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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article">
  <front>
    <journal-meta><journal-id journal-id-type="publisher">TC</journal-id><journal-title-group>
    <journal-title>The Cryosphere</journal-title>
    <abbrev-journal-title abbrev-type="publisher">TC</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">The Cryosphere</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1994-0424</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/tc-20-2317-2026</article-id><title-group><article-title>Changes in 1958–2019 Greenland surface mass balance are attributable to both greenhouse gases and anthropogenic aerosols</article-title><alt-title>Attributing Greenland surface mass balance changes</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Kuo</surname><given-names>Yan-Ning</given-names></name>
          <email>yk545@cornell.edu</email>
        <ext-link>https://orcid.org/0000-0001-5590-3897</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Culberg</surname><given-names>Riley</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4460-2359</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Lehner</surname><given-names>Flavio</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4632-9701</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth and Atmospheric Sciences, Cornell University, Ithaca, NY, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Polar Bears International, Bozeman, MT, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yan-Ning Kuo (yk545@cornell.edu)</corresp></author-notes><pub-date><day>23</day><month>April</month><year>2026</year></pub-date>
      
      <volume>20</volume>
      <issue>4</issue>
      <fpage>2317</fpage><lpage>2329</lpage>
      <history>
        <date date-type="received"><day>29</day><month>August</month><year>2025</year></date>
           <date date-type="rev-request"><day>13</day><month>October</month><year>2025</year></date>
           <date date-type="rev-recd"><day>2</day><month>March</month><year>2026</year></date>
           <date date-type="accepted"><day>3</day><month>March</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Yan-Ning Kuo et al.</copyright-statement>
        <copyright-year>2026</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026.html">This article is available from https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026.html</self-uri><self-uri xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026.pdf">The full text article is available as a PDF file from https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e106">Greenland Ice Sheet (GrIS) mass loss is a main contributor to rising Global Mean Sea Level (GMSL), exhibiting decadal variability due to surface mass balance (SMB) changes. Greenhouse gases (GHG) have long been identified as a key driver of GrIS mass loss through warming-induced runoff. However, there has not been a formal attribution of historical GrIS SMB changes to GHG and the potential role for other forcings such as anthropogenic aerosols (AAER). Here, we use the Community Earth System Model version 2 large ensemble and single forcing large ensemble (CESM2-LE and CESM2-SFLE) to formulate a detection and attribution analysis for historical GrIS SMB changes. We show that the decadal variability of SMB is forced by historical radiative forcing attributable to both GHG and AAER through their forced changes of runoff. This highlights that, in addition to the frequently mentioned GHG, AAER also contributes to SMB changes during the historical period. GHG influences GrIS runoff mainly through long-term radiatively-forced warming, while AAER influences it through the decadal variability of atmospheric circulation that projects onto a Greenland blocking pattern, leading to relative cooling from cyclonic circulation over Greenland pre-1980 and relative warming from anti-cyclonic circulation thereafter. The attribution of SMB, and specifically runoff, to AAER has a lower signal-to-noise ratio (S <inline-formula><mml:math id="M1" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N) than the attribution to GHG due to both a weaker signal and wider confidence intervals. The lower S <inline-formula><mml:math id="M2" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N in attributing runoff changes to AAER is partly due to a smaller temperature response in AAER than in GHG and partly due to a mean state temperature dependency of the runoff sensitivity. In simulations with only AAER, the climate is colder than in simulations with all forcings or only GHG, leading to more time below freezing when temperature variations do not affect runoff as much. We resolve this issue by comparing simulations with all forcings with simulations in which everything-but-AAER is changing, thereby stressing the need to account for mean state dependencies when conducting detection and attribution with single forcing simulations.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung</funding-source>
<award-id>PZ00P2_174128</award-id>
</award-group>
<award-group id="gs2">
<funding-source>National Aeronautics and Space Administration</funding-source>
<award-id>80NSSC24K1445</award-id>
<award-id>80NSSC24K1037</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e132">The global mean sea level (GMSL) has been rising at an averaged rate of 1.56 mm yr<sup>−1</sup> since 1900 <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx20 bib1.bibx5" id="paren.1"/> and has accelerated to 3.3 mm yr<sup>−1</sup> since the 1990s <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx5" id="paren.2"/>. A growing contribution to GMSL rise is from the ocean mass increase (barystatic sea level rise), due to freshwater input to the ocean from terrestrial water, mountain glaciers, and polar ice sheets, including both the Greenland Ice Sheet (GrIS) and Antarctic Ice Sheet. Glaciers remain the least constrained component of the climate change-driven sea level rise <xref ref-type="bibr" rid="bib1.bibx27" id="paren.3"/>. Among these glacial GMSL sources, the GrIS is one of the largest barystatic sea level contributors to GMSL since 1900 (accounting for 29 % of the total GMSL increase) <xref ref-type="bibr" rid="bib1.bibx15" id="paren.4"/>. Along with contributing to GMSL rise, GrIS mass loss can further increase regional sea level rise rate, such as for the North American East Coast <xref ref-type="bibr" rid="bib1.bibx40" id="paren.5"/>, resulting in higher risk of coastal flooding <xref ref-type="bibr" rid="bib1.bibx62" id="paren.6"/>.</p>
      <p id="d2e178">GrIS mass loss comes from two factors <xref ref-type="bibr" rid="bib1.bibx41" id="paren.7"/>: (1) changes in the surface mass balance (SMB), defined as the difference between precipitation, evaporation/sublimation, and runoff, and (2) changes in ice discharge related to glacial dynamics, manifested in calving and ocean melting trends. Observational records show that declining GrIS SMB has become an increasingly important contributor to rising GMSL in recent decades <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx31 bib1.bibx41" id="paren.8"/> and GrIS SMB change is identified as the largest source of GMSL uncertainty in future projections <xref ref-type="bibr" rid="bib1.bibx48" id="paren.9"/>. Thus, understanding why the SMB has changed historically can be informative for projecting future changes of GMSL due to GrIS mass loss.</p>
      <p id="d2e191">GrIS SMB reduction has been linked to rising air temperature over Greenland, as warming leads to more surface melting and runoff <xref ref-type="bibr" rid="bib1.bibx60 bib1.bibx61 bib1.bibx59" id="paren.10"/>. Greenhouse Gases (GHG) amplify warming over the Arctic <xref ref-type="bibr" rid="bib1.bibx63" id="paren.11"/>, and the consequent runoff increase is consistent with the monotonic long-term decline in GrIS SMB projected for the future under strong radiative forcing scenarios <xref ref-type="bibr" rid="bib1.bibx24" id="paren.12"/>. However, there has not been a formal attribution of historical GrIS SMB changes to radiative forcing, despite the emerging signal from GHG-induced global mean temperature warming in recent decades <xref ref-type="bibr" rid="bib1.bibx9" id="paren.13"/>. The GrIS SMB decline since the 1990s has also been linked to the increasing frequency of subsidence-induced warming from Greenland blocking, itself linked to the negative phase of the North Atlantic Oscillation (NAO). NAO-related GrIS SMB change has thus far been treated as internal variability on decadal time scales <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx3 bib1.bibx19" id="paren.14"/>. However, new literature attributes the negative NAO transition to anthropogenic aerosols (AAER; <xref ref-type="bibr" rid="bib1.bibx11" id="text.15"/>) and provides evidence of AAER-forced historical decadal variability for different aspects of North Atlantic climate, including storm tracks <xref ref-type="bibr" rid="bib1.bibx28" id="paren.16"/> and sea surface temperatures (SSTs; <xref ref-type="bibr" rid="bib1.bibx21" id="text.17"/>). We hypothesize that internal variability might not be the only reason for the recent decadal GrIS SMB changes; instead, both GHG and AAER could have also contributed.</p>
