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  <front>
    <journal-meta><journal-id journal-id-type="publisher">BG</journal-id><journal-title-group>
    <journal-title>Biogeosciences</journal-title>
    <abbrev-journal-title abbrev-type="publisher">BG</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Biogeosciences</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1726-4189</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/bg-18-4937-2021</article-id><title-group><article-title>Estimated effect of the permafrost carbon feedback on the zero emissions commitment to climate change</article-title><alt-title>ZEC and the permafrost carbon feedback</alt-title>
      </title-group><?xmltex \runningtitle{ZEC and the permafrost carbon feedback}?><?xmltex \runningauthor{A.~H.~MacDougall}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>MacDougall</surname><given-names>Andrew H.</given-names></name>
          <email>amacdoug@stfx.ca</email>
        <ext-link>https://orcid.org/0000-0001-7899-9940</ext-link></contrib>
        <aff id="aff1"><institution>Climate &amp; Environment, St. Francis Xavier University, Antigonish, B2G 2W5, Canada</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Andrew H. MacDougall (amacdoug@stfx.ca)</corresp></author-notes><pub-date><day>10</day><month>September</month><year>2021</year></pub-date>
      
      <volume>18</volume>
      <issue>17</issue>
      <fpage>4937</fpage><lpage>4952</lpage>
      <history>
        <date date-type="received"><day>21</day><month>May</month><year>2021</year></date>
           <date date-type="accepted"><day>7</day><month>August</month><year>2021</year></date>
           <date date-type="rev-recd"><day>6</day><month>August</month><year>2021</year></date>
           <date date-type="rev-request"><day>26</day><month>May</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 Andrew H. MacDougall</copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021.html">This article is available from https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021.html</self-uri><self-uri xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021.pdf">The full text article is available as a PDF file from https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e79">Zero Emissions Commitment (ZEC), the expected change in global temperature following the cessation of anthropogenic greenhouse gas emissions, has recently been assessed by the Zero Emissions Commitment Model Intercomparison Project (ZECMIP). ZECMIP concluded that the component of ZEC from <inline-formula><mml:math id="M1" 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> emissions will likely be close to zero in the decades following the cessation of emissions. However, of the 18 Earth system models that participated in ZECMIP only 2 included a representation of the permafrost carbon feedback to climate change. To better assess the potential impact of permafrost carbon decay on ZEC, a series of perturbed parameter experiments are here conducted with an Earth system model of intermediate complexity. The experiment suggests that the permafrost carbon cycle feedback will directly add  0.06 [0.02 to 0.14] <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> to the benchmark the ZEC value assesses 50 <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after 1000 <inline-formula><mml:math id="M4" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M5" 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> has been emitted to the atmosphere. An additional 0.04 [0 to 0.06] <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> is likely to been added relative to the benchmark ZEC value from the thaw-lag effect unaccounted for in the ZECMIP experiment design. Overall I assess that the permafrost carbon feedback is unlikely to change the assessment that ZEC is close to zero on decadal timescales; however, the feedback is expected to become more important over the coming centuries.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e157">The Zero Emissions Commitment (ZEC) is the change in global temperature expected to occur following the cessation of anthropogenic emissions of greenhouse gases and aerosols <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx22" id="paren.1"/>. ZEC is one of five metrics needed to compute the “remaining carbon budget”, which in turn quantifies the total emissions compatible with meeting a given temperature change guardrail <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx23" id="paren.2"><named-content content-type="pre">e.g.</named-content></xref>, such as those set out in the Paris Agreement <xref ref-type="bibr" rid="bib1.bibx41" id="paren.3"/>. ZEC was recently the focus of a model intercomparison project organized through the Coupled Model Intercomparison Project phase 6 (CMIP6) <xref ref-type="bibr" rid="bib1.bibx14" id="paren.4"/>. The project, formally called the Zero Emissions Commitment Model Intercomparison Project (ZECMIP)  <xref ref-type="bibr" rid="bib1.bibx14" id="paren.5"/>, gathered simulations from 18 Earth system models of full and intermediate complexity <xref ref-type="bibr" rid="bib1.bibx22" id="paren.6"/> and assessed the <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> component of ZEC. For the tier-one idealized experiment where 1000 <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M9" 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> was emitted to the atmosphere before cessation of emissions, ZEC ranged from <inline-formula><mml:math id="M10" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.36 to 0.29 <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> with a model ensemble mean of <inline-formula><mml:math id="M12" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.07 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> 50 <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions ceased. However, only 2 of the 18 models that participated in ZECMIP had a representation of the permafrost carbon feedback to climate change, a feedback process that is expected to release <inline-formula><mml:math id="M15" 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 <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the atmosphere for centuries after emissions cease <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx24" id="paren.7"/>. Thus the effect of the permafrost carbon feedback on ZEC has yet to be well quantified.</p>
      <p id="d1e286">The soils of the Northern Hemisphere permafrost region are estimated to contain between 1100 and 1500 <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of organic matter <xref ref-type="bibr" rid="bib1.bibx13" id="paren.8"/>, about half of which is held in the perennially frozen zone of these soils <xref ref-type="bibr" rid="bib1.bibx13" id="paren.9"/>. As climate warms and permafrost thaws, organic matter in permafrost-affected soils is exposed to increased periods of time where local temperature is above freezing, and hence to enhanced rate of decay releasing <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M19" 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> to the atmosphere <xref ref-type="bibr" rid="bib1.bibx34" id="paren.10"><named-content content-type="pre">e.g.</named-content></xref>. A recent informal (non-CMIP) model intercomparison exercise<?pagebreak page4938?> quantifying the permafrost carbon feedback estimated a release of carbon of between 74 and 652 <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> by year 2300 under the high-end Representative Concentration Pathway 8.5 scenario, with substantially lower release or even gain of soil carbon under mitigation scenarios <xref ref-type="bibr" rid="bib1.bibx24" id="paren.11"/>. Thus the permafrost carbon feedback to climate change has the potential to affect the value of ZEC in a fashion that was poorly quantified by ZECMIP.</p>
      <p id="d1e348">Uncertainty in projections from Earth system models can be classified into three components: (1) structural uncertainty, (2) parameter uncertainty, and (3) scenario uncertainty <xref ref-type="bibr" rid="bib1.bibx20" id="paren.12"><named-content content-type="pre">e.g.</named-content></xref>. Structural uncertainty is created from the discrepancy between the system the model is intended to represent and the system the model actually describes <xref ref-type="bibr" rid="bib1.bibx37 bib1.bibx7" id="paren.13"/>. Examining different models of the same system with standardized forcings through model intercomparison projects such as ZECMIP is the principle way of quantifying structural uncertainty in climate sciences <xref ref-type="bibr" rid="bib1.bibx7" id="paren.14"/>. Parameter uncertainty is uncertainty about the value that model parameter should take on <xref ref-type="bibr" rid="bib1.bibx37" id="paren.15"/>. As model parameters are sometimes quantities measurable in the natural world, parameter uncertainty is some cases equivalent to measurement uncertainty. In other cases parameters represent an amalgam of natural processes; in such cases defining parameter uncertainty becomes more ambiguous <xref ref-type="bibr" rid="bib1.bibx37" id="paren.16"/>. Parameter uncertainty can be quantified with perturbed parameter experiments, wherein ensembles of model variants  with parameter values selected from defined probability distribution functions are run under the same experiment conditions <xref ref-type="bibr" rid="bib1.bibx8" id="paren.17"><named-content content-type="pre">e.g.</named-content></xref>. Several such experiments have been conducted to assess uncertainty in the permafrost carbon feedback <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx20 bib1.bibx11" id="paren.18"/>. Scenario uncertainty is created by uncertainty about what humans will do in the future and is well explored by the coordinated scenario framework of CMIP <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx29" id="paren.19"/>.</p>
