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  <front>
    <journal-meta><journal-id journal-id-type="publisher">NPG</journal-id><journal-title-group>
    <journal-title>Nonlinear Processes in Geophysics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">NPG</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Nonlin. Processes Geophys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1607-7946</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/npg-33-385-2026</article-id><title-group><article-title>A simple dynamical system for representing  climate tipping points with hysteresis</article-title><alt-title>Simple hysteresis model</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Huntingford</surname><given-names>Chris</given-names></name>
          <email>chg@ceh.ac.uk</email>
        <ext-link>https://orcid.org/0000-0002-5941-7770</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Ritchie</surname><given-names>Paul D. L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7649-2991</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Clarke</surname><given-names>Joseph</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6250-1543</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>UK Centre for Ecology and Hydrology, Benson Lane, Wallingford, Oxfordshire, OX10 8BB, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Mathematics and Statistics, Faculty of Environment, Science and Economy,  University of Exeter, North Park Road, Exeter, EX4 4QE, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Global Systems Institute, Faculty of Environment, Science and Economy,  University of Exeter, North Park Road, Exeter, EX4 4QE, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Chris Huntingford (chg@ceh.ac.uk)</corresp></author-notes><pub-date><day>6</day><month>August</month><year>2026</year></pub-date>
      
      <volume>33</volume>
      <issue>3</issue>
      <fpage>385</fpage><lpage>399</lpage>
      <history>
        <date date-type="received"><day>29</day><month>January</month><year>2026</year></date>
           <date date-type="rev-request"><day>10</day><month>February</month><year>2026</year></date>
           <date date-type="rev-recd"><day>21</day><month>July</month><year>2026</year></date>
           <date date-type="accepted"><day>21</day><month>July</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Chris Huntingford et al.</copyright-statement>
        <copyright-year>2026</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://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026.html">This article is available from https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026.html</self-uri><self-uri xlink:href="https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026.pdf">The full text article is available as a PDF file from https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e118">The risk that the climate system may contain tipping points remains a concern. Firstly, a level of global warming may be reached at which relatively small additional warming could cause major parts of the Earth system to transition to a new state. Depending on the location and specific Earth system component, this could disproportionately impact large sectors of society. Secondly, the Earth system component may exhibit hysteresis effects, and therefore, if global temperatures are subsequently lowered after triggering a jump in state, a return to earlier conditions may not occur until warming is substantially reduced. Earth System Models (ESMs) are numerical frameworks that operate at fine spatial scales. Such models are designed to estimate how all components of the climate system will evolve in response to changes in atmospheric greenhouse gas concentrations caused by human activity. Many ESM projections suggest that various parts of the climate system are capable of tipping. Yet, these models are computationally demanding and have therefore been operated only over a small range of scenarios. Very few “overshoot” simulations with ESMs exist, where climate change is reversed, resulting in limited understanding of hysteresis effects following a tipping event.</p>

      <p id="d2e121">Advances in nonlinear mathematics include developing dynamical systems whose equations frequently contain a bifurcation parameter. These equations can accurately replicate tipping points, jumps in state, and hysteresis as the bifurcation parameter changes. Recent progress in ESM development often introduces higher spatial resolution, enhancing process representation and increasing accuracy in predicting local changes. However, mapping the broad behaviour of the components of ESM projections onto simpler dynamical system models may also offer many advantages, including the overall characterisation of climate models and a method to rapidly extrapolate their projections to a wider range of forcing scenarios. The bifurcation parameters in such equations may represent changing forcings, such as an increasing warming level that leads to a tipping event. Progress has already been made in mapping many components of the Earth system onto large-scale variables for representation as dynamical systems. Most advances to date have focused on understanding whether tipping events can be avoided if systems possess substantial inertia, i.e. respond over long timescales, allowing climate change to temporarily exceed thresholds that might otherwise trigger major nonlinear change. However, potential hysteresis effects in the context of climate change are less well represented in equation form. Achieving such a mathematical formulation requires a dynamic system to describe a climate system component not only at the point of tipping but also for substantial periods before and after. This behaviour corresponds to a bifurcation parameter that first increases and then decreases, with the modelled behaviours differing significantly during the return phase.</p>

      <p id="d2e124">To support such necessary developments, we present a parameter-sparse dynamical system model that can exhibit hysteresis following a tipping occurrence, offering the potential for characterising Earth system components with this feature. We place particular emphasis on presenting in full the algebra needed to map known or modelled key attributes of a system that can tip onto the simplified dynamical system equation.  We drive the equation with a time-evolving forcing representing an “overshoot” trajectory of global warming that exceeds a threshold for potential tipping. Calculations are performed over a range of system inertia values, illustrating a threshold inertia above which full tipping and hysteresis can be avoided.  We use scale analysis to relate this threshold to those reported in existing climate research on behaviour near potential tipping points.</p>