      <p id="d2e219">Unlike GHG, historical AAER emissions had a non-monotonic spatio-temporal trajectory, owing to, for example, the timing of social-economic development and air quality regulations in different countries <xref ref-type="bibr" rid="bib1.bibx49" id="paren.18"/>. This heterogeneous characteristic of AAER has been argued to induce historical decadal variability in various aspects of the Earth's climate; prominent recent examples include tropical SST patterns <xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx10 bib1.bibx57" id="paren.19"/>, regional hydroclimate change <xref ref-type="bibr" rid="bib1.bibx33" id="paren.20"/>, and mid-latitude circulation <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx47" id="paren.21"/>. Together with the literature supporting AAER-forced historical decadal variability of North Atlantic climate, we hypothesize that AAER contributes to GrIS SMB changes through its impacts on atmospheric circulation.</p>
      <p id="d2e235">However, the forced response to AAER often has a low signal-to-noise ratio (S <inline-formula><mml:math id="M5" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N) <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx47 bib1.bibx32" id="paren.22"/>, and so do externally forced NAO changes <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx52" id="paren.23"/>. Different external radiative forcings can also create nonlinear (or non-additive) responses in the climate system <xref ref-type="bibr" rid="bib1.bibx55 bib1.bibx33" id="paren.24"/>. As such, nonlinear interactions between AAER and GHG forcings cannot be captured in the single forcing runs of AAER-only or GHG-only simulations. New climate model large ensembles are designed to better isolate subtle signals and responses to individual forcings from internal variability <xref ref-type="bibr" rid="bib1.bibx8" id="paren.25"/>. Therefore, in this study, we utilize the Community Earth System Model version 2 (CESM2; <xref ref-type="bibr" rid="bib1.bibx6" id="text.26"/>) large ensemble (CESM2-LE; <xref ref-type="bibr" rid="bib1.bibx50" id="text.27"/>) and its single forcing large ensemble (CESM2-SFLE) with both <italic>forcing-only</italic> and <italic>all-but-forcing</italic> experimental setups <xref ref-type="bibr" rid="bib1.bibx55" id="paren.28"/> to better understand whether the historical decadal variability of GrIS SMB is forced by both GHG and AAER.</p>
      <p id="d2e273">In this paper, we apply the detection and attribution (D&amp;A) framework from <xref ref-type="bibr" rid="bib1.bibx1" id="text.29"/> to formally assess whether historical radiative forcings can account for GrIS SMB changes between 1958–2019. We demonstrate that both GHG and AAER contributed to the 1958–2019 GrIS SMB changes and highlight a previously underappreciated source of uncertainty in D&amp;A when the climate response has mean state temperature dependency. This mean state temperature dependency can lead to different S <inline-formula><mml:math id="M6" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N for the attribution to GHG compared to AAER. Finally, we will discuss implications of these uncertainties for the general D&amp;A framework.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Data</title>
<sec id="Ch1.S2.SS1.SSS1">
  <label>2.1.1</label><title>Reference data</title>
      <p id="d2e308">In this study, reconstruction data, reanalysis data, and a regional climate model simulation driven by reanalysis since 1958 are included as reference data for the historical period. <xref ref-type="bibr" rid="bib1.bibx15" id="text.30"/>'s reconstruction for GrIS mass loss was used to assess the impact of SMB change on GrIS GMSL contributions since 1958. The <xref ref-type="bibr" rid="bib1.bibx15" id="text.31"/>'s reconstruction data comes from a Monte Carlo simulation perturbing the known prior estimate based on three estimates of GrIS mass loss data, including a reconstruction from geological inference of historical ice sheet surface elevation <xref ref-type="bibr" rid="bib1.bibx31" id="paren.32"/>, an input-output estimate <xref ref-type="bibr" rid="bib1.bibx41" id="paren.33"/>, and a synthesis of satellite observations with a multi-method assessment <xref ref-type="bibr" rid="bib1.bibx2" id="paren.34"/>. With 5000 ensemble members, this reconstruction provides a range of observational uncertainty of the GMSL contribution from GrIS mass loss. To understand the drivers of the GrIS GMSL contribution, we use 1958–2019 annual mean SMB, precipitation (<inline-formula><mml:math id="M7" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>), and runoff (<inline-formula><mml:math id="M8" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>), averaged over the GrIS, from the polar regional climate model RACMO2.3p2 simulation forced with the reanalysis data sets from ECMWF Reanalysis (ERA), hereafter RACMO-ERA <xref ref-type="bibr" rid="bib1.bibx45" id="paren.35"/>. RACMO-ERA is run at 5.5 km resolution and statistically downscaled to 1 km <xref ref-type="bibr" rid="bib1.bibx45" id="paren.36"/>. This RACMO-ERA simulation has been compared against in-situ meteorological data and point measurements of GrIS SMB and showed good agreement with these observations <xref ref-type="bibr" rid="bib1.bibx42" id="paren.37"/>. Here, these RACMO-ERA outputs are treated as the reference data to formulate a D&amp;A analysis. Additionally, annual means of near-surface temperature at 2 m (TAS) and 500 hPa geopotential height (<inline-formula><mml:math id="M9" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) from monthly gridded ERA5 reanalysis <xref ref-type="bibr" rid="bib1.bibx23" id="paren.38"/> are included to investigate the atmospheric drivers of the SMB changes.</p>
</sec>
<sec id="Ch1.S2.SS1.SSS2">
  <label>2.1.2</label><title>CESM2 large ensemble and single forcing large ensemble (CESM2-LE and CESM2-SFLE)</title>
      <p id="d2e373">CESM2-LE and CESM2-SFLE are used for the D&amp;A analysis. CESM2 <xref ref-type="bibr" rid="bib1.bibx6" id="paren.39"/> is a climate model developed by the National Center for Atmospheric Research (NCAR). It includes a land ice model (CISM) <xref ref-type="bibr" rid="bib1.bibx34" id="paren.40"/> of the GrIS at 4 km spatial resolution. CESM2-LE and CESM2-SFLE are run setups with a fixed ice sheet topography so that CISM does not feed back to other parts of the climate system but provides the finer grids to downscale SMB. CESM2 has been evaluated against observations and shown to capture the variability of GrIS SMB well <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx44 bib1.bibx45" id="paren.41"/>.</p>
      <p id="d2e385">We take the 50-member ensemble from CESM2-LE <xref ref-type="bibr" rid="bib1.bibx50" id="paren.42"/> that is forced with the full historical radiative forcings (ALL), using smoothed biomass burning forcing (<italic>smbb</italic>). Each ensemble member differs from the others due to initial condition perturbations (see <xref ref-type="bibr" rid="bib1.bibx50" id="text.43"/>) to quantify the uncertainty originating from internal variability. CESM2-SFLE <xref ref-type="bibr" rid="bib1.bibx55" id="paren.44"/> uses the same CESM2 version but instead of the ALL forcing, individual forcings are applied in isolation. We use the 15-member GHG and AAER simulations, as GHG and AAER are two dominant anthropogenic forcings for historical climate change <xref ref-type="bibr" rid="bib1.bibx9" id="paren.45"/>. In CESM2-SFLE, the GHG (AAER) simulation is forced with time-evolving GHG (AAER) forcing, with other forcing held fixed at 1850 levels (i.e., the <italic>forcing-only</italic> experimental setup). We also include the 10-member all-but-aerosols (xAAER; the <italic>all-but-forcing</italic> experimental setup) simulations and follow <xref ref-type="bibr" rid="bib1.bibx9" id="text.46"/> to calculate the contribution of anthropogenic aerosols as the difference between ALL and xAAER (ALL-minus-xAAER). With xAAER and ALL-minus-xAAER, we can assess the robustness of D&amp;A results given the potential non-additivity issue reported in <xref ref-type="bibr" rid="bib1.bibx55" id="text.47"/>.</p>
      <p id="d2e416">We use the annual SMB, and monthly <inline-formula><mml:math id="M10" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M11" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>, TAS, and <inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from these simulations. Monthly CESM2 outputs are converted to an annual sum (<inline-formula><mml:math id="M13" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M14" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) or annual mean (TAS, <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) to compare against annual SMB. The area-weighted SMB, <inline-formula><mml:math id="M16" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M17" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> (unit: mm yr<sup>−1</sup>) is summed over Greenland and divided by the global ocean area derived from the CESM2 land mask to convert into a GMSL equivalent (unit: mm GMSL equivalent per year). This GMSL equivalent is multiplied by 361.8 to convert to Gt yr<sup>−1</sup>. Anomalies are calculated by removing the 1958–2019 climatological means for regression analyses.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Detection and attribution (D&amp;A) approach</title>
      <p id="d2e518">D&amp;A is commonly performed with a regression of the observation (<inline-formula><mml:math id="M20" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>) onto the fingerprint(s) of the external forcing (<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) as

