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<journal-meta>
<journal-id journal-id-type="publisher-id">Front. Clim.</journal-id>
<journal-title-group>
<journal-title>Frontiers in Climate</journal-title>
<abbrev-journal-title abbrev-type="pubmed">Front. Clim.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2624-9553</issn>
<publisher>
<publisher-name>Frontiers Media S.A.</publisher-name>
</publisher>
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<article-meta>
<article-id pub-id-type="doi">10.3389/fclim.2026.1739394</article-id>
<article-version article-version-type="Version of Record" vocab="NISO-RP-8-2008"/>
<article-categories>
<subj-group subj-group-type="heading">
<subject>Original Research</subject>
</subj-group>
</article-categories>
<title-group>
<article-title>The role of internal variability and external forcing on the emergence of hot and dry compound extremes in the CESM2 large ensemble</article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author" corresp="yes">
<name><surname>Dwyer</surname> <given-names>Ashley E.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="corresp" rid="c001"><sup>&#x0002A;</sup></xref>
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<contrib contrib-type="author">
<name><surname>Hurrell</surname> <given-names>James W.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
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<contrib contrib-type="author">
<name><surname>Barnes</surname> <given-names>Elizabeth A.</given-names></name>
<xref ref-type="aff" rid="aff1"><sup>1</sup></xref>
<xref ref-type="aff" rid="aff2"><sup>2</sup></xref>
<xref ref-type="aff" rid="aff3"><sup>3</sup></xref>
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<aff id="aff1"><label>1</label><institution>Department of Atmospheric Science, Colorado State University</institution>, <city>Fort Collins</city>, <state>CO</state>, <country country="us">United States</country></aff>
<aff id="aff2"><label>2</label><institution>Faculty of Computing and Data Sciences, Boston University</institution>, <city>Boston</city>, <state>MA</state>, <country country="us">United States</country></aff>
<aff id="aff3"><label>3</label><institution>Department of Earth and Environment, Boston University</institution>, <city>Boston</city>, <state>MA</state>, <country country="us">United States</country></aff>
<author-notes>
<corresp id="c001"><label>&#x0002A;</label>Correspondence: Ashley E. Dwyer, <email xlink:href="mailto:aedwyer@colostate.edu">aedwyer@colostate.edu</email></corresp>
</author-notes>
<pub-date publication-format="electronic" date-type="pub" iso-8601-date="2026-03-03">
<day>03</day>
<month>03</month>
<year>2026</year>
</pub-date>
<pub-date publication-format="electronic" date-type="collection">
<year>2026</year>
</pub-date>
<volume>8</volume>
<elocation-id>1739394</elocation-id>
<history>
<date date-type="received">
<day>04</day>
<month>11</month>
<year>2025</year>
</date>
<date date-type="rev-recd">
<day>03</day>
<month>02</month>
<year>2026</year>
</date>
<date date-type="accepted">
<day>06</day>
<month>02</month>
<year>2026</year>
</date>
</history>
<permissions>
<copyright-statement>Copyright &#x000A9; 2026 Dwyer, Hurrell and Barnes.</copyright-statement>
<copyright-year>2026</copyright-year>
<copyright-holder>Dwyer, Hurrell and Barnes</copyright-holder>
<license>
<ali:license_ref start_date="2026-03-03">https://creativecommons.org/licenses/by/4.0/</ali:license_ref>
<license-p>This is an open-access article distributed under the terms of the <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution License (CC BY)</ext-link>. The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.</license-p>
</license>
</permissions>
<abstract>
<p>Extreme hot and dry compound events pose significant hazards to human health, agriculture, and ecosystems, making it critical to better understand what drives their occurrence and spatiotemporal variability. Although the role of internal climate variability in driving compound events has been previously studied, we leverage a large ensemble to enable a more robust understanding of the response of hot and dry events to both large-scale internal climate variability and external forcing. We explore the influence of well-known large-scale climate modes including the El Ni&#x000F1;o Southern Oscillation (ENSO), Pacific Decadal Oscillation (PDO), Indian Ocean Dipole (IOD), and the North Atlantic Oscillation (NAO) on the occurrence of hot and dry compound events in the Community Earth System Model 2 Large Ensemble (CESM2-LE). We also investigate when anthropogenic changes in hot and dry compound events emerge from internal variability. Overall, we find that internal climate variability is, and will continue to be, a strong influence on compound event occurrence, although external forcing will likely cause changes in frequency patterns over the 21<sup><italic>st</italic></sup> century. We also find that under SSP 3-7.0, frequencies of compound events in most of the world will emerge from internal variability by 2100. Knowledge of drivers from an internal variability perspective combined with an understanding of greenhouse gas forced changes can aid in quantifying the predictability of extreme compound events on regional scales.</p></abstract>
<kwd-group>
<kwd>climate</kwd>
<kwd>climate variability</kwd>
<kwd>compound event drivers</kwd>
<kwd>compound extremes</kwd>
<kwd>time of emergence</kwd>
</kwd-group>
<funding-group>
<funding-statement>The author(s) declared that financial support was received for this work and/or its publication. This work was supported by the National Science Foundation (NSF) Grant number AGS-2210068.</funding-statement>
</funding-group>
<counts>
<fig-count count="6"/>
<table-count count="0"/>
<equation-count count="0"/>
<ref-count count="58"/>
<page-count count="13"/>
<word-count count="8324"/>
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<custom-meta-group>
<custom-meta>
<meta-name>section-at-acceptance</meta-name>
<meta-value>Predictions and Projections</meta-value>
</custom-meta>
</custom-meta-group>
</article-meta>
</front>
<body>
<sec sec-type="intro" id="s1">
<label>1</label>
<title>Introduction</title>
<p>Hot and dry compound events pose significant hazards through impacts on human health (e.g., temperature-related deaths), agriculture (e.g., reduction in crop yield), and ecosystems (<xref ref-type="bibr" rid="B48">Tabari and Willems, 2023</xref>; <xref ref-type="bibr" rid="B38">Niggli et al., 2022</xref>; <xref ref-type="bibr" rid="B58">Zscheischler et al., 2020b</xref>), making it critical to better understand what drives their occurrence and spatiotemporal variability. Although drivers of compound events, including and most often the El Ni&#x000F1;o Southern Oscillation (ENSO) (<xref ref-type="bibr" rid="B3">Brett et al., 2025</xref>), have been analyzed through the observational record (e.g., <xref ref-type="bibr" rid="B36">Mukherjee et al., 2020</xref>; <xref ref-type="bibr" rid="B19">Hao et al., 2018</xref>), recent work demonstrates the utility of large climate ensembles to advance physical understanding of the events and their drivers (e.g., <xref ref-type="bibr" rid="B1">Bevacqua et al., 2023</xref>; <xref ref-type="bibr" rid="B42">Reddy et al., 2022</xref>; <xref ref-type="bibr" rid="B24">Kamae et al., 2017</xref>). For example, <xref ref-type="bibr" rid="B42">Reddy et al. (2022)</xref> leveraged a large ensemble to quantify which combinations of ENSO and the Indian Ocean Dipole (IOD) phases have the greatest influence on compound events in Australia (<xref ref-type="bibr" rid="B42">Reddy et al., 2022</xref>).</p>
