, because they provide a
spatially explicit framework in which to test hypotheses. In
a perfect world, science would have access to palaeo-proxy
data that provide accurate estimates of past environmental
conditions for every point on Earth throughout Earth history.
In reality, palaeo-proxy data are spatially discontinuous, and
while it can provide robust palaeoenvironmental constraints
on local scales, it is often temporally limited. To generate
longer term environmental records, data are compiled such
that they represent globally averaged signals (e.g., Zachos
etal. 2008), and thus it can be challenging to disentangle the
causal processes responsible for regional biological patterns
from such global compilations.
Palaeoclimate models fill proxy data-deficient gaps, pro-
viding higher resolution spatial and temporal constraints on
the biotic responses to climate. When coupled with eco-
logical niche modelling (ENM: Myers etal. 2015; Peterson
etal. 2011; Svenning etal. 2011), palaeoclimate models also
provide critical insight on both the rate at which species are
Fig. 3 Distribution of biomes
as displayed on a hypothetical
“supercontinent” (after Troll
1948) for present-day (after
Klink 2008) and the geologi-
cal past. The distribution was
created through combination of
vegetation simulation informed
by palaeoclimate simulations
as well as palaeobotanical data
to create a spatial reconstruc-
tion of global vegetation for
the Miocene (Tortonian; Pound
etal. 2011), the Pliocene (Pia-
cenzian; Salzmann etal. 2008)
and the Last Glacial Maximum;
Kageyama etal. 2012; Tarasov
etal. 2000)
A.M.Haywood et al.
1 3
able to respond to changing conditions, and on those species
most vulnerable to them. The record of responses to differ-
ing rates of environmental change in the past is capable of
elucidating whether a given species can survive the rapid
and unprecedented rate of present-day climate change via
either adaptation and/or environmental range shifts (Dawson
etal. 2011; Harrison and Prentice 2003; Davis and Shaw
2001; Parmesan and Yohe 2003; Chen etal. 2011; Saupe
etal. 2014; Lawing and Polly 2011). Palaeoclimate models
can also be used to estimate a species’ traits, such as their
abiotic niches, to examine whether these traits result in dif-
ferential extinction risk (Saupe etal. 2015) and to question
the role of climate in influencing evolutionary, ecological
and biogeochemical processes at varying spatial and tem-
poral scales (e.g., Svenning etal. 2015). Such models have
been used to study the co-evolution of Earth and life, with
focus on how climate regulates the tempo and mode of spe-
ciation, extinction and adaptation. Examples in the latter
category include work that aims to quantify rates of within-
lineage abiotic niche evolution (Saupe etal. 2014; Jackson
and Blois 2015; Stigall 2014; Veloz etal. 2012), also of
relevance to the UN goal of conserving biodiversity.
Palaeoclimate models have the ability to contribute to
debates regarding the role of climate in regulating past biotic
events, particularly major extinctions. For example, the late
Pleistocene and early Holocene witnessed the extinction of
more than 97 genera of megafauna (animals > 44kg; Bar-
nosky etal. 2004), but the kill mechanism(s) for this event
are debated. Over hunting by humans and climate change
have been proposed as the two primary mechanisms (Sven-
ning etal. 2011), and the latter hypothesis has been tested
by climate models, helping to produce estimates of the
degree to which suitable habitats for various taxa changed
as climate warmed. Results are variable, with some studies
finding available habitat increased for taxa (Martinez-Meyer
etal. 2004; Varela etal. 2010) and others finding that it
decreased (Nogués-Bravo etal. 2008), potentially reflect-
ing where each taxa was distributed latitudinally (Svenning
etal. 2011).
Ecological patterns and processes may also be influenced
by climate, and palaeoclimate models can test the extent to
which climate controls patterns of distribution, dispersal,
community composition and assembly (Lawing and Polly
2011; Gavin etal. 2014). Moritz etal. (2009), for example,
used palaeoclimate models to examine the origins of a suture
zone—shared regions of secondary contact between long-
isolated lineages—in the Australian Wet Tropics rainforest.
The authors found that the zones of contact were clustered
in a corridor between two major Quaternary refugia, sug-
gesting it was unsuitable for the species during the mid-
Holocene, and that the current suture zone was established
only within the last few 1000 years.
Understanding how climate regulates the biological con-
trols of major element cycling, in particular carbon, is of
critical importance for accurate estimations of the effects
of elevated atmospheric CO2 on global temperatures, natu-
ral carbon sources and sinks, future ocean chemistry and
ecosystem responses (e.g., Cox etal. 2000; Le Quéré etal.
2009; Sarmiento etal. 2004). The palaeontological perspec-
tive allows us to ground truth our understanding of these
systems. At the broadest scale Earth System Models of Inter-
mediate Complexity (EMICs), or even simpler models, have
been used to investigate the impact major biological innova-
tions such as evolution of photosynthesis ~ 2.5 billion years
ago on ocean chemistry (Lenton and Daines 2017), and the
colonisation of the land by plants and its effect on weather-
ing and atmospheric CO2 (Berner 1998). The integration of
biogeochemical processes into palaeoclimate models also
allows us to reconstruct the influence of changing climate
and biogeochemistry on shorter timescales and gain a greater
understanding of thresholds, sensitivity and tipping points.
More temporally constrained work allows us to investigate
the impact of glacial–interglacial climates on ocean chem-
istry and carbon cycling on timescales relevant to humans
(Buchanan etal. 2016; Adloff etal. 2018).
The geological record provides a direct source of infor-
mation about biological processes against a backdrop of
varying climate, allowing us to investigate system/species
baselines, resiliencies and failure points in different climate
states. To use this rich resource from a modelling perspec-
tive, we require higher spatial resolution transient climate
simulations that will provide greater spatial and temporal
constraints on speciation, extinction dynamics, niche evo-
lution through time, and dispersal corridors and refugia in
the face of rapidly changing environments. This will facili-
tate fundamental knowledge capable of informing strategies
for the management of future biodiversity. Where transient
simulations with high spatial resolution are computationally
prohibitive, running snapshots over geologically and evolu-
tionarily meaningful timescales, particularly around peri-
ods with major climate transitions and aberrations, provide
highly valuable initial benchmarks.
5 Melting Ice Sheets andSea‑Level Change
A major scientific and societal challenge is understanding
the response of ice sheets to warming, and the resulting
rates, magnitudes and impacts of regional sea-level change
in the next 100years and beyond (Church etal. 2013). By
reconstructing past ice sheet variability, changes over cen-
tennial to millennial (and longer timescales) can be under-
stood. This is central to understanding societal impacts and
risks associated with future climate change.
What can Palaeoclimate Modelling doforyou?