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M22" display="block"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>m</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the scaling factor(s) to best match the time-dependent fingerprint(s) to the observation. The fingerprint(s) <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are usually estimated by averaging many simulations (e.g., ensemble mean), and <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the residual not explained by the simulated forced response (e.g., internal variability) <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx56" id="paren.48"/>. In this paper, we treat the RACMO-ERA simulation as <inline-formula><mml:math id="M26" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> as there is no in-situ observation of GrIS SMB at the temporal and spatial coverages necessary for this D&amp;A analysis; <inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are estimated by the ensemble mean of CESM2-LE and CESM2-SFLE. For the univariate case (<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is estimated by the ensemble mean from ALL as <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">ALL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; for the bivariate case (<inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are estimated by the ensemble mean from GHG and AAER as <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (or <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">xAAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mtext>ALL-minus-xAAER</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>). Eq. (1) can be solved by performing an ordinary least squares (OLS) regression with <inline-formula><mml:math id="M37" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. In this case, we assume <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is observed without uncertainty. When <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is significantly larger than 0, the forced response from fingerprint <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is considered detectable; when <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is not significantly different from 1, the forced response is considered attributable to the fingerprint <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The significance level of <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is usually determined from the distribution of <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> due to internal variability, estimated from climate models (e.g., from pre-industrial simulations (<italic>PiControl</italic>) or historical simulations from which the ensemble mean has been removed), and follows the IPCC guidance to indicate the significance of <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the confidence of attributing this signal to a given forcing(s).</p>
      <p id="d2e846">In practice, <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> contains uncertainties, such as from the choice of climate models and the errors due to averaging over a finite number of ensemble members. A total least squares (TLS) regression is a common solution to perform D&amp;A to account for uncertainty in <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx30 bib1.bibx53" id="paren.49"/>. Eq. (1) can be rewritten as