<p>Numerous studies have examined how the variability, amplitude, and teleconnections of large-scale climate modes may be altered by anthropogenic climate change in the 21<sup><italic>st</italic></sup> century (e.g., <xref ref-type="bibr" rid="B30">Maher et al., 2023</xref>; <xref ref-type="bibr" rid="B5">Cai et al., 2022</xref>; <xref ref-type="bibr" rid="B32">McKenna and Maycock, 2022</xref>). Such changes may lead to changes in extreme event occurrence in the future (<xref ref-type="bibr" rid="B7">Cai et al., 2015</xref>; <xref ref-type="bibr" rid="B13">Deser et al., 2024</xref>). Studies have also shown that the frequency of hot and dry compound events are changing due to the response of temperature and precipitation under climate change (e.g., <xref ref-type="bibr" rid="B54">Zhang et al., 2022</xref>; <xref ref-type="bibr" rid="B37">Mukherjee and Mishra, 2021</xref>; <xref ref-type="bibr" rid="B51">Vogel et al., 2021</xref>; <xref ref-type="bibr" rid="B52">Wu et al., 2021</xref>). Quantifying when changes in the frequency of hot and dry compound events may emerge from internal variability has primarily been analyzed in reanalysis and observational datasets. For example, <xref ref-type="bibr" rid="B45">Schmutz et al. (2025)</xref> analyzed the year of emergence in ECMWF version 5 reanalysis data (<xref ref-type="bibr" rid="B21">Hersbach et al., 2020</xref>) across Europe and northern Africa and found that, in most locations, compound events have emerged from internal variability (<xref ref-type="bibr" rid="B45">Schmutz et al., 2025</xref>). Although observational and reanalysis datasets provide crucial insight on historical patterns, large ensemble datasets, when compared to the short duration of observations and reanalysis products, increase the power of analyzing extreme events and allow for more robust assessments of future changes in compound event frequency.</p>
<p>Our study uses a large climate model ensemble to analyze the influence of four different internal climate modes on compound events at a global scale. Leveraging a large ensemble, with its large sample size, enables a more robust understanding of the possible response of these events to both unforced and forced climate variability across the historical record in addition to the 21<sup><italic>st</italic></sup> century. We strive to expand understanding of the influence of large-scale patterns of internal climate variability on hot and dry compound events within the climate model. After removing the external forcing signal, we explore how well-known, large-scale climate modes including El Ni&#x000F1;o Southern Oscillation (ENSO), Pacific Decadal Oscillation (PDO), Indian Ocean Dipole (IOD), and the North Atlantic Oscillation (NAO) influence hot and dry compound events. We use the Community Earth System Model 2 Large Ensemble (CESM2-LE), which is a set of 100 historical and future climate simulations under SSP 3-7.0 (<xref ref-type="bibr" rid="B44">Rodgers et al., 2021</xref>; <xref ref-type="bibr" rid="B11">Danabasoglu et al., 2020</xref>). We compare this analysis with the ECMWF Reanalysis Version 5 (ERA5) dataset (<xref ref-type="bibr" rid="B21">Hersbach et al., 2020</xref>) to visualize the similarities between the two datasets. We then investigate how conditional frequencies of compound events are changing over the 21<sup><italic>st</italic></sup> century and compare this to the historical period. This builds on previous research on changing climate mode variability by analyzing its impact on future compound events. We then retain the external forcing component and investigate when hot and dry compound events emerge from internal variability in the CESM2-LE.</p>
</sec>
<sec sec-type="materials|methods" id="s2">
<label>2</label>
<title>Materials and methods</title>
<sec>
<label>2.1</label>
<title>Data</title>
<p>We employ the CESM2-LE to study hot and dry compound events in preindustrial, present, and future climates (<xref ref-type="bibr" rid="B44">Rodgers et al., 2021</xref>; <xref ref-type="bibr" rid="B11">Danabasoglu et al., 2020</xref>). CESM2-LE follows protocols provided by the Coupled Model Intercomparison Project Phase 6 (CMIP6), with historical forcings for 1850-2014 and SSP3-7.0 forcings for 2014-2100 (<xref ref-type="bibr" rid="B14">Eyring et al., 2016</xref>). Monthly data for precipitation rate (PRECT), 2m temperature (TREFHT), surface temperature (TS), and surface-level pressure (PSL) are used to define and analyze compound events on a 0.94&#x000B0; by 1.25&#x000B0; horizontal grid. The ensemble mean over all 100 members is computed monthly and subtracted from each member to remove the forced response and the seasonal cycle. Temperature and precipitation anomalies are then analyzed for each month of every year from 1850 to 2100.</p>
<p>Monthly El Ni&#x000F1;o Southern Oscillation (ENSO), Indian Ocean Dipole (IOD), and Pacific Decadal Oscillation (PDO) indices from the CESM Climate Variability Diagnostics Package (<xref ref-type="bibr" rid="B29">Maher et al., 2024</xref>; <xref ref-type="bibr" rid="B39">Phillips et al., 2014</xref>) are used to explore the connection between modes of internal climate variability and hot and dry compound events (calculations of these indices are defined in the <xref ref-type="supplementary-material" rid="SM1">Supplementary material</xref>). Monthly North Atlantic Oscillation (NAO) indices are calculated in each member from the difference of normalized sea level pressure between Ponta Delgada, Azores (38.17 N, 25 W) and Stykkisholmur/Reykjavik, Iceland (63.61 N, 22.5 W) (<xref ref-type="bibr" rid="B22">Hurrell and Deser, 2009</xref>). Although climate change could impact the spatial patterns of the modes of internal variability, there is no consensus on how potential shifts may be manifested. We therefore have chosen to compute the large-scale climate mode indices in a consistent manner over time (e.g., <xref ref-type="bibr" rid="B30">Maher et al., 2023</xref>; <xref ref-type="bibr" rid="B32">McKenna and Maycock, 2022</xref>). The positive phase of each of these four modes is defined as the anomalies in the indices (standard deviation) that are &#x02265;0.5, the negative phase as &#x02264; &#x02013;0.5, and the neutral phase as the anomalies between these two bounds.</p>
<p>All climate models, including CESM2, exhibit biases in their simulation of internal climate modes and their teleconnections relative to observations. For instance, during El Ni&#x000F1;o, CESM2 tends to exhibit a dry bias over the Maritime Continent in June-November and a wet bias the rest of the year (<xref ref-type="bibr" rid="B29">Maher et al., 2024</xref>; <xref ref-type="bibr" rid="B41">Phillips et al., 2020a</xref>). There is also a dry bias in the majority of Australia in all seasons, but a regional wet bias does occur in some members (<xref ref-type="bibr" rid="B29">Maher et al., 2024</xref>; <xref ref-type="bibr" rid="B41">Phillips et al., 2020a</xref>). For highly variable metrics&#x02014;such as those associated with modes of internal variability&#x02014;the extent to which CESM2 aligns with the single realization that the observations represent is highly dependent on the CESM2 ensemble member chosen for comparison (<xref ref-type="bibr" rid="B29">Maher et al., 2024</xref>), which is not surprising as it is a free-running simulation. Despite these biases and challenges in comparing with observations, the simulation of climate modes and their teleconnections in CESM2 are improved over earlier versions of the model and many aspects are consistent with the observational record (e.g., <xref ref-type="bibr" rid="B9">Chen et al., 2021</xref>; <xref ref-type="bibr" rid="B8">Capotondi et al., 2020</xref>; <xref ref-type="bibr" rid="B11">Danabasoglu et al., 2020</xref>; <xref ref-type="bibr" rid="B40">Phillips et al., 2020b</xref>; <xref ref-type="bibr" rid="B47">Simpson et al., 2020</xref>; <xref ref-type="bibr" rid="B34">Meehl et al., 2020</xref>; <xref ref-type="bibr" rid="B27">Lawrence et al., 2019</xref>). Existing research further demonstrates CESM2&#x00027;s ability to simulate extremes (e.g., <xref ref-type="bibr" rid="B10">Chen et al., 2023</xref>; <xref ref-type="bibr" rid="B17">Gessner et al., 2023</xref>; <xref ref-type="bibr" rid="B33">McKinnon and Simpson, 2022</xref>). Here, our primary purpose is to leverage the 100 member CESM2-LE to calculate robust statistics of simulated compound events and explore the influence of both internal climate variability and anthropogenic climate change on them.</p>