1 3
The palaeo record helps constrain the drivers of ice-sheet
change, and therefore, associated sea-level change, during
differing climate states. Over the last 65 million years, major
climate transitions associated with growth and decay of ice
sheets were superimposed upon a gradual trend of atmos-
pheric cooling (Zachos etal. 2008). Due to the sparse nature
of geological evidence for ice sheet extent and sea-level his-
tory, ice sheet and palaeoclimate models have fundamen-
tally changed our understanding of ice-sheet growth in both
hemispheres, disentangling the role of CO2 versus the role of
tectonics in driving ice sheet expansion over major climate
transitions. For example, DeConto and Pollard (2003) found
that Antarctic Ice Sheet growth at the Eocene Oligocene
Transition (~ 34Ma) was driven by decreasing atmospheric
CO2, countering the prevailing view that the opening of the
Drake Passage and subsequent thermal isolation of the con-
tinent was responsible (Kennett 1977). Tectonics and moun-
tain building have also been implicated in the gradual onset
of northern hemisphere glaciation between 3.6 and 2.4Ma
(e.g., Mudelsee and Raymo 2005). Lunt etal. (2008) estab-
lished that decreasing atmospheric CO2, rather than tecton-
ics, was the dominant control on Greenland ice sheet growth.
Models also highlight that the scale of growth is sensitive to
whether the ice sheet was growing from an entirely ice-free
state or not (Contoux etal. 2015).
Whilst palaeoclimate modelling has been informative in
understanding the growth of ice sheets, of more pressing
concern is the scale and rate of future ice sheet mass loss
in a higher CO2 world. Instrumental records (e.g., satellite
data) of glacier extent only systematically capture the last
4 decades of change and, therefore, limit our capability to
understand large-scale, long-term changes in ice volume.
Global mean sea level (GMSL) rise from 1901 to 2010 has
been 1.7mm/year (Church etal. 2013). However, during
the last deglaciation (ca. 21–7ka) magnitudes and rates of
GMSL rise were significantly larger. Combined palaeocli-
mate and ice sheet modelling has identified an acceleration
in ice mass loss at 14.5ka, triggered by abrupt warming,
driving separation of the North American Ice Sheet into
regional ice domes (a process termed saddle collapse) and
contributing 5–6m to GMSL at a rate of ~ 14.7 to 17.6mm/
year (Gregoire etal. 2016; Gregoire etal. 2012). This pro-
vides a mechanism to explain a significant proportion of the
rise in GMSL at 14.5ka. Given that sea level is projected
to rise well beyond 2100 (Clark etal. 2016) assessing the
ability of models to reproduce rates of sea-level change on
centennial to millennial timescales, and potential mecha-
nisms for rapid collapse, is central to have confidence when
applying them to long-term future projections.
Models have helped refine our understanding of potential
rates and scales of sea-level rise, which can be attributed to
specific processes during previous climatically warm periods.
During the last interglacial (LIG) (ca. 129–116ka), GMSL is
thought to have been 6–9m above present (Dutton etal. 2015)
when the climate was 3–5°C warmer at polar latitude (Capron
etal. 2014). Moreover, it is likely that there was a period dur-
ing the LIG in which GMSL rose at a 1000-year average rate
exceeding 3mm/year (Kopp etal. 2010), but it is important
to understand which ice sheet(s) contributed to this rapid rate.
Coupled palaeoclimate-ice sheet simulations, consistent with
geologic data, indicate a retreat of ice in Greenland during the
LIG (Fig.4) leading to a GMSL rise of ca. 1.4m. Models also
suggest that Antarctica could have also contributed 3–4m to
the LIG highstand (Goelzer etal. 2016), with one study sug-
gesting that with > 2–3°C of Southern Ocean warming there
is the potential for complete collapse of the West Antarctic
ice sheet (Sutter etal. 2016), the recurrence of which is a key
concern in the context of future climate change.
The LIG, and the even warmer mid-Pliocene Warm
Period (mPWP, 3–3.3Ma), have been used as analogues to
understand future Earth system responses to warming at the
poles. DeConto and Pollard (2016) calibrated a palaeocli-
mate and ice sheet-modelling framework against the geo-
logical record of sea-level change during these time periods
to predict future ice mass loss from Antarctica. To reconcile
past records of GMSL with modelled ice mass loss, they
invoked a new mechanism that enhances the sensitivity of
the ice sheet where it meets the ocean. If this is applied
under future climate scenarios, Antarctica has the potential
to contribute more than 1m to GMSL by 2100 and more
than 15m by 2500. A challenge to these future predictions
is that we require supporting empirical evidence that these
processes operated in the past (Ritz etal. 2015).
Palaeoclimate modelling has been critical in improv-
ing understanding of how ice sheets, and thus sea level,
respond to increasing greenhouse gases. Progress towards
addressing the UN SDGs and the WCRP grand challenges
will come from fully coupling palaeoclimate and ice sheet
models to perform transient simulations at higher resolutions
than previously possible so that feedbacks between these
components of the Earth system can be better quantified.
Current modelling efforts focus largely on ice-sheet contri-
butions to GMSL, but in the future regional sea level will
significantly deviate from the global mean. Incorporation of
other controls on sea level such as ocean-density changes,
glacio-isostatic adjustment, dynamic topography and ero-
sion and sediment transport (Church etal. 2013) will help
reduce uncertainty in long-term (centennial to millennial)
projections.
6 Palaeoclimate Models andHydrology
Much of the climate change debate, particularly when
discussing the past, is focussed on changes in tempera-
ture. However, the WCRP grand challenges highlight the
A.M.Haywood et al.
1 3
importance of water supply for food production as well as the
role of extreme hydrological events (floods and droughts).
Both of these aspects are also closely linked to the UN Sus-
tainability Goals of ending hunger and improving food secu-
rity as well as delivering clean water and sanitation.
Until recently, most palaeoclimate modelling has
focussed on improving our understanding and ability to
model the mean changes in temperature/precipitation. This
type of modelling includes long timescale changes, such
as the role of Tibetan uplift in enhancing the South Asian
monsoon system (e.g., Manabe and Terpstra 1974; Ramstein
etal. 1997; Lunt etal. 2010b) or evaluation of simulated
monsoon changes resulting from orbital changes in the late
Quaternary and their impact on lake levels (e.g., Kutzbach
and Street-Perrott 1985). In addition to orbital enhance-
ment of summer monsoons, recent advances in computing
power allow palaeoclimate modelling of transient changes,
indicating the importance of changes in CO2 and meltwater
during the Quaternary as having affected the evolution of
rainfall patterns (Otto-Bliesner etal. 2014). Thus, the late
Quaternary provides a challenging test for models for forc-
ings relevant to the present.