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M49" display="block"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>m</mml:mi></mml:munderover><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></disp-formula>

          where now, <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ϵ</mml:mi><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is introduced to account for the uncertainties in simulated forced response in <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. A singular value decomposition (SVD) on the system of equations can solve <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in a deterministic way for the TLS regression <xref ref-type="bibr" rid="bib1.bibx1" id="paren.50"/>.</p>
      <p id="d2e969">The choice of whether to use an OLS or TLS regression should be made with caution, as TLS regression is not necessarily preferred over OLS for climate change D&amp;A <xref ref-type="bibr" rid="bib1.bibx39" id="paren.51"/>. For example, the deterministic solutions of TLS regression can be considered as a linear transformation of OLS regression coefficients and, mathematically, such a transformation could introduce an upward bias for the regression coefficients, leading to a potential false positive in D&amp;A when determining <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with TLS regression <xref ref-type="bibr" rid="bib1.bibx39" id="paren.52"/>. Moreover, climate models have biases in simulating the internal variability, either too large or too small a magnitude, which makes estimating the significance level of <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from internal variability based on that from climate models an imperfect approach.</p>
      <p id="d2e1001">In this study, we instead construct a Bayesian TLS regression to reduce bias and account for the uncertainty from using a climate model large ensemble from a single model (CESM2-LE and CESM2-SFLE). We first construct an ensemble of numerical experiments for an ideal case of one-dimensional linear regression <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:mi>x</mml:mi></mml:mrow></mml:math></inline-formula> where both sampled data <inline-formula><mml:math id="M56" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M57" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> have noise (see Supplementary Information). This experiment confirms that the deterministic TLS regression solution overestimates the regression coefficients when compared with OLS regression and that our Bayesian TLS regression can alleviate this upward bias (Fig. S1). We also calculate the scaling factor for attributing GrIS SMB changes to ALL historical forcings with CESM2-LE with a deterministic OLS regression, a deterministic TLS regression, and a Bayesian TLS regression (Fig. S2). Our results demonstrate that our Bayesian TLS regression provides the most conservative estimate of the significance level of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and does not overestimate the scaling factor in the same way as the deterministic TLS solution (Fig. S2).</p>
<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Bayesian TLS regression</title>
      <p id="d2e1050">A Bayesian TLS regression with a Markov Chain Monte Carlo (MCMC) technique is used to address concerns of using a deterministic TLS regression for D&amp;A <xref ref-type="bibr" rid="bib1.bibx29" id="paren.53"/>. With prior knowledge about the data and the uncertainty it might introduce for the D&amp;A analysis, we define three parameters to set up the Bayesian TLS regression: the scaling factors (<inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), the uncertainty of estimating the true forced response with CESM2-LE and CESM2-SFLE (<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and the uncertainty of observing the true forced response in the reference data (i.e., usually due to internal variability; <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). With a Bayesian TLS regression, the parameters in a regression model (<inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) are estimated in a probabilistic way, with the priors of their distributions determined from the data from RACMO-ERA, CESM2-LE, and CESM2-SFLE. In addition, a latent variable, <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">latent</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:mi>x</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, is introduced to represent an unknown true forced response(s) from CESM2-LE/CESM2-SFLE (i.e., <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">latent</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, the true unknown fingerprint(s), is a draw from a normal distribution with mean determined by <inline-formula><mml:math id="M67" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> with a spread of <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>). Therefore, we formulate the D&amp;A with

              <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M69" display="block"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">latent</mml:mi></mml:msub><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">ensmean</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>(</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">ensmean</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:msqrt><mml:mi>n</mml:mi></mml:msqrt></mml:mfrac></mml:mstyle><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p id="d2e1232">The mean of <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">latent</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is estimated by the ensemble mean from the simulation(s) used for D&amp;A (<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">ensmean</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) with a spread defined as the standard error of the estimated forced response from that ensemble mean (<inline-formula><mml:math id="M72" display="inline"><mml:mstyle displaystyle="false"><mml:mfrac style="text"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">ensmean</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:msqrt><mml:mi>n</mml:mi></mml:msqrt></mml:mfrac></mml:mstyle></mml:math></inline-formula>), where <inline-formula><mml:math id="M73" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number of ensemble members. With the assumption of the posterior distribution of <inline-formula><mml:math id="M74" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> as

              <disp-formula id="Ch1.E4" content-type="numbered"><label>4</label><mml:math id="M75" display="block"><mml:mrow><mml:mi>y</mml:mi><mml:mo>∼</mml:mo><mml:mi mathvariant="script">N</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:msub><mml:mi>x</mml:mi><mml:mi mathvariant="normal">latent</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>y</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula>

            the Bayesian TLS regression coefficient (<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is solved with PyMC. Technical details (including the setup for priors) and idealized numerical experiments can be found in the Supplementary Information.</p>
      <p id="d2e1336">In this paper, we use the Bayesian TLS regression to obtain 10 000 posterior samples of <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> so that we can estimate the confidence level of the attribution based on the posterior distributions of <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. This Bayesian TLS regression is also applied to estimate the temperature sensitivity of SMB and <inline-formula><mml:math id="M79" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> to TAS in the reference data and the forced responses simulated by CESM2 (see Table S1 for setups of priors).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Decadal variability in GMSL due to GrIS SMB changes</title>
      <p id="d2e1385">Reconstruction data from <xref ref-type="bibr" rid="bib1.bibx15" id="text.54"/> shows that total GrIS mass loss has decadal variability and this decadal variability comes from the anomalous SMB relative to its long-term climatology (Fig. 1; correlation coefficient between SMB and total mass loss is 0.72, <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, at interannual time scales; 0.92, <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, for 10-year running means with effective degree of freedom, eDOF, reduced to 6). For example, there are positive SMB anomalies during 1970–2000, slowing the rise in GMSL due to GrIS mass loss (Fig. 1); in turn, the greater decline in SMB after 2000 leads to an accelerated rise in GMSL contributed by the GrIS. We note that the high correlations between the total mass loss from <xref ref-type="bibr" rid="bib1.bibx15" id="text.55"/> and the RACMO-simulated SMB reported here could also be influenced by the fact that reconstructed GrIS mass loss data includes RACMO-simulated SMB.</p>

      <fig id="F1"><label>Figure 1</label><caption><p id="d2e1420">Decadal variability in GrIS' contribution to Global Mean Sea Level (GMSL) is observable and explained by decadal variability in surface mass balance (SMB). The anomalous (long-term mean subtracted) annual GrIS mass loss from the <xref ref-type="bibr" rid="bib1.bibx15" id="text.56"/> reconstruction (green) and the anomalous annual GrIS SMB simulated by RACMO with ERA5 reanalysis (RACMO-ERA; black). The thick green lines are the 5000-member ensemble mean values of the <xref ref-type="bibr" rid="bib1.bibx15" id="text.57"/> reconstruction, and the shadings are <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> standard deviation across the 5000 ensemble members.</p></caption>
          <graphic xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026-f01.png"/>