<p>To compare our compound event results from the CESM2-LE to observational estimates, we use the ECMWF Reanalysis V5 data (ERA5; <xref ref-type="bibr" rid="B21">Hersbach et al., 2020</xref>). Monthly 2m temperature (t2m), precipitation (tp; converted to a monthly rate), and surface temperature (skt) from ERA5 is analyzed from January 1940 through December 2023 after regridding to the CESM2-LE spatial grid using bilinear interpolation via the Climate Data Operators package (<xref ref-type="bibr" rid="B46">Schulzweida, 2023</xref>). We also use a 3rd order polynomial fit (e.g., <xref ref-type="bibr" rid="B18">Gordon and Diffenbaugh, 2025</xref>; <xref ref-type="bibr" rid="B31">Mayer et al., 2025</xref>) for each month and at every grid point to estimate and remove climate forcing and deseasonalize the ERA5 data to produce monthly anomalies. We note that although ERA5 does have biases, the reanalysis data compares well to other observational products when used for compound event research (<xref ref-type="bibr" rid="B36">Mukherjee et al., 2020</xref>).</p>
</sec>
<sec>
<label>2.2</label>
<title>Methods</title>
<p>We investigate multivariate extremes, or two hazards that occur in the same place at the same time (<xref ref-type="bibr" rid="B56">Zscheischler et al., 2020a</xref>). The 90th percentile of monthly 2m temperature anomalies across the 100 members in the CESM2-LE is used to define extreme high temperatures. The 10th percentile of monthly precipitation rate anomalies across the 100 members is used to define extreme low precipitation. Concurrent hot and dry events (T90/P10) at a grid point thus occur when the monthly temperature anomaly exceeds the 90th percentile and the concurrent precipitation anomaly is below the 10th percentile. We use different baselines to calculate percentiles for hot and dry compound events. For the results shown in <xref ref-type="fig" rid="F1">Figures 1</xref>&#x02013;<xref ref-type="fig" rid="F4">4</xref>, temperature and precipitation percentiles are calculated over 1940&#x02013;2024. We use this baseline for consistency between CESM2-LE and ERA5. For <xref ref-type="fig" rid="F5">Figure 5</xref>, we use a 1850&#x02013;1950 baseline for compound event analysis for that same period, and a 2000&#x02013;2100 baseline for the later period as our aim is to extract any variance or distribution changes even when external forcing is removed. Compound event frequencies for both 1850&#x02013;1950 and 1940&#x02013;2024 are very similar when external forcing is removed (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S1</xref>, <xref ref-type="supplementary-material" rid="SM1">S2</xref>), facilitating comparison between results. For results in Section 3.2, we use the 1850&#x02013;1900 period to establish a pre-industrial baseline for evaluating anthropogenic changes in hot and dry compound events. We investigate what drives compound events regardless of time of year; therefore, percentiles for each variable are computed for each month after combining the ensemble members. In this way, anomalies from internal variability in specific seasons can be isolated and investigated (e.g., warm and dry extremes can occur in winter months and in wet seasons). A value of 1 is assigned to a gridpoint to signify a compound event in a given month, and a value of 0 is assigned if there is not a compound event. Analysis is then performed based on this binary classification. The global distribution of T90/P10 compound event frequencies are computed by averaging across all ensemble members over the 1940&#x02013;2024 period. We then display the results as a percentage relative to this reference period.</p>
<fig position="float" id="F1">
<label>Figure 1</label>
<caption><p>Frequency of T90/P10 compound events due to detrended anomalies <bold>(a)</bold> 1940&#x02013;2024 from the 100 member CESM2-LE and <bold>(b)</bold> 1940&#x02013;2024 ERA5 data. <bold>(c)</bold> Difference of frequencies for CESM2-LE from the average of the 99 scrambled ensemble-mean frequencies under the null hypothesis (see Methods). Stippling indicates where the null hypothesis cannot be rejected and the frequencies of T90/P10 events are consistent with independence. Areas that are shaded green without stippling indicate frequencies of T90/P10 compound events that are greater than independent chance whereas areas that are pink without stippling indicate frequencies that are less than independent chance.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0001.tif">
<alt-text content-type="machine-generated">Eight-panel figure presents global maps comparing sea surface temperature anomalies for four regions&#x02013;Northern Brazil, Northeast Nigeria, Central Spain, and Southeast Australia&#x02013;using CESM2-LE model (left) and ERA5 reanalysis (right). Each map highlights temperature anomalies in blue to red, with light blue X marking the region of interest, and sample size (N) displayed. A color bar below indicates the temperature anomaly range from minus one to plus one degrees Celsius.</alt-text>
</graphic>
</fig>
<p>We compare our T90/P10 frequencies to independent frequencies, where temperature and precipitation variables are uncorrelated, to determine the extent to which internal variability is influencing the frequency of compound events. Independent frequencies are calculated via bootstrapping, where T90/P10 events are computed across scrambled ensemble members. Namely, the ensemble members for temperature are kept fixed and the ensemble members for precipitation are shifted down by one member (e.g., pairing temperature of member 1 with precipitation of member 2, temperature of member 2 with precipitation of member 3, etc.). The ensemble-mean frequencies across the 100 member pairings are then computed. We then proceed to shift the precipitation members again and run the same calculation. This is continued through the last possible combination. The result is 99 ensemble-mean frequencies under the null hypothesis of independent, uncorrelated variables. From here, we compute the 1st and 99th percentiles to define the bounds of independent chance. If the unscrambled frequencies fall outside of these bounds, we suggest that there may be evidence that internal climate variability drives correlations between T90 and P10 events, leading to more (or less) frequent extremes.</p>
<p>We also recognize the impact of climate change on T90/P10 compound events and thus analyze results when the forced response is retained. In this case, 1850&#x02013;1900 is used as the baseline period for percentile calculation and compound events are determined using the same methods as before with the exception that the ensemble mean is not removed.</p>