Providing a clean water supply can also be facilitated by
learning from the past. For instance, there is considerable
concern about the recent decreases in the area of Lake Chad
(e.g., Lemoalle etal. 2012). However, in the Holocene and
Pliocene Lake Chad was much larger (the so-called Mega-
Chad). Palaeoclimate modelling (e.g., Sepulchre etal. 2008;
Contoux etal. 2013; Haywood etal. 2004) has shown that
this is a result of modest shifts in the position of the ITCZ
and hence implies that communities must expect and adapt
to high variability in Lake Chad on decadal and longer time-
scales. Considerably more work is needed to expand these
studies to other hydrological systems. Similarly, many areas
Fig. 4 Simulated Greenland Ice Sheet minimum extent for a the mid-
Pliocene warm period (mPWP ~ 3 to 3.3 Ma) and b the Last Inter-
glacial (LIG ~ 125 Ka) simulated by ice sheet models with multiple
climate model forcings for each period. The shading indicates the
number of model simulations that predict ice being present at a given
location. Nine models simulations are included for the LIG (Otto-
Bliesner et al. 2006; Solomon 2007; IPCC 2013; Yau et al. 2016)
and eight models are included for the mPWP (Dolan et al. 2015).
The combination of climate and ice sheet modelling can lead to new
insights regarding ice sheet extent and variability for time periods
where direct geological evidence is sparse or entirely missing
What can Palaeoclimate Modelling doforyou?
1 3
of Africa rely on groundwater sources, and some of these
reservoirs still contain water accumulated many thousands
of years ago. We have a poor understanding of many of these
systems and future work must target improvements in this
area.
Palaeoclimate modelling that directly targets the grand
challenge areas of hydrological extremes and water supply
are at an early stage of development, but should become one
of the major priorities for research. Until recently, extreme
events were hard to simulate but improvements in the spatial
resolution of models are allowing palaeoclimate models to
tackle such issues (see outlook section). Initial work (e.g.,
Haywood etal. 2004) used regional models to show that the
hydrological cycle associated with extreme warm periods
operated very differently, and this affected the interpretation
of the sedimentary structures found for such periods. More
recent work is increasingly focussing directly on the science
of palaeo-tempestology and extreme events. For instance,
Peng etal. (2014) modelled severe and persistent droughts
in China during the last millennium and suggested that these
droughts (and the East Asian monsoon system) could have
been modulated by variations in solar output.
7 Palaeoclimate Modelling andHuman
Systems
Palaeoanthropologists and archaeologists have a long his-
tory of collaboration with climate modellers. From a mod-
elling perspective, palaeoclimate proxies (e.g., pollen data,
microfauna, malacofauna) obtained from dated archaeo-
logical deposits allow climatologists to test model perfor-
mance in non-analogue situations (Braconnot etal. 2012).
From an archaeological perspective, palaeoenvironmental
reconstruction and palaeoclimate modelling provide essen-
tial context for understanding past human adaptations. Pal-
aeoanthropology, firmly rooted in evolutionary ecology,
has long recognised that climate change has an impact on
hominin evolution (Vrba 1995) and palaeoclimate mod-
els feature prominently in palaeoanthropological debates.
Palaeoclimate models are also increasingly integrated into
archaeological models that seek to understand the pattern of
hominin dispersals out of Africa, for example, or to explore
how past climate conditions affected the spatial distribution
and structure of human populations, altering the course of
cultural evolution. The pioneering ‘Stage 3 Project’ (Van
Andel and Davies 2003) is an example of the interdiscipli-
nary nature of archaeological research, demonstrating the
integration of palaeoclimate models and archaeological data
to design research that sheds light on the dynamics of human
populations in the past.
Early human evolution is currently framed as a series
of adaptive responses to environmental changes linked to
orbital forcing mechanisms. Within this framework, climate
models are used in conjunction with palaeoenvironmental
data to interpret the paleontological record (Grove 2011).
For example, although the origins of bipedalism (which
defines the hominin lineage) extend further back in time,
the evolution of obligate bipedalism during the Pliocene
is linked to transformations of the African landscape and
the expansion of C4-dominated grasslands. This event and
others like it (e.g., the emergence of the genus Homo) are
thought to have been triggered ultimately by orbital forc-
ing (Maslin and Christensen 2007). Climate models have
also been used to assess the impact of climate variability on
hominin populations. The variability selection hypothesis,
for example, suggests that trends in variability during the
Plio-Pleistocene resulted in a selection for plasticity that
characterises our lineage (Potts and Faith 2015), which could
explain why humans have dispersed more widely than any
other primate species.
Our understanding of the mechanisms shaping the pattern
of hominin dispersals, which are major events in the history
of our species, is framed in terms of environmental change.
The earliest hominin dispersals, for example, likely coin-
cided with climate events that reshaped the biogeographi-
cal map of Africa (Larrasoaña etal. 2013). Later dispersals,
such as the dispersal of modern humans into Eurasia during
the late Pleistocene, are also best understood from a climate
perspective (Hughes etal. 2007; Timmermann and Friedrich
2016; Eriksson etal. 2012). Modern human dispersals to
Australia and the New World coincide with megafaunal
extinctions and climate models provide us with the data we
need to contextualise this information, attributing causal-
ity where it is due (Prescott etal. 2012). If climate change
shaped the pattern of human dispersals in the past, climate
variability has been shown to affect modern societies too,
increasing conflict (O’Loughlin etal. 2014), which is linked
to modern population displacements.
High-resolution palaeoclimate models have been used to
study the response of human systems to climate instability
(Banks etal. 2013), to assess the impact of climate events
such as the Last Glacial Maximum on population structure
and demography (Tallavaara etal. 2015), and test the sensi-
tivity of human systems to climate predictors such as ecolog-
ical risk (Burke etal. 2017). Modelling the complex interac-
tions between human systems and the environment allows us
to appreciate how demographic patterns such as population
size and connectivity, which are affected by climate change,
can drive technological innovation and cultural complex-
ity. By developing spatially explicit models that incorpo-
rate climate models or simply make use of model outputs,
archaeologists gain a richer and more dynamic appreciation
of the environmental response to climate change and the
various mechanisms that allow human systems to adapt.
These archaeological models, in turn, hold lessons for the
A.M.Haywood et al.
1 3
future as we attempt to gauge the resilience of small-scale, or
“traditional” societies and judge what is required to preserve
human cultural diversity.
Collaborations between palaeoclimate modellers, archae-
ologists and palaeoanthropologists have provided rich
opportunities for modelling human/environment interactions
as well as contributing to improving climate model design.
However, difficulties arise because of differences in the reso-
lution of model outputs and signals from the palaeoclimate
record that limits the application of palaeoclimate models
to the study of early human evolution, for example. Further-
more, human populations perceive and respond to environ-
mental change at a wide range of temporal and spatial scales.
Increased capability and capacity in palaeoclimate research
and improvements to the scale of resolution of model out-
puts, as well as greater efforts towards improving the acces-
sibility of climate model outputs for non-specialists, will
improve this situation in the future.