      <p id="d2e127">In some instances, a basic equation may be too simple to capture the dominant qualitative behaviour of a large-scale environmental system. In those cases, a more complex model from any hierarchy of suggested simulations of climate components may be appropriate. However, should a system be amenable to representation by a dynamical system, we hope the framework we present offers a simple-to-use equation structure that may quantify tipping points in the climate system. Such a framework may illustrate a more complete description of behaviours both before and after tipping, and depending on the post-tipping forcing scenario, it may involve substantial hysteresis.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Advanced Research and Invention Agency</funding-source>
<award-id>SCOP-PR01-P003</award-id>
</award-group>
<award-group id="gs2">
<funding-source>European Space Agency</funding-source>
<award-id>4000146344/24/I-LR</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Horizon 2020</funding-source>
<award-id>101137601</award-id>
</award-group>
<award-group id="gs4">
<funding-source>Natural Environment Research Council</funding-source>
<award-id>NE/W004895/1</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e139">Climate tipping points represent critical thresholds, typically expressed as levels of global warming, beyond which positive feedbacks can cause components of the Earth system to irreversibly shift to a new state <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx36 bib1.bibx37 bib1.bibx1" id="paren.1"/>.  Dansgaard–Oeschger events, observed in paleoclimate records, provide evidence of the capability of the Earth system to undergo such abrupt transitions <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx13" id="paren.2"/>.  With arguably insufficient progress being made on reducing human reliance on burning of fossil fuels, crossing climate tipping points in the near future is an increasingly likely scenario. Multiple generations of sophisticated climate models have displayed tipping behaviour in future climate scenarios <xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx3" id="paren.3"/>. Examples include, but are not limited to, dieback of the Amazon rainforest <xref ref-type="bibr" rid="bib1.bibx40 bib1.bibx42" id="paren.4"/>, collapse of large scale circulation currents in the Atlantic Ocean <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx38 bib1.bibx25 bib1.bibx39" id="paren.5"/>, melting of the polar ice sheets <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx56" id="paren.6"/> and alterations to atmospheric circulations <xref ref-type="bibr" rid="bib1.bibx39" id="paren.7"/>.</p>
      <p id="d2e164">The tipping behaviour observed in these complex climate models (or complex ESMs) may be amenable to characterisation and replication by low-dimensional nonlinear dynamical systems <xref ref-type="bibr" rid="bib1.bibx22" id="paren.8"/>.  Specifically, varying a parameter beyond a fold bifurcation can lead to bifurcation-induced tipping to an alternative state <xref ref-type="bibr" rid="bib1.bibx5" id="paren.9"/>. However, if the parameter only temporarily exceeds a fold bifurcation, tipping of the system may not occur <xref ref-type="bibr" rid="bib1.bibx50" id="paren.10"/>.  The peak distance beyond the bifurcation and the duration of such an overshoot follow an inverse square law relationship, with the proportionality constant depending on the inertia of a system <xref ref-type="bibr" rid="bib1.bibx49" id="paren.11"/>. A system with high inertia, such as large-scale ice sheets, is more likely to avoid tipping than a system with low inertia, such as coral reefs. This overshoot behaviour has been observed in both conceptual models <xref ref-type="bibr" rid="bib1.bibx50" id="paren.12"/> and complex climate models <xref ref-type="bibr" rid="bib1.bibx8" id="paren.13"/>.  Policymakers are increasingly interested in considering the possibility of a climate overshoot <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx46" id="paren.14"/>, which corresponds to a temporary period of warming above key target thresholds, after which temperatures are lowered back to those levels, potentially using engineering solutions.  The “Paris Target” <xref ref-type="bibr" rid="bib1.bibx55" id="paren.15"/> aims for society to limit global warming to 1.5 <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">°</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> above pre-industrial levels.  However, the temperatures recorded in recent years suggest that the planet may be very close to exceeding that threshold <xref ref-type="bibr" rid="bib1.bibx7" id="paren.16"/>, or may even be in the process of crossing it <xref ref-type="bibr" rid="bib1.bibx14" id="paren.17"/>. Hence, any final stabilisation at the 1.5° threshold is likely to occur after a temporary overshoot in global warming.</p>
      <p id="d2e208">However, a second key attribute of tipping points, should they be activated and a rapid move to a new state occur, is the potential for hysteresis.  This effect arises when lowering the forcing that initially triggered a tipping point may not result in a return to the pre-tipping state, and instead, the system remains locked in the new state. Hence, if a temporary period of warming overshoot causes a tipping point to occur, the reduction of temperatures after a peak level and back to below the tipping point threshold may not lead to a reversion to the states observed when temperatures were increasing.  Proposed examples of hysteresis in the climate system include the potential behaviour of the oceanic thermohaline circulation <xref ref-type="bibr" rid="bib1.bibx45" id="paren.18"/>, large-scale ice sheets <xref ref-type="bibr" rid="bib1.bibx28" id="paren.19"/>, the extent of mountain forest cover <xref ref-type="bibr" rid="bib1.bibx2" id="paren.20"/>, the level of tropical forest cover at key locations <xref ref-type="bibr" rid="bib1.bibx52" id="paren.21"/> and the position of the intertropical convergence zone <xref ref-type="bibr" rid="bib1.bibx34" id="paren.22"/>. A broad summary of the climate attributes investigated for hysteresis, using one ESM that has been driven by a substantial ramp-up and ramp-down forcing in atmospheric <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and thus global warming, is presented in <xref ref-type="bibr" rid="bib1.bibx12" id="text.23"/>. However, some quantities, such as mean local rainfall in many locations, may show little hysteresis when mapped against a global temperature profile that reverses <xref ref-type="bibr" rid="bib1.bibx59" id="paren.24"/>.  Understanding hysteresis requires a comprehensive assessment of a system that can tip, extending beyond merely quantifying its behaviour at the time or threshold of tipping.  Instead, a more wide-scale analysis is needed to determine the importance of hysteresis by identifying how much temperatures may need to decrease before a return to initial states is achieved.  Hence, capturing all these factors likely requires dynamical system models with more degrees of freedom and parameters than are needed to investigate the tipping point alone.</p>
      <p id="d2e244">Yet, although there are more complexities in understanding a system that can both tip and exhibit hysteresis when driven by forcings with reversal, much can still be gained from identifying dynamical system models that can capture such behaviours. One key benefit is that if the mapping of a full-complexity system onto a simpler structure is believed to be robust and captures the broad features of a nonlinear component of the Earth system, it may be forced for an extended set of pathways. This enables calculations for a much broader range of potential futures, which are not possible to perform with full Earth System Models (ESMs) due to their heavy computational requirements. This possibility is especially important for “overshoot” scenarios, as very few ESMs have been routinely forced for such trajectories. A second advantage is that valid simpler models capture overall behaviours, often through their bulk parameters.  Should a single simpler model be fitted to a range of ESMs, the resulting different parameter values provide a potentially concise way to quantify inter-ESM differences.  In the context of tipping points, this may involve characterising warming thresholds for tipping, the size of the jump to an alternative state, and the level of global cooling required to avoid hysteresis and return to any initial state. A third advantage is that if more high-frequency variability is added to the simpler model, and it is found to interact with nonlinearities in a way that mimics features of ESMs, this may open a path to creating better early warning systems for approaching tipping elements. Developing early warning systems for climate tipping points remains an area of active research <xref ref-type="bibr" rid="bib1.bibx21" id="paren.25"/> and discussion <xref ref-type="bibr" rid="bib1.bibx48" id="paren.26"/>.  All of these advantages are possible if candidate dynamical system models are available for calibration against ESMs, both locally at tipping points and for their broader behaviours, including the period before tipping and any irreversibility (i.e. hysteresis) post-tipping.</p>
      <p id="d2e254">Nonlinear mathematics has advanced substantially over recent decades <xref ref-type="bibr" rid="bib1.bibx26" id="paren.27"><named-content content-type="pre">e.g.</named-content></xref>, yielding sets of equations with bifurcation parameters <xref ref-type="bibr" rid="bib1.bibx35" id="paren.28"><named-content content-type="pre">e.g.</named-content></xref>. Upon adjustment of such parameters, these equations often exhibit simulated changes of state and irreversibility. Considerable progress has been made in mapping features of the climate system that are expected to have the potential to tip onto dynamical systems equations. The emphasis thus far has focused on studying the period when the system is near or at the tipping threshold.  Specifically, theory has been developed <xref ref-type="bibr" rid="bib1.bibx49" id="paren.29"/> to understand whether, for some components of the Earth system, there is sufficient inertia to allow a temporary overshoot of a global warming level that, in equilibrium, would definitely cause tipping. Quantification of the possibility of inertia preventing tipping during a climate overshoot period has been undertaken for multiple parts of the Earth system <xref ref-type="bibr" rid="bib1.bibx50 bib1.bibx51" id="paren.30"/>.</p>
      <p id="d2e273">To date, there has been far less progress in mapping the nonlinear behaviours of the Earth system onto dynamical systems when considering the full periods before and after tipping, or when tipping is averted due to inertia during temporary periods of high global warming. This omission is notable given the potential advances in understanding that could arise from such mappings. To bridge this gap, we present a relatively simple equation that exhibits tipping point and hysteresis effects.  The particular novelty of our contribution lies in our explicit identification of key parameters that define a potential large-scale component of the climate system that exhibits such nonlinearity. The proposed system consists of five parameters: the level of global warming at which tipping occurs, the extent of the system at the point of tipping, a lower temperature representing the end of any hysteresis, the extent of the system at that lower temperature, and finally, a parameter defining inertia.  A reader jumping to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) will find a proposed dynamical system with the required properties. The equations shown before Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) allow a mapping of the parameters of the latter onto the five system-related parameters.  Additionally, a reader can proceed to Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>), which outlines a forcing trajectory in global warming. This trajectory consists of the historical period, smoothly transitioning into an idealised future “upturned” quadratic pathway, with the ability to set the peak warming level.</p>
      <p id="d2e282">To support reproducibility, we replicate every step of the algebraic derivations, acknowledging that this makes the manuscript lengthy.  We hope that this approach enables the analysis to serve as a valuable manual on how, starting from scratch, one can map Earth system components onto a potential descriptive dynamical system equation.  This equation can then be used to explore tipping points, hysteresis, and inertial effects, as well as a range of potential global warming pathways, both with and without overshoot.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Mathematical model and parameterisation</title>
      <p id="d2e293">Our aim is to provide an equation and a forcing profile capable of replicating a system that exhibits a tipping point, hysteresis behaviour, and inertia effects.  We illustrate how the equation set may be calibrated (i.e. parameterised) and hope it will be useful to researchers wishing to quantify components of the Earth system believed to have strong nonlinear responses to climate change. Such beliefs may be driven by direct process understanding or based on assessments of projections by ESMs.  We have aimed for a parameter-sparse model framework, but its development still requires substantial algebraic manipulations to illustrate how the main equations can be fitted to process knowledge. For full reproducibility, we have chosen to present all such algebra, though the majority of the background derivations are placed in the Appendix.</p>
      <p id="d2e296">The paper leads to three main equations.  Equation (<xref ref-type="disp-formula" rid="Ch1.E7"/>) describes the time-evolution of the Earth system component of interest, with the preceding algebra showing how to relate it to parameters that define an actual system. Equation (<xref ref-type="disp-formula" rid="Ch1.E16"/>) presents a representative future “overshoot” forcing profile in temperature, with the preceding algebra relating it to a prescribed maximum level of global warming and ensuring a smooth transition onwards from the historical record of global warming. Equation (<xref ref-type="disp-formula" rid="Ch1.E24"/>) provides a condition that differentiates whether, for the parameters provided, a system exhibits tipping and hysteresis, or if the warming trajectory instead avoids a change of state.</p>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Mathematical model</title>
      <p id="d2e312">Guided by a model of hysteresis to describe the Atlantic Meridional Overturning Circulation (AMOC) <xref ref-type="bibr" rid="bib1.bibx57" id="paren.31"><named-content content-type="pre">e.g.</named-content></xref>, we start with an equation of the form:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M3" display="block"><mml:mrow><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>x</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mi>x</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Here, <inline-formula><mml:math id="M4" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> is a variable representing a changing component of the Earth system, which will be scaled to reflect the actual magnitude of this quantity.  We consider <inline-formula><mml:math id="M5" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> as a bifurcation parameter whose value changes according to a metric of human-induced climate change. Metrics of climate change could include altered radiative forcing (<inline-formula><mml:math id="M6" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>), atmospheric carbon dioxide equivalent <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>e (ppm), or global warming (K). Alternatively, if an attribute of the Earth system is strongly controlled by a regional and changing forcing from another part of the Earth system, then that attribute could instead determine the value of the evolving bifurcation parameter, <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>. Here, <inline-formula><mml:math id="M9" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> represents time (years) and <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is system inertia.</p>
      <p id="d2e438">We set the bifurcation parameter as a linear function of the amount of global warming since the pre-industrial period, <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> (K), as:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M12" display="block"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">γ</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e476">Many use this form of “cubic” model (e.g. Eq. <xref ref-type="disp-formula" rid="Ch1.E1"/>) to describe generic thermohaline circulations and often to better understand the effect of additional stochastic noise <xref ref-type="bibr" rid="bib1.bibx15" id="paren.32"><named-content content-type="pre">e.g.</named-content></xref>, or to explain features of palaeo records <xref ref-type="bibr" rid="bib1.bibx11" id="paren.33"/>. <xref ref-type="bibr" rid="bib1.bibx10" id="text.34"/> investigates Early Warning Systems (EWSs) specific to the Atlantic Meridional Overturning Circulation (AMOC) by considering high-frequency variability combined with such a dynamical system. Recently, <xref ref-type="bibr" rid="bib1.bibx62" id="text.35"/> presented such a model to describe the risk of deforestation and related atmospheric feedbacks that may cause the remaining forest to also transition to grassland, with their detailed use of an illustrative dynamical system highlighted by <xref ref-type="bibr" rid="bib1.bibx30" id="text.36"/>.  Coupled cubic dynamical systems are used to investigate the risk of cascading tipping points <xref ref-type="bibr" rid="bib1.bibx60 bib1.bibx61" id="paren.37"/>.</p>
      <p id="d2e502">A more general analysis of the cubic form of a dynamical system with added noise is presented by <xref ref-type="bibr" rid="bib1.bibx6" id="text.38"/>. Similarly, <xref ref-type="bibr" rid="bib1.bibx18" id="text.39"/>, with such a dynamical system, consider whether EWSs designed to alert to approaching tipping may be made more accurate when accounting for any temporal autocorrelation in forcing. <xref ref-type="bibr" rid="bib1.bibx23" id="text.40"/> illustrate, using such a model, that standard EWSs based on critical slowing down should be considered trustworthy only if both variance and autocorrelation increase.  The difficulty of understanding equilibrium states that may be far from contemporary observations is shown by such a cubic dynamical system <xref ref-type="bibr" rid="bib1.bibx20" id="paren.41"/>.  Associated with tipping points are the mathematical properties of related EWSs that additionally entrain spatial variation. <xref ref-type="bibr" rid="bib1.bibx17" id="text.42"/> consider cubic models at multiple locations with spatial connectivity, finding that, in some circumstances, accounting for spatial variation can produce more refined predictive statistics for distance to tipping. In some instances, a large scale process may be represented by a dynamical system, but it has to be more complex, potentially including more than one timescale (via parameter <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) or more than one state variable, <inline-formula><mml:math id="M14" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>, suggesting coupled equations.  In some particular cases, the equations may contain switches, with behaviour conditional on the state variable or forcing level. However, the form of Eq. (1) in the literature, which describes many aspects of large-scale environmental change, is well established, and our aim here is to facilitate its application to further Earth system components when the values of key underlying defining attributes are known.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Calibration of equilibrium model</title>
      <p id="d2e549">We first determine the equilibrium solutions of Eqs. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) and (<xref ref-type="disp-formula" rid="Ch1.E2"/>) as a function of different mean global temperatures above pre-industrial levels, which we consider to be the bifurcation parameter. We set the system to have a tipping point at <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. The hysteresis is such that a return to earlier original states occurs at <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. Hence, <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> represents a second tipping point, and <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> describes the width, in terms of global warming, over which hysteresis may occur. The quantity of interest, which is our state variable, is denoted as <inline-formula><mml:math id="M19" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, and is a scaled version of variable <inline-formula><mml:math id="M20" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>.  Our quantity of interest has a pre-industrial starting value of <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>PI</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> when <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and has a bifurcation (tipping point) at <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> when <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>.  Equilibrium solutions for higher temperatures beyond this point correspond to <inline-formula><mml:math id="M25" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> being in a substantially different state.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e717">Equilibrium solutions to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) for the tipping point defined at <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and for a second tipping point that marks the end of potential hysteresis for lowering temperatures at <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. Equations (<xref ref-type="disp-formula" rid="Ch1.E3"/>)–(<xref ref-type="disp-formula" rid="Ch1.E6"/>) are used to derive values of <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, respectively, as needed in Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>). These four parameters are functions of the prescribed values of <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> used in this study.  Additionally, vertical dashed lines are plotted independently at <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, as well as horizontal dashed lines at <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mi>X</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. The intersection of these lines at the tipping points provides visual verification of the algebra.</p></caption>
          <graphic xlink:href="https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026-f01.png"/>