<p>We then investigate the year of emergence of T90/P10 compound events from internal variability to demonstrate when climate change has or will become a significant influence on the occurrence of T90/P10 compound events under historical and SSP 3-7.0 forcing. As defined here, compound events emerge from internal variability when the median number of events in the 100-member ensemble exceeds and remains above the 90th percentile of compound events from all members over the 1850&#x02013;1900 period. Time series of compound events in different locations are visualized by taking a five-year forward moving sum of the events (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S3</xref>).</p>
</sec>
</sec>
<sec sec-type="results" id="s3">
<label>3</label>
<title>Results</title>
<sec>
<label>3.1</label>
<title>Role of internal variability</title>
<p>In the first part of our results, we quantify the influence of internal climate variability on the occurrence of T90/P10 compound events (henceforth referred to as compound events or CEs). We begin by computing frequencies in CESM2-LE and ERA5 from 1940&#x02013;2024 (<xref ref-type="fig" rid="F1">Figures 1a</xref>, <xref ref-type="fig" rid="F1">b</xref>). Our results demonstrate the ability and need for a large ensemble to analyze compound events due to the large sample size and its ability to capture similar historical patterns of CE frequency to ERA5 data (<xref ref-type="fig" rid="F1">Figures 1a</xref>, <xref ref-type="fig" rid="F1">b</xref>). Particular locations, including northern South America, eastern Africa, the Indian subcontinent, and the Indonesian archipelago, depict the highest frequencies of compound events in both the CESM2-LE and ERA5 (<xref ref-type="fig" rid="F1">Figures 1a</xref>, <xref ref-type="fig" rid="F1">b</xref>). While ERA5 generally shows higher compound event frequencies than CESM2-LE, the two datasets exhibit largely similar spatial patterns (<xref ref-type="fig" rid="F1">Figures 1a</xref>, <xref ref-type="fig" rid="F1">b</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S1</xref>). Despite this frequency bias, we leverage the large ensemble size of CESM2-LE to calculate robust statistics for the drivers of hot and dry CEs.</p>
<p>Internal climate modes influence the dependency between precipitation and temperature anomalies (e.g., <xref ref-type="bibr" rid="B15">Feng and Hao, 2021</xref>, Supplementary Figures S4, S5) which then impacts the occurrence of compound events (<xref ref-type="bibr" rid="B57">Zscheischler and Seneviratne, 2017</xref>). However, even if the temperature and precipitation values are treated as independent variables, random sampling of their distributions would still result in CEs. We use a bootstrapping technique (see Methods) to calculate 99 ensemble-mean frequencies under the null hypothesis of independent, uncorrelated variables. We compare our unscrambled frequencies with the 99 ensemble-mean frequencies under this null hypothesis to analyze where frequencies are greater or less than independent chance (<xref ref-type="fig" rid="F1">Figure 1c</xref>). Most of the land areas in the world exhibit frequencies of CEs that are distinguishable from independent chance (<xref ref-type="fig" rid="F1">Figure 1c</xref>), and regions with CEs that are not distinguishable from independent chance are often found in transition regions. Dry regions, such as some high-latitude areas (including the ice sheet regions) and the Saharan and Arabian deserts, have compound event frequencies that are below independent chance because precipitation and precipitation variance is low.</p>
<p>To investigate the connection between internal climate modes and compound events, we first examine the mean sea surface temperature (SST) conditions during months containing compound events at twenty different locations (<xref ref-type="fig" rid="F2">Figure 2</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S7</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM1">S10</xref>). This is done to obtain a qualitative understanding of SST relationships to compound event occurrence and identify large-scale climate modes to investigate in this study. Specific grid points are selected to build on previous studies investigating internal climate drivers of compound events (e.g., <xref ref-type="bibr" rid="B36">Mukherjee et al., 2020</xref>; <xref ref-type="bibr" rid="B20">Hao et al., 2020</xref>, <xref ref-type="bibr" rid="B19">2018</xref>). We also pick locations that are underrepresented in the current literature, including South America, Africa, and Southeast Asia (<xref ref-type="bibr" rid="B3">Brett et al., 2025</xref>) (<xref ref-type="fig" rid="F2">Figure 2</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S7</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM1">S10</xref>). Furthermore, the grid points are representative of regional averages (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S11</xref>).</p>
<fig position="float" id="F2">
<label>Figure 2</label>
<caption><p>Mean sea surface temperature (SST) for all months that contain a T90/P10 compound event for a location over <bold>(a, b)</bold> northern Brazil (teal box; 3.298 S, 60.0 W), <bold>(c, d)</bold> northeast Nigeria (12.72 N, 13.75 E), <bold>(e, f)</bold> central Spain (40.05 N, 3.80 W), and <bold>(g, h)</bold> southeast Australia (32.51 S, 150.0 E). The left column depicts frequencies computed in CESM2-LE and the right column denotes those from ERA5, 1940&#x02013;2024. The number of compound events at the selected grid cell is located in the white box in the lower left of each panel.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0002.tif">
<alt-text content-type="machine-generated">Eight global maps display regional changes in T90/P10 compound extremes conditional frequencies between 1850-1950 and 2000-2100 for El Ni&#x000F1;o, La Ni&#x000F1;a, PDO, IOD, and NAO, using a green-to-purple color scale to represent percentage differences from minus one to one.</alt-text>
</graphic>
</fig>
<p>For many regions, the SST patterns during CEs in CESM2-LE and ERA5 resemble combinations of multiple large-scale climate modes that are known to influence local weather patterns (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S4, S5</xref>). For example, CEs for locations in northern Brazil, northeast Nigeria, and southeast and southwest Australia are accompanied by SST patterns that resemble El Ni&#x000F1;o-like conditions and a positive PDO (<xref ref-type="fig" rid="F2">Figure 2</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S10</xref>). Additionally, SST anomalies during events for locations in southwest and southeast Australia and northern Brazil show conditions resembling a positive IOD (<xref ref-type="fig" rid="F2">Figure 2</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S10</xref>). Thus, we include ENSO, the PDO, and the IOD in the following analysis. Furthermore, despite previous studies (e.g., <xref ref-type="bibr" rid="B23">Hurrell and Van Loon, 1997</xref>) documenting the effects of the NAO on temperature and precipitation patterns in Europe, we find that neither CESM2-LE nor ERA5 show SST patterns typically associated with NAO during CE occurrence in Europe (<xref ref-type="fig" rid="F2">Figures 2e</xref>, <xref ref-type="fig" rid="F2">f</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S7</xref>, <xref ref-type="supplementary-material" rid="SM1">S9</xref>, <xref ref-type="supplementary-material" rid="SM1">S10</xref>). We then analyze sea level pressure patterns during CEs in CESM2-LE for further investigation (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S12</xref>), finding NAO-like conditions during CEs in multiple locations, and include NAO in our analysis.</p>