8 Palaeoclimate Modelling, Industry
andInnovation
There is a strong focus on the impact of contemporary cli-
mate change on various aspects of industry. However, the
fact that many important aspects of society’s requirements
need a longer term perspective either for the future or of the
deep past is often overlooked.
One of the most challenging demands of modern society
is the use of the Earth’s geological resources and reserves.
The growth of the world economy is demanding greater sup-
plies of many metals such as aluminium, as well as ever
increasing demands for fossil fuels. The geographical distri-
bution of aluminium’s chief ore (bauxite) and organic-rich
source rocks for hydrocarbons both depend on past climates.
Hence prediction (or retrodiction) of past climates can help
in frontier exploration for these resources. Since the earliest
days of palaeoclimate modelling, efforts have been made
to retrodict source rocks. Parrish and Curtis (1982) and
Scotese and Summerhayes (1986) developed a conceptual
and a computer model of atmospheric circulation patterns
to predict where oceanic upwelling occurs. Such regions
are typically associated with high organic productivity that
subsequently is buried and potentially becomes source rocks.
Further work with palaeoclimate models extended these
predictions by quantifying them (e.g., Barron 1985). More
recent work (Harris etal. 2017) continues this research with
full ESMs, making use of simulated atmospheric and ocean
circulation (including aspects such as storminess and solar
radiation) as well as aspects of the modelled carbon cycle
to make very specific regional predictions of source rocks.
These are used for frontier exploration.
Palaeoclimate modelling also plays a major role in risk
assessment of the long-term storage of nuclear waste. Any
site proposed as a nuclear waste repository requires a risk
assessment measured up to 100,000years into the future. On
such long time scales, future orbitally forced climate change
becomes as important as anthropogenic forcing. Early stud-
ies (e.g., Goodess etal. 1990) simply extrapolated past long-
term changes into the future, but more recent work has made
extensive use of more detailed palaeoclimate models. The
latest approaches (e.g., Lindborg etal. 2005) use a com-
bination of simple and full complexity climate models to
provide detailed predictions of site-specific climate up to
200,000years into the future, using methodologies identical
to many palaeoclimate modelling studies.
The methodologies of palaeoclimate modelling have been
utilised in some aspects of geoengineering research. This is
because palaeoclimate modelling has often pioneered the
use of ESMs, including detailed representations of the car-
bon cycle. Hence, many ideas of carbon sequestration have
used palaeoclimate modelling tools to evaluate their efficacy.
For example, Taylor etal. (2016) discussed the artificial
acceleration of rock weathering as a potential method for
enhanced drawdown of CO2 and reduced ocean acidification.
Many aspects of society are also vulnerable to extreme
events. Almost by definition (e.g., 100year return period),
these extreme events are beyond the observational record
and palaeoclimate studies are required to give context to
any event. Palaeoclimate proxy observations of storm events
have frequently been used in infrastructure planning (such as
flooding events and the location of nuclear power stations),
but more recently palaeoclimate modelling of extreme
events has also helped in planning process. For instance,
model predictions of storm events during the last millennium
(Kozar etal. 2013) were considered as a part of the evidence
based in the New York City Panel on Climate Change 2015
Report (Horton etal. 2015). These include estimating the
frequency of extreme events for flood protection, the risk
assessment for nuclear power stations and long-term storage
of nuclear waste.
9 Outlook
9.1 Overcoming Current Methodological/
Technological Limitations
A thorough understanding of physical processes, the robust
application of mathematics and statistical techniques, the
availability of accurate geological boundary conditions and
forcing estimates, combined with the required research-
intensive computer facilities and appropriate computational
and software engineering support, are central to the overall
capability of palaeoclimate modelling (Fig.5).
What can Palaeoclimate Modelling doforyou?
1 3
One of the most fundamental strengths of palaeoclimate
modelling is that it provides a unique way to examine the
response of the Earth system to forcing mechanisms in an
integrated way. Key uncertainties associated with future cli-
mate change projection stem from the strength of positive
feedbacks associated with components of the climate system
that respond to forcing over medium to long timescales (e.g.,
ocean circulation and ice sheets; IPCC 2013), and the geo-
logical record is uniquely capable of preserving signals of
change associated with slower responding components of the
Earth system (Haywood etal. 2013). ESMs that incorporate
the representation of many earth system processes, and their
associated feedbacks on climate, are now available and can
be run at higher and higher spatial resolutions (Peng etal.
2014). Such models are capable of simulating the response
and longer term climate feedbacks stemming from a wide
array of earth system processes, and from climate-relevant
processes that operate over medium to long timescales.
Fig. 5 Summary illustration showing a key data and technological/
knowledge requirements that underpin palaeoclimate modelling, b
key areas of contribution to understanding different physical systems
and life on Earth, c the human value components of the contributions
shown in b, and d, e the direction of travel required to address out-
standing critical research questions with significant human impor-
tance
A.M.Haywood et al.
1 3
However, with increasing resolution and model complexity
comes increasing computational demand and cost. In addi-
tion, using high-resolution ESMs to simulate the past comes
with its own unique scientific and technological challenges
that can dramatically increase the computational expense
and time associated with producing simulations.
For example, uncertainties in geological boundary con-
ditions often necessitate the production of an ensemble of
climate simulations for a specific interval of time (Hay-
wood etal. 2013). In addition, reconfiguring ESMs so that
they can simulate the deeper past successfully is extremely
challenging. Such models are not developed with the spe-
cific needs of palaeoclimate modellers in mind. As such,
the reconfiguration of the land/sea mask, land elevation,
ocean bathymetry, land cover, etc., creates challenges that
require dedicated software engineering support to overcome,
which is difficult to resource adequately. In addition, with
increasing model capability comes increasing demand for
appropriate boundary conditions and forcing datasets so
that the potential of these new models can be fully realised.
For instance, models that incorporate complex representa-
tions of atmospheric chemistry and/or atmospheric dust/
aerosol-climate interactions may require information on
the initial concentration of CH4 in the atmosphere, or dust
emission sources and emissions of Volatile Organic Com-
pounds (VOC’s). Unless ESMs are developed so that the
model dynamically predicts such parameters, rather than
requiring their initial prescription, it may lead to increased
uncertainty in boundary conditions and forcings within pal-
aeoclimate simulations, as these parameters may be poorly
constrained geologically. Also given the radically different
(from modern) climates such models are applied to, and the
major changes to boundary conditions that are necessary,
palaeoclimate simulations require substantial spin-up time
insofar as they include a dynamic ocean, which can require
several thousand simulated years to fully adjust, though
atmospheric spin-up time is much faster (several decades to
a century of simulation). Here computational efficiency and
scalability of the model code (across computer processors)
become paramount. Any model that cannot reliably achieve
at least 10–30 model years per wall clock day with a reason-
able total CPU demand/cost will be very challenging, if not
practically impossible, to apply effectively to palaeoclimate
applications and the assessment of uncertainty in past cli-
mate simulation.