        </fig>

      <p id="d2e945">We initially seek the form of Eqs. (<xref ref-type="disp-formula" rid="Ch1.E1"/>) and (<xref ref-type="disp-formula" rid="Ch1.E2"/>) that align with the specification of the parameters set out above, as described in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>. This gives an equation for <inline-formula><mml:math id="M38" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> as 

            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M39" display="block"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mfenced close="]" open="["><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">27</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:mfrac></mml:mstyle><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfenced><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></disp-formula>

          and an equation for <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as

            <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M41" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:mfrac></mml:mstyle><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e1066">We map from the actual variable (i.e. quantity) of interest, <inline-formula><mml:math id="M42" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, which is in its physical units, to the variable <inline-formula><mml:math id="M43" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> via a scaling of <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>X</mml:mi></mml:mrow></mml:math></inline-formula> (also shown as Eq. <xref ref-type="disp-formula" rid="App1.Ch1.S1.E32"/>). From this we derive in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/> that <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are given by

            <disp-formula id="Ch1.E5" content-type="numbered"><label>5</label><mml:math id="M47" display="block"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mfenced open="[" close="]"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow><mml:mn mathvariant="normal">4</mml:mn></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></disp-formula>

          and

            <disp-formula id="Ch1.E6" content-type="numbered"><label>6</label><mml:math id="M48" display="block"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:msup><mml:mfenced close="]" open="["><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow><mml:mn mathvariant="normal">4</mml:mn></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          We can now write out the governing equation as a function of the state variable, <inline-formula><mml:math id="M49" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>. Equations (<xref ref-type="disp-formula" rid="Ch1.E1"/>) and (<xref ref-type="disp-formula" rid="Ch1.E2"/>) may be combined, and with the scaling of Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E32"/>) and with <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, this gives:

            <disp-formula id="Ch1.E7" content-type="numbered"><label>7</label><mml:math id="M51" display="block"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>X</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>X</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>X</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Here, <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, as a consequence of changing from the quantity <inline-formula><mml:math id="M53" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> to <inline-formula><mml:math id="M54" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> in the left-hand time derivative of Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>).</p>
      <p id="d2e1435">We highlight Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) as it represents our dynamical system model in terms of the actual quantity of interest, <inline-formula><mml:math id="M55" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>.  Critically, using Eqs. (<xref ref-type="disp-formula" rid="Ch1.E3"/>)–(<xref ref-type="disp-formula" rid="Ch1.E6"/>), allows the four parameters of <inline-formula><mml:math id="M56" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) to be expressed as functions of the four user-defined quantities of <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx19" id="paren.43"><named-content content-type="pre">this has a similarity to the recent approach taken by</named-content></xref>. The user can also specify <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is a measure of system inertia. Additionally, the user can specify the bifurcation parameter and its changes, which here is global warming, <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, for which we explore different options in the sections below.</p>
      <p id="d2e1569">To provide a numerical example, we arbitrarily set the four defining parameters as <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.3</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">8.4</mml:mn></mml:mrow></mml:math></inline-formula> (in units of <inline-formula><mml:math id="M69" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>) and <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10.85</mml:mn></mml:mrow></mml:math></inline-formula> (units of <inline-formula><mml:math id="M71" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>). With these values, we determine the equilibrium solution (or solutions) for <inline-formula><mml:math id="M72" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> as a function of <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, corresponding to solving Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) with the left-hand side of that equation set to zero. These calculations are presented in Fig. <xref ref-type="fig" rid="F1"/>. The algebra is also applicable if <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>&gt;</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and therefore valid for any system that tips downward, which could correspond to an event such as the shutdown of AMOC or the loss of rainforest cover in the Amazon.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1700">Transient solutions to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) are examined for different but invariant values of the bifurcation parameter, <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, which here represents global warming.  We adopt the same parameter values for <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> as those used in Fig. <xref ref-type="fig" rid="F1"/>. Additionally, we set <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="unit"><mml:mo>(</mml:mo><mml:mi mathvariant="normal">K</mml:mi><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi mathvariant="normal">year</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mtext mathvariant="italic">X</mml:mtext><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">unit</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Each arrow represents a solution to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) with the starting point of the arrows defined by a set of initial conditions of <inline-formula><mml:math id="M80" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, and where the latter remains fixed during each calculation. Equation (<xref ref-type="disp-formula" rid="Ch1.E7"/>) is solved in each example for a simulated period of 15 years, with the tip of the arrow indicating the final timepoint of the calculation. Retained from Fig. <xref ref-type="fig" rid="F1"/> is the presentation of the equilibrium solution, which is now subdivided into the stable part (continuous line) and the unstable part (dashed line).</p></caption>
          <graphic xlink:href="https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026-f02.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Stability of equilibrium solutions with invariant bifurcation parameter</title>
      <p id="d2e1843">We first consider the temporal features of our model, without adjusting the bifurcation parameter, which implies keeping <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> invariant.  This scenario corresponds to a type of non-climatic forcing that adjusts our quantity <inline-formula><mml:math id="M83" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, after which it resets back towards a stable equilibrium state. We select a range of different initial states for <inline-formula><mml:math id="M84" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, and from these, we solve Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), with the latter temperature variable fixed. We perform calculations for the same selection of values for <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, as used for the equilibrium solutions of Fig. <xref ref-type="fig" rid="F1"/>. Additionally, we set the inertia to <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> (K year (X unit)<sup>−1</sup>). With these starting conditions and parameters, we solve for a period of 15 years using a simple explicit solver (calculating at 0.1 year timesteps). In Fig. <xref ref-type="fig" rid="F2"/>, each arrow corresponds to a solution, with the beginning of the arrow representing the starting conditions and the end of the arrow indicating the final value derived after the simulated 15 year period.  Hence, arrow length is representative of solution “velocity”.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Introduction of temporal forcing</title>
      <p id="d2e1962">We now consider a fully evolving system where the bifurcation parameter, representing global mean warming, adjusts over time.  Such an approach extends our analysis, as well as that of other researchers <xref ref-type="bibr" rid="bib1.bibx19" id="paren.44"><named-content content-type="pre">e.g.</named-content></xref>.  We create time-evolving scenarios for future global warming, extending the known historical record since pre-industrial times.  This extension is achieved by adding a quadratic temperature overshoot profile to the historical record.  We adopt the global mean warming temperature record from NASA-GISS <xref ref-type="bibr" rid="bib1.bibx41" id="paren.45"/> as our historical record, which currently spans the years 1880–2024, setting <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> for the year 1880.  Also included in that timeseries data is a version that is smoothed in time <xref ref-type="bibr" rid="bib1.bibx41" id="paren.46"><named-content content-type="pre">5 year lowess smoothing method; for details, see</named-content></xref>, which forms the basis for the historical values we employ.  We refer to this historical smoothed timeseries as <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>H,S</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. We use both the final values of that smoothed dataset and its gradient in time, leading up to the year <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mtext>2024–1880</mml:mtext></mml:mrow></mml:math></inline-formula> (year), to initialise our parabolic curves of future warming.</p>
      <p id="d2e2029">We first normalise the NASA-GISS smoothed warming record such that it is zero when averaged across the period 1880–1900 inclusive, to give a timeseries <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Hence,