      <p id="d1e380">For the permafrost carbon feedback, uncertainty ranges derived from structural uncertainty and parameter uncertainty assessments have proven similar. The model intercomparison exercise of <xref ref-type="bibr" rid="bib1.bibx24" id="text.20"/>  found a range of 74 to 652 <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> with a mean of 341 <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> released from permafrost soils by year 2300 under Representative Concentration Pathway 8.5, compared to 159 to 587 <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> with a mean of 376 <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for the perturbed parameter experiment of <xref ref-type="bibr" rid="bib1.bibx20" id="text.21"/>, forced under the same scenario.</p>
      <p id="d1e435">In addition to 16 out of the 18 ZECMIP models having no permafrost carbon module, the experimental design of ZECMIP is ill designed to quantify the permafrost carbon feedback. The top-tier idealized ZECMIP experiment branches from the idealized 1pctCO2 experiment where atmospheric <inline-formula><mml:math id="M25" 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> concentration rises at 1 <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">%</mml:mi></mml:mrow></mml:math></inline-formula> a year compounded leading to a quadrupling of <inline-formula><mml:math id="M27" 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> concentration in 140 <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx7" id="paren.22"/>. Following this protocol <inline-formula><mml:math id="M29" 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 hence global temperatures rise much faster than in the historical trajectory, and since it takes time for permafrost soil to thaw and organic matter within these soils to decay, the experimental protocol will tend to underestimate release of carbon from permafrost soils <xref ref-type="bibr" rid="bib1.bibx17" id="paren.23"/>.</p>
      <p id="d1e494">Here I will use a perturbed parameter ensemble approach to estimate the contribution to <inline-formula><mml:math id="M30" 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>-only ZEC from the release of carbon from permafrost soils, following the ZECMIP protocol. I will also conduct an experiment following a more realistic <inline-formula><mml:math id="M31" 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> emission trajectory in order to quantity the thaw-lag effect from the high emission rates of the ZECMIP protocol.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Model description</title>
      <p id="d1e534">The University of Victoria Earth System Climate Model (UVic ESCM) is a climate model of intermediate complexity founded around a three-dimensional ocean general circulation model coupled to a simplified moisture and energy balance atmosphere <xref ref-type="bibr" rid="bib1.bibx42" id="paren.24"/>. The version of the model used here (version 2.9pf) has representation of the oceanic and terrestrial carbon cycles <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx25" id="paren.25"/>. The oceanic carbon cycle has representations of ocean carbonate chemistry <xref ref-type="bibr" rid="bib1.bibx42" id="paren.26"/>, phytoplankton–zooplankton–detritus ocean biology scheme <xref ref-type="bibr" rid="bib1.bibx32" id="paren.27"/>, and interaction between ocean sediments and alkalinity <xref ref-type="bibr" rid="bib1.bibx1" id="paren.28"/>. The terrestrial component is composed of the Top-down Representation of Interactive Foliage and Flora Including Dynamics (Triffid) dynamic vegetation model <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx25" id="paren.29"/>, a multi-layer representation soil respiration <xref ref-type="bibr" rid="bib1.bibx21" id="paren.30"/>, and a permafrost carbon module <xref ref-type="bibr" rid="bib1.bibx20" id="paren.31"/>.</p>
      <?pagebreak page4939?><p id="d1e562">The terrestrial subsurface of the model is composed of 14 layers, reaching a total depth of 250 <inline-formula><mml:math id="M32" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx3" id="paren.32"/>. The top eight layers (10 <inline-formula><mml:math id="M33" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) are active in the hydraulic cycle and deeper layers are impermeable bedrock <xref ref-type="bibr" rid="bib1.bibx3" id="paren.33"/>. The freeze–thaw physics of the soil accounts for the effect of soil valence forces on freezing point, and the frozen and unfrozen fraction of the soil water is calculated using equations the minimize Gibbs free energy <xref ref-type="bibr" rid="bib1.bibx2" id="paren.34"/>. The top six layers of the model (3.35 <inline-formula><mml:math id="M34" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) are active in the carbon cycle. Carbon is assigned to soil layers from Triffid based on the root density in each soil layer, with remaining dead plant matter added to the top soil layer <xref ref-type="bibr" rid="bib1.bibx21" id="paren.35"/>. Root density varies by plant function type and the temperature of the soil layer (roots do not grow in frozen soil) <xref ref-type="bibr" rid="bib1.bibx21" id="paren.36"/>. In model grid cells where permafrost exists (where soil layers have been below 0 <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for two or more consecutive years) a diffusion-based cryoturbation scheme is used to redistribute soil carbon in the soil column. The scheme was originally developed by <xref ref-type="bibr" rid="bib1.bibx15" id="text.37"/> and modified for implementation in the UVic ESCM in <xref ref-type="bibr" rid="bib1.bibx20" id="text.38"/>. The scheme allows for a permafrost carbon pool to be generated alongside regular soil carbon in permafrost soils. The modifications made to the scheme by <xref ref-type="bibr" rid="bib1.bibx20" id="text.39"/> allow the permafrost carbon pool to come into equilibrium during the 5000-<inline-formula><mml:math id="M36" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">year</mml:mi></mml:mrow></mml:math></inline-formula> model spin-up. The version of the UVic ESCM used here does not have a methane production module. Thus emissions of carbon from soils to the atmosphere happen only as <inline-formula><mml:math id="M37" 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>.</p>
      <p id="d1e646">In the version of the UVic ESCM used here <xref ref-type="bibr" rid="bib1.bibx20" id="paren.40"/> permafrost carbon is a separate carbon pool. Permafrost carbon is created when carbon is advected across the permafrost table by the cryoturbation scheme and can only be destroyed by being respired into <inline-formula><mml:math id="M38" 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>. The pool is characterized by a decay rate constant (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">κ</mml:mi><mml:mi>p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), a fraction of the pool that is available for decay (available fraction, <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi>A</mml:mi><mml:mi mathvariant="normal">f</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and a passive pool transformation rate (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">κ</mml:mi><mml:mtext>tf</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>), which is the rate at which the passive permafrost carbon becomes part of the available fraction. The available fraction is essentially the combined size of the fast and slow carbon pools as conceptualized in incubation experiments <xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx20" id="paren.41"/>. This scheme accounts for the large fraction of permafrost carbon that is very resistant to decay <xref ref-type="bibr" rid="bib1.bibx31" id="paren.42"/> while still allowing the pool to decay over millennial time periods <xref ref-type="bibr" rid="bib1.bibx20" id="paren.43"/>. A fourth parameter, the saturation factor (<inline-formula><mml:math id="M42" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>) from the cryoturbation scheme allows the size of the permafrost carbon pool to be tuned <xref ref-type="bibr" rid="bib1.bibx20" id="paren.44"/>. The saturation factor is indexed to the mineral porosity of soils (which vary by grid cell and soil layer) and accounts for the diminishing concentration of soil carbon at depth in permafrost regions <xref ref-type="bibr" rid="bib1.bibx13" id="paren.45"/>.</p>