The majority of latest generation full complexity ESMs
do not meet the requirements for palaeoclimate modelling.
Model development is carried out in isolation from the pal-
aeoclimate community’s specific requirements. There seems
little scope that will change, meaning that the palaeoclimate
modelling community’s future interests could be best served
by adopting a more tailored strategy towards model devel-
opment. Examples of the development of EMICs (Earth
System Models of Intermediate complexity) as well as other
current large-scale research initiatives such as the climate
modelling initiative called PalMod (Paleo Modelling), which
is funded by the German Federal Ministry of Education and
Science to understand climate system dynamics and vari-
ability during the last glacial cycle. Fundamentally, more
considered and flexible strategies will be required to deter-
mine what spatial and vertical resolution and model com-
plexity is actually needed to answer specific challenges in
palaeoclimate science.
9.2 Enhanced Integration ofStatistical
Methodologies toAssess Uncertainty
While current climate models seek to optimally represent
physical processes that determine weather and climate, this
representation is not perfect and models have been tuned to
provide acceptable simulations of modern climate regime.
For palaeoclimate simulations, where boundary conditions
such as atmospheric CO2 concentration differ from mod-
ern climate simulations, the approaches used to ensure that
models deliver the best possible simulation for the mod-
ern (observed) climate may no longer hold. A commonly
employed solution to this problem is to consider ensembles
of models to understand the commonalities and differences
between possible model outputs. Statistical techniques such
as Bayesian Model Averaging (Hoeting etal. 1999) can be
used to compute ensemble averages where greater weight is
given to models that are most compatible with the available
data.
In addition, the impacts associated with global warm-
ing cannot be fully characterised by a change in the spa-
tial and temporal averages of specific climate variables.
To capture such changes it is necessary to model how the
distribution of a climate variable (instead of just the mean)
depends on changing boundary conditions (such as GHG
concentrations). A variety of statistical techniques have been
used for this purpose: quantile regression is a generalisa-
tion of linear regression, which allows for the estimation
of arbitrary quantiles of the distribution of a climate vari-
able instead of just the mean (e.g., Janson and Rajaratnam
2014). For example, extreme value theory describes the
tails of a distribution, with the aim of predicting extremes
beyond what has been observed in the available time series
of data (e.g., Mannshardt etal. 2013). Some authors have
also used specialised techniques to simultaneously capture
the correlations between proxy variables and climate vari-
ables across space and time (e.g., the GraphEM method;
Guillot etal. 2015), although such beneficial approaches are
not commonly used, and this highlights the need for further
integration between palaeoclimate modellers and applied
statisticians.
What can Palaeoclimate Modelling doforyou?
1 3
9.3 Removing Barriers toData Sharing
andMultidisciplinary Collaboration
Access to appropriate palaeoclimate model outputs is a
significant limitation for other research disciplines. The
progress already made towards widening access can be
attributed in part to research council requirements to make
publicly funded science widely available in national data
repositories (e.g., the British Atmospheric Data Centre).
In addition, journal requirements for the uploading of data
sets associated with specific publications have had a positive
impact, as well as internationally promoted output standards
and software libraries such as those adopted by the Coupled
Model Intercomparison Project (i.e., CMOR: the Climate
Model Output Rewriter). CMOR ensures that a standard set
of model variables for different climate model experiments
are available on Earth System Grid Federation repositories
(https ://esgf.llnl.gov).
New community-based efforts are underway to support
data sharing across disciplines. For example, the PaleoClim
database provides pre-processed climate data to support eco-
logical niche studies (Brown etal. 2018). These community-
led initiatives are important because the approach towards
processing model outputs can be application specific, and
scientists in the disciplines requiring climate outputs may
not have the required programming skills and experience
to successfully deal with unprocessed palaeoclimate model
data. Initiatives such as PaleoClim provide a template of
how communities can come together to discuss the removal
of barriers and enhance awareness of, and access to, palaeo-
climate modelling data.
Whilst the initiatives described above can improve access
to palaeoclimate model output by other communities, they
will not fully resolve the issue of rigorously embedding pal-
aeoclimate model outputs into other disciplines. There is
an underlying concern as to whether model outputs used
in specific applications contain an adequate appreciation
and expression of uncertainty. The obvious solution is to
embed palaeoclimate modellers within multidisciplinary
teams. However, the global pool of available palaeoclimate
modellers is small, and thus collaborative capacity is lim-
ited. A complementary solution promoted more generally
in efforts to foster multi-disciplinarity is the development
of T-shaped researchers (e.g., Palmer 1990). The develop-
ment of T-shaped skills is a concept promoted for more
than 20years, with the T representing the range of research
expertise an individual develops, and the foundation/depth
of individual understanding represented by the vertical bar
(Palmer 1990). Using this philosophy a researcher first
develops an expertise in their own discipline before subse-
quently developing their skills base in a way that facilitates
the deployment of their knowledge in a wider array of sci-
entific disciplines. The development of T-shaped researchers
is essential to the success of multi-disciplinarity, but it is
unclear how conducive academic environments currently are
to those wishing to adopt a T-shaped research skills base.
The required investment of time versus immediate scientific
return is of paramount consideration for early career scien-
tists, with the requirement to demonstrate sustained levels
of high research performance very clear.
9.4 Developing anEnhanced Focus onPast
forFuture Relevant Science
The potential contribution of different types of palaeocli-
mate modelling to the generation of science underpinning
UN SDGs or global scientific grand challenges is not equal.
This is also the case for the support palaeoclimate modelling
can provide to multidisciplinary research. For the science
to grow its influence in these regards, more targeted and
co-ordinated approaches will be required that maximise the
utility of palaeoclimate modelling. We highlight this need
and opportunity by reference to specific examples.
Mitigation and adaptation strategies for global climate
change are informed by studies that seek to better constrain
the extremes of natural variability in climate and weather
phenomena from the past (beyond the observed climate
period). However, a weakness of approaches that consider
only the very recent past, for example the last millennium,
is that the effect of the warming trend since the onset of
the industrial revolution is omitted from the assessment of
the behaviour of weather and climate extremes. Given the
current and projected rates of GHG emission, and the asso-
ciated rapid warming trend, palaeoclimate modelling is pay-
ing increasing attention to warmer (than the pre-industrial)
intervals, and also to intervals when CO2 concentrations in
the atmosphere were analogous to current and near future
concentrations (e.g., Haywood etal. 2013). Given the cur-
rent rapid rate of temperature increase, it is necessary to go
back in time as far as the Pliocene epoch (~ 3 million years
ago) to find the estimated 3°C global annual mean surface
temperature change that we are on track to achieve by the
end of this century (Haywood etal. 2013). This rapid pro-
gress towards analogous past warm climates was recently
highlighted by Burke etal. (2018) who used different cli-
mate model simulations for future GHG scenarios, and then
compared these to different simulated climates of the past
including the Last Glacial Maximum, the Mid-Holocene,
the Last Interglacial, the Pliocene and the early Eocene. Sta-
tistically, the climate state that they considered to be most
similar to what models predict will be reality by 2030–2050
AD was the mid-Pliocene Warm Period (~ 3 million years
ago), and by ~ 2200 AD the early Eocene (Burke etal. 2018).