<p>The SST patterns that occur during CEs qualitatively indicate how internal climate modes may influence the presence of compound events. We quantify the possible influence of ENSO, PDO, IOD, and the NAO on compound events in CESM2-LE and ERA5 by calculating conditional frequencies of CEs during each phase of each climate mode (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>). As ENSO is known to drive temperature and precipitation anomalies globally (<xref ref-type="bibr" rid="B28">Lenssen et al., 2020</xref>; <xref ref-type="bibr" rid="B26">Latif and Keenlyside, 2009</xref>), the analysis for PDO, IOD, and the NAO is conditioned on ENSO being in its neutral phase. Conditional frequencies without the neutral ENSO condition are also calculated for comparison and show minor differences except in regions with known strong ENSO teleconnections (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S13</xref>, <xref ref-type="supplementary-material" rid="SM1">S14</xref>, <xref ref-type="supplementary-material" rid="SM1">S15</xref>). For the calculation of conditional frequencies, we pool all members and sum the number of compound events that occur concurrently with the two phases of the climate modes (e.g., positive PDO and neutral ENSO). We then divide this sum by the total number of months where the two phases of the climate modes are present to determine the conditional frequencies (<xref ref-type="fig" rid="F3">Figure 3</xref>). A chi-square test for independence is used to determine if the conditional frequencies are significant relative to our null hypothesis of independent, uncorrelated variables. Grid points where we do not reject the null hypothesis at 98% are represented through the gray shading (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>). We use this shading to demonstrate the spatial characteristics of the conditional frequencies. We note that significance is likely much more difficult to obtain using ERA5 due to the low sample size in the reanalysis data (1,008 months) and is particularly true for the conditional frequencies with the PDO, IOD, and NAO (<xref ref-type="fig" rid="F4">Figure 4</xref>). Sample sizes for CESM2-LE are more than 100 times larger than the ERA5 sample sizes, allowing for more confidence in our assessments of where climate modes significantly influence compound events (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>).</p>
<fig position="float" id="F3">
<label>Figure 3</label>
<caption><p>Conditional frequencies of T90/P10 compound events given a climate mode for detrended anomalies from CESM2-LE (1940&#x02013;2024) for <bold>(a, b)</bold> ENSO, <bold>(c, d)</bold> PDO, <bold>(e, f)</bold> IOD, <bold>(g, h)</bold> NAO. A chi-square test of independence is employed at the 95% confidence level to determine where compound event frequencies can be considered independent of the climate modes. Any conditional frequency that is not considered independent is then gray scaled. The sample size in the bottom right of each panel indicates the number of months during an active mode phase across the dataset.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0003.tif">
<alt-text content-type="machine-generated">Eight-panel figure display conditional frequency of compound extremes under various climate modes in ERA5: El Ni&#x000F1;o, La Ni&#x000F1;a, positive and negative phases of PDO, IOD, and NAO, the latter three with neutral ENSO. Darker red shading indicates higher frequency percentages, with a color bar scale from zero to eight percent. Each panel displays a sample size N. Panel a emphasizes South America during El Ni&#x000F1;o, while other panels show varied regional frequency patterns.</alt-text>
</graphic>
</fig>
<fig position="float" id="F4">
<label>Figure 4</label>
<caption><p>As in <xref ref-type="fig" rid="F3">Figure 3</xref>, but for ERA5 conditional frequencies from 1940&#x02013;2024. NAO conditional frequencies from 1940&#x02013;2023.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0004.tif">
<alt-text content-type="machine-generated">Eight-panel figure showing world maps marked a through h, each illustrating conditional frequency of compound events (T90/P10 CE) under different climate modes in the CESM2-E model: El Ni&#x000F1;o, La Ni&#x000F1;a, positive and negative phases of PDO, IOD, and NAO, all with neutral ENSO except a and b. Darker red shading indicates higher frequency percentages, with a color bar scale from zero to eight percent. Each panel displays a sample size N. Panel a emphasizes South America during El Ni&#x000F1;o, while other panels show varied regional frequency patterns.</alt-text>
</graphic>
</fig>
<p>For the CESM2-LE, regions with high conditional frequencies during El Ni&#x000F1;o (<xref ref-type="fig" rid="F3">Figure 3a</xref>), such as northern South America, the Indonesian Archipelago, and the Indian subcontinent, can be partially explained by the warmer temperature anomalies and drier conditions that occur during an El Ni&#x000F1;o month (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S4</xref>, <xref ref-type="supplementary-material" rid="SM1">S5</xref>). Despite the precipitation biases in CESM2-LE, including dry biases over Australia in most members during El Ni&#x000F1;o events (see Data), we do see overlap in significant conditional frequencies between the CESM2-LE and ERA5 analyses (<xref ref-type="fig" rid="F3">Figures 3a</xref>, <xref ref-type="fig" rid="F4">4a</xref>). Further, our ERA5 results for the conditional frequencies for ENSO (<xref ref-type="fig" rid="F4">Figures 4a</xref>, <xref ref-type="fig" rid="F4">b</xref>) are largely consistent with previous studies (<xref ref-type="bibr" rid="B55">Zhang et al., 2023</xref>; <xref ref-type="bibr" rid="B20">Hao et al., 2020</xref>).</p>
<p>When investigating the conditional frequencies during the PDO, there are higher frequencies of CEs in India and southeast Asia during the positive PDO and neutral ENSO phases that correspond well with the known lower precipitation and warmer temperature anomalies associated with the PDO in these regions (<xref ref-type="fig" rid="F3">Figure 3c</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S4</xref>, <xref ref-type="supplementary-material" rid="SM1">S5</xref>). Although this assists in demonstrating that temperature and precipitation are largely correlated, we show the need to investigate both these variables in compound event analysis with the example of Alaska and western Canada. Although there are warmer temperature anomalies in Alaska and western Canada during a positive PDO event (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S4</xref>), the region does not experience drier conditions (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S5</xref>). This leads to a low frequency of CEs despite the PDO&#x00027;s influence on temperature (<xref ref-type="fig" rid="F3">Figure 3c</xref>). In an univariate analysis, it would be possible to misinterpret the number of compound events in this region (i.e., warmer temperatures equating to more hot and dry compound events), further demonstrating the need for multivariate analyses.</p>
<p>In the conditional frequencies for the IOD and NAO, we find that the positive phase of the IOD leads to higher frequencies of compound events in India and the conditional frequencies for the negative phase of the IOD has the highest number of compound events in eastern Africa (<xref ref-type="fig" rid="F3">Figures 3e</xref>, <xref ref-type="fig" rid="F3">f</xref>). <xref ref-type="fig" rid="F3">Figures 3g</xref>, <xref ref-type="fig" rid="F3">h</xref> depict the NAO&#x00027;s influence on compound events in Europe and lack of influence in the majority of the Southern Hemisphere (<xref ref-type="fig" rid="F3">Figures 3g</xref>, <xref ref-type="fig" rid="F3">h</xref>), consistent with known NAO teleconnections (<xref ref-type="bibr" rid="B23">Hurrell and Van Loon, 1997</xref>).</p>