      <p id="d1e719">The model experiments here use the permafrost carbon variant of the UVic ESCM 2.9 detailed in <xref ref-type="bibr" rid="bib1.bibx20" id="text.46"/>. A newer version of the UVic ESCM (version 2.10) is now available <xref ref-type="bibr" rid="bib1.bibx26" id="paren.47"/>. I use the older version of the model to allow for the use of legacy code and legacy model spin-ups from <xref ref-type="bibr" rid="bib1.bibx20" id="text.48"/>. Note that the terrestrial component of UVic ESCM 2.10 was taken from the version developed for <xref ref-type="bibr" rid="bib1.bibx20" id="text.49"/>, and thus the terrestrial components of the model versions are virtually identical <xref ref-type="bibr" rid="bib1.bibx26" id="paren.50"/>.</p>
      <p id="d1e738">By changing the flow of outgoing longwave radiation to space as a function of global surface temperature anomaly, the climate sensitivity of the UVic ESCM can be altered <xref ref-type="bibr" rid="bib1.bibx43" id="paren.51"/>. Similarly by changing the meridional diffusivity of the atmosphere within the model, arctic amplification can also be altered <xref ref-type="bibr" rid="bib1.bibx10" id="paren.52"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e749">Probability distribution functions of the six parameters perturbed in this study. MRT is mean residence time. Note that <bold>(d)</bold> has a logarithmic scale. All parameter PDFs except climate sensitivity are that same as in <xref ref-type="bibr" rid="bib1.bibx20" id="text.53"/>.</p></caption>
          <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Perturbed parameter experiments</title>
      <p id="d1e772">To assess the uncertainty in the strength of the permafrost carbon cycle feedback to climate change, <xref ref-type="bibr" rid="bib1.bibx20" id="text.54"/> generated 250 variants of the UVic ESCM by perturbing six model parameters. Four of these parameters control the size and susceptibility to decay of the permafrost carbon pool, and two (climate sensitivity and arctic amplification) are physical climate parameters. The four permafrost carbon parameters are the following: (1) the permafrost carbon decay constant; (2) the available fraction; (3) the passive pool transformation rate; and (4) the permafrost carbon saturation factor – which controls the size of the permafrost carbon pool. The permafrost carbon decay constant controls how fast available permafrost carbon can decay given the temperature and moisture of the soil. The available fraction is the fraction of permafrost carbon that is allowed to decay, effectively the fraction of permafrost carbon that is unprotected or weakly protected from decay. The passive pool transformation rate is the rate at which highly protected permafrost carbon becomes weakly protected.  The probability density functions (PDFs) for the permafrost carbon decay constant and the available fraction were taken from the meta-analysis of permafrost carbon incubation experiments conducted by <xref ref-type="bibr" rid="bib1.bibx31" id="text.55"/>. The passive pool transformation rate is constrained primarily by the non-existence of a remnant mid-latitude permafrost carbon pool from the last glacial maximum, yielding an estimated value of <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.25</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">10</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</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">10</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">s</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>, with a best guess of <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</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">10</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M47" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">s</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> <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx20" id="paren.56"/>. The analysis of <xref ref-type="bibr" rid="bib1.bibx20" id="text.57"/> showed that the passive pool transformation rate has only a weak effect of the permafrost carbon feedback on decadal and centennial timescales. The estimated uncertainty in the size of the permafrost carbon pool  was taken from <xref ref-type="bibr" rid="bib1.bibx13" id="text.58"/>. For each model variant 5000-<inline-formula><mml:math id="M48" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">year</mml:mi></mml:mrow></mml:math></inline-formula> model spin-ups were conducted with year 1850 of the Common Era (CE) radiative forcing to bring the permafrost carbon into equilibrium, representing an investment of 1.25 million model years of simulation time. We have re-used these model spin-ups for the present study.</p>
      <?pagebreak page4940?><p id="d1e880"><xref ref-type="bibr" rid="bib1.bibx20" id="text.59"/> also perturbed two physical model parameters: climate sensitivity and arctic amplification. These parameters do not affect the model spin-up as both affect deviations from the pre-industrial climate; thus they can be changed for the present study. To my knowledge there has been no major update in the uncertainty range of arctic amplification since 2016. However, <xref ref-type="bibr" rid="bib1.bibx35" id="text.60"/> have substantially constrained the uncertainty in equilibrium climate sensitivity to a 5th to 95th percentile range of 2.3 to 4.7 <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for a doubling of atmospheric <inline-formula><mml:math id="M50" 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> concentration. Thus I have computed new climate sensitivity parameters for the 250 model variants. I use the same functional form for the climate sensitivity PDFs as previous papers <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx20" id="paren.61"><named-content content-type="pre">e.g.</named-content></xref>, a product of two normal-inverse Gaussian functions. To get new parameter values for the climate sensitivity PDF a Monte Carlo method was used to fit the function to the distribution outlined by <xref ref-type="bibr" rid="bib1.bibx35" id="text.62"/>: a 5th to 95th percentile range of 2.3 to 4.7 <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, a 66 <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">%</mml:mi></mml:mrow></mml:math></inline-formula> range of 2.6 to 3.9 <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and a median value of 3.0 <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>. The new parameter values for the PDF are given in Appendix <xref ref-type="sec" rid="App1.Ch1.S1"/>.</p>
      <p id="d1e966">Figure <xref ref-type="fig" rid="Ch1.F1"/>
shows the PDFs of each parameter perturbed in this study. Note that all but equilibrium climate sensitivity are identical to <xref ref-type="bibr" rid="bib1.bibx20" id="text.63"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e977">Emissions trajectories for the three experiment sets conducted for this study.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f02.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e989">Model experiments conducted in this study.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Experiment</oasis:entry>
         <oasis:entry colname="col2">A1</oasis:entry>
         <oasis:entry colname="col3">A3</oasis:entry>
         <oasis:entry colname="col4">Historical-SSP4-6.0</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Long name</oasis:entry>
         <oasis:entry colname="col2">esm-1pct-brch-1000PgC</oasis:entry>
         <oasis:entry colname="col3">esm-1pct-brch-2000PgC</oasis:entry>
         <oasis:entry colname="col4">Historical, Shared Socioeconomic</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">Pathway Four version 6.0</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Total <inline-formula><mml:math id="M55" 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> emissions (PgC)</oasis:entry>
         <oasis:entry colname="col2">1000</oasis:entry>
         <oasis:entry colname="col3">2000</oasis:entry>
         <oasis:entry colname="col4">1000</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Simulations with permafrost?</oasis:entry>
         <oasis:entry colname="col2">Yes</oasis:entry>
         <oasis:entry colname="col3">Yes</oasis:entry>
         <oasis:entry colname="col4">Yes</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Simulations without permafrost?</oasis:entry>
         <oasis:entry colname="col2">Yes</oasis:entry>
         <oasis:entry colname="col3">Yes</oasis:entry>
         <oasis:entry colname="col4">No</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Model experiments</title>
      <p id="d1e1118">To quantify the effect of the permafrost carbon feedback on ZEC, we have three key questions: (1) How much warming will the permafrost carbon feedback add to ZEC? (2) What is the magnitude of the thaw-lag permafrost effect from using the 1pctCO2 experiment to quantify ZEC? And (3) how sensitive is the permafrost carbon feedback contribution to ZEC to total <inline-formula><mml:math id="M56" 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> emitted before cessation of emissions?</p>