        </fig>


</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Detection and attribution of historical GrIS SMB changes</title>
      <p id="d2e1455">CESM2-LE with historical forcing (ALL) simulates a decline in SMB that is most apparent after 1990 (Fig. 2a), despite a wide range of internal variability (purple shading) that also covers the interannual variability in RACMO-ERA. According to the D&amp;A framework, the SMB change in RACMO-ERA is detectable and attributable to historical forcing with 99 % confidence (i.e., <italic>virtually certain</italic>; Fig. 2b). SMB changes can be approximated as precipitation (<inline-formula><mml:math id="M83" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>) minus runoff (<inline-formula><mml:math id="M84" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>; Fig. S3, temporal correlation coefficient 0.99, <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, and 1.00, <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, for 10-year running mean time series with 6 eDOF), as sublimation contributes <inline-formula><mml:math id="M87" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 10 % of SMB budget <xref ref-type="bibr" rid="bib1.bibx61" id="paren.58"/>. The individual time series show that both ALL-forced precipitation and runoff increase (Fig. 2c, e; note that <inline-formula><mml:math id="M88" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> is inverted). However, this ALL-forced increase in precipitation is not detected in the observation (Fig. 2d), meaning the observed variability of precipitation could just be internal variability (see also <xref ref-type="bibr" rid="bib1.bibx61" id="text.59"/>).  On the other hand, the increase in <inline-formula><mml:math id="M89" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> is detectable and attributable to ALL historical forcing (Fig. 2f; 99 % confidence, <italic>virtually certain</italic>), agreeing with previous studies that historical GrIS SMB loss is mainly due to warming-driven runoff changes <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx43 bib1.bibx61" id="paren.60"/>.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e1536"><bold>(a, c, e)</bold> Time series of annual GrIS SMB, <inline-formula><mml:math id="M90" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, -<inline-formula><mml:math id="M91" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> since 1958 from RACMO-ERA (black; light gray and gray dashed lines are 10-year and 5-year running mean) and ensemble mean of CESM2-LE (purple). The purple shadings are the full range across ensemble members (i.e., maxima to minima). <bold>(b, d, f)</bold> Univariate scaling factors (<inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ALL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of GrIS SMB, <inline-formula><mml:math id="M93" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M94" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>. The horizontal line is the mean of the 10 000 posterior samples of <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ALL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and the gray shading/thick black vertical line/thin black vertical line is <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.64</mml:mn><mml:mo>/</mml:mo><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.57</mml:mn></mml:mrow></mml:math></inline-formula>  standard deviation of the 10 000 posterior samples of <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ALL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, indicating the 66 %<inline-formula><mml:math id="M98" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>90 %<inline-formula><mml:math id="M99" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>99 % confidence intervals in D&amp;A (<italic>likely</italic>/<italic>very likely</italic>/<italic>virtually certain</italic> based on IPCC guideline). Here, the scaling factor (<inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">ALL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is derived by the Bayesian Total Least Squares regression with <inline-formula><mml:math id="M101" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> from RACMO-ERA and <inline-formula><mml:math id="M102" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> from ensemble mean of CESM2-LE.</p></caption>
          <graphic xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026-f02.png"/>

        </fig>

      <p id="d2e1683">The GrIS SMB changes from ALL (Fig. 2a purple solid line) can be approximated as the sum of the changes from GHG and AAER (Fig. S3; temporal correlation coefficient 0.66, <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, for SMB time series from ALL vs. GHG <inline-formula><mml:math id="M104" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> AAER and 0.93, <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>, for 10-year running means with 6 eDOF), with GHG driving a long-term decline in SMB and AAER contributing to an increase before mid-1980 and a slight decrease thereafter (Fig. 3a). Before mid-1980, GHG and AAER basically cancel each other out, while they combine to drive the decline of ALL-forced SMB afterward (Fig. 3a).</p>
      <p id="d2e1718">A bivariate Bayesian TLS regression is formulated to assess the D&amp;A for these two historical radiative forcings, showing that both GHG (99 % confidence, <italic>virtually certain</italic>) and AAER (90 % confidence, <italic>very likely</italic>) contribute to the GrIS SMB changes (Fig. 3b). Interestingly, the posterior distribution of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has a narrower spread than the posterior distribution of <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, implying a lower S <inline-formula><mml:math id="M108" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N in detecting the AAER-forced signal in RACMO-ERA SMB changes. Consistent with Fig. 2, there is no detectable precipitation change due to either GHG or AAER in RACMO-ERA (Fig. 3c, d). However, there is a detectable GrIS runoff change attributed to both GHG and AAER, but both their influences are potentially underestimated (i.e., <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are both significantly larger than 1), and <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> also has a wider spread in its posterior distribution than <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for runoff (Fig. 3e, f).</p>

      <fig id="F3" specific-use="star"><label>Figure 3</label><caption><p id="d2e1803"><bold>(a, c, e)</bold> Time series of annual GrIS SMB, <inline-formula><mml:math id="M113" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, -<inline-formula><mml:math id="M114" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> since 1958 from ensemble mean of CESM2-SFLE greenhouse gases-only simulation (GHG; red), ensemble mean of CESM2-SFLE anthropogenic aerosols-only simulation (AAER; blue), ensemble mean of CESM2-LE ALL simulation (purple as Fig. 2). The red/blue shadings are the full range across ensemble members (i.e., maxima to minima) in GHG/AAER. <bold>(b, d, f)</bold> Bivariate scaling factors (<inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) of GrIS SMB, <inline-formula><mml:math id="M117" display="inline"><mml:mi>P</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M118" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>. The firebrick plus symbol is the mean of the 10 000 posterior samples of <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and the golden/orange/firebrick confidence ellipses are the 66 %<inline-formula><mml:math id="M121" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>90 %<inline-formula><mml:math id="M122" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>99 % confidence intervals in <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for D&amp;A (<italic>likely/very likely/virtually certain</italic> based on IPCC guideline). When the confidence ellipse includes the point (1, 1) (shown as the crimson star) and excludes the origin (0, 0) (shown as the black dot), a bivariate attribution to both forcings is established. Here, scaling factors (<inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) are derived by the Bayesian Total Least Squares regression with <inline-formula><mml:math id="M127" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> from RACMO-ERA and <inline-formula><mml:math id="M128" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> from ensemble mean of AAER and GHG from CESM2-SFLE.</p></caption>
          <graphic xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026-f03.png"/>