This provides a sobering assessment of the rate of climate
change currently occurring, and underlines the importance
of an increasing focus on past warm intervals.
A.M.Haywood et al.
1 3
However, even a general concentration of community
efforts on warm epochs may not be sufficient to guarantee
the maximum utility of palaeo science in informing UN
SDGs and global scientific grand challenges. Climate vari-
ability is driven by variations in Earth’s orbit around the
sun with predictable periodicities (the Milankovitch cycles).
Orbital forcing has acted as a natural pacemaker for insola-
tion since our planets formation. Therefore, while epochs in
the past may be analogous in the sense of different conceiv-
able CO2 stabilisation scenarios for the future, at any point
in time within these epochs the surface expression of climate
(i.e., difference compared to the pre-industrial baseline) will
not solely be a response to GHG forcing (Haywood etal.
2016). While this does not matter greatly in terms of the
global annual mean temperature response, it is important
for the time-specific expression of climate change locally,
regionally and seasonally. Orbital parameters, and the result-
ing insolation pattern at the top of the atmosphere, are reli-
ably calculable for the Cenozoic (Laskar etal. 2011). It is
possible to isolate specific intervals within a warmer than
pre-industrial epoch with the same, or very similar, insola-
tion forcing (e.g., Haywood etal. 2016). Such an approach
provides an obvious benefit of studying a mean state climate
that is more influenced by a carbon cycle perturbation and
less influenced by other forcing agents. This approach has
been adopted within the scientific strategy underpinning
the second phase of the Pliocene Model Intercomparison
Project36, whereby a specific interglacial within the Pliocene
has been identified for study. Such a methodology differs
from more classical approaches in palaeoclimatology where
the most concentrated effort tends to focus on the most rapid
and/or largest transitions in Earth system behaviour, but that
does not necessarily mean those intervals are the most rele-
vant in the context of the future. The judgement is dependent
upon the scientific question which is asked. Nevertheless, it
is important to recognise that warm (and warming) intervals
in the past characterised by very different orbital forcing
compared to present-day (e.g., the Last Interglacial and the
Last Deglaciation) will remain very important to study. For
example, they are important for the assessment of regional
and seasonal variations in climate (past and future), and for
understanding how the Greenland and Antarctic Ice Sheets
respond to a warmer (and warming) atmosphere and oceans
(Otto-Bliesner etal. 2006).
Palaeoclimate modelling studies have focussed a great
deal on large-scale mean state climate changes. Within such
a context, numerous studies have examined modes of natural
climate variability, but very few have examined the nature of
extreme weather and climate events during warm episodes of
the deeper past. Given that society is likely to experience the
worst initial effects of anthropogenic climate change through
a change in the frequency and/or magnitude of extreme
events (IPCC 2013), a more concerted effort in this regard
is required. Whilst geological data may not always be avail-
able to assess the quality of model results in this regard, data
are available for the climatic mean state. This mean state is
a product of the average weather and climate variability at
any given time and place. Therefore, if models demonstrably
simulate the mean climate faithfully, this may add credence
to their simulation of higher order climate and weather vari-
ability, even if geological data to assess the model predic-
tions of extreme weather and climate events are absent.
10 Conclusion
In conclusion, palaeoclimate modelling over the last 4 dec-
ades has provided a broad and deep contribution to multi-
disciplinary science, and to the science underpinning global
grand challenges and SDGs. First-order questions about the
operation of climate and environmentally relevant processes,
and our planet’s limits in terms of sustaining life during peri-
ods of rapid change remain unanswered. This includes the
fundamental understanding of the carbon cycle, identifica-
tion of critical environmental thresholds for species distribu-
tion and life, and what are the longer term implications of
climate and ecosystem change on human adaptability and
vulnerability. The great strides made in the development
of more and more compete and capable models provide a
wealth of opportunity for further discovery, but only if the
unique challenges associated with simulating climate of the
past are properly appreciated and understood.
Acknowledgements This work was carried out as a part of, and finan-
cially supported by, the Past Earth Network (PEN: https ://www.paste
arth.net/). PEN was one of the UK EPSRC Forecasting Environmental
Change Networks led by J.V. A.M.H and A.M.D.
Author Contributions AMH and PJV conceived and led the overall
effort and contributed directly to the writing of the manuscript. All
authors shared joint responsibility for writing the manuscript and for
the preparation of the figures.
Compliance with Ethical Standards
Conflict of Interest The authors declare no competing interests.
Open Access This article is distributed under the terms of the Crea-
tive Commons Attribution 4.0 International License (http://creat iveco
mmons .org/licen ses/by/4.0/), which permits unrestricted use, distribu-
tion, and reproduction in any medium, provided you give appropriate
credit to the original author(s) and the source, provide a link to the
Creative Commons license, and indicate if changes were made.
What can Palaeoclimate Modelling doforyou?
1 3
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... Paleoclimate simulations (Box 1) enable researchers to understand long-term climate trends, assess the natural variability of the climate system and the impact of climate events on biotic and abiotic systems (e.g. Haywood et al. (2019); Kageyama and Paillard (2021)). For instance, paleoclimate simulations help biogeographers understand historical changes in species distributions (e.g. Brown et al. (2018)), allow cryosphere researchers to track glacial extents and dynamics (e.g. ...
... Proxy records such as ice cores, sediment records and fossil data aided in improving the simulations through testing and validation (e.g. Haywood et al. (2019); Tierney et al. (2020b)) and, more recently, through data-model assimilation (e.g. Tierney et al. (2020a)). ...
... Frontiers of Biogeography 18, 2025, e135871 LGM cooling variability affects biome reconstructions 3 format (e.g. raster), were an advantage over the spatially scattered proxy records (Braconnot et al. 2012;Haywood et al. 2019). Additionally, these datasets include multiple consistent variables, opposed to the few variables that can be derived from a proxy. ...