      <p id="d1e1132">To answer the first question we would ideally compare simulations with and without permafrost carbon that are otherwise identical. In the UVic ESCM framework we can create a version without permafrost carbon by setting the cryoturbation diffusion parameter to zero during model spin-up. Without cryoturbation there will be no permafrost carbon pool, and the active layer carbon pool will also be reduced in size. However, the presence of carbon in soils subtly changes soil thermal and hydraulic properties in the UVic ESCM <xref ref-type="bibr" rid="bib1.bibx2" id="paren.64"/> such that the absence of a permafrost carbon pool could change the baseline climate conditions of the model. To test the magnitude of this effect simulations were conducted with the UVic ESCM with the cryoturbation diffusion parameter set to zero and all other model parameters held at their default settings. The model version was spun up for 5000 <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula>. Both the version of the model with cryoturbation set to zero and the default version of the model were forced with the 1pctCO2 experiment (where <inline-formula><mml:math id="M58" 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> concentration rises at 1 <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">%</mml:mi></mml:mrow></mml:math></inline-formula> per year compounded). Figure <xref ref-type="fig" rid="App1.Ch1.S2.F9"/> shows that the difference between the two simulations is minimal with respect to global average temperature, with a 0.01 <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> difference in baseline global temperature and a smaller difference by the time atmospheric <inline-formula><mml:math id="M61" 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> concentration doubled in year 70 of the experiment. The difference in regular<?pagebreak page4941?> (non-permafrost) soil carbon is also small between the two simulation. The simulation without cryoturbation has 1837 <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of regular soil carbon in the pre-industrial state, and the simulation with cryoturbation has 1853 <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> in the regular soil carbon pools in the pre-industrial state.</p>
      <p id="d1e1213">Thus to quantify the effect of permafrost carbon feedback on ZEC, two parallel sets of experiments were conducted. In one set of experiments model spin-ups from <xref ref-type="bibr" rid="bib1.bibx20" id="text.65"/> were used along with the 250 variants of the model to compute ZEC including permafrost. In a second set of experiments a single model spin-up with the cryoturbation diffusion parameter set to zero was used and 250 model variants were generated using just the climate sensitivity and arctic amplification parameters from the perturbed parameter sets. Thus each parallel variant pair will have the same climate sensitivity and arctic amplification parameters with only the existence of permafrost carbon different between the parallel variants. All model variants were forced with the esm-1pct-brch-1000PgC (A1) ZEC experiment described in <xref ref-type="bibr" rid="bib1.bibx14" id="text.66"/> where the 1000 <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of carbon is emitted following the 1pctCO2 experiment pathway, and emissions instantaneously go to zero once 1000 <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> is reached. All non-<inline-formula><mml:math id="M66" 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> forcings are held either at their year 1850 CE values or their long-term mean for volcanic and solar forcing. The simulations are forced with <inline-formula><mml:math id="M67" 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> emissions diagnosed from the default version of the UVic ESCM 2.9pf such that all simulations are forced with the same <inline-formula><mml:math id="M68" 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> emissions pathway. Thus most model variants will only approximately follow the 1pctCO2 <inline-formula><mml:math id="M69" 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> trajectory, but all variants have the same point in time that emissions cease, greatly simplifying analysis of the results. The difference between parallel variants with and without permafrost carbon quantifies the effect of the permafrost carbon pool on ZEC.</p>
      <p id="d1e1289">To quantify the permafrost thaw-lag effect a set of experiments were conducted with the 250 model variants with permafrost carbon. The model variants were forced with a <inline-formula><mml:math id="M70" 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> emissions trajectory that follows historical emissions until year 2019 <xref ref-type="bibr" rid="bib1.bibx9" id="paren.67"/> and afterwards follows the <inline-formula><mml:math id="M71" 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> emissions trajectory of a Shared Socioeconomic Pathway (SSP) <xref ref-type="bibr" rid="bib1.bibx29" id="paren.68"/> until 1000 <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> has been emitted (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). Thereafter <inline-formula><mml:math id="M73" 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> emissions are set to zero. All non-<inline-formula><mml:math id="M74" 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> forcings are held either at their year 1850 CE values or their long-term mean for volcanic and solar forcing. Eight SSPs were used by CMIP6 to quantify scenario uncertainty <xref ref-type="bibr" rid="bib1.bibx29" id="paren.69"/>. For the experiment conducted here I selected two SSP-based criteria: that the SSP reaches 1000 <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M76" 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> emissions and that the 1000 <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> cumulative <inline-formula><mml:math id="M78" 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> emissions total is reached before emissions begin to approach zero. The second criterion is needed as the ZECMIP bell-shaped curve experiments showed that the Transient Climate Response to Cumulative <inline-formula><mml:math id="M79" 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> Emissions (TCRE) and ZEC effects become mixed as emissions approach zero <xref ref-type="bibr" rid="bib1.bibx22" id="paren.70"/>. Therefore a sudden cessation of emissions is needed to separate TCRE from ZEC. SSP4-6.0 is the lowest emission SSP that reaches 1000 <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> whilst maintaining  near-peak <inline-formula><mml:math id="M81" 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> emissions. Thus using SSP4-6.0 maximizes the time need to reach 1000 <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> and therefore is optimal for assessing the thaw-lag effect. Under SSP4-6.0 <inline-formula><mml:math id="M83" 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> emissions 1000 <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> is reached in year 2067 of the Common Era (CE), allowing permafrost the time to thaw and the organic matter within it to decay.</p>
      <p id="d1e1475">The effect of total <inline-formula><mml:math id="M85" 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> emissions on the permafrost carbon contribution to ZEC is quantified by forcing each of the 250 parallel model variants with the esm-1pct-brch-2000PgC  (A3) ZEC experiment from <xref ref-type="bibr" rid="bib1.bibx14" id="text.71"/>, wherein 2000 <inline-formula><mml:math id="M86" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M87" 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> is emitted following the 1pctCO2 experiment pathway and emissions instantaneously go to zero once 2000 <inline-formula><mml:math id="M88" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> is reached. Again the permafrost carbon effect on ZEC is computed from the difference between parallel variants with and without permafrost carbon. Model experiments are summarized in Table <xref ref-type="table" rid="Ch1.T1"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1530"><bold>(a, b)</bold> Zero Emission Commitment (ZEC) for model versions without <bold>(a)</bold> and with <bold>(b)</bold> a permafrost carbon pool forced by the A1 (1000 <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. ZEC is temperature change relative to the year emissions cease. <bold>(c, d)</bold> Change in atmospheric <inline-formula><mml:math id="M90" 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> concentration relative to year emissions cease for model versions without <bold>(c)</bold> and with <bold>(d)</bold> a permafrost carbon pool, forced by the A1 (1000 <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment.  Grey lines are individual model variants, solid line is the median of the variants, and dashed lines are the 5th and 95th percentile. Sudden increase in warming rate seen in many warmer model variants is associated with the disappearance of perennial sea ice in the Weddell and Ross seas and concurrent changes in overturning circulation.</p></caption>