        </fig>

      <p id="d2e1967">Studies have shown that CESM2 has nonlinear forced responses due to different climate mean states <xref ref-type="bibr" rid="bib1.bibx55" id="paren.61"/> or the non-additive responses to different forcings <xref ref-type="bibr" rid="bib1.bibx33" id="paren.62"/>. Therefore, we repeat the bivariate D&amp;A with SMB, precipitation, and runoff from the xAAER and ALL-minus-xAAER simulations to check the robustness of attributing both anthropogenic aerosols and greenhouse gases when using a climate model (CESM2) with reported nonlinear forced responses. Using xAAER and ALL-minus-xAAER to represent GHG and AAER forcing, this analysis yields robust conclusions: GHG and AAER create forced signals in the historical 1958–2019 GrIS SMB through runoff changes, and the attribution to both xAAER and ALL-minus-xAAER is <italic>virtually certain</italic> (99 % confidence; Fig. S4). Interestingly, the posterior distribution of <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mtext>ALL-minus-xAAER</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> has a narrower spread for both SMB and runoff compared with the posterior distribution of <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Figs. S4b and  3b for SMB and Figs. S4f and  3f for runoff), though <inline-formula><mml:math id="M131" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mtext>ALL-minus-xAAER</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> still have a wider spread than <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">xAAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Additionally, runoff changes are not underestimated in ALL-minus-xAAER and xAAER (Fig. S4f) as they are in GHG and AAER (Fig. 3f), as the means of the posterior bivariate scaling factors are now closer to (1, 1). Thus, there appears to be a state dependence of the attribution to AAER.</p>
      <p id="d2e2046">Overall, our D&amp;A results indicate that historical GrIS SMB changes are attributable to both GHG and AAER through runoff changes. Despite differences in the scaling factors, these attribution results are robust to the sets of single forcing simulations used (<italic>all-but-forcing</italic> or <italic>forcing-only</italic> experimental setups with CESM2). We also point out that there is a lower S <inline-formula><mml:math id="M135" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N when attributing GrIS SMB changes and runoff changes to AAER compared with attributing to GHG. This lower S <inline-formula><mml:math id="M136" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N when attributing to AAER appears in two ways: (1) underestimated response (usually <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> and also <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and (2) wider confidence intervals of <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">AAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> than of <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">GHG</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Mean state temperature affects uncertainty in D&amp;A for AAER</title>
      <p id="d2e2129">GrIS SMB has a stronger sensitivity to warming than to cooling <xref ref-type="bibr" rid="bib1.bibx59" id="paren.63"/>, and runoff has a nonlinear relationship to temperature change <xref ref-type="bibr" rid="bib1.bibx60" id="paren.64"/>. This nonlinear runoff response to temperature is commonly seen in cryospheric variables in response to different mean state temperatures <xref ref-type="bibr" rid="bib1.bibx17" id="paren.65"/> with different energy barriers to overcome and/or different positive degree days to start melting and inducing runoff changes <xref ref-type="bibr" rid="bib1.bibx54" id="paren.66"/>. Here, we hypothesize that the different temperature sensitivities of runoff in these different simulations might contribute to the lower S <inline-formula><mml:math id="M141" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N of the attribution to AAER compared with the attribution to GHG. SMB has a negative temperature sensitivity in RACMO-ERA, ALL, and GHG simulations (Fig. 4a), and all of these simulations demonstrate apparent increases in runoff with warming (Fig. 4b). However, this negative temperature sensitivity is not seen in the AAER simulation (Fig. 4a). There is a nonlinear temperature sensitivity of runoff if the simulations are sorted by their 1958–2019 climatological temperatures (Fig. 4b), explaining the lack of negative temperature sensitivity of SMB in AAER (Fig. 4a). In addition, the mean temperature over the GrIS has a weaker forced response in AAER than in GHG (Fig. S5; also true using ALL-minus-xAAER and xAAER). Together with the weaker temperature sensitivity of SMB in AAER due to the weaker temperature sensitivity of runoff, these two factors lead to a generally lower S <inline-formula><mml:math id="M142" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N in attributing SMB changes to AAER than GHG. Precipitation sensitivity to warming is generally positive across simulations (Figure S6), as precipitation usually increases under warming <xref ref-type="bibr" rid="bib1.bibx22" id="paren.67"/>. Note that precipitation sensitivity is much higher in the ALL-minus-xAAER simulation than in the AAER simulation (Fig. S6), explaining the slightly more positive SMB sensitivity in ALL-minus-xAAER (Fig. 4a).</p>

      <fig id="F4" specific-use="star"><label>Figure 4</label><caption><p id="d2e2164"><bold>(a)</bold> The observed (RACMO-ERA; black) and forced (ALL, GHG, xAAER, AAER, ALL-minus-xAAER; purple, red, orange, blue, light blue respectively) GrIS SMB sensitivity to near-surface temperature during 1958–2019 sorted by the climatological mean near-surface temperature. <bold>(b)</bold> The observed (RACMO-ERA; black) and forced GrIS <inline-formula><mml:math id="M143" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> sensitivity to near-surface temperature during 1958–2019 sorted by the climatological mean near-surface temperature. Here, SMB and <inline-formula><mml:math id="M144" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> sensitivities are derived by the Bayesian Total Least Square regression with SMB or <inline-formula><mml:math id="M145" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> as <inline-formula><mml:math id="M146" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> and TAS as <inline-formula><mml:math id="M147" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> from RACMO, the ensemble mean of CESM2-LE, or the ensemble mean of CESM2-SFLE as appropriate.</p></caption>
          <graphic xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026-f04.png"/>

        </fig>

      <p id="d2e2214">This mean state temperature dependent SMB and runoff sensitivity can also explain why the uncertainty ellipse of <inline-formula><mml:math id="M148" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> using xAAER and ALL-minus-xAAER (Fig. S4) is smaller than the uncertainty ellipse using AAER and GHG (Fig. 3). This is because xAAER and ALL-minus-xAAER simulations both have higher mean state temperatures than GHG and AAER simulations (orange vs. red bars and light blue vs blue bars in Fig. 4). The runoff responses are thus stronger in both the xAAER and ALL-minus-xAAER simulations, and therefore easier to detect; <inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">xAAER</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mtext>ALL-minus-xAAER</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> are both closer to (1, 1) with narrower posterior distributions (Figs. 3f vs. S4f). Although the attribution to AAER is robust across <italic>all-but-forcing</italic> or <italic>forcing-only</italic> experimental setups in CESM2, these results demonstrate that mean state temperatures in different simulations can affect their runoff responses and therefore our confidence in attributing SMB changes to that forcing with this D&amp;A framework.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Atmospheric drivers of forced GrIS runoff changes</title>
      <p id="d2e2260">What are the mechanisms by which GHG and AAER forcing drive long-term trends and decadal variability in GrIS SMB through runoff changes? Here, we focus on the summer (JJA) temperature and circulation patterns, which are linked to the melting-induced runoff changes <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx18 bib1.bibx58" id="paren.68"/>. The trend map for 1958–2019 from ERA5 shows overall JJA polar warming and increasing <inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> over Greenland (Fig. 5a), consistent with the Greenland Block Index (GBI) time series (Fig. S7a). The correlation between annual GrIS runoff and JJA near-surface temperature and JJA <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from ERA5 is positive, i.e., a Greenland blocking pattern (Fig. 5e). Greenland blocking provides more cloudless days and subsidence-induced warming <xref ref-type="bibr" rid="bib1.bibx54" id="paren.69"/>, as well as warm air advection towards Western Greenland <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx58" id="paren.70"/> due to the anti-cyclone over Greenland. The correlation pattern in ERA5 remains consistent even after detrending and temporal smoothing (Fig. S8). Thus, the long-term linear trend has little impact on the correlation pattern seen in ERA5.</p>