            <disp-formula id="Ch1.E8" content-type="numbered"><label>8</label><mml:math id="M94" display="block"><mml:mrow><mml:mtable class="aligned" rowspacing="0.2ex" columnspacing="1em" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>H,S</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">for</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mn mathvariant="normal">0</mml:mn><mml:mo>≤</mml:mo><mml:mi>t</mml:mi><mml:mo>≤</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mspace linebreak="nobreak" width="1em"/><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2024</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1880</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mo>=</mml:mo><mml:msubsup><mml:mover accent="true"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>H,S</mml:mtext></mml:msub><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">21</mml:mn></mml:mrow></mml:msubsup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:math></disp-formula></p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e2175">Historical record of global warming up to the year 2024, normalised so that the average of the first 21 years (1880–1900 inclusive) is zero. From the year 2024 onwards, a quadratic “overshoot” profile is derived, corresponding to setting an upper level of global warming of <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> (as annotated). The vertical dotted line marks the year 2024. The future scenario is designed to transition smoothly from the historical measurement record in the year 2024.</p></caption>
          <graphic xlink:href="https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026-f03.png"/>

        </fig>

      <p id="d2e2206">We denote the final data value of <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, which is for the year 2024, as <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>.  Additionally, we define the final gradient of that smoothing as the change between the years 2014 and 2024, which we divide by ten and name as <inline-formula><mml:math id="M98" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">yr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>).  Hence, the two contemporary boundary conditions are <inline-formula><mml:math id="M100" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M101" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> at time <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, expressed as:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M103" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E9"><mml:mtd><mml:mtext>9</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E10"><mml:mtd><mml:mtext>10</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mfenced open="" close="|"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:msub><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          We calculate the coefficients for a quadratic overshoot function to smoothly extend the historical dataset by satisfying the boundary conditions given in Eqs. (<xref ref-type="disp-formula" rid="Ch1.E9"/>) and (<xref ref-type="disp-formula" rid="Ch1.E10"/>). The quadratic form then proceeds to a user-prescribed maximum value of global warming, <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, before declining. The quadratic form of future warming is defined as

            <disp-formula id="Ch1.E11" content-type="numbered"><label>11</label><mml:math id="M105" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mi>e</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mrow><mml:msup><mml:mo>*</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msup><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mi>g</mml:mi></mml:mrow></mml:math></disp-formula>

          We initially seek the form which incorporates offsets in time and warming as

            <disp-formula id="Ch1.E12" content-type="numbered"><label>12</label><mml:math id="M106" display="block"><mml:mrow><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="1em"/><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Thus, <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> (yr) and <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> (K) at the transition time, i.e. year 2024, moving from the historical record to the future warming scenario.  In Appendix <xref ref-type="sec" rid="App1.Ch1.S2"/> we derive values for <inline-formula><mml:math id="M109" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> as

            <disp-formula id="Ch1.E13" content-type="numbered"><label>13</label><mml:math id="M110" display="block"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          for <inline-formula><mml:math id="M111" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> as

            <disp-formula id="Ch1.E14" content-type="numbered"><label>14</label><mml:math id="M112" display="block"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          and for <inline-formula><mml:math id="M113" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula> as

            <disp-formula id="Ch1.E15" content-type="numbered"><label>15</label><mml:math id="M114" display="block"><mml:mrow><mml:mi>e</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mfenced close=")" open="("><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e2622">Removing the offsets of Eqs. (<xref ref-type="disp-formula" rid="Ch1.E12"/>) in Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>), then in terms of global warming, <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, and time, <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, the future projection for years following the end of the historical dataset (i.e. <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) is given by the key equation:

            <disp-formula id="Ch1.E16" content-type="numbered"><label>16</label><mml:math id="M118" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi>e</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi>g</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          with <inline-formula><mml:math id="M119" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M120" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M121" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> given by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E15"/>), (<xref ref-type="disp-formula" rid="Ch1.E14"/>) and (<xref ref-type="disp-formula" rid="Ch1.E13"/>) respectively. Hence, the quadratic future temperature trajectory parameters are a function of the historical timeseries leading to it, described by parameters <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M123" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>, along with the user-defined peak warming, <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. We regard the end of the extended timeseries as the year in which the quadratic function returns to zero global warming.</p>
      <p id="d2e2801">For our numerical calculations, we extend our historical record and calculate a future temperature trajectory using the boxed Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>), with a maximum level of global warming of <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>. Both the historical record and the future trajectory are shown in Fig. <xref ref-type="fig" rid="F3"/>.</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2831">Transient simulations are described by Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) and conducted with a forcing of global warming <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> given by Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>). The global warming driver is considered to change the bifurcation parameter. In all calculations, the initial condition to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) is that at the year 1880 (and so when <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>), the value of <inline-formula><mml:math id="M128" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> is the equilibrium solution. Calculations are performed for different values of <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, as marked by different colours and the legend. Small black arrows illustrate the direction, in time, of the phase curves. The axes are identical to those of Figs. <xref ref-type="fig" rid="F1"/> and <xref ref-type="fig" rid="F2"/>. The equilibrium solutions are retained from Fig. <xref ref-type="fig" rid="F2"/>, as shown by the black continuous and dashed lines. The maximum, i.e. peak level of global warming, in all five transient simulations is at <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>, as indicated by the inward tick mark on the “<inline-formula><mml:math id="M131" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>” axis.</p></caption>
          <graphic xlink:href="https://npg.copernicus.org/articles/33/385/2026/npg-33-385-2026-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Full model simulations with time-varying global warming</title>
      <p id="d2e2938">We investigate our model of tipping point behaviour when including full transient effects. The complete model is given by Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) combined with our timeseries of global warming described by Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>). It is recalled that in this model framework, we regard global warming, <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, as the bifurcation parameter. Simulations of this ordinary differential equation setup are initialised with the pre-industrial levels of <inline-formula><mml:math id="M133" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> at equilibrium. Specifically, the initial condition for all our calculations in the simulated year 1880 is the solution to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) with both the time derivative term and <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> set to zero.  For the parameters we use (i.e. <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>), this common value in the first year, <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, of all simulations in Fig. <xref ref-type="fig" rid="F4"/>, is <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">PI</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">7.06</mml:mn></mml:mrow></mml:math></inline-formula>. Five calculations are performed, corresponding to different and increasing inertia values, <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="unit"><mml:mo>(</mml:mo><mml:mi mathvariant="normal">K</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">yr</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>[</mml:mo><mml:mi mathvariant="normal">unit</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">of</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mtext>X</mml:mtext><mml:msup><mml:mo>]</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. A simple explicit solver is used again, with a timestep of 0.1 years.</p>
      <p id="d2e3091">Each simulation covers the full historical period plus the future time period of global warming overshoot, as shown in Fig. <xref ref-type="fig" rid="F3"/>. For the lowest inertia of <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F4"/>, red curve), around the time of maximum warming (i.e. <inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> reaches <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), the solution “tips” and moves directly to the equilibrium solution at a higher <inline-formula><mml:math id="M144" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>. At the next highest inertia of <inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula>, (Fig. <xref ref-type="fig" rid="F4"/>, orange curve), the solution also moves to the higher value of <inline-formula><mml:math id="M146" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, but takes longer to do so after the peak warming.  In both these cases, the solution will tip back to the starting branch (given sufficient time) since global warming drops below the lower fold bifurcation <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="unit"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula>. At the next test value of <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula>, (Fig. <xref ref-type="fig" rid="F4"/>, green curve), the solution makes an extensive excursion towards the higher equilibrium solution, but eventually returns towards the initial state for the period simulated.  For <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula>, (Fig. <xref ref-type="fig" rid="F4"/>, magenta curve), there is a similarity to that of the green curve, except that the excursion towards the upper equilibrium solution is much more limited. In the final calculation, with <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1000</mml:mn></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="F4"/>, blue curve), at this very high level of inertia, the solution exhibits very little variation in <inline-formula><mml:math id="M151" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S2.SS6">
  <label>2.6</label><title>Mathematical analysis</title>
      <p id="d2e3256">We now mathematically study the governing equation Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), forced by a potential overshoot scenario of future global temperature as set out in the quadratic form of Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>). Our goal in this section is to understand the factors that determine whether, when temperatures overshoot the tipping threshold, the system exhibits a relatively small excursion in <inline-formula><mml:math id="M152" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> before returning towards the initial state (blue, pink, and green curves in Fig. <xref ref-type="fig" rid="F4"/>) or instead follows a full hysteresis loop (yellow and red curves). In particular, we are interested in the role that inertia of the system, quantified by <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, plays in determining which of these cases occurs.</p>
      <p id="d2e3284">To understand the relative importance of different aspects of the system, we convert the equations into a non-dimensional form. Such a mapping often shows more clearly how different combinations of parameters affect the dynamics.  We introduce shifted <inline-formula><mml:math id="M154" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M155" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> variables, denoted as <inline-formula><mml:math id="M156" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M157" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> respectively, defined as:

            <disp-formula id="Ch1.E17" content-type="numbered"><label>17</label><mml:math id="M158" display="block"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>X</mml:mi></mml:mrow><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="1em"/><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>t</mml:mi><mml:mo>-</mml:mo><mml:msup><mml:mi>t</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mfrac></mml:mstyle><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          Here, <inline-formula><mml:math id="M159" display="inline"><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math id="M160" display="inline"><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula> are characteristic values of the <inline-formula><mml:math id="M161" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M162" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> quantities, and so by construction, <inline-formula><mml:math id="M163" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M164" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> are dimensionless variables.  We set these two new variables to obtain a nondimensional system that is as simple as possible, with the full derivation given in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>.  With

            <disp-formula id="Ch1.E18" content-type="numbered"><label>18</label><mml:math id="M165" display="block"><mml:mrow><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          and

            <disp-formula id="Ch1.E19" content-type="numbered"><label>19</label><mml:math id="M166" display="block"><mml:mrow><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:msqrt><mml:mi mathvariant="italic">β</mml:mi></mml:msqrt><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

          this results (see Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/>) in

            <disp-formula id="Ch1.E20" content-type="numbered"><label>20</label><mml:math id="M167" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          with the three nondimensional parameter clusters <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> equal to:

                <disp-formula specific-use="align" content-type="numbered"><mml:math id="M170" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E21"><mml:mtd><mml:mtext>21</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mrow><mml:mn mathvariant="normal">9</mml:mn></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E22"><mml:mtd><mml:mtext>22</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">8</mml:mn><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mi mathvariant="italic">δ</mml:mi><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mrow><mml:mn mathvariant="normal">27</mml:mn></mml:mfrac></mml:mstyle><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E23"><mml:mtd><mml:mtext>23</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mn mathvariant="normal">81</mml:mn></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          The analysis presented in Appendix <xref ref-type="sec" rid="App1.Ch1.S3"/> leads to an inequality. If this inequality is satisfied, then although the warming threshold for potential tipping is temporarily crossed, the jump to a new state is not achieved, and no major related hysteresis occurs. This inequality is given by the key equation

            <disp-formula id="Ch1.E24" content-type="numbered"><label>24</label><mml:math id="M171" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>≤</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">4</mml:mn></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:msqrt><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mfrac></mml:mstyle></mml:mrow></mml:msqrt></mml:mrow></mml:math></disp-formula>

          and is the same threshold, but in our notation, as in <xref ref-type="bibr" rid="bib1.bibx49" id="text.47"/>. This inequality is expected to be broadly valid for a range of temperature overshoots, not just those that are asymptotically small.  Finally, we can evaluate this inequality. Substituting the parameter choices that lead to Fig. <xref ref-type="fig" rid="F4"/> into Eqs. (<xref ref-type="disp-formula" rid="Ch1.E21"/>)–(<xref ref-type="disp-formula" rid="Ch1.E23"/>), while retaining the dependence on inertia, <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, gives:

            <disp-formula id="Ch1.E25" content-type="numbered"><label>25</label><mml:math id="M173" display="block"><mml:mtable columnspacing="1em" rowspacing="0.2ex" class="aligned" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.03241</mml:mn><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo><mml:mspace width="1em" linebreak="nobreak"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0.01428</mml:mn><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo><mml:mspace width="1em" linebreak="nobreak"/></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">9.18447</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d2e4024">Inserting these Eqs. (<xref ref-type="disp-formula" rid="Ch1.E25"/>) into the inequality Eq. (<xref ref-type="disp-formula" rid="Ch1.E24"/>) reveals that, for a temporary overshoot to avoid full tipping and hysteresis, requires inertia sufficiently large that <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">27.8</mml:mn></mml:mrow></mml:math></inline-formula>, which is in good agreement with Fig. <xref ref-type="fig" rid="F4"/>.</p>
</sec>
</sec>
<sec id="Ch1.S3" sec-type="conclusions">
  <label>3</label><title>Discussion and conclusions</title>
      <p id="d2e4057">The risk of triggering tipping points in major parts of the Earth system remains a key concern regarding potential responses to a changing climate as atmospheric greenhouse gases increase.  Tipping refers to a shift of an Earth system component to a new state, which may occur with relatively little additional climate change. This new state may also exhibit hysteresis, implying that any attempt to reverse climate change after tipping might not restore the system to its original state.  Research centres have contributed Earth System Models (ESMs) to the Climate Model Intercomparison Project version 6 <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx54" id="paren.48"/>, which inform the IPCC reports <xref ref-type="bibr" rid="bib1.bibx33" id="text.49"/>. ESMs predict various tipping points, but there is little consensus among these models about the level of climate change that would trigger their activation. Moreover, specific tipping points do not necessarily appear in all ESMs. To characterise the simulated tipping points, they should ideally be mapped onto a common equation framework, with parameters aligned to each ESM. Such equations may also enable the investigation of additional possible climate change trajectories for which ESMs have not been operated.</p>
      <p id="d2e4066">We begin with a moderately basic nonlinear ordinary differential equation, Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>), which exhibits tipping point and hysteresis effects. This equation, of “cubic” form, has been proposed by many to describe features of the Earth system (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/> for references), but there is presently no routine method to describe how to map climate tipping point features onto this model. To do this, we use a variable <inline-formula><mml:math id="M175" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> to represent our system state, denoting a component of the Earth system of interest. We assume that four quantities are available to define the background equilibrium states, either already known (e.g. estimated from palaeo data) or obtained from more complex ESM calculations. These parameters include the value of <inline-formula><mml:math id="M176" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> at tipping, <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and the global warming temperature at which it occurs, <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>.  The other two parameters are the value of <inline-formula><mml:math id="M179" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> at the end of hysteresis, <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and the corresponding lower global warming temperature at which it occurs, <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. These four parameters are illustrated in Fig. <xref ref-type="fig" rid="F1"/>.</p>
      <p id="d2e4145">The particular form of the governing equation that we propose is our key process Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>). If we initially neglect the transient left-hand-side term (by setting it to zero), the remaining equation describes the pseudo-equilibrium solutions for various values of global warming, <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>. In this context, the assumption is that there are very slow palaeo-timescale changes in <inline-formula><mml:math id="M183" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, which we consider as a bifurcation parameter.  The right-hand side of Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) involves four unknown parameters, <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. These parameters are functions of our four user-defined parameters, <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M187" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, as specified by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E3"/>)–(<xref ref-type="disp-formula" rid="Ch1.E6"/>).</p>
      <p id="d2e4250">We introduce transient effects into our calculations in two ways. We assume that the system simulated by the variable <inline-formula><mml:math id="M188" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> has inertial effects, which we represent by a fifth user-defined parameter, <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, in Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>). Then we introduce a time-evolving profile for global warming, <inline-formula><mml:math id="M190" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, which combines the historical record with a future “overshoot” scenario that we model as quadratic. The three quadratic coefficients are partially constrained by the magnitude (<inline-formula><mml:math id="M191" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) and the rate of change of warming (<inline-formula><mml:math id="M192" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>) for the contemporary period, thereby ensuring a smooth transition from the warming of the recent past to that of the simulated future. The required third constraint is a user-prescribed value for the peak level of global warming, <inline-formula><mml:math id="M193" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.  This warming profile leads to our second key equation, Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>), as illustrated in Fig. <xref ref-type="fig" rid="F3"/> and for our value of <inline-formula><mml:math id="M194" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.8</mml:mn></mml:mrow></mml:math></inline-formula>.  The three parameters of <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>,</mml:mo><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are translated into the three parameters <inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:mi>e</mml:mi><mml:mo>,</mml:mo><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M198" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula>, given by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E15"/>), (<xref ref-type="disp-formula" rid="Ch1.E14"/>) and (<xref ref-type="disp-formula" rid="Ch1.E13"/>) respectively.</p>
      <p id="d2e4401">Our second aim is to investigate and characterise solutions to Eqs. (<xref ref-type="disp-formula" rid="Ch1.E7"/>) and (<xref ref-type="disp-formula" rid="Ch1.E16"/>) for a range of inertial values, <inline-formula><mml:math id="M199" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, in response to human-induced climate change.  The focus on an overshoot warming profile is deliberate, as it allows us to consider the potential for hysteresis should a tipping point be activated and there is a reversal of forcing. If society achieves eventual climate stabilisation at a global warming level of 1.5 or 2 <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">°</mml:mi><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> above pre-industrial levels, this may occur after a temporary period of higher global temperatures. Such an overshoot is possible, given that current emissions levels may not be falling sufficiently fast to allow the climate system to approach a stabilisation maximum temperature only from below.  Using numerical calculations, we find that for high inertia, the variable <inline-formula><mml:math id="M201" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> will not exhibit major tipping and hysteresis (Fig. <xref ref-type="fig" rid="F4"/>). Employing the nondimensionalisation method to our model and forcing equations, we estimate with Eq. (<xref ref-type="disp-formula" rid="Ch1.E24"/>) a threshold that determines whether tipping can be avoided. These calculations relate to existing analysis <xref ref-type="bibr" rid="bib1.bibx49 bib1.bibx50 bib1.bibx51" id="paren.50"><named-content content-type="pre">e.g.</named-content></xref> that estimates the risk of tipping when the equilibrium level for activation is temporarily crossed. If there is additional understanding leading to a known value of <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, then the model equation, Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), is fully constrained by process knowledge.</p>
      <p id="d2e4459">Equation (<xref ref-type="disp-formula" rid="Ch1.E7"/>) is available to assess responses to forcings of alternative future trajectories in global warming, <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>. Our quadratic form, which we consider as eventually returning to pre-industrial conditions, may be replaced with more sophisticated profiles that stabilise at key warming thresholds, either with or without a period of overshoot. Algebraic forms exist for such profiles <xref ref-type="bibr" rid="bib1.bibx32" id="paren.51"><named-content content-type="pre">e.g.</named-content></xref>, opening the possibility of further analytic assessment, again without relying solely on numerical understanding. The equation system is also available for forcing with monotonically increasing global temperatures, which is likely to occur during the 21st Century if society follows any of the standard Shared Socioeconomic Pathways (SSPs) <xref ref-type="bibr" rid="bib1.bibx47" id="paren.52"/> that are associated with the continued substantial burning of fossil fuels.</p>
      <p id="d2e4482">Due to concerns that human-induced climate alteration may cause key components of the Earth system to tip, there is substantial interest in developing early warning systems for such events <xref ref-type="bibr" rid="bib1.bibx21" id="paren.53"><named-content content-type="pre">e.g.</named-content></xref>.  Although generic types of such warning systems exist, such as those that assess for evidence of critical slowing down, more bespoke forms may be developed for particular parts of the climate system. We suggest that a calibrated dynamical system, which accurately describes a key process, could also support the development of such warning systems. For instance, adding high-frequency noise to Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), either to <inline-formula><mml:math id="M204" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M205" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, and studying the simulated responses and how they change as tipping approaches, may lead to the discovery of more accurate warning methods.</p>
      <p id="d2e4509">Our analysis has some caveats. The generic cubic form, in <inline-formula><mml:math id="M206" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, of the right-hand side of Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), to some extent, predetermines any path taken by the state variable in the presence of hysteresis. The actual components of the climate system may exhibit slightly different forms, necessitating more complex algebraic expressions that introduce perturbation terms to the cubic structure.  In addition, utilising the normal form and a linear change in variables assumes a certain symmetry to the problem, for example, as seen in Fig. <xref ref-type="fig" rid="F1"/>.  At the midpoint between the folds of <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> the distances to the basin boundary (the middle unstable branch), from the stable top and lower branches, are the same.  However, some problems might require a nonlinear coordinate change, which could lead to asymmetric basins of attraction.  The equations we provide model only a single state variable, <inline-formula><mml:math id="M209" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, while there is concern that the activation of a tipping point may alter the timing of others, creating a cascade effect.  A suggested set of equations that captures such effects, along with their couplings, is provided by <xref ref-type="bibr" rid="bib1.bibx60" id="text.54"/>.  In our modelling framework, we only consider the passage through fold bifurcations. However, tipping can arise from oscillatory instabilities, which are often attributed to passing through a Hopf bifurcation. Or, alternatively, tipping can even occur without crossing any bifurcations via rate-induced tipping, such as those attributed to peatland fires <xref ref-type="bibr" rid="bib1.bibx16" id="paren.55"/>.</p>
      <p id="d2e4563">In summary, we provide a relatively simple equation on to which the behaviour of climate components expected to exhibit a tipping point, leading to a new state, can potentially be mapped. The equation can simulate hysteresis effects.  Given the interest in the risk of climate tipping points being triggered by further human-induced climate change, and noting that ESMs differ substantially in their projections of the timing of such events, these mappings may offer a direct method to compare climate projections. The key equation is Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), and its parameters are given by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E3"/>)–(<xref ref-type="disp-formula" rid="Ch1.E6"/>). Simplified equations that effectively emulate the bulk features of complex components of the climate system are suitable for investigating a broad range of future climate change scenarios, which may not be feasible with ESMs due to their high computational cost.  We note that some climate research centres are starting to force ESMs with overshoot-type scenarios, and any simulated hysteresis effects may be amenable to mapping onto our dynamical system framework.  Here, we examine overshoot scenarios using the key profile of Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>), with its parameters given by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E13"/>)–(<xref ref-type="disp-formula" rid="Ch1.E15"/>). We utilise this framework to explore how the prescription of system inertia determines whether full tipping with hysteresis occurs, and we link our findings analytically back to the existing literature via Eq. (<xref ref-type="disp-formula" rid="Ch1.E24"/>). There are already extensive and valuable analyses of potential tipping points in the literature, focusing on behaviour at the time when a major change in a climate component might be expected. Such literature includes examples using the “cubic” form (see Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/>), while also noting in particular the historical development of dynamical systems to represent AMOC changes <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx44 bib1.bibx29" id="paren.56"><named-content content-type="pre">e.g.</named-content></xref>.  We hope that the equations presented here provide an opportunity to more fully quantify behaviours over longer periods, both before and after potential climate tipping events.</p>
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    <back><app-group>

<app id="App1.Ch1.S1">
  <label>Appendix A</label><title>Derivation of parameters <inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for the equilibrium solution</title>
      <p id="d2e4633">Here, we present the derivation of parameters <inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, as required in the main model of Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), and expressed as a function of the user-prescribed parameters <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e4711">We first seek solutions at the two turning points (tipping points) in the equilibrium solution. The equilibrium solution, expressed as a function of <inline-formula><mml:math id="M216" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula>, is, from Eq. (<xref ref-type="disp-formula" rid="Ch1.E1"/>), given by

          <disp-formula id="App1.Ch1.S1.E26" content-type="numbered"><label>A1</label><mml:math id="M217" display="block"><mml:mrow><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:msup><mml:mi>x</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mi>x</mml:mi><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        and so if real turning points exist, they satisfy

          <disp-formula id="App1.Ch1.S1.E27" content-type="numbered"><label>A2</label><mml:math id="M218" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">μ</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:msup><mml:mi>x</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Hence, for a given <inline-formula><mml:math id="M219" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> value, the two equilibrium turning point solutions for <inline-formula><mml:math id="M220" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> can be derived from Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E27"/>). When these solutions are placed back in Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E26"/>), this determines <inline-formula><mml:math id="M221" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> as:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M222" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.S1.E28"><mml:mtd><mml:mtext>A3</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo><mml:mspace width="1em" linebreak="nobreak"/><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">β</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>;</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="App1.Ch1.S1.E29"><mml:mtd><mml:mtext>A4</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="1em"/><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">β</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