          <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1592"><bold>(a, b)</bold> Size of carbon sinks following cessation of emissions in the A1 (1000 <inline-formula><mml:math id="M92" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiments with and without permafrost carbon. <bold>(c)</bold> Difference in size of carbon pools between the simulation with and the simulation without permafrost carbon. The total of all carbon sinks remains 1000 <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease.</p></caption>
          <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1630">Difference in ZEC between experiments with and without permafrost carbon. <bold>(a)</bold> Anomalies for the A1 (1000 <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. <bold>(b)</bold> Anomalies for the A2 (2000 <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment.  Grey lines are individual model variants, solid line is the median of the variants, and dashed lines are the 5th and 95th percentile.</p></caption>
          <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f05.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1671">Median anomalies in ZEC created by release of carbon from permafrost soils, and the magnitude of the respective carbon release. Values in square brackets are 5th to 95th percentile ranges from the perturbed parameter experiments.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Years after</oasis:entry>
         <oasis:entry colname="col2">ZEC anomaly A1 (<inline-formula><mml:math id="M96" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col3">ZEC anomaly A3 (<inline-formula><mml:math id="M97" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col4">Permafrost C</oasis:entry>
         <oasis:entry colname="col5">Permafrost C</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">cessation of emissions</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">release A1 (PgC)</oasis:entry>
         <oasis:entry colname="col5">release A3 (PgC)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">0</oasis:entry>
         <oasis:entry colname="col2">–</oasis:entry>
         <oasis:entry colname="col3">–</oasis:entry>
         <oasis:entry colname="col4">29 [10 to 90]</oasis:entry>
         <oasis:entry colname="col5">84 [40 to 213]</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">50</oasis:entry>
         <oasis:entry colname="col2">0.06 [0.02 to 0.14]</oasis:entry>
         <oasis:entry colname="col3">0.06 [0.03 to 0.12]</oasis:entry>
         <oasis:entry colname="col4">73 [32 to 190]</oasis:entry>
         <oasis:entry colname="col5">159 [85 to 300]</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">100</oasis:entry>
         <oasis:entry colname="col2">0.09 [0.04 to 0.21]</oasis:entry>
         <oasis:entry colname="col3">0.09 [0.05 to 0.18]</oasis:entry>
         <oasis:entry colname="col4">100 [46 to 222]</oasis:entry>
         <oasis:entry colname="col5">205 [114 to 354]</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">500</oasis:entry>
         <oasis:entry colname="col2">0.27 [0.12 to 0.49]</oasis:entry>
         <oasis:entry colname="col3">0.24 [0.11 to 0.50]</oasis:entry>
         <oasis:entry colname="col4">178 [70 to 346]</oasis:entry>
         <oasis:entry colname="col5">312 [148 to 505]</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1828">Change in the soil carbon held in permafrost regions relative to
pre-industrial size. <bold>(a)</bold> Change for the A1 (1000 <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. <bold>(b)</bold> Change for the A2 (2000 <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. Grey lines are individual model variants, solid line is the median of the variants, and dashed lines are the 5th and 95th percentile. Vertical red line marks the time emissions cease.</p></caption>
          <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f06.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <?pagebreak page4943?><p id="d1e1874">Figure <xref ref-type="fig" rid="Ch1.F3"/> shows ZEC for the A1 (1000 <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment for
the model versions with and without permafrost carbon. The figure shows that
over centennial timescales the model version with permafrost carbon has a
higher ZEC. Consistent with a higher ZEC, the model version with permafrost
carbon exhibits a slower decline in atmospheric <inline-formula><mml:math id="M101" 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> concentration
after emissions cease. Figure <xref ref-type="fig" rid="Ch1.F5"/>a displays the difference in ZEC
between the simulations with and without permafrost carbon for the A1
(1000 <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. Fifty years after emissions cease the
existence of a permafrost carbon pool has added 0.06 [0.02 to
0.14] <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> to ZEC (median [5th to 95th percentile]), rising to
an addition of 0.09 [0.04 to 0.21] <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> 100 <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after
emissions cease, and 0.27 [0.12 to 0.49] <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> 500 <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula>
after emissions cease (Table <xref ref-type="table" rid="Ch1.T2"/>). The additional warming is being
driven by release of carbon from permafrost soils, which totals 29 [10 to
90] <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> by the time emissions cease, 73 [32 to 190] <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> by
50 <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease, 100 [46 to 222] <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>
100 <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease, and 178 [70 to 346] <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>
500 <inline-formula><mml:math id="M114" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease (Fig. <xref ref-type="fig" rid="Ch1.F6"/>a,
Table <xref ref-type="table" rid="Ch1.T2"/>). The global mean temperature anomaly at the time emissions
cease is 1.51 [1.41 to 1.58] <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for the non-permafrost carbon
experiment and 1.55 [1.47 to 1.67] <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for the permafrost
carbon experiment. Thus, the carbon released from permafrost soils by the time
emissions ceases causes 0.04 [0.01 to 0.12] <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of additional
warming in the model versions with permafrost carbon. The value of ZEC is
determined by a balance of the warming effect of diminishing ocean heat
uptake and the cooling effect of declining atmospheric <inline-formula><mml:math id="M118" 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>
concentration <xref ref-type="bibr" rid="bib1.bibx22" id="paren.72"/>; thus the initial cooling after
emissions cease is likely caused by the initial rapid drop in atmospheric
<inline-formula><mml:math id="M119" 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> concentration (<xref ref-type="fig" rid="Ch1.F3"/>c, and d).</p>
      <p id="d1e2107">Figure <xref ref-type="fig" rid="Ch1.F4"/> shows mean difference in global carbon pool sized in the simulations with and without permafrost carbon, averaged across all of the model variants, for the A1 (1000 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. The excess carbon released from permafrost soils is taken up by vegetation, the ocean, and the atmosphere. Most of the excess carbon resides in the atmosphere for centuries after emissions cease, with the ocean gradually becoming a more significant sink. Vegetation remains a relatively small sink throughout the experiments. Figure <xref ref-type="fig" rid="Ch1.F4"/> also suggests that the source of the rapid fall in atmospheric <inline-formula><mml:math id="M121" 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> in the decades after emissions cease is continued growth of the vegetation and soil carbon sinks. Within a century of cessation of emissions the terrestrial biosphere transitions from a carbon sink to carbon source, a process exacerbated by the existence of permafrost carbon pool.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e2138"><bold>(a)</bold> Difference in ZEC between the SSP4-6.0-based 1000 <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> experiment and the standard ZECMIP A1 (1000 <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment.  <bold>(b)</bold> Change in the soil carbon held in permafrost regions relative to pre-industrial size under the SSP4-6.0-based experiment. Vertical red line marks the time emissions cease. Grey lines are individual model variants, solid line is the median of the variants, and dashed lines are the 5th and 95th percentile.</p></caption>