<p>The variability of climate modes may change over the 21<sup><italic>st</italic></sup> century (<xref ref-type="bibr" rid="B6">Cai et al., 2021</xref>; <xref ref-type="bibr" rid="B16">Geng et al., 2019</xref>). With the forced trend still removed, we investigate how the statistics (i.e., conditional frequencies) of CEs change in the future using CESM2-LE and how this may be related, in part, to changes in internal variability. We take the difference in conditional frequencies for the four climate modes between 2000&#x02013;2100 and 1850&#x02013;1950 to depict future changes of CE occurrence. We note that the earlier period (1850&#x02013;1950) strongly resembles the 1940&#x02013;2024 results shown in <xref ref-type="fig" rid="F1">Figures 1</xref>, <xref ref-type="fig" rid="F3">3</xref> (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S2</xref>, <xref ref-type="supplementary-material" rid="SM1">S16</xref>). A z-test comparison of two proportions is used to determine if our difference in conditional frequencies between the two periods is significant relative to our null hypothesis of equal conditional frequencies.</p>
<p>Overall, conditional frequencies show signs of change under future climate conditions that largely align with each mode&#x00027;s teleconnection pattern of temperature and precipitation. These responses are mostly of the opposing sign between positive and negative phases of the climate mode. Specifically for ENSO, future changes in the conditional frequency with El Ni&#x000F1;o are largest in South America, Africa (south of the Sahara), and the Maritime Continent (<xref ref-type="fig" rid="F5">Figure 5a</xref>). As these regions are most impacted by ENSO teleconnections (<xref ref-type="bibr" rid="B28">Lenssen et al., 2020</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S4, S5</xref>), a change in ENSO, which includes intensification until around 2050 and then weakening through the end of the century (e.g., <xref ref-type="bibr" rid="B30">Maher et al., 2023</xref>; <xref ref-type="bibr" rid="B5">Cai et al., 2022</xref>), may more strongly impact CEs in these regions compared to other locations.</p>
<fig position="float" id="F5">
<label>Figure 5</label>
<caption><p>As in <xref ref-type="fig" rid="F3">Figure 3</xref> but for the changes in conditional frequencies of T90/P10 compound events between 2000&#x02013;2100 and 1850&#x02013;1950 in CESM2-LE after removing external forcing. Positive differences in probabilities (green) illustrate that the modes&#x00027; influence on CEs increases in the future while negative differences in probabilities (pink) illustrate that modes&#x00027; influence decreases in the future.</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0005.tif">
<alt-text content-type="machine-generated">Three world maps compare climate event frequencies and differences from independent chance from 1940 to 2024. Panels a and b show global event frequencies in red shades for CESM2-LE and ERA5 datasets, with highest values in South America and Africa. Panel c illustrates CESM2-LE model differences from independent chance, using green and pink to show positive and negative deviations, with notable differences in South America, Africa, and Southeast Asia. Color bars quantify frequency and differences in percentage.</alt-text>
</graphic>
</fig>
<p>Likewise, the variability and amplitude of the PDO, IOD, and NAO may change throughout the 21<sup><italic>st</italic></sup> century (e.g., <xref ref-type="bibr" rid="B43">Rezaei et al., 2023</xref>; <xref ref-type="bibr" rid="B12">Deser et al., 2017</xref>; <xref ref-type="bibr" rid="B4">Cai et al., 2014</xref>). We find that the conditional frequency changes under the PDO are largest in South America (<xref ref-type="fig" rid="F5">Figures 5c</xref>, <xref ref-type="fig" rid="F5">d</xref>), throughout central Africa (<xref ref-type="fig" rid="F5">Figures 5c</xref>, <xref ref-type="fig" rid="F5">d</xref>), and in Indonesia in the CESM2-LE (<xref ref-type="fig" rid="F5">Figure 5d</xref>). The conditional frequencies under the positive IOD phase increase across the Indonesian archipelago and decrease across the sub-Sahara and India in the future (<xref ref-type="fig" rid="F5">Figure 5e</xref>). Although existing literature predicts a decrease in future precipitation over southern Europe under the positive NAO phase (<xref ref-type="bibr" rid="B32">McKenna and Maycock, 2022</xref>), the change in conditional frequencies in most of this region does not reject the null hypothesis of equal frequencies (<xref ref-type="fig" rid="F5">Figure 5g</xref>). However, under the negative NAO phase we find an increase of compound events over the United Kingdom and Ireland, Iceland, and northern Europe, while there is a decrease in regions surrounding the Mediterranean (<xref ref-type="fig" rid="F5">Figure 5h</xref>). We would also like to note that in southern South America, accounting for the PDO&#x00027;s influence lowers the magnitude of change in conditional NAO frequencies relative to ENSO alone (<xref ref-type="fig" rid="F5">Figure 5g</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S17</xref>).</p>
<p>The changes in conditional frequency between phases for ENSO, PDO, IOD, and NAO are not always identical (or opposite). For example, although conditional frequency for compound events with El Ni&#x000F1;o increases across Australia in the future, conditional frequencies for La Ni&#x000F1;a stay approximately the same (<xref ref-type="fig" rid="F5">Figures 5a</xref>, <xref ref-type="fig" rid="F5">b</xref>). The future conditional frequencies under the positive IOD phase decrease across the Indian subcontinent but largely stay the same for the negative IOD phase (<xref ref-type="fig" rid="F5">Figures 5e</xref>, <xref ref-type="fig" rid="F5">f</xref>). Therefore, changes in the amplitude and/or variability of these climate modes due to anthropogenic climate change could affect the frequency of compound events in different regions and highlights the continued influence of the modes on CEs under anthropogenic climate change.</p>
</sec>
<sec>
<label>3.2</label>
<title>Role of external forcing</title>
<p>Many studies have documented increasing frequencies of hot and dry compound events under historical and future scenarios (e.g., <xref ref-type="bibr" rid="B35">Meng et al., 2022</xref>; <xref ref-type="bibr" rid="B52">Wu et al., 2021</xref>), but few have examined the time of emergence of CEs from internal climate variability (e.g., <xref ref-type="bibr" rid="B45">Schmutz et al., 2025</xref>). Due to the consequential impacts of hot and dry compound events, identifying how they may change over the 21<sup><italic>st</italic></sup> century is crucial for adaptation planning. We use 1850&#x02013;1900 as our baseline period, retain external forcing, and compute the 90th percentile of compound events of the 100 members in CESM2-LE at all grid points. The year of emergence from internal variability is defined to be when the median number of CEs in a 5-year forward moving sum at every grid point exceeds and remains above the 90th percentile of the baseline (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S3</xref>).</p>