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Downscaled paleoclimate datasets are widely used in biogeographical research, aiding our understanding of past environmental shifts and species’ responses to climate change. Numerous datasets exist, varying in spatiotemporal resolution and underlying methodologies, resulting in variation in estimated temperature. Understanding this variability is important for accurately reconstructing past biogeographical dynamics, especially in complex regions like mountains. We compare the Mean Annual Temperature (MAT) at the Last Glacial Maximum (LGM) from five different downscaled paleoclimate datasets — Beyer, CHELSA-TraCE21k, EcoClimate, PALEO-PGEM-series, WorldClim — against MAT estimates from paleoenvironmental proxy records (fossil pollen and plant macrofossils) within and outside mountains. Additionally, we test the performance of a ‘global grid cooling’ method (i.e. lowering local temperatures by a global LGM estimate) against proxy records. Then, we evaluate the implications of inter-dataset variability for reconstructing temperature-delimited biomes in mountains by reconstructing LGM treeline elevations. We find that LGM temperature cooling and treeline reconstructions strongly vary amongst paleoclimate datasets and between datasets and proxy records. The temperature gradient with elevation is poorly captured by datasets with a coarser spatial resolution. Paleoclimate datasets generally suggest a warmer LGM than proxy records, especially in mountains, while the global grid cooling method more closely aligns with proxy records. Inter-dataset variability can strongly affect the outcome of temperature-delimited reconstructions of biomes and their boundaries, such as treelines. We call for greater awareness and more transparency about the limitations of downscaled paleoclimate datasets in mountainous areas and suggest further research to be aimed at capturing the small-scale heterogeneity of mountains in paleotemperature datasets. Highlights LGM cooling is globally both over- and underestimated by downscaled paleoclimate datasets, resulting in overestimation (i.e. too high) and underestimation (i.e. too low) of LGM treeline elevations. Differences in LGM treeline elevation reconstructions can range from 288 to 2779 metres, depending on the paleoclimate dataset. The resolution of several downscaled paleoclimate datasets is unsuitable to capture LGM temperatures in mountainous regions. The median temperature difference between paleoclimate datasets and proxy records is larger within than outside mountain ranges, with substantial differences amongst datasets. Paleoclimate dataset choice strongly impacts biogeographical hypotheses, reconstructions and conclusions and should be carefully evaluated.
... Combining archaeological and climate work can be a rewarding avenue. Archaeological research is often the sole method of providing the necessary human element in human-environmental interaction studies (Mijares et al. 2020), while climate models allow us to assess the way the environment has changed over varying spatiotemporal scales (Haywood et al. 2019). So, how can one responsibly utilize climate models in archaeological work pertaining to disaster, risk, and resilience? ...
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An ideal model of seafaring simulates realistic human decision-making and behavioural patterns to help researchers understand the way past communities functioned within a maritime context. Seafaring involves inherent risk, potential for environmental disaster, and opportunities to demonstrate resilience. Understanding what risks ancient seafarers faced and how they behaved in the face of disaster provides an important lens through which researchers can understand the breadth of human response to environmental disaster, decision-making in the past, and the social ideologies of the societies they study. Computational models are often insufficient to capture the complexities of these junctures in human history. Our assumptions about modern human behaviour and what constitutes a “default” mode (which is often Western or Euro-centric) form input parameters and affect model output. Additionally, the spatiotemporal resolution of climate models often makes the simulation of discrete environmental events challenging. Because disaster, risk, and resilience are poorly realized in computational models, considering past human response, decision-making, and ideologies can improve not only our understanding of past societies but also how we develop models. In this article, we discuss questions and challenges regarding disaster, risk, and resilience that we face in our collective body of work, which spans a diverse temporal and geographical range. We aim to ignite conversations about the role of these experiences in archaeological models and to challenge the status quo to improve the study of past maritime communities. The following questions and their collaborative responses exhibit the candid discussions that the CAST community has facilitated and participated in about how to manage the challenges and opportunities presented by disaster, risk, and resilience in seafaring research.
... Paleo-data has provided invaluable insights into natural cycles/ variability over relatively short (decadal) to long (millions of years) time scales, into abrupt changes in climate as well as into the occurrence and impact of, and recovery from, hazardous events (e.g., McGuire et al., 2023). Paleo-climate data continues to be vitally important for improving and constraining climate models (Schmidt, 2010;Haywood et al., 2019;Tierney et al., 2020), and for assessing climate sensitivity to increases in CO 2 (Sherwood et al., 2020). However, the greatly increased focus on climate modelling and model outputs over the past three decades has effectively decreased the emphasis placed on paleo-data. ...
... Comparing proxy-based reconstructions with climate simulations will re ne our knowledge of climate dynamics (e.g., Phipps et al., 2013) and improve climate models. This approach will contribute to a better comprehension of Earth's evolution and provide insights into the resilience of natural and social systems in the Anthropocene (Haywood et al., 2019). ...
Chapter
Paleoclimate reconstructions are essential for understanding the dynamics of the climate system and its past variations. By utilizing climate-dependent proxies, these reconstructions provide a comprehensive perspective on climatic variations that extend far beyond the limited scope of instrumental records, spanning centuries to millennia. Particularly, proxy-based reconstructions for the last two millennia provide valuable insights into natural climate variability during the preindustrial era and the anthropogenic influence on current climate change. As a result, paleoclimate studies are also critical for interpreting climate projections in the context of anthropogenic forcing. South America, with its vast and diverse climate conditions, is a region rich in high-resolution paleoclimate records, including marine, lacustrine, and fjord sediments, speleothems, ice cores, tree rings, glacial and aeolian deposits, archaeological evidence, and historical documents, among others, all of which capture past climate changes. However, despite numerous paleoclimate reconstructions conducted across the continent and significant advances in understanding its past climate, substantial research gaps remain. These gaps are particularly evident in understudied regions and poorly understood phenomena, hindering a comprehensive understanding of climate variability at both regional and continental scales. To advance paleoclimatic research in South America, future efforts should prioritize (a) the collection of high-resolution records from key locations, (b) the integration of diverse proxies and innovative methodologies, (c) enhancing our understanding of climate-proxy relationships, and (d) developing new proxy calibrations. Collaboration with local communities and indigenous peoples and adopting interdisciplinary approaches will be vital in driving the field forward.
... In the literature the terms SDM or ecological niche modelling (ENM) are used most often to refer to a set of comprising algorithms that model the distribution of species while also connecting them with the concept of ecological niches (Sillero 2011). In recent years this technique has found a wider application in the field of palaeontology to answer ecological and evolutionary questions in deep time (Haywood et al. 2019). Earlier in the 2010s, this technique found a use in a Recent palaeontological context (Graham et al. 1996;Svenning et al. 2011), but authors have previously successfully applied this approach deep into the Phanerozoic as well (Stigall 2012;Myers et al. 2015;Waterson et al. 2016;Chiarenza et al. 2019Chiarenza et al. , 2020Chiarenza et al. , 2021. ...
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... However, there is potential for traditional model evaluation and development to be expanded to utilise proxy data associated with paleoclimate states e.g. [1][2][3][4][5][6] . In particular, paleoclimate model simulations test model behaviour under a wide range of forcings, which encompass those expected in the timescale of the next few centuries and beyond 7,8 . ...