        <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f07.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e2177"><bold>(a, b)</bold> Zero Emission Commitment (ZEC) for model versions without <bold>(a)</bold> and with <bold>(b)</bold> a permafrost carbon pool forced by the 2000 <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> A3 experiment. ZEC is temperature change relative to the year emissions cease. <bold>(c, d)</bold> Change in atmospheric <inline-formula><mml:math id="M125" 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> concentration relative to year emissions cease for model versions without <bold>(c)</bold> and with <bold>(d)</bold> a permafrost carbon pool forced by the A3 (2000 <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. Grey lines are individual model variants, solid line is the median of the variants, and dashed lines are the 5th and 95th percentile.</p></caption>
        <?xmltex \igopts{width=503.61378pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f08.png"/>

      </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e2240">Correlation coefficients between perturbed model parameters and the anomaly in ZEC 50 <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease. Stronger correlation indicates increased influence for a given parameter. MRT is mean residence time.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">A1</oasis:entry>
         <oasis:entry colname="col3">A3</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Permafrost C pool</oasis:entry>
         <oasis:entry colname="col2">0.19</oasis:entry>
         <oasis:entry colname="col3">0.22</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Available fraction</oasis:entry>
         <oasis:entry colname="col2">0.91</oasis:entry>
         <oasis:entry colname="col3">0.64</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Permafrost slow pool MRT</oasis:entry>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M128" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.01</oasis:entry>
         <oasis:entry colname="col3">0.08</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Passive pool transformation rate</oasis:entry>
         <oasis:entry colname="col2">0.22</oasis:entry>
         <oasis:entry colname="col3">0.55</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Equilibrium climate sensitivity</oasis:entry>
         <oasis:entry colname="col2">0.15</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M129" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.11</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Arctic amplification</oasis:entry>
         <oasis:entry colname="col2">0.01</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M130" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.15</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?pagebreak page4944?><p id="d1e2370"><?xmltex \hack{\newpage}?>Figure <xref ref-type="fig" rid="Ch1.F7"/> shows the difference in ZEC between simulations following the A1 (1000 <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) tier-1 ZECMIP experiment protocol and the experiment where emissions follow historical and SSP4-6.0 emissions until 1000 <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M133" 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> has been emitted. In the SSP4-6.0-based experiment ZEC is 0.04 [0 to 0.06] <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, 0.03 [<inline-formula><mml:math id="M135" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.01 to 0.05] <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and 0.03 [<inline-formula><mml:math id="M137" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.02 to 0.08] <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> warmer 50, 100, and 500 <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emission cease, respectively. The slightly larger ZEC is being driven by additional carbon being released from permafrost soils under the SSP4-6.0-based experiment with 51 [22 to 132] <inline-formula><mml:math id="M140" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> released when emissions cease compared to 29 [10 to 90] <inline-formula><mml:math id="M141" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> in the A1 experiment; 50, 100, and 500 <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease 84 [39 to 204] <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>,  107 [50 to 230] <inline-formula><mml:math id="M144" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and 180 [71 to 354] <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> have been released under the SSP4-6.0-based experiment compared to 73 [32 to 190] <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, 100 [46 to 222] <inline-formula><mml:math id="M147" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and 178 [70 to 346] <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> under the A1 experiment, respectively. Notably the effect of the thaw-lag diminishes with time after emissions cease.</p>
      <?pagebreak page4945?><p id="d1e2566">The ZEC for model variants without and with permafrost carbon for the A3 (2000 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiments is shown in Fig. <xref ref-type="fig" rid="Ch1.F8"/>. Similar to the A1 experiment the existence of a permafrost carbon pool adds to the magnitude of ZEC. The difference between the model versions with and without permafrost carbon is shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/>b for the A3 experiment. The difference in ZEC 50, 100, and 500 <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease is 0.06 [0.03 to 0.12] <inline-formula><mml:math id="M151" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, 0.09 [0.05 to 0.18] <inline-formula><mml:math id="M152" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and 0.24 [0.11 to 0.50] <inline-formula><mml:math id="M153" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> (Table <xref ref-type="table" rid="Ch1.T2"/>), respectively, corresponding to a release of carbon from permafrost soils of 84 [40 to 213] <inline-formula><mml:math id="M154" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> when emissions cease and 159 [85 to 300] <inline-formula><mml:math id="M155" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, 205 [114 to 354] <inline-formula><mml:math id="M156" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, and 312 [148 to 505] <inline-formula><mml:math id="M157" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> 50, 100, and 500 <inline-formula><mml:math id="M158" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b, Table <xref ref-type="table" rid="Ch1.T2"/>). Consistent with previous results that examined representative concentration pathway scenarios, the temperature effect of the permafrost carbon cycle feedback is not strongly effected by the total cumulative emissions <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx33" id="paren.73"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d1e2693">To explore which of the perturbed parameters has the greatest effect on the anomaly in ZEC created by the inclusion of permafrost carbon, correlations were computed between the perturbed parameter values and the anomaly in ZEC 50 <inline-formula><mml:math id="M159" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease. These correlations are shown in Table <xref ref-type="table" rid="Ch1.T3"/>. For the A1 (1000 <inline-formula><mml:math id="M160" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment the available fraction parameter has by far the strongest influence with a correlation of 0.91. None of the other parameters have large correlations. For the A3 (2000 <inline-formula><mml:math id="M161" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment both the available fraction (<inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.64</mml:mn></mml:mrow></mml:math></inline-formula>) and the passive pool transformation rate (<inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mi>r</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.55</mml:mn></mml:mrow></mml:math></inline-formula>) have substantial correlation values. These results contrast those for release of carbon from permafrost soils under future scenarios computed by <xref ref-type="bibr" rid="bib1.bibx20" id="text.74"/>, where both available fraction and equilibrium climate sensitivity played the most important roles, and the passive pool transformation rate had little effect on results. The difference may partly be due to the reduced uncertainty range in equilibrium climate sensitivity used here. The prominence of the Passive pool transformation rate in the A3 experiment results is concerning as this parameter is the most poorly constrained of all parameters considered. The available fraction parameter is effectively the combined size of the fast and slow pools as conceptualized in incubation experiments <xref ref-type="bibr" rid="bib1.bibx20" id="paren.75"/>. Thus these results suggest that increased field sampling of, and incubation experiments on, permafrost carbon could substantially reduce the uncertainty in permafrost carbon's contribution to ZEC.</p>