<p>We find that compound events emerge from internal variability before 2025 for most land regions under SSP 3-7.0 (60% of land area, excluding Antarctica, <xref ref-type="fig" rid="F6">Figure 6a</xref>). The majority of the Southern Hemisphere emerges prior to 2025 (87% of land area, excluding Antarctica), except for portions of central Africa and southern South America. In contrast, there is far more heterogeneity in emergence timing over the Northern Hemisphere, with only 50% of the land area emerging prior to 2025 (<xref ref-type="fig" rid="F6">Figure 6c</xref>). Later emergence in the Northern Hemisphere is likely due to higher variability in precipitation and 2m temperature over the Northern Hemisphere relative to the Southern Hemisphere (<xref ref-type="bibr" rid="B50">van Loon, 1991</xref>; <xref ref-type="bibr" rid="B25">Kang et al., 2015</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S18</xref>).</p>
<fig position="float" id="F6">
<label>Figure 6</label>
<caption><p><bold>(a)</bold> Year of emergence for the ensemble median. White indicates no emergence from the 90th percentile before 2096. Time series of the five-year forward moving sum of compound events shown for six locations: <bold>(b)</bold> southeast United States (35.34 N, 88.80 W), <bold>(c)</bold> northern France (48.53 N, 2.50 E), <bold>(d)</bold> northeast India (24.03 N, 87.50 E), <bold>(e)</bold> southeast Brazil (20.26 S, 51.20 W), <bold>(f)</bold> northeast Nigeria (12.72 N, 13.75 E), and <bold>(g)</bold> eastern Indonesia (0.47 S, 113.80 E).</p></caption>
<graphic mimetype="image" mime-subtype="tiff" xlink:href="fclim-08-1739394-g0006.tif">
<alt-text content-type="machine-generated">Composite figure showing a world map with regions colored from blue to green to red corresponding to the year of emergence from 1900 to 2100, and six inset line charts, each connected with arrows to specific locations on the map, depicting compound climate event counts over time from 1850 to 2100. The map is labeled &#x0201C;a) Year of Emergence&#x0201D; with a color bar legend, and charts b) to g) illustrate regional event trends, highlighting increases in event frequency and emergence periods.</alt-text>
</graphic>
</fig>
<p>Regions with the highest frequency of CEs in the early historical period (<xref ref-type="fig" rid="F1">Figures 1a</xref>, <xref ref-type="fig" rid="F1">c</xref>) display a wide range of emergence times. For example, northern Brazil and eastern Africa exhibit similar frequencies of CEs between 1940&#x02013;2024 (<xref ref-type="fig" rid="F1">Figure 1a</xref>), but northern Brazil emerges around 2003 while eastern Africa still has not emerged by the end of the 21<sup><italic>st</italic></sup> century ( <xref ref-type="fig" rid="F6">Figure 6a</xref>). The difference in emergence years likely relies on the mean trends of temperature and precipitation and the correlation between the two variables. Existing literature suggests that, under climate change, mean precipitation trends are more influential than the dependence between temperature and precipitation in determining the frequency of hot and dry compound events (<xref ref-type="bibr" rid="B2">Bevacqua et al., 2022</xref>). Although temperature increases may contribute more to the global frequency of compound events due to globally increasing temperatures (<xref ref-type="bibr" rid="B53">Zeng et al., 2024</xref>), differing mean precipitation trends throughout the world will impact regional emergence. Our results agree with this, as we find that precipitation trends are likely a major reason for late or no emergence in many regions (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S19</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM1">22</xref>). In the northern Brazil and eastern Africa cases, there is a decrease in precipitation over northern Brazil in the 21<sup><italic>st</italic></sup> century and an increase in precipitation over eastern Africa, including South Sudan (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S19</xref>), likely leading to differing emergence years.</p>
<p>Time series of compound events for eighteen locations are shown in <xref ref-type="fig" rid="F6">Figures 6b</xref>&#x02013; <xref ref-type="fig" rid="F6">g</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S19</xref>, <xref ref-type="supplementary-material" rid="SM1">S23</xref>, <xref ref-type="supplementary-material" rid="SM1">S24</xref>. Over northern France, as well as other locations across Europe, a consistently increasing trend of compound events is evident beginning early in the 21<sup><italic>st</italic></sup> century (<xref ref-type="fig" rid="F6">Figure 6c</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S23</xref>, <xref ref-type="supplementary-material" rid="SM1">S24</xref>). This result is consistent with projections of the global average of hot and dry compound events under SSP 3-7.0 found in previous studies (<xref ref-type="bibr" rid="B54">Zhang et al., 2022</xref>; <xref ref-type="bibr" rid="B51">Vogel et al., 2021</xref>). For locations exhibiting earlier emergence, including southern Brazil and the Indonesian Archipelago, emergence during the 20<sup><italic>th</italic></sup> century is followed by stabilization of CE frequencies. This early emergence could be due to observed decrease in natural vegetation in the mid-twentieth century (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S25</xref>). The consistent and stable frequencies across the 21<sup><italic>st</italic></sup> century are likely due to unchanged precipitation patterns when compared to the historical period (<xref ref-type="fig" rid="F6">Figures 6e</xref>, <xref ref-type="fig" rid="F6">g</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S20</xref>). Other regions with historically low frequencies, including northeast India and northeast Nigeria, show minimal changes under climate change ( <xref ref-type="fig" rid="F6">Figures 6d</xref>, <xref ref-type="fig" rid="F6">f</xref>). Locations including the southeast United States, northeast India, and southern Alaska, United States, that have late or no emergence by the end of the century also have increasing mean precipitation trends, affecting how often compound events would occur (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S20</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM1">S22</xref>).</p>
</sec>
</sec>
<sec id="s4">
<label>4</label>
<title>Conclusions</title>
<p>In this study, we explored the roles of internal climate variability and external forcing as drivers for hot and dry compound events in the CESM2-LE, defined by using the 90th percentile of monthly temperature and the 10th percentile of monthly precipitation rate at each land gridpoint over the globe. We analyzed the influence of the El Ni&#x000F1;o Southern Oscillation (ENSO), the Pacific Decadal Oscillation (PDO), the Indian Ocean Dipole (IOD), and the North Atlantic Oscillation (NAO) on compound events through calculations of conditional frequencies (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>). We found that ENSO had the largest impact on northern South America, the Indonesian archipelago, and the Indian subcontinent (<xref ref-type="fig" rid="F3">Figure 3a</xref>, <xref ref-type="fig" rid="F3">b</xref>) and that conditional frequencies for the positive PDO are higher in southeast Asia than in Alaska and western Canada, most likely due to precipitation anomaly differences that occur during the positive PDO phase across these regions (<xref ref-type="fig" rid="F3">Figures 3c</xref>, <xref ref-type="fig" rid="F3">d</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S5</xref>). The IOD has the most influence over eastern Africa and the Indian subcontinent (<xref ref-type="fig" rid="F3">Figures 3e</xref>, <xref ref-type="fig" rid="F3">f</xref>). The NAO impacts the conditional frequencies of CEs over Europe (<xref ref-type="fig" rid="F3">Figures 3g</xref>, <xref ref-type="fig" rid="F3">h</xref>).</p>