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This book provides a first synthetic view of an emerging area of ecology and biogeography, linking individual- and population-level processes to geographic distributions and biodiversity patterns. Problems in evolutionary ecology, macroecology, and biogeography are illuminated by this integrative view. The book focuses on correlative approaches known as ecological niche modeling, species distribution modeling, or habitat suitability modeling, which use associations between known occurrences of species and environmental variables to identify environmental conditions under which populations can be maintained. The spatial distribution of environments suitable for the species can then be estimated: a potential distribution for the species. This approach has broad applicability to ecology, evolution, biogeography, and conservation biology, as well as to understanding the geographic potential of invasive species and infectious diseases, and the biological implications of climate change. The book lays out conceptual foundations and general principles for understanding and interpreting species distributions with respect to geography and environment. Focus is on development of niche models. While serving as a guide for students and researchers, the book also provides a theoretical framework to support future progress in the field.
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While the early Eocene has been considered in many modelling studies, detailed simulations of the middle and late Eocene climate are currently scarce. To understand Antarctic glaciation at the Eocene-Oligocene Transition (~ 34 Ma) as well as middle Eocene warmth, it is vital to have an adequate reconstruction of the middle-to-late Eocene climate. Here, we present a set of high resolution coupled climate simulations using the Community Earth System Model (CESM) version 1. Two middle-to-late Eocene cases are considered with new detailed 38 Ma geographical boundary conditions with a different radiative forcing. With 4 × pre-industrial concentrations of CO2 (i.e. 1120 ppm) and CH4 (~ 2700 ppb), the equilibrium sea surface temperatures correspond well to available late middle Eocene (42–38 Ma) proxies. Being generally cooler, the simulated climate with 2 × pre-industrial values is a good analog for that of the late Eocene (38–34 Ma). Deep water formation occurs in the South Pacific Ocean, while the North Atlantic is strongly stratified and virtually stagnant. A shallow and weak circumpolar current is present in the Southern Ocean with only minor effects on southward oceanic heat transport within wind-driven gyres. Terrestrial temperature proxies, although limited in coverage, also indicate that the results presented here are realistic. The reconstructed 38 Ma climate has a reduced equator-to-pole temperature gradient and a more symmetric meridional heat distribution compared to the pre-industrial reference. Climate sensitivity is similar (~ 0.7 °C/Wm²) to that of the present-day climate (~ 0.8 °C/Wm²; 3 °C per CO2 doubling), with significant polar amplification despite very limited sea ice and snow cover. High latitudes are mainly kept warm by albedo and cloud feedbacks in combination with global changes in geography and the absence of polar ice sheets. The integrated effect of geography, vegetation and ice accounts for a 6–7 °C offset between pre-industrial and 38 Ma Eocene boundary conditions. These 38 Ma simulations effectively show that a realistic middle-to-late Eocene climate can be reconstructed without the need for greenhouse gas concentrations much higher than proxy estimates. The general circulation and radiative budget allow for mild high-latitude regions and little to no snow and ice cover, without making equatorial regions extremely warm.
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In Earth system model simulations we find different carbon cycle sensitivities for recent and glacial climate. This result is obtained by comparing the transient response of the terrestrial carbon cycle to a fast and strong atmospheric CO2 concentration increase (roughly 1000ppm) in C4MIP type simulations starting from climate conditions of the Last Glacial Maximum (LGM) and from Pre-Industrial times (PI). The sensitivity β to CO2 fertilization is larger in the LGM experiment during most of the simulation time: The fertilization effect leads to a terrestrial carbon gain in the LGM experiment almost twice as large as in the PI experiment. The larger fertilization effect in the LGM experiment is caused by the stronger initial CO2 limitation of photosynthesis, implying a stronger potential for its release upon CO2 concentration increase. In contrast, the sensitivity γ to climate change induced by the radiation effect of rising CO2 is larger in the PI experiment for most of the simulation time. Yet, climate change is less pronounced in the PI experiment, resulting in only slightly higher terrestrial carbon losses than in the LGM experiment. The stronger climate sensitivity in the PI experiment results from the vastly more extratropical soil carbon under those interglacial conditions whose respiration is enhanced under climate change. Comparing the radiation and fertilization effect in a factor analysis, we find that they are almost additive, i.e. their synergy is small in the global sum of carbon changes. From this additivity, we find that the carbon cycle feedback strength is more negative in the LGM than in the PI simulations.
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As the world warms due to rising greenhouse gas concentrations, the Earth system moves toward climate states without societal precedent, challenging adaptation. Past Earth system states offer possible model systems for the warming world of the coming decades. These include the climate states of the Early Eocene (ca. 50 Ma), the Mid-Pliocene (3.3–3.0 Ma), the Last Interglacial (129–116 ka), the Mid-Holocene (6 ka), preindustrial (ca. 1850 CE), and the 20th century. Here, we quantitatively assess the similarity of future projected climate states to these six geohistorical benchmarks using simulations from the Hadley Centre Coupled Model Version 3 (HadCM3), the Goddard Institute for Space Studies Model E2-R (GISS), and the Community Climate System Model, Versions 3 and 4 (CCSM) Earth system models. Under the Representative Concentration Pathway 8.5 (RCP8.5) emission scenario, by 2030 CE, future climates most closely resemble Mid-Pliocene climates, and by 2150 CE, they most closely resemble Eocene climates. Under RCP4.5, climate stabilizes at Pliocene-like conditions by 2040 CE. Pliocene-like and Eocene-like climates emerge first in continental interiors and then expand outward. Geologically novel climates are uncommon in RCP4.5 (<1%) but reach 8.7% of the globe under RCP8.5, characterized by high temperatures and precipitation. Hence, RCP4.5 is roughly equivalent to stabilizing at Pliocene-like climates, while unmitigated emission trajectories, such as RCP8.5, are similar to reversing millions of years of long-term cooling on the scale of a few human generations. Both the emergence of geologically novel climates and the rapid reversion to Eocene-like climates may be outside the range of evolutionary adaptive capacity.
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The extent to which climate change has affected the course of human evolution is an enduring question. The ability to maintain spatially extensive social networks and a fluid social structure allows human foragers to “map onto” the landscape, mitigating the impact of ecological risk and conferring resilience. But what are the limits of resilience and to which environmental variables are foraging populations sensitive? We address this question by testing the impact of a suite of environmental variables, including climate variability, on the distribution of human populations in Western Europe during the Last Glacial Maximum (LGM). Climate variability affects the distribution of plant and animal resources unpredictably, creating an element of risk for foragers for whom mobility comes at a cost. We produce a model of habitat suitability that allows us to generate predictions about the probable distribution of human populations and discuss the implications of these predictions for the structure of human populations and their social and cultural evolution during the LGM.