</sec>
<?pagebreak page4946?><sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e2767">ZECMIP found that the inter-model range of ZEC 50 <inline-formula><mml:math id="M164" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease for the A1 (1000 <inline-formula><mml:math id="M165" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment is <inline-formula><mml:math id="M166" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.36 to 0.29 <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> with a median value of <inline-formula><mml:math id="M168" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.05 <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx22" id="paren.76"/>. Thus the additional warming expected from the permafrost carbon cycle feedback of 0.06 [0.02 to 0.14] <inline-formula><mml:math id="M170" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> directly and 0.04 [0 to 0.06] <inline-formula><mml:math id="M171" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> from the thaw-lag effect will not substantially change the expected value of ZEC on decadal timescales. Thus, the overall conclusion that ZEC will be close to zero in the decades following cessation of emissions remains unchanged.</p>
      <p id="d1e2855">Here we have assessed the parameter uncertainty of the permafrost carbon cycle feedback contribution to ZEC and have left structural uncertainty unassessed. To quantify structural uncertainty other Earth system models would have to conduct ZECMIP experiments with and without their permafrost components turned on. As many of the models that participated in ZECMIP do have permafrost carbon capable versions of their models <xref ref-type="bibr" rid="bib1.bibx4" id="paren.77"><named-content content-type="pre">e.g.</named-content></xref>, such a study is possible and would make a valuable contribution to the next iteration of ZECMIP.</p>
      <p id="d1e2863">Here we found that the permafrost carbon feedback contribution to ZEC was insensitive to cumulative <inline-formula><mml:math id="M172" 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> emissions, despite a larger release of <inline-formula><mml:math id="M173" 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> to the atmosphere from permafrost soils in the A3 (2000 <inline-formula><mml:math id="M174" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) experiment. The linear relationship between cumulative emissions of <inline-formula><mml:math id="M175" 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 global temperature change is generated by an atmosphere–ocean phenomenon <xref ref-type="bibr" rid="bib1.bibx16" id="paren.78"/>; thus the atmosphere–ocean system does not distinguish between emissions from the terrestrial biosphere and fossil fuel emissions <xref ref-type="bibr" rid="bib1.bibx36" id="paren.79"/>. Therefore this insensitivity of temperature to carbon released from permafrost soils appears anomalous. However, for intermediate complexity models like the UVic ESCM the cumulative emissions of <inline-formula><mml:math id="M176" 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> vs. global temperature change curve are only approximately linear and the change in temperature with a unit of <inline-formula><mml:math id="M177" 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> emitted declines at high cumulative emission totals, as the logarithmic radiative forcing from <inline-formula><mml:math id="M178" 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> begins to become the dominate effect <xref ref-type="bibr" rid="bib1.bibx19" id="paren.80"/>. Thus the emissions of <inline-formula><mml:math id="M179" 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> from permafrost soil are less effective at warming after 2000 <inline-formula><mml:math id="M180" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M181" 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> has been emitted than when 1000 <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> has been emitted in the UVic ESCM. However, it has been shown the full Earth system models do not have non-linear cumulative emissions of <inline-formula><mml:math id="M183" 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> vs. global temperature change curves <xref ref-type="bibr" rid="bib1.bibx38" id="paren.81"/>. Therefore the insensitivity of the permafrost carbon feedback contribution to ZEC to cumulative <inline-formula><mml:math id="M184" 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> emissions found here should be treated with caution.</p>
      <p id="d1e3023">To date no Earth system model <xref ref-type="bibr" rid="bib1.bibx24" id="paren.82"/> accounts for abrupt thaw processes in permafrost systems. These processes, including thermokarst production, active hill slope erosion, and coastal erosion, could accelerate thaw processes by 40 <inline-formula><mml:math id="M185" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">%</mml:mi></mml:mrow></mml:math></inline-formula> over the next few centuries <xref ref-type="bibr" rid="bib1.bibx40" id="paren.83"/>. Additionally the 2.9pf version of the UVic ESCM (used here) and publicly available 2.10 version of the UVic ESCM do not account for enhanced methane production from permafrost thaw. A methane production scheme has recently been added to a newly developed thread of the model, which preliminarily suggests a warming effect from <inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production from permafrost soils of 0 to 0.24 <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>, depending on parameter values and scenario followed <xref ref-type="bibr" rid="bib1.bibx27" id="paren.84"/>. Such values are consistent with expert assessment of <xref ref-type="bibr" rid="bib1.bibx34" id="paren.85"/>.  Accounting for these processes will likely increase the estimated effect of the permafrost carbon cycle feedback on ZEC, and therefore the effect of the permafrost carbon feedback on ZEC should be reassessed when these processes are better accounted for in Earth system models.</p>
      <p id="d1e3071">UVic ESCM 2.10 was one of the two models that participated in ZECMIP that included a permafrost carbon scheme (the other was CESM). The ZEC 50 <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after <inline-formula><mml:math id="M189" 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> emissions cease for the A1 experiment (1000 <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>) was 0.03 <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for the model version that participated in ZECMIP (UVic ESCM 2.10). This value places UVic ESCM close to the centre of the inter-model range ranking 8th highest of the 18 models that participated in ZECMIP <xref ref-type="bibr" rid="bib1.bibx22" id="paren.86"/>. The model version with permafrost carbon used here ZEC 50 <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease is <inline-formula><mml:math id="M193" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.02 [<inline-formula><mml:math id="M194" display="inline"><mml:mo lspace="0mm">-</mml:mo></mml:math></inline-formula>0.07 to 0.08] <inline-formula><mml:math id="M195" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula>; 750 <inline-formula><mml:math id="M196" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emission cease ZEC is 0.70 [0.35 to 1.06] <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for the A1 experiment for UVic ESCM 2.9pf and was 0.20 <inline-formula><mml:math id="M198" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> for UVic ESCM 2.10 in <xref ref-type="bibr" rid="bib1.bibx22" id="text.87"/>. Evidently the two model versions have similar decadal ZEC values but diverge substantially on centennial timescales. The main difference between UVic ESCM versions 2.9pf and 2.10 is the representation of the ocean <xref ref-type="bibr" rid="bib1.bibx26" id="paren.88"/>, with the newer version of the model having substantially improved ocean dynamics and a state-of-the-art representation of ocean biogeochemistry <xref ref-type="bibr" rid="bib1.bibx26" id="paren.89"/>. Ocean heat and carbon uptake are two of the processes that determine the value of ZEC <xref ref-type="bibr" rid="bib1.bibx22" id="paren.90"/>. Therefore, it is not unexpected that differences in the representation of the ocean would change the ZEC value of a model.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e3208">Here we have used a perturbed parameter ensemble with the UVic ESCM to estimate the impact of the permafrost carbon cycle feedback on the value of the <inline-formula><mml:math id="M199" 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> component of the Zero Emissions Commitment. We find  50 <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease in an experiment where 1000 <inline-formula><mml:math id="M201" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Pg</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math id="M202" 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> is emitted to the atmosphere that the permafrost carbon feedback adds  0.06 [0.02 to 0.14] <inline-formula><mml:math id="M203" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> to ZEC, rising to 0.27 [0.12 to 0.49] <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> 500 <inline-formula><mml:math id="M205" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease. Additionally following a more realistic emissions trajectory based on historical and SSP4-6.0 emissions adds 0.04 [0 to 0.06] <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:math></inline-formula> to ZEC 50 <inline-formula><mml:math id="M207" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">years</mml:mi></mml:mrow></mml:math></inline-formula> after emissions cease. This thaw-lag effect diminishes with time after emissions cease. Overall accounting for<?pagebreak page4947?> the permafrost carbon feedback does not change the conclusion that ZEC will be close to zero on decadal timescales <xref ref-type="bibr" rid="bib1.bibx22" id="paren.91"/>, though the effect of abrupt thaw remains unaccounted for and the feedback is of greater concern over longer timeframes.</p><?xmltex \hack{\clearpage}?>