      <fig id="F5" specific-use="star"><label>Figure 5</label><caption><p id="d2e2296">Trend maps of 500 hPa geopotential height (<inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; contours) and near-surface air temperature (TAS; shading) during 1958–2019 in <bold>(a)</bold> ERA5 reanalysis, <bold>(b)</bold> ensemble mean of all forcings CESM2-LE simulations (50; ALL), <bold>(c)</bold> ensemble mean of GHG-only simulations (15; GHG), and <bold>(d)</bold> ensemble mean of AAER-only simulations (15; AAER). Grid cells with insignificant TAS trends are masked out  (95 % confidence for ERA5, and ensemble mean trend over 1 standard deviation across all trends in the ensemble for climate model simulations). Grid cells with significant <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trends are hatched (95 % confidence for ERA5 and ensemble mean trend over 1 standard deviation across all possible trends in the ensemble for climate model simulations). <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> contours start from <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> (m per 62 years) with contour spacing of 10 (m per 62 years). <bold>(e–f)</bold> Correlation map of GrIS <inline-formula><mml:math id="M157" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> with <inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (contours) and TAS (shading) during 1958–2019 in <bold>(e)</bold> ERA5 reanalysis and <bold>(f)</bold> 15-member mean AAER. Insignificant TAS correlations are masked out and significant <inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> correlations are hatched (95 % confidence). Contours start from 0.1 with contour spacing of 0.1. The significance level of the correlation coefficients is based on a <inline-formula><mml:math id="M160" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>-test with the degrees of freedom corresponding to the length of data (1958–2019, 62 years).</p></caption>
          <graphic xlink:href="https://tc.copernicus.org/articles/20/2317/2026/tc-20-2317-2026-f05.png"/>