<p>Further, although previous comparisons have been made for the changing magnitude, occurrence, and severity of compound events due to future increases in external forcing (e.g., <xref ref-type="bibr" rid="B54">Zhang et al., 2022</xref>; <xref ref-type="bibr" rid="B51">Vogel et al., 2021</xref>; <xref ref-type="bibr" rid="B37">Mukherjee and Mishra, 2021</xref>; <xref ref-type="bibr" rid="B52">Wu et al., 2021</xref>), we add to this by exploring when the occurrence of compound events emerges from internal variability under SSP 3-7.0 (<xref ref-type="fig" rid="F6">Figure 6a</xref>). We find that under climate change, the frequency of compound events emerges from internal variability over many land areas before 2025. Regions with compound events that emerged before 1975, such as southeastern Brazil, may have emerged earlier due to changes in natural vegetation (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S25</xref>). Although there is a decrease in natural vegetation in these early emerging regions, our results are only suggestive and we encourage future investigation to quantify the impact of changes in natural vegetation on compound event frequency. We also find differences in the regional timeseries of these events (<xref ref-type="fig" rid="F6">Figures 6b</xref>&#x02013;<xref ref-type="fig" rid="F6">g</xref>, <xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S19</xref>, <xref ref-type="supplementary-material" rid="SM1">S23</xref>, <xref ref-type="supplementary-material" rid="SM1">S24</xref>), and not all locations (i.e., southeast United States, northeast India) coincide with the average global projection of compound events under SSP 3-7.0 (<xref ref-type="bibr" rid="B54">Zhang et al., 2022</xref>). This could be, in part, due to the influence of internal climate variability (<xref ref-type="fig" rid="F3">Figures 3</xref>, <xref ref-type="fig" rid="F4">4</xref>) as well as precipitation pattern changes (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figures S19</xref>&#x02013;<xref ref-type="supplementary-material" rid="SM1">22</xref>). CESM2 is typical of rainfall changes in other CMIP6 models, and thus could be considered as being representative of other models (<xref ref-type="supplementary-material" rid="SM1">Supplementary Figure S26</xref>, <xref ref-type="bibr" rid="B49">Tebaldi et al., 2021</xref>). Nevertheless, we urge caution on the generalization of the time of emergence of hot and dry compound events in CESM2 due to differences in simulations of precipitation changes between models. Further investigation into other scenarios would assist in understanding the range of possible CE emergence. Expanding such analyses can improve understanding of these events&#x00027; response to internal and external climate drivers, aiding in preparation for the future compound event changes.</p>
<p>Our results demonstrate CESM2&#x00027;s utility to advance understanding of large-scale, unforced, internal climate variability and external forcing as drivers of hot and dry compound events. Although external forcing will likely impact compound events in the future over many regions, we show that internal variability will continue to be a strong influence. Our analysis of the joint influence of ENSO, PDO, IOD, and NAO as drivers of hot and dry CEs adds to the literature that has almost exclusively focused on ENSO&#x00027;s influence. We then quantified frequency differences between the historical and future period due to possible changes in future internal variability. Knowledge of which climate modes impact compound events in certain regions could assist in prediction of these events on seasonal-to-decadal timescales. Better prediction of regional compound events could support more informed decision-making and strengthen preparation, which could then allow for mitigation of adverse impacts on society, e.g., human health. Therefore, although we do not predict compound events in this work, our analysis of compound event drivers on a global scale could assist in regional-scale prediction and forecasts of opportunity.</p>
</sec>
</body>
<back>
<sec sec-type="data-availability" id="s5">
<title>Data availability statement</title>
<p>We use data from the Community Earth System Model Version 2 Large Ensemble (CESM2-LE, <xref ref-type="bibr" rid="B44">Rodgers et al., 2021</xref>) which is provided and maintained by the National Center for Atmospheric Research (NCAR). We also use reanalysis data from the ECMWF Reanalysis Data Version 5 (<xref ref-type="bibr" rid="B21">Hersbach et al., 2020</xref>). The analysis code used in this study is publicly available on Github at <ext-link ext-link-type="uri" xlink:href="https://github.com/ashdwyer/Compound-Event-Drivers">https://github.com/ashdwyer/Compound-Event-Drivers</ext-link>.</p>
</sec>
<sec sec-type="author-contributions" id="s6">
<title>Author contributions</title>
<p>AD: Conceptualization, Writing &#x02013; review &#x00026; editing, Writing &#x02013; original draft, Investigation, Methodology, Software, Visualization, Formal analysis, Validation, Data curation. JH: Funding acquisition, Resources, Methodology, Supervision, Project administration, Writing &#x02013; review &#x00026; editing, Conceptualization. EB: Conceptualization, Writing &#x02013; review &#x00026; editing, Resources, Funding acquisition, Supervision, Project administration, Methodology.</p>
</sec>
<ack><title>Acknowledgments</title><p>The authors extend special thanks to Peter Lawrence for insight on useful metrics for land use changes in CESM2-LE.</p>
</ack>
<sec sec-type="COI-statement" id="conf1">
<title>Conflict of interest</title>
<p>The author(s) declared that this work was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.</p>
</sec>
<sec sec-type="ai-statement" id="s8">
<title>Generative AI statement</title>
<p>The author(s) declared that generative AI was not used in the creation of this manuscript.</p>
<p>Any alternative text (alt text) provided alongside figures in this article has been generated by Frontiers with the support of artificial intelligence and reasonable efforts have been made to ensure accuracy, including review by the authors wherever possible. If you identify any issues, please contact us.</p>
</sec>
<sec sec-type="disclaimer" id="s9">
<title>Publisher&#x00027;s note</title>
<p>All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article, or claim that may be made by its manufacturer, is not guaranteed or endorsed by the publisher.</p>
</sec>
<sec sec-type="supplementary-material" id="s10">
<title>Supplementary material</title>
<p>The Supplementary Material for this article can be found online at: <ext-link ext-link-type="uri" xlink:href="https://www.frontiersin.org/articles/10.3389/fclim.2026.1739394/full#supplementary-material">https://www.frontiersin.org/articles/10.3389/fclim.2026.1739394/full#supplementary-material</ext-link></p>
<supplementary-material xlink:href="Data_Sheet_1.pdf" id="SM1" mimetype="application/pdf" xmlns:xlink="http://www.w3.org/1999/xlink"/>
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<fn-group>
<fn fn-type="custom" custom-type="edited-by" id="fn0001">
<p>Edited by: <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/2076329/overview">Jason Furtado</ext-link>, University of Oklahoma, United States</p>
</fn>
<fn fn-type="custom" custom-type="reviewed-by" id="fn0002">
<p>Reviewed by: <ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1080460/overview">Kevin Grise</ext-link>, University of Virginia, United States</p>
<p><ext-link ext-link-type="uri" xlink:href="https://loop.frontiersin.org/people/1127023/overview">Yong-Yub Kim</ext-link>, University of Bergen, Norway</p>
</fn>
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