</sec>

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

<?pagebreak page4948?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Probability distribution function for climate sensitivity</title>
      <p id="d1e3320">The functional form of the climate sensitivity PDF was taken to be the product of two normal-inverse Gaussian functions following <xref ref-type="bibr" rid="bib1.bibx28" id="text.92"/>. The normal-inverse Gaussian function is as follows:

              <disp-formula id="App1.Ch1.S1.E1" content-type="numbered"><label>A1</label><mml:math id="M208" display="block"><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mtext>PDF</mml:mtext><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mi>K</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mfenced open="(" close=")"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:msqrt><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt></mml:mrow></mml:mfenced></mml:mrow><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:msqrt><mml:mrow><mml:msup><mml:mi mathvariant="italic">δ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msqrt><mml:mrow><mml:msup><mml:mi mathvariant="italic">α</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="italic">β</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>-</mml:mo><mml:mi mathvariant="italic">μ</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

        where <inline-formula><mml:math id="M209" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula> is location, <inline-formula><mml:math id="M210" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is tail heaviness, <inline-formula><mml:math id="M211" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> is an asymmetry parameter, <inline-formula><mml:math id="M212" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> is a scale parameter, and <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is a modified Bessel function of the third kind <xref ref-type="bibr" rid="bib1.bibx28" id="paren.93"/>. The Python <inline-formula><mml:math id="M214" display="inline"><mml:mrow><mml:mi>s</mml:mi><mml:mi>c</mml:mi><mml:mi>i</mml:mi><mml:mi>p</mml:mi><mml:mi>y</mml:mi><mml:mo>.</mml:mo><mml:mi>s</mml:mi><mml:mi>t</mml:mi><mml:mi>a</mml:mi><mml:mi>t</mml:mi><mml:mi>s</mml:mi></mml:mrow></mml:math></inline-formula> software package was used to compute the PDF.</p>
      <p id="d1e3508">The new parameter values fitting the PDF to the <xref ref-type="bibr" rid="bib1.bibx35" id="text.94"/> constraints on equilibrium climate sensitivity are shown in Table <xref ref-type="table" rid="App1.Ch1.S1.T4"/> below.</p>

<?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S1.T4"><?xmltex \currentcnt{A1}?><label>Table A1</label><caption><p id="d1e3519">Parameter values for climate sensitivity PDF composed of the product of two normal-inverse Gaussian (NIG) functions. An additional scaling parameter of 5.9047 is needed to make the integral of the PDF 1.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">NIG <inline-formula><mml:math id="M215" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>1</oasis:entry>
         <oasis:entry colname="col3">NIG – 2</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M216" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2.97</oasis:entry>
         <oasis:entry colname="col3">2.94</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M217" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">2.90</oasis:entry>
         <oasis:entry colname="col3">2.00</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M218" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.11</oasis:entry>
         <oasis:entry colname="col3">1.08</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M219" display="inline"><mml:mi mathvariant="italic">μ</mml:mi></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.78</oasis:entry>
         <oasis:entry colname="col3">2.38</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<?xmltex \hack{\clearpage}?>
</app>

<?pagebreak page4949?><app id="App1.Ch1.S2">
  <?xmltex \currentcnt{B}?><label>Appendix B</label><title>Effect of existence of permafrost carbon pool on simulated global climate</title>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S2.F9"><?xmltex \currentcnt{B1}?><?xmltex \def\figurename{Figure}?><label>Figure B1</label><caption><p id="d1e3638">Simulations of the 1pctCO2 experiment for two versions of the UVic ESCM one with default settings (permafrost carbon) and a second starting from a model spin-up where cryoturbation diffusion parameter has been set to zero, and hence there is no permafrost carbon pool. Since the 1pctCO2 is a concentration-driven scenario, the presence or absence of permafrost carbon does not have an effect on the atmospheric carbon pool.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://bg.copernicus.org/articles/18/4937/2021/bg-18-4937-2021-f09.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e3653">UVic ESCM 2.9 and 2.10 are available from <uri>http://terra.seos.uvic.ca/model/</uri> <xref ref-type="bibr" rid="bib1.bibx6" id="paren.95"/>.</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3665">Model output produced for this study is available at <ext-link xlink:href="https://doi.org/10.5683/SP2/I75BZ0" ext-link-type="DOI">10.5683/SP2/I75BZ0</ext-link> <xref ref-type="bibr" rid="bib1.bibx18" id="paren.96"/>.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3677">The contact author has declared that there are no competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3683">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3689">I am grateful for support from the Natural Sciences and Engineering Research Council of Canada Discovery Grant program and for computational support from Compute Canada. Chris Jones and Charles Koven provided helpful critiques of an early draft of the manuscript. I thank the two anonymous reviewers for their helpful comments.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3694">This research has been supported by the Natural Sciences and Engineering Research Council of Canada.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3700">This paper was edited by Alexey V. Eliseev and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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<abstract-html><p>Zero Emissions Commitment (ZEC), the expected change in global temperature following the cessation of anthropogenic greenhouse gas emissions, has recently been assessed by the Zero Emissions Commitment Model Intercomparison Project (ZECMIP). ZECMIP concluded that the component of ZEC from CO<sub>2</sub> emissions will likely be close to zero in the decades following the cessation of emissions. However, of the 18 Earth system models that participated in ZECMIP only 2 included a representation of the permafrost carbon feedback to climate change. To better assess the potential impact of permafrost carbon decay on ZEC, a series of perturbed parameter experiments are here conducted with an Earth system model of intermediate complexity. The experiment suggests that the permafrost carbon cycle feedback will directly add  0.06 [0.02 to 0.14]&thinsp;°C to the benchmark the ZEC value assesses 50 years after 1000&thinsp;Pg C of CO<sub>2</sub> has been emitted to the atmosphere. An additional 0.04 [0 to 0.06]&thinsp;°C is likely to been added relative to the benchmark ZEC value from the thaw-lag effect unaccounted for in the ZECMIP experiment design. Overall I assess that the permafrost carbon feedback is unlikely to change the assessment that ZEC is close to zero on decadal timescales; however, the feedback is expected to become more important over the coming centuries.</p></abstract-html>
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