        Next, we attempt to satisfy the two boundary conditions for the tipping point at the higher <inline-formula><mml:math id="M223" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> value i.e. at the user-supplied value of <inline-formula><mml:math id="M224" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and also at the lower tipping point of <inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, which marks the end of hysteresis.  As this involves satisfying two equations with two unknowns, we set <inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, and solve for <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M228" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> (where the latter is assumed to be positive and real). Hence, from Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>) with <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:mi mathvariant="italic">γ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, and using Eqs. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E28"/>) and (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E29"/>), and noting we wish the higher <inline-formula><mml:math id="M230" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> value (e.g. Eq. <xref ref-type="disp-formula" rid="App1.Ch1.S1.E28"/>) to correspond to <inline-formula><mml:math id="M231" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, the equations to be solved are:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M232" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.S1.E30"><mml:mtd><mml:mtext>A5</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">β</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="App1.Ch1.S1.E31"><mml:mtd><mml:mtext>A6</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">β</mml:mi></mml:mrow><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

        Subtracting Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E31"/>) from Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E30"/>) and then rearranging for <inline-formula><mml:math id="M233" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> gives Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). Adding Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E31"/>) to Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E30"/>) and then rearranging, gives an equation for <inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, as Eq. (<xref ref-type="disp-formula" rid="Ch1.E4"/>).</p>
      <p id="d2e5162">We next consider the boundary conditions on <inline-formula><mml:math id="M235" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula>. We map from the actual variable (i.e. quantity) of interest, <inline-formula><mml:math id="M236" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, which is in its physical units, to the variable <inline-formula><mml:math id="M237" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> via a scaling of

          <disp-formula id="App1.Ch1.S1.E32" content-type="numbered"><label>A7</label><mml:math id="M238" display="block"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi>X</mml:mi><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Noting that the analytical solutions of model behaviour, given by Eqs. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E28"/>) and (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E29"/>), occur at the two turning points of <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula>, we relate these to prescribed representative features of <inline-formula><mml:math id="M240" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>.  We specify the value of <inline-formula><mml:math id="M241" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> at the tipping point as <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and at the lower temperature tipping point that marks the end of hysteresis, as <inline-formula><mml:math id="M243" display="inline"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>. From Eqs. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E30"/>) and (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E31"/>), this implies that:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M244" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.S1.E33"><mml:mtd><mml:mtext>A8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="App1.Ch1.S1.E34"><mml:mtd><mml:mtext>A9</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

        Subtracting Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E33"/>) from Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E34"/>) and then rearranging for <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> gives

          <disp-formula id="App1.Ch1.S1.E35" content-type="numbered"><label>A10</label><mml:math id="M246" display="block"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Adding Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E33"/>) to Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E34"/>), rearranging for <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and substituting for <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E35"/>) gives

          <disp-formula id="App1.Ch1.S1.E36" content-type="numbered"><label>A11</label><mml:math id="M249" display="block"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msqrt><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msqrt><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        In a final calculation, we eliminate <inline-formula><mml:math id="M250" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> in Eqs. (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E35"/>) and (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E36"/>). Noting from Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>) that we can write <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msqrt><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msqrt><mml:mo>=</mml:mo><mml:mo>[</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>)</mml:mo><mml:mo>/</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:msup><mml:mo>]</mml:mo><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, this gives Eq. (<xref ref-type="disp-formula" rid="Ch1.E5"/>) for <inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and Eq. (<xref ref-type="disp-formula" rid="Ch1.E6"/>) for <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</app>

<app id="App1.Ch1.S2">
  <label>Appendix B</label><title>Derivation of parameters <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:mi>e</mml:mi><mml:mo>,</mml:mo><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M255" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> for the future quadratic warming scenario</title>
      <p id="d2e5619">Here, we derive the parameters <inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:mi>e</mml:mi><mml:mo>,</mml:mo><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M257" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula>, which are required in Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>), and where this equation is a quadratic form for a future warming scenario.  These parameters depend on the absolute values and the time gradient at the end of the NASA-GISS <xref ref-type="bibr" rid="bib1.bibx41" id="paren.57"/> dataset, ensuring a smooth transition to the projection of future warming. The projection includes a maximum warming, <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which is a quantity available to set by the user, and thus also influences the parameterisation of the quadratic.</p>
      <p id="d2e5659">The boundary condition that <inline-formula><mml:math id="M259" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, combined with Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>), yields the equation for <inline-formula><mml:math id="M260" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> as Eq. (<xref ref-type="disp-formula" rid="Ch1.E13"/>).  Differentiating Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>) with respect to <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, and calculating that quantity at <inline-formula><mml:math id="M262" display="inline"><mml:mrow><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, in conjunction with the second boundary condition, Eq. (<xref ref-type="disp-formula" rid="Ch1.E10"/>), gives the equation for <inline-formula><mml:math id="M263" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> as Eq. (<xref ref-type="disp-formula" rid="Ch1.E14"/>).</p>
      <p id="d2e5730">The third boundary condition allows a user to specify a maximum (i.e. peak) level of global warming, <inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, which therefore corresponds to when the profile has a zero gradient in time.  Hence, from Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>) with boundary condition (<xref ref-type="disp-formula" rid="Ch1.E14"/>), this occurs at the time when

          <disp-formula id="App1.Ch1.S2.E37" content-type="numbered"><label>B1</label><mml:math id="M265" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></disp-formula>

        which implies that <inline-formula><mml:math id="M266" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>e</mml:mi><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="italic">δ</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and so occurs at time

          <disp-formula id="App1.Ch1.S2.Ex1"><mml:math id="M267" display="block"><mml:mrow><mml:msup><mml:mi>t</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi>e</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Substituting this time, along with the boundary conditions Eqs. (<xref ref-type="disp-formula" rid="Ch1.E13"/>) and (<xref ref-type="disp-formula" rid="Ch1.E14"/>), back into Eq. (<xref ref-type="disp-formula" rid="Ch1.E11"/>) results in a peak warming, <inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>T</mml:mi><mml:mi mathvariant="normal">p</mml:mi><mml:mo>*</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, of:

          <disp-formula id="App1.Ch1.S2.E38" content-type="numbered"><label>B2</label><mml:math id="M269" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msubsup><mml:mi>T</mml:mi><mml:mi mathvariant="normal">p</mml:mi><mml:mo>*</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mi>e</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        Here, the peak level of global warming, <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (K), is defined above pre-industrial levels.  Hence by accounting for the offset between <inline-formula><mml:math id="M271" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>*</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula>, given by <inline-formula><mml:math id="M273" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (see Eq. <xref ref-type="disp-formula" rid="Ch1.E12"/>), and combining this with Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S2.E38"/>), we obtain

          <disp-formula id="App1.Ch1.S2.Ex2"><mml:math id="M274" display="block"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mi>e</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula>

        which, upon rearrangement, provides the parameter <inline-formula><mml:math id="M275" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula> as Eq. (<xref ref-type="disp-formula" rid="Ch1.E15"/>).</p>
</app>

<app id="App1.Ch1.S3">
  <label>Appendix C</label><title>Derivation of nondimensionalisation of the governing equation</title>
      <p id="d2e5999">This section provides a nondimensionalisation of the main equation, while simultaneously accounting for the scenario of future global warming that is quadratic in form.</p>
      <p id="d2e6002">We insert Eqs. (<xref ref-type="disp-formula" rid="Ch1.E17"/>) into Eq. (<xref ref-type="disp-formula" rid="Ch1.E7"/>), and then substituting for <inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> using Eq. (<xref ref-type="disp-formula" rid="Ch1.E16"/>) yields

          <disp-formula id="App1.Ch1.S3.E39" content-type="numbered"><label>C1</label><mml:math id="M277" display="block"><mml:mtable rowspacing="0.2ex" columnspacing="1em" class="aligned" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mfrac></mml:mstyle><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>-</mml:mo><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:msup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>e</mml:mi><mml:msup><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:mi>g</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

        Dividing Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E39"/>) throughout by <inline-formula><mml:math id="M278" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula>, and noting that <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mi>g</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>, this reduces to

          <disp-formula id="App1.Ch1.S3.E40" content-type="numbered"><label>C2</label><mml:math id="M280" display="block"><mml:mtable columnspacing="1em" rowspacing="0.2ex" class="aligned" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:msup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:mi>e</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

        We can now choose the parameters <inline-formula><mml:math id="M281" display="inline"><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math id="M282" display="inline"><mml:mover accent="true"><mml:mi>t</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:math></inline-formula> to simplify the analysis. First, we eliminate the constant (i.e. set it to unity) in front of the <inline-formula><mml:math id="M283" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> term of Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E40"/>) by selecting the time scaling of Eq. (<xref ref-type="disp-formula" rid="Ch1.E18"/>) which gives

          <disp-formula id="App1.Ch1.S3.E41" content-type="numbered"><label>C3</label><mml:math id="M284" display="block"><mml:mtable columnspacing="1em" rowspacing="0.2ex" class="aligned" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow><mml:mi mathvariant="italic">β</mml:mi></mml:mfrac></mml:mstyle><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo stretchy="false" mathvariant="normal">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:mi>e</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:msubsup><mml:mover accent="true"><mml:mi>X</mml:mi><mml:mo mathvariant="normal" stretchy="false">^</mml:mo></mml:mover></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula>