        </fig>

      <p id="d2e2407">JJA near-surface warming and <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increasing trends over the North Atlantic sector are visible in both ALL (Fig. 5b) and GHG (Fig. 5c). Though the ALL-forced <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trend is weaker than the observed <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trend (consistent with GBI in Fig. S7 and <xref ref-type="bibr" rid="bib1.bibx7" id="text.71"/>), the observed trend is within the range of possible trends from the 50-member ALL ensemble. The forced temperature and <inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trends from ALL and GHG are overall alike, confirming that GHG contributes to the long-term linear trend seen in these atmospheric variables related to GrIS runoff changes. However, in GHG, the Atlantic Meridional Overturning Circulation (AMOC) declines more rapidly than in ALL, as it lacks the offsetting North Atlantic cooling from AAER (Fig. 9 in <xref ref-type="bibr" rid="bib1.bibx55" id="text.72"/>), leading to cooling in the Subpolar Gyre. Additionally, ALL-forced JJA <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increases with a blocking-like structure over Greenland, while GHG-forced JJA <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> increases more uniformly (Fig. 5b vs. c contour). A cooling of the Subpolar Gyre in GHG simulation and a stronger subsidence trend in ALL together lead to <italic>less</italic> warming in GHG than in ALL (Fig. 5b vs. c).</p>
      <p id="d2e2487">In addition, the Subpolar Gyre cooling correlates with a more positive NAO <xref ref-type="bibr" rid="bib1.bibx14" id="paren.73"/>. This implies a less negative NAO/reduced Greenland blocking as a result of this air-sea coupled feedback over the Subpolar Gyre, which may explain why GHG-forced runoff (Fig. 3e) and GBI (Fig. S7b) plateaus after 2000 when the Subpolar Gyre cooling intensifies. This is also supported by the significant correlations of an emerging Greenland blocking pattern in GHG (Fig. S9a) that differs from its uniform warming and <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trends (Fig. 5c), regardless of whether linear trends in GHG are removed or not (Fig. S9a vs. b). Although beyond the scope of this study, idealized experiments to distinguish the circulation changes originating from direct GHG radiative forcing versus from GHG-induced Subpolar Gyre SSTs would help advance understanding of the role of atmospheric circulation changes in GrIS mass loss.</p>
      <p id="d2e2504">AAER, on the other hand, contributes almost nothing to this long-term trend pattern (Fig. 5a vs. d). These trend maps imply that the detected signal from AAER during 1958–2019 (Fig. 3b, f) does not arise through the long-term linear trend but through forced decadal variability undergoing phase changes during this time period. We compare maps of the correlation from ERA5 (Fig. 5e) and from the ensemble mean of AAER during 1958–2019 (Fig. 5f). The AAER-based correlation map shows a pattern that is distinct from its long-term trend (Fig. 5f vs. d); instead, the correlation map shows a pattern more similar to the ERA5-based correlation map (Fig. 5e vs. f). Both ERA5 and AAER have positive correlations between GrIS runoff and near-surface temperature and <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Figure 5f confirms a similar correlation pattern due to AAER, supporting an AAER-forced change in the variability of circulation, imprinted onto a pattern that reinforces Greenland blocking, consistent with <xref ref-type="bibr" rid="bib1.bibx35" id="text.74"/>.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Discussion and Conclusion</title>
      <p id="d2e2530">In this paper, we formulate a D&amp;A analysis with CESM2-LE and CESM2-SFLE to investigate 1958–2019 GrIS SMB change and show that the historical SMB change is attributable not only to GHG but also to AAER. To our knowledge, this is the first manuscript demonstrating that parts of the historical GrIS SMB change are attributable to AAER. Specifically, GHG drives the long-term SMB decline, while AAER contributes to the decadal variability of SMB, consistent with a growing literature on how AAER induces decadal variations to other aspects of historical North Atlantic climate change <xref ref-type="bibr" rid="bib1.bibx52" id="paren.75"/>.</p>
      <p id="d2e2536">To understand the mechanisms of forced SMB change, we consider two perspectives. First, from a mass balance perspective, we demonstrate that the historical forced SMB changes in a ERA5 reanalysis-based RACMO simulation are mainly driven by runoff changes, irrespective of the underlying forcing (GHG or AAER). Second, we investigate the atmospheric pathways by which these forcings affect runoff, demonstrating that the GHG-forced runoff change is mainly driven by long-term warming and the AAER-driven runoff change relates to atmospheric circulation variability of Greenland blocking on decadal time scales <xref ref-type="bibr" rid="bib1.bibx54 bib1.bibx3 bib1.bibx19" id="paren.76"/>. These results highlight that different climate forcings can drive SMB changes through different physical mechanisms, with different spatial patterns and time scales (i.e., long-term trend vs decadal variability).</p>
      <p id="d2e2542">Attribution of regional climate change to AAER often has a low S <inline-formula><mml:math id="M169" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N compared to GHG attribution (e.g., <xref ref-type="bibr" rid="bib1.bibx37" id="text.77"/>) and our study confirms this tendency. In the case of attributing GrIS SMB, this is due to the temperature sensitivity of runoff being weaker in AAER than GHG, as the sensitivity strongly depends on mean state temperatures in each simulation. We compare the sets of <italic>forcing-only</italic> (GHG and AAER) and <italic>all-but-forcing</italic> (xAAER and ALL-minus-xAAER) CESM2 experiments, where we show robust attribution of historical GrIS SMB changes to both GHG and AAER through runoff changes. The mean state temperature dependency of runoff response can also explain the difference of S <inline-formula><mml:math id="M170" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> N in the <italic>forcing-only</italic> and <italic>all-but-forcing</italic> sets, as their mean state temperatures are different. Although we show that both AAER and GHG contribute to the historical GrIS SMB changes, such a mean state temperature dependence of the forced SMB response implies a potential bias in the current D&amp;A framework – certain forcings, such as GHG, can individually create a mean state with a stronger response that is more likely to be attributed. Future work will need to develop D&amp;A methods that can systematically account for mean state temperature dependency in climate responses.</p>
      <p id="d2e2575">CESM2 and RACMO simulate reasonable SMB and water budgets <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx61" id="paren.78"/>; however, both are subject to model structural uncertainty. The model structural uncertainty accounts for most of the uncertainty in SMB future projections <xref ref-type="bibr" rid="bib1.bibx25" id="paren.79"/>. The snow parameterization uncertainty contributes to part of the high model structural uncertainty in SMB but does not serve as the main contributor <xref ref-type="bibr" rid="bib1.bibx25" id="paren.80"/>. Instead, it comes from atmospheric variables, as GrIS precipitation, temperature, and <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">500</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> all show high model structural uncertainties in their future projections <xref ref-type="bibr" rid="bib1.bibx64" id="paren.81"/>. One motivation to conduct D&amp;A with Bayesian regression, instead of a deterministic regression, is to account for the uncertainty in estimates of forced responses (from CESM2) and of observations (from RACMO). Still, we acknowledge the caveat that this study does not fully sample model structural uncertainty. Future work to extend D&amp;A with more climate models could enhance the robustness of the results presented here. Such efforts could also support the development of observational constraints on SMB projections, for example, based on the temperature sensitivity presented here.</p>
      <p id="d2e2602">On top of the different runoff responses due to the mean state temperature dependence, we note that historical aerosol emissions used in CMIP6 simulations have large uncertainties, especially pre-1980 <xref ref-type="bibr" rid="bib1.bibx36" id="paren.82"/>. Beyond the scope of this paper, future works should thus explore the impacts of aerosol emissions and forcing uncertainties on D&amp;A of GrIS SMB changes.</p>
      <p id="d2e2608">The mean state temperature dependency of runoff found in our study implies that GrIS SMB changes might accelerate in the future, especially as we expect continued increases in greenhouse gases with simultaneous reductions in anthropogenic aerosols <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx49" id="paren.83"/>. Thus, under stronger warming in these future projections, further growth in the contribution of GrIS SMB reduction to GMSL rise is foreseeable.</p>
</sec>

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

      <p id="d2e2619">The global mean sea level (GMSL) contributed by Greenland Ice Sheet (GrIS) reconstruction dating back to 1900 is taken from <xref ref-type="bibr" rid="bib1.bibx15" id="text.84"/> with their data publicly accessible from Zenodo (<ext-link xlink:href="https://doi.org/10.5281/zenodo.3862995" ext-link-type="DOI">10.5281/zenodo.3862995</ext-link>, <xref ref-type="bibr" rid="bib1.bibx16" id="altparen.85"/>). RACMO-ERA from <ext-link xlink:href="https://doi.org/10.5281/zenodo.7100706" ext-link-type="DOI">10.5281/zenodo.7100706</ext-link> <xref ref-type="bibr" rid="bib1.bibx46" id="paren.86"/>. Instructions on how to access data from Community Earth System Model version 2 large ensemble and single forcing large ensemble can be found at <uri>https://www.cesm.ucar.edu/community-projects/lens2/data-sets</uri> (20 January 2026).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d2e2641">The supplement related to this article is available online at <inline-supplementary-material xlink:href="https://doi.org/10.5194/tc-20-2317-2026-supplement" xlink:title="pdf">https://doi.org/10.5194/tc-20-2317-2026-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e2650">All the authors were involved in the conceptualization of this project, the discussion of the interpretations of results, and the revision of the drafts. YNK analyzed the data, created the visualization, and wrote the first draft of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e2656">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e2662">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e2668">The authors appreciate insightful discussions with Lorenzo Polvani, You-Ting Wu, Angeline Pendergrass, John Fasullo, William Lipscomb, and Natalie Mahowald when preparing the manuscript. The authors also thank the editor and reviewers for their constructive feedback during the revision to improve the manuscript.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e2673">This research has been supported by the Swiss National Science Foundation (grant no. PZ00P2_174128). Riley Culberg was supported in part by NASA grants 80NSSC24K1445 and 80NSSC24K1037.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e2679">This paper was edited by Xavier Fettweis and reviewed by two anonymous referees.</p>
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