        The temporal scaling of Eq. (<xref ref-type="disp-formula" rid="Ch1.E18"/>) illustrates the inertia of the system, as it will have longer natural timescales for higher values of <inline-formula><mml:math id="M285" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.  Second, we eliminate the constant in front of the <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> term of Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E41"/>), which provides a natural scale for <inline-formula><mml:math id="M287" display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> which is Eq. (<xref ref-type="disp-formula" rid="Ch1.E19"/>), which results in

          <disp-formula id="App1.Ch1.S3.E42" content-type="numbered"><label>C4</label><mml:math id="M288" display="block"><mml:mtable class="aligned" columnspacing="1em" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mi>y</mml:mi><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mrow><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>+</mml:mo><mml:mi>f</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:mi>e</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi>c</mml:mi><mml:mi>p</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mn mathvariant="normal">7</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:msubsup><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d2e6773">Finally, we can introduce the non-dimensional parameter clusters <inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M290" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which we set equal to the parameters in front of the constant, linear and quadratic terms in <inline-formula><mml:math id="M292" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>, respectively, of Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E42"/>). With these definitions, the governing equation of motion simplifies to the form of Eq. (<xref ref-type="disp-formula" rid="Ch1.E20"/>).  From Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E42"/>), we write the five parameters <inline-formula><mml:math id="M293" display="inline"><mml:mrow><mml:mi mathvariant="italic">β</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">μ</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:mi>e</mml:mi><mml:mo>,</mml:mo><mml:mi>f</mml:mi></mml:mrow></mml:math></inline-formula> in terms of the original parameters that define the physical problem (<inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>TP</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi>X</mml:mi><mml:mtext>HYS</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and the forcing (<inline-formula><mml:math id="M296" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msup><mml:mi>T</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>,</mml:mo><mml:mi mathvariant="italic">δ</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">P</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). This is achieved using the five Eqs. (<xref ref-type="disp-formula" rid="Ch1.E3"/>), (<xref ref-type="disp-formula" rid="Ch1.E4"/>), (<xref ref-type="disp-formula" rid="App1.Ch1.S1.E35"/>), (<xref ref-type="disp-formula" rid="Ch1.E15"/>) and (<xref ref-type="disp-formula" rid="Ch1.E14"/>), which reveal the <inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> non-dimensional parameter clusters as given by Eqs. (<xref ref-type="disp-formula" rid="Ch1.E21"/>)–(<xref ref-type="disp-formula" rid="Ch1.E23"/>).  In the simplified non-dimensional form of Eq. (<xref ref-type="disp-formula" rid="Ch1.E20"/>), the bifurcation structure of the system becomes parameter independent. The system has bifurcations at <inline-formula><mml:math id="M299" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mrow></mml:math></inline-formula> when <inline-formula><mml:math id="M300" display="inline"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mo>∓</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d2e7038">Using the approach of <xref ref-type="bibr" rid="bib1.bibx49 bib1.bibx50 bib1.bibx51" id="text.58"/>, we can quantify whether the forcing, <inline-formula><mml:math id="M301" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>T</mml:mi></mml:mrow></mml:math></inline-formula> (which is implicit in the variable <inline-formula><mml:math id="M302" display="inline"><mml:mi mathvariant="italic">π</mml:mi></mml:math></inline-formula>), can overshoot the threshold, <inline-formula><mml:math id="M303" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi>T</mml:mi><mml:mtext>TP</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, without causing tipping and thus avoiding hysteresis. Such findings can include any dependence on inertia, <inline-formula><mml:math id="M304" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.  The analysis of <xref ref-type="bibr" rid="bib1.bibx49" id="text.59"/> requires information about the forcing, as well as two parameters, which we refer to as <inline-formula><mml:math id="M305" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M306" display="inline"><mml:mi mathvariant="italic">κ</mml:mi></mml:math></inline-formula>. If the non-dimensional model is written as <inline-formula><mml:math id="M307" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>y</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>=</mml:mo><mml:mi>F</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">π</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">τ</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, then <inline-formula><mml:math id="M308" display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M309" display="inline"><mml:mi mathvariant="italic">κ</mml:mi></mml:math></inline-formula> are defined as partial derivatives of <inline-formula><mml:math id="M310" display="inline"><mml:mi>F</mml:mi></mml:math></inline-formula>, evaluated at the tipping point <inline-formula><mml:math id="M311" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">π</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>/</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. These parameters are given by:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M312" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.S3.E43"><mml:mtd><mml:mtext>C5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi mathvariant="italic">π</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.33em" linebreak="nobreak"/><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="App1.Ch1.S3.E44"><mml:mtd><mml:mtext>C6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">κ</mml:mi></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">λ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msup><mml:mo>∂</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi>F</mml:mi></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:msup><mml:mi>y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d2e7296">The information about the (non-dimensional) forcing required to determine whether an overshoot causes tipping is its peak amplitude, <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, and its curvature at the peak, <inline-formula><mml:math id="M314" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">π</mml:mi><mml:mo mathvariant="normal">¨</mml:mo></mml:mover><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">π</mml:mi><mml:mo mathvariant="normal">¨</mml:mo></mml:mover><mml:mo>=</mml:mo><mml:msup><mml:mi mathvariant="normal">d</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi mathvariant="italic">π</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi mathvariant="italic">τ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>. As <inline-formula><mml:math id="M316" display="inline"><mml:mi mathvariant="italic">π</mml:mi></mml:math></inline-formula> is quadratic in <inline-formula><mml:math id="M317" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>, these two quantities can easily be derived to be:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M318" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="App1.Ch1.S3.E45"><mml:mtd><mml:mtext>C7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="App1.Ch1.S3.E46"><mml:mtd><mml:mtext>C8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mover accent="true"><mml:mi mathvariant="italic">π</mml:mi><mml:mo mathvariant="normal">¨</mml:mo></mml:mover><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mspace linebreak="nobreak" width="0.33em"/><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

        Using our notation, the relationship found by <xref ref-type="bibr" rid="bib1.bibx49" id="text.60"/> that sets limits on the overshoot required to avoid tipping is given by: 

          <disp-formula id="App1.Ch1.S3.E47" content-type="numbered"><label>C9</label><mml:math id="M319" display="block"><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub><mml:mo>≤</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">2</mml:mn><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:msqrt><mml:mn mathvariant="normal">3</mml:mn></mml:msqrt></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">λ</mml:mi></mml:mfrac></mml:mstyle><mml:msqrt><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">π</mml:mi><mml:mo mathvariant="normal">¨</mml:mo></mml:mover><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">κ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:msqrt><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

        If this inequality holds, then although the warming threshold for potential tipping is temporarily crossed, the jump to a new state is not activated, and no major related hysteresis occurs.  Substituting <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">κ</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="italic">π</mml:mi><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M321" display="inline"><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">π</mml:mi><mml:mo mathvariant="normal">¨</mml:mo></mml:mover><mml:msub><mml:mo>|</mml:mo><mml:mtext>peak</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> from Eqs. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E43"/>)–(<xref ref-type="disp-formula" rid="App1.Ch1.S3.E46"/>) into Eq. (<xref ref-type="disp-formula" rid="App1.Ch1.S3.E47"/>), we can rearrange to give the condition in terms of the non-dimensional parameters, <inline-formula><mml:math id="M322" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>,</mml:mo><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M323" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">π</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, as Eq. (<xref ref-type="disp-formula" rid="Ch1.E24"/>).</p>
</app>
  </app-group><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d2e7600">Most of this research is analytical. However, the python computer code leading to the four figures is available, on request, from Chris Huntingford (chg@ceh.ac.uk).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d2e7606">No data sets were used in this article.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e7612">CH devised the original concept and framework and performed the algebra leading to the diagrams. JC undertook the nondimensionalisation, and PDLR aligned this with previous analysis of inertia effects at the point of tipping. All authors supported writing the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e7618">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e7624">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e7630">This research has been supported by the Advanced Research and Invention Agency, the European Space Agency, the European Union and the Natural Environment Research Council. Views and opinions expressed are, however, those of the author(s) only and do not necessarily reflect those of the European Union or the European Climate, Infrastructure and Environment Executive Agency (CINEA) or other funders.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e7635">Chris Huntingford and Paul D. L. Ritchie acknowledge funding by the Advanced Research and Invention Agency (ARIA) (grant SCOP-PR01-P003 – Advancing Tipping Point Early Warning, “AdvanTip”). Chris Huntingford and Joseph Clarke acknowledge funding by the European Space Agency (ESA), (contract no. 4000146344/24/I-LR). Chris Huntingford was supported by the TerraFIRMA program of the Natural Environment Research Council, grant number NE/W004895/1. Paul D. L. Ritchie was supported by the European Union's Horizon Europe research and innovation programme under grant agreement No. 101137601 (ClimTip).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e7641">This paper was edited by Vicente Perez-Munuzuri and reviewed by Marek Stastna and three anonymous referees.</p>
  </notes><ref-list>
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